126 citations · 304 across the 8 of their papers we have counts for
9 papers
A Two-Population von Mises--Fisher Distribution of the Magnetic Field Direction in the Young Solar Wind
Gang Li, N. H. Bian, S. Y. Huang +6
The one-point distribution of the magnetic field direction in the young solar wind is found to be a superposition of two populations rather than a single exponential. Using Parker…
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…
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 evolution of compressible solar wind turbulence in the inner heliosphere: PSP, THEMIS and MAVEN observations
N. Andrés, F. Sahraoui, L. Z. Hadid +5
The first computation of the compressible energy transfer rate from 0.2 AU up to 1.7 AU is obtained using PSP, THEMIS and MAVEN observations. The compressible energy…
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…
On the Existence of the Kolmogorov Inertial Range in the Terrestrial Magnetosheath Turbulence
S. Y. Huang, L. Z. Hadid, F. Sahraoui +2
In the solar wind, power spectral density (PSD) of the magnetic field fluctuations generally follow the so-called Kolmogorov spectrum f^-5/3 in the inertial range, where the dynami…
Kinetic Turbulence in the Terrestrial Magnetosheath: Cluster Observations
S. Y. Huang, F. Sahraoui, X. H. Deng +5
We present a first statistical study of subproton and electron scales turbulence in the terrestrial magnetosheath using the Cluster Search Coil Magnetometer (SCM) waveforms of the…