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Naturalists at Large: Atmosphere
Atmosphere


                       Thin envelope of
    Weather            gases that surrounds       Climate
                       the planet.


The state of the                              Weather conditions
atmosphere at a                               at a locality averaged
given place and time                          over a specified time
                                              period
Naturalists at Large: Atmosphere
Atmosphere is divided into four
 distinct zones of contrasting
 temperature due to differential
 absorption of solar energy.




There is little mixing between
layers.
As you move higher in altitude
the atmosphere thins out.
Troposphere contains about
75% of the mass the earth’s air,
but is only about 17km thick.
Most weather events occur here.
It’s composition is uniform due
to mixing caused by winds.
Temperatures drop with altitude.
The sharp boundary in
temperature at the tropopause
limits mixing with upper layers
Stratosphere extends to about
50km thick.
Similar in composition to the
troposphere except in two ways.
It contains1000 times less water
and is 1000 times higher in
ozone.
Ozone is produced by lightning
and solar irradiation of oxygen
molecules.
The Stratosphere is relatively
calm, volcanic ash or human
caused pollution can remain in
suspension in the stratosphere
for many years.
Past and Present Composition
The composition of the Earth’s atmosphere has changed since the
formation of the Earth. The Earth’s first atmosphere was mainly
helium and hydrogen. Volcanic emissions later added carbon
dioxide, nitrogen, water, sulfur dioxide and other elements.
Large amounts of carbon dioxide from volcanoes caused the
Earth’s past climate to be warmer than today’s.




Without carbon dioxide no life could be present on earth. Primitive
bacteria and algae in oceans could now photosynthesis.
But no life on land due to solar radiation from the sun.
But life in oceans is protected from radiation and can
develop due to presence of carbon-dioxide
Naturalists at Large: Atmosphere
Free oxygen gas was absent in the earth’s early atmosphere.
 Any oxygen produced by photosynthesis reacted with other chemicals
and was trapped in the form of oxide compounds in rock, Fe2O3 .
It took millions of years before oxygen was present as a gas in the
atmosphere
  Nearly all the molecular oxygen in the atmosphere today was
  produced by photosynthesis.

            Sunlight + CO2 + H2O → O2 (g) + C6H12O6

Living organisms are responsible for the evolution of our
atmosphere. Free oxygen made it possible for life to evolve on land.
Before large amounts of free oxygen were present in the
atmosphere, lethal intensities of solar radiation flooded the Earth’s
surface.
Free oxygen reacts in the stratosphere to form ozone (O3). This ozone
layer shields the Earth’s Surface from lethal radiation.
Oxygen produced by photosynthesis builds up in the atmosphere. This
turns into ozone due to solar radiation.
Gas        Symbol Percent by Volume
        Nitrogen         N2       78.08 %
        Oxygen           O2       20.94 %
        Argon            Ar       0.934 %
        Carbon Dioxide   CO2      0.033 %
        Neon             Ne       0.00182 %
        Helium           He       0.00052%
        Methane          CH4      0.00015 %
        Krypton          Kr       0.00011 %
        Hydrogen         H        0.00005 %
        Nitrous oxide    N2O      0.00005 %
        Xenon            Xe       0.000009 %

Water vapor varies depending on the location. From 0.01% to 5%
Suspended particles within the Atmosphere are called aerosols.

Aerosols can be both solid and
liquid. Some are too small to
see, other are clustered together
and can be seen as clouds.

 Volcanoes are one major
 source of natural aerosols
How does the Earth keep itself warm?
The average radiant energy from the sun falling on the surface
at about 343 watts /m2.
As it passes through the atmosphere, 6% is scattered back into
space by atmospheric molecules.10% is reflected back into
space from land and ocean surface.
The remaining 84% actually heats up the surface.
 To balance this the Earth itself needs to radiate the same
 amount of energy back into space.
The Earth emits long-wave length radiation in the form of
infrared radiation. (this depends on the temperature of the
surface and the type of surface)
But the amount of energy is not balanced.
Nitrogen and Oxygen gas can neither absorb or emit thermal radiation.
It is Water vapor, carbon dioxide, and some other minor gases which
absorb long-wave thermal radiation leaving the surface.
 This is why the average surface temperature is 15°C instead of
 -6°C which it should be it balanced.


