Evidence linking coronal transients to the evolution of coronal holes

descriptionPublicationkeyboard_double_arrow_right Article 01 Jul 1978 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 58, pages 389-396 (issn: 0038-0938, eissn: 1573-093X,

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Authors: David F. Webb; Patrick S. MciIntosh; Jerome T. Nolte; Craig V. Solodyna;

doi: 10.1007/bf00157283

Evidence linking coronal transients to the evolution of coronal holes

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Abstract

The positions of X-ray coronal transients outside of active regions observed during Skylab were superposed on H-alpha synoptic charts and coronal hole boundaries for seven solar rotations. A detailed spatial association between the transients and neutral lines was confirmed. It was 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 holes.

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