A numerical model of a coronal mass ejection: Shock development with implications for the acceleration of GeV protons

Astrophysical Journal

Volumn 605, Issue 1 II, 2004, Pages

  Roussev, I I ^a   Sokolov, I V ^a   Forbes, T G ^b   Gombosi, T I ^a   Lee, M A ^b   Sakai, J I ^c  

^a UNIVERSITY OF MICHIGAN   (United States)

^b University of New Hampshire   (United States)

^c UNIVERSITY OF TOYAMA   (Japan)

Author keywords

Acceleration of particles; MHD; Shock waves; Solar wind; Sun: coronal mass ejections (CMEs); Sun: magnetic fields

Indexed keywords

EID: 2542530820     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/392504     Document Type: Article

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