Dynamical and Chemical Behavior of the Lower Stratosphere and Interactions with the Troposphere

Equivalent-barotropic calculations, in tandem with Lagrangian analyses, reveal how changes of total ozone follow from vertical and horizontal transport by planetary waves. Those calculations also throw light on how diabatic motions comprising the Brewer-Dobson circulation develop from quasi-horizont...

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Main Author: Salby, Murry L.
Language:unknown
Published: 1999
Subjects:
Online Access:http://hdl.handle.net/2060/19990025898
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spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19990025898 2023-05-15T18:02:18+02:00 Dynamical and Chemical Behavior of the Lower Stratosphere and Interactions with the Troposphere Salby, Murry L. Unclassified, Unlimited, Publicly available 1999 application/pdf http://hdl.handle.net/2060/19990025898 unknown Document ID: 19990025898 http://hdl.handle.net/2060/19990025898 No Copyright CASI Geophysics 1999 ftnasantrs 2019-08-31T23:05:44Z Equivalent-barotropic calculations, in tandem with Lagrangian analyses, reveal how changes of total ozone follow from vertical and horizontal transport by planetary waves. Those calculations also throw light on how diabatic motions comprising the Brewer-Dobson circulation develop from quasi-horizontal advection by planetary waves. Potential temperature along a material surface indicates organized subsidence inside the polar-night vortex, resembling tracer observations from UARS. Lagrangian histories illustrate that this sinking motion follows in large part from parcels being driven out of thermodynamic equilibrium by planetary waves, especially at high latitudes. Irreversible heat transfer then produces a net drift of air across isentropic surfaces as parcels orbit about the displaced vortex. By driving mean-meridional overturning in the stratosphere, this downward drift is ultimately responsible for transferring ozone from the tropics to the extratropical lower stratosphere. It also introduces horizontal structure into the distribution of total ozone, which surfaces clearly in ozone trends. High-resolution global cloud imagery constructed from 6 satellites simultaneously observing the Earth was used to investigate the spectrum of equatorial waves generated by tropical convection and propagating vertically into the stratosphere. The results indicate that temperature variability is dominated by planetary-scale equatorial waves like the Kelvin mode, which agrees with satellite observations of the tropical stratosphere. However, the Kelvin mode accounts for only about 30 - 50% of the eastward momentum flux radiating into the stratosphere, the remainder coming from gravity waves. An algorithm was developed to determine 3-dimensional atmospheric motion from satellite tracer measurements. Based on Lagrangian constraints, the algorithm circumvents limitations of the traditional scheme for inferring motion from temperature measurements and determines the circulation in the tropics as reliably as elsewhere. A study of deep convection revealed that the highest towers (those penetrating into stratospheric air and controlling tropopause height and composition through convective mixing) occur in close association with the diurnal cycle of convection. Clouds colder than 220 K develop almost entirely in association with the diurnal cycle of convection over tropical landmasses and substantially in association with it even over maritime regions. Other/Unknown Material polar night NASA Technical Reports Server (NTRS)
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic Geophysics
spellingShingle Geophysics
Salby, Murry L.
Dynamical and Chemical Behavior of the Lower Stratosphere and Interactions with the Troposphere
topic_facet Geophysics
description Equivalent-barotropic calculations, in tandem with Lagrangian analyses, reveal how changes of total ozone follow from vertical and horizontal transport by planetary waves. Those calculations also throw light on how diabatic motions comprising the Brewer-Dobson circulation develop from quasi-horizontal advection by planetary waves. Potential temperature along a material surface indicates organized subsidence inside the polar-night vortex, resembling tracer observations from UARS. Lagrangian histories illustrate that this sinking motion follows in large part from parcels being driven out of thermodynamic equilibrium by planetary waves, especially at high latitudes. Irreversible heat transfer then produces a net drift of air across isentropic surfaces as parcels orbit about the displaced vortex. By driving mean-meridional overturning in the stratosphere, this downward drift is ultimately responsible for transferring ozone from the tropics to the extratropical lower stratosphere. It also introduces horizontal structure into the distribution of total ozone, which surfaces clearly in ozone trends. High-resolution global cloud imagery constructed from 6 satellites simultaneously observing the Earth was used to investigate the spectrum of equatorial waves generated by tropical convection and propagating vertically into the stratosphere. The results indicate that temperature variability is dominated by planetary-scale equatorial waves like the Kelvin mode, which agrees with satellite observations of the tropical stratosphere. However, the Kelvin mode accounts for only about 30 - 50% of the eastward momentum flux radiating into the stratosphere, the remainder coming from gravity waves. An algorithm was developed to determine 3-dimensional atmospheric motion from satellite tracer measurements. Based on Lagrangian constraints, the algorithm circumvents limitations of the traditional scheme for inferring motion from temperature measurements and determines the circulation in the tropics as reliably as elsewhere. A study of deep convection revealed that the highest towers (those penetrating into stratospheric air and controlling tropopause height and composition through convective mixing) occur in close association with the diurnal cycle of convection. Clouds colder than 220 K develop almost entirely in association with the diurnal cycle of convection over tropical landmasses and substantially in association with it even over maritime regions.
author Salby, Murry L.
author_facet Salby, Murry L.
author_sort Salby, Murry L.
title Dynamical and Chemical Behavior of the Lower Stratosphere and Interactions with the Troposphere
title_short Dynamical and Chemical Behavior of the Lower Stratosphere and Interactions with the Troposphere
title_full Dynamical and Chemical Behavior of the Lower Stratosphere and Interactions with the Troposphere
title_fullStr Dynamical and Chemical Behavior of the Lower Stratosphere and Interactions with the Troposphere
title_full_unstemmed Dynamical and Chemical Behavior of the Lower Stratosphere and Interactions with the Troposphere
title_sort dynamical and chemical behavior of the lower stratosphere and interactions with the troposphere
publishDate 1999
url http://hdl.handle.net/2060/19990025898
op_coverage Unclassified, Unlimited, Publicly available
genre polar night
genre_facet polar night
op_source CASI
op_relation Document ID: 19990025898
http://hdl.handle.net/2060/19990025898
op_rights No Copyright
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