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Temperature structure and conductive flux in the chromosphere-corona transition region

โœ Scribed by G. Elwert; P. K. Raju

Publisher
Springer
Year
1972
Tongue
English
Weight
451 KB
Volume
25
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES

On the inhomogeneous structure of the ch
On the inhomogeneous structure of the chromosphere-corona transition region above sunspot umbrae
โœ J. Staude ๐Ÿ“‚ Article ๐Ÿ“… 1985 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 398 KB ๐Ÿ‘ 2 views

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โœ Max Kuperus; R. Grant Athay ๐Ÿ“‚ Article ๐Ÿ“… 1967 ๐Ÿ› Springer ๐ŸŒ English โš– 610 KB

Qualitative arguments are presented to show that in the chromosphere-corona transition region the energy which is transported downwards by heat conduction cannot be disposed of by radiative losses only. The region therefore is unstable and forced to be in motion, which may give rise to spicule-like