๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

The relationship between meridional drift and rotation of the large-scale solar magnetic field

โœ Scribed by S. Latushko

Publisher
Springer
Year
1993
Tongue
English
Weight
270 KB
Volume
146
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

Meridional drift of the large-scale sola
Meridional drift of the large-scale solar magnetic fields in different phases of solar activity
โœ S. Latushko ๐Ÿ“‚ Article ๐Ÿ“… 1996 ๐Ÿ› Springer ๐ŸŒ English โš– 344 KB

An analysis is made of mean latitudinal profiles of the meridional drift of the large-scale solar magnetic fields. The previously detected equaturward migration of the drift pattern in the course of a cycle is confirmed. Evidence for the existence of a near-equatorial narrow zone -t-7 ~ with an equa

The concentration of the large-scale sol
The concentration of the large-scale solar magnetic field by a meridional surface flow
โœ C. R. DeVore; N. R. Sheeley; J. P. Boris ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Springer ๐ŸŒ English โš– 649 KB

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

Rotation of the large-scale solar magnet
Rotation of the large-scale solar magnetic fields in the equatorial region
โœ S. Latushko ๐Ÿ“‚ Article ๐Ÿ“… 1996 ๐Ÿ› Springer ๐ŸŒ English โš– 325 KB

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

The relationship between the slowly vary
The relationship between the slowly varying component of solar radio emission and large scale photospheric magnetic field patterns
โœ P. H. Scherrer; M. El-Raey ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 385 KB

Daily solar radio flux observations have been examined for a relationship to the large-scale photospheric magnetic field structure. Interplanetary magnetic field sector boundaries were used to indicate boundaries between photospheric field regions of opposite polarity. An enhancement in emission was