Comparisons of images derived from independent Zeeman Doppler imaging codes

Monthly Notices of the Royal Astronomical Society

Volumn 318, Issue 4, 2000, Pages 961-973

  Hussain, G A J ^a   Donati, J F ^b   Collier Cameron, A ^a   Barnes, J R ^c  

^a UNIVERSITY OF ST ANDREWS   (United Kingdom)

^b OBSERVATOIRE MIDI PYRÉNÉES   (France)

^c CENTRO DE ASTROFÍSICA   (Portugal)

Author keywords

Polarization; Stars: activity; Stars: imaging; Stars: individual: HD 36705; Stars: late type; Stars: magnetic fields

Indexed keywords

LUMINANCE; MAGNETIC FIELD EFFECTS; SIGNAL TO NOISE RATIO; STARS;

DOPPLER IMAGING; MAGNETIC-FIELD; STAR: ACTIVITY; STAR: INDIVIDUAL: HD 36705; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MAGNETIC FIELD; STARS:IMAGING; STARS:LATE TYPE; SURFACE BRIGHTNESS; SURFACE MAP;

DOPPLER EFFECT;

EID: 0000850694     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03573.x     Document Type: Article

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