Waves and Modern Physics 203-SN3-RE • CEGEP, Montreal
Corrected exercises: greenhouse effect, albedo and radiative forcing (203-SN3-RE)
This is a set of fifteen corrected exercises on the greenhouse effect, albedo and radiative forcing, the second half of element 4 of the course 203-SN3-RE (formerly 203-NYC), Waves and Modern Physics, in the revised Natural Science program (200.B1). The course outline asks students to evaluate the effects of radiative forcing and of the greenhouse effect on global warming: here we do it with the tools of the course, the Stefan-Boltzmann law, Wien's law, the photon and differential calculus.
Part A builds the radiative budget of a planet, from the solar constant to the single-layer model and the forcing of CO₂. Part B moves on to the mechanisms that decide how large the warming is: the Planck response, feedbacks, Arctic ice, the link with the stoichiometry of combustion, and a comparison with Venus and Mars. Part C goes through the classics, from snowball Earth to the energy budget of the surface.
The thread of the set: a planet is in equilibrium when it sends back to space exactly the energy it absorbs. Any disturbance of this balance, a forcing, is paid for in degrees until the outgoing radiation catches up with the incoming radiation. Before every calculation, ask yourself what comes in, what goes out, and at what temperature the two become equal.
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•Solar constant: S=4πd2L≈1361 W/m² for the Earth. Mean flux per square metre of surface: 4S, the ratio of the sphere 4πR2 to the intercepting disc πR2.
•Albedo α: the fraction of solar radiation that is reflected. Mean absorbed flux: (1−α)4S, that is 238 W/m² for α=0.30.
•Radiative equilibrium temperature: σTe4=(1−α)4S, which gives Te≈255 K for the Earth, against 288 K observed at the surface.
•Wien's law: λmaxT=2.898×10−3 m·K. Sun: visible; Earth: infrared near 10 µm, where H₂O, CO₂ and CH₄ absorb.
•Single-layer model with absorptivity f: Ts=Te(2−f2)1/4; opaque layer (f=1): Ts=21/4Te.
•Radiative forcing of CO₂: ΔF=5.35lnC0C W/m², that is 3.7 W/m² per doubling.
•Planck response: λP=4σTe3≈3.7 W/(m²·K). With feedbacks of factor g<1: ΔT=λP(1−g)ΔF.
•Time response of a reservoir of heat capacity C: CdtdT=ΔF−λT, hence T(t)=λΔF(1−e−t/τ) with τ=λC.
Part A: the basics (/50)
Exercise 1: From the Sun to the Earth: the solar constant and the factor of 4
The luminosity of the Sun is L=3.828×1026 W and the mean Earth-Sun distance is d=1.496×1011 m. Radius of the Earth: R=6.371×106 m. The mean albedo of the Earth is α=0.30. The diagram below, not to scale, shows the situation.
a) Calculate the solar constant S, the flux received on a surface perpendicular to the rays at the distance of the Earth.
b) Calculate the total power intercepted by the Earth.
c) Calculate the mean solar flux received per square metre of the Earth's surface.
d) Where does the factor 4 between S and this mean flux come from?
e) Calculate the mean flux absorbed by the Earth, per square metre.
Show the solution
Answers
a)S=1361 W/m²
b)P=1.74×1017 W
c)S/4=340 W/m²
d)Sphere 4πR2 over disc πR2
e)238 W/m²
a)
The power of the Sun is spread over a sphere of radius d: S=4πd2L=4π×(1.496×1011)23.828×1026=1361 W/m².
b)
The Earth intercepts the beam as a DISC of radius R: P=πR2S=π×(6.371×106)2×1361=1.74×1017 W.
c)
On average over a day and over the whole globe, this power is spread over the entire SPHERE: 4πR2πR2S=4S=340 W/m².
d)
It is the ratio of the surface area of the sphere, 4πR2, to that of the shadow disc, πR2. It combines two effects: half of the globe is in night, and on the lit half the rays arrive at a slant on average.
e)
30 % is reflected: (1−α)4S=0.70×340=238 W/m². This is the flux that the Earth must re-emit to space in order to stay in equilibrium.
