Deep-Sea Research Part II: Topical Studies in Oceanography 2018 DOI
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Basic Concepts in Oceanography
Chapter 1 XA0101461 BASIC CONCEPTS IN OCEANOGRAPHY L.F. SMALL College of Oceanic and Atmospheric Sciences, Oregon State University, Corvallis, Oregon, United States of America Abstract Basic concepts in oceanography include major wind patterns that drive ocean currents, and the effects that the earth's rotation, positions of land masses, and temperature and salinity have on oceanic circulation and hence global distribution of radioactivity. Special attention is given to coastal and near-coastal processes such as upwelling, tidal effects, and small-scale processes, as radionuclide distributions are currently most associated with coastal regions. 1.1. INTRODUCTION Introductory information on ocean currents, on ocean and coastal processes, and on major systems that drive the ocean currents are important to an understanding of the temporal and spatial distributions of radionuclides in the world ocean. 1.2. GLOBAL PROCESSES 1.2.1 Global Wind Patterns and Ocean Currents The wind systems that drive aerosols and atmospheric radioactivity around the globe eventually deposit a lot of those materials in the oceans or in rivers. The winds also are largely responsible for driving the surface circulation of the world ocean, and thus help redistribute materials over the ocean's surface. The major wind systems are the Trade Winds in equatorial latitudes, and the Westerly Wind Systems that drive circulation in the north and south temperate and sub-polar regions (Fig. 1). It is no surprise that major circulations of surface currents have basically the same patterns as the winds that drive them (Fig. 2). Note that the Trade Wind System drives an Equatorial Current-Countercurrent system, for example. -
World Ocean Thermocline Weakening and Isothermal Layer Warming
applied sciences Article World Ocean Thermocline Weakening and Isothermal Layer Warming Peter C. Chu * and Chenwu Fan Naval Ocean Analysis and Prediction Laboratory, Department of Oceanography, Naval Postgraduate School, Monterey, CA 93943, USA; [email protected] * Correspondence: [email protected]; Tel.: +1-831-656-3688 Received: 30 September 2020; Accepted: 13 November 2020; Published: 19 November 2020 Abstract: This paper identifies world thermocline weakening and provides an improved estimate of upper ocean warming through replacement of the upper layer with the fixed depth range by the isothermal layer, because the upper ocean isothermal layer (as a whole) exchanges heat with the atmosphere and the deep layer. Thermocline gradient, heat flux across the air–ocean interface, and horizontal heat advection determine the heat stored in the isothermal layer. Among the three processes, the effect of the thermocline gradient clearly shows up when we use the isothermal layer heat content, but it is otherwise when we use the heat content with the fixed depth ranges such as 0–300 m, 0–400 m, 0–700 m, 0–750 m, and 0–2000 m. A strong thermocline gradient exhibits the downward heat transfer from the isothermal layer (non-polar regions), makes the isothermal layer thin, and causes less heat to be stored in it. On the other hand, a weak thermocline gradient makes the isothermal layer thick, and causes more heat to be stored in it. In addition, the uncertainty in estimating upper ocean heat content and warming trends using uncertain fixed depth ranges (0–300 m, 0–400 m, 0–700 m, 0–750 m, or 0–2000 m) will be eliminated by using the isothermal layer. -
The 17Th International Colloquium on Amphipoda
Biodiversity Journal, 2017, 8 (2): 391–394 MONOGRAPH The 17th International Colloquium on Amphipoda Sabrina Lo Brutto1,2,*, Eugenia Schimmenti1 & Davide Iaciofano1 1Dept. STEBICEF, Section of Animal Biology, via Archirafi 18, Palermo, University of Palermo, Italy 2Museum of Zoology “Doderlein”, SIMUA, via Archirafi 16, University of Palermo, Italy *Corresponding author, email: [email protected] th th ABSTRACT The 17 International Colloquium on Amphipoda (17 ICA) has been organized by the University of Palermo (Sicily, Italy), and took place in Trapani, 4-7 September 2017. All the contributions have been published in the present monograph and include a wide range of topics. KEY WORDS International Colloquium on Amphipoda; ICA; Amphipoda. Received 