ATM OCN 100 Summer 2002 1 ATM OCN 100 – Summer 2002 LECTURE 3 PHYSICAL & CHEMICAL COMPOSITION of...

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MADISON’S CURRENT WEATHER MADISON’S CURRENT WEATHER Madison Weather at 1000 AM CDT THR JUN 20 2002 Updated twice an hour at :05 and :25 Sky/Weather: CLOUDY Temperature: 78 F (25 C) Dew Point: 66 F (18 C)

Transcript of ATM OCN 100 Summer 2002 1 ATM OCN 100 – Summer 2002 LECTURE 3 PHYSICAL & CHEMICAL COMPOSITION of...

MADISON’S CURRENT WEATHERMADISON’S CURRENT WEATHER

Madison Weather at 1000 AM CDT THR JUN 20 2002 Updated twice an hour at :05 and :25

Sky/Weather: CLOUDY Temperature: 78 F (25 C) Dew Point: 66 F (18 C) Relative Humidity: 66% Wind: SW9G17 MPH Barometer: 30.21R (1023.0 mb)

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QUIZ!!!QUIZ!!!

Which way does the wind circulate Which way does the wind circulate around a high pressure center?around a high pressure center?

And around a Low?And around a Low? Why sunny skies?Why sunny skies? Answers….Answers….

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Current Surface Weather Map Current Surface Weather Map with Isobars (“iso” = equal & “bar” = weight), Fronts and Radarwith Isobars (“iso” = equal & “bar” = weight), Fronts and Radar

IsobarsIsobars

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Current Surface Winds Current Surface Winds with Streamlines & Isotachs (“iso” = equal & “tach” = speed)with Streamlines & Isotachs (“iso” = equal & “tach” = speed)

IsobarsIsobars HHHH

LL

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Current Temperatures (Current Temperatures (°°F) & IsothermsF) & Isotherms(“iso” = equal +”therm” = temperature)(“iso” = equal +”therm” = temperature)

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Tomorrow AM Forecast MapTomorrow AM Forecast Map

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Did You know that –Did You know that –Tomorrow is summer solstice (8:24 AM CDT)Tomorrow is summer solstice (8:24 AM CDT)

See Fig. 2.10 Moran & Morgan (1997)See Fig. 2.10 Moran & Morgan (1997)

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AnnouncementsAnnouncements

Sign-upSign-up

– Class listClass list

– Official registration (NLT Fri. 21 June) Official registration (NLT Fri. 21 June)

– Course SyllabusCourse SyllabusNOTE Change Wed. to Fri. 21 Dec. on backNOTE Change Wed. to Fri. 21 Dec. on back

Homework 1: Due next Thurs. 27 JuneHomework 1: Due next Thurs. 27 June

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ATM OCN 100 – ATM OCN 100 – Summer 2002Summer 2002LECTURE 2ALECTURE 2A

PHYSICAL & CHEMICAL COMPOSITION PHYSICAL & CHEMICAL COMPOSITION of EARTH’S ATMOSPHEREof EARTH’S ATMOSPHERE

A. PRACTICAL QUESTIONSA. PRACTICAL QUESTIONS

– What makes Planet Earth special?What makes Planet Earth special?

– How has the atmosphere evolvedHow has the atmosphere evolved??

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Earth-Rise Earth-Rise (Apollo Mission)(Apollo Mission)

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SUNRISE FROM SPACESUNRISE FROM SPACE

From STS-52 (JSC-NASA)From STS-52 (JSC-NASA)

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B. PRESENT EARTH’S ATMOSPHEREB. PRESENT EARTH’S ATMOSPHERE BackgroundBackground

– Early Greek ThoughtEarly Greek Thought The 4 Elements: Earth, Air, Water, Fire.The 4 Elements: Earth, Air, Water, Fire.

