Magnetic field evolution leading to solar flares II. Cases with high magnetic shear and flare-related shear change

Publications of the Astronomical Society of Japan

Volumn 52, Issue 3, 2000, Pages 483-497

  Li, Hui ^a,b   Sakurai, Takashi ^b   Ichimoto, Kiyoshi ^b   UeNo, Satoru ^c  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c KYOTO UNIVERSITY   (Japan)

Author keywords

Sun: flares; Sun: magnetic fields; Sun: X rays

Indexed keywords

ACTIVE REGIONS; FIELD EVOLUTION; MAGNETIC FLARES; MAGNETIC SHEAR; MAGNETIC-FIELD; NEUTRAL LINE; SOLAR FLARE; SUN:FLARES; SUN:MAGNETIC FIELDS; SUN:X-RAYS;

MAGNETIC FIELDS;

EID: 0034349668     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/52.3.483     Document Type: Article

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