Wind-Driven Ocean Circulation TEACHER’S GUIDE
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North America Other Continents
Arctic Ocean Europe North Asia America Atlantic Ocean Pacific Ocean Africa Pacific Ocean South Indian America Ocean Oceania Southern Ocean Antarctica LAND & WATER • The surface of the Earth is covered by approximately 71% water and 29% land. • It contains 7 continents and 5 oceans. Land Water EARTH’S HEMISPHERES • The planet Earth can be divided into four different sections or hemispheres. The Equator is an imaginary horizontal line (latitude) that divides the earth into the Northern and Southern hemispheres, while the Prime Meridian is the imaginary vertical line (longitude) that divides the earth into the Eastern and Western hemispheres. • North America, Earth’s 3rd largest continent, includes 23 countries. It contains Bermuda, Canada, Mexico, the United States of America, all Caribbean and Central America countries, as well as Greenland, which is the world’s largest island. North West East LOCATION South • The continent of North America is located in both the Northern and Western hemispheres. It is surrounded by the Arctic Ocean in the north, by the Atlantic Ocean in the east, and by the Pacific Ocean in the west. • It measures 24,256,000 sq. km and takes up a little more than 16% of the land on Earth. North America 16% Other Continents 84% • North America has an approximate population of almost 529 million people, which is about 8% of the World’s total population. 92% 8% North America Other Continents • The Atlantic Ocean is the second largest of Earth’s Oceans. It covers about 15% of the Earth’s total surface area and approximately 21% of its water surface area. -
How the Ocean Affects Weather & Climate
Ocean in Motion 6: How does the Ocean Change Weather and Climate? A. Overview 1. The Ocean in Motion -- Weather and Climate In this program we will tie together ideas from previous lectures on ocean circulation. The students will also learn about the similarities and interactions between the atmosphere and the ocean. 2. Contents of Packet Your packet contains the following activities: I. A Sea of Words B. Program Preparation 1. Focus Points OThe oceans and the atmosphere are closely linked 1. the sun heats the atmosphere as well as the oceans 2. water evaporates from the ocean into the atmosphere a. forms clouds and precipitation b. movement of any fluid (gas or liquid) due to heating creates convective currents OWeather and climate are two different things. 1. Winds a. Uneven heating and cooling of the atmosphere creates wind b. Global ocean surface current patterns are similar to global surface wind patterns c. wind patterns are analogous to ocean currents 2. Four seasons OAtmospheric motion 1. weather and air moves from high to low pressure areas 2. the earth's rotation also influences air and weather patterns 3. Atmospheric winds move surface ocean currents. ©1998 Project Oceanography Spring Series Ocean in Motion 1 C. Showtime 1. Broadcast Topics This broadcast will link into discussions on ocean and atmospheric circulation, wind patterns, and how climate and weather are two different things. a. Brief Review We know the modern reason for studying ocean circulation is because it is a major part of our climate. We talked about how the sun provides heat energy to the world, and how the ocean currents circulate because the water temperatures and densities vary. -
Basic Concepts in Oceanography
Chapter 1 XA0101461 BASIC CONCEPTS IN OCEANOGRAPHY L.F. SMALL College of Oceanic and Atmospheric Sciences, Oregon State University, Corvallis, Oregon, United States of America Abstract Basic concepts in oceanography include major wind patterns that drive ocean currents, and the effects that the earth's rotation, positions of land masses, and temperature and salinity have on oceanic circulation and hence global distribution of radioactivity. Special attention is given to coastal and near-coastal processes such as upwelling, tidal effects, and small-scale processes, as radionuclide distributions are currently most associated with coastal regions. 1.1. INTRODUCTION Introductory information on ocean currents, on ocean and coastal processes, and on major systems that drive the ocean currents are important to an understanding of the temporal and spatial distributions of radionuclides in the world ocean. 