On the differences in composition between solar energetic particles and solar wind

Space Science Reviews

Volumn 130, Issue 1-4, 2007, Pages 207-219

  Mewaldt, R A ^a   Cohen, C M S ^a   Mason, G M ^b   Cummings, A C ^a   Desai, M I ^c   Leske, R A ^a   Raines, J ^d   Stone, E C ^a   Wiedenbeck, M E ^e   Von Rosenvinge, T T ^f   Zurbuchen, T H ^d  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b JOHNS HOPKINS UNIVERSITY APPLIED PHYSICS LABORATORY   (United States)

^c SOUTHWEST RESEARCH INSTITUTE   (United States)

^d UNIVERSITY OF MICHIGAN   (United States)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

Acceleration of particles; Sun: abundances; Sun: coronal mass ejections (CMEs); Sun: flares; Sun: particle emission; Sun: solar wind

Indexed keywords

INTERPLANETARY FLIGHT; PARTICLE BEAM DYNAMICS; PHASE COMPOSITION; SHOCK WAVES; SOLAR ENERGY;

ACCELERATION OF PARTICLES; CORONAL MASS EJECTIONS (CME); PARTICLE EMISSION; SOLAR ENERGETIC PARTICLES (SEP);

SOLAR WIND;

EID: 34748907822     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/s11214-007-9187-1     Document Type: Conference Paper

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