Lectures 1-12

Lecture 1: Introduction

  • The ocean interacts with chemistry, physics, society, geology, and biology

  • We study the ocean because of some major problems in the world

    • Climate change: coral dies

    • Acidification: ocean pH lowers

    • Deoxygenation: less or no oxygen in the water

    • Pollution: garbage accumulates in the water

  • The ocean was mainly used for seaborne travel/transport and trade early

    • It became used for bad purposes

      • Extract marine resources

      • Military purposes

    • Scientific Revolution increased exploration

  • Studying the ocean became the government’s responsibility

    • HMS Beagle (Darwin)

    • HMS Challenger (main one)

  • New technology came about to study the ocean

    • Ocean floor topography: mountain ranges found

    • Hydrothermal vents: heated water that dissolves minerals

    • Plate tectonics: continental drift

    • Microbial life/genetics: horizontal gene transfer

  • The ocean as a tool

    • Exclusives economic zones: countries have control of parts of the ocean off their coasts

    • Fisheries

    • Mining and drilling

    • Military 

    • Transportation

    • Trade: the ocean is how most materials are moved (economically best)

  • Limitations to studying the ocean

    • Biological issues: can’t breathe underwater

    • Deep ocean: pressure is very high

    • Water interacts with electromagnetic radiation differently: reflects waves

    • Seawater is corrosive

    • Dynamic surface: waves move

    • It is expensive

  • Bathymetry: seafloor topography can be studied using:

    • Sounders

    • Echo sounders

    • Satellites

  • Seafloor sediments can be studied using:

    • Grab samplers and box corers

    • Gravity and piston corers

    • Drilling ships

    • Seismic/magnetic/gravity surveys

    • Dredges

  • Ocean physics and chemistry can be studied using:

    • Water collection

    • Reversing thermometer

    • CTD: collects water samples and measures multiple things including temperature

    • Drifters/drogues/floats: measures ocean currents

    • Mechanical current meters

    • Acoustic/Doppler current meters: uses Doppler effect

  • Organisms can be studied using:

    • Trawl/tow nets, traps, and water samples

    • Visual surveys

    • CTD: accidentally capture an organism

  • Technological advances in fieldwork

    • Scuba and habitats

    • Piloted submersibles

    • ROVs: controlled vehicles

    • AUVs: automated vehicles

      • Argo network

    • Satellites

    • Computers and modeling

  • Measuring oceanographic data

    • Graphs: can be useful but also deceiving

    • Contour plots

    • Maps

  • Units

    • SI units (ex: m)

    • Derived units (ex: m^3)

    • Exceptions:

      • Sv: volumetric flow rate (1 Sv = 100 m^3/s)

      • mbar: pressure (atmosphere; 1 mbar = 100 Pa)

      • kt: speed (1 kt = ~.51 m/s)


Lecture 2: Plate Tectonics and Ocean Evolution

  • We know the earth is layered because of seismic waves/earthquakes

  • Body waves: pass through the interior of the earth 

    • P-waves (primary): compressional seismic waves moving through the earth

      • Extremely fast

      • Like a slinky

      • Not destructive

      • Travels through solids and liquids

      • First to be recorded on seismographs

      • Moho discontinuity: changes in P-wave velocity and angles due to boundary between the crust and mantle

    • S-waves (secondary): seismic shear waves passing through the earth

      • Moderately fast

      • Goes up and down

      • Not destructive

      • Travels through solids

        • This is how we identify that the outer core of the earth is liquid, since the S-waves stop traveling in the “Shadow Zone”

    • The velocity of waves varies and depends on the sediment through which they are passing

      • Can create curvature of waves

  • Surface waves: travel along the earth’s surface

    • L-waves and R-waves

  • How the earth became layered: density

    • The density of each layer of the earth increases the closer we move to the core