1.2. GLOBAL PROCESSES 1.2.1 Global Wind Patterns and Ocean Currents The wind systems that drive aerosols and atmospheric radioactivity around the globe eventually deposit a lot of those materials in the oceans or in rivers. The winds also are largely responsible for driving the surface circulation of the world ocean, and thus help redistribute materials over the ocean's surface. The major wind systems are the Trade Winds in equatorial latitudes, and the Westerly Wind Systems that drive circulation in the north and south temperate and sub-polar regions (Fig. 1). It is no surprise that major circulations of surface currents have basically the same patterns as the winds that drive them (Fig. 2). Note that the Trade Wind System drives an Equatorial Current-Countercurrent system, for example. -
Hadley Cell and the Trade Winds of Hawai'i: Nā Makani
November 19, 2012 Hadley Cell and the Trade Winds of Hawai'i Hadley Cell and the Trade Winds of Hawai‘i: Nā Makani Mau Steven Businger & Sara da Silva [email protected], [email protected] Iasona Ellinwood, [email protected] Pauline W. U. Chinn, [email protected] University of Hawai‘i at Mānoa Figure 1. Schematic of global circulation Grades: 6-8, modifiable for 9-12 Time: 2 - 10 hours Nā Honua Mauli Ola, Guidelines for Educators, No Nā Kumu: Educators are able to sustain respect for the integrity of one’s own cultural knowledge and provide meaningful opportunities to make new connections among other knowledge systems (p. 37). Standard: Earth and Space Science 2.D ESS2D: Weather and Climate Weather varies day to day and seasonally; it is the condition of the atmosphere at a given place and time. Climate is the range of a region’s weather over one to many years. Both are shaped by complex interactions involving sunlight, ocean, atmosphere, latitude, altitude, ice, living things, and geography that can drive changes over multiple time scales—days, weeks, and months for weather to years, decades, centuries, and beyond for climate. The ocean absorbs and stores large amounts of energy from the sun and releases it slowly, moderating and stabilizing global climates. Sunlight heats the land more rapidly. Heat energy is redistributed through ocean currents and atmospheric circulation, winds. Greenhouse gases absorb and retain the energy radiated from land and ocean surfaces, regulating temperatures and keep Earth habitable. (A Framework for K-12 Science Education, NRC, 2012) Hawai‘i Content and Performance Standards (HCPS) III http://standardstoolkit.k12.hi.us/index.html 1 November 19, 2012 Hadley Cell and the Trade Winds of Hawai'i STRAND THE SCIENTIFIC PROCESS Standard 1: The Scientific Process: SCIENTIFIC INVESTIGATION: Discover, invent, and investigate using the skills necessary to engage in the scientific process Benchmarks: SC.8.1.1 Determine the link(s) between evidence and the Topic: Scientific Inquiry conclusion(s) of an investigation. -
Chapter 7 100 Years of the Ocean General Circulation
CHAPTER 7 WUNSCH AND FERRARI 7.1 Chapter 7 100 Years of the Ocean General Circulation CARL WUNSCH Massachusetts Institute of Technology, and Harvard University, Cambridge, Massachusetts RAFFAELE FERRARI Massachusetts Institute of Technology, Cambridge, Massachusetts ABSTRACT The central change in understanding of the ocean circulation during the past 100 years has been its emergence as an intensely time-dependent, effectively turbulent and wave-dominated, flow. Early technol- ogies for making the difficult observations were adequate only to depict large-scale, quasi-steady flows. With the electronic revolution of the past 501 years, the emergence of geophysical fluid dynamics, the strongly inhomogeneous time-dependent nature of oceanic circulation physics finally emerged. Mesoscale (balanced), submesoscale oceanic eddies at 100-km horizontal scales and shorter, and internal waves are now known to be central to much of the behavior of the system. Ocean circulation is now recognized to involve both eddies and larger-scale flows with dominant elements and their interactions varying among the classical gyres, the boundary current regions, the Southern Ocean, and the tropics. 1. Introduction physical regimes, understanding of the ocean until relatively recently greatly lagged that of the atmo- In the past 100 years, understanding of the general sphere. As in almost all of fluid dynamics, progress circulation of the ocean has shifted from treating it as an in understanding has required an intimate partnership essentially laminar, steady-state, slow, almost geological, between theoretical description and observational or flow, to that of a perpetually changing fluid, best charac- laboratory tests. The basic feature of the fluid dynamics terized as intensely turbulent with kinetic energy domi- of the ocean, as opposed to that of the atmosphere, has nated by time-varying flows. -
