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Coronal holes as sources of solar windWe investigate the association of high-speed solar wind with coronal holes during the Skylab mission by: (1) direct comparison of solar wind and coronal X-ray data; (2) comparison of near-equatorial coronal hole area with maximum solar wind velocity in the associated streams; and (3) examination of the correlation between solar and interplanetary magnetic polarities. We find that all large near-equatorial coronal holes seen during the Skylab period were associated with high-velocity solar wind streams observed at 1 AU.
Document ID
19770027726
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1007/BF00149859
Authors
Nolte, J. T. (American Science and Engineering, Inc. Cambridge, MA, United States)
Krieger, A. S. (American Science and Engineering, Inc. Cambridge, Mass., United States)
Timothy, A. F. (NASA Headquarters Washington, DC United States)
Gold, R. E. (American Science and Engineering, Inc. Cambridge, MA, United States)
Roelof, E. C. (Johns Hopkins University Laurel, Md., United States)
Vaiana, G. (Harvard College Observatory and Smithsonian Astrophysical Observatory Cambridge, Mass., United States)
Lazarus, A. J. (American Science and Engineering, Inc. Cambridge, MA, United States)
Sullivan, J. D. (MIT Cambridge, Mass., United States)
Mcintosh, P. S. (NOAA Boulder, Colo., United States)
Date Acquired
August 8, 2013
Publication Date
February 1, 1976
Publication Information
Publication: Solar Physics
Volume: 46
Subject Category
Solar Physics
Accession Number
77A10578
Funding Number(s)
CONTRACT_GRANT: NAS8-31374
CONTRACT_GRANT: F19628-73-C-0070
CONTRACT_GRANT: NAS5-11062
CONTRACT_GRANT: NAS8-27758
Distribution Limits
Public
Copyright
Other

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