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User manual - Viso Systems

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1. Centre of rotation Alignment of the lamp Aligning the sample lamp is key in ensuring precise measurements Specific tools designed to align the lamp relative to the centre of rotation namely centre alignment bracket and an aligning laser box are included with the LabSpion system First place the centre alignment bracket in the middle of the rotating opening It is designed in such a way that it will always sit in the middle of the opening Then place the laser box on the base of the LabSpion and make sure it is centred relative to the centre bracket as shown in the pictures below alignment bracket centred laser box 22 LabSpion user guide The laser box will shoot two perpendicular beams upwards which form a crossing That is the exact centre of rotation so the measuring lamp has to be aligned accordingly It is important to notice that sometimes it can be a little tricky figuring out the centre of the lamp For example in the picture above the centre of the lamp is the plane of the LED chip the rest is just metalic housing Another example is in the picture below a flat LED panel the laser beam is just on the brink of it turned on laser 23 LabSpion user guide Adjustment of the lamp holder arm There can be cases when a measuring lamp is very Spacious for instance a high bay lamp The large horizontal dimensions of the lamp will make it impossible to align the lamp with the centre of rotation
2. rrrnrnerrnnnnevnnnn Ibsen Photonics FREEDOM EEE ENE Custom viso high sensitive transmission grating Spectrometer range srrnnnnnnnnnnnnnnnnn 360 830nm 1024 pixels Spectrometer detector rrrrrrrnnnrnrrrrrnnnrnvvnnnnnn SONY ILX511B Calibration srrrernnnnnnrr Fully calibrated plug and play solution Re calibration ccccsscccsseeeeeeees Every 1 year Maximum 2 years Control and interface COMO MEM ACC aja USB 2 0 COMMON CONMECION sdear a USB B Connections AC power in power supply ccccseeeeeeeeeeeeeeeeeeseeeeeees IEC 3 pin AC power out lamp rrrrrrnnnrnvrrrrnnnnnvnvrrnnnnnrrnnnnnn Universal socket Light Source adaptors rrrrnnnnnnrrnnnnnnnr E27 E14 B22 GU10 gg eae Re ae ee USB B Approvals Power Supply ccccsseeeeeeeeeeeeeeees cUL UL CE CCC TUV FCC Power analyzer LabSensor rrrrnrrnnrrnvvnrrnnnnnvrnrnnnnnennnnnnsnne CE Ordering information VAD SIO IN eee P N LABSPO01 55 LabSpion user guide
3. Edet pictures Saving measurement Fill in and store all the necessary information about each measurement in the appropriate section as shown in the picture To save the measurement simply click on the save icon or select H File gt Save as Measurement name Save Product name Demo 1 Date and time 30 juli 2012 09 03 52 Item number PLED 43987 Price 495 Minimum Order Quantity 1000 Additional information Bulb measured at factory during inspection period Measurements are stored in the Measurement library in an alphabetic order Measurements are physically stored in My documents Viso Systems Light Inspector as fixture files The folder can also be opened through selecting File gt Open measure folder When some files are added or removed it is then necessary to restart the program so the library can be updated 48 LabSpion user guide File View Setup Measurement Help New teal Save as Export gt Open measure folder ta Bawer Exporting to IES LDT It is possible to export the measurements to IES or LDT formats to be further used in Dialux or other 3D lighting design software To export to IES simply select File gt Export gt IES or LDT IR File View Setup Measurement Help GM y gt New atal Measureme kj Save as pt 2 8 Open measure folder PNG image PEAK
4. Q t To Manager g OneNote d X Delete Rep Reply Forward v _ Move v Translate Zoom amp Junk ly eply BB S team E mail we E Actions Y Follow Up n Delete Respond Quick Steps F Move Tags P Editing Zoom monitor lightspion lt monitorsend luminetwork com gt Sent ma19 11 2012 17 46 viso visosystems com Measurement results for Demo 1 er ee es SYSTEMS 00000 LightSpion measurement results Light efficiency Vatt Output 258 Im Light quality Peak 354 cd Color temperature Power 4 0 WwW lt PF Beam angle Product name Demo 1 Date and time 30 juli 2012 09 03 52 item number Price Minimum order quantatity Additional information c monitor_lightspion 53 LabSpion user guide Specifications Measurement method rrrrrnnnnnnvnvrnnnnnvonnrnnnnnrrnnnnnnnnnenn Far Field Physical dimensions Shipping dimensions Lx W x H See shipping dimensions Shipping weight cc cssecceecceeseceeescseseeesscesseeeesseeseeeeeees 69 Kg Dimensions L x W x H rrerrrnnnnrronnrnnnnnvrnnnnnenr See dimensions Weight ciate ateieduearceun iene itemixanaah seisaaetisaaceeshtenmitidaananmenientamuaaniiaaid 63 Kg SET 50m to 0 5m EEE Sensor distance gt lamp length x10 Sensor distance setup Laser range finder build into sensor Lamp diameter range 0 1 5m at 2 axis 1 axis up to 6m Lamp maximum weight rrrrnnnnnnro
