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Books on the topic 'Deep water flow'

Author: Grafiati

Published: 4 June 2021

Last updated: 11 February 2022

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1

O'Reilly, Andrew M. A method for simulating transient ground-water recharge in deep water-table settings in central Florida by using a simple water-balance/transfer-function model. Reston, Va: U.S. Geological Survey, 2004.

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2

O'Reilly, Andrew M. A method for simulating transient ground-water recharge in deep water-table settings in central Florida by using a simple water-balance/transfer-function model. Reston, Va: U.S. Geological Survey, 2004.

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3

Barker, René A. Regional hydrology and simulation of deep ground-water flow in the southeastern coastal plain aquifer system in Mississippi, Alabama, Georgia, and South Carolina. [Washington, D.C.]: U.S. G.P.O., 1992.

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4

Wirojanagud, Prakob. Numerical modeling of regional ground-water flow in the Deep-Basin Brine aquifer of the Palo Duro Basin, Texas Panhandle. Austin, Tex: Bureau of the Economic Geology, University of Texas at Austin, 1986.

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5

Division, Alberta Fisheries Management. Report on Red Deer River instream flow needs study. Calgary, Alta., Canada: Golder Associates, 1999.

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6

D, Crevello Paul, and Harris Paul M. 1931-, eds. Deep-water carbonates: Buildups, turbidites, debris flows and chalks : a core workshop. Tulsa, OK: SEPM, 1985.

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7

Goater, Lori. Aquatic environment impact ratings a method for evaluating SSRB flow scenarios: Red Deer River case study. 4th ed. [Alberta]: Alberta Environment, 2008.

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8

Wolfe, William J. Recent sedimentation and surface-water flow patterns on the flood plain of the North Fork Forked Deer River, Dyer County, Tennessee. Nashville, Tenn: U.S. Dept. of the Interior, U.S. Geological Survey, 1993.

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9

J, Wolfe William. Recent sedimentation and surface-water flow patterns on the flood plain of the North Fork Forked Deer River, Dyer County, Tennessee. Nashville, Tenn: U.S. Dept. of the Interior, U.S. Geological Survey, 1993.

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10

Wolfe, William J. Recent sedimentation and surface-water flow patterns on the flood plain of the North Fork Forked Deer River, Dyer County, Tennessee. Nashville, Tenn: U.S. Dept. of the Interior, U.S. Geological Survey, 1993.

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11

Wolfe, William J. Recent sedimentation and surface-water flow patterns on the flood plain of the North Fork Forked Deer River, Dyer County, Tennessee. Nashville, Tenn: U.S. Dept. of the Interior, U.S. Geological Survey, 1993.

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12

D, Crevello Paul, Harris Paul M, and Society of Economic Paleontologists and Mineralogists., eds. Deep-water carbonates: Buildups, turbidites, debris flows and chalks : a core workshop : SEPM Core Workshop no. 6, New Orleans, March 23-24, 1985. [Tulsa]: Society of Economic Paleontologists and Mineralogists, 1985.

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13

P, Dunning C., Milwaukee (Wis ), Geological Survey (U.S.), and United States. Environmental Protection Agency. Region V., eds. Simulation of ground-water flow, surface-water flow, and a deep sewer tunnel system in the Menomonee Valley, Milwaukee, Wisconsin. Reston, Va: U.S. Dept. of the Interior, U.S. Geological Survey, 2004.

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14

P, Dunning C., Milwaukee (Wis ), Geological Survey (U.S.), and United States. Environmental Protection Agency. Region V., eds. Simulation of ground-water flow, surface-water flow, and a deep sewer tunnel system in the Menomonee Valley, Milwaukee, Wisconsin. Reston, Va: U.S. Dept. of the Interior, U.S. Geological Survey, 2004.

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15

Simulation of ground-water flow, surface-water flow, and a deep sewer tunnel system in the Menomonee Valley, Milwaukee, Wisconsin. Reston, Va: U.S. Dept. of the Interior, U.S. Geological Survey, 2004.

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16

Simulation of ground-water flow, surface-water flow, and a deep sewer tunnel system in the Menomonee Valley, Milwaukee, Wisconsin. Reston, Va: U.S. Dept. of the Interior, U.S. Geological Survey, 2004.

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17

D, Crevello Paul, Harris Paul M. 1949-, and Society of Economic Paleontologists and Mineralogists., eds. Deep-water carbonates: Buildups, turbidites, debris flows and chalks : a core workshop. [Tulsa, Okla.]: Society of Economic Paleontologists and Mineralogists, 1985.

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18

D, Crevello Paul, ed. Deep-water carbonates, buildups, turbidites, debris flows and chalks: A Core Workshop, New Orleans, March 23-24, 1985. Tulsa, OK: Society of Economic Paleontologists and Mineralogists, 1985.

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19

1951-, Crevello Paul D., ed. Deep-water carbonates, buildups, turbidites, debris flows and chalks: A Core Workshop, New Orleans, March 23-24, 1985. Tulsa, OK: Society of Economic Paleontologists and Mineralogists, 1985.