    • Density and temperature have an inverse relationship

      • Warmer = less density, colder = more density

    • Liquids are attempting to find areas of equal density as itself

      • Density below is higher, density above is lower

    • Gravitational separation works similar to density

      • Heavier elements go inside

      • Lighter elements go outside

    • Earth age = 4.6 billion years

    • The formation of the earth

  1. Cold accretion

  • Unsorted materials

  • Very cold

  • This homogenous mass eventually becomes layered

  1. Solar winds

  • The diameter of the earth was 100x larger than today

  • The mass of the earth was 500x greater than today

  • Gravity compacted the earth

  • The solar winds boiled away lighter elements

  • Heat arises from collisions 

  • Radioactive decay melted much of the earth

  1. Add heat

  • The earth separates based on density of materials

  • The earth began to heat up due to:

    • Gravitational contraction 

    • Radioactive decay of K-40 and U-235 (5x more radioactive heat production than today since these elements are becoming increasingly stable) 

      • Nuclear fission creates energy, which creates heat

    • Large meteorite impacts 

      • Energy of motion is converted into heat

  • Differentiation: materials become molten due to high temperatures

    • Molten iron and nickel sink toward the center to create the core

    • The surface crust becomes composed of lighter materials (K, Na, Si)

    • The mantle becomes Mg

    • Differentiation led to the formation of a magnetic field, ocean and atmosphere, and different layers

  • Outer layers

    • Lithosphere: all the crust and part of the upper mantle (rigid)

      • Thickness varies

      • Plates float on the asthenosphere

      • The interior flow is critical for the movement of plates

      • Isostasy: as density increases, height above water/other material floating in will decrease not on exam

    • Asthenosphere: part of the mantle that can flow (not liquid)

    • Continental crust: basement rocks are very old

      • Cratons: shields and platforms

      • 31% is submerged

      • Rich in aluminum silicates

    • Oceanic crust

      • Younger and thinner than continental crust

      • Rich in magnesium silicates

      • Has 3 layers: sediments, basalt/dolerite, and gabbro

    • Crust: outer shell

      • Different chemistry than the mantle

      • Consists of the oceanic and continental crust

  • The earth began cooling around 4.4 Ga and is still cooling

    • Convection overturn: internal heat from the interior is transferred to the surface by convection

      • Convection dissipates the heat rapidly and the earth cooled quickly


Lecture 3: Plate Tectonics and Ocean Evolution

  • The earth has plates in the lithosphere that can move as if they are puzzle pieces

  • Alfred Wegener: German meteorologist/Arctic climate scientist who came up with the theory of continental drift

    • Observations he made:

      • Fit of the continents: “Pangaea” was a single land mass

      • Paleoclimate data: certain environments were different latitudes from the equator in the past

        • glacial striations in tropical climates

        • Coal is found where swamps once were

        • Coral reef existence

      • Distribution of fossils: same species fossils are found on distant continents

      • Matching geologic units: rock layers are the same on different continents

        • Mountain ranges are created at the same time, but split onto different continents

    • Theory was highly criticized as plate tectonics were not discovered yet

      • Other theory proposed: land bridges eroded away

  • Observations by other scientists

  • Paleomagnetism

  • Seafloor spreading

  • Volcano/earthquake distribution

  • World War II: sonar was used to map the ocean floor; bathymetry was used to measure water depth

    • Deep sea trenches and ocean ridges were discovered

  • Seafloor anatomy: along continental margins there are shelfs, slopes, and rises

  • Other observations

    • Ocean sediment is thinnest at the mid ocean ridges and thickest at margins

    • The oldest ocean crust is younger than the age of the earth

    • Ocean crust (basalt) has a different chemistry than continental crust (granite)

    • More heat rises beneath the mid ocean ridges than elsewhere, causing uneven heat distribution

    • Seafloor spreading: magma rises and pushes mid ocean ridges apart

      • Testing this theory

        • Earth’s magnetic field is strongest near the poles

          • Geodynamo theory: the magnetic field is generated by the convecting, liquid metal region of the outer core

