Dayside transient phenomena and their impact on the magnetosphere and ionosphere

H Zhang, Q Zong, H Connor, P Delamere… - Space Science …, 2022 - Springer
Dayside transients, such as hot flow anomalies, foreshock bubbles, magnetosheath jets, flux
transfer events, and surface waves, are frequently observed upstream from the bow shock …

Simultaneous macroscale and microscale wave–ion interaction in near-earth space plasmas

ZY Liu, QG Zong, R Rankin, H Zhang, YF Wang… - Nature …, 2022 - nature.com
Identifying how energy transfer proceeds from macroscales down to microscales in
collisionless plasmas is at the forefront of astrophysics and space physics. It provides …

Global propagation of magnetospheric Pc5 ULF waves driven by foreshock transients

B Wang, T Liu, Y Nishimura, H Zhang… - Journal of …, 2020 - Wiley Online Library
Abstract Pc5 (2–7 mHz) ultralow frequency (ULF) waves play a significant role in resonating
with particles and transferring energy in the coupled magnetospheric and ionospheric …

Energy modulations of magnetospheric ions induced by foreshock transient‐driven ultralow‐frequency waves

B Wang, H Zhang, Z Liu, T Liu, X Li… - Geophysical …, 2021 - Wiley Online Library
Although foreshock transients can generate strong magnetospheric Pc5 ultralow‐frequency
(ULF) waves, whether they can modulate the energy of magnetospheric ions is still poorly …

Ionospheric oxygen outflows directly injected into the inner magnetosphere: Van Allen Probes statistics

ZY Liu, QG Zong - Journal of Geophysical Research: Space …, 2022 - Wiley Online Library
Ionospheric oxygen outflows (IOOs) are frequently observed in Earth's inner
magnetosphere. As a potential fast mass source of the inner magnetosphere, they have …

Global ULF waves excited by solar wind dynamic pressure impulses: 1. Timescales and geomagnetic activity dependence

ZK Xie, QG Zong, J Ren, C Yue, ZY Liu… - Journal of …, 2023 - Wiley Online Library
Solar wind dynamic pressure pulse is one of the sources of ultra‐low frequency (ULF)
waves. Based on 1‐second resolution magnetic field observations from SuperMAG from …

Magnetospheric response to solar wind forcing: ultra-low-frequency wave–particle interaction perspective

Q Zong - Annales geophysicae, 2022 - angeo.copernicus.org
Solar wind forcing, eg, interplanetary shock and/or solar wind dynamic pressure pulses
impacting Earth's magnetosphere, manifests many fundamental important space physics …

Global ULF waves excited by solar wind dynamic pressure impulses: 2. The spatial distribution asymmetry

ZK Xie, QG Zong, J Ren, C Yue, ZY Liu… - Journal of …, 2023 - Wiley Online Library
Asymmetry is a prevalent characteristic in numerous space physics phenomena. In this
study, we investigate the statistical properties and spatial variations of ultra‐low frequency …

Comparative study of dayside pulsating auroras induced by ultralow-frequency waves

XY Li, QG Zong, JJ Liu, ZF Yin, ZJ Hu, XZ Zhou, C Yue… - Universe, 2023 - mdpi.com
Pulsating auroras are usually observed with ultralow-frequency (ULF) waves in the Pc 3–5
band (period 10–600 s). These auroras are thought to result from interactions between …

Van Allen Probes observations of symmetric stormtime compressional ULF waves

K Takahashi, C Crabtree, AY Ukhorskiy… - Journal of …, 2022 - Wiley Online Library
Previous spacecraft studies showed that stormtime poloidal ultralow‐frequency (ULF) waves
in the ring current region have an antisymmetric (second harmonic) mode structure about …