Climate Change and Freshwater Fisheries
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A Global Assessment of Parasite Diversity in Galaxiid Fishes
diversity Article A Global Assessment of Parasite Diversity in Galaxiid Fishes Rachel A. Paterson 1,*, Gustavo P. Viozzi 2, Carlos A. Rauque 2, Verónica R. Flores 2 and Robert Poulin 3 1 The Norwegian Institute for Nature Research, P.O. Box 5685, Torgarden, 7485 Trondheim, Norway 2 Laboratorio de Parasitología, INIBIOMA, CONICET—Universidad Nacional del Comahue, Quintral 1250, San Carlos de Bariloche 8400, Argentina; [email protected] (G.P.V.); [email protected] (C.A.R.); veronicaroxanafl[email protected] (V.R.F.) 3 Department of Zoology, University of Otago, P.O. Box 56, Dunedin 9054, New Zealand; [email protected] * Correspondence: [email protected]; Tel.: +47-481-37-867 Abstract: Free-living species often receive greater conservation attention than the parasites they support, with parasite conservation often being hindered by a lack of parasite biodiversity knowl- edge. This study aimed to determine the current state of knowledge regarding parasites of the Southern Hemisphere freshwater fish family Galaxiidae, in order to identify knowledge gaps to focus future research attention. Specifically, we assessed how galaxiid–parasite knowledge differs among geographic regions in relation to research effort (i.e., number of studies or fish individuals examined, extent of tissue examination, taxonomic resolution), in addition to ecological traits known to influ- ence parasite richness. To date, ~50% of galaxiid species have been examined for parasites, though the majority of studies have focused on single parasite taxa rather than assessing the full diversity of macro- and microparasites. The highest number of parasites were observed from Argentinean galaxiids, and studies in all geographic regions were biased towards the highly abundant and most widely distributed galaxiid species, Galaxias maculatus. -
A Comparative Introduction to the Biology and Limnology of the African Great Lakes
J. Great Lakes Res. 29 (Supplement 2):3–18 Internat. Assoc. Great Lakes Res., 2003 A Comparative Introduction to the Biology and Limnology of the African Great Lakes Harvey A. Bootsma1,* and Robert E. Hecky2 1Great Lakes WATER Institute University of Wisconsin-Milwaukee 600 E. Greenfield Ave. Milwaukee, Wisconsin 53204 2Biology Department University of Waterloo 200 University Ave. W. Waterloo, Ontario N2L 3G1 ABSTRACT. The East African rift valley region contains the earth’s largest aggregation of tropical lakes. Three of these lakes—Victoria, Tanganyika, and Malawi—hold one quarter of the earth’s total surface freshwater supply, and are home to a myriad of fish species. Apart from the diversity and endemicity of their biota, properties that distinguish the African Great Lakes from their North American counterparts include their great age, long sedimentary records, long residence times, persistent stratifi- cation, continuously warm temperatures at all depths, major ion composition, and a propensity for nitrogen limitation. Current management problems include over-fishing, increased input of sediment and nutrients, and in the case of Lake Victoria, loss of endemic fish species and the proliferation of the introduced water hyacinth. As in the Laurentian Great Lakes basin, the harmonization of research pro- grams and management strategies among the various riparian countries is a challenge. While research activities on all three lakes have increased in the last decade, there remains a need for integrated, multi- disciplinary research in order to develop conceptual and numerical models that provide insight into the functioning of large, tropical, freshwater aquatic ecosystems. Particular issues that may be pursued most profitably in the African Great Lakes include the links between climate and biogeochemical cycles, the role of biodiversity in ecosystem functioning, and paleoclimate reconstruction over millions of years. -
Wheeler River Project Provincial Technical Proposal and Federal Project Description
Wheeler River Project Provincial Technical Proposal and Federal Project Description Denison Mines Corp. May 2019 WHEELER RIVER PROJECT TECHNICAL PROPOSAL & PROJECT DESCRIPTION Wheeler River Project Provincial Technical Proposal and Federal Project Description Project Summary English – Page ii French – Page x Dene – Page xx Cree – Page xxviii PAGE i WHEELER RIVER PROJECT TECHNICAL PROPOSAL & PROJECT DESCRIPTION Summary Wheeler River Project The Wheeler River Project (Wheeler or the Project) is a proposed uranium mine and processing plant in northern Saskatchewan, Canada. It is located in a relatively undisturbed area of the boreal forest about 4 km off of Highway 914 and approximately 35 km north-northeast of the Key Lake uranium operation. Wheeler is a joint venture project owned by Denison Mines Corp. (Denison) and JCU (Canada) Exploration Company Ltd. (JCU). Denison owns 90% of Wheeler and is the operator, while JCU