The influence of the sunspot model on the Li-abundance

Solar Physics ◽  
1971 ◽  
Vol 21 (1) ◽  
pp. 96-100 ◽  
Author(s):  
G. Stellmacher ◽  
E. Wiehr
Keyword(s):  
Author(s):  
Rhona Maclean ◽  
Colin Beveridge ◽  
Dana Longcope ◽  
Daniel Brown ◽  
Eric Priest

The magnetic breakout model gives an elegant explanation for the onset of an eruptive solar flare, involving magnetic reconnection at a coronal null point which leads to the initially enclosed flux ‘breaking out’ to large distances. In this paper we take a topological approach to the study of the conditions required for this breakout phenomenon to occur. The evolution of a simple delta sunspot model, up to the point of breakout, is analysed through several sequences of potential and linear force-free quasi-static equilibria. We show that any new class of field lines, such as those connecting to large distances, must be created through a global topological bifurcation and derive rules to predict the topological reconfiguration due to various types of bifurcation.


Solar Physics ◽  
1987 ◽  
Vol 109 (2) ◽  
pp. 403-404 ◽  
Author(s):  
V. I. Zhukov ◽  
V. I. Efremov ◽  
B. T. Nuraliev

2014 ◽  
Vol 70 ◽  
pp. 1-14 ◽  
Author(s):  
Yosr Boukhris ◽  
Leila Gharbi ◽  
Nadia Ghrab-Morcos

Solar Physics ◽  
1971 ◽  
Vol 16 (2) ◽  
pp. 398-403 ◽  
Author(s):  
Hong Sik Yun
Keyword(s):  

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