– ““Modern” Chemistry Modern” Chemistry (since 18(since 18thth century) century)ElementElementCompoundCompoundMixtureMixture

Chemical CompositionChemical Composition– Air is a mixtureAir is a mixture– With the following gases:With the following gases:

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Atmospheric Gases isolated by 18Atmospheric Gases isolated by 18thth Century ChemistsCentury Chemists

Nitrogen (NNitrogen (N22))– Importance in Food Chain (Nitrogen Fixation)Importance in Food Chain (Nitrogen Fixation)

Oxygen (OOxygen (O22))– Critical Importance for Life (Respiration)Critical Importance for Life (Respiration)

Argon (Ar)Argon (Ar)– Unknown ImportanceUnknown Importance

Carbon Dioxide (COCarbon Dioxide (CO22))– Critical Importance for Life (Photosynthesis)Critical Importance for Life (Photosynthesis)

(also Asphyxiation) (also Asphyxiation)

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FRACTIONAL VOLUMETRIC COMPOSITION OF DRY AIR in

HOMOSPHERE

Ar0.93%

CO2

0.03%O2

21%

N2 78%

See Table 1.2 Moran & Morgan (1997)See Table 1.2 Moran & Morgan (1997)

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B. PRESENT EARTH’S ATMOSPHERE B. PRESENT EARTH’S ATMOSPHERE (con’t.)(con’t.)

Vertical Variations of Atmospheric Vertical Variations of Atmospheric CompositionComposition– Criterion Criterion

ChemicalChemical

– DivisionsDivisions HOMOSPHEREHOMOSPHERE HETEROSPHEREHETEROSPHERE

– Where ...Where ...

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VERTICAL COMPOSITION VARIATIONS VERTICAL COMPOSITION VARIATIONS (con’t.)(con’t.)

HOMOSPHEREHOMOSPHERE– ““Homo” Homo” = same = same ((percentage composition)percentage composition);;– Turbulent mixing;Turbulent mixing;– Below 80 km altitude.Below 80 km altitude.

HETEROSPHEREHETEROSPHERE– ““Hetero” Hetero” = different (= different (compositioncomposition););– Fractional diffusion Fractional diffusion (by molecular weight)(by molecular weight);;– Above 80 km altitude.Above 80 km altitude.

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CONSTITUENTS OF AIR CONSTITUENTS OF AIR in the in the HOMOSPHEREHOMOSPHERE

(Below 80 km)(Below 80 km)

Principal Permanent Gases of “Dry Air”Principal Permanent Gases of “Dry Air” Principal Variable gasesPrincipal Variable gases Anthropogenic GasesAnthropogenic Gases AerosolsAerosols

– Liquids Liquids oror solids suspended in Atmosphere solids suspended in Atmosphere CloudsClouds

– Liquid droplets Liquid droplets oror ice crystals in Atmosphere ice crystals in Atmosphere

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PRINCIPAL VARIABLE GASESPRINCIPAL VARIABLE GASESin the Homospherein the Homosphere

Water Vapor (HWater Vapor (H22O) O) << 4% by volume4% by volume

Carbon Dioxide (COCarbon Dioxide (CO22) ) 360 ppm = 0.036%360 ppm = 0.036%

Methane (CHMethane (CH44) ) < 1700 ppb = 0.00017%< 1700 ppb = 0.00017%

Ozone (OOzone (O33) ) < 8 ppm = 0.0008%< 8 ppm = 0.0008%

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Recent Atmospheric CORecent Atmospheric CO22 Concentrations Concentrations

See Fig. 2.25 Moran & Morgan (1997)See Fig. 2.25 Moran & Morgan (1997)

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Mauna Loa Observatory, HIMauna Loa Observatory, HI

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OzoneOzone

A paradoxA paradox

– Good and BadGood and Bad Natural production & destructionNatural production & destruction

where…where…

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Ozone FormationOzone FormationFigure 2.18 Moran & Morgan (1997)Figure 2.18 Moran & Morgan (1997)

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Ozone Destruction (Natural)Ozone Destruction (Natural)Figure 2.18 Moran & Morgan (1997)Figure 2.18 Moran & Morgan (1997)

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OzoneOzone

A paradoxA paradox Natural production & destructionNatural production & destruction Location in AtmosphereLocation in Atmosphere

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VERTICAL OZONE PROFILE US STANDARD ATMOSPHERE 1976

020406080

100120140

0 1 2 3 4 5 6 7 8 9

MIXING RATIO [PPMV]