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Exercise 2: Radiative equilibrium temperature and sensitivity to albedo
A planet with no atmosphere, which absorbs (1−α)4S and radiates like a blackbody σTe4, reaches an equilibrium temperature Te. Data: S=1361 W/m², α=0.30, σ=5.67×10−8 W/(m²·K⁴). The mean temperature observed at the surface of the Earth is 288 K. The diagram below shows the situation.
a) Calculate Te for the Earth.
b) What gap, in kelvins, separates the observed temperature from Te?
c) Show that dαdTe=−4(1−α)Te and calculate this derivative.
d) Estimate the change in Te if the albedo goes from 0.30 to 0.31.
e) What is the gap in part b) due to?
Show the solution
Answers
a)Te=254.6 K
b)33 K
c)−90.9 K per unit of albedo
d)ΔTe≈−0.91 K
e)The greenhouse effect
a)
σTe4=(1−α)4S, so Te=(4×5.67×10−80.70×1361)1/4=254.6 K, or about −19 °C.
b)
288−254.6=33 K. Without this extra warming, the surface would be frozen on average.
c)
Te=(4σS)1/4(1−α)1/4, so dαdTe=−41(4σS)1/4(1−α)−3/4=−4(1−α)Te. Numerically: −2.8254.6=−90.9 K per unit of albedo.
d)
To first order: ΔTe≈−90.9×0.01=−0.91 K. The exact calculation gives 253.7 K, which is also −0.91 K: the linearization is excellent for such small changes. One hundredth of albedo is almost a degree.
e)
To the GREENHOUSE EFFECT: the atmosphere, transparent to most of the solar radiation, absorbs a large part of the infrared radiation emitted by the surface and sends part of it back down. The surface therefore receives more than the 238 W/m² of solar radiation and must be warmer to re-emit it.
Exercise 3: Two radiations that do not overlap
The Sun radiates like a blackbody at 5772 K, the Earth like a blackbody at about 255 K. Wien's law: λmaxT=2.898×10−3 m·K. Planck's constant h=6.63×10−34 J·s, c=3.00×108 m/s. The diagram below shows the situation.
a) Calculate the wavelength of maximum emission of the Sun, in nm.
b) Calculate that of the radiation from the Earth, in µm.
c) By what factor do the two wavelengths differ?
d) Calculate the energy of a photon at the terrestrial λmax, in eV (1 eV =1.60×10−19 J).
e) Why does this shift allow the atmosphere to let solar energy in while holding terrestrial energy back?
Show the solution
Answers
a)502 nm
b)11.4 µm
c)Factor 22.6
d)E≈0.109 eV
e)Selective absorption in the infrared
a)
λmax=57722.898×10−3=5.02×10−7 m =502 nm, in the visible.
b)
λmax=2552.898×10−3=1.14×10−5 m =11.4 µm, in the thermal infrared.
c)
Wien's law makes λmax inversely proportional to T: the ratio of the wavelengths is the ratio of the temperatures, 2555772=22.6. The two spectra, each about a factor of ten wide around its maximum, barely overlap: we speak of “shortwave” and “longwave” radiation.
d)
E=λhc=1.14×10−56.63×10−34×3.00×108=1.75×10−20 J =0.109 eV. This energy matches the gaps between VIBRATIONAL levels of molecules such as CO₂ and H₂O, whereas a visible photon, twenty times more energetic, does not excite them.
e)
Absorption depends on wavelength. Greenhouse gases (H₂O, CO₂, CH₄), transparent in the visible, absorb strongly in the infrared, where their molecules have vibrational modes. Because the two radiations occupy separate ranges, the atmosphere can be nearly transparent to one and nearly opaque to the other.
Exercise 4: The single-layer model, with a partially absorbing atmosphere
The atmosphere is modelled as a single layer, transparent to solar radiation, which absorbs a fraction f of the infrared radiation from the surface and radiates fσTa4 upward and the same amount downward. The surface, at Ts, receives (1−α)4S=σTe4 with Te=254.6 K. We accept that this model leads to Ts=Te(2−f2)1/4 and Ta=21/4Ts.
a) Calculate Ts for a layer that is totally opaque to infrared (f=1).
b) What value of f gives the observed temperature Ts=288 K?
c) Then calculate the temperature Ta of the layer.
d) Calculate the infrared flux that the layer sends back to the surface.
e) Check the equilibrium of the surface: compare what it receives ((1−α)S/4 plus the flux from part d) with what it emits, σTs4.
