Science.gov

Sample records for 2-3 billion people

  1. Four billion people facing severe water scarcity.

    PubMed

    Mekonnen, Mesfin M; Hoekstra, Arjen Y

    2016-02-01

    Freshwater scarcity is increasingly perceived as a global systemic risk. Previous global water scarcity assessments, measuring water scarcity annually, have underestimated experienced water scarcity by failing to capture the seasonal fluctuations in water consumption and availability. We assess blue water scarcity globally at a high spatial resolution on a monthly basis. We find that two-thirds of the global population (4.0 billion people) live under conditions of severe water scarcity at least 1 month of the year. Nearly half of those people live in India and China. Half a billion people in the world face severe water scarcity all year round. Putting caps to water consumption by river basin, increasing water-use efficiencies, and better sharing of the limited freshwater resources will be key in reducing the threat posed by water scarcity on biodiversity and human welfare. PMID:26933676

  2. Four billion people facing severe water scarcity

    PubMed Central

    Mekonnen, Mesfin M.; Hoekstra, Arjen Y.

    2016-01-01

    Freshwater scarcity is increasingly perceived as a global systemic risk. Previous global water scarcity assessments, measuring water scarcity annually, have underestimated experienced water scarcity by failing to capture the seasonal fluctuations in water consumption and availability. We assess blue water scarcity globally at a high spatial resolution on a monthly basis. We find that two-thirds of the global population (4.0 billion people) live under conditions of severe water scarcity at least 1 month of the year. Nearly half of those people live in India and China. Half a billion people in the world face severe water scarcity all year round. Putting caps to water consumption by river basin, increasing water-use efficiencies, and better sharing of the limited freshwater resources will be key in reducing the threat posed by water scarcity on biodiversity and human welfare. PMID:26933676

  3. Harnessing Energy from the Sun for Six Billion People

    ScienceCinema

    Daniel Nocera

    2013-07-19

    Daniel Nocera, a Massachusetts Institute of Technology professor whose recent research focuses on solar-powered fuels, presents a Brookhaven Science Associates Distinguished Lecture, titled "Harnessing Energy from the Sun for Six Billion People -- One at a Time."

  4. Harnessing Energy from the Sun for Six Billion People

    SciTech Connect

    Daniel Nocera

    2011-09-12

    Daniel Nocera, a Massachusetts Institute of Technology professor whose recent research focuses on solar-powered fuels, presents a Brookhaven Science Associates Distinguished Lecture, titled "Harnessing Energy from the Sun for Six Billion People -- One at a Time."

  5. The Population of China. One Billion, Eight Million People.

    ERIC Educational Resources Information Center

    Murphy, Elaine M.; Cancellier, Patricia

    1983-01-01

    Several programs have been instituted in China over the past 30 years in order to slow the birth rate. The population, set at 1,008,175,288 people by a 1982 census, is by far the largest of any nation. A 10-year family planning program, begun in 1957, caused the birth rate to drop considerably through the mid-1960's. In 1971, "wan xi shao," the…

  6. How to Bring Solar Energy to Seven Billion People (LBNL Science at the Theater)

    ScienceCinema

    Wadia, Cyrus

    2011-04-28

    By exploiting the powers of nanotechnology and taking advantage of non-toxic, Earth-abundant materials, Berkeley Lab's Cyrus Wadia has fabricated new solar cell devices that have the potential to be several orders of magnitude less expensive than conventional solar cells. And by mastering the chemistry of these materials-and the economics of solar energy-he envisions bringing electricity to the 1.2 billion people now living without it.

  7. Enrolling people with prediabetes ages 60-64 in a proven weight loss program could save Medicare $7 billion or more.

    PubMed

    Thorpe, Kenneth E; Yang, Zhou

    2011-09-01

    Rising chronic disease prevalence among Medicare beneficiaries, including new enrollees, is a key driver of health care spending. Randomized trials have shown that lifestyle modification interventions such as those in the National Diabetes Prevention Program clinical trial reduce the incidence of chronic disease and that community-based programs applying the same principles can produce net health care savings. We propose expanding a proven, community-based weight loss program nationwide and enrolling overweight and obese prediabetic adults ages 60-64. We estimate that making the program available to a single cohort of eligible people could save Medicare $1.8-$2.3 billion over the following ten years. Estimated savings would be even higher ($3.0-$3.7 billion) if equally overweight people at risk for cardiovascular disease were also enrolled. We estimate that lifetime Medicare savings could range from approximately $7 billion to $15 billion, depending on how broadly program eligibility was defined and actual levels of program participation, for a single "wave" of eligible people. In this context we propose that Medicare expand its new wellness benefit to include reimbursement for this and other qualifying behavior change programs. PMID:21900657

  8. Providing safe drinking water to 1.2 billion unserved people

    SciTech Connect

    Gadgil, Ashok J.; Derby, Elisabeth A.

    2003-06-01

    Despite substantial advances in the past 100 years in public health, technology and medicine, 20% of the world population, mostly comprised of the poor population segments in developing countries (DCs), still does not have access to safe drinking water. To reach the United Nations (UN) Millennium Goal of halving the number of people without access to safe water by 2015, the global community will need to provide an additional one billion urban residents and 600 million rural residents with safe water within the next twelve years. This paper examines current water treatment measures and implementation methods for delivery of safe drinking water, and offers suggestions for making progress towards the goal of providing a timely and equitable solution for safe water provision. For water treatment, based on the serious limitations of boiling water and chlorination, we suggest an approach based on filtration coupled with ultraviolet (UV) disinfection, combined with public education. Additionally, owing to the capacity limitations for non-governmental organizations (NGOs) to take on this task primarily on their own, we suggest a strategy based on financially sustainable models that include the private sector as well as NGOs.

  9. Missing billions.

    PubMed

    Conly, S

    1997-01-01

    This article discusses funding of population programs that support the Cairo International Conference on Population and Development's Plan of Action. The Plan of Action calls for a quadrupling of annual financial commitments for population programs to $17 billion by the year 2000 and $22 billion by 2015. The increased expenditures would cover the increased demand for services from unmet need and population growth. Donor countries are expected to increase their share from the current 25% to about 33%, or $5.7 billion by the year 2000. The estimates are in 1993 constant dollars. $17 billion is less than the $40 billion that is spent worldwide on playing golf. During 1993-94, general donor support increased to $1.2 billion. Denmark, Germany, Japan, the Netherlands, the United Kingdom, and the United States increased their support. The United States doubled its support for population programs during 1992-95 to $583 million. During 1996-97 the US Congress cut funding back to the 1995 level. France, Italy, Spain, Belgium, and Austria have lagged in support for population programs in the present and the past. Equal burden sharing would require the US to increase funding to $1.9 billion. Developed country assistance declined to the lowest share of combined gross national product since 1970. This shifts the burden to multilateral sources. The European Union is committed to increasing its funding, and the World Bank increased funding for population and reproductive health to about $600 million in 1996 from $424 million in 1994. Bangladesh, China, India, Indonesia, Mexico, South Africa, and Turkey spent 85% of all government expenditures on family planning in developing countries. External donors in Africa are the main support of family planning. Private consumers in Latin America pay most of the costs of family planning. External assistance will be needed for some time. PMID:12321013

  10. Nine billion or bust?

    NASA Astrophysics Data System (ADS)

    nerd, nerd; Pepperday, Mike; Szautner, a. a. z.

    2014-02-01

    In reply to a review of Tony Ryan and Steve McKevitt's book Project Sunshine, which explores ways in which the Earth could support a future population of nine billion people (Letting the sunshine in, November 2013 pp50-51, http://ow.ly/r0FTM).

  11. Can the World's Farmers Feed a World of 10 Billion People In Spite of Climate Change? (Invited)

    NASA Astrophysics Data System (ADS)

    Easterling, W. E.

    2010-12-01

    The rapid rise in agricultural productivity due to technological innovation and science-based methods was one of the great human achievements of the 20th century. We now face the prospect of needing to double agricultural output by the latter third of the current century to match the growth of demand for food and fiber—albeit the pace of growth in demand shows signs of slowing in the future. How farmers and the agricultural industry deal with climate change will, in large measure, determine success or failure. The Earth is committed to about the same amount of warming in the future as has been experienced over the past hundred years regardless of future greenhouse gas emissions trajectories; such will require adaptive responses by plants, animals, producers and consumers if society’s goals for global food security are to be met. In this paper, I summarize the state-of-the science of how climate change may affect our global agricultural production system. I review the latest thinking on the combined effects of rising atmospheric CO2 concentration and climate changes on crop productivity across the globe. Prospects for adaptation in agriculturally important regions are examined. While it appears that global food production will be adequate to meet global food demand in spite of advancing climate change, it is clear that many parts of the tropics and dry sub-tropics will see yield decreases and possible loss of comparative advantage. In those regions, continued large population growth and deleterious climate changes will contribute to declining per capita agricultural production. Increasing numbers of people at risk of hunger are probable there.

  12. Spend Billions and They Will Come

    ERIC Educational Resources Information Center

    Fox, Bette-Lee

    2004-01-01

    People look at one billion dollars in one of two ways: if it is the result of the long, hard effort of years of fundraising, they rejoice; if it signifies an astronomical budget deficit, they cringe. How, then, should people respond as a community to reaching the $1 billion mark ($1,242,436,438, to be exact) in this year's spending for public…

  13. People

    NASA Astrophysics Data System (ADS)

    2001-05-01

    microscopes, chemical analyses etc. The NHM has big labs—like a university—in the basement. I write papers, give talks... For the public galleries of the NHM my group provides expert input to exhibitions-when the meteorite pavilion was recently refurbished we suggested a layout, wrote text and selected samples, but this was then 'edited' by the exhibition designers. I'm also working on a new website with virtual meteorite specimens. As an expert on Martian meteorites I often get interviewed by the media: for example, I am on a new Channel 4 programme called Destination Mars. I have also just finished a general interest book—it's called Search for Life; the NHM have just published it (in March). And do you get to go to exciting places? As a researcher I go to conferences I am just off to the States this week. I went to Antarctica ten years ago meteorite collecting and I am hoping to go to Australia this year. It is good fun but they really do need an expert who can recognise a meteorite. I'll be going to the Nullarbor region of Australia for 2 3 weeks depending on the weather if it's too green there is too much grass, so you can't see the meteorites. How do you find people respond to meteorites? People love touching rocks from outer space, especially primary school children. You can see how they are burnt on the outside. When you feel the weight of them it really brings it home: iron meteorites are heavy! They'll often say 'Wow, it fell from the sky' as they glance upwards, half expecting another one to come crashing through the ceiling. Everyone finds it amazing that a solid object has come as if from nowhere. And they are so old. They can't believe how old they are. We want to know where we come from. There is always lots of media coverage about what is happening in the sky (eclipses and the like). It's there and it's a bit of a mystery. If we can get to grips with how our planets and how our own Sun formed it can put us in the picture as to where we have come from and

  14. Atmospheric oxygenation three billion years ago.

    PubMed

    Crowe, Sean A; Døssing, Lasse N; Beukes, Nicolas J; Bau, Michael; Kruger, Stephanus J; Frei, Robert; Canfield, Donald E

    2013-09-26

    It is widely assumed that atmospheric oxygen concentrations remained persistently low (less than 10(-5) times present levels) for about the first 2 billion years of Earth's history. The first long-term oxygenation of the atmosphere is thought to have taken place around 2.3 billion years ago, during the Great Oxidation Event. Geochemical indications of transient atmospheric oxygenation, however, date back to 2.6-2.7 billion years ago. Here we examine the distribution of chromium isotopes and redox-sensitive metals in the approximately 3-billion-year-old Nsuze palaeosol and in the near-contemporaneous Ijzermyn iron formation from the Pongola Supergroup, South Africa. We find extensive mobilization of redox-sensitive elements through oxidative weathering. Furthermore, using our data we compute a best minimum estimate for atmospheric oxygen concentrations at that time of 3 × 10(-4) times present levels. Overall, our findings suggest that there were appreciable levels of atmospheric oxygen about 3 billion years ago, more than 600 million years before the Great Oxidation Event and some 300-400 million years earlier than previous indications for Earth surface oxygenation. PMID:24067713

  15. People

    NASA Astrophysics Data System (ADS)

    2001-01-01

    Thrilled at @Bristol Kathy Sykes in conversation with Liz Whitelegg. Kathy Sykes is Senior Science Consultant at @Bristol - a new area on Bristol's Harbourside with a Science Centre Explore, a Wildlife Centre Wildscreen, with sculptures and fountains. Kathy was one of five people in 1999 to be awarded an IOP Public Awareness of Physics award. Dr Kathy Sykes What attracted you to Physics in the first place? It was really when I discovered that Physics was all about making models of the world, because then suddenly the ability to be creative became important. I liked the idea that you could have a picture of the world that might work quite well but you could always replace that with a better one. That was what made science come alive and make it seem like something that I'd really love to be involved in, rather than science as a stale body of facts that I needed to learn. I was much more interested in ideas than in facts. I think that finding out about 'models' happened around the time I was discovering quantum mechanics and how the act of observing something can actually affect the outcome. I found it incredibly exciting - especially how that changed the whole philosophy of science. I also had a fantastic teacher in physics and I owe an awful lot to him. He just swooped in at the last moment when I was considering giving it up so that made an enormous difference. After my degree I went to teach maths and physics A-level in Zimbabwe with the VSO, and it was partly wanting to share my excitement with other people about physics that made me want to go and teach abroad. When I came back and began my PhD in Physics at Bristol University, I missed teaching and thought it was important to get the public more involved in science and debates about science. My supervisor, Pete Barham, was doing lots of this himself, and he helped and encouraged me enormously. I can't thank him enough. Did you consider teaching as a career? Well I like having the carpet whipped away from

  16. People

    NASA Astrophysics Data System (ADS)

    2001-01-01

    Thrilled at @Bristol Kathy Sykes in conversation with Liz Whitelegg. Kathy Sykes is Senior Science Consultant at @Bristol - a new area on Bristol's Harbourside with a Science Centre Explore, a Wildlife Centre Wildscreen, with sculptures and fountains. Kathy was one of five people in 1999 to be awarded an IOP Public Awareness of Physics award. Dr Kathy Sykes What attracted you to Physics in the first place? It was really when I discovered that Physics was all about making models of the world, because then suddenly the ability to be creative became important. I liked the idea that you could have a picture of the world that might work quite well but you could always replace that with a better one. That was what made science come alive and make it seem like something that I'd really love to be involved in, rather than science as a stale body of facts that I needed to learn. I was much more interested in ideas than in facts. I think that finding out about 'models' happened around the time I was discovering quantum mechanics and how the act of observing something can actually affect the outcome. I found it incredibly exciting - especially how that changed the whole philosophy of science. I also had a fantastic teacher in physics and I owe an awful lot to him. He just swooped in at the last moment when I was considering giving it up so that made an enormous difference. After my degree I went to teach maths and physics A-level in Zimbabwe with the VSO, and it was partly wanting to share my excitement with other people about physics that made me want to go and teach abroad. When I came back and began my PhD in Physics at Bristol University, I missed teaching and thought it was important to get the public more involved in science and debates about science. My supervisor, Pete Barham, was doing lots of this himself, and he helped and encouraged me enormously. I can't thank him enough. Did you consider teaching as a career? Well I like having the carpet whipped away from

  17. People

    NASA Astrophysics Data System (ADS)

    2001-09-01

    ASE: Attend, Socialize, Enjoy Bob Kibble reflects on the enriching effects of the annual meeting Bob Kibble is a teacher trainer at the University of Edinburgh, Scotland. I remember my first ASE meeting in Reading. Perhaps in 1978 or thereabouts. I had been teaching for a few years and thought I'd check out this local convention of science teachers. It was indeed a revelation that so many people had so much to say about teaching science. There was talk about N and F levels and the 'I level grill'. Someone had ordered something called a BBC machine (later revealed to me as the latest in hi-tech teaching). I remember it well. But it was a lonely affair for a recent recruit. People seemed to know each other and there was much friendly exchanging. However, nobody knew me and I knew nobody else. The professional revelations were accompanied by a personal isolation. A strange set of memories indeed for a new recruit, unskilled and clumsy in the social arena. Bob practising for the ASE singalong session this year. This year I went to the ASE Centenary meeting in Guildford, my sixteenth ASE annual meeting. Things have changed since the early days. Thursday started with a formal Cathedral service in celebration of 100 years of the ASE. I sat next to a lady from Oxford and behind my good friend Dave from Croydon. Things snowballed from there. I went to a workshop on the water cycle and was brought face to face with my own misconceptions about the life story of a water molecule. Got a freebie coloured bracelet as well. Thanks Margaret. A chap from Bournemouth gave me loads of ideas about how best to set up a shared lesson observation scheme as well as how to run a professional development workshop. Thanks Stuart. At a third session I joined Brenda from Cambridge and we spent an enjoyable hour discovering ways to approach the teaching of light and in particular Ibn al Haytham's revelations courtesy of a chap from Kingston. That afternoon I was invited to present a talk to

  18. People

    NASA Astrophysics Data System (ADS)

    2001-11-01

    the war Hoyle returned to Cambridge, but kept in close contact with his collaborators. Fred Hoyle was a canny and media-savvy scientist, 40 years before such things were recognized. Martin Rees said after his death '[He] also had other dimensions to his career, his inventiveness and skill as a communicator'. It is hard to realize now the impact that Hoyle's broadcasts had in post-war Britain. His programmes for the BBC on The Nature of the Universe won greater audiences than such unlikely rivals as Bertrand Russell and Tommy Handley. Even today many people recall how they were affected by listening to these broadcasts. Hoyle used one of his broadcasts to ridicule the hot explosion theory. He referred to the idea of a 'big bang as fanciful'. Unfortunately the name stuck, much to Hoyle's chagrin. In the 1950s Hoyle began a fruitful collaboration with Willy Fowler of the California Institute of Technology in Pasadena. Hoyle was interested in the origin of the chemical elements. Hans Bethe, Charles Critchfield and Karl-Frederich von Weizsäcker had calculated in 1939 how stars could turn protons into helium nuclei by nuclear fusion. Part of the Vela supernova remmant, the debris left after the type of massive explosion in which Hoyle predicted that heavy nuclei were formed. (© Royal Observatory, Edinburgh, Anglo-Australian Observatory.) Building on earlier collaboration with Ed Saltpeter, Hoyle used data supplied by Geoffrey and Margaret Burbidge and, working with Fowler, began to piece together how the elements were formed. By looking at very large stars near the end of their lives and examining their chemical composition, they noticed that the abundances of elements almost exactly corresponded to those with a low nuclear capture cross section. Hoyle argued that all of the elements in our bodies had been formed in stars that had been and gone before our solar system had even formed. In their classic paper the elements are produced by three basic methods. The

  19. People

    NASA Astrophysics Data System (ADS)

    2001-11-01

    the war Hoyle returned to Cambridge, but kept in close contact with his collaborators. Fred Hoyle was a canny and media-savvy scientist, 40 years before such things were recognized. Martin Rees said after his death '[He] also had other dimensions to his career, his inventiveness and skill as a communicator'. It is hard to realize now the impact that Hoyle's broadcasts had in post-war Britain. His programmes for the BBC on The Nature of the Universe won greater audiences than such unlikely rivals as Bertrand Russell and Tommy Handley. Even today many people recall how they were affected by listening to these broadcasts. Hoyle used one of his broadcasts to ridicule the hot explosion theory. He referred to the idea of a 'big bang as fanciful'. Unfortunately the name stuck, much to Hoyle's chagrin. In the 1950s Hoyle began a fruitful collaboration with Willy Fowler of the California Institute of Technology in Pasadena. Hoyle was interested in the origin of the chemical elements. Hans Bethe, Charles Critchfield and Karl-Frederich von Weizsäcker had calculated in 1939 how stars could turn protons into helium nuclei by nuclear fusion. Part of the Vela supernova remmant, the debris left after the type of massive explosion in which Hoyle predicted that heavy nuclei were formed. (© Royal Observatory, Edinburgh, Anglo-Australian Observatory.) Building on earlier collaboration with Ed Saltpeter, Hoyle used data supplied by Geoffrey and Margaret Burbidge and, working with Fowler, began to piece together how the elements were formed. By looking at very large stars near the end of their lives and examining their chemical composition, they noticed that the abundances of elements almost exactly corresponded to those with a low nuclear capture cross section. Hoyle argued that all of the elements in our bodies had been formed in stars that had been and gone before our solar system had even formed. In their classic paper the elements are produced by three basic methods. The

  20. Endemic Cardiovascular Diseases of the Poorest Billion.

    PubMed

    Kwan, Gene F; Mayosi, Bongani M; Mocumbi, Ana O; Miranda, J Jaime; Ezzati, Majid; Jain, Yogesh; Robles, Gisela; Benjamin, Emelia J; Subramanian, S V; Bukhman, Gene

    2016-06-14

    The poorest billion people are distributed throughout the world, though most are concentrated in rural sub-Saharan Africa and South Asia. Cardiovascular disease (CVD) data can be sparse in low- and middle-income countries beyond urban centers. Despite this urban bias, CVD registries from the poorest countries have long revealed a predominance of nonatherosclerotic stroke, hypertensive heart disease, nonischemic and Chagas cardiomyopathies, rheumatic heart disease, and congenital heart anomalies, among others. Ischemic heart disease has been relatively uncommon. Here, we summarize what is known about the epidemiology of CVDs among the world's poorest people and evaluate the relevance of global targets for CVD control in this population. We assessed both primary data sources, and the 2013 Global Burden of Disease Study modeled estimates in the world's 16 poorest countries where 62% of the population are among the poorest billion. We found that ischemic heart disease accounted for only 12% of the combined CVD and congenital heart anomaly disability-adjusted life years (DALYs) in the poorest countries, compared with 51% of DALYs in high-income countries. We found that as little as 53% of the combined CVD and congenital heart anomaly burden (1629/3049 DALYs per 100 000) was attributed to behavioral or metabolic risk factors in the poorest countries (eg, in Niger, 82% of the population among the poorest billion) compared with 85% of the combined CVD and congenital heart anomaly burden (4439/5199 DALYs) in high-income countries. Further, of the combined CVD and congenital heart anomaly burden, 34% was accrued in people under age 30 years in the poorest countries, while only 3% is accrued under age 30 years in high-income countries. We conclude although the current global targets for noncommunicable disease and CVD control will help diminish premature CVD death in the poorest populations, they are not sufficient. Specifically, the current framework (1) excludes deaths of

  1. Food security: the challenge of feeding 9 billion people.

    PubMed

    Godfray, H Charles J; Beddington, John R; Crute, Ian R; Haddad, Lawrence; Lawrence, David; Muir, James F; Pretty, Jules; Robinson, Sherman; Thomas, Sandy M; Toulmin, Camilla

    2010-02-12

    Continuing population and consumption growth will mean that the global demand for food will increase for at least another 40 years. Growing competition for land, water, and energy, in addition to the overexploitation of fisheries, will affect our ability to produce food, as will the urgent requirement to reduce the impact of the food system on the environment. The effects of climate change are a further threat. But the world can produce more food and can ensure that it is used more efficiently and equitably. A multifaceted and linked global strategy is needed to ensure sustainable and equitable food security, different components of which are explored here. PMID:20110467

  2. Agroecohydrology: Key to Feeding 9 Billion?

    NASA Astrophysics Data System (ADS)

    Herrick, J.

    2011-12-01

    Agricultural production necessary to feed 9 billion people in 2050 depends on increased production on existing croplands, and expanding onto 'marginal' lands. A high proportion of these lands are marginal because they are too steep or too dry to reliably support crop production. These same characteristics increase their susceptibility to accelerated erosion, leading (for most soil profiles) to further reductions in plant available water as infiltration and soil profile water holding capacity decline. Sustaining production on these marginal lands will require careful land use planning. In this paper, we present a land use planning framework that integrates 4 elements: (1) potential production (based on soil profile characteristics), (2) edaphic, topographic and climatic limitations to production, (3) soil resistance to degradation, and (4) resilience. This framework expands existing land capability classification systems through the integration of biophysical feedbacks and thresholds. State and transition models, similar to those currently applied to rangelands in the United States and other countries, are used to organize and communicate knowledge about the sustainability of different land use changes and management actions at field to regional scales. This framework emphasizes hydrologic characteristics of soil profiles and landscapes over fertility because fertility declines are more easily addressed through increased inputs. The presentation will conclude with a discussion of how research in ecohydrology can be more effectively focused to support sustainable food production in the context of increasingly rapid social and economic changes throughout the world.

  3. Life with Four Billion Atoms

    SciTech Connect

    Knight, Thomas

    2013-04-10

    Today it is commonplace to design and construct single silicon chips with billions of transistors. These are complex systems, difficult (but possible) to design, test, and fabricate. Remarkably, simple living systems can be assembled from a similar number of atoms, most of them in water molecules. In this talk I will present the current status of our attempts at full understanding and complexity reduction of one of the simplest living systems, the free-living bacterial species Mesoplasma florum. This 400 nm diameter cell thrives and replicates every 40 minutes with a genome of only 800 kilobases. Our recent experiments using transposon gene knockouts identified 354 of 683 annotated genes as inessential in laboratory culture when inactivated individually. While a functional redesigned genome will certainly not remove all of those genes, this suggests that roughly half the genome can be removed in an intentional redesign. I will discuss our recent knockout results and methodology, and our future plans for Genome re-engineering using targeted knock-in/knock-out double recombination; whole cell metabolic models; comprehensive whole cell metabolite measurement techniques; creation of plug-and-play metabolic modules for the simplified organism; inherent and engineered biosafety control mechanisms. This redesign is part of a comprehensive plan to lay the foundations for a new discipline of engineering biology. Engineering biological systems requires a fundamentally different viewpoint from that taken by the science of biology. Key engineering principles of modularity, simplicity, separation of concerns, abstraction, flexibility, hierarchical design, isolation, and standardization are of critical importance. The essence of engineering is the ability to imagine, design, model, build, and characterize novel systems to achieve specific goals. Current tools and components for these tasks are primitive. Our approach is to create and distribute standard biological parts

  4. Countdown to Six Billion Teaching Kit.

    ERIC Educational Resources Information Center

    Zero Population Growth, Inc., Washington, DC.

    This teaching kit features six activities focused on helping students understand the significance of the world population reaching six billion for our society and our environment. Featured activities include: (1) History of the World: Part Six Billion; (2) A Woman's Place; (3) Baby-O-Matic; (4) Earth: The Apple of Our Eye; (5) Needs vs. Wants; and…

  5. 2,3-Dichloropropanol

    Integrated Risk Information System (IRIS)

    2,3 - Dichloropropanol ; CASRN 616 - 23 - 9 Human health assessment information on a chemical substance is included in the IRIS database only after a comprehensive review of toxicity data , as outlined in the IRIS assessment development process . Sections I ( Health Hazard Assessments for Noncarcino

  6. Billion shot flashlamp for spaceborne lasers

    NASA Technical Reports Server (NTRS)

    Richter, Linda; Schuda, Felix; Degnan, John

    1990-01-01

    A billion-shot flashlamp developed under a NASA contract for spaceborne laser missions is presented. Lifetime-limiting mechanisms are identified and addressed. Two energy loadings of 15 and 44 Joules were selected for the initial accelerated life testing. A fluorescence-efficiency test station was used for measuring the useful-light output degradation of the lamps. The design characteristics meeting NASA specifications are outlined. Attention is focused on the physical properties of tungsten-matrix cathodes, the chemistry of dispenser cathodes, and anode degradation. It is reported that out of the total 83 lamps tested in the program, 4 lamps reached a billion shots and one lamp is beyond 1.7 billion shots, while at 44 Joules, 4 lamps went beyond 100 million shots and one lamp reached 500 million shots.

  7. Where Have All the Billions Gone?

    ERIC Educational Resources Information Center

    Leask, Linda; And Others

    1987-01-01

    Providing a basis to help Alaskans determine future spending levels and priorities, this report traces how the state spent more than $26 billion in general funds from fiscal years 1981 through 1986 before oil prices crashed and brought state revenues tumbling down with them. Figures indicate that cumulative general fund expenditures over the…

  8. Thirteen billion years in half an hour

    NASA Astrophysics Data System (ADS)

    Bassett, Bruce A.

    2005-10-01

    We take a high-speed tour of the approximately thirteen billion-year history of our universe focusing on unsolved mysteries and the key events that have sculpted and shaped it - from inflation in the first split second to the dark energy which is currently causing the expansion of the cosmos to accelerate.

  9. Conservation in a World of Six Billion: A Grassroots Action Guide.

    ERIC Educational Resources Information Center

    Hren, Benedict J.

    This grassroots action guide features a conservation initiative working to bring the impacts of human population growth, economic development, and natural resource consumption into balance with the limits of nature for the benefit of current and future generations. Contents include information sheets entitled "Six Billion People and Growing,""The…

  10. Teledesic pushes $9-billion, 900-satellite system

    NASA Astrophysics Data System (ADS)

    1994-03-01

    Teledesic Corp. is seeking FCC approval to deploy a communication satellite system, costing $9 billion and using more than 900 satellites in low Earth orbit. This system would provide telephone and broadband data service to remote areas and developing countries. The two major stockholders in Teledesic are William Gates (of Microsoft Corp.) and Craig McCaw (of McCaw Cellular Communications). Each satellite would act as a node in a packet-switching network. The satellites would provide continuous global coverage.

  11. The nonprofit sector's $100 billion opportunity.

    PubMed

    Bradley, Bill; Jansen, Paul; Silverman, Les

    2003-05-01

    Imagine what an extra $100 billion a year could do for philanthropic and other nonprofit institutions. According to a new study, the nonprofit sector could free that amount--maybe even more--by making five changes in the way it operates. The study asked two central questions: Does the sector's money flow from its source to its ultimate use as efficiently and effectively as possible? If not, where are the big opportunities to increase social benefit? According to former senator Bill Bradley and McKinsey's Paul Jansen and Les Silverman, nonprofits could save roughly $25 billion a year by changing the way they raise funds. By distributing funds more quickly, they could put an extra $30 billion to work. Organizations could generate more than $60 billion a year by streamlining and restructuring the way in which they provide services and by reducing administrative costs. And they could free up even more money--an amount impossible to estimate--by better allocating funds among service providers. The authors admit that making those changes won't be easy. The nonprofit world, historically seen as a collection of locally focused charities, has become an enormous sector, but it lacks the managerial processes and incentives that help keep the for-profit world on track. And when the baby boomers start to retire in less than a decade, public budgets will be squeezed even more than they are today. If the nonprofit sector is to help the nation cope with the stresses ahead, it must become more efficient and challenge its traditional concepts of stewardship. PMID:12747166

  12. Medicare Spends Billions on Chronic Kidney Disease, Study Finds

    MedlinePlus

    ... nlm.nih.gov/medlineplus/news/fullstory_158020.html Medicare Spends Billions on Chronic Kidney Disease, Study Finds ... affects nearly 14 percent of Americans and costs Medicare billions of dollars a year, a new study ...

  13. Delivering on Obama's renewables promise will cost billions

    SciTech Connect

    2009-04-15

    For wind energy in the eastern half of the U.S., costs would be $50 billion to $80 billion for transmission lines, in addition to the $700 billion to $1.1 trillion to build the wind farms to generate power.

  14. Simulating Billion-Task Parallel Programs

    SciTech Connect

    Perumalla, Kalyan S; Park, Alfred J

    2014-01-01

    In simulating large parallel systems, bottom-up approaches exercise detailed hardware models with effects from simplified software models or traces, whereas top-down approaches evaluate the timing and functionality of detailed software models over coarse hardware models. Here, we focus on the top-down approach and significantly advance the scale of the simulated parallel programs. Via the direct execution technique combined with parallel discrete event simulation, we stretch the limits of the top-down approach by simulating message passing interface (MPI) programs with millions of tasks. Using a timing-validated benchmark application, a proof-of-concept scaling level is achieved to over 0.22 billion virtual MPI processes on 216,000 cores of a Cray XT5 supercomputer, representing one of the largest direct execution simulations to date, combined with a multiplexing ratio of 1024 simulated tasks per real task.

  15. Chinese TV: Better Broadcasting for the Billion.

    ERIC Educational Resources Information Center

    Hollstein, Milton

    Chinese television started in 1958 but variety in programming and production of sets priced within reach of individuals were slowed by the Cultural Revolution. Since the economic and political reform movement began in 1979, Chinese television has been maturing as an important cultural and political force. The People's Republic of China is a Third…

  16. Uranium in Canada: A billion dollar industry

    SciTech Connect

    Ruzicka, V. )

    1989-12-01

    In 1988, Canada maintained its position as the world's leading producer of uranium with an output of more than 12,400 MT of uranium in concentrates, worth $1.1 billion Canadian. As domestic requirements represent only 15% of current Canadian production, most of the output was exported. With current implementation of the Canada/US Free Trade Agreement, the US has become Canada's major uranium export customer. With a large share of the world's known uranium resources, Canada remains the focus of international uranium exploration activity. In 1988, the uranium exploration expenditures in Canada exceeded $58 million Canadian. The principal exploration targets were deposits associated with Proterozoic unconformities in Saskatchewan and Northwest Territories, particularly those in the Athabasca and Thelon basin regions of the Canadian Shield. Major attention was also paid to polymetallic deposits in which uranium is associated with precious metals, such as gold and platinum group elements. Conceptual genetic models for these deposit types represent useful tools to guide exploration.

  17. Eight billion asteroids in the Oort cloud

    NASA Astrophysics Data System (ADS)

    Shannon, Andrew; Jackson, Alan P.; Veras, Dimitri; Wyatt, Mark

    2015-01-01

    The Oort cloud is usually thought of as a collection of icy comets inhabiting the outer reaches of the Solar system, but this picture is incomplete. We use simulations of the formation of the Oort cloud to show that ˜4 per cent of the small bodies in the Oort cloud should have formed within 2.5 au of the Sun, and hence be ice-free rock-iron bodies. If we assume that these Oort cloud asteroids have the same size distribution as their cometary counterparts, the Large Synoptic Survey Telescope should find roughly a dozen Oort cloud asteroids during 10 years of operations. Measurement of the asteroid fraction within the Oort cloud can serve as an excellent test of the Solar system's formation and dynamical history. Oort cloud asteroids could be of particular concern as impact hazards as their high mass density, high impact velocity, and low visibility make them both hard to detect and hard to divert or destroy. However, they should be a rare class of object, and we estimate globally catastrophic collisions should only occur about once per billion years.

  18. Fuel efficient stoves for the poorest two billion

    NASA Astrophysics Data System (ADS)

    Gadgil, Ashok

    2012-03-01

    About 2 billion people cook their daily meals on generally inefficient, polluting, biomass cookstoves. The fuels include twigs and leaves, agricultural waste, animal dung, firewood, and charcoal. Exposure to resulting smoke leads to acute respiratory illness, and cancers, particularly among women cooks, and their infant children near them. Resulting annual mortality estimate is almost 2 million deaths, higher than that from malaria or tuberculosis. There is a large diversity of cooking methods (baking, boiling, long simmers, brazing and roasting), and a diversity of pot shapes and sizes in which the cooking is undertaken. Fuel-efficiency and emissions depend on the tending of the fire (and thermal power), type of fuel, stove characteristics, and fit of the pot to the stove. Thus, no one perfect fuel-efficient low-emitting stove can suit all users. Affordability imposes a further severe constraint on the stove design. For various economic strata within the users, a variety of stove designs may be appropriate and affordable. In some regions, biomass is harvested non-renewably for cooking fuel. There is also increasing evidence that black carbon emitted from stoves is a significant contributor to atmospheric forcing. Thus improved biomass stoves can also help mitigate global climate change. The speaker will describe specific work undertaken to design, develop, test, and disseminate affordable fuel-efficient stoves for internally displaced persons (IDPs) of Darfur, Sudan, where the IDPs face hardship, humiliation, hunger, and risk of sexual assault owing to their dependence on local biomass for cooking their meals.

  19. Redefining agricultural yields: from tonnes to people nourished per hectare

    NASA Astrophysics Data System (ADS)

    Cassidy, Emily S.; West, Paul C.; Gerber, James S.; Foley, Jonathan A.

    2013-09-01

    Worldwide demand for crops is increasing rapidly due to global population growth, increased biofuel production, and changing dietary preferences. Meeting these growing demands will be a substantial challenge that will tax the capability of our food system and prompt calls to dramatically boost global crop production. However, to increase food availability, we may also consider how the world’s crops are allocated to different uses and whether it is possible to feed more people with current levels of crop production. Of particular interest are the uses of crops as animal feed and as biofuel feedstocks. Currently, 36% of the calories produced by the world’s crops are being used for animal feed, and only 12% of those feed calories ultimately contribute to the human diet (as meat and other animal products). Additionally, human-edible calories used for biofuel production increased fourfold between the years 2000 and 2010, from 1% to 4%, representing a net reduction of available food globally. In this study, we re-examine agricultural productivity, going from using the standard definition of yield (in tonnes per hectare, or similar units) to using the number of people actually fed per hectare of cropland. We find that, given the current mix of crop uses, growing food exclusively for direct human consumption could, in principle, increase available food calories by as much as 70%, which could feed an additional 4 billion people (more than the projected 2-3 billion people arriving through population growth). Even small shifts in our allocation of crops to animal feed and biofuels could significantly increase global food availability, and could be an instrumental tool in meeting the challenges of ensuring global food security.

  20. Northwest Africa 8159: An approximately 2.3 Billion Year Old Martian Olivine-Bearing Augite Basalt

    NASA Technical Reports Server (NTRS)

    Simon, J. I.; Peters, T. J.; Tappa, M. J.; Agee, C. B.

    2014-01-01

    Based on petrology, mineralogy, and bulk composition, the new NWA 8159 martian meteorite is distinct from all known samples from Mars. In particular, the augite compositional trends are unique, but most similar to those of nakhite intercumulus. Whether NWA 8159 represents a new lithology or is related to a known meteorite group remains to be determined. Sr and Nd isotopic analyses will allow comparison of source characteristics with SNC and other new ungrouped meteorites (e.g., NWA 7635). Here we report initial Rb-Sr and Sm-Nd isotopic results for NWA 8159 with the objective to determine its formation age and to potentially identify similarities and potential source affinities with other martian rocks.

  1. Economic toll of AIDS put at $10 billion in Canada.

    PubMed

    1996-11-29

    John McCallum, Chief economist at the Royal Bank of Canada, announced that AIDS has cost the nation's economy $10 billion since 1981. These calculations included losses in both direct medical care and human capital. This monetary figure is expected to rise to $36 billion by 2010. An estimated 42,500 to 45,000 Canadians are infected with HIV. PMID:11364044

  2. 41 CFR 51-2.3 - Notice of proposed addition or deletion.

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... Relating to Public Contracts COMMITTEE FOR PURCHASE FROM PEOPLE WHO ARE BLIND OR SEVERELY DISABLED 2-COMMITTEE FOR PURCHASE FROM PEOPLE WHO ARE BLIND OR SEVERELY DISABLED § 51-2.3 Notice of proposed...

  3. 41 CFR 51-2.3 - Notice of proposed addition or deletion.

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... Relating to Public Contracts COMMITTEE FOR PURCHASE FROM PEOPLE WHO ARE BLIND OR SEVERELY DISABLED 2-COMMITTEE FOR PURCHASE FROM PEOPLE WHO ARE BLIND OR SEVERELY DISABLED § 51-2.3 Notice of proposed...

  4. 41 CFR 51-2.3 - Notice of proposed addition or deletion.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... Relating to Public Contracts COMMITTEE FOR PURCHASE FROM PEOPLE WHO ARE BLIND OR SEVERELY DISABLED 2-COMMITTEE FOR PURCHASE FROM PEOPLE WHO ARE BLIND OR SEVERELY DISABLED § 51-2.3 Notice of proposed...

  5. 41 CFR 51-2.3 - Notice of proposed addition or deletion.

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... Relating to Public Contracts COMMITTEE FOR PURCHASE FROM PEOPLE WHO ARE BLIND OR SEVERELY DISABLED 2-COMMITTEE FOR PURCHASE FROM PEOPLE WHO ARE BLIND OR SEVERELY DISABLED § 51-2.3 Notice of proposed...

  6. 41 CFR 51-2.3 - Notice of proposed addition or deletion.

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... Relating to Public Contracts COMMITTEE FOR PURCHASE FROM PEOPLE WHO ARE BLIND OR SEVERELY DISABLED 2-COMMITTEE FOR PURCHASE FROM PEOPLE WHO ARE BLIND OR SEVERELY DISABLED § 51-2.3 Notice of proposed...

  7. Palaeoclimates: the first two billion years

    PubMed Central

    Kasting, James F; Ono, Shuhei

    2006-01-01

    Earth's climate during the Archaean remains highly uncertain, as the relevant geologic evidence is sparse and occasionally contradictory. Oxygen isotopes in cherts suggest that between 3.5 and 3.2 Gyr ago (Ga) the Archaean climate was hot (55–85 °C); however, the fact that these cherts have experienced only a modest amount of weathering suggests that the climate was temperate, as today. The presence of diamictites in the Pongola Supergroup and the Witwatersrand Basin of South Africa suggests that by 2.9 Ga the climate was glacial. The Late Archaean was relatively warm; then glaciation (possibly of global extent) reappeared in the Early Palaeoproterozoic, around 2.3–2.4 Ga. Fitting these climatic constraints with a model requires high concentrations of atmospheric CO2 or CH4, or both. Solar luminosity was 20–25% lower than today, so elevated greenhouse gas concentrations were needed just to keep the mean surface temperature above freezing. A rise in O2 at approximately 2.4 Ga, and a concomitant decrease in CH4, provides a natural explanation for the Palaeoproterozoic glaciations. The Mid-Archaean glaciations may have been caused by a drawdown in H2 and CH4 caused by the origin of bacterial sulphate reduction. More work is needed to test this latter hypothesis. PMID:16754607

  8. Palaeoclimates: the first two billion years.

    PubMed

    Kasting, James F; Ono, Shuhei

    2006-06-29

    Earth's climate during the Archaean remains highly uncertain, as the relevant geologic evidence is sparse and occasionally contradictory. Oxygen isotopes in cherts suggest that between 3.5 and 3.2 Gyr ago (Ga) the Archaean climate was hot (55-85 degrees C); however, the fact that these cherts have experienced only a modest amount of weathering suggests that the climate was temperate, as today. The presence of diamictites in the Pongola Supergroup and the Witwatersrand Basin of South Africa suggests that by 2.9 Ga the climate was glacial. The Late Archaean was relatively warm; then glaciation (possibly of global extent) reappeared in the Early Palaeoproterozoic, around 2.3-2.4 Ga. Fitting these climatic constraints with a model requires high concentrations of atmospheric CO2 or CH4, or both. Solar luminosity was 20-25% lower than today, so elevated greenhouse gas concentrations were needed just to keep the mean surface temperature above freezing. A rise in O2 at approximately 2.4 Ga, and a concomitant decrease in CH4, provides a natural explanation for the Palaeoproterozoic glaciations. The Mid-Archaean glaciations may have been caused by a drawdown in H2 and CH4 caused by the origin of bacterial sulphate reduction. More work is needed to test this latter hypothesis. PMID:16754607

  9. Gaia: how to map a billion stars with a billion pixels

    NASA Astrophysics Data System (ADS)

    de Bruijne, J. H. J.

    2008-07-01

    Gaia, ESA's ambitious star-mapper mission due for launch late-2011, will provide multi-epoch micro-arcsecond astrometric and milli-magnitude photometric data for the brightest one billion objects in the sky, down to at least magnitude 20. Spectroscopic data will simultaneously be collected for the subset of the brightest 100 million stars, down to about magnitude 17. This massive data volume will allow astronomers to reconstruct the structure, evolution and formation history of the Milky Way. It will also revolutionize studies of the solar system and stellar physics and will contribute to diverse research areas, ranging from extra-solar planets to general relativity. Underlying Gaia's scientific harvest will lie in a Catalogue, built on the fundamental space-based measurements. During the 5-year nominal operational lifetime, Gaia's payload, with its CCD mosaic containing 1 billion pixels, will autonomously detect all objects of interest and observe them throughout their passage of the focal plane. This paper discusses the workings of the Gaia instrument, details its payload, and discusses in depth how the scientific measurements will be collected. It addresses issues like maintenance of the scanning law, on-board data processing, the detection and confirmation of objects (single and multiple stars), the detection and rejection of cosmic rays and solar protons, the fundamental science measurements themselves composed of windows of CCD samples (pixels), and special strategies employed to maximize the science return for moving (i.e., solar-system) objects. The paper also explains how an on-board priority scheme will ensure catalogue completeness down to the faintest magnitudes possible, despite the limited ground-station availability and the enormous data volume that will be sent to the ground.

  10. 1,2,3-Trichloropropane

    Integrated Risk Information System (IRIS)

    1,2,3 - Trichloropropane ; CASRN 96 - 18 - 4 Human health assessment information on a chemical substance is included in IRIS only after a comprehensive review of toxicity data by U.S . EPA health scientists from several program offices , regional offices , and the Office of Research and Development

  11. NASA Now Minute: Earth and Space Science: 100 Billion Planets

    NASA Video Gallery

    Stephen Kane, co-author of the article, “Study Shows Our Galaxy has 100Billion Planets” reveals details about this incredible study explainsjust how common planets are in our Milky Way galaxy...

  12. Circadian biology: a 2.5 billion year old clock.

    PubMed

    Loudon, Andrew S I

    2012-07-24

    A recent study suggests that circadian clocks may have evolved at the time of the Great Oxidation Event 2.5 billion years ago in order to drive detoxification of reactive oxygen species. PMID:22835791

  13. Academic Pork Barrel Tops $2-Billion for the First Time.

    ERIC Educational Resources Information Center

    Brainard, Jeffrey; Borrego, Anne Marie

    2003-01-01

    Describes how, despite the growing budget deficit, Congress directed a record $2 billion to college projects in 2003, many of them dealing with security and bioterrorism. Includes data tables on the earmarks. (EV)

  14. Understanding "people" people.

    PubMed

    Butler, Timothy; Waldroop, James

    2004-06-01

    Nearly all areas of business--not just sales and human resources--call for interpersonal savvy. Relational know-how comprises a greater variety of aptitudes than many executives think. Some people can "talk a dog off a meat truck," as the saying goes. Others are great at resolving interpersonal conflicts. Some have a knack for translating high-level concepts for the masses. And others thrive when they're managing a team. Since people do their best work when it most closely matches their interests, the authors contend, managers can increase productivity by taking into account employees' relational interests and skills when making personnel choices and project assignments. After analyzing psychological tests of more than 7,000 business professionals, the authors have identified four dimensions of relational work: influence, interpersonal facilitation, relational creativity, and team leadership. This article explains each one and offers practical advice to managers--how to build a well-balanced team, for instance, and how to gauge the relational skills of potential employees during interviews. To determine whether a job candidate excels in, say, relational creativity, ask her to describe her favorite advertising campaign, slogan, or image and tell you why she finds it to be so effective. Understanding these four dimensions will help you get optimal performance from your employees, appropriately reward their work, and assist them in setting career goals. It will also help you make better choices when it comes to your own career development. To get started, try the authors' free online assessment tool, which will measure both your orientation toward relational work in general and your interest level in each of its four dimensions. PMID:15202289

  15. Feeding nine billion people sustainably: conserving land and water through shifting diets and changes in technologies.

    PubMed

    Springer, Nathaniel P; Duchin, Faye

    2014-04-15

    In the early 21st century the extensive clearing of forestland, fresh water scarcity, and sharp rises in the price of food have become causes for concern. These concerns may be substantially exacerbated over the next few decades by the need to provide improved diets for a growing global population. This study applies an inter-regional input-output model of the world economy, the World Trade Model, for analysis of alternative scenarios about satisfying future food requirements by midcentury. The scenario analysis indicates that relying only on more extensive use of arable land and fresh water would require clearing forests and exacerbating regional water scarcities. However, a combination of less resource-intensive diets and improved agricultural productivity, the latter especially in Africa, could make it possible to use these resources sustainably while also constraining increases in food prices. Unlike the scenario outcomes from other kinds of economic models, our framework reveals the potential for a decisive shift of production and export of agricultural products away from developed countries toward Africa and Latin America. Although the assumed changes in diets and technologies may not be realizable without incentives, our results suggest that these regions exhibit comparative advantages in agricultural production due to their large remaining resource endowments and their potential for higher yields. PMID:24635667

  16. Advancing Cancer Survivorship in a Country with 1.35 Billion People: The China Lymphoma Project

    PubMed Central

    Coughlin, Steven; Reno, Jamie

    2016-01-01

    Rates of lymphoma are rising rapidly and lymphoma is now the ninth most common cancer among Chinese males. The China Lymphoma Project was founded to increase awareness of lymphoma in China, including the survivability of the disease and the availability of potentially life-saving treatments, and to provide social support for men, women, and children in China who are living with the disease. The project is working with China government officials, several of the top cancer hospitals in China and the U.S., internationally known oncologists and cancer researchers, pharmaceutical and biotech companies in China and the U.S., healthcare and environmental companies, the Confucius Institute at San Diego State University, and the Asian Heritage Society. Advances in e-Health are being utilized to provide patient education and social support. The project will provide free e-books that profile lymphoma survivors (e.g., Kai-Fu Lee, creator of Google China), new videos, websites, pamphlets, blogs, video logs (vlogs), peer-to-peer counseling and support, and information about the latest treatments and oncology clinical trials.

  17. Winglets Save Billions of Dollars in Fuel Costs

    NASA Technical Reports Server (NTRS)

    2010-01-01

    The upturned ends now featured on many airplane wings are saving airlines billions of dollars in fuel costs. Called winglets, the drag-reducing technology was advanced through the research of Langley Research Center engineer Richard Whitcomb and through flight tests conducted at Dryden Flight Research Center. Seattle-based Aviation Partners Boeing -- a partnership between Aviation Partners Inc., of Seattle, and The Boeing Company, of Chicago -- manufactures Blended Winglets, a unique design featured on Boeing aircraft around the world. These winglets have saved more than 2 billion gallons of jet fuel to date, representing a cost savings of more than $4 billion and a reduction of almost 21.5 million tons in carbon dioxide emissions.

  18. Bill and Melinda Gates Pledge $1-Billion for Minority Scholarships.

    ERIC Educational Resources Information Center

    Monaghan, Peter; Lederman, Douglas; van der Werf, Martin; Pulley, John

    1999-01-01

    Reports on a $1 billion dollar grant from Bill and Melinda Gates to send 20,000 low-income minority students to college. The Gates Millenium Scholars Program will require students to demonstrate financial need and maintain a 3.0 grade point average in college. A list of the largest private gifts to higher education since 1967 is also provided. (DB)

  19. The BIA As Banker: "Trust" Is Hard When Billions Disappear.

    ERIC Educational Resources Information Center

    Johansen, Bruce E.

