Basic Properties of the Atmosphere - PowerPoint PPT Presentation

1 / 35
About This Presentation
Title:

Basic Properties of the Atmosphere

Description:

Basic Properties of the Atmosphere. Heat and Temperature ... The earth's outermost atmosphere is extremely 'hot' but its heat content is negligible ... – PowerPoint PPT presentation

Number of Views:55
Avg rating:3.0/5.0
Slides: 36
Provided by: ShawnM91
Category:

less

Transcript and Presenter's Notes

Title: Basic Properties of the Atmosphere


1
Basic Properties of the Atmosphere
2
Heat and Temperature
  • Temperature Average energy of molecules or atoms
    in a material
  • Heat Total energy of molecules or atoms in a
    material
  • Can have large amount of heat but low
    temperatures
  • Can have high temperatures but little heat

3
Heat and Temperature
  • The Arctic Ocean has a large amount of heat
    (because of large mass) even though the
    temperature is low.
  • Air in an oven at 500 F has high temperature but
    little heat.
  • However, touch anything solid in the oven, and
    youll get burned. Same temperature, much larger
    amount of heat.

4
Heat and Temperature
  • The earths outermost atmosphere is extremely
    hot but its heat content is negligible
  • The surface of the moon can reach 250 F in
    sunlight and -200 F in shadow, but the vacuum
    around the Apollo astronauts contained no heat.
  • It takes time for things to warm up and cool off.

5
Temperature Scales
  • Fahrenheit
  • Water Freezes at 32 F
  • Water Boils at 212 F
  • Centigrade or Celsius
  • Water Freezes at 0 C
  • Water Boils at 100 C
  • Two scales exactly equal at -40

6
Converting C to F In Your Head
  • Double the Centigrade
  • Subtract the first Digit
  • Add 32

7
Converting F to C In Your Head
  • Subtract 32
  • Add the first Digit
  • Divide by two

8
Absolute Temperature
  • Once atoms stop moving, thats as cold as it can
    get
  • Absolute Zero -273 C -459 F
  • Kelvin scale uses Celsius degrees and starts at
    absolute zero
  • Most formulas involving temperature use the
    Kelvin Scale

9
Electromagnetic Radiation
  • Radio cm to km wavelength
  • Microwaves 0.1 mm to cm
  • Infrared 0.001 to 0.1 mm
  • Visible light 0.0004 0.0007 mm
  • Ultraviolet 10-9 4 x 10-7 m
  • X-rays 10-13 10-9 m
  • Gamma Rays 10-15 10-11 m

10
Composition of the Atmosphere
  • Nitrogen 78.08
  • Oxygen 20.95
  • Argon 0.93 (9300 ppm)
  • Carbon Dioxide 0.035 (350 ppm)
  • Neon 18 ppm
  • Helium 5.2 ppm
  • Methane 1.4 ppm
  • Ozone 0.07 ppm

11
Other Components of the Atmosphere
  • Water Droplets
  • Ice Crystals
  • Sulfuric Acid Aerosols
  • Volcanic Ash
  • Windblown Dust
  • Sea Salt
  • Human Pollutants

12
Structure of the Atmosphere
  • Defined by Temperature Profiles
  • Troposphere
  • Where Weather Happens
  • Stratosphere
  • Ozone Layer
  • Mesosphere
  • Thermosphere
  • Ionosphere

13
Troposphere
  • Heating of the Surface creates warm air at
    surface
  • Warm air rises, but air expands as it rises and
    cools as it expands (Adiabatic cooling)
  • Heating Adiabatic Cooling Warm air at
    surface, cooler air above
  • Buoyancy Cool air at surface, warmer air above
  • Two opposing tendencies constant turnover

14
Stratosphere
  • Altitude 11-50 km
  • Temperature increases with altitude
  • -60 C at base to 0 C at top
  • Reason absorption of solar energy to make ozone
    at upper levels (ozone layer)
  • Ozone (O3) is effective at absorbing solar
    ultraviolet radiation

