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Email Scott.Denning@ColoState.edu - PowerPoint Presentation

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Email Scott.Denning@ColoState.edu - PPT Presentation

for a copy of this presentation Climate Change Simple Serious Solvable Scott Denning Director of Education ESMEI Atmospheric Science CSU Simple 2 Serious 3 Solvable Simple 2 Serious ID: 777732

surface molecules radiation heat molecules surface heat radiation earth energy thermal wavelengths emission temperature absorbed hot infrared h2o waves

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Slide1

Email

Scott.Denning@ColoState.edu for a copy of this presentation

Climate Change:Simple, Serious, Solvable

Scott DenningDirector of Education, ESMEIAtmospheric Science, CSU

Slide2

Simple

2. Serious3. Solvable

Slide3

Simple

2. Serious3. Solvable

Slide4

Heat Transfer

Conduction is by hot molecules colliding with neighbors

Convection is by hot stuff moving in bulk from place to place

Slide5

Electromagnetic Radiation

Changing electric fields create changing magnetic fields …

and vice versa!

This makes energy move even through empty space

We can see it, feel it

Plants harvest it directly, and we harvest them!

Travels at 3x10

8

m/s

= 186,000 miles / sec !

Distance it goes in one cycle is called the wavelength

Slide6

Electromagnetic Radiation

Radiation travels as waves or photons

Waves do not require molecules to propagate

Shorter waves carry more energy than longer ones

Slide7

Blackbody Emission

Hot objects emit much more than cold objects at every wavelengthPeak emission at shorter waves at higher temperatures

Slide8

Thermal ImagingImages taken in thermal infrared wavelengths (corrected for emissivity) produce accurate measurements of temperature

Slide9

Solar

Emission

Solar radiation has peak intensities in the shorter wavelengths, dominant in the region we know as visible, but extends at low intensity into longwave regions.

Slide10

Both are almost perfect blackbodies!

The hot sun radiates at shorter (visible) wavelengths that carry more energy

Energy absorbed by the cooler earth is then re-radiated at longer (thermal infrared) wavelengths

Thermal EmissionSUNEARTH

Slide11

30% reflected by clouds, air, dust, and surface

19% absorbed by the atmosphere (mostly clouds)

51% absorbed at the surface

Solar Radiation

Slide12

Molecules and PhotonsMolecules

are groups of atoms that share electrons (chemical bonds)Molecular transitions involve changes in vibration, rotation, bending, and stretching of chemical bondsPhotons can interact with molecules to change statesTransitions involve specific amounts of energy, so only certain wavelengths are activeMolecular transitions typically absorb & emit in thermal infrared

Slide13

PhET Simulation

Slide14

Dancing Molecules and Heat Rays!

Nearly all of the air is made of oxygen (O2) and nitrogen (N2) in which two atoms of the same element share electronsInfrared (heat) energy radiated up from the surface can be absorbed by these molecules, but not very wellN

N

OO

Diatomic molecules can vibrate back and forth like balls on a spring, but the ends are

identical

No electric dipole!

Slide15

Dancing Molecules and Heat Rays!

Carbon dioxide (CO2) and water vapor (H2O) are different!They have many more ways to vibrate and rotate, so they are very good at absorbing and emitting infrared (heat) radiation

Molecules that have many ways to wiggle are called

“Greenhouse” moleculesO

O

C

H

H

O

Slide16

CO2 Vibrations

15 mm7.2 mm4.3 mmC

CC

COO

O

O

O

O

O

O

Resting or ground state

No dipole … weak!

Temporary electric dipole … strong!

Slide17

H2O Vibrations

Water molecules are “bent!”This gives them a positively charged end (with the hydrogen) and a negatively charged end (with the oxygen) This “permanent dipole moment” allows H2O to absorb & emit photons without moving bonds2.7 mm6.3 mm

Slide18

Earth-Atmosphere Energy Balance

Earth's

surface absorbs the 51 units of shortwave and 96 more of

longwave energy units from atmospheric gases and clouds.These 147 units gained by earth are due to shortwave and longwave greenhouse gas absorption and emittance

.

Earth's surface loses these 147 units through convection, evaporation, and radiation.

Slide19

Greenhouse Effect

CO2O3H2OH2

OHot surface emits directly to space in window regionCold upper layers emit to space in optically thick regionsTotal emission much less than from sfc

Slide20

Bathtub AnalogyIf faucet runs faster than drain, level risesAnd vice versaDrain runs faster when water is deep

Adding glass to layer model acts like a clog in the drainWater rises until drainage = inflow againFaucet ~ SunDrain ~ Thermal emissionWater level ~ temperature

Slide21

Slide22

8 PM surface temperature = 20 °C = 68

°F Spring Nightin Colorado

radiationemittedby soil

420 W m

-2

4 inches

= 10 cm

s

T

4

Slide23

Spring Night

in Colorado8 AM surface temperature = -60 °C = -78 °F radiationemittedb

y soil

420 W m

-2

4 inches

= 10 cm

Slide24

6 AM surface temperature = 10 °C = 50

°F Spring Nightin Coloradoradiation

emittedby soil

420 W m

-2

4 inches

= 10 cm

radiation

emitted

by air

340 W m

-2

Slide25

The strongest evidence for theGreenhouse Effect

is that we can survive night!

Slide26

Common Sense

Doubling CO2 would add 4 watts to every square meter of the Earth, 24/7/365Doing that would make the surface warmerThis was known before light bulbs were invented!

4 Watts

1 m

1 m

John Tyndall, January 1863

Slide27

Common Myth #1

“Scientists expect a warmer future because it’s been warming up recently”

WRONG! It’s because we know that when we add heat to things, they warm up

Slide28

RememberHeat in minus heat out equals change of heat (“First Law Thermodynamics”)Earth can only exchange heat through electromagnetic radiation

Trace gases CO2 and H2O control rate of heat emission by EarthGreenhouse effect makes Earth habitable, allowed life to evolve