Relativistic Effects in Heating and Current Drive by Electron Bernstein Waves

2003 ◽  
Author(s):  
A. K. Ram
2009 ◽  
Author(s):  
V. Shevchenko ◽  
A. Saveliev ◽  
Volodymyr Bobkov ◽  
Jean-Marie Noterdaeme

2000 ◽  
Vol 7 (5) ◽  
pp. 1352-1355 ◽  
Author(s):  
C. B. Forest ◽  
P. K. Chattopadhyay ◽  
R. W. Harvey ◽  
A. P. Smirnov

1987 ◽  
Vol 37 (3) ◽  
pp. 449-465 ◽  
Author(s):  
P. A. Robinson

Extraordinary solutions of the weakly relativistic, electromagnetic dispersion relation are investigated for waves propagating perpendicular to a uniform magnetic field in a Maxwellian plasma. As in a companion paper, which treated ordinary modes, weakly relativistic effects are found to modify dramatically the dispersion predicted by strictly non-relativistic ‘classical’ theory in the neighbourhood of harmonics of the cyclotron frequency Ωe. The infinite families of classical Gross–Bernstein and Dnestrovskii–Kostomarov modes are truncated to include only harmonics s satisfying s ≲ (ω2p mc2/4kB TΩ2e)⅓ and s ≲(ωp/Ωe)⅔/8 respectively where ωp is the plasma frequency and T the temperature. All classical cut-offs and resonances are removed apart from the x– and z– mode cut-offs. The only coupling between large- and small-wave-vector modes is between the z mode and a Gross–Bernstein mode near the upper-hybrid frequency and between the x mode and the second Gross–Bernstein mode near 2Ωe. Dispersion of the weakly relativistic counterpart of the x mode departs only slightly from that predicted by cold plasma theory except near Ωe and 2Ωe.


2007 ◽  
Vol 50 (1) ◽  
pp. 015003 ◽  
Author(s):  
D E McGregor ◽  
R A Cairns ◽  
C N Lashmore Davies ◽  
M R O'Brien

2018 ◽  
Vol 25 (10) ◽  
pp. 102103 ◽  
Author(s):  
Waseem Khan ◽  
Muddasir Ali ◽  
Zafar Iqbal ◽  
Gohar Abbas ◽  
Zahida Ehsan

1994 ◽  
Vol 34 (1) ◽  
pp. 63-74 ◽  
Author(s):  
Yu.V Petrov

1992 ◽  
Author(s):  
I. P. Shkarofsky ◽  
V. Fuchs ◽  
M. Shoucri ◽  
P. Bonoli ◽  
A. Bers ◽  
...  

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