activity
20222026
most citedNew Observations of Solar Wind 1/f Turbulence Spectrum from Parker Solar Probe

35 citations · 80 across the 10 of their papers we have counts for

collaborators

10 papers

physics.plasm-ph2026

Cavitons Associated with Ion-Acoustic-Like Waves in Foreshock Transients

Runyi Liu, Terry Liu, Xin An +2

Foreshock transients upstream of the Earth's bow shock, such as foreshock bubbles and hot flow anomalies, are often characterized by reduced-density cores and strong plasma fluctua…

physics.plasm-ph2025

Energy transfer from MHD-scale slow-mode waves to kinetic-scale ion acoustic waves

Xiaofei Shi, Xin An, Vassilis Angelopoulos

Large-amplitude slow-mode waves are commonly observed near Earth's magnetopause. Recent observations show that these waves can occur simultaneously with kinetic-scale ion acoustic…

physics.space-ph2024★ 4 cited

Picturing global substorm dynamics in the magnetotail using low-altitude ELFIN measurements and data mining-based magnetic field reconstructions

Xiaofei Shi, Grant K. Stephens, Anton V. Artemyev +2

A global reconfiguration of the magnetotail characterizes substorms. Current sheet thinning, intensification, and magnetic field stretching are defining features of the substorm gr…

physics.space-ph2023★ 5 cited

Solar Wind Structures from the Gaussianity of Magnetic Magnitude

Zesen Huang, Chen Shi, Marco Velli +9

One of the primary science objectives of Parker Solar Probe (PSP) is to determine the structures and dynamics of the plasma and magnetic fields at the sources of the solar wind. Ho…

physics.plasm-ph2023

Properties of Intense Electromagnetic Ion Cyclotron Waves: Implications for Quasi-linear, Nonlinear, and Nonresonant Wave-Particle Interactions

Xiaofei Shi, Anton Artemyev, Xiao-Jia Zhang +3

Resonant interactions between relativistic electrons and electromagnetic ion cyclotron (EMIC) waves provide an effective loss mechanism for this important electron population in th…

physics.space-ph2023

Electron resonant interaction with whistler-mode waves around the Earth's bow shock II: the mapping technique

David S. Tonoian, Xiaofei Shi, Anton V. Artemyev +2

Electron resonant scattering by high-frequency electromagnetic whistler-mode waves has been proposed as a mechanism for solar wind electron scattering and pre-acceleration to energ…

physics.space-ph2023

Electron resonant interaction with whistler-mode waves around the Earth's bow shock I: the probabilistic approach

Xiaofei Shi, David S. Tonoian, Anton V. Artemyev +2

Adiabatic heating of solar wind electrons at the Earth's bow shock and its foreshock region produces transversely anisotropic hot electrons that, in turn, generate intense high-fre…

physics.space-ph2023★ 25 cited

Nonresonant scattering of energetic electrons by electromagnetic ion cyclotron waves: spacecraft observations and theoretical framework

Xin An, Anton Artemyev, Vassilis Angelopoulos +4

Electromagnetic ion cyclotron (EMIC) waves lead to rapid scattering of relativistic electrons in Earth's radiation belts, due to their large amplitudes relative to other waves that…

astro-ph.SR2023★ 35 cited

New Observations of Solar Wind 1/f Turbulence Spectrum from Parker Solar Probe

Zesen Huang, Nikos Sioulas, Chen Shi +22

The trace magnetic power spectrum in the solar wind is known to be characterized by a double power law at scales much larger than the proton gyro-radius, with flatter spectral expo…

physics.plasm-ph2022★ 11 cited

Intense whistler-mode waves at foreshock transients: characteristics and regimes of wave-particle resonant interaction

Xiaofei Shi, Terry Liu, Anton Artemyev +3

Thermalization and heating of plasma flows at shocks result in unstable charged-particle distributions which generate a wide range of electromagnetic waves. These waves, in turn, c…