A Database for Simultaneous Observations of the Earth's Magnetosheath by Cluster and MMS Between 2017 and 2021

IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Costel Munteanu, Eliza Teodorescu, Marius Echim, Daniel Dumitru, Gabriel Voitcu, Maximilian Teodorescu, Cătălin Negrea
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Abstract

This paper describes a catalog of simultaneous observations of the Earth's magnetosheath by ESA's Cluster and NASA's MMS missions. The catalog is built from a visual inspection of summary plots provided by the two missions complemented by an analysis of high-resolution magnetic field data. The catalog includes 117 events when Cluster 4 and MMS 4 crossed simultaneously the magnetosheath between January–April, 2017–2021. The dynamical and turbulent features of the magnetosheath are strongly influenced by θBn, the angle between the interplanetary magnetic field (IMF) and the shock normal direction. To facilitate such investigations, we also determine the bow shock geometry for each event based on two different approaches: (a) a minimum variance analysis of in-situ magnetic field measurements, and (b) a geometrical approach which considers a bow shock model parameterized by OMNI data. A description of spacecraft trajectory during each event is also provided. Additional data describe the relative distances between Cluster 4 and MMS 4, a classification of each event as either quasi-parallel or quasi-perpendicular, and the distribution of events per magnetospheric flank. The time intervals for the Cluster - MMS conjunctions are included in the catalog, as well as all associated figures and tables discussed in this paper are made available through an independent online data repository, and can be freely downloaded and used by any interested researcher.

Abstract Image

2017年至2021年由星群和多用途气象卫星同时观测地球磁鞘的数据库
本文介绍了欧空局的星团和美国航天局的 MMS 任务对地球磁鞘的同步观测数据目录。该目录是通过对两个任务提供的汇总图进行目视检查,并辅以对高分辨率磁场数据的分析而建立的。该目录包括2017-2021年1月至4月期间Cluster 4和MMS 4同时穿越磁鞘的117个事件。磁鞘的动力学和湍流特征受到行星际磁场(IMF)和冲击法线方向之间的夹角θBn的强烈影响。为便于此类研究,我们还根据两种不同的方法确定了每个事件的弓形冲击几何形状:(a)原位磁场测量的最小方差分析,以及(b)考虑了由 OMNI 数据参数化的弓形冲击模型的几何方法。此外,还提供了每个事件期间的航天器轨迹描述。其他数据描述了星团 4 和 MMS 4 之间的相对距离、每个事件的准平行或准垂直分类以及每个磁层侧翼的事件分布情况。星团-MMS会合的时间间隔包含在目录中,本文讨论的所有相关图和表都通过一个独立的在线数据储存库提供,任何感兴趣的研究人员都可以免费下载和使用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Earth and Space Science
Earth and Space Science Earth and Planetary Sciences-General Earth and Planetary Sciences
CiteScore
5.50
自引率
3.20%
发文量
285
审稿时长
19 weeks
期刊介绍: Marking AGU’s second new open access journal in the last 12 months, Earth and Space Science is the only journal that reflects the expansive range of science represented by AGU’s 62,000 members, including all of the Earth, planetary, and space sciences, and related fields in environmental science, geoengineering, space engineering, and biogeochemistry.
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