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The Ionospheric Connection Explorer - Prime Mission Review.
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.
Afiliación
  • Immel TJ; Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
  • England SL; Aerospace and Ocean Engineering, Virginia Polytechnic Institute and State University, Blacksburg, VA 24061 USA.
  • Harding BJ; Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
  • Wu YJ; Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
  • Maute A; CIRES, University of Colorado, Boulder, CO 80309 USA.
  • Cullens C; Laboratory for Atmospheric and Space Physics, Univ. of Colorado, Boulder, TX 80309 USA.
  • Englert CR; U.S. Naval Research Laboratory, 4555 Overlook Ave S.W., Washington, DC 20375 USA.
  • Mende SB; Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
  • Heelis RA; William B. Hanson Center for Space Sciences, University of Texas, Dallas, Richardson, TX 75080 USA.
  • Frey HU; Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
  • Korpela EJ; Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
  • Stephan AW; U.S. Naval Research Laboratory, 4555 Overlook Ave S.W., Washington, DC 20375 USA.
  • Frey S; Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
  • Stevens MH; U.S. Naval Research Laboratory, 4555 Overlook Ave S.W., Washington, DC 20375 USA.
  • Makela JJ; Department of Electrical and Computer Engineering, University of Illinois Urbana-Champaign, Urbana, IL 61801 USA.
  • Kamalabadi F; Department of Electrical and Computer Engineering, University of Illinois Urbana-Champaign, Urbana, IL 61801 USA.
  • Triplett CC; Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
  • Forbes JM; Department of Aerospace Engineering Sciences, University of Colorado, Boulder, CO 80303 USA.
  • McGinness E; Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
  • Gasque LC; Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
  • Harlander JM; Space Systems Research Corporation, Alexandria, VA USA.
  • Gérard JC; University of Liège, Liège, Belgium.
  • Hubert B; University of Liège, Liège, Belgium.
  • Huba JD; Syntek Technologies, Arlington, VA USA.
  • Meier RR; George Mason University, Fairfax, VA USA.
  • Roberts B; Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
Space Sci Rev ; 219(5): 41, 2023.
Article en En | MEDLINE | ID: mdl-37469439
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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Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: Space Sci Rev Año: 2023 Tipo del documento: Article

Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: Space Sci Rev Año: 2023 Tipo del documento: Article