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Chapman function
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Chapman function : ウィキペディア英語版
Chapman function
A Chapman function describes the integration of atmospheric absorption along a slant path on a spherical earth, relative to the vertical case. It applies for any quantity with a concentration decreasing exponentially with increasing altitude. To a first approximation, valid at small zenith angles, the Chapman function for optical absorption is equal to
:sec(z),\
where ''z'' is the zenith angle and sec denotes the secant function.
The Chapman function is named after Sydney Chapman.
== See also ==

* Atmospheric physics
* Ionosphere

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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