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Binary Readout System for a Silicon Tracking Detector at LHC
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1. EO 41 5 4 The VME m duls miie tales on Goso ce Gnd ba uides koc M Chaat t Coca pde Le tubers OS aseo 42 544 E The BC96 Bias Cards utente mra n cette per ERAIO 46 6 0 Hybrid Evaluation 7 51 6 1 Introduction p a 51 6 2 The Chip Configurations issena i E E A E 52 6 3 RESTS OR e ra e a t Ges e pected a e aaea a ged aed ected eae 53 0 A CONCUSSIONS anaana a a a a e a aa S uer 59 7 0 Offline Analysis of Test Data from an SCT128B readout chip 61 Tb The Threshold Soa 2o dosi a a aa uet tive dos soko asa 61 7 2 The Basic Front End Parameters Gain Offset and Noise eeeeeee 62 doo JROSUTUS ios edo ime oett dea tuse osse E Ds cis rua etenim tL 66 7 4 Sources of possible misinterpretations due to the test procedure 71 Dod Evaluation uui ca eene bo DRE Ment chic ol a eec ud 73 PO AONE USO s deca Candeut Door E DO RO FU Oana m INS La deridet mds op PUE Nee 76 8 0 TESIDG ONY rier ienn a de Mehta bp a Rod Questar 71 DSL SMODVABION estet ec ui Oesaqe esa staclnaus ns V Sd Gu deu DDR em te M Een e ELT SEU TI 8 2 The 1997 HS Setup a io ess e oC OR UD stie deri ead ETSI AO E YU DNO deco eee 79 83 The HS DAQ RETO D DD E E T ai 80 8 3 1 The Read out Control Board cccccccccssecessscecessecessececesecesesaeceseaceesseesesesaeccseseeseseeeneaaees 81 5322 The TDC o nen ReneGeROn pee Iota medii ipd 82 9 4 The Treger Lotions nenen te oda e
2. e The cable side read strobe CRS is the path which the DAQ can drive a read strobe to the readout chips This is an unused feature in our specific setup The HAC output line is provided with both current mode CDI for low input impedance receivers and voltage mode CDV for conventional receivers sig nals The signals listed below are used for communication between the HAC and the readout chips These are the hybrid side versions of the fibre signals and one test con figuration signal for the readout chips Originally for use with the CDP128 there were an additional five test and configuration signals but these are not used with the SCT128B Hybrid Side Signals HCLKJ Hybrid Side Clock from HAC HTC Hybrid Side Trigger Control Signal from HAC HD Hybrid Side Data Signal from the Readout chips HRS Hybrid Side Read Strobe from HAC TEN Test mode Enable Signal from HAC 4 1 2 Registers and Logic The HAC Status Register consists of 48 bits where 32 are writeable and 16 are read only It includes the state of all counters error flags and programmable registers on the chip Executing a Clear instruction will set all the bits of the status register to zero The Status Register contains the following fields 26 27 May 1999 HAC Status Register DV 5 0 Input to programmable voltage source writeable DI 5 0 Input to programmable current source writeable RSA 1 0 X Read Strobe Algorithm selection re
3. If this information is not pre configured this must be done before 38 27 May 1999 the execution of ResMan ResMan also performs checks for errors ambiguities and undefined states It also displays this information information which includes their logical addresses assigned V XI address space locations self test status communica tion capability status of each slot protocols supported Commander Servant hierarchy and VMEbus IRQ InterRupt reQuest line allocation The VXI bus defined operations performed by ResMan can be summarized as follows e Identification of all VXI bus devices in the system e Management of the system self test and diagnostic sequence To make sure all devices have completed their self tests ResMan waits about 5 seconds before accessing any V XIbus device s configuration registers It then scans the V XI configuration space to locate and identify all the devices on the VXIbus including any mainframe extender devices that may be present in the system Configuration of the systems A24 and A32 address map ResMan determines the address space of each device by reading the device s ID register and allocates a section of appropriate type A16 A24 or A32 address space according to the size requirements set in VXIedit ResMan also determines an available base address for the device s address space Configuration of the systems commander servant hierarchy By reading the Protocol register of ea
4. _ Test Pulse it TET dep xe Offset ff RS p ysi NAL phchebon NN bocce SS pete NNINNE 0000 geese NNI NN petem cAgN SEN NG RA NEN aN R ei tee INNIXNI ene N N pana sal NNI PENN HEE 1 23 H LE SE ee ee i Bs be gl NNI NN Sot 15 channel FIGURE 40 Compounds of the signal arriving at the comparator 7 3 Results The testing procedure described above has been performed on the chip under test The results from these tests will be presented in the following The results are a part of my work at CERN and the chip under test is only an example 66 27 May 1999 1900 2000 3QoQ 2500 5000 7500 10000 200 200 400 600 1000 2000 200 200 400 300 200 1909 3000 2000 1000 E E 50 100 1 fC 507 points 20000 15000 10000 5000 all 50 100 1 5 fC 50 points OTETTA 1500 1000 500 50 100 2 fC 50 points MEERISY eee Tae 4000 2000 5 100 2 5 fC 507 points 1000 500 50 100 3 fC 50 points 0 i 250 500 750 5 100 4 fC 50 points 50 100 1 fC Sigmas 50 100 1 5 fC Sigmas E 50 100 2 fC Sigmas E 50 100 2 5 fC Sigmas m E 50 100 3 fC Sigmas 50 100 4 fC Sigmas 30 29 19 a a 2 4 1 fC all channels together e 80 69 40 gal E 29 M 2 4 amp 1 5 fC all channels together 2 199 75 50 25 E a H 2 4 2 fC all channels togeth
5. 1 nmx 1d 31 offsets I nh 1 nmx put vec con 30 mslop put vec con 31 moffs 1d 40 slopes II nh 1 nmx ld 41 offsets II nh 1 nmx put vec con 40 mpslop put vec con 41 mpoffs END Return MACRO scan vnew On error goto END kA gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt if lt 2 then mess vnew vector size typel endif if S Svexist 1 then v del 1 endif vvv 1 shift sss 1 shift v cr vvv sss Sunquote END Return 27 May 1999 93 MACRO scan getHlimmod On error goto END KS DDS gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt Get limits of histogram for v hfill gt gt gt gt gt gt gt gt gt gt gt KS DDS gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt
6. 82 27 May 1999 The Control Logic Time Out Counter starts The Control Logic waits until the Time Out Counter reaches a preselected Full Scale Time Range During this time an ECL pulse on any input stops the corresponding TAC section When the Time Out Counter reaches the full scale time the Control Logic starts the conversion sequence The output of the TAC sections are sampled The Control Logic checks if the sampled values are in the selected range eIf at least one value is within the range the sampled values in the range are converted and the 12 bit values are stored in the output buffer together with the channel number If no value is within the range no channels are converted and no data is writ ten to the output buffer The Busy is removed and the module is ready for the next acquisition In this specific setup the TDC is used to measure the time between the event trigger and the following clock pulse This is done by feeding the trigger from the scin tillators into the Common Start NIM input and a copy of the Clock into one of the ECL inputs Hereby we can choose the particles that traversed the scintillators in phase with the clock and hence will give maximum signal in the detector at readout 30 This selection of events is done offline 8 4 The Trigger Logic The event trigger is generated by a coincidence of the two scintillators in figure 51 This means that whenever both the two scintillators generate a sig
7. e Jt allows the voltages and currents to the front end chips to be monitored from the VME processor All supplied voltages and currents except detector bias supplies are readable from VME To be more specific all of the controlled voltages have a corre sponding monitored voltage and monitored current These are the voltages and currents readable from VME As mentioned above the monitoring of the detec tor voltages and currents requires the Farside plugin e Front Panel TABLE 1 BC96 Front Panel Connections Number Type Function SKI Lemo size 00 coax Power Interlock Input NIM level JP3 20 way IDC header Connections to SLL card SK2 Lemo size 0S 2 way Det HV A input SK3 Lemo size 0S 2 way Det HV B input SK4 Lemo size 1S 4 way Det HV output to detector module JP1 50 way IDC header Connections to detector module SK5 Lemo size 1B 4 way Vcc and Vdd feeds to det module 48 27 May 1999 In addition to the connectors in Table 1 the front panel accommodates a power switch to control the power to the front end and the on board circuitry supplying other voltages and signals to the front end this can also be done via the VME bus a power interlock input and LEDs to show the status and VME activity Like on the DSP onboard switches are used to set the A24 VME base address The only difference is that instead of an 8 bit DIP switch the BC96 has 3 hex switches that defines the VME base address A comprehe
8. gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt vO 1 id 2 nb 3 ns 4 tit 5 nx vdim v0 sigma mm vsum v0 nx sigma xx vsum v0 mm 1 2 nx sigma x2 sqrt xx sigma mx mm ns x2 sigma mn mm ns x2 i id 50 then id ELE nb 40 150 Q p id 51 then id BLE nb 200 100 id 61 then id tt nb 200 100 Q p id 62 then id tit nb 100 200 OQ pae id 63 then id tit nb 0 220 id 64 then id tit nb 0 300 OQ p id 65 then id tit nb 25 310 id 66 then id tit nb 100 400 id 71 then id tit nb O 400 Q p id 72 then id trt nb O 130 Q us id 73 then id tdt nb O 70 id 74 then id tit nb 5 15 H D H Bored Ea Mol Eee ETE dee dM Mode E nq eae E RUM pa dif i id 75 then 1 id tit nb 5 15 endif 3 id 76 then id trt nb 5 15 endif v hfill v0 id END Return 94 27 May 1999 MACRO fits hvec On error goto END KS DDS gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt KS DDS gt gt gt gt gt gt gt gt gt gt gt gt gt
9. gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt if 0 then mess hvec id nch opts mess I need a hist id exitm 1 endif if Shexist 1 0 then mess histogram 1 does not exist exitm 1 endif if Svexist hx then v del hx endif if Svexist hy then v del hy endif if Svexist hex then v del hex endif if Svexist hey then v del hey endif if lt 2 then nh Shinfo 1 xbins else nh 2 endif if lt 3 then opt n else opt 3 endif v cr hx nh r v cr hy nh r v cr hex nh r v cr hey nh r rebin 1 hx hy hex hey nh 1 S hinfo 1 xbins END Return opt 27 May 1999 95 96 27 May 1999 8 9 10 11 12 13 14 15 16 17 18 19 References http wwwlhcO01 cern ch April 1999 P E Gaarder Spesifikasjon og design av et utlesningssystem for et LHC eksper iment ved CERN Dec 1994 ATLAS Muon Spectrometer Technical Design Report CERN LHCC 97 22 June 1997 R K Bock The Particle Detector BriefBook Internet version March 1999 Liquid Argon Calorimeter Technical Design Report CERN LHCC 96 41 De cember 1996 Tile Calorimeter Technical Design Report CERN LHCC 96 42 December 1996 D Morgan et a
10. gt r ze il Riz rre BARREL 3 ome v TT 3 zi Pbi eS ros a ddr aun goo tnm 4 n S rd mo obo bm m s aw me um xe i i I I D PIXEL BARREL 2 POS ND SILICON BARREL PIXEL DISCS GALLIUM ARSENIDE SILICON DISC VERTEX BARREL 4 POS ND 4 POS ND 5 POS ND 9 POS hD H EC dI 1 ATLAS INNER TRACKER GEOMETRY ESL EIE dl DIMENSIONS FOR ENGINEERING STUDY acma WEED STEP FERE 8 cn maur ii gt FEMHUE ALL BUFFS DO NOT 4 TCE EEEE TEE pe CE E Y mex sure M ECTS sep ON E CCLRC s THE CENTRAL LABORATORY OF THE REHEMICH C LMCLLS RITIERKOID APPLETON LIEST CALTON d rosrsemieT FILES OF THIS DRAWING ARE ON THE wwwi SINNER TRACKER GEOMETRY P netpi omud ern ch _ pub etlae invegracion Incoming ps ne Fi CSN FUR J FILE NANE IT GEOMETRY M pe anas au ommers anc A 1 1B 0035 0B50 OdQ x TRADERE nemmeno FIGURE 13 The Inner Detector Geometry The main purposes with the ID are pattern recognition and track reconstruction but momentum measurements electron identification and tagging of b jets are also important issues Another important requirement besides the performance require ments is to minimize the amount of material in the Inner Detector This is crucial because of the deterioration of the calorimeter resolution according to an increase in the amount of material preceding the calorimeters This yields detectors electronics cooling system cables and support struc
11. idl 200 800 0 0 This text deserves an explanation Every line starting with a is ignored and are only comments The leftmost column resembles the amount of ones or zeros to add to the bitstream The middle column of zeros is just a spacer and have no effect on the result The character f or 0 in the rightmost column defines whether the amount of bits to be added to the bitstream is a series of ones or a series of zeros The f means and the 0 means 0 To give an example The bitstream defined as Clear HAC consists of three lines 52 27 May 1999 The bitstream will look like this 111100000000 four ones and eight zeros What effect does this bitstream have on the hybrid The first command sent is the above mentioned Clear HAC The Clear com mand clears the state of all counters error flags and readout chip bus control signals RS and FIRST to zero It also has the side effect of resetting the SCT128Bs As an extra safety precaution this is done twice The next command sent is the Write Status Register In response to a Write Status command the HAC shifts the next 32 values on the CTC line into the writeable parts of its status register These 32 bits are labelled Status Register Bits and are shown in detail in the table below Bits Value Effect RSA 1 0 01 Read Strobe generated from command to HAC HPR 9 0 1100000000 Header Pattern lowest order bit first ITEN 1 Test Mode enabled TEEN 1 Edg
12. xl Offset set smgu 0 opt nfit set mtyp END Return zslp mV f C zof mv 92 27 May 1999 MACRO scan del On error goto END K gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt DDD DDD D gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt KS DDS gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt close 0 h del 0 v del END Return MACRO scan xxx On error goto END K gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt DDD DDD gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt K gt gt D gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt DDD DDD DDD DDD DDD DDD DDD DDD DDD DDD DDD gt gt gt gt gt gt D gt gt gt D gt gt gt gt nh vdim mpslop nmx nh 1 1d 30 slopes I nh
13. 128 channels with depths of 132 bits The hit pattern from the input register is shifted through the pipeline during 132 clock cycles When a Levell trigger arrives the pattern from the pipeline output is written to the Readout buffer The slow command CLEAR resets the clock generator while the contents of the pipeline remain unchanged Readout Buffer The Readout buffer is a dual port static RAM array which is 128 bits wide and 9 words deep It holds hit patterns corresponding to each L1 trigger during readout allowed by the readout strobe There are 2 pointers which address the memory one for reading and one for writing allowing for simultaneous reading and writing The point ers are cleared by the slow command CLEAR This buffer serves as a derandomizer which removes the fluctuations from the L1 trigger distribution Output Register The Output register is a 128 bit parallel to serial shift register For each L2 trig ger the oldest data from the readout buffer are shifted to the output register and read out serially Control Logic The control logic is based on the concept used in the CDP128 and the HAC but compared to the CDP128 there are a few new functions which I have already men tioned The DACS for threshold control calibration amplitude and delay control for the calibration strobe are all new Modified software is therefore needed to make use of these functions The control logic comprises a 21 bit register e8 bits for
14. H8 Test Beam Setup The modules which consisted of two 62 x 61 6mm silicon strip detectors with 80 um pitch glued back to back and a hybrid holding the FE chips were placed with their strips vertically in cool box I and horizontally in cool box II These boxes have the combined task of shielding rotation and cooling based on a nitrogen flow The tele scopes and modules were placed on a board which could be rolled into a 1 56T magnet if desired The modules were operated at 7 C 25 8 3 The H8 DAQ The different DAQ modules are housed in one NIM crate and two VME crates The VME crates are connected via a VIC link which consists of a VME card in each crate and a cable between them When like in this particular test beam period the beam is used only for module testing and not for a system test this link is solely used for local intercrate communication In combined runs however where modules from several ATLAS subdetectors are tested in the same beam and the focus of the tests are on how well the different detectors work together the VIC cable bus is the basis for the event building system 25 The CPU in the VME crate is a RAID 8235 Redundant Array of Independent Disks which is a way of storing the same data in different places thus redundantly on multiple hard disks By placing data on multiple disks I O operations can overlap in a balanced way improving performance Since multiple disks increases the mean time between failure
15. a burst EOB TRANSFER mode or transfer of data event by event during the burst RT TRANSFER mode Data transfer in a calibration run is identical to the EOB TRANSFER mode Calibration is initiated by the message calibrate The number of triggers to acquire is set by the message parameter acqui events The DSP will control the start of burst and end of burst signals The DSP also generates the trig gers and calibration pulses pixels or executes a control block strips 5 4 1 The BC96 Bias Card The BiasCard96 is a major upgrade from the previous Bias Card It resides in a VME crate and works with the Binary DSP module with the appropriate LL personal ity card the SLL card One BC96 supports 1 double sided detector module and up to two of them are used with a single DSP SLL module 46 27 May 1999 BASE ADDERE Ho W W NI Scy VME I F VME Active amp Power On CONTROL Interlock CONTROL DRIVER REGISTER CARD PECL LVDS CONTROL VOLTAGES CURRENT SUPPLIES FIGURE 29 Block diagram of the BC 96 47 27 May 1999 ts main functions are e It routes the digital data stream from the support card to the SLL card The datastream arrives at JP1 and is routed unprocessed through JP3 and out to the SLL card t provides the various voltages needed by the analogue and digital sections of the front end and with the means of adjusting them These voltages include digital and analogue power supplies Vdd