30.04.2017; accepted 31.05.2017; printed 30.06.2017 Proceedings of the 17th International Colloquium on Amphipoda (17th ICA), September 4th-7th 2017, Trapani (Italy) The first International Colloquium on Amphi- Poland, Turkey, Norway, Brazil and Canada within poda was held in Verona in 1969, as a simple meet- the Scientific Committee: ing of specialists interested in the Systematics of Sabrina Lo Brutto (Coordinator) - University of Gammarus and Niphargus. Palermo, Italy Now, after 48 years, the Colloquium reached the Elvira De Matthaeis - University La Sapienza, 17th edition, held at the “Polo Territoriale della Italy Provincia di Trapani”, a site of the University of Felicita Scapini - University of Firenze, Italy Palermo, in Italy; and for the second time in Sicily Alberto Ugolini - University of Firenze, Italy (Lo Brutto et al., 2013). Maria Beatrice Scipione - Stazione Zoologica The Organizing and Scientific Committees were Anton Dohrn, Italy composed by people from different countries. -
The C-Floor and Zones
The C-Floor and zones Table of Contents ` ❖ The ocean zones ❖ Sunlight zone and twilight zone ❖ Midnight and Abyssal zone ❖ The hadal zone ❖ The c-floor ❖ The c-floor definitions ❖ The c-floor definitions pt.2 ❖ Cites ❖ The end The ocean zones 200 meters deep 1,000 Meters deep 4,000 Meters deep 6,000 Meters deep 10,944 meters deep Sunlight zone Twilight zone ❖ The sunlight zone is 200 meters from the ocean's ❖ The twilight zone is about 1,000 meters surface deep from the ❖ Animals that live here ocean's surface sharks, sea turtles, ❖ Animals that live jellyfish and seals here are gray ❖ Photosynthesis normally whales, greenland occurs in this part of the Shark and clams ocean ❖ The twilight get only a faint amount of sunlight DID YOU KNOW Did you know That no plants live That the sunlight zone in the twilight zone could be called as the because of the euphotic and means well lit amount of sunlight in greek Midnight zone Abyssal zone ❖ The midnight zone is ❖ The abyssal zone is 4,000 meters from 6,000 meters from the the ocean's surface ocean’s surface ❖ Animals that live in ❖ Animals that live in the the midnight zone Abyssal zone are fangtooth fish, pacific are, vampire squid, viperfish and giant snipe eel and spider crabs anglerfish ❖ Supports only ❖ Animals eat only the DID YOU KNOW invertebrates and DID YOU KNOW leftovers that come That only 1 percent of light fishes That most all the way from the travels through animals are sunlight zone to the the midnight zone either small or midnight zone bioluminescent The Hadal Zone (Trench ● The Hadal Zone is 10,944 meters under the ocean ● Snails, worms, and sea cucumbers live in the hadal zone ● It is pitch black in the Hadal Zone The C-Floor The C-Floor Definitions ❖ The Continental Shelf - The flat part where people can walk. -
EXPLORING DEEP SEA HYDROTHERMAL VENTS on EARTH and OCEAN WORLDS. P. Sobron1,2, L. M. Barge3, the Invader Team. 1Impossible Sensing, St
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 2505.pdf EXPLORING DEEP SEA HYDROTHERMAL VENTS ON EARTH AND OCEAN WORLDS. P. Sobron1,2, L. M. Barge3, the InVADER Team. 1Impossible Sensing, St. Louis, MO ([email protected]) 2SETI Institute, Mtn. View, CA, , 3Jet Propulsion Laboratory, Pasadena, CA The Mission: InVADER (In-situ Vent Analysis precipitates showing exposed minerals and organic Divebot for Exobiology Research, Figure 4.1, content. The UNOLS ROV will use our coring tool and https://invader-mission.org/) is NASA’s most advanced its own manipulator and cameras to take ground truth subsea sensing payload, a tightly integrated imaging and samples as part of the InVADER deplotment. laser Raman spectroscopy/laser-induced breakdown In contrast to existing methods, InVADER allows spectroscopy/laser induced native fluorescence in-situ, autonomous, non-destructive measurements of instrument capable of in-situ, rapid, long-term these vent characteristics. InVADER will fill these gaps, underwater analyses of vent fluid and precipitates. and advance readiness in vent exploration on Earth and Such analyses are critical for finding and studying Ocean Worlds by simplifying operational strategies for life and life’s precursors at vent systems on Ocean identifying and characterizing seafloor environments. Worlds. To demonstrate the scientific potential and We will use statistical analysis tools for the fusion of functionality of the instrument, in July 2021 our team multi-sensor datasets, and develop real-time science will deploy InVADER on the Ocean Observatories data evaluation and payload control routines to Initiative’s (OOI) Regional Cabled Array (RCA), a establish, and then validate, adaptive science operations power/data distribution network off the Oregon coast, at strategies that maximize science return in a mission-like the underwater hydrothermal systems of Axial scenario. -
