Coronal electron temperature from the solar wind scaling law throughout the space age

Astrophysical Journal

Volumn 739, Issue 1, 2011, Pages

  Schwadron, N A ^a   Smith, C W ^a   Spence, H E ^a   Kasper, J C ^b   Korreck, K ^b   Stevens, M L ^b   Maruca, B A ^b   Kiefer, K K ^b   Lepri, S T ^c   McComas, D ^d,e  

^a UNIVERSITY OF NEW HAMPSHIRE   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c UNIVERSITY OF MICHIGAN   (United States)

^d SOUTHWEST RESEARCH INSTITUTE   (United States)

^e UNIVERSITY OF TEXAS AT SAN ANTONIO   (United States)

Author keywords

solar wind; Sun: corona; Sun: coronal mass ejections (CMEs); Sun: dynamo; Sun: evolution; sunspots

Indexed keywords

EID: 80053472431     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/739/1/9     Document Type: Article

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