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Physical Parameters of a Reactor-Stellarator with Small Ripples of the Helical Magnetic Field
The paper describes the calculation data on the physical parameters of a reactor-stellarator, where the nonuniformities of the helical field are smaller than the toroidal magnetic field nonuniformities: ε h < ε t . Unlike the previous studies, where the ion-component transport coefficients had th...
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Published in: | Plasma physics reports 2018-09, Vol.44 (9), p.783-790 |
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Main Author: | |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites |
Online Access: | Get full text |
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Summary: | The paper describes the calculation data on the physical parameters of a reactor-stellarator, where the nonuniformities of the helical field are smaller than the toroidal magnetic field nonuniformities: ε
h
< ε
t
. Unlike the previous studies, where the ion-component transport coefficients had the collision frequency dependence proportional to ν
1/2
, this being equivalent to the ε
h
> ε
t
case, in the present calculations, these coefficients were assumed to be in proportion to the first power of the collision frequency,
D
i
∝ ν for
ν
eff
< 2ω
E
, and to
D
i
∝ ν
−1
for the inverse inequality. Here, ω
E
is the rotation frequency of plasma in the radial electric field. As before, the plasma electrons corresponded to the mode of
D
e
∝ ν
−1
. As initial parameters for numerical calculations, a reactor with
R
= 8 m,
r
p
= 2 m, and
B
0
= 5 Т was taken. A numerical code was used to solve the set of equations that describes the plasma space−time behavior in the reactor-stellarator under the conditions of equal diffusion fluxes. The start of reactor operation in the mode of thermonuclear burning was provided by heating sources with a power of several tens of megawatts. Steady-state operating conditions of a self-sustained thermonuclear reaction were attained by maintaining the plasma density through DT fuel pellet injection into the plasma. |
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ISSN: | 1063-780X 1562-6938 |
DOI: | 10.1134/S1063780X18090118 |