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Wind Driven Circulation I: Planetary boundary Layer near the sea surface

Wind Driven Circulation I: Planetary boundary Layer near the sea surface

Wind Driven Circulation I: Planetary boundary Layer near the sea surface. Monin-Obukhoff Similarity Theory. Surface layer (several tens of meters above surface, 10-15% of the planetary boundary layer) in nearly steady condition Vertical turbulent flux is nearly constant

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237 views • 23 slides
Wind Driven Circulation I: Planetary boundary Layer near the sea surface

Wind Driven Circulation I: Planetary boundary Layer near the sea surface

Wind Driven Circulation I: Planetary boundary Layer near the sea surface. Monin-Obukhoff Similarity Theory. Surface layer (several tens of meters above surface, 10-15% of the planetary boundary layer) in nearly steady condition Vertical turbulent flux is nearly constant

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559 views • 21 slides
Wind Driven Circulation I: Planetary boundary Layer near the sea surface

Wind Driven Circulation I: Planetary boundary Layer near the sea surface

Wind Driven Circulation I: Planetary boundary Layer near the sea surface. Monin-Obukhoff Similarity Theory. Surface layer (several tens of meters above surface, 10-15% of the planetary boundary layer) in nearly steady condition Vertical turbulent flux is nearly constant

★ ★ ★ ★ ★

229 views • 21 slides
Wind Driven Circulation I: Planetary boundary Layer near the sea surface

Wind Driven Circulation I: Planetary boundary Layer near the sea surface

Wind Driven Circulation I: Planetary boundary Layer near the sea surface. Monin-Obukhoff Similarity Theory. Surface layer (several tens of meters above surface, 10-15% of the planetary boundary layer) in nearly steady condition Vertical turbulent flux is nearly constant

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218 views • 21 slides
The ? -spiral Determining absolute velocity from density field

The ? -spiral Determining absolute velocity from density field

The ? -spiral Determining absolute velocity from density field. Assumptions: 1) Geostrophic. 2) incompressible. 3) steady state. 2) + 3) ?. Use the thermal wind equation with Boussinesq approximation. Take into. Write u and v to polar format as. In the northern hemisphere,

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201 views • 19 slides

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