๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

On the filamentary nature of solar magnetic fields

โœ Scribed by Robert Howard; J. O. Stenflo


Publisher
Springer
Year
1972
Tongue
English
Weight
844 KB
Volume
22
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Studies of solar magnetic fields
โœ Robert Howard ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 505 KB
Studies of solar magnetic fields
โœ Robert Howard ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 692 KB

Solar magnetic flux data accumulated from the magnetograph of the Mount Wilson Observatory are used to infer average east-west field inclination angles for the interval 196%1973. In all latitude zones the total flux (IF +] ยง measurements indicate that the field is inclined so as to trail the rotatio

Studies of solar magnetic fields
โœ Robert Howard ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 274 KB

In order to provide a smooth transition to a smaller aperture for the Mount Wilson daily magnetograms, a 2-step change was made, with two daily observations made using two different apertures covering an interval of several months. A comparison of these observations has made possible a check on the

Studies of solar magnetic fields
โœ Robert Howard ๐Ÿ“‚ Article ๐Ÿ“… 1977 ๐Ÿ› Springer ๐ŸŒ English โš– 299 KB

An estimate of the average magnetic field strength at the poles of the Sun from Mount Wilson measurements is made by comparing low latitude magnetic measurements in the same regions made near the center of the disk and near the limb. There is still some uncertainty because the orientation angle of t

On the nature of photospheric magnetic f
โœ S. Frankenthal; A. S. Krieger ๐Ÿ“‚ Article ๐Ÿ“… 1977 ๐Ÿ› Springer ๐ŸŒ English โš– 810 KB

We consider proposed mechanisms for the formation of coronal holes, and identify as crucial the issue whether the holes are permeated by rigidly rotating fields. It is suggested that the interaction between such a field and the differentially rotating, diffusive solar envelope will produce a fore af

On the nature of the apparent response o
โœ J. M. Wilcox; P. H. Scherrer ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 575 KB

The apparent response of the vorticity area index to the solar magnetic field is confined to tropospheric regions of intense circulation. Discussions and calculations that include larger volumes of the troposphere would not be expected to show a significant Sun-weather effect. Analysis of the effect