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Welcome to Class Define radiation, convection, and conduction

Welcome to Class Define radiation, convection, and conduction

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Today’s Agenda Quiz Wind/Convection Cell Notes Wind Presentations Coriolis Effect –Demos Movie

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Page 1: Welcome to Class Define radiation, convection, and conduction

Welcome to Class

Define radiation, convection, and conduction

Page 2: Welcome to Class Define radiation, convection, and conduction

• Radiation – energy from the sun– Come from fire, sun, heat lamp

• Conduction – heat transfer by touching

• Convection – hot rises, cold sinks– Cycle– Substance moves (water, wind)

Page 3: Welcome to Class Define radiation, convection, and conduction

Today’s Agenda

• Quiz• Wind/Convection Cell Notes• Wind Presentations• Coriolis Effect

– Demos• Movie

Page 4: Welcome to Class Define radiation, convection, and conduction

Seasons Review

• Earth is tilted at 23.5 degrees

• Earth points away from the sun in winter

• Earth points towards the sun in summer

• New Vocab

Page 5: Welcome to Class Define radiation, convection, and conduction

WIND

Page 6: Welcome to Class Define radiation, convection, and conduction

Convection Cells

• Cold air is more dense than warm air– Hot/warm air rises– Causes convection and wind

• Convection cells (Hadley Cells) AND the rotation of the Earth create wind

Page 7: Welcome to Class Define radiation, convection, and conduction

How Convection Cells Work• Warm air rises at the equator

– Spreads out• The poles are cooler and the air sinks• Sinking air fills in the void where the warm

air rose

Page 8: Welcome to Class Define radiation, convection, and conduction

Importance of Convection Cells

• 3 cells in each hemisphere

Page 9: Welcome to Class Define radiation, convection, and conduction

Climate and Convection Cells

• A cell about every 30o

• Warm moist air rises in the tropics = rainfall

• Cool, dry air descends at subtropical latitudes = deserts

Page 10: Welcome to Class Define radiation, convection, and conduction
Page 11: Welcome to Class Define radiation, convection, and conduction

Global Winds and Weather

• Each hemisphere contains three convection cells

• Each convection cell correlates to an area of Earth’s surface, called a wind belt– characterized by winds flowing in one

direction – prevailing winds

Page 12: Welcome to Class Define radiation, convection, and conduction
Page 13: Welcome to Class Define radiation, convection, and conduction

Wind Presentations• You and your group will present 1 of the

winds

• You will need to present them to the class– The rest of the class will need to take notes

• You will need to come up with 1 question (and answer) to put on a test/quiz

• Page 562

Page 14: Welcome to Class Define radiation, convection, and conduction

• Land and Sea Breezes• Mountain and Valley Breezes• Jet Streams• Doldrums and Horse Latitudes• Polar Easterlies• Westerlies• Trade Winds

Page 15: Welcome to Class Define radiation, convection, and conduction

Trade Winds• trade wind - prevailing winds that blow from

east to west from 30º latitude to the equator in both hemispheres

• Like all winds, trade winds are named according to the direction from which they flow

• In the Northern Hemisphere, they are the northeast trade winds

• In the Southern Hemisphere, they are the southeast trade winds

Page 16: Welcome to Class Define radiation, convection, and conduction

Global Winds• westerlies - prevailing winds that blow from west

to east between 30º and 60º latitude in both hemispheres

• Between 30º and 60º latitude, some of the descending air moving toward the poles is deflected by the Coriolis effect

• In the Northern Hemisphere, the westerlies are the southwest winds– In the Southern Hemisphere, they are the northwest

winds

Page 17: Welcome to Class Define radiation, convection, and conduction

Global Winds

• polar easterlies prevailing winds that blow from east to west between 60 and 90 latitude in both hemispheres

• Surface winds created by the polar high pressure are deflected by the Coriolis effect and become the polar easterlies

• Where the polar easterlies meet warm air from the westerlies, a stormy region known as a front forms

Page 18: Welcome to Class Define radiation, convection, and conduction

The Doldrums and Horse Latitudes

• The trade wind systems of the Northern Hemisphere and Southern Hemisphere meet at the equator in a narrow zone called the doldrums

• As the air approaches 30º latitude, it descends and a high-pressure zone forms. These subtropical high-pressure zones are called horse latitudes

• surface winds are weak and variable in both of these zones.

Page 19: Welcome to Class Define radiation, convection, and conduction

Wind and Pressure Shifts• As the sun’s rays shift northward and southward during

the changing seasons of the year, the positions of the pressure belts and wind belts shift

• Although the area that receives direct sunlight can shift by up to 46 º north and south of the equator, the average shift for the pressure belts and wind belts is only about 10º of latitude

• However, even this small change causes some areas of Earth’s surface to be in different wind belts during different times of the year

Page 20: Welcome to Class Define radiation, convection, and conduction

Jet Streams• jet streams a narrow band of strong winds that

blow in the upper troposphere– exist in the Northern and Southern Hemisphere

• One jet stream is the polar jet stream– reach speeds of 500 km/h– affect airline routes and the paths of storms

• A second jet stream is a subtropical jet stream

Page 21: Welcome to Class Define radiation, convection, and conduction

Local Winds

• Movement of air are also influenced by local conditions, and local temperature variations commonly cause local winds

• Local winds are not part of the global wind belts.

• Gentle winds that extend over distances of less than 100 km are called a breeze.

Page 22: Welcome to Class Define radiation, convection, and conduction

Land and Sea Breezes

• Equal areas of land and water may receive the same amount of energy from the sun. However, land surfaces heat up faster than water surfaces do.

• The cool wind moving from water to land is called a sea breeze

• Overnight, the land cools more rapidly than water does, and the sea breeze is replaced by a land breeze

Page 23: Welcome to Class Define radiation, convection, and conduction

Mountain and Valley Breezes• A valley breeze forms when warm air from the

valleys moves upslope

• At night, the mountains cool more quickly than the valleys do. At that time, cool air descends from the mountain peaks to create a mountain breeze

• Areas near mountains may experience a warm afternoon that turns to a cold evening soon after sunset

Page 24: Welcome to Class Define radiation, convection, and conduction

Coriolis Effect

• Coriolis effect - curving of the path of a moving object from an otherwise straight path due to Earth’s rotation

• Detectable only on objects that move very fast or that travel over long distances– Oceans, Atmosphere, planes

Page 25: Welcome to Class Define radiation, convection, and conduction
Page 26: Welcome to Class Define radiation, convection, and conduction