Coronal seismology by means of kink oscillation overtones

Space Science Reviews

Volumn 149, Issue 1-4, 2009, Pages 3-29

  Andries, J ^a,d   Van Doorsselaere, T ^b   Roberts, B ^c   Verth, G ^d   Verwichte, E ^b   Erdelyi R ^e  

^a MONASH UNIVERSITY   (Australia)

^b UNIVERSITY OF WARWICK   (United Kingdom)

^c UNIVERSITY OF ST ANDREWS   (United Kingdom)

^d CENTRE FOR PLASMA ASTROPHYSICS   (Belgium)

^e UNIVERSITY OF SHEFFIELD   (United Kingdom)

Author keywords

Magnetohydrodynamics (MHD); Sun corona; Sun magnetic fields; Sun oscillations; Waves

Indexed keywords

CORONA-SUN; CORONAL LOOPS; CORONAL SEISMOLOGY; EIGEN MODES; EQUILIBRIUM PARAMETERS; EQUILIBRIUM PROPERTIES; ERROR BARS; LONGITUDINAL RESOLUTION; MAGNETIC FIELDS-SUN; MAGNETOHYDRODYNAMICS SUNS;

MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; MODEL CHECKING; SEISMOLOGY;

SUN;

EID: 77249177512     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/s11214-009-9561-2     Document Type: Article

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