The energy of a photon is proportional to its frequency and
therefore inversely proportional to wavelength. In order to produce
a signal proportional to the photon flux (number of photons per unit
of area per second) the detector’s spectral power response (in
Amps/[W/cm2]) must be inversely proportional to the photon’s
frequency and therefore proportional to wavelength. Traditionally the quantum flux is measured in micro-moles (also
called micro-Einsteins) per second per square meter. The conversion
factor is:
1µE/s/m2 = 1µmole/s/m2 = 6.02*1017 quanta/s/m2
The angular response of the PMA2132 detector is cosine corrected and
suitable for measurements of diffuse radiation or radiation from
extended sources.

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