Estimates of Proton and Electron Heating Rates Extended to the Near-Sun Environment
R Bandyopadhyay, CM Meyer… - The Astrophysical …, 2023 - iopscience.iop.org
A central problem of space plasma physics is how protons and electrons are heated in a
turbulent, magnetized plasma. The differential heating of charged species due to dissipation …
turbulent, magnetized plasma. The differential heating of charged species due to dissipation …
Analytic Model and Magnetohydrodynamic Simulations of Three-dimensional Magnetic Switchbacks
Abstract Parker Solar Probe observations reveal that the near-Sun space is almost filled with
magnetic switchbacks (" switchbacks" hereinafter), which may be a major contributor to the …
magnetic switchbacks (" switchbacks" hereinafter), which may be a major contributor to the …
Solar Orbiter Observations of Proton and Alpha Particle Kinetic Signatures Related to the Presence of Switchbacks in the Inner Heliosphere: A Case Study
We investigate how ions, namely protons and alpha particles, kinetically react to the
presence of strong deflections in the magnetic field, the so-called switchbacks, in the first …
presence of strong deflections in the magnetic field, the so-called switchbacks, in the first …
Analytic model and MHD simulations of three-dimensional magnetic switchbacks
Parker Solar Probe observations reveal that the near-Sun space is almost filled with
magnetic switchbacks (``switchbacks''hereinafter), which may be a major contributor to the …
magnetic switchbacks (``switchbacks''hereinafter), which may be a major contributor to the …