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The Gas Laws

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Title: The Gas Laws


1
  • The Gas Laws

2
Temperature (T)
  • Measure of the kinetic energy of the molecules.
  • Average speed of an air molecule at room T ??
  • 450 m/sec 1000 mph !
  • Heating ? speeding up molecules
  • Cooling ? slowing down molecules
  • Absolute zero (0 K) No thermal motion

3
Charles Law
  • V c2 T (at constant pressure)
  • V is proportional to T.
  • V1/V2 T1/T2
  • Example 2 litres/ 3 liters 200 K/ 300 K

4
Temperature scales
  • Kelvin (K) Centigrade (C) Fahrenheit (F)
  • Boiling 373 100 212
  • Freezing 273 0 32
  • Ab. Zero 0 -273 -459
  • Temperature conversions
  • K C 273 for example 0 C 273 K
  • C 5/9 (F-32) for example 70 F 21 C 32 F
    0 C
  • F 9/5 C 32 for example 0 C 32 F 40 C
    104 F
  • http//www.eskimo.com/jet/javascript/convert.ht
    ml

5
Pressure -- P
  • Pressure is defined as force/unit area.
  • It is the force exerted by the weight of the
    atmosphere.
  • 1 atmosphere 1013 mb 14.7 lbs./in.2
  • How much force does the atmosphere exert on your
    body?
  • 1000 in.2 x 14.7 lbs./in.2 14,700 lbs. over 7
    tons of force!
  • Air molecules at sea level collide 109 times per
    second.
  • Air pressure decreases with height (faster in
    cold air).
  • 29.92 in. of mercury 34 feet of water
  • 1 atmosphere 1013.25 millibars (mb) 1013.25
    hPascals
  • This is standard sea level pressure

6
An experiment on a bird in the air pump, by
Joseph Wright
7
Magdeburg Hemispheres (1657)
  • In Germany Otto von Guericke constructed an air
    pump which he used to evacuate two large sealed
    hemispheres. The weight of the air pushing the
    hemispheres together was so great that 16 horses
    were needed to pull them apart.

8
Torricellian Experiment (1644)
  • Nature does not abhor a vacuum and the air has
    weight.

9
  • Density -- ?? mass/volume kg/m3
  • Dry air is slightly denser than moist air at the
    same T and P

10
Boyles Law
  • PV constant
  • P1V1 P2V2
  • Example 1 atm. x 1 liter 0.5 atm. x 2 liters
  • In the atmosphere, use density instead of volume.
  • P c1 ? (at constant temperature)

11
  • Ideal Gas Law
  • P ? RT
  • Where P is pressure, ? is density, R is the gas
    constant, and T is temperature in degrees Kelvin.
  • At the same pressure, cold air is denser than
    warm air.

12
  • Daltons Law of Partial Pressures
  • The total pressure of the air is the sum of the
    partial pressures of its component gases.
  • Ptotal PN2 PO2 e Ptrace

13
Moisture and Clouds
14
Moisture
  • Moisture is critically important to all sorts of
    weather phenomena.
  • If our atmosphere was as dry as Mars, we would
    have winds and sandstorms, and thats about it.
  • On Earth, we have dew, fog, mist, clouds, frost,
    rain, snow, sleet, hail, ice, colored sunsets,
    rivers, lakes, oceans, and many other phenomena
    -- all because of moisture.

15
Measuring humidity
  • Sling psychrometer -- ventilated wet bulb and dry
    bulb thermometers.
  • Hair hygrometer -- hair lengthens with humidity
    (about 2.5). Twisted hair generates torsion.
  • Dew Cell -- measures humidity by an electrical
    conductor coated with LiCl, a chemical whose
    conductivity varies with moisture.

16
Hydrologic Cycle
17
Moisture controls the heat budget of the planet
  • Water vapor is a major greenhouse gas.
  • Clouds, snow and ice reflect sunlight back to
    space.
  • Sensible heat is carried by winds and ocean
    currents
  • Oceans store heat and moderate coastal climates.
  • Snow is an effective insulator.
  • Vegetation alters both the heat and moisture
    budgets.
  • Latent (or hidden) heat is exchanged when water
    changes from one phase to another.
  • Latent heat powers weather systems

18
  • Ice Liquid Vapor
  • highly orderly one free surface random
  • lower energy higher energy
  • lower temperature higher temperature
  • Sublimation, melting, and evaporation all require
    heat from the environment.
  • Deposition, freezing, and condensation all
    release heat to the environment.

