Nomaly Patterns in the Near-Surface Baroclinicity And
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Comparing Historical and Modern Methods of Sea Surface Temperature
EGU Journal Logos (RGB) Open Access Open Access Open Access Advances in Annales Nonlinear Processes Geosciences Geophysicae in Geophysics Open Access Open Access Natural Hazards Natural Hazards and Earth System and Earth System Sciences Sciences Discussions Open Access Open Access Atmospheric Atmospheric Chemistry Chemistry and Physics and Physics Discussions Open Access Open Access Atmospheric Atmospheric Measurement Measurement Techniques Techniques Discussions Open Access Open Access Biogeosciences Biogeosciences Discussions Open Access Open Access Climate Climate of the Past of the Past Discussions Open Access Open Access Earth System Earth System Dynamics Dynamics Discussions Open Access Geoscientific Geoscientific Open Access Instrumentation Instrumentation Methods and Methods and Data Systems Data Systems Discussions Open Access Open Access Geoscientific Geoscientific Model Development Model Development Discussions Open Access Open Access Hydrology and Hydrology and Earth System Earth System Sciences Sciences Discussions Open Access Ocean Sci., 9, 683–694, 2013 Open Access www.ocean-sci.net/9/683/2013/ Ocean Science doi:10.5194/os-9-683-2013 Ocean Science Discussions © Author(s) 2013. CC Attribution 3.0 License. Open Access Open Access Solid Earth Solid Earth Discussions Comparing historical and modern methods of sea surface Open Access Open Access The Cryosphere The Cryosphere temperature measurement – Part 1: Review of methods, Discussions field comparisons and dataset adjustments J. B. R. Matthews School of Earth and Ocean Sciences, University of Victoria, Victoria, BC, Canada Correspondence to: J. B. R. Matthews ([email protected]) Received: 3 August 2012 – Published in Ocean Sci. Discuss.: 20 September 2012 Revised: 31 May 2013 – Accepted: 12 June 2013 – Published: 30 July 2013 Abstract. Sea surface temperature (SST) has been obtained 1 Introduction from a variety of different platforms, instruments and depths over the past 150 yr. -
Potential Vorticity
POTENTIAL VORTICITY Roger K. Smith March 3, 2003 Contents 1 Potential Vorticity Thinking - How might it help the fore- caster? 2 1.1Introduction............................ 2 1.2WhatisPV-thinking?...................... 4 1.3Examplesof‘PV-thinking’.................... 7 1.3.1 A thought-experiment for understanding tropical cy- clonemotion........................ 7 1.3.2 Kelvin-Helmholtz shear instability . ......... 9 1.3.3 Rossby wave propagation in a β-planechannel..... 12 1.4ThestructureofEPVintheatmosphere............ 13 1.4.1 Isentropicpotentialvorticitymaps........... 14 1.4.2 The vertical structure of upper-air PV anomalies . 18 2 A Potential Vorticity view of cyclogenesis 21 2.1PreliminaryIdeas......................... 21 2.2SurfacelayersofPV....................... 21 2.3Potentialvorticitygradientwaves................ 23 2.4 Baroclinic Instability . .................... 28 2.5 Applications to understanding cyclogenesis . ......... 30 3 Invertibility, iso-PV charts, diabatic and frictional effects. 33 3.1 Invertibility of EPV ........................ 33 3.2Iso-PVcharts........................... 33 3.3Diabaticandfrictionaleffects.................. 34 3.4Theeffectsofdiabaticheatingoncyclogenesis......... 36 3.5Thedemiseofcutofflowsandblockinganticyclones...... 36 3.6AdvantageofPVanalysisofcutofflows............. 37 3.7ThePVstructureoftropicalcyclones.............. 37 1 Chapter 1 Potential Vorticity Thinking - How might it help the forecaster? 1.1 Introduction A review paper on the applications of Potential Vorticity (PV-) concepts by Brian -
OCEAN WARMING • the Ocean Absorbs Most of the Excess Heat from Greenhouse Gas Emissions, Leading to Rising Ocean Temperatures
