In a recent paper,1 one of the main conclusions in Ref. 2 is called erroneous and some arguments are advanced to sustain this verdict.

Precisely, the authors of Ref. 1 disagree with the statement in Ref. 2 that “the condition Fp=0 … cannot be satisfied within the single-mode approaches …, but requires the presence of two coupled (1, 1) and (1, –1) modes (for a circular plasma …).”

In the both cases,1,2 the analysis starts from the calculation of the integral

(1)

for a circular plasma and a coaxial resistive wall. The notation is the same as in Ref. 2: FXα is the eX-projection of the electromagnetic force on the current carriers inside the torus α, α=in or out denotes the wall sides, B0 is the axially symmetric part of the magnetic field B=B0+b, with b being the perturbation,

(2)

ζ is the toroidal angle in the cylindrical coordinates (R,ζ,z) related to the main axis of the torus, and ei are the unit vectors.

In the toroidal geometry,

(3)

making, thereby, eX a unit vector in a fixed direction, eX/ζ=0, which property is used in derivations in Ref. 2. Also,

(4)

where nα is the unit normal to the toroidal surface Sα, dp is the length element of the contour of Sα in the cross section ζ=const, and

(5)

with r and θ being the minor radius and the poloidal angle in that cross section centered at R=R0 (see Figs. 1 and 2 in Ref. 2). By using Eqs. (2), (4), and (5) and

(6)

with constant B0 for the toroidal magnetic field in the plasma-wall vacuum gap, we have

(7)

where dSαcyl is the “cylindrical” analog of Sα,

(8)

This closes the gap between Eq. (1) and its quasi-cylindrical consequence,

(9)

which are Eqs. (13) and (18) in Ref. 2, respectively. It is clear that B0 must be a constant in Eq. (9), and it was treated as such in Ref. 2. This constant was obtained from multiplication of Eqs. (4) and (6). A reader can blame us that this step has not been so meticulously explained in Ref. 2, but the simplicity of the intermediate actions (4)–(8) makes it an easy exercise if any doubt would appear.

The fact that B0=const in Eq. (9) has been explicitly stipulated in Ref. 2. However, in Ref. 1, it was proposed that this B0 should be replaced by B0R0/R. No proof is given there although this (incorrect) substitution alters the integral in Eq. (9), which affects the subsequent derivations and the outcome in Ref. 1.

This first unjustified deviation from the procedure developed in Ref. 2 does not yet allow us to make Fp=0, with b represented by a single harmonic, but it is aggravated by another one; the use of the Resistive Wall Mode (RWM) dispersion relation [Eqs. (4) and (5) in Ref. 1],

(10)

that for m/n=1/1 is reduced to

(11)

since κrpl/rw and the safety factor qr2 outside the plasma.

The combination of Eq. (11) with Eq. (9) deliberately, but groundlessly modified by

(12)

completes derivations in Ref. 1 and gives FXα different from that in Ref. 2.

It is explained above why substitution (12) is a mistake. Another question is whether Eq. (11) should be considered, as emphatically alleged in Ref. 1, “a definite and universal relation between γτm and the value of the safety factor q” for m/n=1/1?

Neither arguments nor, at least, references are given in Ref. 1 to support this surprising statement. However, even within the ideal MHD and the quasi-cylindrical model, Eq. (11) has an extremely narrow applicability area, as illustrated by a wide spectrum of results in Sec. 27 “Resistive-Wall Mode Instability” in Ref. 3. Besides, it is well known that the ideal MHD cannot describe the main features of the observed RWM dynamics (see Refs. 4 and 5 and reviews in Refs. 6 and 7). In search of a better approach, a great variety of dispersion relations for RWMs have been proposed,6,7 and most of them can be covered by the following formula:7,8

(13)

where Wiw and Wno are the “ideal MHD” perturbed energies with and without an ideal wall, the time constant τD is given by Eq. (8) in Ref. 8 [originally introduced in Eq. (66) of Ref. 9], and Wadd is the combined contribution7,10 due to the non-MHD and non-ideal effects (for example, responsible for b×(ξ×B0) in the plasma) and the difference in the magnetic field b in the plasma-wall vacuum gap from the Haney–Freidberg9 test function,

(14)

with cno+ciw=1 and ciw=cnoγτD. Incorporation of bbHF into the stability tasks is described in detail in Refs. 7, 8, and 11.

