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EARTH STRUCTURE Layered Earth o Crust Oceanic – Maximum depth generally less than 10km Continental – Maximum depth generally less than 70km, less dense than oceanic crust o Mantle Lithosphere – Rigid (solid rock) • 10km – 100km depth • ~90km thick Asthenosphere – Fluid-like (plastic rock) • 100km – 350km depth • Approaches surface at mid-ocean ridges • ~250km thick o Core Core is entirely metallic Outer Core – Liquid metal (iron) • 2,890km – 5,150km depth Inner Core – Solid metal (iron) • 5,150km starting depth o Different density (resulting from different chemical and mineral compositions o Different strengths o Gets more and more dense as you go deeper Isostasy – Less dense materials float on top of more dense material Continental crust is less dense than the mantle or the core and so can “float” on it o Mountains for example don’t just sit on the earth’s surface but actually embed themselves into the lithosphere and asthenosphere o The liquid-like asthenosphere is able to accommodate this extra continental “root” and so a large portion of the mountain actually exists below sea-level Behavior of Materials o Elastic – Deformation is recovered, object returns to original shape (earthquakes) o Ductile – Deformation is permanent, stress applied over long time or at high temperatures o Brittle – Deformation is permanent, stress applied very quickly to shatter or break object (mudslide) o Difference between brittle and ductile is the time scale over which the material deforms Internal Sources of Energy o The mantle is heated by various sources o Impact energy – Tremendous number of smaller bodies hit the Earth early after its formation, converting energy to motion to heat o Gravitational energy – As Earth pulled to smaller and denser mass, gravitational energy was released as heat o Radioactive elements – Unstable radioactive atoms decay and release heat at an exponentially decreasing rate; rate is characterized by half-life o Heat from these sources is still flowing to the surface today Heat Transfer o The mantle is solid but behaves ductily over long period of time, so it loses heat by convection o The asthenosphere loses heat by convection o The crust is solid and brittle, so it cannot convect, it loses heat by conduction o The Earth loses heat to space by radiation Gravity is attraction between objects Gm1m2 o Fg = r2 G =6.673e-11 Nm2/kg2 PLATE TECTONICS The lithosphere of the Earth is broken into pieces called plates The gigantic pieces of lithosphere (plates) are constantly being pulled, pushed, created, and destroyed in a process called the tectonic cycle Plate-edge interactions are directly responsible for most of the earthquakes, volcanic eruptions, and mountains on Earth Tectonic Cycle o Magma rises from the asthenosphere to the surface at mid-oceanic volcanic ridges o New magma solidifies and adds to the plate edges o New lithosphere cools and slowly moves laterally away from the zones of oceanic crust formation, called spreading centers o Subduction - When the leading edge of a moving slab of oceanic lithosphere collides with another slab, the older, colder, denser slab turns downward and is pulled by gravity back into the asthenosphere, where it is destroyed o The less dense, more buoyant slab stays “afloat” while the the denser slab subducts beneath it The continents and seafloor are simply passengers on the moving lithosphere above which they rest Evidence for Plate Tectonics o Magnetization patterns on the seafloors Running parallel to the mid-Atlantic spreading ridge are striped parallel bands of magnetized rock showing alternate polarities The Earth reverses its magnetic poles every few thousand years Magma is injected into the ocean ridges and is imprinted with the Earth’s magnetic orientation as it cools to form new rock The fact that the seafloor represents alternating magnetic patters suggests that seafloor is continually being created (and presumably destroyed) o Ages of the ocean basin The ocean floor is only about 200M years old, significantly younger than any other feature on the Earth’s surface o o o o o o Oceans are young features that are continually being transformed and created along oceanic ridges and destroyed at subduction zones Fit of the continents Rock types and fossils on the different continents match up along boundaries Earthquake epicenters outline plate boundaries Oceanic mountain ranges and deep ocean trenches Deep earthquakes Movement of tectonic plates using GPS EARTHQUAKES Most earthquakes are explainable based on plate tectonics theory The lithosphere is broken into rigid plates that move away from, past, and into other rigid plates As the tectonic plates move, points along the fault line are