Spectropolarimetric multi line analysis of stellar magnetic fields

Astronomy and Astrophysics

Volumn 512, Issue 13, 2010, Pages

  Vélez, J C Ramírez ^a,b   Semel, M ^b   Stift, M ^c,d   González, M J Martínez ^d,e   Petit, P ^f   Dunstone, N ^g  

^a UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c UNIVERSITY OF VIENNA   (Austria)

^d OBSERVATOIRE DE PARIS   (France)

^e INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^f UNIVERSITÉ DE TOULOUSE   (France)

^g UNIVERSITY OF ST ANDREWS   (United Kingdom)

Author keywords

Line: formation; Line: profiles; Magnetic fields; Polarization; Radiative transfer

Indexed keywords

IMAGING TECHNIQUES; MAGNETIC MATERIALS; POLARIZATION; RADIATIVE TRANSFER;

CROSS CORRELATIONS; DOPPLER IMAGING TECHNIQUES; INVERSION CODE; LINE SPECTRA; LINE: FORMATION; LINE: PROFILES; MAGNETIC FIELD VECTORS; PHYSICAL PARAMETERS; POLARIZATION PROPERTIES; POLARIZATION SIGNATURES; POLARIZED SIGNALS; POLARIZED SIGNATURES; PRINCIPAL COMPONENTS; PRINCIPLE COMPONENTS ANALYSIS; PSEUDO-LINES; RADIATIVE TRANSFER EQUATIONS; SIGNAL TO NOISE; SOLAR MAGNETIC FIELDS; STELLAR MAGNETIC FIELDS; STELLAR SPECTRA; SYNTHETIC SPECTRA;

MAGNETIC FIELDS;

EID: 77950682888     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200810484     Document Type: Article

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