Steady 2D prominence-like solutions of the MHD equations with field-aligned compressible flow

Astronomy and Astrophysics

Volumn 429, Issue 3, 2005, Pages 1081-1092

  Petrie, G J D ^a   Tsinganos, K ^a   Neukirch, T ^b  

^a UNIVERSITY OF ATHENS   (Greece)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

Author keywords

Magnetohydrodynamics (MHD); Methods: analytical; Sun: corona; Sun: filaments; Sun: magnetic fields

Indexed keywords

ASTROPHYSICS; COMPUTER SIMULATION; GRAVITATIONAL EFFECTS; HEATING; MAGNETIC FIELDS; SOLAR SYSTEM; THERMAL CONDUCTIVITY; VECTORS; VELOCITY MEASUREMENT;

METHODS: ANALYTICAL; SUN: FILAMENTS; SUN: MAGNETIC FIELDS; SUN:CORONA;

MAGNETOHYDRODYNAMICS;

EID: 11844278536     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041706     Document Type: Article

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