A Quasi-linear Diffusion Model for Resonant Wave–Particle Instability in Homogeneous Plasma
SY Jeong, D Verscharen, RT Wicks… - The Astrophysical …, 2020 - iopscience.iop.org
In this paper, we develop a model to describe the generalized wave–particle instability in a
quasi-neutral plasma. We analyze the quasi-linear diffusion equation for particles by …
quasi-neutral plasma. We analyze the quasi-linear diffusion equation for particles by …
Effect of geomagnetic storms on a power network at mid latitudes
Solar activities may disturb the geomagnetic field and impact the power grid via
geomagnetically induced currents. We study active and reactive powers as well as the …
geomagnetically induced currents. We study active and reactive powers as well as the …
Complex network for solar protons and correlations with flares
We study the properties of the complex network for solar proton flux (SPF) at six integral
energy channels (> 1,> 5,> 10,> 30,> 50, and> 100 MeV). We construct a growing visibility …
energy channels (> 1,> 5,> 10,> 30,> 50, and> 100 MeV). We construct a growing visibility …
BO-KM: A comprehensive solver for dispersion relation of obliquely propagating waves in magnetized multi-species plasma with anisotropic drift kappa-Maxwellian …
W Bai, H Xie, C Wu, Y Pu, P Yu - Computer Physics Communications, 2025 - Elsevier
The observation of superthermal plasma distributions in space reveals a multitude of
distributions with high-energy tails, and the kappa-Maxwellian distribution is a type of non …
distributions with high-energy tails, and the kappa-Maxwellian distribution is a type of non …
Electromagnetic Instability in Plasma with Kappa Distribution Function in the Presence of Coulomb Collision
F Nejadtaghi, M Mahdavi, S Hassan Pour… - Iranian Journal of …, 2024 - ijaa.du.ac.ir
In this research, an analytical expression of the Weibel electromagnetic instability growth
rate is investigated for strongly coupled plasma in the presence of Coulomb collisions in the …
rate is investigated for strongly coupled plasma in the presence of Coulomb collisions in the …
Periodic behavior of fast small-scale brightening on the solar disk
S Zeighami, E Tavabi, E Amirkhanlou - Iranian Journal of …, 2024 - ijgeophysics.ir
A distinct difference is seen between different parts of the solar chromosphere, including the
bright points (BPs) at the boundary and within the network, and the darker regions formed …
bright points (BPs) at the boundary and within the network, and the darker regions formed …
Periodic behavior of fast small-scale brightening on the solar disk
S Zeighami, E Tavabi, E Amirkhanlou - Iranian Journal of …, 2024 - ijgeophysics.ir
A distinct difference is seen between different parts of the solar chromosphere, including the
bright points (BPs) at the boundary and within the network, and the darker regions formed …
bright points (BPs) at the boundary and within the network, and the darker regions formed …