Show the solution
Answers
a)Ts=302.8 K
b)f≈0.78
c)Ta≈242 K
d)152 W/m²
e)238+152=390=σTs4
a)
Ts=21/4Te=1.189×254.6=302.8 K. An opaque atmosphere overestimates the greenhouse effect by 15 K: the real atmosphere lets part of the infrared escape through the “window” from 8 to 13 µm.
b)
(254.6288)4=2−f2, so 1.637=2−f2 and f=2−1.6372=0.78. The atmosphere of the model absorbs 78 % of the radiation from the surface.
c)
Ta=1.189288=242 K. The layer is colder than the surface: that is what lets it hold energy back, since it radiates less to space than the surface sends it.
d)
fσTa4=0.779×5.67×10−8×242.24=152 W/m².
e)
Received: 238+152=390 W/m². Emitted: σ×2884=390 W/m². The equality holds, and it shows the key to the mechanism: the surface receives MORE than the solar energy, because the atmosphere returns part of it.
Exercise 5: The radiative forcing of carbon dioxide
Radiative forcing ΔF is the change in the energy balance at the top of the atmosphere caused by a disturbance, before any response of the temperature. For CO₂, an empirical formula gives ΔF=5.35lnC0C in W/m². For methane, neglecting band overlaps, ΔF≈0.036(M−M0), with M in ppb.
a) Calculate the forcing due to CO₂ rising from 280 ppm (preindustrial era) to 420 ppm.
b) Calculate the forcing of a doubling of the preindustrial concentration.
c) What fraction of the forcing of a doubling is already reached at 420 ppm?
d) Calculate the forcing of methane rising from 722 to 1900 ppb.
e) Why does the forcing of CO₂ grow like a logarithm, and not in proportion to the concentration?
Show the solution
Answers
a)ΔF=2.17 W/m²
b)3.71 W/m²
c)58.5 %
d)0.60 W/m²
e)Absorption band saturated at its centre
a)
ΔF=5.35ln280420=5.35ln1.5=2.17 W/m².
b)
ΔF2×=5.35ln2=3.71 W/m². Note that it does not depend on the starting concentration: every doubling adds the same forcing.
c)
ln2ln1.5=0.585: with only half of the way covered in concentration (+140 ppm out of +280), 58.5 % of the forcing is already there.
d)
ΔF=0.036(1900−722)=0.036×(43.59−26.87)=0.60 W/m², a little over a quarter of that of CO₂ although the concentration is two hundred times smaller: molecule for molecule, methane is far more effective.
e)
At the centre of the CO₂ absorption band near 15 µm, the atmosphere is already SATURATED: adding gas there changes almost nothing. The additional forcing comes from the wings of the band, where absorption increases more and more slowly. Hence slow, logarithmic growth; methane, less saturated, follows a square-root law.
Part B: problems and reasoning (/50)
Exercise 6: The Planck response and the feedback factor
A planet that warms by ΔT emits more to space, which brings the balance back toward equilibrium: this is the Planck response. The emission is modelled by F=σTe4 with Te=254.6 K. Feedbacks (water vapour, ice, clouds) amplify the response: if ΔT0 is the warming without feedback, the final warming is ΔT=1−gΔT0, where g is the feedback factor. Forcing of a doubling of CO₂: 3.71 W/m². The diagram below shows this feedback loop.
a) Calculate λP=dTdF at Te, in W/(m²·K).
b) Calculate the warming ΔT0 from a doubling of CO₂ with no feedback at all.
c) With g=0.60, calculate the final warming.
d) What value of g would give a warming of 4.5 K?
e) What would happen if g reached 1?
Show the solution
Answers
a)λP=3.74 W/(m²·K)
b)ΔT0≈0.99 K
c)ΔT≈2.5 K
d)g≈0.78
e)Runaway: the response diverges
a)
λP=dTd(σT4)=4σTe3=4×5.67×10−8×254.63=3.74 W/(m²·K). Each extra kelvin sends 3.74 W/m² more back to space.
b)
The warming offsets the forcing when λPΔT0=ΔF: ΔT0=3.743.71=0.99 K. With no feedback, a doubling of CO₂ would warm the planet by about one degree.
c)
ΔT=1−0.600.99=2.5 K. Feedbacks multiply the basic response by 2.5. The main one is water vapour: warmer air holds more of it, and it is itself a greenhouse gas.
d)
1−g=4.50.99, so g=0.78. Going from 2.5 K to 4.5 K takes only a slightly larger feedback factor: this is why the uncertainty on feedbacks, especially that of clouds, dominates the uncertainty on future warming.
e)
The denominator would vanish: the response would no longer have a finite value, and a small disturbance would trigger a runaway with no equilibrium state. This is the “runaway greenhouse effect” invoked for Venus. For the Earth today, g<1: feedbacks amplify, but the system remains stable.
