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Determination of the Height of Hard X-Ray Sources in the Solar Atmosphere by Measurement of Photospheric Albedo Photons

Published online by Cambridge University Press:  14 August 2015

John C. Brown  and
H. F. Van Beek
John C. Brown
Affiliation:
Space Research Laboratory of the Astronomical Institute, Utrecht, The Netherlands
H. F. Van Beek
Affiliation:
Space Research Laboratory of the Astronomical Institute, Utrecht, The Netherlands

Summary

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The importance and difficulties of determining the height of hard X-ray sources in the solar atmosphere, in order to distinguish source models, have been discussed by Brown and McClymont (1974) and also in this Symposium (Brown, 1975; Datlowe, 1975). Theoretical predictions of this height, h, range between and 105 km above the photosphere for different models (Brown and McClymont, 1974; McClymont and Brown, 1974). Equally diverse values have been inferred from observations of synchronous chromospheric EUV bursts (Kane and Donnelly, 1971) on the one hand and from apparently behind-the-limb events (e.g. Datlowe, 1975) on the other.

Type
Part 3: Solar Flares
Information
Symposium - International Astronomical Union , Volume 68: Solar X, Gamma, and EUV Radiation , 1975 , pp. 239 - 241
Copyright
Copyright © Reidel 1975 

References

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