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119 Cards in this Set

  • Front
  • Back
What is Geography?
geo = "earth" and graphein = "to write"
a method, holistic, eclectic
Geographers use
spatial analysis, Earth systems science
5 Geographic Themes
location - absolute, relative
Region
Human - Earth relationships
Movement
Place
Geography studies the relationships among:
natural systems
geographic areas
society
cultural activities
and the interdependence of these over space
Physical Geography
spatial analysis of all the physical elements and processes that make up the environment (e.g. biogeography, climatology, geomorphology, hydrogeography)
Human/Cultural Geography
Behavioral geography, economic geography, historical geography, marketing, medical, political)
System
interrelated set of entities, linked by flows of energy and matter, as distinct from the surrounding environment as the system
Earth's systems
dynamic - matter and energy are stored and retrieved
Energy is transformed from one type to another
Matter:
mass that has a physical shape and occupies space
Energy:
the capacity to change the motion of matter
Open System
Energy/matter flow in and out of the system (as inputs or outputs)
How Earth is an open system?
Get energy from the sun and energy travels from Earth to space
Closed System
System that is self-contained, or shut off from the surrounding environment (rarely found in nature)
How Earth is a closed system?
In terms of physical matter and resources (not energy), Earth could be a closed system
Earth's four spheres
Atmosphere, Hydrosphere, Lithosphere, Biosphere
Earth shape
bulges at equator, flat at poles
Erastothenes (247 BC)
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
Equatorial circumference:
24,902 mi
Polar circumference:
7,926 mi
Latitude
Angular distance N or S of the equator, measured from the center of the Earth
Equator latitude
Divides two poles in half
Degree of 0
Latitude Range
90 degrees N at N Pole to 90 degrees S at S Pole
Parallel
imaginary line connecting all points of the same latitude - parallels run parallel to the equator
How latitude is determined?
reference to fixed celestial objects such as the Sun or starts
Polaris
North Star
Almost directly overhead at N Pole
Tail of Little Dipper
Longitude
angular distance E or W of a point on the earth's surface, measured from the center of the earth
Meridians
Lines of longitude that run N and S at right angles to parallels
Earth's Prime Meridian
Runs through Royal Observatory in Greenwich, England
Louisville's Coordinates
38N, 86W
One degree of latitude
69 miles
At equator, one degree of longitude
69 miles
At 60 degrees, one degree of longitude
35 miles
At 90 degrees, one degree of longitude
0 miles
Great Circle
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
Time zones in the 1800s
Most countries had their own prime meridians
US lived by local "railroad time"
1884 - International Prime Meridian Conference
Washington, DC
Greenwich Mean time established as world standard
How fast does Earth rotate?
360 degrees every 24 hrs = 15 degrees per hour
Controlling meridian
7.5 degrees on either side
Galileo's use of two clocks
one clock indicates time at home port, second clock is reset each day at noon. difference shows longitude difference
Pendulum didn't work at sea
1760 John Harrison invented marine chronometer
180 degree meridian line
International Date Line - when this line is crossed the calendar changes a day
Increase westward, decrease eastward
Scale
ratio of map units to ground units
Projection
process of transforming spherical Earth to flat map
1:24,000
one unit on the map represents 24,000 units on the ground
Smaller the denominator in the fraction =
the larger the scale is
Smaller scale =
less detail (large denominator in fraction)
Spatial information on a globe
must be converted to a flat surface
Important spatial features on a globe:
distance
direction
area
shape
proximity
Map Projections
- 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
Classes of projections
Cylindrical
conic
planar
oval
Lingua franca
longs/lats are a form of
common data exchange format
Mercator projections
Gerardus Mercator, 1569
straight line is a line of constant direction
invented Rhumb Line - mathematical creation
Active Remote Sensing
beam of energy is directed at a surface and the energy that is reflected back is analyzed (e.g. radar)
Passive Remote Sensing
record energy that is radiated from a surface, usually visible light and infrared (e.g. satellite imagery)
Geographic Information Systems (GIS)
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
Greenhouse gas
gas in atmosphere that keeps heat from escaping
60% of US pollution
automobile pollution
Invasive species
African bees
Snakehead Fish
Pythons in Everglades
Speed Earth is spinning at equator
1600kmph
Louisville's controlling meridian
90 degress W, yet we're in Eastern time zone (75 degrees W)
Location of our solar system
