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On the influence of the local maxima of total pressure on the current sheet stability to the kink-like (flapping) mode. / Korovinskiy, D. B.; Erkaev, N. V.; Semenov, V. S.; Ivanov, I. B.; Kiehas, S. A.; Ryzhkov, I. I.
в: Physics of Plasmas, Том 25, № 2, 022904, 02.2018.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - On the influence of the local maxima of total pressure on the current sheet stability to the kink-like (flapping) mode
AU - Korovinskiy, D. B.
AU - Erkaev, N. V.
AU - Semenov, V. S.
AU - Ivanov, I. B.
AU - Kiehas, S. A.
AU - Ryzhkov, I. I.
PY - 2018/2
Y1 - 2018/2
N2 - The stability of the Fadeev-like current sheet with respect to transversally propagating kink-like perturbations (flapping mode) is considered in terms of two-dimensional linear magnetohydrodynamic numerical simulations. It is found that the current sheet is stable when the total pressure minimum is located in the sheet center and unstable when the maximum value is reached there. It is shown that an unstable spot of any size enforces the whole sheet to be unstable, though the increment of instability decreases with the reduction of the unstable domain. In unstable sheets, the dispersion curve of instability shows a good match with the double-gradient (DG) model prediction. Here, the typical growth rate (short-wavelength limit) is close to the DG estimate averaged over the unstable region. In stable configurations, the typical frequency matches the maximum DG estimate. The dispersion curve of oscillations demonstrates a local maximum at wavelength similar to 0.7 sheet half-width, which is a new feature that is absent in simplified analytical solutions. (C) 2018 Author(s).
AB - The stability of the Fadeev-like current sheet with respect to transversally propagating kink-like perturbations (flapping mode) is considered in terms of two-dimensional linear magnetohydrodynamic numerical simulations. It is found that the current sheet is stable when the total pressure minimum is located in the sheet center and unstable when the maximum value is reached there. It is shown that an unstable spot of any size enforces the whole sheet to be unstable, though the increment of instability decreases with the reduction of the unstable domain. In unstable sheets, the dispersion curve of instability shows a good match with the double-gradient (DG) model prediction. Here, the typical growth rate (short-wavelength limit) is close to the DG estimate averaged over the unstable region. In stable configurations, the typical frequency matches the maximum DG estimate. The dispersion curve of oscillations demonstrates a local maximum at wavelength similar to 0.7 sheet half-width, which is a new feature that is absent in simplified analytical solutions. (C) 2018 Author(s).
KW - MAGNETIC-FIELD
KW - PLASMA SHEET
KW - SHEAR-FLOW
KW - MAGNETOTAIL
KW - CLUSTER
KW - CONFIGURATIONS
KW - OSCILLATIONS
KW - INSTABILITY
KW - EQUILIBRIA
UR - http://www.scopus.com/inward/record.url?scp=85042064428&partnerID=8YFLogxK
UR - http://www.mendeley.com/research/influence-local-maxima-total-pressure-current-sheet-stability-kinklike-flapping-mode
U2 - 10.1063/1.5016934
DO - 10.1063/1.5016934
M3 - статья
VL - 25
JO - Physics of Plasmas
JF - Physics of Plasmas
SN - 1070-664X
IS - 2
M1 - 022904
ER -
ID: 27873938