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Sample records for scientists solve mystery

  1. Solving the Mystery of the Missing Neutrinos

    E-print Network

    John Bahcall

    2004-06-09

    The three years 2001 to 2003 were the golden years of solar neutrino research. In this period, scientists solved a mystery with which they had been struggling for four decades. The solution turned out to be important for both physics and for astronomy. In this article, I tell the story of those fabulous three years.

  2. Solve Medical Mysteries

    ERIC Educational Resources Information Center

    Miller, Leslie

    2007-01-01

    Wondering how to make the study of the immune system and infectious agents more relevant to your students' lives? The online adventure series, Medical Mysteries, can provide the context and motivation. The series combines the drama of television's "CSI" episodes with science to address several of the National Science Education Content Standards.…

  3. Pulsating Star Mystery Solved

    NASA Astrophysics Data System (ADS)

    2010-11-01

    By discovering the first double star where a pulsating Cepheid variable and another star pass in front of one another, an international team of astronomers has solved a decades-old mystery. The rare alignment of the orbits of the two stars in the double star system has allowed a measurement of the Cepheid mass with unprecedented accuracy. Up to now astronomers had two incompatible theoretical predictions of Cepheid masses. The new result shows that the prediction from stellar pulsation theory is spot on, while the prediction from stellar evolution theory is at odds with the new observations. The new results, from a team led by Grzegorz Pietrzy?ski (Universidad de Concepción, Chile, Obserwatorium Astronomiczne Uniwersytetu Warszawskiego, Poland), appear in the 25 November 2010 edition of the journal Nature. Grzegorz Pietrzy?ski introduces this remarkable result: "By using the HARPS instrument on the 3.6-metre telescope at ESO's La Silla Observatory in Chile, along with other telescopes, we have measured the mass of a Cepheid with an accuracy far greater than any earlier estimates. This new result allows us to immediately see which of the two competing theories predicting the masses of Cepheids is correct." Classical Cepheid Variables, usually called just Cepheids, are unstable stars that are larger and much brighter than the Sun [1]. They expand and contract in a regular way, taking anything from a few days to months to complete the cycle. The time taken to brighten and grow fainter again is longer for stars that are more luminous and shorter for the dimmer ones. This remarkably precise relationship makes the study of Cepheids one of the most effective ways to measure the distances to nearby galaxies and from there to map out the scale of the whole Universe [2]. Unfortunately, despite their importance, Cepheids are not fully understood. Predictions of their masses derived from the theory of pulsating stars are 20-30% less than predictions from the theory of the evolution of stars. This embarrassing discrepancy has been known since the 1960s. To resolve this mystery, astronomers needed to find a double star containing a Cepheid where the orbit happened to be seen edge-on from Earth. In these cases, known as eclipsing binaries, the brightness of the two stars dims as one component passes in front of the other, and again when it passes behind the other star. In such pairs astronomers can determine the masses of the stars to high accuracy [3]. Unfortunately neither Cepheids nor eclipsing binaries are common, so the chance of finding such an unusual pair seemed very low. None are known in the Milky Way. Wolfgang Gieren, another member of the team, takes up the story: "Very recently we actually found the double star system we had hoped for among the stars of the Large Magellanic Cloud. It contains a Cepheid variable star pulsating every 3.8 days. The other star is slightly bigger and cooler, and the two stars orbit each other in 310 days. The true binary nature of the object was immediately confirmed when we observed it with the HARPS spectrograph on La Silla." The observers carefully measured the brightness variations of this rare object, known as OGLE-LMC-CEP0227 [4], as the two stars orbited and passed in front of one another. They also used HARPS and other spectrographs to measure the motions of the stars towards and away from the Earth - both the orbital motion of both stars and the in-and-out motion of the surface of the Cepheid as it swelled and contracted. This very complete and detailed data allowed the observers to determine the orbital motion, sizes and masses of the two stars with very high accuracy - far surpassing what had been done before for a Cepheid. The mass of the Cepheid is now known to about 1% and agrees exactly with predictions from the theory of stellar pulsation. However, the larger mass predicted by stellar evolution theory was shown to be significantly in error. The much-improved mass estimate is only one outcome of this work, and the team hopes to find other examples of these

  4. Distance Measurement Solves Astrophysical Mysteries

    NASA Astrophysics Data System (ADS)

    2003-08-01

    Location, location, and location. The old real-estate adage about what's really important proved applicable to astrophysics as astronomers used the sharp radio "vision" of the National Science Foundation's Very Long Baseline Array (VLBA) to pinpoint the distance to a pulsar. Their accurate distance measurement then resolved a dispute over the pulsar's birthplace, allowed the astronomers to determine the size of its neutron star and possibly solve a mystery about cosmic rays. "Getting an accurate distance to this pulsar gave us a real bonanza," said Walter Brisken, of the National Radio Astronomy Observatory (NRAO) in Socorro, NM. Monogem Ring The Monogem Ring, in X-Ray Image by ROSAT satellite CREDIT: Max-Planck Institute, American Astronomical Society (Click on Image for Larger Version) The pulsar, called PSR B0656+14, is in the constellation Gemini, and appears to be near the center of a circular supernova remnant that straddles Gemini and its neighboring constellation, Monoceros, and is thus called the Monogem Ring. Since pulsars are superdense, spinning neutron stars left over when a massive star explodes as a supernova, it was logical to assume that the Monogem Ring, the shell of debris from a supernova explosion, was the remnant of the blast that created the pulsar. However, astronomers using indirect methods of determining the distance to the pulsar had concluded that it was nearly 2500 light-years from Earth. On the other hand, the supernova remnant was determined to be only about 1000 light-years from Earth. It seemed unlikely that the two were related, but instead appeared nearby in the sky purely by a chance juxtaposition. Brisken and his colleagues used the VLBA to make precise measurements of the sky position of PSR B0656+14 from 2000 to 2002. They were able to detect the slight offset in the object's apparent position when viewed from opposite sides of Earth's orbit around the Sun. This effect, called parallax, provides a direct measurement of distance. "Our measurements showed that the pulsar is about 950 light-years from Earth, essentially the same distance as the supernova remnant," said Steve Thorsett, of the University of California, Santa Cruz. "That means that the two almost certainly were created by the same supernova blast," he added. With that problem solved. the astronomers then turned to studying the pulsar's neutron star itself. Using a variety of data from different telescopes and armed with the new distance measurement, they determined that the neutron star is between 16 and 25 miles in diameter. In such a small size, it packs a mass roughly equal to that of the Sun. The next result of learning the pulsar's actual distance was to provide a possible answer to a longstanding question about cosmic rays. Cosmic rays are subatomic particles or atomic nuclei accelerated to nearly the speed of light. Shock waves in supernova remnants are thought to be responsible for accelerating many of these particles. Scientists can measure the energy of cosmic rays, and had noted an excess of such rays in a specific energy range. Some researchers had suggested that the excess could come from a single supernova remnant about 1000 light-years away whose supernova explosion was about 100,000 years ago. The principal difficulty with this suggestion was that there was no accepted candidate for such a source. "Our measurement now puts PSR B0656+14 and the Monogem Ring at exactly the right place and at exactly the right age to be the source of this excess of cosmic rays," Brisken said. With the ability of the VLBA, one of the telescopes of the NRAO, to make extremely precise position measurements, the astronomers expect to improve the accuracy of their distance determination even more. "This pulsar is becoming a fascinating laboratory for studying astrophysics and nuclear physics," Thorsett said. In addition to Brisken and Thorsett, the team of astronomers includes Aaron Golden of the National University of Ireland, Robert Benjamin of the University of Wiscons

  5. Solving the mystery of memory.

    PubMed

    Worley, Paul; Shuler, Marshall

    2014-01-01

    The word "memory" is derived from the ancient Greek myth of Mnemosyne, the mother of the Muses, who was "said to know everything, past, present, and future." Memory is essential to our existence, and one of neuroscience's primary missions is to understand how the brain processes memory and to improve treatments for Alzheimer's disease, traumatic brain injury, drug addiction, and the many other afflictions associated with disrupted memory. Our article traces scientists' progress in understanding memory over the last 15 years. PMID:25009692

  6. NIH Scientists Shed Light on Mystery Surrounding Hepatitis B Virus

    MedlinePLUS

    ... on Research 2013 January 2013 NIH Scientists Shed Light on Mystery Surrounding Hepatitis B Virus Discovery Is ... the University of Oxford, U.K., have shed light on a long-standing enigma about the structure ...

  7. 12/13/12 Solving a biological mystery | Harvard Gazette 1/2news.harvard.edu/gazette/story/2012/12/solvingabiologicalmystery/

    E-print Network

    Extavour, Cassandra

    12/13/12 Solving a biological mystery | Harvard Gazette 1/2news.harvard.edu/gazette/story/2012/12/solvingabiologicalmystery/ Solving a biological mystery Researchers find gene related to germ cell formation older than Harvard scientists have solved the longstanding mystery of how some insects form germ cells

  8. Swinging arms as we walk 'helps preserve energy' The mystery of why we swing our arms as we walk may have been solved, after scientists

    E-print Network

    Collins, Steven H.

    humans move the arms when strolling, since they play no obvious role in helping propel the body forward, the scientists found. "Although arm swinging is relatively easy to achieve, its effect on energy use://www.telegraph.co.uk/health/swine-flu-information/) The Ashes (http://www.telegraph.co.uk/sport/cricket/international/theashes/) 8/2/2009 Swinging arms as we

  9. Mystery of Cometary X-Rays Solved

    NASA Astrophysics Data System (ADS)

    2000-07-01

    On July 14, 2000 NASA's Chandra X-ray Observatory imaged Comet C/1999 S4 (LINEAR) and detected X-rays from oxygen and nitrogen ions. The details of the X-ray emission, as recorded on Chandra's Advanced CCD Imaging Spectrometer, show that they are produced by collisions of ions racing away from the Sun with gas in the comet. "This observation solves one mystery. It proves how comets produce X-rays," said Dr. Carey Lisse of the Space Telescope Science Institute (STScI) leader of a team of scientists from STScI, NASA's Goddard Space Flight Center, Max Planck Institute in Germany, Johns Hopkins University, the University of California, Berkeley, and the Harvard-Smithsonian Center for Astrophysics. "With an instrument like Chandra, we can now study the chemistry of the solar wind, and observe the X-ray glow from the atmospheres of comets as well as planets such as Venus. It may even be possible to observe other, nearby solar systems." Comets, which resemble "dirty snow balls" a few miles in diameter, were thought to be too cold for such energetic emission, so the detection of X-rays by the ROSAT observatory from comet Hyakutake in 1996 was a surprise. Several explanations were suggested, but the source of cometary X-ray emission remained a puzzle until the Chandra observation of Comet C/1999 S4 (LINEAR). Chandra's imaging spectrometer revealed a strong X-ray signal from oxygen and nitrogen ions, clinching the case for the production of X-rays due to the exchange of electrons in collisions between nitrogen and oxygen ions in the solar wind and electrically neutral elements (predominantly hydrogen) in the comets atmosphere. The Chandra observation was taken with the Advanced CCD Imaging Spectrometer (ACIS) on July 14, 2000 for a total of 2 ½ hours. The comet will be re-observed with Chandra during the weeks of July 29 - Aug 13. Comet C/1999 S4 (LINEAR) was discovered in September 1999 by the Lincoln Near Earth Asteroid Research (LINEAR) project, which is operated by the Massachusetts Institute of Technology's Lincoln Laboratory to search for Earth-approaching objects. In addition to Dr. Lisse, the science team involved with the Chandra observations includes: Drs. Damian Christian (CSC/STScI), Konrad Dennerl (MPE), Frank Marshall, Robert Petre, and Steven Snowden (NASA/GSFC), Harold Weaver (JHU), Brett Stroozas (CEA), and Scott Wolk (CfA) ) The ACIS instrument was built for NASA by the Massachusetts Institute of Technology, Cambridge, and Pennsylvania State University, University Park. NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program. TRW, Inc., Redondo Beach, Calif., is the prime contractor for the spacecraft. The Smithsonian's Chandra X-ray Center controls science and flight operations from Cambridge, Mass. To follow Chandra's progress, visit the Chandra site at: http://chandra.harvard.edu AND http://chandra.nasa.gov

  10. Solving the Mystery of the Fermi Bubbles?

    NASA Astrophysics Data System (ADS)

    Bartlett, David F.; Cumalat, John Perry

    2015-05-01

    The Fermi Bubbles are large structures that stretch symmetrically between galactic latitudes of -55 degrees and +55 degress and between galactic longitudes of -45 degrees and +45 degrees. For almost a decade they have been under the intense scrutiny of the Fermi-Large Area Telescope, a gamma-ray detector in orbit about the earth. The Bubbles remain mysterious: Are the gamma-rays - with energies up to a few hundred GeV - produced by hadrons or do they come from Inverse Compton scattering of galactic electrons with the low energy interstellar radiation field? Why are the edges of the bubbles only 3 degree wide? How old are the bubbles.For some time we have been considering a non-Newtonian Cosinusoidal potential U=-G M Cos[ko r]/r, and its complement, a non-Coulombic electric potential U=Q Exp[-ko r]. In both cases, ko =2 pi/400 pc. In this talk we present evidence that our putative potentials acting in concert can help answer the mysteries of the Bubbles.

  11. Internet Investigations: Solving Mysteries on the Information Superhighway.

    ERIC Educational Resources Information Center

    Riley, Tracy; Brown, Mark

    1998-01-01

    Describes how a group of gifted primary-school children in New Zealand explored the Internet in a workshop project organized around solving the mystery of what happened to the Titanic. Insets include the student "contract," a listing of Web sites, and the evaluation instrument. (DB)

  12. Reply to comment by B. Andreotti et al. on ``Solving the mystery of booming sand dunes''

    E-print Network

    Clayton, Robert W.

    Reply to comment by B. Andreotti et al. on ``Solving the mystery of booming sand dunes'' Nathalie M to comment by B. Andreotti et al. on ``Solving the mystery of booming sand dunes,'' Geophys. Res. Lett., 35

  13. Comment on ``Solving the mystery of booming sand dunes'' by Nathalie M. Vriend et al.

    E-print Network

    Clayton, Robert W.

    Comment on ``Solving the mystery of booming sand dunes'' by Nathalie M. Vriend et al. B. Andreotti), Comment on ``Solving the mystery of booming sand dunes'' by Nathalie M. Vriend et al., Geophys. Res. Lett

  14. Baby Stars in Orion Solve Solar System Mystery

    NASA Technical Reports Server (NTRS)

    Wanjek, Christopher

    2003-01-01

    What do X-rays, meteoroids, infant stars in the Orion Nebula, and our solar system have in common? Perhaps much more than anyone thought. Eric Feigelson of Penn State University stumbled onto a connection one day while his thoughts were far from the solar system, turned toward the vibrant neighborhood of young stars, hot gas, and caliginous dust of the Orion Nebula. This nebula, 1500 light-years away, is visible to the naked eye in the constellation Orion, a gem to behold with a good pair of binoculars or a telescope under dark skies. In Orion, Feigelson inadvertently found a possible solution to a long-standing mystery about our own solar system: the presence of exotic isotopes locked away in meteoroids. Scientists have assumed that these short-lived isotopes - special forms of atomic nuclei, such as aluminum-26 and calcium-41 - were transported here by a nearby supernova. Only tenuous evidence for such an explosion exists, but what else could have made the isotopes? The isotopes are about as old as the solar system, and the Sun couldn t possibly have been powerful enough to create them. Well, maybe we need to give the Sun a little more credit. Feigelson found that very young, midsized stars in the Orion Nebula - in the same stellar class as our Sun except they are only a million years old - produce powerful flares visible in X-rays. His team spotted these X-ray flares with the Chandra X-Ray Observatory. These baby-tantrum flares are indeed energetic enough to forge heavy isotopes, Feigelson says. If the infant stars in Orion can do it now, then our Sun could have done the same when the solar system was forming about 4.5 billion years ago, when the Sun itself was only a few million years old.

  15. "Short, Hard Gamma-Ray Bursts - Mystery Solved?????"

    NASA Technical Reports Server (NTRS)

    Parsons, A.

    2006-01-01

    After over a decade of speculation about the nature of short-duration hard-spectrum gamma-ray bursts (GRBs), the recent detection of afterglow emission from a small number of short bursts has provided the first physical constraints on possible progenitor models. While the discovery of afterglow emission from long GRBs was a real breakthrough linking their origin to star forming galaxies, and hence the death of massive stars, the progenitors, energetics, and environments for short gamma-ray burst events remain elusive despite a few recent localizations. Thus far, the nature of the host galaxies measured indicates that short GRBs arise from an old (> 1 Gyr) stellar population, strengthening earlier suggestions and providing support for coalescing compact object binaries as the progenitors. On the other hand, some of the short burst afterglow observations cannot be easily explained in the coalescence scenario. These observations raise the possibility that short GRBs may have different or multiple progenitors systems. The study of the short-hard GRB afterglows has been made possible by the Swift Gamma-ray Burst Explorer, launched in November of 2004. Swift is equipped with a coded aperture gamma-ray telescope that can observe up to 2 steradians of the sky and can compute the position of a gamma-ray burst to within 2-3 arcmin in less than 10 seconds. The Swift spacecraft can slew on to this burst position without human intervention, allowing its on-board x ray and optical telescopes to study the afterglow within 2 minutes of the original GRB trigger. More Swift short burst detections and afterglow measurements are needed before we can declare that the mystery of short gamma-ray burst is solved.

  16. Rosetta - a new target to solve planetary mysteries

    NASA Astrophysics Data System (ADS)

    2004-01-01

    This delay meant that the original mission's target, Comet Wirtanen, could no longer be reached. Instead, a new target has been selected, Comet 67P/Churyumov-Gerasimenko, which Rosetta will encounter in 2014 after a ‘billiard ball’ journey through the Solar System lasting more than ten years. Rosetta’s name comes from the famous ‘Rosetta Stone’, from which Egyptian hieroglyphics were deciphered almost 200 years ago. In a similar way, scientists hope that the Rosetta spacecraft will unlock the mysteries of the Solar System. Comets are very interesting objects for scientists, since their composition reflects how the Solar System was when it was very young and still 'unfinished', more than 4600 million years ago. Comets have not changed much since then. In orbiting Comet Churyumov-Gerasimenko and landing on it, Rosetta will collect information essential to an understanding of the origin and evolution of our Solar System. It will also help discover whether comets contributed to the beginnings of life on Earth. In fact comets are carriers of complex organic molecules that, delivered to Earth through impacts, perhaps played a role in the origin of living forms. Furthermore, ‘volatile’ light elements carried by comets might also have played an important role in forming the Earth’s oceans and atmosphere. “Rosetta is one of the most challenging missions undertaken so far,” says Professor David Southwood, ESA Director of Science. “No one has ever attempted such a mission, unique for its scientific implications as well as for its complex and spectacular interplanetary space manoeuvres.” Before reaching its target in 2014, Rosetta will circle the Sun four times on wide loops in the inner Solar System. During its long trek, the spacecraft will have to endure some extreme thermal conditions. Once it is close to Comet Churyumov-Gerasimenko, scientists will take it through a delicate braking manoeuvre; the spacecraft will then closely orbit the comet, and gently drop a lander on it. It will be landing on a small, fast-moving ‘cosmic bullet’ about whose 'geography' very little is known yet. An amazing 10-year interplanetary trek Rosetta is a three-tonne box-type spacecraft about three metres high, with two 14-metre solar panels. It consists of an orbiter and a lander. The lander is approximately one metre across and 80 centimetres high. It will be attached to the side of the orbiter during the journey to Comet Churyumov-Gerasimenko. Rosetta carries 21 experiments in total, 10 of them on the lander. They will be kept in hibernation during most of its 10-year trek towards the comet. Why does Rosetta's cruise need to take so long? To reach Comet Churyumov-Gerasimenko, the spacecraft needs to go out into deep space as far out from the Sun as Jupiter. No launcher could possibly get Rosetta there directly. ESA's spacecraft will gather speed from gravitational ‘kicks’ provided by four planetary fly-bys: one of Mars in 2007 and three of Earth in 2005, 2007 and 2009. During the trip, Rosetta will also twice pass through the asteroid belt, where a fly-by with one or more of these primitive objects is possible. A number of candidate targets have already been identified, but the final selection will be made after launch, once the amount of surplus fuel has been verified by mission engineers. During these encounters, scientists plan to switch on Rosetta's instruments for scientific studies of these largely unexplored Solar System bodies. Long trips in deep space include many hazards, such as extreme changes in temperature. Rosetta will leave the benign environment of near-Earth space to the dark, frigid regions beyond the asteroid belt. To manage these thermal loads, experts have done very tough pre-launch tests to study Rosetta's endurance. For example, they have heated its external surfaces to more than 150°C, then cooled it to -150°C in the next test. The spacecraft will be fully reactivated prior to the comet rendezvous manoeuvre in 2014. Then, Rosetta will orbit the comet - an object only about 4 kilometres in d

  17. Solving the Mystery of Short Gamma Ray Bursts

    NASA Technical Reports Server (NTRS)

    Gehrels, Neil

    2006-01-01

    Gamma-ray bursts are among the most fascinating occurrences in the cosmos. Until this year, the origin of short gamma-ray bursts was a complete mystery. A new NASA satellite named Swift has now captured the first images of these events and found that they are caused by tremendous explosions in the distant universe.

  18. Mystery #1

    Atmospheric Science Data Center

    2013-04-22

    article title:  MISR Mystery Image Quiz #1     View ... Burr. What is the name of the garden?   Mystery Solved     MISR was built and is managed by ... project:  MISR category:  gallery mystery Pacific date:  Jun 12, 2001 Images:  ...

  19. Surprising spread of volcanic ash key to solving Earth's mysteries: U of A grad

    E-print Network

    Wang, Hao "Howard"

    of science that uses layers of "tephra," or ash, to link and date events in Earth's history. When a volcano Surprising spread of volcanic ash key to solving Earth's mysteries: U of A grad EDMONTON Volcanic ash, which can provide valuable snapshots of Earth's history, appears to drift much farther than

  20. Solving a Mediterranean Mystery: Why Do Winter-Deciduous Trees Dominate Some

    E-print Network

    is very short (e.g. riparian forests), winter-deciduous leaves achieve the larger annual C gain because525 Solving a Mediterranean Mystery: Why Do Winter-Deciduous Trees Dominate Some Woodlands?1 Chris Ineich2 Abstract Current theory suggests Mediterranean climates favor evergreen over winter-deciduous

  1. ALMA to Help Solving Acute Mountain Sickness Mystery

    NASA Astrophysics Data System (ADS)

    2007-04-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) astronomical project will not only enlarge our knowledge of the vast Universe beyond the imaginable. It will also help scientists learn more about the human body. Located 5000m above sea level, in the Chilean Atacama desert, ALMA is the highest site for ground-based astronomy. This property will be put to good use for academic institutions in Chile and in Europe in order to study the human response to extreme altitude conditions. During a ceremony held on 2 April in Antofagasta, the largest town close to ESO's Very Large Telescope, representatives from ALMA, ESO and the University of Antofagasta have officially launched a collaborative agreement that also involves the University of Chile and the University of Copenhagen (Denmark). The newly established cooperation aims at contributing to the promotion of teaching, scientific research, and the expansion of altitude physiology and medicine or other related areas considered appropriate. ESO PR Photo 20/07 ESO PR Photo 20/07 Working at 5000 metres "An increasing number of people are periodically exposed to brisk changes in altitude, and not only for astronomical research," said Jacques Lassalle, the ALMA Safety Manager. "Short stays at high altitude alternate with short stays at sea level but the corresponding shifts are very often established by agreement, and not based on scientific arguments. With this project, we aim at improving our knowledge and procedures in order to protect the long term health of the operators, engineers, and scientists as well as ALMA visitors of all ages and all physical conditions," he added. Around the world, a large number of people systematically commute between sea level and high altitude, for example when working in mountainous mines. This poses stringent conditions that may affect health, wellbeing and working performance. Some of the factors in question are the shift work regime, the perturbation of circadian rhythms, fatigue, family and social isolation, commuting, intermittent high altitude exposure and other environmental challenges such as low temperatures. "An adequate acclimatisation to 2500m altitude requires around two weeks, and we can thus speculate that going to 5000m would require more than one month to achieve complete acclimatisation," said Professor Juan Silva Urra, from the University of Antofagasta. However, short and long term effects of regular commuting between sea level and high altitude have scarcely been studied in biomedical terms. Scientifically based guidelines for appropriate preventive handling and care under these conditions are lacking and the new study will help bridging this gap. Among the studies to be done, some involve continuous monitoring of the human body through portable devices, including measurements of hormone levels and application of psychometric tests. All measurements at 5000m will be carried out on a voluntary basis, under strict safety protocols, with the presence of a doctor from the investigation team, paramedic personnel form ALMA and an ambulance. The symptoms of Acute Mountain Sickness are headache, sicknesses, gastrointestinal inconveniences, fatigue and insomnia that, depending on their intensities, decrease the capacity to carry out the most routine activities. The valuable data collected will enhance our knowledge of human physiology in extreme environments, generating recommendations that will improve wellbeing and health not only in high-altitude observatories, but also in mining and Antarctic personnel. "We are pleased that ALMA is contributing to other disciplines, like medicine, even before the antennas begin to explore the universe," said Felix Mirabel, ESO's representative in Chile. "This outstanding long-term research that will provide crucial information of human physiology to experts worldwide, has been made possible thanks to the combined effort of Chilean and European universities, in collaboration with ALMA". The Atacama Large Millimeter/submillimeter Array (ALMA), a

  2. Rosetta - a comet ride to solve planetary mysteries

    NASA Astrophysics Data System (ADS)

    2003-01-01

    Comets are very interesting objects for scientists, since their composition reflects how the Solar System was when it was very young and still 'unfinished', more than 4600 million years ago. Comets have not changed much since then. By orbiting Comet Wirtanen and landing on it, Rosetta will collect essential information to understand the origin and evolution of our Solar System. It will also help discover whether comets contributed to the beginnings of life on Earth. In fact comets are carriers of complex organic molecules, that - delivered to Earth through impacts - perhaps played a role in the origin of living forms. Furthermore, “volatile” light elements carried by comets may have also played an important role in forming the Earth’s oceans and atmopshere. “Rosetta is one of the most challenging missions ever undertaken so far”, says Prof. David Southwood, ESA Director of Science, “No one before attempted a similar mission, unique for its scientific implications as well as for its complex and spectacular interplanetary space manoeuvres”. Before reaching its target in 2011, Rosetta will circle the Sun almost four times on wide loops in the inner Solar System. During its long trek, the spacecraft will have to endure some extreme thermal conditions. Once it is close to Comet Wirtanen, scientists will take it through a delicate braking manoeuvre; then the spacecraft will closely orbit the comet, and gently drop a lander on it. It will be like landing on a small, fast-moving cosmic bullet that still has - at present - an almost unknown 'geography'. An amazing 8-year interplanetary trek Rosetta is a 3-tonne box-type spacecraft about 3 metres high, with two 14-metre long solar panels. It consists of an orbiter and a lander. The lander is approximately 1 metre across and 80 centimetres high. It will be attached to the side of the Rosetta orbiter during the journey to Comet Wirtanen. Rosetta carries 21 experiments in total, 10 of them on the lander. They will be kept in hibernation during most of its 8-year trek towards Wirtanen. What makes Rosetta's cruise so long? To reach Comet Wirtanen, the spacecraft needs to go out in deep space as far from the Sun as Jupiter is. No launcher could possibly get Rosetta there directly. ESA's spacecraft will gather speed from gravitational ‘kicks’ provided by three planetary fly-bys: one of Mars in 2005 and two of Earth in 2005 and 2007. During the trip, Rosetta will also visit two asteroids, Otawara (in 2006) and Siwa (in 2008). During these encounters, scientists will switch on Rosetta's instruments for calibration and scientific studies. Long trips in deep space include many hazards, such as extreme changes in temperature. Rosetta will leave the benign environment of near-Earth space to the dark, frigid regions beyond the asteroid belt. To manage these thermal loads, experts have done very tough pre-launch tests to study Rosetta's endurance. For example, they have heated its external surfaces to more than 150°C, then quickly cooled it to -180°C in the next test. The spacecraft will be fully reactivated prior to the comet rendezvous manoeuvre in 2011. Then, Rosetta will orbit the comet - an object only 1.2 km wide - while it cruises through the inner Solar System at 135 000 kilometres per hour. At that time of the rendezvous - around 675 million km from the Sun - Wirtanen will hardly show any surface activity. It means that the carachteristic coma (the comet’s ‘atmosphere’) and the tail will not be formed yet, because of the large distance from the Sun. The comet's tail is in fact made of dust grains and frozen gases from the comet's surface that vapourise because of the Sun's heat. During 6-month, Rosetta will extensively map the comet surface, prior to selecting a landing site. In July 2012, the lander will self-eject from the spacecraft from a height of just one kilometre. Touchdown will take place at walking speed - less than 1 metre per second. Immediately after touchdown, the lander will fire a harpoon into the ground to avoid bouncing off the surface back in

  3. SNO: solving the mystery of the missing neutrinos

    SciTech Connect

    Jelley, Nick; Poon, Alan

    2007-03-30

    The end of an era came on 28 November 2006 when the Sudbury Neutrino Observatory (SNO) finally stopped data-taking after eight exciting years of discoveries. During this time the Observatory saw evidence that neutrinos, produced in the fusion of hydrogen in the solar core, change flavour while passing through the Sun on their way to the Earth. This observation explained the longstanding puzzle as to why previous experiments had seen fewer solar neutrinos than predicted and confirmed that these elusive particles have mass. Solar neutrinos were first detected in Ray Davis's radiochemical experiment in 1967, for which discovery he shared the 2002 Nobel Prize in Physics. Surprisingly he found only about a third of the number predicted from models of the Sun's output. This deficit, the so-called Solar Neutrino Problem, was confirmed by Kamiokande-II while other experiments saw related deficits of solar neutrinos. A possible explanation for this deficit, suggested by Gribov and Pontecorvo in 1969, was that some of the electron-type neutrinos, which are produced in the Sun, had ''oscillated'' into neutrinos that could not be detected in the Davis detector. The oscillation mechanism requires that neutrinos have non-zero mass. The unique advantage, which was pointed out by the late Herb Chen in 1985, of using heavy water (D{sub 2}O) to detect the neutrinos from {sup 8}B decays in the solar fusion process is that it enables both the number of electron-type and of all types of neutrinos to be measured. A comparison of the flux of electron-type neutrinos to that of all flavours could then reveal whether flavour transformation is the cause of the solar neutrino deficit. In heavy water neutrinos of all types can break a deuteron apart into its constituent proton and neutron (neutral-current reaction), while only electron-type neutrinos can change the deuteron into two protons and release an electron (charged-current reaction). SNO was designed by scientists from Canada, the USA and the UK to attain a detection rate of about 10 solar neutrinos per day using 1000 tonnes of heavy water. Neutrino interactions were detected by 9,456 photomultiplier tubes surrounding the heavy water, which was contained in a 12-m diameter acrylic sphere. This sphere was surrounded by 7000 tonnes of ultra-pure water to shield against radioactivity. Figure 1 shows the layout of the SNO detector, which is located about 2 km underground in Inco's Creighton nickel mine near Sudbury in Canada, to all but eliminate cosmic rays from reaching the detector. The pattern of hit photomultiplier tubes following the creation of an electron by an electron-type neutrino is shown in Figure 2.

  4. ESA's Integral solves thirty-year old gamma-ray mystery

    NASA Astrophysics Data System (ADS)

    Integral solves mystery hi-res Size hi-res: 60 kb Credits: Credit: ESA, F. Lebrun (CEA-Saclay). ESA's Integral solves thirty-year old gamma-ray mystery The central regions of our galaxy, the Milky Way, as seen by Integral in gamma rays. With its superior ability to see faint details, Integral correctly reveals the individual sources that comprised the foggy, gamma-ray background seen by previous observatories. The brightest 91 objects seen in this image were classified by Integral as individual sources, while the others appear too faint to be properly characterized at this stage. During the spring and autumn of 2003, Integral observed the central regions of our Galaxy, collecting some of the perpetual glow of diffuse low-energy gamma rays that bathe the entire Galaxy. These gamma rays were first discovered in the mid-1970s by high-flying balloon-borne experiments. Astronomers refer to them as the 'soft' Galactic gamma-ray background, with energies similar to those used in medical X-ray equipment. Initially, astronomers believed that the glow was caused by interactions involving the atoms of the gas that pervades the Galaxy. Whilst this theory could explain the diffuse nature of the emission, since the gas is ubiquitous, it failed to match the observed power of the gamma rays. The gamma rays produced by the proposed mechanisms would be much weaker than those observed. The mystery has remained unanswered for decades. Now Integral's superb gamma-ray telescope IBIS, built for ESA by an international consortium led by Principal Investigator Pietro Ubertini (IAS/CNR, Rome, Italy), has seen clearly that, instead of a fog produced by the interstellar medium, most of the gamma-rays are coming from individual celestial objects. In the view of previous, less sensitive instruments, these objects appeared to merge together. In a paper published today in "Nature", Francois Lebrun (CEA Saclay, Gif sur Yvette, France) and his collaborators report the discovery of 91 gamma-ray sources towards the direction of the Galactic centre. Lebrun's team includes Ubertini and seventeen other European scientists with long-standing experience in high-energy astrophysics. Much to the team's surprise, almost half of these sources do not fall in any class of known gamma-ray objects. They probably represent a new population of gamma-ray emitters. The first clues about a new class of gamma-ray objects came last October, when Integral discovered an intriguing gamma-ray source, known as IGRJ16318-4848. The data from Integral and ESA's other high-energy observatory XMM-Newton suggested that this object is a binary system, probably including a black hole or neutron star, embedded in a thick cocoon of cold gas and dust. When gas from the companion star is accelerated and swallowed by the black hole, energy is released at all wavelengths, mostly in the gamma rays. However, Lebrun is cautious to draw premature conclusions about the sources detected in the Galactic centre. Other interpretations are also possible that do not involve black holes. For instance, these objects could be the remains of exploded stars that are being energised by rapidly rotating celestial 'powerhouses', known as pulsars. Observations with another Integral instrument (SPI, the Spectrometer on Integral) could provide Lebrun and his team with more information on the nature of these sources. SPI measures the energy of incoming gamma rays with extraordinary accuracy and allows scientist to gain a better understanding of the physical mechanisms that generate them. However, regardless of the precise nature of these gamma-ray sources, Integral's observations have convincingly shown that the energy output from these new objects accounts for almost ninety per cent of the soft gamma-ray background coming from the centre of the Galaxy. This result raises the tantalising possibility that objects of this type hide everywhere in the Galaxy, not just in its centre. Again, Lebrun is cautious, saying, "It is tempting to think that we can simply extrapolate our results to the entire Galaxy.

