Atmospheric Circulation The Coriolis Effect, Winds and Breezes Chapter 22.3.

Slides:



Advertisements
Similar presentations
Wind and Weather.
Advertisements

22.3 Atmospheric Circulation
Bell work Write a poem about moving air. The poem should include an explanation of why air moves.
Wind Notes.
Chapter 16 Section 3: Winds.
Mrs. Wharton’s Science Class
Global and Local Winds.
Global and Local Winds.
Air Earth’s Atmosphere.
Chapter 22 Section 3 Handout
Aim: What are some of Earth’s wind patterns? I. Winds and Pressure Belts A. Convection cell – when air circulates by rising in one place and sinking at.
Wind and the Coriolis Effect
Atmospheric Pressure and Wind
Chapter 22 Section 3 Review
WIND.
Global and Local Winds.
Section 3: Atmospheric Circulation Objectives ◦ Explain the Coriolis effect. ◦ Describe the global patterns of air circulation, and name three global wind.
Key Ideas Explain the Coriolis effect.
Wind coulter.
J. Shevlin April 11, 2012 Eastern Illinois University.
What causes wind? The uneven heating of Earth’s surface by the sun causes temperature differences in air. Warm air rises, creating areas of low pressure.
Unit 10 Lesson 4 Wind in the Atmosphere Copyright © Houghton Mifflin Harcourt Publishing Company.
Chapter 22 Section 3 Review
Winds Chapter 2, Section 3 p What causes wind? Wind: The horizontal movement of air from an area of high pressure to an area of lower pressure.
Welcome to Class Define radiation, convection, and conduction.
Chapter 4 Section 3 Air Movement
Chapter 15: Atmosphere Section 3: Air movement Study Guide.
Wind Why air moves Pressure Belts Moving air Wind is created by differences in air pressure  The greater the difference, the faster the wind moves  The.
Winds. Wind is the horizontal movement of air from an area of high pressure to an area of low pressure. All winds are caused by differences in air pressure.
Chapter 2 Weather Factors Section 3 Winds. What causes wind? Wind: The horizontal movement of air from an area of high pressure to an area of lower pressure.
Atmospheric Circulation
15-3 Atmospheric Pressure and Winds pgs IN: What causes winds?
Wind Read each slide carefully. Make sure pay attention to any diagrams. Complete the questions when finished! 3 3 Air Movement.
Section 3: Atmospheric Circulation
Air Currents in the Atmosphere. Why is it warmer at the equator?
C. 22 Section 3 Atmospheric Circulation Air near Earth’s surface generally flows from the poles toward the equator.
Winds Chapter 2, Section 3, p What Is Wind? Air is a fluid so it can move easily – Winds are caused by differences in air pressure Wind: horizontal.
Wind Notes:.
Global Winds. Air Movement Wind is the movement of air caused by differences in air pressure Wind is the movement of air caused by differences in air.
Wind What are winds?.
Ch. 2 Sec. 3 WINDS. OBJECTIVE #1: Describe the factors that influence wind. OBJECTIVE #2: DISTINGUISH BETWEEN LOCAL AND GLOBAL WINDS AND LOCATE THE MAJOR.
Chapter 10, Section 2 Chapter 22, Section 3. Coriolis Effect The tendency of a moving object to follow a curved path rather than a straight one because.
Heating the Earth Weather is the daily conditions of the atmosphere The factors that interact to cause weather are heat energy, air pressure, winds, and.
Welcome to Class Define radiation, convection, and conduction.
Air Movement (53) Areas of Earth receive different amounts of radiation from the Sun because Earth is curved.
Atmospheric Circulation Earth and Space Science Ms. Pollock
Earth Science Chapter 22 The Atmosphere.
Unit 3 Lesson 3 Wind in the Atmosphere Copyright © Houghton Mifflin Harcourt Publishing Company.
Local and Global Winds. Wind Wind is created by the unequal warming of the Earth (convection currents) Differences in atmospheric pressure cause the movement.
Global and Local Winds. What is Wind? The movement of air caused by differences in air pressure. These differences in air pressure are generally caused.
Journal #35 What is the Coriolis Effect? In which direction does air flow?
Wind Atmospheric Circulation (22:39min). Wind The horizontal movement of air from an area of high pressure to an area of lower pressure. Caused by the.
Chapter 19: The Atmosphere in Motion
Unit 3 Lesson 3 Wind in the Atmosphere
Bell work Write a poem about moving air. The poem should include an explanation of why air moves.
Global winds.
Wind and the Coriolis Effect
Global and Local Winds.
Handout (green) Atmospheric Circulation
Atmospheric Circulation
Global Winds.
Wind and the Coriolis Effect
Wind.
Convection Notes.
Wind and the Coriolis Effect
Global and Local Winds.
Section 3: Atmospheric Circulation
Unit 3 Lesson 3 Wind in the Atmosphere
Wind and the Coriolis Effect
Presentation transcript:

Atmospheric Circulation The Coriolis Effect, Winds and Breezes Chapter 22.3

The Coriolis Effect Air follows a curved path due to the rotation of the Earth. Air follows a curved path due to the rotation of the Earth. The faster an object travels, the greater the Coriolis Effect on the object. The faster an object travels, the greater the Coriolis Effect on the object.