5. The LabSpion comes with a standard IEC power in connector and with a standard euro power cable but any power cable can be used as the Labspion supports any outlet voltage from 90 260VAC The power in connector supplies power both to the goniometer motor and to the power analyser and then subsequently to the measuring light source It means that the power is identical to the one of the measuring light source AC power supply cable plug Warning Risk of an electric shock Plug installation shall be performed by a qualified electrician A grounding type earthed power plug that fits the local power outlet must be used You can acquire an IEC power cable with a suitable grounding type plug from most of consumer electronics stores When installing the plug connect pins as follows Yellow and green wire to grounding earth Blue wire to neutral Brown wire to live 15 LabSpion user guide Connecting USB The LabSpion is connected to the computer using a USB connector type B A 2m USB cable type A to B is included with the LabSpion however any USB cable supporting USB2 0 can be used The USB provides communication and power to the LabSpion s main board processor power analyser and photo spectrometer meaning that the photo spectrometer can be used only with the connected USB Start the Viso Light Inspector software after having connected the USB the connection to the Labspion will be established automa
6. cold The point corresponding to the measured colour is shown with a black cross It can be used to check the whiteness of a colour by checking how close it is to the black body curve the closer it is to the black body curve the more accurate is the white colour 40 LabSpion user guide Power details A detailed voltage and current data can be viewed by clicking on the scope button or selecting View gt Power details The real eo ti me d ata Power 5 2 W PF 0 62 of the voltage i I Voltage 238 6 V an d Current 0 035 A current is shown in the power details window the green line illustrates voltage it should have a sinus curve The upper part of the sinus curve can sometimes have a flat top which is explained by the power grid distortions The current is presented with a red line it is displaying how the current is consumed by the light source The power factor is an indication of how well the current is consumed through a voltage period The power factor is calculated according to the following principle the value of the actually consumed power is divided by the product of the voltage and the current PF Power Voltage x Current 5 2 238 6 x 0 035 5 2 8 35 0 62 When the transformation of the current by the light source is not efficient the source will consume more current than necessary When the current is not consumed by the light source efficiently the cabling during in
7. 32 6 LabSpion user guide Manual POWEr COMO wixsissisleswidiaesianl tl paeddanstendiauieaui 35 Manual integration time S tUD cccccseceseeeeeeeeeeenees 36 Independently running spectrometer ccceceneeeees 37 Measurement datta cccccecccseccececseeeceeeceeseseeeeseeesseeens 38 POWEr JEANS css ccecesacdsidc ohncseensnsen e E 41 GRIS AS 43 SPHENC klimi Luanda 46 Attaching pICtUreS savnet eide 47 Saving measurement rrnrannrnnnnrnrannnnnnnrnnanennnnnennnnennnn 48 Exporting I ES ED T save 49 PO DP ir saiecccu eterna 50 EXPOMMING to PNG rerne a E ene 50 EXDOUING TOG SV sa 52 Emailing MEASULEMENL ccccccseecceeeseeeneeeneeeneeeneeenes 53 SPECICAUONS 2 54 7 LabSpion user guide Safety Information Warning This product Is not for household use Read this manual before installing and operating the controller follow the safety warnings listed below and study all the cautions in the manual Preventing electric shocks Make sure the power supply IS always grounded Use a source of AC power that complies with the local building and electrical codes that has both overload and ground fault protection lf the controller or the power supply are in any way damaged defective wet or show signs of overheating disconnect the power supply from the AC power and contact Viso Service for assistance Do not install or use the device outdoors Do not spray with or immerse in water or any
8. other liquid Do not remove any covers or attempt to repair the controller or the power supply Refer any service to Viso Disposing of this product Viso products are supplied in compliance with Directive 2002 96 EC of the European Parliament and of the Council of the European Union on WEEE Waste Electrical and Electronic Equipment as amended by Directive 2003 108 EC where applicable Help preserve the environment Ensure that this product is recycled at the end of its lifetime Your supplier can give details of local arrangements for the disposal of Viso products 8 LabSpion user guide Introduction About the LabSpion The LabSpion is a revolutionary new far field goniometer system with a spectrometer sensor that makes it possible to measure all photometric measurements quickly and efficiently The Light Inspector software enables to quickly measure save and export the newly obtained data System content LabSensor with a spectrometer sensor J 7 and an integrated laser C Plane goniometer my 0 measure the with lamp bracket ie to the abSpion LabSpion base with imi q integrated gonio drivers and a power analyser Tripod for LabSensor ha ml 3 point base table for LabSpion base The LabSpion package contains the following items e LabSpion goniometer base e C plane goniometer with a lamp bracket e 3 points base table e LabSensor e Tripod for the LabSensor e Light Inspe
