Kinetic Structure of an Interplanetary Shock Observed at Two Heliocentric Longitudes

Interplanetary (IP) shocks ripple through the heliosphere, altering the solar wind. These shocks are characterized by abrupt changes in the solar wind properties. Due to their size, different sections of an IP shock sweep through solar wind regions wi

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Publication Details

Published
2025-09-29
DOI
https://doi.org/10.22541/essoar.175917269.90761815/v1
Primary Topic
Solar and Space Plasma Dynamics
Type
article
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article

Kinetic Structure of an Interplanetary Shock Observed at Two Heliocentric Longitudes

A. P. Dimmock, Ahmad Lalti, P. Louarn, M. André et al.
Solar and Space Plasma Dynamics
article

Kinetic Structure of an Interplanetary Shock Observed at Two Heliocentric Longitudes

A. P. Dimmock, Ahmad Lalti, P. Louarn, M. André, A. Fedorov, D. B. Graham, Christopher John Owen, M. Maksimović, M. Morooka, Y. V. Khotyaintsev, David Píša, J. J. Boldú, Jan Souček
article en

Abstract

Interplanetary (IP) shocks ripple through the heliosphere, altering the solar wind. These shocks are characterized by abrupt changes in the solar wind properties. Due to their size, different sections of an IP shock sweep through solar wind regions wi

Swedish Institute of Space Physics (SE), Observatoire de Paris (FR), Northumbria University (GB), Institute for Resource Analysis and Policy (IN), Czech Academy of Sciences, Institute of Atmospheric Physics (CZ)
National Aeronautics and Space Administration, UK Space Agency, UK Research and Innovation, Grantová Agentura České Republiky, Swedish National Space Agency, Centre National d’Etudes Spatiales, Agenzia Spaziale Italiana, Centre National de la Recherche Scientifique, Science and Technology Facilities Council
Openalex Percentile: Top 81%
Solar and Space Plasma Dynamics
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Kinetic Structure of an Interplanetary Shock Observed at Two Heliocentric Longitudes — A. P. Dimmock, Ahmad Lalti, et al. · (2025) | TGRS Research Map | TGRS