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Lab 2 – September 11, 2013 Lab 2 – September 11, 2013

Lab 2 – September 11, 2013 - PowerPoint Presentation

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Lab 2 – September 11, 2013 - PPT Presentation

More on Radiation The Four Seasons Solstice and Equinox Sun Angle and the Surface Seasonality Radiation Review Everything emits radiation Tgt0 Kelvin StefanBoltzmann Law E σT 4 StefanBoltzmann Constant σ 00000000567 Wm ID: 569519

sun radiation surface seasonality radiation sun seasonality surface temperature water energy bodies atmosphere angle head solar equator higher clouds

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Slide1

Lab 2 – September 11, 2013

More on Radiation, The Four Seasons, Solstice and Equinox, Sun Angle and the Surface, SeasonalitySlide2

Radiation Review

Everything emits radiation (T>0 Kelvin)

Stefan-Boltzmann Law:

E = σT4Stefan-Boltzmann Constant σ = 0.0000000567 W/(m2K4)Energy Emitted ∝ Temperature (to the fourth power)

Where is the greatest radiation

measurement? The least?

Note: Temp of Clouds < Temp of SurfaceSlide3

Downwelling Radiation

Downward emission of infrared energy (in our case, from clouds)

Results in higher surface temperatures

e.g. Cloudy nights are typically warmer than clear nights

Intensity of

downwelling

radiation

Increased surface temperaturesSlide4

Incoming Solar Radiation and the Atmosphere

Some solar radiation traveling through the atmosphere is

back-scattered

Solar radiation striking the earth at an angle travels through more atmosphere

Clouds in the atmosphere back-scatter

a lot of incoming sunlight

Which person experiences more intense sunlight?Slide5

The Four Seasons

Earth’s axis always points in the same direction in space

Time-lapse photography showing concentric, circular star trails

What astronomical feature is in the center?Slide6

The Four Seasons

Variations in seasonal temperatures is a result of the Earth’s tilt

Sun Directly over-head at 23.5° S

Sun Directly over-head at 0°

Sun Directly over-head at 0°

Sun Directly over-head at 23.5° NSlide7

Solstice and Equinox

(Northern Hemisphere)

Date

Latitude of Direct Sunlight

Summer SolsticeJune 2123.5° N (Tropic of Cancer)Winter Solstice

December 21

or

22

23.5° S (Tropic of Capricorn)

Autumnal Equinox

September 22

(Equator)Vernal (Spring) EquinoxMarch 200° (Equator)

Note: Solstices are reversed for Southern HemisphereSlide8

Sun Angle and the Surface

The greater the sun angle, the more concentrated the radiation is when it strikes the surfaceSlide9

Seasonality

Annual range of temperature at a location

i.e. swings in temperature between summer and winter

Major controllers in seasonality:LatitudeProximity to large bodies of waterSlide10

Seasonality (Latitude)

Higher latitudes receive widely varying solar radiation throughout the year

Think about hours of daylight in each season

North Pole?Equator?Slide11

Seasonality (Bodies of Water)

Heat Capacity – a measure of the ratio of the amount of energy absorbed (or released) by a substance to the corresponding temperature increase (or decrease)

If it requires 40 units of energy to increase the temperature of one gram of dirt by one Kelvin and requires 120 units of energy to increase the temperature of one gram of water one Kelvin, which substance has a higher heat capacity?

H.C. Water > H.C. LandSlide12

Seasonality (Bodies of Water)Slide13

Seasonality (Bodies of Water)Slide14

Lab 2 Problems

2.7a,b

2.10a,b

2.11a,b2.13a,c,d3.13.43.63.9a,b,cDUE FRIDAY

BEFORE CLASS