Climate change 101 - Introduction to Climate Change Science (UNDP presentation)
Introduction to Climate
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Transcript of Introduction to Climate
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Introduction to ClimateIntroduction to Climate
Geography 1050Geography 1050
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Weather and Weather and ClimateClimate
Weather: daily phenomenaoMarked fluctuationsoCan be predicted 7-10 days in advanceoHighly variable from year to year
Climate: long-term average of weather conditions
o30 – 50 year average
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Climate ParametersClimate Parameters
If you were trying to describe the climate of If you were trying to describe the climate of northeast Avalon to your distant cousin in northeast Avalon to your distant cousin in Melbourne, Australia, what would you say?Melbourne, Australia, what would you say?
TemperatureTemperature Precipitation (rain, snow)Precipitation (rain, snow) WindsWinds SunshineSunshine Other things of interestOther things of interest
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Climate FactorsClimate Factors
• elevation• latitude• prevailing winds• topographic barriers• ocean currents• proximity to the ocean (or a large lake)
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Torngat Mts
Mealy Mts
Examples from Labrador
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• higher altitude = cooler temperatures
• 22 active glaciers in the Torngat Mountains
active tundra conditions on the Mealy Mountain summits compared to boreal forest along Lake Melville
ElevationElevation
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LatitudeLatitude• Temperatures decrease northward
• linked to solar insolation (length of day, Solar angle)
Hebron 58° 12’ N
Near Hopedale, 55° N
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Prevailing Winds and TopographyPrevailing Winds and Topography
Westerly winds (from west)Westerly winds (from west) Effect of Labrador Current limitedEffect of Labrador Current limited Winds funnelled along fjordsWinds funnelled along fjords
Interior Labrador has:
• lighter winds
• colder winters, but less wind chill
• warmer summers
Molson Lake, Lab. West
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Labrador Current Labrador Current & Proximity to the Ocean& Proximity to the Ocean
Reduces summer temperatures
Increases winter temp, but sea ice cover limits influence
topographic influencesHutton Beach, Iron Strand
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InsolationInsolation
Incoming solar radiationIncoming solar radiation ultimate source of energy for Earth ultimate source of energy for Earth reaches upper limit of atmosphere as reaches upper limit of atmosphere as
visible light, near infrared and visible light, near infrared and ultraviolet radiationultraviolet radiation
amount of insolation supplied by amount of insolation supplied by Sun varies systematicallySun varies systematically
e.g. sunspot cycles from 11 - 1000s e.g. sunspot cycles from 11 - 1000s of yearsof years
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Seasonal VariationSeasonal Variation
distance of Earth from Sun varies
146,000,000 km (perihelion, January 3)
152,000,000 km (aphelion, July 4)
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Earth’s AtmosphereEarth’s Atmosphere
The atmosphere is vital for maintaining life on The atmosphere is vital for maintaining life on Earth because it:Earth because it:
shields the Earth from harmful radiationshields the Earth from harmful radiation helps redistribute energy on Earthhelps redistribute energy on Earth reduces heat losses from Earthreduces heat losses from Earth provides a water transfer and storage facilityprovides a water transfer and storage facility
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Modal Atmospheric ChemistryModal Atmospheric ChemistryGas Proportional
Volume (dry air)Nitrogen (N2) 78.08 %Oxygen (O2) 20.95 %Argon (Ar) 0.93 %Carbon dioxide (CO2) 375 ppmNeon (Ne) 18.2 ppmHelium (He) 5.2 ppmMethane (CH4) 1.7 ppmKrypton (Kr) 1.1 ppmHydrogen (H2) 0.5 ppmNitrous oxide (N2O) ≤ 0.1 ppm
Sulphur dioxide (SO2)& S-aerosols ≤ 0.1 ppmOzone (O3) ≤ 0.001 ppm- Dry air, lowest troposphere
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Present Present situationsituation
14 %
25%
Earth 53%:
Direct 31%,
Diffused 22 %
Albedo
Radiated
Absorbed
• 47% of Insolation does not reach Earth surface
• less than 47% of the total insolation is available for conversion into long-wave (infrared) radiation
Insolation
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When insolation reaches surface …When insolation reaches surface …
Insolation absorbed by Insolation absorbed by EarthEarth
Albedo- % of incoming Albedo- % of incoming radiation that is radiation that is reflected reflected
Changes in albedo Changes in albedo causes further change causes further change (positive feedback)(positive feedback)
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After Adsorption…After Adsorption…
subsequently reradiated as long-wave subsequently reradiated as long-wave thermal infrared radiationthermal infrared radiation
slightly <50% of total provided by Sunslightly <50% of total provided by Sun Thermal infrared radiation responsible for Thermal infrared radiation responsible for
warming warming Must be retained in atmosphereMust be retained in atmosphere
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Trapping Thermal IRTrapping Thermal IR
Thermal IR responsible for warming EarthThermal IR responsible for warming Earth depends upon successful trapping by depends upon successful trapping by
greenhouse gases (GHG):greenhouse gases (GHG): COCO22 (carbon dioxide) (carbon dioxide)
CHCH44 (methane) (methane)
NONO22 (nitrous oxide) (nitrous oxide) and water vapour and water vapour
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Contrasting NeighboursContrasting Neighbours Mars: low greenhouse Mars: low greenhouse
gas concentrationsgas concentrations Mean temp -63Mean temp -63°C°C
Venus: high greenhouse Venus: high greenhouse gas concentrationsgas concentrations
Mean temp 464Mean temp 464°C°C
Mars: astrogeology.usgs.gov; Venus: www.bnsc.gov.uk
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Current Earth SituationCurrent Earth Situation
COCO22 – 375 ppm – 375 ppm
CHCH44 (methane) – 1.8 ppm (methane) – 1.8 ppm water vapour (0-4 %)water vapour (0-4 %) Together, trap about half Together, trap about half
the thermal IR emitted the thermal IR emitted from Earth’s surfacefrom Earth’s surface
< 25% of original < 25% of original insolationinsolation
Mean Surface Temp 16°C
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““Greenhouse Effect”Greenhouse Effect”
•naturally occurring phenomenon• necessary for life on Earth• maintains temp. at 16°C, • but … Changes in the concentrations of GHGs will impact climate