𝔖 Bobbio Scriptorium
✦   LIBER   ✦

On the origin of continuum emission during decametric solar noise storms

✍ Scribed by B. N. Levin; V. O. Rapoport

Book ID
104643001
Publisher
Springer
Year
1985
Tongue
English
Weight
511 KB
Volume
96
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

✦ Synopsis

The stationary current of diffusely-distributed super-thermal electrons along a weakly inhomogeneous coronal magnetic field is considered as a possible model of the noise storm continuum source in decametric wavelengths. It is shown that the realization of such a streaming leads to a considerably increased level of plasma noise in the diffuse component region and then to enhanced radio emission from this region.

πŸ“œ SIMILAR VOLUMES

Variations of the radiation signatures o
Variations of the radiation signatures of noise storm-emitting sunspot groups during a solar cycle
✍ A. BΓΆhme πŸ“‚ Article πŸ“… 1989 πŸ› Springer 🌐 English βš– 881 KB

The flux density of a noise storm continuum is known to depend on importance parameters of the associated sunspot group, e.g., its total areaA. A study of the continua at 287, 234, 113, and 64 MHz, however, reveals in case of the two cycles Nos. 20 and 21 that the radiation signatures of sunspot gro