๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Magnetic polarimetric refraction in the solar corona

โœ Scribed by Y. N. Gnedin; E. D. Lopez

Publisher
Springer
Year
1996
Tongue
English
Weight
282 KB
Volume
164
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

โœฆ Synopsis

We present expressions which describe the angular displacement of radio sources due to refraction in a magnetized plasma. The main objective of the present paper is to take into account the combined effect of gradients of the electron density and the magnetic field. We use the geometrical optics approximation for the determination of the angular broadening of the radiation. The expressions obtained are applied to the case of the solar corona.

๐Ÿ“œ SIMILAR VOLUMES

Atlas of magnetic fields in the solar co
Atlas of magnetic fields in the solar corona
โœ Gordon Newkirk; Dorothy E. Trotter; Martin D. Altschuler; Robert Howard ๐Ÿ“‚ Article ๐Ÿ“… 1972 ๐Ÿ› Springer ๐ŸŒ English โš– 105 KB

Figs. la-b. An example of the weak field (a) and strong field (b) maps contained in the 'Atlas of Magnetic Fields in the Solar Corona'.

The magnetic non-equilibrium of buoyant
The magnetic non-equilibrium of buoyant flux tubes in the solar corona
โœ P. K. Browning; E. R. Priest ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Springer ๐ŸŒ English โš– 678 KB

The equilibrium shape of a slender flux tube in the stratified solar atmosphere is studied. The path is determined by a balance between the downwards magnetic tension, which depends on the curvature of the loop, and the upwards buoyancy force. Previous results for untwisted slender tubes are extende