Exercise 7: The ice-albedo feedback in the Arctic
At the end of summer, Arctic sea ice has lost about 4.0×106 km² compared with the 1980s. Ice has an albedo of 0.60, open ocean 0.07. Take a mean solar flux of 200 W/m² at the surface during the four months of the melt season, and zero for the rest of the year. Surface area of the Earth: 5.10×108 km². The diagram below shows the situation.
a) Calculate the extra solar power absorbed during the melt season.
b) Express this power as a mean flux over the whole surface of the Earth, during the season.
c) Express it as an annual average.
d) Compare with the forcing of CO₂ since the preindustrial era (2.17 W/m²): what percentage does it represent?
e) Why is this called a positive feedback?
Show the solution
Answers
a)ΔP≈4.2×1014 W
b)0.83 W/m²
c)0.28 W/m²
d)About 13 %
e)It amplifies its own cause
a)
Each square metre that changes from ice to water absorbs an extra (0.60−0.07)×200=106 W. Over 4.0×1012 m²: ΔP=4.0×1012×106=4.2×1014 W. Watch the square kilometres: 1 km² =106 m².
b)
5.10×10144.24×1014=0.83 W/m².
c)
The season lasts only a third of the year: 30.83=0.28 W/m².
d)
2.170.28=0.13: about 13 % of the forcing of CO₂, from an area that does not even cover 1 % of the globe. The estimate is rough (clouds, sun angle, spring ice), but the order of magnitude is right.
e)
Because the effect reinforces its own cause: warming melts the ice, the surface becomes darker, it absorbs more energy, which warms it further and melts even more ice. A negative feedback, on the other hand, would oppose the disturbance, like the Planck response.
Exercise 8: Five statements to correct
Each of the following statements is false, or false through a decisive detail. Choose the correct statement and justify it. Two points each.
a) “The greenhouse effect is caused by the hole in the ozone layer.”
b) “The greenhouse effect is a harmful phenomenon that should be eliminated.”
c) “CO₂ warms the atmosphere because it absorbs sunlight.”
d) “Water vapour is not a greenhouse gas, since clouds cool the planet.”
e) “A garden greenhouse heats up by exactly the same mechanism as the Earth's atmosphere.”
Show the solution
Answers
a)UV and ozone; infrared and the greenhouse effect
b)Without it, about −19 °C
c)It absorbs terrestrial infrared
d)Main greenhouse gas, acting as a feedback
e)The greenhouse mainly blocks convection
a)
Two distinct phenomena. The ozone hole lets more ULTRAVIOLET reach the ground, a health problem caused by CFCs. The greenhouse effect concerns the INFRARED emitted by the surface. CFCs are also powerful greenhouse gases, which keeps the confusion alive, but the hole itself is not the cause of the warming.
b)
Without the greenhouse effect, the mean surface temperature would be about 255 K, or −19 °C, instead of 15 °C. The natural phenomenon makes the Earth habitable; it is its STRENGTHENING by human emissions, of the order of 2 W/m² of forcing, that is the problem.
c)
CO₂ is almost transparent to solar radiation, which is mostly visible. It absorbs the INFRARED emitted by the surface and the atmosphere, in particular near 15 µm, and then re-emits it in all directions, including toward the ground.
d)
Water vapour is the MAIN greenhouse gas, by its total contribution. But its concentration is set by temperature, not by our direct emissions: it acts as a FEEDBACK that amplifies the warming caused by CO₂. Clouds have a double effect: they reflect sunlight and they hold back infrared.
e)
A garden greenhouse heats up mainly because its glass BLOCKS CONVECTION: the air warmed at ground level cannot rise and be replaced. Wood's experiment (1909), with a pane transparent to infrared, showed this. The atmosphere has no lid: it works by absorbing and re-emitting infrared radiation. The name is an analogy, not an identity.
