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environmental determinism
environment determines human behavior
Systems theory
set of ordered, interrelated components, linked by flows of energy and matter, distinct from the surrounding environment outside the system. includes subsystems
Milky way galaxy
100,000 light years in diameter. flat disk of stars
negative feedback
discourages change in a system, leading to stability, or selfregulation. counteracting
positive feedback
the encouragement of change in a system, can lead to a ‘snowballing’ effect, leading to instability +death eg. ocean level rise
Steady-state equilibrium
maintain structure and character over time. energy and material system that remains balanced over time, are constant or recur, is in a steady-state condition.
Dynamic equilibrium
steady-state system demonstrates a changing trend over time. appears gradually or suddenly; thresholds/tipping points
Speed of light
300,000 km/second. Universe is 12 billion light-years in all directions
Earth’s speed in orbit
averages 107,280 km/hr
tropic
either of two parallels of latitude about 23.5 N or S. ‘to turn’, or ‘change’ (a turning back point)
equinox
either of two times of the year when the sun crosses the plane of the earth's equator and day and night are of equal length
solstice
sol + sistere “to stand still”. either of the two times of the year when the sun is at its greatest distance from the celestial equator. Dec 21/22 & June 21. Sun’s declination is at its position farthest north at the Tropic of Cancer (23 degrees N), or south, at the Tropic of Capricorn (23 degrees S).
Axial parallelism
as the Earth revolves in its orbit its axis always appears parallel to itself. axial tilt- tilted by an average of 23.5 degrees away from a right angle with the plane of the ecliptic
Perihelion
closest position to sun on Jan. 3 in Northern hemisphere winter is 147,255,000 km
Aphelion
farthest distance to sun on July 4 during Northern hemisphere summer is 152,083,000 km
Reasons for seasons
Earth’s revolution around the Sun
Earth’s daily rotation on its axis
Earth’s tilted axis
Axial parallelism
Sphericity (geoid-shape of the Earth)
coriolis force
a force due to the earth's rotation; flows are turned toward the right in the northern hemisphere and toward the left in the southern hemisphere
Heliophysics
the study of the sun and its interactions with Earth and the solar system
Radiation
energy from a source in the form of waves or particles = electromagnetic waves
solar wind
a stream of protons moving radially from the sun. needing about 3 days to reach Earth, sometimes augmented by coronal mass ejections
Sunspots
surface disturbances caused by magnetic storms
Auroras
Latin: ‘dawn; goddess of the dawn’, Solar winds make contact with Earth’s magnetic field = magnetosphere. borealis in the north, australis in the south
Insolation
incident solar radiation
loss of insolation
A) Absorption (e.g. absorption bands) B) Scattering C) Reflection
Solar Constant
rate at which radiant solar energy is received at the outer layer of the earth's atmosphere. total solar irradiance = amount of solar radiation received by Earth within the Earth’s thermopause at 480 km altitude
EM Spectrum
all possible wavelengths of electromagnetic energy emitted by a body; Portions of the electromagnetic spectrum of radiant energy are either visible or invisible to the human eye
Transmissivity
atmospheric ‘windows’. ability of the atmosphere to allow radiation to pass through
Velocity
(v) = rate of movement in some direction (v = distance/time, expressed e.g. meters/second)
Wavelength
( λ) = distance between corresponding points on any two successive waves (expressed in micrometers, μm)
Frequency
(f) = the number of waves passing a fixed point in 1 second (expressed in hertz, Hz).
Wave
a disturbance or variation that transfers energy progressively from point to point in a medium
Intensity
(I) is the amount of solar radiation striking an object (expressed as watts/m 2 )
Inverse Square Law
Total energy is constant so more distance, less intensity per unit area, 2x distance, 1/4 radiation
Albedo
the ratio of reflected to incident light, reflective quality of a surface. Earth average = 30%. light color, smooth texture= high albedo
Mie scattering- Gustav Mie
(nonmolecular scattering), or aerosol particle scattering takes place in the troposphere, spherical particles present with diameters=to the size of the wavelength of the incident ray. makes clouds white
Air
mixture of gases that is naturally odorless, colorless, tasteless and formless, blended as if it were a single gas
pressure
exerted by a gas, sum total of the impact of the particles composing it. (F/A). In atmospheric science, pressure is often measured as pascals (Pa). Pa at sea level =101,325 Pa
kinetic energy
energy of motion, the vibrational energy we measure as temperature: KE = 1/2mv2
Temperature
avg. KE of individual particles, or molecules, in matter. A measure of sensible heat energy present in the atmosphere and other media
Heat
flow of KE from one body to another, resulting in a temp difference between them; depends upon density or mass of substance/body. Heat flow stops when the temperatures (amounts of kinetic energy) are equal. sensible & latent heat transferred by radiation, conduction, convection, advection
mean free path
distance a particle travels before colliding with another molecule
Noctilucent clouds (NLCs)
upper mesosphere = cosmic or meteoric dust particles, acting a nuclei around which fine ice crystals form, highest clouds, ice crystals
photodissociation
Reaction w/ sunlight degrades compounds by incoming photons, breaking apart molecules of CO2 to create oxygen (O2 ), providing minuscule amounts of oxygen which will combine to create ozone. O2+UV---> O+O (atomic O) O+ O2 ---> 03 (ozone, creation) O3+ UV---> O+O2 (destructionn)
ozonosphere
Consists of 3 linked oxygen molecules. ozone is destroyed by reactions with chlorine, bromine, nitrogen, hydrogen, and oxygen gases. methane (CH4 ), chlorofluorocarbons (CFCs), nitrous oxide (N2O) contribute to catalytic reactions
catalytic reaction cycle
set of chemical reactions resulting in destruction of ozone molecules while the molecule that started the reaction is reformed to continue the process.
