Investigation of mass flows in the transition region and corona in a three-dimensional numerical model approach

Astronomy and Astrophysics

Volumn 531, Issue , 2011, Pages

  Zacharias, P ^a   Peter, H ^b   Bingert, S ^b  

^a KIEPENHEUER INSTITUT FÜR SONNENPHYSIK   (Germany)

^b MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

Stars: coronae; Sun: corona; Sun: transition region; Sun: UV radiation; Techniques: spectroscopic

Indexed keywords

STARS: CORONAE; SUN : CORONA; SUN: TRANSITION REGION; SUN: UV RADIATION; TECHNIQUES: SPECTROSCOPIC;

DOPPLER EFFECT; ELECTROMAGNETIC WAVE EMISSION; INVESTMENTS; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; MAGNETOPLASMA; MASS TRANSFER; THERMAL LOGGING; ULTRAVIOLET RADIATION;

THREE DIMENSIONAL;

EID: 79959527530     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016047     Document Type: Article

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