owns 10%. Denison is a uranium exploration and development company with interests focused in the Athabasca Basin region of northern Saskatchewan, Canada with a head office in Toronto, Ontario and technical office in Saskatoon, Saskatchewan. Historically Denison has had over 50 years of uranium mining experience in Saskatchewan, Elliot Lake, Ontario, and in the United States. Today, the company is part owner (22.5%) of the McClean Lake Joint Venture which includes the operating McClean Lake uranium mill in northern Saskatchewan. To advance the Project, Denison is applying an innovative approach to uranium mining in Canada called in situ recovery (ISR). The use of ISR mining at Wheeler means that there will be no need for a large open pit mining operation or multiple shafts to access underground mine workings; no workers will be underground as the ISR process is conducted from surface facilities. -
Planetary Surfaces
Chapter 4 PLANETARY SURFACES 4.1 The Absence of Bedrock A striking and obvious observation is that at full Moon, the lunar surface is bright from limb to limb, with only limited darkening toward the edges. Since this effect is not consistent with the intensity of light reflected from a smooth sphere, pre-Apollo observers concluded that the upper surface was porous on a centimeter scale and had the properties of dust. The thickness of the dust layer was a critical question for landing on the surface. The general view was that a layer a few meters thick of rubble and dust from the meteorite bombardment covered the surface. Alternative views called for kilometer thicknesses of fine dust, filling the maria. The unmanned missions, notably Surveyor, resolved questions about the nature and bearing strength of the surface. However, a somewhat surprising feature of the lunar surface was the completeness of the mantle or blanket of debris. Bedrock exposures are extremely rare, the occurrence in the wall of Hadley Rille (Fig. 6.6) being the only one which was observed closely during the Apollo missions. Fragments of rock excavated during meteorite impact are, of course, common, and provided both samples and evidence of co,mpetent rock layers at shallow levels in the mare basins. Freshly exposed surface material (e.g., bright rays from craters such as Tycho) darken with time due mainly to the production of glass during micro- meteorite impacts. Since some magnetic anomalies correlate with unusually bright regions, the solar wind bombardment (which is strongly deflected by the magnetic anomalies) may also be responsible for darkening the surface [I]. -
RUNNING HEAD: Farrow-Aspects of the Life Cycle of Apharyngostrigea Pipientis
RUNNING HEAD: Farrow-Aspects of the life cycle of Apharyngostrigea pipientis Aspects of the life cycle of Apharyngostrigea pipientis in Central Florida wetlands Abigail Farrow Florida Southern College RUNNING HEAD: Farrow-Aspects of the life cycle of Apharyngostrigea pipientis Abstract Apharyngostrigea pipientis (Trematoda: Strigeidae) is known to form metacercariae around the pericardium of anuran tadpoles in Michigan and other northern locations. Definitive hosts are thought to be wading birds, while the intermediate host is a freshwater snail. Apharyngostrigea pipientis is not commonly reported from Florida, yet we have found several populations of snails (Biopholaria havaensis) and tadpoles, primarily the Cuban treefrog (Osteopilus septentrionalis), to host this trematode. We used experimental infections to elucidate the transmission dynamics and development of A. pipientis inside the tadpole host. Surprisingly, we found two types (species?) of cercariae being shed from B. havaensis that enter Cuban treefrog tadpoles to form seemingly identical metacercariae. Further, both of these develop into metaceracariae inside the tadpoles over 5-7 days after wondering inside the host's body cavity as mesocercariae, and metacercariae are commonly concentrated around the pericardium cavity. However, they differ in entry mode, with one being ingested, whereas the other penetrates the skin. This project is ongoing. 1. Introduction The study of parasitology plays a vital role in understanding the foundation of communities in different ecosystems. Parasites have the ability to exploit their hosts, directly affecting the health of the organism and the environment. By having these abilities, it could mean a change in the way the organism contributes to and balances the overall ecosystem (Poulin, 1999). -
Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
Literaturverweise
