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当前模型所呈现的大规模日球层结构。

The Structure of the Large-Scale Heliosphere as Seen by Current Models.

作者信息

Kleimann Jens, Dialynas Konstantinos, Fraternale Federico, Galli André, Heerikhuisen Jacob, Izmodenov Vladislav, Kornbleuth Marc, Opher Merav, Pogorelov Nikolai

机构信息

Theoretische Physik IV, Ruhr-Universität Bochum, 44780 Bochum, Germany.

Office of Space Research and Technology, Academy of Athens, 10679 Athens, Greece.

出版信息

Space Sci Rev. 2022;218(4):36. doi: 10.1007/s11214-022-00902-6. Epub 2022 May 31.

DOI:10.1007/s11214-022-00902-6
PMID:35664863
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC9156516/
Abstract

This review summarizes the current state of research aiming at a description of the global heliosphere using both analytical and numerical modeling efforts, particularly in view of the overall plasma/neutral flow and magnetic field structure, and its relation to energetic neutral atoms. Being part of a larger volume on current heliospheric research, it also lays out a number of key concepts and describes several classic, though still relevant early works on the topic. Regarding numerical simulations, emphasis is put on magnetohydrodynamic (MHD), multi-fluid, kinetic-MHD, and hybrid modeling frameworks. Finally, open issues relating to the physical relevance of so-called "croissant" models of the heliosphere, as well as the general (dis)agreement of model predictions with observations are highlighted and critically discussed.

摘要

本综述总结了旨在通过解析和数值模拟来描述全球日球层的研究现状，特别是从整体等离子体/中性流和磁场结构及其与高能中性原子的关系方面进行描述。作为关于当前日球层研究的更大篇幅内容的一部分，它还阐述了一些关键概念，并描述了该主题的若干经典（尽管仍具相关性）早期研究成果。关于数值模拟，重点放在磁流体动力学（MHD）、多流体、动理学-MHD和混合建模框架上。最后，强调并批判性地讨论了与日球层所谓“羊角面包”模型的物理相关性相关的未决问题，以及模型预测与观测结果的总体（不）一致性。

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