Dayside transient phenomena and their impact on the magnetosphere and ionosphere
Dayside transients, such as hot flow anomalies, foreshock bubbles, magnetosheath jets, flux
transfer events, and surface waves, are frequently observed upstream from the bow shock …
transfer events, and surface waves, are frequently observed upstream from the bow shock …
Complex systems methods characterizing nonlinear processes in the near-earth electromagnetic environment: Recent advances and open challenges
G Balasis, MA Balikhin, SC Chapman… - Space Science …, 2023 - Springer
Learning from successful applications of methods originating in statistical mechanics,
complex systems science, or information theory in one scientific field (eg, atmospheric …
complex systems science, or information theory in one scientific field (eg, atmospheric …
Atmospheric escape processes and planetary atmospheric evolution
The habitability of the surface of any planet is determined by a complex evolution of its
interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive …
interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive …
Bifurcation, chaotic and multistability analysis of the -dimensional elliptic nonlinear Schrödinger equation with external perturbation
S Samina, A Jhangeer, Z Chen - Waves in Random and Complex …, 2022 - Taylor & Francis
This paper presents a theory of weakly nonlinear wave propagation in superposed fluids in
the existence of magnetic fields. The extended direct algebraic approach has been utilized …
the existence of magnetic fields. The extended direct algebraic approach has been utilized …
Information theoretical approach to discovering solar wind drivers of the outer radiation belt
The solar wind‐magnetosphere system is nonlinear. The solar wind drivers of
geosynchronous electrons with energy range of 1.8–3.5 MeV are investigated using mutual …
geosynchronous electrons with energy range of 1.8–3.5 MeV are investigated using mutual …
Polarization and spatial distribution features of Pc4 and Pc5 waves in the magnetosphere
Ultra‐low frequency waves interact with different particle populations all over the
magnetosphere. Some interaction mechanisms are associated with certain wave modes, but …
magnetosphere. Some interaction mechanisms are associated with certain wave modes, but …
Review of solar wind entry into and transport within the plasma sheet
The plasma sheet is populated in part by the solar wind plasma. Four solar entry
mechanisms are examined:(1) double cusp or double lobe reconnection,(2) Kelvin …
mechanisms are examined:(1) double cusp or double lobe reconnection,(2) Kelvin …
Plasma transport driven by the three‐dimensional Kelvin‐Helmholtz instability
X Ma, P Delamere, A Otto… - Journal of Geophysical …, 2017 - Wiley Online Library
It has been well demonstrated that the nonlinear Kelvin‐Helmholtz (KH) instability plays a
critical role for the solar wind interaction with the Earth's magnetosphere. Although the two …
critical role for the solar wind interaction with the Earth's magnetosphere. Although the two …
Untangling the solar wind and magnetospheric drivers of the radiation belt electrons
Many solar wind parameters correlate with one another, which complicates the causal‐effect
studies of solar wind driving of the magnetosphere. Conditional mutual information (CMI) is …
studies of solar wind driving of the magnetosphere. Conditional mutual information (CMI) is …
Magnetized Kelvin–Helmholtz instability: theory and simulations in the Earth's magnetosphere context
M Faganello, F Califano - Journal of Plasma Physics, 2017 - cambridge.org
The Kelvin–Helmholtz instability, proposed a long time ago for its role in and impact on the
transport properties at magnetospheric flanks, has been widely investigated in the Earth's …
transport properties at magnetospheric flanks, has been widely investigated in the Earth's …