Lecture 2-07: The greenhouse, global heat engine.

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Lecture 2-07: The greenhouse, global heat engine http://en.wikipedia.org/

the sun s ultraviolet (left) and infrared radiation imagers.gsfc.nasa.gov/ems/uv.html www.odysseymagazine.com/images

SOLAR FLARES (inset: ultraviolet image) 28x2003 cfa-www.harvard.edu/previous/102803.html www.msnbc.msn.com

Wien s law: peak radiation occurs at a wavelenth of 2897/T (in microns...10-6 m, and T in degrees Kelvin) (this comes from Planck s law for radiation of a black body as a function of wavelength and temperature)

www.andor.com/image_lib

From Planck s law follows two more: Wien s formula for the peak of the radiation curve, λ max = 2897/T for the wavelength (hence color ) of maximum radiation from a ideal body with temperature T, and the Stefan-Boltzmann law for the area under the curve, that is the total radiation; F = σt 4 where σ is the constant emissivity, 5.67 x 10-8 watts/(m 2 K 4 )

GLOBAL WARMING www.keele.ac.uk/chem Atkins & de Paula 2005 See Atkins Box 19.1, p 500 The intensity of infrared radiation that would be lost from the Earth in the absence of greenhouse gases is shown by the smooth line. The jagged line is the intensity of the radiation actually emitted. The maximum wavelength of radiation absorbed by each greenhouse gas is indicated.

Water is the main absorber of the sunlight. The 13 million million tons of water in the atmosphere (~0.33% by weight) is responsible for about 70% of all atmospheric absorption of radiation, mainly in the infrared region where water shows strong absorption. It contributes significantly to the greenhouse effect ensuring a habitable planet, but operates a negative feedback effect, due to cloud formation, to attenuate global warming. The infrared radiation strikes a molecule such as carbon dioxide and causes the bonds to bend and vibrate - this is called the absorption of IR energy. The molecule gains kinetic energy by this absorption of IR radiation. This extra kinetic energy may then be transmitted to other molecules such as oxygen and nitrogen and causes a general heating of the atmosphere. Analogy: Think of a partially stretched "toy slinky" - if you bump the slinky, the energy of the bump is absorbed by the vibrations in the slinky. http://www.elmhurst.edu/~chm/vchembook/globalwarma5.html http://www.lsbu.ac.uk/water/vibrat.html scale: 1/wavelength in cm 2000 = 5 µm source: http://www.lsbu.ac.uk/water/vibrat.html

http://www.lsbu.ac.uk/water/vibrat.html

Atmospheric trace gases and their contribution to the greenhouse effect (note water vapor makes the biggest contribution of all yet is not shown here). The major natural greenhouse gases are water vapour, which causes about 36-70% of the greenhouse effect on Earth (not including clouds); carbon dioxide, which causes 9-26%; methane, which causes 4-9%, and ozone, which causes 3-7%. It is not possible to state that a certain gas causes a certain percentage of the greenhouse effect, because the influences of the various gases are not additive. (The higher ends of the ranges quoted are for the gas alone; the lower ends, for the gas counting overlaps.)[2][3] Other greenhouse gases include, but are not limited to, nitrous oxide, sulfur hexafluoride, hydrofluorocarbons, perfluorocarbons and chlorofluorocarbons (see IPCC list of greenhouse gases). (text from Wikipedia).

Infrared radiation upward from the Earth, assuming a 280K temperature red+yellow+blue = total radiation of the earth at +7 C in the range between 400 and 1800 cm-1. blue = radiation that is absorbed by greenhouse gases. yellow = radiation that is allowed to pass by greenhouse gases. (red = absence of an absorption spectrum due to technical reasons concerning the measurements.) http://www.espere.net/unitedkingdom/water/uk_watervapour.html

solar radiation (kilowatt-hours per square meter, per day) varies with latitude and season (here neglecting the great effect of cloudiness) www.fao.org/docrep/003/x6541e/x6541e03.htm

reflected sunshine (upper) and infrared (long-wave) heat radiation (lower) CERES satellite radiometer Jan 2002 clouds, snow, ice, deserts are bright absorbing areas are dark..roughly 30% of incoming radiation is reflected heat emitted from Earth is proportional to the 4 th power of temperature

Single pane of glass model of the greenhouse effect incoming solar radiation, I 0 in watts/meter 2 some is simply reflected back to space I 0 I 0 the rest is absorbed by ocean and land and atmosphere yet re-radiated as infrared heat, both upward and downward (red arrows) Earth s surface 2I 0 I o The net effect of the blanket of atmosphere is to have more downward radiation toward the Earth s surface than just the incident sunlight.

Flow of incoming energy from sun: F in = 1372 watts/m 2 average night and day, tropics, poles: => F in /4 mostly as visible light (wavelengths 400-700 x 10-9 m) Flow of outgoing energy upward from Earth: use black-body formula from physics, F out = σt 4 where σ= 5.67 x10-8 J/m 2 sec o K 4

Observed atmosphere and its greenhouse effect: radiation in watts/m 2 Incoming ¼ x 1372 watts /m 2 = 342 watts/m figure source: Wikipedia reduced by simple reflection (albedo ~ 0.3) to 235. of which 168 reaches the Earth s surface. Yet the total downward radiation (visible + infrared is 492 watts/m 2 which is 3 times the direct, visible light s power. Present human modification of this due to gas emissions/deforestration ~ +2.5 watts/m 2

How cold? The air temperature on 2 Jan 1993 at the surface of the Earth. The cold (blue) air forms a dome in the Arctic, which is dense (heavy) and tends to slide southwater beneath less dense air. This leads to both the overturning circulation and the westerly winds and jet stream.

figure source: EOS 2007 How hot?

Australia, with few mountains, cannot catch the moisture from the sea and has been experiencing severe drought. This is expected to worsen with global warming. Below the red regions show recent anomalously high temperatures.

INFRARED SPECTRUM OF DAVE McGARVEY S BREATH 100 %T 80 60 40 H O H H O H O C O 20 0 4000 3500 www.keele.ac.uk/chem O C O 3000 2500 2000 1500 wavenumber/cm -1 O C O 1000 500

so F in /4 = σ T 4 T = F in /4σ = 255 K = -18 o C snowball Earth? No, 290 K is about our average surface temperature. Albedo effect: some of the sunlight reflects from the whiter regions of Earth (snow, ice particularly), reducing the available sunlight Greenhouse effect: a blanket of water vapor and CO 2 and methane CH 4 traps the upward infra-red long-wave or heat radiation. The pane-of-glass model assumes total absorption of upward infrared waves yet no absorption of visible light..both of which are not completely accurate, hence the numbers are not applicable to the real atmosphere, yet demonstrate the effect. Tropics/poles effect: more sunshine in low latitudes, more upward radiation in high latitudes: =>need a flow of heat from Equator toward poles. called meridional heat transport.