Exercise 9: Problem: from combustion to the rise in atmospheric CO₂
Gasoline is modelled as octane C₈H₁₈ (M=114.23 g/mol), of density 0.70 kg/L, which burns according to 2C8H18+25O2→16CO2+18H2O. M(CO2)=44.01 g/mol. In the atmosphere, 1 ppm of CO₂ corresponds to 7.8 billion tonnes (Gt) of CO₂. Humanity emits about 40 Gt of CO₂ per year, of which 45 % remains in the atmosphere. The diagram below shows the situation.
a) Calculate the mass of CO₂ produced by burning 1.0 L of gasoline.
b) A car uses 7.5 L/100 km and travels 15,000 km per year. Calculate its annual emissions, in tonnes.
c) Calculate the yearly rise in the atmospheric concentration of CO₂, in ppm/yr.
d) At this constant rate, how many years does it take to go from 420 to 560 ppm, double the preindustrial value?
e) Why does the mass of CO₂ produced exceed the mass of gasoline burned?
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Answers
a)2.16 kg of CO₂ per litre
b)2.4 t per year
c)2.3 ppm/yr
d)About 61 years
e)The oxygen of the air goes into the CO₂
a)
0.70 kg of octane, so n=114.23700=6.13 mol. From the equation, 1 mol of octane gives 8 mol of CO₂: 49.0 mol, that is 49.0×44.01=2.16×103 g =2.16 kg.
b)
15,000 km at 7.5 L/100 km: 1125 L, so 1125×2.16=2.43×103 kg =2.4 t of CO₂ per year.
c)
40×0.45=18 Gt remain in the air, that is 7.818=2.3 ppm/yr, the order of magnitude of current measurements.
d)
2.31560−420=61 years. In practice emissions are not constant, but the calculation shows what a business-as-usual scenario implies.
e)
The carbon of the gasoline combines with the oxygen of the AIR: each carbon atom (12 g/mol) leaves in a CO₂ molecule of 44 g/mol. The mass of the dioxygen consumed is added, and conservation of mass is respected.
Exercise 10: Problem: Venus, Earth and Mars
Three planets are compared. Solar constant at the distance of the Earth S=1361 W/m²; distances to the Sun: Venus 0.723 AU, Mars 1.524 AU. Albedos: Venus 0.77, Mars 0.25. Observed surface temperatures: Venus 737 K, Mars 210 K. σ=5.67×10−8 W/(m²·K⁴). In a model with n opaque layers, the surface reaches Ts=(n+1)1/4Te. The diagram below places the three planets, distances to scale.
a) Calculate the solar constant at the distance of Venus.
b) Calculate the equilibrium temperature of Venus.
c) Calculate that of Mars.
d) How many opaque layers would be needed to explain the surface temperature of Venus?
e) Venus receives almost twice as much flux as the Earth, and yet its equilibrium temperature is lower. Why?
Show the solution
Answers
a)SV≈2604 W/m²
b)Te≈227 K
c)Te≈210 K
d)n≈111
e)Albedo 0.77: it absorbs less than the Earth
a)
The flux falls off as d21: SV=0.72321361=2604 W/m².
b)
Te=(4σ0.23×2604)1/4=227 K. The surface is at 737 K: the Venusian greenhouse effect is worth more than 500 K.
c)
SM=1.52421361=586 W/m² and Te=(4σ0.75×586)1/4=210 K, exactly the observed temperature: the very thin Martian atmosphere has practically no greenhouse effect.
d)
(n+1)=(226.7737)4=112, so n≈111 layers. The atmosphere of Venus, 93 times more massive than that of the Earth and made almost entirely of CO₂, is opaque to infrared over an enormous thickness: the figure gives an order of magnitude, not a real number of layers.
e)
Its albedo of 0.77: its sulfuric acid clouds send back more than three quarters of the radiation. Venus absorbs only 0.23×42604=150 W/m², less than the 238 W/m² of the Earth. Its scorching surface comes not from the flux received but from the greenhouse effect.
