Ocean and Atmosphere. Earth’s Heat Budget and Atmospheric Circulation Atmospheric properties Earth’s Energy Budget Vertical Atmospheric Circulation Surface.

Slides:



Advertisements
Similar presentations
Do Now – In Binders Describe how wind is created. What is the relationship between density and pressure? What happens to air pressure as I hike up a mountain?
Advertisements

Atmospheric Circulation Causes of Atmospheric Circulation 1) Uneven solar energy inputs 2) Rotation of the Earth Global Circulation Patterns Local Events.
The General Circulation of the Atmosphere
Global Wind Patterns and Weather & Weather Basic
Earth’s Climate System (part 2) revisiting the radiation budget heat capacity heat transfer circulation of atmosphere (winds) Coriolis Effect circulation.
Atmosphere 78% nitrogen, 21% oxygen. Water Vapor up to 4% by volume leaves atmosphere as dew, rain or snow.
General Circulation and Climate Zones Martin Visbeck DEES, Lamont-Doherty Earth Observatory
Composition of the Atmosphere. Air Density Temperature –Warmer air is less dense than cold air Humidity –Humid air is less dense, dry air is more dense.
Class 3b: Winds (global and local)
Atmosphere 78% nitrogen, 21% oxygen. Water Vapor up to 4% by volume leaves atmosphere as dew, rain or snow.
Atmosphere 78% nitrogen, 21% oxygen. Water Vapor up to 4% by volume leaves atmosphere as dew, rain or snow.
Wind and Ocean Currents Global winds Ocean Currents Local winds.
Unit 2: Climate Winds and Climate
“ What Causes Our Weather” n I. Factors that cause weather : A. Weather-Is the present state of our atmosphere. B. What causes our weather? 1. The interaction.
Chris Parkes Rm 455 Kelvin Building
Air masses and Fronts.
ATMOSPHERE Air Circulation
“ I. What Causes Our Weather” 1. Weather-Is the present state of our atmosphere. 2. The interaction between the earth’s air, water, land and the sun causes.
Earth's Atmosphere Troposphere- the layer closest to Earth's surface extending roughly 16 km (10 miles) above Earth. Densest – N, O, & water vapor Stratosphere-
Heat and Atmospheric Circulation. Solar Energy Sun is a star of average size, temp. & color Sun captured 99.9% of nebula’s matter.1% formed planets, moons,
WHAT MAKES THE WIND BLOW?. Recall the effect of solar radiation.
Meteorology: the study of Earth’s atmosphere Meteor – In ancient Greek – meant “High in the air” Current meanings still apply Meteor – astronomical entity.
Questions for Today:  What is Weather and Climate?  What are four major factors that determine Global Air Circulation?  How do Ocean Currents affect.
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.
Lecture 14 4 February 2005 Atmospheric and Oceanic Circulations (continued) Chapter 6.
Unit 10 Lesson 4 Wind in the Atmosphere Copyright © Houghton Mifflin Harcourt Publishing Company.
Movement of Air in Earth’s Atmosphere. What is wind? The movement of air from an area of higher pressure to an area of lower pressure. The movement of.
Welcome to Class Define radiation, convection, and conduction.
ATMOSPHERIC CIRCULATION NOTES- AIR/SEA INTERFACE, CORIOLIS, & WIND.
Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water.
Chapter 4 Global Climates and Biomes.  Weather – the short term conditions of the atmosphere in a local area  Includes: temperature, humidity, clouds,
A2 Module 4: Global Change
Lecture 14 7 February 2005 Atmospheric and Oceanic Circulations (continued) Chapter 6.
Ch Winds. Low air pressure at the equator, due to the constant rising of heated air. Low air pressure at the equator, due to the constant rising.
Wind & Climate Wind – the horizontal movement of air. Low pressure – warm air rising. High pressure – cold air falling. Winds always blow from high pressure.
Weather Review. Air Masses Air Mass – A large body of air through which temperature and moisture are the same. Types 1. Continental – formed over land.
C. 22 Section 3 Atmospheric Circulation Air near Earth’s surface generally flows from the poles toward the equator.
What causes winds? Uneven heating between the equatorial poles causes global winds. Since Earth is a sphere AND it is tilted on its axis, the sun’s energy.
Air Pressure/Winds Air Pressure –weight of the atmosphere pushing down on Earth (we don’t feel it because air is pushing on all sides, not just down from.
Do Now: Analyze the following images
Atmospheric Circulation and Weather  Composition and Properties of the Atmosphere Lower atmosphere nearly homogenous mixture of nitrogen 78.1% and oxygen.
Atmosphere. Atmosphere structure Tropopause Troposphere 20 km 40 km 10 mi 20 mi 30 mi Weather zone Water Vapor Dry Ozone Stratosphere Stratopause Mesosphere.
Wind What are winds?.
Wind and the Ocean. Wind Currents of air Develop when two adjacent bodies of air have different densities. Denser air sinks, pushing less dense air upward.
Winds What causes winds?.
Air-Sea interactions Chapter 8. SOLAR CONNECTION- Air and Sun “Others” represents the percentage of Water Vapor and Aerosols.
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.
Atmospheric Circulation
Tropical to subtropical circulation. Major Zones ITCZ (Intertropical convergence zone) Subtropics (30 degrees, north/south hemisphere) Front Poles.
Heating of the Earth. Temperature Layers of the Atmosphere.
Paper 1 Physical Core Atmosphere and Weather 1 GeographyCambridge AS level syllabus 9696.
GCM’s Heating of the Earth Uneven Solar Energy Inputs: Earth is heated unevenly by the sun due to different angles of incidence between the horizon and.
Coriolis Effect: Deflection of moving objects/large masses due to the rotation of Earth on its axis (EX: currents & missiles) –Northern Hemisphere: RIGHT.
Latitudinal effects Intensity of insolation is not the same at all latitudes Earth is roughly spherical, so insolation passing through 1 m 2 screen –Illuminates.
Chapter 4 Global Climates and Biomes. Global Processes Determine Weather and Climate Weather- the short term conditions of the atmosphere in a local area.
Energy From the Sun Chapter 15: The Atmosphere. Energy Transfer The Sun gives off lots of energy, and most of it reaches our atmosphere. The energy the.
The Atmosphere A thin fragile shell of gases that provides all our weather and allows life on earth.
Global Climates and Biomes
Weather vs. Climate Weather- short-term conditions of atmosphere in local area. (Temperature, humidity, clouds, precipitation, wind speed, & atmospheric.
Wind & Climate Wind – the horizontal movement of air.
Module 10 Air Currents After reading this module you should be able to
Warm-up 22SEP2014 What are the two factors that make up climate?
Winds Cause of Wind.
“ What Causes Our Weather”
Winds What causes winds?.
14.3 Air Movement and Wind.
Lesson /12/17 SWBAT explain how energy flow in the atmosphere affects weather Do Now: Pollination by native insects is considered an ecosystem.
Winds What causes winds?.
Global Climates and Biomes
“ What Causes Our Weather”
Presentation transcript:

