Atmospheric and Oceanic 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. -
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. -
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. -
11 General Circulation
Copyright © 2017 by Roland Stull. Practical Meteorology: An Algebra-based Survey of Atmospheric Science. v1.02 “Practical Meteorology: An Algebra-based Survey of Atmospheric Science” by Roland Stull is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License. View this license at http://creativecommons.org/licenses/by- nc-sa/4.0/ . This work is available at https://www.eoas.ubc.ca/books/Practical_Meteorology/ 11 GENERAL CIRCULATION Contents A spatial imbalance between radiative inputs and outputs exists for the earth-ocean-atmosphere 11.1. Key Terms 330 system. The earth loses energy at all latitudes due 11.2. A Simple Description of the Global Circulation 330 to outgoing infrared (IR) radiation. Near the trop- 11.2.1. Near the Surface 330 ics, more solar radiation enters than IR leaves, hence 11.2.2. Upper-troposphere 331 there is a net input of radiative energy. Near Earth’s 11.2.3. Vertical Circulations 332 poles, incoming solar radiation is too weak to totally 11.2.4. Monsoonal Circulations 333 offset the IR cooling, allowing a net loss of energy. 11.3. Radiative Differential Heating 334 The result is differential heating, creating warm 11.3.1. North-South Temperature Gradient 335 equatorial air and cold polar air (Fig. 11.1a). 11.3.2. Global Radiation Budgets 336 This imbalance drives the global-scale general 11.3.3. Radiative Forcing by Latitude Belt 338 circulation of winds. Such a circulation is a fluid- 11.3.4. General Circulation Heat Transport 338 dynamical analogy to Le Chatelier’s Principle of 11.4. -
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. -
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. -
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. -
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 -
Dicionarioct.Pdf
McGraw-Hill Dictionary of Earth Science Second Edition McGraw-Hill New York Chicago San Francisco Lisbon London Madrid Mexico City Milan New Delhi San Juan Seoul Singapore Sydney Toronto Copyright © 2003 by The McGraw-Hill Companies, Inc. All rights reserved. Manufactured in the United States of America. Except as permitted under the United States Copyright Act of 1976, no part of this publication may be repro- duced or distributed in any form or by any means, or stored in a database or retrieval system, without the prior written permission of the publisher. 0-07-141798-2 The material in this eBook also appears in the print version of this title: 0-07-141045-7 All trademarks are trademarks of their respective owners. Rather than put a trademark symbol after every occurrence of a trademarked name, we use names in an editorial fashion only, and to the benefit of the trademark owner, with no intention of infringement of the trademark. Where such designations appear in this book, they have been printed with initial caps. McGraw-Hill eBooks are available at special quantity discounts to use as premiums and sales promotions, or for use in corporate training programs. For more information, please contact George Hoare, Special Sales, at [email protected] or (212) 904-4069. TERMS OF USE This is a copyrighted work and The McGraw-Hill Companies, Inc. (“McGraw- Hill”) and its licensors reserve all rights in and to the work. Use of this work is subject to these terms. Except as permitted under the Copyright Act of 1976 and the right to store and retrieve one copy of the work, you may not decom- pile, disassemble, reverse engineer, reproduce, modify, create derivative works based upon, transmit, distribute, disseminate, sell, publish or sublicense the work or any part of it without McGraw-Hill’s prior consent. -
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For DLP, Current Affairs Magazine & Test Series related regular updates, follow us on www.facebook.com/drishtithevisionfoundation www.twitter.com/drishtiias CONTENTS UNIT-I : GEOMORPHOLOGY 1. Introduction to Geography 3-5 2. Origin of Universe, Earth & Life 6-11 3. Our Earth 12-29 4. Rocks & Minerals 30-32 5. Weathering, Mass Movement & Erosion 33-40 6. Landforms 41-51 7. Soil 52-62 UNIT-II : CLIMATOLOGY 8. Weather & Climate 65-67 9. Composition & Structure of Atmosphere 68-71 10. Distribution of Temperature & Heat Budget 72-80 11. Pressure & Wind Systems 81-100 12. Condensation & Precipitation 101-108 13. Classification of Climate 109-114 UNIT-III : OCEANOGRAPHY 14. Oceans 117-130 15. Oceanic Resources 131-136 UNIT-IV : HUMAN & ECONOMIC GEOGRAPHY 16. Population 139-154 17. Human Development 155-160 18. Settlement & Migration 161-173 19. Agriculture 174-201 20. Resources of the World 202-224 21. Location of Industries 225-247 22. Transport 248-254 Previous Years’ UPSC Questions (Solved) 255-261 Practice Questions 262 Pressure & Wind Systems 11 Chapter The weight of a column of air contained in a unit area from the mean sea level to the top of the atmosphere is called the air or atmospheric pressure. The atmospheric pressure is expressed in units of millibar. At sea level the average atmospheric pressure is 1,013.2 millibar. Due to gravity, the air at the surface is denser and hence has higher pressure. Air pressure is measured with the help of a mercury barometer or the aneroid barometer. The pressure decreases with height. At any elevation it varies from place to place and its variation is the primary cause of air motion, i.e.