          • Geomagnetism: earth’s magnetic field polarity reverses poles periodically

        • Paleomagnetism: when magma cools, iron bearing minerals align with earth’s magnetic field

          • Basalt crystalizes and materials align with the magnetic field

        • Magnetometer: measures magnetism, which is the direction, strength, or relative change of a magnetic field at a particular location

          • Ocean crust should record earth’s magnetic reversals

      • Harry Hess proposed idea of seafloor spreading

        • Continents and ocean crust move together

        • Deep sea drilling and age of crust show how the seafloor could have spread

          • No sediment found older than 180 million years found during a deep sea drilling project

          • Thickness of sediment decreases towards ocean ridges

  • Plate tectonic theory: plate movement causes continents to move and interactions at boundaries result in earthquakes, volcanoes, and mountain building

    • Ring of fire: substantial seismic activity occurs around the Pacific plate

    • Earth’s surface (lithosphere) consists of 20 plates and they move relative to each other

      • They float on the soft asthenosphere

    • Plates move around partly due to convection, but it is most likely more complex than that

    • Ridge push force: force that drives plates away from a mid ocean ridge

    • Slab pull force: force down-going plates/slabs apply to oceanic lithosphere at a convergent margin


Lecture 4: Plate Tectonics and Ocean Evolution

  • Plate boundaries: where the action occurs

    • Divergent: plates move apart

      • Found in oceans and mid-ocean ridges

        • Atlantic Mid-Ocean Ridge

      • New crust is formed

      • Earthquakes occur and there are small volcanic eruptions

      • Seafloor spreading with oceanic ridges: seafloor is elevated, which forms oceanic ridges

        • Along the axis of some ridge segments is a deep rift valley

      • Continental rifting: divergent plate boundaries that develop within a continent

    • Convergent: plates move together

      • More dense plate sinks under less dense plate and one plate is consumed

      • Earthquakes occur and there are large volcanic eruptions

      • Types of collisions

        • Oceanic-continental: forms continental volcanic arc and felsic rocks

          • Chile is extremely earthquake and tsunami prone

        • Oceanic-oceanic: forms oceanic island arc and felsic rocks

          • The Aleutian island arc has many volcanoes

        • Continental-continental: forms mountain range and metamorphic rocks

          • The Himalayan mountains were created by this

    • Transform: plates move along each other

      • No new crust forms

      • No plate is consumed

      • No volcanic eruptions occur but earthquakes do

      • The San Andreas Fault doesn’t form any rock

      • Transform fault boundary: two plates grind against each other without the production or destruction of lithosphere

        • Fracture zones: active transform faults and their inactive extensions into the plate interior

      • Seafloor spreading can cause plates to run into each other

  • Continental margins

    • Passive: not on a plate boundary

      • Wide shelf

      • Shallow slope

      • No earthquakes

      • No volcanoes

    • Active: on a plate boundary

      • Narrow shelf: subduction of crust causes no buildup of crust

      • Steep slope

      • Earthquakes

      • Volcanoes

  • Hot spot: location at the base of the lithosphere/top of a mantle plume where temperatures can cause melting

    • Hot spot under oceanic crust stays in the same place with the lithosphere moves across the hot spot

      • Hawaii was created from this, and plate movement directions can be determined by looking at the island chain

    • Yellowstone hot spot is in continental crust

  • Atolls: forms around a hotspot and the island moves off the hotspot and begins eroding away; coral reef forms around island

    • Lagoon built off coral reef is left

  • Triple junction: meeting point between 3 plates

  • Ocean basins are formed from continental rifting

    • Rift valley will hold water

  • Water exists between 273-373 K

  • Meteorites can be used for testing in place of the mantle to see how much water is in the mantle

  • Cometary ice hypothesis: ocean water is theorized to have come from comets instead of inside the earth

  • Hydrogen in ocean water is more like meteors than comets

  • Water sources: outgassing of the earth (80-90%) and cometary ice (10-20%)


