Variability in the Sea Surface Temperature Gradient and Its Impacts on Chlorophyll-A Concentration in the Kuroshio Extension
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PICES Sci. Rep. No. 2, 1995
TABLE OF CONTENTS Page FOREWORD vii Part 1. GENERAL INTRODUCTION AND RECOMMENDATIONS 1.0 RECOMMENDATIONS FOR INTERNATIONAL COOPERATION IN THE OKHOTSK SEA AND KURIL REGION 3 1.1 Okhotsk Sea water mass modification 3 1.1.1Dense shelf water formation in the northwestern Okhotsk Sea 3 1.1.2Soya Current study 4 1.1.3East Sakhalin Current and anticyclonic Kuril Basin flow 4 1.1.4West Kamchatka Current 5 1.1.5Tides and sea level in the Okhotsk Sea 5 1.2 Influence of Okhotsk Sea waters on the subarctic Pacific and Oyashio 6 1.2.1Kuril Island strait transports (Bussol', Kruzenshtern and shallower straits) 6 1.2.2Kuril region currents: the East Kamchatka Current, the Oyashio and large eddies 7 1.2.3NPIW transport and formation rate in the Mixed Water Region 7 1.3 Sea ice analysis and forecasting 8 2.0 PHYSICAL OCEANOGRAPHIC OBSERVATIONS 9 2.1 Hydrographic observations (bottle and CTD) 9 2.2 Direct current observations in the Okhotsk and Kuril region 11 2.3 Sea level measurements 12 2.4 Sea ice observations 12 2.5 Satellite observations 12 Part 2. REVIEW OF OCEANOGRAPHY OF THE OKHOTSK SEA AND OYASHIO REGION 15 1.0 GEOGRAPHY AND PECULIARITIES OF THE OKHOTSK SEA 16 2.0 SEA ICE IN THE OKHOTSK SEA 17 2.1 Sea ice observations in the Okhotsk Sea 17 2.2 Ease of ice formation in the Okhotsk Sea 17 2.3 Seasonal and interannual variations of sea ice extent 19 2.3.1Gross features of the seasonal variation in the Okhotsk Sea 19 2.3.2Sea ice thickness 19 2.3.3Polynyas and open water 19 2.3.4Interannual variability 20 2.4 Sea ice off the coast of Hokkaido 21 -
Pressure Gradient Force Examples of Pressure Gradient Hurricane Andrew, 1992 Extratropical Cyclone
4/29/2011 Chapter 7: Forces and Force Balances Forces that Affect Atmospheric Motion Pressure gradient force Fundamental force - Gravitational force FitiFrictiona lfl force Centrifugal force Apparent force - Coriolis force • Newton’s second law of motion states that the rate of change of momentum (i.e., the acceleration) of an object , as measured relative relative to coordinates fixed in space, equals the sum of all the forces acting. • For atmospheric motions of meteorological interest, the forces that are of primary concern are the pressure gradient force, the gravitational force, and friction. These are the • Forces that Affect Atmospheric Motion fundamental forces. • Force Balance • For a coordinate system rotating with the earth, Newton’s second law may still be applied provided that certain apparent forces, the centrifugal force and the Coriolis force, are • Geostrophic Balance and Jetstream ESS124 included among the forces acting. ESS124 Prof. Jin-Jin-YiYi Yu Prof. Jin-Jin-YiYi Yu Pressure Gradient Force Examples of Pressure Gradient Hurricane Andrew, 1992 Extratropical Cyclone (from Meteorology Today) • PG = (pressure difference) / distance • Pressure gradient force goes from high pressure to low pressure. • Closely spaced isobars on a weather map indicate steep pressure gradient. ESS124 ESS124 Prof. Jin-Jin-YiYi Yu Prof. Jin-Jin-YiYi Yu 1 4/29/2011 Gravitational Force Pressure Gradients • • Pressure Gradients – The pressure gradient force initiates movement of atmospheric mass, widfind, from areas o fhihf higher to areas o flf -
Chapter 5. Meridional Structure of the Atmosphere 1
Chapter 5. Meridional structure of the atmosphere 1. Radiative imbalance 2. Temperature • See how the radiative imbalance shapes T 2. Temperature: potential temperature 2. Temperature: equivalent potential temperature 3. Humidity: specific humidity 3. Humidity: saturated specific humidity 3. Humidity: saturated specific humidity Last time • Saturated adiabatic lapse rate • Equivalent potential temperature • Convection • Meridional structure of temperature • Meridional structure of humidity Today’s topic • Geopotential height • Wind 4. Pressure / geopotential height • From a hydrostatic balance and perfect gas law, @z RT = @p − gp ps T dp z(p)=R g p Zp • z(p) is called geopotential height. • If we assume that T and g does not vary a lot with p, geopotential height is higher when T increases. 4. Pressure / geopotential height • If we assume that g and T do not vary a lot with p, RT z(p)= (ln p ln p) g s − • z increases as p decreases. • Higher T increases geopotential height. 4. Pressure / geopotential height • Geopotential height is lower at the low pressure system. • Or the high pressure system corresponds to the high geopotential height. • T tends to be low in the region of low geopotential height. 4. Pressure / geopotential height The mean height of the 500 mbar surface in January , 2003 4. Pressure / geopotential height • We can discuss about the slope of the geopotential height if we know the temperature. R z z = (T T )(lnp ln p) warm − cold g warm − cold s − • We can also discuss about the thickness of an atmospheric layer if we know the temperature. RT z z = (ln p ln p ) p1 − p2 g 2 − 1 4. -
