๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

A model of the solar radio slowly varying component

โœ Scribed by Zhao Ren-yang; Qian Shan-jie

Publisher
Elsevier Science
Year
1982
Tongue
English
Weight
542 KB
Volume
6
Category
Article
ISSN
0275-1062

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

The slowly varying component of solar me
The slowly varying component of solar meter wavelength radiation: A non-thermal radio source
โœ A. C. Riddle ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 306 KB

The slowly varying component of solar centimeter wavelength radiation can often be attributed to thermal emission from density enhancements above an active region. This assertion is justified by the success in reproducing the observations by ray tracing calculations in appropriate coronal models. Si

Spectrum of slowly varying component of
Spectrum of slowly varying component of solar radio emission on millimeter wavelengths
โœ Atsushi Tsuchiya; Kozo Takahashi ๐Ÿ“‚ Article ๐Ÿ“… 1968 ๐Ÿ› Springer ๐ŸŒ English โš– 146 KB

The spectrum of the S-component of solar radio emission has been investigated at 4 GHz, 17 GHz, 35 GHz, 70 GHz, and 94 GHz. The spectrum for a spot group which appeared late in March 1966 (McMath plage No. 8223), seems to be fiat at the frequencies above about 35 GHz. This implies that the emission