Dayside transient phenomena and their impact on the magnetosphere and ionosphere
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 …
transfer events, and surface waves, are frequently observed upstream from the bow shock …
Whistler wave observations by Parker Solar Probe during encounter 1: Counter-propagating whistlers collocated with magnetic field inhomogeneities and their …
Observations of the young solar wind by the Parker Solar Probe (PSP) mission reveal the
existence of intense plasma wave bursts with frequencies between 0.05 and 0.20f ce (tens …
existence of intense plasma wave bursts with frequencies between 0.05 and 0.20f ce (tens …
Velocity-space Signatures of Resonant Energy Transfer between Whistler Waves and Electrons in the Earth's Magnetosheath
Wave–particle interactions play a crucial role in transferring energy between
electromagnetic fields and charged particles in space and astrophysical plasmas. Despite …
electromagnetic fields and charged particles in space and astrophysical plasmas. Despite …
Self-consistent kinetic model of nested electron-and ion-scale magnetic cavities in space plasmas
Abstract NASA's Magnetospheric Multi-Scale (MMS) mission is designed to explore the
proton-and electron-gyroscale kinetics of plasma turbulence where the bulk of particle …
proton-and electron-gyroscale kinetics of plasma turbulence where the bulk of particle …
Low-frequency whistler waves modulate electrons and generate higher-frequency whistler waves in the solar wind
The role of whistler-mode waves in the solar wind and the relationship between their
electromagnetic fields and charged particles is a fundamental question in space physics …
electromagnetic fields and charged particles is a fundamental question in space physics …
Generation of Subion Scale Magnetic Holes from Electron Shear Flow Instabilities in Plasma Turbulence
G Arrò, F Pucci, F Califano, ME Innocenti… - The Astrophysical …, 2023 - iopscience.iop.org
Magnetic holes (MHs) are coherent structures associated with strong magnetic field
depressions in magnetized plasmas. They are observed in many astrophysical …
depressions in magnetized plasmas. They are observed in many astrophysical …
Secondary Whistler and Ion-cyclotron Instabilities Driven by Mirror Modes in Galaxy Clusters
F Ley, EG Zweibel, D Miller… - The Astrophysical …, 2024 - iopscience.iop.org
Electron cyclotron waves (whistlers) are commonly observed in plasmas near Earth and the
solar wind. In the presence of nonlinear mirror modes, bursts of whistlers, usually called lion …
solar wind. In the presence of nonlinear mirror modes, bursts of whistlers, usually called lion …
On the origin of donut‐shaped electron distributions within magnetic cavities
Magnetic cavities, also known as magnetic holes, are ubiquitous in space plasmas
characterized by depressed magnetic strength and enhanced plasma pressure. Most of the …
characterized by depressed magnetic strength and enhanced plasma pressure. Most of the …
Whistler waves as a signature of converging magnetic holes in space plasmas
Magnetic holes are plasma structures that trap a large number of particles in a magnetic field
that is weaker than the field in its surroundings. The unprecedented high time-resolution …
that is weaker than the field in its surroundings. The unprecedented high time-resolution …
Kinetic generation of whistler waves in the turbulent magnetosheath
I Svenningsson, E Yordanova… - Geophysical …, 2022 - Wiley Online Library
The Earth's magnetosheath (MSH) is governed by numerous physical processes which
shape the particle velocity distributions and contribute to the heating of the plasma. Among …
shape the particle velocity distributions and contribute to the heating of the plasma. Among …