Chapter 7 100 Years of the Ocean General Circulation
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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. -
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. -
El Niño and La Niña
About the Images What are El Niño and La Niña? The images show El Niño, neutral, and La Niña sea surface The naturally occurring El Niño and La Niña phenomenon rep- heights (SSHs) relative to a reference state established in resents a “dance” between the atmosphere and ocean in the 1992. In the equatorial region of the Pacific Ocean, the SSH equatorial Pacific Ocean. Sometimes the atmosphere leads the during El Niño was higher by more than 18 cm over a large ocean and causes ocean conditions, and sometimes the ocean longitudinal region. The warmer water associated with El Niño leads the atmosphere and produces atmospheric motions that— displaces colder water in the upper layer of the ocean causing when strong enough—influence global atmospheric circulation. an increase in SSH because of thermal expansion. During La Sea surface temperature (SST) is the critical variable connecting Niña the temperature of the upper ocean is lower than normal, the atmosphere and ocean. Since SSH measurements yield criti- causing SSH to decrease because of thermal contraction. The cal information about the depth of the subsurface temperatures, neutral condition occurs when the upper-ocean temperature e.g., the thermocline, they provide key information on the onset, is “normal.” Red and white shades indicate high SSHs relative maintenance, and dissipation of El Niño and La Niña events. to the reference state, while blue and purple shades indicate SSHs lower than the reference state. Neutral conditions appear The 2015 El Niño Event green. The El Niño and neutral images are derived using data After five consecutive months with SSTs 0.5 °C above the acquired by the Ocean Surface Topography Mission (OSTM)/Jason-2 long-term mean, the National Oceanic and Atmospheric Admin- satellite. -
Atmospheric General Circulation
LectureLecture 5:5: AtmosphericAtmospheric GeneralGeneral CirculationCirculation JS JP HadleyHadley CellCell FerrelFerrel CellCell PolarPolar CellCell (driven by eddies) LHL H Basic Structures and Dynamics General Circulation in the Troposphere General Circulation in the Stratosphere Wind-Driven Ocean Circulation ESS55 Prof. Jin-Yi Yu SingleSingle--CellCell Model:Model: ExplainsExplains WhyWhy ThereThere areare TropicalTropical EasterliesEasterlies Without Earth Rotation With Earth Rotation Coriolis Force (Figures from Understanding Weather & Climate and The Earth System) ESS55 Prof. Jin-Yi Yu BreakdownBreakdown ofof thethe SingleSingle CellCell ÎÎ ThreeThree--CellCell ModelModel Absolute angular momentum at Equator = Absolute angular momentum at 60°N The observed zonal velocity at the equatoru is ueq = -5 m/sec. Therefore, the total velocity at the equator is U=rotational velocity (U0 + uEq) The zonal wind velocity at 60°N (u60N) can be determined by the following: (U0 + uEq) * a * Cos(0°) = (U60N + u60N) * a * Cos(60°) (Ω*a*Cos0° - 5) * a * Cos0° = (Ω*a*Cos60° + u60N) * a * Cos(60°) u60N = 687 m/sec !!!! This high wind speed is not observed! ESS55 Prof. Jin-Yi Yu PropertiesProperties ofof thethe ThreeThree CellsCells thermally indirect circulation thermally direct circulation JS JP HadleyHadley CellCell FerrelFerrel CellCell PolarPolar CellCell (driven by eddies) LHL H Equator 30° 60° Pole (warmer) (warm) (cold) (colder) ESS55 Prof. Jin-Yi Yu AtmosphericAtmospheric Circulation:Circulation: ZonalZonal--meanmean ViewsViews Single-Cell Model Three-Cell Model (Figures from Understanding Weather & Climate and The Earth System) ESS55 Prof. Jin-Yi Yu TheThe ThreeThree CellsCells ITCZ Subtropical midlatitude High Weather system (Figures from Understanding Weather & Climate and The Earth System) ESS55 Prof. Jin-Yi Yu ThermallyThermally Direct/IndirectDirect/Indirect CellsCells Thermally Direct Cells (Hadley and Polar Cells) Both cells have their rising branches over warm temperature zones and sinking braches over the cold temperature zone. -
The Earth's Rotation and Atmospheric Circulation, from 1963 to 1973 Kurt
Geophys. J. R. astr. Soc. (1981) 64,67-89 The Earth’s rotation and atmospheric circulation, from 1963 to 1973 Kurt Lambeck and Peter Hopgood Research School of Earth Sciences, Australian National University, Canberra 2600, Australia Received 1980 June 13; in original form 1980 March 17 ‘If everybody minded their own business, the world would go round a deal faster than it does.’ Alice’s Adventures in Wonderland Lewis Carroll Summary. The zonal angular momentum of the atmospheric circulation has been evaluated month-by-month and compared with astronomical observa- tions of the length-of-day for the 10 years from 1963 May to 1973 April. The reason for undertaking this study is to enable the astronomical observa- tions to be ‘corrected’ for the zonal wind effect and to investigate the residual excitation function for solid-Earth contributions. The principal conclusions reached are the following: (i) The annual change in length-of-day is almost entirely due to the seasonal changes in the zonal circulation with tidal, oceanographic and hydrologic phenomena contributing together at most 10 per cent of the total excitation. (ii) The semi-annual term is pre- dominantly due to the zonal wind and the body tide, with oceanic and hydrologic terms contributing about 10 per cent. (iii) The atmospheric circulation plays a dominant role in length-of-day changes in the period range from 1 to about 4 yr. This is partly associated with the quasi-biennial oscilla- tion and its harmonics. Both the period and amplitude of these fluctuations are very variable. (iv) At longer periods the atmosphere may still contribute to the total excitation but other excitation functions begin to rise above the spectrum of the meteorological excitation. -
