Seasonal evolution of Titan's stratosphere during the Cassini mission

Titan's stratosphere exhibits significant seasonal changes, including breakup and formation of polar vortices. Here we present the first analysis of midinfrared mapping observations from Cassini's Composite InfraRed Spectrometer to cover the entire mission (Lₛ=293–93°, 2004–2017)—midnorthe...

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Main Authors: Teanby, N, Sylvestre, M, Sharkey, J, Nixon, C, Vinatier, S, Irwin, P
Format: Journal article
Published: Wiley 2019
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author Teanby, N
Sylvestre, M
Sharkey, J
Nixon, C
Vinatier, S
Irwin, P
author_facet Teanby, N
Sylvestre, M
Sharkey, J
Nixon, C
Vinatier, S
Irwin, P
author_sort Teanby, N
collection OXFORD
description Titan's stratosphere exhibits significant seasonal changes, including breakup and formation of polar vortices. Here we present the first analysis of midinfrared mapping observations from Cassini's Composite InfraRed Spectrometer to cover the entire mission (Lₛ=293–93°, 2004–2017)—midnorthern winter to northern summer solstice. The north polar winter vortex persisted well after equinox, starting breakup around Lₛ∼60° and fully dissipating by Lₛ∼90°. Absence of enriched polar air spreading to lower latitudes suggests large‐scale circulation changes and photochemistry control chemical evolution during vortex breakup. South polar vortex formation commenced soon after equinox and by Lₛ∼60° was more enriched in trace gases than the northern middle‐winter vortex and had temperatures ∼20 K colder. This suggests that early‐winter and middle‐winter vortices are dominated by different processes—radiative cooling and subsidence‐induced adiabatic heating respectively. By the end of the mission (Lₛ=93°) south polar conditions were approaching those observed in the north at Lₛ=293°, implying seasonal symmetry in Titan's vortices.
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spelling oxford-uuid:977c06b8-d905-4827-bb97-cc33dc8984f32022-03-26T23:59:58ZSeasonal evolution of Titan's stratosphere during the Cassini missionJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:977c06b8-d905-4827-bb97-cc33dc8984f3Symplectic Elements at OxfordWiley2019Teanby, NSylvestre, MSharkey, JNixon, CVinatier, SIrwin, PTitan's stratosphere exhibits significant seasonal changes, including breakup and formation of polar vortices. Here we present the first analysis of midinfrared mapping observations from Cassini's Composite InfraRed Spectrometer to cover the entire mission (Lₛ=293–93°, 2004–2017)—midnorthern winter to northern summer solstice. The north polar winter vortex persisted well after equinox, starting breakup around Lₛ∼60° and fully dissipating by Lₛ∼90°. Absence of enriched polar air spreading to lower latitudes suggests large‐scale circulation changes and photochemistry control chemical evolution during vortex breakup. South polar vortex formation commenced soon after equinox and by Lₛ∼60° was more enriched in trace gases than the northern middle‐winter vortex and had temperatures ∼20 K colder. This suggests that early‐winter and middle‐winter vortices are dominated by different processes—radiative cooling and subsidence‐induced adiabatic heating respectively. By the end of the mission (Lₛ=93°) south polar conditions were approaching those observed in the north at Lₛ=293°, implying seasonal symmetry in Titan's vortices.
spellingShingle Teanby, N
Sylvestre, M
Sharkey, J
Nixon, C
Vinatier, S
Irwin, P
Seasonal evolution of Titan's stratosphere during the Cassini mission
title Seasonal evolution of Titan's stratosphere during the Cassini mission
title_full Seasonal evolution of Titan's stratosphere during the Cassini mission
title_fullStr Seasonal evolution of Titan's stratosphere during the Cassini mission
title_full_unstemmed Seasonal evolution of Titan's stratosphere during the Cassini mission
title_short Seasonal evolution of Titan's stratosphere during the Cassini mission
title_sort seasonal evolution of titan s stratosphere during the cassini mission
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