Geography Review Exam I

Similar documents
Winds and Global Circulation

Week: Dates: 3/2 3/20 Unit: Climate

Divergence, Spin, and Tilt. Convergence and Divergence. Midlatitude Cyclones. Large-Scale Setting

Atmospheric Circulation

Science 1206 Chapter 1 - Inquiring about Weather

Weather Notes. Chapter 16, 17, & 18

Wind: Global Systems Chapter 10

Fluid Circulation Review. Vocabulary. - Dark colored surfaces absorb more energy.

CHAPTER 6 Air-Sea Interaction Pearson Education, Inc.

Meteorology Practice Test

The Atmosphere. Characteristics of the Atmosphere. Section 23.1 Objectives. Chapter 23. Chapter 23 Modern Earth Science. Section 1

The Atmosphere - Chapter Characteristics of the Atmosphere

Space Atmospheric Gases. the two most common gases; found throughout all the layers a form of oxygen found in the stratosphere

General Circulation. Nili Harnik DEES, Lamont-Doherty Earth Observatory

Weather is the of the Earth s atmosphere at a place and time. It is the movement of through the atmosphere o Energy comes from the

Chapter 9 External Energy Fuels Weather and Climate

WEATHER. Review Note Cards

ATMOSPHERIC ENERGY and GLOBAL TEMPERATURES. Physical Geography (Geog. 300) Prof. Hugh Howard American River College

COMPOSITION OF THE ATMOSPHERE

GEO1010 tirsdag

CHAPTER 2 - ATMOSPHERIC CIRCULATION & AIR/SEA INTERACTION

Chapter 8 Circulation of the Atmosphere

Website Lecture 3 The Physical Environment Part 1

ATMOSPHERE PACKET CHAPTER 22 PAGES Section 1 page 546

The Planetary Circulation System

- tornadoes. Further Reading: Chapter 08 of the text book. Outline. - cyclones and anti-cyclones. -tropical storms. -Storm surge

The Atmosphere. All weather occurs here 99% of water vapor found here ~75 % of total mass of the atmosphere

Climate and the Atmosphere

ESS 111 Climate & Global Change. Week 1 Weather vs Climate Structure of the Atmosphere Global Wind Belts

F = ma. ATS 150 Global Climate Change Winds and Weather. Scott Denning CSU CMMAP 1. Please read Chapter 6 from Archer Textbook

Chapter 9 Atmosphere Study Guide

Website Lecture 3 The Physical Environment Part 1

General Atmospheric Circulation

Observation: predictable patterns of ecosystem distribution across Earth. Observation: predictable patterns of ecosystem distribution across Earth 1.

The Earth is a Rotating Sphere

Unit 2 Meteorology Test **Please do not write on this test** 5. El Nino & La Nina 6. Photosynthesis 7. Coriolis Effect 8.

Final Weather Unit Study Guide

The Earth s Radiation Balance

Ch. 3: Weather Patterns

Science Chapter 13,14,15

Chapter 2. Heating Earth's Surface & Atmosphere

Next quiz: this Friday, questions. Plus more on Wednesday.

surrounds Earth and protects it somewhat from solar radiation. Like all other matter, air has weight,

2/22/ Atmospheric Characteristics

ATMO 436a. The General Circulation. Redacted version from my NATS lectures because Wallace and Hobbs virtually ignores it

The Atmosphere of Earth

Climate vs. Weather. Weather: Short term state of the atmosphere. Climate: The average weather conditions in an area over a long period of time

Global Weather Trade Winds etc.notebook February 17, 2017

IV. Atmospheric Science Section

Weather Systems. Section

The Atmosphere. Importance of our. 4 Layers of the Atmosphere. Introduction to atmosphere, weather, and climate. What makes up the atmosphere?

Lecture Outlines PowerPoint. Chapter 16 Earth Science 11e Tarbuck/Lutgens

World Geography Chapter 3

Weather Atmospheric condition in one place during a limited period of time Climate Weather patterns that an area typically experiences over a long

Energy Transfer in the Atmosphere

Chapter 4 Lesson 1: Describing Earth s Atmosphere

10.1 TEMPERATURE, THERMAL ENERGY AND HEAT Name: Date: Block: (Reference: pp of BC Science 10)

CHAPTER 9 ATMOSPHERE S PLANETARY CIRCULATION MULTIPLE CHOICE QUESTIONS

Atmosphere and Weather

THE ATMOSPHERE IN MOTION

Name Period 4 th Six Weeks Notes 2013 Weather

- tornadoes. Further Reading: Chapter 08 of the text book. Outline. -tropical storms. -Storm surge

Topic # 12 How Climate Works

GEOG 1010 B. Come to the PASS workshop with your mock exam complete. During the workshop you can work with other students to review your work.

