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
{"title":"The Ionospheric Connection Explorer - Prime Mission Review.","authors":"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","doi":"10.1007/s11214-023-00975-x","DOIUrl":null,"url":null,"abstract":"<p><p>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.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 5","pages":"41"},"PeriodicalIF":9.1000,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10352447/pdf/","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Space Science Reviews","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1007/s11214-023-00975-x","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2023/7/17 0:00:00","PubModel":"Epub","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
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.
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.