The Voyage of the “Challenger”
The Voyage of the "Challenger" From 1872 to 1876 a doughty little ship sailed the seven seas and gathered an unprecedented amount of information about them, thereby founding the science of oceanography by Herbert S. Bailey, Jr. UST 77 years ago this month a spar since that pioneering voyage. It was the philosophy at the University of Edin decked little ship of 2,300 tons Challenger, rigged with crude but in burgh. He did some dredging in the sailed into the harbor of Spithead, genious sounding equipment, that Aegean Sea, studying the distribution JEngland. She was home from a voyage charted what is still our basic map of of flora and fauna and their relation to of three and a half years and 68,890 the world under the oceans. depths, temperatures and other factors. miles over the seven seas. Her expedition Before the Challenger, only a few iso Forbes never dredged deeper than about had been a bold attack upon the un lated soundings had been taken in the 1,200 feet, and he acquired some curious known in the tradition of the great sea deep seas. Magellan is believed to have notions, including a belief that nothing explorations of the 15th and 16th cen made the Rrst. During his voyage around lived in the sea below 1,500 feet. But turies. The unknown she had explored the globe in 1521 he lowered hand lines his pioneering work led the way for the was the sea bottom. When she had left to a depth of perhaps 200 fathoms Challenger expedition. -
Atmospheric Circulation and Weather Systems
CHAPTER ATMOSPHERIC CIRCULATION AND WEATHER SYSTEMS arlier Chapter 9 described the uneven pressure is measured with the help of a distribution of temperature over the mercury barometer or the aneroid barometer. Esurface of the earth. Air expands when Consult your book, Practical Work in heated and gets compressed when cooled. This Geography — Part I (NCERT, 2006) and learn results in variations in the atmospheric about these instruments. The pressure pressure. The result is that it causes the decreases with height. At any elevation it varies movement of air from high pressure to low from place to place and its variation is the pressure, setting the air in motion. You already primary cause of air motion, i.e. wind which know that air in horizontal motion is wind. moves from high pressure areas to low Atmospheric pressure also determines when pressure areas. the air will rise or sink. The wind redistributes the heat and moisture across the planet, Vertical Variation of Pressure thereby, maintaining a constant temperature In the lower atmosphere the pressure for the planet as a whole. The vertical rising of decreases rapidly with height. The decrease moist air cools it down to form the clouds and amounts to about 1 mb for each 10 m bring precipitation. This chapter has been increase in elevation. It does not always devoted to explain the causes of pressure decrease at the same rate. Table 10.1 gives differences, the forces that control the the average pressure and temperature at atmospheric circulation, the turbulent pattern selected levels of elevation for a standard of wind, the formation of air masses, the atmosphere. -
Miles Down! Oceanography Through History
MILES DOWN! OCEANOGRAPHY THROUGH HISTORY The history of oceanography is an international story of invention, individual adventure, and exploration that remains little-known. This exhibition presents an historical overview, using timelines, text, photographs, and profiles of oceanographic expeditions and individual scientists from around the world. Image: Colette Kerry From water’s edge, the oceans are as mysterious as the stars. In the 21st century, deep-sea exploration – like space exploration - is no longer a fantastic idea, but a fact of scientific life. How did we move below the surface to study the depths of the sea? This exhibition tells the story of curious humans posing questions about the oceans and developing the tools and technology to move miles down to explore the sea. The oceans that cover 71% of the world’s surface hide complex worlds within their depths. How ocean waters behave, what creatures inhabit the seas, what lies on the ocean floors, what makes up seawater: these are the questions that underlie the scientific study of the oceans - the science of oceanography. Oceanography is the scientific study of the oceans as complex, interrelated systems. It is a mixed science that combines many different approaches to understanding the watery portion of our planet. Physics explores the physical properties of the oceans, the currents and waves. It’s a study of matter and energy and the relation between them. Chemistry is concerned with the properties, composition, and structure of substances in the oceans and the changes they undergo when they combine or react. The geology of the seafloor explores the earth’s history, composition, structure and processes. -