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20

D, Crevillo Paul, Harris Paul M, and Society of Economic Paleontologists and Mineralogists., eds. Deep-water carbonates: Buildups, turbidites, debris flows and chalks : a core workshop, New Orleans, March 23-24, 1985. Tulsa, OK: Society of Economic Paleontologists and Mineralogists, 1985.

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21

1951-, Crevello Paul D., ed. Deep-water carbonates, buildups, turbidites, debris flows and chalks: A Core Workshop, New Orleans, March 23-24, 1985. Tulsa, OK: Society of Economic Paleontologists and Mineralogists, 1985.

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22

Froese, Marc D. Formal International Institutions and the Regulation of Flows of Goods and Services. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190846626.013.399.

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Trade governance rests upon certain economic assumptions and the ensuing political compromises made possible by the growth of an incremental legal consensus. The main economic assumptions are that trade will deliver upon the objectives of socio-economic development, stable, long-term employment opportunities and poverty reduction. These assumptions are theoretically sound, but are increasingly challenged by the complex political realities of global trade. The study of trade in the field of international political economy (IPE) has deep roots in the postwar disciplines of economics and political science. The literature on the history of trade regulation places the current system, with its emphasis on the legitimizing imprimatur of political power and the significance of binding treaty, into a more nuanced context in which present practices, while sometimes novel, are frequently older than most policy makers realize. In the two decades since the finalization of the Uruguay Round and the creation of the World Trade Organization (WTO), a host of significant issues have arisen as scholars and policy makers attempt to implement the WTO’s mandate and navigate the political waters of trade regulation as it relates to domestic law and policy. These include the set of issues raised by the broadening of trade regulation post-Uruguay Round to include trade related intellectual property rights and trade in services, the contentious issue of trade and economic development, and the issue of WTO reform.

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23

Clarke, Andrew. Temperature, growth and size. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780199551668.003.0013.

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Growth involves two flows of energy. The first is chemical potential energy in the monomers used to construct the proteins, lipids, polysaccharides and nucleic acids forming the new tissue. The second is the metabolic energy (ATP or GTP) used to construct the new tissue; this is the metabolic cost of growth and can be expressed as a dimensionless fraction of the energy retained in the new tissue. Its value is ~0.33. Typical temperature sensitivities for growth in the wild lie in the range Q10 1.5 – 3. Within species there may be evolutionary adjustments to growth rate to offset the effects of temperature, though these involve trade-offs with other physiological factors affecting fitness. Outside the tropics, many mammals and birds exhibit a cline in size, with larger species at higher latitudes (Bergmann’s rule). Carl Bergmann predicted such a cline from biophysical arguments based on endotherm thermoregulatory costs; Bergmann’s rule thus applies only to mammals and birds. Many ectotherms grow more slowly but attain a larger adult size when grown at lower temperatures (the temperature-size rule). The large size of some aquatic invertebrates at lower temperatures (notably in the polar regions and the deep sea) is associated with a higher oxygen content of the water.

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24

Bridges, John C. Evolution of the Martian Crust. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190647926.013.18.

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This is an advance summary of a forthcoming article in the Oxford Encyclopedia of Planetary Science. Please check back later for the full article.Mars, which has a tenth of the mass of Earth, has cooled as a single lithospheric plate. Current topography gravity maps and magnetic maps do not show signs of the plate tectonics processes that have shaped the Earth’s surface. Instead, Mars has been shaped by the effects of meteorite bombardment, igneous activity, and sedimentary—including aqueous—processes. Mars also contains enormous igneous centers—Tharsis and Elysium, with other shield volcanoes in the ancient highlands. In fact, the planet has been volcanically active for nearly all of its 4.5 Gyr history, and crater counts in the Northern Lowlands suggest that may have extended to within the last tens of millions of years. Our knowledge of the composition of the igneous rocks on Mars is informed by over 100 Martian meteorites and the results from landers and orbiters. These show dominantly tholeiitic basaltic compositions derived by melting of a relatively K, Fe-rich mantle compared to that of the Earth. However, recent meteorite and lander results reveal considerable diversity, including more silica-rich and alkaline igneous activity. These show the importance of a range of processes including crystal fractionation, partial melting, and possibly mantle metasomatism and crustal contamination of magmas. The figures and plots of compositional data from meteorites and landers show the range of compositions with comparisons to other planetary basalts (Earth, Moon, Venus). A notable feature of Martian igneous rocks is the apparent absence of amphibole. This is one of the clues that the Martian mantle had a very low water content when compared to that of Earth.The Martian crust, however, has undergone hydrothermal alteration, with impact as an important heat source. This is shown by SNC analyses of secondary minerals and Near Infra-Red analyses from orbit. The associated water may be endogenous.Our view of the Martian crust has changed since Viking landers touched down on the planet in 1976: from one almost entirely dominated by basaltic flows to one where much of the ancient highlands, particularly in ancient craters, is covered by km deep sedimentary deposits that record changing environmental conditions from ancient to recent Mars. The composition of these sediments—including, notably, the MSL Curiosity Rover results—reveal an ancient Mars where physical weathering of basaltic and fractionated igneous source material has dominated over extensive chemical weathering.

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