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Chapman Function for an Atmosphere with a Constant Temperature Gradient

Geophysical Journal of the Royal Astronomical Society (1968) 15(1-2) 137-145
DOI: 10.1111/j.1365-246X.1968.tb05753.x
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Abstract

Chapman's function is derived for an atmosphere with linear temperature decrease or increase (inversion) for larger zenith distances of the rays, as well as for grazing incidence. For the temperature gradient approaching to zero the proper limits are derived and the results brought to the form of the original Chapman function, derived for an isothermal atmosphere. Copyright © 1968, Wiley Blackwell. All rights reserved

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APA

Sekera, Z. (1968). Chapman Function for an Atmosphere with a Constant Temperature Gradient. Geophysical Journal of the Royal Astronomical Society, 15(1–2), 137–145. https://doi.org/10.1111/j.1365-246X.1968.tb05753.x

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