If anybody wants to say “universal,” Eq. (13) is much better suited for that than one of its primitive offshoots, Eq. (11). Dispersion relations with the structure of Eq. (13) and various Wadd values often appear in studies devoted to RWMs, such as in Refs. 12–16. As explained in Refs. 7, 8, and 11, the universal form is the consequence of using b=bHF instead of properly calculated b, and the popularity is enhanced by an easy success15 that can be reached by almost anything6,7 resulting in Wadd0. Just note that Eq. (13) turns into an equation for Wadd, if τD is given (as in Refs. 12 and 14), γ is adjusted to experimental data, and both Wiw and Wno are evaluated somehow. Thus found Wadd can be attributed to a number of mechanisms by means of one or two fitting parameters, while the mentioned and similar models contain them much more. Such a “success” does not solve the problem without further search for real physics behind Wadd and even can be misleading, when overvalued as in Ref. 15, but it shows that, at least, Eq. (13) may be a good option, though with yet unknown Wadd.

In contrast, Eq. (11) cannot be matched with or supported by experimental results. Irrespective of the plasma pressure, it gives unphysical γτw=2 with the wall at infinity. The excuse1 that “the mode m/n=1/1 exists only in the external kink mode stability gap qpl<κ2 with the ideal wall at rw” is clearly incompatible with the observation17 that “a comprehensive disruption database of JET tokamaks,18 containing thousands of cases, clearly indicates that the sideway forces are result of a m/n=1/1 mode, well distinguished from the m/n=2/1 mode, which is invisible in measurements.” Also, Eq. (10) positioned as universal in Ref. 1 does not allow pressure-driven RWMs, while they are excited in experiments.6,19–21

To summarize, Eq. (11) is a product of oversimplified modeling. In reality, γ is different, which destroys the proof in Ref. 1 irrespective of Eq. (12). Equation (9) has a purely electromagnetic origin and is valid at any γ that appeared and was considered as a parameter in Ref. 2. The demonstrated careful inspection confirms that B0=const in Eq. (9). Then, erroneous are the mentioned arguments and conclusions in Ref. 1, but not the contested approach and the coupled kink mode requirement in Ref. 2.

