How the Earth Works: Atmosphere Flashcards

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1
Q

What wavelength of radiation does the atmosphere absorb?

A

Longwave.

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2
Q

Give examples of strong absorbers of longwave energy in the atmosphere.

A
  • Atmospheric H2O vapour
  • CO2

(This is why the atmosphere heats up from bottom to top!)

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3
Q

Give 5 examples of trace gases.

A
  • CO2
  • CH4
  • N2O
  • O3
  • Halocarbons
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4
Q

State the barometric law.

A

Atmospheric pressure decreases by a factor of 10 for every 16km in altitude.

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5
Q

What are the four regions of the atmosphere and what distinguishes them?

A
Thermosphere🌤
         ⬆️
Mesosphere
         ⬆️
Stratosphere      
         ⬆️         
Troposphere🌱
Distinguished by temperature.🌡
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6
Q

Describe the troposphere.

A
  • Gases are relatively well mixed.

* Temperature is due to heating of the Earth’s surface and emission of longwave radiation.

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7
Q

Describe the reason for the temperature in the stratosphere.

A

Temperature is due to UV absorption by ozone and emission of longwave radiation.

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8
Q

How have CFCs affected the ozone layer?

A

Atmospheric O3 absorbs UV radiation. CFCs deplete O3 allowing more UV to reach the Earth’s surface.

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9
Q

What is the dominant ozone-depleting substance in the 21st century?

A

N2O

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10
Q

What is the driving force behind atmospheric circulation?

A

Solar energy distribution.☀️

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11
Q

Describe temperature gradients.

A

The Earth varies in temperature from the equator to the poles leading to density and pressure differences which drive global movement of air.

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12
Q

State the relationship between temperature, air density and pressure.

A

As temperature decreases, air density and pressure increase.

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13
Q

What is the ‘Polar Front Zone’?

A

The area where cold polar air meets warm rising air from the subtropics.

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14
Q

What are ‘Ferrel Cells’?

A

When air in mid-latitudes is forced to flow counter to the Hadley and Polar air movements.

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15
Q

Which three factors determine the Earth’s surface temperature?

A
  1. Amount of incoming solar radiation.
  2. Earth’s reflectivity.
  3. Amount of warming provided by Earth’s atmosphere. (i.e. Greenhouse effect)
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16
Q

What causes the temperature profile in the stratosphere?

A

UV absorption by ozone and emission of long wave radiation.

17
Q

Describe Hadley cells.

A

Heating land leads to convective uplift of air. As air reaches high pressure the air cools it begins to sink due to buoyancy loss. The cycle repeats.