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FORMATION OF COUPLED SPECTRAL LINES IN A PLANETARY ATMOSPHERE: II. NUMERICAL EVALUATION OF APPROXIMATE SOLUTIONS.

Author
CHAMBERLAIN JN; SMITH GR
DEP. SPACE PHYS. ASTRON., RICE UNIV., HOUSTON, TEX. 77001
Source
ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 199; NO 1 PART. 1; PP. 282-288; BIBL. 8 REF.
Document type
Article
Language
English
Keyword (fr)
ATMOSPHERE PLANETAIRE CALCUL NUMERIQUE FORMATION RAIE SPECTRALE TRANSFERT RADIATIF FONCTION H ASTRONOMIE
Keyword (en)
PLANETARY ATMOSPHERE NUMERICAL CALCULATION SPECTRAL LINE FORMATION RADIATIVE TRANSFER H FUNCTION ASTRONOMY
Keyword (es)
ASTRONOMIA
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
PASCAL7730287647

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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