9. out the uaktauaiiv ability of the light source to transmit colours thus indicating the quality of the radiated light 0 being the worst quality and 100 being the best quality equal to that of the Sun The CRI can only be used for white light If the CRI is not indicated that means that either the radiated light does not meet the criteria for white light or that light levels are too low to be measured 7 The photometric colour temperature indicates the colour of the white light and is displayed in kelvin Where 6000K is considered as cold and 2500K as colsiirtemperatiire warm The Kelvin scale was initially derived from the temperature of the tungsten filament Therefore the high temperature of the filament is considered 39 LabSpion user guide as cold light and vice versa If the colour temperature is not displayed it means that either the radiated light does not meet the criteria for white light or that light levels are too low to be measured 8 At a closer look the radiated colour is shown with x and y coordinates in the CIE1931 diagram The diagram illustrates all visible to the human eye colours It is based on an experiment conducted in 1931 with a number of participants aiming at figuring out the eye s perception of colour The black line in diagram is called the black body curve It Measured colour i illustrates all colours that are defined as white Black body curve T colours from warm to
10. CSV Tab seperated I 60 0 j l Power 40W ture DIAL light building software 49 LabSpion user guide Exporting to PDF All measurements can be exported directly to a PDF document Firstly select the measurement and then click File gt Export gt PDF It is also possible to implement your own logo in the PDF and export to different languages like English German and Chinese A typical export procedure is shown below Export to PDF YOUR LOGO Company Greven ou Export language English v Select language 50 tput 2701m ower 40W C eton temperatere P I PF 0 40 Product zame Demo 4 E27 LED BULB Date and b re 05 08 2013 13 57 10 nem number E27 46 45876 TBO am order qaa 100 i directions al E27 light t bulb Omn ma ed RED led e CRI Logo click to edit Om LOGO Company Export gt gt Export directly to PDF Add your own logo THE LED Company Lage tory i output 270 im Peak 35 0 cd is Camin 40W mere 0 48 IIK cS ll Click and add logo LabSpion user guide e e e me e e M e rv Brg ma 3347 Det 3 15 18 47 ae te 40816 Nee an Teal 100 Soana annie received Girectly from production part of zero tener to be verified for otection Exporting to PNG All measurements can be exported to a PNG picture file to be used in reports sales and marketing materials To export
11. LabSpion Patent pending User guide Last edited 09 September 2015 VISO SYSTEMSese Dimensions 9 5cm LabSpion base height l l ae 2007 Viso Systems ApS Denmark All rights reserved No part of this manual may be reproduced in any form or by any means without permission in writing from Viso Systems ApS Denmark Information subject to change without notice Viso Systems ApS and all affiliated companies disclaim liability for any injury damage direct or indirect loss consequential or economic loss or any other loss occasioned by the use of inability to use or reliance on the information contained in this manual Distance to the sensor L The measurement method used in the LabSpion system is far field which means the distance between the measuring light source and the sensor should be much greater than the dimensions of the light source itself Much greater applicable to our case means at least eight times larger than the light source However we recommend to calculate the distance using the factor of 10 Black backdrop wall L 10xD 3 LabSpion user guide Package contents and weight The LabSpion system consists of six separate parts as shown below Base 25 kg Tower 13 kg Stand 20 kg C plane head 6 kg Tripod 5 kg C plane bracket 3 kg Sensor 2 kg lt 4 LabSpion user guide Package dimensions and their weight Shipping packages Shipping dimensions
12. Therefore the default geometry of the LabSpion has to be modified Consider the following two pictures Default setup Extended setup Centre The figure to the left is the default configuration of the LabSpion whereas the right drawing shows the modified version of the LabSpion s geometry The arm with the lamp holder frame is tilted backwards leaving more room for horizontally expansive lighting fixtures To tilt the arm backwards you need to replace two long screws the one on top of the arm which is holding the head and the other one connecting the arm with the base There are two placements for the screws a default position 24 LabSpion user guide is shown in the picture below to the left The second position is shown in the same picture to the right Default setting Adjusted setting A An example of a high bay lamp placement is presented below Default setup Extended setup 25 LabSpion user guide Another example of measuring light from a street lighting fixture where the weight of the lamp is unevenly distributed The centre mass point of such a lamp is not coinciding with the central alignment of the LabSpion To balance the central position of such a lighting fixture a counter weight is used Look at the picture below Counter weight 26 LabSpion user guide Mounting of fixtures with a static base It is convenient to keep the base of the LabSpion still when mounting various lig
