arrow
返回

Ambipolar diffusion: Self-similar solutions and MHD code testing

delete2022-06-10
delete3
delete
OA
AI
D
Daniel Nóbrega-Siverio
E
E. R. Priest
A
A. W. Hood
DOI:10.1051/0004-6361/202141449delete
delete原文链接
delete原文求助
delete分享
delete收藏
摘要

摘要

En 中文
Context. Ambipolar diffusion is a process occurring in partially ionised astrophysical systems that imparts a complicated mathematical and physical nature to Ohm's law. The numerical codes that solve the magnetohydrodynamic (MHD) equations have to be able to deal with the singularities that are naturally created in the system by the ambipolar diffusion term. Aims. The global aim is to calculate a set of theoretical self-similar solutions to the nonlinear diffusion equation with cylindrical symmetry that can be used as tests for MHD codes which include the ambipolar diffusion term. Methods. First, following the general methods developed in the applied mathematics literature, we obtained the theoretical solutions as eigenfunctions of a nonlinear ordinary differential equation. Phase-plane techniques were used to integrate through the singularities at the locations of the nulls, which correspond to infinitely sharp current sheets. In the second half of the paper, we consider the use of these solutions as tests for MHD codes. To that end, we used the Bifrost code, thereby testing the capabilities of these solutions as tests as well as (inversely) the accuracy of Bifrost's recently developed ambipolar diffusion module. Results. The obtained solutions are shown to constitute a demanding, but nonetheless viable, test for MHD codes that incorporate ambipolar diffusion. Detailed tabulated runs of the solutions have been made available at a public repository. The Bifrost code is able to reproduce the theoretical solutions with sufficient accuracy up to very advanced diffusive times. Using the code, we also explored the asymptotic properties of our theoretical solutions in time when initially perturbed with either small or finite perturbations. Conclusions. The functions obtained in this paper are relevant as physical solutions and also as tests for general MHD codes. They provide a more stringent and general test than the simple Zeldovich-Kompaneets-Barenblatt-Pattle solution.
Keyword:
magnetic fields
plasmas
diffusion
methods: numerical
methods: analytical

期刊

Astronomy and Astrophysics 封面图
Astronomy and Astrophysics
IF:
5.8
论文数:
5.0W
被引数:
18.3W

机构

U
university of st andrews
学者数:
9.5K
论文数: 1.0W
被引数: 15
I
instituto de astrofisica de canarias
学者数:
4.3K
论文数: 5.0K
被引数: 31
引用论文

引用论文

Numerical simulations of quiet Sun magnetic fields seeded by the Biermann battery
err2017-08-07
err39
errOAAI
errKhomenko, E.; Vitas, N.; Collados, M.; de Vicente, A.
err分享
err收藏
Non-equilibrium hydrogen ionization in 2D simulations of the solar atmosphere
err2007-07-17
err141
errOAAI
errLeenaarts, J.; Carlsson, M.; Hansteen, V.; Rutten, R. J.
err分享
err收藏
err分享
err收藏
On the Velocity Drift between Ions in the Solar Atmosphere
err2020-09-07
err13
errOAAI
errMartinez-Sykora, Juan; Szydlarski, Mikolaj; Hansteen, Viggo H.; De Pontieu, Bart
err分享
err收藏
Ion-neutral Interactions and Nonequilibrium Ionization in the Solar Chromosphere
err2020-01-29
err41
errOAAI
errMartinez-Sykora, Juan; Leenaarts, Jorrit; De Pontieu, Bart; Nobrega-Siverio, Daniel; Hansteen, Viggo H.; Carlsson, Mats; Szydlarski, Mikolaj
err分享
err收藏
A Simflowny-based high-performance 3D code for the generalized induction equation
err2019-04-01
err24
errOAAI
errVigano, Daniele; Martinez-Gomez, David; Pons, Jose A.; Palenzuela, Carlos; Carrasco, Federico; Minano, Borja; Arbona, Antoni; Bona, Carles; Masso, Joan
err分享
err收藏
err分享
err收藏
学者 查看更多内容