Physics
Scientific paper
Mar 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985stin...8616179s&link_type=abstract
Unknown
Physics
Brightness, Solar Corona, Solar Prominences, Solar Wind, Distribution (Property), Emission Spectra, Solar Cycles, Solar Maximum Mission, Stellar Luminosity
Scientific paper
Synoptic observations of the solar corona in white light and in three emission lines (CaXV at 5964 A, FeXIV at 5303 A, and Fe X at 6374 A) were carried out during most of 1984 at the High Altitude Observatory's Mauna Loa Solar Observatory and at Sacramento Peak Observatory. These observations were partly in support of the scientific program of the repaired SMM spacecraft. The observations provide a record of the distribution and brightness of the hotter regions of the corona over the year. The authors present these data in the form of synoptic maps for each rotation during the year for the purpose of providing a context for the investigations which are to take place during the Joint Study of Coronal and Prominence Plasmas organized by Goddard Space Flight Center/NASA. In this way, they propose both to describe the data coverage achieved and summarize the large scale properties of the corona in this late descending phase of the solar cycle.
Altrock Richard C.
Fisher Richard Royal
Sime D. G.
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