Robert Fovell rfovell@albany.edu Meteorology – Lecture 6 Robert Fovell rfovell@albany.edu.

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Robert Fovell rfovell@albany.edu Meteorology – Lecture 6 Robert Fovell rfovell@albany.edu

Important notes These slides show some figures and videos prepared by Robert G. Fovell (RGF) for his “Meteorology” course, published by The Great Courses (TGC). Unless otherwise identified, they were created by RGF. In some cases, the figures employed in the course video are different from what I present here, but these were the figures I provided to TGC at the time the course was taped. These figures are intended to supplement the videos, in order to facilitate understanding of the concepts discussed in the course. These slide shows cannot, and are not intended to, replace the course itself and are not expected to be understandable in isolation. Accordingly, these presentations do not represent a summary of each lecture, and neither do they contain each lecture’s full content.

Animations linked in the PowerPoint version of these slides may also be found here: http://people.atmos.ucla.edu/fovell/meteo/

Pressure

Picture a vertical cross-section

Isobar = line of equal pressure Here are 1000 and 500 mb isobars

Half of the atmospheric mass is found in between…

Only 5.5 km/3.5 mi thick… on average

Temperature affects the thickness of this layer

Temperature affects the thickness of this layer Pressure decreases with height… faster in colder air

Temperature differences make pressure differences

Start with the same thickness everywhere Start with the same thickness everywhere. This implies temperature is the same

Introduce a T difference Introduce a T difference. The 500 mb isobar is now tilted down towards the colder air

Pick a point along the 500 mb isobar Pick a point along the 500 mb isobar. Do you see a horizontal pressure difference?

Pressure differences make winds. Nature wants to move mass from H to L Pressure differences make winds. Nature wants to move mass from H to L. Wind! But we’re not done…

This wind (mass flow) has consequences... Transport of mass (air) out of the warmer column causes its surface pressure to drop. That mass collects in the colder column, making its surface pressure to rise.

So the 1000 mb isobar is now tilted as well. Now we have a circulation. The circulation is called thermally direct. Notice at the surface the flow is cold towards warm.

Apply to the sea-breeze

We start with ocean and land

Which surface absorbs more solar radiation during the day? The ocean does, because it’s darker than land when the sun is high in the sky. But, the ocean doesn’t heat up much during the day.

The sea-breeze circulation Warm air rising over the heated land Cool air sinking over the cooler ocean The surface sea-breeze blowing inland It’s about 1-2 km deep or so We label winds by where they come from. A sea-breeze blows from sea to land

Example: Los Angeles sea-breeze Colored field is surface temperature (green = cool; red = hot) Greens cool… reds will be hot Vectors are surface winds For 12Z August 1 NOON in London 5AM PDT Cool everywhere Winds are weak

Example: Los Angeles sea-breeze By 19Z… Noon in LA Land’s warmed up a lot Little temperature rise over the sea… thermal inertia Winds have increased Blowing sea to land

Example: Los Angeles sea-breeze 00Z August 2… midnight in London… 5PM August 1 in LA The wind vector LENGTH indicates wind speed Winds a lot stronger now Very hot inland, especially SFV The cool sea air is keeping UCLA a lot cooler

Example: Los Angeles sea-breeze After sunset the land cools off quickly (low thermal inertia) And as the temperature difference disappears, the winds die down Warmest in SFV; sea-breeze reaches there last and is weakest If land becomes colder at night, a land-breeze may develop

Sea- and land-breezes

Wind chill

Consider a familiar example: hot soup in a cool room

The soup loses heat energy to the room air via conduction

This warms up the air in contact with the soup This warms up the air in contact with the soup. Air, a poor conductor, does not carry this heat energy vertically away efficiently

As a result, the soup-air T difference DECREASES As a result, the soup-air T difference DECREASES. This decreases the heat loss. The air is actually acting as an INSULATING BLANKET helping to keep the soup warm

BLOW that insulating blanket away, replacing it with more cool air BLOW that insulating blanket away, replacing it with more cool air. Temperature difference is again LARGER and the heat loss has increased. The soup has been subjected to wind chill

Descending and ascending air

DESCENDING AIR Descending air warms at a RAPID RATE 10C/km ~ 30F/mi Temperature change due to VOLUME CHANGE ALONE There is NO heat transfer “Dry adiabatic” Ascending air cools at that same rate, at least at first!

“Santa Ana” winds

Topography of Southwestern US

Colored field: density of the air at 850 mb level (about 1 Colored field: density of the air at 850 mb level (about 1.5 km or 1 mi above sea-level.) Red = less dense, blue = more dense

For animation, see http://people.atmos.ucla.edu/fovell/meteo/ Added 850 mb wind vectors. At this time, the air in Southern California has low density and LA has a seabreeze

“Santa Ana” winds become warm (or hot) owing to elevation change

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