๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

An investigation of the structure of coronal active regions

โœ Scribed by J. H. Parkinson


Publisher
Springer
Year
1973
Tongue
English
Weight
333 KB
Volume
28
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


The temperature and density structure of a 'typical' coronal active region is deduced from X-ray observations of several active regions. Observations of the limb transits of three regions from OSO-5 indicate that the X-ray emission originates between 2 x 104 km and 1.5 โ€ข 105 km. An emission measure-temperature distribution is deduced from high resolution X-ray spectra obtained with a rocket observation of two similar regions. These observations are combined to give a model of a 'typical' active region, the temperature varying from 2 to 6 โ€ข 106 K with corresponding densities between 2 โ€ข 109 and 101~ cms -8.


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