Observational evidence favors a resistive wave heating mechanism for coronal loops over a viscous phenomenon

Astronomy and Astrophysics

Volumn 471, Issue 1, 2007, Pages 311-314

  Van Doorsselaere, T ^a   Andries, J ^b,c   Poedts, S ^b  

^a UNIVERSITY OF WARWICK   (United Kingdom)

^b CENTRE FOR PLASMA ASTROPHYSICS   (Belgium)

^c RESEARCH FOUNDATION FLANDERS FWO   (Belgium)

Author keywords

Sun: corona; Sun: oscillations

Indexed keywords

ENERGY ABSORPTION; FUNCTION EVALUATION; HEATING; PLASMA WAVES;

HEATING PROFILES; SUN: CORONA; SUN: OSCILLATIONS;

SOLAR RADIATION;

EID: 34547958940     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066658     Document Type: Article

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