Ocean and Atmosphere

Earth’s Heat Budget and Atmospheric Circulation Atmospheric properties Earth’s Energy Budget Vertical Atmospheric Circulation Surface Atmospheric Circulation

Atmospheric Temperature

Water vapor saturation pressure How much water vapor the air can “hold”

Density of Air Which is more dense, DRY air or HUMID air? –Air:N 2 (14*2=28) O 2 (16*2=32) –Water: H 2 O (2+16=18) Light molecules displace heavier molecules…

Density of Air Humid air is light, and rises Dry air is heavy, and sinks

Water vapor, convection, condensation 1. Adiabatic Expansion  Cooling 2. Condensation  Release latent heat of vaporization

Water Budget

Earth’s Heat Sources Geothermal = 0.1 cal/cm 2 /day Solar = cal/cm 2 /day BALANCED BUDGET! –Wavelength (μm) = 2900 / T (K o ) SUN = 2900/5600 ≈ 0.5 μm (visible light) Earth = 2900/290 ≈ 10 μm (infrared)

Sun’s Radiation

Earth’s Heat Budget

Atmosphere reflection and absorbance

Global Warming: Increased heat absorption in the atmosphere

Seasonal variability in solar radiation

Latitudinal variability in solar radiation

Latitudinal Heat Budget

So what are the effects of uneven heating? Less Dense Air: –HOT –HUMID More Dense Air: –COLD –DRY

Atmospheric Convection in a NON-Rotating Earth LOW Surface Air Pressure HIGH Surface Air Pressure

Low & High Pressure

But… The Earth Spins! FLASH NEWS: The US attempts to stop the axis of Evil by bombing Quito (Ecuador), using cannons located in Buffalo (NY)!

Bombing of Quito from Buffalo

Earth Rotation: Coriolis Effect Apparent deflection force due to Earth’s rotation Acts on freely moving objects North Hemisphere: Deflection to the right South Hemisphere: Deflection to the left C = (2Ωsin(lat))v –V=velocity of a particle in motion –Ω=constant (angular velocity of Earth) So: –High v = high C ; High latitude = high C –No Coriolis at equator, maximum at poles

Figure 6.16

Figure 6.17

Atmospheric Convection Cells

Figure 6.19

Global atmospheric generalities Hadley Cells (subtropical) are quite stable Pressure systems: –Equator: LOW (Doldrums or ITCZ- Inter Tropical Convergence Zone) –30 ’s : HIGH (Horse Latitudes) –60 ’s : LOW

Figure 6.21

Horse latitudes Doldrums

Global atmospheric generalities Hadley Cell is quite stable Pressure systems: –Equator: LOW (Doldrums or ITCZ- Inter Tropical Convergence Zone) –30 ’s : HIGH (Horse Latitudes) –60 ’s : LOW In between Pressure systems: –WIND!! Trade Winds Westerlies: (Roaring Forties, Screaming Fifties)

Figure 6.19

Seasonal Wind Variation

Monsoons (Indian Ocean)

Precipitation / Evaporation

Surface Ocean Salinities

Land – Ocean Temperatures

Local Winds: Sea Breeze

Local Winds: Coastal Fog

Local Winds: Mountain or Island Effect