16. and Vcc and a series of digital and analogue control voltages The supplies are fed to the chips through SK5 and the control voltages through JP1 e t offers a path to connect external detector bias supplies to the support card To complete this path a Farside daughter card or a few straps at the right places is needed The bias supplies are fed to the BC96 through the SK2 and SK3 one LEMO for each of the two sides of the double sided detector module and into the Farside plugin From there it can be routed two ways either through a LEMO that transmits nothing else than these bias voltages SK4 or by setting jumpers through the 50 way JP1 To be able to monitor the detector voltages and currents though there is no way around the Farside card t routes the digital control signals from the DSP SLL to the support card clock trigger calibrates While the older front end chips like CAFE CDP LBIC CDP SCT128B need control signals in PECL Positive Emitter Coupled Logic the ABC chip and the newer models ABCD etc will require LVDS Low Voltage Differen tial Signalling signals as well as a few other minor modifications The BC96 can of course only generate and transmit signals to the front end chips in one of these two modes Therefore the interface circuitry is on a daughter card which can be exchanged when necessary The driver card installed in our setup is since the chip under test is the SCT128B the PECL edition
17. chapter 5 0 a series of questions about what is important to know about a rea dout chip were raised and a series of requirements to its performance and functionality were presented In this chapter test data from a threshold scan of a single unbonded not connected to a detector SCT128B chip will be presented and analysed The data has been acquired with a VME based DAQ system clocked at 40MHz and read out by an SCT128B readout chip bonded to a hybrid with a HAC The analysis has been per formed using a set of PAW routines originally written by C Lacasta at CERN The KUMAC files in which the analysis is performed are presented in Appendix A without any comment Prior to the presentation of the results of the analysis the different steps in the testing procedure will be explained First the series of events that a threshold scan con sists of will be described 7 1 The Threshold Scan A range of calibration pulses of different sizes is chosen The sizes of these should of course be on the order of one MIP Minimum Ionizing Particle It is of no use if the sizes of the testpulses are fundamentally different from the charges ionized by a particle traversing a silicon detector in an experiment During a traversal of the 300 u m thick detector 22 000 electron hole pairs are created This results in 1 6x10 C x 220002 3 5fC deposited charge It is also of importance that the chip gives a reasonable response to charges lower than this to ensu
18. electronic noise This results in a signal which is statistically distributed in a Gaussian manner around the pulseheight see figure 38 pulses Pulse height FIGURE 38 Illustration of the signalheight variation 27 May 1999 63 By denoting the gaussian distribution in figure 38 P pulse height noise and normalizing it to 1 it describes the probability of an injection charge resulting in a cer tain pulse height The s curve will emerge when plotting F thr in the equation below thr F thr 1 P pulse height noise 0 To each s curve a fit with the shape of F thr is applied The threshold value that according to this s curve fit results in triggers in 50 of the events is called the 50 point and is since the distribution is gaussian equal to the pulse height The width of the distribution yields the noise the wider the distribution the noisier chan nel The noise is given as the standard deviation of the signal height distribution in figure 38 The gain of a channel is calculated by plotting the 50 values as a function of injection charge and applying a linear fit The slope of this line is the gain and has unit mV fC To put this in a more understandable way The fact that the 50 threshold which is equal to the signal height of the test pulse increases with increasing test pulse height is due to the chips ability to produce a response proportional to the amount of charge injected into the inputs of each chan
19. from the rest this causes a few non fatal incompatibilities between the HAC and the SCT128B The chip controls and buffers the bit stream from the readout chips adds a header with start code and trigger count detects certain error conditions timeout overflow under flow and drives the data line to the fibre optic header Stop Diode SCT1246 fille UWE AST He Hill He gt M FIGURE 19 Block Diagram of Readout System 27 May 1999 25 The signals listed below are involved in the fibre optic header to HAC connec tion These signals pass through the fibre optic link Cable Side Signals CCLK Cable side Clock from DAQ CTC Cable side Trigger Control Signal from DAQ CDV Cable side Data Signal voltage signals to DAQ CDI Cable side Data Signal current signals to DAQ CRS Cable side Read Strobe optional from DAQ e The clock CCLK is a pulse train with approximately 50 duty cycle and fre quency range from 100kHz to 60 MHz The design clock frequency for the elec tronics are as mentioned earlier 40 MHz The trigger control signal CTC is used by the DAQ to program both the HAC and the readout chips command certain actions such as calibration or status dump and the logical trigger signal of the physics experiment The data signal CDV in our case carries information header and hit pattern from the HAC and the readout chips to the DAQ
20. in a Read out Sequence Figure 20 shows the logical events in a read out sequence involving a hybrid with two SCT128B s Readout is initiated by the receipt of a pulse on the CTC line This is passed on to the hybrid followed by an HRS read strobe pulse When the HAC has completed transmission of the header containing start code and trigger count FIRST is asserted initiating the token chain The first SCT128B then unloads its 128 bit output register onto the HD line and then raises its NEXT signal This is the token pass to the second SCT128B in the chain labelled TOKEN in the figure The second SCT128B then unloads its output register When complete it raises its NEXT signal which since this is the last read out chip in the chain also is the END signal of the token chain When the HAC senses that END has been asserted it lowers FIRST ter minating the read out sequence for the corresponding trigger Bug List The Time Out flag is reset at the beginning of each read out sequence Because the Time Out flag is part of the header its resultant value for a read out sequence in progress is not known until after the header has been sent up the cable Therefore the TOF is always FALSE in a header Its actual value for a read out sequence can only be known by reading the status register after the read out sequence According to 10 there are four dead clocks between the header and the begin ning of chip data coming through the CD line Th
21. its performance is good enough to serve in a physics experiment This can be done in three different ways 1 After the detector is bonded to the hybrid populated with readout chips the test pulses are injected in the same manner as before This way the effects of the adding of capacitive load are very clear since the rest of the procedure is exactly the same as before the bonding The detector is exposed to a natural radioactive source while being read out by the front end chips This is a way of testing the module which can be executed in any lab The module is placed in a high energy beam between already working detectors with high spatial resolution The motivation for this kind of test and a short description of my work in the H8 Test Beam 97 setup will be presented in the following chapter This particular chip under test must already after this test be rejected primarily due to the very high offset spread Two non functioning channels and a relatively high noise and gain spread is also an indication of a bad chip since the addition of a capaci tive load which the bonding to a detector will imply will further deteriorate the noise and gain spread The procedure and analysis outlined in this chapter show however how a typical binary FE ASIC for the ATLAS SCT will be characterized and evaluated 76 27 May 1999 8 0 Testbeam This chapter will present a short description of my participation at the H8 test beam du
22. of millions of sensor elements and readout channels will be very demanding and the data bundling will be extremely complex In order to reach the high luminosity required 1074 cm s the LHC uses two counter rotating beams made up of 2835 closely spaced bunches of 1 1x10 particles each The luminosity L is defined as in the equation below where f denotes the col lision frequency N and N5 denote the number of particles in each bunch and A 47 0 0 is the beam cross sections at the collision point 2 NN A Dr The LHC will consist of two colliding synchrotrons installed in the 27 km LEP tunnel They will be filled with protons delivered from the SPS and its pre accel erators at 0 45 TeV Two superconducting magnetic channels will accelerate the pro tons to 7 on 7 TeV after which the beams will counter rotate for several hours colliding at the experiments until they become so degraded that the machine will have to be emptied and refilled The basic layout of the accelerator features eight straight sections each approxi mately 528 m long available for experimental insertions or utilities The two high luminosity insertions are located at diametrically opposite straight sections point 1 ATLAS A Toroidal LHC ApparatuS and point 5 CMS Compact Muon Solenoid Two more experimental insertions are located at point 2 ALICE A Large Ion Collider Experiment and point 8 LHC B B physics This layout is s
23. pb200c300 pb200c400 npts SWORDS files v cr calp npts r 11 5 22 5 3 4 lun 20 do i 1 npts lun lun 1 SWORD files i 1 mess ff hbook ff h file ae f hbook vnam fc i If Ds A then v del fc i endif v cr vnam 128 r get vec con lun lun 20 fc i sigma vnam vnam vnam fcmod i if vexist vnam then v del fcmod i endif v cr vnam 128 r vscale fc i 100 vnam sigma am vnam vnam fe i if pio o OMA then v del fe i endif v cr vnam 128 r get vec con lun lun 21 fe i sigma vnam vnam vnam femod i if vexist vnam then v del femod i endif v cr vnam 128 r vscale fe i 100 vnam sigma vnam vnam enddo if vexist ch then v del ch endif if Svexist eh then v del eh endif 27 May 1999 87 nh 0 do i 1 128 id 1000 i hrin id if SHINFO id sum gt 0 then nh nh 1 endif h del id enddo mess nh active channels found v cr ch npts nh v cr eh npts nh if Svexist modcalp then v del modcalp endif if vexist modch then v del modch endif v cr modcalp 4 r v cr modch 4 128 f exec scan vnew par 3 3E exec scan vnew mpslop nh r exec scan vnew mpoffs nh r x0 1l k 0 do i 1 128 id 1000 i hrin id if SHINFO id sum 0 goto otro k k 1 do j 1 npts v inp ch j k femod j i v inp eh j k femod j i enddo do 121 4 m 1 2 v in
24. software readable 6 differential ECL direct output lines software controlled Temperature sensor 4 DIP switches software readable 3 LEDs software controlled 42 27 May 1999 Low Level 256E x 22 Level Connecto Vete i R AW Connector 320031 DSP Piggyback lt Connectors gt upplementat ow Level SUPLL onnector for TCC Quad DAC Direct Output Connector FIGURE 26 DSP Overview As shown in figure 26 the three I O connectors are HL LL and PB and they are each meant to support a card The HL card is the VME interface of this system while the LL card SLL in this setup is the interface to the detector or module The Piggy Back connector is designed for the TCC Trigger Control Card which is used to handle external triggers in the H8 testbeam The HL card is a VME bus interface card and contains 2Kx32 dual port RAM and some logic This dual port RAM can be accessed simultaneously by the DSP and the VME bus The DSP can be reset and interrupted via the VME bus and the DSP can generate a VME bus interrupt The SLL card contains the drivers receivers logic etc necessary to interface the DSP card to the silicon strip detector module It also holds the shift registers FIFOs and logic for the 40 MHz serial stream from the silicon strip readout chips 27 May 1999 43 LL Data Bus 0 MHz Senal Links Prograrunable Output FIFO A M Delay Calibration D50 ns 8 from modules Input FIFO
25. storing data redundantly increases fault tolerance A RAID appears to the operating system to be a single logical hard disk 26 To manage the run control and monitoring there are two SUN workstations run ning real time UNIX and a simple serial text terminal with 32 Mb memory for install ing and booting of the RAID This terminal runs EP LX which also is a variant of UNIX 1 The strips on one of the detectors are actually rotated 40 mrad with respect to the other on each mod ule 80 27 May 1999 Some of the hardware setup is similar to that described in chapter 5 0 and which was used in the Oslo Uppsala lab setup Each module is provided with a bias card and a DSP They handle the readout and control signals and the depletion of the detector Instead of by the SEQSI module the clock is provided by a TCC card which is plugged directly onto the piggyback connector on the DSP motherboard It also performs clock conversion and synchronization of external triggers to the DSP clock as well as featur ing a programmable trigger delay 27 The analogue telescope modules are read out by IRAM modules which are also VME modules instead of the Binary DSPs Since the details of the telescopes are beside the point of this chapter this will not be discussed any further 8 3 1 The Read out Control Board The Read out Control Board is also a VME module and is called RCB 8047 CORBO This section summarizes the most important points from 28 and
26. the data is limited to probing directly on the data link with the oscilloscope The Front end parameters like gain off set and noise can therefore not be tested Oscilloscope screenshots printed out with a plotter and then scanned into a GIF file will be presented as illustration The system is initialized and configured as described in chapter 5 0 and the clock is provided by a programmable pulse generator The DSP driver is downloaded into the UCI DSP card using the Sheffield LabDaq v1 0 Labview software package As mentioned above this DSP software is insufficient to unpack the data from the hybrid For cooling a small fan is used as well as an aluminium plate directly beneath the hybrid and in contact with the beryllia The hybrid used in our setup is a beryllia Oslo hybrid populated with 6 SCT128B chips and a HAC chapter 4 0 It is interfaced to the BC96 by a PCB which routes all the different signals between the HAC and the 50 way cable connected to the BC96 The HAC SCT128B configurations and the triggers are also downloaded using the LabDaq v1 0 by sending controlblock files to the hybrid in loops They are sent in loops to be able to see on the oscilloscope whether the response from the hybrid is stable or fundamentally different from time to time The system proved to be very dependant of the clock frequency The plots throughout this chapter will therefore be acquired with somewhat varying frequencies About the oscilloscope plots I
27. with potentially different offsets the offset variation will be a source of further spread in pulse heights To get a better view of the channel to channel spread of the 50 points and the noise it is illustrative to make the following plot Divide the 1st axis which now repre sents the 50 threshold and noise respectively into intervals and plot the number of channels with 50 thresholds or noise within this interval along the second axis Such plots are shown in figure 42 for each injection charge 68 27 May 1999 uci Ana 85 01 Sem PEE 2645 1413 30D 1fC noise 190 0 100 200 0 50 100 1 5 fC 50 points ALLCHAN 1242 fmf 20 11 Constont B424 Maan 1288 ma 0 1005 o 100 20D 3090 6 8 16 12 14 2 5 fC noise 100 200 300 6 8 10 12 14 3fC noise o 0 x 100 200 300 400 6 8 10 12 14 440 50 points 4fC noise FIGURE 42 Spread of 50 thresholds and noise 27 May 1999 69 Comparing these plots to the ones in figure 41 there is one thing which must be mentioned The spikes in these plots are deliberately left out by restraining the histo gram limits to values expected from normal channels since these will have the effect of corrupting the illustrative effect of the plots However it is important to note that there are such strongly deviating channels and the parameter ALLCHAN in the statis tics boxes show the number of channels inside the limits of the histogra
28. 1999 1 D Rif io spao AULT iste fb dj H8 po PP n 2d eijeedbenditegpesedeenieedernd enn f E l E LINC tle bel bre 19 735 0ns At 2 110 0ns 1 At 9 091MMz The 4 bit Read Strobe counter is a part of the header In these two plots this counter is enclosed by the cursors From the top plot to the bottom plot we can see that the counter is increased by 1 from 1001 to 1010 Also note the dead clocks between the header and the datastream 27 May 1999 57 toca lesse eoe vo heres rer ert POR dee te deae te bets ps tegede Ee eed a te Peseta prgugrpegatoie 4 gt DIT 24 sl r xb 3e i as vassaa 4 P t thee d tree eee a mee E E P x E en m M svete j a N nee a H t ines Kew aes STs qm HE E dn b 1 3 fox i E a d 1 EI 4 Dd 1 H M t M teat t i a eae bara 2LIN f Dod i ot Doc 1 H ti 13 735 t2 At 4 260u5 1 At 23A 7kHz FIGURE 34 L1 trigger This plot features the only statistics our setup was able to produce The line LINK is as mentioned before the result of a single readout sequence The additional line scopel is a trigger count averaged over the last 256 readout sequences and since the mask register was set t
29. 3 The software is not running There is no point in reading out an event if it is not recorded by the software This signal is activated when a run is started and deactivated when the required amount of events is acquired This is also an out put from the CORBO When we denote the discriminated signals from the scintillators as S1 and S2 and VETO is defined as VETO out of spill OR software busy OR software not running an ACCEPTED TRIGGER can be expressed as the following ACCEPTED TRIGGER S1 amp 52 amp NOT VETO The detailed trigger scheme is shown in figure 53 Discr Coincidence Scint 1 Si g East Coinc 52 lo Prompt Iz Veto el LF ssa Dual Timer Stact of Burst SPS Timing Repeater Fanout SPSE EE Looms End of Burst Dual Timer SPS WE 2 65 Dual Timer Global Busy FIGURE 53 H8 Trigger Scheme based on 30 8 5 Conclusions The information from module testing in a lab including both source tests and pure electrical testing is limited Therefore the need for module testing in a high energy particle beam is present A DAQ system in the H8 area has been set up to exploit the SPS beam spill for this kind of module testing 84 27 May 1999 9 0 Conclusions The main purpose with this project was to set up a test system for evaluation of binary front end electronics to test such electronics and analyse the test data The test syst
