I would propose if you have AM1.5 incident solar radiation spectrum in units w/m^2 nm that you express the shortcircuit current equation in terms of lambda rather that the photon energy. This is ataright forward calculations:
-At first assume P(lambda) ia given
- Convert P(lambda) into photons /m^2 nm by simply dividing every value in the curve by hc/ lambda where lambda that corresponds to a specifci P.
That is the spectrum in photons/m^2/nm = Pph= P lambda/hc,
Then multiply by q and integrate with respect to lambda that is
Jsc= q integal P(Lambda) lambda dlambda from lambda=0 to lambda= Lambda cutoff
I would propose if you have AM1.5 incident solar radiation spectrum in units w/m^2 nm that you express the shortcircuit current equation in terms of lambda rather that the photon energy. This is ataright forward calculations:
-At first assume P(lambda) ia given
- Convert P(lambda) into photons /m^2 nm by simply dividing every value in the curve by hc/ lambda where lambda that corresponds to a specifci P.
That is the spectrum in photons/m^2/nm = Pph= P lambda/hc,
Then multiply by q and integrate with respect to lambda that is
Jsc= q integal P(Lambda) lambda dlambda from lambda=0 to lambda= Lambda cutoff