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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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 |
_version_ |
1766270733813547008 |