Climate Flashcards

1
Q

Describe Earth’s energy balance

A
  • Incoming shortwave radiation from the Sun
  • Outgoing long wave radiation
  • Energy balance equation:
    S_0/4 * (1-alpha)=epsilonsigmaT^4

S_0= solar constant (avg intensity in upper atmosphere)
Alpha = albedo (0.3)
Epsilon = emissivity (0.62)
Sigma = Stefan’s constant

  • Lower latitudes receive greater insolation, driving atmospheric circulation
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2
Q

What is radiative forcing and what affects it?

A

delta F = S_0(1-alpha)-4epsilonsigma*T^4
* Difference between incoming energy from the Sun and emitted by Earth

Solar constant
* Sunspots - greater solar activity
* Faint young sun paradox - Sun was 30% fainter when Earth formed but liquid water present

Albedo
* Snow/ice/clouds have high albedo, water/vegetation/soil has low albedo
* Sulfate aerosols (volcanic and anthropogenic) increase albedo

Emissivity
* Decreased by absorption of IR by greenhouse gases (water vapour, CO2, CH4, CFCs)

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3
Q

List six climate feedback loops and explain them.

A

Water vapour
* Positive feedback: water vapour is a GHG, absorbs IR causing Earth to warm, increased evaporation (fast - years)

*Negative feedback: water vapour condenses to form high-albedo clouds, causing cooling (fast - years)

CO2
* Positive feedback: CO2 increases causing Earth to warm, sea temperatures rise, solubility decreases so CO2 released into the atmosphere (fast - surface ocean (decades), slow - deep ocean (centuries))

Silicate weathering
* Negative feedback: high temp increases rate of weathering which consumes CO2, leading to cooling (slow - millennia)

Ice
* Positive feedback: high temp causes ice to melt, decreasing avg albedo of Earth, leading to more warming and melting (slow - centuries)

Vegetation
* Increased CO2 means increased rate of photosynthesis in vegetation, hence decreased CO2 and cooling (slow - centuries)

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4
Q

What is climate sensitivity?

A
  • Temperature change for given forcing (lambda)
    *delta T = lambda * delta F

lambda = dT/dE = (d/dT(epsilonsigmaT^4))^-1
* Ignores feedbacks

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5
Q

What is the carbon cycle?

A
  • Carbon stored in reservoirs and can move between them (box model)
  • Residence time: average lifetime of C in reservoir (total mass/flux out). Slow feedbacks = longer residence time
  • Reservoirs by size: rocks and sediments, deep ocean, land biosphere, surface ocean, atmosphere
  • Biosphere-atmosphere exchange - photosynthesis
    *Atmosphere-ocean exchange - CO2 dissolves to form DICs
  • Atmosphere-ocean-lithosphere exchange: Volcano emits CO2, acid rain dissolves rocks, DICs run into sea, marine organisms make shells, seafloor subducted
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6
Q

What are anthropogenic carbon sinks?

A
  • Increase in CO2 less than anthropogenic emissions
  • Uptake by oceans (ocean acidification) and biosphere
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7
Q

How can palaeoclimate be reconstructed?

A
  • Use of proxies

Ice cores
* Depth proportional to age (oldest core 800ka - recent climate only)
* Trapped air bubbles used to analyse atmosphere (CO2 conc)
* Gas younger than ice around it (air in snow and firn exchanges with atmosphere)
* Deuterium ice isotopic ratio is a temperature proxy (lighter=warmer)
*d18O also used

Marine sediment cores
* Foraminifera (CaCO3 shells) - d18O ratio
* Benthic - deep ocean temp proxy. Planktic - surface ocean temp and glaciation proxy
* Increased temp decreases d18O
* Glaciation increases d18O as 16O more likely to evaporate, then precipitated and locked away as ice

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8
Q

Describe the trends in climate through the Cenozoic

A
  • Early Cenozoic ice free, about 10C hotter than today
  • First glaciation 34Ma
  • Trend of cooling and increased glaciation
  • Evidence: decrease in CO2 (proxy data), albedo feedback, opening of the Drake passage (cold currents around Antarctica)
  • CO2 concentrations varied with glacial/interglacial cycles (800ka) however conc never as high as today
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9
Q

Describe the recent trend in Northern Hemisphere glaciation and its causes

A
  • Intensification 2.6Ma

Milankovitch theory
* Summer insolation controls whether glaciers advance/retreat, affected by orbital parameters

Obliquity
* Tilt of Earth’s axis varies over time (22-24.5deg, period 40ka)
* Increase in obliquity increases summer insolation at poles (poles closer to Sun)

Precession
* Axial precession - rotation of Earth’s rotational axis (period 25ka)
* Elliptical precession - rotation of Earth’s orbit around the sun
* Changes time of year of aphelion/perihelion
* If perihelion coincides with N Hemisphere summer, increased insolation

Eccentricity
* Increased eccentricity means smaller distance to Sun at perihelion, so increased summer insolation
* Only effect which changes solar constant

Evidence
Deep sea d18O data

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