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Water’s Three States of Matter

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Presentation on theme: "Water’s Three States of Matter"— Presentation transcript:

1 Water’s Three States of Matter
Water’s Thermal Properties Water is solid, liquid, and gas at Earth’s surface. Water influences Earth’s heat budget. Water’s Three States of Matter

2 How much energy to sublimate?
Latent Heat of Vaporization = 600 calories / 1g Latent Heat of Condensation = 600 calories / 1g Latent Heat of Fusion= 80 calories / 1g How much energy to sublimate?

3 Surface Salinity Variation by Latitude

4 Temperature and Density Variation With Depth
Pycnocline – abrupt change of density with depth Thermocline – abrupt change of temperature with depth

5 CHAPTER 6 Air-Sea Interaction
The atmosphere and the ocean are coupled in many ways. Earth has seasons because of the tilt on its axis. There are three major wind belts in each hemisphere. The Coriolis effect influences atmosphere and ocean behavior. Oceanic climate patterns are related to solar energy distribution.

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7 Heat Gained and Lost © 2011 Pearson Education, Inc.

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9 Density Variations in the Atmosphere
Convection cell – rising and sinking air Warm air rises Less dense Cool air sinks More dense Moist air rises Dry air sinks © 2011 Pearson Education, Inc.

10 Movement of the Atmosphere
Air always flows from high to low pressure. Wind – moving air © 2011 Pearson Education, Inc.

11 Coriolis Force varies with latitude:
Figure 6.15: Except at the equator, a free-moving object heading either east or west (or any other direction) will appear from the earth to deviate from its path as the earth rotates beneath it. The deviation (Coriolis force) is greatest at the poles and decreases to zero at the equator.

12 Movements in the Air Example: a non-rotating Earth
Air rises at equator (low pressure) Air sinks at poles (high pressure) Air flows from high to low pressure One convection cell or circulation cell © 2011 Pearson Education, Inc.

13 Global Atmospheric Circulation
Circulation Cells – one in each hemisphere Hadley Cell: 0–30 degrees latitude Ferrel Cell: 30–60 degrees latitude Polar Cell: 60–90 degrees latitude © 2011 Pearson Education, Inc.

14 Global Atmospheric Circulation
High pressure zones – descending air Subtropical highs – 30 degrees latitude Polar highs –90 degrees latitude Clear skies Low pressure zones – rising air Equatorial low – equator Subpolar lows – 60 degrees latitude Overcast skies with lots of precipitation © 2011 Pearson Education, Inc.

15 Circulation Cells – one in each hemisphere
Polar Cell: 60–90 degrees latitude Ferrel Cell: 30–60 degrees latitude Hadley Cell: 0–30 degrees latitude

16 Winds Cyclonic flow Anticyclonic flow
Counterclockwise around a low in Northern Hemisphere Clockwise around a low in Southern Hemisphere Anticyclonic flow Clockwise around a low in Northern Hemisphere Counterclockwise around a low in Southern Hemisphere © 2011 Pearson Education, Inc.

17 Figure 6.18: Winds and related forces around areas of low and high pressure above the friction level in the Northern Hemisphere. Notice that the pressure gradient force (PGF) is in red, while the Coriolis force (CF) is in blue. Winds and related forces around areas of low and high pressure above the friction level in the Northern Hemisphere. Notice that the pressure gradient force (PGF) is in red, while the Coriolis force (CF) is in blue.

18 Fronts Fronts – boundaries between air masses
Warm front Cold front Storms typically develop at fronts. Jet Stream – may cause unusual weather by steering air masses. © 2011 Pearson Education, Inc.

19 CHAPTER 7 Ocean Circulation

20 Ekman Spiral Surface currents move at an angle to the wind.
The Ekman spiral describes speed and direction of seawater flow at different depths. Each successive layer moves increasingly to the right in the Northern Hemisphere Coriolis effect © 2011 Pearson Education, Inc.

21 Ekman Transport Average movement of seawater under influence of wind
90 degrees to right of wind in Northern hemisphere 90 degrees to left of wind in Southern hemisphere © 2011 Pearson Education, Inc.

22 Geostrophic Flow Ekman transport piles up water within subtropical gyres. Surface water flows downhill and to the right. Geostrophic flow – balance of Coriolis Effect and gravitational forces Ideal geostrophic flow Friction generates actual geostrophic flow © 2011 Pearson Education, Inc.

23 Coastal Upwelling Ekman transport moves surface seawater offshore.
Cool, nutrient-rich deep water comes up to replace displaced surface waters. Example: U.S. West Coast © 2011 Pearson Education, Inc.

24 Coastal Downwelling Ekman transport moves surface seawater toward shore. Water piles up, moves downward in water column Lack of marine life © 2011 Pearson Education, Inc.

25 Atmospheric-Ocean Connections in the Pacific Ocean
Walker Circulation Cell – normal conditions Air pressure across equatorial Pacific is higher in eastern Pacific Strong southeast trade winds Pacific warm pool on western side of ocean Thermocline deeper on western side Upwelling off the coast of Peru © 2011 Pearson Education, Inc.

26 Normal Conditions, Walker Circulation
© 2011 Pearson Education, Inc.

27 El Niño – Southern Oscillation (ENSO)
Walker Cell Circulation disrupted High pressure in eastern Pacific weakens Weaker trade winds Warm pool migrates eastward Thermocline deeper in eastern Pacific Downwelling Lower biological productivity Peruvian fishing suffers © 2011 Pearson Education, Inc.

28 ENSO Conditions in the Pacific Ocean
© 2011 Pearson Education, Inc.

29 La Niña – ENSO Cool Phase
Increased pressure difference across equatorial Pacific Stronger trade winds Stronger upwelling in eastern Pacific Shallower thermocline Cooler than normal seawater Higher biological productivity © 2011 Pearson Education, Inc.

30 La Niña Conditions © 2011 Pearson Education, Inc.

31 Occurrence of ENSO Events
El Niño warm phase about every 2–10 years Highly irregular Phases usually last 12–18 months 10,000-year sediment record of events ENSO may be part of Pacific Decadal Oscillation (PDO) Long-term natural climate cycle Lasts 20–30 years © 2011 Pearson Education, Inc.

32 Thermohaline Circulation
© 2011 Pearson Education, Inc.

33 The term thermohaline circulation (THC) refers to a part of the large-scale ocean circulation that is driven by global density gradients created by surface heat and freshwater fluxes. The adjective thermohaline derives from thermo- referring to temperature and -haline referring to salt content, factors which together determine the density of sea water. Wind-driven surface currents (such as the Gulf Stream) travel polewards from the equatorial Atlantic Ocean, cooling enroute, and eventually sinking at high latitudes (forming North Atlantic Deep Water). This dense water then flows into the ocean basins . While the bulk of it upwells in the Southern Ocean, the oldest waters (with a transit time of around 1600 years) upwell in the North Pacific. Extensive mixing therefore takes place between the ocean basins, reducing differences between them and making the Earth's oceans a global system. On their journey, the water masses transport both energy (in the form of heat) and matter (solids, dissolved substances and gases) around the globe. As such, the state of the circulation has a large impact on the climate of the Earth.

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