Oceanographic Structure in the Bering Sea
Title OCEANOGRAPHIC STRUCTURE IN THE BERING SEA Author(s) OHTANI, Kiyotaka Citation MEMOIRS OF THE FACULTY OF FISHERIES HOKKAIDO UNIVERSITY, 21(1), 65-106 Issue Date 1973-10 Doc URL http://hdl.handle.net/2115/21855 Type bulletin (article) File Information 21(1)_P65-106.pdf Instructions for use Hokkaido University Collection of Scholarly and Academic Papers : HUSCAP OCEANOGRAPHIC STRUCTURE IN THE BERING SEA Kiyotaka OHTANI Faculty of Fisherie8, Hokkaido Univer8ity, Hakodate, Japan Contents 1. Introduction ..•••••....•.•.•...•.•••••.....•.••.•.•.•..••......... 65 1. Preface ...................................................... 65 2. Subarctic region ............................................. 66 3. Sources of data . .. 67 4. Bottom configuration ............................................ 68 II. Waters Coming into the Bering Sea from the Pacific Ocean .............. 70 ill. Current Pattern in the Bering Sea . .. 73 IV. Waters in the Bering Sea Basin . .. 76 1. Vertical structure of the basin water ..... .. .. .. .. .. .. .. .. .. ... 76 2. Types of vertical distribution of salinity and temperature .. .. 81 3. Process of formation of various Types .............................. 82 V. Waters on the Continental Shelf ...................................... 85 1. Horizontal distribution of salinity and temperature ............... 85 2. Vertical section ............................................... 91 3. Classification to type of vertical structure ....................... 94 VI. Interaction between the Shelf Waters and the Basin Waters -
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]]. -
Pressure Gradient Force
2/2/2015 Chapter 7: Forces and Force Balances Forces that Affect Atmospheric Motion Pressure gradient force Fundamental force - Gravitational force Frictional force Centrifugal force Apparent force - Coriolis force • Newton’s second law of motion states that the rate of change of momentum (i.e., the acceleration) of an object, as measured relative to coordinates fixed in space, equals the sum of all the forces acting. • For atmospheric motions of meteorological interest, the forces that are of primary concern are the pressure gradient force, the gravitational force, and friction. These are the • Forces that Affect Atmospheric Motion fundamental forces. • Force Balance • For a coordinate system rotating with the earth, Newton’s second law may still be applied provided that certain apparent forces, the centrifugal force and the Coriolis force, are • Geostrophic Balance and Jetstream ESS124 included among the forces acting. ESS124 Prof. Jin-Yi Yu Prof. Jin-Yi Yu Pressure Gradient Force Examples of Pressure Gradient Hurricane Andrew, 1992 Extratropical Cyclone (from Meteorology Today) • PG = (pressure difference) / distance • Pressure gradient force goes from high pressure to low pressure. • Closely spaced isobars on a weather map indicate steep pressure gradient. ESS124 ESS124 Prof. Jin-Yi Yu Prof. Jin-Yi Yu 1 2/2/2015 Balance of Force in the Vertical: Pressure Gradients Hydrostatic Balance • Pressure Gradients – The pressure gradient force initiates movement of atmospheric mass, wind, from areas of higher to areas of lower pressure Vertical -
Late Pleistocene and Holocene Paleoenvironments of the North Pacific Coast
Quaternary Science Reviews, Vol. 14, pp. 449-47 1, 1995. Pergamon Copyright 0 1995 Elsevier Science Ltd. Printed in Great Britain. All rights reserved. 0277-3791l95 $29.00 0277-3791(9S)ooo&X LATE PLEISTOCENE AND HOLOCENE PALEOENVIRONMENTS OF THE NORTH PACIFIC COAST DANIEL H. MANN* and THOMAS D. HAMILTON? *Alaska Quaternary Center; University of Alaska Museum, 907 Yukon Drive, Fairbanks, AK 99775, U.S.A. I-US. Geological Survey, 4200 University Drive, Anchorage, AK 99508, U.S.A. Abstract - Unlike the North Atlantic, the North Pacific Ocean probably remained free of sea ice during the last glacial maximum (LGM), 22,000 to 17,000 BP. Following a eustatic low in sea level of ca. -120 m at 19,000 BP, a marine transgression had flooded the Bering and Chukchi shelves by 10,000 BP. Post-glacial sea-level history varied widely in other parts of the North QSR Pacific coastline according to the magnitude and timing of local tectonism and glacio-isostatic rebound. Glaciers covered much of the continental shelf between the Alaska Peninsula and British Columbia during the LGM. Maximum glacier extent during the LGM was out of phase between southern Alaska and southern British Columbia with northern glaciers reaching their outer limits earlier, between 23,000 and 16,000 BP, compared to 15,00&14,000 BP in the south. Glacier retreat was also time-transgressive, with glaciers retreating from the continental shelf of southern Alaska before 16,000 BP but not until 14,000-13,000 BP in southwestern British Columbia. Major climat- ic transitions occurred in the North Pacific at 24,000-22,000, 15,000-13,000 and 11,OOO-9000 BP. -