Lecture 5 & 6: Properties of Water and Seawater

  • Water is vital for:

    • Life

    • Climate regulation

    • Transport (biogeochemistry)

      • Water cycle: biogeochemical cycle

    • Economies, industries, and cultures

  • Oceans first formed during Archean Eon

  • Amount of water: 2.0*10^9 km^3

  • Where the water is: 96.5% in ocean, 3.5% is freshwater

    • In freshwater:

      • Ice caps/glaciers: 1.78%

      • Surface waters: .013%

      • Air/soil: .002%

      • Groundwater: 1.69%

  • Amount of potable/drinkable water: comparable to a drop of water in a 5 gallon bucket

  • Water makes earth unique as other planets do not have liquid, solid, and gas water all at once on the surface

  • Bonds in water

    • Van der Waals force: weakest

    • Hydrogen bond: electrostatic, hydrogen (+), donor (-), acceptor (-), important structural role

    • Ionic bond: electrostatic polarity, soluble in water, great electric conductor in solution

    • Covalent bond: strongest, electron sharing

  • Unique properties of water

    • Heat capacity: amount of heat needed to change an object’s temperature; high for water

    • Latent heat: what you need for a phase change

      • Sensible heat: what you feel

      • Types of latent heat: fusion and vaporization

        • Vaporization is higher than that of any other substance

        • High amount of energy needed for a phase change

    • Thermal expansion: solid is normally denser than liquid which is denser than gas, but this is not true for water

      • Water has its max density at 4 degrees C

      • Seawater freezes below 0 degrees C

        • Temperature and salinity affect at what point ocean water freezes

    • Solvent: water is a universal solvent

      • Solute dissolves in solvent

      • Solution is the combination of solute and solvent

      • Helps with extracting minerals and having chemical reactions and biogeochemical cycles

        • Reservoirs hold water naturally and residence time is how long the water stays there

        • Biogeochemical cycle examples: water cycle, carbon cycle, marine nitrogen cycle

      • Major dissolved elements in ocean water (constituents): mainly chlorine and sodium (salt)

        • Created from erosion

        • Also calcium: makes parts of marine lifes’ habitats

        • [ ] = concentration

        • Precipitation/evaporation can remove these constituents from the ocean

        • Salinity does not vary drastically

      • Minor constituents: mainly bromine and carbon

        • Precipitation is not a main way to take them from the ocean

        • Short residence times due to variability

      • All constituents: 99.6% of dissolved solids

      • Trace elements: .4% of dissolved solids

        • Lots of variability

        • Mainly zinc

      • Radionuclides: natural and anthropogenic isotopes

        • Helps measure ocean circulation and food webs

      • Organic compounds: wide array exists but less than 1% have been identified

        • Can be natural or synthetic

        • Some are essential and some are highly toxic

        • Helpful to bacteria and archaea

      • Dissolved gases: move between the atmosphere and the ocean

        • Measured by saturation solubility and their concentration in seawater

        • Gases are more soluble in colder temperatures

        • Air-sea interactions drive the movement of gases in and out of solutions

          • Photosynthesis and respiration help

        • Ocean is a major carbon dioxide sink (similar to a reservoir)

          • Critical for pH buffering

    • Surface tension: molecules pulled together by van der Waals force

      • Hydrogen bonds make this possible

      • Distance between molecules is shorter in liquids than air

  • Electromagnetic radiation and water interactions

    • Limited transmission of wavelengths

    • Infrared and UV wavelengths are absorbed rapidly

    • On the visible spectrum, red is the shallowest and blue/green is the deepest

      • Depends on what is in the water

  • Sound in the ocean: dependent on salinity, temperature, and pressure

    • 4 times faster in water than in air

    • Acoustic thermometry: precisely measures temperature

      • Heard Island experiment used this

    • The bloop: loudest sound underwater

    • Krakatoa eruption: loudest sound above water


Lecture 7: Ocean-Atmosphere Interactions

  • Ocean drives climate/weather

    • Affects temperature distribution, wind/circulation, precipitation, and storms

  • Layers of the atmosphere (highest to lowest)

