lecture #2 weather. convection and atmospheric pressure much of solar energy absorbed by the earth...

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Lecture #2 Weather

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Page 1: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Lecture #2

Weather

Page 2: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Convection and Atmospheric Pressure

• Much of solar energy absorbed by the Earth is used to evaporate water.– Energy stored in water vapor as latent heat.– When water vapor condenses, heat energy is

released.– Heat and water move from warmer areas near the

equator towards cooler areas at poles. Heat redistribution prevents extreme temperature fluctuation.

Page 3: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Circulation Patterns

Page 4: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Convection Currents

• Releasing latent heat causes air to rise, cool, and lose more water vapor as precipitation.

• Warm air close to equator vs. cold air at poles also produces pressure differences that cause weather.– Air near surface warms and becomes less dense

than the air above it; rises above cool air creating vertical convection currents.• Low pressure - air is rising• High pressure - air is sinking

– Pressure differences cause winds.

Page 5: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Convection Currents

Page 6: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Weather Happens

• Weather - physical conditions in the atmosphere (humidity, temperature, air pressure, wind and precipitation) over short time scales– Rain• Air cools as it rises, and water condenses as air

cools.• Cooling occurs because pressure decreases as

air rises.• Condensation nuclei (tiny particles) must also

be present to have precipitation.

Page 7: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Coriolis Effect

• As air warms at the equator, rises, and moves northward, it sinks and rises in several intermediate bands, forming circulation cells.– Surface flows do not move straight north and

south, but are deflected due to Coriolis effect. The curving pattern results from the fact that the earth rotates in an eastward direction as winds move above it.

– Winds and currents move clockwise in Northern Hemisphere and counterclockwise in the Southern Hemisphere.

Page 8: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Coriolis Effect

• Major zones of subsidence occur at about 30o North and South latitude.– Where dry, subsiding air falls on continents, it

creates subtropical deserts.

• On a regional scale, the Coriolis effect produces cyclonic winds, which spiral clockwise out of an area of high pressure in the Northern Hemisphere and counterclockwise into an area of low pressure. You can see these on weather maps.

Page 9: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Jet Streams• Jet streams - hurricane

force winds at the top of the trophosphere which follow an undulating path

Page 10: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Ocean Currents

• Warm and cold ocean currents strongly influence climate conditions on land.– As surface water moves, deep water wells up to

replace it.• Ocean circulation also driven by differences in

water density due to temperature and saltiness of water–Gyres - huge cycling currents carrying water

north and south–Currents can shift abruptly.

Page 11: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water
Page 12: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Seasonal Winds and Monsoons

• Monsoon - seasonal reversal of wind patterns caused by differential heating and cooling rates of oceans and continents– Most prevalent in subtropical and tropical areas.– Tilt of Earth’s axis changes location where the Sun is

most intense over the course of the year. Places where the Sun shines most directly have evaporation and convection currents which bring thunderstorms.

– Seasonal rains support tropical forests and fill great rivers such as Ganges and Amazon.

Page 13: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Frontal Weather• Cold Front - boundary formed when cooler air

displaces warmer air – Cold air is more dense, thus hugs ground and

pushes warm air up.• Warm air cooled adiabatically (without loss or

gain of energy), precipitation.• Warm Front - boundary formed when warm air

displaces cooler air– Warm air is less dense and slides over cool air,

creating a long wedge-shaped band of clouds and precipitation.

Page 14: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water
Page 15: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Cyclonic Storms

• When rising air is laden with water vapor, latent energy released by condensation intensifies convection currents and draws up more warm air and water vapor.– Storm cell will exist as long as temperature

differential exists.• Hurricanes (Atlantic)–Katrina in 2005 caused greatest natural disaster

in North American history.• Typhoons (Western Pacific)• Cyclones (Indian Ocean)

Page 16: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Cyclonic Storms

• Tornadoes - swirling funnel clouds– Rotation not generated by Coriolis forces– Generated by “supercell” frontal systems where

strong dry cold fronts collide with warm humid air• Greater air temperature differences in the

spring, thus more tornadoes– Downbursts - disorganized supercells that cause

downdrafts and straight line winds

Page 17: Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water

Cyclonic Storms