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Magnetosheath jets at Mars

Plasma entities, known as magnetosheath jets, with higher dynamic pressure than the surrounding plasma, are often seen at Earth. They generate waves and contribute to energy transfer in the magnetosheath. Affecting the magnetopause, they cause surface waves and transfer energy into the magnetosphere...

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Autores principales: Gunell, Herbert, Hamrin, Maria, Nesbit-Östman, Sara, Krämer, Eva, Nilsson, Hans
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2023
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10413640/
https://www.ncbi.nlm.nih.gov/pubmed/37267367
http://dx.doi.org/10.1126/sciadv.adg5703
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author Gunell, Herbert
Hamrin, Maria
Nesbit-Östman, Sara
Krämer, Eva
Nilsson, Hans
author_facet Gunell, Herbert
Hamrin, Maria
Nesbit-Östman, Sara
Krämer, Eva
Nilsson, Hans
author_sort Gunell, Herbert
collection PubMed
description Plasma entities, known as magnetosheath jets, with higher dynamic pressure than the surrounding plasma, are often seen at Earth. They generate waves and contribute to energy transfer in the magnetosheath. Affecting the magnetopause, they cause surface waves and transfer energy into the magnetosphere, causing throat auroras and magnetic signatures detectable on the ground. We show that jets exist also beyond Earth’s environment in the magnetosheath of Mars, using data obtained by the MAVEN spacecraft. Thus, jets can be created also at Mars, which differs from Earth by its smaller bow shock, and they are associated with an increased level of magnetic field fluctuations. Jets couple large and small scales in magnetosheaths in the solar system and can play a similar part in astrophysical plasmas.
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spelling pubmed-104136402023-08-11 Magnetosheath jets at Mars Gunell, Herbert Hamrin, Maria Nesbit-Östman, Sara Krämer, Eva Nilsson, Hans Sci Adv Earth, Environmental, Ecological, and Space Sciences Plasma entities, known as magnetosheath jets, with higher dynamic pressure than the surrounding plasma, are often seen at Earth. They generate waves and contribute to energy transfer in the magnetosheath. Affecting the magnetopause, they cause surface waves and transfer energy into the magnetosphere, causing throat auroras and magnetic signatures detectable on the ground. We show that jets exist also beyond Earth’s environment in the magnetosheath of Mars, using data obtained by the MAVEN spacecraft. Thus, jets can be created also at Mars, which differs from Earth by its smaller bow shock, and they are associated with an increased level of magnetic field fluctuations. Jets couple large and small scales in magnetosheaths in the solar system and can play a similar part in astrophysical plasmas. American Association for the Advancement of Science 2023-06-02 /pmc/articles/PMC10413640/ /pubmed/37267367 http://dx.doi.org/10.1126/sciadv.adg5703 Text en Copyright © 2023 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution License 4.0 (CC BY). https://creativecommons.org/licenses/by/4.0/This is an open-access article distributed under the terms of the Creative Commons Attribution license (https://creativecommons.org/licenses/by/4.0/) , which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
spellingShingle Earth, Environmental, Ecological, and Space Sciences
Gunell, Herbert
Hamrin, Maria
Nesbit-Östman, Sara
Krämer, Eva
Nilsson, Hans
Magnetosheath jets at Mars
title Magnetosheath jets at Mars
title_full Magnetosheath jets at Mars
title_fullStr Magnetosheath jets at Mars
title_full_unstemmed Magnetosheath jets at Mars
title_short Magnetosheath jets at Mars
title_sort magnetosheath jets at mars
topic Earth, Environmental, Ecological, and Space Sciences
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10413640/
https://www.ncbi.nlm.nih.gov/pubmed/37267367
http://dx.doi.org/10.1126/sciadv.adg5703
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