The Earth and Its Atmosphere
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Transcript of The Earth and Its Atmosphere
Chapter 1
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There is no upper limit of the atmosphere, but it rather becomes thinner and thinner, merging with empty space.
greenhouse effect = warming that results when solar radiation is trapped by the atmosphere; caused by atmospheric gases that allow sunshine to pass through but absorb heat that is radiated back from the warmed surface of the earth.
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Water is the only substance that can be found naturally in the atmosphere in its 3 phases (solid->ice, liquid->water, gas->water vapor)
-laughing gas
Fig. 1-4, p. 7
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CarbonDioxidecycle
Vertical Structure of the Atmosphere Air Pressure and Air Density
Weight (force acting on an object due to gravity) = mass x gravitational acceleration = m x g
Density = mass/volume (air density at sea level ~ 1.2 kg/m3 )
Pressure = force/areaAt the Earth’s surface the pressure of the atmosphere is
14.7 lbs/in2 . Standard sea level pressure is:
1013.25mb=1013.25hPa=29.92 in.Hg.Atmospheric pressure decreases with an increase in
height.
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~ 9km
Vertical Structure of the Atmosphere
Layers of the Atmosphere- Pressure & Density decrease with height- Air temperature has a complicated vertical profile
Lapse rate = the rate of change (decrease) in temperature with a change in height; the average lapse rate in Troposphere = - 6.5 C / 1 km.
Inversion layer = change in the sign of the lapse rate, + 6.5 C / 1 km.
Isothermal environment = no change in temperature with height
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Fig. 1-11, p. 13
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Layers of the atmosphereas related to averageprofile of airtemperature.
Vertical Structure of the Atmosphere
Observation: RadiosondeWeather balloonInstrument and transmitterAir temperature, humidity, pressure
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Vertical Structure of the Atmosphere
The IonosphereNot a true layer but an electrified region within the upper
atmosphere (from about 60 km to the top of the atmosphere) where fairly large concentrations of ions and free electrons exist.
Ions = molecule with an additional or minus an electron
Sun light creates layers: F (at 180 km) ,E (at 120 km),D (at 60 km) layers
Ionosphere plays a major role in AM radio communications
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At night, the F region of ionosphere strongly reflects AM radio waves, allowing them to be sent over great distances. During the day, the lower D region strongly absorbs and weakens AM radio waves, preventing them from being picked up by distant receivers.
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(more solareruptions)
Based on composition of the atmosphere
Weather and Climate Weather: short term changing in air
temperature, air pressure, humidity, clouds, precipitation, visibility, and wind
Climate: long term patterns and average weather; not just magnitude but also frequency
Assignment 1
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Weather & Climate Meteorology
Study of the atmosphere and its phenomena Aristotle 340 B.C. – book on natural philosophy, Meterologica. – Greek
word = meteoros = “high in air” – sum of knowledge at that time
The birth of Meteorology as a natural science did not take place until the invention of weather instruments: thermometer ( end of 16th century), barometer (17th century), hygrometer (18th century).
1843 telegraph invented 1920s concepts of air masses and fronts 1940s upper air balloons 1950s radar and computers 1960s satellite
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Doppler radar has the capacity of estimating rainfallintensity.
Weather & Climate Satellite’s View
Geostationary satellite: situated at about 36,000Km (22,300mi) above the earth. Satellite travels at the same rate as the earth spins, which allows it to remain positioned above the same spot.
Meridians measure longitude (W-E): lines running from north to south. Prime meridian (00meridian) runs through Greenwich, England.
Parallels to equator (00latitude) measure latitude (N-S)
Weather maps: pressure cells, fronts, surface stations
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Fig. 1-15, p. 209/2/2009 17
SatelliteImage:clouds+stormsat surface
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Simplified surface weather map that correlates with the satellite image shown .
Weather & Climate Weather and Climate in Our Lives
Two general reasons for studying how weather and climate impacts our lives: economic efficiency and public safety.
Crops Utilities Extreme cold and heat Tornados and hurricanes Clothing
Meteorologist Any person with a college degree in meteorology or atmospheric science;
not just the TV weather person Half of 9000 meteorologists employed by the US National Weather Service Researchers and operational meteorologists
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Chapters 2 and 19
Energy, Temperature, & Heat Energy is the ability to do work (push, pull, lift)
on some form of matter. Potential energy is the potential for work.
Gravitational potential energy:
Kinetic energy is energy of a moving object
Total energy = PE + KE Temperature is a measure of the average speed of atoms
and molecules. High temperature corresponds to high average speeds
mghPE
2
21 mvKE
Cold, more dense air
Warm, lessdense air
Energy, Temperature, & Heat Which has more energy?
A lake or a cup of hot tea?
Heat is the energy in the process of being transferred from one object to another because of a difference in temperature.
First Law of Thermodynamics: Energy cannot be destroyed or created conservation of energy
Temperature Scales Fahrenheit (early 18th century): 32 freeze, 212 boil
(180 equal divisions)
Celsius (later in the 18th century): 0 freeze, 100 boil (100 equal divisions)
Kelvin (19 century): absolute; 0K = -273°C (no thermal motion)
3295 00 FC
27300 CK