The Ionospheric Connection Explorer - Prime Mission Review.

IF 9.1 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Space Science Reviews Pub Date : 2023-01-01 Epub Date: 2023-07-17 DOI:10.1007/s11214-023-00975-x
Thomas J Immel, Scott L England, Brian J Harding, Yen-Jung Wu, Astrid Maute, Chihoko Cullens, Christoph R Englert, Stephen B Mende, Roderick A Heelis, Harald U Frey, Eric J Korpela, Andrew W Stephan, Sabine Frey, Michael H Stevens, Jonathan J Makela, Farzad Kamalabadi, Colin C Triplett, Jeffrey M Forbes, Emma McGinness, L Claire Gasque, John M Harlander, Jean-C Gérard, Benoit Hubert, Joseph D Huba, Robert R Meier, Bryce Roberts
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引用次数: 1

Abstract

The two-year prime mission of the NASA Ionospheric Connection Explorer (ICON) is complete. The baseline operational and scientific objectives have been met and exceeded, as detailed in this report. In October of 2019, ICON was launched into an orbit that provides its instruments the capability to deliver near-continuous measurements of the densest plasma in Earth's space environment. Through collection of a key set of in-situ and remote sensing measurements that are, by virtue of a detailed mission design, uniquely synergistic, ICON enables completely new investigations of the mechanisms that control the behavior of the ionosphere-thermosphere system under both geomagnetically quiet and active conditions. In a two-year period that included a deep solar minimum, ICON has elucidated a number of remarkable effects in the ionosphere attributable to energetic inputs from the lower and middle atmosphere, and shown how these are transmitted from the edge of space to the peak of plasma density above. The observatory operated in a period of low activity for 2 years and then for a year with increasing solar activity, observing the changing balance of the impacts of lower and upper atmospheric drivers on the ionosphere.

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电离层连接探索者-主要任务回顾。
美国国家航空航天局电离层连接探测器(ICON)为期两年的主要任务已经完成。如本报告所述,已经达到并超过了基准业务和科学目标。2019年10月,ICON被发射到一个轨道上,该轨道为其仪器提供了对地球空间环境中密度最高的等离子体进行近乎连续测量的能力。ICON通过收集一组关键的现场和遥感测量数据,这些数据凭借详细的任务设计具有独特的协同作用,能够对在地磁安静和活跃条件下控制电离层热层系统行为的机制进行全新的研究。在包括深太阳极小期在内的两年时间里,ICON阐明了电离层中由低层和中层大气的能量输入引起的一些显著影响,并展示了这些影响是如何从太空边缘传输到上面等离子体密度的峰值的。该天文台在低活动期运行了2年,然后在太阳活动增加的情况下运行了一年,观察到低层和高层大气驱动因素对电离层影响的平衡变化。
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来源期刊
Space Science Reviews
Space Science Reviews 地学天文-天文与天体物理
CiteScore
19.70
自引率
3.90%
发文量
60
审稿时长
4-8 weeks
期刊介绍: Space Science Reviews (SSRv) stands as an international journal dedicated to scientific space research, offering a contemporary synthesis across various branches of space exploration. Emphasizing scientific outcomes and instruments, SSRv spans astrophysics, physics of planetary systems, solar physics, and the physics of magnetospheres & interplanetary matter. Beyond Topical Collections and invited Review Articles, Space Science Reviews welcomes unsolicited Review Articles and Special Communications. The latter encompass papers related to a prior topical volume/collection, report-type papers, or timely contributions addressing a robust combination of space science and technology. These papers succinctly summarize both the science and technology aspects of instruments or missions in a single publication.
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