NASA NTRS · 19830011420
Solar coronal non-thermal processes (Solar Maximum Mission)
Abstract
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.
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Hudson, H. S.. 1983-02-01. Solar coronal non-thermal processes (Solar Maximum Mission). https://ntrs.nasa.gov/citations/19830011420
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