Small-scale composition and haze layering in Titan's polar vortex

Fine scale layering of haze and composition in Titan's stratosphere and mesosphere was investigated using visible/UV images from Cassini's Imaging Science Sub-system (ISS) and IR spectra from Cassini's Composite Infra-Red Spectrometer (CIRS). Both ISS and CIRS independently show fine...

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Những tác giả chính: Teanby, N, de Kok, R, Irwin, P
Định dạng: Journal article
Ngôn ngữ:English
Được phát hành: 2009
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author Teanby, N
de Kok, R
Irwin, P
author_facet Teanby, N
de Kok, R
Irwin, P
author_sort Teanby, N
collection OXFORD
description Fine scale layering of haze and composition in Titan's stratosphere and mesosphere was investigated using visible/UV images from Cassini's Imaging Science Sub-system (ISS) and IR spectra from Cassini's Composite Infra-Red Spectrometer (CIRS). Both ISS and CIRS independently show fine layered structures in haze and composition, respectively, in the 150-450 km altitude range with a preferred vertical wavelength of around 50 km. Layers are most pronounced around the north polar winter vortex, although some weaker layers do exist at more southerly latitudes. The amplitude of composition layers in each trace gas profile is proportional to the relative enrichment of that species in the winter polar vortex compared to equatorial latitudes. As enrichment is caused by polar subsidence, this suggests a dynamical origin. We propose that the polar layers are caused by cross-latitude advection across the vortex boundary. This is analogous to processes that lead to ozone laminae formation around Earth's polar vortices. © 2009 Elsevier Inc. All rights reserved.
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spelling oxford-uuid:816f77a0-401f-46ea-8e01-9d6d21c3ce632022-03-26T21:30:11ZSmall-scale composition and haze layering in Titan's polar vortexJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:816f77a0-401f-46ea-8e01-9d6d21c3ce63EnglishSymplectic Elements at Oxford2009Teanby, Nde Kok, RIrwin, PFine scale layering of haze and composition in Titan's stratosphere and mesosphere was investigated using visible/UV images from Cassini's Imaging Science Sub-system (ISS) and IR spectra from Cassini's Composite Infra-Red Spectrometer (CIRS). Both ISS and CIRS independently show fine layered structures in haze and composition, respectively, in the 150-450 km altitude range with a preferred vertical wavelength of around 50 km. Layers are most pronounced around the north polar winter vortex, although some weaker layers do exist at more southerly latitudes. The amplitude of composition layers in each trace gas profile is proportional to the relative enrichment of that species in the winter polar vortex compared to equatorial latitudes. As enrichment is caused by polar subsidence, this suggests a dynamical origin. We propose that the polar layers are caused by cross-latitude advection across the vortex boundary. This is analogous to processes that lead to ozone laminae formation around Earth's polar vortices. © 2009 Elsevier Inc. All rights reserved.
spellingShingle Teanby, N
de Kok, R
Irwin, P
Small-scale composition and haze layering in Titan's polar vortex
title Small-scale composition and haze layering in Titan's polar vortex
title_full Small-scale composition and haze layering in Titan's polar vortex
title_fullStr Small-scale composition and haze layering in Titan's polar vortex
title_full_unstemmed Small-scale composition and haze layering in Titan's polar vortex
title_short Small-scale composition and haze layering in Titan's polar vortex
title_sort small scale composition and haze layering in titan s polar vortex
work_keys_str_mv AT teanbyn smallscalecompositionandhazelayeringintitanspolarvortex
AT dekokr smallscalecompositionandhazelayeringintitanspolarvortex
AT irwinp smallscalecompositionandhazelayeringintitanspolarvortex