held in place due to the friction that exists between the two surfaces of the contacting plates The shear stress due to friction builds up at the fault line until the energy buildup can overcome the friction, causing an earthquake These global-scale processes are seen on the ground as individual faults where the Earth ruptures and the two sides move past each other in earthquake-generating events Hypocenter – Actual location of the Earthquake deep underground Epicenter – The location on the surface directly above the hypocenter Types of Plate boundaries o Divergent Boundary – Plate boundaries where two plates are moving apart from each other and so new crust must be created to fill in the gap Most common in oceanic spreading centers located in the middle of oceans, where new sea floor is created, Generally higher than the average depth of the sea floor Typically result in normal fault Can also occur in continental rock (East African Rift) ex. Mid-Atlantic ridge, Nazca Plate/Pacific Plate o Convergent Boundary – Plate boundaries where two plates are moving toward each other and so some material must get overlapped Thrust faulting • Southern California/Pacific Plate, Indian Plate/Eurasian Plate Subduction zones - A convergent plate boundary where material gets overlapped • When a subduction zone is between oceanic crust and continental crust, the oceanic crust subducts because it is more dense • In continent-continent convergence zones (Himalayas) continental crust (Indian plate) can subduct beneath other continental crust (Eurasian plate) • ex. Nazca Plate/South American Plate, Pacific Plate/Eurasian Plate o Transform/Shearing – Plate boundaries where two plates are moving past each other, parallel to the boundary Crust is not being consumed are created Typically result in strike-slip faults ex. San Andreas Fault, North Anatolian Fault (1999 Ismit earthquake), North American Plate/Pacific Plate Types of Faults o Normal o Reverse o Strike-slip Seismic Cycle o Deformation during an earthquake is very quick and is greatest near the fault and tapers off the farther away you go from the fault line o On the long term, deformation is elastic and all points on the two plates move away from each other equally, regardless of the distance from the fault line itself o Between earthquakes, the deformation is relatively elastic and the plates continues to move apart but points along the fault line are held still due to friction Sliding and Friction o τ = μσ N o (Shear Force) = (Coefficient of Friction)(Normal Force) o Byerlee’s law states that the coefficient of friction for most rocks is 0.6 ≤ μ ≥ 0.85 o Newton’s 2nd Law: F = ma o Hooke’s Law: F = kx o Equate the two expressions for force and we have a mathematical relationship between elastic deformation and accelerations: ma = kx Waves o Amplitude – Displacement (Half the distance from peak to trough) o Wavelength – Distance from peak to peak o Period – Time between waves o Frequency – Number of waves in one second (1/period) Seismic Waves o Body Waves – Move through the interior of the Earth P (Primary) Waves • Fastest of all waves • First to reach recording station • Move as push-pull – alternating pulse of compression and extension • Velocity depends on density and compressibility of substance they are traveling through • V = 4.8 km/s (approx.) through granite • Can travel through air and so may be audible near epicenter S (Secondary) Waves • Slower • Transverse motion – Shearing or shaking particles at right angles to the wave’s path, actual waves • V = 3.0km/s (approx.) • Up-and-down and side-to-side shaking, do a lot of damage • Can only travel through solid o Surface Waves - Faster than body waves, short period, high frequency, most energetic near epicenter Travel near the Earth’s surface, created by body waves disturbing the surface Longer period than body waves (carry energy farther) Do the most damage Love Wave • Travel similar to S- waves but side-to-side in horizontal plane • Travel faster than Rayleigh waves • Do not move through water Rayleigh Wave • Backward-rotating, elliptical motion o Wave Speeds Wave propagation speed depends on the material through which it is propagating (the density and the sheer modulus) P-Waves (Primary wave, arrives first) – Faster k + ( 4 )G 3 • VP = ρ • K-Modulus of incompressibility (function of material) • P – Density • G - Shear modulus S-Wave (Secondary wave, arrives second) – Slower G • VS = ρ Wave Speed and Relative Damage o Waves can be amplified due to slow wave speeds in week soils o Energy of seismic wave is given by E = cλρA2 C - Constant of proportionality λ - Wavelength ρ - Density A - Amplitude o Wavelength of seismic wave is given by λ = vT λ - Wavelength T – Period v - Velocity o Energy is