  5. In a Flash, NASA Helps Solve 35-Year-Old Cosmic Mystery

    NASA Astrophysics Data System (ADS)

    2005-10-01

    Scientists have solved the 35-year-old mystery of the origin of powerful, split-second flashes of light known as short gamma-ray bursts. These flashes, brighter than a billion galaxies, yet lasting only a few milliseconds, have been simply too fast to catch - until now. Through the unprecedented coordination of observations from several ground-based telescopes and NASA satellites, scientists determined the flashes arise from violent collisions in space. The clashes are either between a black hole and a neutron star or between two neutron stars. In either scenario, the impact creates a new black hole. In at least one burst, scientists saw tantalizing, first-time evidence of a black hole eating a neutron star. The neutron star was first stretched into a crescent, then swallowed by the black hole. Two recently detected bursts are featured in four papers in this week's Nature magazine. These observations could enable direct detection of exotic gravitational waves that have never before been seen. "Gamma-ray bursts in general are notoriously difficult to study, but the shortest ones have been next to impossible to pin down," said Dr. Neil Gehrels, principal investigator for the Swift satellite at NASA's Goddard Space Flight Center, Greenbelt, Md. "All that has changed. We now have the tools in place to study these events," he said. Hubble Optical Image of GRB 050709 Hubble Optical Image of GRB 050709 Gamma-ray bursts, first detected in the 1960s, are the most powerful explosions known. They are random, fleeting and can occur from any region of the sky. Two years ago, scientists discovered longer bursts, lasting more than two seconds, arise from the explosion of very massive stars. About 30 percent of bursts are short and under two seconds. The Swift satellite detected a short burst on May 9, and NASA's High-Energy Transient Explorer (HETE) detected another on July 9. The May 9 event marked the first time scientists identified an afterglow for a short gamma-ray burst, something commonly seen after long bursts. "We had a hunch that short gamma-ray bursts came from a neutron star crashing into a black hole or another neutron star, but these new detections leave no doubt," said Dr. Derek Fox, assistant professor of Astronomy & Astrophysics at Penn State University, State College, Pa. Fox is lead author of one Nature report detailing a multi-wavelength observation. Animation of Colliding Binary Neutron Stars Animation of Colliding Binary Neutron Stars Fox's team discovered the X-ray afterglow of the July 9 burst with NASA's Chandra X-ray Observatory. A team led by Jens Hjorth, a professor at the University of Copenhagen identified the optical afterglow using the Danish 1.5-meter telescope at the La Silla Observatory in Chile. Fox's team continued studying the afterglow with NASA's Hubble Space Telescope and ground-based telescopes of the Carnegie Institution, the National Astronomical Observatory of Japan, and the National Radio Astronomy Observatory. "The July 9 burst was like the dog that didn't bark," said Dr. George Ricker, HETE principal investigator at the Massachusetts Institute of Technology, Cambridge, and co-author of another Nature article. "Powerful telescopes detected no supernova as the gamma-ray burst faded, arguing against the explosion of a massive star. Also, the July 9 burst, and probably the May 9 burst, are located in the outskirts of their host galaxies, just where old merging binaries are expected," he added. Mergers create gravitational waves, ripples in space-time predicted by Einstein but never directly detected. The July 9 burst was about 2 billion light-years away. A big merger closer to the Earth could be detected by the National Science Foundation's Laser Interferometer Gravitational-Wave Observatory (LIGO). If Swift detects a nearby short burst, scientists could go back and check the data with a precise time and location. "This is good news for LIGO," said Dr. Albert Lazzarini, Data & Computing group leader at the California Institut

  6. Mystery #23

    Atmospheric Science Data Center

    2013-04-22

    ... as an analogue for an extraterrestrial environment during scientific simulation studies.   Mystery Solved   ... RIS/ Jet Propulsion Laboratory) and Shirley Mims (Glendale Community College/Jet Propulsion Laboratory). Other formats available at ...

  7. Neolithic trepanation decoded- A unifying hypothesis: Has the mystery as to why primitive surgeons performed cranial surgery been solved?

    PubMed Central

    Faria, Miguel A.

    2015-01-01

    The perplexing mystery of why so many trephined skulls from the Neolithic period have been uncovered all over the world representing attempts at primitive cranial surgery is discussed. More than 1500 trephined skulls have been uncovered throughout the world, from Europe and Scandinavia to North America, from Russia and China to South America (particularly in Peru). Most reported series show that from 5-10% of all skulls found from the Neolithic period have been trephined with single or multiple skull openings of various sizes. The unifying hypothesis proposed by the late medical historian Dr. Plinio Prioreschi (1930-2014) regarding the reason for these trepanations (trephinations) is analyzed. It is concluded that Dr. Prioreschi's cohesive explanation to explain the phenomenon is valid and that his intriguing hypothesis is almost certainly correct. In the opinion of this author, the mystery within an enigma has been solved. PMID:25984386

  8. The Reading Detective Club: Solving the Mysteries of Reading. A Teacher's Guide.

    ERIC Educational Resources Information Center

    Goodman, Debra

    Noting that readers are a lot like detectives, this two-part book (a professional book for teachers and a fun "nonworkbook" for students) introduces students and teachers to "mystery cases" that are actually reading strategy lessons for third through eighth graders and their teachers. The teacher section offers a comprehensive overview of the…

  9. Mysterious POND Mysterious POND

    E-print Network

    Kitamura, Yoshifumi

    Mysterious POND *1 *2 *2 Mysterious POND Satoshi Sakurai*1 , Kazuhiro Asai*2 and Yoshifumi Kitamura*2 Abstract -- We present a media art work"Mysterious POND", which gives a mysterious illusion of Mysterious POND, followed by some sceneries of the demonstrations. Finally, the future extensions of the work

  10. VLBA "Movie" Gives Scientists New Insights On Workings of Mysterious Microquasars

    NASA Astrophysics Data System (ADS)

    2004-01-01

    Astronomers have made a 42-day movie showing unprecedented detail of the inner workings of a strange star system that has puzzled scientists for more than two decades. Their work is providing new insights that are changing scientists' understanding of the enigmatic stellar pairs known as microquasars. SS 433 Frame from SS 433 Movie: End to end is some 200 billion miles. CREDIT: Mioduszewski et al., NRAO/AUI/NSF Image Files Single Frame Overall Jet View (above image) VLBA Movie (animated gif, 2.3 MB) Animated graphic of SS 433 System (18MB) (Created using software by Robert Hynes, U.Texas) Annotated brightening graphic Unannotated brightening Frame 1 Unannotated brightening Frame 2 "This once-a-day series of exquisitely-detailed images is the best look anyone has ever had at a microquasar, and already has made us change our thinking about how these things work," said Amy Mioduszewski, of the National Radio Astronomy Observatory (NRAO), in Socorro, New Mexico. The astronomers used the National Science Foundation's Very Long Baseline Array (VLBA), a system of radio telescopes stretching from Hawaii to the Caribbean, to follow daily changes in a binary-star system called SS 433, some 15,000 light-years from Earth in the constellation Aquila. Mioduszewski worked with Michael Rupen, Greg Taylor and Craig Walker, all of NRAO. They reported their findings to the American Astronomical Society's meeting in Atlanta, Georgia. SS 433 consists of a neutron star or black hole orbited by a "normal" companion star. The powerful gravity of the neutron star or black hole is drawing material from the stellar wind of its companion into an accretion disk of material tightly circling the dense, central object prior to being pulled onto that object. This disk propels jets of subatomic particles outward from its poles. In SS 433, the particles in the jets move at 26 percent of the speed of light; in other microquasars, the jet material moves at 90-95 percent of light speed. The disk in SS 433 wobbles like a child's top, causing its jets to move in a circle every 164 days. By imaging SS 433 daily, the astronomers were able to trace individual ejections of material in these jets as they moved outward from the center. In addition, they could track the jets' precession, the movement caused by the disk's wobble. In other microquasars, blobs of material shot from the core become fainter, as seen with radio telescopes, as they move outward. However, in SS 433, blobs routinely brighten at specific distances from the core. From earlier studies, researchers had concluded that such brightening always occurs at one specific distance. The VLBA movie shows, instead, that there are multiple brightening regions and not all blobs brighten at all the regions. "We think the ejected material brightens because it's slamming into something," Rupen said. "However, whatever it's hitting has to be replenished somehow so that the brightening can occur again when the jet sweeps through that area the next time," he added. "It also appears that it isn't always replenished, because the brightening doesn't always happen," Mioduszewski pointed out. The VLBA movie revealed vital new information about another part of SS 433 -- material moving outward from the core, but not part of the superfast jets. This material moves outward in a direction not quite perpendicular to the direction of the jets. Discovered with the VLBA in 2000, this material had been seen only in one-time snapshots before, but the movie shows the steady evolution of its movement for the first time. That motion was the key to a possible answer to two riddles -- the source of the slower-moving material itself and the source of whatever the jet blobs are hitting when they brighten. "What seems most plausible to us is that the accretion disk is putting out a broad wind," Rupen explained. That broad wind from the disk hits a denser wind coming from the "normal" companion star to generate the radio waves seen coming from the nonjet region. The same

  11. Perfecting scientists’ collaboration and problem-solving skills in the virtual team environment

    Technology Transfer Automated Retrieval System (TEKTRAN)

    Perfecting Scientists’ Collaboration and Problem-Solving Skills in the Virtual Team Environment Numerous factors have contributed to the proliferation of conducting work in virtual teams at the domestic, national, and global levels: innovations in technology, critical developments in software, co-lo...

  12. The mysteries of the sea: How magnetics can help to solve them

    NASA Astrophysics Data System (ADS)

    Barckhausen, Udo

    2015-04-01

    Determination of the Earth's magnetic field over the oceans played a key role in understanding plate tectonics in the 1960s and has helped to answer many geodynamic questions since then. Satellite missions have nicely charted the Earth's magnetic field over its entire surface during the last 20 years. However, at the altitude of satellite orbits merely wavelengths greater than ~ 100 km can be resolved, thus, implying that most of the geologically interesting anomalies with sources in the Earth's crust can only be measured on the ground. For a long time these ground measurements have been carried out with the robust and easy-to-use Proton Precession magnetometers towed astern of research vessels. By using oriented Vector Magnetometers we are now returning to the Gaussian roots of measurements, quantifying the magnetic field in its components. This is realised either with towed instruments or with sensors mounted to the superstructure of research vessels. Applications for the use of modern instruments and methods applicable to vector data range from large scale analysis of seafloor spreading anomalies over addressing long standing tectonic questions in isolated ocean basins to high resolution investigations of mineral deposits at the seafloor. In the equatorial Eastern Pacific it was possible to precisely date the age of the oceanic crust over large areas between the Clarion and Galapagos fracture zones, where differences to existing global age models of more than 10 m.y. in some places could be found. In the Colombia Basin of the Caribbean, the analysis of vector data provides an unexpected new insight into the tectonic origin of at least one part of the Caribbean platform. High-resolution magnetic mapping at the sea surface and deep tow profiles reveal hydrothermally-altered rocks near active spreading centres and associated polymetallic sulphide deposits. During marine survey expeditions, magnetic measurements can be carried out almost any time and in combination with a wide range of other geophysical investigations. Modern magnetometers can be piggy-backed to many deep towed instruments, providing additional information with little extra effort. Latest technical developments combine deep tow magnetics with electromagnetic methods, opening a further fascinating window to the mysteries of the sea.

  13. Specular Reflections from Titan's Equatorial Region: Solving the Decade Old Mystery

    NASA Astrophysics Data System (ADS)

    Hofgartner, J. D.; Campbell, D. B.; Hayes, A.; Lunine, J. I.

    2014-12-01

    Specular reflections from Titan's equatorial region have been detected using the Arecibo Observatory's (AO) 13 cm wavelength radar system (Campbell et al., 2003, Science, 302, 431). Fitting the echo spectra to radar scattering models indicated that they originated from smooth surfaces with root-mean-square slopes of only a few degrees; on this basis they were interpreted as evidence for liquid surfaces. The Cassini Saturn Orbiter however has detected stable surface liquids only in the polar regions and not in the southern tropical regions covered by the AO tracks. High resolution Cassini imagery that overlaps with the AO tracks between the years 2000 and 2008 does not suggest the presence of hydrocarbon liquids and exhibits no apparent correlation with the 13 cm scattering (Black et al., 2011, Icarus, 212, 300). In this work in progress, we explore alternative explanations for the origin of these low latitude specular reflections and attempt to resolve this now decade old mystery. In particular, we use the accumulating Cassini RADAR altimetry coverage to compare the nadir backscatter at 2.2 cm to that at 13 cm. This nadir-to-nadir comparison allows us to constrain whether the southern tropical regions are also smooth and specular at smaller scales. We also plan to constrain whether these regions are representative of Titan in general or have unusually smooth surface by utilizing the complete Cassini altimetry dataset that includes observations dispersed around the globe. Distant Cassini RADAR scatterometry-mode observations suggest that Titan exhibits a greater nadir backscatter than expected from traditional quasi-specular plus diffuse backscattering models (L. Wye, 2011, Ph.D. Thesis, Stanford University), hinting that unusually specular radar echoes may be the general behavior for Titan. Additionally, we employ the long baseline of Cassini observations over nearly half a Titan year, to constrain the possible temporal evolution in backscatter that was suggested by the AO echoes. We will also update the comparison of the Arecibo tracks with overlapping Cassini imagery, both by incorporating new coverage and through improvements in determining the regions of overlap.

  14. NCI Scientists Solve Structure of Protein that Enables MERS Virus to Spread | Poster

    Cancer.gov

    Scientists at the Frederick National Lab have produced three crystal structures that reveal a specific part of a protein that can be targeted to fight the Middle East respiratory syndrome coronavirus (MERS-CoV), which causes an emerging viral respiratory illness. Senior Investigator David Waugh, Ph.D., Macromolecular Crystallography Laboratory, has solved the structure of an enzyme known as the 3C-like protease (3CLpro), which, if blocked, can prevent the virus from replicating...

  15. Young Stars in Orion May Solve Mystery of Our Solar System

    NASA Astrophysics Data System (ADS)

    2001-09-01

    Scientists may have to give the Sun a little more credit. Exotic isotopes present in the early Solar System--which scientists have long-assumed were sprinkled there by a powerful, nearby star explosion--may have instead been forged locally by our Sun during the colossal solar-flare tantrums of its baby years. The isotopes--special forms of atomic nuclei, such as aluminum-26, calcium-41, and beryllium-10--can form in the X-ray solar flares of young stars in the Orion Nebula, which behave just like our Sun would have at such an early age. The finding, based on observations by the Chandra X-ray Observatory, has broad implications for the formation of our own Solar System. Eric Feigelson, professor of astronomy and astrophysics at Penn State, led a team of scientists on this Chandra observation and presents these results in Washington, D.C., today at a conference entitled "Two Years of Science with Chandra". "The Chandra study of Orion gives us the first chance to study the flaring properties of stars resembling the Sun when our solar system was forming," said Feigelson. "We found a much higher rate of flares than expected, sufficient to explain the production of many unusual isotopes locked away in ancient meteorites. If the young stars in Orion can do it, then our Sun should have been able to do it too." Scientists who study how our Solar System formed from a collapsed cloud of dust and gas have been hard pressed to explain the presence of these extremely unusual chemical isotopes. The isotopes are short-lived and had to have been formed no earlier than the creation of the Solar System, some five billion years ago. Yet these elements cannot be produced by a star as massive as our Sun under normal circumstances. (Other elements, such as silver and gold, were created long before the creation of the solar system.) The perplexing presence of these isotopic anomalies, found in ancient meteoroids orbiting the Earth, led to the theory that a supernova explosion occurred very close to the Solar System's progenitor gas cloud, simultaneously triggering its collapse and seeding it with short-lived isotopes. Solar flares could produce such isotopes, but the flares would have to be hundreds of thousands of times more powerful and hundreds of times more frequent than those our Sun generates. Enter the stars in the Orion Nebula. This star-forming region has several dozen new stars nearly identical to our Sun, only much younger. Feigelson's team used Chandra to study the flaring in these analogs of the early Sun and found that nearly all exhibit extremely high levels of X-ray flaring--powerful and frequent enough to forge many of the kinds of isotopes found in the ancient meteorites from the early solar system. "This is a very exciting result for space X-ray astronomy," said Donald Clayton, Centennial Professor of Physics and Astronomy at Clemson University. "The Chandra Penn State team has shown that stellar-flare acceleration produces radioactive nuclei whether we want them or not. Now the science debate can concentrate on whether such irradiation made some or even all of the extinct radioactivities that were present when our solar system was formed, or whether some contamination of our birth molecular cloud by external material is also needed." "This is an excellent example of how apparently distant scientific fields, like X-ray astronomy and the origins of solar systems, can in fact be closely linked," said Feigelson. The Orion observation was made with Chandra's Advanced CCD Imaging Spectrometer, which was conceived and developed for NASA by Penn State and Massachusetts Institute of Technology under the leadership of Gordon Garmire, the Evan Pugh Professor of Astronomy and Astrophysics at Penn State. The Penn State observation team includes Pat Broos, James Gaffney, Gordon Garmire, Leisa Townsley and Yohko Tsuboi. Collaborators also include Lynne Hillenbrand of CalTech and Steven Pravdo of the NASA Jet Propulsion Laboratory. Background: Isotopes are atoms whose nuclei have d

  16. Solving Wakulla Springs underwater mysteries. Using GPS to map Florida's underground caverns

    USGS Publications Warehouse

    Am, Ende B.

    2002-01-01

    Located in the Woodville Karst Plain stretching south from Tallahassee to the Gulf of Mexico, Florida's Wakulla Springs is one of the largest and deepest freshwater Springs in the world. It is also a gateway into one of the longest underwater cave system in the United States, a system that remained largely unexplored until recently. Soon, however, thanks to one of the world's most extreme scientific and exploration-related diving projects ever undertaken, visitors to Wakulla Springs State Park will be able to take a virtual tour through the Spring's huge underwater labyrinth. Using such cutting-edge technology as a 3D Digital Wall Mapper (DWM) and the Global Positioning System (GPS), the Wakulla 2 Expedition - with 151 volunteer cave divers, scientists and engineers from all over the world - created the world's first three-dimensional digital map of an underwater cave. Underwater caves are priceless treasures, helping supply fresh water to the region as well as acting as 'time capsules' to the past. Home to creatures found in few other places, areas such as Wakulla face threats of pollution and over-development. Wakulla 2 hopes their 3D interactive 'swim through' will help increase the understanding and preservation of these important areas.

  17. Perfecting Scientists' Collaboration and Problem-Solving Skills in the Virtual Team Environment

    NASA Astrophysics Data System (ADS)

    Jabro, A.; Jabro, J.

    2012-04-01

    PPerfecting Scientists' Collaboration and Problem-Solving Skills in the Virtual Team Environment Numerous factors have contributed to the proliferation of conducting work in virtual teams at the domestic, national, and global levels: innovations in technology, critical developments in software, co-located research partners and diverse funding sources, dynamic economic and political environments, and a changing workforce. Today's scientists must be prepared to not only perform work in the virtual team environment, but to work effectively and efficiently despite physical and cultural barriers. Research supports that students who have been exposed to virtual team experiences are desirable in the professional and academic arenas. Research supports establishing and maintaining established protocols for communication behavior prior to task discussion provides for successful team outcomes. Research conducted on graduate and undergraduate virtual teams' behaviors led to the development of successful pedagogic practices and assessment strategies.

  18. Geometry-Lithology-Origin: Solving the mystery of the Late Miocene mounded features below Lake Balaton

    NASA Astrophysics Data System (ADS)

    Visnovitz, Ferenc; Horváth, Ferenc; Surányi, Gergely

    2014-05-01

    The Department of Geophysics and Space Sciences of Eötvös University has carried out single- and multichannel water seismic surveys at the Lake Balaton since 1993. The dense grid of 2D profiles offers a high resolution image of the Late Miocene sedimentary strata (Tihany, Somló and Szák Formations) up to a thickness of 200 meters below the lake. These strata can be divided into smaller sedimentary units by numerous parasequence boundaries (Sztanó&Magyar, 2007). In one of these parasequence interesting, high amplitude mounded features have been observed that follow a seismic horizon over large area. It means that these features indicate a Late Miocene regional event. In terms of their shape these mounds are few tens of meters wide, several tens to a hundreds of meters long and few meters high. Their geometry and inner structure were mapped from 2D segments that were used for 3D reconstructions. The shape and stratigraphic position of these features have inspired Sacchi and Horvath (1999) to interpret them as the subsurface equivalent of the fresh-water siliceous-limestone mounds exposed on the Tihany Peninsula. They held these mounds as an evidence of dryland conditions in the time period of the formation of a Late Miocene erosional surface (PAN-2) that they regarded as a 3rd order sequence boundary. In addition to this so called "travertine" concept another explanation was also formulated as the mounds are the product of sedimentary failures e.g. slumps or water escape. To solve the problem an offshore drilling with a total depth of 19 meters was accomplished in October 2013 to sample one of these mounds and determine their origin. The well has not crossed any travertine body, instead alternating layers of clay-silt and very fine sand - without any convincing sign of fluid escape structures - were found in the core (typical lithology of the Tihany Formation). 3D structural analysis of the mounds revealed spherical organization composing bodies that are superposed on each other. The latter can be interpreted as series of small thrusts in a relatively thin mudstone layer. As coring has found silty material, without the presence of any fluid escape structures the most possible explanation for these features is sheet slumping mechanism that could be induced by seismicity. Although "travertine" concept has been rejected, these mounds should indicate a regionally important geological event that could strengthen correlation of erosional surfaces such us PAN-2 from outcrop to water seismic images. Such an event could be possible the start of the 8 Ma volcanism in the area. Work was financed by OTKA NK83400 research fund. References: Sacchi, M.; Horváth, F.; Magyari O. (1999). Role of unconformity-bounded units in the stratigraphy of the continental record: a case study from the Late Miocene of the western Pannonian basin, Hungary. In: Durand, B. Jolivet, L., Horváth F. & Séranne, M. (eds), The Mediterranean Basins: Tertiary Extension within the Alpine Orogen. Geological Society, London, Special Publications, 156, 357-390. Sztanó, O. & Magyar I. (2007): Deltaic parasequences on gamma logs, ultra-high resolution seismic images and outcrops of Lake Pannon deposits. Joannea Geol. Palaont. 9: 105-108.

  19. Century-old Mystery of Puccinia striiformis Life History Solved with the Identification of Berberis as an Alternate Host

    Technology Transfer Automated Retrieval System (TEKTRAN)

    The life history of Puccinia striiformis remains a mystery because the alternate host has never been found. Inoculation of grasses using aeciospores from naturally infected Berberis chinensis and B. koreana resulted in infection on Poa pratensis, producing uredinia typical of stripe rust caused by P...

  20. The Mysterious Chamber of Commerce Selmer Bringsjord

    E-print Network

    Bringsjord, Selmer

    The Mysterious Chamber of Commerce Selmer Bringsjord September 13, 1995 Some mysteries are harder­of­cake mystery: Why does the Rensselaer Chamber of Commerce support the Green Island Incinerator while? In order to obtain some valuable clues that may help in solving this mystery, I encourage readers to obain

  1. Mystery Person

    ERIC Educational Resources Information Center

    O'Brien, Tom

    2011-01-01

    This article features a mathematical game called "Mystery Person." The author describes how the Mystery Person game was tried with first-graders [age 6]. The Mystery games involve the generation of key questions, the coordination of information--often very complex information--and the formulation of consequences based on this coordination.…

  2. Modern Solar Mysteries

    NASA Technical Reports Server (NTRS)

    Hathaway, David H.

    2004-01-01

    100 years ago we thought that the Sun and stars shone as a result of slow gravitational contraction over a few tens of millions of years - putting astronomers at odds with geologists who claimed that the Earth was much, much older. That mystery was solved in the 1920s and 30s with the discovery of nuclear energy (proving that the geologists had it right all along). Other scientific mysteries concerning the Sun have come and gone but three major mysteries remain: 1) How does the Sun produce sunspots with an 11-year cycle? 2) What produces the huge explosions that result in solar flares, prominence eruptions, and coronal mass ejections? and 3) Why is the Sun's outer atmosphere, the corona, so darned hot? Recent progress in solar astronomy reveals a single key to understanding all three of these mysteries.

  3. Mysterious Beginnings

    ERIC Educational Resources Information Center

    Pinkcombe, Josie; Ellyn, Tracy

    2009-01-01

    Introduce students to humankind's mysterious beginnings with a captivating sense of mystery. Low lighting and simple percussion music will add to the mood. Allow students time to leave behind the sunshine of this modern era and crawl through the narrow tunnel of their imaginations into an immense, dark, underground cave. This is, in fact, was what…

  4. Mystery Boxes, X Rays, and Radiology.

    ERIC Educational Resources Information Center

    Thomson, Norman

    2000-01-01

    Indicates the difficulties of teaching concepts beyond light and color and creating memorable learning experiences. Recommends sequential activities using the mystery box approach to explain how scientists and doctors use photon applications. (YDS)

  5. Biology Today. Ah, Sweet Mysteries of Life.

    ERIC Educational Resources Information Center

    Flannery, Maura C.

    1991-01-01

    Mysteries of the biological past that paleontologists are trying to solve are discussed. Topics include first seeds, fossils and computers, packrat middens, charcoal clues, soft parts, Burgess shale, halkieriids, toe count, whales with feet, long necks, and changing functions. (KR)

  6. Detective Scientist - Duration: 31 seconds.

    NASA Video Gallery

    NASA has many detectives looking for clues to solve a mystery, like "science detective" Monsi Roman. She is making sure the water and air on board the International Space Station are safe for the a...

  7. Murder Mystery Day Day event for young people in care in school years 10-13

    E-print Network

    Jackson, Sophie

    Murder Mystery Day Day event for young people in care in school years 10-13 Develop your scientific investigative skills while investigating a fiendish crime! Take part in solving a murder mystery activity, plus: Saturday 11 July 2015 www.cam.ac.uk/care-events #12;Murder Mystery Day www

  8. Guided Research in Middle School: Mystery in the Media Center. Second Edition

    ERIC Educational Resources Information Center

    Harrington, LaDawna

    2011-01-01

    A little imagination, a little drama, a little mystery. Using the guided inquiry model in this updated, second edition, students become detectives at Information Headquarters. They solve a mystery-and enhance their problem-solving and literacy skills. Middle school is a crucial time in the development of problem-solving, critical-thinking, and…

  9. A Coprolite Mystery: Who Dung It?

    ERIC Educational Resources Information Center

    Clary, Renee; Wandersee, James

    2011-01-01

    Discover the secrets contained in fossilized feces. Few topics in middle school classrooms capture students' enthusiasm and interest as do coprolites. These trace fossils offer classroom opportunities for integrated life and Earth sciences study, a stranger-than-fiction history of science, and an opportunity to solve mysteries. (Contains 8…

  10. Using Classic Mystery Stories in Teaching.

    ERIC Educational Resources Information Center

    Sheldon, Stephen H.; Noronha, Peter A.

    1990-01-01

    One third-year clinical clerkship in pediatrics has included Sherlock Holmes mysteries in its introductory curriculum, providing students with a model clinical problem-solving process and a list of issues on which they will need information. The nonclinical cases provide an effective and entertaining vehicle for learning clinical reasoning. (MSE)

  11. The Mystery Begins

    ERIC Educational Resources Information Center

    Harrington, LaDawna

    2008-01-01

    All teachers and media specialists are looking for the "hook" that will engage their students and make them want to learn--and according to the author, mystery stories are a perfect way to create that hook. Here, she presents a unit on mysteries, intended for collaboration between media specialists and language arts teachers. The unit uses…

  12. Element Genesis - Solving the Mystery (Video Presentation)

    NASA Astrophysics Data System (ADS)

    Mochizuki, Yuko

    2001-10-01

    Our institute (RIKEN) produced a video on nucleosynthesis. Its new English version is presented. Y. M., I. Tanihata, Y. Yano, and R. Boyd are science editors for this. Time length of the video is 30 minutes. The primary characteristic of this video is that we have employed a number of 2-D and 3-Dimensional visualizations and animations based on an updated understanding of nuclear physics and astrophysics. One of the emphasized points is that microscopic physics (i.e., nuclear physics) and macroscopic physics (i.e., astrophysics) are strongly connected. It contains explanation on the chart of the nuclides, nuclear burning in the sun, big-bang nucleosynthesis, stellar nucleosynthesis, ``beta-stability valley", the s-process, the r-process, production of an RI beam, etc., and professors D. Arnett, T. Kajino, K. Langanke, K. Sato, C. Sneden, I. Tanihata, and F.-K. Thielemann appear as interviewees. Our prime target is college freshmen. We hope that this video would be useful for education both in the fields of astrophysics and nuclear physics at universities and even at high schools. Our institute is accordingly developing a distribution system of this video and it will be available soon at the cost price (please visit our web site for details: http://www.rarf.riken.go.jp/video). The Japanese version was awarded the prize of the Minister of Education, Culture, Sports, Science, and Technology of Japan 2001.

  13. Ideas in action: Solving a cavitation mystery

    SciTech Connect

    1995-12-31

    Cavitation caused significant erosion from 1985 through 1990 on turbine runners at the 970-MW Murray 1 Power Station operated by Snowy Mountains Hydro-Electric Authority (SMHEA) in Australia. The problem was perplexing because no obvious cause could be found. Investigation eventually showed the problems stemmed form the runners sagging slightly from the correct height. Corrective measures, which included adjustment of runners and new control settings for the units, appear to have relieved the cavitation. The adjustments also reduced stress on the unit thrust-bearings, eliminating a future maintenance headache.

  14. Solving the Mystery of Plant Names.

    ERIC Educational Resources Information Center

    Mardiney, Robert

    1986-01-01

    Details how the study of wildflower names provides clues to their history, use, or appearance and ties in with other disciplines such as religion, linguistics, medicine, and history. Cites seven references. (NEC)

  15. The Paluxy River Footprint Mystery--Solved.

    ERIC Educational Resources Information Center

    Cole, John R., Ed.; Godfrey, Laurie R., Ed.

    1985-01-01

    This document points out that creationists claim that humans and dinosaurs lived together in Texas just before Noah's flood by citing alleged human footprints found side-by-side with those of dinosaurs in the Cretaceous limestone of the Paluxy River near Glen Rose, Texas. An investigation was conducted to determine if this claim were true.…

  16. Word Detectives: Solving the Mystery of Vocabulary.

    ERIC Educational Resources Information Center

    Elliott, Deborah A.; Formhals, Marilyn A.; Wheat, Jon G.

    This research addressed vocabulary knowledge, which refers to the understanding of words, the overall ideas and concepts being communicated, and the ability to use those words in the appropriate context. The targeted population consisted of students in kindergarten, first grade, and fourth grade. An analysis of School Improvement Plans revealed a…

  17. Building Collections. Mystery and Adventure

    ERIC Educational Resources Information Center

    Krapp, JoAnn Vergona

    2005-01-01

    Mystery and Adventure travel the same path. Within every mystery is an adventure, be it a struggle for survival, network of suspense, or matching of wits. A mystery is a secret jigsaw puzzle. Its popularity lies in the author's skillful engagement of the reader in putting together the pieces by using such elements as clues, foreshadowing, and…

  18. Martian Mysteries Is there any life on Mars right now?

    E-print Network

    Lawrence, Rick L.

    Martian Mysteries · Is there any life on Mars right now? · Was there ever life on Mars? · Can humans live on Mars? · How would YOU find the answers? #12;Scientists have been trying to answer these questions by sending space probes to Mars. Enjoy these 3-D photos from Mars missions. #12;Mars Pathfinder 3D

  19. Increasing the Relevance: A Who Done It Mystery

    ERIC Educational Resources Information Center

    Peterson, Nancy

    2009-01-01

    In this article, the author describes the approach she used to teach American government to high school seniors. Beginning with a court procedure unit, the central strategy she used for this unit was a murder mystery that peaked the students' curiosity and encouraged them to think like scientists and lawyers. The court procedure lesson uses a…

  20. Passport to Mystery

    ERIC Educational Resources Information Center

    Williams, Wilda

    2010-01-01

    Mystery and suspense fiction remain as popular as ever for as many reasons as there are readers. "Those who wish for escape or respite read cozies, historicals, or romance crossovers," says Poisoned Pen editor Barbara Peters. "Those who want to stay on the cutting edge of society read thrillers [from authors] like Daniel Silva, Alex Berenson, or…

  1. Mystery Box Marvels

    ERIC Educational Resources Information Center

    Santos, Joel; Centurio, Tina

    2012-01-01

    What happens in the first week of school could very well set the stage for the rest of the school year. Setting high standards for science activities based in inquiry can start on the first day of science class and develop as the year unfolds. With the use of simple, readily available, inexpensive materials, an efficient mystery box lesson can be…

  2. Big Mysteries: Extra Dimensions

    SciTech Connect

    Lincoln, Don

    2014-06-10

    The weakness of gravity compared to the other subatomic forces is a real mystery. While nobody knows the answer, one credible solution is that gravity has access to more spatial dimensions than the other three known forces. In this video, Fermilab's Dr. Don Lincoln describes this idea, with the help of some very urbane characters.

