Long time incompressible 2D MHD simulations of coronal loop heating: The role of photospheric time-scales

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 575, 2004, Pages 523-528

  Romeou, Zaharenia ^c   Velli, Marco ^a   Einaudi, Giorgio ^b  

^a UNIVERSITY OF FLORENCE   (Italy)

^b UNIVERSITY OF PISA   (Italy)

^c NONE

Author keywords

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

Indexed keywords

ENERGY DISSIPATION; HEAT RADIATION; MAGNETIC FIELD EFFECTS; MAGNETOHYDRODYNAMICS; PLASMAS; TURBULENCE;

SPATIAL DISTRIBUTION; SUN:ACTIVITY; SUN:CORONA; SUN:MAGNETIC FIELDS;

SUN;

EID: 22144495798     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

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