Significant Dissipation of Tidal Energy in the Deep Ocean Inferred from Satellite Altimeter Data
letters to nature 3. Rein, M. Phenomena of liquid drop impact on solid and liquid surfaces. Fluid Dynamics Res. 12, 61± water is created at high latitudes12. It has thus been suggested that 93 (1993). much of the mixing required to maintain the abyssal strati®cation, 4. Fukai, J. et al. Wetting effects on the spreading of a liquid droplet colliding with a ¯at surface: experiment and modeling. Phys. Fluids 7, 236±247 (1995). and hence the large-scale meridional overturning, occurs at 5. Bennett, T. & Poulikakos, D. Splat±quench solidi®cation: estimating the maximum spreading of a localized `hotspots' near areas of rough topography4,16,17. Numerical droplet impacting a solid surface. J. Mater. Sci. 28, 963±970 (1993). modelling studies further suggest that the ocean circulation is 6. Scheller, B. L. & Bous®eld, D. W. Newtonian drop impact with a solid surface. Am. Inst. Chem. Eng. J. 18 41, 1357±1367 (1995). sensitive to the spatial distribution of vertical mixing . Thus, 7. Mao, T., Kuhn, D. & Tran, H. Spread and rebound of liquid droplets upon impact on ¯at surfaces. Am. clarifying the physical mechanisms responsible for this mixing is Inst. Chem. Eng. J. 43, 2169±2179, (1997). important, both for numerical ocean modelling and for general 8. de Gennes, P. G. Wetting: statics and dynamics. Rev. Mod. Phys. 57, 827±863 (1985). understanding of how the ocean works. One signi®cant energy 9. Hayes, R. A. & Ralston, J. Forced liquid movement on low energy surfaces. J. Colloid Interface Sci. 159, 429±438 (1993). source for mixing may be barotropic tidal currents. -
Introduction to Oceanography
Introduction to Oceanography Introduction to Oceanography Lecture 14: Tides, Biological Productivity Memorial Day holiday Monday no lab meetings Go to any other lab section this week (and let the TA know!) Bay of Fundy -- low tide, Photo by Dylan Kereluk, . Creative Commons A 2.0 Generic, Mudskipper (Periophthalmus modestus) at low tide, photo by OpenCage, Wikimedia Commons, Creative http://commons.wikimedia.org/wiki/File:Bay_of_Fundy_-_Tide_Out.jpg Commons A S-A 2.5, http://commons.wikimedia.org/wiki/File:Periophthalmus_modestus.jpg Tides Earth-Moon-Sun System Planet-length waves Cyclic, repeating rise & fall of sea level • Earth-Sun Distance – Most regular phenomenon in the oceans 150,000,000 km Daily tidal variation has great effects on life in & around the ocean (Lab 8) • Earth-Moon Distance 385,000 km Caused by gravity and Much closer to Earth, but between Earth, Moon & much less massive Sun, their orbits around • Earth Obliquity = 23.5 each other, and the degrees Earth’s daily spin – Seasons Photos by Samuel Wantman, Creative Commons A S-A 3.0, http://en.wikipedia.org/ wiki/File:Bay_of_Fundy_Low_Tide.jpg and Figure by Homonculus 2/Geologician, Wikimedia Commons, http://en.wikipedia.org/wiki/ Creative Commons A 3.0, http://en.wikipedia.org/wiki/ File:Bay_of_Fundy_High_Tide.jpg File:Lunar_perturbation.jpg Tides are caused by the gravity of the Moon and Sun acting on Scaled image of Earth-Moon distance, Nickshanks, Wikimedia Commons, Creative Commons A 2.5 Earth and its ocean. Pluto-Charon mutual orbit, Zhatt, Wikimedia Commons, Public -
Exploration of the Deep Gulf of Mexico Slope Using DSV Alvin: Site Selection and Geologic Character
