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Author Peng, Ivy Bo ♦ Markidis, Stefano ♦ Laure, Erwin ♦ Johlander, Andreas ♦ Vaivads, Andris ♦ Khotyaintsev, Yuri ♦ Henri, Pierre ♦ Lapenta, Giovanni
Source United States Department of Energy Office of Scientific and Technical Information
Content type Text
Language English
Subject Keyword PLASMA PHYSICS AND FUSION TECHNOLOGY ♦ ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ♦ COMPUTERIZED SIMULATION ♦ EARTH MAGNETOSPHERE ♦ ELECTRON CYCLOTRON-RESONANCE ♦ IONS ♦ MAGNETIC DIPOLES ♦ MAGNETIC FIELD CONFIGURATIONS ♦ MAGNETIC FIELDS ♦ PLANETS ♦ SHOCK WAVES ♦ SOLAR WIND ♦ WHISTLERS
Abstract We carried out global Particle-in-Cell simulations of the interaction between the solar wind and a magnetosphere to study the kinetic collisionless physics in super-critical quasi-perpendicular shocks. After an initial simulation transient, a collisionless bow shock forms as a result of the interaction of the solar wind and a planet magnetic dipole. The shock ramp has a thickness of approximately one ion skin depth and is followed by a trailing wave train in the shock downstream. At the downstream edge of the bow shock, whistler waves propagate along the magnetic field lines and the presence of electron cyclotron waves has been identified. A small part of the solar wind ion population is specularly reflected by the shock while a larger part is deflected and heated by the shock. Solar wind ions and electrons are heated in the perpendicular directions. Ions are accelerated in the perpendicular direction in the trailing wave train region. This work is an initial effort to study the electron and ion kinetic effects developed near the bow shock in a realistic magnetic field configuration.
ISSN 1070664X
Educational Use Research
Learning Resource Type Article
Publisher Date 2015-09-15
Publisher Place United States
Journal Physics of Plasmas
Volume Number 22
Issue Number 9


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