exam 2 Flashcards
radiant energy
energy transferred from the sun; travels in the form of waves that release energy when they’re absorbed by an object
electromagnetic waves
waves that share properties of electricity and magnetism
wavelength
a measure by which different forms of electromagnetic waves are distinct from each other
speed
the measure of how far the wave crest moves in 1 second
frequency
the number of wave crests passing a fixed point in 1 second
visible light
wavelengths ranging from .4 to .7 microns
ultraviolet light
wavelengths less than .4 microns
infra-red light
wavelengths more than .7 microns
radiative equilbrium
when an object radiates and absorbs energy at equal rates; an object’s temperature won’t change
kirchoff’s law
an object’s efficiency of absorption of a certain wavelength of energy is exactly equal to its emission efficiency at the same wavelength
black body
any object that is both a perfect emitter and absorber
radiative equilibrium temperature
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
selective absorber
any object that absorbs and emits only some wavelengths; transparent to others
atmospheric windows
regions in the spectrum in which none of the gases absorb radiation
atmospheric greenhouse effect
carbon dioxide absorbs nearly all infra-red radiation; any surface temperature is much higher than its radiative equilbrium temperature
positive feedback
an increase in water vapor content exacerbates the warming instigated by the increase in carbon dioxide
angle of incidence
the angle at which the light/radiation is exposed to the surface
summer solstice
where the northern hemisphere is pointed maximally towards the sun; June 22
land of the midnight sun
everywhere above 66.5 degrees north never see the sunset
autumnal equinox
not pointed towards/away from the sun, everywhere on Earth gets the same length of day; September 21
winter solstice
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
vernal equinox
axis not tilted towards/away from the sun; everyday is the same length; March 21
sensible heat
the transfer where the tropics are made cooler and the higher latitudes are made warmer; accounts for the redistribution of radiative energy
radiation iversion
temperature inversion where the temperature is lowest at the ground than in the air; the ground is more efficient at radiating energy
albedo
fraction of incident solar radiation that’s reflected back into space
stefan-boltzmann law
objects w/ very high temperatures emit energy at a greater intensity than objects at lower temperatures; E = (constant)(temperature to the power of four)
wein’s displacement law
states that the wavelength of max emission of an object is related to the object’s temperature; Lambda = 3000/Temp