activity
20202026
most citedPossible Generation Mechanism for Compressional Alfvénic Spikes as Observed by Parker Solar Probe

29 citations · 71 across the 9 of their papers we have counts for

collaborators

9 papers

physics.space-ph2026

Proton Temperature Anisotropy Across Interplanetary Shocks: A Statistical Analysis with WIND observations

Zeping Jin, Lingling Zhao, Xingyu Zhu +6

Interplanetary (IP) shocks efficiently modify the proton temperature anisotropy of the solar wind. Analyzing ~800 IP shocks observed by the Wind spacecraft from 1997-2024, we prese…

astro-ph.SR2024

Characterization of Turbulent Fluctuations in the Sub-Alfvenic Solar Wind

Gary P. Zank, Lingling Zhao, Laxman Adhikari +8

Parker Solar Probe (PSP) observed sub-Alfvenic solar wind intervals during encounters 8 - 14, and low-frequency magnetohydrodynamic turbulence in these regions may differ from that…

physics.plasm-ph2022★ 12 cited

Coherence of ion cyclotron resonance for damping ion cyclotron waves in space plasmas

Qiaowen Luo, Xingyu Zhu, Jiansen He +4

Ion cyclotron resonance is one of the fundamental energy conversion processes through field-particle interaction in collisionless plasmas. However, the key evidence for ion cyclotr…

physics.space-ph2021

Observations of rapidly growing whistler waves in front of space plasma shock

Jiansen He, Xingyu Zhu, Qiaowen Luo +8

Whistler mode wave is a fundamental perturbation of electromagnetic fields and plasmas in various environments including planetary space, laboratory and astrophysics. The origin an…

astro-ph.SR2021★ 7 cited

Growth of Outward Propagating Fast-Magnetosonic/Whistler Waves in the Inner Heliosphere Observed by Parker Solar Probe

Jiansen He, Ying Wang, Xingyu Zhu +3

The solar wind in the inner heliosphere has been observed by Parker Solar Probe (PSP) to exhibit abundant wave activities. The cyclotron wave modes in the sense of ions or electron…

physics.plasm-ph2021★ 3 cited

Power Anisotropy, Dispersion Signature and Turbulence Diffusion Region in the 3D Wavenumber Domain of Space Plasma Turbulence

Rong Lin, Jiansen He, Xingyu Zhu +4

We explore the multi-faceted important features of turbulence (e.g., anisotropy, dispersion, diffusion) in the three-dimensional (3D) wavenumber domain (, $k_{\perp,1}…

physics.plasm-ph2020★ 20 cited

Contribution of Magnetic Reconnection Events to Energy Dissipation in Magnetosheath Turbulence

Chuanpeng Hou, Jiansen He, Xingyu Zhu +1

By analyzing the magnetosheath measurements from MMS, we obtain the statistical results for the contribution of magnetic reconnection (MR) events at electron scales to the energy d…

physics.space-ph2020

Wave Composition, Propagation, and Polarization of MHD Turbulence within 0.3AU as Observed by PSP

Xingyu Zhu, Jiansen He, Daniel Verscharen +2

Turbulence, a ubiquitous phenomenon in interplanetary space, is crucial for the energy conversion of space plasma at multiple scales. This work focuses on the propagation, polariza…

astro-ph.SR2020★ 29 cited

Possible Generation Mechanism for Compressional Alfvénic Spikes as Observed by Parker Solar Probe

Jiansen He, Xingyu Zhu, Liping Yang +4

The solar wind is found by Parker Solar Probe (PSP) to be abundant with Alfvénic velocity spikes and magnetic field kinks. Temperature enhancement is another remarkable feature ass…