13. Weight 1 Stand Sensor Cables 101 x 58 x 57 cm 30 kg 2 Tower C plane Gonio Bracket Tripod 118 x 32 x 42 cm 28 kg 3 Base 55 X 55 x 32 cm 28 kg Total shipping weight 86 kg The shipment is done in a total of three packages 5 LabSpion user guide Contents MEOAUENON He 9 ADOUT ING LabdSPiN aa 9 SYyStem Content aars 9 About this document arrnannnnnnnannnannnnnnnnnnnnnnnannnnnnnnnnnn 10 HEAT 11 Measurement room cccecccecccecccececeeeceeeceecceeeceeenass 11 Narrow room CONSICErAatIONS ccceceeeeeeeeeeeeeeeeeeeeneees 11 Software installation ororrnrernnrrrarerrarernnrrranennanennnnnn 14 GONNECING POMERS 15 Connecting USB aar 16 Connecting LabSensor rararnnnnrnrannrvnnnrnrannnrnnnrnnnnennnn 17 Connecting the C plane goniometer rrrrrrrarennnnennnnn 18 Connecting a lamp power rrrrnnnrnnnnnnnnnnenrnnrnrnnnennnnnnnn 19 Connecting diagram ranannnnnnnnnnrvrnnnnnnnnenrnnnnnnnnennnnnnen 20 Making MEASUEMENMS cccceeeceeeceeeceeeeeeeeeeeeeeteeeeeeees 21 Alignment of the SENSE 21 Alignment of the lamp ccccsecseeceeeseeeseeeseeeseeenes 22 Adjustment of the lamp holder arm cccccceeeeeeeees 24 Mounting of fixtures with a static base r rrrrnrrnnrernre 27 Photometric parameters and Corrections rrnnrnnnrnnn 28 Radio WAVES precautions cccseccceeeeceeeeeeeeeeeeeeeeeaes 30 VA see 31 PUNY AO MAC sesion EE
14. ctor USB stick Windows e 5m IEC power cord 9 LabSpion user guide e 5m USB cable e 20m RJ45 cat 5 for connection between LabSpion and LabSensor About this document These guidelines describe the installation process of the LabSpion controller followed by the typical measurements of various light sources 10 LabSpion user guide Installation Measurement room To get the most accurate results it is important to consider the measurement room as well The LabSpion system is used in a dark room or in an open environment When using in an open environment the backside behind the goniometer must be of a black non reflective surface as shown below Open environment top view gt ms z ag a ne Gonore f Han ee en AS ik Sensor Thee eeeeeeeees ikenen et Se an r g a Recommended black back wall size Lamp size L Senor distance w h width and height 0 25m 2 5m 1 75m 0 50m 5m 3 5m 1 00m 10m 7m Narrow room considerations Sometimes providing dark room environment isn t sufficient for elimination of the background radiation For example measuring light in a narrow corridor yields stray light reflected from the surfaces of the corridor Two pictures below show a particular instance with a check for the stray light inside of the corridor walls One of the simplest solutions to eliminate unnecessary light is to set an additi
15. ed R9 value due to the lack of red light in the spectrum Example 4 Shows a LED bulb with an additional red colour boost so that the LED s R9 value is increased 45 CRI information c g px CRI details RI R15 R1 R8 CRI 99 7 109 100 100 109 100 100 400 90 co 199 100 1 Ri RZ Ra m PS OG R OG Ro ND RIV RIF RIG f RA Spectre CRI information a x CRI details RIH R15 R1 R8 CRI 81 6 va vo at 88 en 83 2 9 RE 7a a 2 ear hi 2 5 NG 87 i NYT WI RO Ata MS Spectra CRI information e 5 CRI details RI R 15 R1 R8 CRI 59 6 v3 i 72 73 ar 5 a 53 r i 47 3 30 87 2 nS Ei Ri RZ R3 Re 25 BG R I Ril Ri2 RIS 1 RIA R R1 R8 CRI 89 8 Spectra A z x CRI details R1 R15 a e eS ee 92 oo 87 Ww El n wa 76 oz Aa LP A n ha KU nn we RO RIO fit RID RG At Ris LabSpion user guide Spherical limit Spherical limit allows the user to constrain the area of the luminous flux integration It is also Known as measuring luminous flux in a cone Luminous flux measurement is generally done in a full sphere of 360 The new EU regulations EU No 1194 2012 however require the measurement of the directional lamps in a 90 or 120 cone meaning that light illuminated only I inside of that cone is considered for the v calculation of the efficient SEE EN luminous flux Light Inside 90 Cone The s
16. f the individual spectra in the spatial distribution Thus it represents the equivalent of a spectrum obtained from an integrating sphere 3 The complete integrated spherical Output 252 Im spectrum calculated in the previous step Peak 1021 cd is utilised to calculate the luminous flux in lumens The peak intensity output in candela is also displayed which accords to the highest level of the light output during goniometer measurement 4 The power is measured by sampling a Power 5 2W voltage and a current ata rate of 50 000 PF 0 62 samples per second to ensure high resolution and thus high power precision 38 LabSpion user guide The power factor PF indicates the quality of power consumption where 1 0 being the best it is generally achieved with a pure resistive load such as a tungsten lamp and 0 0 being the worst For a satisfactory level the PF value should be located between 0 5 1 0 You can refer to the quality chapter in order to figure out the power standards for different countries and regions 5 The efficiency in lumens per watt is calculated by dividing the luminous flux in lumens to the power consumption The result is displayed in the efficiency _bsbtefficiency bar with a corresponding colour enst where 100 lumen watt it shown as the outmost green The standard maximum value of 100 efficiency is 683 lumen watt 6 The CRI is calculated using the standard 8 reflectance colours in order to figure