30. Binary Readout System for a Silicon Tracking Detector at LHC Eirik Olsen May 27 1999 Thesis submitted to the Cand Scient Degree Department of physics University of Oslo Binary Readout System for a Silicon Tracking Detector at LHC Eirik Olsen May 27 1999 Preface The project described in this thesis has involved many persons In particular I wish to thank my supervisor and spellchecker Steinar Stapnes for his guidance and direction and for sharing his knowledge about the best pizza and pasta spots in the CERN area In addition my fellow student Suleyman Azman deserves acknowledge ment for his cooperation throughout a substantial part of this work Further I wish to thank Gisle Midttun Bj rn Magne Sundal and Peter W Phillips for sharing their com petence in the laboratory Introduction aoo oen comedi t has dude E ee Re tee 1 POC Neto sas H 3 VD P L 3 1 2 The standard Model ode io de eel to o p taeda eee 5 2 0 The ATLAS Detector eeeeeettenttentennttnntens 7 2 L he Mio Detectors ite Una eti Gro e aca odadatedtt ise etate 8 2 1 1 Th Precision Charnbers neret eret reete nere rere ehe PEE eth deer E enden 10 21 2 The Tris Ser Chambers et Ree errem coner mte liie odere ier e pet 10 2 1 3 Performance Physics Requirement 2 0 0 0 cess eeceeceeeeeeeeeeecaeeseecaeesaecaecsaecnecsaeeeeeseeerens 11 2 2 The Calorimeters 4 aee ct tee ative teo nee lair Dad ee eri icai
31. E 47 Channel 33 Clearly this is a channel which is not working well since it regardless of the size of the test pulse gives triggers only at very low thresholds A possible explanation to this is that the test pulse is obstructed on its way to the comparator somewhere between the input and the comparator the line is corrupted in such a way that the result is a big resistor The resulting s curve histograms do not look like s curves at all and the 50 thresholds give no meaning since all of them are extracted from the earlier mentioned linear fit The resulting values for gain and offset are therefore also mean ingless There are 2 of these defective channels 33 and 43 According to 18 the chip was designed to have a gain on the order of 100 mV fC A mean gain of 81 mV fC is therefore a low but reasonable result A spread in gain of 6 1 rms is relatively high but not alarming To evaluate the noise it is useful to convert the values to Equivalent Noise Charge which is done as follows 7A 27 May 1999 noise 1 ENC gain Qelectron The performance of a binary readout system with a common threshold for many channels is determined both by the noise performance of a single channel and the spread of gain and offset The noise requirement is according to 19 a total ENC 1500 electrons after the detector is bonded This includes the pure electrical noise in each channel the spread in offsets and the detect
32. FIGURE 8 Overview of the muon system indicating where the different chamber technologies are used 2 1 3 Performance Physics Requirements When designing a detector there must exist a set of rough guidelines for the dif ferent requirements for the detector a general idea of how it should work and what it should discover For the muon detector these can be summarized as follows e Like the rest of the LHC the muon detector must feature the largest possible discovery range of both expected and unexpected physics t must provide a good discrimination against difficult background conditions e Stable operation during the anticipated lifetime of the LHC is required Although ATLAS is a general purpose pp detector it is impossible to be equally sensitive to all the possible varieties of new physics The discovery potential of the muon detector is therefore optimized with certain benchmark processes in mind Standard model and supersymmetric Higgs decays i e H ZZ 4 1 and H 5 ZZ 4l e New vector bosons i e Z gt UU and W gt Vult eSemileptonic b and t decays i e b ux CP violating processes The full description of the ATLAS Muon Spectrometer can be found in 3 This section summarizes the basic concepts 27 May 1999 11 2 2 The Calorimeters A calorimeter is a composite detector using total absorption of particles to measure the energy and position of incident particles or jets In the process
33. It can also be done for the whole chip to get an impression of the mean characteristics of the chip The efficiency along the 2nd axis is then a mean efficiency In the figure below such s curves for the 6 different injection charges for one channel channel 22 from the chip under test are presented Channel 22 1 1 0 75 0 75 0 5 0 5 0 25 0 25 g D 250 590 0 250 500 D 250 500 S curve 1fTC S curve 1 5fC S curve 21C 1 1 0 75 0 75 Q 5 5 0 25 0 25 o 250 500 0 250 500 i 0 250 599 S curve 2 5fC S curve 3fC S curve 4fC FIGURE 36 S curves for channel 22 for various injection charges 7 2 The Basic Front End Parameters Gain Offset and Noise One might ask why these curves are s shaped and not with a sharp edge at the threshold level corresponding to the pulseheight See figure 37 for an illustration of such an ideal and hypothetical curve 62 27 May 1999 Efficiency Pulse height Threshold mV FIGURE 37 Plot of Efficiency vs Threshold in an ideal case Both the size of the testpulse and the threshold in the comparator are certainly defined with an accuracy too good to create such an efficiency spread At first sight there seem to be no reason for this spread provided that the size of the signal that reaches the comparator has the same size every time The latter is not the case The rea son for this spread is that the signal arriving at the comparator is a superposed signal consisting of the testpulse and some
34. ND KS DDS gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt KS DDS gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt zone 1 1 set mtyp 20 opt nfit set smgu 0 45 npts vdim ch 1 if S vexist par then v del par endif v cr par 3 r nfit 4 npts 1 if Svexist modcalp v del modcalp endif then if vexist modch then v del modch endif v cr modcalp 4 r v cr modch 4 128 do i 1 4 k i 2 r v inp modcalp i calp k l do j 1 128 v inp modch i 3 ch Ik 31 enddo enddo opt utit title channel 1 v fit modcalp modch v pl modch 1 npts sigma gain par 2 Le nfrit u 1 1 pl qw 2 par 1 1 1 modcalp ps sigma offset par 1 zslp Sformat gain 1 F6 2 zoff format offset 1 F6 2 mess gain zslp mess offs zoff xl ch 6 1 15 x2 x1 10 set txfp 02 set chhe 4 set txal 13 itx 2 x2 Gain itx 2
35. P 1 but then the signal must be differential ECL 44 27 May 1999 decide captures a fixed length data block once a header is detected The GAL could alternatively be programmed to capture some types of variable length data blocks Software The software is also designed with one part common to all detector types the system software and one part which is detector specific Communication between the VME CPU In this case it will be the VME MXI2 card and the DSP is primarily done by exchange of messages Messages are transmitted to the dual port memory of the VME interface I O memory which is part of the DSP card This I O memory is mapped and accessible from both the VME CPU and the DSP The DSP also supports a set of 32 bit flag words which can be directly accessed by both the DSP and the VME CPU The DSP for example maintains a flag word that represents the current DSP state idle gathering data etc and monitors another flag which the VME CPU can set to abort data acquisition The flags will primarily be used to monitor and control the DSP especially during debugging The DSP s boot loader loads the boot code from the EEPROM into the appro priate section of the SRAM The code is then executed The DSP reads blocks of code passed by the VME CPU from the dual port RAM and loads them into the appropriate sections of the internal RAM and the SRAM It then starts execution of the code loaded which includes setting some flag
36. TIE Dirt te Phyngir Husl arw ot Cnm Me NEVE MG mamme ae 2O2070P3 FIGURE 16 Structure of the SCT Barrel Section Silicon is because of its fast signal speed and excellent spatial segmentation used as the detector material here but there are a lot of other considerations for a well working detector system than just the properties of the detector medium and the basic detector units A lot of practical problems must also be taken into account 20 27 May 1999 The expected lifetime of the SCT is 10 years at full luminosity and during that time one cannot expect to have too much access to the inner detector Therefore we must minimise the need for maintenance and repair and hence make the design as reliable as possible The Silicon detectors the front end electronics the hybrids and the cables must be cooled with a specially designed cooling system using binary ice This is to minimize the leakage current and the effects of radiation induced doping changes and to remove heat generated by front end chips and DC voltage drops The thermal expansion of the material in the support structures must be as small as possible to ensure the exact locations of the modules The temperature variations can be up to 30 C 3 3 2 Modules A module consists of 2 pairs of daisy chained detectors each with an active area of 61 6x62 0 mm 1 pair is aligned on each side of the module with the back side detectors rotated by 40mrad to the fr
37. alibration Amplitude Pulse Amplitude Charge Injected via a 100 fF capacitor Range 0 160 mV 0 16 fC Resolution 0 625 mV bit 0 0625 fC bit 4 A DAC for threshold control The threshold is determined by a differential volt age applied either from external pads VT1 VT2 or from this internal 8 bit DAC These DAC circuits comprise internal voltage references The range of the threshold DAC is 640 mV with a resolution of 2 5 mV bit 27 May 1999 31 4 2 3 Registers and Logic Input Register The Input Register has 2 functions edge sensing of signals delivered from the discriminators and channel masking For every hit detected by a discriminator only a single pulse of duration 1 clock period is provided regardless of the time response from the discriminator The channel mask register is used for disabling bad or noisy channels so that the data from these are not written to the pipeline To mask a channel one must set the corresponding bit in the mask register to 1 In Test mode selected by the TEN signal the mask register can be used to apply test patterns to the pipeline The mask register is loaded serially Pipeline The binary pipeline is designed as a multiplexed FIFO circuit in which an array of nxn dynamic memory cells are controlled by n non overlapping clock signals In each clock cycle only n cells out of nxn are switched while the effective delay provided by such a block is equal to nx n 1 clock cycles The pipeline has
38. amp Input FIFO amp Input FIFO amp Input FIFO to from iiim DSF module 8 4 es a ae DSP s DAC Outputs FIGURE 27 SLL Overview The SLL card handles 4 trigger control links and 4 calibration links both to the detector modules and 4 data links from the modules The rising edge of the calibra tion lines can be delayed with up to 50ns with 8 bit resolution A 40 MHz TTL clock signal CLK arrives on the SLL card from in our setup from a programmable pulse generator In testbeam this clock is provided by the TCC A delayed version of this clock is transmitted to the modules via the digital connector JP8 This delay may be adjusted via a twisted pair cable between JP6 and JP7 The SLL sends both CLK and a serial bitstream to the trigger control link driver This serial bitstream contains both trigger and control information To send control information the DSP writes the control bitstream into the output FIFO on the SLL A single 2K x 8 FIFO is used for all trigger control links as well as the four calibration controls so var ious bitstreams may be sent to all links simultaneously Data arriving from the data link receiver are first passed through an adjustable delay and then into an 8 bit shift register A GAL decides when the data in the shift reg ister should be clocked into a 2K x 8 FIFO The current method the GAL uses to 1 It is also possible to feed the clock into the Direct Inputs Connector on the DSP card J
39. ay 1999 37 with the program called ResMan which is a system initialization program executed on power up or after a backplane reset see below The VME system uses the Resource Manager only to initialize the hardware interface between our computer and the VME bus Unlike VME devices VXI devices have a unique logical address which serves as a way of accessing the device Since VXI uses an 8 bit logical address it is possible to include up to 256 VXI devices in a VXI system In this specific setup there are only two the PCI MXI 2 and the VME MXI 2 The configuration registers which is required for all VXI devices enables the system to identify each VXI device its type model and manufacturer address space and memory requirements The V XIbus specification defines a Commander Servant communication proto col which can be used to construct hierarchical systems with conceptual layers of VXI devices A commander is any device in the hierarchy with one or more associated lower level devices or Servants A Servant is any device in the sub tree of a com mander Every VXI module has one and only one commander Since VME devices do not support the VXI defined concept of a Commander Servant hierarchy it does not apply to VME systems Our setup therefore consist of one Commander the PCI MXI 2 and one Servant the VME MXI 2 The NI VXI utilities used in our setup are the three application programs VXI init a VXIlocal hardware initialization p
40. ch message based device ResMan finds all Commanders and their associated Servants It also supports the VXI inter rupt TTL ECL Trigger and Utility bus extension e Allocation of the VME bus IRQ lines The last thing ResMan does before initiating normal system operation is to allocate the VMEbus IRQ lines among the various interrupt handlers and inter rupters in the system e Initiation of normal system operation The Startup Resource Manager is a superset of the VXI bus defined Resource Manager Therefore ResMan also supports some more extensive capabilities Multiple mainframe support using standard VXI bus mainframe extensions Support for dynamically configured devices on a pr mainframe basis e Integration of non VXI VME and pseudo V XI devices on a pr mainframe basis using the VXIedit utility VXIedit VXIedit is a collection of interactive editors which serves as an adjunct to ResMan and are used to configure the system hardware and maintain the VXI information databases Each of the editors in VXIedit generates a database table used by ResMan when configuring the VXI system With this informa tion ResMan can associate names and numbers with the bits encoded in the device s registers and display information about system status during initializa tion 27 May 1999 39 The different editors and displays Resource Manager Display This display displays the ResMan table which contains informati
41. ch will be described more extensively in the two chapters to come and its solenoid the Calorimetry part which is divided into hadronic and electromagnetic subsections and the Muon Detectors at the outermost of the ATLAS detector 27 May 1999 7 2 1 The Muon Detector The only particle in addition to the neutrino that is not completely stopped by the calorimeters is the muon The muon is a Lepton with a mass 200 times the electron mass and has no hadronic interaction Since the cross section for bremsstrahlung which is the dominating type of energy loss at this part of the energy scale is inversely proportional to the square of the particle mass the bremsstrahlung cross section for the muon compared to the electron is reduced by a factor of 40 000 In other words the probability for stopping the muon with the calorimeter is vanishingly small To exploit the physics signature potential of high momentum final state muons an additional tracker in a magnetic field is built outside the calorimeters namely the muon detector FIGURE 5 The muon detector are arranged in 3 layers around the calorimeters and the inner detector The most important role of the muon detector is to reconstruct and identify the muon tracks measure their momenta and provide information to be matched with data from the inner detector Muon tracks are identified and measured after passing through about 2m of material lead LAr scintillators and Iron in the calor
42. charge number of the incident particle and x Xq is the thickness of the detector in radiation lengths To illustrate the point let an electron with the above mentioned maximum end point energy traverse a 300um thick silicon detector Since one radiation length in sil icon is 9cm this angle of deflection turns out to be 0 18 radians or 10 degrees The direction of the particle trajectories are then deflected to such an extent that the paths from the source to the other side of the detectors are not straight lines see figures 49and 50 and it is impossible to know which strips are actually hit and which are not In turn this makes it impossible to know how many triggers to expect from each strip and efficiency and position resolution are impossible to calculate 1 The spectrum of energies available to the electron ranges between 0 and the total energy of the decay 3 54 MeV It is most probable for the neutrino and the electron to carry away about the same amount of energy so the spectrum is peaked at mid energies 27 May 1999 77 Rh Source Telescope DUT Telescope Scintillator FIGURE 49 Irradiating a module with a 106Rh source Beam Pipe F peMeD MEE ii 180 GeV pio Telescope DUT Telescope Scintillator Scintillator FIGURE 50 Irradiating a module with protons from an accelerator 78 27 May 1999 Note that the modules labelled Telescope are not used in the source test They ha
43. ciencies at very low thresholds are not as high as could be expected from intuition namely 100 and from the fact that this efficiency is 100 for higher thresholds with the same charge injected 27 May 1999 71 0 8 0 8 0 6 OE Q 4 Q 4 Q 2 0 2 J o Q 200 409 600 0 200 400 600 channel 1 channel 2 0 8 0 6 Q 4 0 2 Q 200 4090 BOO D 200 400 600 channel 3 channel 4 FIGURE 45 4fC s curves As shown in figure 45 the efficiency does not reach 1 until the threshold is raised to about 50 mV in any of the channels When operating with very low thresh olds all channels are firing all the time the ones not receiving the test pulse are trig ging on noise This is a completely unphysical situation which causes overload problems for the chip and it starts to oscillate This makes the output a bit more unpre dictable A glance back at figure 41 shows as mentioned that a lot of the 1fC 50 thresholds are negative Of course interpreting this without any critical sense is useless since the test procedure contains no usage of negative thresholds What happens is merely the fact that these 1fC s curves rarely reach 50 effi ciency or too few thresholds result in high efficiencies such that the resulting histo gram at best looks like the tail of an s curve Furthermore since the lowest thresholds are corrupted due to the earlier mentioned oscillations these s curves do not even qual ify as a such a tail In such cases it i