The Coriolis Effect and Wind Wind that blows from increased to decreased pressure curve because of the Coriolis Effect. Wind that blows from increased to decreased pressure curve because of the Coriolis Effect. In the Northern Hemisphere winds curve right. In the Northern Hemisphere winds curve right. In the Southern Hemisphere winds curve south. In the Southern Hemisphere winds curve south. file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual% 20Concepts%20CD/student/ch22/sec03/vc02/hq622_03_v02fs.htm file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual% 20Concepts%20CD/student/ch22/sec03/vc02/hq622_03_v02fs.htm file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual% 20Concepts%20CD/student/ch22/sec03/vc02/hq622_03_v02fs.htm file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual% 20Concepts%20CD/student/ch22/sec03/vc02/hq622_03_v02fs.htm

Global Winds Winds do not flow in a single straight line. Winds do not flow in a single straight line. Each Hemisphere has 3 patterns of air flow (winds). Each Hemisphere has 3 patterns of air flow (winds). Wind Belts: Area of the Earth characterized by winds that flow in one main direction. Wind Belts: Area of the Earth characterized by winds that flow in one main direction. 6 wind belts- 3 in each Hemisphere. 6 wind belts- 3 in each Hemisphere. Winds are named by the direction the wind comes from. Winds are named by the direction the wind comes from.

Trade Winds Winds that flow towards the equator between 30° and 0° latitude. Winds that flow towards the equator between 30° and 0° latitude. N. Hemisphere called Northeast Tradewinds N. Hemisphere called Northeast Tradewinds S. Hemisphere called Southeast Trade Winds. S. Hemisphere called Southeast Trade Winds. Called trade winds because trading ships sailed on these winds during the 18 th and 19 th centuries. Called trade winds because trading ships sailed on these winds during the 18 th and 19 th centuries.

Westerlies Winds that flow between 30° and 60° latitude towards the poles. Winds that flow between 30° and 60° latitude towards the poles. N. Hemisphere- southwest westerlie N. Hemisphere- southwest westerlie S. Hemisphere- northwest westerlie S. Hemisphere- northwest westerlie These winds are felt in the continental U.S. These winds are felt in the continental U.S.

Polar Easterlies Winds that blow from about 60° to 90° (the poles) Winds that blow from about 60° to 90° (the poles) These winds are created by the polar high pressure and are deflected by the Coriolis Effect These winds are created by the polar high pressure and are deflected by the Coriolis Effect Strongest over Antarctica Strongest over Antarctica Where the polar easterlies and the westerlies meet are regions called fronts. Where the polar easterlies and the westerlies meet are regions called fronts.

Doldrums and Horse Latitudes Areas where winds are weak and variable. Areas where winds are weak and variable. Doldrums are where tradewinds from N. and S. Hemisphere meet (at equator). Doldrums are where tradewinds from N. and S. Hemisphere meet (at equator). Horse Latitudes are subtropical high pressure zones around 30° latitude. Horse Latitudes are subtropical high pressure zones around 30° latitude.

Jet Streams Narrow bands of high speed winds that blow high above the surface of the Earth. Narrow bands of high speed winds that blow high above the surface of the Earth. Can affect airline travel Can affect airline travel

The diagram below shows the different wind belts on Earth.

Local Winds Wind we usually feel that cover less than 100 km are called breezes. Wind we usually feel that cover less than 100 km are called breezes. During the day, the land gets hotter faster, and the hot air rises, creating an area of lower pressure. Wind blows from the sea to the land. This is a sea breeze. During the day, the land gets hotter faster, and the hot air rises, creating an area of lower pressure. Wind blows from the sea to the land. This is a sea breeze. At night, the land cools off faster than the sea. Cooler air descends creating an area of higher pressure. Wind blows from the land to the sea. This is a land breeze. At night, the land cools off faster than the sea. Cooler air descends creating an area of higher pressure. Wind blows from the land to the sea. This is a land breeze. file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual%20Conc epts%20CD/student/ch22/sec03/vc03/hq622_03_v03fs.htm file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual%20Conc epts%20CD/student/ch22/sec03/vc03/hq622_03_v03fs.htm file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual%20Conc epts%20CD/student/ch22/sec03/vc03/hq622_03_v03fs.htm file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual%20Conc epts%20CD/student/ch22/sec03/vc03/hq622_03_v03fs.htm

file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual% 20Concepts%20CD/student/ch22/sec03/vc04/hq622_03_v04fs.htm file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual% 20Concepts%20CD/student/ch22/sec03/vc04/hq622_03_v04fs.htm file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual% 20Concepts%20CD/student/ch22/sec03/vc04/hq622_03_v04fs.htm file:///B:/Earth%20Science/Earth%20Science%20Resourse/Visual% 20Concepts%20CD/student/ch22/sec03/vc04/hq622_03_v04fs.htm