Geophysical Fluid Dynamics: Whence, Whither and Why? Rspa.Royalsocietypublishing.Org Geoffrey K
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MIMOC: a Global Monthly Isopycnal Upper-Ocean Climatology with Mixed Layers*
1 * 1 MIMOC: A Global Monthly Isopycnal Upper-Ocean Climatology with Mixed Layers 2 3 Sunke Schmidtko1,2, Gregory C. Johnson1, and John M. Lyman1,3 4 5 1National Oceanic and Atmospheric Administration, Pacific Marine Environmental 6 Laboratory, Seattle, Washington 7 2University of East Anglia, School of Environmental Sciences, Norwich, United 8 Kingdom 9 3Joint Institute for Marine and Atmospheric Research, University of Hawaii at Manoa, 10 Honolulu, Hawaii 11 12 Accepted for publication in 13 Journal of Geophysical Research - Oceans. 14 Copyright 2013 American Geophysical Union. Further reproduction or electronic 15 distribution is not permitted. 16 17 8 February 2013 18 19 ______________________________________ 20 *Pacific Marine Environmental Laboratory Contribution Number 3805 21 22 Corresponding Author: Sunke Schmidtko, School of Environmental Sciences, University 23 of East Anglia, Norwich, NR4 7TJ, UK. Email: [email protected] 2 24 Abstract 25 26 A Monthly, Isopycnal/Mixed-layer Ocean Climatology (MIMOC), global from 0–1950 27 dbar, is compared with other monthly ocean climatologies. All available quality- 28 controlled profiles of temperature (T) and salinity (S) versus pressure (P) collected by 29 conductivity-temperature-depth (CTD) instruments from the Argo Program, Ice-Tethered 30 Profilers, and archived in the World Ocean Database are used. MIMOC provides maps 31 of mixed layer properties (conservative temperature, Θ, Absolute Salinity, SA, and 32 maximum P) as well as maps of interior ocean properties (Θ, SA, and P) to 1950 dbar on 33 isopycnal surfaces. A third product merges the two onto a pressure grid spanning the 34 upper 1950 dbar, adding more familiar potential temperature (θ) and practical salinity (S) 35 maps. -
Role of Regional Ocean Dynamics in Dynamic Sea Level Projections by the End of the 21St Century Over Southeast Asia
EGU21-8618, updated on 25 Sep 2021 https://doi.org/10.5194/egusphere-egu21-8618 EGU General Assembly 2021 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Role of Regional Ocean Dynamics in Dynamic Sea Level Projections by the end of the 21st Century over Southeast Asia Dhrubajyoti Samanta1, Svetlana Jevrejeva2, Hindumathi K. Palanisamy2, Kristopher B. Karnauskas3, Nathalie F. Goodkin1,4, and Benjamin P. Horton1 1Nanyang Technological University, Singapore ([email protected]) 2Centre for Climate Research Singapore, Singapore 3University of Colorado Boulder, USA 4American Museum of Natural History, USA Southeast Asia is especially vulnerable to the impacts of sea-level rise due to the presence of many low-lying small islands and highly populated coastal cities. However, our current understanding of sea-level projections and changes in upper-ocean dynamics over this region currently rely on relatively coarse resolution (~100 km) global climate model (GCM) simulations and is therefore limited over the coastal regions. Here using GCM simulations from the High-Resolution Model Intercomparison Project (HighResMIP) of the Coupled Model Intercomparison Project Phase 6 (CMIP6) to (1) examine the improvement of mean-state biases in the tropical Pacific and dynamic sea-level (DSL) over Southeast Asia; (2) generate projection on DSL over Southeast Asia under shared socioeconomic pathways phase-5 (SSP5-585); and (3) diagnose the role of changes in regional ocean dynamics under SSP5-585. We select HighResMIP models that included a historical period and shared socioeconomic pathways (SSP) 5-8.5 future scenario for the same ensemble and estimate the projected changes relative to the 1993-2014 period. -
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Vol. 62 Bollettino Vol. 62 - SUPPLEMENT 1 pp. 327 di Geofisica An International teorica ed applicata Journal of Earth Sciences IMDIS 2021 International Conference on Marine Data and Information Systems 12-14 April, 2021 Online Book of Abstracts SUPPLEMENT 1 Guest Editors: Michèle Fichaut, Vanessa Tosello, Alessandra Giorgetti BOLLETTINO DI GEOFISICA teorica ed applicata 210109 - OGS.Supp.Vol62.cover_08dorso19.indd 3 03/05/21 10:54 EDITOR-IN-CHIEF D. Slejko; Trieste, Italy EDITORIAL COUNCIL SUBSCRIPTIONS 2021 A. Camerlenghi, N. Casagli, F. Coren, P. Del Negro, F. Ferraccioli, S. Parolai, G. Rossi, C. Solidoro; Trieste, Italy ASSOCIATE EDITORS A. SOLID EaRTH GeOPHYsICs N. Abu-Zeid; Ferrara, Italy J. Ba; Nanjing, China R. Barzaghi; Milano, Italy J. Boaga; Padova, Italy C. Braitenberg; Trieste, Italy A. Casas; Barcelona, Spain G. Cassiani; Padova, Italy F. Cavallini; Trieste, Italy A. Del Ben; Trieste, Italy P. dell’Aversana; San Donato Milanese, Italy C. Doglioni; Roma, Italy F. Ferrucci, Vibo Valentia, Italy E. Forte; Trieste, Italy M.