44. ctive ones and is characterized by a decrease in V referred to as beneficial annealing A high temperature is an advantage for this process At longer time scales V pg increases due to the transformation of defects into active acceptor sites described as the anti annealing period A low temperature is preferred to slow down this process A more detailed study on the subject can be found in 7 This section summarizes some of the basic points Within the barrels all modules are identical but in the disks the modules require a wedge like shape which will not be discussed here 27 May 1999 21 3 3 3 Detectors The detector consists of p strips on n type substrate 0 2 mecrohi 3 C l mictoh AL om unplant icm cons 300 ime bans ty pe 5i crystal T unplant Llimetean Al FIGURE 17 Layout of a p in n type Si microstrip detector With a binary readout of the detector the resolution is a function of the readout pitch and is given by the variance o f a x dx of a uniform probability distribution f x with width Pitch where f x is normalized such that a 2 fl SE r Pitch This results in a variance o Taking the variance o as the resolution 12 of the detector and given the pitch of 80 um and the binary readout of individual strips we have a point resolution in b of 234m The sign less than is used since a small percentage of the traversing particles the ones traversing nea
45. cts of the SCT oper ation This is necessary due to the inaccessibility of the system 27 May 1999 23 The readout electronics use a binary readout strategy This means that instead of reading out the whole shape of the signal collected by a strip a discriminator fires a hit no hit signal depending on the amount of charge collected by the strip A hit is regis tered when the amount of charge collected exceeds a certain preset value The output is then stored in a pipeline until a trigger initiates a readout for that particular event Amplifier Discriminator Fipeline Buffer Readout Analog hn s E FIGURE 18 Figure of the Front end Electronics logic Front End FE electronics are the electronics between the detector and the Rea dout Driver and has the following different functional components 8 e FE analogue or analogue digital processing LVLI buffer in which information analogue digital is stored and is retained long enough to accommodate the LVL trigger latency e Derandomizer in which the data corresponding to a LVL trigger accept are stored before being sent to the next level To obtain a low noise performance the FE electronics must be mounted directly on the silicon strip electrodes This means that these electronics must be in the active volume of the detector which in turn sets a constraint to the mass and power consump tion of the FE electronics Another requirement for maintaining a stable and satisfyin
46. d none 896v aln Aa ve Prem tte nae bras osoattldummeos proh un n o 0 An a rsoewmovtvhtanyvues atsev zov maua rvv nppee Beare ane tere ETTET gt a a P n etvwoe fetohhnmansbovtvoreves PETORESEHE TERE TFA PASO PERE OE eee DEP EEE ee 4 9 ootteesvuantsus sh hb aseanuoettan sss Deecrrarrthu ptetasesv stsocetoormmmtttittt on Ee ti 7 805ms t2 7 880m At 3 830u8 1 At 261 ikHe FIGURE 32 Close up of the rightmost bitcluster the SCT128B Setup on the CTC line from the HAC Reset plot 27 May 1999 55 This plot is also a close up of a part of figure 30 It shows the part of the plot where the second cluster of bits is being sent to the hybrid the SCT128B configura tion part H M t gt H d ti il 13Ous t2 3i 77us 36 54us 1 At 32 84kHz FIGURE 33 L1 Trigger In figure 33 the response from the hybrid is shown when a single L1 trigger is sent without any test pattern applied Again the structure with a header and a datast ream enclosed by the cursors is evident This plot was acquired with a clock fre quency of 25 MHz so the At 30 64u s duration of the datastream output equals 766 clock cycles This is again due to the earlier mentioned HAC bug report a reasonable result for a readout sequence of a 6 chip hybrid 56 27 May
47. e Mode enabled CT 0 No Clock through CC 0 Normal Phase default Before the configuration of the SCT128Bs a long series of zeros is sent Then the first thing done is choosing calibration line 3 Secondly the DAC amp Delay Register is set to the maximum threshold and maximum calibration amplitude Note the x010x combination in this register setting The last thing done is applying a test pattern with 128 ones by setting the Mask Register to 128 ones 6 3 Results The first plot is simply showing the above described configuration file being sent 27 May 1999 53 M ugs d 4 7 907ms t 21 8605 1 68t 45 75kHe srrvtttt n ae H 1 P r a t M 1 basiss FIGURE 30 Overview of the HAC reset This plot shows an overview of what happens when we send the controlblock file HAC reset at a clock frequency of 35MHz and temperature 26 3 C As the two next plots will show in more detail this contains the commands HAC reset Set Con trol Register for the HAC and set DAC amp Delay register followed by set mask register for the SCT128B The HAC commands are separated by a few 0 s from the SCT128B commands This is done for easier visual inspection of the plots and has no practical function As one can see on the Data line the hybrid gives some sort of response to our commands even though there is nothing at first sight in the controlblock file that
48. e pixel detector are determined by the per formance requirements and the desired lifetime of each part of the system These can be summarized as follows excellent pattern recognition in high multiplicity environment excellent transverse impact parameter resolution and 3D vertexing capability excellent b tagging and b triggering capabilities e lifetimes of about 3 years at reduced LHC luminosity 10 ems and 1 year at design luminosity 10 4 cm 2s for the innermost barrel the B layer e lifetimes of about 7 years at design luminosity for the rest of the pixel detector 18 27 May 1999 3 2 The TRT The TRT surrounds the pixel and SCT system and are aligned both parallel and perpendicular to the beam direction It consists of layers of straw detectors where each straw is a cylindrical gaseous drift chamber with a diameter of 4mm The TRT is designed as 1 barrel with 52 544 axial straws of about 150cm length and 2 end cap parts with 319 488 radial straws of 39 55cm length The intrinsic radiation hardness and the low cost compared to other large volume tracking solutions made this com bined straw tracking and transition radiation detecting system very practical The price to pay for these advantages is however a high detector occupancy with the 370 000 straws and the 420 000 electronic channels FIGURE 15 Layout of the TRT Detector This system provides almost continuous tracking at large radii in the Inner Detector du
49. e to cope with the demanding rate and background conditions In the barrel region the chambers are arranged in 3 cylindrical layers around the beam axis while in the end cap and transition regions the chambers are aligned vertically also in 3 layers or stations Each MDT detector plane is made of 2 multilayers of pressurized AI drift tubes while the CSC s are multiwire proportional chambers 2 1 2 The Trigger Chambers A Levell muon trigger is a rough muon pj measurement derived from 3 trig ger stations Each station is made of 2 3 in the TGC s planes of strips or wires with X and Y read out The trigger is based on a coincidence between a strip or a wire hit in the Ist station and a range of strips wires in the 2nd and 3rd station The trigger chambers are also responsible for bunch crossing identification The trigger chambers use Resistive Plate Chambers RPC s in the barrel region and Thin Gap Chambers TGC s in the end cap region and together they cover the region n lt 2 4 The trigger chambers also provide a second coordinate measurement of the track position along an axis parallel to the MDT wires and in a direction parallel to the magnetic field lines The trigger chambers are fast but have a coarse spatial res olution The RPC s are gaseous parallel plate detectors while the TGC s are multiwire proportional chambers 10 27 May 1999 Cathode Sip Resisiive Plate Chambers Monitored Drit Tube Chambers
50. e to its many measurement points each particle hits on the average about 36 straws This makes the TRT a powerful tool for pattern recognition The perform ance requirements can be summarized like this tracking detection of transition radiation e good ability to trigger high p muons at Level2 together with the EM calorimeter contribute to the electron identification e momentum measurements precise measurements in the R plane 27 May 1999 19 To obtain this performance the analogue front end readout electronics operates with 2 thresholds One low about 200ev for detecting MIPs Minimum Ionizing Parti cles and one high 6 7keV for detecting transition radiation photons X rays 3 3 SCT The SCT consists of Silicon microstrip detectors These detectors have success fully been used as tracking devices the past years but due to the hostile conditions at LHC at full luminosity 109 cm b challenges connected to radiation damage scale and readout procedures arises I will concentrate only on the readout procedures and general performance here 3 3 1 General Description The SCT modules are aligned in 4 cylindrical central barrels and 9 forward and 9 backward disks with a total sensitive area of 50m de CONNECTOR OPTICAL FIBERS MATH PIGTAILS CONNECTOR CARBON FIBER SPRING PIGTAIL SUPPORT GARBIER knELE NL mi BRACKET MOQULE FIXATION SERVICESIAXO VIEW omer gi WHI WERSI
51. e to read out anything from the status register while the working limit for all other commands was 36MHz Remembering that the design frequency is 40MHz for this system this needs some investigation 6 4 Conclusions The plots show that the system is able to produce reasonable responds from the hybrid and as far as to unpacking the data it is a functioning DAQ system for binary readout However a few problems caused by the fact that the HAC and the SCT128B are not 100 compatible are evident The combination x010x in the SCT128B config uration bitstreams is interpreted as a Levell trigger and a readout sequence is initiated The main problem however is the temperature Without any cooling of the hybrid we experienced that as soon as the temperature exceeded 31 32 C the hybrid stopped responding to our commands and we had to wait until the temperature dropped below this critical level before we were able to proceed with our tests With a simple fan as a cooling system we managed to keep a stable 26 27 C operating temperature which was good enough to produce the plots presented throughout this chapter How ever the system was still very frequency dependent since for frequencies exceeding 36 MHz there was no response from the readout chips For a for a system to run steadily at design frequency a better cooling system is needed 27 May 1999 59 60 27 May 1999 7 0 Offline Analysis of Test Data from an SCT128B readout chip In
52. eda 12 2 2 1 The Electromagnetic Calorimeter essere 13 2 2 2 Fhe Hadroni Calorimeter ien ient ERG HE 15 3 0 The Inner DelecIOr enceinte pto mta td tested ale 17 3T The Pixel detector uei eit det reet trei eir ea ede Ghee 17 3 2 bhe TR BE m 19 SM SG pec CEN 20 3 3 General Description 2 eaa nU POR rp HS 20 S MAN On cT 21 3 3 3 Detectors iie E peter tere et ee tede e eee reete de FR tes 22 EE Michiel EE REES 23 3 3 3 BIeCtfOnICS ois ve cos tases ett e toti ert T m d e RO E RESET NIST E TA Cea o o Goss eo eed 23 4 0 Read Out Electronics een 25 4 1 The HAC H ader Adder Chip iex ieecs uu eset ee eee een eo qe aee 3n ede e RUE eec Re en eun 25 4 1 1 Architecture sucer e i eter tono rese ee ea e ete e Ree ele Qe VES eo e We ERE red d 25 4 1 2 Registers and LOg1C reete ote eee EEE E EEEE e theo 26 AVS ReadoUt s see eere t tib e eerte p eee Ro ote eerte Ex PS UE 28 T2 SCTIZSE Lie eer E 30 4 2 T Architecture uet e nn an e cet eet Ea ee dre e e dates e te exe ERE S 30 42 2 Bront End ire Re en eet te pent egt ee intor reget 31 4 2 3 Registers and Logic iens eae r ei DE E ER ER 32 4 2 4 Levell and Control Commands eeseseeeseseseeeeeeee enne nee nennen nens 33 5 0 The System Setup for Module Measurement 35 5 1 The VXI VME eXtensions for Instrumentation System sss 37 33 QC
53. em setup which is more thoroughly described in chapter 5 0 is a VME based system with a DSP a BC96 and a pulse generator SEQSI residing in the VME crate With the VME PCI8000 interface and the VXI software package from National Instruments this system is controllable via a PC To manage the testing and launch the control block files the LabDaq v1 0 labview package from Sheffield was used With the setup described in chapter 5 0 we experienced some difficulties get ting data out of the readout chips By probing directly on the Data line from the hybrid to the BC96 with an oscilloscope and sending our commands in a loop we were able to see how the chips on the hybrid responded The HAC responded reasonably to our commands but the SCT128Bs did not respond at all This could be an effect of several parameters No cooling of the hybrid was used so the temperature is a natural field to improve Also the clock provided by the SEQSI module was of poor quality The hybrid was then moved to a similar setup in Uppsala where the tests were continued In chapter 6 0 we showed that the system is able to produce reasonable responds from the hybrid and as far as to unpacking the data is a functioning DAQ system for binary readout However a few problems caused by the fact that the HAC and the SCT128B are not 100 compatible were evident The combination x010x in the SCT128B configuration bitstream is interpreted as a Levell trigger and a readout seque
54. er e 199 50 9 o 2 4 2 5 fC all channels together nm 1900 50 s o 2 4 3 fC all channels together a 0 2 4 6 4 fC all channels together FIGURE 41 50 points and noise for each channel and all channel s curves for each injection charge 27 May 1999 67 The first column of plots in figure 41 shows the 50 points for all the channels on the chip and for each injection charge The unit on the second axis is milliVolt mV eA lot of the 1fC and some of the 1 5fC 50 thresholds are negative This will be discussed at a later time The second column shows the noise in each channel The unit along the second axis is mV e Some of the plots are not very informative because of some very noisy chan nels The third column is a collection of s curves for all the channels together and one for each injection charge Note that 100 efficiency here means that all the channels gave triggers in all the events at that particular threshold The curve is not normalized and 10096 efficiency equals 128 in this plot As for single channel s curves the 5096 threshold increases as the injection charge increases but the transition from 100 to 0 efficiency is a lot wider In other words the pulse height distribution is much wider This is due to the fact that it is no longer just the noise that causes the widening of this distribu tion When merging data from 128 different channels into one plot all channels
55. eractions and the photons created in this process are absorbed in the presampler The measured photon energy is then added to the corresponding particle This presampler consists of an active LAr layer of l 1cm in the barrel section and 0 5cm in the end cap section 27 May 1999 13 Towers in Sampling 3 ApxaAy 0 0245 0 05 Ru quate towers in Sampling 2 FIGURE 10 Layout of the EM barrel calorimeter and LAr accordion geometry The barrel part which is contained in a barrel cryostat surrounding the inner detector cavity consists of two identical half barrels The EM end caps are divided into two coaxial wheels and are also contained in cryostats together with the end cap and forward hadronic calorimeters See figure 12 To ensure an acceptable level of high energy shower containment the total thickness of the EM barrel is at least 24 X thick and at least 26 Xy thick in the end caps The full description of the ATLAS LAr Calorimeter can be found in 5 This section summarizes the basic concepts 14 27 May 1999 2 2 2 The Hadronic Calorimeter The hadronic calorimeter consists of three main parts the barrel the end cap and the forward calorimeter FIGURE 11 The plastic scintillating tile The barrel part is subdivided in a central barrel and two extended barrels The sampling technique used here uses plastic scintillating plates or tiles shown in the figure to the left embedded in an iron absorber T
56. es the computer to the VXIbus and the VMEbus backplanes The VME MXI 2 is a single slot double height VMEbus device with optional VMEbus System Controller functions It uses address mapping to convert MXIbus cycles into VMEbus cycles and vice versa The VME MXI 2 automatically determines whether it is located in the first slot of a VMEbus chassis and if it is the MXIbus Sys tem Controller 5 3 VME VME is an acronym for VersaModule Eurocard and is a widely accepted back plane interconnection bus system developed by a consortium of companies led by Motorola now standardised as IEEE 1014 12 It provides power mechanical support cooling and a backplane for intermodule communication Communication via external cables are of course also possible A VMEbus board can be either single or double height A single height board is 100mm x 160mm with one 96 pin DIN 41612 connector called P1 on the rear that plugs into the backplane A double height board is 233mm x 160mm and may have a second 96 pin DIN connector named P2 A single height board is also known as a 3U and a double height a 6U The backplane can have up to 21 slots providing the J1 connectors for the boards to plug into The J2 connectors if required can be supplied with a second backplane board or in one piece with both J1 and J2 connectors A J1 on the back plane matches to a P1 on the board and a J2 to a P2 Power is supplied to the VME bus board through P1 and P2 if u