19
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20
  • Temperature and phase changes of 1 gram of ice as
    energy is added.

21
Relative Humidity
  • Vapor pressure, e is that portion of the total
    air pressure exerted by the water vapor. From
    Daltons Law of Partial Pressures, e P (H2O).
  • Saturation vapor pressure, es is the maximum
    possible e at a given T. It assumes that the
    water vapor and a plane water surface are in
    equilibrium.
  • Relative Humidity RH e/es x 100
  • Air does not hold water vapor the dry gases in
    the air coexist with water vapor near the ground.
  • It is temperature (mainly) that affects the rate
    of water vaporization.
  • Imagine water molecules leaving and entering
    Johnson Pond. When they are inequilibrium (for a
    given T) then you measure e.
  • As temperatures drop overnight e lowers and RH
    rises
  • If a fog covers the pond, then you can assume e
    es

22
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23
Dew Point
  • Dew Point, Td is the temperature to which air
    must be cooled at constant pressure to reach
    saturation. Dew point indicates the temperature
    at which dew, frost, fog may occur.
  • Often the dew point temperature in the evening is
    a good predictor of the overnight minimum
    temperature? Why?
  • High Td means high absolute humidity.
  • If T and Td are almost the same then RH is high.
  • If T Td, then RH 100

24
Saturation vapor pressure as a function of T
25
Boiling
  • The boiling point is defined as the temperature
    at which the saturation vapor pressure of a
    liquid (es) is equal to the surrounding
    atmospheric pressure.
  • For water, es 1 atm. at 100 C.
  • At pressures greater than 1 atm. (e.g. in a
    pressure cooker), the boiling temperature is
    greater than 100 C.
  • At pressures lower than 1 atm. (e.g. on a
    mountain top), the boiling temperature is less
    than 100 C.

26
BOILING occurs when es 1 atm.
27
Clouds
  • Clouds are aesthetically pleasing. They generate
    rainbows, cloudbows, halos, and gorgeous sunsets.
    Cloudscapes are half of all landscapes.
    Clouds indicate important meteorological
    processes such as convection, fronts, and
    mountain waves. Clouds are the source of rain,
    snow, thunder, lightning, hail, and many other
    weather phenomena. The Earth from space appears
    to be about 50 covered by white clouds of all
    shapes.

28
Clouds
  • Eternal Clouds, let us appear let us arise from
    the roaring depths of Ocean, our father let us
    fly towards the lofty mountains, spread our damp
    wings over their forest-laden summits. . . let us
    shake off the rainy fogs, which hide our immortal
    beauty and sweep the earth from afar with our
    gaze
  • -- Aristophanes, The Clouds
  • I am the daughter of Earth and Water,
  • And the nursling of the Sky
  • I pass through the pores of the ocean and shores
  • I change, but I cannot die.
  • -- Percy Bysshe Shelley, The Cloud

29
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30
Fog is a Cloud on the Ground
  • How Fog is Formed
  • Radiation fog (local)-- Radiational cooling of a
    shallow moist layer with dry layer above it.
    Dissipates with morning sun.
  • Evaporation fog (local) -- Cold air in contact
    with a warmer water surface (e.g. lakes in
    autumn).
  • Upslope fog (mountains) -- gentle lifting of a
    moist layer.
  • Advection fog (regional) -- warm moist air moves
    over a cold surface. E.g. Pacific coast cold
    ocean surface.
  • Precipitation fog (regional) -- warm rain falls
    through a layer of cold air or over a snowfield.

31
Four Basic Cloud Types
  • High, above 6 km
  • Cirrus (Ci), Cirrostratus (Cs), Cirrocumulis
    (Cc)
  • Middle, 2-6 km
  • Altostratus (As), Altocumulus (Ac)
  • Low, 0-2 km
  • Stratus (St), Stratocumulus (Sc), Fog
  • Vertical Development, 1-10 km
  • Cumulus (Cu), Cumulonimbus (Cb)
  • Luke Howard (1803) Stratus layer, Nimbus
    rain, Alto mid-level, Cumulus heap, Cirrus
    wisp

32
  • UK Met Office Cloud Guide
  • http//www.metoffice.com/bookshelf/clouds/

33
  • Cloud type information and photos
  • Plymouth State University
  • Meteorology Program
  • Cloud Boutique
  • http//vortex.plymouth.edu/clouds.html
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