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The Quasi-Stationary and Transient States of the Solar Wind

โœ Scribed by NEUGEBAUER, M.

Book ID
121150487
Publisher
American Association for the Advancement of Science
Year
1991
Tongue
English
Weight
449 KB
Volume
252
Category
Article
ISSN
0036-8075

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๐Ÿ“œ SIMILAR VOLUMES

Relationships of quasi-stationary solar
Relationships of quasi-stationary solar wind flows with their sources on the Sun
โœ V. G. Eselevich ๐Ÿ“‚ Article ๐Ÿ“… 1992 ๐Ÿ› Springer ๐ŸŒ English โš– 1000 KB

In this paper, by considering an example of four Carrington rotations ( 167 l, 1672, 1681, and 1682), it is shown that there generally exists an exhaustive correspondence between quasi-stationary flows of'fast' and 'slow' solar wind (SW), on the one hand, and their sources on the Sun: coronal holes

Solar wind: The quasi-radial approximati
Solar wind: The quasi-radial approximation and its limitations
โœ S. T. Suess; S. F. Nerney ๐Ÿ“‚ Article ๐Ÿ“… 1975 ๐Ÿ› Springer ๐ŸŒ English โš– 496 KB

The mathematical basis for approximating the solar wind expansion as nearly radial is examined and defined, removing earlier restrictions thought to occur in the presence of a magnetic field and large variations in latitude. The equations and side conditions governing quasi-radial flow are derived a