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 …
Investigating Mercury's environment with the two-spacecraft BepiColombo mission
A Milillo, M Fujimoto, G Murakami, J Benkhoff… - Space science …, 2020 - Springer
Abstract The ESA-JAXA BepiColombo mission will provide simultaneous measurements
from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric …
from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric …
Reconnection-driven particle acceleration in relativistic shear flows
Particle energization in shear flows is invoked to explain nonthermal emission from the
boundaries of relativistic astrophysical jets. Yet the physics of particle injection, ie, the …
boundaries of relativistic astrophysical jets. Yet the physics of particle injection, ie, the …
Cross-scale processes of magnetic reconnection
KJ Hwang, R Nakamura, JP Eastwood… - Space Science …, 2023 - Springer
Various physical processes in association with magnetic reconnection occur over multiple
scales from the microscopic to macroscopic scale lengths. This paper reviews multi-scale …
scales from the microscopic to macroscopic scale lengths. This paper reviews multi-scale …
Characteristics of the flank magnetopause: THEMIS observations
S Haaland, A Runov, A Artemyev… - Journal of …, 2019 - Wiley Online Library
The terrestrial magnetopause is the boundary that shields the Earth's magnetosphere on
one side from the shocked solar wind and its embedded interplanetary magnetic field on the …
one side from the shocked solar wind and its embedded interplanetary magnetic field on the …
On the growth and development of non‐linear Kelvin–Helmholtz instability at mars: Maven observations
In this study, we have analyzed Mars Atmosphere and Volatile EvolutioN (MAVEN)
observations of fields and plasma signatures associated with an encounter of fully …
observations of fields and plasma signatures associated with an encounter of fully …
Effects of fluctuating magnetic field on the growth of the Kelvin‐Helmholtz instability at the Earth's magnetopause
TKM Nakamura, JE Stawarz… - Journal of …, 2020 - Wiley Online Library
At the Earth's magnetopause, the Kelvin‐Helmholtz (KH) instability, driven by the persistent
velocity shear between the magnetosheath and the magnetosphere, has been frequently …
velocity shear between the magnetosheath and the magnetosphere, has been frequently …
Satellite data‐based 3‐D simulation of Kelvin‐Helmholtz instability and induced magnetic reconnection at the Earth's magnetopause
M Sisti, M Faganello, F Califano… - Geophysical Research …, 2019 - Wiley Online Library
We present a 3‐D two‐fluid simulation using plasma parameters as measured by MMS on 8
September 2015 concerning the nonlinear development of the Kelvin‐Helmholtz instability …
September 2015 concerning the nonlinear development of the Kelvin‐Helmholtz instability …
MMS observations of double mid-latitude reconnection ion beams in the early non-linear phase of the Kelvin-Helmholtz instability
The MMS satellites encountered a Kelvin-Helmholtz instability (KHI) period in the early non-
linear phase at the post-noon flank magnetopause on 8 Sep 2015. The adjacent …
linear phase at the post-noon flank magnetopause on 8 Sep 2015. The adjacent …
Generation of turbulence in Kelvin‐Helmholtz vortices at the Earth's magnetopause: Magnetospheric Multiscale observations
H Hasegawa, TKM Nakamura… - Journal of …, 2020 - Wiley Online Library
Abstract The Kelvin‐Helmholtz instability (KHI) at Earth's magnetopause and associated
turbulence are suggested to play a role in the transport of mass and momentum from the …
turbulence are suggested to play a role in the transport of mass and momentum from the …