Particle transport through localized interactions with sharp magnetic field bends in MHD turbulence
M Lemoine - Journal of Plasma Physics, 2023 - cambridge.org
Particle transport through localized interactions with sharp magnetic field bends in MHD
turbulence Page 1 J. Plasma Phys. (2023), vol. 89, 175890501 © The Author(s), 2023 …
turbulence Page 1 J. Plasma Phys. (2023), vol. 89, 175890501 © The Author(s), 2023 …
Large-scale structure and turbulence transport in the inner solar wind: Comparison of Parker Solar Probe's first five orbits with a Global 3D Reynolds-averaged MHD …
Simulation results from a global magnetohydrodynamic model of the solar corona and solar
wind are compared with Parker Solar Probe (PSP) observations during its first five orbits …
wind are compared with Parker Solar Probe (PSP) observations during its first five orbits …
Pressure–strain interaction. II. Decomposition in magnetic field-aligned coordinates
PA Cassak, MH Barbhuiya, HA Weldon - Physics of Plasmas, 2022 - pubs.aip.org
In weakly collisional and collisionless magnetized plasmas, the pressure–strain interaction
describes the rate of conversion between bulk flow and thermal energy density. In this study …
describes the rate of conversion between bulk flow and thermal energy density. In this study …
Magnetic curvatures of a uniformly magnetized tesseroid using the Cartesian kernels
In recent years, the gravitational curvatures, the third-order derivatives of the gravitational
potential (GP), of a tesseroid have been introduced in the context of gravity field modeling …
potential (GP), of a tesseroid have been introduced in the context of gravity field modeling …
Discontinuity analysis of the leading switchback transition regions
Context. Magnetic switchbacks are magnetic structures characterized as intervals of sudden
reversal in the radial component of the pristine solar wind's magnetic field. Switchbacks …
reversal in the radial component of the pristine solar wind's magnetic field. Switchbacks …
First-order derivatives of principal and main invariants of magnetic gradient tensor of a uniformly magnetized tesseroid and spherical shell
Similar to the gravitational curvatures in the gravity field, the magnetic curvatures (ie, third-
order derivatives of the magnetic potential) have been recently proposed in the magnetic …
order derivatives of the magnetic potential) have been recently proposed in the magnetic …
Particle-in-cell Simulation of Energy Conversion at the Turbulent Region Downstream of the Reconnection Front
Y Yi, Y Pang, L Song, R Jin, X Deng - The Astrophysical Journal, 2023 - iopscience.iop.org
We study the energy conversion in the turbulent region (TR) downstream of the reconnection
front (RF) via 2.5 D particle-in-cell simulations. Our study shows that most magnetic energy …
front (RF) via 2.5 D particle-in-cell simulations. Our study shows that most magnetic energy …
Observations of magnetic field line curvature and its role in the space plasma turbulence
Recent numerical simulations of plasma turbulence showed that magnetic field line
curvature plays a key role in particle energization. Based on in situ high-resolution data …
curvature plays a key role in particle energization. Based on in situ high-resolution data …
Magnetic Energy Conversion in Magnetohydrodynamics: Curvature Relaxation and Perpendicular Expansion of Magnetic Fields
The mechanisms and pathways of magnetic energy conversion are an important subject for
many laboratory, space, and astrophysical systems. Here, we present a perspective on …
many laboratory, space, and astrophysical systems. Here, we present a perspective on …
Curvature of magnetic field and its role on plasma in turbulent magnetosheath
Y Ji, C Shen, N Ren, L Ma, YH Ma… - The Astrophysical …, 2022 - iopscience.iop.org
This study presents statistical features of magnetic field curvature in the magnetosheath
region. Two sets of high-quality field and plasma data measured by the Magnetospheric …
region. Two sets of high-quality field and plasma data measured by the Magnetospheric …