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Surface winds An air parcel initially at rest will move from high pressure to low pressure (pressure gradient force) Geostrophic wind blows parallel to.
Documents Surface winds An air parcel initially at rest will move from high pressure to low pressure (pressure...

Slide 1 Surface winds An air parcel initially at rest will move from high pressure to low pressure (pressure gradient force) Geostrophic wind blows parallel to the isobars…

Vorticity. The Law of conservation of Vorticity Relative vorticity is defined as The time rate of change of vorticity can be written by taking the equations.
Documents Vorticity. The Law of conservation of Vorticity Relative vorticity is defined as The time rate of...

Slide 1 Vorticity Slide 2 The Law of conservation of Vorticity Relative vorticity is defined as The time rate of change of vorticity can be written by taking the equations…

Ocean & Atmospheric circulation redux 1) Unequal planetary heating creates pressure gradients which make winds blow on ocean surface in trade-wind & westerly.
Documents Ocean & Atmospheric circulation redux 1) Unequal planetary heating creates pressure gradients which....

Slide 1 Ocean & Atmospheric circulation redux 1) Unequal planetary heating creates pressure gradients which make winds blow on ocean surface in trade-wind & westerly…

AOSS 401, Fall 2006 Lecture 19 October 26, 2007 Richard B. Rood (Room 2525, SRB) rbrood@umich.edu 734-647-3530 Derek Posselt (Room 2517D, SRB) dposselt@umich.edu.
Documents AOSS 401, Fall 2006 Lecture 19 October 26, 2007 Richard B. Rood (Room 2525, SRB) [email protected]...

AOSS 401, Fall 2006 Lecture 19 October 26, 2007 Richard B. Rood (Room 2525, SRB) [email protected] 734-647-3530 Derek Posselt (Room 2517D, SRB) [email protected] 734-936-0502…

Modeling Deep Convective Zonal Flows on the Giant Planets Jonathan Aurnou UCLA Earth & Space Sciences aurnou@ucla.edu Cassini Image.
Documents Modeling Deep Convective Zonal Flows on the Giant Planets Jonathan Aurnou UCLA Earth & Space...

Modeling Deep Convective Zonal Flows on the Giant Planets Jonathan Aurnou UCLA Earth & Space Sciences [email protected] Cassini Image Acknowledgements Moritz Heimpel University…

AOSS 401, Fall 2006 Lecture 19 October 26 , 2007
Documents AOSS 401, Fall 2006 Lecture 19 October 26 , 2007

AOSS 401, Fall 2006 Lecture 19 October 26, 2007 Richard B. Rood (Room 2525, SRB) [email protected] 734-647-3530 Derek Posselt (Room 2517D, SRB) [email protected] 734-936-0502…

Intrinsic Errors in Physical Ocean Climate Models Matthew Hecht Los Alamos National Laboratory.
Documents Intrinsic Errors in Physical Ocean Climate Models Matthew Hecht Los Alamos National Laboratory.

Intrinsic Errors in Physical Ocean Climate Models Matthew Hecht Los Alamos National Laboratory Satellite observation of sea surface temperature Climate simulations low resolution:…

Modeling Deep Convective Zonal Flows on the Giant Planets
Documents Modeling Deep Convective Zonal Flows on the Giant Planets

Modeling Deep Convective Zonal Flows on the Giant Planets Jonathan Aurnou UCLA Earth & Space Sciences [email protected] Cassini Image Acknowledgements Moritz Heimpel University…

Complex 2D Fields: Analysis of Eddies in the Southern Indian Ocean
Documents Complex 2D Fields: Analysis of Eddies in the Southern Indian Ocean

Eddies in the Agulhas Current Background Info Complex 2D Fields: Analysis of Eddies in the Southern Indian Ocean Project Leader: Greta Leber Joni Lum Changheng Chen David…

Q-G vorticity equation Q-G thermodynamic equation We now have two equations in two unknowns, and We will solve these to find an equation for , the.
Documents Q-G vorticity equation Q-G thermodynamic equation We now have two equations in two unknowns, and .....

Slide 1 Q-G vorticity equation Q-G thermodynamic equation We now have two equations in two unknowns,  and  We will solve these to find an equation for , the vertical…

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