12.003 Physics of Atmospheres and Oceans, Fall 2007

The laws of classical mechanics and thermodynamics are used to explore how the properties of fluids on a rotating Earth manifest themselves in, and help shape, the global patterns of atmospheric winds, ocean currents, and the climate of the Earth. Theoretical discussion focuses on the physical proce...

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Main Author: Marshall, John C.
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Learning Object
Language:en-US
Published: 2007
Subjects:
Online Access:http://hdl.handle.net/1721.1/47288
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author Marshall, John C.
author2 Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
author_facet Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Marshall, John C.
author_sort Marshall, John C.
collection MIT
description The laws of classical mechanics and thermodynamics are used to explore how the properties of fluids on a rotating Earth manifest themselves in, and help shape, the global patterns of atmospheric winds, ocean currents, and the climate of the Earth. Theoretical discussion focuses on the physical processes involved. Underlying mechanisms are illustrated through laboratory demonstrations, using a rotating table, and through analysis of atmospheric and oceanic data.
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spelling mit-1721.1/472882025-02-26T17:35:06Z 12.003 Physics of Atmospheres and Oceans, Fall 2007 Physics of Atmospheres and Oceans Marshall, John C. Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Characteristics of the atmosphere global energy balance greenhouse effect greenhouse gases Atmospheric layers pressure and density Convection adiabatic lapse rate Humidity Convective clouds Temperature Pressure and geopotential height Winds Fluids in motion Hydrostatic balance Incompressible flow compressible flow radial inflow Geostrophic motion Taylor-Proudman Theorem Ekman layer Coriolis force Rossby number Hadley circulation ocean seawater salinity geostrophic and hydrostatic balance inhomogeneity Abyssal circulation thermohaline circulation The laws of classical mechanics and thermodynamics are used to explore how the properties of fluids on a rotating Earth manifest themselves in, and help shape, the global patterns of atmospheric winds, ocean currents, and the climate of the Earth. Theoretical discussion focuses on the physical processes involved. Underlying mechanisms are illustrated through laboratory demonstrations, using a rotating table, and through analysis of atmospheric and oceanic data. 2007-12 Learning Object 12.003-Fall2007 local: 12.003 local: IMSCP-MD5-87c60b72bfdf4b8ba03babd7732b1a15 http://hdl.handle.net/1721.1/47288 en-US Usage Restrictions: This site (c) Massachusetts Institute of Technology 2003. Content within individual courses is (c) by the individual authors unless otherwise noted. The Massachusetts Institute of Technology is providing this Work (as defined below) under the terms of this Creative Commons public license ("CCPL" or "license"). The Work is protected by copyright and/or other applicable law. Any use of the work other than as authorized under this license is prohibited. By exercising any of the rights to the Work provided here, You (as defined below) accept and agree to be bound by the terms of this license. The Licensor, the Massachusetts Institute of Technology, grants You the rights contained here in consideration of Your acceptance of such terms and conditions. text/html Fall 2007
spellingShingle Characteristics of the atmosphere
global energy balance
greenhouse effect
greenhouse gases
Atmospheric layers
pressure and density
Convection
adiabatic lapse rate
Humidity
Convective clouds
Temperature
Pressure and geopotential height
Winds
Fluids in motion
Hydrostatic balance
Incompressible flow
compressible flow
radial inflow
Geostrophic motion
Taylor-Proudman Theorem
Ekman layer
Coriolis force
Rossby number
Hadley circulation
ocean
seawater
salinity
geostrophic and hydrostatic balance
inhomogeneity
Abyssal circulation
thermohaline circulation
Marshall, John C.
12.003 Physics of Atmospheres and Oceans, Fall 2007
title 12.003 Physics of Atmospheres and Oceans, Fall 2007
title_full 12.003 Physics of Atmospheres and Oceans, Fall 2007
title_fullStr 12.003 Physics of Atmospheres and Oceans, Fall 2007
title_full_unstemmed 12.003 Physics of Atmospheres and Oceans, Fall 2007
title_short 12.003 Physics of Atmospheres and Oceans, Fall 2007
title_sort 12 003 physics of atmospheres and oceans fall 2007
topic Characteristics of the atmosphere
global energy balance
greenhouse effect
greenhouse gases
Atmospheric layers
pressure and density
Convection
adiabatic lapse rate
Humidity
Convective clouds
Temperature
Pressure and geopotential height
Winds
Fluids in motion
Hydrostatic balance
Incompressible flow
compressible flow
radial inflow
Geostrophic motion
Taylor-Proudman Theorem
Ekman layer
Coriolis force
Rossby number
Hadley circulation
ocean
seawater
salinity
geostrophic and hydrostatic balance
inhomogeneity
Abyssal circulation
thermohaline circulation
url http://hdl.handle.net/1721.1/47288
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