// lecture 07 Flashcards
molecules with
one atom or two of the same atoms aren’t GHGs. the primary gases in our atmosphere are thus transparent to longwave radiation.
polyatomic molecules are GHGs:
water vapor (H2O), carbon dioxide (CO2), methane (CH4), nitrous oxide (N2O), ozone (O3), and CFCs. they rotate and vibrate, so that means they can absorb the right frequencies of longwave.
all GHGs are rather a small fraction of the atmosphere:
water vapor 0.4%, CO2 0.04%, and methane 0.0002%.
“trace gases”
have a remarkable effect on the atmosphere. such as ozone
water vapor
gas form of water (humidity); #1 GHG. powerful because of its molecular structure and because there’s a lot of it. not controlled by humans so its a feedback. increasing global warming. bent triatomic molecule: H2O.
CO2
primary contributor to the antropogenic GHE (63% of it so far). extremely long-lived. increases primarily due to fossil fuel burning (80%) and deforestation (20%). 50% of what we emit quickly gets taken up by the ocean or land. most else sticks around for over 100 yrs.
methane (CH4)
natural gas; much more potent on a per molecule basis than CO2. lifetime is 8 yrs. natural sources: marshes (swamp gas) and other wetlands. increase anthropogenically due to farm animals, landfills, coal mining, gas leakage, and rice farming.
nitrous oxide (N2O)
laughing gas; more potent on a per molecule basis than CO2. global warming potential: 310. comes from agriculture, chemical energy, and deforestation. small concentrations of only 0.3 ppm.
ozone (O3)
occurs in two places in the atmosphere:
- in the ozone layer: good ozone, protects us from ultraviolet radiation and skin cancer.
- near earth’s surface: bad ozone, caused by air pollution.
bad ozone
a GHG and is more potent on a per molecule basis than CO2, but it’s very short-lived.
CFCs
ozone depleting chemicals and are strong GHGs. almost phased out. some replacements like HFCs are still strong GHGs though. global warming potentials of up to 11,000.
the natural GH contributions:
H2O (water vapor): 60%, (but less than 1% of mass of atmopshere), CO2: 26% (but 400 ppmv, ~0.04% of mass), and all others: 14%.
unnatural GHE
increasing levels of CO2 and other GHGs leads to a strong GHE. with more GHGs, it’s harder for outgoing radiation to escape to space.
contributors to the “anthropogenic” GHE
CO2: 63%, methane: 18%, CFCs and HFCS: 12%, and nitrous oxide: 6%.
global warming potential (GWP)
how much GHE emission of a given gas causes over a fixed amount of time.