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 app
โฆ LIBER โฆ
The nonlinear acceleration of a magnetic disturbance in the solar corona
โ Scribed by Martin D. Altschuler; Dean F. Smith; Paul N. Swarztrauber; Eric R. Priest
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 947 KB
- Volume
- 32
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Magnetic polarimetric refraction in the
โ
Y. N. Gnedin; E. D. Lopez
๐
Article
๐
1996
๐
Springer
๐
English
โ 282 KB
Stochastic acceleration by lower hybrid
โ
G. S. Lakhina; B. Buti
๐
Article
๐
1996
๐
Springer
๐
English
โ 421 KB
Atlas of magnetic fields in the solar co
โ
Gordon Newkirk; Dorothy E. Trotter; Martin D. Altschuler; Robert Howard
๐
Article
๐
1972
๐
Springer
๐
English
โ 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'.
Langmuir turbulence in the solar corona
โ
Song Mu-tao; Li Xiao-qing
๐
Article
๐
1981
๐
Elsevier Science
๐
English
โ 486 KB
Resonant scattering of particles and sec
โ
D. B. Melrose
๐
Article
๐
1974
๐
Springer
๐
English
โ 714 KB
Effective acceleration of particles by hydromagnetic turbulence requires that the particles be scattered at a rate v comparable with the frequency o9 of the turbulence. The only effective scattering process is due to resonant wave-particle interactions. The resonant waves are HM waves for ions with
Non-radial magnetic field structures in
โ
N. Gopalswamy; M. R. Kundu; A. Raoult; M. Pick
๐
Article
๐
1994
๐
Springer
๐
English
โ 439 KB