Search Publications

Nonlinear evolutions of large amplitude oblique whistler waves
DOI: 10.1063/1.5011775 Bibcode: 2018PhPl...25f2904D

Yoon, Peter H.; Hwang, Kyoung-Joo; Min, Kyoung-Wook +3 more

This paper investigates nonlinear evolutions of large amplitude oblique whistler waves (LOWWs) and the interaction with electrons using one-dimensional electromagnetic kinetic simulations. The present research is motivated by recent studies about the nonlinear phenomena of LOWWs. When the propagation angle is not close to the resonance cone angle,…

2018 Physics of Plasmas
Cluster 4
Current sheet bending as destabilizing factor in magnetotail dynamics
DOI: 10.1063/1.5046175 Bibcode: 2018PhPl...25i2901K

Korovinskiy, D. B.; Semenov, V. S.; Erkaev, N. V. +2 more

The problem of the magnetohydrodynamical stability of bent magnetotail current sheets is considered by means of 2.5-dimensional numerical simulations. This study is focused on the cross-tail transversal mode, modeling the magnetotail flapping motions, at the background of the Kan-like magnetoplasma equilibrium. It is found that in symmetrical curr…

2018 Physics of Plasmas
Cluster 3
Electron holes in phase space: What they are and why they matter
DOI: 10.1063/1.4976854 Bibcode: 2017PhPl...24e5601H

Hutchinson, I. H.

This is a tutorial and selective review explaining the fundamental concepts and some currently open questions concerning the plasma phenomenon of the electron hole. The widespread occurrence of electron holes in numerical simulations, space-craft observations, and laboratory experiments is illustrated. The elementary underlying theory is developed…

2017 Physics of Plasmas
Cluster 134
Simulation of magnetic holes formation in the magnetosheath
DOI: 10.1063/1.5003017 Bibcode: 2017PhPl...24l2121A

Raeder, Joachim; Ahmadi, Narges; Germaschewski, Kai

Magnetic holes have been frequently observed in the Earth's magnetosheath and are believed to be the consequence of the nonlinear evolution of the mirror instability. Mirror mode perturbations mainly form as magnetic holes in regions where the plasma is marginally mirror stable with respect to the linear instability criterion. We present an expand…

2017 Physics of Plasmas
Cluster 22
Nonlinear propagation of kinetic Alfvén wave and turbulent spectrum in reconnection region of magnetotail
DOI: 10.1063/1.4985151 Bibcode: 2017PhPl...24f2902Y

Sharma, R. P.; Yadav, Nitin; Sharma, Prachi +2 more

Kinetic Alfvén waves (KAWs) are known to play an important role in magnetic reconnection as well as in turbulence. In the present work, we have derived the dynamical equation of KAWs propagating through Harris sheet. It is assumed that background density gets modified due to nonlinearity and background field gets modified due to the presence of Ha…

2017 Physics of Plasmas
Cluster 3
Nonlinear evolution of 3D whistler waves in space plasmas
DOI: 10.1063/1.4985305 Bibcode: 2017PhPl...24f2104P

Sharma, R. P.; Pathak, Neha; Yadav, Nitin

The present model is proposed to study the nonlinear effects related to quasi-transverse 3D whistler waves in three different regions of space plasmas which are Earth's radiation belt, magnetopause, and solar wind plasma at 1 A.U. We have analysed the effect of considering the third dimension in the dynamics of whistler waves on Localization of wh…

2017 Physics of Plasmas
Cluster 3
Nonlinear effects associated with kinetic Alfvén wave in magnetic islands
DOI: 10.1063/1.4973656 Bibcode: 2017PhPl...24a2302R

Sharma, R. P.; Sharma, Swati; Yadav, Nitin +1 more

Observations show that kinetic Alfvén waves (KAWs) play a very important role in turbulence as well as in magnetic reconnection and have also been a topic of debate in the context of particle heating. In this paper, we aim to investigate the effect of magnetic islands on the dynamics of the nonlinear KAW. The formation of current sheet/coherent st…

2017 Physics of Plasmas
Cluster 1
Kinetic models of magnetic flux ropes observed in the Earth magnetosphere
DOI: 10.1063/1.4958319 Bibcode: 2016PhPl...23g2901V

Petrukovich, A. A.; Zelenyi, L. M.; Artemyev, A. V. +3 more

Magnetic flux ropes (MFR) are universal magnetoplasma structures (similar to cylindrical screw pinches) formed in reconnecting current sheets. In particular, MFR with scales from about the ion inertial length to MHD range are widely observed in the Earth magnetosphere. Typical MFR have force-free configuration with the axial magnetic field peaking…

2016 Physics of Plasmas
Cluster 12
Kinetic models of sub-ion cylindrical magnetic hole
DOI: 10.1063/1.4972093 Bibcode: 2016PhPl...23l2903S

Artemyev, A. V.; Vasko, I. Y.; Yushkov, E. V. +1 more

Magnetic holes are magnetoplasma structures very similar to the classical θ-pinch. They are widely observed in the space plasma and identified by the substantial magnetic field depressions on scales from magnetohydrodynamic range to electron scales. In this paper, we develop the kinetic models of cylindrically symmetric magnetic holes with sub-ion…

2016 Physics of Plasmas
Cluster 11
Study of electric and magnetic field fluctuations from lower hybrid drift instability waves in the terrestrial magnetotail with the fully kinetic, semi-implicit, adaptive multi level multi domain method
DOI: 10.1063/1.4952630 Bibcode: 2016PhPl...23e2902I

Lapenta, G.; Norgren, C.; Markidis, S. +3 more

The newly developed fully kinetic, semi-implicit, adaptive multi-level multi-domain (MLMD) method is used to simulate, at realistic mass ratio, the development of the lower hybrid drift instability (LHDI) in the terrestrial magnetotail over a large wavenumber range and at a low computational cost. The power spectra of the perpendicular electric fi…

2016 Physics of Plasmas
Cluster 10