Fronts in the World Ocean's Large Marine Ecosystems. ICES CM 2007
- 1 - This paper can be freely cited without prior reference to the authors International Council ICES CM 2007/D:21 for the Exploration Theme Session D: Comparative Marine Ecosystem of the Sea (ICES) Structure and Function: Descriptors and Characteristics Fronts in the World Ocean’s Large Marine Ecosystems Igor M. Belkin and Peter C. Cornillon Abstract. Oceanic fronts shape marine ecosystems; therefore front mapping and characterization is one of the most important aspects of physical oceanography. Here we report on the first effort to map and describe all major fronts in the World Ocean’s Large Marine Ecosystems (LMEs). Apart from a geographical review, these fronts are classified according to their origin and physical mechanisms that maintain them. This first-ever zero-order pattern of the LME fronts is based on a unique global frontal data base assembled at the University of Rhode Island. Thermal fronts were automatically derived from 12 years (1985-1996) of twice-daily satellite 9-km resolution global AVHRR SST fields with the Cayula-Cornillon front detection algorithm. These frontal maps serve as guidance in using hydrographic data to explore subsurface thermohaline fronts, whose surface thermal signatures have been mapped from space. Our most recent study of chlorophyll fronts in the Northwest Atlantic from high-resolution 1-km data (Belkin and O’Reilly, 2007) revealed a close spatial association between chlorophyll fronts and SST fronts, suggesting causative links between these two types of fronts. Keywords: Fronts; Large Marine Ecosystems; World Ocean; sea surface temperature. Igor M. Belkin: Graduate School of Oceanography, University of Rhode Island, 215 South Ferry Road, Narragansett, Rhode Island 02882, USA [tel.: +1 401 874 6533, fax: +1 874 6728, email: [email protected]]. -
Climate and Atmospheric Circulation of Mars
Climate and QuickTime™ and a YUV420 codec decompressor are needed to see this picture. Atmospheric Circulation of Mars: Introduction and Context Peter L Read Atmospheric, Oceanic & Planetary Physics, University of Oxford Motivating questions • Overview and phenomenology – Planetary parameters and ‘geography’ of Mars – Zonal mean circulations as a function of season – CO2 condensation cycle • Form and style of Martian atmospheric circulation? • Key processes affecting Martian climate? • The Martian climate and circulation in context…..comparative planetary circulation regimes? Books? • D. G. Andrews - Intro….. • J. T. Houghton - The Physics of Atmospheres (CUP) ALSO • I. N. James - Introduction to Circulating Atmospheres (CUP) • P. L. Read & S. R. Lewis - The Martian Climate Revisited (Springer-Praxis) Ground-based observations Percival Lowell Lowell Observatory (Arizona) [Image source: Wikimedia Commons] Mars from Hubble Space Telescope Mars Pathfinder (1997) Mars Exploration Rovers (2004) Orbiting spacecraft: Mars Reconnaissance Orbiter (NASA) Image credits: NASA/JPL/Caltech Mars Express orbiter (ESA) • Stereo imaging • Infrared sounding/mapping • UV/visible/radio occultation • Subsurface radar • Magnetic field and particle environment MGS/TES Atmospheric mapping From: Smith et al. (2000) J. Geophys. Res., 106, 23929 DATA ASSIMILATION Spacecraft Retrieved atmospheric parameters ( p,T,dust...) - incomplete coverage - noisy data..... Assimilation algorithm Global 3D analysis - sequential estimation - global coverage - 4Dvar .....? - continuous in time - all variables...... General Circulation Model - continuous 3D simulation - complete self-consistent Physics - all variables........ - time-dependent circulation LMD-Oxford/OU-IAA European Mars Climate model • Global numerical model of Martian atmospheric circulation (cf Met Office, NCEP, ECMWF…) • High resolution dynamics – Typically T31 (3.75o x 3.75o) – Most recently up to T170 (512 x 256) – 32 vertical levels stretched to ~120 km alt. -
