Retrieval of stratospheric aerosol size information from OSIRIS limb scattered sunlight spectra

Recent work has shown that the retrieval of stratospheric aerosol vertical profiles is possible using limb scattered sunlight measurements at optical wavelengths. The aerosol number density profile is retrieved for an assumed particle size distribution and composition. This result can be used to der...

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Main Authors: A. E. Bourassa, D. A. Degenstein, E. J. Llewellyn
Format: Article
Language:English
Published: Copernicus Publications 2008-11-01
Series:Atmospheric Chemistry and Physics
Online Access:http://www.atmos-chem-phys.net/8/6375/2008/acp-8-6375-2008.pdf
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spelling doaj-b351a158cfb14e1b8ea9f3f38aa58b822020-11-24T22:26:14ZengCopernicus PublicationsAtmospheric Chemistry and Physics1680-73161680-73242008-11-0182163756380Retrieval of stratospheric aerosol size information from OSIRIS limb scattered sunlight spectraA. E. BourassaD. A. DegensteinE. J. LlewellynRecent work has shown that the retrieval of stratospheric aerosol vertical profiles is possible using limb scattered sunlight measurements at optical wavelengths. The aerosol number density profile is retrieved for an assumed particle size distribution and composition. This result can be used to derive the extinction at the measured wavelength. However, large systematic error can result from the uncertainty in the assumed size distribution when the result is used to estimate the extinction at other wavelengths. It is shown in this work that the addition of information obtained from the near infrared limb radiance profile at 1530 nm measured by the imaging module of the OSIRIS instrument yields an indication of the aerosol size distribution profile that can be used to improve the fidelity of the retrievals. A comparison of the estimated extinction profile at 1020 nm with two coincident occultation measurements demonstrates agreement to within approximately 15% from 12 to 27 km altitude. http://www.atmos-chem-phys.net/8/6375/2008/acp-8-6375-2008.pdf
collection DOAJ
language English
format Article
sources DOAJ
author A. E. Bourassa
D. A. Degenstein
E. J. Llewellyn
spellingShingle A. E. Bourassa
D. A. Degenstein
E. J. Llewellyn
Retrieval of stratospheric aerosol size information from OSIRIS limb scattered sunlight spectra
Atmospheric Chemistry and Physics
author_facet A. E. Bourassa
D. A. Degenstein
E. J. Llewellyn
author_sort A. E. Bourassa
title Retrieval of stratospheric aerosol size information from OSIRIS limb scattered sunlight spectra
title_short Retrieval of stratospheric aerosol size information from OSIRIS limb scattered sunlight spectra
title_full Retrieval of stratospheric aerosol size information from OSIRIS limb scattered sunlight spectra
title_fullStr Retrieval of stratospheric aerosol size information from OSIRIS limb scattered sunlight spectra
title_full_unstemmed Retrieval of stratospheric aerosol size information from OSIRIS limb scattered sunlight spectra
title_sort retrieval of stratospheric aerosol size information from osiris limb scattered sunlight spectra
publisher Copernicus Publications
series Atmospheric Chemistry and Physics
issn 1680-7316
1680-7324
publishDate 2008-11-01
description Recent work has shown that the retrieval of stratospheric aerosol vertical profiles is possible using limb scattered sunlight measurements at optical wavelengths. The aerosol number density profile is retrieved for an assumed particle size distribution and composition. This result can be used to derive the extinction at the measured wavelength. However, large systematic error can result from the uncertainty in the assumed size distribution when the result is used to estimate the extinction at other wavelengths. It is shown in this work that the addition of information obtained from the near infrared limb radiance profile at 1530 nm measured by the imaging module of the OSIRIS instrument yields an indication of the aerosol size distribution profile that can be used to improve the fidelity of the retrievals. A comparison of the estimated extinction profile at 1020 nm with two coincident occultation measurements demonstrates agreement to within approximately 15% from 12 to 27 km altitude.
url http://www.atmos-chem-phys.net/8/6375/2008/acp-8-6375-2008.pdf
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