M3L1 - Energy & Feedback Loops Flashcards

1
Q

Emissivity

A

The proportion of energy received to emitted

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2
Q

Black body

A

Something that emits 100% of energy it absorbs (emissivity = 1)

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3
Q

Planck’s law

A

For a given object, the energy at any specific wavelength is dependent on temperature (measured in kelvin)

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4
Q

Stefan-Boltzmann Law

A

There is a direct relationship between an object’s temperature and how much radiation it emits

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5
Q

What does EMR scattering in the atmosphere depend on

A
  • Wavelength of the EMR compared to particle size
  • Amount of particles/gasses
  • How far the EMR travels through the atmosphere
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6
Q

Three types of scatter

A
  • Rayleigh scattering
  • Mie scattering
  • Nonselective (geometric scattering)
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7
Q

Rayleigh scattering

A
  • Shorter wavelengths of visible spectrum are scattered by particles smaller than the wavelengths of light (including dust, NO2 and O2)
  • Explains why sky is blue
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8
Q

Mie scattering

A
  • Occurs when the wavelength of EMR is similar to the particles in the atmosphere (or particles are larger)
  • Driven by presence of aerosols
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9
Q

Aerosols

A

Mixture of gasses, dust, water vapour

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10
Q

Nonselective (geometric scattering)

A
  • Scattering by particles much larger than the wavelength
  • Water vapour and clouds
  • Why clouds are white (scatter all wavelengths equally)
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11
Q

Why do contributions to greenhouse effect vary

A

Based on characteristics of the gas, how much there is, and what indirect effects it has

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12
Q

Water vapour

A
  • High relative contribution to greenhouse effect
  • Humans not influencing the amount directly
  • Residence time is short (~9 days)
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13
Q

New and emerging compounds

A
  • Sulphur hexafluoride is a growing concern
  • 23,500 more potent than CO2
  • Used in high voltage electrical applications
  • Often unaware of implications of new compounds until they have been around for a while
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14
Q

Carbon sources and sinks

A
  • Most things are in balance
  • Known out of balance (burning fossil fuels faster than they are forming)
  • Unknowns (permafrost flux, methane hydrate amount)
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15
Q

What is global warming potential standardised to

A

CO2

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16
Q

Methane hydrate

A

Formed when water and methane gas come together at
high pressures and low temperatures in oceans

17
Q

Ocean acidification

A
  • Oceans absorb ~1/3 of co2 released in atmosphere
  • Increases concentration of hydrogen ions, decreasing pH
  • Carbonic acid acid formation and subsequently dissociates releasing hydrogen ions (H+) and bicarb (HCO3-)
18
Q

Radiative forcing

A
  • Measure of influence a factor has in altering the balance of incoming and outgoing energy in the Earth-atmosphere system
  • Internal forcings: atmospheric, surface
  • External (solar forcing)
19
Q

Feedback loops

A
  • Positive adds to initial change
  • Negative reduces initial change
20
Q

Environmental stability

A
  • Stable: Deviations up to a certain point from equilibrium end up returning to equilibrium, or new
    equilibrium
  • Unstable: Small perturbations result in larger shifts and a lack of ability to return to equilibrium
21
Q

Resiliency

A
  • Ability for a system to keep functioning after being subjected to disturbance
  • Not always a positive
  • Examples: Soil resilience in agriculture; overfishing; deforestation; electrical grids