๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Heating of the solar chromosphere and corona

โœ Scribed by S. P. S. Anand

Publisher
Springer Netherlands
Year
1976
Tongue
English
Weight
519 KB
Volume
43
Category
Article
ISSN
0004-640X

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

Solar rotation in the chromosphere and c
Solar rotation in the chromosphere and corona
โœ William Henze; A. K. Dupree ๐Ÿ“‚ Article ๐Ÿ“… 1973 ๐Ÿ› Springer ๐ŸŒ English โš– 275 KB

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

Heating of the solar corona
Heating of the solar corona
โœ N. D'Angelo ๐Ÿ“‚ Article ๐Ÿ“… 1969 ๐Ÿ› Springer ๐ŸŒ English โš– 444 KB
Is the solar 5 min oscillation an import
Is the solar 5 min oscillation an important heating mechanism for the chromosphere and the corona?
โœ Peter Ulmschneider ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 233 KB

Missing power in the spectrum of intensity fluctuations of both XUV and radio emission in the transition layer and inner corona as well as the 90 ~ phase shift between intensity and velocity fluctuations in the chromosphere indicate that the 5 rain oscillation transports little energy and is not a s