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Enhanced ion acceleration due to high-shear tangential discontinuities upstream of quasi-perpendicular shocks

Enhanced ion acceleration due to high-shear tangential discontinuities upstream of quasi-perpendicular shocks
Enhanced ion acceleration due to high-shear tangential discontinuities upstream of quasi-perpendicular shocks

Collisionless shock waves are efficient ion accelerators. Previous numerical and observational studies have shown that quasi-parallel (Q) shocks are more effective than quasi-perpendicular (Q) shocks at generating energetic ions under steady upstream conditions. Here, we use a local, 2D, hybrid particle-in-cell model to investigate how ion acceleration at super-critical Q shocks is modulated when tangential discontinuities (TDs) with large magnetic shear are present in the upstream plasma. We show that such TDs can significantly increase the ion acceleration efficiency of 2D Q shocks, up to a level comparable to Q shocks. Using data from the hybrid model and test particle simulations, we show that the enhanced energization is related to the magnetic field change associated with the discontinuity. When shock-reflected ions cross the TD during their upstream gyromotion, the sharp field change causes the ions to propagate further upstream, and gain additional energy from the convection electric field associated with the upstream plasma flow. Our findings illustrate that the presence of upstream discontinuities can lead to bursts of energetic ions, even when they do not trigger the formation of foreshock transients. These results emphasize the importance of time-variable upstream conditions when considering ion energization at shocks.

bow shock, collisionless shocks, particle acceleration, solar wind, tangential discontinuities
2169-9380
Steinvall, K.
442a9f09-0f5c-4437-b50f-3658f0c77ba9
Gingell, I.
ba7b8113-3833-40d8-a879-aab3f987455d
Steinvall, K.
442a9f09-0f5c-4437-b50f-3658f0c77ba9
Gingell, I.
ba7b8113-3833-40d8-a879-aab3f987455d

Steinvall, K. and Gingell, I. (2024) Enhanced ion acceleration due to high-shear tangential discontinuities upstream of quasi-perpendicular shocks. Journal of Geophysical Research: Space Physics, 129 (6), [e2024JA032543]. (doi:10.1029/2024JA032543).

Record type: Article

Abstract

Collisionless shock waves are efficient ion accelerators. Previous numerical and observational studies have shown that quasi-parallel (Q) shocks are more effective than quasi-perpendicular (Q) shocks at generating energetic ions under steady upstream conditions. Here, we use a local, 2D, hybrid particle-in-cell model to investigate how ion acceleration at super-critical Q shocks is modulated when tangential discontinuities (TDs) with large magnetic shear are present in the upstream plasma. We show that such TDs can significantly increase the ion acceleration efficiency of 2D Q shocks, up to a level comparable to Q shocks. Using data from the hybrid model and test particle simulations, we show that the enhanced energization is related to the magnetic field change associated with the discontinuity. When shock-reflected ions cross the TD during their upstream gyromotion, the sharp field change causes the ions to propagate further upstream, and gain additional energy from the convection electric field associated with the upstream plasma flow. Our findings illustrate that the presence of upstream discontinuities can lead to bursts of energetic ions, even when they do not trigger the formation of foreshock transients. These results emphasize the importance of time-variable upstream conditions when considering ion energization at shocks.

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JGR Space Physics - 2024 - Steinvall - Enhanced Ion Acceleration Due To High‐Shear Tangential Discontinuities Upstream of - Version of Record
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Accepted/In Press date: 17 June 2024
e-pub ahead of print date: 21 June 2024
Published date: 21 June 2024
Keywords: bow shock, collisionless shocks, particle acceleration, solar wind, tangential discontinuities

Identifiers

Local EPrints ID: 496206
URI: http://eprints.soton.ac.uk/id/eprint/496206
ISSN: 2169-9380
PURE UUID: 837aa730-d914-4d8c-9cb2-c5bb38ac066f
ORCID for I. Gingell: ORCID iD orcid.org/0000-0003-2218-1909

Catalogue record

Date deposited: 06 Dec 2024 17:48
Last modified: 07 Dec 2024 03:02

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Contributors

Author: K. Steinvall
Author: I. Gingell ORCID iD

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