  3. A Microbial Murder Mystery.

    ERIC Educational Resources Information Center

    Mitchell, Melissa A.; Mitchell, James K.

    2002-01-01

    Proposes a microbial mystery activity to test students' knowledge of human anatomy and their ability to identify microbes. Provides an opportunity for students to develop logical deductive reasoning. Includes national science education standards related to this activity, activity sheets with whole procedures, and Internet resources. (KHR)

  4. Mystery in Progress.

    ERIC Educational Resources Information Center

    Hall, Kristen

    1989-01-01

    Describes "Mystery in Progress," a traveling exhibit which traces the development of Predynastic Egypt. The exhibit provides a time line for Predynastic Egypt, depicts the history of the Hierakonpolis expedition, documents the formation of Egypt's first centralized nation state, and summarizes the emergence of a unified Egypt. (LS)

  5. Big Mysteries: Extra Dimensions

    ScienceCinema

    Lincoln, Don

    2014-08-07

    The weakness of gravity compared to the other subatomic forces is a real mystery. While nobody knows the answer, one credible solution is that gravity has access to more spatial dimensions than the other three known forces. In this video, Fermilab's Dr. Don Lincoln describes this idea, with the help of some very urbane characters.

  6. Sustainable Scientists

    SciTech Connect

    Mills, Evan

    2008-12-31

    Scientists are front and center in quantifying and solving environmental problems. Yet, as a spate of recent news articles in scientific journals point out, much can be done to enhance sustainability within the scientific enterprise itself, particularly by trimming the energy use associated with research facilities and the equipment therein (i,ii,iii, iv). Sponsors of research unwittingly spend on the order of $10 billion each year on energy in the U.S. alone, and the underlying inefficiencies drain funds from the research enterprise while causing 80 MT CO2-equivalent greenhouse-gas emissions (see Box). These are significant sums considering the opportunity costs in terms of the amount of additional research that could be funded and emissions that could be reduced if the underlying energy was used more efficiently. By following commercially proven best practices in facility design and operation, scientists--and the sponsors of science--can cost-effectively halve these costs, while doing their part to put society on alow-carbon diet.

  7. Earth's mysterious atmosphere. ATLAS 1: Teachers guide with activities

    SciTech Connect

    Not Available

    1991-11-01

    One of our mission's primary goals is to better understand the physics and chemistry of our atmosphere, the thin envelope of air that provides for human life and shields us from the harshness of space. The Space Shuttle Atlantis will carry the ATLAS 1 science instruments 296 km above Earth, so that they can look down into and through the various layers of the atmosphere. Five solar radiometers will precisely measure the amount of energy the Sun injects into Earth's environment. The chemistry at different altitudes will be measured very accurately by five other instruments called spectrometers. Much of our time in the cockpit of Atlantis will be devoted to two very exciting instruments that measure the auroras and the atmosphere's electrical characteristics. Finally, our ultraviolet telescope will probe the secrets of fascinating celestial objects. This Teacher's Guide is designed as a detective story to help you appreciate some of the many questions currently studied by scientists around the world. Many complex factors affect our atmosphere today, possibly even changing the course of global climate. All who live on Earth must recognize that they play an ever-growing role in causing some of these changes. People must solve this great atmospheric mystery if they are to understand all these changes and know what to do about them.

  8. Earth's mysterious atmosphere. ATLAS 1: Teachers guide with activities

    NASA Technical Reports Server (NTRS)

    1991-01-01

    One of our mission's primary goals is to better understand the physics and chemistry of our atmosphere, the thin envelope of air that provides for human life and shields us from the harshness of space. The Space Shuttle Atlantis will carry the ATLAS 1 science instruments 296 km above Earth, so that they can look down into and through the various layers of the atmosphere. Five solar radiometers will precisely measure the amount of energy the Sun injects into Earth's environment. The chemistry at different altitudes will be measured very accurately by five other instruments called spectrometers. Much of our time in the cockpit of Atlantis will be devoted to two very exciting instruments that measure the auroras and the atmosphere's electrical characteristics. Finally, our ultraviolet telescope will probe the secrets of fascinating celestial objects. This Teacher's Guide is designed as a detective story to help you appreciate some of the many questions currently studied by scientists around the world. Many complex factors affect our atmosphere today, possibly even changing the course of global climate. All of us who live on Earth must recognize that we play an ever-growing role in causing some of these changes. We must solve this great atmospheric mystery if we are to understand all these changes and know what to do about them.

  9. New VLA Images Unlocking Galactic Mysteries

    NASA Astrophysics Data System (ADS)

    2008-01-01

    Astronomers have produced a scientific gold mine of detailed, high-quality images of nearby galaxies that is yielding important new insights into many aspects of galaxies, including their complex structures, how they form stars, the motions of gas in the galaxies, the relationship of "normal" matter to unseen "dark matter," and many others. An international team of scientists used more than 500 hours of observations with the National Science Foundation's Very Large Array (VLA) radio telescope to produce detailed sets of images of 34 galaxies at distances from 6 to 50 million light-years from Earth. Their project, called The HI Nearby Galaxy Survey, or THINGS, required two years to produce nearly one TeraByte of data. HI ("H-one") is an astronomical term for atomic hydrogen gas. The astronomers presented their initial findings to the American Astronomical Society's (AAS) meeting in Austin, Texas. "Studying the radio waves emitted by atomic hydrogen gas in galaxies is an extremely powerful way to learn what's going on in nearby galaxies. The THINGS survey uses that tool to provide sets of images of the highest quality and sensitivity for a substantial sample of galaxies of different types," said Fabian Walter, of the Max-Planck Institute for Astronomy in Heidelberg, Germany. IC2574M74 Dwarf galaxy IC2574, left, and spiral galaxy M74, in THINGS images. Credit: Walter et al., NRAO/AUI/NSF Click images for high-resolution files (33 KB & 25 KB) Spiral Galaxies in THINGS Most of the galaxies studied in the THINGS survey also have been observed at other wavelengths, including Spitzer space telescope infrared images and GALEX ultraviolet images. This combination provides an unprecedented resource for unravelling the mystery of how a galaxy's gaseous material influences its overall evolution. Analysis of THINGS data already has yielded numerous scientific payoffs. For example, one study has shed new light on astronomers' understanding of the gas-density threshold required to start the process of star formation. "Using the data from THINGS in combination with observations from NASA's space telescopes has allowed us to investigate how the processes leading to star formation differ in big spiral galaxies like our own and much smaller, dwarf galaxies," said Adam Leroy and Frank Bigiel of the Max-Planck Insitute for Astronomy at the Austin AAS meeting. Because atomic hydrogen emits radio waves at a specific frequency, astronomers can measure motions of the gas by noting the Doppler shift in frequency caused by those motions. "Because the THINGS images are highly detailed, we have been able to measure both the rotational motion of the galaxies and non-circular random motions within the galaxies," noted Erwin de Blok of the University of Cape Town, South Africa. Galaxy Dynamics in THINGS The motion measurements are providing new information about the mysterious, unseen "dark matter" in the galaxies. "The non-circular motions revealed by the THINGS observations, turn out to be too small to solve a long-standing problem in cosmology, namely the inability of state-of-the-art computer simulations to describe the distribution of dark matter in disk galaxies. It was thought that random motions could explain that inability, but our data show otherwise," de Blok explained. The THINGS images revealed what Elias Brinks of the University of Hertfordshire, UK, called a "stunning complexity of structures in the tenuous interstellar medium of the galaxies." These structures include large shells and "bubbles," presumably caused by multiple supernova explosions of massive stars. Analyzing the detail of these complex structures will help astronomers better understand the differences in star formation processes in the varied types of galaxies. Even such a simple question such as how big are the disks of gas in spiral galaxies had largely eluded astronomers previously. "The quality and sensitivity of the THINGS images has allowed us to see the actua

  10. The Fish Kill Mystery: Using Case Studies in the Middle School Classroom

    ERIC Educational Resources Information Center

    Heid, Christy; Biglan, Barbara; Ritson, Margaret

    2008-01-01

    Case studies are an excellent method for engaging middle school students in the current work of scientists. Students learn to think like scientists as they decide how to investigate the dilemma presented in the case study. This article describes one such case study, the Fish Kill Mystery, which takes place at a popular vacation spot--the beaches…

  11. History Mystery: A Documents-Based Lesson on Women's Rights.

    ERIC Educational Resources Information Center

    Libresco, Andrea S.

    2000-01-01

    Presents a lesson used with fourth and fifth graders focusing on women's rights in the 1880s in which students solve a mystery through historical research. States the lesson prepares elementary students to investigate historical questions by examining primary sources. (CMK)

  12. Medical Scientists

    MedlinePLUS

    ... by investigating safe dosage limits. <- Summary Work Environment -> Work Environment About this section Medical scientists usually work ... they take precautions that ensure a safe environment. Work Schedules Most medical scientists work full time. <- What ...

  13. Challenge to the Mystery of the Charged Lepton Mass Formula

    E-print Network

    Yoshio Koide

    2005-06-24

    Why the charged lepton mass formula m_e +m_\\mu +m_\\tau = {2/3} (\\sqrt{m_e}+\\sqrt{m_\\mu} +\\sqrt{m_\\tau})^2 is mysterious is reviewed, and guiding principles to solve the mystery are presented. According to the principles, an example of such a mass generation mechanism is proposed, where the origin of the mass spectrum is attributed not to the structure of the Yukawa coupling constants, but to a structure of vacuum expectation values of flavor-triplet scalars under Z_4 \\times S_3 symmetries.

  14. The mystery of reincarnation

    PubMed Central

    Nagaraj, Anil Kumar Mysore; Nanjegowda, Raveesh Bevinahalli; Purushothama, S. M.

    2013-01-01

    One of the mysteries puzzling human mind since the origin of mankind is the concept of “reincarnation” which literally means “to take on the flesh again.” As the civilizations evolved, beliefs got discriminated and disseminated into various religions. The major division manifested was “East” and “West.” The eastern religions being more philosophical and less analytical, have accepted reincarnation. However, the different eastern religions like Hinduism, Jainism, and Buddhism have differed in their faith on rebirth. Further, the Islam as well as the most dominant religion of the world, Christianity, having its origin in the west, have largely denied reincarnation, though some sub-sects still show interest in it. Also many mystic and esoteric schools like theosophical society have their unique description on rebirth. This article describes reincarnation as perceived by various religions and new religious movements as well as some research evidence. PMID:23858250

  15. The mystery of reincarnation.

    PubMed

    Nagaraj, Anil Kumar Mysore; Nanjegowda, Raveesh Bevinahalli; Purushothama, S M

    2013-01-01

    One of the mysteries puzzling human mind since the origin of mankind is the concept of "reincarnation" which literally means "to take on the flesh again." As the civilizations evolved, beliefs got discriminated and disseminated into various religions. The major division manifested was "East" and "West." The eastern religions being more philosophical and less analytical, have accepted reincarnation. However, the different eastern religions like Hinduism, Jainism, and Buddhism have differed in their faith on rebirth. Further, the Islam as well as the most dominant religion of the world, Christianity, having its origin in the west, have largely denied reincarnation, though some sub-sects still show interest in it. Also many mystic and esoteric schools like theosophical society have their unique description on rebirth. This article describes reincarnation as perceived by various religions and new religious movements as well as some research evidence. PMID:23858250

  16. Oriental mystery: ginseng

    SciTech Connect

    Yun, T.K.; Cho, H.O.; Yun, Y.S.

    1985-01-01

    As a mysterious cure-all medicine Korea ginseng has been, since four or five thousand years ago, used as a tonic in the orient. Ginseng has been known to have a tonic effect and it is the general opinion of many investigators that ginseng has the effect of normalization of physical conditions, that is; maintaining individual homeostasis. On the other hand, the authors have found that ginseng extract inhibits the incidence and also the proliferation of tumors induced by carcinogens such as urethane, DMBA and aflatoxin B. The anticarcinogenic effect of ginseng was due to its ability to enhance the natural killer activity of the host. Korea ginseng is highly effective in preventing or curing various disease such as diabetes, cancer, high blood pressure, etc.

  17. A long-standing mystery solved: the formation of 3-hydroxydesloratadine is catalyzed by CYP2C8 but prior glucuronidation of desloratadine by UDP-glucuronosyltransferase 2B10 is an obligatory requirement.

    PubMed

    Kazmi, Faraz; Barbara, Joanna E; Yerino, Phyllis; Parkinson, Andrew

    2015-04-01

    Desloratadine (Clarinex), the major active metabolite of loratadine (Claritin), is a nonsedating long-lasting antihistamine that is widely used for the treatment of allergic rhinitis and chronic idiopathic urticaria. For over 20 years, it has remained a mystery as to which enzymes are responsible for the formation of 3-hydroxydesloratadine, the major active human metabolite, largely due to the inability of any in vitro system tested thus far to generate this metabolite. In this study, we demonstrated that cryopreserved human hepatocytes (CHHs) form 3-hydroxydesloratadine and its corresponding O-glucuronide. CHHs catalyzed the formation of 3-hydroxydesloratadine with a Km of 1.6 ?M and a Vmax of 1.3 pmol/min per million cells. Chemical inhibition of cytochrome P450 (P450) enzymes in CHHs demonstrated that gemfibrozil glucuronide (CYP2C8 inhibitor) and 1-aminobenzotriazole (general P450 inhibitor) inhibited 3-hydroxydesloratadine formation by 91% and 98%, respectively. Other inhibitors of CYP2C8 (gemfibrozil, montelukast, clopidogrel glucuronide, repaglinide, and cerivastatin) also caused extensive inhibition of 3-hydroxydesloratadine formation (73%-100%). Assessment of desloratadine, amodiaquine, and paclitaxel metabolism by a panel of individual CHHs demonstrated that CYP2C8 marker activity robustly correlated with 3-hydroxydesloratadine formation (r(2) of 0.70-0.90). Detailed mechanistic studies with sonicated or saponin-treated CHHs, human liver microsomes, and S9 fractions showed that both NADPH and UDP-glucuronic acid are required for 3-hydroxydesloratadine formation, and studies with recombinant UDP-glucuronosyltransferase (UGT) and P450 enzymes implicated the specific involvement of UGT2B10 in addition to CYP2C8. Overall, our results demonstrate for the first time that desloratadine glucuronidation by UGT2B10 followed by CYP2C8 oxidation and a deconjugation event are responsible for the formation of 3-hydroxydesloratadine. PMID:25595597

  18. Working Like Real Scientists

    ERIC Educational Resources Information Center

    Lunn, Stephen

    2006-01-01

    "Real" science is about formulating and trying to solve practical and conceptual problems on the basis of shared beliefs about the world. Scientists build theories and test hypotheses by observation and experiment. They try their best to eliminate personal bias, and are "extremely canny in their acceptance of the claims of others" (Ziman, 2000).…

  19. The Mystery Soil

    NASA Technical Reports Server (NTRS)

    2004-01-01

    [figure removed for brevity, see original site] Click for larger view

    This high-resolution image from the panoramic camera on the Mars Exploration Rover Spirit shows the region containing the patch of soil scientists examined at Gusev Crater just after Spirit rolled off the Columbia Memorial Station. Scientists examined this patch on the 13th and 15th martian days, or sols, of Spirit's journey. Using nearly all the science instruments located on the rover's instrument deployment device or 'arm,' scientists yielded some puzzling results including the detection of a mineral called olivine and the appearance that the soil is stronger and more cohesive than they expected. Like detectives searching for clues, the science team will continue to peruse the landscape for explanations of their findings.

    Data taken from the camera's red, green and blue filters were combined to create this approximate true color picture, acquired on the 12th martian day, or sol, of Spirit's journey.

    The yellow box (see inset above) in this high-resolution image from the panoramic camera on the Mars Exploration Rover Spirit outlines the patch of soil scientists examined at Gusev Crater just after Spirit rolled off the Columbia Memorial Station.

  20. TheTheTheThe MysteryMysteryMysteryMystery ofofofof the Black Lakethe Black Lakethe Black Lakethe Black Lake

    E-print Network

    Alfonseca, Manuel

    of the Black LakeThe Mystery of the Black Lake Book 2 in the Chronicles of the Magic Jigsaw Puzzle Manuel ........................................... 19 5. The kingdom of shadows .................................... 24 6. The gloomy forest

  1. Exquisite Corpses : an architectural mystery

    E-print Network

    Canizares, Galo

    2014-01-01

    In 1937, writing about the parallels between mystery fiction and urban dwelling, Walter Benjamin wrote, ""in times of terror, when everyone is something of a conspirator, everybody will be in the position of having to play ...

  2. Roman mystery iron blades from Serbia

    SciTech Connect

    Balos, Sebastian; Benscoter, Arlan; Pense, Alan

    2009-04-15

    A First to Forth Century Roman spear blade from Serbia was found to have an unusual microstructure inconsistent with typical Roman Period iron. An analysis of the blade undertaken at Lehigh University in the US and at the Faculty of Technical Sciences in Novi Sad, Serbia established that it was metallic in appearance, magnetic and had an external layer of red rust. But as metallographically polished, it appeared to contain multiple internal phases and internal cracking. Even after aggressive etching, no typical low carbon microstructure was developed. Scanning electron microscopy, classical and energy dispersive X-ray analysis indicated that the specimen was essentially iron, although its microhardness was too high for typical Roman iron. It was then dubbed 'Mystery Iron.' Analysis of all the data led to the proposal that it was essentially a Roman iron 'fossil' in which the iron had been converted to high temperature iron oxide while retaining the form of the blade, conversion probably occurring in a fire. Subsequent X-ray diffraction analysis confirmed that the blade consisted of FeO and Fe{sub 3}O{sub 4} and the mystery of the iron fossil was at least partially solved. A hypothesis is proposed regarding a potential cause for the fire.

  3. Dr. Earl N. Meyer, in the lab, with a scalpel: a murder mystery as a biochemistry recruitment tool.

    PubMed

    Vulcu, Felicia; Heirwegh, Meagan

    2015-01-01

    Increasing student participation in science is an ongoing challenge for many universities. In this active learning workshop, centered on inquiry and teamwork, we introduce high-school students to biochemistry and molecular biology techniques using a murder mystery activity. During this intensive 3 hr workshop, we engage students in a murder scenario entitled "The Case of the Silenced Scientist." A commercially available DNA fingerprinting kit was used as a basis to create a customized scenario whereby students collaborate with one another to solve a murder mystery. Through analysis of DNA samples taken from the crime scene and suspects, students can identify the murderer while developing technical, teamwork, and critical thinking skills. Emphasis is placed on teamwork by immersing students in the collaborative process of research inquiry. Though short in duration, this workshop aims to build student relationships to science through creativity and exploration. In this article, we describe the key customized applications of this workshop as a blueprint for science recruitment. We focus on the workshop facilitators' perceived learning impact on students. PMID:25395001

  4. Big Mysteries: Dark Energy

    SciTech Connect

    Lincoln, Don

    2014-04-15

    Scientists were shocked in 1998 when the expansion of the universe wasn't slowing down as expected by our best understanding of gravity at the time; the expansion was speeding up! That observation is just mind blowing, and yet it is true. In order to explain the data, physicists had to resurrect an abandoned idea of Einstein's now called dark energy. In this video, Fermilab's Dr. Don Lincoln tells us a little about the observations that led to the hypothesis of dark energy and what is the status of current research on the subject.

  5. Big Mysteries: Dark Energy

    ScienceCinema

    Lincoln, Don

    2014-08-07

    Scientists were shocked in 1998 when the expansion of the universe wasn't slowing down as expected by our best understanding of gravity at the time; the expansion was speeding up! That observation is just mind blowing, and yet it is true. In order to explain the data, physicists had to resurrect an abandoned idea of Einstein's now called dark energy. In this video, Fermilab's Dr. Don Lincoln tells us a little about the observations that led to the hypothesis of dark energy and what is the status of current research on the subject.

  6. Questioning Many Mysteries

    NASA Astrophysics Data System (ADS)

    Martin, Sara F.

    2015-04-01

    The first section of this memoir queries my formative years. Indirectly I address the question, did my childhood and early years make a difference in my choice of career? Why and how did I begin my journey to becoming a scientist? Did I choose the field of solar astronomy or did circumstances dictate it for me? In the second section, I travel through my work environments and experiences, talking about interactions and aspects of being a scientist that do not appear in our research papers. What parts of my research were happenstances and what parts did I plan? What does it feel like to be on scientific quests? Using examples in my journey, I also turn to questions that have intrigued me throughout my sojourn as a solar astronomer. How do scientific discoveries come about? What factors lead to little discoveries? And what factors lead to major exciting discoveries? Are there timely questions we do not think to ask? How can small, seemingly scattered pieces of knowledge suddenly coalesce into a deeper understanding - what is called the "Aha!" experience - the times when our mental light switches on, and with child-like wonder we behold a "big picture"?

  7. The 'Razorback' Mystery

    NASA Technical Reports Server (NTRS)

    2004-01-01

    The pointy features in this image may only be a few centimeters high and less than 1 centimeter (0.4 inches) wide, but they generate major scientific interest. Dubbed 'Razorback,' this chunk of rock sticks up at the edge of flat rocks in 'Endurance Crater.' Based on their understanding of processes on Earth, scientists believe these features may have formed when fluids migrated through fractures, depositing minerals. Fracture-filling minerals would have formed veins composed of a harder material that eroded more slowly than the rock slabs.

    Possible examination of these features using the instruments on NASA's Mars Exploration Rover Opportunity may further explain what these features have to do with the history of water on Mars. This false-color image was taken by the rover's panoramic camera.

  8. Swedish Scientists have Solved Honey's Enigma

    Technology Transfer Automated Retrieval System (TEKTRAN)

    Recently, it was discovered by Olofsson and Vasquez (2008) that a novel flora composed of lactic acid bacteria (LAB) of the genera Lactobacillus and Bifidobacterium, exists in the honey stomach of the honey bee Apis mellifera. The twelve different flora members varied numerically with the sources o...

  9. The Fellowship of the Mystery

    ERIC Educational Resources Information Center

    Hotchkiss, Wesley

    1976-01-01

    Author states that religion involves cosmic vision as well as ethical philosophy, and that religious ethics become impotent without this vision. Mystery, defined as the sense of wonder at the revelation of the nature of the cosmos, can be expressed only through art. (RW)

  10. Theorem of Mystery: Part 1

    ERIC Educational Resources Information Center

    Lopez-Real, Francis

    2008-01-01

    While the author was searching the web, he came across an article by Michael Keyton of IMSA (Illinois Mathematics and Science Academy) called "Theorems of mystery". The phrase is Keyton's own, and he defines such a theorem as "a result that has considerable structure with minimal hypotheses." The simplest of his 10 examples is one that many…

  11. How To Write a Mystery.

    ERIC Educational Resources Information Center

    Beinhart, Larry

    Drawing on examples from the best and most popular works in mystery writing--from Raymond Chandler and Mickey Spillane to Scott Turow and Thomas Harris--this book introduces the fledgling writer to his or her most indispensable "partners in crime": character, plot, and procedure; the secrets to creating heroes and villains; the art of scripting…

  12. Creative Ventures: Mysteries and UFO's.

    ERIC Educational Resources Information Center

    Stark, Rebecca

    This book published in 1987 provides open-ended activities to extend the imagination and creativity of students and encourage them to examine their feelings and values. Williams' model of cognitive-intellective and affective-feeling domains are addressed. Nearly 60 pages of exercises focus on the historical, the scientific, the mysterious, the…

  13. BIBLIOTHECAALEXANDRINA TIME'S MYSTERIES AND MIRACLES

    E-print Network

    Zewail, Ahmed

    -in-Publication Data Zewail, Ahmed H. Time's mysteries and miracles : consonance with physical and life sciences I Sciences Lecture delivered byAhmed Zewail during BioVision Alexandria, Nobel Laureates Day lecture delivered by Ahmed Zewail during BioVision Alexandria, Nobel Laureates Day, Bibliotheca

  14. Geological mysteries on Ganymede

    NASA Technical Reports Server (NTRS)

    1997-01-01

    This image shows some unusual features on the surface of Jupiter's moon, Ganymede. NASA's Galileo spacecraft imaged this region as it passed Ganymede during its second orbit through the Jovian system. The region is located at 31 degrees latitude, 186 degrees longitude in the north of Marius Regio, a region of ancient dark terrain, and is near the border of a large swathe of younger, heavily tectonised bright terrain known as Nippur Sulcus. Situated in the transitional region between these two terrain types, the area shown here contains many complex tectonic structures, and small fractures can be seen crisscrossing the image. North is to the top-left of the picture, and the sun illuminates the surface from the southeast. This image is centered on an unusual semicircular structure about 33 kilometers (20 miles) across. A 38 kilometer (24 miles) long, remarkably linear feature cuts across its northern extent, and a wide east-west fault system marks its southern boundary. The origin of these features is the subject of much debate among scientists analyzing the data. Was the arcuate structure part of a larger feature? Is the straight lineament the result of internal or external processes? Scientists continue to study this data in order to understand the surface processes occurring on this complex satellite.

    The image covers an area approximately 80 kilometers (50 miles) by 52 kilometers (32 miles) across. The resolution is 189 meters (630 feet) per picture element. The images were taken on September 6, 1996 at a range of 9,971 kilometers (6,232 miles) by the solid state imaging (CCD) system on NASA's Galileo spacecraft.

    The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC. JPL is an operating division of California Institute of Technology (Caltech).

    This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov.

  15. The Scientist

    E-print Network

    Sun, Wei

    /crzucidlo/My%20Documents... 1 of 7 5/9/2005 2:29 PM Photo: Aileen Constans 3D PRINTING: This precision extruding-so-distant future, scientists would be able to print whole replacement organs, and eventually whole bodies, using the parts themselves. Unlike most 3-D manufacturing technologies, which remove material from a solid block

  16. Citizen Scientists

    ERIC Educational Resources Information Center

    Bennett, Katherine

    2010-01-01

    The Harvard Forest Schoolyard Ecology Program provides teachers and students with the opportunity and materials to participate in regionally focused ecological studies under the guidance of a mentor scientist working on a similar study. The Harvard Forest is part of a national network of ecological research sites known as the Long Term Ecological…

  17. Ranking scientists

    NASA Astrophysics Data System (ADS)

    Dorogovtsev, S. N.; Mendes, J. F. F.

    2015-11-01

    Currently the ranking of scientists is based on the $h$-index, which is widely perceived as an imprecise and simplistic though still useful metric. We find that the $h$-index actually favours modestly performing researchers and propose a simple criterion for proper ranking.

  18. Playing Scientist

    ERIC Educational Resources Information Center

    Campbell, Ashley

    2012-01-01

    Engaging students in the study of genetics is essential to building a deep understanding of heredity, a core idea in the life sciences (NRC 2012). By integrating into the curriculum the stories of famous scientists who studied genetics (e.g., Mendel, Franklin, Watson, and Crick), teachers remind their students that science is a human endeavor.…

  19. USGS Scientist

    USGS Multimedia Gallery

    Janice Albers presents study results at the 6th International Symposium on Sturgeon in Wuhan, China in 2009. USGS scientists and their collaborators in the Comprehensive Sturgeon Research Project provided six presentations at the symposium on topics ranging from reproductive readiness, migration, sp...

  20. Mystery big cats’ in the Peruvian Amazon: morphometrics solve a cryptozoological mystery

    PubMed Central

    Sakamoto, Manabu; Hocking, Peter; Sanchez, Gustavo

    2014-01-01

    Two big cat skulls procured from hunters of Yanachaga National Park, Peru, were reported as those of cats informally dubbed the ‘striped tiger’ and ‘anomalous jaguar’. Observations suggested that both skulls were distinct from those of jaguars, associated descriptions of integument did not conform to this species, and it has been implied that both represent members of one or two novel species. We sought to resolve the identity of the skulls using morphometrics. DNA could not be retrieved since both had been boiled as part of the defleshing process. We took 36 cranial and 13 mandibular measurements and added them to a database incorporating nearly 300 specimens of over 30 felid species. Linear discriminant analysis resolved both specimens as part of Panthera onca with high probabilities for cranial and mandibular datasets. Furthermore, the specimens exhibit characters typical of jaguars. If the descriptions of their patterning and pigmentation are accurate, we assume that both individuals were aberrant. PMID:24688867

  1. Mystery of a cryptogenic stroke solved by an abdominal angiogram.

    PubMed

    Sundar, Kaushik; Venkatasubramanian, Shankar; Umaiorubahan, Meenakshisundaram; Cannigaiper, Velmurugendran

    2015-01-01

    Despite advances in the field of imaging and diagnostics, the incidence of cryptogenic stroke is still around 30-40% in modern stroke databases. Our patient presented with recurrent midbrain infarcts over 3?years and was initially labelled as a patient with cryptogenic stroke. His blood investigations were normal, work up for autoimmune disorders was negative, CT brain angiogram was normal and a two-dimensional echo showed a small patent foramen ovale with a left to right shunt. He later presented with a right perinephric haematoma and an abdominal angiogram revealed multiple microaneurysms of the renal arteries, coeliac trunk and the mesenteric arterial system. The feeding renal artery was embolised. A diagnosis of polyarteritis nodosa was made. The patient was subjected to digital subtraction angiography of neck and intracranial vessels, which revealed multiple microaneurysms in internal and external carotid artery territory. He was discharged with steroids and azathioprine. PMID:26677149

  2. The enigmatic star EZ Pegasi - A mystery solved?

    NASA Technical Reports Server (NTRS)

    Howell, S. B.; Bopp, B. W.

    1985-01-01

    EZ Peg, a ninth-magnitude G star that has been classified by various authors as an irregular variable, a U Gem system, and a contact binary, is shown to have all the spectroscopic and photometric characteristics of an active-chromosphere RS CVn binary. It is suggested that the reported outburst of 1943, when the spectrum appeared to be that of a B star, never occurred. The strong Ca II H and K reversals, viewed with low spectral resolution, caused the photospheric Ca II absorption to appear abnormally weak, mimicking a much earlier spectral type.

  3. Comment on "Solving the mystery of booming sand dunes"

    E-print Network

    B. Andreotti; L. Bonneau; E. Clement

    2007-10-30

    We show here that the standard physical model used by Vriend et al. to analyse seismograph data, namely a non-dispersive bulk propagation, does not apply to the surface layer of sand dunes. According to several experimental, theoretical and field results, the only possible propagation of sound waves in a dry sand bed under gravity is through an infinite, yet discrete, number of dispersive surface modes. Besides, we present a series of evidences, most of which have already been published in the literature, that the frequency of booming avalanches is not controlled by any resonance as argued in this article. In particular, plotting the data provided by Vriend et al. as a table, it turns out that they do not present any correlation between the booming frequency and their estimate of the resonant frequency.

  4. Solving the Mystery of Fading Fingerprints with London Dispersion Forces.

    ERIC Educational Resources Information Center

    Kimbrough, Doris R.; DeLorenzo, Ronald

    1998-01-01

    Focuses on the kidnapping of a child whose fingerprints were not found inside the crime vehicle. Discusses the investigation that followed and led to knowledge of the differences between the fingerprints of children and adults. (DDR)

  5. Latitude: How American Astronomers Solved the Mystery of Variation

    NASA Astrophysics Data System (ADS)

    Ray, Richard D.

    First longitude, now latitude. From Latitude's title we cannot help thinking of Dava Sobel's recent bestseller, Longitude. I suppose it's unlikely to be such a moneymaker, but this delightful new book by Bill and Merri Sue Carter, a father and daughter team, is similar to Sobel's book. Both are physically small, with short chapters, which makes for a quick read. And both have a clear hero: John Harrison and his chronometers for longitude; and Seth Carlo Chandler Jr. and his almucantar for latitude. Both books eschew academic-style footnoting, although Latitude does list a few useful sources for each chapter and provides a comprehensive list of Chandler's astronomical publications. Chandler's name is known to most AGU members for its association with the 14-month wobble of the Earth's pole. He also discovered the slightly smaller annual wobble, and an argument can be made that he was the principal discoverer of polar motion, or latitude variation, in general.