conserved as a wave passes from one type of rock to another E1 = E2 A2 v1 ρ1 = A1 v2 ρ 2 o Soft Rock (less dense) – Waves move much slower, spend more time in that area, amplitude increases, amplifies ground shaking Creep - The amount of gradual slide that occurs between plates between earthquakes o Causes the gradual offset of sidewalks and buildings o Does not cause earthquakes o A lot of build up energy can be dissipated through creep Locating earthquake position o Differences in wave speeds can be used to approximate earthquake positions o Compare the arrival times of the P and S waves and calculate a general radius using the wave speed equation above o Using triangulation, compare seismographic readings at different stations (minimum three) to accurately pinpoint epicenter Seismic Moment – A measure of energy release during an earthquake o M 0 = GLDd o M0 – Magnitude (seismic moment) o (G) Sheer modulus ~ 3 x 1010 Pa for most rocks o (d) Slip of the earthquake, how far the two pieces slid past each other, movement along the rupture o (L) Length o (D) Depth o Area = LD o Measured in Newton meters Moment Magnitude Scale ⎛2⎞ o M W = ⎜ ⎟(log(M 0 ) − 9.1) ⎝3⎠ o MW – Moment magnitude (a number between 0 and 10) o M0 – Seismic moment = GAd Focal Mechanisms o “Beach-ball” diagrams o Shaded – Compression o White – Tension (pulling apart) o Strike/Slip Earthquake – Circle is divided into 4 quarters o Dip Earthquake – Circle is shaded in more elaborate patterns Coulomb Failure Stresses – The theory that an earthquake, by adding strain and stress due to the displacement it causes, may be able to induce an earthquake on another plane o At the same time, if an earthquake pushes two zones together, it may be able to clamp it shut and retard its ability it have an earthquake o We can use GPS to measure the deformation associated with an earthquake. These displacements can then be used to calculate the stresses (forces exerted by the earthquake) o σ = Gε Stress = (Shear Modulus) x (Strain) ΔL o ε= L o Stress is a measure of force exerted (on another fault plane that might rupture) Change in Coulomb Failure Stresses o Δσ = Δτ + μ ' (σ ) f η s Δσ - Change in Coulomb Failure Stress f Δτ - Change in shear stress component s μ ' (σ ) - (Coefficient of friction) x (Normal stress) η Paleosiesmology – The investigation of past earthquakes by examination of their geological records o An earthquake deforms the Earth’s surface and that deformation can be preserved beneath layers of sediment o Allows scientists to study earthquake history and study it more closely Assessing Earthquake Hazard o Degrees of Seismic Risk – What sort of fault is nearby? Is it locked/creeping? What is the seismic history of the location o Building Type – Factors influencing vulnerability include: flexible materials, “soft” first stories (such as garages), use of sheared walls, braced frames Good – Soft building materials that move with the motion of the earthquake; ex. wood Bad – Stone masonry; soft first stories like garages simply collapse and the entire building up above it simply falls and pancakes the first story o Ground Type – The amplitude of seismic waves strongly depends on the type of ground it passes through because seismic energy is conserved as a seismic wave passes from one rock type to another, keeping E (energy) constant E = cλρA2 • c-constant of proportionality, λ-wavelength, ρ-density, A-wave amplitude λ = vT • v-velocity, T-period Soft Rock (less dense) – Waves move much slower, spend more time in that area, amplitude increases, amplifies ground shaking • ex. Marina District-SF, Back Bay-Boston, Mexico City Great Sumatra Earthquake/Tsunami (2004) o Magnitude 9.1 o Rupture length: 1300km o Slip 10 meters o Dip-Slip (Reverse faulting) o Setting: Subduction zones o Occurred underwater o Deadly because it caused a tsunami o Tsunami was so deadly because it occurred far enough off shore that it was able to grow and pick up speed Also, because of the location, the tsunami bounced back and forth North Ridge Earthquake (1994) o Magnitude 6.7 o Rupture length: 30km o Slip: 4 meters o Continental thrust faulting While the relative motion of the Pacific Plate and the North American plate is generally strike-slip, some areas are prone to compression energy and material buildup, which rupture as continental thrusting o Rupture did not reach surface but occurred underground Loma Prieta – World Series Earthquake (1989) o Magnitude 6.9 o Slip: 5 meters o Rupture length: 70km o Continental strike-slip faulting o Associated with San Andreas fault o California, 10km north of Santa Cruise, 60km south of San Francisco TSUNAMIS Tsunamis can be triggered by earthquakes Four Requirements for an earthquake to cause a tsunami o Must occur under