The Cl-36 in the stratosphere

Initial measurements of the cosmogenic radionuclide, Cl-36, in the lower stratosphere were made by accelerator mass spectrometry. Samples were obtained using the large volume LASL air sampling pods on a NASA WB-57F aircraft. Untreated (for collection of particulates only) and tetrabutyl ammonium hyd...

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Main Authors: Wahlen, Martin, Weyer, Harley, Kubik, Peter, Deck, Bruce, Gove, Harry, Sharma, Pankaj
Format: Other/Unknown Material
Language:unknown
Published: 1991
Subjects:
Online Access:http://hdl.handle.net/2060/19910016145
id ftnasantrs:oai:casi.ntrs.nasa.gov:19910016145
record_format openpolar
spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19910016145 2023-05-15T13:42:52+02:00 The Cl-36 in the stratosphere Wahlen, Martin Weyer, Harley Kubik, Peter Deck, Bruce Gove, Harry Sharma, Pankaj Unclassified, Unlimited, Publicly available JAN 1, 1991 application/pdf http://hdl.handle.net/2060/19910016145 unknown Document ID: 19910016145 Accession ID: 91N25459 http://hdl.handle.net/2060/19910016145 No Copyright CASI ENVIRONMENT POLLUTION NASA, Washington, 4th Airborne Geoscience Workshop; p 131-132 1991 ftnasantrs 2015-03-15T05:17:19Z Initial measurements of the cosmogenic radionuclide, Cl-36, in the lower stratosphere were made by accelerator mass spectrometry. Samples were obtained using the large volume LASL air sampling pods on a NASA WB-57F aircraft. Untreated (for collection of particulates only) and tetrabutyl ammonium hydroxide treated (for collection of particulates and HCl) IPC-1478 filters were flown on three flights in the lower stratosphere. Chlorine (Cl) and Cl compounds are important trace constituents for stratospheric chemistry, in particular with respect to O3 destruction. Stratospheric Cl chemistry has recently received increased attention with the observation of strong O3 depletion in the Antarctic winter vortex and in the weaker and more complex Arctic winter vortices. Cosmogenic (Cl-36) is produced by spallation reactions from Ar mainly in the stratosphere, and has had several applications as a geochemical tracer. The large amounts of Cl-36 introduced by nuclear weapon testing have been removed from the stratosphere by now, and measurements in the stratosphere to obtain cosmogenic production rates and concentration distributions is now possible. The use of cosmogenic Cl-36 as a tracer for stratospheric Cl chemistry and for stratospheric/tropospheric exchange processes is investigated. A first attempt to determine stratospheric and tropospheric production rates, the partitioning of Cl-36 among particulate and gaseous Cl compounds, and the respective inventories and removal rates is being made. Results from a flight at 13.7 km, 30-33 degrees N, 97-107 degrees W, and from a second flight at 17.7 km, 43-45-36 degrees N, 92-94 degrees W, for the untreated and treated filters respectively are presented. Other/Unknown Material Antarc* Antarctic Arctic NASA Technical Reports Server (NTRS) Arctic Antarctic The Antarctic
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic ENVIRONMENT POLLUTION
spellingShingle ENVIRONMENT POLLUTION
Wahlen, Martin
Weyer, Harley
Kubik, Peter
Deck, Bruce
Gove, Harry
Sharma, Pankaj
The Cl-36 in the stratosphere
topic_facet ENVIRONMENT POLLUTION
description Initial measurements of the cosmogenic radionuclide, Cl-36, in the lower stratosphere were made by accelerator mass spectrometry. Samples were obtained using the large volume LASL air sampling pods on a NASA WB-57F aircraft. Untreated (for collection of particulates only) and tetrabutyl ammonium hydroxide treated (for collection of particulates and HCl) IPC-1478 filters were flown on three flights in the lower stratosphere. Chlorine (Cl) and Cl compounds are important trace constituents for stratospheric chemistry, in particular with respect to O3 destruction. Stratospheric Cl chemistry has recently received increased attention with the observation of strong O3 depletion in the Antarctic winter vortex and in the weaker and more complex Arctic winter vortices. Cosmogenic (Cl-36) is produced by spallation reactions from Ar mainly in the stratosphere, and has had several applications as a geochemical tracer. The large amounts of Cl-36 introduced by nuclear weapon testing have been removed from the stratosphere by now, and measurements in the stratosphere to obtain cosmogenic production rates and concentration distributions is now possible. The use of cosmogenic Cl-36 as a tracer for stratospheric Cl chemistry and for stratospheric/tropospheric exchange processes is investigated. A first attempt to determine stratospheric and tropospheric production rates, the partitioning of Cl-36 among particulate and gaseous Cl compounds, and the respective inventories and removal rates is being made. Results from a flight at 13.7 km, 30-33 degrees N, 97-107 degrees W, and from a second flight at 17.7 km, 43-45-36 degrees N, 92-94 degrees W, for the untreated and treated filters respectively are presented.
format Other/Unknown Material
author Wahlen, Martin
Weyer, Harley
Kubik, Peter
Deck, Bruce
Gove, Harry
Sharma, Pankaj
author_facet Wahlen, Martin
Weyer, Harley
Kubik, Peter
Deck, Bruce
Gove, Harry
Sharma, Pankaj
author_sort Wahlen, Martin
title The Cl-36 in the stratosphere
title_short The Cl-36 in the stratosphere
title_full The Cl-36 in the stratosphere
title_fullStr The Cl-36 in the stratosphere
title_full_unstemmed The Cl-36 in the stratosphere
title_sort cl-36 in the stratosphere
publishDate 1991
url http://hdl.handle.net/2060/19910016145
op_coverage Unclassified, Unlimited, Publicly available
geographic Arctic
Antarctic
The Antarctic
geographic_facet Arctic
Antarctic
The Antarctic
genre Antarc*
Antarctic
Arctic
genre_facet Antarc*
Antarctic
Arctic
op_source CASI
op_relation Document ID: 19910016145
Accession ID: 91N25459
http://hdl.handle.net/2060/19910016145
op_rights No Copyright
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