Multi-scale processes of the Kelvin-Helmholtz instability at Earth's magnetopause
The Kelvin-Helmholtz Instability (KHI) is a large scale convective instability which occurs
anywhere the velocity shear between two fluids is large, such as Earth's magnetopause …
anywhere the velocity shear between two fluids is large, such as Earth's magnetopause …
The three-fluid generalized Ohm's law: A theoretical study
The two-fluid generalized Ohm's law (GOL) is based on the assumption that plasma is
composed of only protons and electrons. The three-fluid GOL is obtained theoretically for the …
composed of only protons and electrons. The three-fluid GOL is obtained theoretically for the …
Kelvin–Helmholtz instability at mars: in situ observations and kinetic simulations
L Wang, C Huang, A Du, Y Ge, G Chen… - The Astrophysical …, 2023 - iopscience.iop.org
Kelvin–Helmholtz (KH) instability is a fundamental boundary instability between two fluids
with different speeds, exchanging the mass, momentum, and energy across the boundary …
with different speeds, exchanging the mass, momentum, and energy across the boundary …
Design and construction of a ground-based plasma device for Martian boundary layer investigation
Laboratory experiments have contributed significantly to the exploration of the fundamental
physics of Earth's and planetary space plasma. In this work, a ground-based plasma device …
physics of Earth's and planetary space plasma. In this work, a ground-based plasma device …
Intermittent plasma turbulence in the Martian plasma environment
Due to the absence of a global intrinsic magnetic field, Mars presents an induced
magnetosphere, which is formed by the interaction between the solar wind and the …
magnetosphere, which is formed by the interaction between the solar wind and the …
Ion loss within a reconnection exhaust near Mars: MAVEN observations
We present observations from Mars Atmosphere and Volatile EvolutioN of a reconnection
exhaust, which was probably not ongoing, in the Martian magnetosheath. The reconnection …
exhaust, which was probably not ongoing, in the Martian magnetosheath. The reconnection …
Solar control of the pickup ion plume in the dayside magnetosheath of Venus
Abstract Using the 8.5‐year Venus Express measurements, we demonstrate the asymmetric
plasma distributions in the Venusian magnetosheath. An escaping plume is formed by …
plasma distributions in the Venusian magnetosheath. An escaping plume is formed by …
Electron density variability in the day-side ionosphere of Mars: The role of gravity waves
ABSTRACT Mars Atmosphere and Volatile EvolutioN (MAVEN) has observed oscillations in
the density, velocity, and temperature of ionospheric plasma on Mars. Atmospheric gravity …
the density, velocity, and temperature of ionospheric plasma on Mars. Atmospheric gravity …
A linearized coupled model of acoustic-gravity waves and the lower ionosphere at Mars
Context. Highly variable ionospheric structures were recently detected on Mars using
spacecraft measurements. Acoustic-gravity waves (AGWs) could be the underlying …
spacecraft measurements. Acoustic-gravity waves (AGWs) could be the underlying …
A comparative study of ion beam and velocity shear driven resonant instability of kinetic Alfvén waves with κ-electrons
A comparative analysis is carried out between the ion beam and velocity shear as the
possible source of free energy in the generation of kinetic Alfvén waves (KAWs) through a …
possible source of free energy in the generation of kinetic Alfvén waves (KAWs) through a …