World Ocean Thermocline Weakening and Isothermal Layer Warming
applied sciences Article World Ocean Thermocline Weakening and Isothermal Layer Warming Peter C. Chu * and Chenwu Fan Naval Ocean Analysis and Prediction Laboratory, Department of Oceanography, Naval Postgraduate School, Monterey, CA 93943, USA; [email protected] * Correspondence: [email protected]; Tel.: +1-831-656-3688 Received: 30 September 2020; Accepted: 13 November 2020; Published: 19 November 2020 Abstract: This paper identifies world thermocline weakening and provides an improved estimate of upper ocean warming through replacement of the upper layer with the fixed depth range by the isothermal layer, because the upper ocean isothermal layer (as a whole) exchanges heat with the atmosphere and the deep layer. Thermocline gradient, heat flux across the air–ocean interface, and horizontal heat advection determine the heat stored in the isothermal layer. Among the three processes, the effect of the thermocline gradient clearly shows up when we use the isothermal layer heat content, but it is otherwise when we use the heat content with the fixed depth ranges such as 0–300 m, 0–400 m, 0–700 m, 0–750 m, and 0–2000 m. A strong thermocline gradient exhibits the downward heat transfer from the isothermal layer (non-polar regions), makes the isothermal layer thin, and causes less heat to be stored in it. On the other hand, a weak thermocline gradient makes the isothermal layer thick, and causes more heat to be stored in it. In addition, the uncertainty in estimating upper ocean heat content and warming trends using uncertain fixed depth ranges (0–300 m, 0–400 m, 0–700 m, 0–750 m, or 0–2000 m) will be eliminated by using the isothermal layer. -
Tube-Nosed Seabirds) Unique Characteristics
PELAGIC SEABIRDS OF THE CALIFORNIA CURRENT SYSTEM & CORDELL BANK NATIONAL MARINE SANCTUARY Written by Carol A. Keiper August, 2008 Cordell Bank National Marine Sanctuary protects an area of 529 square miles in one of the most productive offshore regions in North America. The sanctuary is located approximately 43 nautical miles northwest of the Golden Gate Bridge, and San Francisco California. The prominent feature of the Sanctuary is a submerged granite bank 4.5 miles wide and 9.5 miles long, which lay submerged 115 feet below the ocean’s surface. This unique undersea topography, in combination with the nutrient-rich ocean conditions created by the physical process of upwelling, produces a lush feeding ground. for countless invertebrates, fishes (over 180 species), marine mammals (over 25 species), and seabirds (over 60 species). The undersea oasis of the Cordell Bank and surrounding waters teems with life and provides food for hundreds of thousands of seabirds that travel from the Farallon Islands and the Point Reyes peninsula or have migrated thousands of miles from Alaska, Hawaii, Australia, New Zealand, and South America. Cordell Bank is also known as the albatross capital of the Northern Hemisphere because numerous species visit these waters. The US National Marine Sanctuaries are administered and managed by the National Oceanic and Atmospheric Administration (NOAA) who work with the public and other partners to balance human use and enjoyment with long-term conservation. There are four major orders of seabirds: 1) Sphenisciformes – penguins 2) *Procellariformes – albatross, fulmars, shearwaters, petrels 3) Pelecaniformes – pelicans, boobies, cormorants, frigate birds 4) *Charadriiformes - Gulls, Terns, & Alcids *Orders presented in this seminar In general, seabirds have life histories characterized by low productivity, delayed maturity, and relatively high adult survival. -
Introduction to Oceanography
