SPACE-CABIN ATMOSPHERES Part III /Physiological Factors of Inert Gases
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Blending Hydrogen Into Natural Gas Pipeline Networks: a Review of Key Issues
Blending Hydrogen into Natural Gas Pipeline Networks: A Review of Key Issues M. W. Melaina, O. Antonia, and M. Penev NREL is a national laboratory of the U.S. Department of Energy, Office of Energy Efficiency & Renewable Energy, operated by the Alliance for Sustainable Energy, LLC. Technical Report NREL/TP-5600-51995 March 2013 Contract No. DE-AC36-08GO28308 Blending Hydrogen into Natural Gas Pipeline Networks: A Review of Key Issues M. W. Melaina, O. Antonia, and M. Penev Prepared under Task No. HT12.2010 NREL is a national laboratory of the U.S. Department of Energy, Office of Energy Efficiency & Renewable Energy, operated by the Alliance for Sustainable Energy, LLC. National Renewable Energy Laboratory Technical Report 15013 Denver West Parkway NREL/TP-5600-51995 Golden, Colorado 80401 March 2013 303-275-3000 • www.nrel.gov Contract No. DE-AC36-08GO28308 NOTICE This report was prepared as an account of work sponsored by an agency of the United States government. Neither the United States government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States government or any agency thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States government or any agency thereof. -
Atmospheric Gases Student Handout Atmospheric Gases
Atmospheric Gases Student Handout Atmospheric Gases Driving Question: What is our atmosphere made of? In this activity you will: 1. Explore the variety and ratio of compounds and elements that make up the Earth’s atmosphere. 2. Understand volumetric measurements of gases in the atmosphere. 3. Visually depict the composition of the atmosphere. Background Information: Understanding Concentration Measurements In this activity, we will investigate the gas composition of our planet’s atmosphere. We use percentages to represent units of gas composition. A percent (%) is equivalent to 1 part out of 100 equal units. 1% = 1 part out of 100 For smaller concentrations scientists use parts per million (ppm) to represent concentrations of gases (or pollutants) in the atmosphere). One ppm is equivalent to 1 part out of 1,000,000 if the volume being measured is separated into 1,000,000 equal units. 1 ppm = 1 part out of 1,000,000 In this activity, you will use graph paper to represent the concentration of different gases in the atmosphere. Copyright © 2011 Environmental Literacy and Inquiry Working Group at Lehigh University Atmospheric Gases Student Handout 2 Here are some examples to help visualize parts per million: The common unit mg/liter is equal to ppm concentration Four drops of ink in a 55-gallon barrel of water would produce an "ink concentration" of 1 ppm. 1 12-oz can of soda pop in a 30-meter swimming pool 1 3-oz chocolate bar on a football field Atmospheric Composition Activity You will be creating a graphic model of the atmosphere composition using the Atmospheric Composition of Clean Dry Air activity sheet. -
Tracer Applications of Noble Gas Radionuclides in the Geosciences
To be published in Earth-Science Reviews Tracer Applications of Noble Gas Radionuclides in the Geosciences (August 20, 2013) Z.-T. Lua,b, P. Schlosserc,d, W.M. Smethie Jr.c, N.C. Sturchioe, T.P. Fischerf, B.M. Kennedyg, R. Purtscherth, J.P. Severinghausi, D.K. Solomonj, T. Tanhuak, R. Yokochie,l a Physics Division, Argonne National Laboratory, Argonne, Illinois, USA b Department of Physics and Enrico Fermi Institute, University of Chicago, Chicago, USA c Lamont-Doherty Earth Observatory, Columbia University, Palisades, New York, USA d Department of Earth and Environmental Sciences and Department of Earth and Environmental Engineering, Columbia University, New York, USA e Department of Earth and Environmental Sciences, University of Illinois at Chicago, Chicago, IL, USA f Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, USA g Center for Isotope Geochemistry, Lawrence Berkeley National Laboratory, Berkeley, USA h Climate and Environmental Physics, Physics Institute, University of Bern, Bern, Switzerland i Scripps Institution of Oceanography, University of California, San