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119 Cards in this Set
- Front
- Back
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What is Geography?
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geo = "earth" and graphein = "to write"
a method, holistic, eclectic |
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Geographers use
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spatial analysis, Earth systems science
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5 Geographic Themes
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location - absolute, relative
Region Human - Earth relationships Movement Place |
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Geography studies the relationships among:
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natural systems
geographic areas society cultural activities and the interdependence of these over space |
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Physical Geography
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spatial analysis of all the physical elements and processes that make up the environment (e.g. biogeography, climatology, geomorphology, hydrogeography)
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Human/Cultural Geography
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Behavioral geography, economic geography, historical geography, marketing, medical, political)
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System
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interrelated set of entities, linked by flows of energy and matter, as distinct from the surrounding environment as the system
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Earth's systems
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dynamic - matter and energy are stored and retrieved
Energy is transformed from one type to another |
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Matter:
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mass that has a physical shape and occupies space
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Energy:
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the capacity to change the motion of matter
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Open System
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Energy/matter flow in and out of the system (as inputs or outputs)
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How Earth is an open system?
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Get energy from the sun and energy travels from Earth to space
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Closed System
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System that is self-contained, or shut off from the surrounding environment (rarely found in nature)
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How Earth is a closed system?
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In terms of physical matter and resources (not energy), Earth could be a closed system
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Earth's four spheres
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Atmosphere, Hydrosphere, Lithosphere, Biosphere
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Earth shape
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bulges at equator, flat at poles
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Erastothenes (247 BC)
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Librarian in Alexandria, Egypt
On June 21, travelers reported that sun shone directly into well in Syene (Aswan) Sun never overhead in Alexandria, always a shadow |
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Equatorial circumference:
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24,902 mi
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Polar circumference:
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7,926 mi
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Latitude
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Angular distance N or S of the equator, measured from the center of the Earth
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Equator latitude
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Divides two poles in half
Degree of 0 |
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Latitude Range
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90 degrees N at N Pole to 90 degrees S at S Pole
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Parallel
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imaginary line connecting all points of the same latitude - parallels run parallel to the equator
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How latitude is determined?
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reference to fixed celestial objects such as the Sun or starts
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Polaris
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North Star
Almost directly overhead at N Pole Tail of Little Dipper |
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Longitude
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angular distance E or W of a point on the earth's surface, measured from the center of the earth
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Meridians
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Lines of longitude that run N and S at right angles to parallels
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Earth's Prime Meridian
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Runs through Royal Observatory in Greenwich, England
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Louisville's Coordinates
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38N, 86W
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One degree of latitude
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69 miles
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At equator, one degree of longitude
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69 miles
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At 60 degrees, one degree of longitude
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35 miles
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At 90 degrees, one degree of longitude
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0 miles
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Great Circle
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any circle the size of the earth's circumference that passes through the center of the earth
shortest distance between two points is along great circle route |
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Time zones in the 1800s
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Most countries had their own prime meridians
US lived by local "railroad time" |
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1884 - International Prime Meridian Conference
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Washington, DC
Greenwich Mean time established as world standard |
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How fast does Earth rotate?
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360 degrees every 24 hrs = 15 degrees per hour
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Controlling meridian
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7.5 degrees on either side
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Galileo's use of two clocks
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one clock indicates time at home port, second clock is reset each day at noon. difference shows longitude difference
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Pendulum didn't work at sea
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1760 John Harrison invented marine chronometer
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180 degree meridian line
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International Date Line - when this line is crossed the calendar changes a day
Increase westward, decrease eastward |
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Scale
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ratio of map units to ground units
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Projection
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process of transforming spherical Earth to flat map
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1:24,000
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one unit on the map represents 24,000 units on the ground
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Smaller the denominator in the fraction =
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the larger the scale is
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Smaller scale =
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less detail (large denominator in fraction)
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Spatial information on a globe
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must be converted to a flat surface
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Important spatial features on a globe:
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distance
direction area shape proximity |
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Map Projections
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- must make a decision about whether to preserve area or shape
- involve the development of a grid, graticule on a flat surface - grid represents lines of longitude and latitude |
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Classes of projections
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Cylindrical
conic planar oval |
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Lingua franca
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longs/lats are a form of
common data exchange format |
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Mercator projections
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Gerardus Mercator, 1569
straight line is a line of constant direction invented Rhumb Line - mathematical creation |
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Active Remote Sensing
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beam of energy is directed at a surface and the energy that is reflected back is analyzed (e.g. radar)
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Passive Remote Sensing
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record energy that is radiated from a surface, usually visible light and infrared (e.g. satellite imagery)
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Geographic Information Systems (GIS)
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Combine spatial and attribute data
Every entity in every database is geographically referenced Maps contain: physical and cultural features layers added to create composite overlay |
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Greenhouse gas
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gas in atmosphere that keeps heat from escaping
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60% of US pollution
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automobile pollution
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Invasive species
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African bees
Snakehead Fish Pythons in Everglades |
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Speed Earth is spinning at equator
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1600kmph
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Louisville's controlling meridian
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90 degress W, yet we're in Eastern time zone (75 degrees W)
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Location of our solar system
