A clearly evident large-scalc pattern in the interplanetary magnetic field during 1964 is used to search for a similar large-scale pattern in thc selar magnetic field. It is found that such a pattern did exist in the photospheric ticld observations on both sides of the equator over a range of at lea
The non-axisymmetrical configuration of a large-scale solar and stellar magnetic field
โ Scribed by Wen-Rui Hu
- Publisher
- Springer Netherlands
- Year
- 1983
- Tongue
- English
- Weight
- 515 KB
- Volume
- 90
- Category
- Article
- ISSN
- 0004-640X
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
We calculate analytical and numerical solutions to the magnetic flux transport equation in the absence of new bipolar sources of flux, for several meridional flow profiles and a range of peak flow speeds. We find that a polcward flow with a broad profile and a nominal 10 m s-1 maximum speed concentr
A study is made of the rotation of large-scale magnetic fields using the synoptic maps from the Kitt Peak National Observatory for the time interval 1976-1985. The auto-correlation method and the mass-centers method of magnetic structures was applied to infer mean differential rotation profiles and