Pickup protons at quasi-perpendicular shocks: full particle electrodynamic simulations

We have performed 3 one-dimensional full particle electromagnetic simulations of a quasi-perpendicular shock with the same Alfvén Mach number <I>M<sub>A</sub></I>~5, shock normal-magnetic field angle &Theta;<sub><I>Bn</I></sub>=87&deg; and i...

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Main Authors: S. Matsukiyo, M. Scholer, D. Burgess
Format: Article
Language:English
Published: Copernicus Publications 2007-02-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/25/283/2007/angeo-25-283-2007.pdf
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spelling doaj-bc959c3fa7bc48e7876f6a381c4714212020-11-24T22:23:38ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762007-02-012528329110.5194/angeo-25-283-2007Pickup protons at quasi-perpendicular shocks: full particle electrodynamic simulationsS. Matsukiyo0M. Scholer1M. Scholer2D. Burgess3Earth System Science and Technology, Kyushu University, Fukuoka, JapanAstronomy Unit, Queen Mary, University of London, UKalso at: Max-Planck-Institut für extraterrestrische Physik, Garching, GermanyAstronomy Unit, Queen Mary, University of London, UKWe have performed 3 one-dimensional full particle electromagnetic simulations of a quasi-perpendicular shock with the same Alfvén Mach number <I>M<sub>A</sub></I>~5, shock normal-magnetic field angle &Theta;<sub><I>Bn</I></sub>=87&deg; and ion and electron beta (particle to magnetic field pressure) of 0.1. In the first run we used an ion to electron mass ratio close to the physical one (<I>m<sub>i</sub>/m<sub>e</sub></i>=1024). As expected from previous high mass ratio simulations the Modified Two-Stream instability develops in the foot of the shock, and the shock periodically reforms itself. We have then self-consistently included in the simulation 10% pickup protons distributed on a shell in velocity space as a third component. In a run with an unrealistically low mass ratios of 200 the shock still reforms itself; reformation is due to accumulation of specularly reflected particles at the upstream edge of the foot. In a third run including pickup protons we used a mass ratio of 1024. The shock reforms periodically as in the low mass ratio run with a somewhat smaller time constant. The specular reflection of pickup protons results in an increase of the shock potential some distance ahead of the shock foot and ramp. The minimum scale of the cross shock potential during reformation is about 7 electron inertial length &lambda;<sub>e</sub>. We do not find any pickup proton acceleration in the ramp or downstream of the shock beyond the energy which specularly reflected ions gain by the motional electric field of the solar wind during their upstream gyration.https://www.ann-geophys.net/25/283/2007/angeo-25-283-2007.pdf
collection DOAJ
language English
format Article
sources DOAJ
author S. Matsukiyo
M. Scholer
M. Scholer
D. Burgess
spellingShingle S. Matsukiyo
M. Scholer
M. Scholer
D. Burgess
Pickup protons at quasi-perpendicular shocks: full particle electrodynamic simulations
Annales Geophysicae
author_facet S. Matsukiyo
M. Scholer
M. Scholer
D. Burgess
author_sort S. Matsukiyo
title Pickup protons at quasi-perpendicular shocks: full particle electrodynamic simulations
title_short Pickup protons at quasi-perpendicular shocks: full particle electrodynamic simulations
title_full Pickup protons at quasi-perpendicular shocks: full particle electrodynamic simulations
title_fullStr Pickup protons at quasi-perpendicular shocks: full particle electrodynamic simulations
title_full_unstemmed Pickup protons at quasi-perpendicular shocks: full particle electrodynamic simulations
title_sort pickup protons at quasi-perpendicular shocks: full particle electrodynamic simulations
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2007-02-01
description We have performed 3 one-dimensional full particle electromagnetic simulations of a quasi-perpendicular shock with the same Alfvén Mach number <I>M<sub>A</sub></I>~5, shock normal-magnetic field angle &Theta;<sub><I>Bn</I></sub>=87&deg; and ion and electron beta (particle to magnetic field pressure) of 0.1. In the first run we used an ion to electron mass ratio close to the physical one (<I>m<sub>i</sub>/m<sub>e</sub></i>=1024). As expected from previous high mass ratio simulations the Modified Two-Stream instability develops in the foot of the shock, and the shock periodically reforms itself. We have then self-consistently included in the simulation 10% pickup protons distributed on a shell in velocity space as a third component. In a run with an unrealistically low mass ratios of 200 the shock still reforms itself; reformation is due to accumulation of specularly reflected particles at the upstream edge of the foot. In a third run including pickup protons we used a mass ratio of 1024. The shock reforms periodically as in the low mass ratio run with a somewhat smaller time constant. The specular reflection of pickup protons results in an increase of the shock potential some distance ahead of the shock foot and ramp. The minimum scale of the cross shock potential during reformation is about 7 electron inertial length &lambda;<sub>e</sub>. We do not find any pickup proton acceleration in the ramp or downstream of the shock beyond the energy which specularly reflected ions gain by the motional electric field of the solar wind during their upstream gyration.
url https://www.ann-geophys.net/25/283/2007/angeo-25-283-2007.pdf
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AT mscholer pickupprotonsatquasiperpendicularshocksfullparticleelectrodynamicsimulations
AT dburgess pickupprotonsatquasiperpendicularshocksfullparticleelectrodynamicsimulations
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