57. explains how the module is used in the H8 setup This VME module handles up to 4 event inter rupt signals and it takes care of VME interrupt generation event counting Dead Time generation and control The interrupt signals the CORBO receives as inputs in this spe cific setup are event triggers Start Of Burst triggers SOB and End Of Burst triggers EOB The event triggers are generated from a coincidence of two scintillators and SOB and EOB triggers are provided by the SPS Timing Repeater The details of the trigger logic are expounded in chapter 8 4 The CORBO module houses 4 identical and independent channels Each of them contains a TRIGGER input a BUSY output two VME interrupt generators and two counters one Event Counter used to count the TRIGGER inputs and the other to measure the BUSY width Dead Time Counter The main use described on the flow chart of figure 52 is the following When the trigger input occurs a BUSY signal is asserted as well as a VME interrupt The Event Counter is incremented by one and the Dead Time Counter starts counting Slow Clock signal 100us The BUSY signal will remain active until it is cleared by a VME access As long as BUSY is asserted no other trigger is accepted The content of the Dead Time Counter gives a measure of the BUSY active time e If the BUSY remains active too long a VME interrupt is sent 27 May 1999 81 TRIG INPUT Y Asset BUSY se IT N IT_ACK Inc
58. g operation is that noise pick up discriminator performance and threshold are well con trolled One of the most challenging aspects of the SCT design is the compromise between optimizing performance parameters noise efficiency bandwidth reliability and minimizing power consumption amount of material and cost The full description of the ATLAS detector can be found in 9 This chapter is a summary of the most important points 24 27 May 1999 4 0 Read Out Electronics Up until now I have given a quite general description of the ATLAS detector From now on this thesis will present a more detailed description of one specific solu tion of the readout electronics This solution is outlined in figure 19 4 1 The HAC Header Adder Chip A comprehensive presentation of the HAC is found in 10 This section sum marizes the most important points 4 1 1 Architecture The HAC is the local cable interface and readout sequence manager for the rea dout chips on a hybrid It is designed to receive control signals from a fibre optic header electrically buffer and decode these control signals and trigger readout sequences from a bank of chips In our case this will be the SCT128B chip which facil itates both the preamplifier shaper discriminator circuitry and the binary pipeline in one unit However since the HAC was originally designed only to serve the pipeline part CDP128 of the older readout system where the pipeline was separated
59. gister writeable HPR 8 0 Header Pattern Register writeable TD 3 0 Test mode Data Register writeable TEN Test mode Enable read only EEN Edge mode Enable read only TOF Time Out Error Flag read only OFF Read Out Buffer Overflow Flag writeable UFF Read Out Buffer Underflow Flag writeable RS 3 0 Read Strobe Counter read only CC 1 Compliment Hybrid Clock Control Bit writeable CC 0 Compliment Latch Clock Control Bit writeable CT Clock Through Control Bit writeable BOR 8 0 Buffer Occupancy Register read only When writing to the status register 32 bits must be supplied via the CTC signal following the Write Status command When reading from it 48 bits will be asserted serially on the CDV signal in response to the Read Status command The read strobe signal is produced according to one of three algorithms an externally supplied RS RSA 1 0 0 an RS generated from command to HAC RSA 1 0 1 and a locally generated RS RSA 1 0 2 The option in use in our setup is RSA 1 an RS generated from command to HAC To decide the read strobe condition the HAC uses a string of 9 flip flops called the Buffer Occupancy Register BOR This register keeps track of the SCT128B read out buffer For every trigger received one flop is set and for every read strobe one flop is cleared If all flip flops become set and an additional trigger arrives the OverFlow Flag OFF is asserted This indicates that data has been overwritten in the SCT128B s 9 eve
60. gnets bend the tracks while in the transition region between it is a combination of these two FIGURE 7 Three dimensional view of the superconducting air core toroid magnet system The right hand end cap magnet is shown retracted from its operating position The requirement of the best possible transverse momentum resolution that is constant over a large pseudorapidity range leads to the choice of an open geometry system of superconducting toroidal magnets The magnet system consists of three air core superconducting toroids figure 7 designed to produce a large volume magnetic field covering the pseudorapidity range 0 lt n 2 7 with an open structure that mini mizes the contribution of multiple scattering to the momentum resolution 27 May 1999 9 2 1 1 The Precision Chambers The momentum of a charged particle can be determined from its deflection in a magnetic field To be more precise it is proportional to the radius of the curvature of the track The track is measured in 3 stations and in each station several layers of detectors measure the position and direction of the track Two different techniques are used to acquire the high precision track coordinate measurements The Monitored Drift Tubes MDT s are used over most of the pseudor apidity range while close to the interaction point and at large pseudorapidities the Cath ode Strip Chambers are used due to their higher granularity This makes the CSC s more suitabl
61. he tiles are aligned perpendicular to the beam direction and staggered in depth To provide a good hadronic shower containment and minimize punch through for the muon system the thickness of the calorimeter is an essential param eter The total thickness of the barrel calorimeter EM tile at 0 is about 9 2 absorption lengths This is sufficient to achieve a good reso lution on high energy jets The total amount of Coble tao material in front of the muon system is 11X including outer support and is enough to reduce the punch through to an acceptable level In the end caps and the forward calorimeters where a higher radiation resist ance is needed the more radiation hard LAr technology LAr is easily replaced during operation is used The hadronic end cap calorimeter is a copper LAr detector with parallel plate geometry It consists of two separate wheels with equal diameter and together they have 12A active material Hadronio detectors eruo Faedthroughs FIGURE 12 A more detailed view of an end cap cryostat with its content 27 May 1999 15 The forward calorimeter is a dense 9 A in a rather short longitudinal space LAr detector consisting of regularly spaced longitudinal channels filled with rod elec trodes in a metal matrix It consists of three longitudinal sections The first one is in copper the other two are in tungsten The sensitive medium LAr fills the gap between the rod and the matr
62. hown in figure 1 These latter straight sections also contain the injection systems The beams cross from one ring to the other only at these four locations ALICE is a heavy ion colliding experi ment while both the CMS and ATLAS are proton proton colliding experiments 27 May 1999 3 Low 8 pp High Luminosity Octant3 s B physics FIGURE 1 Schematic Overview of the LHC Accelerator LHC is as mentioned a synchrotron and therefore a three step accelerating machine e An alternating electrical field of RF frequency 400MHz boosts particle bunches with 25ns spacing that is Every tenth RF bucket is filled e Dipole magnets of 8 36T bends the tracks Superconductivity makes this pos sible This is the ability of certain materials usually at very low temperatures to conduct electric current without resistance and power losses and therefore pro duce high magnetic fields For comparable power consumption the LHC can delivery 25 times the energy and 10 000 times the luminosity of the SPS col lider Quadropole magnets and other multipole magnets are used to collimate the beam To achieve a high luminosity the point is to keep the bunch of particles as focused as possible the cross section of the bunch as small as possible In order to achieve the desired magnetic field strengths the magnets need to be operated at a temperature as low as 1 9K In all LHC cryogenics will need to cool down 31 000 tons of material and
63. ile up effect due to the high rate and particle fluxes and minimise the effect such a pile up could have on the physics performance Extreme radiation resistance capabilities are also required because of the 10 year at least operation time in this hostile environment The calorimetry is divided in two main parts The electromagnetic and the hadronic calorimeter The EM calorimeter is mainly sensitive to electrons and photons through bremsstrahlung and pair production which dominate at high energy while the hadronic calorimeter is sensitive to hadrons The main tasks of the ATLAS calorimetry are e accurate measurements of the energy and position of electrons and photons EM calorimeter measurement of the energy and direction of jets Hadronic calorimeter measurement of the missing transverse energy of the event EM Hadronic calorimeter e particle identification i e separation of electrons and photons from hadrons and jets and separation of t hadronic decays from jets event selection at the trigger level 2 2 1 The Electromagnetic Calorimeter The EM calorimeter consists of a barrel and two end caps and is a lead Liquid Argon detector with lead absorber plates and accordion shaped kapton electrodes It is preceded by a presampler detector which task is to correct for the energy loss in the material upstream of the calorimeters the inner detector the cryostats and the coil This energy loss is due to bremsstrahlung int
64. imeters in total 11A absorption lengths in the barrel region and 12 in the end cap sections The measurements start at 5m from the IP and extends over a distance of 5 10m The muon detector is a high precision spectrometer with stand alone triggering and momentum 1 This is not completely true since high energy particles of different flavours can punch through the calorimeters and be part of the background radiation in the muon detector 8 27 May 1999 measurement capability and covers a wide range of transverse momentum pseudora pidity and azimuthal angle The pseudorapidity n at a space point is Se iut defined as n In tan0 2 where 0 Hh is defined as the angle between the line between this space point and the Interac J i tion Point and the beam axis as shown in figure 6 on the left The particles are symmetrically distributed in and in hadronic collisions the particle density is more or less proportional with n 1 T Beam Axis z FIGURE 6 Definition of the spherical coordinates Q and 0 The system consists of high precision tracking chambers and separate trigger chambers operating inside a magnetic field generated by large superconducting air core toroid magnets The magnetic deflection of the muon tracks in the pseudorapidity region n 1 0 is provided by a large barrel magnet surrounding the hadronic calo rimeter In the pseudorapidity region 1 4 n 2 7 two end cap ma
65. is means that the first four bits from the read out chip will be lost For the CDP these were taken from the column code and did not result in any loss of data However for the SCT128B which does not provide such a column code four bits of data will be lost FIRST is not lowered for 17 clocks following END This leads to some waste of time but should not cause any loss of data 27 May 1999 29 The hybrid side output signals from the HAC are not defined during a write sta tus register operation Stabilizing these signals during this operation would be an advantage to prevent disruption of the read out chips during status register writes 4 2 SCT128B A comprehensive presentation of the SCT128B is found in 11 This section summarizes the most important points 4 2 1 Architecture The SCT128B chip is a 128 channel integrated circuit for binary readout of sili con strip detectors for the ATLAS SCT designed for the DMILL technology The preamplifier shaper discriminator circuitry and the binary pipeline are both imple mented in one single chip To be able to use it in an already existing readout system the back end and control logic are compatible with the architecture of the previous ver sion CDP128 and the HAC The block diagram is shown below PETIT C oc u ugz nurj PLFELINE R e 8 1 5 1 e t Toa cm ga Co oo Ds d L1 Le CLK TEN FIGURE 21 Block Diagram of SCT128B 30 27 May 1999 4 2 2 F
66. ix The forward calorimeter is also integrated in the end cap cryo stat with its front about 5 meters from the interaction point Due to the high level of radiation this makes it an especially challenging detector It provides however signifi cant advantages for the forward jet tagging and the g miss measurements The full description of the ATLAS Tile Calorimeter can be found in 6 This section summarizes the basic concepts 16 27 May 1999 3 0 The Inner Detector The ATLAS inner Detector covers the pseudorapidity region n 2 5 and is composed by 3 main parts the TRT Transition Radiation Tracker the Pixel detector and the SCT SemiConductor Tracker 7 I Y I z I z Y z 7 EI I 7 I L3 7 I ri I Li I I IB 0035 060 00 M acr QO EF mmm mnm n EES Aa Tee RE RREN S ae pap wine AERE Par Geste VS MN PI LEARANCES BARREL MD FORWARD SERVICES S PU MI ze b CRYOSTAT fu cin ek sham Aor Tu LLL 384 5 EL gm m NS TAT J A Ef teri here pore WN tera ES P rere EA REUS rs REC SH EP EPI EE S EE E m f Ar E mal gju ism Benz sre E pm Bou D lens h p m 3
67. l Annealing of Irradiated Silicon Strip Detectors for the ATLAS Experiment at CERN 10 sept 1998 Atlas Trigger DAQ Steering Group Trigger amp DAQ Interfaces with Front End Systems Requirement Document v2 0 ATLAS Internal Note DAQ NO 103 09 June 1998 ATLAS Inner Detector Technical Design Report 1997 J DeWitt Header adder HAC Chip 1995 SCT128B Binary Readout Chip for the ATLAS SCT Project description Rev 1 0 The Free On line Dictionary of Computing 15Feb98 R J Boys 1996 January 5 Version 9 http www ee ualberta ca archive vme faq html S Pier The UCI DSP Project 1997 B Schmid Pixel Strips DSP Card Software 1995 http www hep phy cam ac uk atlas biascard96 html The BC96 users manual 1997 Dabrowski Anghinolfi et al A Single Chip Implementation of the Binary Re adout Architecture for Silicon Strip Detectors in the ATLAS Silicon Tracker 1997 ATLAS Inner Detector TDR 1997 20 21 22 23 24 25 26 27 28 29 30 31 Dabrowski Kaplon et al SCT128B a Prototype Radiation Hard Chip for Binary Readout of Silicon Strip Detectors 1997 http tweedledee wonderland caltech edu derose labs tabis html May 1999 Physical Review D Particles and Fields July 1996 Part1 P Allport et al ATLAS silicon strip beam results 2nd Intern Symp on Devel opment and Application of Semiconductor Tracking Detectors Hiroshima Ja pan Oct 10 13 1995 http www fys uio no epf a
68. m If a more detailed information about the deviating channels is desired the plots in figure 41 will give an idea of this After calculating the gain and offset of all the channels this information can be summarized in the plots of figures 43 and 44 500 D m ur I Puna Lena y 250 490 500 750 500 1000 ie 1250 1500 ida 1750 2000 Q 2250 0 50 100 D 50 100 Gains Offsets FIGURE 43 Gains and Offsets for each channel These plots show the gain and offset as a function of channel number and are also suffering from loss of informativity due to two strongly deviating channels How ever figure 44 shows the distribution of gains and offsets when the biggest spikes from figure 43 are left out The mean gain value is 81mV fC with a spread of 5 1mV fC rms 6 396 The offsets are centered around 16mV with a spread of 28mV rms 70 27 May 1999 net 14 22 5 1637 2781 nat 1267 mean 20 175 15 12 5 10 75 2 5 i D 50 75 100 125 159 200 100 gains offsets FIGURE 44 Spread of Gains and Offsets 7 4 Sources of possible misinterpretations due to the test procedure As some of the plots have shown the chip under test is apparently not in perfect condition This is partly due to the test procedure partly due to the chip itself In the following this will be investigated further and explanations to these irregularities will be given As the reader probably have noticed the effi
69. n most plots there are 3 different lines included The top one labelled 0 BCO shows the clock and is in some of the plots totally superfluous since the time base on the scope is so large that the BCO line is not showing anything with any accuracy anyway In other plots it is quite useful however so it is included in most of them if not for anything else just to get an idea of the time base The second line labelled 1 CTC reflects whatever we write to the hybrid CTC is short for Cable side Trigger Control and monitors the signals arriving at the HAC The bottom one labelled 2 LINK is the Data Link and shows the response from the hybrid Whether it is the HAC or the SCT128B responding depends on the command sent 27 May 1999 51 6 2 The Chip Configurations Prior to every plot the HAC and SCT128Bs are initialized and configured by sending the controlblock file HAC reset cb reset HAC Set Data Mode Header 110 xxx xx Set Up HAC Set Up SCT128B 1111 Generate LlTrigger Irt Clear HAC 4 0f 400 400 aS Clear HAC 4 0f 400 400 ee Write status register 4 0f 200 0 f 0 0 lg E Status register bits 7 0 0 2 Oe E L 0 0 10f 400 2 0 3E 500 idl 200 000 0 Set Up SCT128B repeat calLink commandlink bb 3 4 0f 100 S Qf 000 Use Set Control Register d QE 0 0 80 f 0 0 L O f 000 yp Set Mask register 136 0 0 0
70. nal greater than a preset threshold with just a few nanoseconds in time difference a trigger is gen erated One out of two things will happen with this trigger 1 The trigger initiates a readout of all modules and all telescopes and raises a BUSY signal on the CORBO which persists as long as the readout procedure takes Due to the slow analogue readout of the telescopes this time is equal to the time it takes to read out these telescopes 2 The trigger is VETOed This means that the DAQ system for some reason is not ready to perform a new readout sequence and the trigger does not result in any thing A trigger can be VETOed for three reasons The trigger is out of spill This means that the trigger arrived at a time inbe tween two bursts In other words The trigger arrived when no particle from the beampipe possibly could have traversed the scintillators since we know there was no beam Such a trigger can be caused either by cosmic particles or noise there is still a small probability for noise triggers even when there are two scin tillators This signal is an output from a dual timer and is an information pro vided by the SPS Timing Repeater The software is busy reading out another event and does not accept a new trig ger until the readout sequence is complete This signal is handled by the CORBO and is activated every time a new trigger is accepted and deactivated when the readout sequence is complete 27 May 1999 8
