分析磁重联原位观测的先进方法
空间物理
2024-06-26 v3 地球与行星天体物理
等离子体物理
摘要
太阳系中存在大量磁重联的证据，但从等离子体粒子与电磁场的原位测量中可视化、确定恰当的研究途径与参考系，进而阐明重联区起作用的物理过程，是一项非平凡的任务。本文概述了一系列单航天器与多航天器数据分析技术，这些技术对揭示空间磁重联原位观测的背景，以及探测并分析离子和/或电子发生退磁的扩散区至关重要。我们聚焦于 Magnetospheric Multiscale 任务时代的最新进展，该任务已对地球磁层内外磁重联进行了电子尺度、多点测量。
引用
@article{arxiv.2307.05867,
title = {Advanced methods for analyzing in-situ observations of magnetic reconnection},
author = {H. Hasegawa and M. R. Argall and N. Aunai and R. Bandyopadhyay and N. Bessho and I. J. Cohen and R. E. Denton and J. C. Dorelli and J. Egedal and S. A. Fuselier and P. Garnier and V. Genot and D. B. Graham and K. J. Hwang and Y. V. Khotyaintsev and D. B. Korovinskiy and B. Lavraud and Q. Lenouvel and T. C. Li and Y. -H. Liu and B. Michotte de Welle and T. K. M. Nakamura and D. S. Payne and S. M. Petrinec and Y. Qi and A. C. Rager and P. H. Reiff and J. M. Schroeder and J. R. Shuster and M. I. Sitnov and G. K. Stephens and M. Swisdak and A. M. Tian and R. B. Torbert and K. J. Trattner and S. Zenitani},
journal= {arXiv preprint arXiv:2307.05867},
year = {2024}
}
备注
submitted to Space Science Reviews (116 pages, incl. 31 figures, 7 tables)