Solar-wind model including the effects of rotation, magnetic fields, and anisotropic heat conduction

1969 ◽  
Vol 3 (1) ◽  
pp. 139-149 ◽  
Author(s):  
S. Grzędzielski
2020 ◽  
Vol 901 (2) ◽  
pp. L23
Author(s):  
M. Nakanotani ◽  
G. P. Zank ◽  
L. Adhikari ◽  
L.-L. Zhao ◽  
J. Giacalone ◽  
...  

2014 ◽  
Vol 796 (2) ◽  
pp. 111 ◽  
Author(s):  
Roberto Lionello ◽  
Marco Velli ◽  
Cooper Downs ◽  
Jon A. Linker ◽  
Zoran Mikić

2019 ◽  
Vol 1332 ◽  
pp. 012015
Author(s):  
S. Tasnim ◽  
Iver H. Cairns ◽  
M. S. Wheatland ◽  
B. Li ◽  
Gary P. Zank

2006 ◽  
Vol 2 (S235) ◽  
pp. 189-189
Author(s):  
N. Asai ◽  
N. Fukuda ◽  
R. Matsumoto

AbstractWe carried out 3D magnetohydrodynamic simulations of a subcluster moving in turbulent ICM by including anisotropic heat conduction. Since magnetic fields stretched along the subcluster surface suppress the heat conduction across the front, cold fronts are formed and sustained.


1986 ◽  
Vol 91 (A3) ◽  
pp. 2950 ◽  
Author(s):  
Ruth Esser ◽  
Egil Leer ◽  
Shadia R. Habbal ◽  
George L. Withbroe

2008 ◽  
Vol 113 (A3) ◽  
pp. n/a-n/a ◽  
Author(s):  
O. Cohen ◽  
I. V. Sokolov ◽  
I. I. Roussev ◽  
T. I. Gombosi

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