52 citations · 151 across the 9 of their papers we have counts for
9 papers
Kinetic-Scale Topological Structures Associated with Energy Dissipation in the Turbulent Reconnection Outflow
S. Y. Huang, J. Zhang, Q. Y. Xiong +7
Assisted with Magnetospheric Multiscale (MMS) mission capturing unprecedented high-resolution data in the terrestrial magnetotail, we apply a local streamline-topology classificati…
Satellite galaxies' drag on field stars in the Milky Way
Xilong Liang, Jifeng Liu, Jingkun Zhao +1
With Gaia EDR3 data, velocity dispersion of Milky Way field stars around satellite galaxies have been investigated. We have fitted velocity dispersion against distance to satellite…
Anisotropy of Magnetic Field Spectra at Kinetic Scales of Solar Wind Turbulence as Revealed by Parker Solar Probe in the Inner Heliosphere
S. Y. Huang, S. B. Xu, J. Zhang +11
Using the Parker Solar Probe data taken in the inner heliosphere, we investigate the power and spatial anisotropy of magnetic-field spectra at kinetic scales (i.e., around sub-ion…
Electron-only Reconnection in Ion-scale Current Sheet at the Magnetopause
S. Y. Huang, Q. Y. Xiong, L. F. Song +5
In the standard model of magnetic reconnection, both ions and electrons couple to the newly reconnected magnetic field lines and are ejected away from the reconnection diffusion re…
In Situ Detection of Kinetic-Size Magnetic Holes in the Martian Magnetosheath
S. Y. Huang, R. T. Lin, Z. G. Yuan +7
Depression in magnetic field strength with a scale below one proton gyroradius is referred to as kinetic-size magnetic hole (KSMH). KSMHs are frequently observed near terrestrial s…
Observational Evidence of Magnetic Reconnection in the Terrestrial Foreshock Region
K. Jiang, S. Y. Huang, H. S. Fu +10
Electron heating/acceleration in the foreshock, by which electrons may be energized beyond thermal energies prior to encountering the bow shock, is very important for the bow shock…
The Ion Transition Range of Solar Wind Turbulence in the Inner Heliosphere: Parker Solar Probe Observations
S. Y. Huang, F. Sahraoui, N. Andrés +15
The scaling of the turbulent spectra provides a key measurement that allows to discriminate between different theoretical predictions of turbulence. In the solar wind, this has dri…
Characteristics of Magnetic Holes in the Solar Wind Revealed by Parker Solar Probe
L. Yu, S. Y. Huang, Z. G. Yuan +6
We present a statistical analysis for the characteristics and radial evolution of linear magnetic holes (LMHs) in the solar wind from 0.166 to 0.82 AU using Parker Solar Probe obse…
Kinetic Scale Slow Solar Wind Turbulence in the Inner Heliosphere: Co-existence of Kinetic Alfvén Waves and Alfvén Ion Cyclotron Waves
S. Y. Huang, J. Zhang, F. Sahraoui +12
The nature of the plasma wave modes around the ion kinetic scales in highly Alfvénic slow solar wind turbulence is investigated using data from the NASA's Parker Solar Probe taken…