Measurements of Self-Generated Magnetic Fields Influence on Electron Heat Conduction in Dense Plasmas

2010 ◽  
Author(s):  
L. Lancia ◽  
C. Fourment ◽  
M. Nakatsutsumi ◽  
S. Hulin ◽  
S. Bastiani-Ceccotti ◽  
...  
Keyword(s):  
Heat Conduction ◽  
Magnetic Fields ◽  
Dense Plasmas ◽  
Electron Heat

scholarly journals Three-Dimensional MHD Simulations of a Subcluster Plasma Moving in Turbulent ICM

2006 ◽  
Vol 2 (S235) ◽  
pp. 189-189
Author(s):  
N. Asai ◽  
N. Fukuda ◽  
R. Matsumoto
Keyword(s):  
Heat Conduction ◽  
Magnetic Fields ◽  
Three Dimensional ◽  
Cold Fronts ◽  
Mhd Simulations ◽  
Anisotropic Heat Conduction ◽  
Magnetohydrodynamic Simulations

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.

scholarly journals Nonlocal Electron Heat Transport in Magnetized Dense Plasmas

2014 ◽  
Vol 9 (0) ◽  
pp. 1404096-1404096
Author(s):  
Akio NISHIGUCHI
Keyword(s):  
Heat Transport ◽  
Dense Plasmas ◽  
Electron Heat

Measuring electron heat conduction in non-uniform laser-produced plasmas using imaging Thomson scattering

2010 ◽  
Vol 5 (11) ◽  
pp. P11005-P11005 ◽  
Author(s):  
J L Kline ◽  
D S Montgomery ◽  
R P Johnson ◽  
T Shimada
Keyword(s):  
Heat Conduction ◽  
Thomson Scattering ◽  
Electron Heat

Electron Heat Conduction and Suprathermal Particles

1992 ◽  
Vol 32 (3-4) ◽  
pp. 255-260 ◽  
Author(s):  
S. I. Krasheninnikov ◽  
O. G. Bakunin
Keyword(s):  
Heat Conduction ◽  
Electron Heat ◽  
Suprathermal Particles

Modelling of Quiet Sun Coronal Structures

1994 ◽  
Vol 144 ◽  
pp. 169-176
Author(s):  
S. Serio
Keyword(s):  
Thermal Stability ◽  
Heat Conduction ◽  
Magnetic Fields ◽  
Solar Corona ◽  
Thermal Stratification ◽  
Recent Progress ◽  
Coronal Loops ◽  
Dynamic Heating ◽  
Thermal Stability Of ◽  
Coronal Structures

AbstractThe 1978 paper by Rosner et al. has set the basis for a new way of understanding thermal stratification in the solar corona, taking into account the constraints of magnetic fields on heat conduction. This paper will review recent progress in modelling of coronal loops, and in particular the effects of deviations from Spitzer conductivity, stationary siphon flows and shocks, thermal stability of the transition region, and possible diagnostics of dynamic heating of the coronal plasma.

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