๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

A Rate-Independent Test for Solar Flare Sympathy

โœ Scribed by M. S. Wheatland

Publisher
Springer
Year
2006
Tongue
English
Weight
171 KB
Volume
236
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

A search for solar neutrons during solar
A search for solar neutrons during solar flares
โœ S. O. Ifedili ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 478 KB

The upperlirnit on the solar neutron flux from 1-20 MeV has been measured, by a neutron detector on the OGO-6 satel!ite, to be less than 5 :-< 10 -z n cm -2 s -1 at the 95% confidence level for several flares including two flares of importance 3B and a solar proton event of importance 3B. The measur

A flare-associated mechanism for solar s
A flare-associated mechanism for solar surges
โœ Per Carlqvist ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 840 KB

An ejection mechanism for solar surges is discussed. The mechanism is closely related to an earlier proposed model for solar flares founded on current disruption. Hence, the observed connection between surges and flares may be explained in a simple way. The mechanism can also offer explanations of o

A classification scheme for solar flare
A classification scheme for solar flare models
โœ D. S. Spicer; J. C. Brown ๐Ÿ“‚ Article ๐Ÿ“… 1980 ๐Ÿ› Springer ๐ŸŒ English โš– 369 KB

We present a classification scheme for solar flare models that utilize magnetic free energycurrents. The classification scheme is geometry independent and delineates models into two categories: those models utilizing currents flowing parallel to B and those utilizing currents flowing perpendicular t

Thermal nonequilibrium: A trigger for so
Thermal nonequilibrium: A trigger for solar flares?
โœ A. W. Hood; E. R. Priest ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 989 KB

In this paper, we suggest that a solar flare may be triggered by a lack of thermal equilibrium rather than by a magnetic instability. The possibility of such a thermal nonequilibrium (or catastrophe) is demonstrated by solving approximately the energy equation for a loop under a balance between ther