A time dependent three-dimensional simulation of the Earth's magnetosphere: Reconnection events

1982 ◽  
Vol 87 (A8) ◽  
pp. 6098 ◽  
Author(s):  
Stephen H. Brecht ◽  
John G. Lyon ◽  
Joel A. Fedder ◽  
K. Hain
Materials ◽  
2020 ◽  
Vol 13 (13) ◽  
pp. 3033
Author(s):  
Devashish Pandey ◽  
Xavier Oriols ◽  
Guillermo Albareda

The so-called Born–Huang ansatz is a fundamental tool in the context of ab-initio molecular dynamics, viz., it allows effectively separating fast and slow degrees of freedom and thus treating electrons and nuclei with different mathematical footings. Here, we consider the use of a Born–Huang-like expansion of the three-dimensional time-dependent Schrödinger equation to separate transport and confinement degrees of freedom in electron transport problems that involve geometrical constrictions. The resulting scheme consists of an eigenstate problem for the confinement degrees of freedom (in the transverse direction) whose solution constitutes the input for the propagation of a set of coupled one-dimensional equations of motion for the transport degree of freedom (in the longitudinal direction). This technique achieves quantitative accuracy using an order less computational resources than the full dimensional simulation for a typical two-dimensional geometrical constriction and upto three orders for three-dimensional constriction.


2017 ◽  
Vol 83 (6) ◽  
Author(s):  
Matteo Faganello ◽  
Francesco Califano

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 magnetosphere context. This review covers more than fifty years of theoretical and numerical efforts in investigating the evolution of Kelvin–Helmholtz vortices and how the rich nonlinear dynamics they drive allow solar wind plasma bubbles to enter into the magnetosphere. Special care is devoted to pointing out the main advantages and weak points of the different plasma models that can be adopted for describing the collisionless magnetospheric medium and in underlying the important role of the three-dimensional geometry of the system.


2009 ◽  
Vol 102 (24) ◽  
Author(s):  
P. J. M. van der Slot ◽  
H. P. Freund ◽  
W. H. Miner Jr. ◽  
S. V. Benson ◽  
M. Shinn ◽  
...  

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