Earth's Energy Flashcards

1
Q

Ozone in Stratosphere (CFC)

A

Chlorofluorocarbons + Ultra Violet -> Chlorine

  • from fridges, propellants
  • 1 molecule Cl destroys thousands of Ozone
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2
Q

Natural Pollutants

A
  • volcanoes
  • plants (decaying and alive)
  • forest fires
  • ocean
  • soil
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3
Q

Anthropogenic Pollutants

A
  • vehicle emissions (CO, carbon monoxide)

- fertilizers (nitrogen oxides)

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4
Q

Atmosphere and Energy: what it removes and how

A
  • breaks incoming shortwave electromagnetic radiation

- removes through absorption and scattering by gases, water vapor and aerosols

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5
Q

Reflection

A

-portion of arriving radiation which bounces right back from Earth to space

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6
Q

albedo

A

-ratio of reflected solar radiation to the incident solar radiation

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7
Q

Earth’s average albedo

A

around 30%

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8
Q

scattering

A

atmospheric gases, dust, clouds, and water vapor change the direction of waves without altering the wavelength

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9
Q

Transmission

A

-passage of short and long wave energy THROUGH atmosphere/water

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10
Q

Absorption

A

-the assimilation of short and long waves

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11
Q

Greenhouse gases (examples and effects)

A
  • Carbon Dioxide , Nitrous oxide, water vapor, methane

- trap heat from escaping

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12
Q

Clouds and Waves

A
  • SW are reflected and scattered

- LW are absorbed and re-radiated

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13
Q

heat

A

form of kinetic energy between molecules due to temperature difference

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14
Q

sensible heat

A

can be felt

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15
Q

latent heat

A

results from phase changes

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16
Q

convection

A

energy transffered through movement of molecules

17
Q

radiation

A

energy transferred through electromagnetic waves

18
Q

conduction

A

energy that moves from molecule to molecule

19
Q

convection and advection (directionally)

A
  • vertically

- horizontally

20
Q

Eo equation involving So and amount of energy hitting sphere

A

So/4

21
Q

Albedo: Angle, surface, texture

A
  • less angle, higher albedo
  • lighter, higher albedo
  • smoother, higher albedo
22
Q

blackbody

A

perfectly absorbs all received energy and radiates all

23
Q

Stefan Boltzman E equation

A

E= sigma T^4

24
Q

Emissivity

A

ratio of energy radiated from surface, to that of a perfect emitter (blackbody) at same conditions

25
Q

whitebody and blackbody emissivity

A

whitebody: 0
blackbody: 1

26
Q

Outgoing thermal energy, including emissivity

A

E = epsilon*sigma T^4