
illuminance Measurement Trio | 0 20 40 60 80 100 |
| Ra |
Illuminance Spectrophotometer | R1 |
R2 | |
R3 | |
R4 | |
R5 | |
R6 | |
R7 | |
| R8 |
R9 | |
R10 | |
R11 | |
R12 | |
R13 | |
R14 |
D a t a M a n a g e m e n t S o f t w a r e C L - S 1 0 w ( S t a n d a r d a c c e s s o r y )
R15 |
For evaluation of
M a in F e a t u r e s
Convenient,
Reads measurement data from the
Since peak wavelengths can be seen easily, classification and grading of light sources can be performed easily at high accuracy. In addition, numerical data at 1 nm can also be viewed in list form.
0.00E+00360nm 410nm 460nm 510nm 560nm 610nm 660nm 710nm 760nm
The
The
Data Management Software
The
The
In addition to quantifying the color variations which are a major problem in the LED industry, the software is also equipped with function to enable easy binning.
0.5000 |
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| Dominant |
| wavelength |
| Black body |
0.4500 | locus |
2700K | |
| 3000K |
| 3500K |
| 4000K |
PASS
FAIL
Theintegrating sphere for total flux measurements of lightHigh-speed measurement possible sources and lamps.
Using the SDK,0 | 20 | 40 | 60 | 80 |
| 100 |
Ra |
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R2 |
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R3 |
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R4 |
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R5 |
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R6 |
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R7 |
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R8 |
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R9 |
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R10 |
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R11 |
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R12 |
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| 100 | |
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| R15 | R2 | ||
R13 |
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| R14 |
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R14 |
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R15 |
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| R9 | R8 |
0.4000 | 4500K |
| 5000K |
| 5700K |
| 6500K |
0.3500
0.3000
0.2500
0.2000 xy
0.2000 0.2500 0.3000 0.3500 0.4000 0.4500 0.5000
10 Illuminance Spectrophotometer | Illuminance Spectrophotometer |