Scattering of Ions at a Rippled Shock

In a collisionless shock the energy of the directed flow is converted to heating and acceleration of charged particles, and to magnetic compression. In low-Mach number shocks the downstream ion distribution is made of directly transmitted ions. In higher-Mach number shocks ion reflection is importan...

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Main Authors: Michael Gedalin, Nikolai V. Pogorelov, Vadim Roytershteyn
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/acd63c
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author Michael Gedalin
Nikolai V. Pogorelov
Vadim Roytershteyn
author_facet Michael Gedalin
Nikolai V. Pogorelov
Vadim Roytershteyn
author_sort Michael Gedalin
collection DOAJ
description In a collisionless shock the energy of the directed flow is converted to heating and acceleration of charged particles, and to magnetic compression. In low-Mach number shocks the downstream ion distribution is made of directly transmitted ions. In higher-Mach number shocks ion reflection is important. With the increase of the Mach number, rippling develops, which is expected to affect ion dynamics. Using ion tracing in a model shock front, downstream distributions of ions are analyzed and compared for a planar stationary shock with an overshoot and a similar shock with ripples propagating along the shock front. It is shown that rippling results in the distributions, which are substantially broader and more diffuse in the phase space. Gyrotropization is sped up. Rippling is able to generate backstreaming ions, which are absent in the planar stationary case.
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spelling doaj.art-bc04081899e6412082c195865c7741a32023-09-03T11:11:49ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-0195116510.3847/1538-4357/acd63cScattering of Ions at a Rippled ShockMichael Gedalin0https://orcid.org/0000-0003-1236-4787Nikolai V. Pogorelov1https://orcid.org/0000-0002-6409-2392Vadim Roytershteyn2https://orcid.org/0000-0003-1745-7587Department of Physics, Ben Gurion University of the Negev , Beer-Sheva, Israel ; gedalin@bgu.ac.ilDepartment of Space Science, The University of Alabama in Huntsville , AL 35805, USA; Center for Space Plasma and Aeronomic Research, The University of Alabama in Huntsville , AL 35805, USASpace Science Institute , Boulder, CO 80301, USAIn a collisionless shock the energy of the directed flow is converted to heating and acceleration of charged particles, and to magnetic compression. In low-Mach number shocks the downstream ion distribution is made of directly transmitted ions. In higher-Mach number shocks ion reflection is important. With the increase of the Mach number, rippling develops, which is expected to affect ion dynamics. Using ion tracing in a model shock front, downstream distributions of ions are analyzed and compared for a planar stationary shock with an overshoot and a similar shock with ripples propagating along the shock front. It is shown that rippling results in the distributions, which are substantially broader and more diffuse in the phase space. Gyrotropization is sped up. Rippling is able to generate backstreaming ions, which are absent in the planar stationary case.https://doi.org/10.3847/1538-4357/acd63cShocks
spellingShingle Michael Gedalin
Nikolai V. Pogorelov
Vadim Roytershteyn
Scattering of Ions at a Rippled Shock
The Astrophysical Journal
Shocks
title Scattering of Ions at a Rippled Shock
title_full Scattering of Ions at a Rippled Shock
title_fullStr Scattering of Ions at a Rippled Shock
title_full_unstemmed Scattering of Ions at a Rippled Shock
title_short Scattering of Ions at a Rippled Shock
title_sort scattering of ions at a rippled shock
topic Shocks
url https://doi.org/10.3847/1538-4357/acd63c
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AT nikolaivpogorelov scatteringofionsatarippledshock
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