Greenhouse gases Flashcards

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1
Q

How does data from ice cores show atmospheric CO₂ changes since 1950

A

Before 1950 around 300ppm
Now around 400ppm

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2
Q

Which are the top 3 sectors contributing to global GHG emissions

A
  • Fossil fuels and industrial processes (65%)
  • Argiculture (16%)
  • Forestry and other land use (11%)
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3
Q

Why does increasing CO₂ levels lead to increasing global temperatures

A
  • GHGs like CO₂ absorb infrared radiation which traps heat
  • This is due to their molecular bonds altering energy levels when hit by infrared radiation of certain wavelengths
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4
Q

Solar radiation hits the earth as …….. radiation
And leaves the earth’s surfaces as …….. radiation

A

Shortwave (UV)
Longwave (IR)

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5
Q

Increasing levels of GHGs results in…

A

a reduced amount of energy the Earth’s surface radiates to space, thus warming the planet

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6
Q

The shorter the wavelenght (λ) of a wave

A

The higher energy it is

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7
Q

True of false
Electromagnetic waves don’t need molecules like sound to travel

A

true

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8
Q

The earths ozone prevents what type of waves from entering the troposphere

A

High energy waves: gamma, x-rays and UV
The atmosphere absorbs this energy

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9
Q

Which energy wavelengths does penetrate the atmosphere

A

Energy in the visible part of the spectrum

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10
Q

Energy absorbed by the atmosphere is inversely correlated to

A

energy intensity (i.e. the wavelength)

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11
Q

What is the atmospheric window

A

it is a band of IR radiation which can freely pass through to the Earth’s surface - important to avoid the atmosphere being to warm
(this is opposite to an absorption band which is the portion of the electromagnetic spectrum that is blocked)

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12
Q

What is the difference between UV-A, B and C

A
  • wavelength decreases in size from UV-A to UV-C
  • UV-C is totally absorbed by ozone in the atmosphere
  • UV-B is 90% absorbed by ozone (this is what causes sunburn
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13
Q

What is the radiation balance of the earth assumed to be?

A

Amount of heat absorbed = heat radiation emitted
(climate change is a difference in this balance)

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14
Q

What is a Radiative forcing (W m‾²)

A
  • The influence a given climatic factor has on the amount of downward-directed radiant energy impingging upon Earth’s surface (strongest for water vapour)
  • Imbalance on the steady state
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15
Q

What is Radiative efficiency (aₓ)

A

The efficiency is determined by the capacity of each molecule (e.g. CO₂, CH₄) to absorb long IR radiation

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16
Q

What is GWP

A

Global warming potential
(no units)

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17
Q

Which of the following molecules has the highest radoative efficiency?
CO₂, CH₄, NO₂

A

NO₂

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18
Q

Molecular vibrations can derermine the radiative efficiency of molecule?
What are molecular vibrations?

A
  • to absorb IR the electrical dipole moment of the molecule must change when electrons are displaced
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19
Q

What is a dipole moment?

A

Tension between a positive and negetive pole within the molecule
This can only occcur in molecules which are heteronuclear diatomic - unsymmetrical distribution of change

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20
Q

If a vibrating molecules absorbs radiation of a matching frequency ….

A

… it becomes more ‘energetic’
amplitude of vibration increases

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21
Q

A molecule can lose vibrational energy by ….

A

… re-emitting radiation (energy) and return to the original state
(this repeats and this is what allows the atmosphere to heat up)

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22
Q

CO₂ is a linear triatomic molecule
Which vibration modes are IR active?

A

Asymmetrical stretching (v3)
Symmetrical bending (v2)

23
Q

Why is the symmetrical stretching (v1) mode of CO₂ IR inactive

A

Due to there being no change in the dipole moment

24
Q

SO₂ is a bent triatomic molecule
Which vibrational modes are IR active?

