On the efficiency of plasma heating by Pedersen current dissipation from the photosphere to the lower corona

Astronomy and Astrophysics

Volumn 416, Issue 3, 2004, Pages 1159-1178

  Goodman, M L ^a,b  

^a Institute for Scientific Research Incorporated   (United States)

^b CATHOLIC UNIVERSITY OF AMERICA   (United States)

Author keywords

MHD; Stars: atmospheres; Sun: chromosphere; Sun: corona; Sun: magnetic fields; Sun: transition region

Indexed keywords

ASTROPHYSICS; CARRIER CONCENTRATION; ELECTRIC CONDUCTIVITY; ELECTRIC FIELD EFFECTS; ENERGY DISSIPATION; ENERGY TRANSFER; EXTRATERRESTRIAL ATMOSPHERES; HEAT CONVECTION; MAGNETIZATION; MAGNETOHYDRODYNAMICS; MATHEMATICAL MODELS; PLASMA HEATING; SPACE RESEARCH; TENSORS; THERMAL EFFECTS;

CHROMOSPHERE; PHOTOSPHERES; SUN CORONA;

SUN;

EID: 1642587877     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031719     Document Type: Article

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