71. nce is initiated The main problem however was the temperature Without any cooling of the hybrid we experienced that as soon as the temperature exceeded 31 32 C the hybrid stopped responding to our commands and we had to wait until the temperature dropped below this critical level before we were able to proceed with our tests With a simple fan as a cooling system we managed to keep a stable 26 27 C operating temperature which was good enough to produce the plots presented throughout chapter 6 0 How ever the system was still very frequency dependent since for frequencies exceeding 36 MHz there was no response from the readout chips For a for a system to run steadily at design frequency a better cooling system is needed In chapter 7 0 test data from an SCT128B readout chip was analysed and the chip was evaluated on background of design specifications and performance require ments The test procedure the Threshold Scan requires some care when analysing the data When operating with very low thresholds the efficiencies are not as high as could be expected from intuition namely 100 and from the fact that this efficiency is 100 for higher thresholds with the same charge injected The reason for this anomaly at low thresholds is that all channels are firing all the time the ones not receiving the test pulse are trigging on noise This is a completely unphysical situation which causes overload problems for the chip and it starts to oscilla
72. ndications of poor chip quality since the add ing of a capacitive load will further deteriorate the noise and gain spread The procedure and analysis outlined in chapter 7 0 show however how a typical binary FE ASIC for the ATLAS SCT will be characterized and evaluated However a well func tioning front end chip also needs to undergo tests with a detector bonded to it before a final conclusion can be made about whether its performance is good enough to serve in a physics experiment These extended tests can either be performed in the same way as before the bonding they can involve a radioactive source that irradiates the modules or the module can be placed in a high energy beam The information from module testing in a lab including both source tests and pure electrical testing is limited Therefore the need for module testing in a high energy particle beam is present A motivation for the need for extensive module testing in a high energy beam was given in chapter 8 0 and a DAQ system in the H8 area was set up to exploit the SPS beam spill for this kind of module testing This system was described in the same chapter Throughout this thesis I have concentrated solely on the SCT128B readout chip This chip is just a prototype and will not be used in the ATLAS detector The new ABCD chip has a design which is much closer to the final version Perhaps the direct applicability of what is achieved in this thesis is somewhat limited because of this bu
73. nel The gain is a measure of this propor tionality factor 64 27 May 1999 349 Gain 88 06 mV fC Offset 6 93 mV 320 3QQ 280 260 249 220 200 189 150 2 2 25 2 5 2 75 3 3 25 3 5 3 75 4 channel 22 FIGURE 39 Calculating gain and offset for channel 22 from the 50 point vs inj ch plot As shown in figure 39 only a selection of injection charges are used in the cal culation of the gain and the offset The 1 and 1 5 fC 50 points are deliberately omit ted which will be explained later Another characteristics of each channel which is appropriate to mention at this stage is the offset By extrapolating the straight line resulting from the linear fit it intersects the 2nd axis at x 0 that is injection charge 0 at a certain point This point is called the channels offset and resembles an intrinsic DC voltage level in the channel Clearly this will also have an effect on the size of the signal being discrimi nated The offset value is added to the test pulse and the noise and this total signal is discriminated against the fixed threshold in the comparator see figure 40 The spread of offsets from channel to channel can also be viewed as a spread in the effective threshold Effective thr thr set by software Offset and as explained in chapter 5 0 this is an effect to be minimized 27 May 1999 65 Total signal MY arriving at the PEN HW 1 RN comparator lt lt Noise
74. ns Inter mainframe trigger configuration is used to define which triggers will imported from or exported to a particular mainframe Utility Bus Configuration Editor This editor defines inter mainframe configurations for the utility bus Inter mainframe utility bus configuration is used to define whether some system interrupt conditions SYSRESET SYS FAIL and ACFAIL will be imported from or exported to a particular main frame 5 2 The VME PCIS000 interface The VME PCIS000 interface links any computer directly to the VMEbus and consists of three parts the PCI MXI 2 interface board residing in the PCI slot of the local CPU the VME MXI 2 the VME card in slot 0 of the VME crate and the cable between these two cards 40 27 May 1999 The PCI MXI 2 is a PCI compatible plug in circuit board that plugs into an expansion slot in a PCI based computer It links the computer directly to the MXIbus and vice versa Because the PCI MXI 2 uses the same communication register set that other VXIbus message based devices use other MXIbus devices view the PCI MXI 2 as a VXIbus device The PCI MXI 2 can also function as the MXIbus System control ler which in our system it is and can terminate MXIbus signals directly on the PCI MXI 2 The MXIbus Multisystem eXtension Interface the cable and connectors between the PCI MXI 2 and the VME MXI 2 is a high speed communication link that interconnects devices using round flexible cables MXI coupl
75. nsive description of the BC96 can be found in 16 and 17 27 May 1999 49 50 27 May 1999 6 0 Hybrid Evaluation With the setup described in the previous chapter we experienced some difficul ties getting data out of the readout chips By probing directly on the Data line from the hybrid to the BC96 with an oscilloscope and sending our commands in a loop we were able to see how the chips on the hybrid responded The HAC responded reasona bly to our commands but the SCT128Bs did not respond at all This could be an effect of several parameters No cooling of the hybrid was used so the temperature is a natu ral field to improve Also the clock provided by the SEQSI module was of poor qual ity To continue the tests the hybrid was moved to Uppsala and tested in a similar setup 6 1 Introduction The main purpose with this chapter is to show that our setup works as far as get ting the DSP to unpack the data that is It is possible to communicate with the chips on the hybrid and probe the response from them with an oscilloscope This chapter will show that it is possible to reproduce the expected responses from the chips on the hybrid It will also show a few problems caused by the fact that the HAC and the SCT128B are not 100 compatible further explanations will be given later It is not however possible to produce much information of statistic character due to the lack of DSP software control and the fact that our view of
76. nt read out buffer If none are set and a read strobe occurs the UnderFlow Flag UFP is asserted This indicates that an unwritten buffer location is being read from The HAC also detects the time out condition by using a 10 bit time out counter This counter starts counting from 0 when FIRST is asserted and if it reaches 1024 clock cycles before the END signal arrives at the HAC the Time Out Flag in the HAC status register is set and FIRST is lowered The CC1 and CCO status bits allow adjustment of relative timing between clock data and clock hybrid side control signals respectively The CC1 bit allows adjustment of the relative phases of the hybrid clock and hybrid control signals and the CCO con trols which edge of the clock cycle data is latched into the HAC from the hybrid The CT status bit is used to put the HAC into Clock Through mode This means that if this bit 1s set the HAC drives the clock as received back out the CD line 27 May 1999 27 Commands The HAC decodes four commands from the CTC line These are initiated by sending the sequences listed below through the CTC line The Clear command clears the state of all counters error flags and readout chip bus control signals RS and FIRST to zero eIn response to a Read Status command the HAC shifts out the state of its 48 bit status register onto the CD line eIn response to a Write Status command the HAC shifts the next 32 values on the CTC line into the w
77. ntext The following chapters will therefore give a brief introduction to CERN and LHC chapter 1 0 and a more detailed description of the ATLAS detector chapter 2 0 its Inner Detector and the SCT system chapter 3 0 Then the work with my project the evaluations and a conclusion will be presented 27 May 1999 1 27 May 1999 1 0 CERN CERN the European Laboratory for Particle Physics is the most important research centre for experimental particle physics in the world CERN is a gigantic accelerator centre for nuclear and particle physics sited right outside Geneva in Swit zerland The most important activity at CERN the last years has been the LEP Large Electron Positron collider a ring shaped accelerator with a circumference of 27km 1 1 LHC Inside the LEP tunnel a new collider is being built the LHC Large Hadron Collider A detailed description of the LHC project can be found in 1 This section briefly summarizes the most important points Before the opening of the LHC in 2005 there are still a lot of technical problems to overcome These problems arise mainly from the much stricter requirements to the LHC detectors compared to the LEP detec tors The extremely high collision rates 20 collision every 25ns at LHC requires very fast detectors and readout electronics This must be achieved without fatal loss in effectivity signal noise ratio The much higher luminosity requires radiation hard detectors Synchronisation
78. o 0 s for all channels before the L1 trigger was sent the trig gers hence give us an idea of the relative noise levels chip to chip and channel to chan nel It s not too difficult to separate the chips from each other in this plot As one can see the noise level differences from one chip to another are quite significant To clarify this point 4 26us x 30MHz 128 clock cycles channels that clearly has a much higher trigger rate than the neighbouring channels are enclosed by the cursors It is not too presumptuous to guess that these enclosed channels belong to the same chip 58 27 May 1999 I I TERM jr ejbeojenbeebesejsdisefen i H x 2L1N i H r 4 f E wy P td oe 1 ti 320 0ns te 1 37008 At 1 050u8 1 At 952 4kHz FIGURE 35 Read HAC Status Register The command being sent here is the Read HAC Status Register 1111 0001 The frequency was 25MHz and the temperature was 25 9 C This is a 48 bit register so never mind the meaningless cursors The reason why this plot is included is not to go into detail in the contents of this register but just to have an apt illustration to a dis cussion of the somewhat strange frequency and temperature dependency As a matter of fact this mis feature was especially evident for this particular command For fre quencies over 30MHz it was impossibl
79. of absorp tion showers are generated by cascades of interactions bremsstrahlung and pairpro duction Characteristic interactions with matter e g atomic excitation ionization are used to generate a detectable effect via particle charges The result of a series of statis tical processes is more predictable when the number of processes are large The basic phenomena in showers are statistical processes hence the intrinsic limiting accuracy expressed as a fraction of total energy improves with increasing energy as 4 AE 1 x E JE The calorimeters will play an essential role in ATLAS and at the rest of the LHC Since they have the advantage of improved relative resolution with increasing energy in contrast to magnetic spectrometers the LHC energy scale makes the calo rimeters very powerful and suitable detectors The ability of detecting Higgs bosons depends heavily on the calorimeter performances Most decay modes have final states that will be reconstructed mainly in the calorimeters ATLAS Calorimetry EM Accordion Calorimeters Hadronic Tile Calorimeters Forward LAr Calorimeters Hadronic LAr End Cap Calorimeters FIGURE 9 Overview of the ATLAS Calorimetry 12 27 May 1999 The LHC parameters such as the large center of mass energy and the high lumi nosity requires good detector performance in an unprecedented part of the energy scale ATLAS must also feature the ability to deal with the p
80. of discovering new unexpected physics The following chapters will give a presentation of the ATLAS detector and its subdetectors with a more detailed description of the Inner Detector 6 27 May 1999 2 0 The ATLAS Detector The purpose of the ATLAS detector is to measure whatever happens after the high energy proton proton collisions provided by the LHC accelerator The cross sec tions for the physics processes to be studied with ATLAS are small over a large part of the parameter space to be explored at the LHC In other words Most of these processes are very rare For instance Only 1 proton proton inelastic interaction in 10 3 would result in a Higgs boson decaying into 4 leptons The goal is therefore to operate at high luminosity 10 4cm s It is also important with a detector providing as many signa tures as possible electron gamma muon jet missing transverse energy measurements Eis and b tagging The wide selection of signatures is important to achieve solid and unambiguous physics results and measurements in a high rate environment such as the LHC ATLAS Hadron Calorimeters Calorimeters S C Solenoid H Fi S C Air Core Toroids Detector EM Calorimeters FIGURE 4 Overview of the ATLAS detector indicating where the different subdetectors are located The entire ATLAS detector consists of three main parts From the Interaction Point IP and outwards these are the Inner Detector whi
81. of the voltage generated in the chip as a function of injection charge How this parameter is calculated will be explained in chapter 7 0 Offset Every channel has an intrinsic DC voltage level which in general is different from channel to channel and is due to the processing of the chip Reading out an analogue signal of a channel if it was possible without any charge injected into the input would result in a signal with signalheight equal to the offset Efficiency The percentage of channels that gave triggers during a read out sequence is defined as the Efficiency Noise Occupancy There will always be a certain level of noise on the inputs of the chip This noise can also result in triggers if the amplitude of this noise exceeds the threshold level The percentage of channels that averaged over a long time are defined as hit because of noise triggers is called Noise Occupancy With these definitions in mind it is possible to form a list of requirements to chip performance and functionality 27 May 1999 35 The possibility to fix a threshold such that with an injection charge corre sponding to about 1 MIP Minimum Ionizing Particle the noise occupancy does not exceed 5x10 and efficiency does not drop below 99 Efficiency Threshold Acceptable Thr Range FIGURE 24 Sketch illustrating the above requirement The channel to channel gain spread should be minimized this to keep
82. on about all the VXI devices present in the system such as manufacturer name logical address model name model code man ufacturer ID mainframe Commander s logical address Servant s logical address memory requirements interrupt line and handler assignments Configuration Editor This editor configures the local VXI hardware including the V XIbus interface and local CPU logical address parameters Manufacturer Name Editor This editor keeps record of the manufacturer names and numbers ResMan uses this data to assign ASCII names to VXI devices Model Name Editor This editor keeps record of the model names and their associated manufacturer names and the model numbers ResMan uses this data to assign ASCII names to VXI devices Device Name Editor This editor assigns device names to the VXI devices installed in the system The device name is associated with a manufacturer name model name logical address physical location slot nr and or the mainframe extender Non VXI Editor This editor assigns address space and interrupt lines to non VXI devices ResMan needs information about the attributes of the installed non V XI devices so it can avoid conflicts when dynamically config uring the V XI devices Interrupt Configuration Editor This editor defines individual and inter mainframe interrupt configurations Trigger Configuration Editor This editor defines inter mainframe trigger TTL and or ECL configuratio
83. ontside strips which are parallel to the beam direc tion The rotation is due to the requirement to provide z measurement capability So why not align the strips orthogonally Any particularly good resolution in the z meas urement is not needed because the magnet bends the particle trajectory in the r plane With the backside detector rotated by 40mrad it also provides an extra r measurement When operating in a 2 Tesla magnetic field as is the case at LHC the particles trajectories are diverted according to the Lorentz force This causes a signal spread in the detector due to the angle the particle hits the detector with To minimise this effect the modules are mounted on the support structure with a tilt angle of 10deg to the tan gent The modules are slightly overlapping each other to minimise loss of information or dead areas in the system The optimal operating temperature of the Silicon detectors under these radiation conditions is 7 C This temperature is a compromise between annealing and anti annealing effects Highly energetic particles cause bulk damage in silicon by displacing atoms from the lattice causing a change in dopant concentration A change in the full deple tion voltage Vy and the leakage current is observed The time dependence of V pg can be separated into a short and long term period The short term annealing is believed to be dominated by the recombination of radiation induced acceptor sites into ina
