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On the dependence of the two-level source function on its radiation field.The consequences of the universally made assumption that the stimulated emission profile is identical to the absorption profile are quantitatively investigated for a two-level atom with Doppler redistribution. The nonlinear terms arising in the source function are evaluated iteratively. We find that the magnitude of the effects is probably completely negligible for visible and UV solar lines.
Document ID
19730057403
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Steinitz, R.
Shine, R. A.
(Joint Institute for Laboratory Astrophysics Boulder, Colo., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Publication Information
Publication: Royal Astronomical Society
Subject Category
Space Sciences
Accession Number
73A42205
Funding Number(s)
CONTRACT_GRANT: NGR-06-003-057
CONTRACT_GRANT: NBS-(G)-164-IS-TA-A10
CONTRACT_GRANT: AF ORDER Y73-802
Distribution Limits
Public
Copyright
Other

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