Lisun LMS-9000B 고정밀 CCD 분광 방사 측정기 (380 ~ 800nm)

LMS-9000A/LMS-9000B is according to LM-79 clause 9.1. It is designed 

to have a capability of producing any visible spectral distribution, 

mimicking various light sources in the visible region by feedback 

control of the radiant power emitted by individual LEDs. This LED 

test system will be used as a transfer standard for photometric, 

colorimetric and radiometric applications.

LMS-9000B is quick test with high accuracy, it used in Scientific 

lab test. Due to the test speed and LMS-9000B can work with LSG-1600B

/LSG-1800B/LSG-1900/LSG-2000 goniophotometer to do the Spatial color 

and Spectrum test.

Measures:

• Colorimetric: Chromaticity Coordinates, CCT, Color Ratio, Peak 

Wavelength, Half Bandwidth, Dominant Wavelength, Color Purity, CRI, Spectrum Test

• Photometric: Luminous Flux, Luminous Efficiency, Radiant Power, 

Pupil Flux, Pupil Flux Efficiency, Pupil Factor, Cirtopic Flux

• Electrical: Voltage, Current, Power, Power Factor

Specifications:

• Spectral Range Wavelength: 380nm~800nm

• Spectral Wavelength Accuracy: ±0.5nm(LMS-9000A), ±0.3nm(LMS-9000B), 

Wavelength Reproducibility: ±0.5nm(LMS-9000A), ±0.1nm(LMS-9000B)

• Sample Scanning Steps: ±0.1nm

• Accuracy of Chromaticity Coordinate (Δx, Δy): ±0.003 (LMS-9000A) and ±0.002 (LMS-9000B)

• Correlated Color Temperature CCT: 1, 500K~25, 000K(LMS-9000A), 1500K~100, 000K(LMS-9000B), CCT Accuracy: ±0.5%(LMS-9000A), ±0.3%(LMS-9000B)

• Color Rendering Index Range: 0~100.0, Accuracy: ±(0.3%rd±0.3)

• Photometric linear: ±0.5% (LMS-9000A) and ±0.3% (LMS-9000B)

• Stray light: <0.015%(600nm) and <0.03%(435nm)

• Time of integration: 0.1mS~20S (LMS-9000A) and 0μs-10s (LMS-9000B)

• It can measure the temperature inside and outside of integrating sphere

LMS-9000A/LMS-9000B used the Band pass-filter Wheel Correcting Technique, Spectrometer & Broadband-radiometer & photometer Combined Technique, and modified NIST stray light correction technology, the LMS-9000A/LMS-9000B spectroradiometer can realize ultra low stray light and super photometry linearity in overall dynamic range.

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