Application of the theory of damping of kink oscillations by radiative cooling of coronal loop plasma

Astronomy and Astrophysics

Volumn 519, Issue 3, 2010, Pages

  Morton, R J ^a   Erdelyi R ^a  

^a UNIVERSITY OF SHEFFIELD   (United Kingdom)

Author keywords

magnetohydrodynamics (MHD); plasmas; Sun: corona; waves

Indexed keywords

COOLING; DAMPING; DYNAMICS; MAGNETOHYDRODYNAMICS; MAGNETOPLASMA; SOLAR WIND;

COMPARATIVE STUDIES; CONSTANT FREQUENCY; COOLING PROCESS; CORONAL LOOPS; DATA POINTS; DISSIPATIVE MECHANISMS; DYNAMIC NATURE; LOOP PLASMA; RADIATIVE COOLING; RESONANT ABSORPTION; SOLAR PLASMA; SUN: CORONA; THEORETICAL MODELS; TIME-DEPENDENT; TIME-SCALES; TRACE OBSERVATIONS; TRANSVERSE OSCILLATION; VARYING BACKGROUND;

PLASMA MAGNETOHYDRODYNAMIC WAVES;

EID: 77956529436     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014504     Document Type: Article

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