Article (Scientific journals)
Laboratory Study of the Cameron Bands, the First Negative Bands, and Fourth Positive Bands in the Middle Ultraviolet 180–280 nm by Electron Impact Upon CO
Lee, Rena A.; Ajello, Joseph M.; Malone, Charles P. et al.
2021In Journal of Geophysical Research. Planets, 126 (1)
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Keywords :
carbon monoxide (CO); cascade; electron impact; emission cross sections; fluorescence lifetimes; MAVEN IUVS; Earth and Planetary Sciences (miscellaneous); Space and Planetary Science
Abstract :
[en] We have analyzed medium-resolution (full width at half maximum, FWHM = 1.2 nm), Middle UltraViolet (MUV; 180–280 nm) laboratory emission spectra of carbon monoxide (CO) excited by electron impact at 15, 20, 40, 50, and 100 eV under single-scattering conditions at 300 K. The MUV emission spectra at 100 eV contain the Cameron Bands (CB) CO(a 3Π → X 1Σ+), the fourth positive group (4PG) CO(A 1Π → X 1Σ+), and the first negative group (1NG) CO+(B 2Σ+ → X 2Σ) from direct excitation and cascading-induced emission of an optically thin CO gas. We have determined vibrational intensities and emission cross sections for these systems, important for modeling UV observations of the atmospheres of Mars and Venus. We have also measured the CB “glow” profile about the electron beam of the long-lived CO (a 3Π) state and determined its average metastable lifetime of 3 ± 1 ms. Optically allowed cascading from a host of triplet states has been found to be the dominant excitation process contributing to the CB emission cross section at 15 eV, most strongly by the d 3Δ and a' 3Σ+ electronic states. We normalized the CB emission cross section at 15 eV electron impact energy by multilinear regression (MLR) analysis to the blended 15 eV MUV spectrum over the spectral range of 180–280 nm, based on the 4PG emission cross section at 15 eV that we have previously measured (Ajello et al., 2019, https://doi.org/10.1029/2018ja026308). We find the CB total emission cross section at 15 eV to be 7.7 × 10−17 cm2.
Research Center/Unit :
STAR - Space sciences, Technologies and Astrophysics Research - ULiège
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Lee, Rena A. ;  Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States ; Now at Earth and Planetary Sciences, School of Ocean and Earth Sciences and Technology, University of Hawaii, Honolulu, United States
Ajello, Joseph M. ;  Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States
Malone, Charles P. ;  Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Evans, J. Scott ;  Computational Physics Inc., Springfield, United States
Veibell, Victoir ;  Computational Physics Inc., Springfield, United States
Holsclaw, Gregory M. ;  Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States
McClintock, William E. ;  Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States
Hoskins, Alan C.;  Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States
Jain, Sonal ;  Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States
Gérard, Jean-Claude  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO)
Schneider, Nicholas M. ;  Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States
Language :
English
Title :
Laboratory Study of the Cameron Bands, the First Negative Bands, and Fourth Positive Bands in the Middle Ultraviolet 180–280 nm by Electron Impact Upon CO
Publication date :
November 2021
Journal title :
Journal of Geophysical Research. Planets
ISSN :
2169-9097
eISSN :
2169-9100
Publisher :
Blackwell Publishing Ltd
Volume :
126
Issue :
1
Peer reviewed :
Peer reviewed
Funders :
BELSPO - Politique scientifique fédérale [BE]
Funding text :
This work was primarily performed at the Laboratory for Atmospheric and Space Physics (LASP), University of Colorado (CU) Boulder, and the Jet Propulsion Laboratory (JPL), California Institute of Technology (Caltech), under a contract with the National Aeronautics and Space Administration (NASA). We gratefully acknowledge financial support through NASA's Solar System Workings (SSW), Cassini Data Analysis Program (CDAP), the Heliophysics H-TIDeS and Geospace Science programs, Mars Data Analysis Program (MDAP), and the National Science Foundation (NSF) GEO-AGS Aeronomy program. J.-C. G?rard is supported by the PRODEX program managed by the European Space Agency (ESA) with help from the Belgian Federal Science Policy Office (BELSPO). R. A. Lee thanks the NSF Research Experience for Undergraduates (REU) program for support. We thank X. Liu for 4PG rovibrational spectral models. We thank Karl Hubbell for technical support and Bruce Jakosky, and the MAVEN team, for usage of the IUVS optical-engineering unit (OEU). U.S. government sponsorship is acknowledged.This work was primarily performed at the Laboratory for Atmospheric and Space Physics (LASP), University of Colorado (CU) Boulder, and the Jet Propulsion Laboratory (JPL), California Institute of Technology (Caltech), under a contract with the National Aeronautics and Space Administration (NASA). We gratefully acknowledge financial support through NASA's Solar System Workings (SSW), Cassini Data Analysis Program (CDAP), the Heliophysics H‐TIDeS and Geospace Science programs, Mars Data Analysis Program (MDAP), and the National Science Foundation (NSF) GEO‐AGS Aeronomy program. J.‐C. Gérard is supported by the PRODEX program managed by the European Space Agency (ESA) with help from the Belgian Federal Science Policy Office (BELSPO). R. A. Lee thanks the NSF Research Experience for Undergraduates (REU) program for support. We thank X. Liu for 4PG rovibrational spectral models. We thank Karl Hubbell for technical support and Bruce Jakosky, and the MAVEN team, for usage of the IUVS optical‐engineering unit (OEU). U.S. government sponsorship is acknowledged.
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