Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Monte Carlo approach to identification of the composition of stratospheric aerosols from infrared solar occultation measurements

Not Accessible

Your library or personal account may give you access

Abstract

We describe an inversion method for determining the composition, density, and size of stratospheric clouds and aerosols by satellite remote sensing. The method, which combines linear least-squares minimization and Monte Carlo techniques, is tested with pure synthetic IR spectra. The synthetic spectral data are constructed to mimic mid-IR spectra recorded by the Improved Limb Atmospheric Spectrometer (ILAS-I and ILAS-II) instruments, which operate in the solar occultation mode and record numerous polar stratospheric cloud events. The advantages and limitations of the proposed technique are discussed. In brief we find that stratospheric aerosol in the size range from 0.5 to 4.0 μm can be retrieved to an accuracy of 30%. We also show that the chemical composition of common stratospheric aerosols can be determined, whereas identification of their phases from mid-IR satellite remote-sensing data alone appears to be questionable.

© 2005 Optical Society of America

Full Article  |  PDF Article
More Like This
Simultaneous stratospheric gas and aerosol retrievals from broadband infrared occultation measurements

Sergey Oshchepkov, Yasuhiro Sasano, Tatsuya Yokota, Nobuyuki Uemura, Hisashi Matsuda, Yasuhiro Itou, and Hideaki Nakajima
Appl. Opt. 44(22) 4775-4784 (2005)

Determination of polar stratospheric cloud particle refractive indices by use of in situ optical measurements and T-matrix calculations

Claudio Scarchilli, Alberto Adriani, Francesco Cairo, Guido Di Donfrancesco, Carlo Buontempo, Marcel Snels, Maria Luisa Moriconi, Terry Deshler, Niels Larsen, Beiping Luo, Konrad Mauersberger, Joelle Ovarlez, Jim Rosen, and Jochen Schreiner
Appl. Opt. 44(16) 3302-3311 (2005)

Retrieval of stratospheric aerosol size and composition information from solar infrared transmission spectra

Helen M. Steele, Annmarie Eldering, Bhaswar Sen, Geoffrey C. Toon, Franklin P. Mills, and Brian H. Kahn
Appl. Opt. 42(12) 2140-2154 (2003)

Cited By

You do not have subscription access to this journal. Cited by links are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.

Contact your librarian or system administrator
or
Login to access Optica Member Subscription

Figures (5)

You do not have subscription access to this journal. Figure files are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.

Contact your librarian or system administrator
or
Login to access Optica Member Subscription

Equations (6)

You do not have subscription access to this journal. Equations are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.

Contact your librarian or system administrator
or
Login to access Optica Member Subscription

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.