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Simulation Models for Exploring Magnetic Reconnection

delete2025-09-09
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OA
AI
M
M. A. Shay *
S
Subash Adhikari
N
Naoki Beesho
J
J. Birn
J
Jörg Büchner
P
P. A. Cassak
L
Li‐Jen Chen
Y
Yuxi Chen
G
Giulia Cozzani *
J
J. F. Drake
F
Fan Guo
M
M. Hesse
N
Neeraj Jain
Y
Yann Pfau‐Kempf
Y
Yi-Hsin Liu
M
M. Oka
Y
Y. A. Omelchenko
M
Minna Palmroth
O
Oreste Pezzi
P
P. H. Reiff
M
M. Swisdak
F
F. Toffoletto
G
G. Tóth
R
R. A. Wolf
DOI：10.1007/s11214-025-01210-5delete
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摘要

摘要

En 中文
模拟在推进我们对磁重联的认识方面发挥了关键作用。然而，由于重联本身具有多尺度特性，不可能在所有尺度上模拟所有物理现象。因此，已设计出一系列广泛的模拟方法来研究磁重联的特定方面和后果。本文回顾了其中许多方法，阐述了关键假设、数值技术，并给出了科学结果的示例。描述的等离子体模型包括磁流体动力学（MHD）、霍尔MHD、混合模型、动力量子粒子网格（PIC）、动力学Vlasov、嵌入PIC的流体模型、来自高能粒子群的直接反馈的流体模型，以及Rice对流模型（RCM）。
Keyword:
Plasma simulation
Magnetic reconnection
Plasma physics
Magnetosphere
Solar corona
Turbulence
Numerical methods
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Space Science Reviews 封面图
Space Science Reviews
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