    • Exosphere

    • Thermosphere

    • Mesosphere

    • Stratosphere

    • Troposphere

  • Layers of the atmosphere

    • There are pauses between the layers

    • They have differences in density which varies due to pressure, temperature, and water vapor

    • Ozone layer blocks UV radiation, but hole is problematic

    • Ionosphere, homosphere, heterosphere

    • Planetary boundary layer

  • Composition of the atmosphere

    • Early atmosphere: H/H- compounds

    • Prebiotic atmosphere: N2, CO2, and inert gases

    • Biotic atmosphere: mainly N2 and O2 with inert gases

    • Composition of gases vary through time

  • Water vapor: varies across temperature

    • Temperature increases concentration of water vapor and decreases density

    • Clausius-Clapeyron relationship increases temperature and decreases concentration of water vapor

    • When air is decreased and rises, pressure decreases

    • Transferring heat uses water vapor (hurricanes)


Lecture 8: Ocean-Atmosphere Interactions

  • Water budget: the input of water into a reservoir and output of water that is regulated

  • Heat budget: the balance between incoming and outgoing radiation

    • Shortwaves are incoming and longwaves are outgoing

      • If they are not equal, water can be gained and temperatures drop, or water can be lost and temperatures rise

        • We are currently in a period of warming of the earth

    • Heat is transferred by conduction (sensible heat), vaporization (latent heat), and radiation

  • There is a relationship between latitude and radiation

    • Insolation becomes diffuse as the sun’s rays do not hit the earth flat at higher latitudes, causing the concentration of the ray to be smaller per square meter

    • There is an equator and pole difference between absorption rate (large) and radiation rate (small)

    • Milankovitch cycles over a long period of time

      • The changes in earth’s orbit; long term climate change

  • Heat is transferred to the poles through ocean currents and atmospheric circulation

    • Ocean currents take warmer temperatures to the poles, and the earth’s atmospheric circulation is set up in a 3-cell model

      • Cells: polar, mid-latitude, and hadley

  • Coriolis force and effect: force on an object due to earth’s rotation; dependent on latitude and direction is dependent on hemisphere

  • If the planet was not rotating, temperature and pressure would drive single-cell circulation

  • Intertropical convergence zone: a band of storms (tropical cyclones) that migrates seasonally

  • The earth’s axis tilt leads to seasonal variability

    • Landmass distribution complicates this

    • Lag in the timing of the max and min of temperatures in the ocean and land

      • Land heats up before the ocean

    • Water properties influence the seasons

    • A monsoon is a seasonal reversal of winds driven by pressure changes


Lecture 8: Ocean-Atmosphere Interactions

  • Surface salinity: amount of salt in the ocean

    • Tends to be low around the equator

    • Controlled by evaporation/precipitation rates, runoff (freshwater input from rivers and glaciers), and upwelling/downwelling

      • Adding water (precipitation) decreases salinity and taking water (evaporation) increases salinity

  • Dissolved salts are staying in the solution

  • Runoff: freshwater input from land from rivers/estuaries

  • Upwelling: driven by winds; Ekman transport/spiral

    • Salinity increases with depth

  • Salinity is typically highest in marginal seas

    • Mediterranean Sea: ~38% surface salinity; 100 year residence time

      • Sills (pieces of land that come up in water) block water moving around; there could be more exchange of water between bodies of water without them

      • Messinian salinity crisis: drying of the Mediterranean Sea

        • Millions of years ago

        • Sea level drop and evaporite formation (salt deposits)

        • Zanclean floods: flooding from the Strait of Gibraltar of 10 or more meters per day

  • El Niño (ocean) Southern Oscillation (atmosphere): affects ocean and atmosphere conditions