NOVEMBER 2017 OCEAN WARMING • The ocean absorbs most of the excess heat from greenhouse gas emissions, leading to rising ocean temperatures. • Increasing ocean temperatures affect marine species and ecosystems. Rising temperatures cause coral bleaching and the loss of breeding grounds for marine fishes and mammals. • Rising ocean temperatures also affect the benefits humans derive from the ocean – threatening food security, increasing the prevalence of diseases and causing more extreme weather events and the loss of coastal protection. • Achieving the mitigation targets set by the Paris Agreement on climate change and limiting the global average temperature increase to well below 2°C above pre-industrial levels is crucial to prevent the massive, irreversible impacts of ocean warming on marine ecosystems and their services. • Establishing marine protected areas and putting in place adaptive measures, such as precautionary catch limits to prevent overfishing, can protect ocean ecosystems and shield humans from the effects of ocean warming. The distribution of excess heat in the ocean is not What is the issue? uniform, with the greatest ocean warming occurring in The ocean absorbs vast quantities of heat as a result the Southern Hemisphere and contributing to the of increased concentrations of greenhouse gases in subsurface melting of Antarctic ice shelves. the atmosphere, mainly from fossil fuel consumption. The Fifth Assessment Report published by the Intergovernmental Panel on Climate Change (IPCC) in 2013 revealed that the ocean had absorbed more than 93% of the excess heat from greenhouse gas emissions since the 1970s. This is causing ocean temperatures to rise. Data from the US National Oceanic and Atmospheric Administration (NOAA) shows that the average global sea surface temperature – the temperature of the upper few metres of the ocean – has increased by approximately 0.13°C per decade over the past 100 years. -
A Review of Ocean/Sea Subsurface Water Temperature Studies from Remote Sensing and Non-Remote Sensing Methods
water Review A Review of Ocean/Sea Subsurface Water Temperature Studies from Remote Sensing and Non-Remote Sensing Methods Elahe Akbari 1,2, Seyed Kazem Alavipanah 1,*, Mehrdad Jeihouni 1, Mohammad Hajeb 1,3, Dagmar Haase 4,5 and Sadroddin Alavipanah 4 1 Department of Remote Sensing and GIS, Faculty of Geography, University of Tehran, Tehran 1417853933, Iran; [email protected] (E.A.); [email protected] (M.J.); [email protected] (M.H.) 2 Department of Climatology and Geomorphology, Faculty of Geography and Environmental Sciences, Hakim Sabzevari University, Sabzevar 9617976487, Iran 3 Department of Remote Sensing and GIS, Shahid Beheshti University, Tehran 1983963113, Iran 4 Department of Geography, Humboldt University of Berlin, Unter den Linden 6, 10099 Berlin, Germany; [email protected] (D.H.); [email protected] (S.A.) 5 Department of Computational Landscape Ecology, Helmholtz Centre for Environmental Research UFZ, 04318 Leipzig, Germany * Correspondence: [email protected]; Tel.: +98-21-6111-3536 Received: 3 October 2017; Accepted: 16 November 2017; Published: 14 December 2017 Abstract: Oceans/Seas are important components of Earth that are affected by global warming and climate change. Recent studies have indicated that the deeper oceans are responsible for climate variability by changing the Earth’s ecosystem; therefore, assessing them has become more important. Remote sensing can provide sea surface data at high spatial/temporal resolution and with large spatial coverage, which allows for remarkable discoveries in the ocean sciences. The deep layers of the ocean/sea, however, cannot be directly detected by satellite remote sensors. -
Deep Learning of Sea Surface Temperature Patterns to Identify Ocean Extremes
remote sensing Article Deep Learning of Sea Surface Temperature Patterns to Identify Ocean Extremes J. Xavier Prochaska 1,2,3,*,†,‡ , Peter C. Cornillon 4,‡ and David M. Reiman 5 1 Affiliate of the Department of Ocean Sciences, University of California, Santa Cruz, CA 95064, USA 2 Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA 3 Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), 5-1-5 Kashiwanoha, Kashiwa 277-8583, Japan 4 Graduate School of Oceanography, University of Rhode Island, Narragansett, RI 02882, USA; [email protected] 5 Department of Physics, University of California, Santa Cruz, CA 95064, USA; [email protected] * Correspondence: [email protected] † Current address: 1156 High St., University of California, Santa Cruz, CA 95064, USA. ‡ These authors contributed equally to this work. Abstract: We performed an OOD analysis of ∼12,000,000 semi-independent 128 × 128 pixel2 SST regions, which we define as cutouts, from all nighttime granules in the MODIS R2019 L2! public dataset to discover the most complex or extreme phenomena at the ocean’s surface. Our algorithm (ULMO) is a PAE, which combines two deep learning modules: (1) an autoencoder, trained on ∼150,000 random cutouts from 2010, to represent any input cutout with a 512-dimensional latent vector akin to a (non-linear) EOF analysis; and (2) a normalizing flow, which maps the autoencoder’s latent space distribution onto an isotropic Gaussian manifold. From the latter, we calculated a LL value for each cutout and defined outlier cutouts to be those in the lowest 0.1% of the distribution. -
