6.4 Flashcards

1
Q

what types of molecules trap heat?

A

2+ atoms (polyatomic)

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2
Q

99.9% of molecules in atmosphere don’t absorb IR radiation including:

A
  • N2 = 78%
  • O2= 21%
  • Ar = 0.9%
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3
Q

2 molecular requirements for IR absorption:

A
    1. energy of radiation matches energy of molecular transition (nuclei/electron vibrations)
    1. molecular transition (atmospheric molecules) must change electric field (alter molecule’s dipole moment)
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4
Q

why does Ar NOT absorb IR?

A

no nuclei vibrations

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5
Q

dipole moment =

A

(vector sum of atomic charges) * (distance from molecule’s center of mass)

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6
Q

why do N2 and O2 NOT absorb IR?

A
  • they have nuclei vibrations BUT
  • NO change in dipole moment (bc symmetrical dipole always = 0)
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7
Q

all homonuclear diatomic molecules =

A

infrared inactive

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8
Q

homonuclear diatomic molecules

A

molecule w/ 2 of the same atoms (H2, O2, N2, etc.)

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9
Q

all heteronuclear diatomic molecules =

A

have altered dipole moment = absorb IR

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10
Q

heteronuclear diatomic molecules

A

molecules w/ 2 diff atoms (CO, NO, HCI)

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11
Q

polyatomic molecules w/ vibrations that change dipole =

A

IR active

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12
Q

all gasses that contribute to GHG effect =

A

polyatomic

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13
Q

2 most important GHG molecules =

A

H2O and CO2

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14
Q

H2O:

A

3 vibrations = 3 Δ-dipole

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15
Q

CO2:

A

symmetric = no Δ-dipole
- BUT net Δ-dipole = altered by stretch/bending of vibrations

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16
Q

molecular vibrational transitions allow for absorption of …

A

specific energies

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17
Q

rates of rotation

A

for each vibration, IR photons change rotational levels

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18
Q

rotational absorptions = ? and allow for absorption of…

A

gain/loss of energy during collision
- broad absorption band

19
Q

CO2: bending vibration

20
Q

CO2: main absorption band

A

15 µ band

21
Q

1 µ =

A

1 µm = 1000 nm = 1 x 10^6 m

22
Q

H2O: bending vibration

A

6269 nm (major absorption band)

23
Q

H2O rotational vibrations =

A

wavelengths > 20,000 nm

24
Q

why do CO2 and H2O absorb no significant radiation

A

wavelengths = short

25
atmospheric window
region 8000-12,000 nm where radiation can escape
26
chlorofluorocarbons
polyatomic molecules; major destroyers of stratospheric ozone - CH4, N2O, O3 - major GHGs
27
CO2 absorptions =
nearly saturated
28
“saturated” absorption
most radiation emitted w/in absorption bands = already absorbed
29
CO2 molecules = contribute __ amnt to total absorption
small
30
CFC molecules = contribute __ amnt to total absorption bc...
large - they absorb small amnts from window regions
31
1 CFC molecule =___ effect of 1 CO2 molecule
times thousands
32
Beer-Lambert Law:
evaluating UV screening effect of ozone layer
33
any form of radiation passing through absorbing material (beer-lambert equation=...)
T = I/I0 = e-El
34
Beer-Lambert: T =
% transmitted light thru global layer of absorbing gas
35
Beer-Lambert: l =
equivalent thickness
36
Beer-Lambert: E =
absorptivity
37
ozone layer = Δ-transmitted fraction produced by small change in absorbing gas (beer-lambert equation=...)
dT = -e-El dl - dT = Δ-light
38
Δ-% outgoing IR = __ as ↑ GHG
39
if [initial concentration] = small, [dependence] = __ bc..
linear - e^-El approaches e^0 =1
40
effect of outgoing radiation/molecule = greatest @ __ concentrations or __ absorptivity
LOW
41
main effects of CO2/H2O added =
↓ transmitted light at edges of absorption bands (E ↓ rapidly)
42
adding molecules found in low concentration =
absorb light in proportion to absorptivity in atmospheric window
43
2 vibrational modes involved in CO2 absorption
asymmetrical stretching + bending = net Δ-dipole = absorbs IR