or near a large body of water o Must be a normal or reverse fault (must cause vertical movement of the seafloor) o Must have a magnitude greater than 7.5 o Must have a shallow focus (less than 70km) In deep water, tsunamis travel very fast (>800km/hr) and have a very low wave height In shallow waters, the waves slow down and the wave height increases dramatically Wave Speed in Relation to Ocean Depth o v = gD o v – velocity of tsunami (m/s) o g – acceleration due to gravity (m/s2) o D – depth of water through which the wave is travelling (m) VOLCANOLOGY Volcanism is closely linked with plate tectonics, particularly subduction zones o As a plate subducts, a few hundred kilometers away from the subduction zone, the subducted plate heats up and begins to melt o As a result, the molten material becomes more buoyant and begins to migrate upwards o The molten material breaks through the continental crust above, creating a volcano o Because of the linear nature of a subduction zone, often times chains of volcanoes are created 90% of volcanism is associated with plate boundaries o 80% at spreading centers o 10% at subduction zones Remaining 10% of volcanism occurs above hot spots Variations in magma’s chemical composition, ability to flow (viscosity), gas content, and volume determines whether eruptions are peaceful or explosive Of 92 naturally occurring elements: o Eight make up more than 98% of Earth’s crust o Twelve make up 99.23% of Earth’s crust o Oxygen and silicon are by far the most abundant Magma – Molten or liquid rock with some crystallized solids (minerals o Magma hardens to volcanic rock when cooled at the surface, or plutonic rock when cooled within the Earth Lava – Magma that flows on the Earth’s surface Three V’s of Volcanology o Viscosity may be low or high Controls whether magma flows easily or piles up High viscosity gives rise to explosive volcanism because it is more difficult to cause that initial eruption Factors affecting viscosity • Temperature • Silica (SiO2) – Higher Silica content, more viscous (∴ explosive) • Amount of crystallized materials (mineral solid) o Volatile abundance may be low, medium, or high Volatiles refer to gasses, oxygen water, and other light elements that are able to dissolve into the rock matrix If they are trapped in a high viscosity matrix, they may cause explosive eruptions May ooze out harmlessly or explode Factors affecting volatility • Concentration of dissolved gasses (especially water) • At high pressure and low temperature, gasses stay dissolved • As magma rises, pressure decreases, dissolved water turns to steam, and, in the presence of thick magma, becomes explosive o Volume may be small, medium, or large Greater volume Æ More intense eruptions Subduction Zone Volcanism o As an oceanic plate subducts, it carries water-saturated sediments down with it o The water lowers the melting point of the subducted slab and rocks around it, causing partial melting of these rocks and magma formation o The magma then rises, and as it contact the rock of the overlying plate, those rocks also experience melting o Subduction zone volcanoes exhibit higher SiO2 content, higher water content, and lower-temperature magmas than magmas at spreading centers o These factors cause subduction zone volcanoes to experience more explosive eruption o Typical subduction zone volcano type: stratovolcano (and sometimes scoria cone) Three Factors Will Cause Rock to Rise o Lowering Pressure As soon as the subterranean magma chamber is exposed to lower pressure, it begins to rises, causing a runaway process in which magma continues to rise further and further as it is exposed to less and less pressure o Raising Temperature o Increasing Water Content Under high pressure, water mixes with magma and forms a solution As the magma rises and the pressure decreases, water escapes as gas air bubbles The rapid escape of gas from the magma often causes explosive reactions Hotspot Volcanism o Hotspots – Areas of earthquakes and volcanoes not necessarily located on plate boundaries o Occur when unusually hot portions of the mantle send plumes of magma upwards into the crust o Locations of hotspots are fixed and therefore can provide an example of the motion of tectonic plates Hot spots, often times found in the middle of the ocean, create islands As tectonic plates move above the hot spot over time, the hot spot creates island chains (ex. Hawaii-Emperor islands) In a chain of islands, the oldest islands have generally fallen below the ocean surface due to continued erosion and other natural forces Use the shape of hotspot trail to determine movement of tectonic plate with respect to the hotspot Rock Types o Igneous – Formed when magma cools Intrusive – Cools slowly underground Extrusive – Cools quickly at surface o Non-explosive volcanic rock types Pahoehoe Aa Gabbro (formed underground) Deposited slowly o Explosive volcanic rock types Pyroclastic debris – Broken up magma and rock from violent gaseous explosions, classified by size Deposited very quickly May be deposited as • Air-fall layers (settled from ash cloud) • High-speed, gas-charged flow that surges over surface (pyroclastic flow) o Other volcanic material Obsidian – Volcanic glass forms when magma cools very fast Pumice – Porous rock from cooled froth of magma and bubbles, indicates that the eruption had a lot of gasses associated with it Eruption Styles o Non-Explosive: Icelandic o Non-Explosive: Hawaiian o Somewhat Explosive: Strombolian o Explosive: Vulcanian – Alternating between thick flows and pyroclastic eruptions ex. Aeolian Islands, Sicily o Explosive: Plinian – Gas powered vertical eruptions, lots of pumice, etc. Often the final phase of a volcano after vulcanian phase Signs of Increasing Volcano Activity o Bulging of the volcano face due to increased subterranean magma movements o Increased seismic activity also due to increased subterranean magma movements o Increased presence of gasses (CO2) in area near volcano InSAR and Volcanoes o InSAR is a satellite tool that can be used to detect deformation of the Earth’s surface from space o These deformations, which can be caused by various factors including movement of magma under volcanoes and displacement across faults, can be used to assess volcano activity Magma Type Magma Type Viscosity Volatility Tectonic Setting Rock Types Basalt Low Low 45% Basilica content Andesite Medium Rhyolite High Medium 55% Basilica content High 70% Basilica content Mid-ocean ridges Shield volcanoes Flood basalts (India) Subduction zones Aa Pahoehoe Gabbro Diorite (intrusive) Mt. Rainer Cone shaped volcano Dome shaped volcano Granite (intrusive) Obsidian (extrusive) Pumice (extrusive) Volcano Morphology and Eruption Style Volcano Type Shape Magma Eruption Style Tectonic Setting Shield Volcano Width is much larger than height, very gentle slopes, convex upward Basaltic (fluid) Hawaiian, Not very explosive Hot spots, Hawaii Scoria Cones (Cinder Cone) Large, sloped, straight sides with steep slopes, large summit crater Andesite/Basaltic Strombolian, Explosive Subduction zones, Andes Stratovolcano (Composite Volcano) Gentle lower slopes but steep upper slopes, concave upward, small summit crater Rhyolite, Andesite Vulcanian, Plinian Subduction zone, pacific northwest MASS WASTING EVENT Triggers of Mass Movements o Heavy rains o Earthquakes o Thawing of frozen ground o Construction projects Add weight to top of slope Remove vegetation Cut into the base of slope Types of Mass Movements o Slide – Material moves as semisolid mass along basal surface (planar or curved) Creates “terraced” landscape or hillside o Fall – Material moves as a block or coherent mass with a dominantly vertical downward motion; free fall o Flow – Material flows over landscape as a very viscous fluid-like mass Turbulence within moving mass o Subsides – Material collapses into a void as a block or coherent mass with a dominantly vertical downward motion Scarp – The remaining edge left after a mass wasting event removes a chunk of earth Energy o Kinetic Energy – Energy of motion ⎛1⎞ K = ⎜ ⎟mv 2 ⎝2⎠ K – kinetic energy m – mass v - velocity o Potential Energy – Stored energy U = mgh g – acceleration due to gravity h - height Slide Types o Rotational slide Move downward and outward above curved slip surface with movement rotational about an axis parallel to slope Head moves downward and rotates backward Toe moves upward on top of landscape Move short distance Associated with rather steep slopes ex. Ensenada, Baja California 1976 o Creep Particularly common in areas that experience freeze-thaw cycles Slowest, more widespread form of slop failure Soil expands perpendicular to ground surface shrinks straight downward in response to gravity Requires water content o Translational Slip surface has a constant orientation Move on planer slip surface such as a fault, joint, clay-rich layer Associated with a shallower slope Coulomb-Terzaghi Failure o τ = σ + (P − Pw ) tan φ o τ – Shear resistance o σ – Cohesion o P – Pressure of soil load o PW – Pressure of water o tan φ – Failure angle Water reduces the contact between mineral grains, making it difficult for the surface ground to transfer the normal load at depth o See page 243 for chart of speed versus wetness of mass wasting events Strength of hillside comes from cohesion (how well it sticks together) plus the weight of all materials under gravity Roots and vegetation hold ground together and prevent it from sliding Strength is offset by pore-water pressure and angle