Oceanography - Oce 1001 Chapt 6 Water _ Ocean Structure

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Chap 6 Water & Ocean Structure Physical Oceanography Water and Heat Sun is exclusive source of energy driving ocean and atmospheric currents.  The Sun radiates throughout the electromagnetic spectrum, but principle radiation is in visible part of the spectrum.  Visible light is strongly absorbed by seawater  – energy produced by random vibration of atoms or molecules.  Temperature – object’s response to an input or removal of heat.  Specific heat – heat required to raise the temperature of 1 g of substance by 1 °C. (calories / g)  Heat Infrared Energy clear water, only 10% reaches 25 m, only 0.5% reaches 100 m, .0025% reaches 200 m  essentially all energy gain in the oceans takes place in upper 10 -100 m of water  in Concept of Steady State  Averaged over the globe and over a year, the Earth loses as much energy as it gains.  Green house effect may be changing the steady state There is a net gain of energy at low latitudes and a net loss of energy at high latitudes.  This latitudinal difference is energy gain and loss drives both ocean and atmospheric circulation.  All energy exchange by the oceans occurs at the surface  This exchange of energy controls the temperature of ocean water masses  Density / volume (g / cm3)  Density depends on temperature and salinity  Ocean density ranges from 1.02 to 1.03 g/cc.  Density differences, together with winds, are the principal factors determining ocean currents.  Mass Freezing Water  Density curve (6.6) shows the relationship between the temperature or salinity of a substance and its density.  Water density decreases as the water freezes  Angle between water molecules expand from 105 ° to 109 °  Forms a crystalline lattice – less dense, hence ice float. Sensible heat loss – detectable decrease in heat, measured with a thermometer, before ice freezes  Latent [hidden] heat of fusion – amount of heat removed to form ice per g of water (80 calories)  This process of freezing and thawing moderates global temperature swings. Why?  Review the Concepts  Heat is transmitted in the ocean in which wave length?  Define density  The density of a parcel of seawater will be affected by which factors Evaporating Water  Latent heat of evaporation – amount of energy required to break hydrogen bonds cal / g at 20 °C  Why such a big difference between latent heat of evaporation and the latent heat of fusion?  585 Sea Water vs. Pure Water Solids dissolved lowers specific heat by 4% (heats faster)  Ions also interfere with the freezing point, the saltier the lower the freezing point  No solids, water requires 1 cal to heat up vs. 0.96 cal sea water.  No ions to interfere with the freezing point  Solar Energy Inputs the sun 'makes a direct hit' at equator, while the same sunlight is spread over a larger area at the poles.  This is just another way of showing that the equator is heated up more than the north or south poles of the Earth.  This uneven heating of our round globe causes the air at the equator to rise, cool, and then wring out its moisture as rain.   The equator, then, is a zone of low pressure systems and lots of rainfall.  This zone extends from roughly 5°N to 5°S of the equator.  The air doesn't keep rising forever.  It eventually reaches an altitude where it is the same temperature (and density) as the surrounding air.  It then spreads out laterally, both in a north direction, and in a south direction.  As it moves poleward (either north or south from the equator), the air continues to cool, and finally, sinks. Where it sinks, the pressure is high.  Heat budget is balance (p.163, f. 7.10) Density Structure of the Ocean Winds are the primary driving force of the surface circulation, which is also called winddriven circulation,  density differences drive the deep, or vertical, circulation of the oceans.  The density of seawater is controlled by temperature and salinity, so the deep circulation is also called the thermohaline circulation.  Review the Concepts  Contrast sea water and fresh water  What causes the seasonal changes?  Why the poles are cold? Temperature differences as small as a few hundredths of a degree and salinity differences of a few parts  in a hundred thousand can be important.  Both temperature and salinity are conservative properties of seawater, that is, there are determined by processes occurring at the surface.  Salinity  Salinity refers to the weight fraction of dissolved solids in water.  Average salinity of seawater is about 35‰ (‰ and ppt mean “parts per thousand).  Principal processes that change salinity are:  1. dilution (by rainwater and river water)  2. Evaporation freezing (& thawing) of sea ice  Salinity changes occur only at the surface of the ocean  Because temperature and salinity change only at the surface density changes occur only at surface  Water masses can be identified by their temperature-salinity characteristics.  Density, together with winds, govern ocean currents Ocean Structure  Upper 100-500 m to have uniform temperature and salinity because of mixing by waves.(6.13)  Below this, to a depth of ~1000 m, Temp., Salinity, and density change ( Thermocline, Halocline, Pycnocline) (6.12)  In deep water, temperature, salinity and density are relatively uniform  This structure varies latitudinally. At mid-latitudes, it also varies seasonally: upper mixed layer will deepen in summer;  thermocline might largely disappear in winter Sound  Is a form of energy transmitted by rapid pressure changes in an elastic medium.  Intensity decreases as it travels through seawater until eventually is absorbed and converted into heat  Speed is 1,500 m / s, almost five time the speed in air Echolocation Marine mammals use sound rather than light to “see” in the ocean  Echolocation –use of reflected sound to detect environmental objects  MM use echolocation to detect prey and avoid obstacles  Speed of sound increases as temperature and pressure increases (6.21)  Travels faster at the surface than in deeper, cooler water.  Minimum speed at 600 – 1,200 m  Below this depth the pressure offsets the temperature and speed increases again  SOFAR Layer Sound Fixing and Ranging  Transmission of sound in this minimumvelocity layer is very efficient because refraction tends to cause sound energy to remain within the layer (6.20)  Loud sounds made at this depth can be heard for thousands of kilometers  Sound generated in the India Ocean was hear as far a way as the Oregon Coast (Box 6.1)  SONAR  Sound Navigation and Ranging  Active SONAR – projection of short pulses of high frequency sound to search for objects in the ocean.  Operator can tell direction, size, heading and even the composition by analyzing the composition of the returned ping Sonar – towed behind a vessel (6.22)  Used for geological and archeological studies, and the location of downed ships and airplanes  Side-Scan Review the Concepts What kind of temperature does most of the world ocean has?  What is characteristic about the ocean's deep sound channel (sofar layer) ?  What is called a zone in which the ocean's salinity increases rapidly with increasing depth?  Which zone does the most pronounced or marked all year around thermoclines exist? 

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