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On a cold emission in the solar corona

โœ Scribed by K. V. Alikayeva


Publisher
Springer
Year
1975
Tongue
English
Weight
432 KB
Volume
41
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


The faint emission of hydrogen, helium and metals in the corona which appeared near an active prominence is studied. The calculations showed that the temperature of the emission region is in the limits from 10000 K to 30000 K and the electron density is between 109-10 x~ cm -3, respectively.


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