Meteoric material and the behavior of upper stratospheric polar zone

Ozone mixing ratios as a function of pressure level and time are presented based on data obtained with the Nimbus-7 SBUV instrument between 1979 and 1984, and implications of this data for the explanations of the spring Antarctic ozone depletion are considered. It is suggested that meteoric atoms re...

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Main Authors: Aikin, A. C., Mcpeters, R. D.
Language:unknown
Published: 1986
Subjects:
46
Online Access:http://ntrs.nasa.gov/search.jsp?R=19870036278
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spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19870036278 2023-05-15T14:01:08+02:00 Meteoric material and the behavior of upper stratospheric polar zone Aikin, A. C. Mcpeters, R. D. Unclassified, Unlimited, Publicly available Nov 1, 1986 http://ntrs.nasa.gov/search.jsp?R=19870036278 unknown http://ntrs.nasa.gov/search.jsp?R=19870036278 Accession ID: 87A23552 Copyright Other Sources 46 1986 ftnasantrs 2012-02-15T17:09:53Z Ozone mixing ratios as a function of pressure level and time are presented based on data obtained with the Nimbus-7 SBUV instrument between 1979 and 1984, and implications of this data for the explanations of the spring Antarctic ozone depletion are considered. It is suggested that meteoric atoms react with the atmosphere to bond to OH, and subsequently react with HCl to form salts, resulting in the accumulation of chlorine during polar winter. The sudden release of this chlorine from photodissociation of these salts during spring could account for the loss of ozone in the upper atmosphere. Other/Unknown Material Antarc* Antarctic NASA Technical Reports Server (NTRS) Antarctic
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic 46
spellingShingle 46
Aikin, A. C.
Mcpeters, R. D.
Meteoric material and the behavior of upper stratospheric polar zone
topic_facet 46
description Ozone mixing ratios as a function of pressure level and time are presented based on data obtained with the Nimbus-7 SBUV instrument between 1979 and 1984, and implications of this data for the explanations of the spring Antarctic ozone depletion are considered. It is suggested that meteoric atoms react with the atmosphere to bond to OH, and subsequently react with HCl to form salts, resulting in the accumulation of chlorine during polar winter. The sudden release of this chlorine from photodissociation of these salts during spring could account for the loss of ozone in the upper atmosphere.
author Aikin, A. C.
Mcpeters, R. D.
author_facet Aikin, A. C.
Mcpeters, R. D.
author_sort Aikin, A. C.
title Meteoric material and the behavior of upper stratospheric polar zone
title_short Meteoric material and the behavior of upper stratospheric polar zone
title_full Meteoric material and the behavior of upper stratospheric polar zone
title_fullStr Meteoric material and the behavior of upper stratospheric polar zone
title_full_unstemmed Meteoric material and the behavior of upper stratospheric polar zone
title_sort meteoric material and the behavior of upper stratospheric polar zone
publishDate 1986
url http://ntrs.nasa.gov/search.jsp?R=19870036278
op_coverage Unclassified, Unlimited, Publicly available
geographic Antarctic
geographic_facet Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source Other Sources
op_relation http://ntrs.nasa.gov/search.jsp?R=19870036278
Accession ID: 87A23552
op_rights Copyright
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