The rate of photoionization between heights z and is equal to
where for solar zenith angle ,
is the absorption cross-section, and n(z) is the number density of the absorbing gas. Assume an isothermal atmosphere so
Plugging (3) into (2) yields
Plugging (4) into (1) gives
But is monotonic, so f(x) and have maxima and minima at the same values of x. Therefore, there are extrema at
This is a maximum since
Physically, there are many absorbers but few photons near the surface, and many photons but few absorbers at the top of the atmosphere. The product of the two must therefore have a maximum where the two are balanced. Solving (8), the maximum is at
and the photoionization rate at this level is
The integrated rate over the entire atmosphere is then
(1)
where for solar zenith angle ,
(2)
is the absorption cross-section, and n(z) is the number density of the absorbing gas. Assume an isothermal atmosphere so
(3)
Plugging (3) into (2) yields
(4)
Plugging (4) into (1) gives
(5)
(6)
But is monotonic, so f(x) and have maxima and minima at the same values of x. Therefore, there are extrema at
(7)
(8)
This is a maximum since
(9)
Physically, there are many absorbers but few photons near the surface, and many photons but few absorbers at the top of the atmosphere. The product of the two must therefore have a maximum where the two are balanced. Solving (8), the maximum is at
(10)
and the photoionization rate at this level is
(11)
The integrated rate over the entire atmosphere is then
(12)
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