-J. Jimenez; Madrid, Spain C. Layland-Bachmann, Berkeley, U.S.A. Bollettino di Geofisica Teorica ed Applicata G. Li; Zhoushan, China c/o Istituto Nazionale di Oceanografia P. Paganini; Trieste, Italy e di Geofisica Sperimentale V. Paoletti, Naples, Italy Borgo Grotta Gigante, 42/c E. Papadimitriou; Thessaloniki, Greece 34010 Sgonico, Trieste, Italy R. Petrini; Pisa, Italy e-mail: [email protected] M. Pipan; Trieste, Italy G. Seriani; Trieste, Italy http-server: bgta.eu A. Shogenova; Tallin, Estonia E. Stucchi; Milano, Italy S. Trevisani; Venezia, Italy M. Vellico; Trieste, Italy A. Vesnaver; Trieste, Italy V. Volpi; Trieste, Italy A. -
Shallow Water Waves and Solitary Waves Article Outline Glossary
Shallow Water Waves and Solitary Waves Willy Hereman Department of Mathematical and Computer Sciences, Colorado School of Mines, Golden, Colorado, USA Article Outline Glossary I. Definition of the Subject II. Introduction{Historical Perspective III. Completely Integrable Shallow Water Wave Equations IV. Shallow Water Wave Equations of Geophysical Fluid Dynamics V. Computation of Solitary Wave Solutions VI. Water Wave Experiments and Observations VII. Future Directions VIII. Bibliography Glossary Deep water A surface wave is said to be in deep water if its wavelength is much shorter than the local water depth. Internal wave A internal wave travels within the interior of a fluid. The maximum velocity and maximum amplitude occur within the fluid or at an internal boundary (interface). Internal waves depend on the density-stratification of the fluid. Shallow water A surface wave is said to be in shallow water if its wavelength is much larger than the local water depth. Shallow water waves Shallow water waves correspond to the flow at the free surface of a body of shallow water under the force of gravity, or to the flow below a horizontal pressure surface in a fluid. Shallow water wave equations Shallow water wave equations are a set of partial differential equations that describe shallow water waves. 1 Solitary wave A solitary wave is a localized gravity wave that maintains its coherence and, hence, its visi- bility through properties of nonlinear hydrodynamics. Solitary waves have finite amplitude and propagate with constant speed and constant shape. Soliton Solitons are solitary waves that have an elastic scattering property: they retain their shape and speed after colliding with each other. -
Trophic Diversity of Plankton in the Epipelagic and Mesopelagic Layers of the Tropical and Equatorial Atlantic Determined with Stable Isotopes
diversity Article Trophic Diversity of Plankton in the Epipelagic and Mesopelagic Layers of the Tropical and Equatorial Atlantic Determined with Stable Isotopes Antonio Bode 1,* ID and Santiago Hernández-León 2 1 Instituto Español de Oceanografía, Centro Oceanográfico de A Coruña, Apdo 130, 15080 A Coruña, Spain 2 Instituto de Oceanografía y Cambio Global (IOCAG), Universidad de las Palmas de Gran Canaria, Campus de Taliarte, Telde, Gran Canaria, 35214 Islas Canarias, Spain; [email protected] * Correspondence: [email protected]; Tel.: +34-981205362 Received: 30 April 2018; Accepted: 12 June 2018; Published: 13 June 2018 Abstract: Plankton living in the deep ocean either migrate to the surface to feed or feed in situ on other organisms and detritus. Planktonic communities in the upper 800 m of the tropical and equatorial Atlantic were studied using the natural abundance of stable carbon and nitrogen isotopes to identify their food sources and trophic diversity. Seston and zooplankton (>200 µm) samples were collected with Niskin bottles and MOCNESS nets, respectively, in the epipelagic (0–200 m), upper mesopelagic (200–500 m), and lower mesopelagic layers (500–800 m) at 11 stations. Food sources for plankton in the productive zone influenced by the NW African upwelling and the Canary Current were different from those in the oligotrophic tropical and equatorial zones. In the latter, zooplankton collected during the night in the mesopelagic layers was enriched in heavy nitrogen isotopes relative to day samples, supporting the active migration of organisms from deep layers. Isotopic niches showed also zonal differences in size (largest in the north), mean trophic diversity (largest in the tropical zone), food sources, and the number of trophic levels (largest in the equatorial zone). -
