On the relationship between shear Alfven waves, auroral electron acceleration, and field line resonances
This article describes the relationship between shear Alfvén waves and auroral electron
acceleration, with an emphasis on long-period standing waves that correlate with redline …
acceleration, with an emphasis on long-period standing waves that correlate with redline …
Kinetic theory of the Alfvén wave acceleration of auroral electrons
RL Lysak, Y Song - Journal of Geophysical Research: Space …, 2003 - Wiley Online Library
Recent observations have indicated that in addition to the classical “inverted‐V” type
electron acceleration, auroral electrons often have a field‐aligned distribution that is broad …
electron acceleration, auroral electrons often have a field‐aligned distribution that is broad …
Collisionless reconnection: Effects of Hall current and electron pressure gradient
X Wang, A Bhattacharjee, ZW Ma - Journal of Geophysical …, 2000 - Wiley Online Library
An analytical treatment is given of two‐dimensional, quasi‐steady collisionless reconnection
on the basis of the generalized Ohm's law, including the effects of the Hall current and scalar …
on the basis of the generalized Ohm's law, including the effects of the Hall current and scalar …
Coupling between density structures, electromagnetic waves and ionospheric feedback in the auroral zone
AV Streltsov, W Lotko - Journal of Geophysical Research …, 2008 - Wiley Online Library
This paper presents results from a numerical study of nonlinear interactions between ultra‐
low‐frequency (ULF) electromagnetic waves and the magnetospheric‐ionospheric plasma …
low‐frequency (ULF) electromagnetic waves and the magnetospheric‐ionospheric plasma …
Shear Alfvén waves on stretched magnetic field lines near midnight in Earth's magnetosphere
The spectrum of toroidal standing shear Alfvén waves (SAWs) is derived for a stretched
magnetic field line geometry that is approximated by the Tsyganenko 96 magnetic field …
magnetic field line geometry that is approximated by the Tsyganenko 96 magnetic field …
Finite element modeling of nonlinear dispersive field line resonances: Trapped shear Alfvén waves inside field‐aligned density structures
Using a new two‐dimensional nonlinear finite element model, we investigate the interaction
of dispersive shear Alfvén wave (SAW) field line resonances (FLRs) and ion acoustic waves …
of dispersive shear Alfvén wave (SAW) field line resonances (FLRs) and ion acoustic waves …
Numerical study of the influence of electron inertial effects and electron dynamics on tearing mode instability
B Shi, J Wang, D Liu, Z Ma - Plasma Physics and Controlled …, 2024 - iopscience.iop.org
The tearing mode instabilities were numerically studied in two distinct models: the finite
electron inertial magnetohydrodynamics (MHD) and the electron MHD (EMHD). The finite …
electron inertial magnetohydrodynamics (MHD) and the electron MHD (EMHD). The finite …
Ionospheric cusp flows pulsed by solar wind Alfvén waves
P Prikryl, G Provan, KA McWilliams… - Annales …, 2002 - angeo.copernicus.org
Pulsed ionospheric flows (PIFs) in the cusp foot-print have been observed by the
SuperDARN radars with periods between a few minutes and several tens of minutes. PIFs …
SuperDARN radars with periods between a few minutes and several tens of minutes. PIFs …
MHD field line resonances and global modes in three‐dimensional magnetic fields
CZ Cheng - Journal of Geophysical Research: Space Physics, 2003 - Wiley Online Library
By assuming a general isotropic pressure distribution P= P (ψ, α), where ψ and α are three‐
dimensional scalar functions labeling the field lines with B=∇ ψ×∇ α, we have derived a set …
dimensional scalar functions labeling the field lines with B=∇ ψ×∇ α, we have derived a set …
Nonlinear acceleration of dispersive effects in field line resonances
Nonlinear dynamics of a dispersive field line resonance (FLR) is investigated in a dipolar
magnetic geometry using a new finite element code TOPO. Time dependent dispersion and …
magnetic geometry using a new finite element code TOPO. Time dependent dispersion and …