Computer Science
Scientific paper
Dec 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8128032h&link_type=abstract
Unknown
Computer Science
Coronagraphs, Solar Corona, Solar Flares, Solar Observatories, Magnetic Disturbances, Solar Activity, Sunspots, X Ray Spectroscopy
Scientific paper
Part 1: Large-scale emission features visible in soft X-ray photographs from the spectrographic telescope S-054 on Skylab have been superposed on Ha Synoptic Charts for Carrington Rotations 1601 through 1610. The charts identify loop arcades and loop complexes associated with strong magnetic fields, as well as coronal holes and areas devoid of emission loops. Althrough not adequate for the study of the geometry of individual features, the charts convey a global sense of coronal structure which is often difficult to obtain from individual (disk) images. Part 2: Charts of time versus longitude for each of Carrington Rotations 1600 - 1611 depict: (1) Ha importance, brightness, and location of confirmed flares; (2) peak flare X-ray flux 1-8 A; (3) peak flare decimetric radio intensity; and (4) flux of 1.8 - 4.5 Mev protons plotted at their high coronal emission longitude estimated from simulataneously measured solar wind velocity.
Gold Robert E.
Hanson John M.
Roelof Edmond C.
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