Part C: the classics (/50)
Exercise 11: Snowball Earth and its two equilibria
About 700 million years ago, the Earth is thought to have been almost entirely covered in ice. We use the single-layer model again, with absorptivity f=0.78, where Ts=Te(2−f2)1/4 and σTe4=(1−α)4S, with S=1361 W/m² and σ=5.67×10−8 W/(m²·K⁴). An ice-covered planet has an albedo of about 0.60. The diagram below shows the situation.
a) Calculate the equilibrium temperature Te of an ice-covered Earth.
b) Calculate its surface temperature Ts.
c) Can this planet escape the glaciation by itself?
d) What maximum albedo would allow Ts=273 K to be reached with the same atmosphere?
e) With the same Sun, the present-day Earth (α=0.30) is at 288 K. What do we conclude?
Show the solution
Answers
a)Te≈221 K
b)Ts≈250 K
c)No, the ice-covered state is stable
d)α≈0.44
e)Two equilibria: hysteresis
a)
Te=(4×5.67×10−80.40×1361)1/4=221 K.
b)
(1.222)1/4=1.1315, so Ts=221.3×1.1315=250 K, or −23 °C.
c)
No: at 250 K the ice does not melt, the albedo stays at 0.60 and the planet stays cold. The ice-covered state is STABLE. In reality, it was the slow accumulation of volcanic CO₂, no longer absorbed by rock weathering under the ice, that eventually increased f and freed the planet.
d)
We need Te=1.1315273=241.3 K, so 1−α=S4σTe4=0.565 and α=0.44. The albedo would have to drop from 0.60 to 0.44, which a frozen surface cannot do on its own.
e)
For the SAME sunlight, the system has two equilibrium states, one warm and dark, the other cold and bright: this is hysteresis. The state the system is in depends on its history, and moving from one to the other takes a strong disturbance. The ice-albedo feedback is what creates these two states.
Exercise 12: Ocean inertia: the response time of the climate
The surface ocean layer, well mixed over h=70 m, is modelled as a reservoir of heat capacity per unit area C=ρch (ρ=1025 kg/m³, c=3990 J/(kg·K)). Subject to a constant forcing ΔF, its temperature difference T satisfies CdtdT=ΔF−λT, with λ=1.2 W/(m²·K). Take ΔF=3.7 W/m², and one year equal to 3.156×107 s. The diagram below shows the situation.
a) Calculate C, in J/(m²·K).
b) The solution is T(t)=λΔF(1−e−t/τ). Calculate τ=λC, in years.
c) Calculate the equilibrium warming.
d) Calculate the warming reached after 10 years.
e) After how many years is half of the equilibrium warming reached?
Show the solution
Answers
a)C=2.86×108 J/(m²·K)
b)τ≈7.6 years
c)Teq≈3.08 K
d)2.26 K
e)τln2≈5.2 years
a)
C=1025×3990×70=2.86×108 J/(m²·K). It takes nearly three hundred megajoules to warm the water column under each square metre by one kelvin.
b)
τ=1.22.863×108=2.39×108 s, that is 3.156×1072.39×108=7.6 years. We check the solution: T(0)=0, and CdtdT=λτCΔFe−t/τ=ΔF−λT.
c)
When dtdT=0: Teq=λΔF=1.23.7=3.1 K.
d)
T(10)=3.08×(1−e−10/7.56)=3.08×0.734=2.26 K.
e)
1−e−t/τ=21, so t=τln2=7.56×0.693=5.2 years. The climate “runs after” the forcing: part of the warming due to past emissions is not yet visible. With the deep ocean, much slower, part of it arrives over centuries.
Exercise 13: Emission altitude: why adding CO₂ warms the planet
Seen from space, the Earth emits on average 240 W/m² of infrared. We accept that this radiation leaves from a single emission altitude, where the air radiates like a blackbody, and that the temperature falls by 6.5 K per kilometre from the surface, at 288 K. σ=5.67×10−8 W/(m²·K⁴). The graph below shows this temperature profile.
a) Calculate the radiating temperature of the Earth.
b) Calculate the emission altitude.
c) An addition of CO₂ makes the atmosphere more opaque and raises the emission altitude by 150 m, without changing the temperature profile. What is the new emission temperature?
d) Calculate the drop in the flux emitted to space.
e) How does the system regain equilibrium?
