The influence of longitudinal density variation in coronal loops on the eigenfunctions of kink-oscillation overtones

Astronomy and Astrophysics

Volumn 497, Issue 1, 2009, Pages 265-272

  Andries, J ^a,b   Arregui, I ^c   Goossens, M ^a  

^a CENTRE FOR PLASMA ASTROPHYSICS   (Belgium)

^b MONASH UNIVERSITY   (Australia)

^c UNIVERSITAT DE LES ILLES BALEARS   (Spain)

Author keywords

Magnethohydrodynamics (MHD); Sun: corona; Sun: magnetic fields; Sun: oscillations; Waves

Indexed keywords

APPROXIMATE ANALYTICAL RESULTS; CORONAL LOOPS; DENSITY STRATIFICATIONS; DENSITY VARIATIONS; EIGEN FUNCTIONS; EQUILIBRIUM DENSITIES; LINEAR EXPANSIONS; LONGITUDINAL DIRECTIONS; LONGITUDINAL PROFILES; MAGNETHOHYDRODYNAMICS (MHD); NUMERICAL COMPUTATIONS; OSCILLATION AMPLITUDES; OSCILLATION MODES; SUN: CORONA; SUN: MAGNETIC FIELDS; SUN: OSCILLATIONS; THIN TUBES;

MAGNETIC FIELDS; MOTION ESTIMATION;

SUN;

EID: 63849250789     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811481     Document Type: Article

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