Observation of electron beam propagation in closed magnetic structures in the solar corona
โ Scribed by H Aurass; K.-L Klein
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 442 KB
- Volume
- 17
- Category
- Article
- ISSN
- 0273-1177
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
The conditions required for the stability of a steady-state electron beam propagating in the solar corona are determined using the quasi-linear theory. The growth rate for electron plasma waves in a magnetized plasma is evaluated, with the electron distribution function being given by an analytic so
Daily images of the white light corona between 3 and 10 R| have been recorded by a coronagraph aboard the OSO-7 unmanned satellite since October 3, 1971. Images for the years 1972 and 1973 have been examined for persistent coronal forms. For most of 1972 there passed over the Sun's east limb a regul
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'.