Ripple loss of suprathermal alpha particles during slowing-down in a tokamak reactor

1983 ◽  
Vol 23 (5) ◽  
pp. 657-665 ◽  
Author(s):  
K. Tani ◽  
T. Takizuka ◽  
M. Azumi ◽  
H. Kishimoto
1978 ◽  
Vol 18 (6) ◽  
pp. 859-866 ◽  
Author(s):  
M. Ohnishi ◽  
N. Ao ◽  
J. Wakabayashi

2018 ◽  
Vol 84 (5) ◽  
Author(s):  
A. Cardinali ◽  
C. Castaldo ◽  
R. Ricci

In a reactor plasma like demonstration power station (DEMO), when using the radio frequency (RF) for heating or current drive in the lower hybrid (LH) frequency range (Frankeet al.,Fusion Engng Des., vol. 96–97, 2015, p. 46; Cardinaliet al.,Plasma Phys. Control. Fusion, vol. 59, 2017, 074002), a large fraction of the ion population (the continuously born$\unicode[STIX]{x1D6FC}$-particle, and/or the neutral beam injection (NBI) injected ions) is characterized by a non-thermal distribution function. The interaction (propagation and absorption) of the LH wave must be reformulated by considering the quasi-linear approach for each species separately. The collisional slowing down of such an ion population in a background of an electron and ion plasma is balanced by a quasi-linear diffusion in velocity space due to the propagating electromagnetic wave. In this paper, both propagations are considered by including the ion distribution function, solution of the Fokker–Planck equation, which describes the collisional dynamics of the$\unicode[STIX]{x1D6FC}$-particles including the effects of frictional slowing down, energy diffusion and pitch-angle scattering. Analytical solutions of the Fokker–Planck equation for the distribution function of$\unicode[STIX]{x1D6FC}$-particles with a background of ions and electrons at steady state are included in the calculation of the dielectric tensor. In the LH frequency domain, ray tracing (including quasi-linear damping), can be analytically solved by iterating with the Fokker–Planck solution, and the interaction of the LH wave with$\unicode[STIX]{x1D6FC}$-particles, thermal ions and electrons can be accounted self-consistently and the current drive efficiency can be evaluated in this more general scenario.


2012 ◽  
Vol 52 (5) ◽  
pp. 054010
Author(s):  
M.F. Heyn ◽  
I.B. Ivanov ◽  
S.V. Kasilov ◽  
W. Kernbichler ◽  
A. Loarte ◽  
...  

1991 ◽  
Vol 33 (14) ◽  
pp. 1805-1824 ◽  
Author(s):  
M von Hellermann ◽  
W Mandl ◽  
H P Summers ◽  
A Boileau ◽  
R Hoekstra ◽  
...  

2005 ◽  
Vol 125 (11) ◽  
pp. 938-942 ◽  
Author(s):  
Keiji Tani ◽  
Kenji Tobita ◽  
Shunji Tsuji-Iio ◽  
Hiroaki Tsutsui ◽  
Satoshi Nishio ◽  
...  

1996 ◽  
Vol 36 (1) ◽  
pp. 55-67 ◽  
Author(s):  
M.N Rosenbluth ◽  
F.L Hinton

2019 ◽  
Vol 85 (2) ◽  
Author(s):  
Peter J. Catto

Alpha particle confinement is a serious concern in stellarators and provides strong motivation for optimizing magnetic field configurations. In addition to the collisionless confinement of trapped alphas in stellarators, excessive collisional transport of the trapped alpha particles must be avoided while they tangentially drift due to the magnetic gradient (the $\unicode[STIX]{x1D735}B$ drift). The combination of pitch angle scatter off the background ions and the $\unicode[STIX]{x1D735}B$ drift gives rise to two narrow boundary layers in the trapped region. The first is at the trapped–passing boundary and enables the finite trapped response to be matched to the vanishing passing response of the alphas. The second layer is a region that encompasses the somewhat more deeply trapped alphas with vanishing tangential $\unicode[STIX]{x1D735}B$ drift. Away from (and between) these boundary layers, collisions are ineffective and the alpha $\unicode[STIX]{x1D735}B$ drift simply balances the small radial drift of the trapped alphas. As this balance does not vanish as the trapped–passing boundary is approached, the first collisional boundary layer is necessary and gives rise to $\surd \unicode[STIX]{x1D708}$ transport, with $\unicode[STIX]{x1D708}$ the collision frequency. The vanishing of the tangential drift results in a separate, somewhat wider boundary layer, and significantly stronger superbanana plateau transport that is independent of collisionality. The constraint imposed by the need to avoid significant energy depletion loss in the slowing down tail distribution function sets the allowed departure of a stellarator from an optimal quasisymmetric configuration.


1983 ◽  
Vol 23 (4) ◽  
pp. 533-535 ◽  
Author(s):  
W.N.G. Hitchon ◽  
R.J. Hastie

1979 ◽  
Vol 29 (7) ◽  
pp. 744-757 ◽  
Author(s):  
T. D. Kaladze ◽  
J. G. Lominadze ◽  
A. B. Mikhailovskii ◽  
A. R. Khvoles ◽  
L. V. Tsamalaschvili

Author(s):  
Samuel A Lazerson ◽  
Alexandra LeViness ◽  
Jorrit Lion

Abstract Gyrocenter following simulations of fusion born alpha particles in a stellarator reactor are preformed using the BEAMS3D code. The Wendelstein 7-X high mirror configuration is scaled in geometry and magnetic field to reactor relevant parameters. A 2×1020 m−3 density plasma with 20 keV core temperatures is assumed and fusion birth rates calculated for various fusion products assuming a 50/50 deuterium-tritium mixture. It is found that energetic He4 ions comprise the vast majority of the energetic particle inventory. Slowing down simulations of the He4 population suggest plasma heating consistent with scaled energy confinement times for a stellarator reactor. Losses for this configuration appear large suggesting optimization beyond the scope of the W7-X device is key to a future fusion reactor. These first simulations are designed to demonstrate the capability of the BEAMS3D code to provide fusion alpha birth and heating profiles for stellarator reactor designs.


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