What a Hurricane Needs to Develop

Atmospheric Layers. Earth s atmosphere is divided into several different atmospheric layers extending from Earth s surface outward.

CLIMATE AND CLIMATE CHANGE MIDTERM EXAM ATM S 211 FEB 9TH 2012 V1

Lecture 5: Atmospheric General Circulation and Climate

also known as barometric pressure; weight of the air above the surface of the earth; measured by a barometer air pressure, high

Common Elements: Nitrogen, 78%

Section 13-1: Thunderstorms

Climate versus Weather

The Transfer of Heat

Meteorology. I. The Atmosphere - the thin envelope of gas that surrounds the earth.

ATMOSPHERE M E T E O R O LO G Y

Warming Earth and its Atmosphere The Diurnal and Seasonal Cycles

Earth Science Chapter 16 and 17. Weather and Climate

Weather Atmospheric condition in one place during a limited period of time Climate Weather patterns that an area typically experiences over a long

Atmospheric Composition and Structure

Energy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate

warmest (coldest) temperatures at summer heat dispersed upward by vertical motion Prof. Jin-Yi Yu ESS200A heated by solar radiation at the base

Chapter 11 Lecture Outline. Heating the Atmosphere

HEATING THE ATMOSPHERE

b. The boundary between two different air masses is called a.

Your web browser (Safari 7) is out of date. For more security, comfort and the best experience on this site: Update your browser Ignore

Global Wind Patterns

Temperature Pressure Wind Moisture

Unit: Weather Study Guide

Hadley Circulation in Action. MET 200 Lecture 12! Global Winds: The General Circulation of the Atmosphere. Scales of Motion

Topic # 11 HOW CLIMATE WORKS continued (Part II) pp in Class Notes

The most abundant gas in the atmosphere by volume is. This gas comprises 78% of the Earth atmosphere by volume.

Forecasting Weather: Air Masses and Fronts

The Atmosphere. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems

UNIT 13: WEATHER AND CLIMATE

Unit 5. Seasons and Atmosphere

Background: What is Weather?

World geography 3200/3202 Unit 2 review

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

Transient/Eddy Flux. Transient and Eddy. Flux Components. Lecture 7: Disturbance (Outline) Why transients/eddies matter to zonal and time means?

Chapter 02 Energy and Matter in the Atmosphere

Transcription:

Geography Review Exam I Test bank of questions at: http://www.msubillings.edu/sciencefaculty/spring%202010%20handouts.htm

The Earth is a sphere

The Shape of the Earth the Earth s shape is very close to spherical (oblate ellipsoid or spheroid (flattened at the poles) D polar D equator = 7900 miles = 12,714 km = 7926 miles = 12,756 km Earth

The Geographic Grid a) Latitude (Parallels) 1 degree latitude = a constant 111 km b) Longitude (Meridians) 1 degree of longitude = 111 km at the equator and 0 at the poles Figure 1.3, p. 28

Earth s Revolution around the Sun sun is not in the middle of the plane of the ecliptic Aphelion - the Earth furthest away from Sun (July 4) Perihelion - the Earth closest to Sun (January 3) E 152 million km 147 million km SUN E variation in distance of ~ 3% When are we closest to the Sun?

Earth s Revolution around the Sun the Earth rotates about its axis from west to east once every 23 hours and 56 minutes the Earth s axis always points the same way as it revolves around the sun

Earth s Revolution around the Sun at equinox, the circle of illumination passes through both poles the subsolar point is the equator each location on Earth experiences 12 hours of sunlight and 12 hours of darkness Figure 1.18, p. 41

Earth s Revolution around the Sun Solstice ( sun stands still ) On June 22, the subsolar point is 23½ N (Tropic of Cancer) On Dec. 22, the subsolar point is 23½ S (Tropic of Capricorn)

Polar Projection centered on north or south pole meridians are radiating straight lines parallels are concentric circles spacing of parallels (scale fraction) increases outward from the pole Map Projections

Mercator Projection rectangular grid of meridians (straight vertical lines) and parallels (straight horizontal lines) meridians are evenly spaced, spacing of parallels increases with latitude Map Projections Used to show surface flows, e.g. weather, oceans

