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The Sun as a Flare Star: X-Ray Spatial and Plasma Properties Derived from a Solar Eclipse Observed by Goes

Published online by Cambridge University Press:  27 September 2017

P. L. Bornmann
P. L. Bornmann*
Affiliation:
Cooperative Institute for Research in Environmental Sciences

Abstract

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The size, location, and flux of four solar soft X-ray sources, including a flare, were derived from the disk-integrating GOES X-Ray Sensors during a solar eclipse. The fluxes were used to derive the temperatures and emission measures of these sources. If an incorrect amount of flux is attributed to the flare source, then the evolution of these derived plasma properties seems unphysical.

Type
Session II: Solar Flares
Information
International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 157 - 160
Copyright
Copyright © Kluwer 1989