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Soft X-Radiation from Single Active Regions

Published online by Cambridge University Press:  14 August 2015

D. H. Brabban ,
E. B. Dorling ,
W. M. Glencross  and
J. R. H. Herring
D. H. Brabban
Affiliation:
Mullard Space Science Laboratory, Dept. of Physics and Astronomy, University College London, WC1E 6BT, England
E. B. Dorling
Affiliation:
Mullard Space Science Laboratory, Dept. of Physics and Astronomy, University College London, WC1E 6BT, England
W. M. Glencross
Affiliation:
Mullard Space Science Laboratory, Dept. of Physics and Astronomy, University College London, WC1E 6BT, England
J. R. H. Herring
Affiliation:
Mullard Space Science Laboratory, Dept. of Physics and Astronomy, University College London, WC1E 6BT, England

Summary

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The MSSL/Leicester University package on OSO 5 contained proportional counters having fields of view small compared with the area of the solar disk (Herring et al., 1971). Results discussed here were obtained with a detector sensitive in the band 0.3–0.9 nm. This had an entrance window collimated to examine a strip of angular width 2′ lying across the Sun.

Type
Part 2: Active Regions
Information
Symposium - International Astronomical Union , Volume 68: Solar X, Gamma, and EUV Radiation , 1975 , pp. 101 - 102
Copyright
Copyright © Reidel 1975 

References

Glencross, W. M., Dorling, E. B., and Herring, J. R. H.: 1974, Solar Phys. 38, 183.CrossRefGoogle Scholar
Herring, J. R. H., Glencross, W. M., Parkinson, J. H., and Pounds, K. A.: 1971, Proc. Roy. Soc. Lond. A 321, 493.Google Scholar