Three-dimensional global MHD simulation code for the Earth's magnetosphere using HPF/JA

2002 ◽  
Vol 14 (8-9) ◽  
pp. 631-646 ◽  
Author(s):  
Tatsuki Ogino
Keyword(s):  
Three Dimensional ◽  
Simulation Code ◽  
Mhd Simulation ◽  
Earth’S Magnetosphere ◽  
Earth's Magnetosphere ◽  
Global Mhd Simulation

scholarly journals Real-time global MHD simulation of the solar wind interaction with the earth’s magnetosphere

2008 ◽  
Vol 42 (9) ◽  
pp. 1504-1509 ◽  
Author(s):  
H. Shimazu ◽  
K. Kitamura ◽  
T. Tanaka ◽  
S. Fujita ◽  
M.S. Nakamura ◽  
...  
Keyword(s):  
Solar Wind ◽  
Real Time ◽  
Solar Wind Interaction ◽  
Mhd Simulation ◽  
Earth’S Magnetosphere ◽  
Earth's Magnetosphere ◽  
Global Mhd Simulation

scholarly journals One year in the Earth's magnetosphere: A global MHD simulation and spacecraft measurements

Space Weather ◽  
2016 ◽  
Vol 14 (5) ◽  
pp. 351-367 ◽  
Author(s):  
G. Facskó ◽  
I. Honkonen ◽  
T. Živković ◽  
L. Palin ◽  
E. Kallio ◽  
...  
Keyword(s):  
Mhd Simulation ◽  
Earth’S Magnetosphere ◽  
Earth's Magnetosphere ◽  
Global Mhd Simulation ◽  
One Year

A three-dimensional high Mach number asymmetric magnetopause model from global MHD simulation

2015 ◽  
Vol 120 (7) ◽  
pp. 5645-5666 ◽  
Author(s):  
Z.-Q. Liu ◽  
J. Y. Lu ◽  
C. Wang ◽  
K. Kabin ◽  
J. S. Zhao ◽  
...  
Keyword(s):  
Mach Number ◽  
Three Dimensional ◽  
Mhd Simulation ◽  
High Mach Number ◽  
Global Mhd Simulation ◽  
High Mach

scholarly journals Magnetized Kelvin–Helmholtz instability: theory and simulations in the Earth’s magnetosphere context

2017 ◽  
Vol 83 (6) ◽  
Author(s):  
Matteo Faganello ◽  
Francesco Califano
Keyword(s):  
Three Dimensional ◽  
Solar Wind Plasma ◽  
Helmholtz Instability ◽  
Earth’S Magnetosphere ◽  
Instability Theory ◽  
Earth's Magnetosphere ◽  
Long Time ◽  
Weak Points ◽  
The Rich

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.

Sign in / Sign up

Export Citation Format

Share Document