REGULAR AND IRREGULAR BAROCLINIC WAVES IN A MARTIAN GENERAL-CIRCULATION MODEL - A ROLE FOR DIURNAL FORCING

The development and evolution of baroclinic transient waves are simulated in a high resolution, general circulation model (GCM) of the Martian atmosphere, including simulations both with and without a representation of the diurnal cycle of solar heating. Simulations with diurnally-averaged insolatio...

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Main Authors: Collins, M, Lewis, S, Read, P
Format: Conference item
Published: 1995
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author Collins, M
Lewis, S
Read, P
author_facet Collins, M
Lewis, S
Read, P
author_sort Collins, M
collection OXFORD
description The development and evolution of baroclinic transient waves are simulated in a high resolution, general circulation model (GCM) of the Martian atmosphere, including simulations both with and without a representation of the diurnal cycle of solar heating. Simulations with diurnally-averaged insolation are found to develop highly regular baroclinic transients during northern hemisphere autumn, winter and spring seasons, characterized by zonal wavenumber 1 or 2 and periods of 2-6 sols (a sol being a Martian day). With a diurnal cycle, however, transients are found to be significantly more irregular throughout the winter season, sporadically changing their dominant wavenumber and frequency, and resemble more closely data from the Viking Lander time series. These results are discussed with reference to some simple conceptual models in nonlinear dynamics, in terms either of a periodically-perturbed, self-exciting oscillator, or of attractor-merging near a crisis in a periodically perturbed bistable system.
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spelling oxford-uuid:449b73b8-160f-4c5d-a828-359cb9ee65642022-03-26T15:02:37ZREGULAR AND IRREGULAR BAROCLINIC WAVES IN A MARTIAN GENERAL-CIRCULATION MODEL - A ROLE FOR DIURNAL FORCINGConference itemhttp://purl.org/coar/resource_type/c_5794uuid:449b73b8-160f-4c5d-a828-359cb9ee6564Symplectic Elements at Oxford1995Collins, MLewis, SRead, PThe development and evolution of baroclinic transient waves are simulated in a high resolution, general circulation model (GCM) of the Martian atmosphere, including simulations both with and without a representation of the diurnal cycle of solar heating. Simulations with diurnally-averaged insolation are found to develop highly regular baroclinic transients during northern hemisphere autumn, winter and spring seasons, characterized by zonal wavenumber 1 or 2 and periods of 2-6 sols (a sol being a Martian day). With a diurnal cycle, however, transients are found to be significantly more irregular throughout the winter season, sporadically changing their dominant wavenumber and frequency, and resemble more closely data from the Viking Lander time series. These results are discussed with reference to some simple conceptual models in nonlinear dynamics, in terms either of a periodically-perturbed, self-exciting oscillator, or of attractor-merging near a crisis in a periodically perturbed bistable system.
spellingShingle Collins, M
Lewis, S
Read, P
REGULAR AND IRREGULAR BAROCLINIC WAVES IN A MARTIAN GENERAL-CIRCULATION MODEL - A ROLE FOR DIURNAL FORCING
title REGULAR AND IRREGULAR BAROCLINIC WAVES IN A MARTIAN GENERAL-CIRCULATION MODEL - A ROLE FOR DIURNAL FORCING
title_full REGULAR AND IRREGULAR BAROCLINIC WAVES IN A MARTIAN GENERAL-CIRCULATION MODEL - A ROLE FOR DIURNAL FORCING
title_fullStr REGULAR AND IRREGULAR BAROCLINIC WAVES IN A MARTIAN GENERAL-CIRCULATION MODEL - A ROLE FOR DIURNAL FORCING
title_full_unstemmed REGULAR AND IRREGULAR BAROCLINIC WAVES IN A MARTIAN GENERAL-CIRCULATION MODEL - A ROLE FOR DIURNAL FORCING
title_short REGULAR AND IRREGULAR BAROCLINIC WAVES IN A MARTIAN GENERAL-CIRCULATION MODEL - A ROLE FOR DIURNAL FORCING
title_sort regular and irregular baroclinic waves in a martian general circulation model a role for diurnal forcing
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AT readp regularandirregularbaroclinicwavesinamartiangeneralcirculationmodelarolefordiurnalforcing