1.
A. A.
Martynov
and
S. Yu.
Medvedev
,
Phys. Plasmas
27
,
012508
(
2020
).
2.
D. V.
Mironov
and
V. D.
Pustovitov
,
Phys. Plasmas
24
,
092508
(
2017
).
3.
A. B.
Mikhailovskii
,
Instabilities in a Confined Plasma
(
IOP
,
Bristol
,
1998
).
4.
M. J.
Lanctot
,
H.
Reimerdes
,
A. M.
Garofalo
,
M. S.
Chu
,
Y. Q.
Liu
,
E. J.
Strait
,
G. L.
Jackson
,
R. J.
La Haye
,
M.
Okabayashi
,
T. H.
Osborne
, and
M. J.
Schaffer
,
Phys. Plasmas
17
,
030701
(
2010
).
5.
Z. R.
Wang
,
M. J.
Lanctot
,
Y. Q.
Liu
,
J.-K.
Park
, and
J. E.
Menard
,
Phys. Rev. Lett.
114
,
145005
(
2015
).
6.
M. S.
Chu
and
M.
Okabayashi
,
Plasma Phys. Controlled Fusion
52
,
123001
(
2010
).
7.
V. D.
Pustovitov
,
J. Plasma Phys.
81
,
905810609
(
2015
).
8.
V. D.
Pustovitov
, in
Proceedings of the 46th EPS Conference on Plasma Physics
, Europhysics Conference Abstracts, Contributed Papers, Milan, Italy, edited by
C.
Riconda
,
S.
Brezinsek
,
K.
McCarty
,
K.
Lancaster
,
D.
Burgess
,
P.
Brault
, and
D.
Farina
(
European Physical Society
,
2019
), p.
P4.1048
. http://ocs.ciemat.es/EPS2019PAP/pdf/P4.1048.pdf
9.
S. W.
Haney
and
J. P.
Freidberg
,
Phys. Fluids B
1
,
1637
(
1989
).
10.
V. D.
Pustovitov
,
Phys. Plasmas
24
,
112513
(
2017
).
11.
N. D.
Lepikhin
and
V. D.
Pustovitov
,
Phys. Plasmas
21
,
042504
(
2014
).
12.
G. Z.
Hao
,
Y. Q.
Liu
,
A. K.
Wang
,
G.
Matsunaga
,
M.
Okabayashi
,
Z. Z.
Mou
, and
X. M.
Qiu
,
Phys. Plasmas
20
,
062502
(
2013
).
13.
Y. Q.
Liu
,
I. T.
Chapman
,
J. P.
Graves
,
G. Z.
Hao
,
Z. R.
Wang
,
J. E.
Menard
,
M.
Okabayashi
,
E. J.
Strait
, and
A.
Turnbull
,
Phys. Plasmas
21
,
056105
(
2014
).
14.
Y. L.
He
,
Y. Q.
Liu
,
Y.
Liu
,
C.
Liu
,
G. L.
Xia
,
A. K.
Wang
,
G. Z.
Hao
,
L.
Li
, and
S. Y.
Cui
,
Phys. Plasmas
23
,
012506
(
2016
).
15.
J. W.
Berkery
,
S. A.
Sabbagh
,
R. E.
Bell
,
S. P.
Gerhardt
, and
B. P.
LeBlanc
,
Phys. Plasmas
24
,
056103
(
2017
).
16.
X.
Bai
,
Y. Q.
Liu
,
Z.
Gao
,
G. L.
Xia
, and
S. X.
Yang
,
Phys. Plasmas
25
,
090701
(
2018
).
17.
L. E.
Zakharov
and
X.
Li
,
Phys. Plasmas
21
,
094701
(
2014
).
18.
S. N.
Gerasimov
,
T. C.
Hender
,
J.
Morris
,
V.
Riccardo
,
L. E.
Zakharov
, and
JET EFDA Contributors
,
Nucl. Fusion
54
,
073009
(
2014
).
19.
E. J.
Strait
,
T. S.
Taylor
,
A. D.
Turnbull
,
J. R.
Ferron
,
L. L.
Lao
,
B.
Rice
,
O.
Sauter
,
S. J.
Thompson
, and
D.
Wroblewski
,
Phys. Rev. Lett.
74
,
2483
(
1995
).
20.
E. J.
Strait
,
J.
Bialek
,
I. N.
Bogatu
,
M. S.
Chance
,
M. S.
Chu
,
D. H.
Edgell
,
A. M.
Garofalo
,
G. L.
Jackson
,
T. H.
Jensen
,
L. C.
Johnson
,
J. S.
Kim
,
R. J.
La Haye
,
G. A.
Navratil
,
M.
Okabayashi
,
H.
Reimerdes
,
J. T.
Scoville
,
A. D.
Turnbull
,
M. L.
Walker
, and
DIII-D Team
,
Nucl. Fusion
43
,
430
(
2003
).
21.
M.
Takechi
,
G.
Matsunaga
,
N.
Aiba
,
T.
Fujita
,
T.
Ozeki
,
Y.
Koide
,
Y.
Sakamoto
,
G.
Kurita
,
A.
Isayama
, and
Y.
Kamada
,
Phys. Rev. Lett.
98
,
055002
(
2007
).