Numerical simulation of an ECE diagnostic to measure magnetic fluctuations in fusion plasmas (abstract)

1988 ◽  
Vol 59 (8) ◽  
pp. 1644-1644
Author(s):  
C. E. Thomas ◽  
G. R. Hanson
2010 ◽  
Vol 6 (S274) ◽  
pp. 116-119
Author(s):  
Antonella Greco ◽  
Sergio Servidio ◽  
William H. Matthaeus ◽  
Pablo Dmitruk

AbstractIn recent analyses of numerical simulation and solar wind dataset, the idea that the magnetic discontinuities may be related to intermittent structures that appear spontaneously in MHD turbulence has been explored in details. These studies are consistent with the hypothesis that discontinuity events founds in the solar wind might be of local origin as well, i.e. a by-product of the turbulent evolution of magnetic fluctuations.Using simulations of 2D MHD turbulence, we are exploring a possible link between tangential discontinuities and magnetic reconnection. The goal is to develop numerical algorithms that may be useful for solar wind applications.


1988 ◽  
Vol 59 (9) ◽  
pp. 1990-1997 ◽  
Author(s):  
C. E. Thomas ◽  
G. R. Hanson ◽  
R. F. Gandy ◽  
D. B. Batchelor ◽  
R. C. Goldfinger

2009 ◽  
Vol 00 (00) ◽  
pp. 090904073309027-8
Author(s):  
H.W. Wang ◽  
S. Kyriacos ◽  
L. Cartilier

Sign in / Sign up

Export Citation Format

Share Document