Map Projections Goode Projection indicates the true sizes of the Earth s surface but distorts the shapes of areas Used to show land features Figure 1.10, p.32

Global Time Zones How many degrees does the Earth rotate in an hour? the Earth rotates 15 per hour so time zones differ by 1 hour (360 /15 = 24 hours)

The Atmosphere and the Global Radiation Budget

Atmospheric Pressure and Density Gravity holds most of the air close to the ground The weight of the overlying air is the pressure at any point

Composition of the Atmosphere Constant gases in the Troposphere Nitrogen 78% (converted by bacteria into a useful form in soils) Oxygen 21% (produced by green plants in photosynthesis and used in respiration) Argon ~1% (inert) Figure 2.12, p. 62

The atmosphere is layered according to its temperature structure In some layers the temperature increases with height In others it decreases with height or is constant Heated by collisions of cosmic rays Heated by ozone absorption of UV Heated by the ground Why? pause is a level; sphere is a layer

IG4e_02_01

Electromagnetic Radiation - Everything above -273 C (absolute zero, 0 Kelvin) emits radiation - Hotter objects emit more energy at shorter wavelengths - Colder objects emit more energy at longer wavelengths

What happens to the Sun s radiation as it travels through the atmosphere? It can be reflected It can be scattered It can be absorbed It can be transmitted Glass of water and laser

Earth's annual energy balance between solar insolation and terrestrial infrared radiation Earth's Energy Balance A global balance is maintained by transferring excess heat from the equatorial region toward the poles

Heat is transported to the Polar regions

Planetary Energy Balance Energy In = Energy Out S(1 ) R 4 R T 2 2 4 o T 18 C But the observed T s is about +15 C

Greenhouse Effect Increasing Greenhouse Gases increases the amount of heat absorbed by the atmosphere and re-radiated back (counterradiation) to the Earth surface. The Earth is 33 C (~60 F) warmer as a result.

Greenhouse gas concentrations Human activities have caused dramatic increases in greenhouse gas concentrations

Winds and Global Circulation

Winds and Global Circulation Atmospheric Pressure Winds Global Wind and Pressure Patterns Oceans and Ocean Currents

How is Energy Transported to its escape zones? Both atmospheric and ocean transport are crucial Buoyancy-driven convection drives vertical transport Latent heat is at least as important as sensible heat

Atmospheric Circulation in a nutshell Hot air rises (rains a lot) in the tropics Air cools and sinks in the subtropics (deserts) Three convective cells develop in each Hemisphere Coriolis causes direction of prevailing surface winds Poleward-flow is deflected by the Coriolis force into westerly jet streams in the temperate zone Jet streams are unstable to small perturbations, leading to huge eddies (storms and fronts) that finish the job

Atmospheric Circulation in a nutshell Winds are initially generated by differences in heating at the Earth s surface Geostrophic winds result in rotational movement around high and low pressure centers.

How winds are made

Two columns of air same temperature same distribution of mass 500 mb level 1000 mb 1000 mb

Cool the left column; warm the right column The cooled column contracts The heated column expands 500 mb original 500 mb level 500 mb 1000 mb 1000 mb

Air moves from high to low pressure at the surface Air is rising in the column on the right. There is a low pressure center at the surface original 500 mb level Low High High Low 1003 mb 997 mb Air is sinking in the column on the left. There is a high pressure center at the surface

Global Circulation

90 o N 60 o N 30 o N 0 o Cold High Pressure Warm Low Pressure But heat is transported from the Equator to the Poles - how? SUN 30 o S 60 o S 90 o N Earth

How is Energy Transported to its escape zones? Both atmospheric and ocean transport are crucial Buoyancy-driven convection drives vertical transport Latent heat is at least as important as sensible heat

What a single cell convection model would look like for a non-rotating earth Thermal convection leads to formation of convection cell in each hemisphere Energy transported from equator toward poles What would prevailing wind direction be over N. America with this flow pattern on a rotating earth?

