Advanced Oceanography Ocean Circulation - Chapter 1 A Review Circulation in both the oceans and the atmosphere is driven by energy from the Sun and modified.

Slides:



Advertisements
Similar presentations
Chapter 10 Wind: Global Systems.
Advertisements

The General Circulation of the Atmosphere
Earth’s Climate System Air and Ocean Circulation
Chapter 4 Atmospheric Circulation. Earth Regions near the equator receive light at 90 o High latitudes receive light at low angles.
Chapter 1 Introduction Fig.1-1 The spiral eddies in the central Mediterranean Sea were photographed from the Space Shuttle Challenger. The waters of the.
Winds and Ocean Currents. Latent Heat Transport 580 cal/g Surface wind Surface wind.
Global Wind Patterns and Weather & Weather Basic
Circulation in the atmosphere
How Does Air Move Around the Globe?
Wind.
General Circulation and Climate Zones Martin Visbeck DEES, Lamont-Doherty Earth Observatory
Thermohaline Circulation
The Coriolis Effect and Weather
Atmosphere 78% nitrogen, 21% oxygen. Water Vapor up to 4% by volume leaves atmosphere as dew, rain or snow.
Atmosphere 78% nitrogen, 21% oxygen. Water Vapor up to 4% by volume leaves atmosphere as dew, rain or snow.
Atmospheric Pressure and Wind. Atmospheric pressure: –force exerted by a column of air per unit area –Normal atmospheric pressure at sea level = 1013.
Winds
Winds.   at home  
More Climatic Interactions
General Atmospheric Circulation
Unit 2: Climate Winds and Climate
Chapter 21 Section 1 Review Page 524
ATMOSPHERE Air Circulation
Weather Water Cycle: the continuous movement of water between the atmosphere, the land, and the oceans Evaporation occurs when solar energy heats water.
Physical Science Lecture 154 Instructor: John H. Hamilton.
Basic Meteorology Concepts. Spheres of the Earth.
Movement of Air in Earth’s Atmosphere. What is wind? The movement of air from an area of higher pressure to an area of lower pressure. The movement of.
Global Wind Patterns.
Heat Energy Transfer SNC2D.
Ocean and Atmosphere. Earth’s Heat Budget and Atmospheric Circulation Atmospheric properties Earth’s Energy Budget Vertical Atmospheric Circulation Surface.
Practice NAB questions The differing albedos across the earth’s surface will have an impact on the amount of solar radiation reflected by the earth’s surface.
Global Climates and Biomes
Lesson 3 Reading Guide - Vocab wind trade winds westerlies polar easterlies Air Currents jet stream sea breeze land breeze.
A2 Module 4: Global Change
Ocean Currents Ocean Density. Energy in = energy out Half of solar radiation reaches Earth The atmosphere is transparent to shortwave but absorbs longwave.
Energy Balance and Circulation Systems. 2 of 12 Importance Energy from Sun (Energy Budget) –“Drives” Earth’s Atmosphere  Creates Circulation Circulation.
Wind & Climate Wind – the horizontal movement of air. Low pressure – warm air rising. High pressure – cold air falling. Winds always blow from high pressure.
Atmospheric movements We learned that energy is transferred from the Sun to the Earth creating convection currents. But, what type of currents???
Do Now: Analyze the following images
How Does Air Move Around the Globe?
Atmospheric Circulation and Weather  Composition and Properties of the Atmosphere Lower atmosphere nearly homogenous mixture of nitrogen 78.1% and oxygen.
THE ATMOSPHERE. aTMOSPHERIC pRESSURE Air Pressure- the measure of the force with which the air molecules push on a surface. Air pressure changes throughout.
Global Climate Change Climate Review. Global Circulation The solar radiation hitting the Earth is unequal…WHY? –Earth is oblate (slightly flattened)
WIND Movement of air in the atmosphere.. Remember Convection Principles Solar energy strikes the _____________________, heating the air, land and water.
PLANETARY WIND SYSTEM.
Meteorology / Weather Chapter 38. Standards  5 a, b  6:a, b  Objectives:  Student will be able to describe weather and climate.  Students will be.
Osmosis (Revisited) Video. Density mass per volume of seawater Determined by temperature and salinity Density of seawater increases all the way to its.
Movin' Around Students do not have to start a new page of notes but they can if they want.
Weather Systems. Circulation Cells Insolation is greatest at the equator, humidity is high, the airmass is unstable. The cold air at the poles is.
1 0º Equator90º Pole LP HP  At the Equator the atmosphere is heated  Air becomes less dense and rises.  Rising air creates low pressure at the equator.
TOC: Winds I STARTER: Think back to the demos, does air move from low pressure to high pressure or the other way around?? Explain…..
Chapter 4 Global Climates and Biomes. Global Processes Determine Weather and Climate Weather- the short term conditions of the atmosphere in a local area.
Fact Statements.  Surface currents are mainly caused by prevailing winds.  Their flow is controlled by the winds, Earth’s rotation and location of the.
Latitudinal effects Intensity of insolation is not the same at all latitudes Earth is roughly spherical, so insolation passing through 1 m 2 screen –Illuminates.
Atmospheric Circulation. Winds on a Non-Rotating Earth Air at the equator warms and rises. Once aloft, air flows back towards the poles where it cools.
Atmospheric Pressure and Wind
• At the poles (areas which receive less solar radiation), the air is cold and descends towards the equator through the lower layers of the atmosphere.
Lesson 1 Earth’s Atmosphere Lesson 2 Energy Transfer in the Atmosphere
Atmosphere and Weather
8.8 Energy Transfer within the Climate System
19.2 Pressure Centers and Winds
Ocean-Air Interaction
Earth’s Climate System Air and Ocean Circulation
Earth’s Climate System Air and Ocean Circulation
PLANETARY WIND SYSTEM.
Circulation in the atmosphere
Global Winds.
Earth’s Climate System Air and Ocean Circulation
THE ATMOSPHERE I CAN EXPLAIN HOW HEAT IS TRANSFERRED IN THE ATMOSPHERE. I CAN DESCRIBE CONDUCTION. I CAN DESCRIBE CONVECTION. I CAN DESCRIBE RADIATION.
Presentation transcript:

