SCOPUS 정보 검색 플랫폼

Astronomy and Astrophysics

Volumn 385, Issue 3, 2002, Pages 1056-1072

A two-component model of the solar photosphere from the inversion of spectral lines

(2) Borrero, J M a Bellot Rubio, L R b

a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG (Germany)

b INSTITUTO DE ASTROFÍSICA DE CANARIAS (Spain)

Author keywords

Atomic data; Line: profiles; Stars: abundances; Stars: atmospheres; Sun: abundances; Sun: photosphere

Indexed keywords

ATMOSPHERIC SPECTRA; ATMOSPHERIC STRUCTURE; ATMOSPHERIC TEMPERATURE; MATHEMATICAL MODELS; SOLAR SYSTEM; THERMAL STRATIFICATION; THERMODYNAMIC PROPERTIES;

LINE TRANSITION PARAMETER; SOLAR PHOTOSPHERE;

ASTROPHYSICS;

EID: 0036531439 PISSN: 00046361 EISSN: None Source Type: Journal
DOI: 10.1051/0004-6361:20020176 Document Type: Article

Times cited : (65)

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