The correlation among the rise velocity of a soft X-ray loop, the ejection velocity of a plasmoid, and the height above the loop top of the hard X-ray source in Masuda-type flares, and its interpretation based on the reconnection model of flares

Astrophysical Journal

Volumn 683, Issue 2 PART 2, 2008, Pages

  Shimizu, M ^a   Nishida, K ^a   Takasaki, H ^b   Shiota, D ^c   Magara, T ^c   Shibata, K ^a  

^a KYOTO UNIVERSITY   (Japan)

^b ACCENTURE   (United States)

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Gamma rays; Subject headings: MHD; Sun: flares; Sun: X rays

Indexed keywords

EID: 65549113331     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/591645     Document Type: Article

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