Observational Characteristics of Electron Distributions in the Martian Induced Magnetotail

Abstract Mars's magnetotail represents a unique case within the solar system, embodying both intrinsic and induced magnetic fields. Yet, the electron dynamics within this region have remained largely unexplored. Utilizing nine years of electron and magnetic field data from the Mars Atmosphere and Volatile EvolutioN mission (MAVEN), we conducted a comprehensive statistical analysis to uncover the average electron characteristics in the Martian induced magnetotail for the first time. Our findings revealed a distinct pattern of electron behavior: in the lobe regions, electrons tend to converge toward the current sheet, driven by an ambipolar electric field that is directed from the current sheet toward the lobe. Additionally, we observed that electrons are more energetic in the +E hemisphere, where the solar wind electric field points away from Mars, compared to the opposite hemisphere. This mirrors the behavior of planetary ions and supports the hypothesized formation mechanism of sinuous auroras.

Authors

Institutions

Publication Details

Journal
Geophysical Research Letters
Published
2025-03-29
DOI
https://doi.org/10.1029/2024gl113030
Citations
8
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
9.24

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Observational Characteristics of Electron Distributions in the Martian Induced Magnetotail

Hongyang Zhou, D. L. Mitchell, Shannon Curry, Yuki Harada et al.
8 citations
Geophysical Research Letters
Planetary Science and Exploration
9.24
article

Observational Characteristics of Electron Distributions in the Martian Induced Magnetotail

Hongyang Zhou, D. L. Mitchell, Shannon Curry, Yuki Harada, Zhi‐Yang Liu, Chi Zhang, Jun Qin, Chuanfei Dong, Jan Deca, Shaosui Xu, C. Mazelle
article en
8 citations

Abstract

Abstract Mars's magnetotail represents a unique case within the solar system, embodying both intrinsic and induced magnetic fields. Yet, the electron dynamics within this region have remained largely unexplored. Utilizing nine years of electron and magnetic field data from the Mars Atmosphere and Volatile EvolutioN mission (MAVEN), we conducted a comprehensive statistical analysis to uncover the average electron characteristics in the Martian induced magnetotail for the first time. Our findings revealed a distinct pattern of electron behavior: in the lobe regions, electrons tend to converge toward the current sheet, driven by an ambipolar electric field that is directed from the current sheet toward the lobe. Additionally, we observed that electrons are more energetic in the +E hemisphere, where the solar wind electric field points away from Mars, compared to the opposite hemisphere. This mirrors the behavior of planetary ions and supports the hypothesized formation mechanism of sinuous auroras.

Geophysical Research LettersVol. 52(7)
Boston University (US), Centre National de la Recherche Scientifique (FR), Université Toulouse III - Paul Sabatier (FR), University of Colorado Boulder (US), Kyoto University (JP), Laboratory for Atmospheric and Space Physics (US), Institut de Recherche en Astrophysique et Planétologie (FR), University of California, Berkeley (US)
National Aeronautics and Space Administration, Centre National d’Etudes Spatiales, Nuclear Safety and Security Commission
Openalex Percentile: Top 2%
Planetary Science and Exploration
9.24
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.