Impact of the Pycnocline Layer on Bacterioplankton
MARINE ECOLOGY - PROGRESS SERIES Vol. 38: 295403, 1987 Published July 13 Mar. Ecol. Prog. Ser. l Impact of the pycnocline layer on bacterioplankton: diel and spatial variations in microbial parameters in the stratified water column of the Gulf of Trieste (Northern Adriatic Sea) Gerhard J. ~erndl'& Vlado ~alaCiC~ ' Institute for Zoology. University of Vienna. Althanstr. 14, A-1090 Vienna, Austria Marine Biology Station Piran, Cesta JLA 65, YU-66330 Piran. Yugoslavia ABSTRACT: Die1 variations in bacterial density, frequency of bvidlng cells (FDC) and bssolved organic carbon (DOC) in the stratified water column of the Gulf of Trieste were investigated at various depths. In the surface layers morning and afternoon DOC peaks (up to 10 mg I-') were observed in 3 out of 4 diel cycles. Bacterial abundance remained fairly constant over the diel cycles; however, bacterial activity as measured by FDC showed pronounced peaks in late afternoon and dawn coinciding with the DOC maximum concentrations. The pycnocline layer exhibited DOC concentrations similar to those of the overlying waters. The frequency of dividing cells (FDC), however, remained high throughout the entire diel cycle. The observed pronounced diel variations in bacterial production were therefore largely restricted to the layers well above the pycnocline; bacterial production contributed less than 20 % to the overall diel production (500 to 1000 pg C 1-' d-') in the uppermost 5 m water body. Highest diel production was found in the pycnocline layer at the end of the phytoplankton bloom (June and July) probably reflecting the formation of nutrient-enriched microzones around decaying phytoplankton cells due to reduced sinking velocities in the pycnocline layer. -
Dispersion in the Open Ocean Seasonal Pycnocline at Scales of 1–10Km and 1–6 Days
FEBRUARY 2020 S U N D E R M E Y E R E T A L . 415 Dispersion in the Open Ocean Seasonal Pycnocline at Scales of 1–10km and 1–6 days a MILES A. SUNDERMEYER AND DANIEL A. BIRCH University of Massachusetts Dartmouth, North Dartmouth, Massachusetts JAMES R. LEDWELL Woods Hole Oceanographic Institution, Woods Hole, Massachusetts b MURRAY D. LEVINE, STEPHEN D. PIERCE, AND BRANDY T. KUEBEL CERVANTES Oregon State University, Corvallis, Oregon (Manuscript received 23 January 2019, in final form 14 November 2019) ABSTRACT Results are presented from two dye release experiments conducted in the seasonal thermocline of the 2 2 Sargasso Sea, one in a region of low horizontal strain rate (;10 6 s 1), the second in a region of intermediate 2 2 horizontal strain rate (;10 5 s 1). Both experiments lasted ;6 days, covering spatial scales of 1–10 and 1–50 km for the low and intermediate strain rate regimes, respectively. Diapycnal diffusivities estimated from 26 2 21 2 21 the two experiments were kz 5 (2–5) 3 10 m s , while isopycnal diffusivities were kH 5 (0.2–3) m s , with the range in kH being less a reflection of site-to-site variability, and more due to uncertainties in the background strain rate acting on the patch combined with uncertain time dependence. The Site I (low strain) experiment exhibited minimal stretching, elongating to approximately 10 km over 6 days while maintaining a width of ;5 km, and with a notable vertical tilt in the meridional direction. By contrast, the Site II (inter- mediate strain) experiment exhibited significant stretching, elongating to more than 50 km in length and advecting more than 150 km while still maintaining a width of order 3–5 km. -
An Unconditionally Stable Scheme for the Shallow Water Equations*
810 MONTHLY WEATHER REVIEW VOLUME 128 An Unconditionally Stable Scheme for the Shallow Water Equations* MOSHE ISRAELI Computer Science Department, Technion, Haifa, Israel NAOMI H. NAIK AND MARK A. CANE Lamont-Doherty Earth Observatory, Columbia University, Palisades, New York (Manuscript received 24 September 1998, in ®nal form 1 March 1999) ABSTRACT A ®nite-difference scheme for solving the linear shallow water equations in a bounded domain is described. Its time step is not restricted by a Courant±Friedrichs±Levy (CFL) condition. The scheme, known as Israeli± Naik±Cane (INC), is the offspring of semi-Lagrangian (SL) schemes and the Cane±Patton (CP) algorithm. In common with the latter it treats the shallow water equations implicitly in y and with attention to wave propagation in x. Unlike CP, it uses an SL-like approach to the zonal variations, which allows the scheme to apply to the full primitive equations. The great advantage, even in problems where quasigeostrophic dynamics are appropriate in the interior, is that the INC scheme accommodates complete boundary conditions. 