Chapter 11

Characteristics of the Atmosphere

Make sure you read this chapter

 

I.              Structure of the Atmosphere: Know figure 11-2

-       Gases:  Nitrogen 78%, Oxygen 21% and Argon .93%

-       Compounds: Carbon dioxide and Water vapor (0.0 to 4.0%) (water cycle)- regulate amount of energy absorbed in atmosphere

-       Layered into zones

-       Ozone- importance to humans (protection from UV radiation)

-       Atmospheric Dust- small particles-example H2O

A.         Troposphere- all weather takes place

Carbon dioxide and Water Vapor

Thickest layer over the equator and a thinner layer over poles

Temperature decreases as altitude increases

Tropopause- temp. remains constant

B.          Stratosphere- ozone concentrated

Ozone- “heavy oxygen”: O3

Stratopause- high temperature zone

C.          Mesosphere- coldest layer of the atmosphere. Air thin and chemical reactions are taking place (-130° F)

D.         Thermosphere- Nitrogen/Oxygen absorb solar energy. Sometimes called

Ionsphere- ions and free electrons.

Exosphere- indefinite altitude

I.               Solar Energy- know figure 11-5

a. Radiation-transfer of energy through space by electromagnetic waves (remember the electromagnetic spectrum).

- Higher temperatures emit shorter     wavelengths. More energy!

-       50% of incoming solar radiation is absorbed directly or indirectly.

-       Water heats up and cools down more slowly than land

-       Earth reradiates solar energy back into the atmosphere at larger wavelengths.

Conduction- transfer of energy that occurs when molecules collide

-       Energy is transferred from surface to lowest layer of atmosphere.

-       Substances must be in contact with each other

-        Convection- transfer of energy by flow of heated substance. Similar to the Sun and ocean.

Temperature vs Heat

Temperature: how rapidly or slowly molecules move around (Kinetic Energy). Used to measure and interpret energy.

Heat: transfer of energy

-flow of heat from an object of higher temperature to an object of low temperature.

-Transfer of energy that fuels the atmospheric processes.

Temperature- Fahrenheit or Celsius

      Fahrenheit = 1.8 x Celsius + 32.0

      Celsius = (Fahrenheit-32.0)/1.8

Kelvin-

-       Zero Degrees Kelvin= -523° F

-       Lowest possible temperature-no motion

Dew Point- (condensation temperature)

-       constant pressure, cooler temperature to reach saturation

-       saturation-air holds as much water vapor as it possible can

-       condensation- gas to liquid

ex. Water changes state to fall as rain

-Temperature decrease in troposphere with increasing distance from surface

-       Individual air masses can be warmer or cooler and wetter or drier than air around it.

-       Lifted Condensation level- clouds begin to form-base of clouds

Air Pressure/Density/Temperature:

Know table 11-2 pg. 280

-       Pressure decreases with height

-       Density- number of particles of air occupying a particular space

-       Temperature varies according to the ratio of pressure to density

-       Temperature Inversion- cool on surface warm above-pollution trapped

Wind & Relative Humidity

-       Wind- imbalance between air masses-movement from high pressure to low pressure.

-       Humidity-water vapor

-       Relative humidity-how much air can hold-varies with temperature-warm air more moisture than cool

Cloud Formation

       Form when warm, moist air rises, expands and cools in convection current

       Condensation nuclei-small particles in the atmosphere around which cloud droplets can form.

       Air reaches its dew point, the water vapor in the air condenses around nuclei

Orographic Lifting

       Clouds form when warm moist air is forced to rise over a mountain

       When two air masses of different temperatures meet

Stability: ability of an air mass to resist rising. Cooling air resists rising-it is stable.

Latent Heat: condensation-heat is released. Energy is stored in water vapor and released when condensation occurs. Stored energy is called Latent Heat

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