Chapter 8 Wind and Weather. Wind –The local motion of air relative to the rotating Earth Wind is measured using 2 characteristics –Direction (wind sock)

Slides:



Advertisements
Similar presentations
What we now know: Difference between weather and climate.
Advertisements

Atmospheric Circulation and Weather Systems
Wind and Weather.
Factors Affecting Wind
Chapter 6: Air Pressure and Winds
Chapter 16 Section 3: Winds.
The General Circulation of the Atmosphere
Chapter 4. Atmospheric Pressure and Wind
Chapter 13 The Atmosphere in Motion
What Makes the Wind Blow?
Air Pressure and Winds III
Air pressure and atmospheric motion
Visualizing Physical Geography Copyright © 2008 John Wiley and Sons Publishers Inc. Chapter 5 Winds and Global Circulation.
Visualizing Physical Geography Copyright © 2008 John Wiley and Sons Publishers Inc. Chapter 5 Winds and Global Circulation Visualizing Physical Geography.
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 Wind is movement of air caused by differences in air pressure.
How Does Air Move Around the Globe?
The General Circulation of the Atmosphere
General Circulation and Kinetic Energy
Chapter 7 Atmospheric Pressure and Wind
Chapter 10: Atmospheric Dynamics
What Makes the Wind Blow? ATS 351 Lecture 8 October 26, 2009.
Atmospheric Circulation
Atmospheric Pressure and Wind. Atmospheric pressure: –force exerted by a column of air per unit area –Normal atmospheric pressure at sea level = 1013.
Air Pressure and Winds Dr. R. B. Schultz. Air Pressure Air pressure is the pressure exerted by the weight of air above. Average air pressure at sea level.
Warning! In this unit, we switch from thinking in 1-D to 3-D on a rotating sphere Intuition from daily life doesn’t work nearly as well for this material!
EARTH SCIENCE Air Pressure and Wind.
General Atmospheric Circulation
Atmospheric Force Balances
Class #13 Monday, September 27, 2010 Class #13: Monday, September 27 Chapter 7 Global Winds 1.
What Causes the Wind Worksheet.
Air Pressure and Wind Pgs. D52-D61.
Force Balance (Chap. 6) ATM100. Topics of the Day ◦ Review Test 1 ◦ Newton’s Laws of Motion ◦ Review of vectors and forces ◦ Forces that act to move the.
General Circulation of the Atmosphere Lisa Goddard 19 September 2006.
Atmospheric pressure and winds
Guided Notes for Weather Systems
Basic Meteorology Concepts. Spheres of the Earth.
The Atmosphere in Motion Chapter 18
What set the atmosphere in motion?. Review of last lecture Thickness of the atmosphere: less than 2% of Earth’s thickness Thickness of the atmosphere:
Science News. What is WIND? The horizontal motion of air across Earth’s surface; movement produced by differences in air pressure from an area of high.
Planetary Atmospheres, the Environment and Life (ExCos2Y) Topic 6: Wind Chris Parkes Rm 455 Kelvin Building.
Chapter 6 Atmospheric Forces and Wind
Lecture 14 4 February 2005 Atmospheric and Oceanic Circulations (continued) Chapter 6.
Global Wind Patterns.
Air Pressure and Winds. Atmospheric Pressure  What causes air pressure to change in the horizontal?  Why does the air pressure change at the surface?
Winds Professor Jeff Gawrych De Anza College. Principle forces Q: What drives the weather in the atmosphere? The uneven heating of the earth Q: What causes.
What set the atmosphere in motion?
Chapter 6: Air Pressure and Winds Atmospheric pressure Atmospheric pressure Measuring air pressure Measuring air pressure Surface and upper-air charts.
C. 22 Section 3 Atmospheric Circulation Air near Earth’s surface generally flows from the poles toward the equator.
How Does Air Move Around the Globe?
The Wind: PGF Pressure gradient force is what sets air in motion
MET 10 1 The General Circulation of the Atmosphere.
Chapter 8 Wind and Weather. Wind –The local motion of air relative to the rotating Earth Wind is measured using 2 characteristics –Direction (wind sock)
1 0º Equator90º Pole LP HP  At the Equator the atmosphere is heated  Air becomes less dense and rises.  Rising air creates low pressure at the equator.
Isobars and wind barbs sea level pressure. factors affecting wind wind is the result of horizontal differences in pressure air flows from higher to lower.
19 Chapter 19 Air Pressure and Wind. Air Pressure Defined 19.1 Understanding Air Pressure  Air pressure is the pressure exerted by the weight of air.
Class #17 Monday, February 16, Class #17: Monday, February 16 Surface pressure and winds Vertical motions Jet streams aloft.
Weather Basics Air Pressure and Winds. Air Pressure Air has a mass and exerts a force called atmospheric pressure Air pressure is measured in millibars.
PRESSURE & WIND, GENERAL CIRCULATION, JET STREAMS.
Atmospheric Pressure and Wind
Understanding Weather and Climate 3rd Edition Edward Aguado and James E. Burt Anthony J. Vega.
Lecture on Atmospheric Pressure
1. What does “stability” mean in the atmosphere. 2
PRESSURE & WIND, GENERAL CIRCULATION, JET STREAMS
Chapter 6: Air Pressure and Winds
Chapter 8 Air Pressure and Winds.
Chapter 10 Wind: Global Systems.
Project Atmosphere American Meteorological Society
Isobars and wind barbs sea level pressure.
Presentation transcript:

Chapter 8 Wind and Weather

Wind –The local motion of air relative to the rotating Earth Wind is measured using 2 characteristics –Direction (wind sock) N, NNE, NE, ENE, E, ESE, SE, SSE, S, etc… Degrees: N = 360 o, E = 90 o, S = 180 o, W = 270 o –Speed (anemometer)