  6. Mysterious Black Water off Florida's Gulf Coast

    NASA Technical Reports Server (NTRS)

    2002-01-01

    In mid-December last year, a mysterious black water overtook the normally bluish green waters of Florida Bay. Over the course of the winter, the extent of the water grew to encompass an area as big as Lake Okeechobee, Florida, before subsiding over the last few weeks. These images taken by the Sea-viewing Wide Field-of-View Sensor (SeaWiFS), flying aboard the Orbview-2 satellite, show the progression of the black water over the last three months. The affected water sits along the southeastern coast of Florida about fifty miles north of the Florida Keys. As of now, scientists do not know why the water appears black in satellite and aerial images or whether the water is harming the wildlife. They speculate that it could be due to an exotic algae bloom, an underwater fountain pushing up sediments from the ocean floor, or possibly chemical and sediment run-off from the nearby Shark River. Researchers at the Florida Marine Research Institute in St. Petersburg and the Mote Marine Research Institute in Sarasota are running tests to determine the chemical make-up of the water. No big fish kills have been reported in the area. But fishermen say the catch has been low this winter. In addition, the black water sits just north of the Florida Keys National Marine Sanctuary, which is home to one of the largest coral reef habitats in the United States. Toxic run-off from the Florida coastline and motor boats in the area have already destroyed many of Florida's reefs. Scientists are concerned that if the extent of the black water grows again, it could endanger these reefs. Information provided by the Naples Daily News. For up-to-date images of the area, view these SeaWiFS Images of Florida Bay. Image courtesy the SeaWiFS Project, NASA/Goddard Space Flight Center, and ORBIMAGE

  7. Halley's Legacy: The Selfless Genius Who Founded Geophysics, Led the Science Community to Solve the Problem of Finding Longitude at Sea, and Whose Work in Areas from Geomagnetism to Planetology Still Has Meaning For Today's Scientists

    NASA Astrophysics Data System (ADS)

    Wakefield, J.

    2005-12-01

    2005 marks the 300th anniversary of Edmond Halley's publication of his infamous synopsis predicting the accurate return of the comet that would come to bear his name. On this occasion, it is time to remember him not only as the founder of geophysics but for his contributions to the world of science beyond his comet work. Halley's comet-transformed by the first triumph of the Newtonian revolution from a dire supernatural omen to a predictable element of the universe's clockwork-remains a recurring symbol of the scientific age of the Enlightenment. His comet is hurtling through space at some 20,000 miles per hour and won't be back until 2061. But it can remind us of past epochs and everlastingly of Halley's contributions to geophysics and the world of science writ large. For a start, Halley completed a series of little known sea voyages in his effort to solve one of his life-long quests: the problem of determining longitude at sea. On the basis of his earlier theories on magnetism, his approach entailed mapping the magnetic deviation across the test-bed of the Atlantic Ocean. In this paper, his findings from the voyages, which technically comprised the first science mission funded by a government and stand as the forerunner of all big science projects, will be reconsidered and put into the context of today's notions about terrestrial magnetism, including the geodynamo. To this day, scientists remain perplexed about exactly how core's dynamo regenerates its energy. When Halley was sailing his vessel, the Paramore, across the North Atlantic and making the first charts of geomagnetism, little did he ever imagine magnetism would underpin today's stunning advances in information technology and electromagnetic engineering. Magnetism also offers ways to study phase transitions, random disorder, and physics in low dimensions, which looks at particle interactions at ever higher energies in order to essentially study matter at smaller and smaller size scales. The presentation will also give an overview of his legacy to geophysics, which includes his contributions to meteorology, hydrology, ocean sciences, among other disciplines.

  8. How mathematics helps unraveling the mystery behind somitogenesis

    E-print Network

    Feng, Peng

    How mathematics helps unraveling the mystery behind somitogenesis Peng Feng DEPARTMENT Mathematical Model How mathematics helps unraveling the mystery behind somitogenesis Peng Feng 2 / 37 #12 Delay Hopf Bifurcation With Discrete Delay How mathematics helps unraveling the mystery behind

  9. Is Teleportation a (quantum) mystery?

    E-print Network

    Berry Groisman

    2008-06-10

    Since its discovery quantum teleportation has often been seen as a manifestation, indeed the epitome, of the very paradoxical and mysterious nature of quantum theory itself. It is commonly regarded as genuinely quantum and essentially paradoxical. Although a common approach to teleportation amongst physicists nowadays is a somewhat operational one, some researchers are making an effort to deflate the above views. On the one hand, it was recently argued that the paradox of information transfer taking place in teleportation is dissolved (Timpson, 2006) by appealing the very notion of information. On the other hand, it was demonstrated that some classical versions of teleportation retain its important features, which hitherto were considered genuinely quantum (Cohen, 2003; Collins&Popescu, 2002; Hardy, 1999; Mor, 2006; Spekkens, 2007). I will present a special version of a quantum teleportation protocol which is in a sense split into classical and quantum steps. This description provides us with a unified picture of teleportation in both domains. It will be explicitly shown how classical teleportation is embedded in the quantum protocol. Moreover, the classical step can be successfully accomplished even if the state shared by the parties is completely disentangled [this is consistent with the result obtained in (Wang, 2005)]. Yet, all the (apparent) paradoxical features usually associated with quantum teleportation are clearly present in this step. In particular, this demonstrates that entanglement cannot be ultimately responsible and not necessary for the (paradoxical?) information transfer. Thus, even if one considers teleportation as mysterious, all its mysteries are shifted from quantum domain into purely classical one.

  10. End of Several Quantum Mysteries

    E-print Network

    C. S. Unnikrishnan

    2011-02-06

    I report on the discovery of quantum compatible local variables that are shared between subsystems of quantum-conventionally entangled physical systems such that they determine the correlations of spatially separated systems while preserving strict Einstein locality. This puts an end to the mystery of spooky action at a distance and alleged collapse at a distance, answering vital questions, first raised in the EPR paper, on the behaviour of spatially separated entangled systems. The solution helps to understand quantitative measures of entanglement in a transparent way. It also provides new insight, consistent with strict locality, of the physics of quantum teleportation and related phenomena.

  11. The Mysteries of Real Materials

    NASA Technical Reports Server (NTRS)

    Laub, Bernard

    2012-01-01

    The presentation will consist of showing arc jet data mysterious to the modelers. It will show pictures from an arc jet test where a material (unidentified) exhibited a failure mode that nobody understands followed by thermocouple data from arc jet tests on another (unidentified) material of interest in which the T/Cs exhibit repeatable, consistent, fascinating yet frustrating response characteristics that have the modelers stumped. This all happens between RT and 200 F. Unless we figure out what the responsible phenomenology is and can model it, we can't size the TPS with any confidence.

  12. Teaching U.S. History as Mystery.

    ERIC Educational Resources Information Center

    Gerwin, David; Zevin, Jack

    One way to engage students in grades 7 through 12 is to encourage them to investigate history as a puzzle, a set of dilemmas, a collection of conflicting viewpoints in short, a mysterious and provocative subject. In this book a collection of cases have been assembled both real mysteries and purposely constructed classroom problems with techniques…

  13. Evaluative Appraisals of Environmental Mystery and Surprise

    ERIC Educational Resources Information Center

    Nasar, Jack L.; Cubukcu, Ebru

    2011-01-01

    This study used a desktop virtual environment (VE) of 15 large-scale residential streets to test the effects of environmental mystery and surprise on response. In theory, mystery and surprise should increase interest and visual appeal. For each VE, participants walked through an approach street and turned right onto a post-turn street. We designed…

  14. Problem Solving with Patents

    ERIC Educational Resources Information Center

    Moore, Jerilou; Sumrall, William J.

    2008-01-01

    Exploring our patent system is a great way to engage students in creative problem solving. As a result, the authors designed a teaching unit that uses the study of patents to explore one avenue in which scientists and engineers do science. Specifically, through the development of an idea, students learn how science and technology are connected.…

  15. Adult Age Differences in Reading and Rereading Processes Associated with Problem Solving

    ERIC Educational Resources Information Center

    Soederberg Miller, Lisa M.; Gagne, Danielle D.

    2008-01-01

    We investigated age differences in reading and rereading processes associated with problem solving and explored the extent to which prior information affects rereading processes. Participants' reading times were recorded as they read short mysteries, twice, at their own pace on a computer, with the goal of providing the solution to the mystery. We…

  16. Quantum Mysteries Disentangled 28 November 2001

    E-print Network

    Gat, Erann

    , the mysteries endure, and the philosophical arguments over such things as whether cats qualify as conscious. Unfortunately, it turns out that the story of QM has a fatal flaw. Not QM itself, mind you, but the story

  17. Medical Mystery: Losing the sense of smell

    MedlinePLUS

    ... Hearing Disorders Medical Mystery: Losing the sense of smell Past Issues / Fall 2008 Table of Contents For ... a teenager that took away her sense of smell. Photo courtesy of Malone University Imagine, if you ...

  18. 6/26/12 Scientists rethink old ideas about the moon -The Boston Globe 1/2www.boston.com/news/science/articles/2012/06/24/scientists_rethink_old_ideas_about_the_moon/?...

    E-print Network

    Weiss, Benjamin P.

    6/26/12 Scientists rethink old ideas about the moon - The Boston Globe 1/2www.boston.com/news/science/articles/2012/06/24/scientists_rethink_old_ideas_about_the_moon/?... A giant leap in interest in the moon By Carolyn Y. Johnson Globe Staff June 24, 2012 As scientific mysteries go, the moon has long seemed a closed

  19. Is part of the mystery surrounding fatigue complicated by context?

    PubMed

    Abbiss, Chris R; Laursen, Paul B

    2007-10-01

    Historically, research into possible causes of exercise-induced fatigue has been found to span numerous scientific disciplines, including medicine, psychology, physiology, neurophysiology, biochemistry, biomechanics, and physics. In order to better understand the mechanisms responsible for fatigue, these disciplines have viewed various aspects of fatigue, including the involvement of physiological, physical, biomechanical, and/or psychological factors. This has resulted in a diverse array of interpretations of the term 'fatigue' among the scientific disciplines. For instance, the word 'fatigue' has been used to define a sensation of tiredness, a physical reduction in force, or the failure of a specific physiological system to maintain homeostatic integrity. As sports scientists begin to take on a holistic approach to understanding fatigue, it seems necessary that the 'context' should be highlighted when using the term and questioning the mystery behind it. PMID:17182280

  20. The mystery of language evolution

    PubMed Central

    Hauser, Marc D.; Yang, Charles; Berwick, Robert C.; Tattersall, Ian; Ryan, Michael J.; Watumull, Jeffrey; Chomsky, Noam; Lewontin, Richard C.

    2014-01-01

    Understanding the evolution of language requires evidence regarding origins and processes that led to change. In the last 40 years, there has been an explosion of research on this problem as well as a sense that considerable progress has been made. We argue instead that the richness of ideas is accompanied by a poverty of evidence, with essentially no explanation of how and why our linguistic computations and representations evolved. We show that, to date, (1) studies of nonhuman animals provide virtually no relevant parallels to human linguistic communication, and none to the underlying biological capacity; (2) the fossil and archaeological evidence does not inform our understanding of the computations and representations of our earliest ancestors, leaving details of origins and selective pressure unresolved; (3) our understanding of the genetics of language is so impoverished that there is little hope of connecting genes to linguistic processes any time soon; (4) all modeling attempts have made unfounded assumptions, and have provided no empirical tests, thus leaving any insights into language's origins unverifiable. Based on the current state of evidence, we submit that the most fundamental questions about the origins and evolution of our linguistic capacity remain as mysterious as ever, with considerable uncertainty about the discovery of either relevant or conclusive evidence that can adjudicate among the many open hypotheses. We conclude by presenting some suggestions about possible paths forward. PMID:24847300

  1. Mars Rock Formation Poses Mystery

    NASA Technical Reports Server (NTRS)

    2004-01-01

    This sharp, close-up image taken by the microscopic imager on the Mars Exploration Rover Opportunity's instrument deployment device, or 'arm,' shows a rock target dubbed 'Robert E,' located on the rock outcrop at Meridiani Planum, Mars. Scientists are studying this area for clues about the rock outcrop's composition. This image measures 3 centimeters (1.2 inches) across and was taken on the 15th day of Opportunity's journey (Feb. 8, 2004).

  2. Introducing New Scientists

    E-print Network

    with innovative ideas who are opening up new directions in science. To help a new scientist come to IsraelIntroducing New Scientists 2009-2010 #12;#12;Table of Contents Support for New Scientists is Vital. Oren Tal 30 Dr. Assaf Vardi 32 Dr. Karina Yaniv 34 Dr. Ofer Yizhar 36 New Scientist Funds and Gifts 38

  3. Pump thrombosis—A riddle wrapped in a mystery inside an enigma

    PubMed Central

    2014-01-01

    This manuscript reviews the state of the art regarding the subject of pump thrombosis (PT). The historical context of PT and the clinical data are described, the etiologic factors are elucidated, preventive strategies are explored, diagnostic modalities are reviewed, and management principles are defined. There clearly remains much work to be done towards solving this riddle wrapped in a mystery inside an enigma, but promising foundations are being established. PMID:25452905

  4. Clueless: Adult Mysteries with Young Adult Appeal 2002.

    ERIC Educational Resources Information Center

    Charles, John; Morrison, Joanna

    2002-01-01

    This annotated bibliography includes adult mysteries that appeal to teen readers under the categories of Sherlock Holmes; reference sources; private investigators; amateur sleuths; historical sleuths; suspense and thrillers; police procedurals; mystery blends; and anthologies. (LRW)

  5. Mystery Bug Theater Renee Bryce and Vicki Allan

    E-print Network

    Bryce, Renee

    Mystery Bug Theater Ren´ee Bryce and Vicki Allan Utah State University Logan, UT 84321 Renee that improve our curriculum. This paper discusses several activities that rely on this data: (1) the "Mystery

  6. The Central Mystery of Quantum Mechanics

    E-print Network

    Partha Ghose

    2009-06-04

    A critical re-examination of the double-slit experiment and its variants is presented to clarify the nature of what Feynmann called the ``central mystery'' and the ``only mystery'' of quantum mechanics, leading to an interpretation of complementarity in which a `wave {\\em and} particle' description rather than a `wave {\\em or} particle' description is valid for the {\\em same} experimental set up, with the wave culminating in the particle sequentially in time. This interpretation is different from Bohr's but is consistent with the von Neumann formulation as well as some more recent interpretations of quantum mechanics.

  7. Creative Ways to Teach the Mysteries of History, Volume 1

    ERIC Educational Resources Information Center

    Pahl, Ronald Hans

    2005-01-01

    This book is developed to make the teaching and learning of history a powerful and enjoyable experience in the classroom through the study of historical mysteries. What better place to snoop around and dig through mysterious graves than in history class? This book takes ten mysterious events in history from ancient Egypt to the 21st century for…

  8. Mysteries of the Lunar Atmosphere

    NASA Astrophysics Data System (ADS)

    Killen, R. M.; Hurley, D. M.

    2012-12-01

    The lunar atmosphere has been probed by various instruments since the Apollo program, and continues to be measured today by the instruments onboard the Lunar Reconnaissance Orbiter, LRO. But like Sisyphus' trek, the progress has not been linear. LAMP, The Lyman Alpha Mapping Project, onboard LRO, measured He in the lunar exosphere, confirming the Apollo 17 result from the Lunar Atmosphere Composition Experiment (LACE) (Hoffman et al., 1973), but LAMP did not observe Ar although the expected 0.1 R should have been detectable by their instrument (Gladstone et al., Science, 2010). A surfeit of O+ was reported in the lunar wake (Mall et al. 1998; Hilchenbach et al. 1992;1993), but the origin of those ions is unknown, since oxygen has not been seen. Water and OH were measured on the surface of the moon, but theory tells us that efficiencies of production of water by solar wind proton bombardment may be low (Burke et al., Icarus, 2011). Starukhina and Shukaratov (LPSC, abstract 1385, 2010) suggest that the observed diurnal variation in the 3 micron band at the moon is due to thermal emission and not to variation in OH. LAMP observed Hg vapor following the LCROSS impact into Cabeus crater, but Hg atoms at 800 K (Wooden et al., LPSC abstract 2025, 2010) are too heavy to reach the altitudes where they would be exposed to sunlight, and thereby resonantly scatter photons, unless they are entrained in a gas with bulk velocity 3.5 km/s (Hurley et al., JGR, 2012). This bulk velocity is high for a 2 km/s impact. Another mystery from LCROSS is the H2 energy budget. Given the large amount of H2 observed after the LCROSS impact, and the high velocity required (a few km/s) to get in the field of view when it did, the kinetic energy associated with the H2 is too large of a fraction of the impactor energy. One possibility is that the H2 is produced by an exothermic reaction, which has implications for how it is stored in the regolith in permanently shadowed regions. The Na density is known to be low in the lunar exosphere when the Moon enters and traverses the Earth's magnetosphere, even though the major source processes should still be operative there. The high-energy component of Na observed in the extended Na tail at the moon, along with the very energetic Ca and Mg atoms observed at Mercury, also suggest the possibility of exothermic chemical reactions at or near the surfaces of these bodies. LCROSS also reported the presence of organics (Colaprete et al., Science, 2010), but their origin is unknown. The Apollo 15 coronal photographs recorded light scattering that was attributed to dust lofted from the lunar surface. More recently, upper limits on line of sight dust column of 103 cm-2 for 0.1 micron grains have been made via an analysis of Clementine star tracker data, much less than that predicted from Apollo results (Glenar et al., NLSI, 2012). We will report on modeling efforts that aim to resolve some of these uncertainties. Future observations by LADEE will be used along with models to further constrain the source and loss rates of volatiles.

  9. Inspiring Future Scientists

    ERIC Educational Resources Information Center

    Betteley, Pat; Lee, Richard E., Jr.

    2009-01-01

    In an integrated science/language arts/technology unit called "How Scientists Learn," students researched famous scientists from the past and cutting-edge modern-day scientists. Using biography trade books and the internet, students collected and recorded data on charts, summarized important information, and inferred meaning from text. Then they…

  10. Putting a Little Mystery in Teaching

    ERIC Educational Resources Information Center

    Goodwin, Bryan; Ristvey, John

    2011-01-01

    Posing mysteries is not just a gimmicky way to increase the entertainment value of a lesson; it taps into students' innate human desire to explore and learn about their environments. Instead of coming right out and providing students with the answers, teachers can build suspense, piquing students' natural curiosity. Teachers can guide students,…

  11. From Mystery Seed to Mangrove Island

    ERIC Educational Resources Information Center

    Frissell, Virginia

    2010-01-01

    Introducing a mystery object is an easy strategy to implement and allows teachers to pre-assess students' knowledge about local natural resources. Misconceptions can be noted as teachers record initial inquiries and wonderings on charts. Using the constructivist approach, students can explore and construct their learning as they continue to use…

  12. NOvA: Exploring Neutrino Mysteries

    SciTech Connect

    Vahle, Tricia; Messier, Mark

    2012-09-06

    Neutrinos are a mystery to physicists. They exist in three different flavors and mass states and may be able to give hints about the origins of the matter-dominated universe. A new long-baseline experiment led by Fermilab called NOvA may provide some answers.

  13. Mystery Boxes: Helping Children Improve Their Reasoning

    ERIC Educational Resources Information Center

    Rule, Audrey C.

    2007-01-01

    This guest editorial describes ways teachers can use guessing games about an unknown item in a "mystery box" to help children improve their abilities to listen to others, recall information, ask purposeful questions, classify items by class, make inferences, synthesize information, and draw conclusions. The author presents information from a…

  14. Taking the "Mystery" Out of Argumentation

    ERIC Educational Resources Information Center

    Lee, Eun Ju; Cite, Suleyman; Hanuscin, Deborah

    2014-01-01

    Many teachers have developed "tried and true" lessons that they look forward to teaching-- mystery powders is one that these authors like. Originally part of the Elementary Science Study curricula in the 1960s, there are now many different versions of this well-known activity in which students examine physical and chemical properties of…

  15. THE FEASIBILITY OF IDENTIFYING MYSTERY OIL SPILLS

    EPA Science Inventory

    Several off-the-shelf passive tagging techniques for identifying the origin of mystery oil spills were evaluated to determine the viability of enforcement provisions of Maine's Oil Conveyance Law. Duplicating the operating conditions experienced during every-day marine terminals ...

  16. Unraveling the Mystery of an Environmental Disease

    SciTech Connect

    Arthur Grollman

    2008-05-15

    For many years, residents of farming villages along the Danube River basin suffered from a fatal kidney disease and an associated urinary tract cancer. The cause of the disease remained a mystery for more than 50 years. Recently, however, Arthur Grollman and his colleagues have determined that home-baked bread is implicated in the disease, known as Balkan endemic nephropathy.

  17. Mysterious quantum Cheshire cat: an illusion

    NASA Astrophysics Data System (ADS)

    Michielsen, K.; Lippert, Th.; De Raedt, H.

    2015-09-01

    We provide a mystery-free explanation for the experimentally observed facts in the neutron interferometry quantum Cheshire cat experiment of Denkmayr et al. [Nat. Comm. 5, 4492, 2014] in terms of a discrete-event simulation model, demonstrating that the quantum Cheshire cat is an illusion.

  18. The Magic and Mysteries of Water

    E-print Network

    Richmond, Geraldine L.

    role in controlling our climate. In our bodies, water is the `canal of life', transporting and passingThe Magic and Mysteries of Water Speaker: Prof. Geri Richmond University of Oregon Water is ubiquitous in our lives. Covering more than two thirds of this planet, water surfaces provide a unique

  19. NOvA: Exploring Neutrino Mysteries

    ScienceCinema

    Vahle, Tricia; Messier, Mark

    2014-08-12

    Neutrinos are a mystery to physicists. They exist in three different flavors and mass states and may be able to give hints about the origins of the matter-dominated universe. A new long-baseline experiment led by Fermilab called NOvA may provide some answers.

  20. Mysterious Magnetar Yielding Secrets to VLA

    NASA Astrophysics Data System (ADS)

    2005-02-01

    A giant flash of energy from a supermagnetic neutron star thousands of light-years from Earth may shed a whole new light on scientists' understanding of such mysterious "magnetars" and of gamma-ray bursts. In the nearly two months since the blast, the National Science Foundation's Very Large Array (VLA) has produced a wealth of surprising information about the event, and "the show goes on," with continuing observations. This graphic illustrates the VLA measurements of the exanding fireball from the December 27, 2004, outburst from the magnetar SGR 1806-20. Each color indicates the observed size of the fireball at a different time. The sequence covers roughly three weeks of VLA observing. The outline of the fireball in each case is not an actual image, but rather a "best-fit" model of the shape that best matches the data from the VLA. Click on image for larger version. CREDIT: G.B. Taylor, NRAO/AUI/NSF The blast from an object named SGR 1806-20 came on December 27, 2004, and was first detected by orbiting gamma-ray and X-ray telescopes. It was the brightest outburst ever seen coming from an object beyond our own Solar System, and its energy overpowered most orbiting telescopes. The burst of gamma rays and X-rays even disturbed the Earth's ionosphere, causing a sudden disruption in some radio communications. While the intensely bright gamma ray burst faded away in a matter of minutes, the explosion's "afterglow" has been tracked by the VLA and other radio telescopes for weeks, providing most of the data needed by astronomers trying to figure out the physics of the blast. A magnetar is a superdense neutron star with a magnetic field thousands of trillions of times more intense than that of the Earth. Scientists believe that SGR 1806-20's giant burst of energy was somehow triggered by a "starquake" in the neutron star's crust that caused a catastrophic disruption in the magnetar's magnetic field. The magnetic disruption generated the huge burst of gamma rays and "boiled off" particles from the star's surface into a rapidly-expanding fireball that continues to emit radio waves for weeks or months. The VLA first observed SGR 1806-20 on January 3, and has been joined by other radio telescopes in Australia, the Netherlands, and India. Scientific papers prepared for publication based on the first month's radio observations report a number of key discoveries about the object. Scientists using the VLA have found: * The fireball of radio-emitting material is expanding at roughly one-third the speed of light. * The expanding fireball is elongated, and may change its shape quickly. * Alignment of the radio waves (polarization) confirms that the fireball is not spherical. * The flare emitted an amount of energy that represents a significant fraction of the total energy stored in the magnetar's magnetic field. Of the dozen or so magnetars known to astronomers, only one other has been seen to experience a giant outburst. In 1998, SGR 1900+14 put out a blast similar in many respects to SGR 1806-20's, but much weaker. National Radio Astronomy Observatory (NRAO) astronomer Dale Frail observed the 1998 outburst and has been watching SGR 1806-20 for a decade. Both magnetars are part of the small group of objects called soft gamma-ray repeaters, because they repeatedly experience much weaker outbursts of gamma rays. In early January, he was hosting a visiting college student while processing the first VLA data from SGR 1806-20's giant outburst. "I literally could not believe what I was looking at," Frail said. "Immediately I could see that this flare was 100 times stronger than the 1998 flare, and 10,000 times brighter than anything this object had done before." "I couldn't stay in my chair, and this student got to see a real, live astronomer acting like an excited little kid," Frail said. The excitement isn't over, either. "The show goes on and we continue to observe this thing and continue to get surprises," said Greg Taylor, an astronomer for

  1. Scientists: Engage the Public!

    PubMed

    Shugart, Erika C; Racaniello, Vincent R

    2015-01-01

    Scientists must communicate about science with public audiences to promote an understanding of complex issues that we face in our technologically advanced society. Some scientists may be concerned about a social stigma or "Sagan effect" associated with participating in public communication. Recent research in the social sciences indicates that public communication by scientists is not a niche activity but is widely done and can be beneficial to a scientist's career. There are a variety of approaches that scientists can take to become active in science communication. PMID:26695633

  2. Mysterious Lava Mineral on Mars

    NASA Technical Reports Server (NTRS)

    2004-01-01

    This graph or spectrum captured by the Moessbauer spectrometer onboard the Mars Exploration Rover Spirit shows the presence of three different iron-bearing minerals in the soil at the rover's landing site. One of these minerals has been identified as olivine, a shiny green rock commonly found in lava on Earth. The other two have yet to be pinned down. Scientists were puzzled by the discovery of olivine because it implies the soil consists at least partially of ground up rocks that have not been weathered or chemically altered. The black line in this graph represents the original data; the three colored regions denote individual minerals and add up to equal the black line.

    The Moessbauer spectrometer uses two pieces of radioactive cobalt-57, each about the size of pencil erasers, to determine with a high degree of accuracy the composition and abundance of iron-bearing minerals in martian rocks and soil. It is located on the rover's instrument deployment device, or 'arm.'

  3. Big Mysteries: The Higgs Mass

    SciTech Connect

    Lincoln, Don

    2014-04-28

    With the discovery of what looks to be the Higgs boson, LHC researchers are turning their attention to the next big question, which is the predicted mass of the newly discovered particles. When the effects of quantum mechanics is taken into account, the mass of the Higgs boson should be incredibly high...perhaps upwards of a quadrillion times higher than what was observed. In this video, Fermilab's Dr. Don Lincoln explains how it is that the theory predicts that the mass is so large and gives at least one possible theoretical idea that might solve the problem. Whether the proposed idea is the answer or not, this question must be answered by experiments at the LHC or today's entire theoretical paradigm could be in jeopardy.

  4. Big Mysteries: The Higgs Mass

    ScienceCinema

    Lincoln, Don

    2014-06-03

    With the discovery of what looks to be the Higgs boson, LHC researchers are turning their attention to the next big question, which is the predicted mass of the newly discovered particles. When the effects of quantum mechanics is taken into account, the mass of the Higgs boson should be incredibly high...perhaps upwards of a quadrillion times higher than what was observed. In this video, Fermilab's Dr. Don Lincoln explains how it is that the theory predicts that the mass is so large and gives at least one possible theoretical idea that might solve the problem. Whether the proposed idea is the answer or not, this question must be answered by experiments at the LHC or today's entire theoretical paradigm could be in jeopardy.

  5. Solving Problems.

    ERIC Educational Resources Information Center

    Hale, Norman; Lindelow, John

    Chapter 12 in a volume on school leadership, this chapter cites the work of several authorities concerning problem-solving or decision-making techniques based on the belief that group problem-solving effort is preferable to individual effort. The first technique, force-field analysis, is described as a means of dissecting complex problems into…

  6. Methods & Strategies: Sculpt-a-Scientist

    ERIC Educational Resources Information Center

    Jackson, Julie; Rich, Ann

    2014-01-01

    Elementary science experiences help develop students' views of science and scientific interests. As a result, teachers have been charged with the task of inspiring, cultivating, recruiting, and training the scientists needed to create tomorrow's innovations and solve future problems (Business Roundtable 2005). Who will these future…

  7. The Gamma-Ray Burst Mystery

    E-print Network

    David L. Band

    1997-12-15

    Gamma-ray bursts are transient events from beyond the solar system. Besides the allure of their mysterious origin, bursts are physically fascinating because they undoubtedly require exotic physics. Optical transients coincident with burst positions show that some, and probably all, bursts originate at cosmological distances, and not from a large Galactic halo. Observations of these events' spectral and temporal behavior will guide and constrain the study of the physical processes producing this extragalactic phenomenon.

  8. The Mystery of Gamma-Ray Bursts

    NASA Technical Reports Server (NTRS)

    Fishman, Gerald J.

    1998-01-01

    Gamma-ray bursts remain on of the greatest mysteries in astrophysics in spite of recent observational advances and intense theoretical work. Although some of the basic properties of bursts were known 25 years ago, new and more detailed observations have been made by the BATSE (Burst and Transient Source Experiment) experiment on the Compton Gamma Ray Observatory in the past five years. Recent observations of bursts and some proposed models will be discussed.

  9. Killing in Okaraygua: An Inspector Irronogaray Mystery

    E-print Network

    Levine, Stuart

    2012-09-05

    stream_size 857 stream_content_type text/plain stream_name Killing in Okaraygua_abstract.pdf.txt stream_source_info Killing in Okaraygua_abstract.pdf.txt Content-Encoding ISO-8859-1 Content-Type text/plain; charset=ISO-8859...-1 1 Citation: Levine, Stuart. (2012) Killing in Okaraygua: An Inspector Irronogaray Mystery [Kindle Edition]. Amazon Digital Services, Amazon.com. Published version: http://www.amazon.com/Killing-Okaraygua-Inspector-Irronogaray- ebook...

  10. Einstein's Biggest Blunder: A Cosmic Mystery Story

    SciTech Connect

    Krauss, Lawrence

    2007-05-30

    The standard model of cosmology built up over 20 years is no longer accepted as accurate. New data suggest that most of the energy density of the universe may be contained in empty space. Remarkably, this is exactly what would be expected if Einstein's cosmological constant really exists. If it does, its origin is the biggest mystery in physics and presents huge challenges for the fundamental theories of elementary particles and fields. Krauss explains Einstein's concept and describes its possible implications.

  11. Einstein's Biggest Blunder: A Cosmic Mystery Story

    ScienceCinema

    Krauss, Lawrence

    2010-09-01

    The standard model of cosmology built up over 20 years is no longer accepted as accurate. New data suggest that most of the energy density of the universe may be contained in empty space. Remarkably, this is exactly what would be expected if Einstein's cosmological constant really exists. If it does, its origin is the biggest mystery in physics and presents huge challenges for the fundamental theories of elementary particles and fields. Krauss explains Einstein's concept and describes its possible implications.

  12. Hidden Attraction - The History and Mystery of Magnetism

    NASA Astrophysics Data System (ADS)

    Verschuur, Gerrit L.

    1996-04-01

    Long one of nature's most fascinating phenomena, magnetism was once the subject of many superstitions. Magnets were thought useful to thieves, effective as a love potion, and as a cure for gout or spasms. They could remove sorcery from women and put demons to flight and even reconcile married couples. It was said that a lodestone pickled in the salt of sucking fish had the power to attract gold. Today, these beliefs have been put aside, but magnetism is no less remarkable for our modern understanding of it. In Hidden Attraction , Gerrit L. Verschuur, a noted astronomer and National Book Award nominee for The Invisible Universe , traces the history of our fascination with magnetism, from the mystery and superstition that propelled the first alchemical experiments with lodestone, through the more tangible works of Faraday, Maxwell, Hertz and other great pioneers of magnetism (scientists responsible for the extraordinary advances in modern science and technology, including radio, the telephone, and computers, that characterize the twentieth century), to state-of-the-art theories that see magnetism as a basic force in the universe. Boasting many informative illustrations, this is an adventure of the mind, using the specific phenomenon of magnetism to show how we have moved from an era of superstitions to one in which the Theory of Everything looms on the horizon.

  13. The mysterious world of plutonium metallurgy: Past and future

    SciTech Connect

    Hecker, S.S.; Hammel, E.F.

    1998-12-31

    The first atomic bomb detonated at the Trinity Site in New Mexico on July 16, 1945, used plutonium, a man-made element discovered < 5 yr earlier. The story of how Manhattan Project scientists and engineers tackled the mysteries of this element and fabricated it into the first atomic bomb is one of the most fascinating in the history of metallurgy and materials. The authors are currently trying to generate renewed interest in plutonium metallurgy because of the challenge posed by President Clinton, i.e., to keep the nuclear stockpile of weapons safe and reliable without nuclear testing. The stockpile stewardship challenge requires either a lifetime extension of the plutonium components or a remanufacture--neither of which can be verified by testing. In turn, this requires that one achieve a better fundamental understanding of plutonium. Of special interest is the effect of self-irradiation on the properties and on the long-term stability of plutonium and its alloys. Additional challenges arise from long-term concerns about disposing of plutonium and dealing with its environmental legacy. It is imperative to interest the next generation of students in these plutonium challenges.

  14. Scientists Shaping the Discussion

    NASA Astrophysics Data System (ADS)

    Abraham, J. A.; Weymann, R.; Mandia, S. A.; Ashley, M.

