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Cosmic-ray intensity versus solar soft X-ray background in cross-correlation analysis

✍ Scribed by Maria Jakimiec; Anna Antalová; Marisa Storini


Book ID
110221855
Publisher
Springer
Year
1999
Tongue
English
Weight
144 KB
Volume
189
Category
Article
ISSN
0038-0938

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High resolution profiles of the Mg xn 8.42 A line in the solar X-ray spectrum were recorded from the Intercosmos 7 satellite. The Mg xaI line intensity provides a sensitive indicator of the hot plasma content (T > 3 • 106K) in coronal condensations and X-ray flare volumes. The ratio of the line inte