January 2021
January 2021 Embargoed , 9 February 2021, 0900 GMT Current Situation and Outlook The 2020-2021 La Niña event appears to have peaked in October-December as a moderate strength event. The latest forecasts from the WMO Global Producing Centers of Long-Range Forecasts indicate a moderate likelihood (65%) that the La Niña event will continue into February-April. The odds shift rapidly thereafter, indicating a 70% chance that the tropical Pacific will return to ENSO-neutral conditions by the April- June 2021 season. The outlook for the second half of the year is currently uncertain. National Meteorological and Hydrological Services will closely monitor changes in the state of El Niño/Southern Oscillation (ENSO) over the coming months and provide updated outlooks. La Niña conditions have been in place since August-September 2020, according to both atmospheric and oceanic indicators. The sea surface temperature anomalies in the central/eastern-central equatorial Pacific reached peak magnitude during October-November 2020. The anomalies in the eastern-central Pacific have somewhat plateaued near -1.0 degree Celsius, with some minor fluctuations over the past several weeks. Cooler than normal sub- surface anomalies arrived in the eastern Pacific during the second quarter of 2020; they began to cool sea surface temperatures there and were subsequently reinforced by enhanced trade winds in the central/western-central equatorial Pacific. Cool anomalies persist in the sub-surface waters, but have weakened since the peak. Enhanced trade winds and stronger-than-average upper level westerly winds have been present in the tropical Pacific since mid-2020. Cloudiness and rainfall have been below average in the central and west-central tropical Pacific, and slightly above average around the Maritime Continent throughout the 2020-2021 La Niña. -
Sea-Surface Temperature and Climate
Current Issue Outline' 79-1 .. ·. : ,._...•• ~":r ·. w•: .('/> .v<jr. ~ ~.., ....,.. .• .• ·.. •.. "'#''1! .· ·.· .•.·~·.··~·· --'..• ·.· ..: ..•. :;. ·.·::'•.··.·. ~- ; ~'*· -c::.: . _- :_. ~- -~ . 't;- ..·. _- -- ~~ ~··.·.···· .. ··. ~.. () ·~ . • . • L'f-• ... r,.r£s C)f r Washington, D.C. r June Hl79 - -~ •,;" .. U.S. DEPARTMENT OF COMMERCE National Oceanic and Atmospheric Administration Environmental Data and Information Service Current Issue Outline 79-i Sea-Surface Temperature And Climate . Washington, D.C. · June 1979 Reprinted June 1980 U.S.----- -------------·--DEPARTMENT OF COMMERCE Juanita M. Kreps, Secretary NatiOriiJI qceiJnlc:.IJ~~ Atmospheric Administration Richard A, Frank, Administrator Environmental Data and Information Service thomas S. Austin, Director CURRENT ISSUE OUTLINE 79-1 SEA-SURFACE TEMPERATURE AND CLIMATE Current Issue Outlines have been developed by the Library and Information Services Division, Environmental Science Information Center, to provide objective background reviews on current topics of high general interest in marine or atmospheric science. Bibliographies of selected material are added so that the reader who wishes can pursue the subject in greater depth. Questions or comments should be directed to: User Services Branch, D822 Library and Information Services Division NOAA Rockville; MD 20852 Telephone number is (301) 443-8358. PREVIOUS TITLES IN THE.SERIES CIO 78-1 Icebergs For Use As Freshwater CIO 78-2 Harnessing Tidal Energy SEA-SURFACE TEMPERATURE AND CLIMATE Issue Definition Climati·c variations are likely to arise from complex interactions among the atmosphere, the oceans, and the Earth's surface. Empirical obser vations as well as studies using climate models have suggested that variation of oceanic conditions, especially variation in sea-surface temperatures, may be the key to understanding monthly and seasonal climatic anomaly patterns. -
Chapter 2 Approximate Thermodynamics