17. he report versus 109 Im from the measurement It is important to keep in or mind that the new flux value also affects the calculated intensity in candela However in the original data file the 444 im measured values will always be displayed S P 30 0 Im 7 y PlayeG peak 60 1 cd in parenthesis above the overridden 133 cd numbers Power 16 7 W PF 1 0 29 LabSpion user guide At present it is Set photometric EI challenging to measure a lighting fixture which emits light in 4rt all directions as the goniometer structure can block some light However to overcome this difficulty the front and STN back of the lighting fixture ee sour Fad an are measured separately The two intensity distributions are then nerver together presenting an overview of a fully spherical illumination Thus the insert measurement button will open a dialogue for the additional data file and then the two curves will be combined Radio waves precautions lt is recommended not to have a receiver or a transmitter of radio waves in the vicinity of a working Labspion Thus tt is advisable to keep your smartphones and other electronic devices away from the system as they can interfere with the spectrometer and perturb the final results 30 LabSpion user guide Quality selection It is possible to manually select the measurement quality beforehand in Setup gt Measurement quality Setup Measure
18. hen measured and stored Measuring power m ee 32 LabSpion user guide 214 4 The complete 360 degrees angular light field is then measured and the beam angle is calculated Light sources with narrow beam angles can have insufficient number of measurements in order to generate an accurate result In such a case the Viso Light Inspector software will ask you automatically whether you would like to have a more detailed scan of the beam section Narrow beam angle The fixture has a narrow beam angle therefore will a more detailed measurement in the beam section source A increase the accuracy of the measurement Er small beom ongle Would you like to make a more detailed measurement of the beam section The increase in measurement quality after a detailed re scan of the narrow beam section can be seen below Before a detailed After a detailed auto re scan auto re scan 33 LabSpion user guide Upon completion the main characteristics are calculated and displayed the total luminous flux in lumen the colour rendering index CRI the efficiency in lumen watt the peak light intensity in candela the power and power factor A ement data Measure L t efficiency eo ae oup zo Light quality Peak 35 0 cd Colour temperature Power 4 0 Ww 3121 K PF 0 40 Further details about the measurement data can be found in the chapter Measurement data 34 LabSpion user guide Manual
19. ht sources for measurement Therefore the newest version of the system comes with a magnetic lock It is located on the back side right in the middle of the base of the LabSpion as shown on pictures below Once you push the lock you fixate the base in stillness An animated message appears on screen of the Light Inspector software bringing your attention to the fact that the base is locked see pictures below Now you can easily mount and align the fixtures In order to proceed further with measurements make sure to release the base lock 4 BASELOCKED 4 4 BASELOCKED 4 BT Please unlock the base before Please unlock the base before continuing measurement continuing measurement Cancel Ignore and continue Cancel Ignore and continue 27 LabSpion user guide Photometric parameters and corrections To calculate the correct lighting outputs for further visualisation it is necessary to insert the dimensions of the measured lighting fixtures bulbs spots and panels in the table as shown in the figures The table is found under Edit gt Photometric gt Dimensions This feature enables the data files to reflect the luminous and physical dimensions for an accurate 3D i i Giving your fixture dimensions ensures the lighting fiture visualisation in lighting delay nd ceed core n Ding programs such as software The photometric adjustments introduced in the relevant compar