    1997-01-01

    The federal government's trust responsibility toward Native Americans involves protection of their lands, resources, and right to self-government and provision of services (including education). However, the Bureau of Indian Affairs has misplaced billions of dollars owed Native American individuals and tribes and now faces class-action litigation.…

  20. Congress Gives Colleges a Billion-Dollar Bonanza.

    ERIC Educational Resources Information Center

    Brainard, Jeffrey; Southwick, Ron

    2000-01-01

    Reports that Congress has earmarked a record amount of money (more than $1 billion) for projects involving specific colleges in the 2000 fiscal year. Notes that such "pork-barrel" spending has tripled since 1996. Charts show trends in earmarks since 1989, year 2000 earmarks by agency, the top 20 recipients of earmarked grants, and ranking of…

  1. Colleges' Billion-Dollar Campaigns Feel the Economy's Sting

    ERIC Educational Resources Information Center

    Masterson, Kathryn

    2009-01-01

    The economy's collapse has caught up with the billion-dollar campaign. In the past 12 months, the amount of money raised by a dozen of the colleges engaged in higher education's biggest fund-raising campaigns fell 32 percent from the year before. The decline, which started before the worst of the recession, has forced colleges to postpone…

  2. A massive galaxy in its core formation phase three billion years after the Big Bang.

    PubMed

    Nelson, Erica; van Dokkum, Pieter; Franx, Marijn; Brammer, Gabriel; Momcheva, Ivelina; Schreiber, Natascha Förster; da Cunha, Elisabete; Tacconi, Linda; Bezanson, Rachel; Kirkpatrick, Allison; Leja, Joel; Rix, Hans-Walter; Skelton, Rosalind; van der Wel, Arjen; Whitaker, Katherine; Wuyts, Stijn

    2014-09-18

    Most massive galaxies are thought to have formed their dense stellar cores in early cosmic epochs. Previous studies have found galaxies with high gas velocity dispersions or small apparent sizes, but so far no objects have been identified with both the stellar structure and the gas dynamics of a forming core. Here we report a candidate core in the process of formation 11 billion years ago, at redshift z = 2.3. This galaxy, GOODS-N-774, has a stellar mass of 100 billion solar masses, a half-light radius of 1.0 kiloparsecs and a star formation rate of solar masses per year. The star-forming gas has a velocity dispersion of 317 ± 30 kilometres per second. This is similar to the stellar velocity dispersions of the putative descendants of GOODS-N-774, which are compact quiescent galaxies at z ≈ 2 (refs 8-11) and giant elliptical galaxies in the nearby Universe. Galaxies such as GOODS-N-774 seem to be rare; however, from the star formation rate and size of this galaxy we infer that many star-forming cores may be heavily obscured, and could be missed in optical and near-infrared surveys. PMID:25162527

  3. The Value Of The Nonprofit Hospital Tax Exemption Was $24.6 Billion In 2011.

    PubMed

    Rosenbaum, Sara; Kindig, David A; Bao, Jie; Byrnes, Maureen K; O'Laughlin, Colin

    2015-07-01

    The federal government encourages public support for charitable activities by allowing people to deduct donations to tax-exempt organizations on their income tax returns. Tax-exempt hospitals are major beneficiaries of this policy because it encourages donations to the hospitals while shielding them from federal and state tax liability. In exchange, these hospitals must engage in community benefit activities, such as providing care to indigent patients and participating in Medicaid. The congressional Joint Committee on Taxation estimated the value of the nonprofit hospital tax exemption at $12.6 billion in 2002--a number that included forgone taxes, public contributions, and the value of tax-exempt bond financing. In this article we estimate that the size of the exemption reached $24.6 billion in 2011. The Affordable Care Act (ACA) brings a new focus on community benefit activities by requiring tax-exempt hospitals to engage in communitywide planning efforts to improve community health. The magnitude of the tax exemption, coupled with ACA reforms, underscores the public's interest not only in community benefit spending generally but also in the extent to which nonprofit hospitals allocate funds for community benefit expenditures that improve the overall health of their communities. PMID:26085486

  4. Conservation of protein structure over four billion years

    PubMed Central

    Ingles-Prieto, Alvaro; Ibarra-Molero, Beatriz; Delgado-Delgado, Asuncion; Perez-Jimenez, Raul; Fernandez, Julio M.; Gaucher, Eric A.; Sanchez-Ruiz, Jose M.; Gavira, Jose A.

    2013-01-01

    SUMMARY Little is known with certainty about the evolution of protein structures in general and the degree of protein structure conservation over planetary time scales in particular. Here we report the X-ray crystal structures of seven laboratory resurrections of Precambrian thioredoxins dating back up to ~4 billion years before present. Despite considerable sequence differences compared with extant enzymes, the ancestral proteins display the canonical thioredoxin fold while only small structural changes have occurred over 4 billion years. This remarkable degree of structure conservation since a time near the last common ancestor of life supports a punctuated-equilibrium model of structure evolution in which the generation of new folds occurs over comparatively short periods of time and is followed by long periods of structural stasis. PMID:23932589

  5. BLINK: Billion Lines INdexing in a clicK

    NASA Astrophysics Data System (ADS)

    Kamennoff, N.; Foucaud, S.; Reybier, S.; Tsai, M.-F.; Tang, C.-H.

    2012-09-01

    The coming generation of sky surveys are going to provide measurements for properties of a number of objects like never have been reached before. Astronomical databases will have to deal with requests on several billions of entries at once, and therefore a new computational framework is vital for the next generation of Data-Centers. As part of the efforts linked to the setting up of the Taiwan Extragalactic Astronomical Data Center (TWEA-DC), Billion Lines INdexing in a clicK (BLINK) is developed to satisfy this role. BLINK is a framework that aims to ease access to large amount of data and share analysis software amongst users. BLINK is also designed to be parallelized and distributed on large amount of heterogeneous resources. BLINK will propose at first a very fast indexing algorithm and cross-matching capability, enabling to gather multiwavelength information of large chunk of the sky in a very limited period of time.

  6. Conservation of protein structure over four billion years.

    PubMed

    Ingles-Prieto, Alvaro; Ibarra-Molero, Beatriz; Delgado-Delgado, Asuncion; Perez-Jimenez, Raul; Fernandez, Julio M; Gaucher, Eric A; Sanchez-Ruiz, Jose M; Gavira, Jose A

    2013-09-01

    Little is known about the evolution of protein structures and the degree of protein structure conservation over planetary time scales. Here, we report the X-ray crystal structures of seven laboratory resurrections of Precambrian thioredoxins dating up to approximately four billion years ago. Despite considerable sequence differences compared with extant enzymes, the ancestral proteins display the canonical thioredoxin fold, whereas only small structural changes have occurred over four billion years. This remarkable degree of structure conservation since a time near the last common ancestor of life supports a punctuated-equilibrium model of structure evolution in which the generation of new folds occurs over comparatively short periods and is followed by long periods of structural stasis. PMID:23932589

  7. Ubiquitous Supercritical Wing Design Cuts Billions in Fuel Costs

    NASA Technical Reports Server (NTRS)

    2015-01-01

    A Langley Research Center engineer’s work in the 1960s and ’70s to develop a wing with better performance near the speed of sound resulted in a significant increase in subsonic efficiency. The design was shared with industry. Today, Renton, Washington-based Boeing Commercial Airplanes, as well as most other plane manufacturers, apply it to all their aircraft, saving the airline industry billions of dollars in fuel every year.

  8. 11 CFR 2.3 - General rules.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... this part. (b) Except as provided in 11 CFR 2.4, every portion of every Commission meeting shall be... 11 Federal Elections 1 2011-01-01 2011-01-01 false General rules. 2.3 Section 2.3 Federal Elections FEDERAL ELECTION COMMISSION SUNSHINE REGULATIONS; MEETINGS § 2.3 General rules. (a)...

  9. 36 CFR 2.3 - Fishing.

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... 36 Parks, Forests, and Public Property 1 2013-07-01 2013-07-01 false Fishing. 2.3 Section 2.3 Parks, Forests, and Public Property NATIONAL PARK SERVICE, DEPARTMENT OF THE INTERIOR RESOURCE PROTECTION, PUBLIC USE AND RECREATION § 2.3 Fishing. (a) Except in designated areas or as provided in this section, fishing shall be in accordance with...

  10. 36 CFR 2.3 - Fishing.

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... 36 Parks, Forests, and Public Property 1 2012-07-01 2012-07-01 false Fishing. 2.3 Section 2.3 Parks, Forests, and Public Property NATIONAL PARK SERVICE, DEPARTMENT OF THE INTERIOR RESOURCE PROTECTION, PUBLIC USE AND RECREATION § 2.3 Fishing. (a) Except in designated areas or as provided in this section, fishing shall be in accordance with...

  11. 36 CFR 2.3 - Fishing.

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... 36 Parks, Forests, and Public Property 1 2011-07-01 2011-07-01 false Fishing. 2.3 Section 2.3 Parks, Forests, and Public Property NATIONAL PARK SERVICE, DEPARTMENT OF THE INTERIOR RESOURCE PROTECTION, PUBLIC USE AND RECREATION § 2.3 Fishing. (a) Except in designated areas or as provided in this section, fishing shall be in accordance with...

  12. 36 CFR 2.3 - Fishing.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... 36 Parks, Forests, and Public Property 1 2010-07-01 2010-07-01 false Fishing. 2.3 Section 2.3 Parks, Forests, and Public Property NATIONAL PARK SERVICE, DEPARTMENT OF THE INTERIOR RESOURCE PROTECTION, PUBLIC USE AND RECREATION § 2.3 Fishing. (a) Except in designated areas or as provided in this section, fishing shall be in accordance with...

  13. 36 CFR 2.3 - Fishing.

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... 36 Parks, Forests, and Public Property 1 2014-07-01 2014-07-01 false Fishing. 2.3 Section 2.3 Parks, Forests, and Public Property NATIONAL PARK SERVICE, DEPARTMENT OF THE INTERIOR RESOURCE PROTECTION, PUBLIC USE AND RECREATION § 2.3 Fishing. (a) Except in designated areas or as provided in this section, fishing shall be in accordance with...

  14. 43 CFR 5511.2-3 - Permits.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ... 43 Public Lands: Interior 2 2013-10-01 2013-10-01 false Permits. 5511.2-3 Section 5511.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND MANAGEMENT, DEPARTMENT OF THE INTERIOR FOREST MANAGEMENT (5000) FREE USE OF TIMBER Free Use Regulations § 5511.2-3 Permits. (a) Application for permit. Before timber...

  15. 45 CFR 1206.2-3 - Definitions.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ... 45 Public Welfare 4 2013-10-01 2013-10-01 false Definitions. 1206.2-3 Section 1206.2-3 Public Welfare Regulations Relating to Public Welfare (Continued) CORPORATION FOR NATIONAL AND COMMUNITY SERVICE GRANTS AND CONTRACTS-SUSPENSION AND TERMINATION AND DENIAL OF APPLICATION FOR REFUNDING Denial of Application for Refunding § 1206.2-3...

  16. Billion particle linac simulations for future light sources

    SciTech Connect

    Ryne, R. D.; Venturini, M.; Zholents, A. A.; Qiang, J.

    2008-09-25

    In this paper we report on multi-physics, multi-billion macroparticle simulation of beam transport in a free electron laser (FEL) linac for future light source applications. The simulation includes a self-consistent calculation of 3D space-charge effects, short-range geometry wakefields, longitudinal coherent synchrotron radiation (CSR) wakefields, and detailed modeling of RF acceleration and focusing. We discuss the need for and the challenges associated with such large-scale simulation. Applications to the study of the microbunching instability in an FEL linac are also presented.

  17. Scalable in-memory RDFS closure on billions of triples.

    SciTech Connect

    Goodman, Eric L.; Mizell, David

    2010-06-01

    We present an RDFS closure algorithm, specifically designed and implemented on the Cray XMT supercomputer, that obtains inference rates of 13 million inferences per second on the largest system configuration we used. The Cray XMT, with its large global memory (4TB for our experiments), permits the construction of a conceptually straightforward algorithm, fundamentally a series of operations on a shared hash table. Each thread is given a partition of triple data to process, a dedicated copy of the ontology to apply to the data, and a reference to the hash table into which it inserts inferred triples. The global nature of the hash table allows the algorithm to avoid a common obstacle for distributed memory machines: the creation of duplicate triples. On LUBM data sets ranging between 1.3 billion and 5.3 billion triples, we obtain nearly linear speedup except for two portions: file I/O, which can be ameliorated with the additional service nodes, and data structure initialization, which requires nearly constant time for runs involving 32 processors or more.

  18. 43 CFR 3105.2-3 - Requirements.

    Code of Federal Regulations, 2012 CFR

    2012-10-01

    ... 43 Public Lands: Interior 2 2012-10-01 2012-10-01 false Requirements. 3105.2-3 Section 3105.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND MANAGEMENT, DEPARTMENT OF THE INTERIOR MINERALS MANAGEMENT (3000) OIL AND GAS LEASING Cooperative Conservation...

  19. 43 CFR 3105.2-3 - Requirements.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ... 43 Public Lands: Interior 2 2013-10-01 2013-10-01 false Requirements. 3105.2-3 Section 3105.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND MANAGEMENT, DEPARTMENT OF THE INTERIOR MINERALS MANAGEMENT (3000) OIL AND GAS LEASING Cooperative Conservation...

  20. 43 CFR 3105.2-3 - Requirements.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... 43 Public Lands: Interior 2 2011-10-01 2011-10-01 false Requirements. 3105.2-3 Section 3105.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND MANAGEMENT, DEPARTMENT OF THE INTERIOR MINERALS MANAGEMENT (3000) OIL AND GAS LEASING Cooperative Conservation...

  1. 43 CFR 3105.2-3 - Requirements.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ... 43 Public Lands: Interior 2 2014-10-01 2014-10-01 false Requirements. 3105.2-3 Section 3105.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND MANAGEMENT, DEPARTMENT OF THE INTERIOR MINERALS MANAGEMENT (3000) OIL AND GAS LEASING Cooperative Conservation...

  2. $17 billion needed for population programme to year 2000: Dr. Nafis Sadik launches State of World Population Report.

    PubMed

    1995-01-01

    Dr. Nafis Sadik, Executive Director of the United Nations Population Fund (UNFPA), in her address on July 11 to the Foreign Press Association in London on the occasion of the release of the "1995 State of the World Population Report," stated that governments needed to invest in people, and that the estimated amount needed to reduce population numbers in developing countries was $17 billion for the year 2000. Two-thirds of the cost would be supplied by the developing countries. She said that coordinating population policies globally through such documents as the Programme of Action from the Cairo Conference would aid in slowing population growth. World population, currently 5.7 billion, is projected to reach 7.1-7.83 billion in 2015 and 7.9-11.9 billion in 2050. She also noted that certain conditions faced by women bear upon unsustainable population growth. The cycle of poverty continues in developing countries because very young mothers, who face higher risks in pregnancy and childbirth than those who delay childbearing until after the age of 20, are less likely to continue their education, more likely to have lower-paying jobs, and have a higher rate of separation and divorce. The isolation of women from widespread political participation and the marginalization of women's concerns from mainstream topics has resulted in ineffective family planning programs, including prevention of illness or impairment related to pregnancy or childbirth. Women, in most societies, cannot fully participate in economic and public life, have limited access to positions of influence and power, have narrower occupational choices and lower earnings than men, and must struggle to reconcile activities outside the home with their traditional roles. Sustainable development can only be achieved when social development expands opportunities for individuals (men and women), and their families, empowering them in the attainment of their social, economic, political, and cultural aspirations. PMID

  3. $75 Billion in Formula Grants Failed to Drive Reform. Can $5 Billion in Competitive Grants Do the Job? Education Stimulus Watch. Special Report 2

    ERIC Educational Resources Information Center

    Smarick, Andy

    2009-01-01

    In early 2009, Congress passed and President Barack Obama signed into law the American Recovery and Reinvestment Act (ARRA), the federal government's nearly $800 billion stimulus legislation. According to key members of Congress and the Obama administration, the education portions of the law, totaling about $100 billion, were designed both to…

  4. Galaxy Evolution over the Last Eight Billion Years

    NASA Astrophysics Data System (ADS)

    Zhu, Guangtun; Blanton, M. R.; Hogg, D. W.; Eisenstein, D. J.; Coil, A. L.; Cool, R. J.; Moustakas, J.; Wong, K. C.

    2011-01-01

    We study galaxy evolution over the last eight billion years with large, deep galaxy surveys, PRIMUS, SDSS and DEEP2. Galaxies have changed dramatically over this period of time. The global star formation rate has declined by roughly an order-of-magnitude. Red galaxies have grown substantially in number and mass. Blue galaxies have faded and grown redder as their star formation rate dropped. I demonstrate these evolutionary features with new results from these surveys. I also introduce PRIMUS, the largest faint galaxy survey to date. We have measured 140,000 robust redshifts to the depths of i (AB) 23 up to z 1, covering 9.1 square degrees of the sky. I show that with the existing deep multi-wavelength imaging in PRIMUS fields we are able to study the evolution in greater detail and investigate proposed physical mechanisms responsible for the evolution.

  5. Bigger, Better Catalog Unveils Half a Billion Celestial Objects

    NASA Technical Reports Server (NTRS)

    2002-01-01

    These frames are samples from the photographic sky surveys, which have been digitized by a technical team at the Space Telescope Science Institute to support the Hubble Space Telescope operations. The team processed these images to create a new astronomical catalog, called the Guide Star Catalog II. This project was undertaken by the Space Telescope Science Institute as an upgrade to an earlier sky survey and catalog (DSS-I and GSC-I), initially done to provide guide stars for pointing the Hubble Space Telescope. By virtue of its sheer size, the DSS-II and GSC-II have many research applications for both professional and amateur astronomers. [Top] An example from the DSS-II shows the Rosette Nebula, (originally photographed by the Palomar Observatory) as digitized in the DSS-I (left) and DSS-II (right). The DSS-II includes views of the sky at both red and blue wavelengths, providing invaluable color information on about one billion deep-sky objects. [Bottom] This blow-up of the inset box in the raw DSS-I scan shows examples of the GSC-I and the improved GSC-II catalogs. Astronomers extracted the stars from the scanned plate of the Rosette and listed them in the catalogs. The new GSC-II catalog provides the colors, positions, and luminosities of nearly half a billion stars -- over 20 times as many as the original GSC-I. The GSC-II contains information on stars as dim as the 19th magnitude. Credit: NASA, the DSS-II and GSC-II Consortia (with images from the Palomar Observatory-STScI Digital Sky Survey of the northern sky, based on scans of the Second Palomar Sky Survey are copyright c 1993-1999 by the California Institute of Technology)

  6. HPF Implementation of NPB2.3

    NASA Technical Reports Server (NTRS)

    Frumkin, Michael; Jin, Hao-Qiang; Yan, Jerry; Saini, Subhash (Technical Monitor)

    1998-01-01

    We present the HPF implementation of BT, SP, LU, FT, and MG of NPB2.3-serial benchmark set, The implementation is based on HPF performance model of the benchmark specific operations with distributed arrays. We present profiling and performance data on SGI origin 2000 and compare the results with NPB2.3. We discuss advantages and limitations of HPF and pghpf compiler.

  7. Older People and HIV

    MedlinePlus

    ... Many older people believe that HIV only affects younger people Most older people get little training in ... diseases among older people, as they do for younger people. Physicians may not diagnose HIV infection in ...

  8. Orbital forcing of climate 1.4 billion years ago.

    PubMed

    Zhang, Shuichang; Wang, Xiaomei; Hammarlund, Emma U; Wang, Huajian; Costa, M Mafalda; Bjerrum, Christian J; Connelly, James N; Zhang, Baomin; Bian, Lizeng; Canfield, Donald E

    2015-03-24

    Fluctuating climate is a hallmark of Earth. As one transcends deep into Earth time, however, both the evidence for and the causes of climate change become difficult to establish. We report geochemical and sedimentological evidence for repeated, short-term climate fluctuations from the exceptionally well-preserved ∼1.4-billion-year-old Xiamaling Formation of the North China Craton. We observe two patterns of climate fluctuations: On long time scales, over what amounts to tens of millions of years, sediments of the Xiamaling Formation record changes in geochemistry consistent with long-term changes in the location of the Xiamaling relative to the position of the Intertropical Convergence Zone. On shorter time scales, and within a precisely calibrated stratigraphic framework, cyclicity in sediment geochemical dynamics is consistent with orbital control. In particular, sediment geochemical fluctuations reflect what appear to be orbitally forced changes in wind patterns and ocean circulation as they influenced rates of organic carbon flux, trace metal accumulation, and the source of detrital particles to the sediment. PMID:25775605

  9. Orbital forcing of climate 1.4 billion years ago

    PubMed Central

    Zhang, Shuichang; Wang, Xiaomei; Hammarlund, Emma U.; Wang, Huajian; Costa, M. Mafalda; Bjerrum, Christian J.; Connelly, James N.; Zhang, Baomin; Bian, Lizeng; Canfield, Donald E.

    2015-01-01

    Fluctuating climate is a hallmark of Earth. As one transcends deep into Earth time, however, both the evidence for and the causes of climate change become difficult to establish. We report geochemical and sedimentological evidence for repeated, short-term climate fluctuations from the exceptionally well-preserved ∼1.4-billion-year-old Xiamaling Formation of the North China Craton. We observe two patterns of climate fluctuations: On long time scales, over what amounts to tens of millions of years, sediments of the Xiamaling Formation record changes in geochemistry consistent with long-term changes in the location of the Xiamaling relative to the position of the Intertropical Convergence Zone. On shorter time scales, and within a precisely calibrated stratigraphic framework, cyclicity in sediment geochemical dynamics is consistent with orbital control. In particular, sediment geochemical fluctuations reflect what appear to be orbitally forced changes in wind patterns and ocean circulation as they influenced rates of organic carbon flux, trace metal accumulation, and the source of detrital particles to the sediment. PMID:25775605

  10. Semantic Sensor Observation Networks in a Billion-Sensor World

    NASA Astrophysics Data System (ADS)

    Bermudez, L. E.; Bogden, P.; Creager, G.; Graybeal, J.

    2008-12-01

    In 2010, there will be 10,000 telemetric devices for every human in the planet (prediction by Ernest and Young). Some of these devices will be collecting data from coastal phenomena. Some will be connected to adaptive sampling systems, which allow observing a phenomenon, forecasting its advance, and triggering of other numerical models, new missions or changes to the sampling frequency of other sensors. These highly sophisticated autonomous and adaptive sensors will help improve the understating of coastal phenomena; however, collaborative arrangements among communities need to happen to be able to interoperate in a world of billions of sensors. Arrangements will allow discovery and sharing of sensor descriptions and understanding and usage of observed data. OOSTethys is an open source collaborative project that helps implement ocean observing system components. Some of these components include sensor interfaces, catalogs of services, and semantic mediators. The OOSTethys team seeks to speed up collaborative arrangements by studying the best standards available, creating easy-to-adopt toolkits, and publishing guides that facilitate the implementation of these components. The interaction of some observing system components, and lessons learned about developing Semantic Sensor Networks using OGC Sensor Observation Services and ontologies, will be discussed.

  11. A Massive Galaxy in Its Core Formation Phase Three Billion Years After the Big Bang

    NASA Technical Reports Server (NTRS)

    Nelson, Erica; van Dokkum, Pieter; Franx, Marijn; Brammer, Gabriel; Momcheva, Ivelina; Schreiber, Natascha M. Forster; da Cunha, Elisabete; Tacconi, Linda; Bezanson, Rachel; Kirkpatrick, Allison; Leja, Joel; Rix, Hans-Walter; Skelton, Rosalind; van der Wel, Arjen; Whitaker, Katherine; Wuyts, Stijn

    2014-01-01

    Most massive galaxies are thought to have formed their dense stellar cores at early cosmic epochs. However, cores in their formation phase have not yet been observed. Previous studies have found galaxies with high gas velocity dispersions or small apparent sizes but so far no objects have been identified with both the stellar structure and the gas dynamics of a forming core. Here we present a candidate core in formation 11 billion years ago, at z = 2.3. GOODS-N-774 has a stellar mass of 1.0 × 10 (exp 11) solar mass, a half-light radius of 1.0 kpc, and a star formation rate of 90 (sup +45 / sub -20) solar mass/yr. The star forming gas has a velocity dispersion 317 plus or minus 30 km/s, amongst the highest ever measured. It is similar to the stellar velocity dispersions of the putative descendants of GOODS-N-774, compact quiescent galaxies at z is approximately equal to 2 (exp 8-11) and giant elliptical galaxies in the nearby Universe. Galaxies such as GOODS-N-774 appear to be rare; however, from the star formation rate and size of the galaxy we infer that many star forming cores may be heavily obscured, and could be missed in optical and near-infrared surveys.

  12. Large data analysis: automatic visual personal identification in a demography of 1.2 billion persons

    NASA Astrophysics Data System (ADS)

    Daugman, John

    2014-05-01

    The largest biometric deployment in history is now underway in India, where the Government is enrolling the iris patterns (among other data) of all 1.2 billion citizens. The purpose of the Unique Identification Authority of India (UIDAI) is to ensure fair access to welfare benefits and entitlements, to reduce fraud, and enhance social inclusion. Only a minority of Indian citizens have bank accounts; only 4 percent possess passports; and less than half of all aid money reaches its intended recipients. A person who lacks any means of establishing their identity is excluded from entitlements and does not officially exist; thus the slogan of UIDAI is: To give the poor an identity." This ambitious program enrolls a million people every day, across 36,000 stations run by 83 agencies, with a 3-year completion target for the entire national population. The halfway point was recently passed with more than 600 million persons now enrolled. In order to detect and prevent duplicate identities, every iris pattern that is enrolled is first compared against all others enrolled so far; thus the daily workflow now requires 600 trillion (or 600 million-million) iris cross-comparisons. Avoiding identity collisions (False Matches) requires high biometric entropy, and achieving the tremendous match speed requires phase bit coding. Both of these requirements are being delivered operationally by wavelet methods developed by the author for encoding and comparing iris patterns, which will be the focus of this Large Data Award" presentation.

  13. People vs. animals.

    PubMed

    Engram, S

    1992-07-12

    Animal rights activists demonstrated against physicians in Pittsburgh, Pennsylvania, who had transplanted a baboon liver into a man. They complained that baboons should not serve as spare parts for humans, but the complaint misfired when another man with liver disease challenged them. Nevertheless the rapidly growing population in the world is threatening animal species such as elephants. In Zimbabwe where a severe drought exists and which has been somewhat able to protect animals from poachers, the government now allows people to kill elephants and other animals for their meat. The great numbers of wildlife have placed considerable population pressure on Gonarezhou National Park. The government hopes the good will plan will reduce the number of illegal poachings in the future. This illustrates the need for population stability to protect the environment. Yet the 1992 UN environment conference in Rio de Janeiro, Brazil, did not address population growth as a threat to biodiversity and the environment. Indeed if population continues to grow at its present rate, the population in 2100 will stand at 19 billion and each year before that the Earth will lose more farmland and forests and witness more days of smog, polluted water, political instabilities, and environmental refugees. Viruses like HIV may afflict the population. Most of the population growth will be in developing countries where drought and economic and political instabilities are common. In 2100 with such a hugh population, a national park for wildlife will most likely only be a luxury. We can no longer be complacent and must take action now to prevent this disaster. It will soon be clear that a growing population does not produce more prosperity as many economists would like us to believe, and discussions about using animals for spare parts will be ludicrous. PMID:12286283

  14. 2,3,4,6-Tetrachlorophenol

    Integrated Risk Information System (IRIS)

    2,3,4,6 - Tetrachlorophenol ; CASRN 58 - 90 - 2 Human health assessment information on a chemical substance is included in the IRIS database only after a comprehensive review of toxicity data , as outlined in the IRIS assessment development process . Sections I ( Health Hazard Assessments for Noncar

  15. 2,3-Dihydrobiflavone from Ginkgo biloba.

    PubMed

    Krauze-Baranowska, M; Sowiński, P

    1999-06-01

    From the yellow leaves of Ginkgo biloba 2,3-dihydrosciadopitysin (5,5'',7''-trihydroxy-7,4',4'''-trimethoxy-3',8''-flavanone/flavone) was isolated as a mixture of two diastereomers. Its structure was elucidated employing 2D NMR techniques. PMID:17260276

  16. 1,2,3-triazolium ionic liquids

    SciTech Connect

    Luebke, David; Nulwala, Hunaid; Tang, Chau

    2014-12-09

    The present invention relates to compositions of matter that are ionic liquids, the compositions comprising substituted 1,2,3-triazolium cations combined with any anion. Compositions of the invention should be useful in the separation of gases and, perhaps, as catalysts for many reactions.

  17. 3.5 billion years of reshaped Moho, southern Africa

    NASA Astrophysics Data System (ADS)

    Stankiewicz, Jacek; de Wit, Maarten

    2013-12-01

    According to some previous studies, Archean continental crust is, on global average, apparently thinner than Proterozoic crust. Subsequently, the validity of this statement has been questioned. To provide an additional perspective on this issue, we present analyses of Moho signatures derived from recent seismic data along swaths 2000 km in length across southern Africa and its flanking ocean. The imaged crust has a near continuous age range between ca. 0.1 and 3.7 billion years, and the seismic data allow direct comparison of Moho depths between adjacent Archean, Proterozoic and Phanerozoic crust. We find no simple secular change in depth to Moho over this time period. In contrast, there is significant variation in depth to Moho beneath both Archean and Proterozoic crust; Archean crust of southern Africa displays as much crustal diversity in thickness as the adjacent Proterozoic crust. The Moho beneath all crustal provinces that we have analysed has been severely altered by tectono-metamorphic and igneous processes, in many cases more than once, and cannot provide unequivocal data for geodynamic models dealing with secular changes in continental crust formation. These results and conclusions are similar to those documented along ca. 2000 km swaths across the Canadian Shield recorded by Lithoprobe. Tying the age and character of the Precambrian crust of southern Africa to their depth diversities is clearly related to manifold processes of tectono-thermal ‘surgery’ subsequent to their origin, the details of which are still to be resolved, as they are in most Precambrian terranes. Reconstructing pristine Moho of the early Earth therefore remains a formidable challenge. In South Africa, better knowledge of ‘fossilised’ Archean crustal sections ‘turned-on-edge’, such as at the Vredefort impact crater (for the continental crust), and from the Barberton greenstone belt (for oceanic crust) is needed to characterize potential pristine Archean Moho transitions.

  18. A Multi-billion Parcel Atmospheric Trajectory Model

    NASA Astrophysics Data System (ADS)

    Cruz, C.; Clune, T. L.; Lait, L. R.; Ranawake, U.; Burns, R. W.

    2009-12-01

    We present a new parallel implementation of an atmospheric trajectory modelling framework which provides improved numerical accuracy, greater flexibility for specifying experiments, and sufficient raw performance to simultaneously simulate billions of parcel trajectories on suitable computing platforms. The application is parallelized using the Message Passing Interface (MPI) library and can scale efficiently on a wide variety of modern computing platforms. The ability to treat such large numbers of parcels is expected to enable a new generation of experiments to explore questions related to global stratosphere-troposphere exchange, age-of-air spectra, and transport of trace gases and aerosols. The modelling framework is written in C++ for easy integration with other computing technologies. It also provides a great deal of flexibility by allowing users to select from (or add to) alternative subclasses for vertical coordinates (pressure, potential temperature), integration schemes (Runge-Kutta, Euler), meteorological data sources (NCEP/NCAR Reanalsyis, MERRA), data interpolation methods (linear, log-linear, splines), and output (parcel histories, summary statistics, min/max quantities encountered). Significantly improved numerical accuracy, especially near the poles, is provided by expressing integration in terms of purely geometric constructs which avoid various complications associated with spherical coordinates near the poles. The entire package has been rigorously developed using Test-Driven Development (TDD) which both provides confidence in the implementation and should also assist other developers that wish to extend the framework. Several tests are performed to demonstrate the fourth-order Runge-Kutta integration scheme with our spherical geometric constructs. Tilted solid body rotation provides a baseline synthetic wind field for assessing model performance, and a time-varying case is used to examine the errors introduced by interpolating linearly in time

  19. Factors Affecting Work Force Development in the People's Republic of China.

    ERIC Educational Resources Information Center

    Sredl, Henry J.

    Work force development in the Peoples' Republic of China (PRC) is affected by sundry but interrelated factors. Included among these are the following: (1) the PRC's population of one billion people; (2) a recent history of political turmoil and violence, resulting in profound changes in national leadership and vacillation in national policy; (3)…

  20. Global carrying capacity: how many people?

    PubMed

    1992-07-01

    During 1980-85 energy consumption in developing countries increased by 22%, of which 50% was used to maintain current levels of use and 50% pertained to real economic growth. Commercial energy consumption during 1970-89 tripled in developing countries. Population growth alone is expected to increase world energy consumption from the current 13.5 terawatts (13.5 trillion watts) to 18 terawatts by 2025 at the same level of use. The increased level of consumption (4.5 terawatts) is the equivalent of total current commercial energy consumption. One terawatt is equal to energy use from 5 billion barrels of oil yearly, 1 billion tons of coal, or 1.6 billion tons of wood. Economic development will require even greater levels of energy use. Since the oil price increases of the 1970s, developed countries increased their energy consumption by about 33%, even while becoming more fuel efficient. During 1990-2025, if developing countries double their per capita energy use and developed countries reduce their use by 50%, world energy consumption will still be almost 21 terawatts. If consumption remains constant at current levels without any population increase, the oil supply will be exhausted in 40 years. Coal consumption will last hundreds of years but air pollution will worsen, and global warming will be accelerated. Developed countries, which are wealthier, are having difficulty switching to non-fossil fuels, and the prospects for developing countries pose even greater challenges. Slowing growth buys time for technological development. World population is expected to reach 8 billion by 2020. Stabilization of growth at 8 billion would occur only if world fertility averages 1.7 children per woman by 2025. One opinion is that the carrying capacity has been reached with the present population of 5.4 billion. Others say that with changes in consumption and technological developments the earth can sustain 8 billion people. The physical limits are 1) the finite capacity of natural

  1. Indoleamine 2,3-dioxygenase vaccination

    PubMed Central

    Andersen, Mads Hald; Svane, Inge Marie

    2015-01-01

    Indoleamine 2,3-dioxygenase (IDO) is an immunoregulatory enzyme. Remarkably, we discovered IDO-specific T cells that can influence adaptive immune reactions in patients with cancer. Further, a recent phase I clinical trial demonstrated long-lasting disease stabilization without toxicity in patients with non-small-cell lung cancer (NSCLC) who were vaccinated with an IDO-derived HLA-A2-restricted epitope. PMID:25949864

  2. Meeting the food, energy, and water demands of nine billion people: Will climate change add a new dimension?

    Technology Transfer Automated Retrieval System (TEKTRAN)

    Climate change will add a new stress to our ability to produce food and supply water and energy for the expanding population. There is an emerging gap between the current production trends in food commodities around the world and the projected needs to meet the demands for the world population. This...

  3. A SWIRE Picture is Worth Billions of Years

    NASA Technical Reports Server (NTRS)

    2005-01-01

    [figure removed for brevity, see original site] Figure 1: SWIRE View of Distant Galaxies [figure removed for brevity, see original site] [figure removed for brevity, see original site] [figure removed for brevity, see original site] Figure 2Figure 3 Figure 4

    These spectacular images, taken by the Spitzer Wide-area Infrared Extragalactic (SWIRE) Legacy project, encapsulate one of the primary objectives of the Spitzer mission: to connect the evolution of galaxies from the distant, or early, universe to the nearby, or present day, universe.

    The Tadpole galaxy (main image) is the result of a recent galactic interaction in the local universe. Although these galactic mergers are rare in the universe's recent history, astronomers believe that they were much more common in the early universe. Thus, SWIRE team members will use this detailed image of the Tadpole galaxy to help understand the nature of the 'faint red-orange specks' of the early universe.

    The larger picture (figure 2) depicts one-sixteenth of the SWIRE survey field called ELAIS-N1. In this image, the bright blue sources are hot stars in our own Milky Way, which range anywhere from 3 to 60 times the mass of our Sun. The fainter green spots are cooler stars and galaxies beyond the Milky Way whose light is dominated by older stellar populations. The red dots are dusty galaxies that are undergoing intense star formation. The faintest specks of red-orange are galaxies billions of light-years away in the distant universe.

    Figure 3 features an unusual ring-like galaxy called CGCG 275-022. The red spiral arms indicate that this galaxy is very dusty and perhaps undergoing intense star formation. The star-forming activity could have been initiated by a near head-on collision with another galaxy.

    The most distant galaxies that SWIRE is able to detect are revealed in a zoom of deep space (figure 4). The colors in this feature represent the same objects as those in the larger field image of ELAIS

  4. SO(2, 3) noncommutative gravity model

    NASA Astrophysics Data System (ADS)

    Dimitrijević, M.; Radovanović, V.

    2014-12-01

    In this paper the noncommutative gravity is treated as a gauge theory of the non-commutative SO(2, 3)★ group, while the noncommutativity is canonical. The Seiberg-Witten (SW) map is used to express noncommutative fields in terms of the corresponding commutative fields. The commutative limit of the model is the Einstein-Hilbert action plus the cosmological term and the topological Gauss-Bonnet term. We calculate the second order correction to this model and obtain terms that are zeroth, first, ... and fourth power of the curvature tensor. Finally, we discuss physical consequences of those correction terms in the limit of big cosmological constant.

  5. Identification of 2,3-dimethyl-2,3-diisobutyl succinonitrile in laser printer emissions.

    PubMed

    Barrero-Moreno, Josefa M; Tirendi, Salvatore; Reniero, Fabiano; Giordano, Giuseppe; Kotzias, Dimitrios

    2008-01-01

    2,3-Dimethyl-2,3-diisobutyl succinonitrile was identified as the main volatile organic compound (>90%) emitted from laser printers during the printing process. Experiments were carried out in a large environmental chamber of 30 m3, where the printers were placed and working simulating 'real office setting' conditions. Air samples were taken on Tenax TA adsorbent cartridges in the vicinity of the printers and further analyzed by thermal desorption gas chromatography/mass spectrometry (TDGC/MS). The structure of the compound has been determined and is presented in this study. Additional data obtained by nuclear magnetic resonance (NMR), Fourier transform infrared (FTIR) spectroscopy, and liquid chromatography/tandem mass spectrometry (LC/MS/MS) support the proposed structure, with no reported CAS number, as 2,3-dimethyl-2,3-diisobutyl succinonitrile. It is a byproduct of the thermal decomposition of 2,2'-azobis(2,4-dimethyl valeronitrile), a commercially available free radical polymerization initiator used in polymerization processes during the manufacture of the toners. By means of head-space GC/MS, 15 toners used in black & white and colour printers have been investigated. Six of them contained 2,3-dimethyl-2,3-diisobutyl succinonitrile, which has also been detected in the respective processed paper. PMID:18205250

  6. The Other Inconvenient Truth: Feeding 9 Billion While Sustaining the Earth System

    NASA Astrophysics Data System (ADS)

    Foley, J. A.

    2010-12-01

    As the international community focuses on climate change as the great challenge of our era, we have been largely ignoring another looming problem — the global crisis in agriculture, food security and the environment. Our use of land, particularly for agriculture, is absolutely essential to the success of the human race: we depend on agriculture to supply us with food, feed, fiber, and, increasingly, biofuels. Without a highly efficient, productive, and resilient agricultural system, our society would collapse almost overnight. But we are demanding more and more from our global agricultural systems, pushing them to their very limits. Continued population growth (adding more than 70 million people to the world every year), changing dietary preferences (including more meat and dairy consumption), rising energy prices, and increasing needs for bioenergy sources are putting tremendous pressure on the world’s resources. And, if we want any hope of keeping up with these demands, we’ll need to double the agricultural production of the planet in the next 30 to 40 years. Meeting these huge new agricultural demands will be one of the greatest challenges of the 21st century. At present, it is completely unclear how (and if) we can do it. If this wasn’t enough, we must also address the massive environmental impacts of our current agricultural practices, which new evidence indicates rival the impacts of climate change. Simply put, providing for the basic needs of 9 billion-plus people, without ruining the biosphere in the process, will be one of the greatest challenges our species has ever faced. In this presentation, I will present a new framework for evaluating and assessing global patterns of agriculture, food / fiber / fuel production, and their relationship to the earth system, particularly in terms of changing stocks and flows of water, nutrients and carbon in our planetary environment. This framework aims to help us manage the challenges of increasing global food

  7. Rules Set for $4 Billion Race to Top Contest: Final Rules Give States Detailed Map in Quest for $4 Billion in Education Stimulus Aid

    ERIC Educational Resources Information Center

    McNeil, Michele

    2009-01-01

    For a good shot at $4 billion in grants from the federal Race to the Top Fund, states will need to make a persuasive case for their education reform agendas, demonstrate significant buy-in from local school districts, and devise plans to evaluate teachers and principals based on student performance, according to final regulations released last…

  8. Corporations Give Record $1.6 Billion to Colleges and Universities in 1984-85; Total Giving Reaches $6.3 Billion.

    ERIC Educational Resources Information Center

    CFAE Newsletter, 1986

    1986-01-01

    Findings from the publication, "Voluntary Support of Education 1984-85," are summarized. The survey report includes contributions to 1,114 colleges and universities. Highlights of findings show that: total estimated voluntary support was $6.32 billion in 1984-1985; for the first time, corporations contributed more than any other donor group ($1.57…

  9. If 1 in 10 U.S. Smokers Quits, $63 Billion Saved

    MedlinePlus

    ... nih.gov/medlineplus/news/fullstory_158758.html If 1 in 10 U.S. Smokers Quits, $63 Billion Saved ... money. That's because health care costs plummet just one year after stopping, new research shows. A 10 ...

  10. Three Principles to REVISE People's Unethical Behavior.

    PubMed

    Ayal, Shahar; Gino, Francesca; Barkan, Rachel; Ariely, Dan

    2015-11-01

    Dishonesty and unethical behavior are widespread in the public and private sectors and cause immense annual losses. For instance, estimates of U.S. annual losses indicate $1 trillion paid in bribes, $270 billion lost due to unreported income, and $42 billion lost in retail due to shoplifting and employee theft. In this article, we draw on insights from the growing fields of moral psychology and behavioral ethics to present a three-principle framework we call REVISE. This framework classifies forces that affect dishonesty into three main categories and then redirects those forces to encourage moral behavior. The first principle, reminding, emphasizes the effectiveness of subtle cues that increase the salience of morality and decrease people's ability to justify dishonesty. The second principle, visibility, aims to restrict anonymity, prompt peer monitoring, and elicit responsible norms. The third principle, self-engagement, increases people's motivation to maintain a positive self-perception as a moral person and helps bridge the gap between moral values and actual behavior. The REVISE framework can guide the design of policy interventions to defeat dishonesty. PMID:26581728

  11. 1,2,3-Triazoles as inhibitors of indoleamine 2,3-dioxygenase 2 (IDO2).

    PubMed

    Röhrig, Ute F; Majjigapu, Somi Reddy; Caldelari, Daniela; Dilek, Nahzli; Reichenbach, Patrick; Ascencao, Kelly; Irving, Melita; Coukos, George; Vogel, Pierre; Zoete, Vincent; Michielin, Olivier

    2016-09-01

    Indoleamine 2,3-dioxygenase 2 (IDO2) is a potential therapeutic target for the treatment of diseases that involve immune escape such as cancer. In contrast to IDO1, only a very limited number of inhibitors have been described for IDO2 due to inherent difficulties in expressing and purifying a functionally active, soluble form of the enzyme. Starting from our previously discovered highly efficient 4-aryl-1,2,3-triazole IDO1 inhibitor scaffold, we used computational structure-based methods to design inhibitors of IDO2 which we then tested in cellular assays. Our approach yielded low molecular weight inhibitors of IDO2, the most active displaying an IC50 value of 51μM for mIDO2, and twofold selectivity over hIDO1. These compounds could be useful as molecular probes to investigate the biological role of IDO2, and could inspire the design of new IDO2 inhibitors. PMID:27469130

  12. Evidence for Oxygenic Photosynthesis Half a Billion Years Before the Great Oxidation Event

    NASA Astrophysics Data System (ADS)

    Planavsky, Noah; Reinhard, Chris; Asael, Dan; Lyons, Tim; Hofmann, Axel; Rouxel, Olivier

    2014-05-01

    Despite detailed investigations over the past 50 years, there is still intense debate about when oxygenic photosynthesis evolved. Current estimates span over a billion years of Earth history, ranging from prior to 3.7 Ga, the age of the oldest sedimentary rocks, to 2.4-2.3 Ga, coincident with the rise of atmospheric oxygen ("The Great Oxidation Event" or GOE). As such, a new, independent perspective is needed. We will provide such a perspective herein by using molybdenum (Mo) isotopes in a novel way to track the onset of manganese(II)oxidation and thus biological oxygen production. The oxidation of Mn(II) in modern marine setting requires free dissolved oxygen. Mn is relatively unique in its environmental specificity for oxygen as an electron acceptor among the redox-sensitive transition metals, many of which, like Fe, can be oxidized under anoxic conditions either through a microbial pathway and/or with alternative oxidants such as nitrate. There are large Mo isotope fractionations associated with the sorption of Mo (as a polymolybdate complex) onto Mn-oxyhydroxides, with an approximately -2.7‰ fractionation in d98Mo associated with Mo sorption onto Mn-oxyhydroxides (e.g., birnessite, vernadite). In contrast, sorption of Mo onto the Fe-oxyhydroxide (e.g., ferrihydrite) results in a fractionation of only -1.1‰ or less. Because of this difference in Mo isotope fractionation, Mo isotope values should become lighter with increasing Mn content, if Mn oxidation occurred during deposition and is an important vector of Mo transfer to the sediment. We find a strong positive correlation between d98Mo values and Fe/Mn ratios in iron formations deposited before and after the Great Oxidation Event. Most strikingly, Mo isotope data and Fe/Mn ratios correlate over a 2.5‰ range in d98Mo values in the Mn-rich (0.1 - 6%) iron formation of the 2.95 Ga Sinqeni Formation, South Africa. The large isotopic shifts occur over a relatively thin (3 meter thick) horizon, reflecting

  13. Crystalline 1H-1,2,3-triazol-5-ylidenes

    DOEpatents

    Bertrand, Guy; Gulsado-Barrios, Gregorio; Bouffard, Jean; Donnadieu, Bruno

    2016-08-02

    The present invention provides novel and stable crystalline 1H-1,2,3 triazolium carbenes and metal complexes of 1H-1,2,3 triazolium carbenes. The present invention also provides methods of making 1H-1,2,3 triazolium carbenes and metal complexes of 1H-1,2,3 triazolium carbenes. The present invention also provides methods of using 1H-1,2,3 triazolium carbenes and metal complexes of 1H-1,2,3 triazolium carbenes in catalytic reactions.

  14. Why make people patients?

    PubMed Central

    Marinker, Marshall

    1975-01-01

    People confront their doctors with three modes of unhealth - disease, illness and sickness. Each is discussed, and the question is asked and answered as to why in this situation people wish to become patients. PMID:1177270

  15. 3.4-Billion-year-old biogenic pyrites from Barberton, South Africa: sulfur isotope evidence

    NASA Technical Reports Server (NTRS)

    Ohmoto, H.; Kakegawa, T.; Lowe, D. R.

    1993-01-01

    Laser ablation mass spectroscopy analyses of sulfur isotopic compositions of microscopic-sized grains of pyrite that formed about 3.4 billion years ago in the Barberton Greenstone Belt, South Africa, show that the pyrite formed by bacterial reduction of seawater sulfate. These data imply that by about 3.4 billion years ago sulfate-reducing bacteria had become active, the oceans were rich in sulfate, and the atmosphere contained appreciable amounts (>>10(-13) of the present atmospheric level) of free oxygen.

  16. 3.4-Billion-year-old biogenic pyrites from Barberton, South Africa: sulfur isotope evidence.

    PubMed

    Ohmoto, H; Kakegawa, T; Lowe, D R

    1993-10-22

    Laser ablation mass spectroscopy analyses of sulfur isotopic compositions of microscopic-sized grains of pyrite that formed about 3.4 billion years ago in the Barberton Greenstone Belt, South Africa, show that the pyrite formed by bacterial reduction of seawater sulfate. These data imply that by about 3.4 billion years ago sulfate-reducing bacteria had become active, the oceans were rich in sulfate, and the atmosphere contained appreciable amounts (>10(-13) of the present atmospheric level) of free oxygen. PMID:11539502

  17. NOAA Budget Increases to $4.1 Billion, But Some Key Items Are Reduced

    NASA Astrophysics Data System (ADS)

    Showstack, Randy

    2008-02-01

    The Bush administration has proposed a US$4.1 billion budget for fiscal year (FY) 2009 for the U.S. National Oceanic and Atmospheric Administration (NOAA). The proposed budget, which would be the agency's largest ever, is $202.6 million, or 5.2%, above the FY 2008 enacted budget. By topping $4 billion and the amount Congress passed for FY 2008, the budget proposal crosses into ``a new threshold,'' according Navy Vice Admiral Conrad Lautenbacher, undersecretary of commerce for oceans and atmosphere and NOAA administrator.

  18. Billions for biodefense: federal agency biodefense funding, FY2001-FY2005.

    PubMed

    Schuler, Ari

    2004-01-01

    Over the past several years, the United States government has spent substantial resources on preparing the nation against a bioterrorist attack. This article analyzes the civilian biodefense funding by the federal government from fiscal years 2001 through 2005, specifically analyzing the budgets and allocations for biodefense at the Department of Health and Human Services, the Department of Homeland Security, the Department of Defense, the Department of Agriculture, the Environmental Protection Agency, the National Science Foundation, and the Department of State. In total, approximately $14.5 billion has been funded for civilian biodefense through FY2004, with an additional $7.6 billion in the President's budget request for FY2005. PMID:15225402

  19. 3. 4-billion-year-old biogenic pyrites from Barberton, South Africa: Sulfur isotope evidence

    SciTech Connect

    Ohmoto, H.; Kakegawa, T. ); Lowe, D.R. )

    1993-10-22

    Laser ablation mass spectroscopy analysis of sulfur isotopic compositions of microscopic-sized grains of pyrite that formed about 3.4 billion years ago in the Barberton Greenstone Belt, South Africa, show that the pyrite formed by bacterial reduction of seawater sulfate. These data imply that by about 3.4 billion years ago sulfate-reducing bacteria had become active, the oceans were rich in sulfate, and the atmosphere contained appreciable amounts (> > 10[sup [minus]13] of the present atmospheric level) of free oxygen.

  20. The 100 People Project

    ERIC Educational Resources Information Center

    McLeod, Keri

    2007-01-01

    This article describes the 100 People Project and how the author integrates the project in her class. The 100 People Project is a nonprofit organization based in New York City. The organization poses the question: If there were only 100 people in the world, what would the world look like? Through the project, students were taught about ethics in…

  1. Counseling with Deaf People.

    ERIC Educational Resources Information Center

    Sussman, Allen E., Ed.; Stewart, Larry G., Ed.

    The book presents information on effective counseling with deaf people by discussing issues that confront counselors and administrators involved in providing counseling services to deaf people. A basic assumption of the book is that deaf people of all ages have been frequently denied counseling services due to communication problems between…

  2. The Sexual and Reproductive Health of Young People in Low and Middle Income Countries

    ERIC Educational Resources Information Center

    Edwards, Orain; Peterson, Nicholas

    2013-01-01

    Young people ages 10-24 account for 25 percent of the world's population: a total of 1.8 billion, most of whom are living in low- and middle-income countries. They face significant challenges, including HIV, sexually transmitted infections (STIs), adolescent pregnancy, unsafe abortion, and gender-based violence. Youth have the right to lead…

  3. Fragmentation pathways of 2,3-dimethyl-2,3-dinitrobutane cations in the gas phase.

    PubMed

    Paine, Martin R L; Kirk, Benjamin B; Ellis-Steinborner, Simon; Blanksby, Stephen J

    2009-09-01

    2,3-Dimethyl-2,3-dinitrobutane (DMNB) is an explosive taggant added to plastic explosives during manufacture making them more susceptible to vapour-phase detection systems. In this study, the formation and detection of gas-phase [M+H](+), [M+Li](+), [M+NH(4)](+) and [M+Na](+) adducts of DMNB was achieved using electrospray ionisation on a triple quadrupole mass spectrometer. The [M+H](+) ion abundance was found to have a strong dependence on ion source temperature, decreasing markedly at source temperatures above 50 degrees C. In contrast, the [M+Na](+) ion demonstrated increasing ion abundance at source temperatures up to 105 degrees C. The relative susceptibility of DMNB adduct ions toward dissociation was investigated by collision-induced dissociation. Probable structures of product ions and mechanisms for unimolecular dissociation have been inferred based on fragmentation patterns from tandem mass (MS/MS) spectra of source-formed ions of normal and isotopically labelled DMNB, and quantum chemical calculations. Both thermal and collisional activation studies suggest that the [M+Na](+) adduct ions are significantly more stable toward dissociation than their protonated analogues and, as a consequence, the former provide attractive targets for detection by contemporary rapid screening methods such as desorption electrospray ionisation mass spectrometry. PMID:19670345

  4. 4 CFR 2.3 - GAO Personnel Appeals Board.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 4 Accounts 1 2011-01-01 2011-01-01 false GAO Personnel Appeals Board. 2.3 Section 2.3 Accounts GOVERNMENT ACCOUNTABILITY OFFICE PERSONNEL SYSTEM PURPOSE AND GENERAL PROVISION § 2.3 GAO Personnel Appeals Board. The Government Accountability Office Personnel Appeals Board is established by 31 U.S.C....