Diego, USA j Department of Geology and Geophysics, University of Utah, Salt Lake City, USA k GEOMAR Helmholtz Center for Ocean Research Kiel, Marine Biogeochemistry, Kiel, Germany l Department of Geophysical Sciences, University of Chicago, Chicago, USA Abstract 81 85 39 Noble gas radionuclides, including Kr (t1/2 = 229,000 yr), Kr (t1/2 = 10.8 yr), and Ar (t1/2 = 269 yr), possess nearly ideal chemical and physical properties for studies of earth and environmental processes. Recent advances in Atom Trap Trace Analysis (ATTA), a laser-based atom counting method, have enabled routine measurements of the radiokrypton isotopes, as well as the demonstration of the ability to measure 39Ar in environmental samples. -
Equation of State for Natural Gas Systems
Equation of State for Natural Gas Systems. m A thesis submitted to the University of London for the Degree of Doctor of Philosophy and for the Diploma of Imperial College by Jorge Francisco Estela-Uribe. Department of Chemical Engineering and Chemical Technology Imperial College of Science, Technology and Medicine. Prince Consort Road, SW7 2BY London, United Kingdom. March 1999. Acknowledgements. I acknowledge and thank the sponsorship I received from the following institutions: Fundacion para el Futuro de Colombia, Colfiituro; Pontificia Universidad Javeriana, Seccional Cali; the Committee of Vice-Chancellors and Principal of the Universities of the United Kingdom and Ruhrgas AG. Without their economic support my stay in London and the completion of this work would have been impossible. My greatest gratitude goes to my Supervisor, Dr Martin Trusler. His expert guidance and advice were always fundamental for the success of this research. He helped me with abundant patience and undying commitment and his optimism regarding the possibilities of the project was always inspirational for me. He also worked shoulder by shoulder with me on solving a good number of experimental problems, some of them were just cases of bad luck and for some prominent ones, I was the only one to blame. Others helped me willingly as well. My labmate, Dr Andres Estrada-Alexanders, was quite helpful in the beginning of my research, and has carried on being so. He not only did do well in his role as the senior student in the laboratory, but also became a good fnend of mine. Another good friend of mine, Dr Abdel Fenghour, has always been an endless source of help and information. -
Appendix a Basics of Landfill
APPENDIX A BASICS OF LANDFILL GAS Basics of Landfill Gas (Methane, Carbon Dioxide, Hydrogen Sulfide and Sulfides) Landfill gas is produced through bacterial decomposition, volatilization and chemical reactions. Most landfill gas is produced by bacterial decomposition that occurs when organic waste solids, food (i.e. meats, vegetables), garden waste (i.e. leaf and yardwaste), wood and paper products, are broken down by bacteria naturally present in the waste and in soils. Volatilization generates landfill gas when certain wastes change from a liquid or solid into a vapor. Chemical reactions occur when different waste materials are mixed together during disposal operations. Additionally, moisture plays a large roll in the speed of decomposition. Generally, the more moisture, the more landfill gas is generated, both during the aerobic and anaerobic conditions. Landfill Gas Production and Composition: In general, during anaerobic conditions, the composition of landfill gas is approximately 50 percent methane and 50 percent carbon dioxide with trace amounts (<1 percent) of nitrogen, oxygen, hydrogen sulfide, hydrogen, and nonmethane organic compounds (NMOCs). The more organic waste and moisture present in a landfill, the more landfill gas is produced by the bacteria during decomposition. The more chemicals disposed in a landfill, the more likely volatile organic compounds and other gasses will be produced. The Four Phases of Bacterial Decomposition: “Bacteria decompose landfill waste in four phases. The composition of the gas produced changes with each of the four phases of decomposition. Landfills often accept waste over a 20-to 30-year period, so waste in a landfill may be undergoing several phases of decomposition at once. -
