Chirping instabilities produced by a runaway electron beam at a spherical tokamak
Abstract Two different types of MHD instabilities with rapidly chirping frequency were found to arise in the Globus-M2 spherical tokamak in substantially different frequency ranges. The first type arises at frequencies of an order of 1 MHz in ohmic plasmas at relatively low density 〈 n e 〉 < 2 ×...
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Published in | Plasma science & technology Vol. 25; no. 7; pp. 75102 - 75107 |
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Main Authors | , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
IOP Publishing
01.07.2023
|
Subjects | |
Online Access | Get full text |
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Summary: | Abstract
Two different types of MHD instabilities with rapidly chirping frequency were found to arise in the Globus-M2 spherical tokamak in substantially different frequency ranges. The first type arises at frequencies of an order of 1 MHz in ohmic plasmas at relatively low density
〈
n
e
〉
<
2
×
10
19
m
−
3
in a wide range of toroidal magnetic fields and plasma currents. This type of instability was identified as compressional Alfvén waves, driven by electrons, accelerated during a sawtooth crush. It was found that the mode frequency is sweeping in time, according to the Berk–Breizman hole–clump nonlinear chirping model. The second type of wave arises in a specific single-swing regime of the central solenoid current with a very narrow plasma column, when the plasma tends to decay at extremely low density
〈
n
e
〉
<
2
×
10
18
m
−
3
and, in fact, is an instability of the runaway electron beam. The exited modes cover the whole observed frequency range and are divided into several (two or three) frequency regions: approximately 0–30 MHz, 60–120 MHz and sometimes 30–60 MHz. Reconnection of the branches was also observed. Single chirps are more rapid than for 1 MHz Alfvén instability and follow an exponential law. This paper, to our knowledge, is the first report of frequency chirping instabilities excited by accelerated electrons at a spherical tokamak. |
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Bibliography: | Institute of Plasma Physics PST-2022-0349.R3 |
ISSN: | 1009-0630 2058-6272 |
DOI: | 10.1088/2058-6272/acb875 |