20. ment Help GY WwW gt The Viso Light Inspector EET Tr USES the low resolution by Measurement quality Low B default Yet there are three ee mate mesten levels of complexity low ane medium and high Each quality level increases the number of measurements made during the goniometer operation it also increases the photo spectrometer integration time whilst lowering the noise level of the photo spectrometer measurements Increasing the quality results in substantial measuring time extension 31 LabSpion user guide Fully automatic The Viso Light Inspector software makes fully automatic measurements by default It adjusts the photo spectrometer to the background light environment by firstly turning off the light source and secondly measuring the background light level which is subsequently subtracted from the following measurements Therefore the measurements can be done even in a lit room The adjustment of the exposure time of the photo spectrometer also known as the integration time is also done automatically A measurement is simply started by clicking on the play icon Setting intergration time Then the integration time is set oe lt automatically Cancel The ambient light level is automatically EE measured by turning off the light source gt Calibrating to ambient light Cancel The light source is then rotated at 180 degrees to prepare for measurement The power is t
21. mum current supported by the lamp is 3A which is 660W at 220VAC and 330 at 110VAC AC power supply cable plug Warning Risk of electric shock Plug installation shall be performed by a qualified electrician A grounding type earthed power plug that fits the local power outlet must be used You can acquire an IEC power cable with a suitable grounding type plug from most of consumer electronics stores When installing the plug connect pins as follows yellow and green wire to grounding earth blue wire to neutral brown wire to live 19 LabSpion user guide Connecting diagram Below there is a connection diagram showing the different connections in order to make the system operational VISO LabS pion CEE Mains In 20 LabSpion user guide Making measurements Alignment of the sensor Before making any measurements it is important to place the sensor at the correct distance and to align it accordingly The LabSpion is a far field goniometer system which means that the distance between the sensor and the lamp is determined by a lamp size The recommended distance between the sensor and the goniometer is 10 times larger than the lamp length diameter The distance can be easily configured using the built in laser in the LabSensor IMPORTANT The distance should be measured to the centre of rotation of the LabSpion goniometer use the centre stick as the laser target 21 LabSpion user guide
22. nnnnnrennnnnnenvnnnnennnnnnnennnnnnen 25K9 Electrical Power supply Input rrrnrrrerrrnnnrnvvnnnnnn 90 to 260 VAC 50 60 Hz Power consumption 0ccccceeeeeeceeseeeceeeeeeeseees 60W Idle 15 W USB current CONSUMPTION cccccseeeceeeeeeeeeeeeeesaeeeeeeeeeas 200 mA Power analyser voltage range 30VAC 400VAC lt 0 2V Power analyser current range 6 OA 3A Avg 0 1mA Power analyser power range OW 300W Avg 0 001W Power analyser sample rate ccccceee 70 000 samples sec Photometric Flux lumen 10M earnnnnnnnrnnrnnnnnnnenn 1 3 000 000 4 00 Flux lumen 20M cc ceceeeeeeeeeeeeee 1 12 000 000 4 00 Flux lumen 40M rernnnnnrvnrnnnnnnnnnne 1 48 000 000 4 00 Intensity candela 10mM 0 07 1 000 000 lt 2 5 54 LabSpion user guide Intensity candela 20mM 0 07 4 000 000 lt 2 5 Intensity candela 40m 0 07 16 000 000 lt 2 5 Colour temperature cccscseeeeseeeees 1 000K 10 000K lt 35K Colour rendering INdex ccccseeceeeeeeeeeeeeeeeeeeaees 0 100 lt 0 7 Angular resolution LOW MODE rrrnnnnernnnnnennnnn 3 6 degree step EEE TT EE Ed About 20 sec measurement time per C plane Angular resolution HIGH MODE rerrrnnnnrnvvnnnnnnnee 1 degree step re ne ace ee About 1 min measurement time per C plane Spectrometer type
23. onal black shield according to the schematic _ Sensor Fd im 12 LabSpion user guide The opening size has a very simple consideration behind it Since the maximum diameter of the measured light source is 1 5 m the aperture at a half way distance is then 75 cm The averaging of it yields a 1 m aperture The practicalities of cutting out such an aperture along with the final result are shown below 13 LabSpion user guide Software installation Before you can start using the LabSpion the Viso Light Inspector software must be installed It is supported on all windows platforms Use the following link to download the latest version http www lightdataserver com software Viso 20Systems Ligh tinspector htm Please make sure the LabSpion is not connected to the computer during software installation Run the msi file and follow the xxx gt installation instruction er rpm Please wat Congratulations You are finished r op USB drivers are automatically i installing your Light Measurement Device drivers iJ n sta ed The divers were successfully installed on this computer L You can now connect your device to fhis computer F your device came wth instructors please read them frst Your measurements are not lost when installing newer versions or uninstalling All measurements will always remain in your document folder 14 LabSpion user guide Connecting power