Exploration of the Deep Gulf of Mexico Slope Using DSV Alvin: Site Selection and Geologic Character Harry H. Roberts1, Chuck R. Fisher2, Jim M. Brooks3, Bernie Bernard3, Robert S. Carney4, Erik Cordes5, William Shedd6, Jesse Hunt, Jr.6, Samantha Joye7, Ian R. MacDonald8, 9 and Cheryl Morrison 1Coastal Studies Institute, Louisiana State University, Baton Rouge, Louisiana 70803 2Department of Biology, Penn State University, University Park, Pennsylvania 16802-5301 3TDI Brooks International, Inc., 1902 Pinon Dr., College Station, Texas 77845 4Department of Oceanography and Coastal Sciences, Louisiana State University, Baton Rouge, Louisiana 70803 5Department of Organismic and Evolutionary Biology, Harvard University, 16 Divinity Ave., Cambridge, Massachusetts 02138 6Minerals Management Service, Office of Resource Evaluation, New Orleans, Louisiana 70123-2394 7Department of Geology, University of Georgia, Athens, Georgia 30602 8Department of Physical and Environmental Sciences, Texas A&M – Corpus Christi, Corpus Christi, Texas 78412 9U.S. Geological Survey, 11649 Leetown Rd., Keameysville, West Virginia 25430 ABSTRACT The Gulf of Mexico is well known for its hydrocarbon seeps, associated chemosyn- thetic communities, and gas hydrates. However, most direct observations and samplings of seep sites have been concentrated above water depths of approximately 3000 ft (1000 m) because of the scarcity of deep diving manned submersibles. In the summer of 2006, Minerals Management Service (MMS) and National Oceanic and Atmospheric Admini- stration (NOAA) supported 24 days of DSV Alvin dives on the deep continental slope. Site selection for these dives was accomplished through surface reflectivity analysis of the MMS slope-wide 3D seismic database followed by a photo reconnaissance cruise. From 80 potential sites, 20 were studied by photo reconnaissance from which 10 sites were selected for Alvin dives. -
DEEP SEA LEBANON RESULTS of the 2016 EXPEDITION EXPLORING SUBMARINE CANYONS Towards Deep-Sea Conservation in Lebanon Project
DEEP SEA LEBANON RESULTS OF THE 2016 EXPEDITION EXPLORING SUBMARINE CANYONS Towards Deep-Sea Conservation in Lebanon Project March 2018 DEEP SEA LEBANON RESULTS OF THE 2016 EXPEDITION EXPLORING SUBMARINE CANYONS Towards Deep-Sea Conservation in Lebanon Project Citation: Aguilar, R., García, S., Perry, A.L., Alvarez, H., Blanco, J., Bitar, G. 2018. 2016 Deep-sea Lebanon Expedition: Exploring Submarine Canyons. Oceana, Madrid. 94 p. DOI: 10.31230/osf.io/34cb9 Based on an official request from Lebanon’s Ministry of Environment back in 2013, Oceana has planned and carried out an expedition to survey Lebanese deep-sea canyons and escarpments. Cover: Cerianthus membranaceus © OCEANA All photos are © OCEANA Index 06 Introduction 11 Methods 16 Results 44 Areas 12 Rov surveys 16 Habitat types 44 Tarablus/Batroun 14 Infaunal surveys 16 Coralligenous habitat 44 Jounieh 14 Oceanographic and rhodolith/maërl 45 St. George beds measurements 46 Beirut 19 Sandy bottoms 15 Data analyses 46 Sayniq 15 Collaborations 20 Sandy-muddy bottoms 20 Rocky bottoms 22 Canyon heads 22 Bathyal muds 24 Species 27 Fishes 29 Crustaceans 30 Echinoderms 31 Cnidarians 36 Sponges 38 Molluscs 40 Bryozoans 40 Brachiopods 42 Tunicates 42 Annelids 42 Foraminifera 42 Algae | Deep sea Lebanon OCEANA 47 Human 50 Discussion and 68 Annex 1 85 Annex 2 impacts conclusions 68 Table A1. List of 85 Methodology for 47 Marine litter 51 Main expedition species identified assesing relative 49 Fisheries findings 84 Table A2. List conservation interest of 49 Other observations 52 Key community of threatened types and their species identified survey areas ecological importanc 84 Figure A1. -
Microbial Community and Geochemical Analyses of Trans-Trench Sediments for Understanding the Roles of Hadal Environments
The ISME Journal (2020) 14:740–756 https://doi.org/10.1038/s41396-019-0564-z ARTICLE Microbial community and geochemical analyses of trans-trench sediments for understanding the roles of hadal environments 1 2 3,4,9 2 2,10 2 Satoshi Hiraoka ● Miho Hirai ● Yohei Matsui ● Akiko Makabe ● Hiroaki Minegishi ● Miwako Tsuda ● 3 5 5,6 7 8 2 Juliarni ● Eugenio Rastelli ● Roberto Danovaro ● Cinzia Corinaldesi ● Tomo Kitahashi ● Eiji Tasumi ● 2 2 2 1 Manabu Nishizawa ● Ken Takai ● Hidetaka Nomaki ● Takuro Nunoura Received: 9 August 2019 / Revised: 20 November 2019 / Accepted: 28 November 2019 / Published online: 11 December 2019 © The Author(s) 2019. This article is published with open access Abstract Hadal trench bottom (>6000 m below sea level) sediments harbor higher microbial cell abundance compared with adjacent abyssal plain sediments. This is supported by the accumulation of sedimentary organic matter (OM), facilitated by trench topography. However, the distribution of benthic microbes in different trench systems has