Ultraviolet Coronagraph Spectrometer observations of a high-latitude coronal hole with high oxygen temperatures and the next solar cycle polarity

Astrophysical Journal

Volumn 560, Issue 2 PART 2, 2001, Pages

  Miralles, M P ^a   Cranmer, S R ^a   Kohl, J L ^a  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Line: profiles; Solar wind; Sun: activity; Sun: corona; Sun: UV radiation; Techniques: spectroscopic

Indexed keywords

EID: 0035923035     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/324314     Document Type: Article

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