Quasi-parallel Antisunward-propagating Whistler Waves Associated with the Electron Deficit in the Near-Sun Solar Wind: Particle-in-cell Simulation
In situ observations of the solar wind have shown that the electron velocity distribution function (VDF) consists of a quasi-Maxwellian core, comprising most of the electron population, and two sparser components: the halo, which are suprathermal and quasi-isotropic electrons, and an escaping beam p...
Saved in:
Main Authors: | Alfredo Micera, Daniel Verscharen, Jesse T. Coburn, Maria Elena Innocenti |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ada3d7 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Autogenous Electron Acceleration by Ion Flow Vortex in Space Plasmas
by: C. M. Liu, et al.
Published: (2025-01-01) -
Extreme Heating of Minor Ions in Imbalanced Solar-wind Turbulence
by: Michael F. Zhang, et al.
Published: (2025-01-01) -
Collisionless Tearing Instability in Relativistic Nonthermal Pair Plasma and Its Application to MHD Turbulence
by: Ivan Demidov, et al.
Published: (2025-01-01) -
Tearing-mediated Alfvénic Turbulence in a Relativistic Plasma
by: Stanislav Boldyrev, et al.
Published: (2025-01-01) -
Pressure-anisotropy-mediated Helical Dynamo in Turbulent Collisionless Plasmas
by: Z. H. Zhao, et al.
Published: (2025-01-01)