The possible detection of OBrO in the stratosphere

International audience The analysis of spectral residua recorded at night by the balloon-borne AMON (Absorption par Minoritaires Ozone et Nox) UV-visible spectrometer during five stratospheric flights at middle and high latitudes shows that some absorption features remain in the 475-550 nm range, wh...

Full description

Bibliographic Details
Published in:Journal of Geophysical Research: Atmospheres
Main Authors: Renard, Jean-Baptiste, Pirre, Michel, Robert, C, Huguenin, Daniel
Other Authors: Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES), Laboratoire de physique et chimie de l'environnement (LPCE), Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève = University of Geneva (UNIGE)
Format: Article in Journal/Newspaper
Language:English
Published: CCSD 1998
Subjects:
Online Access:https://insu.hal.science/insu-02879280
https://insu.hal.science/insu-02879280v1/document
https://insu.hal.science/insu-02879280v1/file/98JD01805.pdf
https://doi.org/10.1029/98JD01805
_version_ 1824233652451540992
author Renard, Jean-Baptiste
Pirre, Michel
Robert, C
Huguenin, Daniel
author2 Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E)
Observatoire des Sciences de l'Univers en région Centre (OSUC)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES)
Laboratoire de physique et chimie de l'environnement (LPCE)
Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)
Observatoire Astronomique de l'Université de Genève (ObsGE)
Université de Genève = University of Geneva (UNIGE)
author_facet Renard, Jean-Baptiste
Pirre, Michel
Robert, C
Huguenin, Daniel
author_sort Renard, Jean-Baptiste
collection Université d'Orléans: HAL
container_issue D19
container_start_page 25383
container_title Journal of Geophysical Research: Atmospheres
container_volume 103
description International audience The analysis of spectral residua recorded at night by the balloon-borne AMON (Absorption par Minoritaires Ozone et Nox) UV-visible spectrometer during five stratospheric flights at middle and high latitudes shows that some absorption features remain in the 475-550 nm range, while the Rayleigh, aerosol, ozone, and NO2 contributions are subtracted. The data reduction relating to these spectral lines is presented for the flight of February 26, 1997, at Kiruna (Sweden) inside the polar vortex. A good agreement exists between these unknown absorption features and those attributed to OBrO during recent laboratory measurements. The results of measurements from the other AMON flights are also presented. Assuming a OBrO cross section maximum similar to that of OC10, an upper limit for the OBrO mixing ratio is found to be around 20 pptv at midlatitude, implying that OBrO would be the principal bromine species at night in the middle stratosphere. At high latitude the OBrO mixing ratio decreases, particularly in the presence of OC10 (also measured by AMON). The results are contradictory to current knowledge and, if confirmed, could argue for major revision of the assumed bromine chemistry in the stratosphere.
format Article in Journal/Newspaper
genre Kiruna
genre_facet Kiruna
geographic Kiruna
geographic_facet Kiruna
id ftunivorleans:oai:HAL:insu-02879280v1
institution Open Polar
language English
op_collection_id ftunivorleans
op_container_end_page 25395
op_doi https://doi.org/10.1029/98JD01805
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1029/98JD01805
doi:10.1029/98JD01805
op_rights info:eu-repo/semantics/OpenAccess
op_source ISSN: 2169-897X
EISSN: 2169-8996
Journal of Geophysical Research: Atmospheres
https://insu.hal.science/insu-02879280
Journal of Geophysical Research: Atmospheres, 1998, 103 (D19), pp.383-408. ⟨10.1029/98JD01805⟩
publishDate 1998
publisher CCSD
record_format openpolar
spelling ftunivorleans:oai:HAL:insu-02879280v1 2025-02-16T15:06:04+00:00 The possible detection of OBrO in the stratosphere Renard, Jean-Baptiste Pirre, Michel Robert, C Huguenin, Daniel Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E) Observatoire des Sciences de l'Univers en région Centre (OSUC) Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES) Laboratoire de physique et chimie de l'environnement (LPCE) Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS) Observatoire Astronomique de l'Université de Genève (ObsGE) Université de Genève = University of Geneva (UNIGE) 1998 https://insu.hal.science/insu-02879280 https://insu.hal.science/insu-02879280v1/document https://insu.hal.science/insu-02879280v1/file/98JD01805.pdf https://doi.org/10.1029/98JD01805 en eng CCSD American Geophysical Union info:eu-repo/semantics/altIdentifier/doi/10.1029/98JD01805 doi:10.1029/98JD01805 info:eu-repo/semantics/OpenAccess ISSN: 2169-897X EISSN: 2169-8996 Journal of Geophysical Research: Atmospheres https://insu.hal.science/insu-02879280 Journal of Geophysical Research: Atmospheres, 1998, 103 (D19), pp.383-408. ⟨10.1029/98JD01805⟩ [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] info:eu-repo/semantics/article Journal articles 1998 ftunivorleans https://doi.org/10.1029/98JD01805 2025-01-21T01:42:04Z International audience The analysis of spectral residua recorded at night by the balloon-borne AMON (Absorption par Minoritaires Ozone et Nox) UV-visible spectrometer during five stratospheric flights at middle and high latitudes shows that some absorption features remain in the 475-550 nm range, while the Rayleigh, aerosol, ozone, and NO2 contributions are subtracted. The data reduction relating to these spectral lines is presented for the flight of February 26, 1997, at Kiruna (Sweden) inside the polar vortex. A good agreement exists between these unknown absorption features and those attributed to OBrO during recent laboratory measurements. The results of measurements from the other AMON flights are also presented. Assuming a OBrO cross section maximum similar to that of OC10, an upper limit for the OBrO mixing ratio is found to be around 20 pptv at midlatitude, implying that OBrO would be the principal bromine species at night in the middle stratosphere. At high latitude the OBrO mixing ratio decreases, particularly in the presence of OC10 (also measured by AMON). The results are contradictory to current knowledge and, if confirmed, could argue for major revision of the assumed bromine chemistry in the stratosphere. Article in Journal/Newspaper Kiruna Université d'Orléans: HAL Kiruna Journal of Geophysical Research: Atmospheres 103 D19 25383 25395
spellingShingle [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
Renard, Jean-Baptiste
Pirre, Michel
Robert, C
Huguenin, Daniel
The possible detection of OBrO in the stratosphere
title The possible detection of OBrO in the stratosphere
title_full The possible detection of OBrO in the stratosphere
title_fullStr The possible detection of OBrO in the stratosphere
title_full_unstemmed The possible detection of OBrO in the stratosphere
title_short The possible detection of OBrO in the stratosphere
title_sort possible detection of obro in the stratosphere
topic [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
topic_facet [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
url https://insu.hal.science/insu-02879280
https://insu.hal.science/insu-02879280v1/document
https://insu.hal.science/insu-02879280v1/file/98JD01805.pdf
https://doi.org/10.1029/98JD01805