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

A

14,922 nm

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
Q

atmospheric window

A

region 8000-12,000 nm where radiation can escape

26
Q

chlorofluorocarbons

A

polyatomic molecules; major destroyers of stratospheric ozone
- CH4, N2O, O3
- major GHGs

27
Q

CO2 absorptions =

A

nearly saturated

28
Q

“saturated” absorption

A

most radiation emitted w/in absorption bands = already absorbed

29
Q

CO2 molecules = contribute __ amnt to total absorption

A

small

30
Q

CFC molecules = contribute __ amnt to total absorption bc…

A

large
- they absorb small amnts from window regions

31
Q

1 CFC molecule =___ effect of 1 CO2 molecule

A

times thousands

32
Q

Beer-Lambert Law:

A

evaluating UV screening effect of ozone layer

33
Q

any form of radiation passing through absorbing material (beer-lambert equation=…)

A

T = I/I0 = e-El

34
Q

Beer-Lambert: T =

A

% transmitted light thru global layer of absorbing gas

35
Q

Beer-Lambert: l =

A

equivalent thickness

36
Q

Beer-Lambert: E =

A

absorptivity

37
Q

ozone layer = Δ-transmitted fraction produced by small change in absorbing gas (beer-lambert equation=…)

A

dT = -e-El dl
- dT = Δ-light

38
Q

Δ-% outgoing IR = __ as ↑ GHG

A

39
Q

if [initial concentration] = small, [dependence] = __ bc..

A

linear
- e^-El approaches e^0 =1

40
Q

effect of outgoing radiation/molecule = greatest @ __ concentrations or __ absorptivity

A

LOW

41
Q

main effects of CO2/H2O added =

A

↓ transmitted light at edges of absorption bands (E ↓ rapidly)

42
Q

adding molecules found in low concentration =

A

absorb light in proportion to absorptivity in atmospheric window

43
Q

2 vibrational modes involved in CO2 absorption

A

asymmetrical stretching + bending = net Δ-dipole = absorbs IR