of slide surface Failure angle is low (near horizontal) for weak materials (clay) and high (near vertical) for stronger materials ATMOSPHERE Adiabatic (Isocaloric) – A process in which no heat is transferred to or from working fluid Boyle’s Law: P1V1 = P2V2 o If pressure increases, volume decreases o If pressure decreases, volume increases Temperature decreases as volume increases due to fewer molecular interactions Summary: ↑P , ↓V, ↑T AND ↓P, ↑V, ↓T Atmospheric pressure, and with it atmospheric temperature, decreases with increasing altitude Parcels of air match the surrounding pressure by: o Rising Ælower pressure Æ higher volume Æ lower temperature o Sinking Æ higher pressure Æ smaller volume Æ higher temperature Adiabatic Lapse Rate – The rate at which a parcel’s temperature changes with altitude o An air parcel will rise if it is warmer than the surrounding atmosphere and sink if it is colder than the surrounding atmosphere o A parcel of air will continue to rise/fall until it reaches an altitude where the surrounding atmosphere has the same temperature o Generally constant at -9.8°C/km Atmospheric Lapse Rate – The rate at which the atmosphere’s temperature changes with altitude Stable Atmosphere – The atmospheric lapse rate is less (negative) than the adiabatic lapse rate, and rising parcels will tend to be pushed back downward Unstable Atmosphere – The atmospheric lapse rate is more (negative) than the adiabatic lapse rate, and rising particles will continue to rise creating rapid vertical motions in the atmosphere and possibly leading to thunderstorms and tornados TORNADO Tornado - A violently rotating column of air pendant from a cumulonimbus cloud and nearly always observable as a funnel cloud or tube Tornados are a product of atmospheric instability Last anywhere between 10 seconds to 30 minutes Basic Requirements for Tornado Formation o Warm, humid, low-level air (often flowing in from the Gulf of Mexico) o Cold, dry, mid-level air (often flowing from Canada or the Rockies) o High-altitude jet stream moving eastward at rapid speeds o The different directions these air masses are travelling induces rotation o The warm air near the surface and the cool air at higher elevations results in an unstable atmosphere It is very difficult to precisely calculate tornado wind speeds because they are transient phenomena that are relatively unpredictable and also very violent, destroying most scientific instrumentation Tornado wind speeds are generally estimated by the damage they cause Tornado Formation o Warm, low altitude, humid air from Gulf collides with cold, mid-altitude, dry air from Canada or Rockies o High altitude jet stream moving east o Different directions of travelling air masses induce rotation (not necessarily a result of Coriolis effect) Hurricane Formation o Sea surface (upper 60m) temperature > 27°C in the upper 60 meters of ocean o Air must be unstable, warm, and humid o Upper-level winds should be weak and blowing in the same direction the storm is moving o Low pressure zone develops, causing winds from higher pressure zones to flow towards it o Interaction between pressure gradient and Coriolis force induces rotation o Rotates around a central core o Core draws warm, moist air up to the stratosphere, where it cools and loses its water vapor by condensation, releasing large amounts of latent heat o Heat warms surrounding air, creating stronger updrafts and fueling upward flow of wind through central core Require large change in wind speed and direction with height Require large horizontal thermal gradient (needed for thunderstorm formation, which can form tornados) Forms over land (solar heating of ground surface contributes to development of thunderstorms associated with tornados) Only small vertical change in wind speed and direction needed Do not require large horizontal temperature gradient o Small, transient phenomena o Can be hundreds of meters wide and last up to a couple of hours o Large, longer-lived phenomena o Can be hundreds of kilometers in diameter and last for several days o Form over water o Lose strength as they pass over land due to loss of power source HURRICANES Pressure Gradient Force – Force due to the difference in pressure over a horizontal distance (directed from high pressure to low pressure) Δpressure o Fpg = ρΔx The Coriolis Effect – An effect caused by the rotation of the Earth, which makes moving objects that are not in contact with the Earth’s surface appear to travel in curved paths o Magnitude of Coriolis Effect (Acceleration) 2Ωvsin(λ) o Magnitude of Coriolis Force (F=ma) 2Ωmvsin(λ) o Deflection due to Coriolis Force Δx 2 Ω sin(λ ) δ = v Deflection is clockwise in the northern hemisphere and counterclockwise in the southern hemisphere