Add to ORKGModeling extreme ‘Carrington-type ’ space weather events using three-dimensional global MHD simulation
Abstract—Taking advantage of the advent of massively parallel computers, sophisticated solution-adap...
We numerically model the coronal mass ejection (CME) event of 2003 October 28 that erupted from AR 1...
We present 3D global MHD simulations of proto-planetary disks calculated with the ZeusMP code. We fo...
Magnetohydrodynamics (MHD) provides an approximate description of agreat variety of processes in spa...
Data of 3D MHD Simulation for manuscript "An almost complete disappearance of open-flux polar cap fo...
Toward the integrated numerical space weather prediction, we have been developing a three dimensiona...
Toward the integrated numerical space weather prediction, we have been developing a three dimensiona...
This is the final report of our NASA AISRP grant entitled 'High Performance Parallel Methods for Spa...
Geomagnetic perturbation is an important aspect to determine the capability of a 3-D MHD model in pr...
MHD data was used in the paper "Identifying and Visualizing Terrestrial Magnetospheric Topology usin...
Abstract—A 3-D parallel adaptive mesh refinement (AMR) scheme is described for solving the partial-d...
Context. The numerical simulation of turbulence and flows in almost ideal, large-Reynolds-number ast...
In the solar coronal numerical simulation, the coronal heating/acceleration and the magnetic diverge...
We numericallymodel the coronalmass ejection (CME) event of 2003October 28 that erupted fromAR 10486...
A fully three-dimensional (3D), time-dependent, MHD interplanetary global model (3D IGM) has been us...
Abstract—Taking advantage of the advent of massively parallel computers, sophisticated solution-adap...
We numerically model the coronal mass ejection (CME) event of 2003 October 28 that erupted from AR 1...
We present 3D global MHD simulations of proto-planetary disks calculated with the ZeusMP code. We fo...
Magnetohydrodynamics (MHD) provides an approximate description of agreat variety of processes in spa...
Data of 3D MHD Simulation for manuscript "An almost complete disappearance of open-flux polar cap fo...
Toward the integrated numerical space weather prediction, we have been developing a three dimensiona...
Toward the integrated numerical space weather prediction, we have been developing a three dimensiona...
This is the final report of our NASA AISRP grant entitled 'High Performance Parallel Methods for Spa...
Geomagnetic perturbation is an important aspect to determine the capability of a 3-D MHD model in pr...
MHD data was used in the paper "Identifying and Visualizing Terrestrial Magnetospheric Topology usin...
Abstract—A 3-D parallel adaptive mesh refinement (AMR) scheme is described for solving the partial-d...
Context. The numerical simulation of turbulence and flows in almost ideal, large-Reynolds-number ast...
In the solar coronal numerical simulation, the coronal heating/acceleration and the magnetic diverge...
We numericallymodel the coronalmass ejection (CME) event of 2003October 28 that erupted fromAR 10486...
A fully three-dimensional (3D), time-dependent, MHD interplanetary global model (3D IGM) has been us...
Abstract—Taking advantage of the advent of massively parallel computers, sophisticated solution-adap...
We numerically model the coronal mass ejection (CME) event of 2003 October 28 that erupted from AR 1...
We present 3D global MHD simulations of proto-planetary disks calculated with the ZeusMP code. We fo...