Detection of magnetospheric ion drift patterns at Mars.


Journal

Nature communications
ISSN: 2041-1723
Titre abrégé: Nat Commun
Pays: England
ID NLM: 101528555

Informations de publication

Date de publication:
27 Oct 2023
Historique:
received: 11 07 2023
accepted: 13 10 2023
medline: 28 10 2023
pubmed: 28 10 2023
entrez: 27 10 2023
Statut: epublish

Résumé

Mars lacks a global magnetic field, and instead possesses small-scale crustal magnetic fields, making its magnetic environment fundamentally different from intrinsic magnetospheres like those of Earth or Saturn. Here we report the discovery of magnetospheric ion drift patterns, typical of intrinsic magnetospheres, at Mars using measurements from Mars Atmosphere and Volatile EvolutioN mission. Specifically, we observe wedge-like dispersion structures of hydrogen ions exhibiting butterfly-shaped distributions (pitch angle peaks at 22.5°-45° and 135°-157.5°) within the Martian crustal fields, a feature previously observed only in planetary-scale intrinsic magnetospheres. These dispersed structures are the results of drift motions that fundamentally resemble those observed in intrinsic magnetospheres. Our findings indicate that the Martian magnetosphere embodies an intermediate case where both the unmagnetized and magnetized ion behaviors could be observed because of the wide range of strengths and spatial scales of the crustal magnetic fields around Mars.

Identifiants

pubmed: 37891189
doi: 10.1038/s41467-023-42630-7
pii: 10.1038/s41467-023-42630-7
pmc: PMC10611764
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

6866

Subventions

Organisme : National Natural Science Foundation of China (National Science Foundation of China)
ID : 41922031, 41774188

Informations de copyright

© 2023. The Author(s).

Références

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pubmed: 16217034
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pubmed: 26436770
Space Sci Rev. 2019;215(1):9
pubmed: 30880847

Auteurs

Chi Zhang (C)

Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, China.
Center for Space Physics and Department of Astronomy, Boston University, Boston, MA, USA.

Hans Nilsson (H)

Swedish Institute of Space Physics, Kiruna, Sweden.

Yusuke Ebihara (Y)

Research Institute for Sustainable Humanosphere, Kyoto University, Uji, Japan.

Masatoshi Yamauchi (M)

Swedish Institute of Space Physics, Kiruna, Sweden.

Moa Persson (M)

Graduate School of Frontier Sciences, The University of Tokyo, Kashiwa, Japan.

Zhaojin Rong (Z)

Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China. rongzhaojin@mail.iggcas.ac.cn.
College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, China. rongzhaojin@mail.iggcas.ac.cn.

Jun Zhong (J)

Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, China.

Chuanfei Dong (C)

Center for Space Physics and Department of Astronomy, Boston University, Boston, MA, USA.

Yuxi Chen (Y)

Center for Space Physics and Department of Astronomy, Boston University, Boston, MA, USA.

Xuzhi Zhou (X)

School of Earth and Space Sciences, Peking University, Beijing, China.

Yixin Sun (Y)

School of Earth and Space Sciences, Peking University, Beijing, China.

Yuki Harada (Y)

Department of Geophysics, Graduate School of Science, Kyoto University, Kyoto, Japan.

Jasper Halekas (J)

Department of Physics and Astronomy, University of Iowa, Iowa City, IA, USA.

Shaosui Xu (S)

Space Sciences Laboratory, University of California, Berkeley, Berkeley, CA, USA.

Yoshifumi Futaana (Y)

Swedish Institute of Space Physics, Kiruna, Sweden.

Zhen Shi (Z)

Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, China.

Chongjing Yuan (C)

Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, China.

Xiaotong Yun (X)

Department of Space Physics, School of Electronic Information, Wuhan University, Wuhan, China.

Song Fu (S)

Department of Space Physics, School of Electronic Information, Wuhan University, Wuhan, China.

Jiawei Gao (J)

Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, China.

Mats Holmström (M)

Swedish Institute of Space Physics, Kiruna, Sweden.

Yong Wei (Y)

Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China. weiy@mail.iggcas.ac.cn.
College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, China. weiy@mail.iggcas.ac.cn.

Stas Barabash (S)

Swedish Institute of Space Physics, Kiruna, Sweden.

Classifications MeSH