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The identification and interaction of network, intranetwork, and ephemeral-region magnetic fieldsNetwork magnetic fields are described as the dynamic product of the merging and cancelling of intranetwork fields, ephemeral regions, and the remnants of active regions. The similarities of these phenomena with solar magnetic features are pointed out. The intranetwork magnetic fields are characterized by the flow of successive fragments in approximately radial patterns away from their apparent source sites.
Document ID
19890035194
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Martin, Sara F.
(Big Bear Solar Observatory Pasadena, CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1988
Publication Information
Publication: Solar Physics
Volume: 117
Issue: 2 19
ISSN: 0038-0938
Subject Category
Solar Physics
Accession Number
89A22565
Funding Number(s)
CONTRACT_GRANT: NGL-05-002-034
CONTRACT_GRANT: AF-AFOSR-82-0018
CONTRACT_GRANT: NSF ATM-85-13577
Distribution Limits
Public
Copyright
Other

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