Journal article
Detection of magnetospheric ion drift patterns at Mars
Nature communications, Vol.14(1), 6866
10/27/2023
DOI: 10.1038/s41467-023-42630-7
PMCID: PMC10611764
PMID: 37891189
Abstract
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.
Mars lacks a global intrinsic magnetic field. Here, the authors show wedge-like dispersion structures of Hydrogen ions exhibiting butterfly-shaped distributions, which was previously found only in intrinsic magnetospheres.
Details
- Title: Subtitle
- Detection of magnetospheric ion drift patterns at Mars
- Creators
- Chi Zhang - University of Chinese Academy of SciencesHans Nilsson - Swedish Institute of Space PhysicsYusuke Ebihara - Kyoto UniversityMasatoshi Yamauchi - Swedish Institute of Space PhysicsMoa Persson - The University of TokyoZhaojin Rong - Institute of Geology and GeophysicsJun Zhong - Institute of Geology and GeophysicsChuanfei Dong - Boston UniversityYuxi Chen - Boston UniversityXuzhi Zhou - Beijing, ChinaYixin Sun - Peking UniversityYuki Harada - Kyoto UniversityJasper Halekas - University of IowaShaosui Xu - University of California, BerkeleyYoshifumi Futaana - Swedish Institute of Space PhysicsZhen Shi - Beijing, China Beijing, ChinaChongjing Yuan - Beijing, China Beijing, ChinaXiaotong Yun - Wuhan UniversitySong Fu - Wuhan UniversityJiawei Gao - University of Chinese Academy of SciencesMats Holmström - Swedish Institute of Space PhysicsYong Wei - Institute of Geology and GeophysicsStas Barabash - Swedish Institute of Space Physics
- Resource Type
- Journal article
- Publication Details
- Nature communications, Vol.14(1), 6866
- DOI
- 10.1038/s41467-023-42630-7
- PMID
- 37891189
- PMCID
- PMC10611764
- NLM abbreviation
- Nat Commun
- ISSN
- 2041-1723
- eISSN
- 2041-1723
- Publisher
- Nature Publishing Group UK
- Grant note
- ; 41922031, 41774188 / ;
- Language
- English
- Date published
- 10/27/2023
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984503059002771
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