Chapter 2 Approximate Thermodynamics 2.1 Atmosphere Various texts (Byers 1965, Wallace and Hobbs 2006) provide elementary treatments of at- mospheric thermodynamics, while Iribarne and Godson (1981) and Emanuel (1994) present more advanced treatments. We provide only an approximate treatment which is accept- able for idealized calculations, but must be replaced by a more accurate representation if quantitative comparisons with the real world are desired. 2.1.1 Dry entropy In an atmosphere without moisture the ideal gas law for dry air is p = R T (2.1) ρ d where p is the pressure, ρ is the air density, T is the absolute temperature, and Rd = R/md, R being the universal gas constant and md the molecular weight of dry air. If moisture is present there are minor modications to this equation, which we ignore here. The dry entropy per unit mass of air is sd = Cp ln(T/TR) − Rd ln(p/pR) (2.2) where Cp is the mass (not molar) specic heat of dry air at constant pressure, TR is a constant reference temperature (say 300 K), and pR is a constant reference pressure (say 1000 hPa). Recall that the specic heats at constant pressure and volume (Cv) are related to the gas constant by Cp − Cv = Rd. (2.3) A variable related to the dry entropy is the potential temperature θ, which is dened Rd/Cp θ = TR exp(sd/Cp) = T (pR/p) . (2.4) The potential temperature is the temperature air would have if it were compressed or ex- panded (without condensation of water) in a reversible adiabatic fashion to the reference pressure pR. -
The Tephigram Introduction Meteorology Is the Study of the Physical State of the Atmosphere
The Tephigram Introduction Meteorology is the study of the physical state of the atmosphere. The atmosphere is a heat engine transporting energy from the warm ground to cooler locations, both vertically and horizontally. The driving force is solar radiation. Shortwave radiation is absorbed primarily at the surface; the working fluid is the atmosphere, which distributes heat by motion systems on all time and space scales; the heat sink is space, to which longwave radiation escapes. The Tephigram is one of a number of thermodynamic diagrams designed to aid in the interpretation of the temperature and humidity structure of the atmosphere and used widely throughout the world meteorological community. It has the property that equal areas on the diagram represent equal amounts of energy; this enables the calculation of a wide range of atmospheric processes to be carried out graphically. A blank tephigram is shown in figure 1; there are five principal quantities indicated by constant value lines: pressure, temperature, potential temperature (θ), saturation mixing ratio, and equivalent potential temperature (θe) for saturated air. Saturation mixing ratio: lines of constant saturation mixing ratio with respect to a plane water surface (g kg-1) Isotherms: lines of constant Isobars: lines of temperature (ºC) constant pressure (mb) Dry Adiabats: lines of constant potential temperature (ºC) Pseudo saturated wet adiabat: lines of constant equivalent potential temperature for saturated air parcels (ºC) Figure 1. The tephigram, with the principal quantities indicated. The principal axes of a tephigram are temperature and potential temperature; these are straight and perpendicular to each other, but rotated through about 45º anticlockwise so that lines of constant temperature run from bottom left to top right on the diagram. -
Dry Adiabatic Temperature Lapse Rate
ATMO 551a Fall 2010 Dry Adiabatic Temperature Lapse Rate As we discussed earlier in this class, a key feature of thick atmospheres (where thick means atmospheres with pressures greater than 100-200 mb) is temperature decreases with increasing altitude at higher pressures defining the troposphere of these planets. We want to understand why tropospheric temperatures systematically decrease with altitude and what the rate of decrease is. The first order explanation is the dry adiabatic lapse rate. An adiabatic process means no heat is exchanged in the process. For this to be the case, the process must be “fast” so that no heat is exchanged with the environment. So in the first law of thermodynamics, we can anticipate that we will set the dQ term equal to zero. To get at the rate at which temperature decreases with altitude in the troposphere, we need to introduce some atmospheric relation that defines a dependence on altitude. This relation is the hydrostatic