Hugh Bradner's Development of the First Wet Suit
UC San Diego SIO Reference Title Wet Suit Pursuit: Hugh Bradner's Development of the First Wet Suit Permalink https://escholarship.org/uc/item/7353g3dj Author Rainey, Carolyn Publication Date 1998-11-01 eScholarship.org Powered by the California Digital Library University of California Wet Suit Pursuit: Hugh Bradner's Development of the First Wet Suit Carolyn Rainey Archives of the Scripps Institution of Oceanography University of California, San Diego La Jolla, CA 92093-0219 November 1998 SIO Reference Number 98-16 In the 100th anniversary issue of Sunset Magazine, published May 1998, the “ongoing timeline of major events” says that in 1952 UC Berkeley physicist Hugh Bradner invented the wet suit. This single fact summarizes a more complex story. In the spring of 1951 Bradner decided to spend some “weekend time” improving the equipment for the navy frogmen. Soon thereafter, he sent ideas and concepts of the wet suit to UC Berkeley physicist, Lauriston C. “Larry” Marshall, who was involved in a U.S. Navy/National Research Council Panel on Underwater Swimmers. In the fall of 1951 the effort to actively develop the wet suit began when colleagues at the Berkeley Radiation Lab joined Bradner in the fabrication and testing of various materials. At the end of 1949, the U.S. Marine Corps, U.S. Navy, and National Research Council agreed to work together using scientific applications to solve amphibious operational problems. A committee was formed under the chairmanship of UC Berkeley engineer Murrough P. “Mike” O’Brien. Several government panels met to discuss and watch East Coast and West Coast underwater demolition teams in action. -
Inert Gas & Winemaking a Moremanual !™ by Shea A.J
Inert Gas & Winemaking A MoreManual !™ by Shea A.J. Comfort www.MoreWineMaking.com 1–800–823–0010 The Importance of Inert Gas therefore eliminating any headspace (as is the case when filling/topping-up barrels), but as we shall see in the next During aging, if a wine is not protected from both microbial section this may not always be practical. spoilage and oxygen at all times it is likely to spoil. Protecting wine usually involves maintaining proper SO 2 Expansion & Contraction — The Need For levels and keeping containers full. Additionally, purging your headspaces with inert gas to effectively remove the Headspaces: oxygen greatly increases the amount of protection. When Unless you are in a situation with a guarantee of temperature stability, as with a glycol-jacketed tank, or a it comes to using SO2, the benefits are widely understood and in-depth information describing its usage is readily temperature-controlled storage area, tanks and carboys available in most winemaking literature. Yet, often when should have a small headspace kept at the top (note that these texts refer to purging with inert gas they fail to barrels should not have any space in them when filled/ explain the actual, step-by-step techniques needed to topped). This headspace is needed because it helps to do so. It is important be aware that creating an effective compensate for the expansion and contraction of the blanket of gas to protect your wine requires more than liquid due to ambient temperature changes (remember just shooting some Argon into the headspace of your things expand when heated and contract when cooled). -
Biological Effects of Noble Gases
Physiol. Res. 56 (Suppl. 1): S39-S44, 2007 Biological Effects of Noble Gases J. RŮŽIČKA, J. BENEŠ, L. BOLEK, V. MARKVARTOVÁ Department of Biophysics, Medical Faculty of Charles University, Plzeň, Czech Republic Received May 23, 2007 Accepted May 29, 2007 On-line available May 31, 2007 Summary Noble gases are known for their inertness. They do not react chemically with any element at normal temperature and pressure. Through that, some of them are known to be biologically active by their sedative, hypnotic and analgesic properties. Common inhalation anesthetics are characterized by some disadvantages (toxicity, decreased cardiac output, etc). Inhalation of xenon introduces anesthesia and has none of the above disadvantages, hence xenon seems to be the anesthetic gas of the future (with just one disadvantage – its cost). It is known that