Remarks on sequence-of-plasma-instabilities models of solar flares

1975 ◽  
Vol 195 ◽  
pp. 545 ◽  
Author(s):  
B. Coppi
Keyword(s):  
Solar Flares ◽  
Plasma Instabilities

Resistive Instabilities and Solar Flares

1968 ◽  
Vol 1 (4) ◽  
pp. 152-153
Author(s):  
G. G. Lister
Keyword(s):  
Solar Flares ◽  
Finite Conductivity ◽  
Plasma Instabilities ◽  
Two Dimensional ◽  
Tearing Mode ◽  
Laboratory Plasmas ◽  
Initial Work

The study of plasma instabilities described by the inclusion of a finite conductivity in the hydromagnetic equations has aroused considerable interest since the initial work of Furth, Killeen and Rosenbluth for a two-dimensional geometry. In particular, the so-called ‘tearing’ mode, which has been observed in laboratory plasmas, has been suggested as a possible source of energy for solar flares.

Studies of the structure and dynamics of theDregion of the polar ionosphere during solar flares in April 2004

2006 ◽  
Vol 6 (2) ◽  
Author(s):  
V. D. Tereshchenko ◽  
E. B. Vasil'ev ◽  
O. F. Ogloblina ◽  
V. A. Tereshchenko ◽  
S. M. Chernyakov
Keyword(s):  
Solar Flares ◽  
Polar Ionosphere ◽  
Structure And Dynamics

The occurrence of single hard x-ray sources in solar flares

2003 ◽  
Vol 32 (12) ◽  
pp. 2483-2488
Author(s):  
C GOFF ◽  
S MATTHEWS ◽  
L HARRA
Keyword(s):  
Solar Flares ◽  
X Ray
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