Deflection is greatest at the poles o Ω = angular velocity of Earth (rad/sec) o v = linear velocity of object traveling above the Earth (m/s) o m = mass of object (kg) o λ = latitude (radians) o Δx = distance traveled over the Earth’s surface (m) o Explanation of Coriolis Force A cannonball sitting in a cannon on the equator, pointed northward, has a sideways velocity component due to the rotation of the Earth When the cannonball is fired it gets a forward velocity component but also retains a sideways velocity component equal to that at the equator Because points north (or south) of the equator have a lower angular velocity (sideways velocity component), the cannonball appears to curve clockwise Geostrophic Balance – The Coriolis effect and the pressure gradient are equal Δpressure o 2Ωvsin(λ) = ρΔ x Pressure (Pa), Δx (m), v (m/s), λ (rad), Ω (rad/s), ρ (kg/m3) Atmosphere Circulation around High and Low Pressure o Air will always seek to flow from high to low pressure o The Coriolis Force will increase along the air’s velocity, exerting a force perpendicular to the wind’s velocity (right in the Northern Hemisphere and left in the Southern Hemisphere) o The pressure gradient force and the Coriolis Force will roughly balance one another out creating a circulation around the high or low pressure system Circulation is clockwise around high pressure systems and counterclockwise around low Linear and Angular Motion o Radians = (Degrees) x (π/180) o Angular Velocity = Ω = (2π/t) 2πr cos(λ ) o Linear Velocity = v = t t - length of day (86400 sec) λ - latitude (radian, converted from degrees) r - radius of Earth at equator (6.3e6 m) Basic Requirements for Hurricane Formation o Must form over water o Minimum sea surface temperature 27°C o Air must be unstable, warm, and humid o Low pressure system o Formation must occur far enough from the equator Bermuda High - Standing area of high pressure over the central Atlantic that pushes new developing hurricanes from the south central Atlantic (where they are created) to the North American continent MASS EXTINCTIONS Mass Extinction – The loss of 40% or more of species in a relatively short time o Months, years (indistinguishable in geologic time), up to hundreds/thousands of years o Global phenomenon Background Extinction – The loss of 10-100 species per year, according to fossil record Major losses of marine species define geologic time o Paleozoic, Mesozoic, Cenozoic Five Major Mass Extinctions o Late Ordovician (440 Mya) o Late Devonian (365 Mya) o Late Permian (251 Mya) – Most severe mass extinction know Between 75 and 95% of marine species went extinct o Late Triassic (199-214 Mya) o Late Cretaceous (65 Mya) Causes for the K-T Extinction 65 million years ago (killed dinosaurs) o Flood volcanism, particularly from the Deccan Traps in Inda Short term: Cooling (ash block sunlight) Long Term: Increase of CO2 in atmosphere raising global temperatures, acid rain o Extraterrestrial Impact Short term: Cooling (dust block sunlight) Long term: warming, acid rain, wildfires ASSESSING COSTS OF DISASTER PREVENTION Decision Tree o The cost of a disaster prevention mechanism is determined by the original cost of implementing it added to the various other costs multiplied by the probability that they will be incurred Disaster Cycle o Ideal: DISASTER Æ Rescue/Relief ÆRehabilitation Æ Reconstruction Æ Mitigation/Prevention Æ Preparedness o Actual: DISASTER Æ Rescue/Relief Æ Rehabilitation o After a disaster governments are very good at responding to the immediate need for rescue/relief/rehabilitation but often times neglect the long-term measures for disaster prevention and mitigation o As a result, the disaster cycle simply repeats itself with equally devastating disasters Hurricane Katrina o According to the main congressional report on Katrina, the levees were all built in the correct locations but were not built to withstand hurricanes of great magnitude o Levee failure occurred for two main reasons Simple overtopping of water rising above the levee wall Breeches/failures in the levee walls, which tended to occur at levee transitions where soil and foundation were weaker o Improvements of levee walls Overtopping erosion protection through provisions of rip-rap, concrete splash slabs, or paving of the ground surface at the inboard faces of the levee floodwalls La Conchita Landslides o In 1995 a slow moving landslide occurred in the town of La Conchita o No casualties but property damage o After this slide, debris from the foot of the new slope was removed and a restraining wall was built o The construction of this wall destabilized the slope o In 2005, following two weeks of heavy rain, a second landslide occurred, this time with high velocity killing 10 people