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SUNSPOT'S MOTIONS AND COMPLEX MAGNETIC FIELDS WITHIN THE AR 5395 (Abstract)

SUNSPOT'S MOTIONS AND COMPLEX MAGNETIC FIELDS WITHIN THE AR 5395 (Abstract)
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摘要 The super-active region AR 5395 emerged from the high latitude zone, rarely. Thephotospheric spots was a big group with complex magnetic fields, i.e., δ-structure. OnMarch 13, 1989 the AR area came to its maximum; 3589 units (1unit=10<sup>-6</sup> Hemisphere). The umbra with S polarity, which presented U-shape, sur-
出处 《天文研究与技术》 CSCD 1990年第4期28-28,共1页 Astronomical Research & Technology
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