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Solar coronal non-thermal processes (Solar Maximum Mission)The Solar Maximum Mission was used to study solar coronal phenomena in hard X-radiation, since its instrument complement included the first solar hard X-ray telescope. Phenomena related to those discovered from OSO-5 and OSO-7 observations were emphasized.
Document ID
19830011420
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Hudson, H. S. (California Univ., San Diego La Jolla, CA, United States)
Date Acquired
September 4, 2013
Publication Date
February 1, 1983
Subject Category
Solar Physics
Report/Patent Number
NAS 1.26:169922
SP-83-04
NASA-CR-169922
Report Number: NAS 1.26:169922
Report Number: SP-83-04
Report Number: NASA-CR-169922
Accession Number
83N19691
Funding Number(s)
CONTRACT_GRANT: NSG-5321
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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