Modeling magnetohydrodynamics and non-equilibrium SoHO/UVCS line emission of CME shocks

Astronomy and Astrophysics

Volumn 481, Issue 3, 2008, Pages 835-844

  Pagano, P ^a,b,c   Raymond, C ^b   Reale, F ^a,c   Orlando, S ^c  

^a UNIVERSITY OF PALERMO   (Italy)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

Author keywords

Magnetohydrodynamics (MHD); Sun: corona; Sun: coronal mass ejections (CMEs)

Indexed keywords

MATHEMATICAL MODELS; SHOCK WAVES; SOLAR SYSTEM; ULTRAVIOLET RADIATION;

CORONAL MASS EJECTIONS (CME); SOLAR CORONA;

MAGNETOHYDRODYNAMICS;

EID: 41649109045     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079088     Document Type: Article

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