1. Introduction is easy to code and boundary conditions for the discre- The two-dimensional linearized shallow water equa- tized equations are fairly natural to impose. At the other tions represent the evolution of small perturbations in end of the spectrum, the CP algorithm is speci®cally the ¯ow ®eld of a shallow basin on a rotating sphere. designed with the characteristics of the physics of the Our interest in these model equations arises from our equatorial ocean dynamics in mind. By separating the interest in solving for the motions in a linear beta-plane free modes into the eastward propagating Kelvin mode deep ocean. -
Geophysical Fluid Dynamics, Nonautonomous Dynamical Systems, and the Climate Sciences
Geophysical Fluid Dynamics, Nonautonomous Dynamical Systems, and the Climate Sciences Michael Ghil and Eric Simonnet Abstract This contribution introduces the dynamics of shallow and rotating flows that characterizes large-scale motions of the atmosphere and oceans. It then focuses on an important aspect of climate dynamics on interannual and interdecadal scales, namely the wind-driven ocean circulation. Studying the variability of this circulation and slow changes therein is treated as an application of the theory of nonautonomous dynamical systems. The contribution concludes by discussing the relevance of these mathematical concepts and methods for the highly topical issues of climate change and climate sensitivity. Michael Ghil Ecole Normale Superieure´ and PSL Research University, Paris, FRANCE, and University of California, Los Angeles, USA, e-mail: [email protected] Eric Simonnet Institut de Physique de Nice, CNRS & Universite´ Coteˆ d’Azur, Nice Sophia-Antipolis, FRANCE, e-mail: [email protected] 1 Chapter 1 Effects of Rotation The first two chapters of this contribution are dedicated to an introductory review of the effects of rotation and shallowness om large-scale planetary flows. The theory of such flows is commonly designated as geophysical fluid dynamics (GFD), and it applies to both atmospheric and oceanic flows, on Earth as well as on other planets. GFD is now covered, at various levels and to various extents, by several books [36, 60, 72, 107, 120, 134, 164]. The virtue, if any, of this presentation is its brevity and, hopefully, clarity. It fol- lows most closely, and updates, Chapters 1 and 2 in [60]. The intended audience in- cludes the increasing number of mathematicians, physicists and statisticians that are becoming interested in the climate sciences, as well as climate scientists from less traditional areas — such as ecology, glaciology, hydrology, and remote sensing — who wish to acquaint themselves with the large-scale dynamics of the atmosphere and oceans. -
MAR 542 – Fundamentals of Atmosphere and Ocean Dynamics Instructor: Marat Khairoutdinov Room: 158 Endeavour Time: Tuesdays and Thursday 11:30 AM – 12:50 PM
MAR 542 – Fundamentals of Atmosphere and Ocean Dynamics Instructor: Marat Khairoutdinov Room: 158 Endeavour Time: Tuesdays and Thursday 11:30 AM – 12:50 PM Text: Atmosphere, Ocean, and Climate Dynamics: An Introductory Text By John R. Marshall and R. Alan Plumb, Academic Press 2008 This course serves as an introduction to atmosphere and ocean dynamics. It is required of first-year atmospheric science graduate students, and it is recommended for first-year physical oceanography students. It assumes a working knowledge of differential and integral calculus, including partial derivatives and simple differential equations. Its purpose is to prepare students in atmospheric sciences and physical oceanography to move onto more advanced courses in these areas, as well as to acquaint each other with some fundamental aspects of dynamics applied to geophysical fluids outside your area of specialization. It is anticipated that the entire book will be covered. The chapter contents of this text are as follows, but some other topics will also be covered. 