exam 2 Flashcards

1
Q

radiant energy

A

energy transferred from the sun; travels in the form of waves that release energy when they’re absorbed by an object

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2
Q

electromagnetic waves

A

waves that share properties of electricity and magnetism

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3
Q

wavelength

A

a measure by which different forms of electromagnetic waves are distinct from each other

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4
Q

speed

A

the measure of how far the wave crest moves in 1 second

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5
Q

frequency

A

the number of wave crests passing a fixed point in 1 second

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6
Q

visible light

A

wavelengths ranging from .4 to .7 microns

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7
Q

ultraviolet light

A

wavelengths less than .4 microns

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8
Q

infra-red light

A

wavelengths more than .7 microns

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9
Q

radiative equilbrium

A

when an object radiates and absorbs energy at equal rates; an object’s temperature won’t change

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10
Q

kirchoff’s law

A

an object’s efficiency of absorption of a certain wavelength of energy is exactly equal to its emission efficiency at the same wavelength

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11
Q

black body

A

any object that is both a perfect emitter and absorber

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12
Q

radiative equilibrium temperature

A

when the amount of shortwave solar radiation absorbed at the surface is exactly equal to the amount of infra-red radiation emitted from the surface

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13
Q

selective absorber

A

any object that absorbs and emits only some wavelengths; transparent to others

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14
Q

atmospheric windows

A

regions in the spectrum in which none of the gases absorb radiation

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15
Q

atmospheric greenhouse effect

A

carbon dioxide absorbs nearly all infra-red radiation; any surface temperature is much higher than its radiative equilbrium temperature

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16
Q

positive feedback

A

an increase in water vapor content exacerbates the warming instigated by the increase in carbon dioxide

17
Q

angle of incidence

A

the angle at which the light/radiation is exposed to the surface

18
Q

summer solstice

A

where the northern hemisphere is pointed maximally towards the sun; June 22

19
Q

land of the midnight sun

A

everywhere above 66.5 degrees north never see the sunset

20
Q

autumnal equinox

A

not pointed towards/away from the sun, everywhere on Earth gets the same length of day; September 21

21
Q

winter solstice

A

the northern hemisphere is pointed away from the sun; the sun never goes up at the north pole nor down at the south pole; December 22

22
Q

vernal equinox

A

axis not tilted towards/away from the sun; everyday is the same length; March 21

23
Q

sensible heat

A

the transfer where the tropics are made cooler and the higher latitudes are made warmer; accounts for the redistribution of radiative energy

24
Q

radiation iversion

A

temperature inversion where the temperature is lowest at the ground than in the air; the ground is more efficient at radiating energy

25
Q

albedo

A

fraction of incident solar radiation that’s reflected back into space

26
Q

stefan-boltzmann law

A

objects w/ very high temperatures emit energy at a greater intensity than objects at lower temperatures; E = (constant)(temperature to the power of four)

27
Q

wein’s displacement law

A

states that the wavelength of max emission of an object is related to the object’s temperature; Lambda = 3000/Temp