  5. 4 CFR 2.3 - GAO Personnel Appeals Board.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... 4 Accounts 1 2010-01-01 2010-01-01 false GAO Personnel Appeals Board. 2.3 Section 2.3 Accounts GOVERNMENT ACCOUNTABILITY OFFICE PERSONNEL SYSTEM PURPOSE AND GENERAL PROVISION § 2.3 GAO Personnel Appeals Board. The Government Accountability Office Personnel Appeals Board is established by 31 U.S.C....

  6. 43 CFR 3107.2-3 - Leases capable of production.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ... 43 Public Lands: Interior 2 2013-10-01 2013-10-01 false Leases capable of production. 3107.2-3 Section 3107.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND MANAGEMENT, DEPARTMENT OF THE INTERIOR MINERALS MANAGEMENT (3000) OIL AND GAS LEASING Continuation, Extension or Renewal § 3107.2-3 Leases capable...

  7. 43 CFR 2920.2-3 - Other land use proposals.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... 43 Public Lands: Interior 2 2011-10-01 2011-10-01 false Other land use proposals. 2920.2-3 Section 2920.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND..., Permits and Easements: General Provisions § 2920.2-3 Other land use proposals. (a) A proposal for a...

  8. 43 CFR 2920.2-3 - Other land use proposals.

    Code of Federal Regulations, 2012 CFR

    2012-10-01

    ... 43 Public Lands: Interior 2 2012-10-01 2012-10-01 false Other land use proposals. 2920.2-3 Section 2920.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND..., Permits and Easements: General Provisions § 2920.2-3 Other land use proposals. (a) A proposal for a...

  9. 43 CFR 2920.2-3 - Other land use proposals.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ... 43 Public Lands: Interior 2 2013-10-01 2013-10-01 false Other land use proposals. 2920.2-3 Section 2920.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND..., Permits and Easements: General Provisions § 2920.2-3 Other land use proposals. (a) A proposal for a...

  10. 43 CFR 2920.2-3 - Other land use proposals.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ... 43 Public Lands: Interior 2 2014-10-01 2014-10-01 false Other land use proposals. 2920.2-3 Section 2920.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND..., Permits and Easements: General Provisions § 2920.2-3 Other land use proposals. (a) A proposal for a...

  11. 22 CFR 2.3 - Notification of foreign officials.

    Code of Federal Regulations, 2010 CFR

    2010-04-01

    ... 22 Foreign Relations 1 2010-04-01 2010-04-01 false Notification of foreign officials. 2.3 Section 2.3 Foreign Relations DEPARTMENT OF STATE GENERAL PROTECTION OF FOREIGN DIGNITARIES AND OTHER OFFICIAL PERSONNEL § 2.3 Notification of foreign officials. (a) Any notification of a foreign official...

  12. 10 CFR 960.5-2-3 - Meteorology.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 10 Energy 4 2011-01-01 2011-01-01 false Meteorology. 960.5-2-3 Section 960.5-2-3 Energy DEPARTMENT OF ENERGY GENERAL GUIDELINES FOR THE PRELIMINARY SCREENING OF POTENTIAL SITES FOR A NUCLEAR WASTE REPOSITORY Preclosure Guidelines Preclosure Radiological Safety § 960.5-2-3 Meteorology. (a)...

  13. 10 CFR 960.5-2-3 - Meteorology.

    Code of Federal Regulations, 2012 CFR

    2012-01-01

    ... 10 Energy 4 2012-01-01 2012-01-01 false Meteorology. 960.5-2-3 Section 960.5-2-3 Energy DEPARTMENT OF ENERGY GENERAL GUIDELINES FOR THE PRELIMINARY SCREENING OF POTENTIAL SITES FOR A NUCLEAR WASTE REPOSITORY Preclosure Guidelines Preclosure Radiological Safety § 960.5-2-3 Meteorology. (a)...

  14. 10 CFR 960.5-2-3 - Meteorology.

    Code of Federal Regulations, 2014 CFR

    2014-01-01

    ... 10 Energy 4 2014-01-01 2014-01-01 false Meteorology. 960.5-2-3 Section 960.5-2-3 Energy DEPARTMENT OF ENERGY GENERAL GUIDELINES FOR THE PRELIMINARY SCREENING OF POTENTIAL SITES FOR A NUCLEAR WASTE REPOSITORY Preclosure Guidelines Preclosure Radiological Safety § 960.5-2-3 Meteorology. (a)...

  15. 10 CFR 960.5-2-3 - Meteorology.

    Code of Federal Regulations, 2013 CFR

    2013-01-01

    ... 10 Energy 4 2013-01-01 2013-01-01 false Meteorology. 960.5-2-3 Section 960.5-2-3 Energy DEPARTMENT OF ENERGY GENERAL GUIDELINES FOR THE PRELIMINARY SCREENING OF POTENTIAL SITES FOR A NUCLEAR WASTE REPOSITORY Preclosure Guidelines Preclosure Radiological Safety § 960.5-2-3 Meteorology. (a)...

  16. 10 CFR 960.5-2-3 - Meteorology.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... 10 Energy 4 2010-01-01 2010-01-01 false Meteorology. 960.5-2-3 Section 960.5-2-3 Energy DEPARTMENT OF ENERGY GENERAL GUIDELINES FOR THE PRELIMINARY SCREENING OF POTENTIAL SITES FOR A NUCLEAR WASTE REPOSITORY Preclosure Guidelines Preclosure Radiological Safety § 960.5-2-3 Meteorology. (a)...

  17. 17 CFR 2.3 - Prohibitions against misuse of seal.

    Code of Federal Regulations, 2011 CFR

    2011-04-01

    ... seal. 2.3 Section 2.3 Commodity and Securities Exchanges COMMODITY FUTURES TRADING COMMISSION OFFICIAL SEAL § 2.3 Prohibitions against misuse of seal. (a) Fraudulently or wrongfully affixing or impressing the Seal to or upon any certificate, instrument, document or paper or with knowledge of its...

  18. 17 CFR 2.3 - Prohibitions against misuse of seal.

    Code of Federal Regulations, 2014 CFR

    2014-04-01

    ... seal. 2.3 Section 2.3 Commodity and Securities Exchanges COMMODITY FUTURES TRADING COMMISSION OFFICIAL SEAL § 2.3 Prohibitions against misuse of seal. (a) Fraudulently or wrongfully affixing or impressing the Seal to or upon any certificate, instrument, document or paper or with knowledge of its...

  19. 17 CFR 2.3 - Prohibitions against misuse of seal.

    Code of Federal Regulations, 2013 CFR

    2013-04-01

    ... seal. 2.3 Section 2.3 Commodity and Securities Exchanges COMMODITY FUTURES TRADING COMMISSION OFFICIAL SEAL § 2.3 Prohibitions against misuse of seal. (a) Fraudulently or wrongfully affixing or impressing the Seal to or upon any certificate, instrument, document or paper or with knowledge of its...

  20. 17 CFR 2.3 - Prohibitions against misuse of seal.

    Code of Federal Regulations, 2012 CFR

    2012-04-01

    ... seal. 2.3 Section 2.3 Commodity and Securities Exchanges COMMODITY FUTURES TRADING COMMISSION OFFICIAL SEAL § 2.3 Prohibitions against misuse of seal. (a) Fraudulently or wrongfully affixing or impressing the Seal to or upon any certificate, instrument, document or paper or with knowledge of its...

  1. 17 CFR 2.3 - Prohibitions against misuse of seal.

    Code of Federal Regulations, 2010 CFR

    2010-04-01

    ... seal. 2.3 Section 2.3 Commodity and Securities Exchanges COMMODITY FUTURES TRADING COMMISSION OFFICIAL SEAL § 2.3 Prohibitions against misuse of seal. (a) Fraudulently or wrongfully affixing or impressing the Seal to or upon any certificate, instrument, document or paper or with knowledge of its...

  2. 28 CFR 2.3 - Same: Narcotic Addict Rehabilitation Act.

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... 28 Judicial Administration 1 2014-07-01 2014-07-01 false Same: Narcotic Addict Rehabilitation Act. 2.3 Section 2.3 Judicial Administration DEPARTMENT OF JUSTICE PAROLE, RELEASE, SUPERVISION AND... § 2.3 Same: Narcotic Addict Rehabilitation Act. A Federal prisoner committed under the Narcotic...

  3. 28 CFR 2.3 - Same: Narcotic Addict Rehabilitation Act.

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... 28 Judicial Administration 1 2012-07-01 2012-07-01 false Same: Narcotic Addict Rehabilitation Act. 2.3 Section 2.3 Judicial Administration DEPARTMENT OF JUSTICE PAROLE, RELEASE, SUPERVISION AND... § 2.3 Same: Narcotic Addict Rehabilitation Act. A Federal prisoner committed under the Narcotic...

  4. 28 CFR 2.3 - Same: Narcotic Addict Rehabilitation Act.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... 28 Judicial Administration 1 2010-07-01 2010-07-01 false Same: Narcotic Addict Rehabilitation Act. 2.3 Section 2.3 Judicial Administration DEPARTMENT OF JUSTICE PAROLE, RELEASE, SUPERVISION AND... § 2.3 Same: Narcotic Addict Rehabilitation Act. A Federal prisoner committed under the Narcotic...

  5. 28 CFR 2.3 - Same: Narcotic Addict Rehabilitation Act.

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... 28 Judicial Administration 1 2013-07-01 2013-07-01 false Same: Narcotic Addict Rehabilitation Act. 2.3 Section 2.3 Judicial Administration DEPARTMENT OF JUSTICE PAROLE, RELEASE, SUPERVISION AND... § 2.3 Same: Narcotic Addict Rehabilitation Act. A Federal prisoner committed under the Narcotic...

  6. 28 CFR 2.3 - Same: Narcotic Addict Rehabilitation Act.

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... 28 Judicial Administration 1 2011-07-01 2011-07-01 false Same: Narcotic Addict Rehabilitation Act. 2.3 Section 2.3 Judicial Administration DEPARTMENT OF JUSTICE PAROLE, RELEASE, SUPERVISION AND... § 2.3 Same: Narcotic Addict Rehabilitation Act. A Federal prisoner committed under the Narcotic...

  7. 4 CFR 2.3 - GAO Personnel Appeals Board.

    Code of Federal Regulations, 2012 CFR

    2012-01-01

    ... 4 Accounts 1 2012-01-01 2012-01-01 false GAO Personnel Appeals Board. 2.3 Section 2.3 Accounts GOVERNMENT ACCOUNTABILITY OFFICE PERSONNEL SYSTEM PURPOSE AND GENERAL PROVISION § 2.3 GAO Personnel Appeals Board. The Government Accountability Office Personnel Appeals Board is established by 31 U.S.C....

  8. 16 CFR 2.3 - Policy as to private controversies.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 16 Commercial Practices 1 2011-01-01 2011-01-01 false Policy as to private controversies. 2.3 Section 2.3 Commercial Practices FEDERAL TRADE COMMISSION ORGANIZATION, PROCEDURES AND RULES OF PRACTICE NONADJUDICATIVE PROCEDURES Inquiries; Investigations; Compulsory Processes § 2.3 Policy as to...

  9. 43 CFR 8365.2-3 - Occupancy and use.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... 43 Public Lands: Interior 2 2011-10-01 2011-10-01 false Occupancy and use. 8365.2-3 Section 8365.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND MANAGEMENT, DEPARTMENT OF THE INTERIOR RECREATION PROGRAMS VISITOR SERVICES Rules of Conduct § 8365.2-3 Occupancy and...

  10. 43 CFR 8365.2-3 - Occupancy and use.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ... 43 Public Lands: Interior 2 2013-10-01 2013-10-01 false Occupancy and use. 8365.2-3 Section 8365.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND MANAGEMENT, DEPARTMENT OF THE INTERIOR RECREATION PROGRAMS VISITOR SERVICES Rules of Conduct § 8365.2-3 Occupancy and...

  11. The economic downturn and its lingering effects reduced medicare spending growth by $4 billion in 2009-12.

    PubMed

    Dranove, David; Garthwaite, Craig; Ody, Christopher

    2015-08-01

    Previous work has found a strong connection between the most recent economic recession and reductions in private health spending. However, the effect of economic downturns on Medicare spending is less clear. In contrast to studies involving earlier time periods, our study found that when the macroeconomy slowed during the Great Recession of 2007-09, so did Medicare spending growth. A small (14 percent) but significant share of the decline in Medicare spending growth from 2009 to 2012 relative to growth from 2004 to 2009 can be attributed to lingering effects of the recession. Absent the economic downturn, Medicare spending would have been $4 billion higher in 2009-12. A major reason for the relatively small impact of the macroeconomy is the relative lack of labor-force participation among people ages sixty-five and older. We estimate that if they had been working at the same rate as the nonelderly before the recession, the effect of the downturn on Medicare spending growth would have been twice as large. PMID:26240251

  12. Two Billion Cars: What it Means for Climate and Energy Policy

    SciTech Connect

    Daniel Sperling

    2009-04-15

    April 13, 2009: Daniel Sperling, director of the Institute of Transportation Studies at UC Davis, presents the next installment of Berkeley Lab's Environmental Energy Technologies Divisions Distinguished Lecture series. He discusses Two Billion Cars and What it Means for Climate and Energy Policy.

  13. Two Billion Cars: What it Means for Climate and Energy Policy

    ScienceCinema

    Daniel Sperling

    2010-01-08

    April 13, 2009: Daniel Sperling, director of the Institute of Transportation Studies at UC Davis, presents the next installment of Berkeley Lab's Environmental Energy Technologies Divisions Distinguished Lecture series. He discusses Two Billion Cars and What it Means for Climate and Energy Policy.

  14. Nitrogen, phosphorus, and potassium requirements to support a multi-billion gallon biofuel industry

    Technology Transfer Automated Retrieval System (TEKTRAN)

    To accomplish the goals for biofuel and bioenergy production, 1 billion tons of biomass will need to be produced annually by the year 2030. Crop production data from a joint study by the U.S. Department of Energy (US DOE) and the U.S. Department of Agriculture (USDA) demonstrated how this goal could...

  15. Multi-Billion Shot, High-Fluence Exposure of Cr(4+): YAG Passive Q-Switch

    NASA Technical Reports Server (NTRS)

    Stephen, Mark A.; Dallas, Joseph L.; Afzal, Robert S.

    1997-01-01

    NASA's Goddard Space Flight Center is developing the Geoscience Laser Altimeter System (GLAS) employing a diode pumped, Q-Switched, ND:YAG laser operating at 40 Hz repetition rate. To meet the five-year mission lifetime goal, a single transmitter would accumulate over 6.3 billion shots. Cr(4+):YAG is a promising candidate material for passively Q-switching the laser. Historically, the performance of saturable absorbers has degraded over long-duration usage. To measure the multi-billion shot performance of Cr(4+):YAG, a passively Q-switched GLAS-like oscillator was tested at an accelerated repetition rate of 500 Hz. The intracavity fluence was calculated to be approximately 2.5 J/cm(exp 2). The laser was monitored autonomously for 165 days. There was no evidence of change in the material optical properties during the 7.2 billion shot test.. All observed changes in laser operation could be attributed to pump laser diode aging. This is the first demonstration of multi-billion shot exposure testing of Cr(4+):YAG in this pulse energy regime

  16. High-Stakes Hustle: Public Schools and the New Billion Dollar Accountability

    ERIC Educational Resources Information Center

    Baines, Lawrence A.; Stanley, Gregory Kent

    2004-01-01

    High-stakes testing costs up to $50 billion per annum, has no impact on student achievement, and has changed the focus of American public schools. This article analyzes the benefits and costs of the accountability movement, as well as discusses its roots in the eugenics movements of the early 20th century.

  17. US Physician Practices Spend More Than $15.4 Billion Annually To Report Quality Measures.

    PubMed

    Casalino, Lawrence P; Gans, David; Weber, Rachel; Cea, Meagan; Tuchovsky, Amber; Bishop, Tara F; Miranda, Yesenia; Frankel, Brittany A; Ziehler, Kristina B; Wong, Meghan M; Evenson, Todd B

    2016-03-01

    Each year US physician practices in four common specialties spend, on average, 785 hours per physician and more than $15.4 billion dealing with the reporting of quality measures. While much is to be gained from quality measurement, the current system is unnecessarily costly, and greater effort is needed to standardize measures and make them easier to report. PMID:26953292

  18. Universities Report $1.8-Billion in Earnings on Inventions in 2011

    ERIC Educational Resources Information Center

    Blumenstyk, Goldie

    2012-01-01

    Universities and their inventors earned more than $1.8-billion from commercializing their academic research in the 2011 fiscal year, collecting royalties from new breeds of wheat, from a new drug for the treatment of HIV, and from longstanding arrangements over enduring products like Gatorade. Northwestern University earned the most of any…

  19. Cancer costs projected to reach at least $158 billion in 2020

    Cancer.gov

    Based on growth and aging of the U.S. population, medical expenditures for cancer in the year 2020 are projected to reach at least $158 billion (in 2010 dollars) – an increase of 27 percent over 2010. If newly developed tools for cancer diagnosis, treatme

  20. Condensed phase preparation of 2,3-pentanedione

    DOEpatents

    Miller, Dennis J.; Perry, Scott M.; Fanson, Paul T.; Jackson, James E.

    1998-01-01

    A condensed phase process for the preparation of purified 2,3-pentanedione from lactic acid and an alkali metal lactate is described. The process uses elevated temperatures between about 200.degree. to 360.degree. C. for heating a reaction mixture of lactic acid and an alkali metal lactate to produce the 2,3-pentanedione in a reaction vessel. The 2,3-pentanedione produced is vaporized from the reaction vessel and condensed with water.

  1. Condensed phase preparation of 2,3-pentanedione

    DOEpatents

    Miller, D.J.; Perry, S.M.; Fanson, P.T.; Jackson, J.E.

    1998-11-03

    A condensed phase process for the preparation of purified 2,3-pentanedione from lactic acid and an alkali metal lactate is described. The process uses elevated temperatures between about 200 to 360 C for heating a reaction mixture of lactic acid and an alkali metal lactate to produce the 2,3-pentanedione in a reaction vessel. The 2,3-pentanedione produced is vaporized from the reaction vessel and condensed with water. 5 figs.

  2. 42 CFR 2.3 - Purpose and effect.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... criminal penalty (a fine—see 42 U.S.C. 290ee-3(f), 42 U.S.C. 290dd-3(f) and 42 CFR 2.4) for violating the... 42 Public Health 1 2011-10-01 2011-10-01 false Purpose and effect. 2.3 Section 2.3 Public Health... ALCOHOL AND DRUG ABUSE PATIENT RECORDS Introduction § 2.3 Purpose and effect. (a) Purpose. Under...

  3. 42 CFR 2.3 - Purpose and effect.

    Code of Federal Regulations, 2010 CFR

    2010-10-01

    ... ALCOHOL AND DRUG ABUSE PATIENT RECORDS Introduction § 2.3 Purpose and effect. (a) Purpose. Under the... criminal penalty (a fine—see 42 U.S.C. 290ee-3(f), 42 U.S.C. 290dd-3(f) and 42 CFR 2.4) for violating the... 42 Public Health 1 2010-10-01 2010-10-01 false Purpose and effect. 2.3 Section 2.3 Public...

  4. LLNL's Big Science Capabilities Help Spur Over $796 Billion in U.S. Economic Activity Sequencing the Human Genome

    SciTech Connect

    Stewart, Jeffrey S.

    2015-07-28

    LLNL’s successful history of taking on big science projects spans beyond national security and has helped create billions of dollars per year in new economic activity. One example is LLNL’s role in helping sequence the human genome. Over $796 billion in new economic activity in over half a dozen fields has been documented since LLNL successfully completed this Grand Challenge.

  5. Psychodrama with Deaf People

    ERIC Educational Resources Information Center

    Clayton, Lynette; Robinson, Luther D.

    1971-01-01

    Observations based on psychodrama with deaf people, relating to interaction between people and the communication process, are made. How role training skills, which involve some of the skills of psychodrama, can be applied by professionals in vocational and social learning situations is illustrated. (KW)

  6. People and Deserts.

    ERIC Educational Resources Information Center

    NatureScope, 1985

    1985-01-01

    Provides: (1) background information on ways people affect deserts and ways deserts affect people; (2) student activities on this topic; and (3) ready-to-copy materials (culture match worksheet and causes worksheet). Each activity includes objective(s), recommended age level(s), subject area(s), list of materials needed, and procedures. (DH)

  7. Managing & Developing People.

    ERIC Educational Resources Information Center

    Brain, Gill, Ed.

    This book presents ideas about and approaches to human resource management (HRM) in British further education (FE) colleges. Introductory material includes author biographies and a preface (Brain) on human resource issues in FE. "Investors in People" (Chambers) considers how working toward recognition as an Investor in People (a British National…

  8. People & Tropical Rain Forests.

    ERIC Educational Resources Information Center

    NatureScope, 1989

    1989-01-01

    Discusses ways people who live in rain forests make a living and some of the products that enrich our lives. Provides activities covering forest people, tropical treats, jungle in the pantry, treetop explorers, and three copyable pages to accompany activities. (Author/RT)

  9. Aid to families with dependent children: who receives more than $22 billion and why?

    PubMed

    Waldman, H B

    1996-01-01

    A general outline of the Aid to Families with Dependent Children program is provided. The $22 billion program provides financial support to 14 million persons (including more than 9 million children). The changing character of the family structure is considered in terms of efforts to control AFDC spending. Additional programs to assist children (Social Security, Supplemental Security Insurance and Food Stamps) are reviewed. PMID:8708125

  10. Severe Obesity In Adults Cost State Medicaid Programs Nearly $8 Billion In 2013.

    PubMed

    Wang, Y Claire; Pamplin, John; Long, Michael W; Ward, Zachary J; Gortmaker, Steven L; Andreyeva, Tatiana

    2015-11-01

    Efforts to expand Medicaid while controlling spending must be informed by a deeper understanding of the extent to which the high medical costs associated with severe obesity (having a body mass index of [Formula: see text] or higher) determine spending at the state level. Our analysis of population-representative data indicates that in 2013, severe obesity cost the nation approximately $69 billion, which accounted for 60 percent of total obesity-related costs. Approximately 11 percent of the cost of severe obesity was paid for by Medicaid, 30 percent by Medicare and other federal health programs, 27 percent by private health plans, and 30 percent out of pocket. Overall, severe obesity cost state Medicaid programs almost $8 billion a year, ranging from $5 million in Wyoming to $1.3 billion in California. These costs are likely to increase following Medicaid expansion and enhanced coverage of weight loss therapies in the form of nutrition consultation, drug therapy, and bariatric surgery. Ensuring and expanding Medicaid-eligible populations' access to cost-effective treatment for severe obesity should be part of each state's strategy to mitigate rising obesity-related health care costs. PMID:26526251

  11. Spatial variability in oceanic redox structure 1.8billion years ago

    NASA Astrophysics Data System (ADS)

    Poulton, Simon W.; Fralick, Philip W.; Canfield, Donald E.

    2010-07-01

    The evolution of ocean chemistry during the Proterozoic eon (2.5-0.542 billion years ago) is thought to have played a central role in both the timing and rate of eukaryote evolution. The timing of the deposition of iron formations implies that, early in the Earth's history, oceans were predominantly anoxic and rich in dissolved iron. However, global deposition of iron formations ceased about 1.84 billion years ago. This termination indicates a major upheaval in ocean chemistry, but the precise nature of this change remains debated. Here we use iron and sulphur systematics to reconstruct oceanic redox conditions from the 1.88- to 1.83-billion-year-old Animikie group from the Superior region, North America. We find that surface waters were oxygenated, whereas at mid-depths, anoxic and sulphidic (euxinic) conditions extended over 100km from the palaeoshoreline. The spatial extent of euxinia varied through time, but deep ocean waters remained rich in dissolved iron. Widespread euxinia along continental margins would have removed dissolved iron from the water column through the precipitation of pyrite, which would have reduced the supply of dissolved iron and resulted in the global cessation of the deposition of `Superior-type' iron formations. We suggest that incursions of sulphide from the mid-depths into overlying oxygenated surface waters may have placed severe constraints on eukaryotic evolution.

  12. MMap: Fast Billion-Scale Graph Computation on a PC via Memory Mapping

    PubMed Central

    Lin, Zhiyuan; Kahng, Minsuk; Sabrin, Kaeser Md.; Chau, Duen Horng (Polo); Lee, Ho; Kang, U

    2015-01-01

    Graph computation approaches such as GraphChi and TurboGraph recently demonstrated that a single PC can perform efficient computation on billion-node graphs. To achieve high speed and scalability, they often need sophisticated data structures and memory management strategies. We propose a minimalist approach that forgoes such requirements, by leveraging the fundamental memory mapping (MMap) capability found on operating systems. We contribute: (1) a new insight that MMap is a viable technique for creating fast and scalable graph algorithms that surpasses some of the best techniques; (2) the design and implementation of popular graph algorithms for billion-scale graphs with little code, thanks to memory mapping; (3) extensive experiments on real graphs, including the 6.6 billion edge YahooWeb graph, and show that this new approach is significantly faster or comparable to the highly-optimized methods (e.g., 9.5× faster than GraphChi for computing PageRank on 1.47B edge Twitter graph). We believe our work provides a new direction in the design and development of scalable algorithms. Our packaged code is available at http://poloclub.gatech.edu/mmap/. PMID:25866846

  13. A 17-billion-solar-mass black hole in a group galaxy with a diffuse core.

    PubMed

    Thomas, Jens; Ma, Chung-Pei; McConnell, Nicholas J; Greene, Jenny E; Blakeslee, John P; Janish, Ryan

    2016-04-21

    Quasars are associated with and powered by the accretion of material onto massive black holes; the detection of highly luminous quasars with redshifts greater than z = 6 suggests that black holes of up to ten billion solar masses already existed 13 billion years ago. Two possible present-day 'dormant' descendants of this population of 'active' black holes have been found in the galaxies NGC 3842 and NGC 4889 at the centres of the Leo and Coma galaxy clusters, which together form the central region of the Great Wall--the largest local structure of galaxies. The most luminous quasars, however, are not confined to such high-density regions of the early Universe; yet dormant black holes of this high mass have not yet been found outside of modern-day rich clusters. Here we report observations of the stellar velocity distribution in the galaxy NGC 1600--a relatively isolated elliptical galaxy near the centre of a galaxy group at a distance of 64 megaparsecs from Earth. We use orbit superposition models to determine that the black hole at the centre of NGC 1600 has a mass of 17 billion solar masses. The spatial distribution of stars near the centre of NGC 1600 is rather diffuse. We find that the region of depleted stellar density in the cores of massive elliptical galaxies extends over the same radius as the gravitational sphere of influence of the central black holes, and interpret this as the dynamical imprint of the black holes. PMID:27049949

  14. Two ten-billion-solar-mass black holes at the centres of giant elliptical galaxies.

    PubMed

    McConnell, Nicholas J; Ma, Chung-Pei; Gebhardt, Karl; Wright, Shelley A; Murphy, Jeremy D; Lauer, Tod R; Graham, James R; Richstone, Douglas O

    2011-12-01

    Observational work conducted over the past few decades indicates that all massive galaxies have supermassive black holes at their centres. Although the luminosities and brightness fluctuations of quasars in the early Universe suggest that some were powered by black holes with masses greater than 10 billion solar masses, the remnants of these objects have not been found in the nearby Universe. The giant elliptical galaxy Messier 87 hosts the hitherto most massive known black hole, which has a mass of 6.3 billion solar masses. Here we report that NGC 3842, the brightest galaxy in a cluster at a distance from Earth of 98 megaparsecs, has a central black hole with a mass of 9.7 billion solar masses, and that a black hole of comparable or greater mass is present in NGC 4889, the brightest galaxy in the Coma cluster (at a distance of 103 megaparsecs). These two black holes are significantly more massive than predicted by linearly extrapolating the widely used correlations between black-hole mass and the stellar velocity dispersion or bulge luminosity of the host galaxy. Although these correlations remain useful for predicting black-hole masses in less massive elliptical galaxies, our measurements suggest that different evolutionary processes influence the growth of the largest galaxies and their black holes. PMID:22158244

  15. 43 CFR 3712.2-3 - Contents of published notice.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... 43 Public Lands: Interior 2 2011-10-01 2011-10-01 false Contents of published notice. 3712.2-3 Section 3712.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND MANAGEMENT, DEPARTMENT OF THE INTERIOR MINERALS MANAGEMENT (3000) PUBLIC LAW 167; ACT OF JULY 23,...

  16. 43 CFR 3107.2-3 - Leases capable of production.

    Code of Federal Regulations, 2012 CFR

    2012-10-01

    ... or Renewal § 3107.2-3 Leases capable of production. No lease for lands on which there is a well... 43 Public Lands: Interior 2 2012-10-01 2012-10-01 false Leases capable of production. 3107.2-3... same, unless the lessee fails to place the lease in production within a period of not less than 60...

  17. 43 CFR 3107.2-3 - Leases capable of production.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... or Renewal § 3107.2-3 Leases capable of production. No lease for lands on which there is a well... 43 Public Lands: Interior 2 2011-10-01 2011-10-01 false Leases capable of production. 3107.2-3... same, unless the lessee fails to place the lease in production within a period of not less than 60...

  18. 43 CFR 3107.2-3 - Leases capable of production.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ... or Renewal § 3107.2-3 Leases capable of production. No lease for lands on which there is a well... 43 Public Lands: Interior 2 2014-10-01 2014-10-01 false Leases capable of production. 3107.2-3... same, unless the lessee fails to place the lease in production within a period of not less than 60...

  19. 16 CFR 2.3 - Policy as to private controversies.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... other action when the alleged violation of law is merely a matter of private controversy and does not... 16 Commercial Practices 1 2010-01-01 2010-01-01 false Policy as to private controversies. 2.3... NONADJUDICATIVE PROCEDURES Inquiries; Investigations; Compulsory Processes § 2.3 Policy as to...

  20. 43 CFR 3453.2-3 - Filing location and fee.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... leased lands proposed for transfer (see 43 CFR subpart 1821). Each instrument of transfer shall be... 43 Public Lands: Interior 2 2011-10-01 2011-10-01 false Filing location and fee. 3453.2-3 Section 3453.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF...

  1. 43 CFR 4110.2-3 - Transfer of grazing preference.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ... 43 Public Lands: Interior 2 2013-10-01 2013-10-01 false Transfer of grazing preference. 4110.2-3 Section 4110.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND... improvements authorized on public lands under § 4120.3 and maintained in conjunction with the...

  2. 43 CFR 4110.2-3 - Transfer of grazing preference.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ... 43 Public Lands: Interior 2 2014-10-01 2014-10-01 false Transfer of grazing preference. 4110.2-3 Section 4110.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND... improvements authorized on public lands under § 4120.3 and maintained in conjunction with the...

  3. 43 CFR 4110.2-3 - Transfer of grazing preference.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... 43 Public Lands: Interior 2 2011-10-01 2011-10-01 false Transfer of grazing preference. 4110.2-3 Section 4110.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND... improvements authorized on public lands under § 4120.3 and maintained in conjunction with the...

  4. 43 CFR 4110.2-3 - Transfer of grazing preference.

    Code of Federal Regulations, 2012 CFR

    2012-10-01

    ... 43 Public Lands: Interior 2 2012-10-01 2012-10-01 false Transfer of grazing preference. 4110.2-3 Section 4110.2-3 Public Lands: Interior Regulations Relating to Public Lands (Continued) BUREAU OF LAND... improvements authorized on public lands under § 4120.3 and maintained in conjunction with the...

  5. 32 CFR 2.3 - Regulatory relief for participating programs.

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ....3 Section 2.3 National Defense Department of Defense OFFICE OF THE SECRETARY OF DEFENSE ACQUISITION PILOT PROGRAM POLICY § 2.3 Regulatory relief for participating programs. (a) A program participating in... the Component, or the DoD Component Acquisition Executive. 1 Copies of this Department of...

  6. 32 CFR 2.3 - Regulatory relief for participating programs.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ....3 Section 2.3 National Defense Department of Defense OFFICE OF THE SECRETARY OF DEFENSE ACQUISITION PILOT PROGRAM POLICY § 2.3 Regulatory relief for participating programs. (a) A program participating in... the Component, or the DoD Component Acquisition Executive. 1 Copies of this Department of...

  7. 40 CFR 35.909 - Step 2+3 grants.

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... 40 Protection of Environment 1 2011-07-01 2011-07-01 false Step 2+3 grants. 35.909 Section 35.909 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY GRANTS AND OTHER FEDERAL ASSISTANCE STATE AND LOCAL ASSISTANCE Grants for Construction of Treatment Works-Clean Water Act § 35.909 Step 2+3 grants. (a) Authority. The Regional...

  8. 43 CFR 3410.2-3 - Surface management agency.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... 43 Public Lands: Interior 2 2011-10-01 2011-10-01 false Surface management agency. 3410.2-3... § 3410.2-3 Surface management agency. The authorized officer may issue an exploration license covering lands the surface of which is under the jurisdiction of any Federal agency other than the Bureau of...

  9. SIRT1, 2, 3 protect mouse oocytes from postovulatory aging

    PubMed Central

    Zhang, Teng; Zhou, Yang; Li, Li; Wang, Hong-Hui; Ma, Xue-Shan; Qian, Wei-Ping; Shen, Wei; Schatten, Heide; Sun, Qing-Yuan

    2016-01-01

    The quality of metaphase II oocytes will undergo a time-dependent deterioration following ovulation as the result of the oocyte aging process. In this study, we determined that the expression of sirtuin family members (SIRT1, 2, 3) was dramatically reduced in mouse oocytes aged in vivo or in vitro. Increased intracellular ROS was observed when SIRT1, 2, 3 activity was inhibited. Increased frequency of spindle defects and disturbed distribution of mitochondria were also observed in MII oocytes aged in vitro after treatment with Nicotinamide (NAM), indicating that inhibition of SIRT1, 2, 3 may accelerate postovulatory oocyte aging. Interestingly, when MII oocytes were exposed to caffeine, the decline of SIRT1, 2, 3 mRNA levels was delayed and the aging-associated defective phenotypes could be improved. The results suggest that the SIRT1, 2, 3 pathway may play a potential protective role against postovulatory oocyte aging by controlling ROS generation. PMID:26974211

  10. Structure of the catalytic domain of the hepatitis C virus NS2-3 protease

    SciTech Connect

    Lorenz,I.; Marcotrigiano, J.; Dentzer, T.; Rice, C.

    2006-01-01

    Hepatitis C virus is a major global health problem affecting an estimated 170 million people worldwide. Chronic infection is common and can lead to cirrhosis and liver cancer. There is no vaccine available and current therapies have met with limited success. The viral RNA genome encodes a polyprotein that includes two proteases essential for virus replication. The NS2-3 protease mediates a single cleavage at the NS2/NS3 junction, whereas the NS3-4A protease cleaves at four downstream sites in the polyprotein. NS3-4A is characterized as a serine protease with a chymotrypsin-like fold, but the enzymatic mechanism of the NS2-3 protease remains unresolved. Here we report the crystal structure of the catalytic domain of the NS2-3 protease at 2.3 Angstroms resolution. The structure reveals a dimeric cysteine protease with two composite active sites. For each active site, the catalytic histidine and glutamate residues are contributed by one monomer, and the nucleophilic cysteine by the other. The carboxy-terminal residues remain coordinated in the two active sites, predicting an inactive post-cleavage form. Proteolysis through formation of a composite active site occurs in the context of the viral polyprotein expressed in mammalian cells. These features offer unexpected insights into polyprotein processing by hepatitis C virus and new opportunities for antiviral drug design.

  11. Air density 2.7 billion years ago limited to less than twice modern levels by fossil raindrop imprints.

    PubMed

    Som, Sanjoy M; Catling, David C; Harnmeijer, Jelte P; Polivka, Peter M; Buick, Roger

    2012-04-19

    According to the 'Faint Young Sun' paradox, during the late Archaean eon a Sun approximately 20% dimmer warmed the early Earth such that it had liquid water and a clement climate. Explanations for this phenomenon have invoked a denser atmosphere that provided warmth by nitrogen pressure broadening or enhanced greenhouse gas concentrations. Such solutions are allowed by geochemical studies and numerical investigations that place approximate concentration limits on Archaean atmospheric gases, including methane, carbon dioxide and oxygen. But no field data constraining ground-level air density and barometric pressure have been reported, leaving the plausibility of these various hypotheses in doubt. Here we show that raindrop imprints in tuffs of the Ventersdorp Supergroup, South Africa, constrain surface air density 2.7 billion years ago to less than twice modern levels. We interpret the raindrop fossils using experiments in which water droplets of known size fall at terminal velocity into fresh and weathered volcanic ash, thus defining a relationship between imprint size and raindrop impact momentum. Fragmentation following raindrop flattening limits raindrop size to a maximum value independent of air density, whereas raindrop terminal velocity varies as the inverse of the square root of air density. If the Archaean raindrops reached the modern maximum measured size, air density must have been less than 2.3 kg m(-3), compared to today's 1.2 kg m(-3), but because such drops rarely occur, air density was more probably below 1.3 kg m(-3). The upper estimate for air density renders the pressure broadening explanation possible, but it is improbable under the likely lower estimates. Our results also disallow the extreme CO(2) levels required for hot Archaean climates. PMID:22456703

  12. Validation of an evacuated canister method for measuring part-per-billion levels of chemical warfare agent simulants.

    PubMed

    Coffey, Christopher C; LeBouf, Ryan F; Calvert, Catherine A; Slaven, James E

    2011-08-01

    The National Institute for Occupational Safety and Health (NIOSH) research on direct-reading instruments (DRIs) needed an instantaneous sampling method to provide independent confirmation of the concentrations of chemical warfare agent (CWA) simulants. It was determined that evacuated canisters would be the method of choice. There is no method specifically validated for volatile organic compounds (VOCs) in the NIOSH Manual of Analytical Methods. The purpose of this study was to validate an evacuated canister method for sampling seven specific VOCs that can be used as a simulant for CWA agents (cyclohexane) or influence the DRI measurement of CWA agents (acetone, chloroform, methylene chloride, methyl ethyl ketone, hexane, and carbon tetrachloride [CCl4]). The method used 6-L evacuated stainless-steel fused silica-lined canisters to sample the atmosphere containing VOCs. The contents of the canisters were then introduced into an autosampler/preconcentrator using a microscale purge and trap (MPT) method. The MPT method trapped and concentrated the VOCs in the air sample and removed most of the carbon dioxide and water vapor. After preconcentration, the samples were analyzed using a gas chromatograph with a mass selective detector. The method was tested, evaluated, and validated using the NIOSH recommended guidelines. The evaluation consisted of determining the optimum concentration range for the method; the sample stability over 30 days; and the accuracy, precision, and bias of the method. This method meets the NIOSH guidelines for six of the seven compounds (excluding acetone) tested in the range of 2.3-50 parts per billion (ppb), making it suitable for sampling of these VOCs at the ppb level. PMID:21874953

  13. Meet the Noodle People.

    ERIC Educational Resources Information Center

    Kananen, Mary King

    1995-01-01

    Presents a hands-on activity for children to build and take home a basic model of the human skeletal system. Describes how to make "noodle people" from ordinary materials including pasta, pipe cleaners, straws, and margarine tub lids. (NB)

  14. People and Oceans.

    ERIC Educational Resources Information Center

    NatureScope, 1988

    1988-01-01

    Discusses people's relationship with oceans, focusing on ocean pollution, use, and protective measures of the sea and its wildlife. Activities included are "Mythical Monsters"; "Globetrotters"; "Plastic in the Sea"; and "Sea of Many Uses." (RT)

  15. Older People and HIV

    MedlinePlus

    ... common than they were before the use of anti-HIV drugs. It is difficult to know what is causing mental problems in older people with HIV. Is it normal aging, or is it HIV disease? Research studies have ...

  16. Healthy Water, Healthy People.

    ERIC Educational Resources Information Center

    Etgen, John

    2002-01-01

    Describes a hands-on activity, Hitting the Mark, which is found in the "Healthy Water, Healthy People Water Quality Educators Guide" in terms of its objectives, materials, background, procedures, activities, and assessment. (KHR)

  17. The Believability of People

    ERIC Educational Resources Information Center

    Ennis, Robert H.

    1974-01-01

    Author presented a set of general criteria for judging the statements of people who speak or write with an air of authority and applied these criteria to a particular case, a printed discussion of tooth care. (Author/RK)

  18. Very happy people.

    PubMed

    Diener, Ed; Seligman, Martin E P

    2002-01-01

    A sample of 222 undergraduates was screened for high happiness using multiple confirming assessment filters. We compared the upper 10% of consistently very happy people with average and very unhappy people. The very happy people were highly social, and had stronger romantic and other social relationships than less happy groups. They were more extraverted, more agreeable, and less neurotic, and scored lower on several psychopathology scales of the Minnesota Multiphasic Personality Inventory. Compared with the less happy groups, the happiest respondents did not exercise significantly more, participate in religious activities significantly more, or experience more objectively defined good events. No variable was sufficient for happiness, but good social relations were necessary. Members of the happiest group experienced positive, but not ecstatic, feelings most of the time, and they reported occasional negative moods. This suggests that very happy people do have a functioning emotion system that can react appropriately to life events. PMID:11894851

  19. Nicotinic acid metabolism. 2,3-Dimethylmalate lyase.

    PubMed

    Pirzer, P; Lill, U; Eggerer, H

    1979-12-01

    1) A new enzyme, 2,3-dimethylmalate lyase, was purified from Clostridium barkeri to about 80% homogeneity. Some of the properties of the enzyme are described. 2) It is shown that the 2,3-dimethylmalic acid (m.p. 143 degrees C) described in the literature represents only one racemic pair. This pair is not attacked by 2,3-dimethylmalate lyase. 3) The isolation of both racemic pairs of 2,3-dimethylmalic acid is described. Half of one pair, m.p. 104-106 degrees C, was converted to propionate and pyruvate by 2,3-dimethylmalate lyase. 4) In combination with earlier work performed by E.R. Stadtman and coworkers the results given under points 1--3 establish 2,3-dimethylmalate as an intermediate in the degradation of nicotinic acid by C. barkeri. 5) Experimental evidence indicates the 2,3-dimethylmalate lyase is no acyl-S-enzyme and that it is different in this respect as well as in quaternary structure from the apparently related enzymes citrate lyase and citramalate lyase. PMID:527937

  20. Fluorination of 1,2,3,4- and 1,2,3,5-tetrahalobenzenes with potassium fluoride in dimethyl sulfone

    USGS Publications Warehouse

    Finger, G.C.; Dickerson, D.R.; Shiley, R.H.

    1972-01-01

    1,2,3,4-Tetrachlorobenzene, 1,2,3,5-tetrachlorobenzene, 2,4,6-trichlorofluorobenzene, and 2,6-dichloro-1,4-difluorobenzene were fluorinated with potassium fluoride and potassium fluoride-cesium fluoride mixtures in dimethyl sulfone. By varying the concentration, temperature and reaction time, the degree of fluorination could be controlled to some extent. The optimum conditions for producing mono-, di- and tri-fluoro-substituted chlorobenzenes and trace amounts of tetrafluorobenzene from the corresponding tetrachlorobenzenes are given. 1,2,3,5-Tetrafluorobenzene was obtained in 44.8% yield from 2,6-dichloro-1,4-difluorobenzene. 1,2,3,4-Tetrafluorobenzene was obtained in only trace amounts from 1,2,3,4-tetrachlorobenzene. A total of 24 new chlorofluorobenzenes and intermediates are described. Fluorination with potassium fluoride and certain other metal fluorides was also investigated. ?? 1972.

  1. Six People to Know

    ERIC Educational Resources Information Center

    Young, Robyn R.

    2012-01-01

    Teaching is a difficult and time-consuming job, but the rewards teachers receive from their students are unquestionably worth it. The good news is that in every school, there are people that they work with who can help to make their daily life much easier--but they are not always the people that they would think to ask for help. New teachers often…

  2. Relationship of frontal D(2/3) binding potentials to cognition: a study of antipsychotic-naive schizophrenia patients.

    PubMed

    Fagerlund, Birgitte; Pinborg, Lars H; Mortensen, Erik Lykke; Friberg, Lars; Baaré, William F C; Gade, Anders; Svarer, Claus; Glenthøj, Birte Y

    2013-02-01

    Studies of in vivo dopamine receptors in schizophrenia have mostly focused on D(2) receptors in striatal areas or on D(1) receptors in cortex. No previous study has examined the correlation between cortical dopamine D(2/3) receptor binding potentials and cognition in schizophrenia patients. The objective was to examine this relation in the frontal cortex in first-episode, drug-naive schizophrenia patients. Based on preclinical and pharmacological evidence, we specifically expected to find a relation between D(2/3) receptor binding potentials and set shifting. This was a cross-sectional, case-control study using single-photon emission computerized tomography with the D(2/3)-receptor ligand [(123)I]epidepride, co-registered with structural magnetic resonance imaging and correlated to cognitive measures. Participants were 24 antipsychotic-naive, first-episode schizophrenia patients and 20 healthy controls matched for gender and age. For patients, a significant linear correlation between D(2/3) BP(ND) and set shifting was found, while significant quadratic associations were observed for verbal fluency, planning and attention. For controls, the only significant association with D(2/3) BP(ND) was a quadratic partial correlation for set shifting. The main findings indicated a relation between D(2/3) receptor binding in the frontal cortex and set shifting, planning and attention, but also support a differential involvement of cortical dopamine D(2/3) receptor binding in at least some cognitive functions, perhaps particularly attention, in schizophrenia patients compared to healthy people. The results suggest that cortical D(2/3) receptor function may be more involved in some cognitive functions (i.e. attention, fluency and planning) in patients with schizophrenia than in healthy people, suggesting that information processing in schizophrenia may be characterized by lower signal:noise ratios. PMID:22338593

  3. Ferromagnetism in Cu 3-thiosemicarbazone- 2,3-dioxoindole complexes

    NASA Astrophysics Data System (ADS)

    Zentková, M.; Kováč, J.; Zentko, A.; Košturiak, A.

    1991-12-01

    We report evidence for ferromagnetic ordering in Cu-chelates of 3-thiosemicarbazone-2,3-dioxoindole (isatine). It has been found that the Curie temperature is 16.8 K and is independent of the Cu content.

  4. Dielectric properties of polyfunctional alcohols: 2,3-butanediol

    NASA Astrophysics Data System (ADS)

    Zhuravlev, V. I.

    2016-08-01

    Using a variety theoretical approaches within the Debye, Davidson-Cole, and Forsman models, and an approach based on the Dissado-Hill theory, dielectric spectra of 2,3-butanediol in the temperature range of 298 to 423 K are analyzed. It is shown that the dielectric spectra of 2,3-butanediole are described by the Davidson-Cole equation, and the βDC parameter depends strongly on temperature. The spectrum of dielectric relaxation of 2,3-butanediol within the Debye theory is presented as the sum of two areas of dispersion, and conclusions are drawn regarding possible mechanisms of dispersion responsible for the obtained fields. The relaxation times of 2,3-butanediol, calculated using different equations describing the nonlinear behavior of relaxation times, are compared. The dipole moments of clusters are obtained for the first time using the Dissado-Hill cluster model, and a preliminary analysis of them is performed.

  5. 43 CFR 2916.2-3 - Renewal of leases.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ..., DEPARTMENT OF THE INTERIOR LAND RESOURCE MANAGEMENT (2000) LEASES Alaska Fur Farm § 2916.2-3 Renewal of... preference right to a renewal. The timely filing of an application will, however authorize the exclusive...

  6. 43 CFR 2916.2-3 - Renewal of leases.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ..., DEPARTMENT OF THE INTERIOR LAND RESOURCE MANAGEMENT (2000) LEASES Alaska Fur Farm § 2916.2-3 Renewal of... preference right to a renewal. The timely filing of an application will, however authorize the exclusive...

  7. 43 CFR 2916.2-3 - Renewal of leases.

    Code of Federal Regulations, 2012 CFR

    2012-10-01

    ..., DEPARTMENT OF THE INTERIOR LAND RESOURCE MANAGEMENT (2000) LEASES Alaska Fur Farm § 2916.2-3 Renewal of... preference right to a renewal. The timely filing of an application will, however authorize the exclusive...

  8. 43 CFR 2916.2-3 - Renewal of leases.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ..., DEPARTMENT OF THE INTERIOR LAND RESOURCE MANAGEMENT (2000) LEASES Alaska Fur Farm § 2916.2-3 Renewal of... preference right to a renewal. The timely filing of an application will, however authorize the exclusive...

  9. 34. DETAILS OF CAISSON FOR PIERS 2, 3, 4 AND ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    34. DETAILS OF CAISSON FOR PIERS 2, 3, 4 AND 5 TO BE BUILT ON SOIL OVERBURDEN - East Bloomsburg Bridge, Spanning Susquehanna River at Pennsylvania Route 487 (Legislative Route 283), Bloomsburg, Columbia County, PA

  10. Asymmetric Organocatalytic Wittig [2,3]-Rearrangement of Oxindoles.

    PubMed

    Ošeka, Maksim; Kimm, Mariliis; Kaabel, Sandra; Järving, Ivar; Rissanen, Kari; Kanger, Tõnis

    2016-03-18

    A highly enantioselective organocatalytic [2,3]-rearrangement of oxindole derivatives is presented. The reaction was catalyzed by squaramide, and this provides access to 3-hydroxy 3-substituted oxindoles in high enantiomeric purities. PMID:26937554

  11. 2,3-Butanediol Metabolism in the Acetogen Acetobacterium woodii.