    • Teleconnection: has a widespread effect on climate

    • Southern Oscillation: pressure difference between Darwin and Tahiti

    • Warm phase/high sea surface temperatures

      • La Niña: cold phase/low sea surface temperatures

    • Winds weaken to allow for warm water to move east

      • La Niña: winds strengthen

    • Thermocline: a layer in the ocean where the temperature rapidly changes with depth

      • El Niño: farther from the surface; warm water layer is prominent

      • La Niña: closer to the surface; cold water layer is prominent

    • Internal climate variability: influences the climate system, but not influenced by the climate system

      • The sun influences our climate, but we do not influence the sun

    • Influences tornadoes and hurricanes


Lecture 9: Ocean-Atmosphere Interactions

  • Oceans follow latitudinal temperature gradient to determine their climate zones

    • More complicated on land because more climate zones exist on land, unlike on the ocean

  • Seasonal temperature lags: there are differences in thermal properties between water, air, and land, even among different places at the same latitude

    • Reason for hurricane season peaking in September

  • Island and mountain effect: air is forced to rise by topographic highs

    • Produces a distinct gradient in precipitation

  • Pressure gradient: drives wind

    • High pressure: cloud free, sunny, crisp weather

      • Diverges at the water’s surface, converges aloft

      • Rotates counterclockwise/right in the southern hemisphere

    • Low pressure: unstable, precipitation, stormy, humid weather

      • Converges at the water’s surface, diverges aloft

      • Rotates clockwise/left in the southern hemisphere

  • Tropical cyclones: not around the equator because the coriolis force does not exist there (warm core)

    • Extratropical cyclone: forms via cyclogenesis and creates a wide range of weather conditions (cold core)

      • Warm/cold fronts are separations of air masses along frontal boundaries

        • Stationary fronts move parallel along each other and do not collide

        • Causes a wave to form around the boundary, and air begins to circulate

          • Low pressure forms as the circulation increases; this is amplified over water

          • Occluded front: sectors form and the cold front catches up with the warm front

            • Eventually the system runs out of energy and dissipates

    • Nor’easters: form over warm waters

      • Winds come from the northeast

      • Type A: forms in the Gulf of Mexico/North Atlantic Bight

      • Type B: forms in the Midwest and catches onto the Gulf Stream

  • Land and sea breezes: thermal differences between the land and sea

    • Land heats up to max temperature first during the day, and the ocean is typically warmer than land at night

    • Essential for reducing temperature variability

  • Coastal fog: coastal upwelling causes cool waters to be nearshore and warm waters to be offshore

    • Moisture is transported via sea breezes, then it condenses and creates fog


Lecture 10: Ocean Circulation

  • Currents: important for movement of water masses, heat, chemical constituents, sediment, and organisms

    • Heat is transported from the tropics to the poles

    • Drives convection

  • Water can be moved by wind and density (temperature, salinity, or pressure gradient)

  • Wind currents: winds move across the ocean surface

    • Friction and kinetic energy causes movement

    • Current velocity is substantially less than wind velocity because water is more viscous than air

    • Energy is transferred downward (max depth is 100-200 m)

    • Currents continue after wind stops due to momentum and the sloping sea surface

      • Convergence, divergence, and the horizontal pressure gradient creates the slope

    • Direction and speed are controlled by friction, the horizontal pressure gradient, the coriolis effect, and coasts

      • Competing components balance currents using the coriolis force

        • Geostrophic current: the balance between the pressure gradient force and coriolis force drives what direction the geostrophic current moves

  • Energy is moving down between layers of water

    • As energy is moving down, each layer is being pushed or pulled, and energy is being lost

      • Friction is created between layers

      • Velocity decreases as energy hits each new layer as it moves down

  • Ekman spiral: the coriolis force deflects water; deflection continues with depth

    • Max depth: 100-200 m

    • Deflection stops below the wind-driven layer

    • Needed for a full Ekman spiral: uniform density, depth, and constant wind for 1+ days

