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The high-energy flare plasma

Published online by Cambridge University Press:  14 August 2015

C. De Jager
C. De Jager*
Affiliation:
University Observatory ‘Sonnenborgh’ and Space Research Laboratory, Utrecht, The Netherlands

Extract

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A solar flare has various aspects: the optical flare is often associated with emissions in the microwave or X-ray regions: this indicates the occurrence of a highly excited plasma, which we call the high-energy flare plasma. The existence of the high-energy flare plasma was first shown by radio observations in the microwave regions (Hachenberg) and later confirmed by X-ray observations in the energy range 102–106 eV.

Type
Part VI: Transient Phenomena
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 480 - 482
Copyright
Copyright © Reidel 1968 

References

Alfvén, H., Carlqvist, P. (1967) Solar Phys., 1, 220.Google Scholar