Literaturverweise Statt eines Vorworts: Das Corona-Experiment 1. Le Quéré, C., Jackson, R. B., Jones, M. W., Smith, A. J. P., Abernethy, S., Andrew, R. M., De-Gol, A. J., Willis, D. R., Shan, Y., Canadell, J. G., Friedlingstein, P., Creutzig, F., Peters, G. P. (2020): Temporary reduction in daily global CO2 emissions during the COVID-19 forced confinement: Nature Climate Change 10 (7), 647-653. 2. Myllyvirta, L. (2020): Coronavirus temporarily reduced China’s CO2 emissions by a quarter. Carbon Brief https://www.carbonbrief.org/analysis-coronavirus-has- temporarily-reduced-chinas-co2-emissions-by-a-quarter 3. Spencer, R.(2020): Why the current Economics slowdown won’t show up in the atmospheric record, https://www.drroyspencer.com/2020/05/why-the-current- economic-slowdown-wont-show-up-in-the-atmospheric-co2-record/ 4. Die Abbauzeit (Lebensdauer) des CO2 ist die Zeit , in der die Konzentration auf ein 1/e (0,3679) des Ausgangswerts gesunken ist. Sie wird berechnet als Quotient des zum Gleichgewicht von 280 ppm hinzugefügten CO2 durch die Größe des Abbaus. 1959 waren das 34 ppm : 0,64 ppm = 55 Jahre. 2019 sind das 130 ppm : 2,6 ppm =50 Jahre. Die Umrechnung in einen Abbau von 50 % (Halbwertszeit) gelingt durch Multiplikation dieser Abbauzeiten mit ln2 = 0,6931. Das sind dann 1959 38 Jahre und 2019 34,7 Jahre. 5. Haverd, V., Smith, B., Canadell, J. G., Cuntz, M., Mikaloff-Fletcher, S., Farquhar, G., Woodgate, W., Briggs, P. R., Trudinger, C. M. (2020): Higher than expected CO2 fertilization inferred from leaf to global observations: Global Change Biology 26 (4), 2390-2402. -
GSIS Newsletter Will Be Published Quarterly, in March, June, September, and December by the Geoscience Information Society
Number 256, December, 2012 ISSN: 0046-5801 CONTENTS Presidents Column…………………………………………………………. 1 Open access publication opportunities for geoscientists……………….. 13 Geoscience Information Society 2012 Officers……………………………. 2 Annual meeting pictures……………………………………………….. 18 Member updates……………………………………………………………. 3 GeoScienceWorld Unveils Open, Map-Based Discovery Prototype…... 20 Greetings from Australia…………………………………………………... 3 Auditor’s Report for 2010……………………………………………… 21 Geoscience journal prices………………………………………………….. 5 Issue to watch: AGU partners with Wiley-Blackwell………………….. 21 GSIS Publications List…………………………………………………. 22 President's Column By Linda Zellmer Now that we have all returned from the meeting the past year: in Charlotte and (in the case of the members in the United States) eaten our Thanksgiving • April Love and Cynthia Prosser - for setting Dinners, we are probably making our lists for up the GSIS Exhibit holiday gifts. While I do not have any gifts to • Clara McLeod - for coordinating Geoscience give out, I would like to take the opportunity to Librarianship 101 (GL 101). offer my heartfelt appreciation to all of the • Amanda Bielskas – for teaching the people who have contributed to the efforts of Collection Development portion of GL 101. Geoscience Information Society during the past • Hannah Winkler - for teaching the year and our recent meeting. Reference Services portion of GL101. • Megan Sapp-Nelson – for developing a presentation on Library Instruction for the We had 5 sponsors for our meeting who Earth Sciences that I presented for her at GL provided funding to help defray the costs of the 101. meeting. They include: American Association of • Adonna Fleming – for helping with publicity Petroleum Geologists, Geoscience World, for GL 101. Gemological Institute of America, Geological • Jan Heagy – for developing certificates of Society of London and Elsevier. -
Regional Oral History Off Ice University of California the Bancroft Library Berkeley, California
Regional Oral History Off ice University of California The Bancroft Library Berkeley, California Richard B. Gump COMPOSER, ARTIST, AND PRESIDENT OF GUMP'S, SAN FRANCISCO An Interview Conducted by Suzanne B. Riess in 1987 Copyright @ 1989 by The Regents of the University of California Since 1954 the Regional Oral History Office has been interviewing leading participants in or well-placed witnesses to major events in the development of Northern California, the West,and the Nation. Oral history is a modern research technique involving an interviewee and an informed interviewer in spontaneous conversation. The taped record is transcribed, lightly edited for continuity and clarity, and reviewed by the interviewee. The resulting manuscript is typed in final form, indexed, bound with photographs and illustrative materials, and placed in The Bancroft Library at the University of California, Berkeley, and other research collections for scholarly use. Because it is primary material, oral history is not intended to present the final, verified, or complete narrative of events. It is a spoken account, offered by the interviewee in response to questioning, and as such it is reflective, partisan, deeply involved, and irreplaceable. All uses of this manuscript are covered by a legal agreement between the University of California and Richard B. Gump dated 7 March 1988. The manuscript is thereby made available for research purposes. All literary rights in the manuscript, including the right to publish, are reserved to The Bancroft Library of the University of California, Berkeley. No part of the manuscript may be quoted for publication without the written permission of the Director of The Bancroft Library of the University of California, Berkeley. -
