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Immel TJ, England SL, Mende SB, Heelis RA, Englert CR, Edelstein J, Frey HU, Korpela EJ, Taylor ER, Craig WW, Harris SE, Bester M, Bust GS, Crowley G, Forbes JM, Gérard JC, Harlander JM, Huba JD, Hubert B, Kamalabadi F, Makela JJ, Maute AI, Meier RR, Raftery C, Rochus P, Siegmund OHW, Stephan AW, Swenson GR, Frey S, Hysell DL, Saito A, Rider KA, Sirk MM. The Ionospheric Connection Explorer Mission: Mission Goals and Design. SPACE SCIENCE REVIEWS 2017; 214:13. [PMID: 33758433 PMCID: PMC7983873 DOI: 10.1007/s11214-017-0449-2] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/30/2016] [Accepted: 11/17/2017] [Indexed: 06/01/2023]
Abstract
The Ionospheric Connection Explorer, or ICON, is a new NASA Explorer mission that will explore the boundary between Earth and space to understand the physical connection between our world and our space environment. This connection is made in the ionosphere, which has long been known to exhibit variability associated with the sun and solar wind. However, it has been recognized in the 21st century that equally significant changes in ionospheric conditions are apparently associated with energy and momentum propagating upward from our own atmosphere. ICON's goal is to weigh the competing impacts of these two drivers as they influence our space environment. Here we describe the specific science objectives that address this goal, as well as the means by which they will be achieved. The instruments selected, the overall performance requirements of the science payload and the operational requirements are also described. ICON's development began in 2013 and the mission is on track for launch in 2017. ICON is developed and managed by the Space Sciences Laboratory at the University of California, Berkeley, with key contributions from several partner institutions.
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Affiliation(s)
- T J Immel
- University of California, Berkeley, USA
| | - S L England
- Virginia Polytechnic Institute and State University, Blacksburg, VA, USA
| | - S B Mende
- University of California, Berkeley, USA
| | - R A Heelis
- University of Texas at Dallas, Dallas, USA
| | - C R Englert
- Naval Research Laboratory, Washington, DC, USA
| | | | - H U Frey
- University of California, Berkeley, USA
| | | | | | - W W Craig
- University of California, Berkeley, USA
| | | | - M Bester
- University of California, Berkeley, USA
| | - G S Bust
- Applied Physics Laboratory, Laurel, MD, USA
| | | | - J M Forbes
- University of Colorado, Boulder, CO, USA
| | | | | | - J D Huba
- Naval Research Laboratory, Washington, DC, USA
| | - B Hubert
- University of Liège, Liège, Belgium
| | | | - J J Makela
- University of Illinois, Champaign-Urbana, USA
| | - A I Maute
- National Center for Atmospheric Research, Boulder, CO, USA
| | - R R Meier
- George Mason University, Fairfax, VA, USA
| | - C Raftery
- University of California, Berkeley, USA
- National Solar Observatory, Boulder, CO, USA
| | - P Rochus
- University of Liège, Liège, Belgium
| | | | - A W Stephan
- Naval Research Laboratory, Washington, DC, USA
| | - G R Swenson
- University of Illinois, Champaign-Urbana, USA
| | - S Frey
- University of California, Berkeley, USA
| | | | - A Saito
- Kyoto University, Kyoto, Japan
| | - K A Rider
- University of California, Berkeley, USA
| | - M M Sirk
- University of California, Berkeley, USA
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Chen HF, Lee YP. Distribution of Internal States of CO from O (1D) + CO Determined with Time-Resolved Fourier Transform Spectroscopy. J Phys Chem A 2006; 110:12096-102. [PMID: 17078603 DOI: 10.1021/jp0640676] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/31/2023]
Abstract
Following collisions of O (1D) with CO, rotationally resolved emission spectra of CO (1 < or = v < or = 6) in the spectral region 1800-2350 cm(-1) were detected with a step-scan Fourier transform spectrometer. O (1D) was produced by photolysis of O3 with light from a KrF excimer laser at 248 nm. Upon irradiation of a flowing mixture of O3 (0.016 Torr) and CO (0.058 Torr), emission of CO (v < or = 6) increases with time, reaches a maximum approximately 10 micros. At the earliest applicable period (2-3 micros), the rotational distribution of CO is not Boltzmann; it may be approximately described with a bimodal distribution corresponding to temperatures approximately 8000 and approximately 500 K, with the proportion of these two components varying with the vibrational level. A short extrapolation from data in the period 2-6 micros leads to a nascent rotational temperature of approximately 10170 +/- 600 K for v = 1 and approximately 1400 +/- 40 K for v = 6, with an average rotational energy of 33 +/- 6 kJ mol(-1). Absorption by CO (v = 0) in the system interfered with population of low J levels of CO (v = 1). The observed vibrational distribution of (v = 2):(v = 3):(v = 4):(v = 5):(v = 6) = 1.00:0.64:0.51:0.32:0.16 corresponds to a vibrational temperature of 6850 +/- 750 K. An average vibrational energy of 40 +/- 4 kJ mol(-1) is derived based on the observed population of CO (2 < or = v < or = 6) and estimates of the population of CO (v = 0, 1, and 7) by extrapolation. The observed rotational distributions of CO (1 < or = v < or = 3) are consistent with results of previous experiments and trajectory calculations; data for CO (4 < or = v < or = 6) are new.
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Affiliation(s)
- Hui-Fen Chen
- Department of Chemistry, National Tsing Hua University, Hsinchu 30013, Taiwan
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