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trailing edge of Milky Way
disk-shaped mass of nearly 400 billion stars |
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Nebula
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solar system condensed from a large, slowly rotating cloud of dust and gas
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Formulation of Sun and its solar system
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dates back to 4.6 billion years ago
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Gravity
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mutual attracting force exerted by mass on all other objects
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Planetesimal Hypothesis
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Suns condense from nebular clouds
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Speed of light
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186,282mps
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Light-year
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distance that light travels in a year
6 trillion miles |
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Average distance from Earth to Sun
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93,000,000 mi
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Perihelion
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Earth closest to Sun at January - 91.5 mi miles
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Aphelion
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Earth furthest from Sun at July - 94.5 million miles
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Solar Energy
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Sun produces thermonuclear energy
Atoms of hydrogen are forced together under intense heat and pressure Pairs of hydrogen are fused and enormous quantities of energy are released Principal outlets - radiant energy and solar wind |
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Energy flows out of the Sun in forms of
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electromagnetic waves
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Insolation
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solar energy that reaches the Earth
INtercepted SOLAr RadiaTION |
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Solar Constant
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average value of insolation received at thermopause - 1372
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Measure of electromagnetic waves
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wavelength - distance from the crest of one wave length to the next crest
micrometers |
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Shortwaves
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Hot bodies radiate
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Long waves
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Cool bodies radiate
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Dividing line between short and long waves
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~ 4 micrometers
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Sun's Energy
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Ultraviolet, visible and shortwave infrared portions of the spectrum
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Earth's ouput wavelengths
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long - thermal infrared
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Net radiation
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balance between incoming shortwave and outgoing long-wave radiation
positive and high in tropics Middle & High latitudes = negative Sahara Desert is anomaly |
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Solar Winds
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Consist of clouds of electrically charged particles
grow stronger in sunspots |
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Sunspots
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caused by magnetic storms
activity cycles of 11 years |
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Solar Wind
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responsible for auroras
(borealis and australis) absorbed energy is reradiated as light energy of varying colors magnetosphere protects Earth from solar winds (deflects to poles) |
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Seasonality factors
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Revolution
Rotation Tilt of Earth's axis Axial parallelism |
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Revolution
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Earth revolves around the Sun in a counterclockwise direction
Voyage takes 365.24 days |
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Rotation
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Earth rotates on its axis once every 24 hours in a counterclockwise direction
West to East rotation accounts for Sun's daily journey |
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Dividing line between day and night
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circle of illumination
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Tilt of Earth's Axis
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23.5 degrees
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axial parallelism
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Axis maintains alignment during orbit around sun
North Pole points toward north star |
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Winter Solstice
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Dec 21 or 22
Subsolar point at Tropic of Capricorn North pole = 0 hrs of daylight |
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Spring (March) equinox
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March 20 - 21
Subsolar point at equator equal day and night sun setting in south pole |
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Summer Solstice
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June 20 - 21
Subsolar point at Tropic of Cancer North pole = 24 hrs of daylight |
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Fall (September) equinox
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Sept. 22 - 23
Subsolar point at equator equal day and night sun setting in north pole |
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Atmosphere
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extends ~ 300 miles above Earth's surface
odorless, tasteless, colorless, formless |
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Above atmosphere
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exosphere = ' outer sphere'
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Air Pressure
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weight of pressure is pulled downward under pull of gravity
Air is compressed and denser near Earth's surface thins rapidly with increasing altitude |
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Sea-level air pressure
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1013.2 millibars
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Inches of mercury
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29.92 (barometer)
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Layers in atmosphere classified by
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composition, temperature, function
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4 zones of atmospheric temperature
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Troposphere
Stratosphere Mesosphere Thermosphere |
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Troposphere
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supports life
Surface to 11 mi 90% of total atmosphere water vapor, clouds, air pollution, life forms |
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Normal lapse rate
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average cooling rate = 3.5F per 1000 feet
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Stratosphere
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11 to 31 mi
Temp. increase with altitude |
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Mesosphere
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30 to 50 mi
coldest portion of atmosphere = mesopause |
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Thermosphere
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50-300 mi
Temp. rise rapidly due to vibration of molecules Density of molecules so low that little actual heat is produced |
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Heterosphere
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outer atmosphere
50 mi outwards gases not evenly mixed layers of gases sorted by gravity due to atomic weight |
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Homosphere
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inner atmosphere
surface to 50 mi density varies, but blend of gases is uniform ozone is exception - 12-31 mi |
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Homosphere makeup
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78% nitrogen
21% in oxygen 1% argon <1% carbon dioxide |
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Atmospheric function zones
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2 zones that protect us from incoming solar radiation and charged particles:
Ionosphere Ozonosphere |
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Ionosphere
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Extends throughout thermosphere and mesosphere
Absorbs cosmic rays, gamma rays, X-rays, and some UV rays |
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Ozonosphere
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part of stratosphere
O3 absorbs UV energy and converts it to heat energy (infrared radiation) Filters most harmful UV radiation ozone at stratosphere is good radiation, at ground level = pollution |
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Ozone depletion
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"holes" over arctic and antarctic
loss is due to "anthropogenic" factors --> chlorine atoms from CFCs |
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CFC
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chlorofluorocarbons like in refrigerants and propellants in aerosol sprays
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single CI molecule
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decomposes more than 100,000 ozone molecules
can reside in atmosphere for 40-100 years |
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Why holes over poles?
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thin icy clouds in stratosphere are catalysts for releases of chlorine
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Variable atmospheric components
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troposphere contains natural and human-caused variable gases, particles, and other elements
natural sources, anthropogenic pollution, Clean Air Act |
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Natural sources
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produce greater quantity of pollutant than human-made sources
Volcanoes, forest fires, Plants, decaying plants, soil, ocean |
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Natural factors that affect air pollution
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Winds - move pollutants from one area to another
Local and Regional landscapes - surrounding hills/mtns can form barriers to air movement and can trap pollutants Temperature inversion - air trapped by warmer layer above and pollutants remain close to earth - do not mix with upper levels |