Introduction to Oceanography Introduction to Oceanography Lecture 14: Tides, Biological Productivity Memorial Day holiday Monday no lab meetings Go to any other lab section this week (and let the TA know!) Bay of Fundy -- low tide, Photo by Dylan Kereluk, . Creative Commons A 2.0 Generic, Mudskipper (Periophthalmus modestus) at low tide, photo by OpenCage, Wikimedia Commons, Creative http://commons.wikimedia.org/wiki/File:Bay_of_Fundy_-_Tide_Out.jpg Commons A S-A 2.5, http://commons.wikimedia.org/wiki/File:Periophthalmus_modestus.jpg Tides Earth-Moon-Sun System Planet-length waves Cyclic, repeating rise & fall of sea level • Earth-Sun Distance – Most regular phenomenon in the oceans 150,000,000 km Daily tidal variation has great effects on life in & around the ocean (Lab 8) • Earth-Moon Distance 385,000 km Caused by gravity and Much closer to Earth, but between Earth, Moon & much less massive Sun, their orbits around • Earth Obliquity = 23.5 each other, and the degrees Earth’s daily spin – Seasons Photos by Samuel Wantman, Creative Commons A S-A 3.0, http://en.wikipedia.org/ wiki/File:Bay_of_Fundy_Low_Tide.jpg and Figure by Homonculus 2/Geologician, Wikimedia Commons, http://en.wikipedia.org/wiki/ Creative Commons A 3.0, http://en.wikipedia.org/wiki/ File:Bay_of_Fundy_High_Tide.jpg File:Lunar_perturbation.jpg Tides are caused by the gravity of the Moon and Sun acting on Scaled image of Earth-Moon distance, Nickshanks, Wikimedia Commons, Creative Commons A 2.5 Earth and its ocean. Pluto-Charon mutual orbit, Zhatt, Wikimedia Commons, Public -
Kenya | Year 2| Important Questions Key Knowledge Vocabulary 1 Where Is Kenya on a a Large Solid Area of Land
Kenya | Year 2| Important Questions Key Knowledge Vocabulary 1 Where is Kenya on a A large solid area of land. Earth has Kenya is in East Africa. Nairobi is the 1 continent world map? seven continents. capital city and Mombasa is the largest An area set aside by a country’s 2 What is life like for city in Kenya. 2 National people living in Kenya? park government. The Tana river is the longest river in 3 Maasai one of the best-known groups of 3 What is a national Kenya. people in Africa. They live in park? southern Kenya Mount Kenya is the highest mountain in 4 Endangered Any type of plant or animal that is 4 Which are the main Kenya. in danger of disappearing forever. animals living in Kenya? 5 migrate Many mammals, birds, fishes, 5 What is Maasai insects, and other animals move culture? Kenya lies on the Equator, which means from one place to another at the climate is hot, sunny and dry for most certain times of the year. What is life like for a 6 of the year. ocean A large body of salt water, which Kenyan child compared 6 The Great Rift Valley is an enormous covers the majority of the earth’s to my life? valley of mountains which runs from the surface. north to south of Kenya. The valley has a 7 Capital A large town. Each country has a chain of volcanoes which are still ‘active’ . city capital city, which is usually one of Lake Victoria, the second largest the largest cities. -
SEMESTER at SEA COURSE SYLLABUS Colorado State
SEMESTER AT SEA COURSE SYLLABUS Colorado State University, Academic Partner Voyage: Spring 2022 Discipline: Natural Resources Course Number and Title: NR 150 Oceanography Division: Lower Faculty Name: Ursula Quillmann Semester Credit Hours: 3 Prerequisites: None COURSE DESCRIPTION Studying the ocean while voyaging on the ocean is a dream-come-true. We will study in the classroom the fundamentals of the four major disciplines in oceanography, 1.) Geological Oceanography (GO), Chemical Oceanography (CO), Physical Oceanography (PO), and Biological Oceanography (BO), and how together they shape our environment and Earth’s climate. The exciting part is that we will see the interaction of these four disciplines coming to life throughout the voyage. We will spend time together on the deck, observing the ocean and hopefully seeing wildlife. We will also discuss the changing ocean environments, including ocean warming, acidification, sea level rise. We will also discuss the pressures humans exert on the marine environments, including pollution, overfishing, destroying coastal habitats. Port discovery will give us a chance to evaluate the role the ocean plays in ten countries and to compare the health of the marine environment in these countries. Before each port, we will look at the pressing coastal marine issues each country is facing, and we will allow ample time to share our experiences with one another and learn from one another. This voyage allows the unique opportunity to see the big picture on how our ocean provides essential services to us. The overarching goal of studying the ocean on our voyage is to become aware that the ocean is our lifeline.