Advanced Oceanography Ocean Circulation - Chapter 1 A Review Circulation in both the oceans and the atmosphere is driven by energy from the Sun and modified by the Earth’s Rotation The oceans are mechanically driven by the atmosphere – winds. The oceans are thermally driven by the atmosphere by inducing changes in temperature and salinity (precipitation and evaporation, review latent and sensible heat fluxes)

Ocean current system involves both wind driven surface currents and density-driven (thermohaline) deep circulation.

Wind bands – Three convection cells in each hemisphere Trade winds = NE (30°N to 0°) and SE (30°S to 0°) Westerlies = 60°N to 30°N and 60°S to 30°S Polar easterlies = 90°N to 60°N and 90°S to 60°S Low pressure at 0°, 60°N, and 60°S Low pressure, ascending air, clouds, increased precipitation High pressure at 30°N, 30°S, 90°N, and 90°S High pressure, descending air, clear skies, low precipitation Look at the winds:

Now look at the currents:

Review the Coriolis Force Air and water masses moving over the surface of the Earth are subject to the Coriolis force. The Coriolis force acts at right angles to the direction of motion, is zero at the Equator and increases to a maximum at the poles.

Review The Radiation Balance The radiation balance of the Earth-ocean- atmosphere system is positive at low latitudes and negative at high latitudes.

Poleward Heat Transport: Upper Atm. Wind systems in the atmosphere and current systems in the ocean redistribute this heat around the planet.

Fig. 6-16, p. 168 Sea-surface average salinities in parts per thousand (‰). Sea-surface temperatures during Northern Hemisphere summer

Fig. 6-14, p. 167 Tropic of Cancer Equator Tropic of Capricorn Salinity Temperature Latitude North South