| Full text | |
| Author(s): |
Total Authors: 3
|
| Affiliation: | [1] INPE. Pós-graduação em Computação Aplicada - Brasil
[2] INPE. Laboratório Associado de Computação e Matemática Aplicada - Brasil
[3] INPE. Divisão de Geofísica Espacial - Brasil
Total Affiliations: 3
|
| Document type: | Journal article |
| Source: | TEMA (São Carlos); v. 18, n. 2, p. 317-333, 2017-08-00. |
| Abstract | |
ABSTRACT This work is concerned with the numerical simulation of the Kelvin-Helmholtz instability using an ideal and resistive two-dimensional magnetohydrodynamics model in the context of an adaptive multiresolution approach. The Kelvin-Helmholtz instabilities are caused by a velocity shear and normally expected in a layer between two fluids with different velocities. Due to its complexity, this kind of problem is a well-known test for numerical schemes and it is important for the verification of the developed code. The aim of this paper is to verify the implemented numerical model with the well-known astrophysics FLASH code. (AU) | |
| FAPESP's process: | 15/50403-0 - Ralf Deiterding | University Southampton - Inglaterra |
| Grantee: | Margarete Oliveira Domingues |
| Support Opportunities: | Research Grants - Visiting Researcher Grant - International |
| FAPESP's process: | 16/50016-9 - Advanced criteria for dynamic mesh adaption in computacional space weather forecasting |
| Grantee: | Margarete Oliveira Domingues |
| Support Opportunities: | Regular Research Grants |
| FAPESP's process: | 15/25624-2 - Development of multiscale modelling for non-linear local plasma instabilities of Astrophysics and Space Geophysics |
| Grantee: | Margarete Oliveira Domingues |
| Support Opportunities: | Regular Research Grants |