    2011-12-01

    Scientific studies which directly impact the larger society require an engagement between the scientists and the larger public. With respect to research on climate change, many third-party groups report on scientific findings and thereby serve as an intermediary between the scientist and the public. In many cases, the third-party reporting misinterprets the findings and conveys inaccurate information to the media and the public. To remedy this, many scientists are now taking a more active role in conveying their work directly to interested parties. In addition, some scientists are taking the further step of engaging with the general public to answer basic questions related to climate change - even on sub-topics which are unrelated to scientists' own research. Nevertheless, many scientists are reluctant to engage the general public or the media. The reasons for scientific reticence are varied but most commonly are related to fear of public engagement, concern about the time required to properly engage the public, or concerns about the impact to their professional reputations. However, for those scientists who are successful, these engagement activities provide many benefits. Scientists can increase the impact of their work, and they can help society make informed choices on significant issues, such as mitigating global warming. Here we provide some concrete steps that scientists can take to ensure that their public engagement is successful. These steps include: (1) cultivating relationships with reporters, (2) crafting clear, easy to understand messages that summarize their work, (3) relating science to everyday experiences, and (4) constructing arguments which appeal to a wide-ranging audience. With these steps, we show that scientists can efficiently deal with concerns that would otherwise inhibit their public engagement. Various resources will be provided that allow scientists to continue work on these key steps.

  15. Africa Steps up Efforts to Train Top Scientists

    ERIC Educational Resources Information Center

    Lindow, Megan

    2008-01-01

    This article reports on new programs that focus on training skilled scientists and mathematicians who will help solve Africa's myriad problems. The African Institute for Mathematical Sciences, in Cape Town, South Africa, offers one of the first working examples of a growing effort to develop a cadre of highly trained, practically minded scientists

  16. USGS Scientist Anna Chalfoun

    USGS Multimedia Gallery

    Dr. Anna D. Chalfoun, a USGS scientist and assistant leader at the Wyoming Cooperative Fish and Wildlife Research Unit, was awarded the 2012 Presidential Early Career Award for Scientists and Engineers (PECASE). This award is the highest recognition granted by the United States government to scien...

  17. Just like Real Scientists

    ERIC Educational Resources Information Center

    Betteley, Pat

    2009-01-01

    How do you inspire students to keep records like scientists? Share the primary research of real scientists and explicitly teach students how to keep records--that's how! Therefore, a group of third-grade students and their teacher studied the work of famous primatologist Jane Goodall and her modern-day counterpart Ian Gilby. After learning about…

  18. USGS Scientist Burke Minsley

    USGS Multimedia Gallery

    Dr. Burke Minsley,  a USGS geophysicist, was awarded the 2012 Presidential Early Career Award for Scientists and Engineers (PECASE). This award is the highest recognition granted by the United States government to scientists and engineers in the early stages of their research careers. Minsl...

  19. USGS Scientist Gavin Hayes

    USGS Multimedia Gallery

    Dr. Gavin Hayes,  a USGS geophysicist, was awarded the 2012 Presidential Early Career Award for Scientists and Engineers (PECASE). This award is the highest recognition granted by the United States government to scientists and engineers in the early stages of their research careers. Haye...

  20. Scientist Examines Tornado Vortex

    NASA Technical Reports Server (NTRS)

    1999-01-01

    In this Quick Time movie, a scientist examines what appears to be a tornado vortex (blue) coming out of a thunderstorm. The scientist uses 3D glasses to be able to see in 3 dimensions the different flows going out into the vortex. Earth science and weather studies are an important ongoing function of NASA and its affiliates.

  1. Stories of Scientists.

    ERIC Educational Resources Information Center

    Mascazine, John R.

    2001-01-01

    Presents three biographical sketches of scientists including John Wesley Powell (first to explore the geology of the Grand Canyon), Joseph von Fraunhofer (his work in optics led to the science of spectroscopy), and Gregor Mendel (of Mendelian genetics fame). Other scientists are mentioned along with sources for additional biographical information.…

  2. Quantum Computing Computer Scientists

    E-print Network

    Yanofsky, Noson S.

    Quantum Computing for Computer Scientists Noson S. Yanofsky and Mirco A. Mannucci #12;© May 2007 Noson S. Yanofsky Mirco A. Mannucci #12;Quantum Computing for Computer Scientists Noson S. Yanofsky.3 Towards Higher-Level Quantum Programming 7.4 Quantum Computation Before Quantum Computers 8 Theoretical

  3. Los Alamos Guns Take Aim at Material's Mysteries

    ScienceCinema

    Byers, Mark; Moore, David; Dimarino, Steve

    2014-05-30

    Los Alamos National Laboratory scientists and technicians conduct thousands of experiments a year, delving into the fundamental nature of everything from supernovas to subatomic particles. One set of instruments used to better understand the fundamental nature of various materials are 10 scientific gun systems that fire various projectiles at high-tech targets to create enormous velocities, pressures, and temperatures - and using laser, x-ray, and other diagnostics - explore the very nature of metals and other materials. The hundreds of gun-based experiments conducted every year at the Laboratory require a highly-skilled staff of scientists and technicians, and has given rise to a special organization called the "gun working group" to foster open communications, cooperation, problem-solving, and a healthy safety culture.

  4. Los Alamos Guns Take Aim at Material's Mysteries

    SciTech Connect

    Byers, Mark; Moore, David; Dimarino, Steve

    2014-04-14

    Los Alamos National Laboratory scientists and technicians conduct thousands of experiments a year, delving into the fundamental nature of everything from supernovas to subatomic particles. One set of instruments used to better understand the fundamental nature of various materials are 10 scientific gun systems that fire various projectiles at high-tech targets to create enormous velocities, pressures, and temperatures - and using laser, x-ray, and other diagnostics - explore the very nature of metals and other materials. The hundreds of gun-based experiments conducted every year at the Laboratory require a highly-skilled staff of scientists and technicians, and has given rise to a special organization called the "gun working group" to foster open communications, cooperation, problem-solving, and a healthy safety culture.

  5. Explaining a Mysterious Maximal Inequality --and a Path to the Law of Large Numbers

    E-print Network

    Steele, J. Michael

    Explaining a Mysterious Maximal Inequality -- and a Path to the Law of Large Numbers J. Michael as mysterious. Here we suggest a straightforward first step analysis that may dispel some of the mystery

  6. Scientists Discover Sugar in Space

    NASA Astrophysics Data System (ADS)

    2000-06-01

    The prospects for life in the Universe just got sweeter, with the first discovery of a simple sugar molecule in space. The discovery of the sugar molecule glycolaldehyde in a giant cloud of gas and dust near the center of our own Milky Way Galaxy was made by scientists using the National Science Foundation's 12 Meter Telescope, a radio telescope on Kitt Peak, Arizona. "The discovery of this sugar molecule in a cloud from which new stars are forming means it is increasingly likely that the chemical precursors to life are formed in such clouds long before planets develop around the stars," said Jan M. Hollis of the NASA Goddard Space Flight Center in Greenbelt, MD. Hollis worked with Frank J. Lovas of the University of Illinois and Philip R. Jewell of the National Radio Astronomy Observatory (NRAO) in Green Bank, WV, on the observations, made in May. The scientists have submitted their results to the Astrophysical Journal Letters. "This discovery may be an important key to understanding the formation of life on the early Earth," said Jewell. Conditions in interstellar clouds may, in some cases, mimic the conditions on the early Earth, so studying the chemistry of interstellar clouds may help scientists understand how bio-molecules formed early in our planet's history. In addition, some scientists have suggested that Earth could have been "seeded" with complex molecules by passing comets, made of material from the interstellar cloud that condensed to form the Solar System. Glycolaldehyde, an 8-atom molecule composed of carbon, oxygen and hydrogen, can combine with other molecules to form the more-complex sugars Ribose and Glucose. Ribose is a building block of nucleic acids such as RNA and DNA, which carry the genetic code of living organisms. Glucose is the sugar found in fruits. Glycolaldehyde contains exactly the same atoms, though in a different molecular structure, as methyl formate and acetic acid, both of which were detected previously in interstellar clouds. Glycolaldehyde is a simpler molecular cousin to table sugar, the scientists say. The sugar molecule was detected in a large cloud of gas and dust some 26,000 light-years away, near the center of our Galaxy. Such clouds, often many light-years across, are the material from which new stars are formed. Though very rarified by Earth standards, these interstellar clouds are the sites of complex chemical reactions that occur over hundreds of thousands or millions of years. So far, about 120 different molecules have been discovered in these clouds. Most of these molecules contain a small number of atoms, and only a few molecules with eight or more atoms have been found in interstellar clouds. The 12 Meter Telescope "Finding glycolaldehyde in one of these interstellar clouds means that such molecules can be formed even in very rarified conditions," said Hollis. "We don't yet understand how it could be formed there," he added. "A combination of more astronomical observations and theoretical chemistry work will be required to resolve the mystery of how this molecule is formed in space." "We hope this discovery inspires renewed efforts to find even more kinds of molecules, so that, with a better idea of the total picture, we may be able to deduce the details of the prebiotic chemistry taking place in interstellar clouds," Hollis said. The discovery was made by detecting faint radio emission from the sugar molecules in the interstellar cloud. Molecules rotate end-for-end, and as they change from one rotational energy state to another, they emit radio waves at precise frequencies. The "family" of radio frequencies emitted by a particular molecule forms a unique "fingerprint" that scientists can use to identify that molecule. The scientists identified glycolaldehyde by detecting six frequencies of radio emission in what is termed the millimeter-wavelength region of the electromagnetic spectrum -- a region between more-familiar microwaves and infrared radiation. The NRAO 12 Meter Telescop

  7. Chipping Away at a Mysterious Iceball

    NASA Astrophysics Data System (ADS)

    Johnson, Rebecca

    2005-03-01

    Pluto, or "Planet X" as it was once known, remains a mystery to astronomers even on the 75th anniversary its discovery. It is a member of a whole class of planet-like objects orbiting billions of miles beyond Neptune called "icy dwarfs" in a region of the solar system called the Kuiper Belt. A spacecraft launched on January 19, 2006 called New Horizons is scheduled to reach Pluto by about 2015 to further unlock some of the secrets of this distant cold planet, Charon, and other objects that lie beyond the orbit of Neptune.

  8. The Mystery of Gamma-Ray Bursts

    NASA Technical Reports Server (NTRS)

    Fishman, Gerald J.

    2004-01-01

    Gamma-ray bursts remain one of the greatest mysteries in astrophysics. Observations of gamma-ray bursts made by the BATSE experiment on the Compton Gamma-Ray Observatory will be described. Most workers in the field now believe that they originate from cosmological distances. This view has been reinforced by observations this year of several optical afterglow counterparts to gamma-ray bursts. A summary of these recent discoveries will be presented, along with their implications for models of the burst emission mechanism and the energy source of the bursts.

  9. Spotlight on Scientists Videos

    Cancer.gov

    NCI scientists, from postdoctoral fellows to principal investigators, discuss various topics including their personal backgrounds, how they came to be in the field of cancer research, their current projects, and a look to the future of medical oncology.

  10. Scientists Track Polar Bears

    USGS Multimedia Gallery

    Scientists track Polar bears with by attaching GPS equipped collars to a sample population.  These collars transmit data that help develop maps like this one that shows a swim of nearly 220 miles long....

  11. Scientists and Human Rights

    NASA Astrophysics Data System (ADS)

    Makdisi, Yousef

    2012-02-01

    The American Physical Society has a long history of involvement in defense of human rights. The Committee on International Freedom of Scientists was formed in the mid seventies as a subcommittee within the Panel On Public Affairs ``to deal with matters of an international nature that endangers the abilities of scientists to function as scientists'' and by 1980 it was established as an independent committee. In this presentation I will describe some aspects of the early history and the impetus that led to such an advocacy, the methods employed then and how they evolved to the present CIFS responsibility ``for monitoring concerns regarding human rights for scientists throughout the world''. I will also describe the current approach and some sample cases the committee has pursued recently, the interaction with other human rights organizations, and touch upon some venues through which the community can engage to help in this noble cause.

  12. The Mystery in Science: A Neglected Tool for Science Education

    ERIC Educational Resources Information Center

    Papacosta, Pangratios

    2008-01-01

    Of the many valuable tools available to science education, the mystery in science is the one that is most ignored, underused, or misunderstood. whenever it is used, it is only as mere entertainment or as an attention grabber. In this article, the author discusses how the mystery in science can improve student attitudes, generate a life-long…

  13. Campus Spies? Using Mystery Students to Evaluate University Performance

    ERIC Educational Resources Information Center

    Douglas, Alex; Douglas, Jacqueline

    2006-01-01

    Background: This paper explores the appropriateness of using mystery customer programmes in higher education institutions (HEIs) in the UK. Purpose: The main aim of the paper is to examine potential advantages and disadvantages of mystery customer programmes within HEIs, and to identify any issues that would need to be successfully resolved were…

  14. Magical Mysteries. Texas Reading Club, 1984. A Librarian's Planning Handbook.

    ERIC Educational Resources Information Center

    Oliver, Jim

    Designed to encourage library use by Texas youth, the Texas Reading Club programs usually include a structured reading program and a variety of entertaining literature-related storyhours, puppet shows, films, and other attractive happenings. This handbook for the 1984 theme--"magical mysteries"--focuses on mysteries, magic, and adventure stories,…

  15. Library Programs for Teens: Mystery Theater. VOYA Guides

    ERIC Educational Resources Information Center

    Siwak, Karen J.

    2010-01-01

    It's no mystery that fun and exciting programs bring teens into the library. Theater programs provide a venue for teens to express themselves creatively, encourage their participation in library programming, and offer them the opportunity for lively interaction with peers and adults. In "Library Programs for Teens: Mystery Theater," Karen Siwak…

  16. Make a Mystery Circuit with a Bar Light Fixture

    ERIC Educational Resources Information Center

    Lietz, Martha

    2007-01-01

    Teachers have been building mystery circuits or so-called "black box circuits" to use as a demonstration with their students for years. This paper presents an easy way to make simple mystery circuits using inexpensive light fixtures (see Fig. 1) available at almost any home improvement store. In a black box circuit, only the lightbulbs are visible…

  17. Goddard Visiting Scientist Program

    NASA Technical Reports Server (NTRS)

    2000-01-01

    Under this Indefinite Delivery Indefinite Quantity (IDIQ) contract, USRA was expected to provide short term (from I day up to I year) personnel as required to provide a Visiting Scientists Program to support the Earth Sciences Directorate (Code 900) at the Goddard Space Flight Center. The Contractor was to have a pool, or have access to a pool, of scientific talent, both domestic and international, at all levels (graduate student to senior scientist), that would support the technical requirements of the following laboratories and divisions within Code 900: 1) Global Change Data Center (902); 2) Laboratory for Atmospheres (Code 910); 3) Laboratory for Terrestrial Physics (Code 920); 4) Space Data and Computing Division (Code 930); 5) Laboratory for Hydrospheric Processes (Code 970). The research activities described below for each organization within Code 900 were intended to comprise the general scope of effort covered under the Visiting Scientist Program.

  18. William Dampier, seaman, scientist

    E-print Network

    Shipman, Joseph C.

    1962-01-01

    stream_size 110715 stream_content_type text/plain stream_name libseries.num15.pdf.txt stream_source_info libseries.num15.pdf.txt Content-Encoding UTF-8 Content-Type text/plain; charset=UTF-8 WILLIAM DAMPIER SEAMAN-SCIENTIST... by Col. John Fraser. Edited by George L. Anderson. 1961. Paper. $1.50 15. William Dumpier: Seaman-Scientist, by Joseph C. Shipman. 1962. Paper, $1.50 The Library Series and other University ot Kansas Publications are offered to learned societies...

  19. Improving Communication Skills in Early Career Scientists

    NASA Astrophysics Data System (ADS)

    Saia, S. M.

    2013-12-01

    The AGU fall meeting is a time for scientists to share what we have been hard at work on for the past year, to share our trials and tribulations, and of course, to share our science (we hope inspirational). In addition to sharing, the AGU fall meeting is also about collaboration as it brings old and new colleagues together from diverse communities across the planet. By sharing our ideas and findings, we build new relationships with the potential to cross boundaries and solve complex and pressing environmental issues. With ever emerging and intensifying water scarcity, extreme weather, and water quality issues across the plant, it is especially important that scientists like us share our ideas and work together to put these ideas into action. My vision of the future of water sciences embraces this fact. I believe that better training is needed to help early career scientists, like myself, build connections within and outside of our fields. First and foremost, more advanced training in effective storytelling concepts and themes may improve our ability to provide context for our research. Second, training in the production of video for internet-based media (e.g. YouTube) may help us bring our research to audiences in a more personalized way. Third, opportunities to practice presenting at highly visible public events such as the AGU fall meeting, will serve to prepare early career scientists for a variety of audiences. We hope this session, ';Water Sciences Pop-Ups', will provide the first steps to encourage and train early career scientists as they share and collaborate with scientists and non-scientists around the world.

  20. 222Rn variations in Mystery Cave, Minnesota

    USGS Publications Warehouse

    Lively, R.S.; Krafthefer, B.C.

    1995-01-01

    222Rn concentrations and meteorological parameters were measured at 4- h intervals over a 2-y period in Mystery Cave, southeastern Minnesota. Continuous radon monitors and meteorological sensors connected to data loggers were installed at several locations along commercial tour routes. 222Rn concentrations ranged as high as 25 kBq m-3 in summer and 20 kBq m-3 in winter. Average winter concentrations were lower than summer by at least a factor of two. Seasonal radon variations were correlative with outside air temperatures. During the winter, radon concentrations were observed to fluctuate periodically by factors of 20 or more in under 24 h. Both the long- and short-term variations are correlative with temperature- induced mixing of cave air with surface air.

  1. Quantum physics and the beam splitter mystery

    E-print Network

    Francois Henault

    2015-09-01

    Optical lossless beam splitters are frequently encountered in fundamental physics experiments regarding the nature of light, including "which-way" determination of light particles, N. Bohr's complementarity principle, or the EPR paradox and all their measurement apparatus. Although they look as common optical components at first glance, their behaviour remains somewhat mysterious since they apparently exhibit stand-alone particle-like features, and then wave-like characteristics when inserted into a Mach-Zehnder interferometer. In this communication are examined and discussed some basic properties of these beamssplitters, both from a classical optics and quantum physics point of view. Herein some convergences and contradictions are highlighted, and the results of a few emblematic experiments demonstrating photon existence are discussed. An alternative empirical model in wave optics is also proposed in order to shed light on some remaining questions

  2. Under the Lens: Investigating the Sun's Mysteries

    NASA Astrophysics Data System (ADS)

    Harwood, William; Klotz, Irene

    2008-11-01

    Sometime around 2012, the waxing 11-year solar cycle once again will reach its peak. Between now and then, magnetically turbulent sunspots, spawned by some still mysterious process, will form near the poles in increasing numbers and migrate toward the Sun's faster-rotating equator in pairs of opposite polarity. Titanic magnetic storms will rage as immense flux tubes rise to the surface in active regions around sunspots and spread out in a boiling sea of electric charge. Magnetic field lines across an enormous range of scales will arc and undulate, rip apart and reconnect, heating the Sun's upper atmosphere and occasionally triggering brilliant flares and multibillion-megaton coronal mass ejections (CMEs) that travel through the solar wind and slam into Earth.

  3. Quantum physics and the beam splitter mystery

    NASA Astrophysics Data System (ADS)

    Hénault, François

    2015-09-01

    Optical lossless beam splitters are frequently encountered in fundamental physics experiments regarding the nature of light, including "which-way" determination or the EPR paradox and their measurement apparatus. Although they look as common optical components at first glance, their behaviour remains somewhat mysterious since they apparently exhibit stand-alone particle-like features, and then wave-like characteristics when inserted into a Mach-Zehnder interferometer. In this communication are examined and discussed some basic properties of these beamssplitters, both from a classical optics and quantum physics point of view. Herein the most evident convergences and contradictions are highlighted, and the results of a few emblematic experiments demonstrating photon existence are discussed. Alternative empirical models are also proposed in order to shed light on some remaining issues.

  4. The peroxisome: still a mysterious organelle

    PubMed Central

    Fahimi, H. Dariush

    2008-01-01

    More than half a century of research on peroxisomes has revealed unique features of this ubiquitous subcellular organelle, which have often been in disagreement with existing dogmas in cell biology. About 50 peroxisomal enzymes have so far been identified, which contribute to several crucial metabolic processes such as ?-oxidation of fatty acids, biosynthesis of ether phospholipids and metabolism of reactive oxygen species, and render peroxisomes indispensable for human health and development. It became obvious that peroxisomes are highly dynamic organelles that rapidly assemble, multiply and degrade in response to metabolic needs. However, many aspects of peroxisome biology are still mysterious. This review addresses recent exciting discoveries on the biogenesis, formation and degradation of peroxisomes, on peroxisomal dynamics and division, as well as on the interaction and cross talk of peroxisomes with other subcellular compartments. Furthermore, recent advances on the role of peroxisomes in medicine and in the identification of novel peroxisomal proteins are discussed. PMID:18274771

  5. Nurturing the Child Scientist

    ERIC Educational Resources Information Center

    Rodgers, Lisa; Basca, Belinda

    2011-01-01

    The natural world fascinates young children. Treasured leaves, shells, stones, and twigs always find their way into the kindergarten classroom. A kindergarten study of collections channels and deepens children's innate impulse to explore and collect. It also lays the foundation for understanding how scientists approach the study of objects in…

  6. Spotlight on Scientists

    Cancer.gov

    These articles put a face to some of the thousands of individuals who contribute to NCI’s intramural and extramural cancer research efforts. The profiles highlight the work of scientists and clinicians and describe the circumstances and motivation behind their work.

  7. Talk Like a Scientist

    ERIC Educational Resources Information Center

    Marcum-Dietrich, Nanette

    2010-01-01

    In the scientific community, the symposium is one formal structure of conversation. Scientists routinely hold symposiums to gather and talk about a common topic. To model this method of communication in the classroom, the author designed an activity in which students conduct their own science symposiums. This article presents the science symposium…

  8. Teaming Up with Scientists.

    ERIC Educational Resources Information Center

    Moreno, Nancy P.; Chang, Kimberly A.; Tharp, Barbara Z.; Denk, James P.; Roberts, J. Kyle; Cutler, Paula H.; Rahmati, Sonia

    2001-01-01

    Introduces the Science Education Leadership Fellows (SELF) program which is an innovative cooperation program between teachers and scientists. Engages teachers in subject areas such as microbiology, molecular biology, immunology, and other professional development activities. Presents an activity in which students observe bacteria cultures and…

  9. USGS Scientist Tonie Rocke

    USGS Multimedia Gallery

    USGS scientist Tonie Rocke is working to immunize populations of free-ranging prairie dogs against plague with an oral sylvatic plague vaccine (SPV). Here, she stands beside a prairie dog hole at the Pitchfork Ranch in Wyoming, holding a sample of the brightly colored, peanut butter flavor...

  10. USGS Scientist Tonie Rocke

    USGS Multimedia Gallery

    USGS scientist Tonie Rocke is working to immunize populations of free-ranging prairie dogs against plague with an oral sylvatic plague vaccine (SPV). If successful, the SPV could help protect endangered black-footed ferret populations in the western U.S. because the ferrets rely on pr...

  11. Sylvie Chambon Research scientist

    E-print Network

    Chambon, Sylvie

    Sylvie Chambon Research scientist French Public Works Research Laboratory (LCPC), Nantes, France with the correlation-based matching methods that can take into account the color information and the occlusion problem of these methods. We are working on global methods based on seeds correspondences. These seeds are determined

  12. On Being a Scientist.

    ERIC Educational Resources Information Center

    National Academy of Sciences - National Research Council, Washington, DC. Committee on the Conduct of Science.

    This booklet was written for students and describes some of the basic features of a life in contemporary research and some of the personal and professional issues that researchers will encounter in their work. This booklet divides the decisions that scientists make into two overlapping categories. Much of the first half of the booklet looks at…

  13. Early Primary Invasion Scientists

    ERIC Educational Resources Information Center

    Spellman, Katie V.; Villano, Christine P.

    2011-01-01

    "We really need to get the government involved," said one student, holding his graph up to USDA scientist Steve Seefeldt. Dr. Steve studies methods to control "invasive" plants, plants that have been introduced to an area by humans and have potential to spread rapidly and negatively affect ecosystems. The first grader and his classmates had become…

  14. Scientist Releases Common Loon

    USGS Multimedia Gallery

    As part of a cooperative project, scientists with the USGS and the Wisconsin Department of Natural Resources tagged common loons in north central Wisconsin to study the distribution and migration movements, as well as foraging patterns and depth profiles of common loons equipped with archiv...

  15. Reading as Scientists

    ERIC Educational Resources Information Center

    Shanahan, Marie-Claire

    2010-01-01

    Using an adapted version of a recently published scientific article, a group of sixth graders worked together identifying conclusions, deciding on appropriate evidence, suggesting improvements for the study, and recommending further investigations for scientists. This experience provided opportunities for these students to use reading to decide on…

  16. Bringing Scientists to Life

    ERIC Educational Resources Information Center

    Casey, Peter

    2010-01-01

    In this article, the author describes how he brings scientists to life when he visits schools. Having retired from teaching Drama and Theatre Studies in Liverpool for more than thirty years, the author set up his one-man Theatre-in-Education company, Blindseer Productions, and now takes his portrayals of Darwin, Galileo and Einstein to schools…

  17. Becoming a Spider Scientist

    ERIC Educational Resources Information Center

    Patrick, Patricia; Getz, Angela

    2008-01-01

    In this integrated unit, third grade students become spider scientists as they observe spiders in their classroom to debunk some common misconceptions about these intimidating creatures. "Charlotte's Web" is used to capture students' interest. In addition to addressing philosophical topics such as growing-up, death, and friendship; E.B. White's…

  18. Women Scientists. American Profiles.

    ERIC Educational Resources Information Center

    Veglahn, Nancy, J.

    This book contains the life stories of 11 American female scientists who had outstanding achievements in their branch of science. The lives of the 11 women included in this book cover a combined time period of more than 120 years. This book argues against the belief that mathematics and science are not for girls and gives examples of very…

  19. Reading about Real Scientists

    ERIC Educational Resources Information Center

    Cummins, Sunday

    2015-01-01

    Although students do need hands-on experiences to master key skills in science, technology, and engineering, Cummins asserts, K-12 teachers should also help students understand key STEM concepts by reading, writing, and talking about the work of professional scientists and engineers. Cummins lists high-quality texts that help young people…

  20. Liangliang Nan Research Scientist

    E-print Network

    Nan, Liangliang

    ;date: Nov. 27, 2014. Application number: PCT/CN2013/083441. Filing date: Sept. 13, 2013 [2] PCT Patent and editing. Academic Positions May.2013 ­ present Research scientist. Visual Computing Center, King Abdullah University of Science and Technology, Saudi Arabia Aug.2011 ­ May.2013 Associate professor. Visual Computing

  1. Problem Solving and Game-Based Learning: Effects of Middle Grade Students' Hypothesis Testing Strategies on Learning Outcomes

    ERIC Educational Resources Information Center

    Spires, Hiller A.; Rowe, Jonathan P.; Mott, Bradford W.; Lester, James C.

    2011-01-01

    Targeted as a highly desired skill for contemporary work and life, problem solving is central to game-based learning research. In this study, middle grade students achieved significant learning gains from gameplay interactions that required solving a science mystery based on microbiology content. Student trace data results indicated that effective…

  2. Investigating Nature's Mysteries for Drug Development

    Cancer.gov

    More than half of the drugs approved to treat cancer come from a natural product or a natural product prototype. Scientists in NCI-Frederick's Natural Products Branch are exploring ways to harness chemicals produced by marine invertebrates, other animals, plants, and microbes for cancer drug discovery.

  3. The Mystery of the Sparkling Spheres

    NASA Technical Reports Server (NTRS)

    2004-01-01

    This image, taken by the microscopic imager, an instrument located on the Mars Exploration Rover Opportunity 's instrument deployment device, or 'arm,' reveals shiny, spherical objects embedded within the trench wall at Meridiani Planum, Mars. Scientists are highly intrigued by these objects and may further investigate them. The area in this image measures approximately 3 centimeters (1.2 inches) across.

  4. THE MYSTERIOUS WORLD OF KARST HYDROLOGY

    EPA Science Inventory

    D. Field collecting stream samples.

    Dr. Malcolm Field works for the National Center for Environmental Assessment, and may be the only EPA scientist actively working in ...

  5. Helping early career research scientists ascend the professional ladder.

    PubMed

    King, Laina

    2013-08-01

    The Keystone Symposia Early Career Investigator Travel Award initiative is a unique successful research mentoring program tailored for 'end of the pipeline' life and biomedical scientists from academia and industry. Using targeted educational, mentoring, and networking activities, the program benefits early career scientists in solving a specific laboratory-based research question that is limiting their evolving research and could increase their ability to obtain new grants and improve their career progression. PMID:23889774

  6. Toughening mystery of natural rubber deciphered by double network

    E-print Network

    Liang, Haiyi

    Toughening mystery of natural rubber deciphered by double network incorporating hierarchical. As an indispensible material for modern society, natural rubber possesses peerless mechanical properties and theoretical investigations have revealed the self-enhancement of natural rubber due to strain

  7. The mystery of missing heritability: Genetic interactions create phantom heritability

    E-print Network

    Sunyaev, Shamil R.

    Human genetics has been haunted by the mystery of “missing heritability” of common traits. Although studies have discovered >1,200 variants associated with common diseases and traits, these variants typically appear to ...

  8. CHIPPING AWAY AT THE MYSTERY OF DRUG RESPONSES

    EPA Science Inventory

    Chipping away at the mystery of drug responses
    John C. Rockett
    Reproductive Toxicology Division, National Health and Environmental Effects Research Laboratory, Office of Research and Development, United States Environmental Protection Agency, Research Triangle Park, NC 2771...

  9. Health Detectives: Uncovering the Mysteries of Disease (LBNL Science at the Theater)

    SciTech Connect

    Bissell, Mina; Canaria, Christie; Celnicker, Susan; Karpen, Gary

    2012-04-23

    In this April 23, 2012 Science at the Theater event, Berkeley Lab scientists discuss how they uncover the mysteries of disease in unlikely places. Speakers and topics include: World-renowned cancer researcher Mina Bissell's pioneering research on the role of the cellular microenvironment in breast cancer has changed the conversation about the disease. How does DNA instability cause disease? To find out, Christie Canaria images neural networks to study disorders such as Huntington's disease. Fruit flies can tell us a lot about ourselves. Susan Celniker explores the fruit fly genome to learn how our genome works. DNA is not destiny. Gary Karpen explores how environmental factors shape genome function and disease through epigenetics.

  10. Health Detectives: Uncovering the Mysteries of Disease (LBNL Science at the Theater)

    ScienceCinema

    Bissell, Mina; Canaria, Christie; Celnicker, Susan; Karpen, Gary

    2014-05-06

    In this April 23, 2012 Science at the Theater event, Berkeley Lab scientists discuss how they uncover the mysteries of disease in unlikely places. Speakers and topics include: World-renowned cancer researcher Mina Bissell's pioneering research on the role of the cellular microenvironment in breast cancer has changed the conversation about the disease. How does DNA instability cause disease? To find out, Christie Canaria images neural networks to study disorders such as Huntington's disease. Fruit flies can tell us a lot about ourselves. Susan Celniker explores the fruit fly genome to learn how our genome works. DNA is not destiny. Gary Karpen explores how environmental factors shape genome function and disease through epigenetics.

  11. The Great Scientists

    NASA Astrophysics Data System (ADS)

    Meadows, Jack

    1989-11-01

    This lively history of the development of science and its relationship to society combines vivid biographies of twelve pivotal scientists, commentary on the social and historical events of their time, and over four hundred illustrations, including many in color. The biographies span from classical times to the Atomic Age, covering Aristotle, Galileo, Harvey, Newton, Lavoisier, Humboldt, Faraday, Darwin, Pasteur, Curie, Freud, and Einstein. Through the biographies and a wealth of other material, the volume reveals how social forces have influenced the course of science. Along with the highly informative color illustrations, it contains much archival material never before published, ranging from medieval woodcuts, etchings from Renaissance anatomy texts, and pages from Harvey's journal, to modern false-color x-rays and infrared photographs of solar flares. A beautifully-designed, fact-filled, stimulating work, The Great Scientists will fascinate anyone with an interest in science and how history can influence scientific discovery.

