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The multi-scale nature of the solar wind
D Verscharen, KG Klein, BA Maruca - Living reviews in solar physics, 2019 - Springer
The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …
associated with its characteristic spatial and temporal scales. The characteristic length …
Recent progress in astrophysical plasma turbulence from solar wind observations
CHK Chen - Journal of Plasma Physics, 2016 - cambridge.org
This paper summarises some of the recent progress that has been made in understanding
astrophysical plasma turbulence in the solar wind, from in situ spacecraft observations. At …
astrophysical plasma turbulence in the solar wind, from in situ spacecraft observations. At …
HelioSwarm: a multipoint, multiscale mission to characterize turbulence
KG Klein, H Spence, O Alexandrova, M Argall… - Space Science …, 2023 - Springer
HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division
designed to explore the dynamic three-dimensional mechanisms controlling the physics of …
designed to explore the dynamic three-dimensional mechanisms controlling the physics of …
The solar orbiter magnetometer
TS Horbury, H O'brien, IC Blazquez, M Bendyk… - Astronomy & …, 2020 - aanda.org
The magnetometer instrument on the Solar Orbiter mission is designed to measure the
magnetic field local to the spacecraft continuously for the entire mission duration. The need …
magnetic field local to the spacecraft continuously for the entire mission duration. The need …
A Quarter Century of Wind Spacecraft Discoveries
LB Wilson III, AL Brosius, N Gopalswamy… - 2021 - Wiley Online Library
The Wind spacecraft, launched on November 1, 1994, is a critical element in NASA's
Heliophysics System Observatory (HSO)—a fleet of spacecraft created to understand the …
Heliophysics System Observatory (HSO)—a fleet of spacecraft created to understand the …
Electron-driven instabilities in the solar wind
D Verscharen, BDG Chandran, E Boella… - Frontiers in Astronomy …, 2022 - frontiersin.org
The electrons are an essential particle species in the solar wind. They often exhibit non-
equilibrium features in their velocity distribution function. These include temperature …
equilibrium features in their velocity distribution function. These include temperature …
Majority of solar wind intervals support ion-driven instabilities
KG Klein, BL Alterman, ML Stevens, D Vech… - Physical review …, 2018 - APS
We perform a statistical assessment of solar wind stability at 1 AU against ion sources of free
energy using Nyquist's instability criterion. In contrast to typically employed threshold models …
energy using Nyquist's instability criterion. In contrast to typically employed threshold models …
The variable source of the plasma sheet during a geomagnetic storm
LM Kistler, K Asamura, S Kasahara, Y Miyoshi… - Nature …, 2023 - nature.com
Both solar wind and ionospheric sources contribute to the magnetotail plasma sheet, but
how their contribution changes during a geomagnetic storm is an open question. The source …
how their contribution changes during a geomagnetic storm is an open question. The source …
Electron–ion heating partition in imbalanced solar-wind turbulence
A likely candidate mechanism to heat the solar corona and solar wind is low-frequency"
Alfvénic" turbulence sourced by magnetic fluctuations near the solar surface. Depending on …
Alfvénic" turbulence sourced by magnetic fluctuations near the solar surface. Depending on …
Pressure anisotropy and viscous heating in weakly collisional plasma turbulence
J Squire, MW Kunz, L Arzamasskiy… - Journal of Plasma …, 2023 - cambridge.org
Pressure anisotropy can strongly influence the dynamics of weakly collisional, high-beta
plasmas, but its effects are missed by standard magnetohydrodynamics (MHD). Small …
plasmas, but its effects are missed by standard magnetohydrodynamics (MHD). Small …