heat & deep ocean currents. heat variations latitude depends on angle sunlight hits surface...

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Heat Heat & & Deep Ocean Currents Deep Ocean Currents

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Page 1: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Heat Heat &&

Deep Ocean CurrentsDeep Ocean Currents

Page 2: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Heat VariationsHeat VariationsLatitudeLatitude

• Depends on angle sunlight hits Depends on angle sunlight hits surfacesurface– At equator, sunlight covers less area; more At equator, sunlight covers less area; more

heat heat

– Sunlight at polar latitudes covers wider area; therefore, Sunlight at polar latitudes covers wider area; therefore, less heatless heat

– Mid latitude heating affected by seasonsMid latitude heating affected by seasons

Page 3: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Heat VariationsHeat VariationsSeasonsSeasons

• Earth’s axis tilted 23.5Earth’s axis tilted 23.5° - ° - orbital inclinationorbital inclination– Northern hemisphere – maximum solar energy in Northern hemisphere – maximum solar energy in

summersummer– Southern hemisphere – max. solar energy in our winterSouthern hemisphere – max. solar energy in our winter

Page 4: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Heat BudgetHeat Budget• Heat input = Heat outputHeat input = Heat output

• 100 units = 30 units + 100 units = 30 units + 70 units70 units(from sun)(from sun) (Reflected)(Reflected) (heat Earth)(heat Earth)

• 70 units70 units = 47 units + 23 units = 47 units + 23 units(absorbed by surface)(absorbed by surface)(by atmosphere)(by atmosphere)

Page 5: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Annual Incoming Solar Annual Incoming Solar RadiationRadiation

•Surplus heat between 38Surplus heat between 38°° N&S latitude N&S latitude

• Heat deficit between 38Heat deficit between 38°°-90-90°° N&S latitude N&S latitude

Why don’t oceans evaporate at equator and freeze at poles?Why don’t oceans evaporate at equator and freeze at poles?

Page 6: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Heat TransferHeat Transfer

• Heat is transferred from equator to polesHeat is transferred from equator to poles– Air CirculationAir Circulation– Ocean currentsOcean currents

Page 7: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

SalinitySalinityEvaporation and PrecipitationEvaporation and Precipitation

•Evaporation and precipitation control Evaporation and precipitation control S S ‰‰

• Evaporation > Evaporation > Precipitation = Precipitation = ↑ S ↑ S ‰‰

– Freezing Freezing ↑↑ S S ‰‰

• 00° (equator); 40°-60° N&S° (equator); 40°-60° N&S– Precipitation > EvaporationPrecipitation > Evaporation

– Lower S ‰Lower S ‰

• 1010°-40° N&S°-40° N&S– Evaporation > PrecipitationEvaporation > Precipitation

– High S ‰High S ‰

• 6060°-90° N&S (Polar Region)°-90° N&S (Polar Region)

Page 8: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Ocean SalinitiesOcean Salinities

• S ‰ variations lead to density stratificationS ‰ variations lead to density stratification– ↑ ↑ S ‰; S ‰; ↑density↑density– Denser HDenser H22O sinksO sinks

• Example of stratification (layering) is Atlantic OceanExample of stratification (layering) is Atlantic Ocean

• Two factors that control densityTwo factors that control density– S S ‰‰

– TemperatureTemperature

Page 9: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Atlantic Water MassesAtlantic Water MassesDensity Driven CurrentsDensity Driven Currents

•Atlantic consists of intermediate, deep, and bottom watersAtlantic consists of intermediate, deep, and bottom waters

• Thickness and extent depends on:Thickness and extent depends on:– Rate of formationRate of formation

– Size of region where formedSize of region where formed

Page 10: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Pacific OceanPacific Ocean

• Pacific Ocean not well definedPacific Ocean not well defined– Small region where water formsSmall region where water forms– Limited HLimited H22O supply from northO supply from north

Page 11: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Atlantic Water FlowAtlantic Water Flow

• Dense, cold Polar HDense, cold Polar H22O sinksO sinks

• Current driven by density contrastCurrent driven by density contrast

• Identify water masses by T-S curve and biologyIdentify water masses by T-S curve and biology

Page 12: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

AtlanticAtlanticDeep Water CirculationDeep Water Circulation

• Currents extensive and interconnectedCurrents extensive and interconnected

Page 13: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Upwelling and DownwellingUpwelling and Downwelling

• Wind blows HWind blows H22O horizontallyO horizontally

• Deeper HDeeper H22O rises to O rises to replace surface Hreplace surface H22OO

• UpwellingUpwelling – process of – process of HH22O risingO rising

• Winds moving toward Winds moving toward shore cause Hshore cause H22O to move O to move downwarddownward

• DownwellingDownwelling – process – process of Hof H22O sinkingO sinking

Page 14: Heat & Deep Ocean Currents. Heat Variations Latitude Depends on angle sunlight hits surface Depends on angle sunlight hits surface – At equator, sunlight

Equatorial UpwellingEquatorial Upwelling

• Deep, nutrient-rich HDeep, nutrient-rich H22O is brought to the surfaceO is brought to the surface