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Evidence linking coronal transients to the evolution of coronal holesThe 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.
Document ID
19790031808
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1007/BF00157283
Authors
Webb, D. F. (American Science and Engineering, Inc. Cambridge, MA, United States)
Nolte, J. T. (American Science and Engineering, Inc. Cambridge, MA, United States)
Solodyna, C. V. (American Science and Engineering, Inc. Cambridge, Mass., United States)
Mcintosh, P. S. (NOAA, Space Environment Laboratory, Boulder Colo., United States)
Date Acquired
August 9, 2013
Publication Date
July 1, 1978
Publication Information
Publication: Solar Physics
Volume: 58
Subject Category
Solar Physics
Accession Number
79A15821
Funding Number(s)
CONTRACT_GRANT: NAS8-27758
Distribution Limits
Public
Copyright
Other

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