Key Stuff Flashcards

1
Q

Energy Budgets

A

models that help to analyse heating + cooling of the atmosphere

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2
Q

shortwave radiation

A
  • incoming solar radiation (insolation)
  • gets emitted from hot body e.g. sun
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3
Q

Longwave Radiation

A
  • the radiation released from earth (1) usually during night time (1)
  • LW radiation easily absorbed by GHG on way out, = greenhouse effect (trapped heat warms air)
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4
Q

radiation cooling

A
  • when the ground cools as a result of outgoing longwave radiation (1)
  • mostly @ night (1)
  • calm conditions + clead skies (1)
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5
Q

how much of incoming SW is reflected

A
  • 29%
  • earth surface (6%)
  • clouds (18%)
  • scattered by atmospheric particles (5%)
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6
Q

how much of incoming SW is absorbed

A
  • 23%
  • scattered to atmosphere 5%
  • absorbed by atmosphere 14%
  • absorbed by clouds 4%
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7
Q

absorbed by surface

A

48%

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8
Q

what happens to absorbed 48%

A
  • 12% re radiated to space directly through Space Window
  • 5% conduction+convection -> sensible heat transfer
  • 25% evap -> latent heat transfer
  • 6% LW radiation from surface
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9
Q

albedo values
- cumulonimbus cloud
- fresh snow
- concrete
- grass
- asphalt
- tarmac

A
  • 92
  • 80
  • 22
  • 25
  • 10
  • 5-10
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10
Q

sensible heat transfer

A
  • caused by the movement of parcels of air (1) into and out of an area usually by convection/conduction taking its heat with it (1)
  • i.e. change of temp, but no change of state
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11
Q

latent heat transfer

A
  • the heat transferred without a change of temperature (1) following a change of state (1), e.g. gas -> liquid, liquid -> gas
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12
Q

albedo

A

the % of incoming SW radiation (1) that is reflected back into space from a surface (1)

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13
Q

conduction

A

transfer of heat as a result of CONTACT
- from solid surface to atmosphere

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14
Q

convection

A

upward movement of air (1) caused as a result of surface heating (1) resulting in less dense air (1)

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15
Q

evap

A

change in state from liquid to gas (1) as a result of heating (1)

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16
Q

condensation

A

formation fo water droplets (gas to liquid) (1) as a result of a drop in temp to the dew point (1)

17
Q

diurnal budget

A

24 hour period, encompassing day and night time energy budgets

18
Q

day time energy budget
6 factor model

A
  1. incoming SW solar radiation
  2. reflected SW solar radiation
  3. absorbed solar radiation
  4. re-radiated LW radiation
  5. sensible heat transfers
  6. latent heat transfers
19
Q

evaluating incoming Sw radiation (day)

A
  • input will vary spatially + temporally
  • depending on latitude + seasonality due to tilt of earth
20
Q

evaluating reflected SW radiation (day)

A

depends on albedo, as amount reflected then changes amount absorbed etc, can change whole budget

21
Q

evaluating surface absorption (day)

A
  • nature of surface
    –dark granite has low albedo + good conductor so easy absorbs radiation, stores deep under surface to re radiate later
    – light limestone has high albedo + bad conductor so doesn’t absorb well, heat in surface layers
  • moisture helps conductivity
  • Urban areas have higher SA than rural, so more absorption
22
Q

evaluating latent heat transfer (day)

A
  • more water will mean more LHT occurs, e.g. at lakes, rivers, vegetation etc. means that in these rural areas there will be more temp lost than in urban areas
23
Q

evaluating sensible heat transfers (day)

A
  • conduction doesnt tranfer as much heat as convection
24
Q

evaluating LW radiation (day)

A
  • GHG in atmosphere better at absorbing LW, so warms atmosphere.
  • clouds also good at absorbing LW, trap it in atmosphere
  • creates greenhouse effect
25
Q

night time energy budget (4 factor model)

A
  1. heat absorbed into surface + given out by conduction
  2. LW radiation (output)
  3. sensible heat transfers
  4. latent heat transfers
26
Q

evaluating heat absorbed into surface + given out by conduction (night)

A
  • heat absorbed in day can be re-radiated at night, can offset radiation cooling
  • material w high thermal capacity (brick, concrete, stone) can absorb + store lots of heat during day, release slowly @ night as LW
27
Q

evaluating latent heat transfers (night)

A
  • radiation cooling @ surface means cold surfaces cool air above them, to dew point temp.
  • any water vapour will condense
  • condensation releases latent heat, providing energy to atmosphere, meaning net gain of energy
28
Q

evaluating sensible heat transfers (night)

A
  • with no insolation, less sensible heat losses at night.
  • HOWEVER, at tropics sensible heat transfers may still occur without solar radiation
  • w/ no SW, convection less important.
29
Q

evaluating LW radiation (night)

A
  • if cloudless, LW will escape easily
  • if cloudy, clouds will absorb and re-radiate to surface, trapping it in lower atmosphere, so less energy loss, less radiation cooling
30
Q

why is there a surplus of radiation energy in some parts of the world and a deficit in the others?

A
  1. angle of overhead sun - tilt and curvature of earth
    - sun always overhead the equator, high intensity @eq.
    - @poles, insolation v. dispersed, less intense. travels through more atmosphere on way to poles bcz angle
  2. tilt of earth + seasonality
    - higher latitudes, insolation amount received by earth surface varies seasonally + decreases overall
    - @poles, less direct sun, less/no insolation for many months
  3. albedo
    - poles, snow, high reflectivity (75-95%), so incoming SW reflected, therefore temp low
    - dark oceans, forests, urban absorb much more
31
Q

cells

A

hadley (@equator) -> ferrel (middle) -> polar (near poles)

32
Q
A