    PubMed

    Hess, Verena; Oyrik, Olga; Trifunović, Dragan; Müller, Volker

    2015-07-01

    The acetogenic bacterium Acetobacterium woodii is able to reduce CO2 to acetate via the Wood-Ljungdahl pathway. Only recently we demonstrated that degradation of 1,2-propanediol by A. woodii was not dependent on acetogenesis, but that it is disproportionated to propanol and propionate. Here, we analyzed the metabolism of A. woodii on another diol, 2,3-butanediol. Experiments with growing and resting cells, metabolite analysis and enzymatic measurements revealed that 2,3-butanediol is oxidized in an NAD(+)-dependent manner to acetate via the intermediates acetoin, acetaldehyde, and acetyl coenzyme A. Ethanol was not detected as an end product, either in growing cultures or in cell suspensions. Apparently, all reducing equivalents originating from the oxidation of 2,3-butanediol were funneled into the Wood-Ljungdahl pathway to reduce CO2 to another acetate. Thus, the metabolism of 2,3-butanediol requires the Wood-Ljungdahl pathway. PMID:25934628

  12. 2,3-Butanediol Metabolism in the Acetogen Acetobacterium woodii

    PubMed Central

    Hess, Verena; Oyrik, Olga; Trifunović, Dragan

    2015-01-01

    The acetogenic bacterium Acetobacterium woodii is able to reduce CO2 to acetate via the Wood-Ljungdahl pathway. Only recently we demonstrated that degradation of 1,2-propanediol by A. woodii was not dependent on acetogenesis, but that it is disproportionated to propanol and propionate. Here, we analyzed the metabolism of A. woodii on another diol, 2,3-butanediol. Experiments with growing and resting cells, metabolite analysis and enzymatic measurements revealed that 2,3-butanediol is oxidized in an NAD+-dependent manner to acetate via the intermediates acetoin, acetaldehyde, and acetyl coenzyme A. Ethanol was not detected as an end product, either in growing cultures or in cell suspensions. Apparently, all reducing equivalents originating from the oxidation of 2,3-butanediol were funneled into the Wood-Ljungdahl pathway to reduce CO2 to another acetate. Thus, the metabolism of 2,3-butanediol requires the Wood-Ljungdahl pathway. PMID:25934628

  13. VIEW OF APALACHICOLA RIVER BRIDGE SPANS 2, 3, AND 4, ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    VIEW OF APALACHICOLA RIVER BRIDGE SPANS 2, 3, AND 4, EAST SIDE, FROM CENTER OF RIVER, FACING WEST - Apalachicola River Bridge, State Route 20 spanning the Apalachicola River, Blountstown, Calhoun County, FL

  14. VIEW OF APALACHICOLA RIVER BRIDGE SPANS 2, 3, 4, AND ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    VIEW OF APALACHICOLA RIVER BRIDGE SPANS 2, 3, 4, AND 5, EAST SIDE, FROM NORTH SHORE OF RIVER (CALHOUN COUNTY SIDE), FACING SOUTH - Apalachicola River Bridge, State Route 20 spanning the Apalachicola River, Blountstown, Calhoun County, FL

  15. VIEW OF APALACHICOLA RIVER BRIDGE SPANS 1, 2, 3, 4, ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    VIEW OF APALACHICOLA RIVER BRIDGE SPANS 1, 2, 3, 4, AND 5, EAST SIDE, FROM SOUTH SHORE OF RIVER (LIBERTY COUNTY SIDE), FACING WEST - Apalachicola River Bridge, State Route 20 spanning the Apalachicola River, Blountstown, Calhoun County, FL

  16. ANCHOR SETTING PLAN FOR PIERS 1, 2, 3, 4, 5 ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    ANCHOR SETTING PLAN FOR PIERS 1, 2, 3, 4, 5 AND 6, APALACHICOLA RIVER BRIDGE, SHEET 5505 TO 8-M1 - Apalachicola River Bridge, State Route 20 spanning the Apalachicola River, Blountstown, Calhoun County, FL

  17. VIEW OF APALACHICOLA RIVER BRIDGE SPANS 2, 3, AND 4, ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    VIEW OF APALACHICOLA RIVER BRIDGE SPANS 2, 3, AND 4, WEST SIDE, FROM CENTER OF RIVER, FACING EAST - Apalachicola River Bridge, State Route 20 spanning the Apalachicola River, Blountstown, Calhoun County, FL

  18. A 17-billion-solar-mass black hole in a group galaxy with a diffuse core

    NASA Astrophysics Data System (ADS)

    Thomas, Jens; Ma, Chung-Pei; McConnell, Nicholas J.; Greene, Jenny E.; Blakeslee, John P.; Janish, Ryan

    2016-04-01

    Quasars are associated with and powered by the accretion of material onto massive black holes; the detection of highly luminous quasars with redshifts greater than z = 6 suggests that black holes of up to ten billion solar masses already existed 13 billion years ago. Two possible present-day ‘dormant’ descendants of this population of ‘active’ black holes have been found in the galaxies NGC 3842 and NGC 4889 at the centres of the Leo and Coma galaxy clusters, which together form the central region of the Great Wall—the largest local structure of galaxies. The most luminous quasars, however, are not confined to such high-density regions of the early Universe; yet dormant black holes of this high mass have not yet been found outside of modern-day rich clusters. Here we report observations of the stellar velocity distribution in the galaxy NGC 1600—a relatively isolated elliptical galaxy near the centre of a galaxy group at a distance of 64 megaparsecs from Earth. We use orbit superposition models to determine that the black hole at the centre of NGC 1600 has a mass of 17 billion solar masses. The spatial distribution of stars near the centre of NGC 1600 is rather diffuse. We find that the region of depleted stellar density in the cores of massive elliptical galaxies extends over the same radius as the gravitational sphere of influence of the central black holes, and interpret this as the dynamical imprint of the black holes.

  19. 10 CFR 2.3 - Resolution of conflict.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 10 Energy 1 2011-01-01 2011-01-01 false Resolution of conflict. 2.3 Section 2.3 Energy NUCLEAR... Resolution of conflict. (a) In any conflict between a general rule in subpart C of this part and a special... not apply to hearings in 10 CFR parts 4, 9, 10, 11, 12, 13, 15, 16, and subparts H and I of 10...

  20. 10 CFR 2.3 - Resolution of conflict.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... not apply to hearings in 10 CFR parts 4, 9, 10, 11, 12, 13, 15, 16, and subparts H and I of 10 CFR... 10 Energy 1 2010-01-01 2010-01-01 false Resolution of conflict. 2.3 Section 2.3 Energy NUCLEAR... Resolution of conflict. (a) In any conflict between a general rule in subpart C of this part and a...

  1. 2.3.1 Biological Effects of Ionizing Radiations

    NASA Astrophysics Data System (ADS)

    Kaul, A.

    This document is part of Subvolume A 'Fundamentals and Data in Radiobiology, Radiation Biophysics, Dosimetry and Medical Radiological Protection' of Volume 7 'Medical Radiological Physics' of Landolt-Börnstein - Group VIII 'Advanced Materials and Technologies'. It contains the Subsection '2.3.1 Biological Effects of Ionizing Radiations' of the Section '2.3 Biological Effects' of the Chapter '2 Radiation and Biological Effects' with the comtents:

  2. Triploblastic animals more than 1 billion years ago: trace fossil evidence from india

    PubMed

    Seilacher; Bose; Pfluger

    1998-10-01

    Some intriguing bedding plane features that were observed in the Mesoproterozoic Chorhat Sandstone are biological and can be interpreted as the burrows of wormlike undermat miners (that is, infaunal animals that excavated tunnels underneath microbial mats). These burrows suggest that triploblastic animals existed more than a billion years ago. They also suggest that the diversification of animal designs proceeded very slowly before the appearance of organisms with hard skeletons, which was probably the key event in the Cambrian evolutionary explosion, and before the ecological changes that accompanied that event. PMID:9756480

  3. Nanobubble collapse on a silica surface in water: billion-atom reactive molecular dynamics simulations.

    PubMed

    Shekhar, Adarsh; Nomura, Ken-ichi; Kalia, Rajiv K; Nakano, Aiichiro; Vashishta, Priya

    2013-11-01

    Cavitation bubbles occur in fluids subjected to rapid changes in pressure. We use billion-atom reactive molecular dynamics simulations on a 163,840-processor BlueGene/P supercomputer to investigate damage caused by shock-induced collapse of nanobubbles in water near an amorphous silica surface. Collapse of an empty bubble generates a high-speed nanojet, which causes pitting on the silica surface. We find pit radii are close to bubble radii, and experiments also indicate linear scaling between them. The gas-filled bubbles undergo partial collapse and, consequently, the damage on the silica surface is mitigated. PMID:24237524

  4. The First Billion Years: The Growth of Galaxies in the Reionization Epoch

    NASA Astrophysics Data System (ADS)

    Illingworth, Garth

    2015-08-01

    Detection and measurement of the earliest galaxies in the first billion years only became possible after the Hubble Space Telescope was updated in 2009 with the infrared WFC3/IR camera during Shuttle servicing mission SM4. The first billion years is a fascinating epoch, not just because of the earliest galaxies known from about 450 Myr after the Big Bang, but also because it encompasses the reionization epoch that peaked around z~9, as Planck has recently shown, and ended around redshift z~6 at 900 Myr. Before 2009 just a handful of galaxies were known in the reionization epoch at z>6. But within the last 5 years, with the first HUDF09 survey, the HUDF12, CANDELS and numerous other surveys on the GOODS and CANDELS fields, as well as detections from the cluster lensing programs like CLASH and the Frontier Fields, the number of galaxies at redshifts 7-10 has exploded, with some 700 galaxies being found and characterized. The first billion years was a period of extraordinary growth in the galaxy population with rapid growth in the star formation rate density and global mass density in galaxies. Spitzer observations in the infrared of these Hubble fields are establishing masses as well as giving insights into the nature and timescales of star formation from the very powerful emission lines being revealed by the Spitzer IRAC data. I will discuss what we understand about the growth of galaxies in this epoch from the insights gained from remarkable deep fields like the XDF, as well as the wide-area GOODS/CANDELS fields, the detection of unexpectedly luminous galaxies at redshifts 8-10, the impact of early galaxies on reionization, confirmation of a number of galaxies at z~7-8 from ground-based spectroscopic measurements, and the indications of a change in the growth of the star formation rate around 500 Myr. The first billion years was a time of dramatic growth and change in the early galaxy population.

  5. Nanobubble Collapse on a Silica Surface in Water: Billion-Atom Reactive Molecular Dynamics Simulations

    NASA Astrophysics Data System (ADS)

    Shekhar, Adarsh; Nomura, Ken-ichi; Kalia, Rajiv K.; Nakano, Aiichiro; Vashishta, Priya

    2013-11-01

    Cavitation bubbles occur in fluids subjected to rapid changes in pressure. We use billion-atom reactive molecular dynamics simulations on a 163 840-processor BlueGene/P supercomputer to investigate damage caused by shock-induced collapse of nanobubbles in water near an amorphous silica surface. Collapse of an empty bubble generates a high-speed nanojet, which causes pitting on the silica surface. We find pit radii are close to bubble radii, and experiments also indicate linear scaling between them. The gas-filled bubbles undergo partial collapse and, consequently, the damage on the silica surface is mitigated.

  6. Electron microscopy reveals unique microfossil preservation in 1 billion-year-old lakes

    NASA Astrophysics Data System (ADS)

    Saunders, M.; Kong, C.; Menon, S.; Wacey, D.

    2014-06-01

    Electron microscopy was applied to the study of 1 billion-year-old microfossils from northwest Scotland in order to investigate their 3D morphology and mode of fossilization. 3D-FIB-SEM revealed high quality preservation of organic cell walls with only minor amounts of post-mortem decomposition, followed by variable degrees of morphological alteration (folding and compression of cell walls) during sediment compaction. EFTEM mapping plus SAED revealed a diverse fossilizing mineral assemblage including K-rich clay, Fe-Mg-rich clay and calcium phosphate, with each mineral occupying specific microenvironments in proximity to carbonaceous microfossil cell walls.

  7. The $1. 5 billion question: Can the US Global Change Research Program deliver on its promises

    SciTech Connect

    Monastersky, R.

    1993-09-04

    President Clinton has continued the funding for scientific investigations of global climatic change, increasing funds to a total of $1.5 billion spread amoung 11 different agencies. However, a growing number of critics warn that the program appears heading toward failure. The main issue is relevancy. Almost every agrees that the research effort will support important scientific work over the next decade, but it will not necessarily provide the information policymakers need to address the threat of climatic change, ozone depletion, deforestation, desertification, and similiar issues. This article summarizes the concerns and comments of critics, and the gap between the climate scientists and governmental policymakers.

  8. Managing the wetlands. People and rivers: Africa.

    PubMed

    Dugan, P

    1993-01-01

    At the current population growth rate in Africa, the population will reach 1 billion by 2010. Water is needed to sustain these people, yet rainfall in Africa is erratic. Africans are already confronting a shortage of freshwater. Agriculture supports 66% of the population of sub-Saharan Africa. Sound agricultural development is needed to curb rural-urban migration, but a constant supply of freshwater is essential. Major rivers (the Limpopo in southern Africa and the Save/Sabi in Zimbabwe and Mozambique) now flow only seasonally. The flows of the Chari-Logona, the Nile, and the Zambezi are falling. Continual mismanagement of Africa's river basins coupled with current projections of global climate change will expand desiccation. All but the White Nile and the Zaire rivers flood seasonally every year, thereby expanding Africa's wetlands. Wetlands have been targeted for development projects (e.g., hydroelectric projects and large dams), largely to meet urban-industrial demands. Development planners tend to ignore the economic value of the wetlands. For example, the Niger Inland Delta sustains 550,000 people, 1 million cattle, and 1 million sheep. Wetlands replenish ground water and serve as natural irrigation. River basin planning often results in environmentally disastrous schemes which do not understand local management practices. Hydrologists, engineers, geologists, and economics design these schemes, but sociologists, anthropologists, and development experts should be included. The unfinished Jonglei Canal in southern Sudan would have adversely affected 400,000 pastoralists. The Volta River Authority's Akosombo Dam displaced 84,000 people and flooded the most productive agricultural land in Ghana. A sustainable future in Africa depends on understanding the interactions of human uses and the ways in which they relate to the natural variations in river flow. The IUCN Wetlands Programme, based on the principles of the World Conservation Strategy, is working with

  9. Deprescribing in older people.

    PubMed

    Page, Amy Theresa; Potter, Kathleen; Clifford, Rhonda; Etherton-Beer, Christopher

    2016-09-01

    Older people with chronic disease have great potential to benefit from their medications but are also at high risk of harm from their medications. The use of medications is particularly important for symptom control and disease progression in older people. Under-treatment means older people can miss out on the potential benefits of useful medications, while over-treatment (polypharmacy) puts them at increased risk of harm. Deprescribing attempts to balance the potential for benefit and harm by systematically withdrawing inappropriate medications with the goal of managing polypharmacy and improving outcomes. The evidence base for deprescribing in older people is growing. Studies to reduce polypharmacy have used a range of methods. Most evidence for deprescribing relates to the withdrawal of specific medications, and evidence supports attempts to deprescribe potentially inappropriate medicines (such as long-term benzodiazepines). There is also evidence that polypharmacy can be reduced by withdrawing specific medications using individualised interventions. More work is needed to identify the sub-groups of older people who may most benefit from deprescribing and the best approaches to undertaking the deprescribing interventions. PMID:27451330

  10. States' Spending on Colleges Rises 19 Pct. in 2 Years, Nears $31-Billion for'85-86.

    ERIC Educational Resources Information Center

    Evangelauf, Jean

    1985-01-01

    The U.S. states' expenditures to nearly $31 billion in tax money mark a continuing recovery in support for higher education. Shaping this year's appropriations levels were concerns about tuition and efforts to promote economic development. (MLW)

  11. 77 FR 15052 - Dataset Workshop-U.S. Billion Dollar Disasters Dataset (1980-2011): Assessing Dataset Strengths...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2012-03-14

    ... Disasters (1980-2011) dataset and associated methods used to develop the data set. An important goal of the... data set addresses; What steps should be taken to enhance the robustness of the billion-dollar...

  12. People and the Earth

    NASA Astrophysics Data System (ADS)

    Rogers, John James William; Feiss, P. Geoffrey

    1998-03-01

    People and the Earth examines the numerous ways in which this planet enhances and limits our lifestyles. Written with wit and remarkable insight, and illustrated with numerous case histories, it provides a balanced view of the complex environmental issues facing our civilization. The authors look at the geologic restrictions on our ability to withdraw resources--food, water, energy, and minerals--from the earth, the effect human activity has on the earth, and the lingering damage caused by natural disasters. People and the Earth examines the basic components of our interaction with this planet, provides a lucid, scientific discussion of each issue, and speculates on what the future may hold. It provides the fundamental concepts that will enable us to make wise and conscientious choices on how to live our day-to-day lives. People and the Earth is an ideal introductory textbook and will also appeal to anyone concerned with our evolving relationship to the earth.

  13. Healthy pets, healthy people.

    PubMed

    Wong, S K; Feinstein, L H; Heidmann, P

    1999-08-01

    Zoonoses, diseases that can be transmitted from animals to humans, can pose serious health risks to immunocompromised people. Although pets can carry zoonoses, owning and caring for animals can benefit human health. Information exists about preventing transmission of zoonoses, but not all physicians and veterinarians provide adequate and accurate information to immunocompromised pet owners. This disease prevention/health promotion project provides physicians and veterinarians with information, created specifically to share with patients and clients, about the health risks and benefits of pet ownership. Further, "Healthy Pets, Healthy People" encourages communication between veterinarians, physicians, clients, and patients and can serve as a model program for a nation-wide effort to aid health professionals in making recommendations about pet ownership for immunocompromised people. PMID:10434969

  14. Method for preparation of 7-hydroxy-1,2,3,4-tetrahydroquinoline from 1,2,3,4-tetrahydroquinoline

    DOEpatents

    Field, George; Hammond, Peter R.

    1994-01-01

    Methods for the efficient preparation of 7-hydroxy-1,2,3,4-tetrahydroquinoline include a first method in which the acylation of m-aminophenol obtains a lactam which is reduced to give the desired quinoline and a second method in which tetrahydroquinoline is nitrated and hydrogenated and then hydrolyzed to obtain the desire quinoline. 7-hydroxy-1,2,3,4-tetrahydroquinoline is used in the efficient synthesis of four lasing dyes of the rhodamine class.

  15. Method for preparation of 7-hydroxy-1,2,3,4-tetrahydroquinoline from 1,2,3,4-tetrahydroquinoline

    DOEpatents

    Field, G.; Hammond, P.R.

    1994-02-01

    Methods for the efficient preparation of 7-hydroxy-1,2,3,4-tetrahydroquinoline include a first method in which the acylation of m-aminophenol obtains a lactam which is reduced to give the desired quinoline and a second method in which tetrahydroquinoline is nitrated and hydrogenated and then hydrolyzed to obtain the desire quinoline. 7-hydroxy-1,2,3,4-tetrahydroquinoline is used in the efficient synthesis of four lasing dyes of the rhodamine class.

  16. On the constancy of the lunar cratering flux over the past 3.3 billion yr

    NASA Technical Reports Server (NTRS)

    Guinness, E. A.; Arvidson, R. E.

    1977-01-01

    Utilizing a method that minimizes random fluctuations in sampling crater populations, it can be shown that the ejecta deposit of Tycho, the floor of Copernicus, and the region surrounding the Apollo 12 landing site have incremental crater size-frequency distributions that can be expressed as log-log linear functions over the diameter range from 0.1 to 1 km. Slopes are indistinguishable for the three populations, probably indicating that the surfaces are dominated by primary craters. Treating the crater populations of Tycho, the floor of Copernicus, and Apollo 12 as primary crater populations contaminated, but not overwhelmed, with secondaries, allows an attempt at calibration of the post-heavy bombardment cratering flux. Using the age of Tycho as 109 m.y., Copernicus as 800 m.y., and Apollo 12 as 3.26 billion yr, there is no basis for assuming that the flux has changed over the past 3.3 billion yr. This result can be used for dating intermediate aged surfaces by crater density.

  17. A solar origin for the large lunar magnetic field at 4.0 billion yr ago

    NASA Technical Reports Server (NTRS)

    Banerjee, S. K.; Mellema, J. P.

    1976-01-01

    A new method (Shaw, 1974) for paleointensity determination has been applied to three subsamples of one polymict breccia, 72215 (of age 4.0 billion yr) to yield an average paleointensity of 0.41 Oe at the Taurus-Littrow region of the moon around the time of breccia formation. Of the present models for lunar magnetism, only the Sonett and Runcorn (1974) model of a central iron core dynamo can explain the presence of such a large field in early lunar history. However, because of the similarity in size of this field and that for the early solar system deduced from carbonaceous chondrites, we draw attention to an apparently little-considered possibility: that the large magnetic field in early lunar history was external and solar in origin, and emanated from a pre-main sequence T-Tauri stage sun. Therefore, there should be no record of such a large magnetic field in lunar rocks younger than approximately 4.0 billion yr.

  18. The evolution in the stellar mass of brightest cluster galaxies over the past 10 billion years

    NASA Astrophysics Data System (ADS)

    Bellstedt, Sabine; Lidman, Chris; Muzzin, Adam; Franx, Marijn; Guatelli, Susanna; Hill, Allison R.; Hoekstra, Henk; Kurinsky, Noah; Labbe, Ivo; Marchesini, Danilo; Marsan, Z. Cemile; Safavi-Naeini, Mitra; Sifón, Cristóbal; Stefanon, Mauro; van de Sande, Jesse; van Dokkum, Pieter; Weigel, Catherine

    2016-08-01

    Using a sample of 98 galaxy clusters recently imaged in the near-infrared with the European Southern Observatory (ESO) New Technology Telescope, WIYN telescope and William Herschel Telescope, supplemented with 33 clusters from the ESO archive, we measure how the stellar mass of the most massive galaxies in the universe, namely brightest cluster galaxies (BCGs), increases with time. Most of the BCGs in this new sample lie in the redshift range 0.2 < z < 0.6, which has been noted in recent works to mark an epoch over which the growth in the stellar mass of BCGs stalls. From this sample of 132 clusters, we create a subsample of 102 systems that includes only those clusters that have estimates of the cluster mass. We combine the BCGs in this subsample with BCGs from the literature, and find that the growth in stellar mass of BCGs from 10 billion years ago to the present epoch is broadly consistent with recent semi-analytic and semi-empirical models. As in other recent studies, tentative evidence indicates that the stellar mass growth rate of BCGs may be slowing in the past 3.5 billion years. Further work in collecting larger samples, and in better comparing observations with theory using mock images, is required if a more detailed comparison between the models and the data is to be made.

  19. The evolution in the stellar mass of brightest cluster galaxies over the past 10 billion years

    NASA Astrophysics Data System (ADS)

    Bellstedt, Sabine; Lidman, Chris; Muzzin, Adam; Franx, Marijn; Guatelli, Susanna; Hill, Allison R.; Hoekstra, Henk; Kurinsky, Noah; Labbe, Ivo; Marchesini, Danilo; Marsan, Z. Cemile; Safavi-Naeini, Mitra; Sifón, Cristóbal; Stefanon, Mauro; van de Sande, Jesse; van Dokkum, Pieter; Weigel, Catherine

    2016-08-01

    Using a sample of 98 galaxy clusters recently imaged in the near infra-red with the ESO NTT, WIYN and WHT telescopes, supplemented with 33 clusters from the ESO archive, we measure how the stellar mass of the most massive galaxies in the universe, namely Brightest Cluster Galaxies (BCG), increases with time. Most of the BCGs in this new sample lie in the redshift range $0.2billion years ago to the present epoch is broadly consistent with recent semi-analytic and semi-empirical models. As in other recent studies, tentative evidence indicates that the stellar mass growth rate of BCGs may be slowing in the past 3.5 billion years. Further work in collecting larger samples, and in better comparing observations with theory using mock images is required if a more detailed comparison between the models and the data is to be made.

  20. Parametrization and Classification of 20 Billion LSST Objects: Lessons from SDSS

    SciTech Connect

    Ivezic, Z.; Axelrod, T.; Becker, A.C.; Becla, J.; Borne, K.; Burke, David L.; Claver, C.F.; Cook, K.H.; Connolly, A.; Gilmore, D.K.; Jones, R.L.; Juric, M.; Kahn, Steven M.; Lim, K-T.; Lupton, R.H.; Monet, D.G.; Pinto, P.A.; Sesar, B.; Stubbs, Christopher W.; Tyson, J.Anthony; /UC, Davis

    2011-11-10

    The Large Synoptic Survey Telescope (LSST) will be a large, wide-field ground-based system designed to obtain, starting in 2015, multiple images of the sky that is visible from Cerro Pachon in Northern Chile. About 90% of the observing time will be devoted to a deep-wide-fast survey mode which will observe a 20,000 deg{sup 2} region about 1000 times during the anticipated 10 years of operations (distributed over six bands, ugrizy). Each 30-second long visit will deliver 5{sigma} depth for point sources of r {approx} 24.5 on average. The co-added map will be about 3 magnitudes deeper, and will include 10 billion galaxies and a similar number of stars. We discuss various measurements that will be automatically performed for these 20 billion sources, and how they can be used for classification and determination of source physical and other properties. We provide a few classification examples based on SDSS data, such as color classification of stars, color-spatial proximity search for wide-angle binary stars, orbital-color classification of asteroid families, and the recognition of main Galaxy components based on the distribution of stars in the position-metallicity-kinematics space. Guided by these examples, we anticipate that two grand classification challenges for LSST will be (1) rapid and robust classification of sources detected in difference images, and (2) simultaneous treatment of diverse astrometric and photometric time series measurements for an unprecedentedly large number of objects.

  1. The evolution in the stellar mass of Brightest Cluster Galaxies over the past 10 billion years

    NASA Astrophysics Data System (ADS)

    Bellstedt, Sabine; Lidman, Chris; Muzzin, Adam; Franx, Marijn; Guatelli, Susanna; Hill, Allison R.; Hoekstra, Henk; Kurinsky, Noah; Labbe, Ivo; Marchesini, Danilo; Marsan, Z. Cemile; Safavi-Naeini, Mitra; Sifón, Cristóbal; Stefanon, Mauro; van de Sande, Jesse; van Dokkum, Pieter; Weigel, Catherine

    2016-05-01

    Using a sample of 98 galaxy clusters recently imaged in the near infra-red with the ESO NTT, WIYN and WHT telescopes, supplemented with 33 clusters from the ESO archive, we measure how the stellar mass of the most massive galaxies in the universe, namely Brightest Cluster Galaxies (BCG), increases with time. Most of the BCGs in this new sample lie in the redshift range 0.2 < z < 0.6, which has been noted in recent works to mark an epoch over which the growth in the stellar mass of BCGs stalls. From this sample of 132 clusters, we create a subsample of 102 systems that includes only those clusters that have estimates of the cluster mass. We combine the BCGs in this subsample with BCGs from the literature, and find that the growth in stellar mass of BCGs from 10 billion years ago to the present epoch is broadly consistent with recent semi-analytic and semi-empirical models. As in other recent studies, tentative evidence indicates that the stellar mass growth rate of BCGs may be slowing in the past 3.5 billion years. Further work in collecting larger samples, and in better comparing observations with theory using mock images is required if a more detailed comparison between the models and the data is to be made.

  2. Greenhouse gas implications of a 32 billion gallon bioenergy landscape in the US

    NASA Astrophysics Data System (ADS)

    DeLucia, E. H.; Hudiburg, T. W.; Wang, W.; Khanna, M.; Long, S.; Dwivedi, P.; Parton, W. J.; Hartman, M. D.

    2015-12-01

    Sustainable bioenergy for transportation fuel and greenhouse gas (GHGs) reductions may require considerable changes in land use. Perennial grasses have been proposed because of their potential to yield substantial biomass on marginal lands without displacing food and reduce GHG emissions by storing soil carbon. Here, we implemented an integrated approach to planning bioenergy landscapes by combining spatially-explicit ecosystem and economic models to predict a least-cost land allocation for a 32 billion gallon (121 billion liter) renewable fuel mandate in the US. We find that 2022 GHG transportation emissions are decreased by 7% when 3.9 million hectares of eastern US land are converted to perennial grasses supplemented with corn residue to meet cellulosic ethanol requirements, largely because of gasoline displacement and soil carbon storage. If renewable fuel production is accompanied by a cellulosic biofuel tax credit, CO2 equivalent emissions could be reduced by 12%, because it induces more cellulosic biofuel and land under perennial grasses (10 million hectares) than under the mandate alone. While GHG reducing bioenergy landscapes that meet RFS requirements and do not displace food are possible, the reductions in GHG emissions are 50% less compared to previous estimates that did not account for economically feasible land allocation.

  3. As its R D budget nears $2 billion Bayer rethinks priorities

    SciTech Connect

    Rotman, D.

    1993-03-17

    With a planned 1993 research and development budget of roughly DM3.2 billion ($1.95 billion), Bayer (Leverkusen) is the industry's biggest R D spender. But while the German giant lays out a healthy 7% of sales on R D, caution is clearly replacing the heady spending spurts of several years ago. And faced with an increasingly rigorous corporate business restructuring, Bayer - like others in the chemical industry - is rethinking its R D strategies. While Bayer's R D stress is clearly on life sciences, the company remains bullish on certain new materials, particularly inorganics. It has developed several engineering ceramics for use in automotive engines, with the most advanced - a silicon nitride - being road tested in Mercedes models. [open quotes]We have the materials and know their properties,[close quotes] says Hauke Fuerstenwerth, Bayer's head of R D coordination. The challenge now, he says, is to demonstrate a commercially attractive process for large-scale production. Bayer is also pursuing new silicon wafer technology. Already in small-scale production, the firm is testing an amorphous silicon that is intended to be far cheaper than existing crystalline silicon wafers, while maintaining suitable properties for applications such as solar collectors.

  4. Enhanced production of 2,3-butanediol from sugarcane molasses.

    PubMed

    Dai, Jian-Ying; Zhao, Pan; Cheng, Xiao-Long; Xiu, Zhi-Long

    2015-03-01

    2,3-Butanediol has been known as a platform green chemical, and the production cost is the key problem for its large-scale production in which the carbon source occupies a major part. Sugarcane molasses is a by-product of sugar industry and considered as a cheap carbon source for biorefinery. In this paper, the fermentation of 2,3-butanediol with sugarcane molasses was studied by reducing the medium ingredients and operation steps. The fermentation medium was optimized by response surface methodology, and 2,3-butanediol production was explored under the deficiency of sterilization, molasses acidification, and organic nitrogen source. Based on these experiments, the fermentation medium with sugarcane molasses as carbon source was simplified to five ingredients, and the steps of molasses acidification and medium sterilization were reduced; thus, the cost was reduced and the production of 2,3-butanediol was enhanced. Under fed-batch fermentation, 99.5 g/L of 2,3-butanediol and acetoin was obtained at 60 h with a yield of 0.39 g/g sugar. PMID:25586489

  5. Drugs and Young People

    MedlinePlus

    Drug abuse is a serious public health problem. It affects almost every community and family in some way. Drug abuse in children and teenagers may pose a ... of young people may be more susceptible to drug abuse and addiction than adult brains. Abused drugs ...

  6. Researching Marginalised Young People

    ERIC Educational Resources Information Center

    Russell, Lisa

    2013-01-01

    Young people not in employment, education or training (NEET) are not a static, homogenous group. For most, being NEET is a temporary state as they move between different forms of participation and non-participation. This paper explores how the complexities of defining NEET, the re-structuring of the careers service and the nature of post-16…

  7. Parasites, Plants, and People.

    PubMed

    Johnson, Marion; Moore, Tony

    2016-06-01

    Anthelminthic resistance is acknowledged worldwide and is a major problem in Aotearoa New Zealand, thus alternative parasite management strategies are imperative. One Health is an initiative linking animal, human, and environmental health. Parasites, plants, and people illustrate the possibilities of providing diverse diets for stock thereby lowering parasite burdens, improving the cultural wellbeing of a local community, and protecting the environment. PMID:27105933

  8. Early Indian People.

    ERIC Educational Resources Information Center

    Doermann, Elisabeth

    1979-01-01

    Using bits and pieces of the past such as charred bits of wood from campfires, broken pieces of clay pots, stone spearpoints and arrowheads, and shell or copper ornaments, the archaeologist tries to put together the story of early Indian people in the Minnesota region. A short story, one of eight articles, re-creates the kill of an Itasca bison…

  9. Esperanto and Older People.

    ERIC Educational Resources Information Center

    Gal, Ilona

    1978-01-01

    Research has indicated that the elderly retain the ability to learn, and specifically to learn new languages. Furthermore, the increasingly greater proportion of old people in the population demands that their need for continued intellectual stimulation be met. In the absence of explicit motives for learning an ethnic language, Esperanto is a good…

  10. People's Theatre in Amerika.

    ERIC Educational Resources Information Center

    Taylor, Karen Malpede

    A history of the people's theatre movement in this country from the early 1920s to the early 1970s, this book deals with the structural and thematic connections between the radical theatre of the twenties and thirties and current work of such revolutionary theatres as the Living Theatre, Open Theatre, Bread and Puppet Theatre, El Teatro Campesino,…

  11. Healthy People 2010

    NASA Technical Reports Server (NTRS)

    Angotti, Catherine M.

    2001-01-01

    Major Healthy People (HP) 2000 goals closely tied to prevention were not met nationally: physical activity did not improve; evidence that it actually decreased; obesity did not decrease but instead increased in all groups, actually doubling in children; and incidence of type 2 diabetes did not decrease, but instead evidence showed that it increased in all age groups.

  12. People of the Appalachians.

    ERIC Educational Resources Information Center

    Adams, George; And Others

    Suitable for use in middle school classes, this interdisciplinary resource book on the culture of Appalachia is divided into 15 units. Topics covered are: stereotyping, values, geography, coal, people, family, housing, biographies, literature, music, crafts, dance, religion, wisdom, and change. Through a variety of learning activities and…

  13. Leading clever people.

    PubMed

    Goffee, Rob; Jones, Gareth

    2007-03-01

    In an economy driven by ideas and intellectual know-how, top executives recognize the importance of employing smart, highly creative people. But if clever people have one defining characteristic, it's that they do not want to be led. So what is a leader to do? The authors conducted more than 100 interviews with leaders and their clever people at major organizations such as PricewaterhouseCoopers, Cisco Systems, Novartis, the BBC, and Roche. What they learned is that the psychological relationships effective leaders have with their clever people are very different from the ones they have with traditional followers. Those relationships can be shaped by seven characteristics that clever people share: They know their worth--and they know you have to employ them if you want their tacit skills. They are organizationally savvy and will seek the company context in which their interests are most generously funded. They ignore corporate hierarchy; although intellectual status is important to them, you can't lure them with promotions. They expect instant access to top management, and if they don't get it, they may think the organization doesn't take their work seriously. They are plugged into highly developed knowledge networks, which both increases their value and makes them more of a flight risk. They have a low boredom threshold, so you have to keep them challenged and committed. They won't thank you--even when you're leading them well. The trick is to act like a benevolent guardian: to grant them the respect and recognition they demand, protect them from organizational rules and politics, and give them room to pursue private efforts and even to fail. The payoff will be a flourishing crop of creative minds that will enrich your whole organization. PMID:17348171

  14. Oral health for older people.

    PubMed

    2016-08-01

    Compared with previous generations, more older people have retained some or all of their teeth, but more than 40% of community-dwelling older people aged 75 and over have unmet oral health needs. However, the importance of oral health can be undervalued by healthcare professionals and older people. Three studies relating to oral health for older people are summarised. PMID:27573957

  15. New 2-aryl-1,2,3,4-tetrahydropyrido[2,3-d]pyrimidin-4-one derivatives as diuretics.

    PubMed

    Monge, A; Martinez-Merino, V; Simon, M A; Sanmartin, C

    1993-12-01

    2-Aryl-1,2,3,4-tetrahydropyrido[2,3-d]pyrimidin-4-one derivatives having various substituents at the 4'-position, H or methyl at 1,3-positions and nitro or amino at 6-position were prepared and tested for their diuretic, natriuretic and kaliuretic activities on male Wistar rats at a dosage of 25 mg/kg or less. 2-(3-Pyridyl) derivatives were inactive. 1,3-Dimethyl-6-nitro-2-phenyl derivatives (1) were active depending on the electronic character of the 4'-substituent but at the same time were sodium-sparing. However, 1(H),3(H)-6-nitro-2-phenyl derivatives (2) were generally inactive as diuretics but active as potassium-sparing drugs. 6-Amino-1(H),3(H)-2-phenyl derivatives (4) were active as diuretics depending on dipolar moment of the substituent at the 4'-position, and induced moderate potassium release. The 6-amino-2-(4-trifluoromethylphenyl)-1, 2,3,4-tetrahydropyrido [2,3-d]pyrimidin-4-one (4f) remained active up to a dosage of 3 mg/kg. The structure-activity relationships were carried out in light of the adaptative least squares (ALS) method and discriminant functions for diuretic compounds were established. PMID:8141821

  16. LOTUS 1-2-3 Macros for Library Applications.

    ERIC Educational Resources Information Center

    Howden, Norman

    1987-01-01

    Describes LOTUS 1-2-3, an advanced spreadsheet with database and text manipulation functions that can be used with microcomputers by librarians to provide customized calculation and data acquisition tools. Macro commands and the menu system are discussed, and an example is given of an invoice procedure. (Author/LRW)

  17. Accident sequence precursor analysis level 2/3 model development

    SciTech Connect

    Lui, C.H.; Galyean, W.J.; Brownson, D.A.

    1997-02-01

    The US Nuclear Regulatory Commission`s Accident Sequence Precursor (ASP) program currently uses simple Level 1 models to assess the conditional core damage probability for operational events occurring in commercial nuclear power plants (NPP). Since not all accident sequences leading to core damage will result in the same radiological consequences, it is necessary to develop simple Level 2/3 models that can be used to analyze the response of the NPP containment structure in the context of a core damage accident, estimate the magnitude of the resulting radioactive releases to the environment, and calculate the consequences associated with these releases. The simple Level 2/3 model development work was initiated in 1995, and several prototype models have been completed. Once developed, these simple Level 2/3 models are linked to the simple Level 1 models to provide risk perspectives for operational events. This paper describes the methods implemented for the development of these simple Level 2/3 ASP models, and the linkage process to the existing Level 1 models.

  18. 43 CFR 3453.2-3 - Filing location and fee.

    Code of Federal Regulations, 2012 CFR

    2012-10-01

    ... leased lands proposed for transfer (see 43 CFR subpart 1821). Each instrument of transfer shall be accompanied by a nonrefundable filing fee (see 43 CFR 3473.2). ... 43 Public Lands: Interior 2 2012-10-01 2012-10-01 false Filing location and fee. 3453.2-3...

  19. 43 CFR 3453.2-3 - Filing location and fee.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ... leased lands proposed for transfer (see 43 CFR subpart 1821). Each instrument of transfer shall be accompanied by a nonrefundable filing fee (see 43 CFR 3473.2). ... 43 Public Lands: Interior 2 2013-10-01 2013-10-01 false Filing location and fee. 3453.2-3...

  20. 43 CFR 3453.2-3 - Filing location and fee.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ... leased lands proposed for transfer (see 43 CFR subpart 1821). Each instrument of transfer shall be accompanied by a nonrefundable filing fee (see 43 CFR 3473.2). ... 43 Public Lands: Interior 2 2014-10-01 2014-10-01 false Filing location and fee. 3453.2-3...

  1. 2,3,7,8-Tetrachlorodibenzo-p-dioxin

    Integrated Risk Information System (IRIS)

    2,3,7,8 - Tetrachlorodibenzo - p - dioxin ( TCDD ) ; CASRN 1746 - 01 - 6 This document has been provided for review to EPA scientists , interagency reviewers from other federal agencies and White House offices , and the public , and peer reviewed by independent scientists external to EPA . Sections

  2. Graphing Online Searches with Lotus 1-2-3.

    ERIC Educational Resources Information Center

    Persson, Olle

    1986-01-01

    This article illustrates how Lotus 1-2-3 software can be used to create graphs using downloaded online searches as raw material, notes most commands applied, and outlines three required steps: downloading, importing the downloading file into the worksheet, and making graphs. An example in bibliometrics and sample graphs are included. (EJS)

  3. Welcome to Lotus 1-2-3. Learning Activity Packets.

    ERIC Educational Resources Information Center

    Mills, Steven; And Others

    This learning activity packet (LAP) contains 11 self-paced study lessons that allow students to proceed along a 36-hour course of study for Lotus 1-2-3 at their own pace. The lessons are organized in the following way: objectives, completion and performance standards, a list of required materials, unit test, and exercises (applications of the…

  4. Substrate Oxidation by Indoleamine 2,3-Dioxygenase

    PubMed Central

    Booth, Elizabeth S.; Basran, Jaswir; Lee, Michael; Handa, Sandeep; Raven, Emma L.

    2015-01-01

    The kynurenine pathway is the major route of l-tryptophan (l-Trp) catabolism in biology, leading ultimately to the formation of NAD+. The initial and rate-limiting step of the kynurenine pathway involves oxidation of l-Trp to N-formylkynurenine. This is an O2-dependent process and catalyzed by indoleamine 2,3-dioxygenase and tryptophan 2,3-dioxygenase. More than 60 years after these dioxygenase enzymes were first isolated (Kotake, Y., and Masayama, I. (1936) Z. Physiol. Chem. 243, 237–244), the mechanism of the reaction is not established. We examined the mechanism of substrate oxidation for a series of substituted tryptophan analogues by indoleamine 2,3-dioxygenase. We observed formation of a transient intermediate, assigned as a Compound II (ferryl) species, during oxidation of l-Trp, 1-methyl-l-Trp, and a number of other substrate analogues. The data are consistent with a common reaction mechanism for indoleamine 2,3-dioxygenase-catalyzed oxidation of tryptophan and other tryptophan analogues. PMID:26511316

  5. 40 CFR 35.909 - Step 2+3 grants.

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... ASSISTANCE Grants for Construction of Treatment Works-Clean Water Act § 35.909 Step 2+3 grants. (a) Authority... design (step 2) and construction (step 3) of a waste water treatment works. (b) Limitations. The Regional... Water and Waste Management finds to have unusually high costs of construction, the...

  6. 40 CFR 35.909 - Step 2+3 grants.

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... ASSISTANCE Grants for Construction of Treatment Works-Clean Water Act § 35.909 Step 2+3 grants. (a) Authority... design (step 2) and construction (step 3) of a waste water treatment works. (b) Limitations. The Regional... Water and Waste Management finds to have unusually high costs of construction, the...

  7. 40 CFR 35.909 - Step 2+3 grants.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... ASSISTANCE Grants for Construction of Treatment Works-Clean Water Act § 35.909 Step 2+3 grants. (a) Authority... design (step 2) and construction (step 3) of a waste water treatment works. (b) Limitations. The Regional... Water and Waste Management finds to have unusually high costs of construction, the...

  8. 40 CFR 35.909 - Step 2+3 grants.

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... ASSISTANCE Grants for Construction of Treatment Works-Clean Water Act § 35.909 Step 2+3 grants. (a) Authority... design (step 2) and construction (step 3) of a waste water treatment works. (b) Limitations. The Regional... Water and Waste Management finds to have unusually high costs of construction, the...

  9. Indeno[1,2,3-cd]pyrene

    Integrated Risk Information System (IRIS)

    Indeno [ 1,2,3 - cd ] pyrene ; CASRN 193 - 39 - 5 Human health assessment information on a chemical substance is included in the IRIS database only after a comprehensive review of toxicity data , as outlined in the IRIS assessment development process . Sections I ( Health Hazard Assessments for Nonc

  10. Midbrain dopamine D2/3 receptor binding in schizophrenia.

    PubMed

    Tuppurainen, Heli; Kuikka, Jyrki T; Laakso, Mikko P; Viinamäki, Heimo; Husso, Minna; Tiihonen, Jari

    2006-09-01

    Several studies suggest that dysregulation of dopaminergic transmission in the midbrain and thalamus may contribute to the symptomatology of schizophrenia. The objective of this study was to examine the putative alteration of dopamine D(2/3 )receptor densities in the thalamus and midbrain of drug-naïve schizophrenic patients. We used the high-affinity single-photon emission tomography ligand [(123)I]epidepride for imaging D(2/3 )receptor binding sites in six neuroleptic-naïve schizophrenic patients, and seven healthy controls. Schizophrenic symptoms were evaluated by the Positive and Negative Syndrome Scale. Significantly lower D(2/3 )values were observed in the midbrain of patients with schizophrenia compared to controls (P = 0.02). No statistically significant difference was observed in the thalamus between two groups. Negative correlations were found between thalamic D(2/3 )receptor binding and general psychopathological schizophrenic symptoms (r from -0.78 to -0.92). These observations implicate altered dopaminergic activity in the midbrain of schizophrenic patients. PMID:16783502

  11. Anxiety Self Report (ASR (1,2,3,4,). X

    ERIC Educational Resources Information Center

    Parsons, Jane S.

    The Anxiety Self Report (ASR 1,2,3,4) is provided, followed by information about the report. The ASR is discussed as to its development, description, response bias, scoring procedures, reliability, stability, validity, and correlation between the ASR and the Manifest Anxiety Scale. (For related documents, see TM 002 928, 929.) (DB)

  12. Structural basis of the impact sensitivities of 1-picryl-1,2,3-triazole, 2-picryl-1,2,3-triazole, 4-nitro-1-picryl-1,2,3-triazole, and 4-nitro-2-picryl-1,2,3-triazole

    SciTech Connect

    Storm, C.B.; Ryan, R.R.; Ritchie, J.P.; Hall, J.H.; Bachrach, S.M. )

    1989-01-26

    The isomeric pairs 1-picryl-1,2,3-triazole, 2-picryl-1,2,3-triazole and 4-nitro-1-picryl-1,2,3-triazole, 4-nitro-1-picryl-1,2,3-triazole differ dramatically in their impact sensitivity. Since these pairs of compounds have identical oxygen balance this strongly suggests that there is a difference in the decomposition mechanism. The authors report here the x-ray crystal structure, molecular orbital calculations, and {sup 13}C and {sup 1}H NMR spectra of the four compounds. The picryl substituents are essentially identical in all four cases. The most significant structural difference in the X-ray structures and in the molecular orbital calculations is a decrease in the N2-N3 bond length, accompanied by a lengthening of the adjacent bonds, in the two 1-picryl isomers relative to the corresponding bond lengths in the 2-picryl isomers. Molecular orbital calculations show that this leads to a low activation energy for the elimination of N{sub 2} from the 1-picryl isomers. They suggest that this initial step then leads to a reactive intermediate and is responsible for the large difference in sensitivity.

  13. 15 CFR Supplement Nos. 2-3 to Part... - [Reserved

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... 15 Commerce and Foreign Trade 2 2010-01-01 2010-01-01 false Nos. Supplement Nos. 2-3 to Part 716 Commerce and Foreign Trade Regulations Relating to Commerce and Foreign Trade (Continued) BUREAU OF INDUSTRY AND SECURITY, DEPARTMENT OF COMMERCE CHEMICAL WEAPONS CONVENTION REGULATIONS INITIAL AND...

  14. 42 CFR 2.3 - Purpose and effect.

    Code of Federal Regulations, 2012 CFR

    2012-10-01

    ... individual who has an alcohol or drug problem and who does not seek treatment. (3) Because there is a... ALCOHOL AND DRUG ABUSE PATIENT RECORDS Introduction § 2.3 Purpose and effect. (a) Purpose. Under the... use of alcohol and drug abuse patient records which are maintained in connection with the...

  15. 42 CFR 2.3 - Purpose and effect.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ... individual who has an alcohol or drug problem and who does not seek treatment. (3) Because there is a... ALCOHOL AND DRUG ABUSE PATIENT RECORDS Introduction § 2.3 Purpose and effect. (a) Purpose. Under the... use of alcohol and drug abuse patient records which are maintained in connection with the...

  16. 42 CFR 2.3 - Purpose and effect.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ... individual who has an alcohol or drug problem and who does not seek treatment. (3) Because there is a... ALCOHOL AND DRUG ABUSE PATIENT RECORDS Introduction § 2.3 Purpose and effect. (a) Purpose. Under the... use of alcohol and drug abuse patient records which are maintained in connection with the...

  17. LS DAM 2.2.3 released —

    Cancer.gov

    Version 2.2.3 of the Life Sciences Domain Analysis Model (LS DAM) has been released. The LS DAM is a shared view of the semantics for life sciences which includes hypothesis driven basic and pre-clinical research as well as discovery sciences.

  18. 13. PRATT STREET BULKHEAD: SECTIONS 2, 3, 4, 5, AND ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    13. PRATT STREET BULKHEAD: SECTIONS 2, 3, 4, 5, AND 6, DRAWER 10, PLAN NO. 1, 1 IN. = 15 FT. AND 1/2 IN. = 1 FT., APRIL 25, 1906, DRAWING SHOWS DESIGN FOR PRATT STREET BULKHEAD BETWEEN PIERS - Baltimore Inner Harbor, Pier 5, South of Pratt Street between Market Place & Concord Street, Baltimore, Independent City, MD

  19. Star Formation in Galaxy Clusters Over the Past 10 Billion Years

    NASA Astrophysics Data System (ADS)

    Tran, Kim-Vy

    2012-01-01

    Galaxy clusters are the largest gravitationally bound systems in the universe and include the most massive galaxies in the universe; this makes galaxy clusters ideal laboratories for disentangling the nature versus nurture aspect of how galaxies evolve. Understanding how galaxies form and evolve in clusters continues to be a fundamental question in astronomy. The ages and assembly histories of galaxies in rich clusters test both stellar population models and hierarchical formation scenarios. Is star formation in cluster galaxies simply accelerated relative to their counterparts in the lower density field, or do cluster galaxies assemble their stars in a fundamentally different manner? To answer this question, I review multi-wavelength results on star formation in galaxy clusters from Coma to the most distant clusters yet discovered at look-back times of 10 billion years (z 2).

  20. Billion-atom synchronous parallel kinetic Monte Carlo simulations of critical 3D Ising systems

    SciTech Connect

    Martinez, E.; Monasterio, P.R.; Marian, J.

    2011-02-20

    An extension of the synchronous parallel kinetic Monte Carlo (spkMC) algorithm developed by Martinez et al. [J. Comp. Phys. 227 (2008) 3804] to discrete lattices is presented. The method solves the master equation synchronously by recourse to null events that keep all processors' time clocks current in a global sense. Boundary conflicts are resolved by adopting a chessboard decomposition into non-interacting sublattices. We find that the bias introduced by the spatial correlations attendant to the sublattice decomposition is within the standard deviation of serial calculations, which confirms the statistical validity of our algorithm. We have analyzed the parallel efficiency of spkMC and find that it scales consistently with problem size and sublattice partition. We apply the method to the calculation of scale-dependent critical exponents in billion-atom 3D Ising systems, with very good agreement with state-of-the-art multispin simulations.

  1. A change in the geodynamics of continental growth 3 billion years ago.

    PubMed

    Dhuime, Bruno; Hawkesworth, Chris J; Cawood, Peter A; Storey, Craig D

    2012-03-16

    Models for the growth of continental crust rely on knowing the balance between the generation of new crust and the reworking of old crust throughout Earth's history. The oxygen isotopic composition of zircons, for which uranium-lead and hafnium isotopic data provide age constraints, is a key archive of crustal reworking. We identified systematic variations in hafnium and oxygen isotopes in zircons of different ages that reveal the relative proportions of reworked crust and of new crust through time. Growth of continental crust appears to have been a continuous process, albeit at variable rates. A marked decrease in the rate of crustal growth at ~3 billion years ago may be linked to the onset of subduction-driven plate tectonics. PMID:22422979

  2. Collision-free spatial hash functions for structural analysis of billion-vertex chemical bond networks

    NASA Astrophysics Data System (ADS)

    Zhang, Cheng; Bansal, Bhupesh; Branicio, Paulo S.; Kalia, Rajiv K.; Nakano, Aiichiro; Sharma, Ashish; Vashishta, Priya

    2006-09-01

    State-of-the-art molecular dynamics (MD) simulations generate massive datasets involving billion-vertex chemical bond networks, which makes data mining based on graph algorithms such as K-ring analysis a challenge. This paper proposes an algorithm to improve the efficiency of ring analysis of large graphs, exploiting properties of K-rings and spatial correlations of vertices in the graph. The algorithm uses dual-tree expansion (DTE) and spatial hash-function tagging (SHAFT) to optimize computation and memory access. Numerical tests show nearly perfect linear scaling of the algorithm. Also a parallel implementation of the DTE + SHAFT algorithm achieves high scalability. The algorithm has been successfully employed to analyze large MD simulations involving up to 500 million atoms.

  3. Extraterrestrial demise of banded iron formations 1.85 billion years ago

    USGS Publications Warehouse

    Slack, J.F.; Cannon, W.F.

    2009-01-01

    In the Lake Superior region of North America, deposition of most banded iron formations (BIFs) ended abruptly 1.85 Ga ago, coincident with the oceanic impact of the giant Sudbury extraterrestrial bolide. We propose a new model in which this impact produced global mixing of shallow oxic and deep anoxic waters of the Paleoproterozoic ocean, creating a suboxic redox state for deep seawater. This suboxic state, characterized by only small concentrations of dissolved O2 (???1 ??M), prevented transport of hydrothermally derived Fe(II) from the deep ocean to continental-margin settings, ending an ???1.1 billion-year-long period of episodic BIF mineralization. The model is supported by the nature of Precambrian deep-water exhalative chemical sediments, which changed from predominantly sulfide facies prior to ca. 1.85 Ga to mainly oxide facies thereafter. ?? 2009 Geological Society of America.

  4. Investigation of Radar Propagation in Buildings: A 10 Billion Element Cartesian-Mesh FETD Simulation

    SciTech Connect

    Stowell, M L; Fasenfest, B J; White, D A

    2008-01-14

    In this paper large scale full-wave simulations are performed to investigate radar wave propagation inside buildings. In principle, a radar system combined with sophisticated numerical methods for inverse problems can be used to determine the internal structure of a building. The composition of the walls (cinder block, re-bar) may effect the propagation of the radar waves in a complicated manner. In order to provide a benchmark solution of radar propagation in buildings, including the effects of typical cinder block and re-bar, we performed large scale full wave simulations using a Finite Element Time Domain (FETD) method. This particular FETD implementation is tuned for the special case of an orthogonal Cartesian mesh and hence resembles FDTD in accuracy and efficiency. The method was implemented on a general-purpose massively parallel computer. In this paper we briefly describe the radar propagation problem, the FETD implementation, and we present results of simulations that used over 10 billion elements.

