๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

The piston model of coronal transients

โœ Scribed by Wen-Rui Hu; Ze-Mei Tang

Book ID
104864660
Publisher
Springer Netherlands
Year
1984
Tongue
English
Weight
731 KB
Volume
100
Category
Article
ISSN
0004-640X

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

The onset of coronal transients
The onset of coronal transients
โœ W. Tend ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 173 KB

A model for the motion of transients in the high corona, recently given by Anzer (1978), is extended to include also the onset of a transient, associated with prominence destabilization. A comparison is made with flare instabilities, and some relevant observations are considered.

Evidence linking coronal transients to t
Evidence linking coronal transients to the evolution of coronal holes
โœ David F. Webb; Patrick S. MciIntosh; Jerome T. Nolte; Craig V. Solodyna ๐Ÿ“‚ Article ๐Ÿ“… 1978 ๐Ÿ› Springer ๐ŸŒ English โš– 464 KB

The positions of X-ray coronal transients outside of active regions observed during Skylab were superposed on Ha synoptic charts and coronal hole boundaries for seven solar rotations. We confirmed a detailed spatial association between the transients and neutral lines. We found that most of the tran

Frequency of coronal transients and sola
Frequency of coronal transients and solar activity
โœ E. Hildner; J. T. Gosling; R. M. MacQueen; R. H. Munro; A. I. Poland; C. L. Ross ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 764 KB

The High Altitude Observatory's white light coronagraph aboard Skylab observed some 110 coronal transients -rapid changes in appearance of the corona -during its 227 days of operation. The longitudes of the origins of these transients were not distributed uniformly around the solar surface (51 of th