๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Experiment to determine the temperature structure in the solar chromosphere and corona

โœ Scribed by C. R. Negus

Publisher
Springer Netherlands
Year
1972
Tongue
English
Weight
76 KB
Volume
13
Category
Article
ISSN
0038-6308

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๐Ÿ“œ SIMILAR VOLUMES

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Extreme ultraviolet spectroheliograms in Mg x (625 ~) and the Lyman continuum (897/~) obtained from OSO-6 are used to determine the differential rotation rate in the solar chromosphere and corona. The equatorial rotation rate agrees with spectroscopic measurements of the photospheric plasma velocity

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The temperature structure of the transition region between the chromosphere and corona is discussed in the context of current ideas about magnetic fields in these layers. Magnetic channeling of the downward conductive heat flow from the corona into the regions of enhanced field at the supergranulati

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โœ W. M. Glencross ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 650 KB

Transfer of material between the chromosphere and corona of the Sun must occur whenever the geometry of any interconnecting magnetic structure changes, and there will also be a flow of plasma along field lines caused by any pressure difference between the two feet of each arch. Part of the energy co