  5. Geodynamo, solar wind, and magnetopause 3.4 to 3.45 billion years ago.

    PubMed

    Tarduno, John A; Cottrell, Rory D; Watkeys, Michael K; Hofmann, Axel; Doubrovine, Pavel V; Mamajek, Eric E; Liu, Dunji; Sibeck, David G; Neukirch, Levi P; Usui, Yoichi

    2010-03-01

    Stellar wind standoff by a planetary magnetic field prevents atmospheric erosion and water loss. Although the early Earth retained its water and atmosphere, and thus evolved as a habitable planet, little is known about Earth's magnetic field strength during that time. We report paleointensity results from single silicate crystals bearing magnetic inclusions that record a geodynamo 3.4 to 3.45 billion years ago. The measured field strength is approximately 50 to 70% that of the present-day field. When combined with a greater Paleoarchean solar wind pressure, the paleofield strength data suggest steady-state magnetopause standoff distances of < or = 5 Earth radii, similar to values observed during recent coronal mass ejection events. The data also suggest lower-latitude aurora and increases in polar cap area, as well as heating, expansion, and volatile loss from the exosphere that would have affected long-term atmospheric composition. PMID:20203044

  6. Atmospheric carbon dioxide: a driver of photosynthetic eukaryote evolution for over a billion years?

    PubMed Central

    Beerling, David J.

    2012-01-01

    Exciting evidence from diverse fields, including physiology, evolutionary biology, palaeontology, geosciences and molecular genetics, is providing an increasingly secure basis for robustly formulating and evaluating hypotheses concerning the role of atmospheric carbon dioxide (CO2) in the evolution of photosynthetic eukaryotes. Such studies span over a billion years of evolutionary change, from the origins of eukaryotic algae through to the evolution of our present-day terrestrial floras, and have relevance for plant and ecosystem responses to future global CO2 increases. The papers in this issue reflect the breadth and depth of approaches being adopted to address this issue. They reveal new discoveries pointing to deep evidence for the role of CO2 in shaping evolutionary changes in plants and ecosystems, and establish an exciting cross-disciplinary research agenda for uncovering new insights into feedbacks between biology and the Earth system. PMID:22232760

  7. Billion-atom synchronous parallel kinetic Monte Carlo simulations of critical 3D Ising systems

    NASA Astrophysics Data System (ADS)

    Martínez, E.; Monasterio, P. R.; Marian, J.

    2011-02-01

    An extension of the synchronous parallel kinetic Monte Carlo (spkMC) algorithm developed by Martinez et al. [J. Comp. Phys. 227 (2008) 3804] to discrete lattices is presented. The method solves the master equation synchronously by recourse to null events that keep all processors' time clocks current in a global sense. Boundary conflicts are resolved by adopting a chessboard decomposition into non-interacting sublattices. We find that the bias introduced by the spatial correlations attendant to the sublattice decomposition is within the standard deviation of serial calculations, which confirms the statistical validity of our algorithm. We have analyzed the parallel efficiency of spkMC and find that it scales consistently with problem size and sublattice partition. We apply the method to the calculation of scale-dependent critical exponents in billion-atom 3D Ising systems, with very good agreement with state-of-the-art multispin simulations.

  8. Barium fluoride whispering-gallery-mode disk-resonator with one billion quality-factor.

    PubMed

    Lin, Guoping; Diallo, Souleymane; Henriet, Rémi; Jacquot, Maxime; Chembo, Yanne K

    2014-10-15

    We demonstrate a monolithic optical whispering-gallery-mode resonator fabricated with barium fluoride (BaF₂) with an ultra-high quality (Q) factor above 10⁹ at 1550 nm, and measured with both the linewidth and cavity-ring-down methods. Vertical scanning optical profilometry shows that the root mean square surface roughness of 2 nm is achieved for our mm-size disk. To the best of our knowledge, we show for the first time that one billion Q-factor is achievable by precision polishing in relatively soft crystals with mohs hardness of 3. We show that complex thermo-optical dynamics can take place in these resonators. Beside usual applications in nonlinear optics and microwave photonics, high-energy particle scintillation detection utilizing monolithic BaF₂ resonators potentially becomes feasible. PMID:25361142

  9. IRON AND {alpha}-ELEMENT PRODUCTION IN THE FIRST ONE BILLION YEARS AFTER THE BIG BANG

    SciTech Connect

    Becker, George D.; Carswell, Robert F.; Sargent, Wallace L. W.; Rauch, Michael E-mail: acalver@ast.cam.ac.uk E-mail: mr@obs.carnegiescience.edu

    2012-01-10

    We present measurements of carbon, oxygen, silicon, and iron in quasar absorption systems existing when the universe was roughly one billion years old. We measure column densities in nine low-ionization systems at 4.7 < z < 6.3 using Keck, Magellan, and Very Large Telescope optical and near-infrared spectra with moderate to high resolution. The column density ratios among C II, O I, Si II, and Fe II are nearly identical to sub-damped Ly{alpha} systems (sub-DLAs) and metal-poor ([M/H] {<=} -1) DLAs at lower redshifts, with no significant evolution over 2 {approx}< z {approx}< 6. The estimated intrinsic scatter in the ratio of any two elements is also small, with a typical rms deviation of {approx}< 0.1 dex. These facts suggest that dust depletion and ionization effects are minimal in our z > 4.7 systems, as in the lower-redshift DLAs, and that the column density ratios are close to the intrinsic relative element abundances. The abundances in our z > 4.7 systems are therefore likely to represent the typical integrated yields from stellar populations within the first gigayear of cosmic history. Due to the time limit imposed by the age of the universe at these redshifts, our measurements thus place direct constraints on the metal production of massive stars, including iron yields of prompt supernovae. The lack of redshift evolution further suggests that the metal inventories of most metal-poor absorption systems at z {approx}> 2 are also dominated by massive stars, with minimal contributions from delayed Type Ia supernovae or winds from asymptotic giant branch stars. The relative abundances in our systems broadly agree with those in very metal-poor, non-carbon-enhanced Galactic halo stars. This is consistent with the picture in which present-day metal-poor stars were potentially formed as early as one billion years after the big bang.

  10. An anoxic, Fe(II)-rich, U-poor ocean 3.46 billion years ago

    NASA Astrophysics Data System (ADS)

    Li, Weiqiang; Czaja, Andrew D.; Van Kranendonk, Martin J.; Beard, Brian L.; Roden, Eric E.; Johnson, Clark M.

    2013-11-01

    The oxidation state of the atmosphere and oceans on the early Earth remains controversial. Although it is accepted by many workers that the Archean atmosphere and ocean were anoxic, hematite in the 3.46 billion-year-old (Ga) Marble Bar Chert (MBC) from Pilbara Craton, NW Australia has figured prominently in arguments that the Paleoarchean atmosphere and ocean was fully oxygenated. In this study, we report the Fe isotope compositions and U concentrations of the MBC, and show that the samples have extreme heavy Fe isotope enrichment, where δ56Fe values range between +1.5‰ and +2.6‰, the highest δ56Fe values for bulk samples yet reported. The high δ56Fe values of the MBC require very low levels of oxidation and, in addition, point to a Paleoarchean ocean that had high aqueous Fe(II) contents. A dispersion/reaction model indicates that O2 contents in the photic zone of the ocean were less than 10-3 μM, which suggests that the ocean was essentially anoxic. An independent test of anoxic conditions is provided by U-Th-Pb isotope systematics, which show that U contents in the Paleoarchean ocean were likely below 0.02 ppb, two orders-of-magnitude lower than the modern ocean. Collectively, the Fe and U data indicate a reduced, Fe(II)-rich, U-poor environment in the Archean oceans at 3.46 billion years ago. Given the evidence for photosynthetic communities provided by broadly coeval stromatolites, these results suggests that an important photosynthetic pathway in the Paleoarchean oceans may have been anoxygenic photosynthetic Fe(II) oxidation.

  11. Searching for Organics Preserved in 4.5 Billion Year Old Salt

    NASA Technical Reports Server (NTRS)

    Zolensky, Michael E.; Fries, M.; Steele, A.; Bodnar, R.

    2012-01-01

    Our understanding of early solar system fluids took a dramatic turn a decade ago with the discovery of fluid inclusion-bearing halite (NaCl) crystals in the matrix of two freshly fallen brecciated H chondrite falls, Monahans and Zag. Both meteorites are regolith breccias, and contain xenolithic halite (and minor admixed sylvite -- KCl, crystals in their regolith lithologies. The halites are purple to dark blue, due to the presence of color centers (electrons in anion vacancies) which slowly accumulated as 40K (in sylvite) decayed over billions of years. The halites were dated by K-Ar, Rb-Sr and I-Xe systematics to be 4.5 billion years old. The "blue" halites were a fantastic discovery for the following reasons: (1) Halite+sylvite can be dated (K is in sylvite and will substitute for Na in halite, Rb substitutes in halite for Na, and I substitutes for Cl). (2) The blue color is lost if the halite dissolves on Earth and reprecipitates (because the newly-formed halite has no color centers), so the color serves as a "freshness" or pristinity indicator. (3) Halite frequently contains aqueous fluid inclusions. (4) Halite contains no structural oxygen, carbon or hydrogen, making them ideal materials to measure these isotopic systems in any fluid inclusions. (5) It is possible to directly measure fluid inclusion formation temperatures, and thus directly measure the temperature of the mineralizing aqueous fluid. In addition to these two ordinary chondrites halite grains have been reliably reported in several ureilites, an additional ordinary chondrite (Jilin), and in the carbonaceous chondrite (Murchison), although these reports were unfortunately not taken seriously. We have lately found additional fluid inclusions in carbonates in several additional carbonaceous chondrites. Meteoritic aqueous fluid inclusions are apparently relatively widespread in meteorites, though very small and thus difficult to analyze.

  12. Monsters are people too

    PubMed Central

    Levy, J.; Foulsham, T.; Kingstone, A.

    2013-01-01

    Animals, including dogs, dolphins, monkeys and man, follow gaze. What mediates this bias towards the eyes? One hypothesis is that primates possess a distinct neural module that is uniquely tuned for the eyes of others. An alternative explanation is that configural face processing drives fixations to the middle of peoples' faces, which is where the eyes happen to be located. We distinguish between these two accounts. Observers were presented with images of people, non-human creatures with eyes in the middle of their faces (`humanoids’) or creatures with eyes positioned elsewhere (`monsters’). There was a profound and significant bias towards looking early and often at the eyes of humans and humanoids and also, critically, at the eyes of monsters. These findings demonstrate that the eyes, and not the middle of the head, are being targeted by the oculomotor system. PMID:23118434

  13. Diabetes in older people.

    PubMed

    Bennett, Katie

    2015-10-01

    The management of diabetes in older people is often challenging and poorly researched. The prevalence of cognitive impairment, chronic kidney disease and other co-existing comorbidities increase with age and have a significant impact on glycaemic control targets and treatment options. This conference examined current clinical practice, highlighted differences in the management of diabetes in the older person and suggested potential areas of future research. PMID:26430187

  14. The International Oryza Map Alignment Project: development of a genus-wide comparative genomics platform to help solve the 9 billion-people question.

    PubMed

    Jacquemin, Julie; Bhatia, Dharminder; Singh, Kuldeep; Wing, Rod A

    2013-05-01

    The wild relatives of rice contain a virtually untapped reservoir of traits that can be used help drive the 21st century green revolution aimed at solving world food security issues by 2050. To better understand and exploit the 23 species of the Oryza genus the rice research community is developing foundational resources composed of: 1) reference genomes and transcriptomes for all 23 species; 2) advanced mapping populations for functional and breeding studies; and 3) in situ conservation sites for ecological, evolutionary and population genomics. To this end, 16 genome sequencing projects are currently underway, and all completed assemblies have been annotated; and several advanced mapping populations have been developed, and more will be generated, mapped, and phenotyped, to uncover useful alleles. As wild Oryza populations are threatened by human activity and climate change, we also discuss the urgent need for sustainable in situ conservation of the genus. PMID:23518283

  15. Photoinduced 1,2,3,4-tetrahydropyridine ring conversions.

    PubMed

    Turovska, Baiba; Lund, Henning; Lūsis, Viesturs; Lielpētere, Anna; Liepiņš, Edvards; Beljakovs, Sergejs; Goba, Inguna; Stradiņš, Jānis

    2015-01-01

    Stable heterocyclic hydroperoxide can be easily prepared as a product of fast oxidation of a 1,2,3,4-tetrahydropyridine by (3)O2 if the solution is exposed to sunlight. The driving force for the photoinduced electron transfer is calculated from electrochemical and spectroscopic data. The outcome of the reaction depends on the light intensity and the concentration of O2. In the solid state the heterocyclic hydroperoxide is stable; in solution it is involved in further reactions. PMID:26664638

  16. Photoinduced 1,2,3,4-tetrahydropyridine ring conversions

    PubMed Central

    Lund, Henning; Lūsis, Viesturs; Lielpētere, Anna; Liepiņš, Edvards; Beljakovs, Sergejs; Goba, Inguna; Stradiņš, Jānis

    2015-01-01

    Summary Stable heterocyclic hydroperoxide can be easily prepared as a product of fast oxidation of a 1,2,3,4-tetrahydropyridine by 3O2 if the solution is exposed to sunlight. The driving force for the photoinduced electron transfer is calculated from electrochemical and spectroscopic data. The outcome of the reaction depends on the light intensity and the concentration of O2. In the solid state the heterocyclic hydroperoxide is stable; in solution it is involved in further reactions. PMID:26664638

  17. Aryne 1,2,3-Trifunctionalization with Aryl Allyl Sulfoxides.

    PubMed

    Li, Yuanyuan; Qiu, Dachuan; Gu, Rongrong; Wang, Junli; Shi, Jiarong; Li, Yang

    2016-08-31

    An aryne 1,2,3-trisubstitution with aryl allyl sulfoxides is accomplished, featuring an incorporation of C-S, C-O, and C-C bonds on the consecutive positions of a benzene ring. The reaction condition is mild with broad substrate scope. Preliminary mechanistic study suggests a cascade formal [2 + 2] reaction of aryne with S═O bond, an allyl S → O migration, and a Claisen rearrangement. PMID:27527334

  18. Galaxy evolution. Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang.

    PubMed

    Tacchella, S; Carollo, C M; Renzini, A; Förster Schreiber, N M; Lang, P; Wuyts, S; Cresci, G; Dekel, A; Genzel, R; Lilly, S J; Mancini, C; Newman, S; Onodera, M; Shapley, A; Tacconi, L; Woo, J; Zamorani, G

    2015-04-17

    Most present-day galaxies with stellar masses ≥10(11) solar masses show no ongoing star formation and are dense spheroids. Ten billion years ago, similarly massive galaxies were typically forming stars at rates of hundreds solar masses per year. It is debated how star formation ceased, on which time scales, and how this "quenching" relates to the emergence of dense spheroids. We measured stellar mass and star-formation rate surface density distributions in star-forming galaxies at redshift 2.2 with ~1-kiloparsec resolution. We find that, in the most massive galaxies, star formation is quenched from the inside out, on time scales less than 1 billion years in the inner regions, up to a few billion years in the outer disks. These galaxies sustain high star-formation activity at large radii, while hosting fully grown and already quenched bulges in their cores. PMID:25883353

  19. Switching To Less-Expensive Blindness Drug Could Save Medicare Part B $18 Billion Over A Ten-Year Period

    PubMed Central

    Hutton, DW; Newman-Casey, PA; Tavag, M; Zacks, DN; Stein, JD

    2014-01-01

    The biologic drugs bevacizumab and ranibizumab have revolutionized treatment of diabetic macular edema and macular degeneration, leading causes of blindness. Ophthalmologic use of these drugs has increased, now accounting for roughly one-sixth of the Medicare Part B drug budget. Ranibizumab and bevacizumab have similar efficacy and potentially minor differences in adverse event rates, but at $2,023 per dose, ranibizumab costs forty times more than bevacizumab. Using modeling methods, we predict ten-year (2010–2020) population-level costs and health benefits of using bevacizumab and ranibizumab. Our results show that if all patients were treated with the less-expensive bevacizumab instead of current usage patterns, Medicare Part B, patients, and the health care system would save $18 billion, $4.6 billion, and $29 billion, respectively. Altering patterns of use with these therapies by encouraging bevacizumab use and hastening approval of biosimilar therapies would dramatically reduce spending without substantially affecting patient outcomes. PMID:24889941

  20. The thermodynamic properties of 2,3-benzothiophene

    SciTech Connect

    Chirico, R.D.; Knipmeyer, S.E.; Nguyen, A.; Steele, W.V.

    1991-01-01

    Upgrading of heavy fossil fuels is normally done by hydrotreating in the presence of catalysts at 5 to 15 MPa pressure of hydrogen and 575 to 700 K. The efficient use of expensive hydrogen in this process is essential to the economic viability of alternative fuel sources (heavy petroleum, tar sands, shale oil, and the products of the liquefaction of coal). 2,3-Benzothiophene is widely used as a model compound in catalyst-comparison and kinetic studies of the hydrodesulfurization (HDS) mechanism. To perform a thermodynamic analysis of the 2,3-benzothiophene/hydrogen reaction network at the process temperatures, Gibbs energies of reaction at those high temperatures are required for the molecules involved. Measurements leading to the calculation of the ideal-gas thermodynamic properties for 2,3-benzothiophene are reported. Experimental methods included adiabatic heat-capacity calorimetry, comparative ebulliometry, inclined-piston gauge manometry, and differential-scanning calorimetry (d.s.c.). The critical temperature and critical density were determined with the d.s.c., and the critical pressure was derived. Entropies, enthalpies, and Gibbs energies of formation were derived for the ideal gas for selected temperatures between 260 K and 750 K. These values were derived by combining the reported measurements with values published previously for the enthalpy of combustion, the enthalpy of fusion, and the absolute entropy and enthalpy of the liquid at the triple-point temperature. Measured and derived quantities were compared with available literature values. 55 refs., 6 figs., 13 tabs.

  1. Flavonolignan 2,3-dehydroderivatives: Preparation, antiradical and cytoprotective activity.

    PubMed

    Pyszková, Michaela; Biler, Michal; Biedermann, David; Valentová, Kateřina; Kuzma, Marek; Vrba, Jiří; Ulrichová, Jitka; Sokolová, Romana; Mojović, Miloš; Popović-Bijelić, Ana; Kubala, Martin; Trouillas, Patrick; Křen, Vladimír; Vacek, Jan

    2016-01-01

    The protective constituents of silymarin, an extract from Silybum marianum fruits, have been extensively studied in terms of their antioxidant and hepatoprotective activities. Here, we explore the electron-donor properties of the major silymarin flavonolignans. Silybin (SB), silychristin (SCH), silydianin (SD) and their respective 2,3-dehydroderivatives (DHSB, DHSCH and DHSD) were oxidized electrochemically and their antiradical/antioxidant properties were investigated. Namely, Folin-Ciocalteau reduction, DPPH and ABTS(+) radical scavenging, inhibition of microsomal lipid peroxidation and cytoprotective effects against tert-butyl hydroperoxide-induced damage to a human hepatocellular carcinoma HepG2 cell line were evaluated. Due to the presence of the highly reactive C3-OH group and the C-2,3 double bond (ring C) allowing electron delocalization across the whole structure in the 2,3-dehydroderivatives, these compounds are much more easily oxidized than the corresponding flavonolignans SB, SCH and SD. This finding was unequivocally confirmed not only by experimental approaches, but also by density functional theory (DFT) calculations. The hierarchy in terms of ability to undergo electrochemical oxidation (DHSCH~DHSD>DHSB>SCH/SD>SB) was consistent with their antiradical activities, mainly DPPH scavenging, as well as in vitro cytoprotection of HepG2 cells. The results are discussed in the context of the antioxidant vs. prooxidant activities of flavonolignans and molecular interactions in complex biological systems. PMID:26582372

  2. U.S. Billion-Ton Update: Biomass Supply for a Bioenergy and Bioproducts Industry

    SciTech Connect

    Downing, Mark; Eaton, Laurence M; Graham, Robin Lambert; Langholtz, Matthew H; Perlack, Robert D; Turhollow Jr, Anthony F; Stokes, Bryce; Brandt, Craig C

    2011-08-01

    The report, Biomass as Feedstock for a Bioenergy and Bioproducts Industry: The Technical Feasibility of a Billion-Ton Annual Supply (generally referred to as the Billion-Ton Study or 2005 BTS), was an estimate of 'potential' biomass based on numerous assumptions about current and future inventory, production capacity, availability, and technology. The analysis was made to determine if conterminous U.S. agriculture and forestry resources had the capability to produce at least one billion dry tons of sustainable biomass annually to displace 30% or more of the nation's present petroleum consumption. An effort was made to use conservative estimates to assure confidence in having sufficient supply to reach the goal. The potential biomass was projected to be reasonably available around mid-century when large-scale biorefineries are likely to exist. The study emphasized primary sources of forest- and agriculture-derived biomass, such as logging residues, fuel treatment thinnings, crop residues, and perennially grown grasses and trees. These primary sources have the greatest potential to supply large, reliable, and sustainable quantities of biomass. While the primary sources were emphasized, estimates of secondary residue and tertiary waste resources of biomass were also provided. The original Billion-Ton Resource Assessment, published in 2005, was divided into two parts-forest-derived resources and agriculture-derived resources. The forest resources included residues produced during the harvesting of merchantable timber, forest residues, and small-diameter trees that could become available through initiatives to reduce fire hazards and improve forest health; forest residues from land conversion; fuelwood extracted from forests; residues generated at primary forest product processing mills; and urban wood wastes, municipal solid wastes (MSW), and construction and demolition (C&D) debris. For these forest resources, only residues, wastes, and small-diameter trees were

  3. Cooling and exhumation of continents at billion-year time scales

    NASA Astrophysics Data System (ADS)

    Blackburn, T.; Bowring, S. A.; Perron, T.; Mahan, K. H.; Dudas, F. O.

    2011-12-01

    The oldest rocks on Earth are preserved within the continental lithosphere, where assembled fragments of ancient orogenic belts have survived erosion and destruction by plate tectonic and surface processes for billions of years. Though the rate of orogenic exhumation and erosion has been measured for segments of an orogenic history, it remains unclear how these exhumation rates have changed over the lifetime of any terrane. Because the exhumation of the lithospheric surface has a direct effect on the rate of heat loss within the lithosphere, a continuous record of lithosphere exhumation can be reconstructed through the use of thermochronology. Thermochronologic studies have typically employed systems sensitive to cooling at temperatures <300 °C, such as the (U-Th)/He and 40Ar/39Ar systems. This largely restricts their application to measuring cooling in rocks from the outer 10 km of the Earth's crust, resulting in a thermal history that is controlled by either upper crustal flexure and faulting and/or isotherm inflections related to surface topography. Combining these biases with the uplift, erosion and recycling of these shallow rocks results in a poor preservation potential of any long-term record. Here, an ancient and long-term record of lithosphere exhumation is constructed using U-Pb thermochronology, a geochronologic system sensitive to cooling at temperatures found at 20-50 km depth (400-650 °C). Lower crustal xenoliths provide material that resided at these depths for billions of years or more, recording a thermal history that is buried deep enough to remain insensitive to upper crustal deformation and instead is dominated by the vertical motions of the continents. We show how this temperature-sensitive system can produce a long-term integrated measure of continental exhumation and erosion. Preserved beneath Phanerozoic sedimentary rocks within Montana, USA, the Great Falls Tectonic Zone formed when two Archean cratons, the Wyoming Province and Medicine

  4. Infections in People with Cancer

    MedlinePlus

    ... window. My Saved Articles » My ACS » Infections in People With Cancer Download Printable Version [PDF] » Cancer itself ... at risk? What are signs of infection in people with cancer? How does your body normally resist ...

  5. Quality of Life Scale: A Measure of Function for People with Pain

    MedlinePlus

    Quality Of Life Scale A Measure Of Function For People With Pain 0 Non-functioning 1 2 3 4 5 6 7 8 Stay in bed all ... in family life Quality Of Life Scale A Measure Of Function For People With Pain ain is ...

  6. The Star Formation History of the Universe over the Past Eight Billion Years

    NASA Astrophysics Data System (ADS)

    Zhu, Guangtun

    How galaxies such as our own Milky Way formed and evolved remains a mystery. There are two general approaches in galaxy formation and evolution studies. One is to infer formation histories via archaeological investigations of galaxies at low redshift, in the local Universe. The other is to study galaxy formation and evolution in action by observing faint distant galaxies, the ancestors of local galaxies, in the more distant and younger Universe, at higher redshift. I employ the first approach to study the formation of elliptical galaxies, the most massive galaxies in the Universe. I investigate the stellar content of 1923 elliptical galaxies, the largest high-fidelity sample in the local Universe, as a function of stellar mass and environment. I infer their star formation histories, finding that isolated low-mass elliptical galaxies formed their stars slightly later than their counterparts in galaxy clusters. I measure the cosmic star formation rate (SFR) density at redshift z ˜ 1, when the Universe was eight billion years younger. The cosmic SFR density measures how many stars are being formed per unit volume of the Universe. I show that galaxies were more actively forming stars eight billion years ago than they are at present, by roughly an order of magnitude. The reason why galaxies are so much less active at present remains unknown, partly due to the small sample size of distant galaxies observed previously. To improve the sample size, we have completed a new galaxy survey, the Prism Multi-object Survey (PRIMUS). We have observed ˜ 120, 000 galaxies spanning distances from the local Universe to redshift z ˜ 1. We specifically targeted fields with existing multi-wavelength data in the X-ray, ultraviolet, optical, and infrared. The large sample and multi-wavelength data allow precise statistical studies of galaxy evolution since z ˜1. As a preliminary result from PRIMUS, I show that 15% of galaxies that appear to lack star formation in the optical actually

  7. A redox-stratified ocean 3.2 billion years ago

    NASA Astrophysics Data System (ADS)

    Satkoski, Aaron M.; Beukes, Nicolas J.; Li, Weiqiang; Beard, Brian L.; Johnson, Clark M.

    2015-11-01

    Before the Great Oxidation Event (GOE) 2.4-2.2 billion years ago it has been traditionally thought that oceanic water columns were uniformly anoxic due to a lack of oxygen-producing microorganisms. Recently, however, it has been proposed that transient oxygenation of shallow seawater occurred between 2.8 and 3.0 billion years ago. Here, we present a novel combination of stable Fe and radiogenic U-Th-Pb isotope data that demonstrate significant oxygen contents in the shallow oceans at 3.2 Ga, based on analysis of the Manzimnyama Banded Iron Formation (BIF), Fig Tree Group, South Africa. This unit is exceptional in that proximal, shallow-water and distal, deep-water facies are preserved. When compared to the distal, deep-water facies, the proximal samples show elevated U concentrations and moderately positive δ56Fe values, indicating vertical stratification in dissolved oxygen contents. Confirmation of oxidizing conditions using U abundances is robustly constrained using samples that have been closed to U and Pb mobility using U-Th-Pb geochronology. Although redox-sensitive elements have been commonly used in ancient rocks to infer redox conditions, post-depositional element mobility has been rarely tested, and U-Th-Pb geochronology can constrain open- or closed-system behavior. The U abundances and δ56Fe values of the Manzimnyama BIF suggest the proximal, shallow-water samples record precipitation under stronger oxidizing conditions compared to the distal deeper-water facies, which in turn indicates the existence of a discrete redox boundary between deep and shallow ocean waters at this time; this work, therefore, documents the oldest known preserved marine redox gradient in the rock record. The relative enrichment of O2 in the upper water column is likely due to the existence of oxygen-producing microorganisms such as cyanobacteria. These results provide a new approach for identifying free oxygen in Earth's ancient oceans, including confirming the age of redox

  8. The First Billion Years project: dark matter haloes going from contraction to expansion and back again

    NASA Astrophysics Data System (ADS)

    Davis, Andrew J.; Khochfar, Sadegh; Dalla Vecchia, Claudio

    2014-09-01

    We study the effect of baryons on the inner dark matter profile of the first galaxies using the First Billion Years simulation between z = 16 and 6 before secular evolution sets in. Using a large statistical sample from two simulations of the same volume and cosmological initial conditions, one with and one without baryons, we are able to directly compare haloes with their baryon-free counterparts, allowing a detailed study of the modifications to the dark matter density profile due to the presence of baryons during the first billion years of galaxy formation. For each of the ≈5000 haloes in our sample (3 × 107 M⊙ ≤ Mtot ≤ 5 × 109 M⊙), we quantify the impact of the baryons using η, defined as the ratio of dark matter mass enclosed in 100 pc in the baryonic run to its counterpart without baryons. During this epoch of rapid growth of galaxies, we find that many haloes of these first galaxies show an enhancement of dark matter in the halo centre compared to the baryon-free simulation, while many others show a deficit. We find that the mean value of η is close to unity, but there is a large dispersion, with a standard deviation of 0.677. The enhancement is cyclical in time and tracks the star formation cycle of the galaxy; as gas falls to the centre and forms stars, the dark matter moves in as well. Supernova (SN) feedback then removes the gas, and the dark matter again responds to the changing potential. We study three physical models relating the motion of baryons to that of the dark matter: adiabatic contraction, dynamical friction, and rapid outflows. We find that dynamical friction plays only a very minor role, while adiabatic contraction and the rapid outflows due to feedback describe well the enhancement (or decrement) of dark matter. For haloes which show significant decrements of dark matter in the core, we find that to remove the dark matter requires an energy input between 1051 and 1053 erg. For our SN feedback proscription, this requires as a

  9. 35C NQR studies in 2,4,6-,2,3,6-, and 2,3,4-trichloro anisoles

    NASA Astrophysics Data System (ADS)

    Rukmani, K.; Ramakrishna, J.

    1985-02-01

    The chlorine-35 NQR frequencies and their temperature variation in 2,4,6-, 2,3,6- and 2,3,4-trichloro anisoles have been studied and compared with the corresponding chlorophenols with a view to studying the effect of hydrogen bonding. The observed frequencies have been assigned to the various chlorines with the help of the additive model of the substituent effect. The temperature dependence has been analysed in terms of the Bayer—Kushida—Brown models. The torsional frequencies and their temperature dependence have been calculated numerically under a two mode approximation. A comparison of the trichloro anisoles with the corresponding trichloro phenols has shown that the resonance frequency decreases due to hydrogen bonding while the torsional frequencies are not affected.

  10. Astronomical activities with disabled people

    NASA Astrophysics Data System (ADS)

    Ortiz-Gil, Amelia; Blay, Pere; Gallego Calvente, A. Teresa; Gómez, Miquel; Guirado, José Carlos; Lanzara, Mariana; Martínez Núñez, Silvia

    2011-06-01

    As we celebrate the International Year of Astronomy, we have been working on four different projects with the goal of making astronomy more accessible to people with special needs. These projects are 1) an astronomy book and web site for blind people, 2) an open source software for people with motor disabilities, 3) a planetarium program for the visually impaired and 4) educational material for intellectually disabled people.

  11. Subjective experiences of watching stereoscopic Avatar and U2 3D in a cinema

    NASA Astrophysics Data System (ADS)

    Pölönen, Monika; Salmimaa, Marja; Takatalo, Jari; Häkkinen, Jukka

    2012-01-01

    A stereoscopic 3-D version of the film Avatar was shown to 85 people who subsequently answered questions related to sickness, visual strain, stereoscopic image quality, and sense of presence. Viewing Avatar for 165 min induced some symptoms of visual strain and sickness, but the symptom levels remained low. A comparison between Avatar and previously published results for the film U2 3D showed that sickness and visual strain levels were similar despite the films' runtimes. The genre of the film had a significant effect on the viewers' opinions and sense of presence. Avatar, which has been described as a combination of action, adventure, and sci-fi genres, was experienced as more immersive and engaging than the music documentary U2 3D. However, participants in both studies were immersed, focused, and absorbed in watching the stereoscopic 3-D (S3-D) film and were pleased with the film environments. The results also showed that previous stereoscopic 3-D experience significantly reduced the amount of reported eye strain and complaints about the weight of the viewing glasses.

  12. Our World of 7 Billion: Population Studies in Today's Social Studies Classroom

    ERIC Educational Resources Information Center

    Wasserman, Pamela

    2011-01-01

    The study of world population integrates so many themes and disciplines in the social studies because it encompasses all of human history--the rise of agriculture and civilizations, scientific progress, territorial conflicts, changing gender roles and more. It is also at the heart of human geography and how people came to dominate and alter the…

  13. 2,3,7,8-TCDD, AND 2,3,7,8-TCDF AND PCB'S IN MARINE SEDIMENTS AND BIOTA: LABORATORY AND FIELD STUDIES

    EPA Science Inventory

    This report describes the bioaccumulation and depuration of 2,3,7,8-tetrachlorodibenzo-p-dioxin (2,3,7,8-TCDD), 2,3,7,8-tetrachlorodibenzofuran (2,3,7,8-TCDF) and polychlorinated biphenyls (PCBs) by three species of marine benthos exposed to contaminated sediment collected from t...

  14. The People Capability Maturity Model

    ERIC Educational Resources Information Center

    Wademan, Mark R.; Spuches, Charles M.; Doughty, Philip L.

    2007-01-01

    The People Capability Maturity Model[R] (People CMM[R]) advocates a staged approach to organizational change. Developed by the Carnegie Mellon University Software Engineering Institute, this model seeks to bring discipline to the people side of management by promoting a structured, repeatable, and predictable approach for improving an…

  15. Learning Opportunities for Older People.

    ERIC Educational Resources Information Center

    MacKeracher, Dorothy

    1980-01-01

    The author summarizes a conference on learning opportunities for older people by discussing six issues: (1) perspectives of older people and service providers; (2) categorization of older learners; (3) learning needs of older people; (4) participation rates; (5) government policies; and (6) curriculum concerns. (SK)

  16. Sharing global CO2 emission reductions among one billion high emitters

    PubMed Central

    Chakravarty, Shoibal; Chikkatur, Ananth; de Coninck, Heleen; Pacala, Stephen; Socolow, Robert; Tavoni, Massimo

    2009-01-01

    We present a framework for allocating a global carbon reduction target among nations, in which the concept of “common but differentiated responsibilities” refers to the emissions of individuals instead of nations. We use the income distribution of a country to estimate how its fossil fuel CO2 emissions are distributed among its citizens, from which we build up a global CO2 distribution. We then propose a simple rule to derive a universal cap on global individual emissions and find corresponding limits on national aggregate emissions from this cap. All of the world's high CO2-emitting individuals are treated the same, regardless of where they live. Any future global emission goal (target and time frame) can be converted into national reduction targets, which are determined by “Business as Usual” projections of national carbon emissions and in-country income distributions. For example, reducing projected global emissions in 2030 by 13 GtCO2 would require the engagement of 1.13 billion high emitters, roughly equally distributed in 4 regions: the U.S., the OECD minus the U.S., China, and the non-OECD minus China. We also modify our methodology to place a floor on emissions of the world's lowest CO2 emitters and demonstrate that climate mitigation and alleviation of extreme poverty are largely decoupled. PMID:19581586

  17. Prodigious degassing of a billion years of accumulated radiogenic helium at Yellowstone

    USGS Publications Warehouse

    Lowenstern, Jacob B.; Evans, William C.; Bergfeld, D.; Hunt, Andrew G.

    2014-01-01

    Helium is used as a critical tracer throughout the Earth sciences, where its relatively simple isotopic systematics is used to trace degassing from the mantle, to date groundwater and to time the rise of continents1. The hydrothermal system at Yellowstone National Park is famous for its high helium-3/helium-4 isotope ratio, commonly cited as evidence for a deep mantle source for the Yellowstone hotspot2. However, much of the helium emitted from this region is actually radiogenic helium-4 produced within the crust by α-decay of uranium and thorium. Here we show, by combining gas emission rates with chemistry and isotopic analyses, that crustal helium-4 emission rates from Yellowstone exceed (by orders of magnitude) any conceivable rate of generation within the crust. It seems that helium has accumulated for (at least) many hundreds of millions of years in Archaean (more than 2.5 billion years old) cratonic rocks beneath Yellowstone, only to be liberated over the past two million years by intense crustal metamorphism induced by the Yellowstone hotspot. Our results demonstrate the extremes in variability of crustal helium efflux on geologic timescales and imply crustal-scale open-system behaviour of helium in tectonically and magmatically active regions.

  18. Half a billion years of good weather: Gaia or good luck?

    NASA Astrophysics Data System (ADS)

    Waltham, Dave

    2007-06-01

    For the past 550 million years, Earth has had a relatively stable climate, with average global temperatures generally fluctuating by less than 10°C from the present value of around 15°C. In the preceding 4 billion years, temperature fluctuations were almost an order of magnitude greater. One explanation for climate stability is that the biosphere evolves to maintain optimum conditions for life (the Gaia hypothesis). But this stability could also result from luck and, without such good fortune, conditions on Earth would have been unsuitable for the evolution of complex life: anthropic selection, in other words. One element of such good luck concerns the climatic impact of the Moon; the properties of the Earth-Moon system only just allow a stable rotation axis for the Earth (considered a prerequisite for climate stability and the evolution of complex life). Axial stability also requires Jupiter and Saturn to be widely spaced, offering a test of the rarity or otherwise of the solar system arrangement among exoplanet systems. Gravitational microlensing surveys should allow this to be tested within a decade.

  19. Prodigious degassing of a billion years of accumulated radiogenic helium at Yellowstone.

    PubMed

    Lowenstern, J B; Evans, W C; Bergfeld, D; Hunt, A G

    2014-02-20

    Helium is used as a critical tracer throughout the Earth sciences, where its relatively simple isotopic systematics is used to trace degassing from the mantle, to date groundwater and to time the rise of continents. The hydrothermal system at Yellowstone National Park is famous for its high helium-3/helium-4 isotope ratio, commonly cited as evidence for a deep mantle source for the Yellowstone hotspot. However, much of the helium emitted from this region is actually radiogenic helium-4 produced within the crust by α-decay of uranium and thorium. Here we show, by combining gas emission rates with chemistry and isotopic analyses, that crustal helium-4 emission rates from Yellowstone exceed (by orders of magnitude) any conceivable rate of generation within the crust. It seems that helium has accumulated for (at least) many hundreds of millions of years in Archaean (more than 2.5 billion years old) cratonic rocks beneath Yellowstone, only to be liberated over the past two million years by intense crustal metamorphism induced by the Yellowstone hotspot. Our results demonstrate the extremes in variability of crustal helium efflux on geologic timescales and imply crustal-scale open-system behaviour of helium in tectonically and magmatically active regions. PMID:24553240

  20. Potentially biogenic carbon preserved in a 4.1 billion-year-old zircon

    PubMed Central

    Bell, Elizabeth A.; Harrison, T. Mark; Mao, Wendy L.

    2015-01-01

    Evidence of life on Earth is manifestly preserved in the rock record. However, the microfossil record only extends to ∼3.5 billion years (Ga), the chemofossil record arguably to ∼3.8 Ga, and the rock record to 4.0 Ga. Detrital zircons from Jack Hills, Western Australia range in age up to nearly 4.4 Ga. From a population of over 10,000 Jack Hills zircons, we identified one >3.8-Ga zircon that contains primary graphite inclusions. Here, we report carbon isotopic measurements on these inclusions in a concordant, 4.10 ± 0.01-Ga zircon. We interpret these inclusions as primary due to their enclosure in a crack-free host as shown by transmission X-ray microscopy and their crystal habit. Their δ13CPDB of −24 ± 5‰ is consistent with a biogenic origin and may be evidence that a terrestrial biosphere had emerged by 4.1 Ga, or ∼300 My earlier than has been previously proposed. PMID:26483481

  1. Potentially biogenic carbon preserved in a 4.1 billion-year-old zircon

    DOE PAGESBeta

    Bell, Elizabeth A.; Boehnke, Patrick; Harrison, T. Mark; Mao, Wendy L.

    2015-10-19

    Here, evidence of life on Earth is manifestly preserved in the rock record. However, the microfossil record only extends to ~3.5 billion years (Ga), the chemofossil record arguably to ~3.8 Ga, and the rock record to 4.0 Ga. Detrital zircons from Jack Hills, Western Australia range in age up to nearly 4.4 Ga. From a population of over 10,000 Jack Hills zircons, we identified one >3.8-Ga zircon that contains primary graphite inclusions. Here, we report carbon isotopic measurements on these inclusions in a concordant, 4.10 ± 0.01-Ga zircon. We interpret these inclusions as primary due to their enclosure in amore » crack-free host as shown by transmission X-ray microscopy and their crystal habit. Their δ13CPDB of –24 ± 5‰ is consistent with a biogenic origin and may be evidence that a terrestrial biosphere had emerged by 4.1 Ga, or ~300 My earlier than has been previously proposed.« less

  2. Potentially biogenic carbon preserved in a 4.1 billion-year-old zircon

    SciTech Connect

    Bell, Elizabeth A.; Boehnke, Patrick; Harrison, T. Mark; Mao, Wendy L.

    2015-10-19

    Here, evidence of life on Earth is manifestly preserved in the rock record. However, the microfossil record only extends to ~3.5 billion years (Ga), the chemofossil record arguably to ~3.8 Ga, and the rock record to 4.0 Ga. Detrital zircons from Jack Hills, Western Australia range in age up to nearly 4.4 Ga. From a population of over 10,000 Jack Hills zircons, we identified one >3.8-Ga zircon that contains primary graphite inclusions. Here, we report carbon isotopic measurements on these inclusions in a concordant, 4.10 ± 0.01-Ga zircon. We interpret these inclusions as primary due to their enclosure in a crack-free host as shown by transmission X-ray microscopy and their crystal habit. Their δ13CPDB of –24 ± 5‰ is consistent with a biogenic origin and may be evidence that a terrestrial biosphere had emerged by 4.1 Ga, or ~300 My earlier than has been previously proposed.

  3. If slow rate of health care spending growth persists, projections may be off by $770 billion.

    PubMed

    Cutler, David M; Sahni, Nikhil R

    2013-05-01

    Despite earlier forecasts to the contrary, US health care spending growth has slowed in the past four years, continuing a trend that began in the early 2000s. In this article we attempt to identify why US health care spending growth has slowed, and we explore the spending implications if the trend continues for the next decade. We find that the 2007-09 recession, a one-time event, accounted for 37 percent of the slowdown between 2003 and 2012. A decline in private insurance coverage and cuts to some Medicare payment rates accounted for another 8 percent of the slowdown, leaving 55 percent of the spending slowdown unexplained. We conclude that a host of fundamental changes--including less rapid development of imaging technology and new pharmaceuticals, increased patient cost sharing, and greater provider efficiency--were responsible for the majority of the slowdown in spending growth. If these trends continue during 2013-22, public-sector health care spending will be as much as $770 billion less than predicted. Such lower levels of spending would have an enormous impact on the US economy and on government and household finances. PMID:23650316

  4. How to make a billion-barrel oil field in offshore California commercial

    SciTech Connect

    Patterson, J.C.; Ballard, J.H.

    1988-02-01

    The major obstacles and challenges involved in exploration and development of a giant deep-water low-gravity oil field are exemplified in the undeveloped Sword field of offshore southern California. In 1979, Conoco Exploration identified a northeast-southwest-trending basement high in the 800 to 2000-ft deep federal waters 12 mi southwest of Pt. Conception at the western end of the Santa Barbara Channel. The intended reservoir was fractured Miocene Monterey chert, silicic shales/siltstones, and dolomites that are draped over the axially faulted structure. Drilling of the initial well in OCS P-0322 in 1982 resulted in discovering the giant Sword field. A confirmation well drilled in OCS P-0320 indicates in-place reserves of well over 1 billion bbl. While the discovered potential is significant, the low gravity (8.5/degree/-10.5/degree/ API) of the oils discovered to date, along with water depths in excess of 1500 ft, currently pose economic challenges to successful field development. Conoco and its partners are addressing the current economic barriers on a number of fronts. Three-dimensional seismic surveys are being conducted to better delineate reservoir geometry and to define probable variations in lithology, fracturing, and oil gravity. A market feasibility study will be undertaken to assess the demand for low-gravity crude from offshore California.

  5. How to make a billion-barrel oil field in offshore California commercial

    SciTech Connect

    Patterson, J.C.; Ballard, J.H.

    1988-01-01

    The major obstacles and challenges involved in exploration and development of a giant deep-water low-gravity oil field are exemplified in the undeveloped Sword field of offshore southern California. In 1979, Conoco Exploration identified a northeast-southwest-trending basement high in the 800 to 2,000-ft deep federal waters 12 mi southwest of Pt. Conception at the western end of the Santa Barbara Channel. The intended reservoir was fractured Miocene Monterey chert, silicic shales/siltstones,m and dolomites that are draped over the axially faulted structure. Drilling of the initial well in OCS P-0322 in 1982 resulted in discovering the giant Sword field. A confirmation well drilled in OCS P-0320 indicates in-place reserves of well over 1 billion bbl. while the discovered potential is significant, the low gravity (8.5/sup 0/-10.5/sup 0/ API) of the oils discovered to data, along with water depths in excess of 1,500 ft, currently pose economic challenges to successful field development.

  6. Rapid oxygenation of Earth’s atmosphere 2.33 billion years ago

    PubMed Central

    Luo, Genming; Ono, Shuhei; Beukes, Nicolas J.; Wang, David T.; Xie, Shucheng; Summons, Roger E.

    2016-01-01

    Molecular oxygen (O2) is, and has been, a primary driver of biological evolution and shapes the contemporary landscape of Earth’s biogeochemical cycles. Although “whiffs” of oxygen have been documented in the Archean atmosphere, substantial O2 did not accumulate irreversibly until the Early Paleoproterozoic, during what has been termed the Great Oxygenation Event (GOE). The timing of the GOE and the rate at which this oxygenation took place have been poorly constrained until now. We report the transition (that is, from being mass-independent to becoming mass-dependent) in multiple sulfur isotope signals of diagenetic pyrite in a continuous sedimentary sequence in three coeval drill cores in the Transvaal Supergroup, South Africa. These data precisely constrain the GOE to 2.33 billion years ago. The new data suggest that the oxygenation occurred rapidly—within 1 to 10 million years—and was followed by a slower rise in the ocean sulfate inventory. Our data indicate that a climate perturbation predated the GOE, whereas the relationships among GOE, “Snowball Earth” glaciation, and biogeochemical cycling will require further stratigraphic correlation supported with precise chronologies and paleolatitude reconstructions. PMID:27386544

  7. Constraints on the first billion years of the geodynamo from paleointensity studies of zircons

    NASA Astrophysics Data System (ADS)

    Tarduno, John; Cottrell, Rory; Davis, William

    2014-05-01

    Several lines of reasoning, including new ideas on core thermal conductivity, suggest that onset of a strong geomagnetic field might have been delayed by one billion years (or more) after the lunar forming event. Here we extend the Proterozoic/Archean to Paleoarchean record of the geomagnetic field constrained by single crystal paleointensity (SCP) analyses (Tarduno et al., Science, 2010) to older times using zircons containing minute magnetic inclusions. Specifically, we focus on samples from the Jack Hills (Yilgarn Craton, Western Australia). We employ a CO2 laser demagnetization system and a small bore (6.3 mm) 3-component DC SQUID magnetometer; the latter offers the highest currently available moment resolution. Sample age is analyzed using SHRIMP U-Pb geochronology. Preliminary data support the presence of a relatively strong Paleoarchean field produced by a core dynamo, extending the known record by at least 100 million years, to approximately 3.55 Ga. These data only serve to exacerbate the apparent problem posed by the presence of a Paleoarchean dynamo. Alternative dynamo driving mechanisms, or efficient core/lowermost mantle heat loss processes unique to the Paleoarchean (and older times) might have been at work. We will discuss these processes, and our efforts to study even older Eoarchean-Hadean zircons.

  8. Ballography: A Billion Nanosecond History of the Bee Bluff Impact Crater of South Texas

    NASA Astrophysics Data System (ADS)

    Graham, R. A.

    2006-07-01

    The Bee Bluff Structure of South Texas in Zavala County near Uvalde has been found to exhibit unusual features permitting study of impactites and meteorite impact processes from the standpoint of grain-level, nanosecond shock-compression science. The site is characterized by a thin cap of Carrizo Sandstone covering a thin hard Indio fm calcareous siltstone. A soft calcareous silt lies below the hard cap. Calculations based on the Earth Impact Effects web-based program indicate that the site is best described by a 60 m diameter iron meteorite striking the ground at 11 km/sec. Such an impact into sandstone is expected to produce a shock pressure of 250 GPa. A large release wave originates from the bottom of the hard target with upward moving melt-vaporization waves of solid, liquid and vapor products that become trapped at the impact interface. Numerous distinctive types of impactites result from this `bottom-up' release behavior. Evidence for hydrodynamic instabilities and resulting density gradients are abundant at the impact interface. An unusually valuable breccia sample called `The Uvalde Crater Rosetta Stone' contains at least seven types of impactites in a well defined arrangement that can be used to read the billion nanosecond history of the impact and identify scattered impactites relative to their place in that history.

  9. Enhanced cellular preservation by clay minerals in 1 billion-year-old lakes.

    PubMed

    Wacey, David; Saunders, Martin; Roberts, Malcolm; Menon, Sarath; Green, Leonard; Kong, Charlie; Culwick, Timothy; Strother, Paul; Brasier, Martin D

    2014-01-01

    Organic-walled microfossils provide the best insights into the composition and evolution of the biosphere through the first 80 percent of Earth history. The mechanism of microfossil preservation affects the quality of biological information retained and informs understanding of early Earth palaeo-environments. We here show that 1 billion-year-old microfossils from the non-marine Torridon Group are remarkably preserved by a combination of clay minerals and phosphate, with clay minerals providing the highest fidelity of preservation. Fe-rich clay mostly occurs in narrow zones in contact with cellular material and is interpreted as an early microbially-mediated phase enclosing and replacing the most labile biological material. K-rich clay occurs within and exterior to cell envelopes, forming where the supply of Fe had been exhausted. Clay minerals inter-finger with calcium phosphate that co-precipitated with the clays in the sub-oxic zone of the lake sediments. This type of preservation was favoured in sulfate-poor environments where Fe-silicate precipitation could outcompete Fe-sulfide formation. This work shows that clay minerals can provide an exceptionally high fidelity of microfossil preservation and extends the known geological range of this fossilization style by almost 500 Ma. It also suggests that the best-preserved microfossils of this time may be found in low-sulfate environments. PMID:25068404

  10. A large neutral fraction of cosmic hydrogen a billion years after the Big Bang.

    PubMed

    Wyithe, J Stuart B; Loeb, Abraham

    2004-02-26

    The fraction of ionized hydrogen left over from the Big Bang provides evidence for the time of formation of the first stars and quasar black holes in the early Universe; such objects provide the high-energy photons necessary to ionize hydrogen. Spectra of the two most distant known quasars show nearly complete absorption of photons with wavelengths shorter than the Lyman alpha transition of neutral hydrogen, indicating that hydrogen in the intergalactic medium (IGM) had not been completely ionized at a redshift of z approximately 6.3, about one billion years after the Big Bang. Here we show that the IGM surrounding these quasars had a neutral hydrogen fraction of tens of per cent before the quasar activity started, much higher than the previous lower limits of approximately 0.1 per cent. Our results, when combined with the recent inference of a large cumulative optical depth to electron scattering after cosmological recombination therefore suggest the presence of a second peak in the mean ionization history of the Universe. PMID:14985754

  11. Potentially biogenic carbon preserved in a 4.1 billion-year-old zircon.

    PubMed

    Bell, Elizabeth A; Boehnke, Patrick; Harrison, T Mark; Mao, Wendy L

    2015-11-24

    Evidence of life on Earth is manifestly preserved in the rock record. However, the microfossil record only extends to ∼ 3.5 billion years (Ga), the chemofossil record arguably to ∼ 3.8 Ga, and the rock record to 4.0 Ga. Detrital zircons from Jack Hills, Western Australia range in age up to nearly 4.4 Ga. From a population of over 10,000 Jack Hills zircons, we identified one >3.8-Ga zircon that contains primary graphite inclusions. Here, we report carbon isotopic measurements on these inclusions in a concordant, 4.10 ± 0.01-Ga zircon. We interpret these inclusions as primary due to their enclosure in a crack-free host as shown by transmission X-ray microscopy and their crystal habit. Their δ(13)CPDB of -24 ± 5‰ is consistent with a biogenic origin and may be evidence that a terrestrial biosphere had emerged by 4.1 Ga, or ∼ 300 My earlier than has been previously proposed. PMID:26483481

  12. Prodigious degassing of a billion years of accumulated radiogenic helium at Yellowstone

    NASA Astrophysics Data System (ADS)

    Lowenstern, J. B.; Evans, W. C.; Bergfeld, D.; Hunt, A. G.