Forsyth Technical Community College Commencement 2015
Forsyth Technical Community College Commencement 2015 Lawrence Joel Veterans Memorial Coliseum 2825 University Parkway Winston-Salem, North Carolina Thursday, May 7, 2015 5:00 p.m. Forsyth Technical Community College Commencement 2015 Lawrence Joel Veteran’s Memorial Coliseum 2825 University Parkway Winston-Salem, North Carolina Thursday, May 7, 2015 5 p.m. Forsyth Technical Community College Board of Trustees Edwin L. Welch, Jr. Chair Ann Bennett-Phillips Nancy W. Dunn Jeffrey R. McFadden Amanda Boston A. Edward Jones R. Alan Proctor SGA President Andrea D. Kepple Vice Chair John M. Davenport, Jr. Arnold G. King Kenneth M. Sadler; D.D.S. Tammy L. Duggins Paul M. Wiles Forsyth Technical Community College Board of Administration Dr. Gary M. Green President Dr. Jewel B. Cherry Mr. Alan K. Murdock Vice President Vice President Student Services Economic & Workforce Development Ms. Rachel M. Desmarais Ms. Mamie M. Sutphin Vice President Vice President Information Services Institutional Advancement Ms. Wendy R. Emerson Dr. Conley F. Winebarger Vice President Vice President Business Services Instructional Services 2015 Commencement Program Processional Presiding......................................................................................................................Dr. Gary M. Green President, Forsyth Technical Community College National Anthem .................................................................................................. Sonya Bennett-Brown Music Instructor, Humanities & Social Sciences Division Introduction of -
Guidance for Using Continuous Monitors in Pm Monitoring
United States Office of Air Quality EPA-454/R-98-012 Environmental Protection Planning and Standards May 1998 Agency Research Triangle Park, NC 27711 Air GUIDANCE FOR USING CONTINUOUS MONITORS IN PM2.5 MONITORING NETWORKS GUIDANCE FOR USING CONTINUOUS MONITORS IN PM2.5 MONITORING NETWORKS May 29, 1998 PREPARED BY John G. Watson1 Judith C. Chow1 Hans Moosmüller1 Mark Green1 Neil Frank2 Marc Pitchford3 PREPARED FOR Office of Air Quality Planning and Standards U.S. Environmental Protection Agency Research Triangle Park, NC 27711 1Desert Research Institute, University and Community College System of Nevada, PO Box 60220, Reno, NV 89506 2U.S. EPA/OAQPS, Research Triangle Park, NC, 27711 3National Oceanic and Atmospheric Administration, 755 E. Flamingo, Las Vegas, NV 89119 DISCLAIMER The development of this document has been funded by the U.S. Environmental Protection Agency, under cooperative agreement CX824291-01-1, and by the Desert Research Institute of the University and Community College System of Nevada. Mention of trade names or commercial products does not constitute endorsement or recommendation for use. This draft has not been subject to the Agency’s peer and administrative review, and does not necessarily represent Agency policy or guidance. ii ABSTRACT This guidance provides a survey of alternatives for continuous in-situ measurements of suspended particles, their chemical components, and their gaseous precursors. Recent and anticipated advances in measurement technology provide reliable and practical instruments for particle quantification over averaging times ranging from minutes to hours. These devices provide instantaneous, telemetered results and can use limited manpower more efficiently than manual, filter-based methods. -
Earth: Atmospheric Evolution of a Habitable Planet
Earth: Atmospheric Evolution of a Habitable Planet Stephanie L. Olson1,2*, Edward W. Schwieterman1,2, Christopher T. Reinhard1,3, Timothy W. Lyons1,2 1NASA Astrobiology Institute Alternative Earth’s Team 2Department of Earth Sciences, University of California, Riverside 3School of Earth and Atmospheric Science, Georgia Institute of Technology *Correspondence: [email protected] Table of Contents 1. Introduction ............................................................................................................................ 2 2. Oxygen and biological innovation .................................................................................... 3 2.1. Oxygenic photosynthesis on the early Earth .......................................................... 4 2.2. The Great Oxidation Event ......................................................................................... 6 2.3. Oxygen during Earth’s middle chapter ..................................................................... 7 2.4. Neoproterozoic oxygen dynamics and the rise of animals .................................. 9 2.5. Continued oxygen evolution in the Phanerozoic.................................................. 11 3. Carbon dioxide, climate regulation, and enduring habitability ................................. 12 3.1. The faint young Sun paradox ................................................................................... 12 3.2. The silicate weathering thermostat ......................................................................... 12 3.3. Geological