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Evidence linking coronal transients to the evolution of coronal holes

โœ Scribed by David F. Webb; Patrick S. MciIntosh; Jerome T. Nolte; Craig V. Solodyna


Publisher
Springer
Year
1978
Tongue
English
Weight
464 KB
Volume
58
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


The positions of X-ray coronal transients outside of active regions observed during Skylab were superposed on Ha synoptic charts and coronal hole boundaries for seven solar rotations. We confirmed a detailed spatial association between the transients and neutral lines. We found that most of the transients were related to large-scale changes in coronal hole area and tended to occur on the borders of evolving equatorial hol&s.


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He I 10830 ~ synoptic maps, obtained at the Kitt Peak National Observatory during 1974-1979, show that the Sun's polar coronal holes have contracted significantly during 1977-1978. Prior to the accelerated increase of sunspot activity in mid-1977, the area of each polar cap was on the order of 8% of