Coriolis Force acts to the right in the Northern Hemisphere Physics

Fig. 7-12, p. 154

Geostrophic Winds

low pressure Coriolis Force 992 996 1000 1004 1008 1012 1016 1020 pressure gradient force geostrophic winds high pressure

High pressure (anticyclone) Side View From above H L H L L air descends surrounding air is relatively low

Low pressure (depressions, cyclone) From above Side View L H L H H air ascends surrounding air is relatively high

Global Temperature patterns and weather

Temperature Patterns Stronger seasonal heating and cooling on land produces asymmetry Poleward distortion of isotherms over northern high latitude oceans Equatorward distortion over subtropics

Seasonal Migration of ITCZ Mean position is somewhat north of Equator Strong departures from zonal mean position driven by seasonal heating over land (Especially over Asia, S. America, Africa)

Monsoons In July the position of the ITCZ moves North low pressure over land causes winds to flow off the ocean this brings heavy rainfall Figure 5.20, p. 167

Monsoons In January high pressure over the land produces dry winds Air is flowing towards the ITCZ Figure 5.20, p. 167

Fast air currents, 1000 s of km s long, a few hundred km wide, a few km thick Typically find two jet streams (subtropical and polar front) at tropopause in NH When would you expect the jets to be strongest? Jet Streams

Smooth westward flow of upper air westerlies Develop at the polar front, and form convoluted waves eventually pinch off Primary mechanism for poleward heat transfere Pools of cool air create areas of low pressure Rossby Waves

Ocean Circulation in a nutshell Surface winds cause large, clockwise rotating gyres in the northern hemisphere and counterclockwise gyres in the southern hemisphere Salinity and temperature differences in water cause sinking of water (deep water formation) in the North Atlantic and Southern Ocean (Antarctic) EL Nino is a quasi periodic rocking of the Ocean-Atmosphere system in the tropical Pacific

Ocean surface currents large continuously moving loops (gyres) produced by winds, Coriolis force and land masses Figure 5.32, p. 175

The Ocean Deep Currents Deep-sea currents driven by differences in temperature and salinity much bigger and slower than surface currents

Global Temperatures

Main Points 1.We measure air temperature in Celsius and/or Fahrenheit 2.Surface temperature changes as a result of changes in NET energy flows resulting from seasonal and daily changes in insolation and radiation from the surface 3.Air temperature is a function of Insolation, Latitude, Surface Characteristics, nearness to water bodies and elevation 4.Cities can produce heat islands 5.The atmosphere is divided into discrete layers based on temperature differences and patterns 6.The Environmental Lapse Rate is the normal change in temperature with elevation 7.Land areas are colder in the winter and hotter in the summer than adjacent areas of water 8.At present global temperatures are rising due to increased Greenhouse gases

Temperature Lags Earth's surface temperature is a balance between incoming solar radiation and outgoing terrestrial radiation. Peak temperature lags after peak insolation because surface continues to warm until infrared radiation exceeds insolation.

Air Temperature The Urban Heat Island the heat island tends to persist over night Figure 3.6, p. 94 parks can reduce the heating desert urban areas often do not exhibit heat islands since irrigated vegetation may make the city cooler

Temperature Structure of the Atmosphere Stratosphere is bounded by the stratopause immediately above is the mesosphere where temperatures decrease with altitude (bounded by the mesopause above) immediately above is the thermosphere Figure 3.9, p. 97

Temperature Structure of the Lower Atmosphere The troposphere is the lower most atmospheric layer temperature decreases on average by 6.4 C per 1000 meters (3.5 F per 1000 feet) in the troposphere (environmental lapse rate)

Heat Transfer in the Atmosphere Conduction (direct heat transfer from the heated ground surface to the atmosphere) Convection (heat transfer by warm air moving to colder upper atmosphere) >> vertical motion: warm air rising and cold air sinking Advection (heat transfer by warm air mixing with colder adjacent air) >> Horizontal winds

Southern hemisphere has fewer land masses and ocean currents that encircle the globe, creating isotherms that are more regular than those in the northern hemisphere. July Isotherms

IG4e_03_16

Main topics for today The Hydrosphere and the Water Cycle Water s properties are due to its polar nature Water has a very high heat capacity and high heat of fusion Warm air can contain more water vapor than cold air Relative Humidity and Dew Point Temperature are the most common ways to express how much water is in the air The Environmental Lapse rate is the observed change in air temperature with change in elevation An Adiabatic Process is the expansion or contraction of an air mass without heat loss or gain

Main points for today (cont) Clouds are classified by altitude and shape Precipitation can occur because of 1) convection, 2) orographic lifting, and/or 3) frontal processes Air Quality

The Water/Hydrologic Cycle

Energy associated with phase change 80 calories 100 calories 540 calories!