Chapter 7 Isopycnal and Isentropic Coordinates
Chapter 7 Isopycnal and Isentropic Coordinates The two-dimensional shallow water model can carry us only so far in geophysical uid dynam- ics. In this chapter we begin to investigate fully three-dimensional phenomena in geophysical uids using a type of model which builds on the insights obtained using the shallow water model. This is done by treating a three-dimensional uid as a stack of layers, each of con- stant density (the ocean) or constant potential temperature (the atmosphere). Equations similar to the shallow water equations apply to each layer, and the layer variable (density or potential temperature) becomes the vertical coordinate of the model. This is feasible because the requirement of convective stability requires this variable to be monotonic with geometric height, decreasing with height in the case of water density in the ocean, and increasing with height with potential temperature in the atmosphere. As long as the slope of model layers remains small compared to unity, the coordinate axes remain close enough to orthogonal to ignore the complex correction terms which otherwise appear in non-orthogonal coordinate systems. 7.1 Isopycnal model for the ocean The word isopycnal means constant density. Recall that an assumption behind the shallow water equations is that the water have uniform density. For layered models of a three- dimensional, incompressible uid, we similarly assume that each layer is of uniform density. We now see how the momentum, continuity, and hydrostatic equations appear in the context of an isopycnal model. 7.1.1 Momentum equation Recall that the horizontal (in terms of z) pressure gradient must be calculated, since it appears in the horizontal momentum equations. -
1050 Clicker Questions Exam 1
Answers to Clicker Questions Chapter 1 What component of the atmosphere is most important to weather? A. Nitrogen B. Oxygen C. Carbon dioxide D. Ozone E. Water What location would have the lowest surface pressure? A. Chicago, Illinois B. Denver, Colorado C. Miami, Florida D. Dallas, Texas E. Los Angeles, California What is responsible for the distribution of surface pressure shown on the previous map? A. Temperature B. Elevation C. Weather D. Population If the relative humidity and the temperature at Denver, Colorado, compared to that at Miami, Florida, is as shown below, how much absolute water vapor is in the air between these two locations? A. Denver has more absolute water vapor B. Miami has more absolute water vapor C. Both have the same amount of water vapor Denver 10°C Air temperature 50% Relative humidity Miami 20°C Air temperature 50% Relative humidity Chapter 2 Convert our local time of 9:45am MST to UTC A. 0945 UTC B. 1545 UTC C. 1645 UTC D. 2345 UTC A weather observation made at 0400 UTC on January 10th, would correspond to what local time (MST)? A. 11:00am January10th B. 9:00pm January 10th C. 10:00pm January 9th D. 9:00pm January 9th A weather observation made at 0600 UTC on July 10th, would correspond to what local time (MDT)? A. 12:00am July 10th B. 12:00pm July 10th C. 1:00pm July 10th D. 11:00pm July 9th A rawinsonde measures all of the following variables except: Temperature Dew point temperature Precipitation Wind speed Wind direction What can a Doppler weather radar measure? Position of precipitation Intensity of precipitation Radial wind speed All of the above Only a and b In this sounding from Denver, the tropopause is located at a pressure of approximately: 700 mb 500 mb 300 mb 100 mb Which letter on this radar reflectivity image has the highest rainfall rate? A B C D C D B A Chapter 3 • Using this surface station model, what is the temperature? (Assume it’s in the US) 26 °F 26 °C 28 °F 28 °C 22.9 °F Using this surface station model, what is the current sea level pressure? A. -
Effect of Pleistocene Glaciation Upon Oceanographic Characteristics of the North Pacific Ocean and Bering Sea
