activity
20202022
most citedThe Ion Transition Range of Solar Wind Turbulence in the Inner Heliosphere: Parker Solar Probe Observations

39 citations · 77 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2022★ 5 cited

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…

physics.space-ph2021

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…

physics.plasm-ph2021

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…

physics.space-ph2021★ 39 cited

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…

physics.space-ph2020★ 33 cited

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…