๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Meridional drift in the large-scale solar magnetic field pattern

โœ Scribed by S. Latushko


Publisher
Springer
Year
1994
Tongue
English
Weight
669 KB
Volume
149
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
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

A large-scale pattern in the solar magne
โœ John M. Wilcox; Robert Howard ๐Ÿ“‚ Article ๐Ÿ“… 1968 ๐Ÿ› Springer ๐ŸŒ English โš– 732 KB

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 concentration of the large-scale sol
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

The large-scale solar magnetic field
โœ Martin D. Altschuler; Dorothy E. Trotter; Gordon Newkirk; Robert Howard ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 823 KB

The large-scale photospheric magnetic field, measured by the Mr. Wilson magnetograph, has been analyzed in terms of surface harmonics (Pn"~(0)cosmq~ and P~m(O) sinm(o) for the years 1959 through 1972. Our results are as follows. The single harmonic which most often characterized the general solar ma

Rotation of the large-scale solar magnet
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