What Causes Wind? Newton’s 2 nd Law of Motion –F = m*a (force = mass * acceleration) Air is at rest, what forces cause it to accelerate? –Pressure gradient force –Centripetal force –Coriolis effect –Friction –Gravity

Pressure Gradient Force (PGF) Same concept as 2 nd Law of Thermodynamics (heat flows from hot to cold objects to eliminate temperature gradient) Horizontal pressures are not equal – therefore there is a gradient PGF –The force that causes air parcels to move as a consequence of an air pressure gradient –Wind is greater where pressure gradient is larger

Centripetal Force Center seeking force The net force is directed inward  toward the center of the orbit and perpendicular to the direction of motion This force operates when an air parcel follows a curved path It is NOT and independent force – it is the result of the imbalance of other forces Causes a change in direction, but not speed

Coriolis Effect It is a net force responsible for curved motion due to changing the coordinate system from non- rotating to rotating Deflects winds to the right (left) in the NH (SH) Coriolis is dependent on latitude –No deflection at equator/Max deflection at poles Coriolis is dependent on wind speed and spatial scale (size and distance)

Friction Friction: the resistance that an object or medium encounters as it moves in contact with another object or medium Friction acts opposite to the wind direction Friction increases with increasing surface roughness –Greater over a forest than a soybean field Friction slows horizontal winds in the lowest kilometer (Sea Breeze)

Gravity Force of gravity is 9.8m/s 2 Always directed downward –Does not modify horizontal winds

Joining Forces These 5 forces all interact to govern the direction and speed of the wind These interactions result in 4 cases –Hydrostatic Equilibrium –Geostrophic Wind –Gradient Wind –Surface Winds

Hydrostatic Equilibrium Balance of the vertical pressure gradient force and gravity Since a balance is in place the net acceleration is zero Parcels that are moving move at a constant speed

Geostrophic Wind Unaccelerated (constant speed) horizontal wind Balance between coriolis effect and horizontal pressure gradient Only develops in large scale systems Frictionless

Gradient Wind Similar to geostrophic wind in that it is a large scale, horizontal, frictionless wind that blows parallel to the isobars The difference is that the path of the gradient wind is curved Forces are not balanced –There is a net centripetal force Develops around highs and lows

Surface Winds Friction at the surface affects speed and direction of wind Friction acts directly opposite the wind direction Friction slows wind speed, which weakens the Coriolis effect and affects balance with the horizontal pressure gradient force causing winds to blow towards low pressure Friction loses influence with height

Scales of Weather Systems CirculationSpace ScaleTime ScaleExample Planetary10, ,000km Weeks to months Trade winds Synoptic ,000km Days to week Hurricanes, air masses Mesoscale1-100kmHours to dayT-storms Microscale1m-1kmSeconds to hour Weak tornado

© AMS21 Idealized Circulation Pattern To start with, assume a non- rotating Earth Also assume a uniform solid surface Sun heats the equatorial regions more intensely than the poles; a temperature gradient develops Convection cell forms when cold, dense air sinks at the poles and flows at the surface toward the equator, where it forces warm, less dense air to rise. Aloft, equatorial air flows toward the poles.

© AMS22 Idealized Circulation Pattern If the idealized planet starts to rotate from west to east, the Coriolis Effect comes into play Northern Hemisphere surface winds are diverted to the right and blow toward the southwest Southern Hemisphere surface winds are diverted to the left and blow toward the northwest Winds blow counter to planet’s direction of rotation

© AMS23 Idealized Circulation Pattern Circulation is maintained in the atmosphere of our idealized Earth because the planetary-scale winds split into 3 belts in each hemisphere 3 belts are: –0 ° to 30 ° –30 ° to 60 ° –60 ° to 90 ° Now some winds blow with and some blow against the planet’s rotation

© AMS24 Idealized Circulation Pattern Surface winds converge along the equator and along 60° latitude circles –Convergence leads to rising air, expansional cooling, cloud development and precipitation –Convergence zones are belts of relatively low surface air pressure Surface winds diverge at the poles and along the 30° latitude circles –Air descends, is compressed and warms, and weather is generally fair –Divergence zones are belts of relatively high surface air pressure

© AMS25 Features of the Planetary-Scale Circulation Schematic representation of the planetary-scale surface circulation of the atmosphere

© AMS26 Features of the Planetary-Scale Circulation Winds Aloft –Aloft, winds in the middle and upper troposphere blow away from the ITCZ –These feed into the subtropical highs –Resulting convection cells are called Hadley cells

© AMS27 Winds Aloft, continued –Aloft in middle latitudes, winds blow from west to east in a wavelike pattern of ridges and troughs –These winds are responsible for the movement of the synoptic-scale weather systems –Their north/south components contribute to poleward heat transport Features of the Planetary-Scale Circulation

© AMS28 Waves in the Westerlies Zonal and Meridional Flow Patterns –Westerlies have 2 components: North-south airflow is the meridional component West-to-east airflow is the zonal component –If north-south component is weak, the result is a zonal flow pattern North-south exchange of air masses is minimal –If flow is in a pattern of deep troughs and sharp ridges, the result is a meridional flow pattern Greater temperature contrasts develop across the U.S. and southern Canada Stage is set for development of extra-tropical cyclones –If northern westerlies have a wave configuration differing from the southern westerlies, a complicated split flow pattern may exist

© AMS29 Zonal and Meridional Flow –These two images illustrate extremes of zonal and meridional flow –Westerlies generally shift back and forth between zonal and meridional flow –There is no regularity to this shift –The affects long-range weather forecasting accuracy Waves in the Westerlies