  12. Scientists want more children.

    PubMed

    Ecklund, Elaine Howard; Lincoln, Anne E

    2011-01-01

    Scholars partly attribute the low number of women in academic science to the impact of the science career on family life. Yet, the picture of how men and women in science--at different points in the career trajectory--compare in their perceptions of this impact is incomplete. In particular, we know little about the perceptions and experiences of junior and senior scientists at top universities, institutions that have a disproportionate influence on science, science policy, and the next generation of scientists. Here we show that having fewer children than wished as a result of the science career affects the life satisfaction of science faculty and indirectly affects career satisfaction, and that young scientists (graduate students and postdoctoral fellows) who have had fewer children than wished are more likely to plan to exit science entirely. We also show that the impact of science on family life is not just a woman's problem; the effect on life satisfaction of having fewer children than desired is more pronounced for male than female faculty, with life satisfaction strongly related to career satisfaction. And, in contrast to other research, gender differences among graduate students and postdoctoral fellows disappear. Family factors impede talented young scientists of both sexes from persisting to research positions in academic science. In an era when the global competitiveness of US science is at risk, it is concerning that a significant proportion of men and women trained in the select few spots available at top US research universities are considering leaving science and that such desires to leave are related to the impact of the science career on family life. Results from our study may inform university family leave policies for science departments as well as mentoring programs in the sciences. PMID:21850232

  13. Gamma-Ray Bursts: A Mystery Story

    NASA Technical Reports Server (NTRS)

    Parsons, Ann

    2007-01-01

    With the success of the Swift Gamma-Ray Burst Explorer currently in orbit, this is quite an exciting time in the history of Gamma Ray Bursts (GRBs). The study of GRBs is a modern astronomical mystery story that began over 30 years ago with the serendipitous discovery of these astronomical events by military satellites in the late 1960's. Until the launch of BATSE on the Compton Gamma-ray Observatory, astronomers had no clue whether GRBs originated at the edge of our solar system, in our own Milky Way Galaxy or incredibly far away near the edge of the observable Universe. Data from BATSE proved that GRBs are distributed isotropically on the sky and thus could not be the related to objects in the disk of our Galaxy. Given the intensity of the gamma-ray emission, an extragalactic origin would require an astounding amount of energy. Without sufficient data to decide the issue, a great debate continued about whether GRBs were located in the halo of our own galaxy or were at extragalactic - even cosmological distances. This debate continued until 1997 when the BeppoSAX mission discovered a fading X-ray afterglow signal in the same location as a GRB. This discovery enabled other telescopes, to observe afterglow emission at optical and radio wavelengths and prove that GRBs were at cosmological distances by measuring large redshifts in the optical spectra. Like BeppoSAX Swift, slews to new GRB locations to measure afterglow emission. In addition to improved GRB sensitivity, a significant advantage of Swift over BeppoSAX and other missions is its ability to slew very quickly, allowing x-ray and optical follow-up measurements to be made as early as a minute after the gamma-ray burst trigger rather than the previous 6-8 hour delay. Swift afterglow measurements along with follow-up ground-based observations, and theoretical work have allowed astronomers to identify two plausible scenarios for the creation of a GRB: either through core collapse of super massive stars or colliding compact objects in distant galaxies. The pieces of the puzzle are beginning to fall into place and yet the story isn't quite finished. I will frame the history of gamma-ray bursts as a mystery story and will end with a description of what we still don't know and what we'll have to do to get the next clues.

  14. The Strength of the Strongest Ties in Collaborative Problem Solving

    E-print Network

    de Montjoye, Yves-Alexandre

    Complex problem solving in science, engineering, and business has become a highly collaborative endeavor. Teams of scientists or engineers collaborate on projects using their social networks to gather new ideas and feedback. ...

  15. Mysterious object He2-90

    NASA Technical Reports Server (NTRS)

    1999-01-01

    Astronomers using NASA's Hubble Space Telescope have stumbled upon a mysterious object that is grudgingly yielding clues to its identity. A quick glance at the Hubble picture at top shows that this celestial body, called He2-90, looks like a young, dust-enshrouded star with narrow jets of material streaming from each side. But it's not. The object is classified as a planetary nebula, the glowing remains of a dying, lightweight star. But the Hubble observations suggest that it may not fit that classification, either. The Hubble astronomers now suspect that this enigmatic object may actually be a pair of aging stars masquerading as a single youngster. One member of the duo is a bloated red giant star shedding matter from its outer layers. This matter is then gravitationally captured in a rotating, pancake-shaped accretion disk around a compact partner, which is most likely a young white dwarf (the collapsed remnant of a sun-like star). The stars cannot be seen in the Hubble images because a lane of dust obscures them.

  16. An investigation into the Paulding Mystery Lights

    NASA Astrophysics Data System (ADS)

    Bos, Jeremy P.; Norkus, William; Maurer, Michael; Sims, Douglas; Middlebrook, Christopher; Roggeman, Michael C.

    2011-09-01

    The Paulding Mystery Lights are a purportedly unexplained optical phenomenon, occurring nightly, deep in the woods of Michigan's Upper Peninsula. The Michigan Tech Student Chapter of the SPIE initiated a project in 2008 to understand the cause of the Paulding Lights. Previous investigations by skeptics attributed the lights to headlights without explicitly identifying a source location. Our team applied a number of straightforward techniques to identify and then verify the source location of the Paulding Light. Beginning with observation through a telescope, the team moved to using tools such as detailed topographical maps and more common tools such as Google Street View to identify a candidate source location. The candidate source location was then validated by first recreating the light using a vehicle parked in that location. Additional verification was achieved by examining the correlation between the occurrence of the light and the passing of cars at the source location. A spectrometer was also used to compare the visible spectrum of the light to automotive headlamps. Our findings, presented here, indicate that the source of the Paulding light is automobile traffic on a stretch of road about 7 km from the viewing location.

  17. Winterover scientists in Antarctic Astrophysics

    NASA Astrophysics Data System (ADS)

    Tothill, N. F. H.; Martin, C. L.

    2013-01-01

    Astronomy in Antarctica is largely carried out in winter, and so winterover scientists are required to run the instruments. A winterover appointment is a unique opportunity for a scientist, but brings challenges for both the scientist and the larger instrument team. We give a brief review of how winterovers work and their experiences. Although recent projects have required less support from winterover scientists, we believe that they will be a feature of Antarctic astronomy and astrophysics into the future.

  18. Emeritus Scientists, Mathematicians and Engineers (ESME) program

    SciTech Connect

    Sharlin, H.I.

    1992-09-01

    The Emeritus Scientists, Mathematicians and Engineers (ESME) program matches retired scientists and engineers with wide experience with elementary school children in order to fuel the children's natural curiosity about the world in which they live. The long-range goal is to encourage students to maintain the high level of mathematical and science capability that they exhibit at an early age by introducing them to the fun and excitement of the world of scientific investigation and engineering problem solving. Components of the ESME program are the emeriti, established teacher-emeriti teams that work to produce a unit of 6 class hours of demonstration or hands-on experiments, and the encounter by students with the world of science/engineering through the classroom sessions and a field trip to a nearby plant or laboratory.

  19. Developmental Potential among Creative Scientists

    ERIC Educational Resources Information Center

    Culross, Rita R.

    2008-01-01

    The world of creative scientists is dramatically different in the 21st century than it was during previous centuries. Whether biologists, chemists, physicists, engineers, mathematicians, or computer scientists, the livelihood of research scientists is dependent on their abilities of creative expression. The view of a solitary researcher who…

  20. NCI Women Scientist Advisors (WSA)

    Cancer.gov

    NIH 1. Hold regular meetings with her Scientific Director in order to advise him/her about issues relevant to women scientists. Attend Lab/Branch Chief meetings to serve as a representative of women scientists. 2. Inform the Institute's women scientists o

  1. NCI Women Scientist Advisors (WSA)

    Cancer.gov

    The NIH Women Scientist Advisors (WSA) was established 1992 for IRP women scientists to have an open forum to discuss and exchange ideas. Each WSA is elected by the women scientists of her IC or appointed and serves a two-year term. The NCI WSA's are resp

  2. Another Kind of Scientist Activism

    ERIC Educational Resources Information Center

    Marino, Lori

    2009-01-01

    In a well-cited 1996 editorial in "Science," "The Activist Scientist," Jaleh Daie calls for scientists to take an assertive role in educating politicians and the public about the importance of government support for research. She writes that most scientists are reluctant to become involved in political lobbying for a variety of reasons--time…

  3. Mental Imagery in Creative Problem Solving.

    ERIC Educational Resources Information Center

    Polland, Mark J.

    In order to investigate the relationship between mental imagery and creative problem solving, a study of 44 separate accounts reporting mental imagery experiences associated with creative discoveries were examined. The data included 29 different scientists, among them Albert Einstein and Stephen Hawking, and 9 artists, musicians, and writers,…

  4. Training the translational scientist.

    PubMed

    Jackson, Rebecca D; Gabriel, Sherine; Pariser, Anne; Feig, Peter

    2010-12-22

    A Clinical and Translational Science Awards Industry Forum titled "Promoting Efficient and Effective Collaborations Among Academia, Government, and Industry" was held in February 2010. A session at this forum was organized to address the training and skills needed to develop a biomedical scientific workforce that interfaces academia, government agencies, and industry to support the process of translating science into applicable means to improve health. By examining the requisite competencies and training resources for scientists in each of these sectors, opportunities for collaboration and adoption of new educational strategies were identified that could help to address barriers to translational research education and career development. PMID:21178132

  5. Astronomer to Data Scientist

    NASA Astrophysics Data System (ADS)

    Kirkpatrick, Jessica

    2015-01-01

    Jessica Kirkpatrick received her PhD in Astrophysics from Berkeley in 2012. After an exhaustive job search within academia and beyond, she accepted a job as a data scientist / analyst for the social network Yammer (acquired by Microsoft) and is now the Director of Data Science for Education Company InstaEDU. Now instead of spending her days finding patterns in the large scale structure of galaxies, she finds patterns in the behaviors of people. She'll talk about her transition from astrophysics to tech, compare and contrast the two fields, and give tips about how to land a tech job, and discuss useful tools which helped her with her transition.

  6. Soviet scientists speak out

    SciTech Connect

    Holloway, D. )

    1993-05-01

    In this article, Russian bomb designers answer the KGB's claim that espionage, not science, produced the Soviet bomb. Yuli Khariton and Yuri Smirnov wholly reject the argument that Soviet scientists can claim little credit for the first Soviet bomb. In a lecture delivered at the Kurchatov Institute, established in 1943 when Igor Kurchatov became the director of the Soviet nuclear weapons project, Khariton and Smironov point to the work done by Soviet nuclear physicists before 1941 and refute assertions that have been made in Western literature regarding the hydrogen bomb.

  7. Eisenhower, Scientists, and Sputnik

    NASA Astrophysics Data System (ADS)

    Rigden, John S.

    2007-04-01

    On October 4, 1957, the Russians launched a 184-pound satellite into Earth orbit. This event had a tremendous impact on Americans as it called into question the capability of U. S. science v'is-a-v'is that of the Russians. President Dwight D. Eisenhower called ``his scientists'' to the Oval Office and a meeting took place that Hans Bethe has called an ``unforgettable hour.'' I. I. Rabi, Chairman of the Science Advisory Committee made several proposals to President Eisenhower which the President accepted immediately. Today, 50-years later, we are still living with the legacy of Sputnik.

  8. The mysterious HI deficiency of NGC 3175

    E-print Network

    Michael Dahlem; Matthias Ehle; Stuart Ryder

    2001-03-06

    Australia Telescope Compact Array HI observations reveal the existence of 5.8x10^8 M_sun of HI gas in the central 7 kpc of the edge-on spiral galaxy NGC 3175. The detected HI and CO gas can explain why star formation, as traced by other emission processes, is going on in the inner part of its disk. On the other hand, the entire outer disk, beyond 3.5 kpc radius, shows no HI emission, has a very red colour and exhibits neither radio continuum nor H-alpha emission. This indicates that the outer part of NGC 3175 is quiescent, i.e. not forming stars at a measurable rate. Its HI deficiency and the small extent of the HI layer, which is confined to the boundaries of the optically visible disk, make NGC 3175 a peculiar spiral galaxy. No intergalactic HI gas in the NGC 3175 group was detected in our interferometric observations. Earlier Parkes telescope single dish HI observations put an upper limit on the amount of diffuse gas that might have been missed by the interferometer at 2x10^8 M_sun. On DSS plates no galaxy in the NGC 3175 group of galaxies (Garcia 1993) is close enough to it and none exhibits disturbances that could indicate a close interaction which might have led to the stripping of large parts of its HI gas. Thus, despite an extensive multi-wavelength investigation, the reason for the unusual absence of HI and star formation activity in the outer disk of NGC 3175 remains an intriguing mystery.

  9. Deciphering the mystery of thalidomide teratogenicity.

    PubMed

    Ito, Takumi; Handa, Hiroshi

    2012-03-01

    Thalidomide was originally developed in 1954 as a sedative that was commonly used to ameliorate morning sickness. However, thalidomide exposure during the first trimester of pregnancy caused multiple birth defects (e.g. phocomelia and amelia), affecting ? 10,000 children worldwide in the late 1950s and early 1960s. Thalidomide is now recognized as a clinically effective, albeit strictly restricted, drug for the treatment of leprosy and multiple myeloma. Investigators have studied thalidomide teratogenicity for half a century, proposing over 30 hypotheses to account for its actions. Among these, the anti-angiogenesis and oxidative stress models have gained widespread support. Nonetheless, the precise molecular mechanisms and direct targets of thalidomide have not heretofore been elucidated. We developed ferrite-glycidyl methacrylate beads that enable magnetic separation and efficient purification of ligand-binding molecules; the beads were recently employed to identify cereblon as a primary target of thalidomide. Cereblon forms an E3 ubiquitin ligase complex with DDB1, Cul4A, and Roc1, which is important for the expression of fibroblast growth factor 8, an essential regulator of limb development. Expression of a drug binding-deficient mutant of cereblon suppressed thalidomide-induced effects in zebrafish and chicks. This suggests that thalidomide downregulates fibroblast growth factor 8 expression and induces limb malformation by binding to wild-type cereblon, inhibiting the function of the associated E3 ubiquitin ligase. The present review summarizes the teratogenicity of thalidomide, including existing models for its mode of action, and discusses the identification of cereblon as a key molecule for deciphering the longstanding mystery of thalidomide teratogenicity. PMID:22348778

  10. Solving the mystery of booming sand dunes Nathalie M. Vriend,1

    E-print Network

    Clayton, Robert W.

    . Introduction [2] Explorers including Marco Polo [Polo, 1984] in the Gobi Desert, the Emperor Baber [Marquess May 2007; accepted 14 June 2007; published 23 August 2007. [1] Desert booming can be heard after by the boom- ing sounds of the desert. Sustained booming is defined as the continuous, loud droning sound

  11. The Mystery of the Deuterium Abundance in the Local Galactic Disk is Solved!

    E-print Network

    Linsky, Jeffrey L.

    Brian E. Wood 1 1 JILA, University of Colorado and NIST, Boulder, CO, 80309­0440, USA Abstract Analyses in the depletion of D onto dust grains can explain these local variations in the gas­phase D/H ratios. The D value for the total (gas plus dust) D/H ratio within 1 kpc of the Sun of 23 ± 4 ppm (parts per million

  12. Role of exposure analysis in solving the mystery of Balkan endemic nephropathy.

    PubMed

    Long, David T; Voice, Thomas C

    2007-06-01

    We evaluated the role of exposure analysis in assessing whether ochratoxin A or aristolochic acid are the agents responsible for causing Balkan endemic nephropathy. We constructed a framework for exposure analysis using the lessons learned from the study of endemic goiter within the context of an accepted general model. We used this framework to develop an exposure analysis model for Balkan endemic nephropathy, evaluated previous findings from the literature on ochratoxin A and aristolochic acid in the context of this model, discussed the strength of evidence for each, and proposed approaches to address critical outstanding questions. The pathway for exposure to ochratoxin A is well defined and there is evidence that humans have ingested ochratoxin A. Factors causing differential exposure to ochratoxin A and how ochratoxin A is implicated in Balkan endemic nephropathy are not defined. Although there is evidence of human exposure to aristolochic acid and that its effects are consistent with Balkan endemic nephropathy, a pathway for exposure to aristolochic acid has been suggested but not demonstrated. Factors causing differential exposure to aristolochic acid are not known. Exposure analysis results suggest that neither ochratoxin A nor aristolochic acid can be firmly linked to Balkan endemic nephropathy. However, this approach suggests future research directions that could provide critical evidence on exposure, which when linked with findings from the health sciences, may be able to demonstrate the cause of this disease and provide a basis for effective public health intervention strategies. One of the key unknowns for both agents is how differential exposure can occur. PMID:17589972

  13. Of mice and men: solving the molecular mysteries of Huntington's disease

    PubMed Central

    SHELBOURNE, P. F.

    2000-01-01

    Recent advances in the manipulation of mouse embryos provide opportunities for the disciplines of neuroscience and molecular genetics to join forces and tackle some previously intractable questions in this area of research. Even Huntington's disease has started to yield clues to its complex pathophysiology as a result of the recent application of transgenic technologies. This short review, while necessarily providing some background clinical information on Huntington's disease, will focus on how modifications of the mouse genome have contributed, and are continuing to contribute, to our understanding of the complex disease process. Such new insights may well turn the hope of developing the first effective treatment for this devastating disease into reality. PMID:10923992

  14. Solving the Mystery of Mock Mummies: Using Scientific Inquiry Skills in an Integrated Lesson

    ERIC Educational Resources Information Center

    Balgopal, Meena; Cornwall, Shaun; Gill-Robinson, Heather; Reinhart, Damien S.

    2009-01-01

    When the nature of science (NOS) is reinforced, middle school students will be able to appreciate scientific inquiry processes and communication, as outlined in the National Science Education Standards (NRC 1996). To this end, the authors developed a mummy-making and dissection activity to help sixth- and seventh-grade students learn more about…

  15. Role of Exposure Analysis in Solving the Mystery of Balkan Endemic Nephropathy

    PubMed Central

    Long, David T.; Voice, Thomas C.

    2007-01-01

    We evaluated the role of exposure analysis in assessing whether ochratoxin A aristolochic acid are the agents responsible for causing Balkan endemic nephropathy. We constructed a framework for exposure analysis using the lessons learned from the study of endemic goiter within the context of an accepted general model. We used this framework to develop an exposure analysis model for Balkan endemic nephropathy, evaluated previous findings from the literature on ochratoxin A and aristolochic acid in the context of this model, discussed the strength of evidence for each, and proposed approaches to address critical outstanding questions. The pathway for exposure to ochratoxin A is well defined and there is evidence that humans have ingested ochratoxin A. Factors causing differential exposure to ochratoxin A and how ochratoxin A is implicated in Balkan endemic nephropathy are not defined. Although there is evidence of human exposure to aristolochic acid and that its effects are consistent with Balkan endemic nephropathy, a pathway for exposure to aristolochic acid has been suggested but not demonstrated. Factors causing differential exposure to aristolochic acid are not known. Exposure analysis results suggest that neither ochratoxin A nor aristolochic acid can be firmly linked to Balkan endemic nephropathy. However, this approach suggests future research directions that could provide critical evidence on exposure, which when linked with findings from the health sciences, may be able to demonstrate the cause of this disease and provide a basis for effective public health intervention strategies. One of the key unknowns for both agents is how differential exposure can occur. PMID:17589972

  16. Archaeological jade mystery solved using a 119-year-old rock collection specimen

    NASA Astrophysics Data System (ADS)

    Harlow, G. E.; Davies, H. L.; Summerhayes, G. R.; Matisoo-Smith, E.

    2012-12-01

    In a recent publication (Harlow et al. 2012), a ~3200-year old small stone artefact from an archaeological excavation on Emirau Island, Bismarck Archipelago, Papua New Guinea was described and determined to be a piece of jadeite jade (jadeitite). True jadeitite from any part of New Guinea was not previously known, either in an archaeological or geological context, so this object was of considerable interest with respect to its geological source and what that would mean about trade between this source and Emirau Island. Fortuitously, the artefact, presumably a wood-carving gouge, is very unusual with respect to both pyroxene composition and minor mineral constituents. Pyroxene compositions lie essentially along the jadeite-aegirine join: Jd94Ae6 to Jd63Ae36, and without any coexisting omphacite. This contrasts with Jd-Di or Jd-Aug compositional trends commonly observed in jadeitites worldwide. Paragonite and albite occur in veins and cavities with minor titanite, epidote-allanite, and zircon, an assemblage seen in a few jadeitites. Surprisingly, some titanite contains up to 6 wt% Nb2O5 with only trace Ta and a single grain of a Y-Nb phase (interpreted as fergusonite) is present; these are unique for jadeitite. In a historical tribute to C.E.A. Wichmann, a German geologist who taught at Utrecht University, the Netherlands, a previously unpublished description of chlormelanite from the Torare River in extreme northeast Papua, Indonesia was given. The bulk composition essentially matches the pyroxene composition of the jade, so this sample was hypothesized as coming from the source. We were able to arrange a loan from the petrology collection at Utrecht University of the specimen acquired by Wichmann in 1893. In addition we borrowed stone axes from the Natural History Museum - Naturalis in Leiden obtained from natives near what is now Jayapura in eastern-most Papua. Petrography and microprobe analysis of sections of these samples clearly show that (1) Wichmann's 1893 Torare River "chloromelanite" is an extremely close match texturally and mineralogically with the jadeitite jade gouge, including Nb-rich titanite—thus a match, but that (2) the axes are omphacitites that have a geologically similar origin (high pressure/low-temperature subduction channel) but do not share the jadeite+aegerine-rich pyroxene or Nb-Y rich accessory phases. This research clearly shows that natural history collections are important archives that contain samples of potentially important value for science and cultural research. Moreover, research like this that connects geology, archaeology, history and preserved collections can yield a story that makes science and collections tangible and interesting to a popular audience. References: Harlow et al. 2012, Eur. J. Mineral. 24, 391-399.

  17. What's in a frog stomach? Solving a 150 year old mystery (Diptera: Calliphoridae)

    Technology Transfer Automated Retrieval System (TEKTRAN)

    The taxon Acanthosoma chrysalis Mayer, 1844, described from Germany on a number of alleged parasites encysted in the peritoneal wall of the stomach of edible frogs, is revised and shown to be first instar larvae of blow flies (Calliphoridae). Based on the shape of mouthhooks and abdominal cuticular ...

  18. Solving the carbon tetrachloride (CCl4) budget mystery using surface observations

    NASA Astrophysics Data System (ADS)

    Liang, Q.; Newman, P. A.; Daniel, J. S.; Reimann, S.; Hall, B. D.; Dutton, G. S.; Kuijpers, L. J. M.

    2014-12-01

    Carbon tetrachloride (CCl4) is a major anthropogenic ozone-depleting substance, with an ozone depletion potential (with respect to CFC-11) of 0.82. CCl4 is also a greenhouse gas and the 100-yr global warming potential is 1,400. In 1987, the Montreal Protocol (MP) included CCl4, and production and consumption were phased out for developed countries in 1996. Developing countries were allowed a delayed reduction, but CCl4 was fully phased out from emissive uses in 2010. However, the near-zero 2007-2012 emissions estimate based on the UNEP reported production and feedstock usage cannot be reconciled with the observed slow decline of atmospheric concentrations, year-to-year variability, and the inter-hemispheric gradient (IHG). We use available source and sink data in the NASA 3-Dimensional (3-D) Chemistry Climate Model, GEOSCCM, to test existing emissions and lifetime estimates against CCl4 mixing ratio observations. Our model results show that the IHG and global trend provide useful information for quantitatively constraining CCl4 emissions and lifetime estimates. The observed IHG (1.5±0.2 ppt for 2000-2012) is primarily caused by ongoing current emissions, while ocean and soil losses and stratosphere-troposphere exchange together contribute a small negative gradient (~0 - -0.3 ppt). Using the observed CCl4 global trend and IHG from the National Oceanic and Atmospheric Administration - Global Monitoring Division (NOAA-GMD) and Advanced Global Atmospheric Gases Experiment (AGAGE) networks, we deduce the mean global emissions for the 2000-2012 period are 39 (34-45, lower-upper limit emission estimates) Gg/yr (~ 30% of the peak 1980s emissions) and a corresponding total lifetime of 35 (37-32, upper-lower limit lifetime estimates) years. These results point to the need for a more accurate bottom-up estimate of CCl4 emissions as well as re-evaluation of the CCl4 best estimate lifetime (currently 25 years).

  19. Mars Rock Formation Poses Mystery-2

    NASA Technical Reports Server (NTRS)

    2004-01-01

    This sharp, close-up image taken by the microscopic imager on the Mars Exploration Rover Opportunity's instrument deployment device, or 'arm,' shows a rock target dubbed 'Robert E,' located on the rock outcrop at Meridiani Planum, Mars. Scientists are studying the spherule, or small sphere, in the center of the image that appears to be protruding from the rock formation. This image measures 3 centimeters (1.2 inches) across and was taken on the 15th day of Opportunity's journey (Feb. 8, 2004).

  20. Women Scientists in Training

    NASA Technical Reports Server (NTRS)

    1975-01-01

    Women scientists in training at Marshall Space Flight Center, (top to bottom) Carolyn Griner, Ann Whitaker, and Dr. Mary Johnston, are shown simulating weightlessness while undergoing training in the Neutral Buoyancy Simulator. These women were part of a special program dedicated to gaining a better understanding of problems involved in performing experiments in space. The three were engaged in designing and developing experiments for space, such as materials processing for Spacelabs. Dr. Johnston specialized in metallurgical Engineering, Dr. Whitaker in lubrication and surface physics, and Dr. Griner in material science. Dr. Griner went on to become Acting Center Director at Marshall Space Flight Center from January to September 1998. She was the first woman to serve

  1. 78 FR 45285 - Culturally Significant Objects Imported for Exhibition Determinations: “Egypt's Mysterious Book...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-07-26

    ... From the Federal Register Online via the Government Publishing Office DEPARTMENT OF STATE Culturally Significant Objects Imported for Exhibition Determinations: ``Egypt's Mysterious Book of the..., 2003), I hereby determine that the objects to be included in the exhibition ``Egypt's Mysterious...

  2. THE MYSTERY OF HISTORICAL CHANNEL SHOALING AT HOUSTON-GALVESTON NAVIGATION CHANNEL, TX

    E-print Network

    US Army Corps of Engineers

    560 THE MYSTERY OF HISTORICAL CHANNEL SHOALING AT HOUSTON-GALVESTON NAVIGATION CHANNEL, TX JULIE. Herein, we review data for the estuarine reaches of the HGNC and explore the mystery of the shoaling data

  3. The Mystery of Dispersionless Injection of Energetic Particles Associated With Magnetospheric Substorms

    E-print Network

    Reeves, Geoffrey D.

    1 The Mystery of Dispersionless Injection of Energetic Particles Associated With Magnetospheric-standing mystery since it did not appear that the particles could all be accelerated locally yet they appeared

  4. 78 FR 45285 - Culturally Significant Objects Imported for Exhibition Determinations: “Egypt's Mysterious Book...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-07-26

    ...Imported for Exhibition Determinations: ``Egypt's Mysterious Book of the Faiyum'' SUMMARY: Notice is hereby given of the following...objects to be included in the exhibition ``Egypt's Mysterious Book of the Faiyum,'' imported from abroad for temporary...

  5. The mystery of Morgellons disease: infection or delusion?

    PubMed

    Savely, Virginia R; Leitao, Mary M; Stricker, Raphael B

    2006-01-01

    Morgellons disease is a mysterious skin disorder that was first described more than 300 years ago. The disease is characterized by fiber-like strands extruding from the skin in conjunction with various dermatologic and neuropsychiatric symptoms. In this respect, Morgellons disease resembles and may be confused with delusional parasitosis. The association with Lyme disease and the apparent response to antibacterial therapy suggest that Morgellons disease may be linked to an undefined infectious process. Further clinical and molecular research is needed to unlock the mystery of Morgellons disease. PMID:16489838

  6. Gigantic Cosmic Corkscrew Reveals New Details About Mysterious Microquasar

    NASA Astrophysics Data System (ADS)

    2004-10-01

    Making an extra effort to image a faint, gigantic corkscrew traced by fast protons and electrons shot out from a mysterious microquasar paid off for a pair of astrophysicists who gained new insights into the beast's inner workings and also resolved a longstanding dispute over the object's distance. Microquasar SS 433 VLA Image of Microquasar SS 433 CREDIT: Blundell & Bowler, NRAO/AUI/NSF (Click on Image for Larger Version) The astrophysicists used the National Science Foundation's Very Large Array (VLA) radio telescope to capture the faintest details yet seen in the plasma jets emerging from the microquasar SS 433, an object once dubbed the "enigma of the century." As a result, they have changed scientists' understanding of the jets and settled the controversy over its distance "beyond all reasonable doubt," they said. SS 433 is a neutron star or black hole orbited by a "normal" companion star. The powerful gravity of the neutron star or black hole draws material from the stellar wind of its companion into an accretion disk of material tightly circling the dense central object prior to being pulled onto it. This disk propels jets of fast protons and electrons outward from its poles at about a quarter of the speed of light. The disk in SS 433 wobbles like a child's top, causing its jets to trace a corkscrew in the sky every 162 days. The new VLA study indicates that the speed of the ejected particles varies over time, contrary to the traditional model for SS 433. "We found that the actual speed varies between 24 percent to 28 percent of light speed, as opposed to staying constant," said Katherine Blundell, of the University of Oxford in the United Kingdom. "Amazingly, the jets going in both directions change their speeds simultaneously, producing identical speeds in both directions at any given time," Blundell added. Blundell worked with Michael Bowler, also of Oxford. The scientists' findings have been accepted by the Astrophysical Journal Letters. SS 433 New VLA Image of SS 433: Red-and-Blue Line Shows Path of Constant-Speed Jets. Note Poor Match of Path to Image. CREDIT: Blundell & Bowler, NRAO/AUI/NSF SS 433 Same Image, With Colored Beads Representing Particle Ejections at Different Speeds. Particle Path Now Matches. CREDIT: Blundell & Bowler, NRAO/AUI/NSF Click Here for Page of Full-Sized Graphics The new VLA image shows two full turns of the jets' corkscrew on both sides of the core. Analyzing the image showed that if material came from the core at a constant speed, the jet paths would not accurately match the details of the image. "By simulating ejections at varying speeds, we were able to produce an exact match to the observed structure," Blundell explained. The scientists first did their match to one of the jets. "We then were stunned to see that the varying speeds that matched the structure of one jet also exactly reproduced the other jet's path," Blundell said. Matching the speeds in the two jets reproduced the observed structure even allowing for the fact that, because one jet is moving more nearly away from us than the other, it takes light longer to reach us from it, she added. The astrophysicists speculate that the changes in ejection speed may be caused by changes in the rate at which material is transferred from the companion star onto the accretion disk. The detailed new VLA image also allowed the astrophysicists to determine that SS 433 is nearly 18,000 light-years distant from Earth. Earlier estimates had the object, in the constellation Aquila, as near as 10,000 light-years. An accurate distance, the scientists said, now allows them to better determine the age of the shell of debris blown out by the supernova explosion that created the dense, compact object in the microquasar. Knowing the distance accurately also allows them to measure the actual brightness of the microquasar's components, and this, they said, improves their understanding of the physical processes at work in the system. The breakthrough image was made us

  7. Students and Scientists Take a "Lichen" To Air Quality Assessment in Ireland.

    ERIC Educational Resources Information Center

    Murphy, Anthony P.

    1998-01-01

    Describes a cooperative project in which students in a number of areas in Ireland collect environmental data for use by scientists working to solve real-life problems. Reports on the follow-up survey to the study. (DDR)

  8. The Murder Mystery Method for Determining Whether a Vector Field is Conservative

    E-print Network

    The Murder Mystery Method for Determining Whether a Vector Field is Conservative Tevian Dray;method, which we call the murder mystery method, in our own classes for many years; students love it this to students as a murder mystery. A crime has been committed by the unknown murderer f ; your job is to find

  9. Twin Dimples Intrigue Scientists

    NASA Technical Reports Server (NTRS)

    2004-01-01

    This image from the Mars Exploration Rover Opportunity is part of the first set of pictures that was returned to Earth after the rover exited 'Eagle Crater.' Scientists are busy analyzing Opportunity's new view of the plains of Meridiani Planum. The plentiful ripples are a clear indication that wind is the primary geologic process currently in effect on the plains. On the left of the image are two depressions--each about a meter (about 3.3 feet) across--that feature bright spots in their centers. One possibility is that the bright material is similar in composition to the rocks in Eagle Crater's outcrop and the surrounding darker material is what's referred to as 'lag deposit,' or erosional remnants that are much harder and more difficult to wear away. These twin dimples might be revealing pieces of a larger outcrop that lies beneath. The depression closest to Opportunity is whimsically referred to as 'Homeplate' and the one behind it as 'First Base.' The rover's panoramic camera is set to take detailed images of the depressions today, on Opportunity's 58th sol. The backshell and parachute that helped protect the rover and deliver it safely to the surface of Mars are also visible near the horizon, in the center of the image. This image was taken by the rover's navigation camera.

  10. Overcoming the obstacles: Life stories of scientists with learning disabilities

    NASA Astrophysics Data System (ADS)

    Force, Crista Marie

    Scientific discovery is at the heart of solving many of the problems facing contemporary society. Scientists are retiring at rates that exceed the numbers of new scientists. Unfortunately, scientific careers still appear to be outside the reach of most individuals with learning disabilities. The purpose of this research was to better understand the methods by which successful learning disabled scientists have overcome the barriers and challenges associated with their learning disabilities in their preparation and performance as scientists. This narrative inquiry involved the researcher writing the life stories of four scientists. These life stories were generated from extensive interviews in which each of the scientists recounted their life histories. The researcher used narrative analysis to "make sense" of these learning disabled scientists' life stories. The narrative analysis required the researcher to identify and describe emergent themes characterizing each scientist's life. A cross-case analysis was then performed to uncover commonalities and differences in the lives of these four individuals. Results of the cross-case analysis revealed that all four scientists had a passion for science that emerged at an early age, which, with strong drive and determination, drove these individuals to succeed in spite of the many obstacles arising from their learning disabilities. The analysis also revealed that these scientists chose careers based on their strengths; they actively sought mentors to guide them in their preparation as scientists; and they developed coping techniques to overcome difficulties and succeed. The cross-case analysis also revealed differences in the degree to which each scientist accepted his or her learning disability. While some demonstrated inferior feelings about their successes as scientists, still other individuals revealed feelings of having superior abilities in areas such as visualization and working with people. These individuals revealed beliefs that they developed these special abilities as a result of their learning differences, which made them better than their non-learning disabled peers in certain areas. Finally, the researcher discusses implications of these findings in the light of special accommodations that can be made by teachers, school counselors, and parents to encourage learning disabled children who demonstrate interest in becoming scientists.

  11. How scientists think: On-line creativity and conceptual change in

    E-print Network

    Dunbar, Kevin N.