15
Mesosphere
  • 50 80 km altitude
  • Temperature decreases with altitude
  • 0 C at base, -95 C at top
  • Top is coldest region of atmosphere

16
Thermosphere
  • 80 km and above
  • Temperature increases with altitude as atoms
    accelerated by solar radiation
  • -95 C at base to 100 C at 120 km
  • Heat content negligible
  • Traces of atmosphere to 1000 km
  • Formerly called Ionosphere

17
Why is the Mesosphere so Cold?
  • Stratosphere warmed because of ozone layer
  • Thermosphere warmed by atoms being accelerated by
    sunlight
  • Mesosphere is sandwiched between two warmer layers

18
Composition and Altitude
  • Up to about 80 km, atmospheric composition is
    uniform (troposphere, stratosphere, mesosphere)
  • This zone is called the homosphere
  • Above 80 km light atoms rise
  • This zone is sometimes called the heterosphere

19
Mean Free Path
  • Below 80 km, an atom accelerated by solar
    radiation will very soon hit another atom
  • Energy gets evenly distributed
  • Above 80 km atoms rarely hit other atoms
  • Light atoms get accelerated more and fly higher
  • Few atoms escape entirely

20
Planets and Atmospheres
  • At top of atmosphere, an atom behaves like any
    ballistic object
  • Velocity increases with temperature
  • If velocity exceeds escape velocity, atom or
    molecule escapes
  • Earth escape velocity 11 km/sec.
  • Moon escape velocity 2.4 km/sec

21
Atmospheric Measurements
  • Temperature
  • Pressure
  • Humidity
  • Wind Velocity and Direction

22
Weather Instruments
  • Temperature Thermometer
  • Pressure Barometer
  • Humidity Hygrometer
  • Wind Velocity and Direction
  • Anemometer and Wind Vane

23
Thermometers
  • Fluid
  • Mercury
  • Alcohol
  • Use expansion of fluid
  • Bimetallic
  • Differential expansion of different metals
  • Electronic
  • Electrical resistance change with temperature

24
Barometers
  • Mercury
  • Air pressure will support 10 meters of water
  • Mercury is 13 times denser
  • Air pressure will support 76 cm of mercury
  • Aneroid
  • Air pressure deforms an evacuated chamber

25
Hygrometers
  • Filament
  • Hair expands and contracts with humidity
  • Sling Psychrometer
  • Measures cooling by evaporation
  • Two thermometers
  • Wet bulb and Dry bulb
  • Electrical
  • Chemicals change resistance as they absorb
    moisture

26
Sounding
  • Balloons carry radiosondes
  • Thermometer
  • Barometer
  • Hygrometer
  • Transmitter
  • Typically reach 30 km before balloon breaks

27
Radar
  • Detect precipitation types and amounts
  • Doppler radar measures velocity of winds

28
Satellite Studies
  • Visual imagery
  • Infrared imagery
  • Laser spectroscopy

29
Earths Radiation Budget
  • What comes in must go out
  • Direct Reflectance (Short Wave)
  • 31
  • Infrared Re-emission (Long Wave)
  • 69

30
How Heat Moves
  • Radiation
  • Conduction
  • Convection

31
Albedo
  • Albedo incident energy reflected by a body
  • Fresh snow 75 95
  • Old snow 40 60
  • Desert 25 30
  • Deciduous forest, grassland 15 20
  • Conifer forest 5 15
  • Camera light meters set to 18

32
Global Albedo
33
Air Pressure
  • By lucky coincidence, earths atmospheric
    pressure is approximately neat round numbers in
    metric terms
  • 14.7 pounds per square inch (1 kg/cm2)
  • Pressure of ten meters of water
  • Approximately one bar or 100 kPa
  • Weather reports use millibars (mb)
  • One mb pressure of one cm water

34
Pressure and Altitude
  • Average at sea level 1013 mb
  • 500 mb at 5 km (upper limit of human settlement)
  • 280 mb at 10 km
  • 56 mb at 20 km
  • 1 mb at 50 km
  • 0.00056 mb at 100 km

35
Pressure and Altitude
Write a Comment
User Comments (0)
About PowerShow.com