First detection of the O III 495.8911 and 500.6843 nm lines in the Earth's upper atmosphere

We report the first detection of two emission lines of the atomic oxygen doubly-charged ion at 495.8911 and 500.6843 nm in the terrestrial upper atmosphere. They correspond to the transitions <sup>1</sup>D<sub>2</sub>-<sup>3</sup>P<sub>1</sub> and &...

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Main Authors: O. Witasse, T. Slanger, R. Thissen
Format: Article
Language:English
Published: Copernicus Publications 2011-12-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/29/2235/2011/angeo-29-2235-2011.pdf
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author O. Witasse
T. Slanger
R. Thissen
author_facet O. Witasse
T. Slanger
R. Thissen
author_sort O. Witasse
collection DOAJ
description We report the first detection of two emission lines of the atomic oxygen doubly-charged ion at 495.8911 and 500.6843 nm in the terrestrial upper atmosphere. They correspond to the transitions <sup>1</sup>D<sub>2</sub>-<sup>3</sup>P<sub>1</sub> and <sup>1</sup>D<sub>2</sub>-<sup>3</sup>P<sub>2</sub> of the O<sup>++</sup> ion, respectively. The measurements were performed on 30 October 2003 during the "Halloween" storms, with the Ultraviolet and Visual Echelle Spectrograph (UVES) mounted on the Very Large Telescope (VLT) in Chile. The intensities of these emissions are ~70 mRayleigh, and ~260 mRayleigh, respectively. These emissions constitute a new diagnostic of the state of the ionosphere.
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spelling doaj.art-ca972580b9fd4df1adf6892b596138b92022-12-22T02:33:37ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762011-12-01292235223810.5194/angeo-29-2235-2011First detection of the O III 495.8911 and 500.6843 nm lines in the Earth's upper atmosphereO. Witasse0T. Slanger1R. Thissen2Research and Scientific Support Department of the European Space Agency, ESTEC, Noordwijk, The NetherlandsMolecular Physics Laboratory, SRI International, Menlo Park, CA, USAUJF-Grenoble 1/CNRS-INSU, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG) UMR 5274, Grenoble, 38041, FranceWe report the first detection of two emission lines of the atomic oxygen doubly-charged ion at 495.8911 and 500.6843 nm in the terrestrial upper atmosphere. They correspond to the transitions <sup>1</sup>D<sub>2</sub>-<sup>3</sup>P<sub>1</sub> and <sup>1</sup>D<sub>2</sub>-<sup>3</sup>P<sub>2</sub> of the O<sup>++</sup> ion, respectively. The measurements were performed on 30 October 2003 during the "Halloween" storms, with the Ultraviolet and Visual Echelle Spectrograph (UVES) mounted on the Very Large Telescope (VLT) in Chile. The intensities of these emissions are ~70 mRayleigh, and ~260 mRayleigh, respectively. These emissions constitute a new diagnostic of the state of the ionosphere.https://www.ann-geophys.net/29/2235/2011/angeo-29-2235-2011.pdf
spellingShingle O. Witasse
T. Slanger
R. Thissen
First detection of the O III 495.8911 and 500.6843 nm lines in the Earth's upper atmosphere
Annales Geophysicae
title First detection of the O III 495.8911 and 500.6843 nm lines in the Earth's upper atmosphere
title_full First detection of the O III 495.8911 and 500.6843 nm lines in the Earth's upper atmosphere
title_fullStr First detection of the O III 495.8911 and 500.6843 nm lines in the Earth's upper atmosphere
title_full_unstemmed First detection of the O III 495.8911 and 500.6843 nm lines in the Earth's upper atmosphere
title_short First detection of the O III 495.8911 and 500.6843 nm lines in the Earth's upper atmosphere
title_sort first detection of the o iii 495 8911 and 500 6843 nm lines in the earth s upper atmosphere
url https://www.ann-geophys.net/29/2235/2011/angeo-29-2235-2011.pdf
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