Laboratory-produced radiation related to the solar flare emission
A review is given of continuing efforts to generate laboratory spectra at photon energies above 1 keV from highly ionized atoms. Emphasis is placed on the most easily-interpreted highest ion stages such as the hydrogenic, helium-like and lithium-like species. The close similarities to solar flare ob...
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Published in: | Space science reviews Vol. 13; no. 4-6; pp. 747 - 760 |
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Main Authors: | , |
Format: | Journal Article |
Language: | English |
Published: |
01-01-1972
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Online Access: | Get full text |
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Summary: | A review is given of continuing efforts to generate laboratory spectra at photon energies above 1 keV from highly ionized atoms. Emphasis is placed on the most easily-interpreted highest ion stages such as the hydrogenic, helium-like and lithium-like species. The close similarities to solar flare observations of certain signatures, such as the line and continuum X-ray spectra and microwave emission as well as their sequence of occurrence, are pointed out and scaling factors are given. |
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Bibliography: | SourceType-Scholarly Journals-2 ObjectType-Feature-2 ObjectType-Conference Paper-1 content type line 23 SourceType-Conference Papers & Proceedings-1 ObjectType-Article-3 |
ISSN: | 0038-6308 1572-9672 |
DOI: | 10.1007/BF00213510 |