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Extending the sun's magnetic field through the three-dimensional heliosphereMethods for inferring the interplanetary magnetic field are reviewed. Estimates of the configuration of the field are presented for each phase of the sunspot cycle. The limitations of the methods for predicting it are presented. A contour map of power in the 0.3-0.5 microHz frequency range is presented for various solar latitudes.
Document ID
19890058804
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0273-1177(89)90108-7
Authors
Hoeksema, J. Todd (Stanford University CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Publication Information
Publication: Advances in Space Research
Volume: 9
Issue: 4 19
ISSN: 0273-1177
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0273-1177
Accession Number
89A46175
Funding Number(s)
CONTRACT_GRANT: NSF ATM-86-18263
CONTRACT_GRANT: N00014-86-K-0085
CONTRACT_GRANT: NGR-05-020-559
Distribution Limits
Public
Copyright
Other

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