    2014-02-01

    Helium is used as a critical tracer throughout the Earth sciences, where its relatively simple isotopic systematics is used to trace degassing from the mantle, to date groundwater and to time the rise of continents. The hydrothermal system at Yellowstone National Park is famous for its high helium-3/helium-4 isotope ratio, commonly cited as evidence for a deep mantle source for the Yellowstone hotspot. However, much of the helium emitted from this region is actually radiogenic helium-4 produced within the crust by α-decay of uranium and thorium. Here we show, by combining gas emission rates with chemistry and isotopic analyses, that crustal helium-4 emission rates from Yellowstone exceed (by orders of magnitude) any conceivable rate of generation within the crust. It seems that helium has accumulated for (at least) many hundreds of millions of years in Archaean (more than 2.5 billion years old) cratonic rocks beneath Yellowstone, only to be liberated over the past two million years by intense crustal metamorphism induced by the Yellowstone hotspot. Our results demonstrate the extremes in variability of crustal helium efflux on geologic timescales and imply crustal-scale open-system behaviour of helium in tectonically and magmatically active regions.

  13. Enhanced cellular preservation by clay minerals in 1 billion-year-old lakes

    NASA Astrophysics Data System (ADS)

    Wacey, David; Saunders, Martin; Roberts, Malcolm; Menon, Sarath; Green, Leonard; Kong, Charlie; Culwick, Timothy; Strother, Paul; Brasier, Martin D.

    2014-07-01

    Organic-walled microfossils provide the best insights into the composition and evolution of the biosphere through the first 80 percent of Earth history. The mechanism of microfossil preservation affects the quality of biological information retained and informs understanding of early Earth palaeo-environments. We here show that 1 billion-year-old microfossils from the non-marine Torridon Group are remarkably preserved by a combination of clay minerals and phosphate, with clay minerals providing the highest fidelity of preservation. Fe-rich clay mostly occurs in narrow zones in contact with cellular material and is interpreted as an early microbially-mediated phase enclosing and replacing the most labile biological material. K-rich clay occurs within and exterior to cell envelopes, forming where the supply of Fe had been exhausted. Clay minerals inter-finger with calcium phosphate that co-precipitated with the clays in the sub-oxic zone of the lake sediments. This type of preservation was favoured in sulfate-poor environments where Fe-silicate precipitation could outcompete Fe-sulfide formation. This work shows that clay minerals can provide an exceptionally high fidelity of microfossil preservation and extends the known geological range of this fossilization style by almost 500 Ma. It also suggests that the best-preserved microfossils of this time may be found in low-sulfate environments.

  14. Rapid oxygenation of Earth's atmosphere 2.33 billion years ago.

    PubMed

    Luo, Genming; Ono, Shuhei; Beukes, Nicolas J; Wang, David T; Xie, Shucheng; Summons, Roger E

    2016-05-01

    Molecular oxygen (O2) is, and has been, a primary driver of biological evolution and shapes the contemporary landscape of Earth's biogeochemical cycles. Although "whiffs" of oxygen have been documented in the Archean atmosphere, substantial O2 did not accumulate irreversibly until the Early Paleoproterozoic, during what has been termed the Great Oxygenation Event (GOE). The timing of the GOE and the rate at which this oxygenation took place have been poorly constrained until now. We report the transition (that is, from being mass-independent to becoming mass-dependent) in multiple sulfur isotope signals of diagenetic pyrite in a continuous sedimentary sequence in three coeval drill cores in the Transvaal Supergroup, South Africa. These data precisely constrain the GOE to 2.33 billion years ago. The new data suggest that the oxygenation occurred rapidly-within 1 to 10 million years-and was followed by a slower rise in the ocean sulfate inventory. Our data indicate that a climate perturbation predated the GOE, whereas the relationships among GOE, "Snowball Earth" glaciation, and biogeochemical cycling will require further stratigraphic correlation supported with precise chronologies and paleolatitude reconstructions. PMID:27386544

  15. Analysis of precious metals at parts-per-billion levels in industrial applications

    NASA Astrophysics Data System (ADS)

    Tickner, James; O'Dwyer, Joel; Roach, Greg; Smith, Michael; Van Haarlem, Yves

    2015-11-01

    Precious metals, including gold and the platinum group metals (notable Pt, Pd and Rh), are mined commercially at concentrations of a few parts-per-million and below. Mining and processing operations demand sensitive and rapid analysis at concentrations down to about 100 parts-per-billion (ppb). In this paper, we discuss two technologies being developed to meet this challenge: X-ray fluorescence (XRF) and gamma-activation analysis (GAA). We have designed on-stream XRF analysers capable of measuring targeted elements in slurries with precisions in the 35-70 ppb range. For the past two years, two on-stream analysers have been in continuous operation at a precious metals concentrator plant. The simultaneous measurement of feed and waste stream grades provides real-time information on metal recovery, allowing changes in operating conditions and plant upsets to be detected and corrected more rapidly. Separately, we have been developing GAA for the measurement of gold as a replacement for the traditional laboratory fire-assay process. High-energy Bremsstrahlung X-rays are used to excite gold via the 197Au(γ,γ‧)197Au-M reaction, and the gamma-rays released in the decay of the meta-state are then counted. We report on work to significantly improve accuracy and detection limits.

  16. Full-sky weak-lensing simulation with 70 billion particles

    NASA Astrophysics Data System (ADS)

    Teyssier, R.; Pires, S.; Prunet, S.; Aubert, D.; Pichon, C.; Amara, A.; Benabed, K.; Colombi, S.; Refregier, A.; Starck, J.-L.

    2009-04-01

    We have performed a 70 billion dark-matter particles N-body simulation in a 2 h-1 Gpc periodic box, using the concordance, cosmological model as favored by the latest WMAP3 results. We have computed a full-sky convergence map with a resolution of Δ θ ≃ 0.74 arcmin2, spanning 4 orders of magnitude in angular dynamical range. Using various high-order statistics on a realistic cut sky, we have characterized the transition from the linear to the nonlinear regime at ℓ ≃ 1000 and shown that realistic galactic masking affects high-order moments only below ℓ < 200. Each domain (Gaussian and non-Gaussian) spans 2 decades in angular scale. This map is therefore an ideal tool for testing map-making algorithms on the sphere. As a first step in addressing the full map reconstruction problem, we have benchmarked in this paper two denoising methods: 1) Wiener filtering applied to the Spherical Harmonics decomposition of the map and 2) a new method, called MRLens, based on the modification of the Maximum Entropy Method on a Wavelet decomposition. While the latter is optimal on large spatial scales, where the signal is Gaussian, MRLens outperforms the Wiener method on small spatial scales, where the signal is highly non-Gaussian. The simulated full-sky convergence map is freely available to the community to help the development of new map-making algorithms dedicated to the next generation of weak-lensing surveys.

  17. A billion years of environmental stability and the emergence of eukaryotes: new data from northern Australia.

    PubMed

    Brasier, M D; Lindsay, J F

    1998-06-01

    Carbon isotopes through 6km of fully cored drill holes in 1.7 to 1.5 Ga carbonates of the Mount Isa and McArthur basins, Australia (which host the earliest known eukaryote biomarkers) provide the most comprehensive and best-dated delta 13C stratigraphy yet obtained from such ancient rocks. Both basins reveal remarkably stable temporal delta 13C trends (mean of -0.6% +/- 2% PDB [Peedee belemnite]) and confirm the impression of delta 13C stasis between 2.0 and 1.0 Ga, which, together with other evidence, suggest a prolonged period of stability in crustal dynamics, redox state of surface environments, and planetary climate. This delta 13C stasis is consistent with great stability in the carbon cycle controlled, we suggest, by P limitation of primary productivity. Recent evidence shows that P depletion is a major factor in obligate associations between photosymbionts and host cells. We argue that a billion years of stability in the carbon and nutrient cycles may have been the driving force that propelled prokaryotes toward photosymbiosis and the emergence of the autotrophic eukaryote cell. PMID:11541449

  18. Vibrational spectrum and internal rotation in 2,3-dimethylpyrazine

    NASA Astrophysics Data System (ADS)

    Arenas, J. F.; Lòpez-Navarrete, J. T.; Marcos, J. I.; Otero, J. C.

    1989-01-01

    The infrared and Raman spectra of 2,3-dimethylpyrazine have been recorded and assigned on the basis of a C2v molecular geometry previously determined by MINDO/3. The potential energy function corresponding to the internal rotation of both methyl groups has been used to solve the Schrödinger equation and to obtain the energy levels of that motion on the basis of a molecular geometry G36. The rotation of the substituents is not independent and they behave as two geared rotors.

  19. Continuous variable (2, 3) threshold quantum secret sharing schemes

    NASA Astrophysics Data System (ADS)

    Lance, Andrew M.; Symul, Thomas; Bowen, Warwick P.; Tyc, Tomás; Sanders, Barry C.; Lam, Ping Koy

    2003-01-01

    We present two schemes to perform continuous variable (2, 3) threshold quantum secret sharing (QSS) on the quadrature amplitudes of bright light beams. Both schemes require a pair of entangled light beams. The first scheme utilizes two phase sensitive optical amplifiers, whilst the second uses an electro-optic feedforward loop for the reconstruction of the secret. We examine the efficacy of QSS in terms of fidelity, as well as the signal transfer coefficients and the conditional variances of the reconstructed output state. We show that both schemes in the ideal case yield perfect secret reconstruction.

  20. Industrial R&D Spending Reached $26.6 Billion in 1976. Science Resources Studies Highlights, May 5, 1978.

    ERIC Educational Resources Information Center

    National Science Foundation, Washington, DC. Div. of Science Resources Studies.

    This report presents data compiled as part of a comprehensive program to measure and analyze the nation's resources expended for research and development (R&D). Industry, which carries out 69% of the R&D in the United States, spent $26.6 billion on these activities in 1976, 10% above the 1975 level. In constant dollars, this presents an increase…

  1. Industrial R&D Expenditures Rise to $22 Billion in 1974. Science Resources Studies Highlights, January 14, 1976.

    ERIC Educational Resources Information Center

    National Science Foundation, Washington, DC. Div. of Science Resources Studies.

    Reported in this newsletter in narrative, graphical, and tabular form are data related to industrial research and development expenditures in 1974, showing a seven percent increase over 1973. It is noted that more than 80 percent of a total of $22.3 billion was spent by five industries; these included electrical equipment and communication,…

  2. $100 Billion: For Reform...or to Subsidize the Status Quo? Education Stimulus Watch. Special Report 1

    ERIC Educational Resources Information Center

    Smarick, Andy

    2009-01-01

    This is the first in a quarterly series of special reports on the K-12 education implications of the federal government's economic stimulus package, the American Recovery and Reinvestment Act (ARRA). That the ARRA, which was signed into law in February, will pump nearly $100 billion--an unprecedented sum of federal money--into K-12 education is…

  3. 77 FR 29458 - Supervisory Guidance on Stress Testing for Banking Organizations With More Than $10 Billion in...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2012-05-17

    ...The Board, FDIC and OCC, (collectively, the ``agencies'') are issuing this guidance, which outlines high-level principles for stress testing practices, applicable to all Federal Reserve-supervised, FDIC- supervised, and OCC-supervised banking organizations with more than $10 billion in total consolidated assets. The guidance highlights the importance of stress testing as an ongoing risk......

  4. 76 FR 35072 - Proposed Guidance on Stress Testing for Banking Organizations With More Than $10 Billion in Total...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2011-06-15

    ... Stress Testing Guidance. The agency form number for the collection is FR 4202. The agency control number... Proposed Guidance on Stress Testing for Banking Organizations With More Than $10 Billion in Total..., Board, and the FDIC (collectively, the ``agencies'') request comment on proposed guidance on...

  5. Recognizing People in Motion.

    PubMed

    Yovel, Galit; O'Toole, Alice J

    2016-05-01

    Natural movements of the face and body, as well as voice, provide converging cues to a person's identity. To date, person recognition has been studied primarily with static images of faces. Face recognition, however, is part of a larger system, whose preeminent goal is to efficiently recognize dynamic familiar people in unconstrained environments. We present a comprehensive framework for understanding person recognition as it happens in the real world. In this framework, dynamic information plays the central role in binding multi-modal information from the face, body, and the voice to achieve robust and highly accurate recognition. The superior temporal sulcus (STS) integrates multisensory, dynamic information from the whole person for recognition, thereby complementing its role in social cognition. PMID:27016844

  6. TSAR2.3. Temporal Scattering And Response

    SciTech Connect

    McLeod, R.R.; Ray, S.L.; Laguna, G.; Allison, M.; Cabral, B.

    1991-12-01

    TSAR2.3 (Temporal Scattering and Response) is a finite-difference time-domain electromagnetics code suite. TSAR2.3 is a software package for simulating the interactions of electromagnetic waves with linear materials through the use of the finite-difference time-domain method. The code suite contains grid generation, grid verification, input-file creation and post-processing utilities. The physics package, written in Fortran 77, can be pre-processed to run on many different architectures including Cray, Vax and many Unix workstations. Tools are provided to easily port the code to new computers. The physics package is an efficient, flexible electromagnetic simulator. A body under study can be represented as a three-dimensional grid of materials with arbitrary linear properties. This grid can be simulated in a number of ways including incident plane waves, dipoles, and arbitrary incident fields. The grid can be terminated with numerous boundary conditions including free-space radiation, electric conductor, or magnetic conductor. Projection to the far-field in both the time and frequency domains is possible. This distribution includes make files for installing and maintaining the entire code suite.

  7. Fragrance material review on 2-(3-methylphenyl) ethanol.

    PubMed

    Scognamiglio, J; Jones, L; Letizia, C S; Api, A M

    2012-09-01

    A toxicologic and dermatologic review of 2-(3-methylphenyl) ethanol when used as a fragrance ingredient is presented. 2-(3-Methylphenyl) ethanol is a member of the fragrance structural group Aryl Alkyl Alcohols and is a primary alcohol. The AAAs are a structurally diverse class of fragrance ingredients that includes primary, secondary, and tertiary alkyl alcohols covalently bonded to an aryl (Ar) group, which may be either a substituted or unsubstituted benzene ring. The common structural element for the AAA fragrance ingredients is an alcohol group -C-(R1)(R2)OH and generically the AAA fragrances can be represented as an Ar-C-(R1)(R2)OH or Ar-Alkyl-C-(R1)(R2)OH group. This review contains a detailed summary of all available toxicology and dermatology papers that are related to this individual fragrance ingredient and is not intended as a stand-alone document. A safety assessment of the entire Aryl Alkyl Alcohols will be published simultaneously with this document; please refer to Belsito et al. (2012) for an overall assessment of the safe use of this material and all other branched chain saturated alcohols in fragrances. PMID:22036978

  8. A new synthesis of 2,3-di- or 2,3,3-trisubstituted 2,3-dihydro-4-pyridones by reaction of 3-ethoxycyclobutanones and N-p-toluenesulfonyl imines using titanium(IV) chloride: synthesis of (+/-)-bremazocine.

    PubMed

    Matsuo, Jun-ichi; Okado, Ryohei; Ishibashi, Hiroyuki

    2010-07-16

    N-p-Toluenesulfonyl (Ts) aldimines reacted with 3-ethoxycyclobutanones by catalysis of titanium(IV) chloride to afford 2,3-di- or 2,3,3-trisubstituted N-Ts-2,3-dihydro-4-pyridones. Synthesis of (+/-)-bremazocine was efficiently accomplished by using this method. PMID:20568828

  9. The First Billion Years project: the escape fraction of ionizing photons in the epoch of reionization

    NASA Astrophysics Data System (ADS)

    Paardekooper, Jan-Pieter; Khochfar, Sadegh; Dalla Vecchia, Claudio

    2015-08-01

    Protogalaxies forming in low-mass dark matter haloes are thought to provide the majority of ionizing photons needed to reionize the Universe, due to their high escape fractions of ionizing photons. We study how the escape fraction in high-redshift galaxies relates to the physical properties of the halo in which the galaxies form, by computing escape fractions in more than 75 000 haloes between redshifts 27 and 6 that were extracted from the First Billion Years project, high-resolution cosmological hydrodynamical simulations of galaxy formation. We find that the main constraint on the escape fraction is the gas column density in a radius of 10 pc around the stellar populations, causing a strong mass dependence of the escape fraction. The lower potential well in haloes with M200 ≲ 108 M⊙ results in low column densities that can be penetrated by radiation from young stars (age <5 Myr). In haloes with M200 ≳ 108 M⊙ supernova feedback is important, but only ˜30 per cent of the haloes in this mass range have an escape fraction higher than 1 per cent. We find a large range of escape fractions in haloes with similar properties, caused by different distributions of the dense gas in the halo. This makes it very hard to predict the escape fraction on the basis of halo properties and results in a highly anisotropic escape fraction. The strong mass dependence, the large spread and the large anisotropy of the escape fraction may strongly affect the topology of reionization and is something current models of cosmic reionization should strive to take into account.

  10. A sawtooth-like timeline for the first billion years of lunar bombardment

    NASA Astrophysics Data System (ADS)

    Morbidelli, A.; Marchi, S.; Bottke, W. F.; Kring, D. A.

    2012-11-01

    We revisit the early evolution of the Moon's bombardment. Our work combines modeling (based on plausible projectile sources and their dynamical decay rates) with constraints from the lunar crater record, radiometric ages of the youngest lunar basins, and the abundance of highly siderophile elements in the lunar crust and mantle. We deduce that the evolution of the impact flux did not decline exponentially over the first billion years of lunar history, but also there was no prominent and narrow impact spike ˜3.9Gy ago, unlike that typically envisioned in the lunar cataclysm scenario. Instead, we show the timeline of the lunar bombardment has a sawtooth-like profile, with an uptick in the impact flux near ˜4.1Gy ago. The impact flux at the beginning of this weaker cataclysm was 5-10 times higher than the immediately preceding period. The Nectaris basin should have been one of the first basins formed at the sawtooth. We predict the bombardment rate since ˜4.1Gy ago declined slowly and adhered relatively close to classic crater chronology models (Neukum and Ivanov, 1994). Overall we expect that the sawtooth event accounted for about one-fourth of the total bombardment suffered by the Moon since its formation. Consequently, considering that ˜12-14 basins formed during the sawtooth event, we expect that the net number of basins formed on the Moon was ˜45-50. From our expected bombardment timeline, we derived a new and improved lunar chronology suitable for use on pre-Nectarian surface units. According to this chronology, a significant portion of the oldest lunar cratered terrains has an age of 4.38-4.42 Gyr. Moreover, the largest lunar basin, South Pole Aitken, is older than 4.3 Gy, and therefore was not produced during the lunar cataclysm.

  11. Searching for the birthplaces of open clusters with ages of several billion years

    NASA Astrophysics Data System (ADS)

    Acharova, I. A.; Shevtsova, E. S.

    2016-01-01

    We discuss the possibility of finding the birthplaces of open clusters (OC) with ages of several billion years. The proposed method is based on the comparison of the results of the chemical evolution modeling of the Galactic disk with the parameters of the cluster. Five OCs older than 7 Gyr are known: NGC6791, BH176, Collinder 261, Berkeley 17, and Berkeley 39. The oxygen and iron abundances in NGC6791 and the oxygen abundance in BH176 are twice the solar level, the heavy-element abundances in other clusters are close to the corresponding solar values. According to chemical evolution models, at the time of the formation of the objects considered the regions where the oxygen and iron abundances reached the corresponding levels extended out to 5 kpc from the Galactic center.At present time theOCs considered are located several kpc from the Galactic center. Some of these clusters are located extremely high, about 1 kpc above the disk midplane, i.e., they have been subject to some mechanism that has carried them into orbits uncharacteristic of this type of objects. It follows from a comparison with the results of chemical evolution that younger clusters with ages of 4-5 Gyr, e.g., NGC1193,M67, and others, may have formed in a broad range of Galactocentric distances. Their large heights above the disk midplane is sufficient to suggest that these clusters have moved away from their likely birthplaces. Clusters are carried far away from the Galactic disk until the present time: about 40 clusters with ages from 0 to 2 Gyr are observed at heights ranging from 300 to 750 pc.

  12. No Photon Left Behind: How Billions of Spectral Lines are Transforming Planetary Sciences

    NASA Astrophysics Data System (ADS)

    Villanueva, Geronimo L.

    2014-06-01

    With the advent of realistic potential energy surface (PES) and dipole moment surface (DMS) descriptions, theoretically computed linelists can now synthesize accurate spectral parameters for billions of spectral lines sampling the untamed high-energy molecular domain. Being the initial driver for these databases the characterization of stellar spectra, these theoretical databases, in combination with decades of precise experimental studies (nicely compiled in community databases such as HITRAN and GEISA), are leading to unprecedented precisions in the characterization of planetary atmospheres. Cometary sciences are among the most affected by this spectroscopic revolution. Even though comets are relatively cold bodies (T˜100 K), their infrared molecular emission is mainly defined by non-LTE solar fluorescence induced by a high-energy source (Sun, T˜5600 K). In order to interpret high-resolution spectra of comets acquired with extremely powerful telescopes (e.g., Keck, VLT, NASA-IRTF), we have developed advanced non-LTE fluorescence models that integrate the high-energy dynamic range of ab-initio databases (e.g., BT2, VTT, HPT2, BYTe, TROVE) and the precision of laboratory and semi-empirical compilations (e.g., HITRAN, GEISA, CDMS, WKMC, SELP, IUPAC). These new models allow us to calculate realistic non-LTE pumps, cascades, branching-ratios, and emission rates for a broad range of excitation regimes for H2O, HDO, HCN, HNC and NH3. We have implemented elements of these compilations to the study of Mars spectra, and we are now exploring its application to modeling non-LTE emission in exoplanets. In this presentation, we present application of these advanced models to interpret highresolution spectra of comets, Mars and exoplanets.

  13. The formation of submillimetre-bright galaxies from gas infall over a billion years.

    PubMed

    Narayanan, Desika; Turk, Matthew; Feldmann, Robert; Robitaille, Thomas; Hopkins, Philip; Thompson, Robert; Hayward, Christopher; Ball, David; Faucher-Giguère, Claude-André; Kereš, Dušan

    2015-09-24

    Submillimetre-bright galaxies at high redshift are the most luminous, heavily star-forming galaxies in the Universe and are characterized by prodigious emission in the far-infrared, with a flux of at least five millijanskys at a wavelength of 850 micrometres. They reside in haloes with masses about 10(13) times that of the Sun, have low gas fractions compared to main-sequence disks at a comparable redshift, trace complex environments and are not easily observable at optical wavelengths. Their physical origin remains unclear. Simulations have been able to form galaxies with the requisite luminosities, but have otherwise been unable to simultaneously match the stellar masses, star formation rates, gas fractions and environments. Here we report a cosmological hydrodynamic galaxy formation simulation that is able to form a submillimetre galaxy that simultaneously satisfies the broad range of observed physical constraints. We find that groups of galaxies residing in massive dark matter haloes have increasing rates of star formation that peak at collective rates of about 500-1,000 solar masses per year at redshifts of two to three, by which time the interstellar medium is sufficiently enriched with metals that the region may be observed as a submillimetre-selected system. The intense star formation rates are fuelled in part by the infall of a reservoir gas supply enabled by stellar feedback at earlier times, not through major mergers. With a lifetime of nearly a billion years, our simulations show that the submillimetre-bright phase of high-redshift galaxies is prolonged and associated with significant mass buildup in early-Universe proto-clusters, and that many submillimetre-bright galaxies are composed of numerous unresolved components (for which there is some observational evidence). PMID:26399829

  14. A Highly Functional Synthetic Phage Display Library Containing over 40 Billion Human Antibody Clones

    PubMed Central

    Weber, Marcel; Bujak, Emil; Putelli, Alessia; Villa, Alessandra; Matasci, Mattia; Gualandi, Laura; Hemmerle, Teresa; Wulhfard, Sarah; Neri, Dario

    2014-01-01

    Several synthetic antibody phage display libraries have been created and used for the isolation of human monoclonal antibodies. The performance of antibody libraries, which is usually measured in terms of their ability to yield high-affinity binding specificities against target proteins of interest, depends both on technical aspects (such as library size and quality of cloning) and on design features (which influence the percentage of functional clones in the library and their ability to be used for practical applications). Here, we describe the design, construction and characterization of a combinatorial phage display library, comprising over 40 billion human antibody clones in single-chain fragment variable (scFv) format. The library was designed with the aim to obtain highly stable antibody clones, which can be affinity-purified on protein A supports, even when used in scFv format. The library was found to be highly functional, as >90% of randomly selected clones expressed the corresponding antibody. When selected against more than 15 antigens from various sources, the library always yielded specific and potent binders, at a higher frequency compared to previous antibody libraries. To demonstrate library performance in practical biomedical research projects, we isolated the human antibody G5, which reacts both against human and murine forms of the alternatively spliced BCD segment of tenascin-C, an extracellular matrix component frequently over-expressed in cancer and in chronic inflammation. The new library represents a useful source of binding specificities, both for academic research and for the development of antibody-based therapeutics. PMID:24950200

  15. Cyanobacterial conversion of carbon dioxide to 2,3-butanediol

    PubMed Central

    Oliver, John W. K.; Machado, Iara M. P.; Yoneda, Hisanari; Atsumi, Shota

    2013-01-01

    Conversion of CO2 for the synthesis of chemicals by photosynthetic organisms is an attractive target for establishing independence from fossil reserves. However, synthetic pathway construction in cyanobacteria is still in its infancy compared with model fermentative organisms. Here we systematically developed the 2,3-butanediol (23BD) biosynthetic pathway in Synechococcus elongatus PCC7942 as a model system to establish design methods for efficient exogenous chemical production in cyanobacteria. We identified 23BD as a target chemical with low host toxicity, and designed an oxygen-insensitive, cofactor-matched biosynthetic pathway coupled with irreversible enzymatic steps to create a driving force toward the target. Production of 23BD from CO2 reached 2.38 g/L, which is a significant increase for chemical production from exogenous pathways in cyanobacteria. This work demonstrates that developing strong design methods can continue to increase chemical production in cyanobacteria. PMID:23297225

  16. Antitumour agents as inhibitors of tryptophan 2,3-dioxygenase.

    PubMed

    Pantouris, Georgios; Mowat, Christopher G

    2014-01-01

    The involvement of tryptophan 2,3-dioxygenase (TDO) in cancer biology has recently been described, with the enzyme playing an immunomodulatory role, suppressing antitumour immune responses and promoting tumour cell survival and proliferation. This finding reinforces the need for specific inhibitors of TDO that may potentially be developed for therapeutic use. In this work we have screened ~2800 compounds from the library of the National Cancer Institute USA and identified seven potent inhibitors of TDO with inhibition constants in the nanomolar or low micromolar range. All seven have antitumour properties, killing various cancer cell lines. For comparison, the inhibition potencies of these compounds were tested against IDO and their inhibition constants are reported. Interestingly, this work reveals that NSC 36398 (dihydroquercetin, taxifolin), with an in vitro inhibition constant of ~16 μM, is the first TDO-selective inhibitor reported. PMID:24269239

  17. Noncommutative SO(2,3) gauge theory and noncommutative gravity

    NASA Astrophysics Data System (ADS)

    Dimitrijević, Marija; Radovanović, Voja

    2014-06-01

    In this paper noncommutative gravity is constructed as a gauge theory of the noncommutative SO(2,3)⋆ group, while the noncommutativity is canonical (constant). The Seiberg-Witten map is used to express noncommutative fields in terms of the corresponding commutative fields. The commutative limit of the model is the Einstein-Hilbert action with the cosmological constant term and the topological Gauss-Bonnet term. We calculate the second order correction to this model and obtain terms that are of zeroth to fourth power in the curvature tensor and torsion. Trying to relate our results with f(R) and f(T) models, we analyze different limits of our model. In the limit of big cosmological constant and vanishing torsion we obtain an x-dependent correction to the cosmological constant; i.e. noncommutativity leads to an x-dependent cosmological constant. We also discuss the limit of small cosmological constant and vanishing torsion and the teleparallel limit.

  18. NADH Oxidase Activity of Indoleamine 2,3-Dioxygenase*

    PubMed Central

    Rosell, Federico I.; Kuo, Hsin H.; Mauk, A. Grant

    2011-01-01

    The heme enzyme indoleamine 2,3-dioxygenase (IDO) was found to oxidize NADH under aerobic conditions in the absence of other enzymes or reactants. This reaction led to the formation of the dioxygen adduct of IDO and supported the oxidation of Trp to N-formylkynurenine. Formation of the dioxygen adduct and oxidation of Trp were accelerated by the addition of small amounts of hydrogen peroxide, and both processes were inhibited in the presence of either superoxide dismutase or catalase. Anaerobic reaction of IDO with NADH proceeded only in the presence of a mediator (e.g. methylene blue) and resulted in formation of the ferrous form of the enzyme. We propose that trace amounts of peroxide previously proposed to occur in NADH solutions as well as solid NADH activate IDO and lead to aerobic formation of superoxide and the reactive dioxygen adduct of the enzyme. PMID:21690092

  19. [Young people first].

    PubMed

    1995-04-01

    In every country, people debate about at what point youth should be informed about sex, if it is normal to be sexually active and at what age, and if it is necessary for youth to have easy access to condoms and other contraceptive methods. The reason for the debate is that young people are being exposed to more and more risks. It is time for them to have the means to protect themselves against HIV infections, other sexually transmitted diseases (STDs), and unwanted pregnancy. More than 50% of the world's population is less than 25 years old. Youth are becoming sexually active at younger ages. More than 50% of HIV cases in the world are younger than 25. The most vulnerable to HIV are young women. When young adults die of AIDS, their children become orphans and must live with other family members. Most deaths among 15-19 year old girls are associated with pregnancy or childbirth. 1 in 20 adolescents has been treated for at least 1 STD. The number is probably higher since most youth do not have access to STD treatment or do not even know they have an STD. Youth often do not have access to sexuality counseling, family planning services, or STD services. Adolescence is a time of considerable physical and emotional change. Youth want to experience new ways to love and to feel loved. These new experiences and the risks that come with the experiences are needed for development but youth need support to avoid risky behavior. Factors that make the already vulnerable youth even more vulnerable are poverty, unemployment, little education, abuse of alcohol and drugs, and violence. Youth need sex education at school; activities in religious, sport, and youth club organizations; use of the mass media to promote sexual responsibility; and access to family planning. Youth programs must be based on specific responses and beliefs, information, and knowledge needs identified by the youth themselves. Youth need more than facts on sex and reproduction. They need to discuss, ask

  20. Resources, people: uneasy balance.

    PubMed

    1984-03-01

    Recently, population growth spurted ahead of the growth of the world's output of goods and services, whose yearly rise averaged only 1.6% from 1979-82. That difference means misery for millions of people. Many nations will be unable to provide enough jobs for its population. Living standards and incomes will plummet, and millions may starve. In developing nations, where population growth sometimes outpaces economic growth by 4 or 5 percentage points, the future looks particularly bleak. Worldwide the production of grain has managed to keep up with population growth, but Africa is undergoing the most explosive growth of any continent in history, and food output there just cannot keep up. Since 1970 the amount of grain available for each African dropped more than 11%. In order to produce more food, Africans need chemical fertilizer and farm machines. The problem is that most African countries are so short of cash that they cannot afford to buy the fertilizer and equipment they need to modernize their farming methods. Theirmain source of cash, besides loans, is from the export of goods and services. Many African nations saw those exports decline during the 1970s. The major element responsible for the deline is costly oil. The era of cheap oil ended in 1973. Exporting nations raised the price of a barrel of oil from about US$2-$12. The output of food, goods, and services slowed as farm and factory owners tried to adjust to the higher costs of energy. In 1979 the price of a barrel of oil moved past US$30, triggering a worldwide economic slump. At the same time the world's people were multiplying faster than the output of goods and services. The specter of large scale famine is real. In the early 1970s Bangladesh attributed nearly 800,000 deaths to diseases related to malnutrition. In 1972, after India's grain harvest failed, there were 829,000 more deaths than in 1971. The governments of both India and Bangladesh have made slowing population growth a major priority

  1. Enhancing young people's awareness.

    PubMed

    Doan Thi Tien

    1995-01-01

    The role of the Vietnam Youth Union (21 million members) is to educate the youth aged 14-28 years about the movement at the grassroots level. Since 1995, it has been entrusted with information, education, and communication (IEC) activities (implemented through the Educational Center for Population, Health, and Development) concerning family planning, the environment, human immunodeficiency virus (HIV) and acquired immunodeficiency syndrome (AIDS). Mass media, direct communication, Youth Union leading staff, Youth Union cultural and arts activities, and advertisement have been used. 16 newspapers and magazines, a radio program, and a TV program disseminate information for the group. 1000 motivators' groups, 1370 Youth Clubs, and Youth Villages at the commune level work to enhance awareness and to change biased attitudes and habits. Leading staff speak at conferences and seminars that are attended by target groups. Art troupes perform at special local events; plays are organized and videos are shown. The HIV/AIDS information and prevention campaign is of great importance because research findings indicate that many young people believe that only prostitutes and drug addicts can be infected, and that condoms are bad and only for use with prostitutes. There are about 2300 persons infected with HIV in 14 provinces, mostly in the south and central regions. 131 are reported to have developed AIDS. PMID:12320323

  2. People who live in green houses.

    PubMed

    Stetson, M

    1991-01-01

    This article examines the struggle between developed and developing countries when it comes to reducing energy consumption and limit carbon emissions, necessary steps for averting global warming. Negotiators from across the world have begun discussing the issue, hoping to come to an agreement by next June, when the UN Conference on Environment and Development will meet in Brazil. Disagreement centers around the question of who is responsible for the greenhouse effect and who will pay to fix the problem. The report discusses energy consumption and its effects, the cost of producing energy, and possible ways of eliminating energy waste -- especially as it relates to the 3rd world. Currently, the industrialized world (along with the USSR and Eastern Europe) account for 70% of all carbon emissions from fossil fuel consumption. Experts predict, however, that by the year 2025, the 3rd World will surpass the industrialized world in fossil fuel consumption. The author emphasizes the difference in energy use between the 2 regions: while people in developing countries burn wood and biomass to take care of basic necessities, much of the consumption in the developed world to goes towards luxuries and amenities. Inefficient power plants waste much of the energy consumed in the 3rd World. Although hundreds of billions of dollars could be saved annually by introducing energy-saving devices, skewed international lending, underpriced electricity, and the vested interests of the 3rd World industries work against such measures. The author explains that the technology necessary to significantly reduced carbon emissions already exists. Furthermore, 3rd World countries and most industrialized nations (with the exception of the US and the USSR) have agreed on the need to reduce carbon emissions. PMID:12343295

  3. Gastrointestinal care for older people.

    PubMed

    Tremayne, Penny; Harrison, Penny

    2016-07-01

    This article discusses gastrointestinal (GI) healthcare in older people. It outlines the physiological changes that occur in the GI tract as a result of ageing, and discusses common GI disorders in older people. These GI disorders include dysphagia, gastrointestinal reflux disease, colorectal cancer, diverticular disease, constipation and anaemia. Healthcare professionals should be aware of the factors that may influence gastrointestinal health in older people, including nutrition, hydration and alcohol use, which are important considerations when delivering person-centred care. PMID:27380703

  4. How many people have ever lived on earth?

    PubMed

    Haub, C

    1995-02-01

    An estimate of the total number of persons who have ever lived on earth depends on two factors: 1) the length of time humans have been on earth; and 2) the average size of human populations at different periods. According to the United Nations' "Determinants and Consequences of Population Trends," modern Homo sapiens appeared about 50,000 B.C. At the dawn of agriculture, about 8000 B.C., the world's population was around 5 million. By 1 A.D., the population had reached 300 million, which indicates a growth rate of 0.0512% per year. Life expectancy at birth averaged 10 years for most of human history. The birth rate would have to be about 80 per 1000 just for the species to survive. Infant mortality in the early days of human life would be high, probably 500 infant deaths per 1000. Children were probably economic liabilities in hunter-gatherer societies; this might have led to infanticide, which in turn would require a disproportionately high birth rate to maintain population growth. By 1650, the world's population had risen to 500 million, although the Black Plague, which began in 542 A.D. in western Asia and killed 50% of the Byzantine Empire in the sixth century (a total of 100 million deaths), had slowed the rate of growth. By 1800, the world's population passed 1 billion and continued to grow to its current total of 5.7 billion. Estimating the number of people ever born requires selecting population sizes for different points from antiquity to the present and applying assumed birth rates to each period. Assuming a constant growth rate and birth rates of 80 per 1000 through 1 A.D., 60 per 1000 from 2 A.D. to 1750, and the low 30s per 1000 by modern times, 105 billion people have lived on earth, of whom 5.5% are alive today. The assumption of constant population growth in the earliest period may have resulted in an underestimate, while an earlier date of the appearance of humans on earth would raise the number. A table of Population Reference Bureau statistics is

  5. Molecular evolution of bacterial indoleamine 2,3-dioxygenase.

    PubMed

    Yuasa, Hajime J; Ushigoe, Akiko; Ball, Helen J

    2011-10-01

    Indoleamine 2,3-dioxygenase (IDO) and tryptophan 2,3-dioxygenase (TDO) are tryptophan-degrading enzymes that catalyze the first step in L-Trp catabolism via the kynurenine pathway. In mammals, TDO is mainly expressed in the liver and primarily supplies nicotinamide adenine dinucleotide (NAD(+)). TDO is widely distributed from mammals to bacteria. Active IDO enzymes have been reported only in vertebrates and fungi. In mammals, IDO activity plays a significant role in the immune system while in fungal species, IDO is constitutively expressed and supplies NAD(+), like mammalian TDO. A search of genomic databases reveals that some bacterial species also have a putative IDO gene. A phylogenetic analysis clustered bacterial IDOs into two groups, group I or group II bacterial IDOs. The catalytic efficiencies of group I bacterial IDOs were very low and they are suspected not to contribute significantly to L-Trp metabolism. The bacterial species bearing the group I bacterial IDO are scattered across a few phyla and no phylogenetically close relationship is observed between them. This suggests that the group I bacterial IDOs might be acquired by horizontal gene transmission that occurred in each lineage independently. In contrast, group II bacterial IDOs showed rather high catalytic efficiency. Particularly, the enzymatic characteristics (K(m), V(max) and inhibitor selectivity) of the Gemmatimonas aurantiaca IDO are comparable to those of mammalian IDO1, although comparison of the IDO sequences does not suggest a close evolutionary relationship. In several bacteria, TDO and the kynureninase gene (kynU) are clustered on their chromosome suggesting that these genes could be transcribed in an operon. Interestingly, G. aurantiaca has no TDO, and the IDO is clustered with kynU on its chromosome. Although the G. aurantiaca also has NadA and NadB to synthesize a quinolinic acid (a precursor of NAD(+)) via the aspartate pathway, the high activity of the G. aurantiaca IDO flanking

  6. Subsampled open-reference clustering creates consistent, comprehensive OTU definitions and scales to billions of sequences.

    PubMed

    Rideout, Jai Ram; He, Yan; Navas-Molina, Jose A; Walters, William A; Ursell, Luke K; Gibbons, Sean M; Chase, John; McDonald, Daniel; Gonzalez, Antonio; Robbins-Pianka, Adam; Clemente, Jose C; Gilbert, Jack A; Huse, Susan M; Zhou, Hong-Wei; Knight, Rob; Caporaso, J Gregory

    2014-01-01

    We present a performance-optimized algorithm, subsampled open-reference OTU picking, for assigning marker gene (e.g., 16S rRNA) sequences generated on next-generation sequencing platforms to operational taxonomic units (OTUs) for microbial community analysis. This algorithm provides benefits over de novo OTU picking (clustering can be performed largely in parallel, reducing runtime) and closed-reference OTU picking (all reads are clustered, not only those that match a reference database sequence with high similarity). Because more of our algorithm can be run in parallel relative to "classic" open-reference OTU picking, it makes open-reference OTU picking tractable on massive amplicon sequence data sets (though on smaller data sets, "classic" open-reference OTU clustering is often faster). We illustrate that here by applying it to the first 15,000 samples sequenced for the Earth Microbiome Project (1.3 billion V4 16S rRNA amplicons). To the best of our knowledge, this is the largest OTU picking run ever performed, and we estimate that our new algorithm runs in less than 1/5 the time than would be required of "classic" open reference OTU picking. We show that subsampled open-reference OTU picking yields results that are highly correlated with those generated by "classic" open-reference OTU picking through comparisons on three well-studied datasets. An implementation of this algorithm is provided in the popular QIIME software package, which uses uclust for read clustering. All analyses were performed using QIIME's uclust wrappers, though we provide details (aided by the open-source code in our GitHub repository) that will allow implementation of subsampled open-reference OTU picking independently of QIIME (e.g., in a compiled programming language, where runtimes should be further reduced). Our analyses should generalize to other implementations of these OTU picking algorithms. Finally, we present a comparison of parameter settings in QIIME's OTU picking workflows and

  7. IDC RP2 & 3 US Industry Standard Cost Estimate Summary.

    SciTech Connect

    Harris, James M.; Huelskamp, Robert M.

    2015-01-01

    Sandia National Laboratories has prepared a ROM cost estimate for budgetary planning for the IDC Reengineering Phase 2 & 3 effort, using a commercial software cost estimation tool calibrated to US industry performance parameters. This is not a cost estimate for Sandia to perform the project. This report provides the ROM cost estimate and describes the methodology, assumptions, and cost model details used to create the ROM cost estimate. ROM Cost Estimate Disclaimer Contained herein is a Rough Order of Magnitude (ROM) cost estimate that has been provided to enable initial planning for this proposed project. This ROM cost estimate is submitted to facilitate informal discussions in relation to this project and is NOT intended to commit Sandia National Laboratories (Sandia) or its resources. Furthermore, as a Federally Funded Research and Development Center (FFRDC), Sandia must be compliant with the Anti-Deficiency Act and operate on a full-cost recovery basis. Therefore, while Sandia, in conjunction with the Sponsor, will use best judgment to execute work and to address the highest risks and most important issues in order to effectively manage within cost constraints, this ROM estimate and any subsequent approved cost estimates are on a 'full-cost recovery' basis. Thus, work can neither commence nor continue unless adequate funding has been accepted and certified by DOE.

  8. The 2.3-Angstrom Structure of Porcine Circovirus 2

    SciTech Connect

    Khayat, Reza; Brunn, Nicholas; Speir, Jeffrey A.; Hardham, John M.; Ankenbauer, Robert G.; Schneemann, Anette; Johnson, John E.

    2012-10-25

    Porcine circovirus 2 (PCV2) is a T = 1 nonenveloped icosahedral virus that has had severe impact on the swine industry. Here we report the crystal structure of an N-terminally truncated PCV2 virus-like particle at 2.3-{angstrom} resolution, and the cryo-electron microscopy (cryo-EM) image reconstruction of a full-length PCV2 virus-like particle at 9.6-{angstrom} resolution. This is the first atomic structure of a circovirus. The crystal structure revealed that the capsid protein fold is a canonical viral jelly roll. The loops connecting the strands of the jelly roll define the limited features of the surface. Sulfate ions interacting with the surface and electrostatic potential calculations strongly suggest a heparan sulfate binding site that allows PCV2 to gain entry into the cell. The crystal structure also allowed previously determined epitopes of the capsid to be visualized. The cryo-EM image reconstruction showed that the location of the N terminus, absent in the crystal structure, is inside the capsid. As the N terminus was previously shown to be antigenic, it may externalize through viral 'breathing'.

  9. Dynamic Spectra Predicted for 2-3 Khz Radio Emission

    NASA Astrophysics Data System (ADS)

    Mitchell, Jeremy J.; Cairns, Iver H.; Robinson, Peter A.

    Radio emissions observed at 2-3 kHz by the Voyager spacecraft occur when global merged interaction regions (GMIRs) reach the heliopause. The radiation is thought to occur when a GMIR enters a region close to the heliopause where the electron speed distribution is primed with a superthermal tail produced by lower hybrid drive. Previously this priming mechanism was combined with a theory for type II solar radio bursts to predict the flux of radio emission in the outer heliosphere. Here this theory is extended in two ways. First theoretical arguments regarding the availability of Langmuir and ion sound waves are used to determine whether emission occurs via three wave processes or processes involving wave scattering off thermal ions (STI). New expressions for conversion efficiencies into radio emission associated with STI are then implemented where appropriate. Second dynamic spectra are calculated for the radio emission generated by shock from the inner solar wind to beyond the heliopause. The results are then compared with existing Voyager observations.

  10. Recent progress in printed 2/3D electronic devices

    NASA Astrophysics Data System (ADS)

    Klug, Andreas; Patter, Paul; Popovic, Karl; Blümel, Alexander; Sax, Stefan; Lenz, Martin; Glushko, Oleksandr; Cordill, Megan J.; List-Kratochvil, Emil J. W.

    2015-09-01

    New, energy-saving, efficient and cost-effective processing technologies such as 2D and 3D inkjet printing (IJP) for the production and integration of intelligent components will be opening up very interesting possibilities for industrial applications of molecular materials in the near future. Beyond the use of home and office based printers, "inkjet printing technology" allows for the additive structured deposition of photonic and electronic materials on a wide variety of substrates such as textiles, plastics, wood, stone, tiles or cardboard. Great interest also exists in applying IJP in industrial manufacturing such as the manufacturing of PCBs, of solar cells, printed organic electronics and medical products. In all these cases inkjet printing is a flexible (digital), additive, selective and cost-efficient material deposition method. Due to these advantages, there is the prospect that currently used standard patterning processes can be replaced through this innovative material deposition technique. A main issue in this research area is the formulation of novel functional inks or the adaptation of commercially available inks for specific industrial applications and/or processes. In this contribution we report on the design, realization and characterization of novel active and passive inkjet printed electronic devices including circuitry and sensors based on metal nanoparticle ink formulations and the heterogeneous integration into 2/3D printed demonstrators. The main emphasis of this paper will be on how to convert scientific inkjet knowledge into industrially relevant processes and applications.

  11. Antitumour agents as inhibitors of tryptophan 2,3-dioxygenase

    SciTech Connect

    Pantouris, Georgios; Mowat, Christopher G.

    2014-01-03

    Highlights: •∼2800 National Cancer Institute USA compounds have been screened as potential inhibitors of TDO and/or IDO. •Seven compounds with anti-tumour properties have been identified as potent inhibitors. •NSC 36398 (taxifolin, dihydroquercetin) is selective for TDO with a K{sub i} of 16 M. •This may help further our understanding of the role of TDO in cancer. -- Abstract: The involvement of tryptophan 2,3-dioxygenase (TDO) in cancer biology has recently been described, with the enzyme playing an immunomodulatory role, suppressing antitumour immune responses and promoting tumour cell survival and proliferation. This finding reinforces the need for specific inhibitors of TDO that may potentially be developed for therapeutic use. In this work we have screened ∼2800 compounds from the library of the National Cancer Institute USA and identified seven potent inhibitors of TDO with inhibition constants in the nanomolar or low micromolar range. All seven have antitumour properties, killing various cancer cell lines. For comparison, the inhibition potencies of these compounds were tested against IDO and their inhibition constants are reported. Interestingly, this work reveals that NSC 36398 (dihydroquercetin, taxifolin), with an in vitro inhibition constant of ∼16 μM, is the first TDO-selective inhibitor reported.

  12. Synthesis and bioactivity of 2',3'-benzoabscisic acid analogs.

    PubMed

    Han, Xiaoqiang; Wan, Chuan; Li, Xiuyun; Li, Hong; Yang, Dongyan; Du, Shijie; Xiao, Yumei; Qin, Zhaohai

    2015-06-01

    2',3'-Benzoabscisic acid 4a is significantly more active than (±)-ABA and can be potentially used as a plant growth regulator for agriculture. In this study, six 4a analogs were designed and synthesized. Bioassay showed that 4a displayed greater activity than (±)-ABA and the six analogs produced less inhibition than 4a itself. Specially, some analogs displayed markedly different activities to different physiological and biochemical process, which were largely different from ABA and 4a. Compared to (±)-ABA, 4b and 4c were more effective germination inhibitors for lettuce, but less effective inhibitors for rice elongation. Five-membered analog 5 was higher or slightly weaker in inhibiting Arabidopsis seed germination and rice elongation, respectively, but at least 10 times less effective than (±)-ABA in lettuce seed germination. Dual acid 6 and alkyne acid 20 nearly produced no inhibitory activity for Arabidopsis seed germination, but displayed excellent activity in inhibiting rice seedling growth. The preference of the analogs to different physiology process indicated that they might provide a strategy to develop novel ABA agonists or antagonist and be used as probe to investigate the function of different ABA receptors. PMID:25913114

  13. The continuing cost of privatization: extra payments to Medicare Advantage plans jump to $11.4 billion in 2009.

    PubMed

    Biles, Brian; Pozen, Jonah; Guterman, Stuart

    2009-05-01

    The Medicare Modernization Act of 2003 explicitly increased Medicare payments to private Medicare Advantage (MA) plans. As a result, MA plans have, for the past six years, been paid more for their enrollees than they would be expected to cost in traditional fee-for-service Medicare. Payments to MA plans in 2009 are projected to be 13 percent greater than the corresponding costs in traditional Medicare--an average of $1,138 per MA plan enrollee, for a total of $11.4 billion. Although the extra payments are used to provide enrollees additional benefits, those benefits are not available to all beneficiaries-- but they are financed by general program funds. If payments to MA plans were instead equal to the spending level under traditional Medicare, the more than $150 billion in savings over 10 years could be used to finance improved benefits for the low-income elderly and disabled, or for expanding health-insurance coverage. PMID:19449498

  14. National R&D Spending to Exceed $50 Billion in 1979. Science Resources Studies Highlights, May 1, 1978.

    ERIC Educational Resources Information Center

    National Science Foundation, Washington, DC. Div. of Science Resources Studies.

    This report presents data compiled as part of a comprehensive program to measure and analyze the nation's resources expended for research and development (R&D). R&D spending in the United States is expected to reach $51 billion in 1979, 9% over the 1978 level. The R&D expenditures are expected to account for 2.2% of the gross national product…

  15. The People Make the Place.

    ERIC Educational Resources Information Center

    Schneider, Benjamin

    1987-01-01

    Presents a framework for understanding the etiology of organizational behavior, based on theory and research from interactional psychology, vocational psychology, industrial/organizational psychology, and organizational theory. Proposes that organizations are functions of the kinds of people they contain and that the people there are functions of…

  16. Leading Work with Young People

    ERIC Educational Resources Information Center

    Harrison, Roger, Ed.; Benjamin, Cathy, Ed.; Curran, Sheila, Ed.; Hunter, Rob, Ed.

    2007-01-01

    "Leading Work with Young People" provides a selection of writing from a complex and dynamic field of work. The editors bring together key readings and newly commissioned material to present a variety of theoretical and practical perspectives on leading and managing work with young people. The book will equip students with the knowledge, skills,…

  17. Racially Mixed People in America.

    ERIC Educational Resources Information Center

    Root, Maria P. P., Ed.

