Preferential heating of particles by H-cyclotron waves generated by a global magnetohydrodynamic mode in solar coronal holes

Astrophysical Journal

Volumn 597, Issue 1 II, 2003, Pages

  Zhang, T X ^a,b  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

Author keywords

Acceleration of particles; Instabilities; Plasmas; Solar wind; Sun: corona; Waves

Indexed keywords

EID: 0242635593     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/379798     Document Type: Article

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