Historical perspective on astrophysical MHD simulations

被引：0
|
作者：
Norman, Michael L. [1 ]
机构：
[1] Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
来源：
COMPUTATIONAL STAR FORMATION | 2011年 / 270期
关键词：
ISM: star formation; ISM: magnetic fields; methods: numerical; ADAPTIVE MESH REFINEMENT; PIECEWISE PARABOLIC METHOD; RADIATION MAGNETOHYDRODYNAMICS CODE; ROTATING INTERSTELLAR CLOUDS; 2 SPACE DIMENSIONS; IDEAL MAGNETOHYDRODYNAMICS; NUMERICAL SIMULATIONS; ISOTHERMAL MAGNETOHYDRODYNAMICS; CONSTRAINED TRANSPORT; MAGNETIZED CLOUDS;
D O I：
10.1017/S174392131100010X
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This contribution contains the introductory remarks that I presented at IAU Symposium 270 on "Computational Star Formation" held in Barcelona.; Spain, May 31 - June 2010. I discuss the historical development of numerical MHD methods in astrophysics from a personal perspective. The recent advent of robust; higher-order accurate MHD algorithms and adaptive mesh refinement numerical simulations promises to greatly improve our understanding of the role of magnetic fields in star formation.
引用
收藏
页码：7 / 18
页数：12
相关论文
共 50 条
  • [1] MHD simulations and astrophysical applications
    Gómez, DO
    Mininni, PD
    Dmitruk, P
    FUNDAMENTALS OF SPACE ENVIRONMENT SCIENCE, 2005, 35 (05): : 899 - 907
  • [2] Numerical simulations of the astrophysical MHD flows
    Dudorov, AE
    Zhilkin, AG
    Kuznetsov, OA
    NUMERICAL ASTROPHYSICS, 1999, 240 : 389 - 390
  • [3] Resistive relativistic MHD simulations of astrophysical jets
    Mattia, G.
    Del Zanna, L.
    Bugli, M.
    Pavan, A.
    Ciolfi, R.
    Bodo, G.
    Mignone, A.
    ASTRONOMY & ASTROPHYSICS, 2023, 679
  • [4] Absorbing boundary conditions for astrophysical MHD simulations
    Dedner, A
    Kröner, D
    Wesenberg, M
    Sofronov, I
    GODUNOV METHODS: THEORY AND APPLICATIONS, 2001, : 217 - 224
  • [5] Criteria for scaled laboratory simulations of astrophysical MHD phenomena
    Ryutov, DD
    Drake, RP
    Remington, BA
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2000, 127 (02): : 465 - 468
  • [6] Energy distribution and substructure formation in astrophysical MHD simulations
    Kayanikhoo, Fatemeh
    Cemeljic, Miljenko
    Wielgus, Maciek
    Kluzniak, Wlodek
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2024, 527 (04) : 10151 - 10167
  • [7] Astrophysical MHD jets
    Heyvaerts, J
    NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 2000, 80 : 51 - 61
  • [8] MHD Simulations of Astrophysical and Laboratory Jets under Different Magnetic Field Configurations
    Toropina, O. D.
    Bisnovatyi-Kogan, G. S.
    Moiseenko, S. G.
    ASTRONOMY REPORTS, 2024, 68 (04) : 395 - 405
  • [9] Unidimensional SPH simulations of reactive shock tubes in an astrophysical perspective
    Busegnies, Y.
    Francois, J.
    Paulus, G.
    SHOCK WAVES, 2007, 16 (4-5) : 359 - 389
  • [10] Unidimensional SPH simulations of reactive shock tubes in an astrophysical perspective
    Y. Busegnies
    J. François
    G. Paulus
    Shock Waves, 2007, 16 : 359 - 389
12345