G131 HOME
INFORMATION
SCHEDULE
RESOURCES
EXERCISES
NOTES
Links to summaries of key issues for each topic
PREAMBLE
Introduction
History

PART I
Water Planet
Plate Tectonics
Sea Floor
Review 1
Physical Prop.
Chemistry
Ocean Stuct.

PART II
Atmosphere
Currents
Waves
Tides

PART III
Coasts/Beaches
Environ. for Life
Production
Plankton
Nekton
Benthos
Environ. Issues



VISUALS

Links to images employed in lectures on a topic-by-topic basis

TEXT
Link to chapter outlines at online learning center at McGraw Hill.
NOTES
Links to summaries of key issues for each topic

 
The Structure of the Oceans

Notes on Topic:

  • The notes represent summaries of key issues for each topic
  • They emphasize the terminology used to describe the various phenomena.

  •  1. Heating and Cooling the Earth's Surface:
    Learning Objectives: 
    • Understanding of the factors that control the Earth's heat budget 
    • Recognition of the role of the oceans in the distribution of heat on Earth
    Distribution of Solar Radiation: 
    • Solar constant (Without atmosphere heat received 2 cal cm-2 /min: . 
    • Greatest heat received (1.6 cal cm-2 /min) in equatorial regions
      • imprint of solar radiation more disperesed at high latitudes
    • Heat absorbed by atmosphere
      • decreases with increasing latitude as radiation more oblique.
    Heat Budget:
    • Heat gains and losses: 
    • Reflection of solar radiation:
      • 31% by atmosphere, 4% by Earth's surface
    • Adsorption of solar radiation:
      • 17.5% by atmosphere, 47.5% by Earth's surface. 
    • Reradiation
      • combined 65% is lost, 59.5% by atmosphere, 5.5% by Earth's surface
    • Transfer of heat from surface to atmosphere:
      • total 42%, 29.5% by evaporation, 12.5% by conduction
    • Heat gain in equatorial regions, most heat lost in polar regions. 
    • Sea surface temperature show strong latitudinal gradients.
    Annual Cycles of Solar Radiation, Heat Capacity of the Oceans: 
    • Seasonal changes in radiation and temperature
      • greatest change at mid and high latitudes. 
      • summer at high latitudes: long duration of low intensity radiation.
    • Annual temperature ranges:
      • variation controlled by heat capacity of oceans
      • oceans dominant role in southern hemisphere. 
      • range on land at high latitudes is greater than in oceans.
    2. Density Structure and Vertical Circulation:
    Learning Objectives:
    • Understanding controls on seawater density and its description
    • Recognition of the layered structure and movement of the ocean
    Surface Processes:
    • Temperature and salinity variations control density
      • As temperature increases, density decreases
      • As salinity increases (or pressure), density increases
      • less dense water at surface
    • Higher density water formed at polar latitudes sinks into deep ocean.
    Changes with Depth:
    • Three depth zones: 
      • surface (mixed layer to ~100m, 2%)
      • pycnocline (100 - 1000m, 18%)
      • deep ocean (>1000m, 80%). 
    • Pycnocline: zone of density change, 
    • Thermocline: depth zone where marked changes in temperature occur
    • Halocline: depth zone where marked changes in salinity occur 
    • Density structure:
      • increases with depth: stable
      • unstable where denser water overlies less dense water
        • overturn occurs. 
      • isopycnal: lines (depths) of equal density
      • isothermal: lines (depths) of equal temperature, 
      • isohaline: lines (depths) of equal salinity 
    Density-driven Circulation: 
    • Thermohaline circulation
      • convective exchange and vertical circulation; 
      • controlled by temperature and salinity
      • seasonal temperature changes create seasonal thermocline
        • affect surface density
        • can form sinking water masses, or freshwater lid.
    • Sigma-t (st): measure of seawater density
      • defined as (density - 1) x 1000. 
      • 1.02677 becomes 26.77 st.
    Movement of Water:
    • Upwelling: ascending water masses
    • Downwelling: sinking water masses
      • maintain continuity of flow, vertical movement (0.1 - 1.5m/day) 
      • Sinking waters may take 1000 years to reach great depths. 
    • Horizontal water movement:
      • convergence (meeting) and divergence (spreading out).
    Chemical Tracers:
    • Used to study water movement in the oceans
      • e.g. tritium, the radioactive isotope of H.


     
       
    Continue >>

    Indiana University
    Department of Geological Sciences, 
    1001 E. Tenth Street, Bloomington, IN 47405-1403
    Phone: (812) 855-5582  Last updated: 15 October 2000
    Comments: simon@indiana.edu
    Copyright 2000, The Trustees of Indiana University