Links between magnetic fields and plasma flows in a coronal hole

Astronomy and Astrophysics

Volumn 432, Issue 1, 2005, Pages

  Wiegelmann, T ^a   Xia, L D ^b   Marsch, E ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

Author keywords

Sun: Corona ; Sun: Doppler shifts; Sun: Magnetic field ; Sun: Uv radiation

Indexed keywords

COMPUTATIONAL METHODS; DOPPLER EFFECT; EXTRAPOLATION; MAGNETIC FIELD EFFECTS; PLASMA FLOW; SUN; TOPOLOGY; ULTRAVIOLET RADIATION;

SUN: CORONA; SUN: DOPPLER SHIFTS; SUN: MAGNETIC FIELD; SUN: UV RADIATION;

ASTROPHYSICS;

EID: 14844284647     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:200500029     Document Type: Article

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