Radiation Flashcards

1
Q

define electromagnetic energy

A
  • a wavelike form of energy
  • travels at the speed of light
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2
Q

What are the five fundamental laws of physics?

A
  1. all matter at temps above 0 emit electromagnetic radiation
  2. substances emit radiation in a wavelike fashion
  3. substances that emit the maximum radiation’s temperature are called blackbodies
  4. the hotter the object, the shorter the wavelength of maximum emission
  5. the amount of energy passing through a unit is inversely proportional to the square of the distance from the source
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3
Q

define fission

A

splitting atoms

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3
Q

define fusion

A

hydrogen converted to helium

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4
Q

define solar constant

A

how much radiation reaches a perpendicular surface at the top of Earth’s atmosphere

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5
Q

what happens every 11 years?

A

solar activity reaches a fever pitch and solar flares erupt near sunspots on a daily basis

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6
Q

insolation and what factors cause variance in winter vs summer?

A

incoming solar radiation
- factors: sun angles and length of day

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7
Q

is solar radiation shortwave or longwave? what about terrestrial?

A

solar = shortwave
terrestrial = longwave

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8
Q

how much insolation that reaches earth is absorbed? what methods inhibit absorption?

A

50%, scattering, reflection, and diffuse reflection

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9
Q

scattering

A

SW radiation is scattered in all directions by gas molecules

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10
Q

___ wavelengths scatter more effectively ( why we have blue sky). Which colors are in sunlight?

A

shorter, all but some scatter better

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11
Q

diffuse reflection

A

scattering by particulate matter (more junk=more color)

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12
Q

absorption

A

conversion of radiant energy to heat energy

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13
Q

albedo

A

reflective percentage of a solid

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14
Q

radiation balance and formula

A

tells us the amount of radiation absorbed:
Q* = incoming SW - outgoing SW + incoming LW - outgoing LW

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15
Q

where is there net surplus and deficit of radiation? what balances this?

A

surplus around tropics, deficit in polars, weather balances it

16
Q

energy balance and formula

A

tells us how the surplus somewhere is allocated

Q* = sensible heat flux + latent heat flux + soil heat flux

17
Q

what is sensible heat flux?

A

heating boundary layer

18
Q

what is latent heat flux?

A

evaporation

19
Q

what is soil heat flux?

A

heating earth surface

20
Q

solar noon

A

when the sun is at it’s highest point in a specific location

21
Q

how do you find SEN?

A

SEN = 90 - Z

Z = latitudinal separation of LP and LS
LS = solar declination
LP = latitude of place

22
Q

what is solar declination/subsolar point? and what is max height?

A
  • latitude where the noonday son is directly overhead
  • can be up to 90% in tropics