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Volumn 548, Issue , 2012, Pages

How reliable is Zeeman Doppler imaging without simultaneous temperature reconstruction?

Author keywords

Methods: numerical; Polarization; Stars: imaging; Stars: magnetic field; Starspots

Indexed keywords

AZIMUTHAL FIELD; DOPPLER IMAGING; FIELD RECONSTRUCTION; FIELD STRENGTHS; FOUR STOKES PARAMETERS; HIGH CONTRAST; INHOMOGENEITIES; LINE PROFILES; LOW LATITUDES; MAGNETIC FEATURES; MAGNETIC FIELD STRENGTHS; METHODS: NUMERICALS; NUMERICAL TESTS; STARS: MAGNETIC FIELD; STARS:IMAGING; STARSPOTS; TEMPERATURE MAPPING; TEMPERATURE RECONSTRUCTION; TEMPERATURE VARIATION;

EID: 84869171660     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219972     Document Type: Article
Times cited : (38)

References (23)
  • 19
    • 0001632176 scopus 로고
    • Semel, M. 1989, A&A, 225, 456
    • (1989) A&A , vol.225 , pp. 456
    • Semel, M.1
  • 20


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.