84. or noise The measured offset spread of 28mV rms equals according to the formula above an equivalent noise charge of 2160 electrons and is alarmingly high The equiv alent input charge corresponding to the offset not only contributes but alone exceeds the requirement for the total noise The mean electrical noise at 4fC is 10 39mV see figure 48 This equals an ENC of 802 electrons and is also high but well within the requirement When adding a detector capacitance of 20 pF one expects the noise up to 1500 electrons 20 This increase in the total noise is calculated from the relation Total Noise y Electronic Noise t Detector Noise where Electronic Noise Ko K Cj 44 and where Kg and K are constants and Cj oad is the added capacitive load Kg is typically 600 electrons and K 60 electrons pF For a 20pF detector this results in an ENC of 600 60 20 1800 electrons com pared to a signal of 22 000 The expected increase in ENC is mainly due to this extra term in the electronic noise The experienced drop in gain and the noise in the detector itself is of little importance Entries Mean RMS ALLCHAN y ndt 81 39 10 Constant 29 19 Mean 10 39 Q 6439 5 6 vi 8 G 19 11 12 13 14 15 4 f noise FIGURE 48 The 4fC noise distribution 27 May 1999 75 7 6 Conclusion A well functioning front end chip also needs to undergo tests with a detector bonded to it before a final conclusion is made about whether
85. ought to induce such actions The cursors are set at the ends of this block of continuous high output and with the Af 21 86u s this equals at 35MHZz 765 clock cycles three less than 6 x 128 768 channels Keeping in mind the HAC bug report one might remem ber that the HAC strips away the 3 first clock cycles from the first chip For the CDP these were taken from the column code but for the SCT128B this is exactly the response one would expect from a L1 trigger with the current control register setting SCT128B in test mode and the mask register set to 128 one s test pattern where all channels should give triggers Inspecting figure 32 these suspicions are confirmed The bits in front of the data stream might very well be a header and by inspection of the controlblock file itself noticing the DAC amp DELAY register setting one discovers that the combination x010x is sent to the hybrid This is interpreted as a L1 trigger by the HAC and a read out of the hybrid is commenced 54 27 May 1999 taacvileoorvsoonoiaer ti 7 805ms t 7 907m t 21 66us izat 45 75kHe FIGURE 31 Close up of the leftmost bitcluster the HAC Setup on the CTC line from the HAC Reset plot This is a close up of the left part of figure 30 the HAC configuration part It consists of a double CLEAR HAC and a Write Status Register with the 32 writea ble bits directly following the comman
86. ow point particles that is We have not yet seen any signs of size or structure for these particles 3 Force carrying particles The 4 fundamental forces each have their force carrying particles The strong force is carried by the massless gluon the electromagnetic force has the photon and the weak force has the massive W and Z particles The theory of gravitation is not implemented in the Standard Model or any other quantum mechanical model and any graviton has in fact never been observed 27 May 1999 5 4 Antiparticles In addition to the former there is an antiparticle for each particle in the Stand ard Model An antiparticle has exactly the same mass as its original and opposite quantum numbers FIGURE 3 Chart of the Elementary Particles in the Standard Model The motivations for the LHC reach both within and beyond the SM The most important issue are the search for the origin of the spontaneous symmetry breaking mechanism in the electroweak sector of the SM or put in a different way the search for the origin of the different particle masses One of the possible manifestations of this spontaneous symmetry breaking mechanism is the existence of the Higgs boson s and the search for these will be of major concern Other important fields of research will be supersymmetric particles composited gauge bosons and leptons CP violations in B decays and detailed studies of the top quark as well as the possibility
87. p modcalp 1 calp m do n 1 128 v inp modch 1 n ch m n enddo enddo sigma mslop fcmod2 fcmodl calp 2 calp 1 sigma moffs mslop calp 1 fcmod1l v inp par 1 3 0 0 0 nfit 4 npts v fit modcalp modch 1 nfit k k eh 1 nfit k k pl wqo 2 par sigma gain par 2 sigma offset par 1 v inp mpslop k gain 1 v inp mpoffs k offset 1 message i otro h del id enddo v wr mpoffs mpslop offsets dump set gsiz 0 45 set yhti 0 7 set ygti 1 2 exec SCaniXxx END Return 88 27 May 1999 MACRO do50pp On error goto END KS D gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt Plot 50 points versus channel gt gt gt gt gt gt gt gt KS DDS gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt npts vdim calp if npts gt 3 then zone 3 3 kw 3 else zone 3 npts kw npts endif kc 0 do i 1 npts if kc kw then kc 0 wait endif kc kc 1 pulse calp il if She
88. r the border between adjacent strips will cause two strips to register a hit This improves the resolu tion since the possibility that one particle causes two strips to fire is equivalent to a finer partitioning of the readout pitch 22 27 May 1999 Heavy particle irradiation is a major problem with these detectors in the LHC environment The effects of such irradiation can be summarised as e An increase in leakage current will occur due to the structural damages i e bulk damage caused by the heavy particles There will also be a change in the effective doping which in turn implies a change in the necessary voltage to keep the detector fully depleted After some time though the detector goes through a type inversion The n type Si crystal will actually have turned into p type Si crystal and the pn junction will have moved from one side of the detector to the other see figure 17 e Due to an increasing amount of impurities and structural damage effects like trapping come into play This causes a decrease in charge collection efficiency because some of the charge carriers get trapped by these impurities After 10 years at full luminosity at LHC we will have type inversion for all sen sors and depletion voltages up to 350V The p n junction will then be on the n side of the detector It is therefore important to always operate the detectors overdepleted since a partially depleted detector will have the un depleted zone on the p
89. re that noise is treated sensibly The injection charges used in this test therefore range from 1 to 4 fC The steps are 1 0 1 5 2 0 2 5 3 0 and 4 0 fC For each threshold scan the number of threshold points and the number of events Nevents are set and for each calibration pulse a threshold range is set The number of events specifies how many times to inject the testpulse per threshold point The threshold range specifies the start and end thresholds of the scan and the number of threshold points Npts in the equation below specifies how many different threshold levels between and including the start and end points to perform the test upon Together they give the resolution the step size of the scan Stepsize Endpoint Startpoint Npts 1 For each threshold point the injection charge is injected Nevents times into each channel The events which resulted in a trigger are counted Ntriggers and compared to the number of events From this the efficiency of the channel is calculated Ntriggers Efficiency NEUOHE 27 May 1999 61 After having injected the same injection charge the requested number of times into all the channels and at all the threshold points specified it is possible to gather these data into a histogram with efficiency along the 2nd axis and threshold along the Ist axis This is done for each channel and is called an s curve because of the typical inverted s like shape of the resulting curve see below
90. required to ensure correct execution of the different commands Commands 3 amp 4 were not implemented in the CDP128 and may have a side effect to the HAC state Execution of the CLEAR command for the HAC is therefore advised after initialization of SCT128B Readout Protocol At the arrival of a L2 trigger readout strobe the oldest data from the readout buffer is written to the output register When a LAST signal is received 128 bits are shifted out serially and a NEXT signal is passed on to the next chip in the chain that may be another SCT128B or the HAC The L1 and L2 signals are validated by the ris ing edge of the clock while the LAST signal is validated by the falling edge A readout sequence with the test pattern FOFOFOFO will look like shown in figures 22 and 23 27 May 1999 33 s eE BEEEIEESIENNAT nu E du a CMT FIGURE 22 Close up of the Start of the Readout Sequence coo ERR ce NUR SE LIP 5 S L12 ee LAST E FIGURE 23 The Complete Sequence 34 27 May 1999 5 0 The System Setup for Module Measurement This chapter describes the hardware setup for module measurements as used in both Uppsala and Oslo When a particle traverses the silicon detector a small electric signal is created and collected by the readout strips This tiny signal is then routed through the different parts of the Front End electronics where it is amplified discriminated and read out To simulate a real experimental situation
91. ring the period August September 1997 and the motivations for performing this type of test My work was mostly concentrated on implementing control signals and trigger logic for the DAQ system Therefore the logic trigger and timing signals for this system will be presented No data from this testbeam will be presented since I was not involved in the analysis work 8 1 Motivation The radioactive beta sources which provide the most energetic electrons emit electrons with energies of a few MeV For instance 106Rh produce electrons with a maximum end point energy of 3 54 MeV 21 which can be used to irradiate a detec tor module This procedure does not require any more equipment than the radioactive source the module with its readout system and a scintillator for generation of triggers It can be executed in any lab around the world and it is useful since it provides a sim ple way of testing the basic functionality of a module However it is not a sufficient procedure for characterizing the module in terms of the front end parameters described in the previous chapter This is because the ener gies of the traversing particles are too low to avoid effects of multiple scattering during traversal of the silicon detectors According to 22 the effect of multiple scattering can be quantized as follows 13 6 MeV 0 aan ae z JX Xo 1 0 038 In x X9 where 0 resembles the angle of deflection Bc p and z are the velocity momentum and
92. riteable parts of its status register _ The Read Strobe command causes the HAC to send a read strobe pulse to the readout chips HAC Commands x11110000x Clear State of HAC x11110001x Read HAC Status Register x11110010x Write HAC Status Register x11111100x Generate Read Strobe As will be clarified later these commands may also have a side effect of trigger ing some instructions to the SCT128B s 4 1 3 Readout A successful readout of an event from the hybrid requires a specific series of events 5 A pending trigger 6 The readout chips receive a Read Strobe pulse 7 FIRST signal LAST signal of the first readout chip in the chain is raised by HAC 8 The readout chips pass read out flag via the LAST NEXT connections 9 The END signal NEXT signal of the last readout chip in the chain is raised by the last readout chip The bit sequence driven down the CD line by the HAC during readout of an event will look like this O bit Header pattern from HPR 8 0 HRS pulsed for one clock at this time Time Out Flag Overflow Flag e Underflow flag e 4 bit read strobe count 28 27 May 1999 FIRST asserted by HAC at this time e 128 bit hit pattern from each SCT128B HAC expects END to become true after the last chip is read out EV T HRS x FIRST Mr CD 12 bit Header Ebit com Ahipl 128 bits NS hip 128 bits TOKENI END FIGURE 20 Logical Events
93. rogram ResMan Startup Resource Man ager and VXIedit VXI Resource Editor All will be explained throughout this chapter VXTinit This program configures the local hardware in our case the PCI MXI 2 card and must always be run at system startup It verifies that the correct hardware is installed and operational and finally it performs basic initialisations that the Startup Resource Manager requires for operation Startup Resource Manager ResMan When executing ResMan all devices in the system must be reset either by cycling power in each mainframe or software reset through each mainframe s back plane This to make sure all devices are in the VXI configure sub state The Startup Resource Manager performs system level configuration of our local CPU This means that information about the whole system is put in our local CPU every time ResMan is run If the local CPU PCI MXI 2 is configured at logical address 0 which is the case in our setup ResMan configures the VXI memory maps and devices with the purpose of integrating VXI devices with non V XI devices This means that the PCI MXI 2 is the highest commander in our system the VXI Resource Manager The options where the local CPU is not configured at logical address 0 will not be discussed here If previously configured ResMan locates and acquires all the necessary infor mation about all types of devices from a database generated by the VXIedit utility see chapter below
94. ront End The Front End part comprises 4 main functional blocks 1 The preamplifier shaper discriminator circuitry with the designed processing parameters Signal Processing Parameters Parameter Value Differential gain at the input of discriminator 100 mV fC Peaking time 20 ns Time Walk 15 ns Double Pulse Resolution 50 ns Discriminator off state output level 4V Discriminator on state output level OV 2 A calibration circuitry Each channel has its own internal calibration capacitor of 100 fF which can be pulsed with signals applied to 1 of 4 external inputs test 0 3 or with signals delivered from the internal calibration circuitry During cal ibration one fourth of the channels are stimulated and tested simultaneously If the internal calibration circuitry is used the calibration line to be activated is selected by a 2 bit address caldO cald1 Calibration Line Addressing Cald0 Cald1 Pulsed Test Line Pulsed Front End Channels 0 0 test O ch 0 4 8 0 1 test 1 ch 1 5 9 1 0 test 2 ch 2 6 10 1 1 test 3 ch 3 7 11 3 A DAC for the calibration amplitude The test signal amplitude is set by this 8 bit internal DAC and the test signal is triggered by a calibration strobe signal generated by the Control Logic following the slow command 10xx The cali bration strobe can be delayed with respect to clock within the range of 50 ns with 5 bits resolution and its duration is fixed and equal to 200 ns C
95. s and turning on the green LED The DSP then calls the initialization function before it goes into the main loop There are 2 major DSP states see figure 28 handling messages while waiting for a start of burst signal and reading trigger and detector data until an end of burst sig nal occurs A flag DSP STATE indicates whether the DSP is idle waiting for mes sages and a start of burst signal is executing an action or whether it is in the burst loop reading data and waiting for the end of burst signal These states are visualized by the LEDs on the DSP card A steady green light indicates the idle state the yellow light is turned on during execution of an action induced by a message the green light is flashing during the burst loop and the red light indicates a fatal error The VME address is set by setting the 8 bit DIP switch S1 on the DSP card The position marked 0 is the most significant bit and only positions 0 4 are used The DSP responds to both 24 bit and 32 bit VME addresses and if the DIP switch is set to xxxDUDUU D Down and U Up positions 7 0 this correspond to address 280000 hex bits 23 19 in 24 bit mode 27 May 1999 45 Major DSP States EOB TRANSFER Run Mode start of burst act on imported message read trigger info and data for burst send error Message FIGURE 28 Major DSP States in EOB TRANSFER mode There are two run modes possible data transfer at the end of
96. s impossible to apply the s curve fit and a linear fit is as an approximation applied instead The 5046 threshold is found by extrapolating 72 27 May 1999 this straight line until it reaches a value of 0 5 on the second axis As seen in figure 46 this will always result in a lower 50 threshold than with the s curve fit and might also very well result in a negative value This is also the case for a lot of the 1 5fC s curves and is the reason why the 1 0 and 1 5 fC 50 points are omitted from the gain and offset calculations 1fC s curves 0 35 f 3 5 d 0 3 H 1 Q 4 Q 25 HI 0 3 0 2 0 15 0 2 0 1 ga 005 a D o 200 400 600 Oo 200 400 600 channel 17 channel 18 0 4 0 9 0 35 0 25 Q 3 0 2 0 25 0 2 0 15 0 15 0 1 Q 1 0 05 0 05 J D 200 409 E 200 400 600 channel 19 channel 20 FIGURE 46 A few 1fC s curves 7 5 Evaluation As mentioned earlier some channels corrupt a couple of the plots in this chapter figures 41 and 43 This needs further investigation Channel 33 is one such channel and in figure 47 more detailed data for this channel is presented 27 May 1999 73 Channel 33 9 2 0 4 0 15 0 3 9 1 0 2 0 05 0 1 a 0 o 250 500 500 500 S curve 1fC rud 1 5fC Pi curve 21C 0 8 ue 0 6 0 75 0 4 0 4 0 2 0 2 0 25 Q 00 o 250 599 500 250 599 S curve 2 5fC Ris curve 3fC S curve 4fC g 1000 2000 Gain 471 09 mVv tfC Offset 2062 77 mV 2 2 25 2 5 2 75 E 5 25 5 5 35 75 4 Gain FIGUR
97. scan getHlimmod v123 id 25 3 pulse fC noise enddo 90 27 May 1999 kc 0 kw 3 do Li kce kw then Set STAT 1001110 h fit id g qw id id 10 h fit id g qw enddo END Return MACRO pltgains On error goto END K gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt DD DDD D gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt KS DDS gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt Gain and offsets opt htit zone 2 2 if hexist 123456 then h del 123456 endif if hexist 50 then h del 50 endif exec scan getHlimmod mpslop 50 25 3 gains opt fit h fit 50 g qw if Shexist 51 then h del 51 endif exec scan getHlimmod mpoffs 51 25 3 offsets h fit 51 g qw nw Svdim mpslop 1d 123456 nw O nw put vec con 123456 mpslop opt utit title Gains u h pl 123456 title Offsets u put_vec con 123456 mpoffs h pl 123456 END Return 27 May 1999 91 MACRO gain On error goto E
98. sed The DIN plugs used are arranged in three rows of 32 pins P1 supports 16 and 24 bit addressing and 8 and 16 bit data paths P2 uses the centre 32 pins to support full 32 bit data and addressing paths The two outer rows of P2 are user defined and are used for i o ports disk drives and other external peripherals A comprehensive description of VME can be found in 13 This section sum marizes the most important points 27 May 1999 41 5 4 The VME modules The SEQSI module was used only to generate a 40MHz clock and will therefore not be described in detail The SEQSI routs by default the clock generated by one of its two onboard crystals to its output By making sure that it was the clock from the 40MBHBz crystal that was distributed the aim with the SEQSI was attained The DSP System A comprehensive description of the DSP system can be found in 14 and 15 This section summarizes the most important points Hardware The DSP hardware consists of three different cards that are put together to form a larger card The DSP card the HL card High Level card and the SLL card UCSC silicon Strips Low Level card The DSP card is a general purpose processing card containing a digital signal processor memory three I O connectors and the following onboard peripherals e TMS320C31 40MHz floating point DSP chip 256Kx32 RAM expandible 32Kx8 boot EEPROM e Four 12 bit DAC channels e 12 differential ECL direct input lines
