scholarly journals Theoretical Studies of Alfven Waves and Energetic Particle Physics in Fusion Plasmas

2017 ◽  
Author(s):  
Liu Chen ◽  
Keyword(s):  
Particle Physics ◽  
Energetic Particle ◽  
Alfven Waves ◽  
Alfvén Waves ◽  
Theoretical Studies ◽  
Fusion Plasmas

Theory of Alfvén waves and energetic particle physics in burning plasmas

2007 ◽  
Vol 47 (10) ◽  
pp. S727-S734 ◽  
Author(s):  
L. Chen ◽  
F. Zonca
Keyword(s):  
Particle Physics ◽  
Energetic Particle ◽  
Alfven Waves ◽  
Alfvén Waves ◽  
Burning Plasmas

scholarly journals Stimulated Emission of Fast Alfvén Waves within Magnetically Confined Fusion Plasmas

2017 ◽  
Vol 118 (18) ◽  
Author(s):  
J. W. S. Cook ◽  
R. O. Dendy ◽  
S. C. Chapman
Keyword(s):  
Alfven Waves ◽  
Stimulated Emission ◽  
Alfvén Waves ◽  
Fusion Plasmas ◽  
Magnetically Confined

scholarly journals Nonlinear Alfvén wave model of spicules and coronal heating

2007 ◽  
Vol 3 (S247) ◽  
pp. 195-200
Author(s):  
Takahiro Kudoh
Keyword(s):  
Wave Model ◽  
Alfven Waves ◽  
Coronal Heating ◽  
Alfven Wave ◽  
Magnetic Flux Tube ◽  
Alfvén Waves ◽  
Theoretical Studies ◽  
Mean Square ◽  
Cool Loop ◽  
Hot Corona

AbstractWe review the theoretical studies of the Alfvén wave model of spicules and coronal heating, mainly based on the papers by Kudoh & Shibata (1999), Saito et al. (2001) and Moriyasu et al. (2004) which performed MHD numerical simulations of nonlinear Alfvén waves propagating along a magnetic flux tube in the solar atmosphere. Kudoh & Shibata (1999) and Saito et al. (2001) found that, if the root mean square of the perturbation is greater than ~ 1 km s−1 in the photosphere, (1) the transition region is lifted up to more than ~ 5000 km (i.e., the spicule is produced), (2) the energy flux sufficient for heating the quiet corona (~ 3.0 × 105 ergs s−1 cm−2) is transported into the corona by Alfvén waves. Moriyasu et al. (2004) demonstrated that a hot corona is created in an initially cool loop as a result of the nonlinear Alfvén waves produced near the photosphere. We conclude that the nonlinear Alfvén wave model is the promising model of spicules and coronal heating.

scholarly journals Nonlinear dynamics of phase space zonal structures and energetic particle physics in fusion plasmas

2015 ◽  
Vol 17 (1) ◽  
pp. 013052 ◽  
Author(s):  
F Zonca ◽  
L Chen ◽  
S Briguglio ◽  
G Fogaccia ◽  
G Vlad ◽  
...  
Keyword(s):  
Nonlinear Dynamics ◽  
Phase Space ◽  
Particle Physics ◽  
Energetic Particle ◽  
Fusion Plasmas

scholarly journals Supplementary heating of fusion plasmas by means of Alfven waves

1977 ◽  
Author(s):  
J A Tataronis ◽  
W Grossmann
Keyword(s):  
Alfven Waves ◽  
Alfvén Waves ◽  
Fusion Plasmas

scholarly journals Energetic particle destabilization of shear Alfven waves in stellarators and tokamaks

1994 ◽  
Author(s):  
D.A. Spong ◽  
B.A. Carreras ◽  
C.L. Hedrick ◽  
J.N. Leboeuf ◽  
A. Weller
Keyword(s):  
Energetic Particle ◽  
Alfven Waves ◽  
Alfvén Waves ◽  
Shear Alfven Waves

Alfvén waves: a journey between space and fusion plasmas

2008 ◽  
Vol 50 (12) ◽  
pp. 124001 ◽  
Author(s):  
Liu Chen
Keyword(s):  
Alfven Waves ◽  
Alfvén Waves ◽  
Fusion Plasmas

scholarly journals Convective and Diffusive Energetic Particle Losses Induced by Shear Alfvén Waves in the ASDEX Upgrade Tokamak

2010 ◽  
Vol 104 (18) ◽  
Author(s):  
M. García-Muñoz ◽  
N. Hicks ◽  
R. van Voornveld ◽  
I. G. J. Classen ◽  
R. Bilato ◽  
...  
Keyword(s):  
Energetic Particle ◽  
Alfven Waves ◽  
Alfvén Waves ◽  
Shear Alfven Waves
Sign in / Sign up

Export Citation Format

Share Document