argon has similar anesthetic properties (under hyperbaric conditions), which is much cheaper and easily accessible. The question is if this could be used in clinical practice, in anesthesia of patients who undergo treatment in the hyperbaric chamber. Xenon was found to be organ-protective. Recent animal experiments indicated that xenon decreases infarction size after ischemic attack on brain or heart. The goal of our study is to check if hyperbaric argon has properties similar to those of xenon. Key words Noble gases • Xenon• Argon • Diving • Anesthesia • Stroke Introduction it is the point of this work. Above all, available information and our own observation concerning xenon Helium, neon, argon, krypton, xenon and radon and argon will be gathered here. are elements of the eighth group of the periodic table of Argon is the longest known and the least rare gas elements. -
CHEMICAL ACTIVITY of NOBLE GASES Kr and Xe and ITS IMPACT on FISSION GAS ACCUMULATION in the IRRADIATED UO2 FUEL M
ANNUAL REPORT 2005 Nuclear Technology in Energy Generation CHEMICAL ACTIVITY OF NOBLE GASES Kr AND Xe AND ITS IMPACT ON FISSION GAS ACCUMULATION IN THE IRRADIATED UO2 FUEL M. Szuta Institute of Atomic Energy It is generally accepted that most of the insoluble We can further assume that above a limiting value inert gas atoms Xe and Kr produced during fissioning of fission fluency (burn-up) a more intensive process of are retained in the fuel irradiated at a temperature lower irradiation induced chemical interaction occurs. Signifi- than the threshold. Some authors assume random diffu- cant part of fission gas product is thus expected to be sion of gas atoms to grain boundaries and consider the chemically bound in the matrix of UO2. effect of trapping the atoms at inter-granular bubbles From the moment of discovering the rare gases until saturation occurs. Others confirmed that bubbles (helium, neon, argon, krypton, xenon and radon) at the tend to concentrate in the grain boundaries during irra- end of XIX century until to the beginning of sixties diation. Likewise, some authors further assume that years of XX century it was considered that the noble most of the gas atoms are retained in solution in the gases are chemically inactive. matrix of grains being there immobilised or are precipi- The nobility of rare gases started to deteriorate af- tated into small fission gas bubbles. ter the first xenon compound was found by Barlett in The experimental data presented in the open litera- 1962 [1]. Barlett showed that the noble gases are capa- ture imply that we can assume that after irradiation ble of forming what one could consider as normal exposure in excess of 1018 fissions/cm3 the single gas chemical compounds, compelling chemists to readjust atom diffusion can be disregarded in description of considerably their thinking regarding these elements. -
Hugh Bradner Papers
http://oac.cdlib.org/findaid/ark:/13030/c8g73kjm Online items available Hugh Bradner Papers Special Collections & Archives, UC San Diego Special Collections & Archives, UC San Diego Copyright 2017 9500 Gilman Drive La Jolla 92093-0175 [email protected] URL: http://libraries.ucsd.edu/collections/sca/index.html Hugh Bradner Papers SMC 0016 1 Descriptive Summary Languages: English Contributing Institution: Special Collections & Archives, UC San Diego 9500 Gilman Drive La Jolla 92093-0175 Title: Hugh Bradner Papers Creator: Bradner, Hugh, 1915-2008 Identifier/Call Number: SMC 0016 Physical Description: 17.5 Linear feet(16 cartons and 3 oversize folders) Date (inclusive): 1935-1998 Abstract: Papers of physicist Hugh Bradner, including his correspondence, research files, teaching material and writings. Scope and Content of Collection Papers of physicist Hugh Bradner, including his correspondence, research files, teaching material and writings. Subjects of note include high energy physics, ocean-bottom seismology, DUMAND and the history of the wet suit. Arranged in nine series: 1) BIOGRAPHICAL FILES, 2) CORRESPONDENCE, 3) SUBJECT FILES, 4) GROUPS AND ORGANIZATIONS, 5) PROJECTS AND RESEARCH, 6) DEEP UNDERWATER MUON AND NEUTRINO DETECTOR PROJECT (DUMAND), 7) DIVING, 8) WRITINGS, COURSE MATERIALS AND NOTES and 9) PHOTOGRAPHS AND SLIDES. Biography Hugh Bradner (1915-2008) was a physicist who worked for the Manhattan Project and the Lawrence Berkeley National Laboratory before joining the SIO Institute of Geophysics and Planetary Physics (IGPP) as a geophysicist. He received his B.A. from Miami University in 1937 and graduated from Caltech with a Ph.D. in Physics in 1941. Bradner worked as a researcher for the Naval Ordnance Laboratory between 1941 and 1943 studying the design of magnetic naval mines. -