Deep-Sea Research, Vol. 30, No. 8A, pp. 851 to 869, 1983. 0198-0149/83 $3.00 + 0.00 Printed in Great Britain. (c) 1983 Pergamon Press Ltd. Effect of Pleistocene glaciation upon oceanographic characteristics of the North Pacific Ocean and Bering Sea CONSTANCE SANCETTA* (Received 23 October 1982; in revisedform 28 January 1983; accepted 28 April 1983) Abstract--During intervals of Pleistocene glaciation, insolation of the high-latitude northern hemisphere was lower than today, particularly during summer. Growth of continental ice sheets resulted in a lowering of sea level by more than 100 m in the Bering Sea. As a result, the Bering Strait was closed and most of the Bering continental shelf exposed. A proposed model predicts that (1) sea-ice formation would occur along the (modern) outer continental shelf, (2)advection would transport the sea ice over the deep basin, and (3) brine would flow into the basin at some inter- mediate depth to enhance the halocline. The result would be a low-salinity surface layer with a cold, thick halocline and reduced vertical mixing. Diatom microfossils and lithologic changes in sediment cores from the North Pacific Ocean and Bering Sea support the model and suggest that the proposed oceanographic conditions extended into the North Pacific, where the cold low-salinity laycr was enhanced by meltwater from continentally derived icebergs. INTRODUCTION IN THE last decade, marine geologists have begun to make observations and interpretations bearing on the physical oceanography and climate of the earth in the past (e.g., CLIMAP, 1976; Coauss, 1979; KEIGWIN, BENDER and KENNETT, 1979). -
Strengthening of the Kuroshio Current by Intensifying Tropical Cyclones
RESEARCH OCEAN CIRCULATION geostrophic adjustment, was first considered by Rossby in 1938 (19) and has since been in- Strengthening of the Kuroshio current by intensifying vestigated in a variety of contexts both linear and nonlinear (20–23). Common to all those tropical cyclones studies is that the flows in question hold less energy at their end states than they do initially, Yu Zhang1*, Zhengguang Zhang1, Dake Chen2,3, Bo Qiu4, Wei Wang1 and energy is dispersed in the form of inertial gravity waves ( 19, 24). It is therefore antici- A positive feedback mechanism between tropical cyclones (TCs) and climate warming can be pated that eddies under the influence of strong seen by examining TC-induced energy and potential vorticity (PV) changes of oceanic geostrophic storms may be perturbed and subsequently eddies. We found that substantial dissipation of eddies, with a strong bias toward dissipation of undertake adjustment processes that atten- anticyclonic eddies, is directly linked to TC activity. East of Taiwan, where TCs show a remarkable uate them (25). intensifying trend in recent decades, the ocean exhibits a corresponding upward trend of positive Evidence continues to mount that both PV anomalies. Carried westward by eddies, increasing numbers of positive PV anomalies impinge on mechanisms described above exist, working the Kuroshio current, causing the mean current to accelerate downstream. This acts in opposition together to reduce the strength of anticyclonic to decreasing basin-scale wind stress and has a potentially important warming impact on the eddies but acting against each other in chang- extratropical ocean and climate. ing cyclonic eddies. Which process dominates, and what overall influence the TCs exert on an underlying eddy field, remains unclear. -
Temperature Gradient
Temperature Gradient Derivation of dT=dr In Modern Physics it is shown that the pressure of a photon gas in thermodynamic equilib- rium (the radiation pressure PR) is given by the equation 1 P = aT 4; (1) R 3 with a the radiation constant, which is related to the Stefan-Boltzman constant, σ, and the speed of light in vacuum, c, via the equation 4σ a = = 7:565731 × 10−16 J m−3 K−4: (2) c Hence, the radiation pressure gradient is dP 4 dT R = aT 3 : (3) dr 3 dr Referring to our our discussion of opacity, we can write dF = −hκiρF; (4) dr where F = F (r) is the net outward flux (integrated over all wavelengths) of photons at a distance r from the center of the star, and hκi some properly taken average value of the opacity. The flux F is related to the luminosity through the equation L(r) F (r) = : (5) 4πr2 Considering that pressure is force per unit area, and force is a rate of change of linear momentum, and photons carry linear momentum equal to their energy divided by c, PR and F obey the equation 1 P = F (r): (6) R c Differentiation with respect to r gives dP 1 dF R = : (7) dr c dr Combining equations (3), (4), (5) and (7) then gives 1 L(r) 4 dT − hκiρ = aT 3 ; (8) c 4πr2 3 dr { 2 { which finally leads to dT 3hκiρ 1 1 = − L(r): (9) dr 16πac T 3 r2 Equation (9) gives the local (i.e.