Illuminance meter Asteria cosine corrector-Asteria cosine collector
Illuminance meter Asteria cosine corrector-Admesy Japan LLC

Illuminance meter Asteria cosine corrector
Admesy Japan LLC


About This Product

Asteria is a high-speed photometer suitable for measuring illuminance. Because it is fast and highly stable, it is possible to measure the waveform of a light source and understand flicker characteristics. Designed for in-line use, Asteria is available in multiple configurations and can be fitted with M8 fiber connectors for installations in limited space. ■Highlights ・Absolute illumination (CIE1931 luminosity function) ・High sampling rate (186,567 samples/sec) Large capacity memory ・Measure high frequency range and low frequency range simultaneously ・Flicker measurement standard: ・Flicker percentage, index (IES) ・IEEE 1789 ・Compatible with Windows, OS X, Linux ・Major programming languages ​​(Labview, Labwindows, Visual Studio, C++/C#/VB) and other programming languages ​​compatible with VISA can be used ・Equipped with auto range function ・User calibration function ・Trigger input/output for inline applications

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    Illuminance meter Asteria cosine corrector

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1 Models of Illuminance meter Asteria cosine corrector

Product Image Part Number Price (excluding tax) Detector Dimensions (height x width x depth) Illuminance/brightness accuracy Integration mode range Interface Measurement parameters Measurement speed Sampling mode Operating temperature Optical system Repeatability Sampling mode range Spectral response Weight
Illuminance meter Asteria cosine corrector-Part Number-Asteria cosine collector

Asteria cosine collector

Available upon quote Silicon photodiode 69mm×31mm×93mm ±2% 0.05lx - 150,000lx
Integration time 1ms to 5 seconds
USB 2.0, RS 232, trigger input/output Illuminance, luminous intensity, flicker (percentage, index), waveform 186,567 samples/sec
Memory for up to 250,000 samples
10℃~35℃ 1cm2 cosine corrector, Lambertian response ±0.03% 10lx - 150,000lx Approximate CIE 1931 brightness curve 320g

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