Factors related to the origin of a gradual coronal mass ejection associated with an eruptive prominence on 1998 June 21-22

Astrophysical Journal

Volumn 534, Issue 1 PART 1, 2000, Pages 468-481

  Srivastava, Nandita ^a   Schwenn, Rainer ^a   Inhester, Bernd ^a   Martin, Sara F ^b   Hanaoka, Yoichiro ^c  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b Helio Research   (United States)

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Sun: activity; Sun: corona; Sun: prominences

Indexed keywords

EID: 0034179535     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/308749     Document Type: Article

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