Basic Humidity Facts Humidity is the amount of water vapor in the atmosphere Warm air can hold much more than cold air Cold dry air can have close to 0% Warm tropical air may have 4-5% Several ways to describe humidity (Dew Point and relative humidity are most common)

Relative Humidity a measure of the amount of water vapor present in air relative to the maximum amount that the air can hold at a given temperature (%) e.g. if relative humidity is 50%, then it contains 1/2 the amount of water vapor it could hold at a given temperature relative humidity decreases as temperature increases (assuming no water vapor is added)

Relative Humidity and Temperature The diurnal cycle if no water vapor is added or removed from the air mass, then Relative Humidity decreases as Temperature increases The diurnal cycle is the inverse of Temperature

Vertical Motion and Temperature Rising air expands, using energy to push outward against its environment, adiabatically cooling the air A parcel of air may be forced to rise or sink, and change temperature relative to environmental air

Dry Adiabatic Lapse Rate Dry Adiabatic Lapse Rate (DALR) - decrease in temperature with altitude: 10 C/1000m Figure 4.10, p. 127

as a parcel of air rises, it cools and becomes saturated at the dew point dew point lapse rate (1.8 degrees per 1000 meters) means that the dew point of the air parcel decreases as the air rises Wet Adiabatic Lapse Rate when it reaches its dew point, condensation occurs (lifting condensation level) Figure 4.10, p. 127

Conditionally unstable air What if the environmental lapse rate falls between the moist and dry adiabatic lapse rates? The atmosphere is unstable for saturated air parcels but stable for unsaturated air parcels This situation is termed conditionally unstable This is the typical situation in the atmosphere

Precipitation: three mechanisms Convection Orographic Frontal (cyclonic)

IG4e_04_19

3.) Frontal (cyclonic) precipitation where air masses with different temperatures come together warm air lifted by cold dense air along a weather front leads to frontal precipitation Cold air Warm air

Air Quality Air pollutants are undesirable gases, aerosols, and particulates injected into the atmosphere by human and natural causes

Weather

Major points for today 1. Most weather in the continental US results from interactions between large air masses coming from the tropics and the polar regions. 2. Cold and Warm Fronts are masses of cold and warm air, respectively. 3. Cold fronts are quickly moving masses of cold air that thrust moisture-laden warm air up to form storm clouds 4. Warm fronts are more slowly moving fronts in which warm air slides up over more dense cold air. 5. Mid latitude cyclones are common in North America and result from a breakout of cold air in the far north

Major points for today (cont) 6.Thunderstorms are caused by rapid uplift of moist air in an unstable atmosphere. They are characterized by strong updrafts and downdrafts. 7.Tropical storms, hurricanes, etc., start as low pressure troughs in easterly trade winds. If conditions are right, they can intensify into massive storms 8.In the big picture, horizontal winds are all about transferring heat from the equator to the poles; whereas severe storms are all about vertical motion of the atmosphere.

Air Masses

Cold and Warm Fronts

Warm Front Cold Front Fronts A Front - is the boundary between air masses; normally refers to where this interface intersects the ground (in all cases except stationary fronts, the symbols are placed pointing to the direction of movement of the interface (front) Stationary Front Occluded Front

Air Mass Fronts Two air masses entering a region, such as the U.S. middle latitudes, have a front, or transition zone, between the strong temperature and humidity differences. Four different fronts are used on weather maps.

IG4e_06_04

Typical Warm Front Structure

Cirrostratus Cirrostratus with Halo

Altostratus Alto Stratus Castellanus

Midlatitude Cyclones

Large-Scale Setting Hemispheric westerlies typically organized into 4-6 long waves

Lifecycle of a Midlatitude Cyclone Stationary front Incipient cyclone Open wave Green shading indicates precipitation Mature stage occlusion dissipating Takes several days to a week, and moves 1000 s of km during lifecycle

Weather Changes Associated with Wave Cyclones Figure 6.10, p. 193

Wave cyclones tend to form in certain areas and travel common paths Cyclone Tracks Mid-latitude wave cyclones tend to travel eastward Tropical cyclones tend to move westward Figure 6.11, p. 194

Severe Weather

Tropical Cyclones hurricanes (western hemisphere) and typhoons (western Pacific in Asia) and cyclone in Indian Ocean develop over warm ocean surfaces between 8 and 15 latitude, migrate westward and curve toward the poles Tropical cyclones often create tremendous damage due to high winds, high waves, flooding (storm surges) and heavy rains

Easterly Waves A simple form of tropical weather system is a slow moving trough of low pressure within the tropical easterly wind belts (trades) Figure 6.16, p. 197

The Atmospheric Circulation