AL

TIT

UD

E [

km

]

8 ppmv = 0.0008%

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ANTHROPOGENIC SUBSTANCESANTHROPOGENIC SUBSTANCES

Chlorofluorocarbons Chlorofluorocarbons (CFCs)(CFCs)

Volatile Organic CompoundsVolatile Organic Compounds– (Hydrocarbons)(Hydrocarbons)

Oxides of nitrogen Oxides of nitrogen (NO, NO(NO, NO22))

Oxides of carbon Oxides of carbon (CO, CO(CO, CO22))

Sulfur compounds Sulfur compounds ((HH22S, SOS, SO22,, SOSO33))

Suspended particulatesSuspended particulates

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AEROSOLSAEROSOLS

What they areWhat they are

– Suspended solid particles or liquid Suspended solid particles or liquid droplets in atmosphere.droplets in atmosphere.

SourcesSources

– NaturalNatural

– Human activityHuman activityWhere….Where….

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Aerosols from WildfiresAerosols from Wildfires

11 May 200011 May 2000 ((NOAA-15)NOAA-15)

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Aerosols from Colorado WildfiresAerosols from Colorado Wildfires

10 June 200210 June 2002 ((SSEC - MODIS)SSEC - MODIS)

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Aerosols from VolcanoesAerosols from VolcanoesMt. St. Helens, WA May 1980Mt. St. Helens, WA May 1980

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Volcanic Plume from Mt. EtnaVolcanic Plume from Mt. Etna

23 July 200123 July 2001 ((NOAA-14)NOAA-14)

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Aerosols-Dust from MongoliaAerosols-Dust from Mongolia

10 Apr 200110 Apr 2001

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Aerosols from Blowing DustAerosols from Blowing Dust

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Aerosols from Sea Spray Aerosols from Sea Spray (Calif. Coast)(Calif. Coast)

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Aerosols from Natural VegetationAerosols from Natural Vegetation

in Great Smoky Mtn. Natl Park, NC-TNin Great Smoky Mtn. Natl Park, NC-TN

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Aerosols from Urban PollutionAerosols from Urban PollutionMadison (from Space Science & Eng. Center)Madison (from Space Science & Eng. Center)

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PRINCIPAL VARIABLE GASESPRINCIPAL VARIABLE GASESin the Heterospherein the Heterosphere

(above 80 km)(above 80 km)

Diatomic nitrogen (NDiatomic nitrogen (N22) ) 85 to 200 km85 to 200 km

Monatomic oxygen (O) Monatomic oxygen (O) 200 to 1100 km200 to 1100 km Helium (He)Helium (He) 1100 to 3500 km1100 to 3500 km Atomic hydrogen (H) Atomic hydrogen (H) 3500 to 11,000 km3500 to 11,000 km

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C. ORIGIN & EVOLUTIONC. ORIGIN & EVOLUTIONof Earth’s Atmosphereof Earth’s Atmosphere

How did our current atmosphere How did our current atmosphere evolve?evolve?

General History of the AtmosphereGeneral History of the Atmosphere

– 4.5 billion yr ago - Solar System 4.5 billion yr ago - Solar System formedformed

– And then…And then…

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C. ORIGIN & EVOLUTION C. ORIGIN & EVOLUTION of Earth’s Atmosphereof Earth’s Atmosphere

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ATMOSPHERIC ORIGIN & EVOLUTION ATMOSPHERIC ORIGIN & EVOLUTION (con’t)(con’t)

RationaleRationale– Planet Earth is special because of Planet Earth is special because of

large amounts of Olarge amounts of O22;;– Atmosphere & Life Co-evolved.Atmosphere & Life Co-evolved.

Human InterventionHuman Intervention– Humans could possibly affect Humans could possibly affect

concentrations of some gases, concentrations of some gases, with following…with following…

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Enhanced “Greenhouse Effect”Enhanced “Greenhouse Effect”

BackgroundBackground

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Enhanced “Greenhouse Effect”Enhanced “Greenhouse Effect”

Increases in “Greenhouse Gases”Increases in “Greenhouse Gases”– COCO2 2 and CHand CH44

Why more COWhy more CO22??

