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Resonance-line transfer with partial redistribution. VIII - Solution in the comoving frame for moving atmospheresThe effects of partial frequency redistribution in the scattering process for lines formed in moving atmospheres are analyzed using a general method that allows the transfer equation to be solved in the comoving frame of the gas. The same chromospheric and atomic model studied by Cannon and Vardavas (1974) is employed in the calculations, but a depth scale with logarithmically spaced points is adopted. It is found that in both static and moving atmospheres, the profiles obtained with complete and partial frequency redistribution are virtually identical. The large differences in profiles obtained by Cannon and Vardavas when they used complete and partial redistribution are shown to be spurious (and physically unreal) effects resulting from angle averaging in the observer's frame instead of the comoving frame.
Document ID
19760050317
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Mihalas, D.
(High Altitude Observatory Boulder, Colo., United States)
Shine, R. A.
(Colorado, University Boulder, Colo., United States)
Kunasz, P. B.
(Joint Institute for Laboratory Astrophysics Boulder, Colo., United States)
Hummer, D. G.
(Joint Institute for Laboratory Astrophysics; Colorado, University Boulder, Colo., United States)
Date Acquired
August 8, 2013
Publication Date
April 15, 1976
Publication Information
Publication: Astrophysical Journal
Volume: 205
Subject Category
Astrophysics
Accession Number
76A33283
Funding Number(s)
CONTRACT_GRANT: NAS5-11363
CONTRACT_GRANT: NSF MPS-72-05026A02
Distribution Limits
Public
Copyright
Other

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