Week 3: Earth's Atmosphere and Greenhouse Effect

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36 Terms

1
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How is matter bound together?

  • Electric fields

  • Atoms bound by sharing electrons

  • Atoms aggregated into gases, liquids/ solids bound by electric forces

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Why is it important for the climate that ice is less dense than water?

  • if water froze and it sunk instead of sitting on top of the water

  • lower albedo of earth as albedo of ice is very high

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How can the state of matter be changed?

Only if EM of the right frequency interacts with it

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The Molecular Absorption Spectra

  • Molecules absorb at more frequencies than atoms

  • Various processes broaden the absorption spectra of molecules

    • collisions/ pressure broadening

    • doppler shift

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What makes a molecule a good absorber of EM radiation?

  • Molecules with an electric dipole

  • Symmetric electrical fields e.g N2 and O2 don’t absorb IR

  • CO2 is symmetric but can produce an electric dipole if distorted → IR absorption for vibrations

  • H2O has a dipole in resting state → IR absorption for vibrations and rotations

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What does Planck’s Law give?

  • the intensity of black-body radiation as a function of wavelength and temperature, i.e. the shapes of the black-body radiation curves

  • Planck’s law is an idealisation → real bodies don’t absorb or emit all wavelengths of light

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How can you calculate thermal emission from real bodies?

Product of Planck’s Law and the Body’s Emissivity

Bλ (λ,T) × ε(λ

  • both functions of wavelength

  • Planck’s law sets the maximum thermal emission for the body.

  • The emissivity sets the fraction of this maximum that is realized at each frequency / wavelength, i.e. the efficiency with which it emits

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What is Kirchoff’s Law?

Absorptivity (aλ ) = emissivity (ελ )

Things are as good at absorbing EM radiation of a specific wavelength as they are at emitting it → absorption lines = emission lines

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How are emissivity and absorptivity measured?

  • As a fraction

  • Range between 0 and 1

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How are concentrations of gases in the atmosphere expressed?

parts per million by volume (ppmv)

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Which gases in the atmosphere have a significant radiative effect?

  • CO2 (~410 ppmv), Methane (1.9 ppmv), Water Vapour

  • ^ have 3 or more parts and so more complex vibrations

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What is the dominant greenhouse gas in the Earth’s atmosphere?

  • Water Vapour

  • Absorbs strongly in many bands

  • Weakly absorbing in atmospheric window

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Where is the atmospheric window?

  • Between ~8 and ~14 ÎĽm

  • Around the peak of Earth’s black-body spectrum

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Why does CO2 have a greater greenhouse effect than H2O?

  • CO2 absorbs over a narrower range of frequencies than water but it has a strong absorption band in the atmospheric window

  • Gases which absorb wavelengths in the atmospheric window can have a greenhouse effect

  • Greenhouse gases (GHGs) are most effective if they absorb frequencies that other GHGs don’t.

  • If they were all absorbing the same frequencing→ less of the spectrum in total absorbed

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Absorption of light by the atmosphere

Some frequencies of incoming light are absorbed by the atmosphere

  • Water vapour absorbs some bands of the near-infrared

  • Ozone absorbs UV strongly

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Where does the blackbody spectrum show emission from?

  • Reflects the temperature and altitude of the last layer which emitted it

  • The Earth’s longwave spectrum follows the black-body spectrum for the surface where it is transparent and the cooler upper atmosphere where it is strongly absorbing

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What is radiative forcing?

measure of the influence a factor has in altering the balance of incoming and outgoing energy in the Earth system.

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Units of radiative forcing

Wm-2

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What effect does a positive radiative forcing have?

  • A positive radiative forcing will cause the Earth to absorb more energy and warm.

  • As it warms it will emit more longwave radiation (Stefan-Boltzmann law) and eventually a new equilibrium temperature will be reached when incoming and outgoing energy balances again

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As you increase the amount of CO2 in the atmosphere, what effect does it have on outgoing longwave radiation

0 → 10 ppmv takes a big bite out of the spectrum and has a large radiative forcing

400 → 410 ppmv has a tiny radiative forcing.

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What does band saturation do?

  • At current CO2 conc. → increasing conc. leads to diminishing increases in radiative forcing due to band saturation

  • Frequencies most effectively absorbed have all been absorbed

  • Increasing CO2 increases absorption at tails of distribution

  • CO2 radiative forcing does not increase linearly with CO2 concentration

  • CO2 absorbs all long-wave emitted from the surface around its peak absorption frequency, and exponentially weakly away from this peak.

22
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Radiative Forcing of CO2

proportional to the number of doublings of the CO2 concentration, i.e., it follows a logarithmic function:

RFCO2 = 3.71 x ln(C/ C0) / ln (2) Wm-2

  • This is because of band saturation

23
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Ideal gas assumptions

  • Molecules are point particles (imagined as tiny balls)

  • Have elastic interactions (don’t lose energy after collision)

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When do assumptions about ideal gases break down?

  • At very high pressure and low temperature

  • Assumption works well for atmospheric conditions

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Equation showing the relationship between kinetic energy of an ideal gas and its temperature

EK = 3/2 nRT

n = number of moles

R= ideal gas constant

T= temperature in Kelvin

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Force =

Mass x Acceleration

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Unit of force

1 Newton (N) = 1 kg ms-2

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Pressure =

force/ area

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Units of Pressure

1 Pascal (Pa)= 1 Nm-2

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What is pressure against a box determined by?

  • Number of collisions over area

  • Kinetic energy of colliding particles

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Ideal Gas Law

PV = nRT

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What does pressure in the ocean depend on?

  • Function of depth

Water:

  • Is effectively incompressible.

  • Pressure is proportional to depth as the weight of water above you increases monotonically

  • Every 10m deeper, pressure rises by 1 atmosphere (atm)

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What does pressure in the atmosphere depend on?

  • Pressure as a function of altitude

Air:

  • Is compressible

  • Air at the bottom is compressed by the weight of air above.

  • Pressure falls exponentially with altitude

<ul><li><p>Pressure as a function of altitude </p></li></ul><p></p><p>Air:  </p><ul><li><p>Is compressible</p></li><li><p>Air at the bottom is compressed by the weight of air above.</p></li><li><p>Pressure falls exponentially with altitude</p></li></ul><p></p>
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What is the scale height of the earth?

8 km

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What is the air pressure at sea level?

1 atm

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What is the air pressure at 8 km?

  • e-1

  • e-folding height

  • every 8 km it falls by the same fraction

  • Most of the mass of the atmosphere is below 8 km