1. Characteristics of the atmosphere 2. The global energy balance 3. The vertical structure of the atmosphere 4. Convection 5. The meridional structure of the atmosphere 6. The equations of fluid motion 7. Balanced flow 8. The general circulation of the atmosphere 9. The ocean and its circulation 10. The wind-driven circulation 11. The thermohaline circulation of the ocean 12. Climate and climate variability • !"#$"%"&'"()*"+(,&-.)*/*0-",+--"1-"2*3&4"5$"6,7" • 8+9:";&<*/-"+2&=(">$"%"&'"()*"?+/()0-"-=/'+;*7" • @)*"+<*/+A*":*.()"&'"()*"&;*+9-"1-"+2&=("B"6,7" • !C$"%"&'"()*"?+/()0-"3+9:"1-"19"()*"D&/()*/9"E*,1-.)*/*7" Atmosphere is very thin: 99.9% of mass is below 50 km Compared to the Earth’s radius (6500 km), it is only 1% which is comparable to the thickness of an apple’s skin Thus, the synoptic-scale systems are quasi-two-dimensional! Vertical structure of the atmosphere Pressure (mb) 0.001 0.01 0.1 1 10 100 1000 Permanent vs. -
Chapter 5 Lecture
ChapterChapter 1 5 Clickers Lecture Essentials of Oceanography Eleventh Edition Water and Seawater Alan P. Trujillo Harold V. Thurman © 2014 Pearson Education, Inc. Chapter Overview • Water has many unique thermal and dissolving properties. • Seawater is mostly water molecules but has dissolved substances. • Ocean water salinity, temperature, and density vary with depth. © 2014 Pearson Education, Inc. Water on Earth • Presence of water on Earth makes life possible. • Organisms are mostly water. © 2014 Pearson Education, Inc. Atomic Structure • Atoms – building blocks of all matter • Subatomic particles – Protons – Neutrons – Electrons • Number of protons distinguishes chemical elements © 2014 Pearson Education, Inc. Molecules • Molecule – Two or more atoms held together by shared electrons – Smallest form of a substance © 2014 Pearson Education, Inc. Water molecule • Strong covalent bonds between one hydrogen (H) and two oxygen (O) atoms • Both H atoms on same side of O atom – Bent molecule shape gives water its unique properties • Dipolar © 2014 Pearson Education, Inc. Hydrogen Bonding • Polarity means small negative charge at O end • Small positive charge at H end • Attraction between positive and negative ends of water molecules to each other or other ions © 2014 Pearson Education, Inc. Hydrogen Bonding • Hydrogen bonds are weaker than covalent bonds but still strong enough to contribute to – Cohesion – molecules sticking together – High water surface tension – High solubility of chemical compounds in water – Unusual thermal properties of water – Unusual density of water © 2014 Pearson Education, Inc. Water as Solvent • Water molecules stick to other polar molecules. • Electrostatic attraction produces ionic bond . • Water can dissolve almost anything – universal solvent © 2014 Pearson Education, Inc. Water’s Thermal Properties • Water is solid, liquid, and gas at Earth’s surface. -
Mix It Up, Mix It Down , Volume 1, a Quarterly 22, Number the O Journal of Intriguing Implications of Ocean Layering
or collective redistirbution of any portion of this article by photocopy machine, reposting, or other means is permitted only with the approval of The approval portionthe ofwith any articlepermitted only photocopy by is of machine, reposting, this means or collective or other redistirbution This article has This been published in HANDS-ON OCEANOGRAPHY Oceanography Mix it Up, Mix it Down journal of The 22, Number 1, a quarterly , Volume Intriguing Implications of Ocean Layering BY PETER J.S. FRANKS AND SHARON E.R. FRANKS O ceanography ceanography PURPOSE OF ACTIVITY The density increase between the surface waters and the S Using a physical simulation, we explore the vertical density deep waters is often confined to a few relatively thin layers ociety. structure within the ocean and how layering (density stratifica- known as pycnoclines. Most ocean basins have a permanent © 2009 by The 2009 by tion) controls water motion, impedes nutrient transport, and pycnocline between about 500 and 1000-m depth, and a sea- regulates biological productivity. Our demonstration enables sonal pycnocline that forms during the summer between about O students to visualize the formation of horizontal layers in the 20 and 100-m depth. ceanography ocean’s interior and the slow undulation of large-amplitude Small density differences between ocean layers reduce the O ceanography ceanography internal waves. We show that stratification limits the vertical gravitational force acting on a layer. The reduced gravity allows S ociety. ociety. transport of energy and nutrients. The region of strong vertical waves inside the ocean—internal waves—to achieve amplitudes A density gradient—the pycnocline—is a barrier to the downward of tens of meters.