MAVEN observation of magnetosonic waves in the Martian magnetotail region

Bibliographic Details
Title: MAVEN observation of magnetosonic waves in the Martian magnetotail region
Authors: ShangChun Teng, JiCheng Sun, JiaWei Gao, Y. Harada, Markus Fraenz, DeSheng Han
Source: Earth and Planetary Physics, Vol 8, Iss 2, Pp 317-325 (2024)
Publisher Information: Science Press, 2024.
Publication Year: 2024
Collection: LCC:Science
LCC:Geophysics. Cosmic physics
LCC:Environmental sciences
Subject Terms: martian magnetotail region, magnetosonic waves, proton escape, Science, Geophysics. Cosmic physics, QC801-809, Environmental sciences, GE1-350
More Details: Magnetosonic waves are an important medium for energy transfer in collisionless space plasma. Magnetosonic waves have been widely investigated in the upstream of the bow shock at Mars. These waves are believed to originate from pickup ions or reflected particles. By utilizing MAVEN spacecraft data, we have observed the occurrence of quasi-perpendicularly propagating magnetosonic emissions near the proton gyrofrequency in the Martian magnetotail region. These plasma waves are associated with a significant enhancement of proton and oxygen flux. The excited magnetosonic waves could possibly heat the protons through resonance and facilitate the ionospheric plasma escape. Our results could be helpful to better understand the Mars’ magnetospheric dynamics and offer insights into possible energy redistribution between waves and plasma in the Martian nightside magnetosphere.
Document Type: article
File Description: electronic resource
Language: English
ISSN: 2096-3955
Relation: https://doaj.org/toc/2096-3955
DOI: 10.26464/epp2024003?pageType=en
DOI: 10.26464/epp2024003
Access URL: https://doaj.org/article/877e157270f34dd68a3aaf59ecd96d49
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  Data: MAVEN observation of magnetosonic waves in the Martian magnetotail region
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  Data: <searchLink fieldCode="AR" term="%22ShangChun+Teng%22">ShangChun Teng</searchLink><br /><searchLink fieldCode="AR" term="%22JiCheng+Sun%22">JiCheng Sun</searchLink><br /><searchLink fieldCode="AR" term="%22JiaWei+Gao%22">JiaWei Gao</searchLink><br /><searchLink fieldCode="AR" term="%22Y%2E+Harada%22">Y. Harada</searchLink><br /><searchLink fieldCode="AR" term="%22Markus+Fraenz%22">Markus Fraenz</searchLink><br /><searchLink fieldCode="AR" term="%22DeSheng+Han%22">DeSheng Han</searchLink>
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  Data: Earth and Planetary Physics, Vol 8, Iss 2, Pp 317-325 (2024)
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  Data: Science Press, 2024.
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  Data: <searchLink fieldCode="DE" term="%22martian+magnetotail+region%22">martian magnetotail region</searchLink><br /><searchLink fieldCode="DE" term="%22magnetosonic+waves%22">magnetosonic waves</searchLink><br /><searchLink fieldCode="DE" term="%22proton+escape%22">proton escape</searchLink><br /><searchLink fieldCode="DE" term="%22Science%22">Science</searchLink><br /><searchLink fieldCode="DE" term="%22Geophysics%2E+Cosmic+physics%22">Geophysics. Cosmic physics</searchLink><br /><searchLink fieldCode="DE" term="%22QC801-809%22">QC801-809</searchLink><br /><searchLink fieldCode="DE" term="%22Environmental+sciences%22">Environmental sciences</searchLink><br /><searchLink fieldCode="DE" term="%22GE1-350%22">GE1-350</searchLink>
– Name: Abstract
  Label: Description
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  Data: Magnetosonic waves are an important medium for energy transfer in collisionless space plasma. Magnetosonic waves have been widely investigated in the upstream of the bow shock at Mars. These waves are believed to originate from pickup ions or reflected particles. By utilizing MAVEN spacecraft data, we have observed the occurrence of quasi-perpendicularly propagating magnetosonic emissions near the proton gyrofrequency in the Martian magnetotail region. These plasma waves are associated with a significant enhancement of proton and oxygen flux. The excited magnetosonic waves could possibly heat the protons through resonance and facilitate the ionospheric plasma escape. Our results could be helpful to better understand the Mars’ magnetospheric dynamics and offer insights into possible energy redistribution between waves and plasma in the Martian nightside magnetosphere.
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        Value: 10.26464/epp2024003?pageType=en
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      – Text: English
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        PageCount: 9
        StartPage: 317
    Subjects:
      – SubjectFull: martian magnetotail region
        Type: general
      – SubjectFull: magnetosonic waves
        Type: general
      – SubjectFull: proton escape
        Type: general
      – SubjectFull: Science
        Type: general
      – SubjectFull: Geophysics. Cosmic physics
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      – SubjectFull: QC801-809
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      – SubjectFull: GE1-350
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      – TitleFull: MAVEN observation of magnetosonic waves in the Martian magnetotail region
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            NameFull: ShangChun Teng
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