๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Photospheric magnetic field rotation: Rigid and differential

โœ Scribed by John M. Wilcox; Kenneth H. Schatten; Andrew S. Tanenbaum; Robert Howard


Publisher
Springer
Year
1970
Tongue
English
Weight
411 KB
Volume
14
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES


Differential rotation of the photospheri
โœ John M. Wilcox; Robert Howard ๐Ÿ“‚ Article ๐Ÿ“… 1970 ๐Ÿ› Springer ๐ŸŒ English โš– 502 KB

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

Differential rotation of photospheric ma
โœ W. M. Adams ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 234 KB

An interesting aspect of solar rotation is the fact that coronal holes seem to exhibit little or no differential rotation. We set out to investigate the question of whether or not the photospheric magnetic fields underlying coronal holes also exhibit reduced differential rotation. In order to accomp

Comparison of the mean photospheric magn
โœ A. Severny; J. M. Wilcox; P. H. Scherrer; D. S. Colburn ๐Ÿ“‚ Article ๐Ÿ“… 1970 ๐Ÿ› Springer ๐ŸŒ English โš– 977 KB

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

Photospheric subrotation, differential r
โœ K. H. Schatten; H. G. Mayr; Randolph H. Levine ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 266 KB

Recently Mayr et aL (1980) have suggested that the superrotation of planetary atmospheres could, in principle, be understood as a 'pirouette'. Equatorial heating is pumping atmospheric material toward the poles, and with a concomitant reduction in moment of inertia, the atmosphere has the tendency

Rigid and differential rotation of the s
โœ Ester Antonucci; Leif Svalgaard ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 423 KB

The rotation of the solar corona has been studied using recurrence properties of the green coronal line (5303 A,) for the interval 1947-1970. Short-lived coronal activity is found to show the same differential rotation as short-lived photospheric magnetic field features. Long-lived recurrences show