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Solar Energy, the Atmosphere and Biomes

Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

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Page 1: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Solar Energy, the Atmosphere and Biomes

Page 2: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Earth-Sun Relationships

Earth’s Motions• Earth has two principal motions—rotation and

revolutionEarth’s Orientation (tilt)• Seasonal changes occur because Earth’s

position relative to the sun continually changes as it travels along its orbit

Page 3: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation
Page 4: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Energy Transfer as HeatThree mechanisms of energy transfer:Conduction is the transfer of heat through matter

by molecular activityConvection is the transfer of heat by circulation

within a substance.Radiation is the transfer of energy (heat) through

space by electromagnetic waves that travel out in all directions

Page 5: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation
Page 6: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

What Happens to Solar Radiation?

• Scattering:–Clouds, dust and gas reflect and bend light

rays; light rays are sent out in all directions–Causes sky to appear blue (blue light is more

easily bent)– Sunsets appear red because longer

wavelengths (red) are able to reach the surface (we are looking through more atmosphere on the horizon)

Page 7: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

What Happens to Solar Radiation?

• Reflection:–20% of solar radiation is absorbed by the

atmosphere–50% is absorbed by the surface–30% is reflected back into space–Albedo: fraction of solar radiation that is

reflected back into space. – Earth’s albedo is 0.3

Page 8: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

What Happens to Solar Radiation?

Absorption & Infrared Energy:• As the surface absorbs radiation, it heats up and

releases IR radiation• IR radiation is trapped by water vapor and CO2 in

the atmosphere• This process is called the greenhouse effect

Page 9: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation
Page 10: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

What Happens to Solar Radiation?

Why Temperatures VaryFactors include:• latitude • heating of land and water, • altitude• geographic position• cloud cover• ocean currents

Page 11: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation
Page 12: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation
Page 13: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Fig. 7-7, p. 145

Prevailing winds pick up moisture from an ocean.

On the windward side of a mountain range, air rises, cools, and releases moisture.

On the leeward side of the mountain range, air descends, warms, and releases little moisture.

Page 14: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Latitude

Tropical Forest

Deciduous Forest

Coniferous Forest

Tundra (herbs, lichens, mosses)

Polar ice and

snow

Fig. 7-9, p. 147

ElevationMountain ice and snowTundra (herbs, lichens, mosses)Coniferous Forest

Deciduous ForestTropical Forest

Stepped Art

Page 15: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Properties of Air

Density• At constant pressure, warm is less dense than

cold air• Therefore, warm air rises, cold air sinks

Page 16: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Properties of Air

Water Vapor Capacity• Warm air has a higher capacity for water• Specific humidity is a measure of the amount

of water vapor in the air• Relative humidity is a ratio of the amount of

water present to the capacity• If RH = 100%, saturation occurs• Dew point is the temperature at which

saturation occurs

Page 17: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Properties of Air

Adiabatic Heating and Cooling• As air rises in the atmosphere rises, P ↓, air

expands and cools• As air sinks toward the surface, P ↑, air

volume ↓ and warms

Page 18: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Properties of Air

Latent Heat Release• As the sun warms surface water, it absorbs

and stores energy as it evaporates• As water vapor in the atmosphere condenses,

it releases this stored (latent) energy

Page 19: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Factors Affecting Wind

• Wind is the result of horizontal differences in air pressure. Air flows from areas of higher pressure to areas of lower pressure

• The unequal heating of Earth’s surface generates pressure differences

• Three factors combine to control wind: pressure differences, the Coriolis effect, and friction

Page 20: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Factors Affecting Wind

Pressure Differences• A pressure gradient is the amount of pressure

change occurring over a given distance• Isobars are lines on a map that connect places

of equal air pressure• Closely spaced isobars indicate a steep pressure

gradient and high winds

Page 21: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Factors Affecting Wind

Coriolis Effect• The Coriolis effect describes how Earth’s

rotation affects moving objects. • In the Northern Hemisphere, all free-moving

objects or fluids, including the wind, are deflected to the right of their path of motion.

• In the Southern Hemisphere, they are deflected to the left

Page 22: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation
Page 23: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation
Page 24: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Factors Affecting Wind

Friction • Friction acts to slow air movement, which

changes wind direction• Jet streams are fast-moving rivers of air that

travel in a west-to-east direction (120 - 240 km/hour); little friction

Page 25: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Global Winds

• Convection Cells:–Warm air rises near the equator–Cooler air from the north replaces it at the

surface–The warm air that rose flows northward

and downward as it cools–The convection cells are called Hadley Cells

Page 26: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Fig. 7-4, p. 143

Heat released radiates to spaceCool, dry

air

Condensation and precipitation

Falls, is compressed, warms

Rises, expands, cools

Warm, dry air

Hot, wet air

Flows toward low pressure, picks up moisture and heat

HIGH PRESSURE Moist surface warmed by sun

LOW PRESSURE

LOW PRESSURE HIGH PRESSURE

Page 27: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Global Winds & Biomes

Page 28: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation
Page 29: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Fig. 7-6, p. 144

Moist air rises, cools, and releases moisture as rainPolar cap

Arctic tundraEvergreen coniferous forest60°

Temperate deciduous forest and grassland

30°Desert

Tropical deciduous forest

Equator 0° Tropical rain forest

30° Desert

60°Temperate deciduous forest and grassland

Tropical deciduous forest

Polar cap

Page 30: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Fig. 7-8, p. 146

Page 31: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Fig. 7-10, p. 147

Cold Polar

TundraSubpolar

TemperateConiferous forest

Desert

Deciduous forest

GrasslandChaparral Tropical

Hot

DesertWet Rain forest Savanna

Tropical seasonal forest

Dry

Scrubland

Page 32: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Biomes

• Tundra• Boreal forest• Temperate rainforest• Temperate seasonal forest• Woodland/shrubland• Tropical rainforest• Subtropical desert

Page 33: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

CURRENTS

Page 34: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Fig. 7-2, p. 142

Page 35: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Fig. 7-5, p. 143

Warm, less salty, shallow current

Cold, salty, deep current

Thermohaline Circulation

Page 36: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

El Nino Southern Oscillation

• 3 – 7 year cycle• Surface currents in the tropical Pacific reverse

direction (trade winds weaken)• Warm water moves westward, suppressing the

upwelling of nutrients off the coast of S. America

• Fish populations are hurt• Global impact: cooler, wetter conditions in SE

US; drier in S Africa, SE Asia

Page 37: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation
Page 38: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Biomes

For your biome PowerPoint:• Describe vegetation and animal life• Describe general climate; include global

location(s)• Include a climate diagram (annual

temperature & rainfall)• 3 – 5 slides; keep it simple!

Page 39: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation
Page 40: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

AQUATIC BIOMESCategorized by salinity, depth, water flow

Page 41: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Streams & Rivers

• Flowing fresh water• Originate from springs or runoff• Rapid flow = few producers; rely on terrestrial

biomes (leaves)• Slow rivers: nutrients settle and provide

substrate for plants• Rapids: high O2 content

Page 42: Solar Energy, the Atmosphere and Biomes. Earth-Sun Relationships Earth’s Motions Earth has two principal motions—rotation and revolution Earth’s Orientation

Lakes and Ponds

• Contain standing water• Divided into distinct zones:• Littoral Zone: shallow area of soil & water

near shore; rooted plants, photosynthesis• Limnetic Zone: rooted plants cannot survive;

phytoplankton photosynthesize• Profundal Zone: deep lakes; low O2 due to

decomposers; muddy bottom: benthic zone