๐”– Bobbio Scriptorium
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Soft x-ray emitting regions in the solar corona

โœ Scribed by M. Landini; B. C. Monsignori Fossi


Publisher
Springer
Year
1971
Tongue
English
Weight
485 KB
Volume
17
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


The soft X-ray emission of the solar corona is investigated by comparison of the signals of several broad band photometers carried on the Solrad 9 satellite, and sensitive to the region 0.5-20 A. Temperature from 1.5 โ€ข 106 to 25 โ€ข 106 K have been measured with 'emission measure' S N~2 dVranging between 10 ~~ cm 3 to 1047 cm -a.

By means of the observational data and assuming magnetic confinement and hydrostatic equilibrium, the model of an active region is investigated. For temperatures larger than 107 K the emission is due to flare activity and two sets of emission measure are observed which appear to be related to the evolution of flares.


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