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The Ionospheric Connection Explorer - Prime Mission Review

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 de...

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Detalles Bibliográficos
Autores principales: Immel, Thomas J., England, Scott L., Harding, Brian J., Wu, Yen-Jung, Maute, Astrid, Cullens, Chihoko, Englert, Christoph R., Mende, Stephen B., Heelis, Roderick A., Frey, Harald U., Korpela, Eric J., Stephan, Andrew W., Frey, Sabine, Stevens, Michael H., Makela, Jonathan J., Kamalabadi, Farzad, Triplett, Colin C., Forbes, Jeffrey M., McGinness, Emma, Gasque, L. Claire, Harlander, John M., Gérard, Jean-C., Hubert, Benoit, Huba, Joseph D., Meier, Robert R., Roberts, Bryce
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Netherlands 2023
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10352447/
https://www.ncbi.nlm.nih.gov/pubmed/37469439
http://dx.doi.org/10.1007/s11214-023-00975-x
Descripción
Sumario: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.