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The formation of the CaiiK line in a spinning spicule

โœ Scribed by Lorne W. Avery


Publisher
Springer
Year
1970
Tongue
English
Weight
851 KB
Volume
13
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


The emission of the CaII K line from a spinning cylindrical spicule model is considered. In order to reproduce the observed spicule K line profiles, the model must have both radial and axial gradients in Ne and Te. The rotating spicule model is optically thin at all heights and is hotter and more dense than a stationary model computed in a previous paper. It is proposed that the so-called Type I and Type II spicules may be structurally the same features, with different rotational velocities.


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