    .C: American Psychological Association Press #12;Page 2 How scientists think: On-line creativity and conceptual solving processes that form the foundation for creative cognition (see Dunbar, in press, Holyoak 1996Page 1 How scientists think: On-line creativity and conceptual change in science Kevin Dunbar, Mc

  12. Mystery of a Dimming White Dwarf

    NASA Astrophysics Data System (ADS)

    Kohler, Susanna

    2015-12-01

    In the wake of the recent media attention over an enigmatic, dimming star, another intriguing object has been discovered: J1529+2928, a white dwarf that periodically dims. This mystery, however, may have a simple solution with interesting consequences for future surveys of white dwarfs.Unexpected VariabilityJ1529+2928 is an isolated white dwarf that appears to have a mass of slightly more than the Sun. But rather than radiating steadily, J1529+2928 dims once every 38 minutes almost as though it were being eclipsed.The team that discovered these variations, led by Mukremin Kilic (University of Oklahoma), used telescopes at the Apache Point Observatory and the McDonald Observatory to obtain follow-up photometric data of J1529+2928 spread across 66 days. The team also took spectra of the white dwarf with the Gemini North telescope.Kilic and collaborators then began, one by one, to rule out possible causes of this objects variability.Eliminating OptionsThe period of the variability is too long for J1529+2928 to be a pulsating white dwarf with luminosity variation caused by gravity-wave pulsations.The variability cant be due to an eclipse by a stellar or brown-dwarf companion, because there isnt any variation in J1529+2928s radial velocity.Its not due to the orbit of a solid-body planetary object; such a transit would be too short to explain observations.It cant be due to the orbit of a disintegrated planet; this wouldnt explain the light curves observed in different filters plus the light curve doesnt change over the 66-day span.Spotty SurfaceTop and middle two panels: light curves from three different nights observing J1529+2928s periodic dimming. Bottom panel: The Fourier transform shows a peak at 37.7 cycles/day (and another, smaller peak at its first harmonic). [Kilic et al. 2015]So what explanation is left? The authors suggest that J1529+2928s variability is likely caused by a starspot on the white dwarfs surface that rotates into and out of our view. Estimates show that the observed light curves could be created by a starspot at about 10,000K (compared to the white dwarfs effective temperature of ~11,900K), covering 14% of the surface area at an inclination of 90.The formation of such a starspot would almost certainly require the presence of magnetic fields. Interestingly, J1529+2928 doesnt have a strong magnetic field; from its spectra, the team can constrain its field strength to be less than 70 kG.Given that up to 15% of white dwarfs are thought to have kG magnetic fields, eclipse-like events such as this one might in fact be common for white dwarfs. If so, then many similar events will likely be observed with future surveys of transients like Keplers ongoing K2 mission, which is expected to image another several hundred white dwarfs, or the upcoming Large Synoptic Survey Telescope, which will image 13 million white dwarfs.CitationMukremin Kilic et al 2015 ApJ 814 L31. doi:10.1088/2041-8205/814/2/L31

  13. Mystery of a Dimming White Dwarf

    NASA Astrophysics Data System (ADS)

    Kohler, Susanna

    2016-01-01

    In the wake of the recent media attention over an enigmatic, dimming star, another intriguing object has been discovered: J1529+2928, a white dwarf that periodically dims. This mystery, however, may have a simple solution with interesting consequences for future surveys of white dwarfs.Unexpected VariabilityJ1529+2928 is an isolated white dwarf that appears to have a mass of slightly more than the Sun. But rather than radiating steadily, J1529+2928 dims once every 38 minutes almost as though it were being eclipsed.The team that discovered these variations, led by Mukremin Kilic (University of Oklahoma), used telescopes at the Apache Point Observatory and the McDonald Observatory to obtain follow-up photometric data of J1529+2928 spread across 66 days. The team also took spectra of the white dwarf with the Gemini North telescope.Kilic and collaborators then began, one by one, to rule out possible causes of this objects variability.Eliminating OptionsThe period of the variability is too long for J1529+2928 to be a pulsating white dwarf with luminosity variation caused by gravity-wave pulsations.The variability cant be due to an eclipse by a stellar or brown-dwarf companion, because there isnt any variation in J1529+2928s radial velocity.Its not due to the orbit of a solid-body planetary object; such a transit would be too short to explain observations.It cant be due to the orbit of a disintegrated planet; this wouldnt explain the light curves observed in different filters plus the light curve doesnt change over the 66-day span.Spotty SurfaceTop and middle two panels: light curves from three different nights observing J1529+2928s periodic dimming. Bottom panel: The Fourier transform shows a peak at 37.7 cycles/day (and another, smaller peak at its first harmonic). [Kilic et al. 2015]So what explanation is left? The authors suggest that J1529+2928s variability is likely caused by a starspot on the white dwarfs surface that rotates into and out of our view. Estimates show that the observed light curves could be created by a starspot at about 10,000K (compared to the white dwarfs effective temperature of ~11,900K), covering 14% of the surface area at an inclination of 90.The formation of such a starspot would almost certainly require the presence of magnetic fields. Interestingly, J1529+2928 doesnt have a strong magnetic field; from its spectra, the team can constrain its field strength to be less than 70 kG.Given that up to 15% of white dwarfs are thought to have kG magnetic fields, eclipse-like events such as this one might in fact be common for white dwarfs. If so, then many similar events will likely be observed with future surveys of transients like Keplers ongoing K2 mission, which is expected to image another several hundred white dwarfs, or the upcoming Large Synoptic Survey Telescope, which will image 13 million white dwarfs.CitationMukremin Kilic et al 2015 ApJ 814 L31. doi:10.1088/2041-8205/814/2/L31

  14. Anania Shirakatsi and "Pagan" Scientists

    NASA Astrophysics Data System (ADS)

    Vardumyan, Gohar

    2014-10-01

    Anania Shirakatsi's approach to the views of "Pagan" scientists is discussed. He had special attitude to ancient science and its representatives. In his various works he criticizes their wrong views. Shirakatsi was especially good in distinguishing the correct and erroneous points of view by different scientists and he could chose the right approach and add his own one.

  15. The Scientist as School Teacher.

    ERIC Educational Resources Information Center

    Waksman, Byron H.

    2003-01-01

    Describes ways in which scientists engage in science education in an attempt to increase knowledge. Discusses intuitional approaches to school teaching, improvement of science education in middle schools, and the scientist's role in science teaching. (Contains 19 references.) (Author/YDS)

  16. USGS Scientists Monitor Animas River

    USGS Multimedia Gallery

    USGS scientist collecting water samples along the Animas River in Farmington, New Mexico on August 8, 2015. Scientists from the USGS New Mexico Water Science Center obtained water samples from the Animas and San Juan Rivers before and after arrival of the August 5 Gold King Mine ...

  17. The Mystery of Matter, World of the Atom Series.

    ERIC Educational Resources Information Center

    Pollard, William G.

    This booklet is one in the "World of the Atome Series" for junior high school students and their teachers. It describes the fascinating story of the search for the key to the structure of matter. These topics are reviewed: the chemical atom of the 19th century, the planetary atom, the wave atom, inside the elementary particles, and the mystery of…

  18. Magical Mystery Tour Voodoo Science. The Road from

    E-print Network

    Turro, Nicholas J.

    Magical Mystery Tour Voodoo Science. The Road from Foolishness to Fraud. Edited by Robert L. Park: The Road from Fool- ishness to Fraud is authored by Robert Park, who has been active in uni- versity may evolve into self-delusion and sometimes even transform into fraud. Park states that TMThe line

  19. Love Murder Mystery pp. 4 9 Poetry pp. 9 11

    E-print Network

    Sin, Peter

    1 Higlights Love Murder Mystery pp. 4 ­ 9 Poetry pp. 9 ­ 11 Autobiographies pp. 11 ­ 12 Food I was a child, I discovered two great tools: my hands. I was fascinated with a ladys thin, long. Without my hands, I could have lost a way of knowing, loving, and understanding the world, people

  20. Martian Mysteries Is there any life on Mars right now?

    E-print Network

    Lawrence, Rick L.

    Slide 1 Martian Mysteries · Is there any life on Mars right now? · Was there ever life on Mars? · Can humans live on Mars? · How would YOU find the answers? NOTES: Ask the students what kind of questions they have about Mars, telling them that you hope to get to all of their questions

  1. The Mystery and Misery of Acid Reflux in Children

    ERIC Educational Resources Information Center

    Davenport, Mike; Davenport, Tracy

    2006-01-01

    When a child is sick, parents want answers. They want to know what is wrong, what they can do, and how to get their child healthy--pronto. Regrettably, there are some puzzling illnesses affecting children that are surrounded by mystery. One of them is gastroesophageal reflux (GER), otherwise known as acid reflux--or "reflux" for short. Reflux…

  2. ORIGINAL ARTICLE Identifying a mysterious aquatic fern gametophyte

    E-print Network

    ORIGINAL ARTICLE Identifying a mysterious aquatic fern gametophyte Fay-Wei Li Æ Benito C. Tan Æ because of its ribbon-like thallus. How- ever, its antheridia are remarkably fern-like in morphology. To corroborate the hypothesis that Su¨ßwassertang is a fern gametophyte and to determine its closest relative, we

  3. Use of the Mystery Motivator for a High School Class

    ERIC Educational Resources Information Center

    Schanding, G. Thomas, Jr.; Sterling-Turner, Heather E.

    2010-01-01

    This study examined the effect of one interdependent group contingency intervention, the mystery motivator, as it affected three students identified as exhibiting problem behaviors, as well as the effects on nonidentified students in a ninth-grade high school biology class. An A/B/A/B single-case design was used to evaluate the effects of the…

  4. Exploring Mystery in Fifth Grade: A Journey of Discovery

    ERIC Educational Resources Information Center

    Sharp, Claudia; Martinez, Miriam

    2010-01-01

    An instructional framework that included the use of a touchstone text, literature circles, and independent reading and writing created a rich context for the study of mysteries in a fifth-grade classroom. Key points include a) the complexity of the touchstone text as a key factor in shaping the instructional goals in this genre study, and b) the…

  5. Quantum Mysteries The Quantum Theory of Motion. An Account

    E-print Network

    Goldstein, Sheldon

    and the claims of Born, Landau and Lifshitz, Heisenberg, and Bohr notwithstanding, in 1952 David Bohm, through reaction as follows: In 1952 I saw the impossible done. It was in papers by David Bohm. Bohm showedQuantum Mysteries The Quantum Theory of Motion. An Account of the de Broglie­Bohm Causal

  6. Prospects & Overviews The mystery of C. elegans aging

    E-print Network

    Gems, David

    assumption: that a fundamental cause of aging is accumulation of molecular damage. Could fat dysho- meostasisProspects & Overviews The mystery of C. elegans aging: An emerging role for fat Distant parallels between C. elegans aging and metabolic syndrome? Daniel Ackerman and David Gemsà New C. elegans studies

  7. The Sneaky Sneaker Spies and the Mysterious Black Ink

    ERIC Educational Resources Information Center

    Savran, Michelle

    2012-01-01

    In this article, the author describes the process of making "The Sneaky Sneaker Spies and the Mysterious Black Ink," a six-minute animation starring five art students who form a detective club. This animation is available online for art teachers to use in their own classrooms. After showing this video in class, art teachers could have students try…

  8. Mystery Motivator: A Tier 1 Classroom Behavioral Intervention

    ERIC Educational Resources Information Center

    Kowalewicz, Eva A.; Coffee, Gina

    2014-01-01

    This study is an examination of the effectiveness of the Mystery Motivator--an interdependent group contingency, variable-ratio, classwide intervention--as a tool for reducing disruptive classroom behavior in eight diverse general-education elementary school classrooms across seven different schools. The study was conducted using an ABAB, changing…

  9. Convergent and Divergent Thinking in the Context of Narrative Mysteries

    ERIC Educational Resources Information Center

    Wenzel, William G.; Gerrig, Richard J.

    2015-01-01

    This project demonstrates how narrative mysteries provide a context in which readers engage in creative cognition. Drawing on the concepts of convergent and divergent thinking, we wrote stories that had either convergent or divergent outcomes. For example, one story had a character give his girlfriend a ring (a convergent outcome), whereas the…

  10. Removing the Mystery of Entropy and Thermodynamics--Part I

    ERIC Educational Resources Information Center

    Left, Harvey S.

    2012-01-01

    Energy and entropy are centerpieces of physics. Energy is typically introduced in the study of classical mechanics. Although energy in this context can be challenging, its use in thermodynamics and its connection with entropy seem to take on a special air of mystery. In this five-part series, I pinpoint ways around key areas of difficulty to…

  11. Weird Stellar Pair Puzzles Scientists

    NASA Astrophysics Data System (ADS)

    2008-05-01

    Astronomers have discovered a speedy spinning pulsar in an elongated orbit around an apparent Sun-like star, a combination never seen before, and one that has them puzzled about how the strange system developed. Orbital Comparison Comparing Orbits of Pulsar and Its Companion to our Solar System. CREDIT: Bill Saxton, NRAO/AUI/NSF Click on image for full caption information and available graphics. "Our ideas about how the fastest-spinning pulsars are produced do not predict either the kind of orbit or the type of companion star this one has," said David Champion of the Australia Telescope National Facility. "We have to come up with some new scenarios to explain this weird pair," he added. Astronomers first detected the pulsar, called J1903+0327, as part of a long-term survey using the National Science Foundation's Arecibo radio telescope in Puerto Rico. They made the discovery in 2006 doing data analysis at McGill University, where Champion worked at the time. They followed up the discovery with detailed studies using the Arecibo telescope, the NSF's Robert C. Byrd Green Bank Telescope (GBT) in West Virginia, the Westerbork radio telescope in the Netherlands, and the Gemini North optical telescope in Hawaii. The pulsar, a city-sized superdense stellar corpse left over after a massive star exploded as a supernova, is spinning on its axis 465 times every second. Nearly 21,000 light-years from Earth, it is in a highly-elongated orbit that takes it around its companion star once every 95 days. An infrared image made with the Gemini North telescope in Hawaii shows a Sun-like star at the pulsar's position. If this is an orbital companion to the pulsar, it is unlike any companions of other rapidly rotating pulsars. The pulsar, a neutron star, also is unusually massive for its type. "This combination of properties is unprecedented. Not only does it require us to figure out how this system was produced, but the large mass may help us understand how matter behaves at extremely high densities," said Scott Ransom of the National Radio Astronomy Observatory. Pulsars are neutron stars whose strong magnetic fields channel lighthouse-like beams of light and radio waves that whirl around as the star spins. Typical pulsars spin a few times a second, but some, like PSR J1903+0327, are much faster, rotating hundreds of times a second. They are called millisecond pulsars. Astronomers think most millisecond pulsars are sped up by material falling onto them from a companion star. This requires the pulsar to be in a tight orbit around its companion that becomes more and more circular with time. The orbits of some millisecond pulsars are the most perfect circles in the Universe, so the elongated orbit of the new pulsar is a mystery. "What we have found is a millisecond pulsar that is in the wrong kind of orbit around what appears to be the wrong kind of star," Champion said. "Now we have to figure out how this strange system was produced." The scientists are considering three possibilities. The first, that the pulsar simply was born spinning quickly, seems unlikely to them. Another possibility, they say, is that the pulsar was formed in a tight group of stars known as a globular cluster, where it had a companion that spun it up. Later, a close encounter with another star in the cluster stripped it of its companion and flung it out of the cluster. For several reasons, including the fact that they don't see a nearby cluster from which it could have come, they don't like that explanation either. A third scenario says the pulsar may be part of a triple, not a double, star system. In this case, the pulsar's 95-day orbit is around a neutron star or white dwarf, not the Sun-like star seen in the infrared image. The Sun-like star would then be in a more-distant orbit around the pulsar and its close companion. "We've found about 50 pulsars in binary systems. We may now have found our first pulsar in a stellar triple system," Ransom said. The international research team is busy trying to get their

  12. Frontier Scientists use Modern Media

    NASA Astrophysics Data System (ADS)

    O'connell, E. A.

    2013-12-01

    Engaging Americans and the international community in the excitement and value of Alaskan Arctic discovery is the goal of Frontier Scientists. With a changing climate, resources of polar regions are being eyed by many nations. Frontier Scientists brings the stories of field scientists in the Far North to the public. With a website, an app, short videos, and social media channels; FS is a model for making connections between the public and field scientists. FS will demonstrate how academia, web content, online communities, evaluation and marketing are brought together in a 21st century multi-media platform, how scientists can maintain their integrity while engaging in outreach, and how new forms of media such as short videos can entertain as well as inspire.

  13. Probing scientists' beliefs: how open-minded are modern scientists?

    NASA Astrophysics Data System (ADS)

    Coll, Richard K.; Taylor, Neil

    2004-06-01

    Just how open-minded are modern scientists? In this paper we examine this question for the science faculty from New Zealand and UK universities. The Exeter questionnaire used by Preece and Baxter (2000) to examine superstitious beliefs of high school students and preservice science teachers was used as a basis for a series of in-depth interviews of scientists across a variety of disciplines. The interviews sought to understand the basis on which scientists form beliefs and how they judge evidence for various propositions, including those from the Exeter questionnaire and other contentious beliefs introduced during discourse. The scientists are dismissive of traditional superstitions like bad luck associated with black cats and inauspicious numbers such as 13, seeing such beliefs as socially grounded. There is a strong socio-cultural aspect to other beliefs and personal experiences, and strongly held personal beliefs are influential, resulting in the scientists keeping an open mind about contentious beliefs like alien life and the existence of ghosts. Testimony of others including media reports are deemed unreliable unless provided by credible witnesses such as 'educated people' or 'experts', or if they coincide with the scientists' personal beliefs. These scientists see a need for potential theoretical explanations for beliefs and are generally dismissive of empirical evidence without underlying explanations.

  14. Solving games Dependence of applicable solving procedures

    E-print Network

    Kuzmanov, Georgi

    Solving games Dependence of applicable solving procedures M.J.H. Heule1 and L.J.M. Rothkrantz2 1 and Computer Sciences Delft University of Technology marijn@heule.nl l.j.m.rothkrantz@tudelft.nl Abstract. We

  15. Schur's Inequality --And Its Mystery Issai Schur (1875-1941) was a mathematical magician who discovered many

    E-print Network

    Steele, J. Michael

    Schur's Inequality -- And Its Mystery Issai Schur (1875-1941) was a mathematical magician who it is the most mysterious of the completely elementary inequalities. We'll ponder its mystery after a quick look the observation that for the sum to be zero, both summands must be zero. Mystery -- To Minimize or Maximize? Part

  16. Brightness Variations of Sun-like Stars: The Mystery Deepens - Astronomers facing Socratic "ignorance"

    NASA Astrophysics Data System (ADS)

    2009-12-01

    An extensive study made with ESO's Very Large Telescope deepens a long-standing mystery in the study of stars similar to the Sun. Unusual year-long variations in the brightness of about one third of all Sun-like stars during the latter stages of their lives still remain unexplained. Over the past few decades, astronomers have offered many possible explanations, but the new, painstaking observations contradict them all and only deepen the mystery. The search for a suitable interpretation is on. "Astronomers are left in the dark, and for once, we do not enjoy it," says Christine Nicholls from Mount Stromlo Observatory, Australia, lead author of a paper reporting the study. "We have obtained the most comprehensive set of observations to date for this class of Sun-like stars, and they clearly show that all the possible explanations for their unusual behaviour just fail." The mystery investigated by the team dates back to the 1930s and affects about a third of Sun-like stars in our Milky Way and other galaxies. All stars with masses similar to our Sun become, towards the end of their lives, red, cool and extremely large, just before retiring as white dwarfs. Also known as red giants, these elderly stars exhibit very strong periodic variations in their luminosity over timescales up to a couple of years. "Such variations are thought to be caused by what we call 'stellar pulsations'," says Nicholls. "Roughly speaking, the giant star swells and shrinks, becoming brighter and dimmer in a regular pattern. However, one third of these stars show an unexplained additional periodic variation, on even longer timescales - up to five years." In order to find out the origin of this secondary feature, the astronomers monitored 58 stars in our galactic neighbour, the Large Magellanic Cloud, over two and a half years. They acquired spectra using the high resolution FLAMES/GIRAFFE spectrograph on ESO's Very Large Telescope and combined them with images from other telescopes [1], achieving an impressive collection of the properties of these variable stars. Outstanding sets of data like the one collected by Nicholls and her colleagues often offer guidance on how to solve a cosmic puzzle by narrowing down the plethora of possible explanations proposed by the theoreticians. In this case, however, the observations are incompatible with all the previously conceived models and re-open an issue that has been thoroughly debated. Thanks to this study, astronomers are now aware of their own "ignorance" - a genuine driver of the knowledge-seeking process, as the ancient Greek philosopher Socrates is said to have taught. "The newly gathered data show that pulsations are an extremely unlikely explanation for the additional variation," says team leader Peter Wood. "Another possible mechanism for producing luminosity variations in a star is to have the star itself move in a binary system. However, our observations are strongly incompatible with this hypothesis too." The team found from further analysis that whatever the cause of these unexplained variations is, it also causes the giant stars to eject mass either in clumps or as an expanding disc. "A Sherlock Holmes is needed to solve this very frustrating mystery," concludes Nicholls. Notes [1] Precise brightness measurements were made by the MACHO and OGLE collaborations, running on telescopes in Australia and Chile, respectively. The OGLE observations were made at the same time as the VLT observations. More information This research was presented in two papers: one appeared in the November issue of the Monthly Notices of the Royal Astronomical Society ("Long Secondary Periods in Variable Red Giants", by C. P. Nicholls et al.), and the other has just been published in the Astrophysical Journal ("Evidence for mass ejection associated with long secondary periods in red giants", by P. R. Wood and C. P. Nicholls). The team is composed of Christine P. Nicholls and Peter R. Wood (Research School of Astronomy and Ast

  17. Developing Nurse Scientist Course Login

    Cancer.gov

    Privacy  |   Disclaimer  |   Help  |   Logout      Developing Nurse Scientist Course User Login / Registration Returning Users Email: Password: Having trouble logging in? New User Registration If you are entering the course for the first time, you must

  18. Analytical Scientist The Epic Saga

    E-print Network

    Kounaves, Samuel P.

    , analytical science is truly ubiquitous. It is practiced in forensics, agriculture, pharmaceutics, commerce science" ­ covering more rigorously error analysis, precision, accuracy, statistics, samplingthe Analytical Scientist The Epic Saga Quantitative analysis and the essence of doing good science

  19. Do Scientists Really Reject God?

    ERIC Educational Resources Information Center

    Scott, Eugenie C.

    1998-01-01

    Suggests that the title of the recent Larson and Witham article in the journal Nature, "Leading Scientists Still Reject God", is premature and without reliable data upon which to base it. (Author/CCM)

  20. Scientists Check for Volcanic Activity

    USGS Multimedia Gallery

    Four scientists are busy reviewing seismic data, checking maps, and uploading activity updates in the USGS Volcano Hazards Program's Volcano Observatory operations room from the Menlo Park, California USGS campus....

  1. SCIENCE, SCIENTISTS, AND POLICY ADVOCACY

    EPA Science Inventory

    Effectively resolving the typical ecological policy issue requires providing an array of scientific information to decision-makers. In my experience, the ability of scientists (and scientific information) to inform constructively ecological policy deliberations has been diminishe...

  2. The Mystery of Ultra-High Energy Cosmic Rays

    E-print Network

    A. V. Olinto

    2000-03-01

    The origin of cosmic rays with energies higher than 10$^{20}$ eV remains a mystery. Accelerating particles up to these energies is a challenge even for the most energetic astrophysical objects known. While the isotropy in arrival directions argues for an extra-galactic origin, the photon-pion production off the cosmic background radiation limits the sources of such particles to systems less than 50 Mpc away from us. The combination of large gyroradii, efficient energy losses, and isotropic arrival directions defies most of the proposed astrophysical accelerators as well as the more exotic alternatives. I briefly review theoretical models for the acceleration and propagation of ultra-high-energy cosmic-rays and discuss the potential for future observatories to resolve this cosmic mystery.

  3. The Mysterious Universe - Exploring Our World with Particle Accelerators

    SciTech Connect

    Brau, James E

    2010-11-23

    The universe is dark and mysterious, more so than even Einstein imagined. While modern science has established deep understanding of ordinary matter, unidentified elements ("Dark Matter" and "Dark Energy") dominate the structure of the universe, its behavior and its destiny. What are these curious elements? We are now working on answers to these and other challenging questions posed by the universe with experiments at particle accelerators on Earth. Results of this research may revolutionize our view of nature as dramatically as the advances of Einstein and other quantum pioneers one hundred years ago. Professor Brau will explain for the general audience the mysteries, introduce facilities which explore them experimentally and discuss our current understanding of the underlying science. The presentation is at an introductory level, appropriate for anyone interested in physics and astronomy.

  4. Make a Mystery Circuit with a Bar Light Fixture

    NASA Astrophysics Data System (ADS)

    Lietz, Martha

    2007-04-01

    Teachers have been building mystery circuits or so-called "black box circuits" to use as a demonstration with their students for years. This paper presents an easy way to make simple mystery circuits using inexpensive light fixtures (see Fig. 1) available at almost any home improvement store.2 In a black box circuit, only the lightbulbs are visible and the wiring in these circuits is hidden from the students. The students are then presented with the challenge of deducing the nature of the electrical connections hidden by the black box. The students may remove one or more lightbulbs from the circuit to watch how the brightness of the other bulbs changes and, from this, deduce which bulbs are connected in series and which are connected in parallel.

  5. The Mysterious Universe - Exploring Our World with Particle Accelerators

    ScienceCinema

    Brau, James E [University of Oregon

    2014-06-25

    The universe is dark and mysterious, more so than even Einstein imagined. While modern science has established deep understanding of ordinary matter, unidentified elements ("Dark Matter" and "Dark Energy") dominate the structure of the universe, its behavior and its destiny. What are these curious elements? We are now working on answers to these and other challenging questions posed by the universe with experiments at particle accelerators on Earth. Results of this research may revolutionize our view of nature as dramatically as the advances of Einstein and other quantum pioneers one hundred years ago. Professor Brau will explain for the general audience the mysteries, introduce facilities which explore them experimentally and discuss our current understanding of the underlying science. The presentation is at an introductory level, appropriate for anyone interested in physics and astronomy.

  6. The mysterious practice of petrol sniffing in isolated indigenous groups.

    PubMed

    Cairney, Sheree; Dingwall, Kylie

    2010-09-01

    The practice of petrol sniffing is a unique and poorly understood phenomenon that is associated with substantial morbidity, mortality and social devastation in affected remote Indigenous communities. For these groups and for the wider community, much mystery has surrounded the practice and its effects. Here we introduce the epidemiology of petrol sniffing among Indigenous groups internationally, review its impact on the brain, behaviour and social functions and summarise related interventions. PMID:20854322

  7. The Unsolved Mysteries of Atmospheric Chemistry for High School Students and Teachers

    NASA Astrophysics Data System (ADS)

    Simonich, S. L.

    2011-12-01

    The grant "CAREER: New Molecular Markers of Asian Air Emissions - Anthropogenic Semi-Volatile Organic Compounds" (ATM-0239823) was funded by NSF from 2003-2008. The CAREER proposal described the integration of research and outreach education activities in the field of atmospheric chemistry, specifically atmospheric measurements and atmospheric transport. The primary objective of the research was to identify anthropogenic semi-volatile organic compounds (SOCs) that could be used as molecular markers for Asian air emissions and trans-Pacific atmospheric transport. The outreach education activity was integrated with the research by developing curriculum to introduce underrepresented minority high school students, and their teachers, to atmospheric chemistry and atmospheric measurements through Oregon State University's National Institute of Environmental Health Sciences funded Hydroville Curriculum Project (http://www.hydroville.org/iaq_resources). A curriculum was developed to allow students to assume the role of "Air Quality Scientist" and measure air temperature, air flow, relative humidity, CO, CO2, O3, and volatile organic compounds in out-door and in-door air. The students gained an understanding of atmospheric transport and compared measured concentrations to recommended guidelines. In addition, the outreach education activities included the development of the "Unsolved Mysteries of Human Health" website (http://www.unsolvedmysteries.oregonstate.edu/), including a specific module on the research conducted under the CAREER grant (http://www.unsolvedmysteries.oregonstate.edu /Gas-Chromatography-Mass-Spectrometry-Overview). The PI of the CAREER proposal, Dr. Staci Massey Simonich, is now a full professor at Oregon State University. To date, she has published over 50 peer-review journal articles, as well as mentored 9 undergraduate students, 20 graduate students, 3 post-doctoral scholars, and 3 international visiting scientists in her laboratory.

  8. Professional Ethics for Climate Scientists

    NASA Astrophysics Data System (ADS)

    Peacock, K.; Mann, M. E.

    2014-12-01

    Several authors have warned that climate scientists sometimes exhibit a tendency to "err on the side of least drama" in reporting the risks associated with fossil fuel emissions. Scientists are often reluctant to comment on the implications of their work for public policy, despite the fact that because of their expertise they may be among those best placed to make recommendations about such matters as mitigation and preparedness. Scientists often have little or no training in ethics or philosophy, and consequently they may feel that they lack clear guidelines for balancing the imperative to avoid error against the need to speak out when it may be ethically required to do so. This dilemma becomes acute in cases such as abrupt ice sheet collapse where it is easier to identify a risk than to assess its probability. We will argue that long-established codes of ethics in the learned professions such as medicine and engineering offer a model that can guide research scientists in cases like this, and we suggest that ethical training could be regularly incorporated into graduate curricula in fields such as climate science and geology. We recognize that there are disanalogies between professional and scientific ethics, the most important of which is that codes of ethics are typically written into the laws that govern licensed professions such as engineering. Presently, no one can legally compel a research scientist to be ethical, although legal precedent may evolve such that scientists are increasingly expected to communicate their knowledge of risks. We will show that the principles of professional ethics can be readily adapted to define an ethical code that could be voluntarily adopted by scientists who seek clearer guidelines in an era of rapid climate change.

  9. The Ozone Hole -- a Mystery Reborn?

    NASA Astrophysics Data System (ADS)

    von Hobe, M.; Grooß, J.; Müller, R.; Stroh, F.

    2007-12-01

    In 1985, Farman et al. discovered the near complete disappearance of the stratospheric ozone layer over Antarctica in spring. This 'Ozone Hole' took the atmospheric research community by surprise as it could not be explained by the known catalytic cycles removing ozone in the stratosphere. McElroy et al. (1986) and Molina and Molina (1987) seemed to have solved the enigma by proposing two new catalytic cycles -- the ClO-BrO-cycle and the ClO dimer cycle -- that could rapidly destroy ozone at cold temperatures and high zenith angles. Subsequent work describing the kinetics of these cycles as well as stratospheric observations of chlorine and bromine compounds supported their theory and led to atmospheric chemistry models reproducing observed ozone loss reasonably well. Today, more than 20 years after the discovery of the ozone hole and the ratification of the Montreal Protocol, a new laboratory study (Pope et al., 2007) -- suggesting much smaller absorption cross sections and hence photolysis rates of the ClO dimer -- seriously calls into question our understanding of how ozone is destroyed in the spring polar stratosphere. With the new cross sections, both the dimer cycle and the ClO-BrO-cycle run much slower, and observations of neither chlorine compounds nor ozone loss are reproduced by model simulations (von Hobe et al., 2007): the known catalytic cycles cannot cause an ozone hole. Obviously, this also calls into question our ability to predict future polar ozone depletion. In search for an explanation, we discuss possible shortcomings of the Pope et al. experiment that could lead to an underestimation of the dimer absorption and examine various new chemical processes for their likelihood to influence chlorine partitioning and cause significant ozone loss in the atmosphere and at the same time go undetected in laboratory based kinetic studies. A strategy is presented for designing the tests needed to unambiguously confirm or rule out proposed solutions to the dilemma. Farman, J.C. et al., Nature 315, 207, 1985. McElroy, M.B. et al., Nature 321, 759, 1986. Molina, L.T. and Molina, M.J., J. Phys. Chem. 91, 433, 1987. Pope, F.D.et al., J. Phys. Chem. A 111, 4322, 2007. von Hobe, M. et al., Atmos. Chem. Phys. 7, 3055, 2007.

  10. Materials Analysis: A Key to Unlocking the Mystery of the Columbia Tragedy

    NASA Technical Reports Server (NTRS)

    Mayeaux, Brian M.; Collins, Thomas E.; Piascik, Robert S.; Russel, Richard W.; Jerman, Gregory A.; Shah, Sandeep R.; McDanels, Steven J.

    2004-01-01

    Materials analyses of key forensic evidence helped unlock the mystery of the loss of space shuttle Columbia that disintegrated February 1, 2003 while returning from a 16-day research mission. Following an intensive four-month recovery effort by federal, state, and local emergency management and law officials, Columbia debris was collected, catalogued, and reassembled at the Kennedy Space Center. Engineers and scientists from the Materials and Processes (M&P) team formed by NASA supported Columbia reconstruction efforts, provided factual data through analysis, and conducted experiments to validate the root cause of the accident. Fracture surfaces and thermal effects of selected airframe debris were assessed, and process flows for both nondestructive and destructive sampling and evaluation of debris were developed. The team also assessed left hand (LH) airframe components that were believed to be associated with a structural breach of Columbia. Analytical data collected by the M&P team showed that a significant thermal event occurred at the left wing leading edge in the proximity of LH reinforced carbon carbon (RCC) panels 8 and 9. The analysis also showed exposure to temperatures in excess of 1,649 C, which would severely degrade the support structure, tiles, and RCC panel materials. The integrated failure analysis of wing leading edge debris and deposits strongly supported the hypothesis that a breach occurred at LH RCC panel 8.