99. side of the detec tor The charge collection then becomes difficult since there is no electrical field near the strips 3 3 4 Hybrid The hybrid is a ceramic piece which carries 6 128 channel chips SCT128B and is glued directly on top of the detector There will be 2 hybrids on each module one on each side It plays an important part in mechanical support cooling transport of heat away from the chips and readout Beryllia BeO is chosen as the material for the hybrid because of its good thermal conductivity and long radiation length 144mm There is also an electric circuitry on the hybrid and this performs the following tasks Distribution of power and ground to the Front end chips Distribution of clock and control to the binary pipeline circuitry Return of data to the off module optical transmission board e Filtering and AC current return of the detector bias line Support of redundancy functions of digital chips bypass lines for chip failures 3 3 5 Electronics Apart from the readout electronics which I will focus on here there are a lot of other features of the SCT which must be put in the rather vague category Electronics The main tasks of these electronics can be summarized as follows Control the operation of the SCT Provide power for the electronics and the detector bias Provide means for calibration and monitoring detecting problems with the SCT before severe damage is done to the system of all aspe
100. t the basic components of a system for binary Front End electronics are now present in the LHC lab in Oslo and are being used as the basis for the next version the ABCD test system Furthermore a procedure for analysing and evaluating the test data from binary readout chips is outlined Issues that need to be developed further to achieve a fully functional and stable DAQ system must be to create a cool environment for the hybrid and the readout chips The need to operate these at a low and stable temperature is crucial In more general terms will the handling cooling and environmental control of the modules in the lab during testing and repair be very important and this thesis has shown this Also the VME hardware and software have to be adapted to the final electronics but this a question of gradual development of existing pieces 86 27 May 1999 Appendix A KUMAC files used in the analysis in chapter 7 0 MACRO loadslp On error goto END kA Computes gains ans offsets for each channel gt gt gt gt gt x gt gt gt gt gt gt KS DDS gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt gt exec scan del if 0 then cwd else cwd 1 endif files pb200c100 pb200c150 pb200c200 pb200c250
101. te This makes the output a bit more unpredictable 27 May 1999 85 This is a problem only with small injection charges since the effect of this oscil lation process is limited to corrupting the s curve fit when the transition from 100 to 0 efficiency region of the s curve histogram appears at low thresholds This was evi dent in the 1 0 and 1 5 fC injection charge s curves where a lot of the 50 thresholds were negative This is the reason why the 50 thresholds from these injection charges were omitted from the gain and offset calculations Evaluating the results of the tests I came to the following conclusions The chip contains two non functioning channels channels 33 and 43 gave triggers only at very low thresholds which were discussed more thoroughly in chapter 7 5 A mean gain of 81 mV fC is a low but reasonable result considering that the chip was designed to have a gain of 100 mV fC The measured offset spread was equivalent to an ENC of 2160 electrons and the pure electrical noise was 802 electrons When adding a capacitive load of 20 pF the noise will increase significantly The noise requirement of a total ENC lt 1500 electrons after the detector is bonded is not met even before the detector is bonded Based upon these results the chip under test was rejected primarily due to the very high offset spread Furthermore the two non functioning channels and the rela tively high noise and gain spread are also i
102. teiment Event Counter Statt BUSY Watchdog ASSERT IT Wait for CLEAR_BUSY CLEAR_BUSY ot WATCHDOG WATCHDOG FIGURE 52 State diagram of the CORBO module 8 3 2 The TDC Another important VME module is the CAEN v488 TDC Time to Digital Con verter This section summarizes the most important points from 29 and explains how the TDC is used in the H8 setup It houses 8 independent 12 bit Time to Digital Conversion channels Each channel is built around a monolithic TAC Time to Ampli tude Converter which can individually be enabled or disabled developed in bipolar ASIC technology The outputs of the TAC sections are multiplexed and subsequently converted by a fast 12 bit ADC module 100 us conversion time A control logic controls the con version sequence It converts and stores in the output buffer only the channels that have values lying in a range defined by a High and Low Threshold The module is Busy dur ing the conversion sequence and the Busy output is set to TTL level 1 The operational mode used is the Common Start mode In this mode all chan nels starts at the same time when a NIM common input at the front panel arrives and are stopped individually by an ECL input If the module is not busy and at least one channel is enabled a NIM pulse on the COM input causes the following e The TAC conversion of the enabled channels starts e The Event Counter is incremented The Busy output is set to 1
103. the response from the channels as uniform as possible Identical signals should be amplified and discriminated equally from one channel to another The threshold spread should be minimized If the threshold is set to 100mV the actual threshold in the chip should not be too far away from this value The largest factor contributing to the threshold spread is however the spread in off sets mV difference from one channel to another in the offset means 1 mV dif ference in the actual threshold The percentage of bad channels on one chip module must be minimized The complete setup of the test system will look as illustrated in figure 25 The details of each component will be explained throughout the rest of this chapter 36 27 May 1999 VME ctate FIGURE 25 The Oslo lab setup 5 1 The VXI VME eXtensions for Instrumentation System The compatible platforms for the National Instruments VXI system is NI embedded controllers and external computers with an MXIbus interface VXIbus VXI is a superset of VME It defines additional board sizes beyond VME cool ing EMC specifications ElectroMagnetic Capability for both the mainframe chassis and the modules in the system VXI reserves a portion of VME address space the upper 16kb of A16 space as VXI configuration space All VXI devices have configuration registers that reside in this part of the memory These registers are used to configure the system This is done 27 M
104. the 25ns bunched beam structure that the final ATLAS detector will experience in experimental situations A burst of particles arrived every 12 5 sec ond The duration of this burst which is also called a spill is 2 seconds The reason why the 25ns bunched beam structure is not used here is simply because this is very difficult to achieve when the protons are extracted from the SPS into a secondary beam The fact that the clock cannot be synchronized with the beam implies that many of the particles in a spill are wasted Sometimes they arrive in phase with the 40 MHz clock in the front end chips but mostly they arrive out of phase The time interval where the arriving particles are considered in phase is 5ns long The fact that a particle arrival is in phase with the front end clock means that we expect max imum signal in the silicon detector when the trigger initiates the readout The other 20ns are considered out of phase In LHC the clock will be synchronized with the collisions Since no results will be presented from the different modules their differences will not be described very thoroughly It is worth mentioning though that several dif ferent binary front end chips are used for reading out the different detectors The setup of the different detectors in this particular testbeam period is shown in figure 51 27 May 1999 79 Cool Box I Cool Box II Scintillators FIGURE 51 The 1997
105. the total inventory of liquid helium will be 700 000 litres 4 27 May 1999 101 1S SC BUS BARS HEAT EXCHANGER PIPE IRON YOKE COLO MASS 43KI SUPERCONDUCTING COILS SHRINKING CYLINDER HE I VESSEL BEAM SCREEN THERMAL SHIELD 55 bo 75K NON MAGNETIC COLLARS VACUUM VESSEL BEHM PIPE RADIATIVE INSULATION SUPPORT POST FIGURE 2 Cross Section of LHC Tunnel The LHC will be able to operate at energies in the neighbourhood of 14 TeV for proton proton collisions and 1250TeV for heavy ion collisions which is completely unknown territory The LHC is of course designed to search for phenomena predicted by current models but since the energies are so high one must be as prepared as possi ble for surprises 1 2 The Standard Model The mathematical model modern particle physics is based upon is the so called Standard Model The main idea here is that there are 3 families of fundamental parti cles 1 Quarks There are 6 different quarks u p d own s trange c harm b ottom and t op They can only exist in a composition with other quarks because of their colour charge and have electrical charge 1 3 or 2 3 These are the constitu ents of all hadrons with 3 quarks in baryons and a quark and an antiquark in mesons 2 Leptons There are 6 of these too 3 negatively charged electron muon and tau and 3 neutral ones neutrinos These exist independently and are as far as we kn
106. threshold control DAC 8 bits for calibration amplitude DAC 5 bits for calibration strobe delay 32 27 May 1999 4 2 4 Levell and Control Commands The L1 trigger commands are summarized in the table below L1 trigger commands x010x One LI trigger x0110x Two consecutive L1 triggers x01110x Three consecutive L1 triggers For each L1 trigger received a 128 bit word is read out of the pipeline and writ ten into the readout buffer The first command is used in normal data taking mode while the other 2 can be used in test mode or for data taking with cosmic radiation If a sequence x01111 is received the next 4 bits are decoded in the following manner Control Commands Command Function 00xx Clear pointers in the RO buffer and the pipeline O01bb Load calibration address register with bb 1110 Load the next 21 bits into the DAC amp Delay register thrDAC calDAC cal pulse delay The most significant bit is always shifted first 1111 Load the next 128 bits into the mask register first bit corresponding to channel 127 After power up the state of the different registers in the chip is undefined The following sequence of commands should therefore be executed in order to define this initial state 1 LI trigger atleast 130x0 010 lt 130x0 gt 2 CLEAR 1111 00xx 0 3 Load DAC amp Delay register 1111 1110 21 bits 0 4 Load mask register 1111 1111 128 bits 0 The additional 0 after each command is
107. tlas 1997 tsp_97_aug htm April 1999 ATLAS TDR Jan 1999 http whatis com raid htm April 1999 mail from P W Phillips 1998 RCB 8047 CORBO User s Manual v1 0 June 1995 CAEN v488 User s manual 1997 mail from S Stapnes 1999 http arkhp 1 kek jp unno beamtests KEK H8Trigger eps Apr 1999
108. ture in short anything that causes radiation to loose energy 3 1 The Pixel detector The Pixel detectors are placed closest to the beam are aligned in barrels and disks of modules The Pixel system provides 3 space points over the whole acceptance of the Inner Detector Each module is a semiconductor detector with pixels instead of microstrips That is the strips are divided into much shorter strips pixels Each pixel measures 300x50um There are 140 million pixels distributed over 3 barrels and 8 disks With the given pixel detector design this gives a total sensitive area of 2 3 m To be sure not to miss any information the sensitive area of each module slightly over laps the neighbouring module 27 May 1999 17 FIGURE 14 Layout of the Pixel Detector The pixel detectors provide 2 dimensional spatial information about where a particle passes through the detector In order to read out every pixel the binary readout electronics have to be mounted on top of the detector From there the electronics are connected to each pixel using a bump bonding technique The innermost layer will be placed as close as possible to the interaction point to achieve an optimal impact param eter resolution These detectors are in addition much more radiation hard than micros trip detectors and can therefore be placed where the density of particles is highest They work both as vertex and tracking devices The parameters and the layout of th
109. ub epu afi eie eae arbos ed enter oe 83 8 2 Conclusions Soo nepote Padus IE WS Ded o deducit ata dass Deoda si tope epi eases 84 9 0 CONCIUSIONS as oto dio Ra ea Rd d dn ad a edd RAM 85 Appendix A e eduseitetost detenti dub ce ats eStats ordin tutos seated 87 Introduction The purpose with a particle physics experiment is always to find answers to fun damental questions about nature CERN is a center where such experiments are exe cuted The work described in this thesis is done as part of the research and development performed by the SCT group in the ATLAS collaboration at CERN The focus of the project has been on the binary readout electronics of the SCT detector modules and the testing of these Prior to allowing these electronics to be put in a physics experiment they need extensive testing and a lot of design parameters need to be optimized The purpose of this thesis is to 1 Describe my work with the setup of a DAQ system for evaluation of binary Front End electronics designed for the ATLAS SCT This is done in chapters 5 0 and 6 0 2 Present a way of analysing test data acquired with a DAQ system similar to the one set up in Oslo and to present an evaluation of the results of these tests This presentation is given in chapter 7 0 3 Give a short description of my work in the H8 test beam area at CERN This description is found in chapter 8 0 To fully understand this thesis however it is necessary to put it in a co
110. ve been included in both figures just to emphasize the point that the source test is not a procedure good enough to test the front end parameters The telescopes which are silicon detectors with slow analogue readout and the ability to locate the particle track position within 2um on the DUT 23 are required in such tests to determine which strips are hit and which are not Additionally the H8 testbeam facilities provide the possibilities of operation in a cooled environment a magnetic field with different depletion voltages and with the possibility to rotate the modules with respect to the beamline However determining the front end parameters of single modules under different operational circumstances are not the only motivations for executing a beamtest The purpose of the beamtest pro gramme is according to 24 Systematic evaluation of complete modules efficiencies noise and resolu tions e Operation with synchronised modules for overall SCT system efficiency meas urements e Operation with a common SCT TRT DAQ compatible with the calorimeter systems Combined running with the TRT for study of tracking efficiency and pattern recognition 8 2 The 1997 H8 setup The H8 testbeam is located at site Pr vessin in the French part of CERN The beam is usually a 180 GeV pion secondary beam provided by the SPS which is the accelerator prior to the LEP in the accelerator chain The structure of the beam in this period was not
111. we simply inject a charge of proper size on the order of the charge ionized by a particle traversing a detector into the calibration capacitor 100 fF at the input The main purpose of this system is to test the electron ics with respect to noise and certain features which will be explained in more detail below like gain and offset What is important to know about a chip before it is bonded to a detector and put in an experiment And what requirements to functionality is set Prior to this discus sion it is necessary to define some key concepts Threshold When a signal is being discriminated what happens is that a com parator compares the amplitude of the amplified pulse with a certain fixed reference value If this amplitude exceeds the reference the signal is defined as a hit and given the binary value 1 which will be the only information about the signal to be stored in the digital pipeline and read out If it does not exceed this value a 0 is written to the pipeline which of course means that no particle traversed the strip corresponding to the channel being read out This fixed value in the comparator is called the Thresh old Gain The charges generated in the silicon detector are very small To be able to discriminate them with some accuracy they are after being driven through a calibration capacitor of 100 fF amplified before they are discriminated and read out The Gain is a measure on the size
112. xist 20 then h del 20 endif if Shexist 21 then h del 21 endif gt Plot 50 points and noise across channels cd lun2 i hrin 20 hrin 21 mx pulse opt utit title pulse fC 50 Y4 points u exec fits hvec 20 vscale hy 100 hy put_vec con 20 hy h pl 20 h del 20 hrin 20 title pulse fC S htitle 21 u exec fits hvec 21 vscale hy 100 hy put_vec con 21 hy h pl 21 h del 21 hrin 21 gt Plot s curve of all together if Shexist 10 then h del 10 endif hrin 10 if Svexist par then v del par 27 May 1999 89 endif if vexist sd then v del sd endif v cr par 5 r 5 0 v cr sd 5 r 5 0 call fit scurve 10 0 par sd opt fit opt utit title pulse fC S htitle 10 u h pl 10 enddo END Return MACRO do50pspread npts vdim calp zone 2 3 opt fit do i 1 npts pulse calp i if Shexist 20 then h del 20 endif if Shexist 21 then h del 21 endif cd lun2 i hrin 20 hrin 21 gt Spread of 50 points nh Svdim mpslop if vexist v123 then v del v123 endif v cr vi123 hinfo 20 xbins r id 60 i if Shexist id then h del id endif get vec con 20 v123 vscale v123 100 v123 exec scan getHlimmod v123 id 25 3 pulse fC 50 Y points Spread of noise id 70 i if Shexist id then h del id endif get vec con 21 v123 vscale v123 100 v123 exec
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