A MHD-turbulence model for solar corona

Advances in Space Research

Volumn 43, Issue 4, 2009, Pages 612-617

  Romeou, Z ^a   Velli, M ^b   Einaudi, G ^c  

^a UNIVERSITY OF PATRAS   (Greece)

^b UNIVERSITY OF FLORENCE   (Italy)

^c UNIVERSITY OF PISA   (Italy)

Author keywords

Magnetohydrodynamics (MHD); Sun: activity; Sun: corona; Sun: magnetic fields; Turbulence

Indexed keywords

SOLAR RADIATION; SOLAR SYSTEM; TEMPERATURE; TURBULENCE; TURBULENCE MODELS;

ELECTRIC CURRENT DISSIPATION; EVOLUTIONARY PHASIS; REDUCED MAGNETOHYDRODYNAMICS; STATISTICAL BEHAVIOR; SUN : CORONA; SUN: ACTIVITY; SUN: MAGNETIC FIELD; TWO-DIMENSIONAL CROSS SECTIONS;

MAGNETOHYDRODYNAMICS;

EID: 59749097827     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2008.10.014     Document Type: Article

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