Shock geometry, seed populations, and the origin of variable elemental composition at high energies in large gradual solar particle events

Astrophysical Journal

Volumn 625, Issue 1 I, 2005, Pages 474-495

  Tylka, A J ^a   Cohen, C M S ^b   Dietrich, W F ^c   Lee, M A ^d   Maclennan, C G ^e   Mewaldt, R A ^b   Ng, C K ^f,g   Reames, D V ^f  

^a NAVAL RESEARCH LABORATORY   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c UNIVERSITY OF CHICAGO   (United States)

^d UNIVERSITY OF NEW HAMPSHIRE   (United States)

^e LUCENT TECHNOLOGIES   (United States)

^f NASA GODDARD SPACE FLIGHT CENTER   (United States)

^g Bldg 142   (United States)

Author keywords

Acceleration of particles; Shock waves; Sun: coronal mass ejections (CMEs); Sun: flares; Sun: particle emission

Indexed keywords

EID: 22144437433     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/429384     Document Type: Article

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