Dynamical response of the solar corona. III - Numerical simulation of the 1973 June 10 coronal transient

1977 ◽  
Vol 215 ◽  
pp. 345 ◽  
Author(s):  
R. S. Steinolfson ◽  
Y. Nakagawa
Keyword(s):  
Numerical Simulation ◽  
Solar Corona ◽  
Dynamical Response ◽  
Coronal Transient

Dynamical Response of the Solar Corona. II. Numerical Simulations Near the Sun

1976 ◽  
Vol 207 ◽  
pp. 300 ◽  
Author(s):  
Richard S. Steinolfson ◽  
Yoshinari Nakagawa
Keyword(s):  
Solar Corona ◽  
Numerical Simulations ◽  
Dynamical Response ◽  
The Sun

Numerical Simulation of Response of Explosion Ground Shock to Buried Gas Pipeline

2013 ◽  
Vol 448-453 ◽  
pp. 3970-3974
Author(s):  
Xiao Fei Jing ◽  
Zhi Yong Cai ◽  
Ke Hui Liu
Keyword(s):  
Numerical Simulation ◽  
Simulation Method ◽  
Dynamical Theory ◽  
Gas Pipeline ◽  
Underground Explosion ◽  
Dynamical Response ◽  
Finite Element Program ◽  
Element Program ◽  
Ground Shock ◽  
Buried Gas Pipeline

In this paper, by using nonlinear dynamical theory and Arbitrary Lagrange Eulerian (ALE) algorithm in LS-DYNA 3D finite element program, a method of numerical simulation is used to study dynamical response of buried gas pipeline underground shock wave of underground explosion. The simulation results shows that it is feasible for the numerical simulation method in this paper to study dynamical response of buried pipelines underground shock waves from explosion. the conclusion in this paper may provide significant reference for the risk evaluation and disaster prevention of buried gas pipeline.

Numerical Simulation of Twisted Solar Corona

1998 ◽  
pp. 467-468 ◽  
Author(s):  
S. Parhi ◽  
B. P. Pandey ◽  
M. Goossens ◽  
G. S. Lakhina
Keyword(s):  
Numerical Simulation ◽  
Solar Corona

Numerical simulation and dynamical response of a moored hydrokinetic turbine operating in the wake of an upstream turbine for control design

2017 ◽  
Vol 114 ◽  
pp. 1134-1145 ◽  
Author(s):  
Parakram Pyakurel ◽  
James H. VanZwieten ◽  
Cornel Sultan ◽  
Manhar Dhanak ◽  
Nikolaos I. Xiros
Keyword(s):  
Numerical Simulation ◽  
Control Design ◽  
Dynamical Response ◽  
Hydrokinetic Turbine

NUMERICAL SIMULATION OF FAST-MODE MAGNETOSONIC WAVES EXCITED BY PLASMOID EJECTIONS IN THE SOLAR CORONA

2015 ◽  
Vol 800 (2) ◽  
pp. 111 ◽  
Author(s):  
Liping Yang ◽  
Lei Zhang ◽  
Jiansen He ◽  
Hardi Peter ◽  
Chuanyi Tu ◽  
...  
Keyword(s):  
Numerical Simulation ◽  
Solar Corona ◽  
Fast Mode

A numerical simulation of the 3-D structure of solar corona in May 1998

2002 ◽  
Vol 26 (2) ◽  
pp. 198-207
Author(s):  
Zhan-yin Ye ◽  
Feng-si Wei ◽  
Xue-shang Feng ◽  
Yong Shi ◽  
Jiu-sheng Yao
Keyword(s):  
Numerical Simulation ◽  
Solar Corona

scholarly journals Numerical Simulation of Twisted Solar Corona

1998 ◽  
Vol 185 ◽  
pp. 467-468
Author(s):  
S. Parhi ◽  
B.P. Pandey ◽  
M. Goossens ◽  
G.S. Lakhina
Keyword(s):  
Numerical Simulation ◽  
Wave Propagation ◽  
Solar Corona ◽  
Temperature Profile ◽  
Resonant Absorption ◽  
Wave Generation ◽  
Coronal Plasma ◽  
Mhd Waves ◽  
Coronal Temperature ◽  
Physical Picture

The solar corona supports a variety of waves generated by convective upwelling motion in the photosphere. In order to explain the observed coronal temperature profile, resonant absorption of MHD waves by coronal plasma (Goossens et al, 1995) has been proposed as a possible candidate. The physical picture is that the footpoint motion in the photosphere constantly stirs the coronal plasma leading to the MHD wave generation which is then resonantly absorbed producing the enhanced heating of the corona. Here we consider the problem of MHD wave propagation in a twisted solar corona.

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