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Highnsolar radio recombination lines

โœ Scribed by A. Greve

Publisher
Springer
Year
1977
Tongue
English
Weight
243 KB
Volume
52
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

For a representative set of atmospheric and atomic parameters we determine the strengths of solar dielectronic recombination lines originating in ions with Z<~ 6 at frequencies of ~>70 GHz. We compare the line strengths derived here with those calculatedby Berger and Simon (1972) and find that our values for representative ions with Z~3 are lower by a factor 102-103, being mainly the result of the inclusion of the electronic pressure broadening. We outline the requirements for the detection of lines, which must establish an upper limit of at least ~10 -5 for the line to continuum ratio.

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