    • Net water transport includes the entire spiral

    • Pycnocline: vertical density gradient

      • Can be a thermocline, halocline, or both

      • Uniform density is needed for a full Ekman spiral

        • Upper layer needs to be well mixed

      • Water masses don/t impart any friction on each other

      • Controls Ekman spiral’s depth

    • Thermocline: vertical temperature gradient

    • Halocline: vertical salinity gradient

    • Pycnocline, thermocline, and haloclines differ spatially and seasonally

    • Ekman transport: movement of water 90 degrees to the right of the wind in the northern hemisphere (left of the wind in the southern hemisphere)

      • On the sea surface, convergence is seen in the northern hemisphere and divergence is seen in the southern hemisphere

  • Open ocean surface currents: Ekman transport on a global scale

    • Atmospheric circulation affects the direction of surface currents

    • Pressure gradients in the atmosphere and the ocean form from Ekman transport and coriolis deflection

    • Gyres represent the average wind energy input

      • Subtropical gyres form clockwise in the northern hemisphere and counterclockwise in the southern hemisphere

      • Polar gyres are less established and rotate in the opposite direction

        • Does not occur in the southern hemisphere

    • Eastern and western boundary currents highlight additional factors that come into play outside of gyres

      • Eastern: in the eastern part of the ocean

        • Nutrient poor and upwelling does not often occur

      • Western: in the western part of the ocean

        • Narrower and faster than eastern currents

        • Upwelling occurs and phytoplankton blooms can occur

      • Coriolis and continents influence them

      • Eastern and western boundary currents have differences in depth, width, volume, velocity, boundaries, temperatures, etc.

      • Westward intensification

    • Equatorial surface currents: flow east to west/west to east without being deflected since coriolis is at its minimum at the equator and maximum at the poles

      • Displacement of ITCZ influences Ekman transport and shifts the surface sea slope

      • A pressure gradient also develops

    • Polar surface currents: more variability in polar gyres than subtropical gyres

      • Winds are more variable and there is complex basin geometry

      • They differ between the hemispheres because of continent concentration and connections between oceans

        • Southern hemisphere: Antarctic coastal current and antarctic circumpolar current

  • Upwelling and downwelling: wind moving water

    • Types: open ocean (wind) and coastal (wind and coastlines)

    • Influences pycnocline depth

    • Biologically and ecologically important for nutrient transport for organisms

      • Increases in photosynthesis and biomass


Lecture 11: Ocean Circulation

  • Upwelling increases primary productivity, causing nutrients to be brought to the photic zone

    • Concentration of nutrients goes up, phytoplankton and zooplankton biomass increases, and catch yield goes up

    • Seasonal variability plays a role in this as summer conditions are more stable than winter conditions

    • Upwelling of nutrients allows for growth

      • Need carbon dioxide, oxygen, water, and sunlight for photosynthesis in the ocean, similar to on land

        • Trace elements promote growth

    • Chlorophyll is more concentrated around the equator and coasts

      • El Niño has less primary productivity compared to La Niña based off of chlorophyll concentration

  • Coastal currents are not a part of larger gyre circulation due to pressure gradients in the atmosphere

    • Size varies due to differences in continental shelf width

      • West coast: shelf is narrower

      • East coast: shelf is wider

    • These are also influenced by coastal winds/storms, tides, freshwater input/rivers, bathymetry, and coastal geomorphology

    • Seasonal changes in winds can cause seasonal changes in coastal currents

      • Winter: the prevailing wind direction is inward toward the coast

      • Summer: the prevailing wind direction is downward parallel to the coast

    • Coastal currents are strongest due to changes in bathymetry and coastal geomorphology

  • Eddies: hurricanes, tornadoes, midlatitude cyclones, and whirlpools

    • They have cultural significance

    • More wind velocity is needed to create an ocean eddie than an atmospheric eddie