trailing edge of Milky Way
disk-shaped mass of nearly 400 billion stars
Nebula
solar system condensed from a large, slowly rotating cloud of dust and gas
Formulation of Sun and its solar system
dates back to 4.6 billion years ago
Gravity
mutual attracting force exerted by mass on all other objects
Planetesimal Hypothesis
Suns condense from nebular clouds
Speed of light
186,282mps
Light-year
distance that light travels in a year
6 trillion miles
Average distance from Earth to Sun
93,000,000 mi
Perihelion
Earth closest to Sun at January - 91.5 mi miles
Aphelion
Earth furthest from Sun at July - 94.5 million miles
Solar Energy
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
Energy flows out of the Sun in forms of
electromagnetic waves
Insolation
solar energy that reaches the Earth
INtercepted SOLAr RadiaTION
Solar Constant
average value of insolation received at thermopause - 1372
Measure of electromagnetic waves
wavelength - distance from the crest of one wave length to the next crest
micrometers
Shortwaves
Hot bodies radiate
Long waves
Cool bodies radiate
Dividing line between short and long waves
~ 4 micrometers
Sun's Energy
Ultraviolet, visible and shortwave infrared portions of the spectrum
Earth's ouput wavelengths
long - thermal infrared
Net radiation
balance between incoming shortwave and outgoing long-wave radiation
positive and high in tropics
Middle & High latitudes = negative
Sahara Desert is anomaly
Solar Winds
Consist of clouds of electrically charged particles
grow stronger in sunspots
Sunspots
caused by magnetic storms
activity cycles of 11 years
Solar Wind
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)
Seasonality factors
Revolution
Rotation
Tilt of Earth's axis
Axial parallelism
Revolution
Earth revolves around the Sun in a counterclockwise direction
Voyage takes 365.24 days
Rotation
Earth rotates on its axis once every 24 hours in a counterclockwise direction
West to East rotation accounts for Sun's daily journey
Dividing line between day and night
circle of illumination
Tilt of Earth's Axis
23.5 degrees
axial parallelism
Axis maintains alignment during orbit around sun
North Pole points toward north star
Winter Solstice
Dec 21 or 22
Subsolar point at Tropic of Capricorn
North pole = 0 hrs of daylight
Spring (March) equinox
March 20 - 21
Subsolar point at equator
equal day and night
sun setting in south pole
Summer Solstice
June 20 - 21
Subsolar point at Tropic of Cancer
North pole = 24 hrs of daylight
Fall (September) equinox
Sept. 22 - 23
Subsolar point at equator
equal day and night
sun setting in north pole
Atmosphere
extends ~ 300 miles above Earth's surface
odorless, tasteless, colorless, formless
Above atmosphere
exosphere = ' outer sphere'
Air Pressure
weight of pressure is pulled downward under pull of gravity
Air is compressed and denser near Earth's surface
thins rapidly with increasing altitude
Sea-level air pressure
1013.2 millibars
Inches of mercury
29.92 (barometer)
Layers in atmosphere classified by
composition, temperature, function
4 zones of atmospheric temperature
Troposphere
Stratosphere
Mesosphere
Thermosphere
Troposphere
supports life
Surface to 11 mi
90% of total atmosphere
water vapor, clouds, air pollution, life forms
Normal lapse rate
average cooling rate = 3.5F per 1000 feet
Stratosphere
11 to 31 mi
Temp. increase with altitude
Mesosphere
30 to 50 mi
coldest portion of atmosphere = mesopause
Thermosphere
50-300 mi
Temp. rise rapidly due to vibration of molecules
Density of molecules so low that little actual heat is produced
Heterosphere
outer atmosphere
50 mi outwards
gases not evenly mixed
layers of gases sorted by gravity due to atomic weight
Homosphere
inner atmosphere
surface to 50 mi
density varies, but blend of gases is uniform
ozone is exception - 12-31 mi
Homosphere makeup
78% nitrogen
21% in oxygen
1% argon
<1% carbon dioxide
Atmospheric function zones
2 zones that protect us from incoming solar radiation and charged particles:
Ionosphere
Ozonosphere
Ionosphere
Extends throughout thermosphere and mesosphere
Absorbs cosmic rays, gamma rays, X-rays, and some UV rays
Ozonosphere
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
Ozone depletion
"holes" over arctic and antarctic
loss is due to "anthropogenic" factors --> chlorine atoms from CFCs
CFC
chlorofluorocarbons like in refrigerants and propellants in aerosol sprays
single CI molecule
decomposes more than 100,000 ozone molecules
can reside in atmosphere for 40-100 years
Why holes over poles?
thin icy clouds in stratosphere are catalysts for releases of chlorine
Variable atmospheric components
troposphere contains natural and human-caused variable gases, particles, and other elements
natural sources, anthropogenic pollution, Clean Air Act
Natural sources
produce greater quantity of pollutant than human-made sources
Volcanoes, forest fires, Plants, decaying plants, soil, ocean
Natural factors that affect air pollution
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