Interview with Wheeler J. North
WHEELER J. NORTH (1922–2002) INTERVIEWED BY SHELLEY ERWIN October 6–December 1, 1998 ARCHIVES CALIFORNIA INSTITUTE OF TECHNOLOGY Pasadena, California Subject area Engineering, environmental engineering, marine ecology Abstract Interview in 1998 with Wheeler North, professor of environmental science, emeritus, in the Division of Engineering and Applied Science. North received a BS in electrical engineering (1944) and biology (1950) from Caltech, and PhD (1953) from the University of California, Scripps Institution of Oceanography. His principal research interest is marine ecology, specifically the kelp beds off Southern California and the sea urchin population. He discusses effects of sewage outfalls and El Niño on kelp beds, the predations of sea urchins, and consulting for California’s kelp-harvesting industry. Recalls diving and experiments with early scuba equipment as student at Caltech. At Scripps, he worked with group studying the physiology of diving. Postgraduate work with NSF fellowship at Cambridge. Returned to Scripps with fellowship from Rockefeller Foundation, worked on photoreception in Metridium, taught diving course. In 1963, he joined Jack McKee’s environmental engineering science program at Caltech. Comments on early days of the program; his work at Caltech’s Kerckhoff Marine Laboratory at Corona del Mar; growing interest in the environment in 1970s and popularity of his ecology course among undergraduates and graduate students in various disciplines. Discusses 1969 oil- http://resolver.caltech.edu/CaltechOH:OH_North_W well blowout off Santa Barbara; contrast with Tampico oil spill off Baja in 1957. Discusses funding from National Science Foundation, after 1973 oil crisis, for kelp farms to produce biomass as an alternative fuel; later funding by General Electric, Department of Energy, and Gas Research Institute. -
Natural Gas Compressibility Factor Correlation Evaluation for Niger Delta Gas Fields
IOSR Journal of Electrical and Electronics Engineering (IOSR-JEEE) e-ISSN: 2278-1676,p-ISSN: 2320-3331, Volume 6, Issue 4 (Jul. - Aug. 2013), PP 01-10 www.iosrjournals.org Natural Gas Compressibility Factor Correlation Evaluation for Niger Delta Gas Fields Obuba, J*.1, Ikiesnkimama, S.S.2, Ubani, C. E.3, Ekeke, I. C.4 12Petroleum/Gas, Engineering/ University of Port Harcourt, Nigeria 3Department of Petroleum and Gas Engineering University of Port Harcourt Port Harcourt, Rivers State. 4Department of Chemical Engineering Federal University of Technology Oweri, Imo State Nigeria. Abstract: Natural gas compressibility factor (Z) is key factor in gas industry for natural gas production and transportation. This research presents a new natural gas compressibility factor correlation for Niger Delta gas fields. First, gas properties databank was developed from twenty-two (22) laboratory Gas PVT Reports from Niger Delta gas fields. Secondly, the existing natural gas compressibility factor correlations were evaluated against the developed database (comprising 22 gas reservoirs and 223 data sets). The developed new correlation was used to compute the z-factors for the four natural gas reservoir system of dry gas, solution gas, rich CO2 gas and rich condensate gas reservoirs, and the results were compared with some exiting correlations. The performances of the developed correction indicated better statistical ranking, good graph trends and best crossplots parity line when compared with correlations evaluated. From the results the new developed correlation has the least standard error and absolute error of (stdEr) of 1.461% and 1.669% for dry gas; 6.661% and 1.674% for solution; 7.758% and 6.660% for rich CO2 and 7.668% and 6.661 % for rich condensate gas reservoirs.