    This book offers a comprehensive look at the social and psychological adjustment of multiracial people, models for identity development, contemporary immigration and marriage patterns, and methodological issues involved in conducting research with mixed-race people, all in the context of America's multiracial past and present. The following 26…

  18. Where Do Young People Work?

    ERIC Educational Resources Information Center

    Maguire, Sue; Huddleston, Prue

    2009-01-01

    The current policy intention, that all young people remain in some form of accredited education or training to the age of 18 by 2015, poses significant challenges. The jobs without training (JWT) group includes young people who are in full-time work and not in receipt of training leading to National Vocational Qualification level 2 (or above);…

  19. Young People and Contemporary Art

    ERIC Educational Resources Information Center

    Illeris, Helene

    2005-01-01

    In this article empirical examples are used to connect theories about young people, contemporary art forms and learning. The first part of the article introduces the new forms of consciousness which, according to the youth researchers Birgitte Simonsen and Thomas Ziehe, characterize young people of today. In the second part, the qualities of…

  20. How Do People Get AIDS?

    MedlinePlus

    ... a Friend Who Cuts? How Do People Get AIDS? KidsHealth > For Teens > How Do People Get AIDS? Print A A A Text Size en español ¿Cómo contrae alguien el SIDA? AIDS stands for acquired immunodeficiency syndrome , a disease that ...

  1. Anemia in People with Cancer

    MedlinePlus

    ... My ACS » Your Local Offices Close + - Text Size Anemia in People With Cancer What is anemia? When you don’t have enough healthy red ... the symptoms that bother people most. What causes anemia? There are many different reasons a person with ...

  2. Information Technology and Indigenous People

    ERIC Educational Resources Information Center

    Dyson, Laurel, Ed.; Hendriks, Max, Ed.; Grant, Stephen, Ed.

    2007-01-01

    Information Technology and Indigenous People provides theoretical and empirical information related to the planning and execution of IT projects aimed at serving indigenous people. It explores many cultural concerns with IT implementation, including language issues and questions of cultural appropriateness, and brings together cutting-edge…

  3. Effective Communication with Young People

    ERIC Educational Resources Information Center

    Shanahan, Patrick; Elliott, David

    2009-01-01

    The Australian Government established the Office for Youth (the Office) in September 2008 in an effort to engage with the young people of Australia. The Office will work with other government agencies to help young people reach their full potential; make effective transitions to adulthood as they continue to learn, start work, make decisions that…

  4. How People Really Detect Lies.

    ERIC Educational Resources Information Center

    Park, Hee Sun; Levine, Timothy R.; McCornack, Steven A.; Morrison, Kelly; Ferrara, Merissa

    2002-01-01

    Considers that participants in previous deception detection experiments may not have had access to the types of information people most often use to detect real-life lies. Suggests that people most often rely on information from third parties and physical evidence when detecting lies, and that the detection of a lie is a process that takes days,…

  5. What Do Happy People Do?

    ERIC Educational Resources Information Center

    Robinson, John P.; Martin, Steven

    2008-01-01

    Little attention in the quality-of-life literature has been paid to data on the daily activity patterns of happy and less happy people. Using ratings-scale information from time-diary studies, this article examines the hypothesis that people who describe themselves as happier engage in certain activities more than those who describe themselves as…

  6. Carbon Solubility of Molten Sulfides at 2-3 GPa

    NASA Astrophysics Data System (ADS)

    Zhang, Z.; Hirschmann, M. M.

    2012-12-01

    Sulfide is molten through much of Earth's upper mantle and so could have an important influence on geochemical and geophysical properties. For example, liquid sulfide could dissolve appreciable carbon, and thereby be a significant sink for reduced carbon in the mantle and perhaps be associated with carbon transport, including diamond precipitation. Here we present experimental data on the phase relations and carbon solubility of sulfides at 2-3 GPa in graphite capsules. Carbon was analyzed by EMPA using an LDE2 crystal and a 10 kV, 80 nA beam, and secondary steel and carbide standards. Repeated analyses of 99.995 wt% Fe indicate a C blank of 0.47 ± 0.12 wt.% (n=38), which was subtracted from the analyses. The limit of detection is therefore likely near 0.1-0.15 wt.%, but we take a more conservative value of 0.27 wt.%, which is the concentration in NIST C1248 steel, the lowest standard for which we unambiguously measure C. FeS monosulfide melts coexist with crystalline sulfide at 2GPa and 1100°C, and at 3GPa and 1200°C, respectively. Lower temperatures are subsolidus and higher temperatures produce only liquids (+graphite). For Fe-S liquids at 2GPa,1500-1600°C and 3GPa, 1600°C, at low bulk S content (5-10 wt.%), a carbide melt coexists with the sulfide. More sulfur-rich bulk compositions produce two immiscible liquids which are approximately (Fe~93%S2~3%C2~4%) and (Fe~70%S~30%)., but Ni addition diminishes the miscibility gap. Carbon solubility in (Fe0.5,Ni0.5)-S liquids diminishes with decreasing metal/sulfide ratio; up to 10 wt.% S, solubility is 2 wt.% C, but diminishes to <1 wt.% at 15 wt% S and is below detection at >20 wt.% S. At 2GPa and 1600°C, other graphite-saturated monosulfide compositions, (Fe1-x,Nix)S (x=0.33,0.50,0.67), FeCuS2 NiS, CuS, and CoS, dissolve less C than detection limit. We detect <0.5 wt.% C in Ni metal and Cu metal in graphite-saturated compositions. In the shallow mantle, where sulfide liquid approximates monosulfide stoichiometry

  7. Laser-spectroscopy measurement of the fine-structure splitting 2 3P1-2 3P2 of 4He

    NASA Astrophysics Data System (ADS)

    Feng, G.-P.; Zheng, X.; Sun, Y. R.; Hu, S.-M.

    2015-03-01

    Laser spectroscopy has been performed on a beam of neutral 4He atoms. By using transverse laser cooling and focusing, we are able to prepare a bright beam of atoms in the metastable state 2 3S1 deflected from the original effusive atomic beam. The initial state preparation is completed with optical pumping on the 2 3P1←2 3S1 transition at the wavelength of 1083 nm, followed by laser spectroscopy on the 2 3P1 ,2←2 3S1 transitions. The 2 3P1-2 3P2 fine-structure splitting is determined to be 2 291 177.69 ±0.36 kHz . The quantum interference effect is included in data extraction. This is the most precise laser spectroscopy measurement of the interval. Our result is in agreement with both the latest QED-based calculation and the most precise measurement conducted with microwave spectroscopy.

  8. THE CHEMICAL EVOLUTION OF STAR-FORMING GALAXIES OVER THE LAST 11 BILLION YEARS

    SciTech Connect

    Zahid, H. Jabran; Kewley, Lisa J.; Geller, Margaret J.; Hwang, Ho Seong; Fabricant, Daniel G.; Kurtz, Michael J.

    2013-07-10

    We calculate the stellar mass-metallicity relation at five epochs ranging to z {approx} 2.3. We quantify evolution in the shape of the mass-metallicity relation as a function of redshift; the mass-metallicity relation flattens at late times. There is an empirical upper limit to the gas-phase oxygen abundance in star-forming galaxies that is independent of redshift. From examination of the mass-metallicity relation and its observed scatter, we show that the flattening at late times is a consequence of evolution in the stellar mass where galaxies enrich to this empirical upper metallicity limit; there is also evolution in the fraction of galaxies at a fixed stellar mass that enrich to this limit. The stellar mass where metallicities begin to saturate is {approx}0.7 dex smaller in the local universe than it is at z {approx} 0.8.

  9. Accurate molecular structures and infrared spectra of trans-2,3-dideuterooxirane, methyloxirane, and trans-2,3-dimethyloxirane

    SciTech Connect

    Barone, Vincenzo; Biczysko, Malgorzata Bloino, Julien; Puzzarini, Cristina

    2014-07-21

    Oxirane derivatives are the most used benchmarks for chiroptical spectroscopies in view of their small size and relative rigidity. The molecular structure, vibrational harmonic and anharmonic frequencies, and infrared intensities of the ground electronic states are analyzed in this paper. Equilibrium structure and harmonic force fields have been evaluated by means of high-level quantum-chemical calculations at the coupled-cluster level including single and double excitations together with a perturbative treatment of triples (CCSD(T)). Extrapolation to the complete basis-set limit as well as core-correlation effects have also been taken into account. Anharmonic contributions have been computed at the CCSD(T)/cc-pVTZ level for trans-2,3-dideuterooxirane. These data can serve as references to evaluate the accuracy of less expensive computational approaches rooted in the density functional theory (DFT). The latter have been used within hybrid CC/DFT approaches, which have been applied to simulate fully anharmonic infrared (IR) spectra. Finally, the best theoretical estimates of the equilibrium structures and vibrational wavenumbers are compared to the most accurate experimental data and show in all cases very good agreement, i.e., within 0.001 Å, 0.1 deg, 10 cm{sup −1}, and 0.5 km mol{sup −1}, for bond lengths, angles, wavenumbers, and IR intensities, respectively.

  10. People hiring people they can trust. Selecting an architect.

    PubMed

    Luers, J

    1994-01-01

    Julie Luers, F.M.P., vice president, marketing director of Ellerbe Becket Construction Services, writes that hiring a consultant is essentially "buying" people and their skills. She offers tips on how to minimize risks. PMID:10134447

  11. Pharmacokinetics of (-)-2'-3'-dideoxy-3'-thiacytidine in woodchucks.

    PubMed Central

    Rajagopalan, P; Boudinot, F D; Chu, C K; Tennant, B C; Baldwin, B H; Schinazi, R F

    1996-01-01

    The woodchuck (Marmota monax) has proven to be a suitable animal model for studying hepatitis B virus (HBV) infection owing to similarities in the course of infection between woodchuck hepatitis virus (WHV) in woodchucks and HBV in humans. (-)-beta-L-2',3'-Dideoxy-3'-thiacytidine (3TC; lamivudine) is a nucleoside analog which has demonstrated antiviral activity against HBV as well as human immunodeficiency virus (HIV). The purpose of the present investigation was to characterize the pharmacokinetics of 3TC following intravenous and oral administration of 20 mg of 3TC per kg of body weight to woodchucks. Following intravenous administration, the concentrations of 3TC in plasma declined, with a terminal half-life of 2.84 +/- 0.85 h (mean +/- standard deviation). The systemic clearance and steady-state volume of distribution of 3TC were 0.22 +/- 0.078 liters/h/kg and 0.75 +/- 0.13 liters/kg, respectively. The renal clearance of the nucleoside analog was 0.063 +/- 0.016 liters/h/kg. The oral bioavailability of 3TC ranged from 18 to 54%. Allometric relationships between pharmacokinetic parameters and body weight developed by Hussey et al. (E.K. Hussey, K.H. Donn, M.J. Daniel, S.T. Hall, A.J. Harker, and G.L. Evans, J. Clin. Pharmacol. 34:975-977, 1994) were augmented by including data from woodchucks, monkeys (S.M. Blaney, M.J. Daniel, A.J. Harker, K. Godwin, and F.M. Balis, Antimicrob. Agents Chemother. 39:2779-2782, 1995), and additional data from rats (P. Rajagopalan, L. Moore, C.K. Chu, R.F. Schinazi, and F.D. Boudinot, submitted for publication). Interspecies scaling of the pharmacokinetic parameters of 3TC demonstrated a good correlation between clearance (0.74 . W0.76 [where W is body weight]; r = 0.93; P < 0.025), apparent volume of distribution (1.62 . W0.81; r = 0.98; P < 0.005), and steady-state volume of distribution (1.09 . W0.94; r = 0.99; P < 0.05) and species body weight. The allometric relationships for clearance and volume of distribution at steady

  12. Publishing Is For People Too

    ERIC Educational Resources Information Center

    Worpole, Ken

    1974-01-01

    Article described a project which aims to provide publishing and distribution opportunities for people in Hackney who would never think of themselves as within the traditional framework of commercial publishing. (Author/RK)

  13. Resolving Differences with Angry People.

    ERIC Educational Resources Information Center

    Margolis, Howard

    1986-01-01

    Presents a practical framework for those, such as urban education administrators, who must work with angry people. Focuses on the causes of anger, the negotiation process, trust building, problem solving, confrontation strategies and deadlocks. (KH)

  14. Worldwide Discoveries Help People Everywhere

    MedlinePlus

    ... Home Current Issue Past Issues Special Section Worldwide Discoveries Help People Everywhere Past Issues / Spring 2008 Table ... shows examples of discoveries and their impact. Diseases Discoveries The Benefits for All Americans Huntington's Disease Venezuela— ...

  15. Clinical Trials and Older People

    MedlinePlus

    ... have a much wider applicability. Researchers need the participation of older people in their clinical trials so ... contact with questions about the study or your participation. Control group —the group of participants who get ...

  16. Enantioselective synthesis of 2,3-disubstituted trans-2,3-dihydrobenzofurans using a Brønsted base/thiourea bifunctional catalyst.

    PubMed

    Barrios Antúnez, Diego-Javier; Greenhalgh, Mark D; Fallan, Charlene; Slawin, Alexandra M Z; Smith, Andrew D

    2016-07-26

    The diastereo- and enantioselective synthesis of 2,3-disubstituted trans-2,3-dihydrobenzofuran derivatives (15 examples, up to 96 : 4 dr, 95 : 5 er) via intramolecular Michael addition has been developed using keto-enone substrates and a bifunctional tertiary amine-thiourea catalyst. This methodology was extended to include non-activated ketone pro-nucleophiles for the synthesis of 2,3-disubstituted indane and 3,4-disubstituted tetrahydrofuran derivatives. PMID:27387095

  17. Television Programming during "People's Time."

    ERIC Educational Resources Information Center

    Austin, Bruce A.

    A study was initiated to answer questions concerning television programing during "people's time" in a medium-sized market. "People's time" is defined as local prime time from 4:00 p.m. to 8:00 p.m. as contrasted with prime or network time and is considered a time when local broadcasters have an opportunity to serve their audience's…

  18. 2,3,7,8-TCDD, 2,3,7,8-TCDF and PCBs in marine sediments and biota: Laboratory and field studies. Final report

    SciTech Connect

    Pruell, R.J.; Rubinstein, N.I.; Taplin, B.K.; LiVolsi, J.A.; Norwood, C.B.

    1990-09-01

    The report describes the bioaccumulation and depuration of 2,3,7,8-tetrachlorodibenzo-p-dioxin (2,3,7,8-TCDD), 2,3,7,8-tetrachlorodibenzofuran (2,3,7,8-TCDF) and polychlorinated biphenyls (PCBs) by three species of marine benthos exposed to contaminated sediment collected from the Passaic River (PR), New Jersey. Organisms were exposed to PR sediments for up to 180 days in the laboratory. In addition, sediments and associated infauna from the New York Bight were collected and analyzed for the same suite of chemical compounds.

  19. NREL Helps Clean Cities Displace Billions of Gallons of Petroleum, One Vehicle at a Time (Fact Sheet)

    SciTech Connect

    Not Available

    2010-10-01

    With more than 15 years and nearly 3 billion gallons of displaced petroleum under its belt, the Clean Cities program relies on the support and expertise of the National Renewable Energy Laboratory (NREL). An initiative of the U.S. Department of Energy (DOE), Clean Cities creates public-private partnerships with a common mission: to reduce petroleum consumption in the transportation sector. Since the inception of Clean Cities in 1993, NREL has played a central role in supporting the program, an effort that stems from the laboratory's strategy to put scientific innovation into action in the marketplace.

  20. SOLSOURCE 3-IN-1: PROVIDING CLEAN ENERGY TO THE POOREST 2.5 BILLION AT A PRICE THEY CAN AFFORD

    EPA Science Inventory

    We expect this project to have the following impacts on people, prosperity, and the planet:

    People: Decreased indoor air pollution exposures, decreased pathogen transmission, decreased injuries and miscarriages during fuel collection along mountain slopes, increased ...

  1. BIOAVAILABILITY OF 2,3,7,8-TCDD, 2,3,7,8-TCDF AND PCBS TO MARINE BENTHOS FROM PASSAIC RIVER SEDIMENTS

    EPA Science Inventory

    The bioaccumulation and depuration of 2,3,7,8-tetrachloro-dibenzo-p-dioxin, 2,3,7,8-tetrachlorodibenzofuran and polychlorinated biphenyls by marine benthos exposed to environmentally contaminated sediment were measured in a laboratory study. andworms (Nereis virens), clams (Macom...

  2. Synthesis and properties of new derivatives of ethyl 7-methyl-2,4-dioxo-1,2,3,4-tetrahydropyrido [2,3-d]pyrimidine-5-carboxylate.

    PubMed

    Sladowska, H; Bartoszko-Malik, A; Zawisza, T

    1990-01-01

    Condensation of diethyl 2-amino-6-methylpyridine-3,4-dicarboxylate with phenyl or cyclohexyl isocyanates gave the corresponding derivatives of ethyl 7-methyl-2,4-dioxo-1,2,3,4-tetrahydropyrido [2,3-d]pyrimidine- 5-carboxylate[(V), (VI)]. Alkylation of (V) and (VI) afforded the corresponding N-1 substituted derivatives (XI-XIX). PMID:2337441

  3. ICT Interface Design for Ageing People and People with Dementia

    NASA Astrophysics Data System (ADS)

    Wallace, Jonathan; Mulvenna, Maurice D.; Martin, Suzanne; Stephens, Sharon; Burns, William

    Ageing population trends, rising healthcare costs and social and digital inclusion are all factors in the background to the problem of older adults interacting with technology. Approaches to address "physical accessibility" and "access to technology" issues, as well as training for existing systems are evident, yet a usability issue still prevails. The primary aim of this chapter is to provide an overview of the research and literature and discuss the differing contexts in which older people and people with dementia interact with computerised systems and their associated issues.

  4. An age difference of two billion years between a metal-rich and a metal-poor globular cluster.

    PubMed

    Hansen, B M S; Kalirai, J S; Anderson, J; Dotter, A; Richer, H B; Rich, R M; Shara, M M; Fahlman, G G; Hurley, J R; King, I R; Reitzel, D; Stetson, P B

    2013-08-01

    Globular clusters trace the formation history of the spheroidal components of our Galaxy and other galaxies, which represent the bulk of star formation over the history of the Universe. The clusters exhibit a range of metallicities (abundances of elements heavier than helium), with metal-poor clusters dominating the stellar halo of the Galaxy, and higher-metallicity clusters found within the inner Galaxy, associated with the stellar bulge, or the thick disk. Age differences between these clusters can indicate the sequence in which the components of the Galaxy formed, and in particular which clusters were formed outside the Galaxy and were later engulfed along with their original host galaxies, and which were formed within it. Here we report an absolute age of 9.9 ± 0.7 billion years (at 95 per cent confidence) for the metal-rich globular cluster 47 Tucanae, determined by modelling the properties of the cluster's white-dwarf cooling sequence. This is about two billion years younger than has been inferred for the metal-poor cluster NGC 6397 from the same models, and provides quantitative evidence that metal-rich clusters like 47 Tucanae formed later than metal-poor halo clusters like NGC 6397. PMID:23903747

  5. An ultraluminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30.

    PubMed

    Wu, Xue-Bing; Wang, Feige; Fan, Xiaohui; Yi, Weimin; Zuo, Wenwen; Bian, Fuyan; Jiang, Linhua; McGreer, Ian D; Wang, Ran; Yang, Jinyi; Yang, Qian; Thompson, David; Beletsky, Yuri

    2015-02-26

    So far, roughly 40 quasars with redshifts greater than z = 6 have been discovered. Each quasar contains a black hole with a mass of about one billion solar masses (10(9) M Sun symbol). The existence of such black holes when the Universe was less than one billion years old presents substantial challenges to theories of the formation and growth of black holes and the coevolution of black holes and galaxies. Here we report the discovery of an ultraluminous quasar, SDSS J010013.02+280225.8, at redshift z = 6.30. It has an optical and near-infrared luminosity a few times greater than those of previously known z > 6 quasars. On the basis of the deep absorption trough on the blue side of the Lyman-α emission line in the spectrum, we estimate the proper size of the ionized proximity zone associated with the quasar to be about 26 million light years, larger than found with other z > 6.1 quasars with lower luminosities. We estimate (on the basis of a near-infrared spectrum) that the black hole has a mass of ∼1.2 × 10(10) M Sun symbol, which is consistent with the 1.3 × 10(10) M Sun symbol derived by assuming an Eddington-limited accretion rate. PMID:25719667

  6. A spin-down clock for cool stars from observations of a 2.5-billion-year-old cluster.

    PubMed

    Meibom, Søren; Barnes, Sydney A; Platais, Imants; Gilliland, Ronald L; Latham, David W; Mathieu, Robert D

    2015-01-29

    The ages of the most common stars--low-mass (cool) stars like the Sun, and smaller--are difficult to derive because traditional dating methods use stellar properties that either change little as the stars age or are hard to measure. The rotation rates of all cool stars decrease substantially with time as the stars steadily lose their angular momenta. If properly calibrated, rotation therefore can act as a reliable determinant of their ages based on the method of gyrochronology. To calibrate gyrochronology, the relationship between rotation period and age must be determined for cool stars of different masses, which is best accomplished with rotation period measurements for stars in clusters with well-known ages. Hitherto, such measurements have been possible only in clusters with ages of less than about one billion years, and gyrochronology ages for older stars have been inferred from model predictions. Here we report rotation period measurements for 30 cool stars in the 2.5-billion-year-old cluster NGC 6819. The periods reveal a well-defined relationship between rotation period and stellar mass at the cluster age, suggesting that ages with a precision of order 10 per cent can be derived for large numbers of cool Galactic field stars. PMID:25539085

  7. A spin-down clock for cool stars from observations of a 2.5-billion-year-old cluster

    NASA Astrophysics Data System (ADS)

    Meibom, Søren; Barnes, Sydney A.; Platais, Imants; Gilliland, Ronald L.; Latham, David W.; Mathieu, Robert D.

    2015-01-01

    The ages of the most common stars--low-mass (cool) stars like the Sun, and smaller--are difficult to derive because traditional dating methods use stellar properties that either change little as the stars age or are hard to measure. The rotation rates of all cool stars decrease substantially with time as the stars steadily lose their angular momenta. If properly calibrated, rotation therefore can act as a reliable determinant of their ages based on the method of gyrochronology. To calibrate gyrochronology, the relationship between rotation period and age must be determined for cool stars of different masses, which is best accomplished with rotation period measurements for stars in clusters with well-known ages. Hitherto, such measurements have been possible only in clusters with ages of less than about one billion years, and gyrochronology ages for older stars have been inferred from model predictions. Here we report rotation period measurements for 30 cool stars in the 2.5-billion-year-old cluster NGC 6819. The periods reveal a well-defined relationship between rotation period and stellar mass at the cluster age, suggesting that ages with a precision of order 10 per cent can be derived for large numbers of cool Galactic field stars.

  8. Earth's air pressure 2.7 billion years ago constrained to less than half of modern levels

    NASA Astrophysics Data System (ADS)

    Som, Sanjoy M.; Buick, Roger; Hagadorn, James W.; Blake, Tim S.; Perreault, John M.; Harnmeijer, Jelte P.; Catling, David C.

    2016-06-01

    How the Earth stayed warm several billion years ago when the Sun was considerably fainter is the long-standing problem of the `faint young Sun paradox'. Because of negligible O2 and only moderate CO2 levels in the Archaean atmosphere, methane has been invoked as an auxiliary greenhouse gas. Alternatively, pressure broadening in a thicker atmosphere with a N2 partial pressure around 1.6-2.4 bar could have enhanced the greenhouse effect. But fossilized raindrop imprints indicate that air pressure 2.7 billion years ago (Gyr) was below twice modern levels and probably below 1.1 bar, precluding such pressure enhancement. This result is supported by nitrogen and argon isotope studies of fluid inclusions in 3.0-3.5 Gyr rocks. Here, we calculate absolute Archaean barometric pressure using the size distribution of gas bubbles in basaltic lava flows that solidified at sea level ~2.7 Gyr in the Pilbara Craton, Australia. Our data indicate a surprisingly low surface atmospheric pressure of Patm = 0.23 +/- 0.23 (2σ) bar, and combined with previous studies suggests ~0.5 bar as an upper limit to late Archaean Patm. The result implies that the thin atmosphere was rich in auxiliary greenhouse gases and that Patm fluctuated over geologic time to a previously unrecognized extent.

  9. White Light Demonstration of One Hundred Parts per Billion Irradiance Suppression in Air by New Starshade Occulters

    NASA Technical Reports Server (NTRS)

    Levinton, Douglas B.; Cash, Webster C.; Gleason, Brian; Kaiser, Michael J.; Levine, Sara A.; Lo, Amy S.; Schindhelm, Eric; Shipley, Ann F.

    2007-01-01

    A new mission concept for the direct imaging of exo-solar planets called the New Worlds Observer (NWO) has been proposed. The concept involves flying a meter-class space telescope in formation with a newly-conceived, specially-shaped, deployable star-occulting shade several meters across at a separation of some tens of thousands of kilometers. The telescope would make its observations from behind the starshade in a volume of high suppression of incident irradiance from the star around which planets orbit. The required level of irradiance suppression created by the starshade for an efficacious mission is of order 0.1 to 10 parts per billion in broadband light. This paper discusses the experimental setup developed to accurately measure the suppression ratio of irradiance produced at the null position behind candidate starshade forms to these levels. It also presents results of broadband measurements which demonstrated suppression levels of just under 100 parts per billion in air using the Sun as a light source. Analytical modeling of spatial irradiance distributions surrounding the null are presented and compared with photographs of irradiance captured in situ behind candidate starshades.

  10. Compound-specific carbon and hydrogen isotope analysis of sub-parts per billion level waterborne petroleum hydrocarbons

    USGS Publications Warehouse

    Wang, Y.; Huang, Y.; Huckins, J.N.; Petty, J.D.

    2004-01-01

    Compound-specific carbon and hydrogen isotope analysis (CSCIA and CSHIA) has been increasingly used to study the source, transport, and bioremediation of organic contaminants such as petroleum hydrocarbons. In natural aquatic systems, dissolved contaminants represent the bioavailable fraction that generally is of the greatest toxicological significance. However, determining the isotopic ratios of waterborne hydrophobic contaminants in natural waters is very challenging because of their extremely low concentrations (often at sub-parts ber billion, or even lower). To acquire sufficient quantities of polycyclic aromatic hydrocarbons with 10 ng/L concentration for CSHIA, more than 1000 L of water must be extracted. Conventional liquid/liquid or solid-phase extraction is not suitable for such large volume extractions. We have developed a new approach that is capable of efficiently sampling sub-parts per billion level waterborne petroleum hydrocarbons for CSIA. We use semipermeable membrane devices (SPMDs) to accumulate hydrophobic contaminants from polluted waters and then recover the compounds in the laboratory for CSIA. In this study, we demonstrate, under a variety of experimental conditions (different concentrations, temperatures, and turbulence levels), that SPMD-associated processes do not induce C and H isotopic fractionations. The applicability of SPMD-CSIA technology to natural systems is further demonstrated by determining the ??13C and ??D values of petroleum hydrocarbons present in the Pawtuxet River, RI. Our results show that the combined SPMD-CSIA is an effective tool to investigate the source and fate of hydrophobic contaminants in the aquatic environments.

  11. Contributions of tryptophan 2,3-dioxygenase and indoleamine 2,3-dioxygenase to the conversion of D-tryptophan to nicotinamide analyzed by using tryptophan 2,3-dioxygenase-knockout mice.

    PubMed

    Maeta, Akihiro; Sano, Mitsue; Fukuwatari, Tsutomu; Funakoshi, Hiroshi; Nakamura, Toshikazu; Shibata, Katsumi

    2014-01-01

    We investigated the contribution percentage of tryptophan 2,3-dioxygenase (TDO) and indoleamine 2,3-dioxygenase (IDO) to the conversion of D-tryptophan to nicotinamide in TDO-knockout mice. The calculated percentage conversions indicated that TDO and IDO oxidized 70 and 30%, respectively, of the dietary L-tryptophan. These results indicate that both TDO and IDO biosynthesize nicotinamide from D-tryptophan and L-tryptophan in mice. PMID:25035993

  12. Mental health of deaf people.

    PubMed

    Fellinger, Johannes; Holzinger, Daniel; Pollard, Robert

    2012-03-17

    Deafness is a heterogeneous condition with far-reaching effects on social, emotional, and cognitive development. Onset before language has been established happens in about seven per 10,000 people. Increased rates of mental health problems are reported in deaf people. Many regard themselves as members of a cultural minority who use sign language. In this Review, we describe discrepancies between a high burden of common mental health disorders and barriers to health care. About a quarter of deaf individuals have additional disabilities and a high probability of complex mental health needs. Research into factors affecting mental health of deaf children shows that early access to effective communication with family members and peers is desirable. Improved access to health and mental health care can be achieved by provision of specialist services with professionals trained to directly communicate with deaf people and with sign-language interpreters. PMID:22423884

  13. "Peoples's Education" in the People's Republic of China.

    ERIC Educational Resources Information Center

    Su, Zhixin

    1989-01-01

    "People's education" in China is rooted in the mass education movement lasting from the 1920s to the 1940s. This article summarizes the Chinese educational system from 1949 to present-day reform efforts. Traditional spoon-feeding and rote learning must yield to a system encouraging sef-understanding and independent, innovative, and critical…

  14. 9 CFR 2.3 - Demonstration of compliance with standards and regulations.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 9 Animals and Animal Products 1 2011-01-01 2011-01-01 false Demonstration of compliance with standards and regulations. 2.3 Section 2.3 Animals and Animal Products ANIMAL AND PLANT HEALTH INSPECTION SERVICE, DEPARTMENT OF AGRICULTURE ANIMAL WELFARE REGULATIONS Licensing § 2.3 Demonstration of...

  15. 9 CFR 2.3 - Demonstration of compliance with standards and regulations.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... 9 Animals and Animal Products 1 2010-01-01 2010-01-01 false Demonstration of compliance with standards and regulations. 2.3 Section 2.3 Animals and Animal Products ANIMAL AND PLANT HEALTH INSPECTION SERVICE, DEPARTMENT OF AGRICULTURE ANIMAL WELFARE REGULATIONS Licensing § 2.3 Demonstration of...

  16. 10 CFR 960.3-2-3 - Recommendation of sites for characterization.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... 10 Energy 4 2010-01-01 2010-01-01 false Recommendation of sites for characterization. 960.3-2-3 Section 960.3-2-3 Energy DEPARTMENT OF ENERGY GENERAL GUIDELINES FOR THE PRELIMINARY SCREENING OF POTENTIAL SITES FOR A NUCLEAR WASTE REPOSITORY Implementation Guidelines § 960.3-2-3 Recommendation of...

  17. 10 CFR 960.3-2-3 - Recommendation of sites for characterization.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 10 Energy 4 2011-01-01 2011-01-01 false Recommendation of sites for characterization. 960.3-2-3 Section 960.3-2-3 Energy DEPARTMENT OF ENERGY GENERAL GUIDELINES FOR THE PRELIMINARY SCREENING OF POTENTIAL SITES FOR A NUCLEAR WASTE REPOSITORY Implementation Guidelines § 960.3-2-3 Recommendation of...

  18. 45 CFR 2.3 - Policy on Presentation of testimony and production of documents.

    Code of Federal Regulations, 2010 CFR

    2010-10-01

    ... 45 Public Welfare 1 2010-10-01 2010-10-01 false Policy on Presentation of testimony and production of documents. 2.3 Section 2.3 Public Welfare DEPARTMENT OF HEALTH AND HUMAN SERVICES GENERAL... PARTY § 2.3 Policy on Presentation of testimony and production of documents. No employee or...

  19. 40 CFR 721.6000 - Tris (2,3-dibromopropyl) phosphate.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... 40 Protection of Environment 30 2010-07-01 2010-07-01 false Tris (2,3-dibromopropyl) phosphate... Substances § 721.6000 Tris (2,3-dibromopropyl) phosphate. (a) Chemical substance and significant new use subject to reporting. (1) The chemical substance tris (2,3-dibromopropyl) phosphate (CAS Number...

  20. 40 CFR 721.6000 - Tris (2,3-dibromopropyl) phosphate.

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... 40 Protection of Environment 31 2011-07-01 2011-07-01 false Tris (2,3-dibromopropyl) phosphate... Substances § 721.6000 Tris (2,3-dibromopropyl) phosphate. (a) Chemical substance and significant new use subject to reporting. (1) The chemical substance tris (2,3-dibromopropyl) phosphate (CAS Number...

  1. 49 CFR 177.841 - Division 6.1 and Division 2.3 materials.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... 49 Transportation 2 2011-10-01 2011-10-01 false Division 6.1 and Division 2.3 materials. 177.841... PUBLIC HIGHWAY Loading and Unloading § 177.841 Division 6.1 and Division 2.3 materials. (See also § 177... by other appropriate method, and the marking removed. (b) (c) Division 2.3 (poisonous gas)...

  2. Genome Sequence of meso-2,3-Butanediol-Producing Strain Serratia marcescens ATCC 14041

    PubMed Central

    Li, Lixiang; Wang, Yu; Li, Kun; Su, Fei; Ma, Cuiqing

    2014-01-01

    Serratia marcescens strain ATCC 14041 was found to be an efficient meso-2,3-butanediol (meso-2,3-BD) producer from glucose and sucrose. Here we present a 5.0-Mb assembly of its genome. We have annotated 4 coding sequences (CDSs) for meso-2,3-BD fermentation and 2 complete operons including 6 CDSs for sucrose utilization. PMID:24948764

  3. CARDIOPATHIC EFFECT OF 1,2,3-TRICHLOROPROPANE AFTER SUBACUTE AND SUBCHRONIC EXPOSURE IN RATS

    EPA Science Inventory

    1,2,3-Trichloropropane (1,2,3-TCP) is an industrial water contaminant with potential for human exposure by the oral route. The systemic toxicology of 1,2,3-TCP was evaluated after subacute or subchronic exposure in male and female Sprague Dawley rate. Animals were treated with 0....

  4. 10 CFR 960.3-2-3 - Recommendation of sites for characterization.

    Code of Federal Regulations, 2012 CFR

    2012-01-01

    ... 10 Energy 4 2012-01-01 2012-01-01 false Recommendation of sites for characterization. 960.3-2-3 Section 960.3-2-3 Energy DEPARTMENT OF ENERGY GENERAL GUIDELINES FOR THE PRELIMINARY SCREENING OF POTENTIAL SITES FOR A NUCLEAR WASTE REPOSITORY Implementation Guidelines § 960.3-2-3 Recommendation of...

  5. 10 CFR 960.3-2-3 - Recommendation of sites for characterization.

    Code of Federal Regulations, 2014 CFR

    2014-01-01

    ... 10 Energy 4 2014-01-01 2014-01-01 false Recommendation of sites for characterization. 960.3-2-3 Section 960.3-2-3 Energy DEPARTMENT OF ENERGY GENERAL GUIDELINES FOR THE PRELIMINARY SCREENING OF POTENTIAL SITES FOR A NUCLEAR WASTE REPOSITORY Implementation Guidelines § 960.3-2-3 Recommendation of...

  6. 10 CFR 960.3-2-3 - Recommendation of sites for characterization.

    Code of Federal Regulations, 2013 CFR

    2013-01-01

    ... 10 Energy 4 2013-01-01 2013-01-01 false Recommendation of sites for characterization. 960.3-2-3 Section 960.3-2-3 Energy DEPARTMENT OF ENERGY GENERAL GUIDELINES FOR THE PRELIMINARY SCREENING OF POTENTIAL SITES FOR A NUCLEAR WASTE REPOSITORY Implementation Guidelines § 960.3-2-3 Recommendation of...

  7. 1 CFR 2.3 - Office of the Federal Register; location; office hours.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 1 General Provisions 1 2011-01-01 2011-01-01 false Office of the Federal Register; location; office hours. 2.3 Section 2.3 General Provisions ADMINISTRATIVE COMMITTEE OF THE FEDERAL REGISTER GENERAL GENERAL INFORMATION § 2.3 Office of the Federal Register; location; office hours. (a) The Office of...

  8. 1 CFR 2.3 - Office of the Federal Register; location; office hours.

    Code of Federal Regulations, 2013 CFR

    2013-01-01

    ... 1 General Provisions 1 2013-01-01 2012-01-01 true Office of the Federal Register; location; office hours. 2.3 Section 2.3 General Provisions ADMINISTRATIVE COMMITTEE OF THE FEDERAL REGISTER GENERAL GENERAL INFORMATION § 2.3 Office of the Federal Register; location; office hours. (a) The Office of...

  9. 1 CFR 2.3 - Office of the Federal Register; location; office hours.

    Code of Federal Regulations, 2014 CFR

    2014-01-01

    ... 1 General Provisions 1 2014-01-01 2012-01-01 true Office of the Federal Register; location; office hours. 2.3 Section 2.3 General Provisions ADMINISTRATIVE COMMITTEE OF THE FEDERAL REGISTER GENERAL GENERAL INFORMATION § 2.3 Office of the Federal Register; location; office hours. (a) The Office of...

  10. 1 CFR 2.3 - Office of the Federal Register; location; office hours.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... 1 General Provisions 1 2010-01-01 2010-01-01 false Office of the Federal Register; location; office hours. 2.3 Section 2.3 General Provisions ADMINISTRATIVE COMMITTEE OF THE FEDERAL REGISTER GENERAL GENERAL INFORMATION § 2.3 Office of the Federal Register; location; office hours. (a) The Office of...

  11. 1 CFR 2.3 - Office of the Federal Register; location; office hours.

    Code of Federal Regulations, 2012 CFR

    2012-01-01

    ... 1 General Provisions 1 2012-01-01 2012-01-01 false Office of the Federal Register; location; office hours. 2.3 Section 2.3 General Provisions ADMINISTRATIVE COMMITTEE OF THE FEDERAL REGISTER GENERAL GENERAL INFORMATION § 2.3 Office of the Federal Register; location; office hours. (a) The Office of...

  12. 40 CFR 721.6000 - Tris (2,3-dibromopropyl) phosphate.

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... 40 Protection of Environment 32 2013-07-01 2013-07-01 false Tris (2,3-dibromopropyl) phosphate... Substances § 721.6000 Tris (2,3-dibromopropyl) phosphate. (a) Chemical substance and significant new use subject to reporting. (1) The chemical substance tris (2,3-dibromopropyl) phosphate (CAS Number...

  13. 40 CFR 721.6000 - Tris (2,3-dibromopropyl) phosphate.

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... 40 Protection of Environment 32 2012-07-01 2012-07-01 false Tris (2,3-dibromopropyl) phosphate... Substances § 721.6000 Tris (2,3-dibromopropyl) phosphate. (a) Chemical substance and significant new use subject to reporting. (1) The chemical substance tris (2,3-dibromopropyl) phosphate (CAS Number...

  14. 40 CFR 721.6000 - Tris (2,3-dibromopropyl) phosphate.

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... 40 Protection of Environment 31 2014-07-01 2014-07-01 false Tris (2,3-dibromopropyl) phosphate... Substances § 721.6000 Tris (2,3-dibromopropyl) phosphate. (a) Chemical substance and significant new use subject to reporting. (1) The chemical substance tris (2,3-dibromopropyl) phosphate (CAS Number...

  15. Metabolism of 1,2,3,4-, 1,2,3,5-, and 1,2,4,5-tetrachlorobenzene in the squirrel monkey

    SciTech Connect

    Schwartz, H.; Chu, I.; Villeneuve, D.C.; Benoit, F.M.

    1987-01-01

    The metabolism of three tetrachlorobenzene isomers (TeCB) was investigated in the squirrel monkey. The animals were administered orally 6 single doses of /sup 14/C-labeled 1,2,3,4-, 1,2,4,5-, or 1,2,3,5-tetrachlorobenzene over a 3-wk period at levels ranging from 50 to 100 mg/kg body weight (b.w) and kept in individual metabolism cages to collect urine and feces for radioassay. Approximately 38% (1,2,3,4-TeCB), 36% (1,2,3,5-TeCB), and 18% (1,2,4,5-TeCB) of the doses were excreted respectively in the feces 48 h post administration. In monkeys dosed with 1,2,3,4-TeCB, unchanged compound accounted for 50% of the fecal radioactivity. Unchanged compound accounted for more than 50% of the fecal radioactivity found in the monkeys dosed with 1,2,3,5-TeCB. The fecal metabolites were identified in both groups. No metabolites were detected in the feces of monkeys dosed with 1,2,4,5-TeCB. While the fecal route represented the major route of excretion for 1,2,3,4-TeCB, the other two isomers were eliminated exclusively in the feces. The above data in the squirrel monkey are different from those obtained with the rat and the rabbit, and demonstrate the different metabolic pathways for the isomers.

  16. People

    NASA Astrophysics Data System (ADS)

    2002-11-01

    Featuring relationships, personalities, interactions, environments and reputations involved in physics and education ON THE MAP (543) Problems and solutions for high school physics in Turkey Mevlut Dogan, Bekir Oruncak and Ilhan Gunbayi PERSONALITY (546) Neil Linford - archaeologist with a specialism in geophysics Kerry Parker talks to Neil Linford, archaeological geophysicist STARTING OUT (548) Physics to avoid daytime TV? Victoria Marie Folgate What Katie did next Katie Pennicott TEACHING ANECDOTES (550) Ernest Rutherford

  17. People

    NASA Astrophysics Data System (ADS)

    2001-07-01

    Exploring Mercury PhD student Mark Bentley explains how and why he got involved Mark Bentley is studying for a PhD in planetary science. He is helping to design and build instruments for a forthcoming ESA mission to explore the surface of Mercury. Mark Bentley Space has excited and inspired me for as long as I can remember; my earliest memory of this is being allowed to stay up 'really late' to watch the Space Shuttle Columbia land in 1981, at the age of five. Science in general has always interested me. Although I probably didn't recognize it as such at the time, my fascination with collecting all sorts of equipment (or as my parents called it, 'junk') and finding out what made them tick was an early demonstration of this. At school it seemed natural to take science subjects (Physics, Chemistry and Maths A-levels) and then to consider University though physics was not my first thought. I was all set for the respectable career of computer science, not realizing that my space interests could lead anywhere, until I flicked through the first prospectus I received. By luck it was from Leicester University, and while computer science was offered it also had something called 'Physics with Space Science and Technology'. The rest, as they say, is history... After graduating I spent the following two years working for a UK company developing satellite simulators. But then I started thinking about doing a PhD attracted by the flexibility of directing my own research. I knew that I wanted something that involved space science and the element of discovery, but also something that looked at the engineering and technology of a space mission. The timing was fortuitous shortly after I committed myself to a PhD, the European Space Agency announced the selection of BepiColombo, a mission to Mercury, as one of its 'Cornerstone' (large scale) missions. Here was a mission big on science (no spacecraft has ever orbited Mercury, let alone landed on it) and technology as well! So that takes me to where I am now in my first year at the Planetary and Space Sciences Research Institute of the Open University in Milton Keynes. If everything goes according to plan, three years later I will be Dr Bentley and know a whole lot more about Mercury! So what am I now? A physicist at heart, but I guess 'planetary scientist' is more accurate... The great thing about studying the planets is that the field can be stretched to encompass just about any aspect of science you care to choose from biology, through engineering, to physics and more. Planetary science fits well with the modern 'trend' for multidisciplinary research as well as being on the leading edge of modern science, and one of the most international areas of study. In studying our solar system we aim to learn more about the processes that formed the planets and ultimately life itself. For the foreseeable future the nine major bodies and their associated moons are our only glimpse back in time to the early life of our corner of the Universe. Over the past few decades, a relatively short period of time, we have expanded our understanding of the planets by orders of magnitude. Instruments like the Hubble Space Telescope have enabled more and more detailed images of both the near and far, whilst robotic space probes have extended scientists' senses to the far corners of the solar system. The two least studied planets lie at the two extreme ends of our system. Pluto sits at the outer edges of the solar system, a small icy ball that astronomers even argue about calling a planet. Mercury, messenger of the Gods, is a relative inferno, closer to the Sun than any other body. Mercury is not an easy target for spacecraft. Tucked deep in the Sun's gravitational well, any mission must lose about 60% of its orbital energy in order to match Mercury's orbit. The only spacecraft to visit Mercury to date was Mariner 10, a NASA mission flown in the mid-70s. It had far too much energy to enter orbit and could just make several quick passes, leaving an incomplete image of only half of the planet. This, and observations m

  18. People

    NASA Astrophysics Data System (ADS)

    2002-07-01

    Featuring relationships, personalities, interactions, environments and reputations involved in physics and education PERSONALITY (350) The Importance of Being Brenda Steven Chapman talks to Brenda Jennison, trainer of physics teachers TEACHING ANECDOTES (352) Dorothy Crowfoot Hodgkin

  19. People

    NASA Astrophysics Data System (ADS)

    2003-09-01

    STARTING OUT (447) What Katie did next: part 6 Katie Pennicott TEACHING ANECDOTES (447) Hertha Ayrton PERSONALITY (448) Hungarian teachers with suitcases full of 'treasures’ Katalin Papp and Anett Nagy Correction (451)

  20. People

    NASA Astrophysics Data System (ADS)

    2002-09-01

    Featuring relationships, personalities, interactions, environments and reputations involved in physics and education PERSONALITY (446) A choice of Materials Bernard Taylor talks to Diane Talbot, Materials Education Coordinator at the Institute of Materials, Minerals and Mining TEACHING ANECDOTES (447) H G Wells ON THE MAP (448) Gordano school - crowded with physics teachers

  1. People

    NASA Astrophysics Data System (ADS)

    2003-01-01

    Featuring relationships, personalities, interactions, environments and reputations involved in physics and education TEACHING ANECDOTES (66) Paul Adrien Maurice Dirac OPINIONS (67) Recommended reading of science fiction Ken Zetie STARTING OUT (70) What Katie did next: part 2 Katie Pennicott

  2. People

    NASA Astrophysics Data System (ADS)

    2003-07-01

    PERSONALITY (340) What makes a good teacher? Bob Kibble PERSONALITY (342) Here’s to you, Mrs Wilson Steven Chapman TEACHING ANECDOTES (343) Marie Curie STARTING OUT (344) What Katie did next: part 5 Katie Pennicott MY FAVOURITE DEMO (345) Make your own rainbow Rick Marshall

  3. People

    NASA Astrophysics Data System (ADS)

    2008-05-01

    INTERVIEW Interview: How Google conquered the sky Carol Christian and Alberto Conti work at the Space Telescope Science Institute (the home of Hubble) in Baltimore and co-created Sky in Google Earth. David Smith spoke to them between stage appearances at Astrofest

  4. People

    NASA Astrophysics Data System (ADS)

    2002-05-01

    Featuring relationships, personalities, interactions, environments and reputations involved in physics and education ON THE MAP (264) Kharkiv National University of Radioelectronics, Ukraine Kerry Parker STARTING OUT (265) Preparation, preparation, preparation Steven Chapman TEACHING ANECDOTES (266) Lise Meitner PERSONALITY (267) The Accidental Astronomer Kerry Parker talks to Marie Radbo, Astronomer

  5. People

    NASA Astrophysics Data System (ADS)

    2001-03-01

    How and why we teach An interview with Mick Nott conducted by David Sang Mick Nott teaches at Sheffield Hallam University. He is editor of School Science Review, and over the last three years he has been organizing a website, book and display for the ASE's Science Teacher Festival. Mick Nott You studied Logic with Physics as your undergraduate degree course, at Sussex, at the end of the 1960s. Wasn't this a rather unusual choice? At school, I loved chemistry, particularly physical chemistry. However, physical chemistry didn't love me when I studied it at university. I grew resentful of the demands made on me with the overcrowded morning lecture programme that was mainly a board-copying exercise and the afternoon hours of labs. I felt stifled; there didn't seem to be any space to express oneself. I wanted a course that allowed me some freedom of thought. So in the summer of 1969 I transferred to the Logic with Physics course. Alongside our 'straight' physics we studied the history of topics like atomic and quantum theory, thermodynamics, mechanics from the Greeks to the Newtonian synthesis and we also had a couple of units in the sociology of science. Amongst the set texts of our first class in the summer of 1969 was Thomas Kuhn's The Structure of Scientific Revolutions. Now well worn with its cover repaired by sticky tape, it still rests on my bookshelves. Reading Kuhn, I understood why I had been dissatisfied with my chemistry course. If I wanted to make it in chemistry I was going to have to conform to thinking exactly like all the other chemists. That wasn't for me. What attracted you into teaching? And where did you teach? I think it was a vocation in that, from the age of 15, I could imagine myself in the role and it was a job I could 'see' myself doing. Now thinking back I suppose it was an obvious way in which a working class child could transcend class barriers. I did my postgraduate teacher training at Sussex because it was assessed by coursework and classroom competence (in the early 1970s most such courses still had written examinations). I thought it was fantastic. We spent three days a week from October to May in one school. I had one regular third-year class every week and the rest of my teaching timetable varied from term to term. It was like being a 0.3/0.4 member of staff and for that one third-year class I had to do parents' evenings, reports etc. The teachers were paid to act as tutors for the preparation of schemes of work, lessons and tutorial work and they assessed my teaching. Teachers, tutors and trainees attended seminars together. My first teaching job was at Holland Park School in London, at a time when it was famous, perhaps even infamous! It was a real baptism of fire - over 2000 pupils, tens of different first languages, a real mix of class and ethnicity, and newly introduced mixed ability teaching for the first three years. We worked very hard writing schemes of work and developing worksheets and audiovisual materials but, on reflection, I am not sure that we were that effective in developing the science curriculum. I remember using Nuffield Combined Science with the first two years and that was in danger of becoming death by a thousand worksheets. After three years I went to teach in a small private school in Madrid for a year. I was the physics department and my title of Head of Physics meant I was in charge of myself. This was highly formative as a teacher - I had nobody to ask if I didn't understand some physics. As the school was poorly equipped I learned to make apparatus and be very resourceful. There was no pupils' practical work in school science in Spain at that time and I spent a lot of time in hardware stores and medical suppliers! After Spain all of my teaching career was in 11-18 mixed comprehensives, in Cheshire and then Peterborough, and I rose to the dizzy heights of Head of Science. By the time I left the school in Peterborough in 1986 we had established the curriculum framework for broad and balanced science for all to age 16. Did your undergraduate studies influence the

  6. People

    NASA Astrophysics Data System (ADS)

    2005-07-01

    WORLD YEAR OF PHYSICS Physics around the world: America Julio Benegas, Don Metz, Jesús Vázquez-Abad, Eduardo Molto, Josip Slisko and Rick Holmes INTERVIEW Things can only get better: a rock star tells of his hopes for popular physics David Smith talks to Brian Cox

  7. People

    NASA Astrophysics Data System (ADS)

    2005-01-01

    WORLD YEAR OF PHYSICS Around the world with physics Stuart Farmer; Leopold Mathelitsch; Rita Wodzinski and Michael Vollmer; Finn Ingebretsen; Mojca Cepic, Gorazd Planinsic and Mirko Cvahte; Ann-Marie Pendrill; Rajka Jurdana-Sepic INTERVIEW Close encounters of the cosmic kind David Smith talks to Frank Close BIOGRAPHIES Meet Physics Education’s family Steven Chapman and Andrea Pomroy

  8. People

    NASA Astrophysics Data System (ADS)

    2005-03-01

    WORLD YEAR OF PHYSICS Physics around the world: Asia Shinjiro Ogawa, Mak Se-yuen and R Subramaniam INTERVIEW Weather forecasting: a bright outlook with high chance of using your physics David Smith talks to Will Lang BIOGRAPHIES Let me introduce you: more members of the extended Physics Education family Clare Thomson and Alan Evans

  9. People

    NASA Astrophysics Data System (ADS)

    2008-03-01

    INTERVIEW Interview: Earth science gets to the core Some 20 years ago, Prof. G David Price was one of the first to establish the now major field of computational mineral physics. He combines experiment, theory and modelling to tackle major deep Earth science problems. He is vice-provost for research and professor of mineral physics at UCL. David Smith quizzed him on behalf of Physics Education.