Show the solution
Answers
a)T=255.1 K
b)z≈5.07 km
c)T=254.1 K
d)ΔF≈3.65 W/m²
e)Warming until 240 W/m² is restored
a)
T=(5.67×10−8240)1/4=255.1 K.
b)
The temperature drops by 288−255.1=32.9 K between the surface and the emission altitude: z=6.532.9=5.07 km. It is near 5 km, and not from the ground, that the Earth cools to space.
c)
Rising by 150 m loses 6.5×0.150=0.98 K: T=254.1 K.
d)
ΔF=σ(255.074−254.094)=3.65 W/m², of the same order as the forcing of a doubling of CO₂. The linear approximation 4σT3ΔT gives 3.67 W/m².
e)
The Earth still receives 240 W/m² but now emits only 236: it accumulates energy and warms. The whole profile shifts toward warmer temperatures until the NEW emission altitude is back at 255 K; the surface, 5.2 km lower, has then gained about one kelvin, before feedbacks.
Exercise 14: Volcanic aerosols and solar geoengineering
A rise Δα in planetary albedo produces a forcing ΔF=−4SΔα, with 4S=340 W/m². The eruption of Pinatubo (1991) produced, for about a year, a mean forcing of −3.0 W/m². We reuse the surface ocean model: λ=1.2 W/(m²·K) and τ=7.6 years, with T(t)=λΔF(1−e−t/τ). The diagram below shows the situation.
a) What rise in albedo would offset the forcing of a doubling of CO₂ (3.71 W/m²)?
b) What relative rise in the present albedo (0.30) is this, in %?
c) If the Pinatubo forcing lasted indefinitely, what equilibrium cooling would it produce?
d) Calculate the cooling actually reached after one year.
e) Why does geoengineering with aerosols not solve the CO₂ problem?
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Answers
a)Δα≈0.0109
b)3.6 %
c)−2.5 K
d)−0.31 K
e)The CO₂ stays, the aerosols fall out
a)
Δα=3403.71=0.0109, about one hundredth.
b)
0.300.0109=3.6 %. It would be enough to send back a little over one percent of the incident sunlight, which explains the interest in, and the risks of, projects to inject aerosols into the stratosphere.
c)
Teq=1.2−3.0=−2.5 K.
d)
T(1)=−2.5×(1−e−1/7.6)=−2.5×0.123=−0.31 K. A global cooling of the order of 0.3 to 0.5 K was measured: the inertia of the ocean prevents a brief forcing from having its full effect, which also explains why the cooling disappeared within two or three years.
e)
Aerosols fall out within a year or two: they would have to be reinjected without interruption for centuries, at the risk of abrupt warming if we stop. Above all, they do not remove the CO₂: ocean acidification continues, and the greenhouse effect and the aerosol screen only cancel on average, not region by region or season by season.
Exercise 15: Problem: the energy budget of the Earth's surface
Recent estimates of the mean surface budget give, in W/m²: absorbed solar radiation 161; infrared radiation received from the atmosphere 333; emitted infrared radiation 396; sensible heat flux (convection) 17; latent heat flux (evaporation) 80. Data: σ=5.67×10−8 W/(m²·K⁴), Lv=2.45×106 J/kg, one year is 3.156×107 s, surface area of the Earth 5.10×1014 m². The diagram below shows these five fluxes.
a) Calculate the net flux received by the surface.
b) Deduce the surface temperature from the emitted flux, assuming an emissivity equal to 1.
c) Latent heat is used to evaporate water that falls back as rain. Calculate the corresponding mean annual precipitation depth, in metres.
d) The Earth system accumulates 0.9 W/m² on average. Calculate the energy accumulated in one year.
e) Which energy input to the surface is the largest?
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Answers
a)+1 W/m²
b)T≈289 K
c)1.03 m per year
d)1.4×1022 J
e)Atmospheric infrared, 333 W/m²
a)
Received: 161+333=494. Lost: 396+17+80=493. Net flux: +1 W/m². The budget is not zero: the surface, mainly the ocean, is slowly warming.
b)
T=(5.67×10−8396)1/4=289 K, or 16 °C, consistent with the observed mean temperature.
c)
Mass evaporated per square metre in one year: 2.45×10680×3.156×107=1.03×103 kg, that is 1.03 m³ of water. On average, 1.03 m of precipitation therefore falls each year: the latent flux drives the water cycle.
d)
E=0.9×3.156×107×5.10×1014=1.4×1022 J per year, of which more than 90 % ends up in the ocean.
e)
The infrared radiation sent back by the atmosphere, 333 W/m², more than double the absorbed solar radiation. This is the direct measure of the greenhouse effect: the surface is heated more by the atmosphere than by the Sun directly.
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