                                                 1. Solar radiation
                                                 2. Radiation from
                                                 greenhouse gases
                                                 3. Radiation scattered
                                                 by atmosphere.
Some wavelengths of radiation from the Earth can escape into space
if there are no clouds. Other wavelengths are absorbed by gases and
re-emitted into space or back to the surface.
    Graph of radiation emitted from Earth’s surface that is
                absorbed by the Atmosphere.
Absorption of solar energy by the atmosphere is selective.
Visible light passes through, ultraviolet is absorbed mostly by
ozone in the stratosphere. Infrared is absorbed mostly by carbon
dioxide and water in the troposphere.
Naturalists at Large: Atmosphere
Solar Radiation and the Atmosphere

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Naturalists at Large: Atmosphere

  • 2. Atmosphere Thin envelope of Weather gases that surrounds Climate the planet. The state of the Weather conditions atmosphere at a at a locality averaged given place and time over a specified time period
  • 4. Atmosphere is divided into four distinct zones of contrasting temperature due to differential absorption of solar energy. There is little mixing between layers. As you move higher in altitude the atmosphere thins out.
  • 5. Troposphere contains about 75% of the mass the earth’s air, but is only about 17km thick. Most weather events occur here. It’s composition is uniform due to mixing caused by winds. Temperatures drop with altitude. The sharp boundary in temperature at the tropopause limits mixing with upper layers
  • 6. Stratosphere extends to about 50km thick. Similar in composition to the troposphere except in two ways. It contains1000 times less water and is 1000 times higher in ozone. Ozone is produced by lightning and solar irradiation of oxygen molecules. The Stratosphere is relatively calm, volcanic ash or human caused pollution can remain in suspension in the stratosphere for many years.
  • 7. Past and Present Composition The composition of the Earth’s atmosphere has changed since the formation of the Earth. The Earth’s first atmosphere was mainly helium and hydrogen. Volcanic emissions later added carbon dioxide, nitrogen, water, sulfur dioxide and other elements.
  • 8. Large amounts of carbon dioxide from volcanoes caused the Earth’s past climate to be warmer than today’s. Without carbon dioxide no life could be present on earth. Primitive bacteria and algae in oceans could now photosynthesis.
  • 9. But no life on land due to solar radiation from the sun. But life in oceans is protected from radiation and can develop due to presence of carbon-dioxide
  • 11. Free oxygen gas was absent in the earth’s early atmosphere. Any oxygen produced by photosynthesis reacted with other chemicals and was trapped in the form of oxide compounds in rock, Fe2O3 . It took millions of years before oxygen was present as a gas in the atmosphere Nearly all the molecular oxygen in the atmosphere today was produced by photosynthesis. Sunlight + CO2 + H2O → O2 (g) + C6H12O6 Living organisms are responsible for the evolution of our atmosphere. Free oxygen made it possible for life to evolve on land. Before large amounts of free oxygen were present in the atmosphere, lethal intensities of solar radiation flooded the Earth’s surface. Free oxygen reacts in the stratosphere to form ozone (O3). This ozone layer shields the Earth’s Surface from lethal radiation.
  • 12. Oxygen produced by photosynthesis builds up in the atmosphere. This turns into ozone due to solar radiation.
  • 13. Gas Symbol Percent by Volume Nitrogen N2 78.08 % Oxygen O2 20.94 % Argon Ar 0.934 % Carbon Dioxide CO2 0.033 % Neon Ne 0.00182 % Helium He 0.00052% Methane CH4 0.00015 % Krypton Kr 0.00011 % Hydrogen H 0.00005 % Nitrous oxide N2O 0.00005 % Xenon Xe 0.000009 % Water vapor varies depending on the location. From 0.01% to 5%
  • 14. Suspended particles within the Atmosphere are called aerosols. Aerosols can be both solid and liquid. Some are too small to see, other are clustered together and can be seen as clouds. Volcanoes are one major source of natural aerosols
  • 15. How does the Earth keep itself warm? The average radiant energy from the sun falling on the surface at about 343 watts /m2. As it passes through the atmosphere, 6% is scattered back into space by atmospheric molecules.10% is reflected back into space from land and ocean surface. The remaining 84% actually heats up the surface. To balance this the Earth itself needs to radiate the same amount of energy back into space. The Earth emits long-wave length radiation in the form of infrared radiation. (this depends on the temperature of the surface and the type of surface) But the amount of energy is not balanced.
  • 16. Nitrogen and Oxygen gas can neither absorb or emit thermal radiation. It is Water vapor, carbon dioxide, and some other minor gases which absorb long-wave thermal radiation leaving the surface. This is why the average surface temperature is 15°C instead of -6°C which it should be it balanced. 1. Solar radiation 2. Radiation from greenhouse gases 3. Radiation scattered by atmosphere.
  • 17. Some wavelengths of radiation from the Earth can escape into space if there are no clouds. Other wavelengths are absorbed by gases and re-emitted into space or back to the surface. Graph of radiation emitted from Earth’s surface that is absorbed by the Atmosphere.
  • 18. Absorption of solar energy by the atmosphere is selective. Visible light passes through, ultraviolet is absorbed mostly by ozone in the stratosphere. Infrared is absorbed mostly by carbon dioxide and water in the troposphere.
  • 20. Solar Radiation and the Atmosphere