Research output: Contribution to journal › Article › peer-review
Numerical linearized MHD model of flapping oscillations. / Korovinskiy, D. B.; Ivanov, I. B.; Semenov, V. S.; Erkaev, N. V.; Kiehas, S. A.
In: Physics of Plasmas, Vol. 23, No. 6, 062905, 01.06.2016.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Numerical linearized MHD model of flapping oscillations
AU - Korovinskiy, D. B.
AU - Ivanov, I. B.
AU - Semenov, V. S.
AU - Erkaev, N. V.
AU - Kiehas, S. A.
N1 - Publisher Copyright: © 2016 Author(s). Copyright: Copyright 2017 Elsevier B.V., All rights reserved.
PY - 2016/6/1
Y1 - 2016/6/1
N2 - Kink-like magnetotail flapping oscillations in a Harris-like current sheet with earthward growing normal magnetic field component Bz are studied by means of time-dependent 2D linearized MHD numerical simulations. The dispersion relation and two-dimensional eigenfunctions are obtained. The results are compared with analytical estimates of the double-gradient model, which are found to be reliable for configurations with small Bz up to values ∼ 0.05 of the lobe magnetic field. Coupled with previous results, present simulations confirm that the earthward/tailward growth direction of the Bz component acts as a switch between stable/unstable regimes of the flapping mode, while the mode dispersion curve is the same in both cases. It is confirmed that flapping oscillations may be triggered by a simple Gaussian initial perturbation of the Vz velocity.
AB - Kink-like magnetotail flapping oscillations in a Harris-like current sheet with earthward growing normal magnetic field component Bz are studied by means of time-dependent 2D linearized MHD numerical simulations. The dispersion relation and two-dimensional eigenfunctions are obtained. The results are compared with analytical estimates of the double-gradient model, which are found to be reliable for configurations with small Bz up to values ∼ 0.05 of the lobe magnetic field. Coupled with previous results, present simulations confirm that the earthward/tailward growth direction of the Bz component acts as a switch between stable/unstable regimes of the flapping mode, while the mode dispersion curve is the same in both cases. It is confirmed that flapping oscillations may be triggered by a simple Gaussian initial perturbation of the Vz velocity.
UR - http://www.scopus.com/inward/record.url?scp=84977489543&partnerID=8YFLogxK
U2 - 10.1063/1.4954388
DO - 10.1063/1.4954388
M3 - Article
VL - 23
JO - Physics of Plasmas
JF - Physics of Plasmas
SN - 1070-664X
IS - 6
M1 - 062905
ER -
ID: 7628135