24. pherical limitation can be set by clicking Edit gt Spherical limit Spherical limitation does not need to be set before a measurement although it Set spherical limit can be set afterwards also for the gt 360 degree defaut previously made full on 360 120 eae measurements Below is an example of the differences in the flux at 90 cone where 57 Im is considered as a waste outside the 90 cone 90 degree Manual 60 46 LabSpion user guide Light efficiency GERAD ouput 250 m Light quality Peak 354 cd Power 4 0W PF 0 56 Color temperature Beam angle 150 mo LL A 165 180 165 Attaching pictures You can easily attach pictures to your measurements via dragging and dropping them towards the area of the picture frame Light efficiency ED ouput 201m Light quality Peak 354 cd Power 40W PF 0 56 Color temperature Beam angle 3 9 o 165 180 165 lt is also possible to use a webcam to snap pictures of the measured light sources for quick references To use the webcam click on the picture frame to open a picture editor Afterwards click on the start webcam button for the webcam to start and add as many pictures as you like The first picture In the picture editor will be used as the primary one which accompanying the measurement by default Pictures can be moved or deleted by right clicking on each pictures 47 LabSpion user guiuc
25. pick a measurement in your measurement library and then select File gt Export gt PNG Image A typical export is shown below Light efficiency Output 258 Im Lame uate Peak 354 cd Color temperature Power 4 0 W k PF 0 56 Beam angle Product name Demo 1 Date and time No 30 juli 2012 09 03 52 item number 190 Price Minimum order quantatity Additional information CIE1931 x 0 427 y 0 403 242 Power voltage Current 0 030 A I i This measurement was made using the Aso Systems Light Spion www wisosystems com copyright 2012 51 LabSpion user guide Exporting to CSV Measurements can be exported to a CSV tab separated file so that the measurement data can be imported into Excel or other calculation software for further manipulation To export to CVS click File gt Export gt CSV Tab separated The contents of the CVS file can be seen below Product name Date and 30 juli time 2012 09 03 52 Efficiency CR 2578 253 75 Pr jose 0408 CIE y Le Angle Candela 046 179 55 178 65 177 66 0 48 176 67 0 47 Etc 52 LabSpion user guide Emailing measurement The Viso Light Inspector software is capable of directly emailing measurements by clicking on the email icon Measurement results for Demo 1 Message HTML Message R 3 5 v SA amre K QQ Qa B Moeta jeus G a
26. power control In some cases it is necessary to control the power of the light source manually For example when measuring flash light on batteries as the LabSpion s power analyser won t be able to turn on and off the light source automatically Another example could be a low voltage light source such as LED chips The external power supply of such chips has low response time when turned on and off therefore it would lead to an inaccurate result of the ambient light level To enable the manual power control select Setup gt Power control and select manual power control Setup power control C Automatically tum power on off Manually tum power on off Save Cancel When the manual power control has been selected the Viso Light Inspector will ask you to manually turn on and off the light source when necessary as shown below 35 LabSpion user guide Manual integration time setup In some rare cases it could be desirable to er le integration time of the photo hac spectrometer manually One case could be when measuring a light source emitting most of the light to the sides instead of in the central direction As the automatic setup of the integration time is done in the centre at 0 degrees the integration time would be too high resulting in saturation of the photo spectrometer and leading to an inaccurate measurement The integration time of the photo spectrometer can be set manually by selecting Se
27. r Ra The value of CRI shows how much the spectrum of a light source resembles that of the Sun thus the ability of the light source to reproduce the colours of an object as if it were illuminated by the Sun The CRI is calculated with the help of the standard test colours which examine the chromatic adaptation of light The standard set consists of 15 test colours but only the first 8 of them known as R1 R8 are used to calculated the CRI whereas the remaining R9 R15 are typically not used However sometimes LED lights do not have a red light component which is considered in the R9 measurement that is why it is becoming more common to include the R9 measurement as well R9 R15 values can be view in the CRI details window which is opened by clicking on the CRI bar or selecting View gt CRI details CRI details R1 R15 R1 R8 CRI 77 6 93 85 75 74 73 A Ri R n According to the colours table above we can see that the red light of R9 is rather low compared to the rest of the 43 LabSpion user guide values In some cases R9 can even be negative due to particularly low levels of the red light 44 LabSpion user guide Example 1 Shows a standard tungsten lamp Its continuous spectrum has the closest resemblance to the Sun therefore the CRI values are the highest Example 2 Shows a Philips LED bulb with a low red R9 value Example 3 Shows a standard LED bulb with a negative r