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. -
Directory of Source Materials for the History of Oceanography; UNESCO
Unesco technical papers in marine science eo Directory of source materials for the history of oceanography Unesco !990 UNESCO TECHNICAL PAPERS IN MARINE SCIENCE Numbers 2. 3. 5, 6, 7,9, IO, II. 12, 13. 15. 16, 17. 18, 20.21.22,23. 24, 27. 28, 29, 30 and 32. arc out of stock. For full titles see inside back cover. Numbers 1, 4, 8 and 14 are incorporated in No. 27. No. Year SCOR No Year SCOR wo WG 19 Manne Science leaching at (he Univcrsit) (.evei 45 The International System of Units (SI) Kepon of lhe Unesco Workshop on Universa) in Oceanography Report of IAPSO Working Cunicula-/!iailabte in Spannh ami Arabic 1974 Group on Symbols. Units and Nomenclature in Physical Oceanography (SUN) 1985 25 Marine science programme for the Red Scj. Recommendations of the workshop held in 46 Opportunities and problems in Hremerhasen. FKG, 22*25 October 1974. satellite measurements of (he sea sponsored h) the Deutsche Forschungsgemein- Report of SCOR Working Group 70 schaft and Unesco 1976 — Available in Ar.. Ch., F.. R.. and S. 1986 WG 70 26 Marine science in the Gulf arca-Rcport of a 47 Research on coastal marine systems consullatisc meeting. Paris, IM4 November 1975 1976 — Report of the third meeting of the Uncsco/SCOR/IABO 3| Coastal bgoon survey (1976-1978) 198tï — consultative panel on coastal systems October 1984 1986 33 Coastal lagoon research, present and future Proceedings of a seminar. Duke University. 48 Coastal off-shore ecosystems relationships August 1978 (Unesco. IABO). 1981 — Final Report of SCOR/IABO/ Unesco Working Group 65 34 The carbon budget of the oceans Report of a Texel. -
Atmospheric Circulation
Atmospheric circulation Trade winds http://science.nasa.gov/science-news/science-at-nasa/2002/10apr_hawaii/ Atmosphere (noun) the envelope of gases (air) surrounding the earth or another planet Dry air: Argon, 0.98% O2, 21% N2, 78% CO2, >400ppm & rising Water vapor can be up to 4% 50% below 5.6 km (18,000 ft) 90% below 16 km (52,000 ft) http://mychinaviews.com/2011/06/into-thin-air.html Drivers of atmospheric circulation Uneven solar heating At poles sun’s energy is spread over a larger region Uneven solar heating At poles sun’s energy is spread over a larger region Uneven solar heating At poles sun’s energy is spread over a larger region Ways to transfer heat Conduction: Transfer of heat by direct contact. Heat goes from warmer areas to colder areas. Ways to transfer heat Radiation: Any object radiates heat as electromagnetic radiation (light, infrared) based on temperature of the object. Ways to transfer heat Convection: Heat carried by a fluid (air, water, etc) from a region of high temperature to a region of lower temperature. Convection cell Warm air rises, then as it cools it sinks back down Thermal (heat) balance Heat in = Heat out, for earth as a whole ! Heat in = Heat out, for latitude bands " Heat out t r o p s n a r Heat in t t a e h t e N RedistributionIncreasing heat of heat drive atmospheric circulation So, might expect Cool air sinking near the poles Warm air rising at equator Lutgens and Tarbuk, 2001 http://www.ux1.eiu.edu/~cfjps/1400/circulation.html Turns out a 3 cell modelis better Polar cell Ferrel cell (Mid-latitude -
Winter / Spring 2007
FOLLOWING SEASEA 2005-2006 Annual Report Issue Winter/Spring 2007 sea at thirty-five TABLETABLE OFOF CONTENTSCONTENTS Winter/Spring 2007 Cover Story SEA at Thirty-five SEA celebrates its 35th Anniversary year . .1 Features Ann Wickes Brewer A tribute to a SEA trustee emeritus . .4 Heading for a ‘roasted world’ John Bullard’s Boston Globe editorial . .9 In Every Issue Passages Events and news of general interest . .8 Scuttlebutt Alumni news from around the world . .10 Science Corner The evolution of oceanographic equipment . .26 Currents Mariah Klingsmith and Jarod Maggio (C-187) volunteer for the Peace Corps in the Philippines . .28 Special Report 2005-2006 Report to Donors From the desk of Board Chair, Linda Cox Maguire . .14 Annual Report . .15 Following SEA Winter/Spring 2007 Editor: Jan Wagner Cover Design: Lori Dolby Design: MBDesign Photography: Sandie Allen, Laurie Bullard, courtesy Colgate University, Mariah Klingsmith, Jarod Maggio, Amy Radar, courtesy Sparkman & Stephens, Jan Wagner, Become an alumni enrollment volunteer! For more information, Jim Watters, Laurie Weitzen contact Laurie Weitzen at (800) 552-3633, ext. 12 or [email protected] Following SEA is available online. If you’d like your prints, slides, or digital images considered for the next issue contact: Kerry Sullivan, ext. 20 or [email protected]. Sea Education Association, Inc., PO Box 6, Woods Hole, Massachusetts 02543 Phone 800-552-3633 Fax 508-457-4673 www.sea.edu Recycled Chlorine-Free Paper / Soy Ink captains October 1982 4 sea A lesson in determinationat thirty-five The story of SEA’s founding and the early years of struggle to gain a pathway to success is a lesson in determination on the part of Corwith Cramer, Jr.