Lec 4 - Solar Radiation, Orbital-Scale CC Flashcards

1
Q

What determines the amount of shortwave radiation received?

A
  1. location
  2. time of year
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2
Q

What are the two fundamental motions of the Earth?

A
  1. spins on its axis once a day
  2. revolves around sun once a year
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3
Q

How does our distance to the Sun change throughout the year?

A

Perihelion: closest position to the sun
Aphelion: farthest position to the sun

  • distance to the sun changes the value of the solar constant!!
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4
Q

What angle is the Earth’s axial tilt?

A

23.5 degrees

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5
Q

How does location affect the amount of solar radiation received?

A
  • spreading of beam
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6
Q

What orbital parameters affect climate?

A
  • axial tilt
  • eccentricity of orbit
  • timing of equinoxes
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7
Q

What effect does a changing axial tilt have?

A

alters the strength of the seasons

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8
Q

What 3 orbital precessions occur?

A
  • axial precession
  • precessions of the ellipse
  • precession of the equinoxes
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9
Q

How does absorption of radiation alter climate?

A
  • atmospheric heating
  • amount of energy transferred to surface
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10
Q

What are the two kinds of scattering that happen to light in the atmosphere?

A
  • Rayleigh scattering: small molecules, scatter short wavelengths (blue)
  • Mie scattering: large scattering agents, large aerosols, directed scattering that stretches wavelengths (warmer colours)
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11
Q

What is the transmission of light?

A

percentage of energy transmitted through the atmosphere the surface

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12
Q

What is the fate of most radiation that encounters our atmosphere?

A
  • absorption by surface
  • absorption by gases/clouds
  • reflection by cloud
  • 30% reflected by atmosphere/clouds/atmosphere
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13
Q
A
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