A
  • Symmetrical stretching (v1)
  • Symmetrical bending (v2)
  • Asymmetrical stretching (v3)
25
Q

Name some other non-linear triatomic molecules

A

H₂O or O₃

26
Q

……….. can cause absorption of ……. giving rise to a shift in the ……….. level

A

IR radiation can cause absorption of photons giving rise to a shift in the vibrational level

27
Q

What peaks would pure CO₂ produce on a IR

A
28
Q

Molecules absorb radiation of different wavelengths depending on their ………..

A

vibrational enery
This means ozone, CO₂ and H₂O will all produce peaks in different places

29
Q

Which molecule is the largest GHG absorber?

A

water

30
Q

Radiative efficiency is determined by?

A

How many vibrational states a molecule has

31
Q

Specific vibration states (determined by the molecular structure) controls ….

A

how much IR energy a molecule can absorb

32
Q

The longer the lifetime of a molecule in the atmosphere, the stronger the GHG it is
What determines lifetime?

A

The sinks of the Greenhouse gases
e.g. short lifetime of methane is due to its high reactivity with OH radical

33
Q

How does ozone react with an OH radical?

A

O₃ + OH → HO₂ + O₂
(occurs in the stratosphere)

34
Q

What is straospheric photolysis (tip: includes N₂O)

A

N₂O → N₂ + O.
(major sink for N₂O)

35
Q

What is Tropospheric photolysis (tip: includes ozone)

A

O₃ + OH → O₂ + O.

36
Q

Lifetime (τ) is defined as

A

τ = 1/k’
it is the time taken for a species concentration too drop by a factor of 1/e
(k is the rate constant)

37
Q

The lifetime of methane is dependent on its reaction with OH. radical
Hence the rate of reaction = k[OH][CH₄]
how can this equatin be simplifed?

A

= k’[CH₄]
assumes that OH concentration is much higher than methanes

38
Q

What are the units of k

A

cm³ molecule‾¹ s‾¹

39
Q

How would you work out the lifetime of a GHG

A

τ = 1/k[OH]

40
Q

if the lifetime of methane is given by: τ = 1/k’
if k = 6 x 10‾¹⁵ cm³ molecules‾¹ s‾¹
and [OH] = 1 x 10⁶ molecules cm‾³
give τ

A

τ(CH₄) = 1/(6 x 10‾¹⁵ x 1 x 10⁶) = 5.3

41
Q

The longer the lifetime of a GHG….

A

…. the further the distance it can travel

42
Q

What is Gloval Warming potential (GWP) for a GHG, and how is it worked out?

A
  • Ratio of the time-intergrated radiative forcing from the instantaneous release of 1kg of a trace substrance relative to that of 1kg of a reference gas (CO₂) - of which the GWP is 1
  • It is worked out by combining a GHGs radiative efficiency and its lifetime in the atmosphere
43
Q

So what factors make a GHG potent

A

Radiative efficiency (how much radiation it can absorb)
Lifetime
Concentration

44
Q

50% of incoming short wave radiation reaches the surface
How much gets scattered back into space

A

30%

45
Q

How much of the incoming solar radiation is taken up by the oceans and the land

A

70% taken up by the oceans
30% taken up by the land

46
Q

What other factors apart from global warming affect the Earth energy balance

A
  • Albdeo (reflectivity) by clouds, ice etc
47
Q

Radiative forcing can be a measure of?

A

Imbalance of the energy budget
(values of change are relative to preindustrial conditions defined at 1750)

48
Q

In Simple terms, radiative forcing is

A

the rate of energy change per unit area

49
Q

If the sun suddenly put out more energy, this is a …….. radiative forcing

A

positive

50
Q

If we put more CO₂ or other GHG into the atmosphere that traps the radiation, this is a ……. radiative forcing

A

Positive

51
Q

If there are more clouds or desert, this is a ……. radiative forcing

A

negative radiative forcing

52
Q

What is the difference between ozone in the troposphere vs straosphere?

A

positive radiative effect in the troposphere
negative radiative effect in the stratosphere

53
Q

Both methane and nitrous oxide have really high Global warming potentials, why are we still more concerned about CO₂

A

Because concentrations are significantly lower