  10. People

    NASA Astrophysics Data System (ADS)

    2001-03-01

    How and why we teach An interview with Mick Nott conducted by David Sang Mick Nott teaches at Sheffield Hallam University. He is editor of School Science Review, and over the last three years he has been organizing a website, book and display for the ASE's Science Teacher Festival. Mick Nott You studied Logic with Physics as your undergraduate degree course, at Sussex, at the end of the 1960s. Wasn't this a rather unusual choice? At school, I loved chemistry, particularly physical chemistry. However, physical chemistry didn't love me when I studied it at university. I grew resentful of the demands made on me with the overcrowded morning lecture programme that was mainly a board-copying exercise and the afternoon hours of labs. I felt stifled; there didn't seem to be any space to express oneself. I wanted a course that allowed me some freedom of thought. So in the summer of 1969 I transferred to the Logic with Physics course. Alongside our 'straight' physics we studied the history of topics like atomic and quantum theory, thermodynamics, mechanics from the Greeks to the Newtonian synthesis and we also had a couple of units in the sociology of science. Amongst the set texts of our first class in the summer of 1969 was Thomas Kuhn's The Structure of Scientific Revolutions. Now well worn with its cover repaired by sticky tape, it still rests on my bookshelves. Reading Kuhn, I understood why I had been dissatisfied with my chemistry course. If I wanted to make it in chemistry I was going to have to conform to thinking exactly like all the other chemists. That wasn't for me. What attracted you into teaching? And where did you teach? I think it was a vocation in that, from the age of 15, I could imagine myself in the role and it was a job I could 'see' myself doing. Now thinking back I suppose it was an obvious way in which a working class child could transcend class barriers. I did my postgraduate teacher training at Sussex because it was assessed by coursework and classroom competence (in the early 1970s most such courses still had written examinations). I thought it was fantastic. We spent three days a week from October to May in one school. I had one regular third-year class every week and the rest of my teaching timetable varied from term to term. It was like being a 0.3/0.4 member of staff and for that one third-year class I had to do parents' evenings, reports etc. The teachers were paid to act as tutors for the preparation of schemes of work, lessons and tutorial work and they assessed my teaching. Teachers, tutors and trainees attended seminars together. My first teaching job was at Holland Park School in London, at a time when it was famous, perhaps even infamous! It was a real baptism of fire - over 2000 pupils, tens of different first languages, a real mix of class and ethnicity, and newly introduced mixed ability teaching for the first three years. We worked very hard writing schemes of work and developing worksheets and audiovisual materials but, on reflection, I am not sure that we were that effective in developing the science curriculum. I remember using Nuffield Combined Science with the first two years and that was in danger of becoming death by a thousand worksheets. After three years I went to teach in a small private school in Madrid for a year. I was the physics department and my title of Head of Physics meant I was in charge of myself. This was highly formative as a teacher - I had nobody to ask if I didn't understand some physics. As the school was poorly equipped I learned to make apparatus and be very resourceful. There was no pupils' practical work in school science in Spain at that time and I spent a lot of time in hardware stores and medical suppliers! After Spain all of my teaching career was in 11-18 mixed comprehensives, in Cheshire and then Peterborough, and I rose to the dizzy heights of Head of Science. By the time I left the school in Peterborough in 1986 we had established the curriculum framework for broad and balanced science for all to age 16. Did your undergraduate studies influence the way you taught science? I think they made me think critically about my teaching right from the start. Although there was much that I admired in the Nuffield approach, I felt that it was unrealistic to expect pupils to discover the whole of Physics for themselves in the time available! In 1973, 'Learning by discovery' was the slogan. My first lesson on my own was with a class of 32 children and 16 brightly illuminated ripple tanks in a dim laboratory. The pupils' task was to 'discover' that v = fλ. The familiar cry, 'What's supposed to happen, Sir?' arose around the room. At the end, as I removed the crocodile clips the pupils had stuck on my jacket, I had to tell them what the result should have been. Nowadays I am convinced that science has to be taught as well as it has to be learned. I don't go along with the teacher as solely a 'facilitator' of learning and the learning environment. Schooling is an enculturation into ways of thinking and important things to know. Teachers have a responsibility to set an agenda for their pupils, e.g. what is important for pupils to learn, why is it important and how does it contribute pupils' personal and social development as well as their potential development as a scientist. You played a big role in the Secondary Science Curriculum Review (SSCR) in the 1980s. What impact did that experience have on you? The SSCR started off as a democratic experiment, trying to 'hand' science curriculum development to class teachers. I worked for the project as an advisory teacher for a year developing problem-solving as a teaching strategy in lower secondary school science. I think the SSCR was crucial to the successful launching of broad and balanced science and the political battle to establish science as a core subject. Can you still discern the influence of the SSCR in today's National Curriculum? I don't think the present science curriculum is what the SSCR envisaged. However, many projects which were partly products of SSCR have had a profound impact (for example the CLIS project Suffolk Coordinated Science and NEAB Modular Science). I welcomed the inclusion of an attainment target on the nature of science (AT17) in the first version of the National Curriculum but it soon became weakened when the Science National Curriculum was revised. However, I think that some aspects have resurfaced in the new emphasis on ideas and evidence. I was involved in the writing of the Nuffield report, Beyond 2000: Science education for the future, and I think this has had an impact at the policy level, but its suggested strategies were not 'periphery to centre' which was the slogan of the SSCR. At Sheffield Hallam University, you have been involved in initial teacher training and you have also taught on undergraduate physics courses. What are your areas of interest in teaching and research today? I am interested in the history and culture of science education: Why do we teach science in the way we do? What are the roots of today's science curriculum? Knowing what we know about the past, how can we develop things in the future? You are now organizing the Science Teacher Festival, celebrating 100 years of the ASE and its forerunners. What made you think this was worth doing? There is an old saying that if we forget our history, we will be condemned to relive it, and I think it was Marx who said that there is no point in studying your past if you are not going to use it to change the future. Looking back through past decades of School Science Review, Physics Education and other journals, you can see the same arguments arising time and again - for example, can pupils learn their science through discovery/problem-solving/investigations? what methods of assessment match our science teaching objectives? should science be taught as general/integrated/separate sciences? These arguments have been with us throughout the past century and the 'winners' and 'losers' rise and fall! I think that to be a profession, we need to recognize our heritage and tradition. At the moment I get the impression that every year is Year Zero as some 'new' initiative starts. We can learn from the past, and next time we try an idea we should take it further, research it deeper and disseminate it wider than we did before.

  11. People

    NASA Astrophysics Data System (ADS)

    2007-05-01

    INTERVIEW From poetry to energy research David Smith talks to John Constable, policy and research director for the Renewable Energy Foundation (REF), a charity providing comment and analysis on the energy sector.

  12. People

    NASA Astrophysics Data System (ADS)

    2007-03-01

    INTERVIEW Lightning strikes in Boston Michael Alexander, the director of public programs at the Boston Museum of Science, talks to David Smith about how to deal with issues and subjects that are difficult to present using more traditional museum methods.

  13. People

    NASA Astrophysics Data System (ADS)

    2002-03-01

    Featuring relationships, personalities, interactions, environments and reputations involved in physics and education ON THE MAP (160) Greenhead College: getting great A-level results Kerry Parker PERSONALITY (161) Physics, sex and politics Lynda Williams, the Physics Chanteuse TEACHING ANECDOTES (163) Yuri Gagarin

  14. People

    NASA Astrophysics Data System (ADS)

    2001-01-01

    Featuring relationships, personalities, interactions, environments and reputations involved in physics and education STARTING OUT (81) DATA: Developing students' abilities to teach astronomy Ruth Jarman and Billy McClune PERSONALITY (82) Music, Creativity and Physics Wendy Sadler Correction: Printed copies of Physics Education contain an incorrect version of this Personality article. The PDF file here contains the correct version. The Editor and publishers apologise to Ms Sadler for the error. Further details will appear in the next issue. ON THE MAP (84) Spreading the resources: South Africa and India Charlie Milward

  15. People

    NASA Astrophysics Data System (ADS)

    2008-11-01

    INTERVIEW Dedicated to Galileo's legacy In 2009 the world will celebrate the International Year of Astronomy to commemorate the 400th anniversary of Galileo's use of a telescope to study the night sky. Galileo scholar Thomas B Settle, guest at the Institute and Museum of the History of Science in Florence, talks to David Smith about the Tuscan hero.

  16. People

    NASA Astrophysics Data System (ADS)

    2001-07-01

    Exploring Mercury PhD student Mark Bentley explains how and why he got involved Mark Bentley is studying for a PhD in planetary science. He is helping to design and build instruments for a forthcoming ESA mission to explore the surface of Mercury. Mark Bentley Space has excited and inspired me for as long as I can remember; my earliest memory of this is being allowed to stay up 'really late' to watch the Space Shuttle Columbia land in 1981, at the age of five. Science in general has always interested me. Although I probably didn't recognize it as such at the time, my fascination with collecting all sorts of equipment (or as my parents called it, 'junk') and finding out what made them tick was an early demonstration of this. At school it seemed natural to take science subjects (Physics, Chemistry and Maths A-levels) and then to consider University though physics was not my first thought. I was all set for the respectable career of computer science, not realizing that my space interests could lead anywhere, until I flicked through the first prospectus I received. By luck it was from Leicester University, and while computer science was offered it also had something called 'Physics with Space Science and Technology'. The rest, as they say, is history... After graduating I spent the following two years working for a UK company developing satellite simulators. But then I started thinking about doing a PhD attracted by the flexibility of directing my own research. I knew that I wanted something that involved space science and the element of discovery, but also something that looked at the engineering and technology of a space mission. The timing was fortuitous shortly after I committed myself to a PhD, the European Space Agency announced the selection of BepiColombo, a mission to Mercury, as one of its 'Cornerstone' (large scale) missions. Here was a mission big on science (no spacecraft has ever orbited Mercury, let alone landed on it) and technology as well! So that takes me to where I am now in my first year at the Planetary and Space Sciences Research Institute of the Open University in Milton Keynes. If everything goes according to plan, three years later I will be Dr Bentley and know a whole lot more about Mercury! So what am I now? A physicist at heart, but I guess 'planetary scientist' is more accurate... The great thing about studying the planets is that the field can be stretched to encompass just about any aspect of science you care to choose from biology, through engineering, to physics and more. Planetary science fits well with the modern 'trend' for multidisciplinary research as well as being on the leading edge of modern science, and one of the most international areas of study. In studying our solar system we aim to learn more about the processes that formed the planets and ultimately life itself. For the foreseeable future the nine major bodies and their associated moons are our only glimpse back in time to the early life of our corner of the Universe. Over the past few decades, a relatively short period of time, we have expanded our understanding of the planets by orders of magnitude. Instruments like the Hubble Space Telescope have enabled more and more detailed images of both the near and far, whilst robotic space probes have extended scientists' senses to the far corners of the solar system. The two least studied planets lie at the two extreme ends of our system. Pluto sits at the outer edges of the solar system, a small icy ball that astronomers even argue about calling a planet. Mercury, messenger of the Gods, is a relative inferno, closer to the Sun than any other body. Mercury is not an easy target for spacecraft. Tucked deep in the Sun's gravitational well, any mission must lose about 60% of its orbital energy in order to match Mercury's orbit. The only spacecraft to visit Mercury to date was Mariner 10, a NASA mission flown in the mid-70s. It had far too much energy to enter orbit and could just make several quick passes, leaving an incomplete image of only half of the planet. This, and observations made from Earth, provide almost all of our knowledge of Mercury. Earth observations, however, are hampered by the planet's proximity to the Sun, making observations possible only at dawn and dusk. A mosaic of images of Mercury from the NASA Mariner 10 spacecraft. ©NASA In the mid-80s improved radar equipment allowed high resolution mapping of surface features from the Earth. Amongst the results were two tantalising mysteries: a large dome feature, similar in some ways to shield volcanoes seen on Mars, observed on the unimaged side of the planet and complex scattering of returned radar from distinct areas around the poles, suggesting that water ice may exist in craters there. Both NASA and the European Space Agency (ESA) are now planning missions to Mercury. The US team are using a newly discovered trajectory that will allow them to reach Mercury using traditional chemical propulsion, incorporating various planetary flybys so-called 'gravity assist' manoeuvres. The European team, on the other hand, has proposed a much more complex mission. In order to get to Mercury, ESA have adopted a novel technology knows as 'solar electric propulsion' (SEP). The basic principle is that electrical energy is produced using solar cells, and this is used to accelerate ions of gas, producing a continuous, if low thrust. The upshot is that the mission is much less constrained by the alignment of the planets and other trajectory concerns and can complete the journey in only two and a half years. BepiColombo, ESA's Mercury mission, will actually consist of three spacecraft! The planetary orbiter will stay close to Mercury and perform remote sensing and mapping of the surface environment. The magnetospheric orbiter, now going to be built by the Institute for Space and Astronautical Science (ISAS) in Japan, will fly in a highly eccentric orbit that takes it from within a few hundred kilometres of the surface to a distance of several planetary radii. This means it will fly in and out of the magnetosphere, the magnetic 'bubble' formed by interaction of the planetary magnetic field with the solar wind. The third and final element is termed the 'MSE' the Mercury Surface Element, or in plain terms a lander, and this is where my research comes in. There is only so much that remote observation can tell us about a planet. The only true way of verifying what we are seeing is to literally go and 'dig the dirt'. The lander on BepiColombo is designed to do just that, using inflated airbags to cushion its descent to the surface. This 'soft landing' will take place in the polar regions of Mercury, where the surface temperature is moderate—between -50 and +70 °C at the sub-solar point at Mercury's closest approach to the Sun the temperature can reach over 400 °C! It is the potential for making these surface measurements that forms my PhD research. There are a whole series of fundamental questions that scientists would like to answer about Mercury. For example: why is the planet much denser than the other 'terrestrial' bodies? And how has such a small planet got a magnetic field? The answers to these questions need data from several complementary sources. The first step is to identify the science goals, then look at what measurements could be made to resolve or constrain these questions, and finally consider the physics of obtaining this data. My project focuses on the surface and sub-surface material on the planet. The surface of Mercury, like the Moon, has been shaped by the impacts upon it and this is still very much in evidence from images of the planet. Craters of many different sizes are evident over most of the surface. These impacts also break up rocks on the surface and produce a finer distribution of particles, known as regolith. The stratigraphy of this material can therefore tell us something about the change in impact environment over time. A conceptual design of the BepiColombo Mercury Surface Element (lander) ©ESA. Conceptual image of the BepiColombo spacecraft at Mercury ©ESA. As well as being interesting in its own right, the regolith also interacts with almost all other aspects of the Mercurian environment. By analysing the regolith we will be able to find out about Mercury's thin atmosphere and also (because the magnetosphere affects the amount of solar wind hitting the planet's surface) changes in the magnetosphere. Planets like the Earth and Jupiter rely on an electrically conductive ionosphere to close the current systems generated by the magnetosphere. Some researchers believe that on Mercury these currents could flow through, or very close to, the surface itself! Designing and building instruments to work in an environment like the surface of Mercury is one of the major challenges I face. Not only must they be capable of surviving extremes of temperature and vibration they must also be small enough to fit into a total lander payload mass of just 7 kg and complete their investigations within the one week expected lifetime of the MSE. In order to take measurements in more than one place, the lander must be equipped with some limited form of mobility. A 'micro-rover' will be carried and deployed after landing, a miniature tracked vehicle that will carry instruments (probably an alpha x-ray spectrometer) to specific target rocks and areas around the lander. To keep things simple the rover will be physically and electronically connected to the lander by a flexible tether. The lander will also carry a 'mole', a slender cylinder (currently being developed for the Beagle-2 Mars lander) with an internal hammering mechanism. Once pushed into the top layer of soil the mole will be able to drive itself down, pushing aside or breaking small rocks, to a depth of several metres, taking measurements as it goes. Over the past few months we have been studying some of the instruments which could be carried by the mole. Concentrating on just one of these it is easy to see how quickly you run into problems! If the MSE lands near the poles, one of the most fascinating activities would be to look for evidence of water ice. In recent years researchers looking at life on the Earth have shown that if water is present, even in the most inhospitable of environments, life often finds a way to survive. The possibility of water on any planet is therefore an exciting prospect! One possible way to look for ice either at or near the surface is to extract a sample using the mole as it penetrates the regolith, heat it at a constant rate and record the amount of energy used to maintain that rate. This technique, differential scanning calorimetry, can observe phase changes in materials and so help to identify them. The technical challenges of performing even this simplistic analysis task are quite daunting. We have to design and build a sample acquisition mechanism that can withstand launch and landing and work at extreme temperatures, heat a sample down a borehole and reject excess heat and the electronics must fit into a 2 cm diameter by 50 cm long mole. So although BepiColombo will not launch until 2009 and will not arrive at Mercury until 2012, there's more than enough work to keep me busy until then!

  17. Inositol 1,2,3-trisphosphate and inositol 1,2- and/or 2,3-bisphosphate are normal constituents of mammalian cells.

    PubMed Central

    Barker, C J; French, P J; Moore, A J; Nilsson, T; Berggren, P O; Bunce, C M; Kirk, C J; Michell, R H

    1995-01-01

    1. An inositol trisphosphate (InsP3) distinct from Ins(1,4,5)P3 and Ins(1,3,4)P3, which we previously observed in myeloid and lymphoid cells [French, Bunce, Stephens, Lord, McConnell, Brown, Creba and Michell (1991) Proc R. Soc. London B 245, 193-201; Bunce, French, Allen, Mountford, Moore, Greaves, Michell and Brown (1993) Biochem. J. 289, 667-673], is present in WRK1 rat mammary tumour cells and pancreatic endocrine beta-cells. 2. It has been identified as Ins(1,2,3)P3 by a combination of oxidation to ribitol, a structurally diagnostic polyol, and ammoniacal hydrolysis to identified inositol monophosphates. 3. Ins(1,2,3)P3 concentration in HL60 cells changed little during stimulation by ATP or fMetLeuPhe or during neutrophilic or monocytic differentiation, and Ins(1,2,3)P3 was unresponsive to vasopressin in WRK1 cells. 4. Ins(1,2,3)P3 was usually more abundant than Ins(1,4,5)P3, often being present at concentrations between approximately 1 microM and approximately 10 microM. 5. HL60, WRK-1 and lymphoid cells also contain Ins(1,2)P2 or Ins(2,3)P2, or a mixture of these two enantiomers, as a major InsP2 species. 6. Ins(1,2,3)P3 and Ins(1,2)P2/Ins(2,3)P2 are readily detected in cells labelled for long periods, but not in acutely labelled cells. This behaviour resembles that of InsP6, the most abundant cellular inositol polyphosphate that includes the 1,2,3-trisphosphate motif, which also achieves isotopic equilibrium with inositol only slowly. 7. Ins(1,2,3)P3 is the major InsP3 that accumulates during metabolism of InsP6 by WRK-1 cell homogenates. 8. Possible metabolic relationships between Ins(1,2,3)P3, Ins(1,2)P2/Ins(2,3)P2 and other inositol polyphosphates in cells, and a possible role for Ins(1,2,3)P3 in cellular iron handling, are considered. PMID:7887911

  18. Young People's Favorite Leisure Activities

    ERIC Educational Resources Information Center

    Zvonovskii, Vladimir; Lutseva, Svetlana

    2004-01-01

    This article presents a study based on surveys conducted annually for the past nine years by the Samara Foundation for Social Research, commissioned by the committee for youth affairs of the administration of Samara Oblast. The sample consists of about 800 young people aged fourteen to thirty. In the present study the authors have focused on…

  19. The People of Color Conference.

    ERIC Educational Resources Information Center

    Brosnan, Michael

    1999-01-01

    Celebration, education, and community characterized the November 1998 People of Color Conference held in San Juan, Puerto Rico. The National Association of Independent Schools is considering whether such a conference is antithetical to diversity initiatives. Renewal of participants' responsibility for creating inclusive school communities may be a…

  20. Warehoused Apartments/Warehoused People.

    ERIC Educational Resources Information Center

    Coalition for the Homeless, New York, NY.

    Between 45,000 and 90,000 habitable New York City apartments are being kept deliberately vacant ("warehoused") by the speculators who own them. Most of these apartments have reasonable rents, affordable by middle- and low-income families. Meanwhile, the housing crisis for poor New Yorkers has grown steadily worse. As many as 75,000 people are…

  1. Bringing science to the people

    Technology Transfer Automated Retrieval System (TEKTRAN)

    This is an opinion editorial piece about the International Society for Horticultural Science (ISHS). It describes the active role that the ISHS takes in bringing scientific information to people throughout the world. The society holds periodic symposia on 10 different crops and 14 different cross-co...

  2. Entrepreneurship among People with Disabilities.

    ERIC Educational Resources Information Center

    Holub, Tamara

    This brief paper reviews the literature on entrepreneurship among people with disabilities. It notes that entrepreneurship by individuals with disabilities is often a consequence of disability discrimination in the workforce and provides both benefits and disadvantages such as independence and freedom from access-related obstacles (benefits) and…

  3. Talking about Plants and People

    ERIC Educational Resources Information Center

    Peacock, Alan

    2004-01-01

    The Eden Project in Cornwall sets out to educate about the interdependence of plants and people. Its tropical and Mediterranean biomes are housed in the largest "greenhouses" in the world, which serve as a backdrop to plants that grow in the temperate zones of the world, grown in Eden's outdoor landscape. Eden has aroused worldwide interest, and…

  4. Productivity, People, and Public Policy.

    ERIC Educational Resources Information Center

    Chamber of Commerce of the United States, Washington, DC.

    This booklet, prepared by the United States Chamber of Commerce, is intended to help create a better public understanding of how productivity affects this country and to suggest how people can change public policy in favor of a revitalized America. The booklet is organized in five sections. The first section defines productivity and introduces the…

  5. Narratives and Understanding Other People

    ERIC Educational Resources Information Center

    Trzebiski, Jerzy

    2005-01-01

    Presenting a story of an ill person, in comparison to a description of illness, as well as activating a narrative approach toward this person increased the probability in subjects of helping behaviour?in this case the promise of donations of bone marrow for leukaemia patients or willingness to spend time on soliciting money for other people's…

  6. Of people, particles and prejudice

    NASA Astrophysics Data System (ADS)

    Jackson, Penny; Greene, Anne; Mears, Matt; Spacecadet1; Green, Christian; Hunt, Devin J.; Berglyd Olsen, Veronica K.; Ilya, Komarov; Pierpont, Elaine; Gillman, Matthew

    2016-05-01

    In reply to Louise Mayor's feature article “Where people and particles collide”, about the experiences of researchers at CERN who are lesbian, gay, bisexual or transgender (LGBT), efforts to make LGBT CERN an officially recognized club, and incidents where posters advertising the club have been torn down or defaced (March pp31–36, http://ow.ly/YVP2Z).

  7. Getting People Back to Work

    ERIC Educational Resources Information Center

    White, Frances L.

    2003-01-01

    Getting people back to work has become a national concern. The nation's economy lost jobs as of July 2003 for six months in a row, dealing another blow to a slow reviving labor market. According to the Labor Department, 486,000 jobs disappeared from the economy. And, the Employment Development Department in California reported a decline of 21,800…

  8. Poor People as Environmental Hazards.

    ERIC Educational Resources Information Center

    Douw, John

    1979-01-01

    In the United States Court of Appeals decision which ruled against New York City's plan to build 160 units of public housing in its West Side Urban Renewal Area, low income people were viewed as a threat to the environment in the same way as more familiar kinds of hazards protected against by federal environmental law. (Author/EB)

  9. When Placement People Are Displaced.

    ERIC Educational Resources Information Center

    Ehrlich, Marianne

    1991-01-01

    Describes the experiences and insights of five laid-off placement people who discover the trauma of job loss. Discusses grieving a job loss, the emotions involved, the challenge of finding a new job, guilt faced by survivors, and advice to colleagues. (NB)

  10. Reading Machines for Blind People.

    ERIC Educational Resources Information Center

    Fender, Derek H.

    1983-01-01

    Ten stages of developing reading machines for blind people are analyzed: handling of text material; optics; electro-optics; pattern recognition; character recognition; storage; speech synthesizers; browsing and place finding; computer indexing; and other sources of input. Cost considerations of the final product are emphasized. (CL)

  11. People and Places for Learning

    ERIC Educational Resources Information Center

    Madden, Peter C.

    1975-01-01

    There's not enough variety of personnel and activity, not enough movement in and out of schools, and not enough cross-fertilization of people and ideas between the schools and the communities of which they are supposed to be a part. (Author)

  12. Disabled People in Japanese Community.

    ERIC Educational Resources Information Center

    Kojima, Yoko, Ed.; And Others

    The volume is intended to give readers a glimpse of the day-to-day life of disabled people in Japan. Eight brief papers present life experiences of a mentally retarded preschooler, severely disabled children, a child with muscular dystrophy, a young girl with polio living in the community, visually disabled and recovering mentally ill people…

  13. Constipation in people prescribed opioids

    PubMed Central

    2010-01-01

    Introduction Constipation is reported in 52% of people with advanced malignancy. This figure rises to 87% in people who are terminally ill and taking opioids. Constipation may be the most common adverse effect of opioids. There is no reason to believe that people with chronic non-malignant disease who take opioids will be any less troubled by this adverse effect. Methods and outcomes We conducted a systematic review and aimed to answer the following clinical questions: What are the effects of: oral laxatives, rectally applied medications, and opioid antagonists for constipation in people prescribed opioids? We searched: Medline, Embase, The Cochrane Library, and other important databases up to August 2009 (BMJ Clinical Evidence reviews are updated periodically, please check our website for the most up-to-date version of this review). We included harms alerts from relevant organisations such as the US Food and Drug Administration (FDA) and the UK Medicines and Healthcare products Regulatory Agency (MHRA). Results We found 23 systematic reviews, RCTs, or observational studies that met our inclusion criteria. We performed a GRADE evaluation of the quality of evidence for interventions. Conclusions In this systematic review we present information relating to the effectiveness and safety of the following interventions: arachis oil enemas, bisacodyl, co-danthrusate/co-danthramer, docusate, glycerol suppositories, ispaghula husk, lactulose, liquid paraffin, macrogols plus electrolyte solutions, magnesium salts, methylcellulose, opioid antagonists, phosphate enemas, senna, sodium citrate micro-enema, and sodium picosulfate. PMID:21718572

  14. Resilience and Young People Leaving Care

    ERIC Educational Resources Information Center

    Stein, Mike

    2008-01-01

    How do we promote the resilience of young people leaving care? This article explores this question by bringing together research findings on the resilience of young people from disadvantaged family backgrounds with research studies on young people leaving care. These findings are applied to young people during their journey to adulthood: their…

  15. Stable Isotope Geochemistry of Extremely Well-Preserved 2.45-Billion-Year-Old Hydrothermal Systems in the Vetreny Belt, Baltic Shield: Insights into Paleohydrosphere

    NASA Astrophysics Data System (ADS)

    Zakharov, D. O.; Bindeman, I. N.

    2015-12-01

    The early Paleoproterozoic was an eventful period in the Earth's history. The first portions of free oxygen emerged in the atmosphere, Snowball Earth glaciations happened several times and the first supercontinent broke up due to extensive rifting. These events should have affected the stable isotopic composition of the hydrosphere. In this study, we use rocks that were altered in underwater hydrothermal systems to investigate the stable isotopic composition of the hydrosphere 2.39-2.45 billion years ago (hereinafter, Ga). Extremely low-δ18O (down to -27.5‰ SMOW) rocks from 2.39 Ga metamorphosed subglacial hydrothermal systems of the Belomorian belt, Baltic Shield formed at near-equatorial latitudes suggesting a Snowball (or Slushball) Earth glaciation. These results motivated us to look at temporally and geographically close hydrothermal systems from the unmetamorhposed 2.45 Ga Vetreny Belt rift. The length of the rift is 250 km and it is composed of high-Mg basalts, mafic-ultramafic intrusions and sedimentary successions. We examined several localities of high-Mg basalt flows that include astonishingly fresh pillow lavas, often with preserved volcanic glass, eruptive breccias, and hydrothermal alteration zones. Collected samples serve a great textural evidence of water-rock interaction that occurred in situ while basalts were cooling. The preliminary results from coexisting quartz and epidote (T, D18O=311°C), and from coexisting calcite and quartz (T, D18O=190°C) yield values of δ18O of involved water between -1.6 and -0.9 ‰. The values of δ13C in calcites vary between -4.0 and -2.3 ‰. It is likely that hydrothermal fluids operated in the Vetreny Belt rift were derived from seawater that is no different from modern oceanic water in terms of δ18O. Apparently, the rift was a Paleoproterozoic analog of the modern Red Sea, filled with oceanic water. The result is important because the Vetreny Belt rift predates the onset of Snowball Earth glaciation at 2

  16. Studies on the isopropylbenzene 2,3-dioxygenase and the 3-isopropylcatechol 2,3-dioxygenase genes encoded by the linear plasmid of Rhodococcus erythropolis BD2.

    PubMed

    Kesseler, M; Dabbs, E R; Averhoff, B; Gottschalk, G

    1996-11-01

    The enzymes responsible for the degradation of isopropylbenzene (IPB) and co-oxidation of trichloroethene (TCE) by Rhodococcus erythropolis BD2 are encoded by the linear plasmid pBD2. Fragments containing IPB catabolic genes were cloned from pBD2 and the nucleotide sequence was determined. By means of database searches and expression of the cloned genes in recombinant strains, we identified five clustered genes, ipbA1A2A3A4C, which encode the three components of the IPB 2,3-dioxygenase system, reductaseIPB (ipbA4), ferredoxinIPB (ipbA3) and the two subunits of the terminal dioxygenase (ipbA1A2), as well as the 3-isopropylcatechol (IPC) 2,3-dioxygenase (ipbC). The protein sequences deduced from the ipbA1A2A3A4C gene cluster exhibited significant homology with the corresponding proteins of analogous degradative pathways in Gram-negative and Gram-positive bacteria, but the gene order differed from most of them. IPB 2,3-dioxygenase and 3-IPC 2,3-dioxygenase could both be expressed in Escherichia coli, but the IPB 2,3-dioxygenase activities were too low to be detected by polarographic and TCE degradative means. However, inhibitor studies with the R. erythropolis BD2 wild-type are in accordance with the involvement of the IPB 2,3-dioxygenase in TCE oxidation. PMID:8969521

  17. Constraint on a varying proton-electron mass ratio 1.5 billion years after the big bang.

    PubMed

    Bagdonaite, J; Ubachs, W; Murphy, M T; Whitmore, J B

    2015-02-20

    A molecular hydrogen absorber at a lookback time of 12.4 billion years, corresponding to 10% of the age of the Universe today, is analyzed to put a constraint on a varying proton-electron mass ratio, μ. A high resolution spectrum of the J1443+2724 quasar, which was observed with the Very Large Telescope, is used to create an accurate model of 89 Lyman and Werner band transitions whose relative frequencies are sensitive to μ, yielding a limit on the relative deviation from the current laboratory value of Δμ/μ=(-9.5 ± 5.4(stat)± 5.3(syst))×10(-6). PMID:25763949

  18. 1.8 Billion Years of Detrital Zircon Recycling Calibrates a Refractory Part of Earth’s Sedimentary Cycle

    PubMed Central

    Hadlari, Thomas; Swindles, Graeme T.; Galloway, Jennifer M.; Bell, Kimberley M.; Sulphur, Kyle C.; Heaman, Larry M.; Beranek, Luke P.; Fallas, Karen M.

    2015-01-01

    Detrital zircon studies are providing new insights on the evolution of sedimentary basins but the role of sedimentary recycling remains largely undefined. In a broad region of northwestern North America, this contribution traces the pathway of detrital zircon sand grains from Proterozoic sandstones through Phanerozoic strata and argues for multi-stage sedimentary recycling over more than a billion years. As a test of our hypothesis, integrated palynology and detrital zircon provenance provides clear evidence for erosion of Carboniferous strata in the northern Cordillera as a sediment source for Upper Cretaceous strata. Our results help to calibrate Earth's sedimentary cycle by showing that recycling dominates sedimentary provenance for the refractory mineral zircon. PMID:26658165

  19. Taking out one billion tones of carbon: the magic of China's 11thFive-Year Plan

    SciTech Connect

    Lin, Jiang; Zhou, Nan; Levine, Mark D.; Fridley, David

    2007-05-01

    China's 11th Five-Year Plan (FYP) sets an ambitious targetfor energy-efficiency improvement: energy intensity of the country sgross domestic product (GDP) should be reduced by 20 percent from 2005 to2010 (NDRC, 2006). This is the first time that a quantitative and bindingtarget has been set for energy efficiency, and signals a major shift inChina's strategic thinking about its long-term economic and energydevelopment. The 20 percent energy intensity target also translates intoan annual reduction of over one billion tons of CO2 by 2010, making theChinese effort one of most significant carbon mitigation effort in theworld today. While it is still too early to tell whether China willachieve this target, this paper attempts to understand the trend inenergy intensity in China and to explore a variety of options towardmeeting the 20 percent target using a detailed endues energymodel.

  20. Taking out 1 billion tons of CO2: The magic of China's 11th Five-Year Plan?

    SciTech Connect

    Zhou, Nan; Lin, Jiang; Zhou, Nan; Levine, Mark; Fridley, David

    2007-07-01

    China's 11th Five-Year Plan (FYP) sets an ambitious target for energy-efficiency improvement: energy intensity of the country's gross domestic product (GDP) should be reduced by 20% from 2005 to 2010 (NDRC, 2006). This is the first time that a quantitative and binding target has been set for energy efficiency, and signals a major shift in China's strategic thinking about its long-term economic and energy development. The 20% energy intensity target also translates into an annual reduction of over 1.5 billion tons of CO2 by 2010, making the Chinese effort one of most significant carbon mitigation effort in the world today. While it is still too early to tell whether China will achieve this target, this paper attempts to understand the trend in energy intensity in China and to explore a variety of options toward meeting the 20% target using a detailed end-use energy model.

  1. The Archean Dongwanzi ophiolite complex, North China craton: 2.505-billion-year-old oceanic crust and mantle.

    PubMed

    Kusky, T M; Li, J H; Tucker, R D

    2001-05-11

    We report a thick, laterally extensive 2505 +/- 2.2-million-year-old (uranium-lead ratio in zircon) Archean ophiolite complex in the North China craton. Basal harzburgite tectonite is overlain by cumulate ultramafic rocks, a mafic-ultramafic transition zone of interlayered gabbro and ultramafic cumulates, compositionally layered olivine-gabbro and pyroxenite, and isotropic gabbro. A sheeted dike complex is rooted in the gabbro and overlain by a mixed dike-pillow lava section, chert, and banded iron formation. The documentation of a complete Archean ophiolite implies that mechanisms of oceanic crustal accretion similar to those of today were in operation by 2.5 billion years ago at divergent plate margins and that the temperature of the early mantle was not extremely elevated, as compared to the present-day temperature. Plate tectonic processes similar to those of the present must also have emplaced the ophiolite in a convergent margin setting. PMID:11349144

  2. 1.8 Billion Years of Detrital Zircon Recycling Calibrates a Refractory Part of Earth's Sedimentary Cycle.

    PubMed

    Hadlari, Thomas; Swindles, Graeme T; Galloway, Jennifer M; Bell, Kimberley M; Sulphur, Kyle C; Heaman, Larry M; Beranek, Luke P; Fallas, Karen M

    2015-01-01

    Detrital zircon studies are providing new insights on the evolution of sedimentary basins but the role of sedimentary recycling remains largely undefined. In a broad region of northwestern North America, this contribution traces the pathway of detrital zircon sand grains from Proterozoic sandstones through Phanerozoic strata and argues for multi-stage sedimentary recycling over more than a billion years. As a test of our hypothesis, integrated palynology and detrital zircon provenance provides clear evidence for erosion of Carboniferous strata in the northern Cordillera as a sediment source for Upper Cretaceous strata. Our results help to calibrate Earth's sedimentary cycle by showing that recycling dominates sedimentary provenance for the refractory mineral zircon. PMID:26658165

  3. Vaccine Assistance To Low- And Middle-Income Countries Increased To $3.6 Billion In 2014.

    PubMed

    Haakenstad, Annie; Birger, Maxwell; Singh, Lavanya; Liu, Patrick; Lim, Stephen; Ng, Marie; Dieleman, Joseph L

    2016-02-01

    In the 2012 Global Vaccine Action Plan, development assistance partners committed to providing sustainable financing for vaccines and expanding vaccination coverage to all children in low- and middle-income countries by 2020. To assess progress toward these goals, the Institute for Health Metrics and Evaluation produced estimates of development assistance for vaccinations. These estimates reveal major increases in the assistance provided since 2000. In 2014, $3.6 billion in development assistance for vaccinations was provided for low- and middle-income countries, up from $822 million in 2000. The funding increase was driven predominantly by the establishment of Gavi, the Vaccine Alliance, supported by the Bill & Melinda Gates Foundation and the governments of the United States and United Kingdom. Despite stagnation in total development assistance for health from donors from 2010 onward, development assistance for vaccination has continued to grow. PMID:26858376

  4. Mechanism of 2,3-butanediol stereoisomers formation in a newly isolated Serratia sp. T241

    PubMed Central

    Zhang, Liaoyuan; Guo, Zewang; Chen, Jiebo; Xu, Quanming; Lin, Hui; Hu, Kaihui; Guan, Xiong; Shen, Yaling

    2016-01-01

    Serratia sp. T241, a newly isolated xylose-utilizing strain, produced three 2,3-butanediol (2,3-BD) stereoisomers. In this study, three 2,3-butanediol dehydrogenases (BDH1-3) and one glycerol dehydrogenase (GDH) involved in 2,3-BD isomers formation by Serratia sp. T241 were identified. In vitro conversion showed BDH1 and BDH2 could catalyzed (3S)-acetoin and (3R)-acetoin into (2S,3S)-2,3-BD and meso-2,3-BD, while BDH3 and GDH exhibited the activities from (3S)-acetoin and (3R)-acetoin to meso-2,3-BD and (2R,3R)-2,3-BD. Four encoding genes were assembled into E. coli with budA (acetolactate decarboxylase) and budB (acetolactate synthase), responsible for converting pyruvate into acetoin. E. coli expressing budAB-bdh1/2 produced meso-2,3-BD and (2S,3S)-2,3-BD. Correspondingly, (2R,3R)-2,3-BD and meso-2,3-BD were obtained by E. coli expressing budAB-bdh3/gdh. These results suggested four enzymes might contribute to 2,3-BD isomers formation. Mutants of four genes were developed in Serratia sp. T241. Δbdh1 led to reduced concentration of meso-2,3-BD and (2S,3S)-2,3-BD by 97.7% and 87.9%. (2R,3R)-2,3-BD with a loss of 73.3% was produced by Δbdh3. Enzyme activity assays showed the decrease of 98.4% and 22.4% by Δbdh1 and Δbdh3 compared with the wild strain. It suggested BDH1 and BDH3 played important roles in 2,3-BD formation, BDH2 and GDH have small effects on 2,3-BD production by Serratia sp. T241. PMID:26753612

  5. 2,3-butanediol production from cellobiose by engineered Saccharomyces cerevisiae.

    PubMed

    Nan, Hong; Seo, Seung-Oh; Oh, Eun Joong; Seo, Jin-Ho; Cate, Jamie H D; Jin, Yong-Su

    2014-06-01

    Production of renewable fuels and chemicals from cellulosic biomass is a critical step towards energy sustainability and reduced greenhouse gas emissions. Microbial cells have been engineered for producing chemicals from cellulosic sugars. Among these chemicals, 2,3-butanediol (2,3-BDO) is a compound of interest due to its diverse applications. While microbial production of 2,3-BDO with high yields and productivities has been reported, there are concerns associated with utilization of potential pathogenic bacteria and inefficient utilization of cellulosic sugars. To address these problems, we engineered 2,3-BDO production in Saccharomyces cerevisiae, especially from cellobiose, a prevalent sugar in cellulosic hydrolysates. Specifically, we overexpressed alsS and alsD from Bacillus subtilis to convert pyruvate into 2,3-BDO via α-acetolactate and acetoin in an engineered cellobiose fermenting S. cerevisiae. Under oxygen-limited conditions, the resulting strain was able to produce 2,3-BDO. Still, major carbon flux went to ethanol, resulting in substantial amounts of ethanol produced as a byproduct. To enhance pyruvate flux to 2,3-BDO through elimination of the pyruvate decarboxylation reaction, we employed a deletion mutant of both PDC1 and PDC5 for producing 2,3-BDO. When a cellobiose utilization pathway, consisting of a cellobiose transporter and intracellular β-glucosidase, and the 2,3-BDO producing pathway were introduced in a pyruvate decarboxylase deletion mutant, the resulting strain produced 2,3-BDO without ethanol production from cellobiose under oxygen-limited conditions. A titer of 5.29 g/l 2,3-BDO with a productivity of 0.22 g/l h and yield of 0.29 g 2,3-BDO/g cellobiose was attained. These results suggest the possibility of producing 2,3-BDO safely and sustainably from cellulosic hydrolysates. PMID:24743979

  6. BIOACCUMULATION FACTORS AND INTAKE OF 2,3,7,8-POLYCHLORINATED DIBENZO-P-DIOXINS IN THE DOMESTIC CHICKEN

    EPA Science Inventory

    One of the most commercially valuable farm animals in the United States is the domestic chicken (Gallus domesticus). Rapidly reared in controlled, intensive environments, the US Department of Agriculture (USDA) estimated the production of these animals exceeded eight billion in ...

  7. The People's Library of Epidemiology.

    PubMed

    Last, John M

    2012-03-01

    The People's Library of Epidemiology is in the process of development. It consists of a website (http://www.jameslindlibrary.org) with links to online excerpts of papers and monographs of historical and scientific importance in epidemiology and related public health sciences that are held by the library of the Royal College of Physicians of Edinburgh. This paper reflects the lively panel discussion which took place on 9 August 2011. The panel members who opened the discussion were Alfredo Morabia, Anne Hardy, Roger Bernier, Jan Vandenbroucke, George Davey Smith, Esther Villalonga and Stephen Walter, who had won the prize awarded by Epidemiology Monitor for an essay on the People's Library of Epidemiology. PMID:22326598

  8. Fatigue in frail elderly people.

    PubMed

    Toye, Christine; White, Kate; Rooksby, Karen

    2006-05-01

    Many frail older people are likely to suffer from fatigue, but tools to measure fatigue in this population are lacking. Stage one of this study explored and described the experiences of fatigue of 12 older people from Australian residential aged care facilities. Themes identified were pacing yourself, battling on, hitting rock bottom, feeling safe, and moving on. Findings indicated that, with support, frail elders may be able to manage fatigue effects themselves. A measure of fatigue was developed from stage one findings, with reference to the literature. In stage two of the study, the Frail Elder Fatigue Assessment Tool was subjected to panel review, piloting, and refinement. The refined tool comprises 20 items in three subscales: fatigue effects; fatigue resources; and adaptation to fatigue. Further work is required to establish the tool's psychometric properties, but it should then be useful for both research and clinical assessment purposes. PMID:16835559

  9. Social capital from carbon property: creating equity for indigenous people.

    PubMed

    Saunders, Lindsay S; Hanbury-Tenison, Robin; Swingland, Ian R

    2002-08-15

    New incentives for protection and in situ use of forests and the services they provide raise hopes for the reversal of tropical and temperate deforestation. Past management of forests appropriated the rights of forest communities, providing incentives to convert natural forest into financial capital through logging, while destroying the underlying physical property. Carbon trading aims to provide a means to convert the forest property into financial capital, while protecting the physical property of forests, thereby providing new incentives for in situ forest management. The potential for carbon-emission trading as a contributor to these new incentives is tempered by concerns that it is another tool for capitalists to exploit the indigenous communities of the developing world. Estimates of annual emission trading amounting to US $200 billion raise alarm bells about the effect of such trade in the developing world. People are right to be concerned, as the history of exploitation of indigenous people, the appropriation of their rights, the loss of forests and their benefits is well documented. This exploitation resulted in the exclusion of forest communities from the basic tenets for development created by the wealth generated by traded property. However, one virtue of trade is that it can be made subject to constraints. Through international treaties and agreements, trade can be constrained and national governments obliged to observe the rules of trade. The value of tradable carbon credits will be discounted or invalid if they do not meet these criteria, providing all parties with strong incentives to achieve the necessary performance standards relating to both processes and contracts. For carbon trading to develop social capital from natural capital requires the admission of forest communities into the polity and management of forest resources. In this paper we argue for responsible carbon-emission trading based on the clear and appropriate definition of carbon

  10. How do people define moderation?

    PubMed

    vanDellen, Michelle R; Isherwood, Jennifer C; Delose, Julie E

    2016-06-01

    Eating in moderation is considered to be sound and practical advice for weight maintenance or prevention of weight gain. However, the concept of moderation is ambiguous, and the effect of moderation messages on consumption has yet to be empirically examined. The present manuscript examines how people define moderate consumption. We expected that people would define moderate consumption in ways that justified their current or desired consumption rather than view moderation as an objective standard. In Studies 1 and 2, moderate consumption was perceived to involve greater quantities of an unhealthy food (chocolate chip cookies, gummy candies) than perceptions of how much one should consume. In Study 3, participants generally perceived themselves to eat in moderation and defined moderate consumption as greater than their personal consumption. Furthermore, definitions of moderate consumption were related to personal consumption behaviors. Results suggest that the endorsement of moderation messages allows for a wide range of interpretations of moderate consumption. Thus, we conclude that moderation messages are unlikely to be effective messages for helping people maintain or lose weight. PMID:26964691

  11. PTSD in older bereaved people.

    PubMed

    O'Connor, Maja

    2010-08-01

    Late life bereavement has been associated with psychological problems, mainly depression. A few studies indicated that posttraumatic stress disorder (PTSD) was an important issue in late life bereavement reactions. This study aimed to assess the prevalence of PTSD in recently bereaved older people compared with married controls and to investigate whether the loss of a spouse in old age, in contrast with earlier assumptions, could lead to PTSD. Two hundred and ninety-six Danish older bereaved people (mean age 73 years, 113 males) were chosen from national registers and assessed two months postbereavement. They were compared with a control group of 276 married older people. The prevalence of PTSD and depression were measured through a self-report questionnaire. Results showed that 16% of the bereaved and 4% of the control group had a PTSD diagnosis (ES = 0.35; Cohen's d = 0.74). Additionally, 37% of the bereaved and 22% of the control group had mild to severe depression (ES = 0.19; Cohen's d = 0.37). The results suggested that late life spousal bereavement result in PTSD with equal frequency to general samples of bereaved persons. Furthermore, the prevalence of PTSD in the first months after bereavement was more elevated than the level of depression. This makes PTSD an important factor when studying late life bereavement reactions. PMID:20686978

  12. Fertility options in transgender people.

    PubMed

    De Roo, Chloë; Tilleman, Kelly; T'Sjoen, Guy; De Sutter, Petra

    2016-01-01

    Hormonal and surgical treatments for transgender people have a devastating effect on the possibility for these patients to reproduce. Additionally, transgender people tend to start sex reassignment treatment at a young age, when reproductive wishes are not yet clearly defined nor fulfilled. The most recent Standards of Care of the World Professional Association for Transgender Health recommend clearly informing patients regarding their future reproductive options prior to initiation of treatment. This review gives an overview of the current knowledge and state-of-the-art techniques in the field of fertility preservation for transgender people. Where genital reconstructive surgery definitely results in sterility, hormone therapy on the other hand also has an important, but partially reversible impact on fertility. The current fertility preservation options for trans men are embryo cryopreservation, oocyte cryopreservation and ovarian tissue cryopreservation. For trans women, sperm cryopreservation, surgical sperm extraction and testicular tissue cryopreservation are possible. Although certain fertility preservation techniques could be applicable in a standardized manner based on clear biological criteria, the technique that eventually will be performed should be the preferred choice of the patient after extended explanation of all possible options. PMID:26835612

  13. Erythrocyte 2,3-diphosphoglycerate and adenosine-triphosphate in cretins living at high altitude.

    PubMed

    Adams, W H

    1976-01-01

    A comparison of concentrations of 2,3-diphosphoglycerate (2,3-DPG) and adenosine-triphosphate (ATP) in the red cells of cretins and normal controls living at 3,700 m in the Nepal Himalayas has shown that 2,3-DPG and ATP levels were higher in the cretins. A negative correlation between hemoglobin and 2.3-DPG level was found. Chronic hypoxia appears to have provided the additional stress required to differentiate the significance of thyroid hormone deficiency in producing anemia from its effect on 2,3-DPG levels. If thyroid hormone is in fact one regulator of 2,3-DPG, the anemia of hypothyroidism appears to be more significant. This also suggest that the anemia of hypothyroidism, is at least in part, "pathologic" as opposed to "adaptive". PMID:822672

  14. BmRobo2/3 is required for axon guidance in the silkworm Bombyx mori.

    PubMed

    Li, Xiao-Tong; Yu, Qi; Zhou, Qi-Sheng; Zhao, Xiao; Liu, Zhao-Yang; Cui, Wei-Zheng; Liu, Qing-Xin

    2016-02-15

    Axon guidance is critical for proper wiring of the nervous system. During the neural development, the axon guidance molecules play a key role and direct axons to choose the correct way to reach the target. Robo, as the receptor of axon guidance molecule Slit, is evolutionarily conserved from planarians to humans. However, the function of Robo in the silkworm, Bombyx mori, remained unknown. In this study, we cloned robo2/3 from B. mori (Bmrobo2/3), a homologue of robo2/3 in Tribolium castaneum. Moreover, BmRobo2/3 was localized in the neuropil, and RNAi-mediated knockdown of Bmrobo2/3 resulted in the longitudinal connectives forming closer to the midline. These data demonstrate that BmRobo2/3 is required for axon guidance in the silkworm. PMID:26625973

  15. 40 CFR 721.3031 - Boric acid (H3BO3), zinc salt (2=3).

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... 40 Protection of Environment 31 2014-07-01 2014-07-01 false Boric acid (H3BO3), zinc salt (2=3... Substances § 721.3031 Boric acid (H3BO3), zinc salt (2=3). (a) Chemical substance and significant new uses subject to reporting. (1) The chemical substance identified as boric acid (H3BO3), zinc salt (2=3) (PMN...

  16. 40 CFR 721.3031 - Boric acid (H3BO3), zinc salt (2=3).

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... 40 Protection of Environment 32 2012-07-01 2012-07-01 false Boric acid (H3BO3), zinc salt (2=3... Substances § 721.3031 Boric acid (H3BO3), zinc salt (2=3). (a) Chemical substance and significant new uses subject to reporting. (1) The chemical substance identified as boric acid (H3BO3), zinc salt (2=3) (PMN...

  17. 40 CFR 721.3031 - Boric acid (H3BO3), zinc salt (2=3).

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... 40 Protection of Environment 32 2013-07-01 2013-07-01 false Boric acid (H3BO3), zinc salt (2=3... Substances § 721.3031 Boric acid (H3BO3), zinc salt (2=3). (a) Chemical substance and significant new uses subject to reporting. (1) The chemical substance identified as boric acid (H3BO3), zinc salt (2=3) (PMN...

  18. 40 CFR 721.3031 - Boric acid (H3BO3), zinc salt (2=3).

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... 40 Protection of Environment 30 2010-07-01 2010-07-01 false Boric acid (H3BO3), zinc salt (2=3... Substances § 721.3031 Boric acid (H3BO3), zinc salt (2=3). (a) Chemical substance and significant new uses subject to reporting. (1) The chemical substance identified as boric acid (H3BO3), zinc salt (2=3) (PMN...

  19. 40 CFR 721.3031 - Boric acid (H3BO3), zinc salt (2=3).

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... 40 Protection of Environment 31 2011-07-01 2011-07-01 false Boric acid (H3BO3), zinc salt (2=3... Substances § 721.3031 Boric acid (H3BO3), zinc salt (2=3). (a) Chemical substance and significant new uses subject to reporting. (1) The chemical substance identified as boric acid (H3BO3), zinc salt (2=3) (PMN...

  20. 2,3-Dihydroxybenzoic acid amides of tetraazaalkanes and tetaaza cycloalkanes

    DOEpatents

    Weitl, Frederick L. [Martinez, CA; Raymond, Kenneth N. [Berkeley, CA

    1980-01-01

    A compound of the formula: ##STR1## wherein X is hydrogen or a conventional electron-withdrawing group, particularly --SO.sub.3 H or a salt thereof; n is 2, 3, or 4; m is 2, 3, or 4; and p is 2 or 3. The present compounds are useful as specific sequestering agents for actinide (IV) ions. Also described is a method for the 2,3-dihydroxybenzamidation of azaalkanes.