28. stallation should be adjusted accordingly The excess current will result in power loss due to cables heating etc A general rule is the following a 10W light source with a PF 0 5 must be connected to an installation capable of supplying 20W The corresponding formula reads installation W Power PF 41 LabSpion user guide Example 1 Shows a standard 60W tungsten bulb with an ideal PF of 1 0 and a current curve that Is identical to the voltage Example 2 Shows a LED bulb that has a passive Capacitor power supply which results in a high phase shift Power 65 W PF 1 00 Voltage 240 4 V Current 0 272 A Voltage 240 4 V Current 0 016 A between current and voltage thus resulting in a very low power factor of 0 19 Example 3 Shows a LED bulb of a medium quality switch mode driver with a high capacity peak load thus a medium quality power factor of 0 62 Power 5 2 W PF 0 62 Voltage 238 6 V Current 0 035A Example 4 Shows a LED bulb having a switch mode driver with a particularly bad filtering It results ina Voltage 226 8 V Current 0 125A high noise level of the current Therefore this level of noise would probably not be able to pass the EMC noise level requirements 42 LabSpion user guide CRI details The CRI defines the quality of white light it is also known as the Colour Rendering Index o
29. tically A successful connection is shown with a green Connected icon in the upper right corner of the Viso Light Inspector software Li vw 3 You can connect and disconnect the USB without restarting the Viso Light Inspector software as the connection is always established automatically as soon as the USB connector is plugged in and vice versa 16 LabSpion user guide Connecting LabSensor The LabSpion is connected to the LabSensor with a RJ45 cable which is supporting the transfer of data and power between the two parts 468 VISO L mai LabSensor s5 msgtemen aes AIC LASER Mea ON DST Warning Do not connect the LabSensor to the C plane motor connector this could damage the LabSensor 17 LabSpion user guide Connecting the C plane goniometer The C plane goniometer is connected to the LabSpion base through a RJ45 cable The LabSpion will automatically detect the C plane goniometer O e POWER VEL LAMP MAX 34 J Q C MOTOR FUSE 6A PHI sv E gt Warning Do not connect the C plane motor to the LabSensor connector this could damage the LabSpion 18 LabSpion user guide Connecting a lamp power The LabSpion has a built in power analyser and a power switch The power switch is used to switch off the lamp before every measurement so that the values of the ambient light are obtained and subsequently subtracted from final measurements The maxi
30. tment of the same table are useful when measuring light sources with asymmetric or tilted intensity distribution curves for example 4 outdoor or automotive EEE OP ROD aS EN lighting fixtures can yield slight tilts which are corrected by the software as shown in the relevant picture 28 LabSpion user guide Correct angle adjusts the off centred intensity distribution relative to the 0 axis so that it becomes symmetric Correct O intensity equates the intensities at the O axis for all of the c planes during a measurement as sometimes the intensity values for different c planes can vary due to goniometer misalignment Correct asymmetry modifies the profile of the distribution to be vertically symmetric Such a symmetry is required for further calculation of UGR unified glare rating in an LDT editor However this modification should not be applied for light sources with off centred beams like street lighting systems Auto shift C plane allows the software to automatically choose and display the C plane with the highest value of the intensity distribution in candela This option is useful when the data files are opened in Dialux or Relux Override option can be Setphotometric EI used to modify the flux in lumen so that the 7 Owe nn exported pdf report EE E shows the desired value in accordance with the customer s desires for instance 110 Im in t
31. tup gt Integration time Intergration time i Spectrometer intergration time 200ms Calibrate to ambient light Set manually V Set intergration time manually WJ 36 LabSpion user guide Independently running spectrometer The photo spectrometer can also be used to run independenily to test different light sources that might be too large tor a complete goniometer measurement or to have a real time update on how the light source behaves over time To start the photo spectrometer independent fm operation click on the spectrum scan icon During the independent run mode the light intensity output in candela CRI and colour temperature are being continuously updated The integration time can be changed during the free run scan as explained in the previous chapter to ensure a correct resolution NOTE After changing the photo spectrometer integration time the spectrum should be Calibrated to ambient light 37 LabSpion user guide Measurement data After the goniometer measurement is complete the following results are displayed 214 4 1 The angular light distribution shows the amount of light from the non rotational symmetrical part of the light source This field distribution is used to calculate the beam angle 2 The complete integrated spherical spectrum is shown in the spectral window Integrated spherical spectrum signifies a spectrum that is mathematically integrated from all o

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