Search Results - "Xiao, SuDong"
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Properties of Solar Wind Current Sheets in the Martian Space Environment
Published in The Astrophysical journal (01-10-2024)“…Abstract Transient current sheets (CSs) are common magnetic structures in the solar wind that can significantly disturb the planetary space environment and…”
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A New Tool for Understanding the Solar Wind–Venus Interaction: Three-dimensional Multifluid MHD Model
Published in The Astrophysical journal (01-03-2023)“…Abstract In this paper, we present a new tool to investigate the interaction of the solar wind with Venus with the approach of a global multifluid…”
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Statistical Analysis of Lunar 1 Hz Waves Using ARTEMIS Observations
Published in The Astrophysical journal (01-01-2023)“…Abstract Like 1 Hz waves occurring in the upstream of various celestial bodies in the solar system, 1 Hz narrowband whistler-mode waves are often observed…”
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Statistical study of magnetic holes in the upstream region of Mercury’s bow shock
Published in Earth and planetary physics (01-03-2024)“…Magnetic holes are magnetic depression structures that exist widely in many plasma environments. The magnetic holes with durations of >1 s in the solar wind at…”
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Interplanetary Coronal Mass Ejections and Stream Interaction Regions Observed by Tianwen-1 and MAVEN at Mars
Published in The Astrophysical journal. Supplement series (01-07-2023)“…Abstract The Tianwen-1 spacecraft is China's first Mars exploration mission. The Mars Orbiter Magnetometer (MOMAG) is a scientific instrument on board the…”
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Tianwen-1 and MAVEN Observations of the Response of Mars to an Interplanetary Coronal Mass Ejection
Published in The Astrophysical journal (01-08-2023)“…Abstract Interplanetary coronal mass ejections (ICMEs) are solar transients that have significant effects on the upper atmosphere and ionosphere of Mars. The…”
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Martian Bow Shock Oscillations Driven by Solar Wind Variations: Simultaneous Observations From Tianwen‐1 and MAVEN
Published in Geophysical research letters (28-08-2023)“…The Martian bow shock stands as the first defense against the solar wind and shapes the Martian magnetosphere. Previous studies showed the correlation between…”
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Unusual Martian Foreshock Waves Triggered by a Solar Wind Stream Interaction Region
Published in Astrophysical journal. Letters (01-04-2023)“…Abstract Planetary bow shocks noncollisionally dissipate the incident bulk flow energy of solar wind into some other forms. To what extent and how solar wind…”
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Responses of the field-aligned currents in the plasma sheet boundary layer to a geomagnetic storm
Published in Earth and planetary physics (01-09-2023)“…Geomagnetic storms can result in large magnetic field disturbances and intense currents in the magnetosphere and even on the ground.As an important medium of…”
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The Dynamic Evolution of Multipoint Interplanetary Coronal Mass Ejections Observed with BepiColombo, Tianwen-1, and MAVEN
Published in Astrophysical journal. Letters (01-07-2023)“…Abstract We present two multipoint interplanetary coronal mass ejections (ICMEs) detected by the Tianwen-1 and Mars Atmosphere and Volatile Evolution…”
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In-flight calibration of the magnetometer on the Mars orbiter of Tianwen-1
Published in Science China. Technological sciences (01-08-2023)“…Mars orbiter magnetometer (MOMAG) is one of seven science payloads onboard Tianwen-1’s orbiter. Unlike most of the satellites, Tianwen-1’s orbiter is not…”
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A statistical study on the shape and position of the magnetotail neutral sheet
Published in Annales geophysicae (1988) (26-02-2016)“…We study the average shape and position of the magnetotail neutral sheet based on magnetic field data obtained by Cluster, Geotail, TC-1, and THEMIS from the…”
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The Mars orbiter magnetometer of Tianwen-1: in-flight performance and first science results
Published in Earth and planetary physics (01-03-2023)“…The Mars Orbiter MAGnetometer(MOMAG)is a scientific instrument onboard the orbiter of China's first mission for Mars—Tianwen-1.Since November 13,2021,it has…”
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Magnetic Fluctuations Associated With Small-Scale Magnetic Holes in the Martian Magnetosheath
Published in Frontiers in astronomy and space sciences (04-04-2022)“…Small-scale magnetic holes are common magnetic structures with a spatial scale always smaller than one thermal proton gyroradius ( ρ i ) in the turbulent…”
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Turbulence in the near‐Venusian space: Venus Express observations
Published in Earth and planetary physics (01-01-2020)“…With Venus Express magnetic field measurements at 32 Hz from 2006 to 2012, we investigate statistically the magnetic fluctuations in the near‐Venusian space…”
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Statistical Properties of Small-scale Linear Magnetic Holes in the Martian Magnetosheath
Published in The Astrophysical journal (01-08-2021)“…Abstract The small-scale linear magnetic hole (LMH) is a magnetic dip with a size less than or on the order of ρ i (proton gyroradius), which may contribute to…”
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Oxygen Ion Escape at Venus Associated With Three‐Dimensional Kelvin‐Helmholtz Instability
Published in Geophysical research letters (28-03-2022)“…How oxygens escape from Venus has long been a fundamental but controversial topic in the planetary research. Among various key mechanisms, the Kelvin‐Helmholtz…”
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18
Achieving Secure On-Orbit Comparison in LEO Satellite-Enabled Offshore Wind Farm Surveillance
Published in IEEE internet of things journal (09-09-2024)“…The low Earth orbit (LEO) satellite constellation holds immense potential for offshore wind farm surveillance since it can provide all-day and all-weather…”
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Calibration of the Zero Offset of the Fluxgate Magnetometer on Board the Tianwen‐1 Orbiter in the Martian Magnetosheath
Published in Journal of geophysical research. Space physics (01-01-2024)“…High‐precision measurements of the magnetic field are critical to explore the near‐Mars environment. The Mars Orbiter MAGnetometer (MOMAG) is one of seven…”
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Trapping and Amplification of Unguided Mode EMIC Waves in the Radiation Belt
Published in Journal of geophysical research. Space physics (01-09-2021)“…Electromagnetic ion cyclotron (EMIC) waves can cause the scattering loss of the relativistic electrons in the radiation belt. They can be classified into the…”
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