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Chapter 17 Atmosphere

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A. Intensity of Insolation. Time of day- Most direct sun rays at noon ... 4. Clouds-The intensity of clouds affects the amount of insolation that reaches the earth. ... – PowerPoint PPT presentation

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Title: Chapter 17 Atmosphere


1
Chapter 17 Atmosphere Weather
  • 17.1 The Atmosphere in Balance
  • 17.2 Heat and the Atmosphere
  • 17.3 Local Temperature Variations
  • 17.4 Human Impact on the Atmosphere

2
17.1 The Atmosphere in Balance
  • The atmosphere is like a space suit that has
    changed greatly with time (evolved)
  • A. The past atmosphere
  • Methane Ammonia (4 Bill. Yrs. Ago by volcanoes)
  • Sunlight gtnitrogen, hydrogen carbon dioxide
  • Sunlight broke down water vapor to ozone or O3
  • Blue-green algae produce oxygen (o2)
  • 600 mill. years ago O2 CO2 stabilized

3
17.1 The Atmosphere in Balance
  • B. The Present Atmosphere
  • Gases The two main gases are Nitrogen (N2)
    Oxygen (O2). Other gases are Carbon Dioxide
    (CO2), Water Vapor (H2O) Argon (Ar)
  • The atmosphere is stable because it has an
    efficient recycling system.

4
17.1 The Atmosphere in Balance
  • 1. Nitrogen living organisms need it to make
    protein bacteria in soil release it for plants
  • 2. Oxygen essential for respiration combustion
    or burning of fuels
  • 3. Carbon Dioxide raw material used by plants
    during photosynthesis, returned by respiration
    "Greenhouse Effect"

5
17.2 Heat and the Atmosphere
  • A. How Heat Energy Moves
  • Three ways Conduction, Convection and
    Radiation
  • 1. Conduction-Transfer of heat energy through
    collisions of the atoms or molecules of a
    substance.
  • 2. Convection-Transfer of heat energy in a liquid
    or gas through the motion of the liquid or gas
    caused by differences in densities.
  • 3. Radiation-Transfer of energy through space in
    the form of visible light, ultraviolet light and
    other types of electromagnetic waves.

6
17.2 Heat and the Atmosphere
  • B. Structure of the Atmosphere
  • Troposphere
  • a. Lowest layer, earth's weather
  • b. height 6 to 17 km
  • c. Convection currents w/n Troposphere (hot air
    rises)
  • d. Temperature Drops 6.5C/km
  • e. Tropopause-boundary

7
17.2 Heat and the Atmosphere
  • 2. Stratosphere
  • a. Stratosphere to about -60 C50 km
  • b. Jet Stream-eastward winds 320 km/hr
  • c. Ozone (O3) combined w/ O2 in lightning
  • 16-60 km ozonosphere
  • absorbs UV light and release heat
  • d. Stratopause (18 C) boundary

8
17.2 Heat and the Atmosphere
  • 3. Mesosphere Thermosphere
  • a. 50-90 km Mesosphere, above 90 km
    Thermosphere
  • b. Meteoroids burn up (shooting stars)

9
17.2 Heat and the Atmosphere
  • 4. Ionosphere- lower part of the thermosphere
  • a. 90-500 km
  • b. Electrically charged atoms-ions
  • c. Reflect radio waves
  • d. Satellites- weather, communication, and
    defense

10
17.2 Heat and the Atmosphere
  • C. Insolation and the Atmosphere
  • Insolation-Incoming Solar radiation
  • The energy transfer from the earth's surface is
    one of the major causes of weather in the
    atmosphere.
  • The accumulation of Carbon Dioxide and Water
    Vapor absorb most of the infrared radiation

11
17.3 Local Temperature Variations
  • A. Intensity of Insolation
  • Time of day- Most direct sun rays at noon
  • Latitude- Equator receives the most direct sun
    rays. Locations at the poles can receive no
    daylight or daylight all day.

12
17.3 Local Temperature Variations
  • 3. Time of Year- In the summer the Northern
    Hemisphere gets direct sunshine and the Southern
    Hemisphere is indirect. The opposite happens in
    winter. (remember proximity of Sun)
  • 4. Clouds-The intensity of clouds affects the
    amount of insolation that reaches the earth.

13
17.3 Local Temperature Variations
  • B. Heating of Water and Land
  • Water and Land cool at different rates
  • Specific Heat- The amount of heat needed to raise
    1 gram of a substance by 1 oC. The specific heat
    of water is almost 3 times that of land.
  • Isotherms-Lines that connect places with the same
    temperature.

14
17.4 Human Impact on the Atmosphere
  • A. Common Air Pollutants
  • Air Pollutant- any airborne gas or particle that
    occurs at a concentration capable of harming
    humans or the environment.
  • Clean Air Act of 1970- Six key pollutants Carbon
    Monoxide, Nitrogen Dioxide, Sulfur Dioxide,
    Particulate Matter, Lead and Ozone.

15
17.4 Human Impact on the Atmosphere
  • B. Acid Rain
  • Forms when sulfur dioxide and nitrogen oxides mix
    with water.
  • Acidity is measured using the pH scale. Ranges
    from 0-14. 7 is neutral. Acid rain is around 5.

16
17.4 Human Impact on the Atmosphere
  • C. Smog
  • Photochemical smog is a brownish haze that forms
    in air polluted with nitrogen oxides and
    hydrocarbons from automobile exhaust.
  • Temperature Inversion- An increase in temperature
    with an increase in altitude occurs when a layer
    of cold air is trapped beneath a layer of warm
    air.

17
17.4 Human Impact on the Atmosphere
  • C. Ozone Depletion
  • Caused by Chlorofluorocarbons (CFCs)
  • Loss of ozone increases exposure to harmful
    ultraviolet radiation.

18
17.4 Human Impact on the Atmosphere
  • E. Global Warming
  • Average temperatures have increased 1 oC since
    1880.
  • Caused by the burning of fossil fuels and global
    deforestation, which raises the amount of CO2 in
    the atmosphere.
  • Creates changes in climate, a rise in sea level
    and increased drought.
  • An Inconvenient Truth - Science
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