not been well explored yet. Here, we carried out small subunit ribosomal RNA gene tag sequencing for 92 sediment subsamples of seven abyssal and seven hadal sediment cores collected from three trench regions in the northwest Pacific Ocean: the Japan, Izu-Ogasawara, and fi 1234567890();,: 1234567890();,: Mariana Trenches. Tag-sequencing analyses showed speci c distribution patterns of several phyla associated with oxygen and nitrate. The community structure was distinct between abyssal and hadal sediments, following geographic locations and factors represented by sediment depth. Co-occurrence network revealed six potential prokaryotic consortia that covaried across regions. Our results further support that the OM cycle is driven by hadal currents and/or rapid burial shapes microbial community structures at trench bottom sites, in addition to vertical deposition from the surface ocean. -
OCEANS ´09 IEEE Bremen
11-14 May Bremen Germany Final Program OCEANS ´09 IEEE Bremen Balancing technology with future needs May 11th – 14th 2009 in Bremen, Germany Contents Welcome from the General Chair 2 Welcome 3 Useful Adresses & Phone Numbers 4 Conference Information 6 Social Events 9 Tourism Information 10 Plenary Session 12 Tutorials 15 Technical Program 24 Student Poster Program 54 Exhibitor Booth List 57 Exhibitor Profiles 63 Exhibit Floor Plan 94 Congress Center Bremen 96 OCEANS ´09 IEEE Bremen 1 Welcome from the General Chair WELCOME FROM THE GENERAL CHAIR In the Earth system the ocean plays an important role through its intensive interactions with the atmosphere, cryo- sphere, lithosphere, and biosphere. Energy and material are continually exchanged at the interfaces between water and air, ice, rocks, and sediments. In addition to the physical and chemical processes, biological processes play a significant role. Vast areas of the ocean remain unexplored. Investigation of the surface ocean is carried out by satellites. All other observations and measurements have to be carried out in-situ using research vessels and spe- cial instruments. Ocean observation requires the use of special technologies such as remotely operated vehicles (ROVs), autonomous underwater vehicles (AUVs), towed camera systems etc. Seismic methods provide the foundation for mapping the bottom topography and sedimentary structures. We cordially welcome you to the international OCEANS ’09 conference and exhibition, to the world’s leading conference and exhibition in ocean science, engineering, technology and management. OCEANS conferences have become one of the largest professional meetings and expositions devoted to ocean sciences, technology, policy, engineering and education. -
The Hadal Zone Deep-Sea Trenches
The Hadal Zone Deep-sea Trenches •! Hadal - Ocean habitats deeper than 6,000m •! Deep-sea trenches comprise the overwhelming majority of these habitats •! Deepest: Mariana Trench – 10,998 m The Hadal Zone Map > 6000 m (Not only trenches!) World Hadal Trenches (Jamieson et al. 2009) 37 deep-sea trenches Most in the Pacific, deepest 9 in the Pacific Trench Environment Temperature: 1.0-2.5oC Temperature increases below 4000 m due to adiabatic heating South Pacific trench temperatures increase from 1.16 to 1.91oC between 6000 and 10000 m (40%) North Pacific trench temperatures rise from 1.67 to 2.40 oC between 6000 and 10000 m. (30%) Tonga Trench Temperature (Jamieson et al. 2009 TREE) Temperatures in trenches are comparable to 3000 m cont. margin Challenger Deep Cross Section CTD Casts Temperature and Salinity Taira et al. 2005 J. Of Oceanography Flow regime: Deep currents ventilate trenches with values up to 8.1 cm/sec in the Challenger Deep Up to 32 cm/s in other trenches Currents exhibit lunar and semi-lunar tidal cycles Mean oxygen in N. Pacific trenches 3.43 ml L-1 Why is the Mariana Trench so deep? 1. Plate configuration – Pacific plate is old and cold and plunging beneath the Philippine plate. The Philippine plate is young and soft and is carried downward with the Pacific plate. 2. Remoteness from sediment sources – it doesn’t fill up over time! Trench Biology – Historical (courtesy of L. Blankenship) •! Challenger – sounding to 8200 m (no fauna) •! Incidental collection of arenaceous foraminiferan at 7228 m Japan Trench (Brady 1984 – 14 spp.) •! In 1899, the “Albatross” trawled the Tonga Trench deeper waters for the first time.