Convective mechanism for the formation of photospheric magnetic fields
โ Scribed by A. V. Getling
- Book ID
- 110127282
- Publisher
- Springer
- Year
- 2001
- Tongue
- English
- Weight
- 158 KB
- Volume
- 45
- Category
- Article
- ISSN
- 1063-7729
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
The differential rotation of the large-scale photospheric magnetic field has been investigated with an autocorrelation technique using synoptic charts of the photospheric field during the interval 1959-66. Near the equator the rotation period of the field is nearly the same as the rotation rate of l
The mean photospheric magnetic field of the sun seen as a star has been compared with the interplanetary magnetic field observed with spacecraft near the earth. Each change in polarity of the mean solar field is followed about 4 89 days later by a change in polarity of the interplanetary field (sect
Possibilities for the storage of energy in coronal electric currents in different magnetic background field configurations are investigated in the framework of the solar flare energy build-up model of Van Tend and Kuperus (1978), The results are compared to characteristics of filaments and X-ray loo