%0 Journal Article
%4 sid.inpe.br/mtc-m21b/2017/11.30.16.09
%2 sid.inpe.br/mtc-m21b/2017/11.30.16.09.58
%@doi 10.5540/tema.2017.018.02.0317
%@issn 1677-1966
%T Ideal and resistive magnetohydrodynamic two-dimensional simulation of the Kelvin-Helmholtz instability in the context of adaptive multiresolution analysis
%D 2017
%9 journal article
%A Gomes, Ana Karina Fontes,
%A Domingues, Margarete Oliveira,
%A Mendes Júnior, Odim,
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@electronicmailaddress annakfg@gmail.com
%@electronicmailaddress margarete.domingues@inpe.br
%@electronicmailaddress odim.mendes@inpe.br
%B Tema: Tendências em Matemática Aplicada e Computacional
%V 18
%N 2
%P 317-333
%K magnetohydrodynamics, Kelvin-Helmholtz instability, adaptive multiresolution analysis, numerical simulation, scientific computing.
%X This work is concerned with the numerical simulation of the KelvinHelmholtz 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.
%@language en
%3 gomes_ideal.pdf