Solar flare plasma properties derived from the disk-integrating GOES X-ray sensors during an eclipse

Details Solar flare plasma properties derived from the disk-integrating GOES X-ray sensors during an eclipse Solar flare plasma properties derived from the disk-integrating GOES X-ray sensors during an eclipse

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...231..525b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 231, no. 2, May 1990, p. 525-535. Research supported by NOAA.

Astronomy and Astrophysics

Astrophysics

6

Goes Satellites, Solar Eclipses, Solar Flares, Solar X-Rays, Emission Spectra, Line Spectra, Solar Corona, Solar Flux, Solar Temperature

Scientific paper

Data from the disk-integrating GOES-6 and GOES-7 X-ray sensors obtained during a partial solar eclipse caused by the moon are analyzed to extract the locations, sizes, and fluxes of the flare and three additional X-ray sources. The results are then compared with spatially resolved observations. The temperature, emission measure, and density of the X-ray sources are discussed, and possible causes for the small differences between the fluxes observed at the two satellites are examined.

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