    • Atmospheric eddies and ocean eddies differ in spatial and temporal scales

      • Ocean: takes longer to form and more strength of winds

      • Atmospheric: takes shorter time to form and are not as strong as ocean eddies

    • Eddies are a transport mechanism along ocean fronts (boundaries between differ water masses)

      • Meanders in currents: there is a boundary dividing cold and warm waters -> currents form in each separately -> warm eddies break off into cold waters and cold eddies break off into warm waters

        • This is due to momentum

        • Warm and cold core eddies exist due to rotation being different depending on if they are warm or cold and divergence

          • Warm core: downwelling

          • Cold core: upwelling

      • Transport between and within basins: heat, nutrients, dissolved materials, and marine organisms are transported

    • Langmuir circulation: streaks of white on the water

      • Wind driven: width and depth are a function of wind speed

      • Zones of convergence and divergence


Lecture 12: Ocean Circulation

  • Thermohaline circulation: driven by density

    • Density is controlled by temperature and salinity

      • Density and temperature have an inverse relationship

      • Density and salinity have a direct relationship

    • Water moves along a density gradient until it has reached a point of equilibrium

  • Pycnocline: made of the thermocline and halocline

    • Mixed layer that has seasonal patterns

    • Summer thermocline is the largest, winter thermocline does not exist

  • Temperature decreases with depth and warmer waters are deeper with higher latitudes (insulation)

  • Bottom water formation: when isotherms restrict/cut off warm water areas at the surface from cold water areas

  • Temperature distribution at surface waters is mostly uniform, but salinity distribution at surface waters is not

    • Temperature ranges are large whereas salinity ranges are not

  • Water from different sources helps create different water masses

    • Ex: Mediterranean Sea and Atlantic Ocean: Mediterranean salinity and temperature > Atlantic salinity and temperature, and the Mediterranean is denser

    • Density can allow for tracking of water masses

  • Water masses in the Atlantic: when convergence occurs, pressure goes up and water wants to sink, and new underwater masses are created

    • Density differences hinder vertical mixing (water masses stay separate)

      • Can be offset by currents, internal waves, and tides, but not significantly

    • Horizontal flow requires less energy opposed to vertical flow

      • Water masses can spread out

  • Bottom water formation: changes in density causing water masses to move vertically on a large scale

    • Water density is increased by lowering temperature and rising salinity

    • Only occurs at specific locations: North Atlantic and Antarctic

    • Meridional overturning circulation: the return flow of water that once was warm, began sinking and got cold, then returned to its original place

    • Mixing can occur due to turbulence from currents, internal waves, and tides

    • Bottom water formation and meridional overturning circulation are important in the climate system as oceans are major sinks for carbon dioxide

      • These processes allow for dissolved gases like oxygen to get to the deep ocean

        • Another source of oxygen in the deep ocean is dark oxygen

      • They are essential for transport in the global climate system which takes around 1000 years to complete

        • New water is created at deep water formation sits

        • Oldest water is located in the North Pacific

        • Important for heat transport

    • Atlantic meridional overturning circulation has weakened and is slowing

      • This is a response to warming and meltwater

      • Widespread effects are seen through positive/negative feedback

        • Positive: allows a cycle to continue; negative: cuts off a cycle

        • Circulation gets stronger/weaker at one point, so all circulation must get stronger/weaker

          • Explained by paleoclimatology and paleoceanography

  • Last glacial maximum: late Pleistocene epoch

    • Ice sheets were at largest extent with dry conditions and lowering sea levels

    • AMOC was weaker and more variable

  • Late glacial interstadial: warm period in between glacial periods

    • Changing circulation and glaciovolcanism

    • Glacial retreat causes meltwater pulses

    • People expand across land

  • Younger dryas: glacial outburst flood leading to rapid cooling in Europe

    • Massive inflow of freshwater in the Atlantic ocean

    • Changes differ between regions

      • Southeast US: warmer and wetter

      • Appalachian Mountain boreal forest: expansion

      • East Asia: increased aridity

    • Named after mountain avens

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