– Burning of fossil fuelsBurning of fossil fuels– DeforestationDeforestation– Changes in Sea Surface TemperatureChanges in Sea Surface Temperature

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Global COGlobal CO22 Emissions Emissions

Marland, et.al. 2001Marland, et.al. 2001 Carbon Dioxide Information Analysis CenterCarbon Dioxide Information Analysis Center

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COCO2 2 measurements at Mauna Loa, HImeasurements at Mauna Loa, HI

See Fig. 2.25 Moran & Morgan (1997)See Fig. 2.25 Moran & Morgan (1997)

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COCO2 2 measurements at South Polemeasurements at South Pole

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Enhanced “Greenhouse Effect”Enhanced “Greenhouse Effect” (con’t.)(con’t.)

Increases in “Greenhouse Gases”Increases in “Greenhouse Gases”– COCO2 2 and CHand CH44

Why more COWhy more CO22??– Burning of fossil fuelsBurning of fossil fuels– DeforestationDeforestation– Changes in Sea Surface TemperatureChanges in Sea Surface Temperature

Potential Implications Potential Implications – Ice cap melting & coastal floodingIce cap melting & coastal flooding– Changes in agricultural areasChanges in agricultural areas– Increases in diseases and pestsIncreases in diseases and pests

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See Fig. 19.9 Moran & Morgan (1997)See Fig. 19.9 Moran & Morgan (1997)

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““Ozone Hole”Ozone Hole”

BackgroundBackground Destruction of Stratospheric OzoneDestruction of Stratospheric Ozone

– From CFCsFrom CFCs

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Destruction of ozone by CFCs. Destruction of ozone by CFCs. See Fig. 2.19, Moran & Morgan (1997)See Fig. 2.19, Moran & Morgan (1997)

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CFC & other SolventCFC & other Solvent Concentrations in Concentrations in Atmosphere Atmosphere

(Source: NOAA/CMDL)(Source: NOAA/CMDL)

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Evolution of the “Ozone Hole”Evolution of the “Ozone Hole” NASA TOMS ProjectNASA TOMS Project

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Recent “Ozone Hole” Status Recent “Ozone Hole” Status NASA TOMS ProjectNASA TOMS Project

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““Ozone Hole” Ozone Hole” (con’t.)(con’t.)

BackgroundBackground Destruction of Stratospheric OzoneDestruction of Stratospheric Ozone

– From CFCsFrom CFCs Potential ImplicationsPotential Implications

– Increased skin cancerIncreased skin cancer– Increased cataractsIncreased cataracts– Unknown changes to food chainUnknown changes to food chain

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D. ATMOSPHERES D. ATMOSPHERES of of OTHER PLANETSOTHER PLANETS

General Composition Considerations:General Composition Considerations:– Planetary Size Planetary Size

(influences planetary gravity) (influences planetary gravity)– Closeness to Sun Closeness to Sun

(influences temperature) (influences temperature) Atmospheric Composition of PlanetsAtmospheric Composition of Planets

– Inner PlanetsInner Planets– Outer PlanetsOuter Planets

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E. VARIATION OF CHARGED E. VARIATION OF CHARGED PARTICLES WITH HEIGHTPARTICLES WITH HEIGHT

CompositionComposition– Ions: Charged ParticlesIons: Charged Particles

LocationLocation– IonosphereIonosphere– MagnetosphereMagnetosphere

ImplicationsImplications– Radio CommunicationsRadio Communications– Aurora Borealis (Australis)Aurora Borealis (Australis)

The Reason - Active SunThe Reason - Active Sun

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IonosphereIonosphereFigure 1.11 Moran & Morgan (1997)Figure 1.11 Moran & Morgan (1997)

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MagnetosphereMagnetosphereSee Fig. 1.13 Moran & Morgan (1997)See Fig. 1.13 Moran & Morgan (1997)

Northern Lights Planetarium Northern Lights Planetarium

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MAGNETOSPHEREMAGNETOSPHERE

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AURORA BOREALISAURORA BOREALIS (from Univ. of Alaska)(from Univ. of Alaska)

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Aurora from Space ShuttleAurora from Space Shuttle