Polar Stratospheric Clouds
Ozone-depleting substances are transported great distances by atmospheric air motions. Contribute to ozone hole of the antarctic. Formed in low temps
Tropopause
‘lid’ keeping cooler air from mixing with warmer (less dense) air in stratosphere
Troposphere
the lowest atmospheric layer; from 4 to 11 miles high. all weather, all forms of water tropos: turn. Hottest at the bottom, pressure is 5x lower at tropopause than it is at earth's surface
Stratosphere
the atmospheric layer between the troposphere and the mesosphere. stratified, not much change. Temperature is increasing with altitude, pressure decreases. Heating in stratosphere by absorbing UV, ozone molecules are broke up with UV radiation, breaking and combining over and over
Mesopause
coldest area in atmosphere. Ignorosphere, Air is too sparse in mesosphere to research
thermosphere
the atmospheric layer between the mesosphere and the exosphere. thermo: heat. temperature increases with height because radiation from the sun is absorbed. Density of air is extremely low, but the air molecules are high temps
Ionosphere
contains thermosphere and mesosphere
magnetosphere
the magnetic field of a planet; the volume around the planet in which charged particles are subject more to the planet's magnetic field than to the solar magnetic field. shield against solar winds, magnetic field that extends past earth's atmosphere
Photodissociation
reaction with sunlight that degrades compounds, CO2 to O2
ideal gas law
air volume is inversely proportional to its pressure (Robert Boyle); that air volume is directly proportional to its temperature (J.A.C. Charles ) . PV = nRT
drift
the airborne movement of agricultural chemicals as droplets, particles or vapor outside of the intended agricultural target area. Pesticides
PM
particular matter. Diverse mixture of fine particles such as haze, smoke, dust; smaller particles are aerosols. Approx. residence time in lower 2 km of troposphere 5 – 9 days; about 1 month in upper troposphere; 2-3 years in stratosphere
SMOG
smoke + fog. industrial smog pollution – coal-burning industries. sulfuric acids
Acid deposition
rain, snow, dust, particulate matter. Sulfur dioxide & nitrogen oxides from fertilizers and fossil fuel combustion. converted to nitric acid (HNO3) and sulfuric acid (H2SO4) in the atmosphere and precipitate
Sensible heat
Energy that changes temperature of a substance
latent heat
heat absorbed or radiated during a change of phase at a constant temperature and pressure. (LE) Energy stored in water vapor as water evaporates. Water absorbs large quantities of this latent heat
specific heat
the heat required to raise the temperature of one gram of a substance one degree centigrade. higher retains more heat. Land is low, water is high
Sir Issac Newton
Inverse Square Law
Stefan-Boltzmann Law
more temperature, more emissive power. total radiant heat energy emitted from a surface is proportional to the fourth power of its absolute temperature. Josef Stefan and Ludwig Boltzmann
Why is the sky blue?- John William Strutt
Rayleigh scattering. Blue light in insolation is scattered by gas molecules more intensely than the other colors
Wein’s Law Displacement Law
Objects radiate energy in wavelengths related to their individual surface temperatures
Henry Cavendish
decribe phlogiston- false concept of hydrogen
Antoine Laviosier
named hydrogen (‘generator of water’). used azot for nitrogen (Greek for something ‘incompatible with life’). first to recognize oxygen its own right, calling it oxygéne (‘maker of acids’)
William Hyde Wollaston
notice that there were gaps in the light spectrum – dark lines where the light seemed to have been stripped out. Joseph von Fraunhofer further mapped out
Robert Bunsen and Gustav Kirchhoff
realized that these “Fraunhofer lines” appeared at same wavelengths as some of emission lines viewed with spectroscope. elements in the atmosphere were absorbing the light
Edward Frankland
named helium (Greek sun god Helios). Norman Lockyer saw a ‘3rd yellow line’ light spectrum gap
Joseph Black
experimented unknowingly with nitrogen
Daniel Rutherford
called nitrogen 'mephitic air’ (a Greek legendary noxious emission). removed oxygen and carbon dioxide from air and was left with nitrogen
William Ramsay and Lord Rayleigh
identified and described argon. Greek for ‘lazy’. highly inert/highly unreactive
galileo
early version of the thermoscope
Santorio
applied a scale to an air thermoscope. supposed inventor of the thermometer
Daniel Fahrenheit
produced an accurate alcohol and mercury thermometer
Anders Celsius
devised a scale that substituted the boiling point of water for body temperature, with 0 degrees C for the freezing point and 100 degrees C for the boiling point of water.
Guillaume Amontons
showed that there was an absolute minimum temp. at which pressure would drop to nothing
William Thomson, (aka Lord Kelvin)
developed an “absolute” temperature scale that would apply to all substances. He set absolute zero as 0 on his scale. Kelvin (K) scale
Blaise Pascal
carried two glass tubes containing mercury to the top of the ‘Puy de Dôme’- early barometer
Evangelista Torricelli
invented the mercury barometer
Joseph Fourier
‘greenhouse effect’
Svante Arrhenius
tied together carbon dioxide levels and global temperatures