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
Cold accretion
Unsorted materials
Very cold
This homogenous mass eventually becomes layered
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
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