relation we have discussed previously. In summary, the adiabatic lapse rate will emerge from combining the hydrostatic relation and the first law of thermodynamics with the heat transfer term, dQ, set to zero. The gravity side The hydrostatic relation is dP = −g ρ dz (1) which relates pressure to altitude. We rearrange this as dP −g dz = = α dP (2) € ρ where α = 1/ρ is known as the specific volume which is the volume per unit mass. This is the equation we will use in a moment in deriving the adiabatic lapse rate. Notice that € F dW dE g dz ≡ dΦ = g dz = g = g (3) m m m where Φ is known as the geopotential, Fg is the force of gravity and dWg is the work done by gravity. -
Introduction to Atmospheric Dynamics Chapter 2
Introduction to Atmospheric Dynamics Chapter 2 Paul A. Ullrich [email protected] Part 3: Buoyancy and Convection Vertical Structure This cooling with height is related to the dynamics of the atmosphere. The change of temperature with height is called the lapse rate. Defnition: The lapse rate is defned as the rate (for instance in K/km) at which temperature decreases with height. @T Γ ⌘@z Paul Ullrich Introduction to Atmospheric Dynamics March 2014 Lapse Rate For a dry adiabatic, stable, hydrostatic atmosphere the potential temperature θ does not vary in the vertical direction: @✓ =0 @z In a dry adiabatic, hydrostatic atmosphere the temperature T must decrease with height. How quickly does the temperature decrease? R/cp p0 Note: Use ✓ = T p ✓ ◆ Paul Ullrich Introduction to Atmospheric Dynamics March 2014 Lapse Rate The adiabac change in temperature with height is T @✓ @T g = + ✓ @z @z cp For dry adiabac, hydrostac atmosphere: @T g = Γd − @z cp ⌘ Defnition: The dry adiabatic lapse rate is defned as the g rate (for instance in K/km) at which the temperature of an Γd air parcel will decrease with height if raised adiabatically. ⌘ cp g 1 9.8Kkm− cp ⇡ Paul Ullrich Introduction to Atmospheric Dynamics March 2014 Lapse Rate This profle should be very close to the adiabatic lapse rate in a dry atmosphere. Paul Ullrich Introduction to Atmospheric Dynamics March 2014 Fundamentals Even in adiabatic motion, with no external source of heating, if a parcel moves up or down its temperature will change. • What if a parcel moves about a surface of constant pressure? • What if a parcel moves about a surface of constant height? If the atmosphere is in adiabatic balance, the temperature still changes with height. -
Stochastic Modelling of the Oceanic Eddies
Stochastic Modelling of the Oceanic Eddies Pavel S. Berloff Woods Hole Oceanographic Institution, USA [email protected] and Department of Applied Mathematics and Theoretical Physics, University of Cambridge, UK 1 Introduction It is widely recognized that the mesoscale oceanic eddies are capable of driving the large-scale oceanic currents. These eddies are generally not resolved in comprehensive oceanic General Circulation Models (GCMs), there- fore the models are rather inaccurate. Developing efficient mathematical models of the eddies is, arguably, the most important problem facing the modern physical oceanography. The eddy effects can be roughly groupped into two classes: dynamic and kinematic. The dynamic effects are associated with divergence of the eddy potential vorticity (PV) or momentum fluxes. The kinematic effects are associated with transport of material quantities. Below, some new stochastic models for both kinds of effects are discussed. The main advantage of the proposed model is their ability to simulate ubiquitous non-diffusive and anti-diffusive oceanic eddy effects, which are a fundamental obstacle in ocean circulation and turbulence closures. The results are tested against the double-gyre, fluid-dynamic ocean model that explicitly resolves the eddies (e.g., Siegel et al. 2001). 2 Dynamic Effects The random-forcing eddy model is developed in Berloff (2005a,b). The new diagnostic method is proposed, which is based on dynamical decomposition of the flow into the large-scale and eddy components. The method yields the time history of the eddy forcing, which can be used as additional, external forcing in the correspond- ing non-eddy-resolving model of the gyres. The main strength of this approach is in its dynamical consistency: the non-eddy-resolving solution driven by the eddy forcing history correctly approximates the original large- scale flow component.