The effect of elliptic shape on the period ratio P1/P2 of emerging coronal loops

Astronomy and Astrophysics

Volumn 502, Issue 1, 2009, Pages 315-323

  Morton, R J ^a   Erdelyi R ^a  

^a UNIVERSITY OF SHEFFIELD   (United Kingdom)

Author keywords

Magnetohydrodynamics (MHD); Plasmas; Sun: Corona; Waves

Indexed keywords

A-DENSITY; ARC SHAPE; CHARACTERISTIC TIME; CORONAL LOOPS; EIGEN FREQUENCIES; ELLIPTIC SHAPE; ELLIPTICAL SHAPES; FIRST HARMONIC; FUNDAMENTAL MODES; MAGNETIC FLUX TUBE; MAGNETOHYDRODYNAMICS (MHD); OSCILLATION PERIODS; SOLAR ATMOSPHERE; STRATIFIED ATMOSPHERE; SUN: CORONA; TRANSVERSAL OSCILLATIONS;

FLUID DYNAMICS; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETIC STRUCTURE; MAGNETOHYDRODYNAMICS; PLASMAS; SUN;

GEOMETRY;

EID: 68349110696     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811405     Document Type: Article

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