Proton enhancement and decreased O6+/H at the heliospheric current sheet: Implications for the origin of slow solar wind

AIP Conference Proceedings

Volumn 1216, Issue , 2010, Pages 363-366

  Liu, Y C M ^a   Galvin, A B ^a   Popecki, M A ^a   Simunac, K D C ^a   Kistler, L ^a   Farrugia, C ^a   Lee, M A ^a   Klecker, B ^b   Bochsler, P ^a,c   Luhmann, J L ^d   Jian, L K ^e   Moebius, E ^a   Wimmer Schweingruber, R ^f   Wurz, P ^c  

^a UNIVERSITY OF NEW HAMPSHIRE   (United States)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c UNIVERSITY OF BERN   (Switzerland)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e UNIVERSITY OF CALIFORNIA   (United States)

^f UNIVERSITY OF KIEL   (Germany)

Author keywords

Heliospheric current sheet; Heliospheric plasma sheet; Proton enhancement; Slow solar wind; Solar wind plasma composition; Streamer belt

Indexed keywords

EID: 77952083493     PISSN: 0094243X     EISSN: 15517616     Source Type: Conference Proceeding    
DOI: 10.1063/1.3395875     Document Type: Conference Paper

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