  11. Do scientists trace hot topics?

    NASA Astrophysics Data System (ADS)

    Wei, Tian; Li, Menghui; Wu, Chensheng; Yan, Xiao-Yong; Fan, Ying; di, Zengru; Wu, Jinshan

    2013-07-01

    Do scientists follow hot topics in their scientific investigations? In this paper, by performing analysis to papers published in the American Physical Society (APS) Physical Review journals, it is found that papers are more likely to be attracted by hot fields, where the hotness of a field is measured by the number of papers belonging to the field. This indicates that scientists generally do follow hot topics. However, there are qualitative differences among scientists from various countries, among research works regarding different number of authors, different number of affiliations and different number of references. These observations could be valuable for policy makers when deciding research funding and also for individual researchers when searching for scientific projects.

  12. Do scientists trace hot topics?

    PubMed Central

    Wei, Tian; Li, Menghui; Wu, Chensheng; Yan, Xiao-Yong; Fan, Ying; Di, Zengru; Wu, Jinshan

    2013-01-01

    Do scientists follow hot topics in their scientific investigations? In this paper, by performing analysis to papers published in the American Physical Society (APS) Physical Review journals, it is found that papers are more likely to be attracted by hot fields, where the hotness of a field is measured by the number of papers belonging to the field. This indicates that scientists generally do follow hot topics. However, there are qualitative differences among scientists from various countries, among research works regarding different number of authors, different number of affiliations and different number of references. These observations could be valuable for policy makers when deciding research funding and also for individual researchers when searching for scientific projects. PMID:23856680

  13. Probing Scientists' Beliefs: How Open-Minded Are Modern Scientists?

    ERIC Educational Resources Information Center

    Coll, Richard; Taylor, Neil

    2004-01-01

    Just how open-minded are modern scientists? In this paper we examine this question for the science faculty from New Zealand and UK universities. The Exeter questionnaire used by Preece and Baxter (2000) to examine superstitious beliefs of high school students and preservice science teachers was used as a basis for a series of in-depth interviews…

  14. The Lord of Rings - the mysterious case of the stolen rings: a critical analysis

    NASA Astrophysics Data System (ADS)

    Sandrelli, S.

    The Lord of Rings - the mysterious case of the stolen rings: a critical analysis S. Sandrelli INAF - Osservatorio Astronomico di Brera, Milano, Italy (stefano.sandrelli@brera.inaf.it / Fax: 02 72001600 / Phone: +39 02 72320337) "The Lord of Rings - the mysterious case of the stolen rings" is a live astronomical role-playing game for kids aged 10 -13. Its goal is to introduce them to some of the main topics of the Solar System: a) the role of gravity; b) the distribution of mass & light; c) the effects of rotation; d) the distribution of water. The game was held both at the Perugia (2004) and the Genova Science Festival (2005), obtaining great success. Teams of about 6-8 members are introduced to Mr Schioppanelli, the astro-detective of the town (the name is a pun: it reminds Schiaparelli, the famous italian astronomer, and it is a slang expression meaning "ring-breaker"). Mr Schioppanelli has his office in an "gastronomical astronomical observatory", known as The Red Giant Pizzeria. Schioppanelli informs the kids that a mysterious Centaur succeded in stealing the rings of Saturn. The partecipants are appointed astro-detectives in-charge and asked to find the rings by browsing around the Solar System, which is scaled so as to fit the town historical centre or a pedestrian area, going from the Sun to Saturn or beyond, depending on the actual area at disposal. Great care must be taken allowing children playing only in a car-free area of the town. At the right scaled distances, the partecipants meet characters playing as the various planets. The kids can talk to them after solving a riddle, obtaining useful informations. A special characters play as a comet, timely going in and out of the inner solar system. The teams can also talk to some shepherd-moons of the rings. They easily discover that the rings were totally destroyed by the Centaur: a real disaster! They are also suggested to gather the necessary ingredients (gravity, light, rotation, inclination, dust and water, represented by simple objects like apples, spinning tops and so on) to re-build the rings. The kids can buy the ingredients from different planets: every planet has ingredients in quantities which are proportionate to the real physical properties of that celestial object. After collecting the ingredients, they must carry them to the "The Red Giant" and indicate their best recipe to Mr Schioppanelli. Depending on the recipe, rings can be too strict or too luminous or too fast rotating and so on. The winning group is the one which prepares the best recipe to cook the rings in the smallest amount of time. After presentig this specific (and mysterious) case, we analyse the advantage- disadvantage ratio of such an activity, beeing as funny as dispersive.

  15. NASA's Great Observatories May Unravel 400-Year Old Supernova Mystery

    NASA Astrophysics Data System (ADS)

    2004-10-01

    Four hundred years ago, sky watchers, including the famous astronomer Johannes Kepler, best known as the discoverer of the laws of planetary motion, were startled by the sudden appearance of a "new star" in the western sky, rivaling the brilliance of the nearby planets. Kepler's Supernova Remnant Multiple Images of Kepler's Supernova Remnant Modern astronomers, using NASA's three orbiting Great Observatories, are unraveling the mysteries of the expanding remains of Kepler's supernova, the last such object seen to explode in our Milky Way galaxy. When a new star appeared Oct. 9, 1604, observers could use only their eyes to study it. The telescope would not be invented for another four years. A team of modern astronomers has the combined abilities of NASA's Great Observatories, the Spitzer Space Telescope (SST), Hubble Space Telescope (HST), and Chandra X-ray Observatory, to analyze the remains in infrared radiation, visible light, and X-rays. Ravi Sankrit and William Blair of the Johns Hopkins University in Baltimore lead the team. The combined image unveils a bubble-shaped shroud of gas and dust, 14 light-years wide and expanding at 4 million mph. Observations from each telescope highlight distinct features of the supernova, a fast-moving shell of iron-rich material, surrounded by an expanding shock wave sweeping up interstellar gas and dust. Interview with Dr. Ravi Sankrit Interview with Dr. Ravi Sankrit "Multi-wavelength studies are absolutely essential for putting together a complete picture of how supernova remnants evolve," Sankrit said. Sankrit is an associate research scientist, Center for Astrophysical Sciences at Hopkins and lead for HST astronomer observations. "For instance, the infrared data are dominated by heated interstellar dust, while optical and X-ray observations sample different temperatures of gas," Blair added. Blair is a research professor, Physics and Astronomy Department at Hopkins and lead astronomer for SST observations. "A range of observations is needed to help us understand the complex relationship that exists among the various components," Blair said. The explosion of a star is a catastrophic event. The blast rips the star apart and unleashes a roughly spherical shock wave that expands outward at more than 22 million mph like an interstellar tsunami. The shock wave spreads out into surrounding space, sweeping up any tenuous interstellar gas and dust into an expanding shell. The stellar ejecta from the explosion initially trail behind the shock wave. It eventually catches up with the inner edge of the shell and is heated to X-ray temperatures. Kepler's Supernova Remnant Hubble Optical Image of Kepler's Supernova Remnant Visible-light images from Hubble's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps that form behind the shock wave. Sankrit and Blair compared their HST observations with those taken with ground-based telescopes to obtain a more accurate distance to the supernova remnant of about 13,000 light-years. Kepler's Supernova Remnant Spitzer Infrared Image of Kepler's Supernova Remnant The astronomers used the SST to probe for material that radiates in infrared light, which shows heated microscopic dust particles that have been swept up by the supernova shock wave. SST is sensitive enough to detect both the densest regions seen by HST and the entire expanding shock wave, a spherical cloud of material. Instruments on SST also reveal information about the chemical composition and physical environment of the expanding clouds of gas and dust ejected into space. This dust is similar to dust which was part of the cloud of dust and gas that formed the sun and planets in our solar system. Interview with Dr. William Blair Interview with Dr. William Blair The Chandra X-ray data show regions of very hot gas. The hottest gas, higher-energy X-rays, is located primarily in the regions directly behind the shock front. These regions also show up

  16. Scientist Using Terrestrial Lidar Equipment

    USGS Multimedia Gallery

    Chris Soulard using the Terrestrial Lidar to scan study area in the Grand Canyon-Parashant National Monument, AZ.  Note the bag of ice on the equipment.  High temperates can cause equipment to overheat, requiring scientists to be creative in protecting equipment....

  17. The Scientists in Schools Project

    ERIC Educational Resources Information Center

    Howitt, Christine; Rennie, Leonie; Heard, Marian; Yuncken, Liz

    2009-01-01

    Scientists in Schools is a project funded by the Australian Government Department of Education, Employment, and Workplace Relations and managed by the Commonwealth Scientific and Industrial Research Organisation, Education Section. This paper describes how the project is working to establish and maintain sustained and ongoing partnerships between…

  18. Science, Scientists, and Public Policy.

    ERIC Educational Resources Information Center

    Schooler, Dean, Jr.

    The politically relevant behavior of scientists in the formulation of public policy by the United States government from 1945-68 is studied. The following types of policy issues are treated: science, space, weather, weapons, deterrence and defense, health, fiscal and monetary, pollution, conservation, antitrust, transportation safety, trade and…

  19. Staff Scientist Health Behavior Branch

    E-print Network

    Rau, Don C.

    ) of the Eunice Kennedy Shriver National Institute of Child Health and Human Development (NICHD), National of children's health and the developmental origins of health across the lifespan. Staff Scientists of mental health, health disparities, and life course epidemiology, as evidenced by training

  20. SCIENCE, SCIENTISTS, AND POLICY ADVOCACY

    EPA Science Inventory

    To effectively resolve many current ecological policy issues, decision-makers require an array of scientific information. Sometimes scientific information is summarized for decision-makers by policy analysts or others, but often it comes directly from scientists to decision-maker...

  1. The five mysteries of the mind, and their consequences.

    PubMed

    Doty, R W

    1998-10-01

    While Western man has recognized for almost 2500 years that mind derives exclusively from brain, clothing this fact with explanatory detail still proves elusive. First, is consciousness per se, created by processes demonstrably limited to certain, but still unspecified, neuronal arrangements and activities. Then there is perception, its ineffable qualia, and the fact that it arises from neuronal activity widely dispersed in space and time within networks of vast complexity. Voluntary control is equally dispersed as to neuronal participation, and nescient as to origin. An often overlooked mystery is the unity of mind and behavior that prevails despite the potential for bihemispheric duplication of processes and experience. Finally, there is memory, which while credibly within grasp of understanding as a synaptic alteration maintained via activation of the nuclear genome, still wholly defies comprehension when viewed as commanded recall of myriad, randomly selectable details of the past, a largely effortless and 'instantaneous' flood of memories. For two centuries science has endeavored to demonstrate how these mysteries proceed from physics and chemistry, as indeed they do; but viewed from this direction alone, mind is but the babbling of a robot, chained ineluctably to crude causality. In a bold and revolutionary stroke, Roger Sperry has conceived a more credible paradigm, that the totality of neuronal action, as a richly intercommunicating system, gives rise to effects transcendent to the individual physicochemical elements that compose it. A major achievement of this position is that it is immediately consonant with everyday human experience and belief. While neither Sperry's vision. nor the reduction of the mysteries to a dance of ions can yet be proven, the vast advantage of Sperry's thesis is that it again imbues human thought and action with responsibility, and opens morality to the light of science, while the long wait for certainty unfolds. PMID:9845053

  2. On the mystery of the cosmic vacuum energy density

    E-print Network

    Norbert Straumann

    2000-09-25

    After a short history of the $\\Lambda$-term it is explained why the (effective) cosmological constant is expected to obtain contributions from short-distance physics, corresponding to an energy at least as large as the Fermi scale. The actual tiny value of the cosmological constant by particle physics standards represents, therefore, one of the deepest mysteries of present-day fundamental physics. Recent proposals of an approach to the cosmological constant problem which make use of (large) extra dimensions are briefly discussed. Cosmological models with a dynamical $\\Lambda$, which attempt to avoid the disturbing cosmic coincidence problem, are also reviewed.

  3. Fecundity of the Chinese mystery snail in a Nebraska reservoir

    USGS Publications Warehouse

    Stephen, Bruce J.; Allen, Craig R.; Chaine, Noelle M.; Fricke, Kent A.; Haak, Danielle M.; Hellman, Michelle L.; Kill, Robert A.; Nemec, Kristine T.; Pope, Kevin L.; Smeenk, Nicholas A.; Uden, Daniel R.; Unstad, Kody M.; VanderHam, Ashley E.; Wong, Alec

    2013-01-01

    The Chinese mystery snail (Bellamya chinensis) is a non-indigenous, invasive species in freshwater ecosystems of North America. We provide fecundity estimates for a population of these snails in a Nebraska reservoir. We dissected 70 snails, of which 29 were females. Nearly all female snails contained developing young, with an average of 25 young per female. Annual fecundity was estimated at between 27.2 and 33.3 young per female per year. Based on an estimated adult population and the calculated fecundity, the annual production for this reservoir was between 2.2 and 3.7 million young.

  4. Building problem solving environments with the arches framework

    SciTech Connect

    Debardeleben, Nathan; Sass, Ron; Stanzione, Jr., Daniel; Ligon, Ill, Walter

    2009-01-01

    The computational problems that scientists face are rapidly escalating in size and scope. Moreover, the computer systems used to solve these problems are becoming significantly more complex than the familiar, well-understood sequential model on their desktops. While it is possible to re-train scientists to use emerging high-performance computing (HPC) models, it is much more effective to provide them with a higher-level programming environment that has been specialized to their particular domain. By fostering interaction between HPC specialists and the domain scientists, problem-solving environments (PSEs) provide a collaborative environment. A PSE environment allows scientists to focus on expressing their computational problem while the PSE and associated tools support mapping that domain-specific problem to a high-performance computing system. This article describes Arches, an object-oriented framework for building domain-specific PSEs. The framework was designed to support a wide range of problem domains and to be extensible to support very different high-performance computing targets. To demonstrate this flexibility, two PSEs have been developed from the Arches framework to solve problem in two different domains and target very different computing platforms. The Coven PSE supports parallel applications that require large-scale parallelism found in cost-effective Beowulf clusters. In contrast, RCADE targets FPGA-based reconfigurable computing and was originally designed to aid NASA Earth scientists studying satellite instrument data.

  5. Chemical Reaction Problem Solving.

    ERIC Educational Resources Information Center

    Veal, William

    1999-01-01

    Discusses the role of chemical-equation problem solving in helping students predict reaction products. Methods for helping students learn this process must be taught to students and future teachers by using pedagogical skills within the content of chemistry. Emphasizes that solving chemical reactions should involve creative cognition where…

  6. Improving Educational Problem Solving.

    ERIC Educational Resources Information Center

    Martinelli, Kenneth J.; Muth, Rodney

    1989-01-01

    Any feasible problem-solving theory must become a master plan defining actions leading to desired results. This article presents an integrated, research-based planning model stressing a contingency approach to problem-solving that recognizes constraints such as time, accountability, learning time, uncertainty, conflicts, and complexity. Includes…

  7. Techniques of Problem Solving.

    ERIC Educational Resources Information Center

    Krantz, Steven G.

    The purpose of this book is to teach the basic principles of problem solving in both mathematical and non-mathematical problems. The major components of the book consist of learning to translate verbal discussion into analytical data, learning problem solving methods for attacking collections of analytical questions or data, and building a…

  8. Solving Recurrence Relations Motivation

    E-print Network

    Klappenecker, Andreas

    in computer science. For example, an interesting example of a heap data structure is a Fibonacci heap the heap property. Analyzing the amortized cost for Fibonacci heaps involves solving the Fibonacci = 5 (gn-5)2 is a nonlinear recurrence relation. #12;Remark Solving linear homogeneous recurrence

  9. Creating Alien Life Forms: Problem Solving in Biology.

    ERIC Educational Resources Information Center

    Grimnes, Karin A.

    1996-01-01

    Describes a project that helps students integrate biological concepts using both creativity and higher-order problem-solving skills. Involves students playing the roles of junior scientists aboard a starship in orbit around a class M planet and using a description of habitats, seasonal details, and a surface map of prominent geographic features to…

  10. Solving Information-Integration Problems Using Category Theory

    E-print Network

    Spivak, David

    to the market intelligence rm IDC, 40% of all enterprise IT budgets are dedicated to solving information problems that plague scientists, engineers, and commercial enterprises. Although category theory has revolu to leverage category theory for data management tasks. #12;Contents I Project Summary 2 Contents 4 II Project

  11. Ions at the Air-Water Interface: An End to a Hundred-Year-Old Mystery? Yan Levin,1

    E-print Network

    Levin, Yan

    Ions at the Air-Water Interface: An End to a Hundred-Year-Old Mystery? Yan Levin,1 Alexandre P. dos. The mystery appeared when Heydweiller [3] measured the surface tension of various electrolyte solutions

  12. Searching for Judy: How Small Mysteries Affect Narrative Processes and Memory

    ERIC Educational Resources Information Center

    Love, Jessica; McKoon, Gail; Gerrig, Richard J.

    2010-01-01

    Current theories of text processing say little about how authors' narrative choices, including the introduction of small mysteries, can affect readers' narrative experiences. Gerrig, Love, and McKoon (2009) provided evidence that 1 type of small mystery--a character introduced without information linking him or her to the story--affects readers'…

  13. Mystery Motivator as an Intervention To Promote Homework Completion and Accuracy.

    ERIC Educational Resources Information Center

    Madaus, Melissa M. R.; Kehle, Thomas J.; Madaus, Joseph; Bray, Melissa A.

    2003-01-01

    Investigates the effectiveness of the mystery motivator intervention as a means to remediate mathematics homework accuracy and completion problems in five fifth- grade students. Results indicated that the mystery motivator intervention was effective for all students on one or both outcome criteria. Additionally, both the teachers and students…

  14. Students Dig Deep in the Mystery Soil Lab: A Playful, Inquiry-Based Soil Laboratory Project

    ERIC Educational Resources Information Center

    Thiet, Rachel K.

    2014-01-01

    The Mystery Soil Lab, a playful, inquiry-based laboratory project, is designed to develop students' skills of inquiry, soil analysis, and synthesis of foundational concepts in soil science and soil ecology. Student groups are given the charge to explore and identify a "Mystery Soil" collected from a unique landscape within a 10-mile…

  15. Hands-On Science Mysteries for Grades 3-6: Standards-Based Inquiry Investigations

    ERIC Educational Resources Information Center

    Taris, James Robert; Taris, Louis James

    2006-01-01

    In "Hands-On Science Mysteries for Grades 3-6," the authors connect science to real-world situations by investigating actual mysteries and phenomena, such as the strange heads on Easter Island, the ghost ship "Mary Celeste," and the "Dancing Stones" of Death Valley. The labs are designed to encourage the development of science inquiry, in which…

  16. The feasibility of identifying mystery oil spills. Final report

    SciTech Connect

    Hunt, G.S.; Mayo, D.W.; Horton, D.B.

    1981-04-01

    Several off-the-shelf passive tagging techniques for identifying the origin of mystery oil spills were evaluated to determine the viability of enforcement provisions of Maine's Oil Conveyance Law. Duplicating the operating conditions experienced during every-day marine terminals activities, ship's samples of all crude oil shipments received during 15 day intervals in Portland (Maine) Harbor were collected. Selected samples from those collected during a test interval were subjected to artificial spills in 500 gallon tanks exposed to outdoor, sea-side ambient conditions experienced in Portland, Maine. Subsamples of each artificial spill were taken during the 15 day test interval to determine the effect of weathering. Attempts were made to match weathered unknowns to collections of known oil containing the 'mystery' oil. Several passive tagging techniques were used such as the comparison of high resolution and low resolution gas chromatography, vanadium-nickel ratios, sulfur nitrogen ratios, and infrared spectra. Successes, failures, and limitations of the passive tagging methods are discussed.

  17. Research Integrity of Individual Scientist

    NASA Astrophysics Data System (ADS)

    Haklak, Rockbill

    We are discussing about many aspects of research integrity of individual scientist, who faces the globalization of research ethics in the traditional culture and custom of Japan. Topics are scientific misconduct (fabrication, falsification, and plagiarism) in writing paper and presenting research results. Managements of research material, research record, grant money, authorship, and conflict of interest are also analyzed and discussed. Finally, we make 5 recommendations to improve research integrity in Japan.

  18. The Scientist as Sentinel (Invited)

    NASA Astrophysics Data System (ADS)

    Oreskes, N.

    2013-12-01

    Scientists have been warning the world for some time about the risks of anthropogenic interference in the climate system. But we struggle with how, exactly, to express that warning. The norms of scientific behavior enjoin us from the communication strategies normally associated with warnings. If a scientist sounds excited or emotional, for example, it is often assumed that he has lost his capac¬ity to assess data calmly and therefore his conclusions are suspect. If the scientist is a woman, the problem is that much worse. In a recently published article my colleagues and I have shown that scientists have systematically underestimated the threat of climate change (Brysse et al., 2012). We suggested that this occurs for norma¬tive reasons: The scientific values of rationality, dispassion, and self-restraint lead us to demand greater levels of evidence in support of surprising, dramatic, or alarming conclusions than in support of less alarming conclusions. We call this tendency 'err¬ing on the side of least drama.' However, the problem is not only that we err on the side of least drama in our assessment of evidence, it's also that we speak without drama, even when our conclusions are dramatic. We speak without the emotional cadence that people expect to hear when the speaker is worried. Even when we are worried, we don't sound as if we are. In short, we are trying to act as sentinels, but we lack the register with which to do so. Until we find those registers, or partner with colleagues who are able to speak in the cadences that communicating dangers requires, our warnings about climate change will likely continue to go substantially unheeded.

  19. Political action committee for scientists

    NASA Astrophysics Data System (ADS)

    Richman, Barbara T.

    Spurred by budget proposals that could severely reduce science funding (Eos, March 24, March 3, February 10), seven scientists currently serving as Congressional Science or State Department Fellows recently founded a political action committee (PAC) for scientists. The Science and Technology Political Action Committee (SCITEC-PAC) aims to make scientists more politically aware and better informed about potential legislative actions that affect research. It will also serve to ‘establish a political presence’ with respect to science, said Donald Stein, SCITEC-PAC's chairman.The organization is not a lobbying group, explained Stein, professor of neurology and psychology at Clark University and the University of Massachusetts Medical Center. ‘Lobbyists seek to influence officials by presenting information to them,’ he said, ‘while a PAC tries to influence the outcome of elections through campaign contributions of money, time, and effort in behalf of candidates that share similar goals and aspirations.’ In other words, the PAC will be a vehicle for promoting candidates for federal office who advocate strong support for scientific research and training. In addition, the PAC will develop and study science policy and budget issues and will attempt to stimulate government and private sector interest in these issues.

  20. The Scientist : The Science of Stress http://www.the-scientist.com/article/print/55118/ The Scientist

    E-print Network

    Storz, Gisela

    to be cutting-edge is not to look around and guess what might be the next big thing, but to stay with a problemThe Scientist : The Science of Stress http://www.the-scientist.com/article/print/55118 Varney | Varneyphoto.com 1 of 5 11/26/08 8:24 AM #12;The Scientist : The Science of Stress http://www.the-scientist.com/article/print

  1. My snowflake is so unique … Experiences of a reluctant Data Scientist

    NASA Astrophysics Data System (ADS)

    Ritchey, N. A.; Kearns, E. J.

    2014-12-01

    As with many data scientists, this wasn't my initial career objective. In fact it wasn't even seen as a viable option at that time. However I needed to manage data for my physical science projects and the teams I supported, so I reluctantly accepted this task as part of my "real" science job. Over the years, many challenges have been solved, that then allow us the ability to address more difficult issues. This presentation will address current data scientist challenges from a "real" scientist's perspective at a federal archive.

  2. Arguably the greatest mystery facing humanity today is the prospect that 75% of the universe is made up of

    E-print Network

    Weijgaert, Rien van de

    Arguably the greatest mystery facing humanity today is the prospect that 75% of the universe is dominated by mysterious dark energy was revealed by two paradigm- shifting studies of supernovae published@star.ucl.ac.uk Darkenergy:howthe paradigmshifted Dark energy is a mysterious substance belie

  3. 3/9/12 Astrophile: The rock that sprayed 'fairy dust' on moon -space -09 March 2012 -New Scientist 1/3www.newscientist.com/article/dn21574-astrophile-the-rock-that-sprayed-fairy-dust-on-moon.html?full

    E-print Network

    Weiss, Benjamin P.

    3/9/12 Astrophile: The rock that sprayed 'fairy dust' on moon - space - 09 March 2012 - New Scientist 1/3www.newscientist.com/article/dn21574-astrophile-the-rock-that-sprayed-fairy-dust-on-moon.html?full Magnetic mysteries of the moon (Image: Science/AAAS) A ophile is our weekl column on curious cosmic objects

  4. Cooperative Problem Solving

    E-print Network

    Minnesota, University of

    is a difficult, time consuming, and frustrating process -- like climbing a steep mountain. Many students try to run around this mountain by using their novice problem-solving strategies. Some of them give up (drop

  5. American Behavioral Scientist 2012 SAGE Publications

    E-print Network

    Wohlfarth, Barbara

    American Behavioral Scientist XX(X) 1­19 © 2012 SAGE Publications Reprints and permission: http.1177/0002764212466241American Behavioral ScientistShin © 2011 SAGE Publications Reprints and permission: http://www. sagepub

  6. The Time of Young Scientists Response

    E-print Network

    2010-01-01

    and innovation. Such activi- ties could be easily ful? lled by more experi- enced senior scientists.and innovation in interdisciplinary ? elds. The last aspect directly strengthens the core business of the young scientist,

  7. USGS Scientist Taking Measurements Along Bear Creek

    USGS Multimedia Gallery

    USGS Scientist Taking Measurements Along Bear Creek - Photo taken by Heidi Koontz, USGS Communications, Friday, Sept. 13. USGS scientist Ben Glass conducting current profiler measurements along Bear Creek near Bear Creek Lake in Morrison, Colo....

  8. Prospects of Solving Grand Challenge Problems

    E-print Network

    Rajan Gupta

    1995-01-17

    The recent woes of the supercomputer industry and changes in federal funding have caused some scientists to re-evaluate the means by which they hope to solve Grand Challenge problems. I evaluate the potential of Massively Parallel Processors (MPP) within this context and the state of today's MPP. I stress that for solving large-scale problems MPP are crucial and that it is essential to seek a balance between CPU performance, memory access time, inter-node communications, and I/O. To achieve this it is important to preserve certain characteristics of the hardware while selecting the hottest processor to design the machine around. I emphasize that for long term stability and growth of parallel computing priority should be given to standardizing software so that the same code can run on different platforms and on machines ranging from clusters of workstations to MPP.

  9. MATHEMATICAL ROUTINES FOR ENGINEERS AND SCIENTISTS

    NASA Technical Reports Server (NTRS)

    Kantak, A. V.

    1994-01-01

    The purpose of this package is to provide the scientific and engineering community with a library of programs useful for performing routine mathematical manipulations. This collection of programs will enable scientists to concentrate on their work without having to write their own routines for solving common problems, thus saving considerable amounts of time. This package contains sixteen subroutines. Each is separately documented with descriptions of the invoking subroutine call, its required parameters, and a sample test program. The functions available include: maxima, minima, and sort of vectors; factorials; random number generator (uniform or Gaussian distribution); complimentary error function; fast Fourier Transformation; Simpson's Rule integration; matrix determinate and inversion; Bessel function (J Bessel function for any order, and modified Bessel function for zero order); roots of a polynomial; roots of non-linear equation; and the solution of first order ordinary differential equations using Hamming's predictor-corrector method. There is also a subroutine for using a dot matrix printer to plot a given set of y values for a uniformly increasing x value. This package is written in FORTRAN 77 (Super Soft Small System FORTRAN compiler) for batch execution and has been implemented on the IBM PC computer series under MS-DOS with a central memory requirement of approximately 28K of 8 bit bytes for all subroutines. This program was developed in 1986.

  10. Swedish scientists take acid-rain research to developing nations

    SciTech Connect

    Abate, T.

    1995-12-01

    In the realm of acid-rain research, Sweden looms large on the world stage. It is the country where scientists first proved more than 30 years ago that airborne chemicals could and did cross international boundaries to acidify lakes and forests far from where the pollution was generated. Now, Swedish scientists are leading an international effort to map acid-rain patterns in the developing countries of Asia, where new industrial activity seems to be recreating problems that European and North American policy makers have already taken steps to solve. Topics covered in this article include acid rain on the rise in Asia; visualizing and validating the data; funding as the key to steady research.

  11. INTERNATIONAL VISITING SCIENTISTS AT LEIBNIZ UNIVERSITT HANNOVER

    E-print Network

    Nejdl, Wolfgang

    INTERNATIONAL VISITING SCIENTISTS AT LEIBNIZ UNIVERSITÄT HANNOVER International Visiting Scientists in research & teaching NO PhD-Students, NO regular students title, surname, name sex: male female institut scientist at your institute / department. With your help we are able · to provide your guest

  12. INTERNATIONAL VISITING SCIENTISTS AT LEIBNIZ UNIVERSITT HANNOVER

    E-print Network

    Nejdl, Wolfgang

    INTERNATIONAL VISITING SCIENTISTS AT LEIBNIZ UNIVERSITÄT HANNOVER International Visiting Scientists in research & teaching NO PhD-Students, NO regular students title, surname, name sex: male female institut visiting scientist at your institute / department. With your help we are able · to provide your guest

  13. Connect the Book: The Tarantula Scientist

    ERIC Educational Resources Information Center

    Brodie, Carolyn S.

    2005-01-01

    This column describes the book, "The Tarantula Scientist," that features the work of arachnologist Sam Marshall, a scientist who studies spiders and their eight-legged relatives. Marshall is one of only four or five scientists who specializes in the study of tarantulas. The informative text and outstanding photographs follow Sam as he takes a…

  14. SURGICAL SCIENTIST PROGRAM Department of Surgery

    E-print Network

    Shoubridge, Eric

    SURGICAL SCIENTIST PROGRAM Department of Surgery McGill University The purpose of the Surgical Scientist Program of the Department of Surgery is to develop surgical scientists who will be the future leaders in academic surgery both at McGill and in other university Departments of Surgery. Application

  15. Developing the Talents of Teacher/Scientists

    ERIC Educational Resources Information Center

    Robinson, George

    2004-01-01

    Going on an expedition enables teachers to become better scientists and researchers and, thus, better classroom instructors. Teachers have the opportunities to go on exotic field trips around the world as amateur research assistants, do hands on research in their own backyards, or vicariously experience another scientist?s work via the Internet. A…

  16. Helping Young People Engage with Scientists

    ERIC Educational Resources Information Center

    Leggett, Maggie; Sykes, Kathy

    2014-01-01

    There can be multiple benefits of scientists engaging with young people, including motivation and inspiration for all involved. But there are risks, particularly if scientists do not consider the interests and needs of young people or listen to what they have to say. We argue that "dialogue" between scientists, young people and teachers…

  17. Some Psychological Knowledge for Scientists' Use

    NASA Astrophysics Data System (ADS)

    Miclea, Mircea

    2008-01-01

    Relying on empirical evidences our paper presents the most salient personality traits, developmental factors and cognitive characteristics of the scientists. We claim that a sound exploration of scientists' mind and patterns of behavior could improve public support for science and enhance scientists' mutual understanding.

  18. Still Persistent Global Problem of Scientists' Image

    ERIC Educational Resources Information Center

    Türkmen, Hakan

    2015-01-01

    Pre-service teachers' views of science and scientists have been widely studied. The purpose of this study is to identify whether there is problem of image of scientists and determine where they receive about scientist image. Three hundred thirty five (105 from Turkey, 162 from Europe, 68 from US) elementary pre-service teachers participated in…

  19. Scientists Talking to Students through Videos

    ERIC Educational Resources Information Center

    Chen, Junjun; Cowie, Bronwen

    2014-01-01

    The benefits of connecting school students with scientists are well documented. This paper reports how New Zealand teachers brought scientists into the classrooms through the use of videos of New Zealand scientists talking about themselves and their research. Two researchers observed lessons in 9 different classrooms in which 23 educational videos…

  20. Give Young Scientists a Break

    SciTech Connect

    Wiley, H. S.

    2009-11-01

    There has been much concern about the impact of tight funding on the careers of young scientists. When only a small percentage of grants are approved, even the smallest problem or error with an application can push it out of the funding range. Unfortunately, the relative lack of grant writing skills by new investigators often has this effect. To avoid a situation where only experienced investigators with polished writing skills are funded, the National Institutes of Health has instituted a more generous ranking scale for new investigators. Not surprisingly, some senior investigators have protested, calling it reverse discrimination. I say that their anger is misplaced. New investigators do deserve a break.

  1. Natural gas hydrates and the mystery of the Bermuda Triangle

    SciTech Connect

    Gruy, H.J.

    1998-03-01

    Natural gas hydrates occur on the ocean floor in such great volumes that they contain twice as much carbon as all known coal, oil and conventional natural gas deposits. Releases of this gas caused by sediment slides and other natural causes have resulted in huge slugs of gas saturated water with density too low to float a ship, and enough localized atmospheric contamination to choke air aspirated aircraft engines. The unexplained disappearances of ships and aircraft along with their crews and passengers in the Bermuda Triangle may be tied to the natural venting of gas hydrates. The paper describes what gas hydrates are, their formation and release, and their possible link to the mystery of the Bermuda Triangle.

  2. Resolving the mystery of transport within internal transport barriers

    SciTech Connect

    Staebler, G. M.; Belli, E. A.; Candy, J.; Waltz, R. E.; Greenfield, C. M.; Lao, L. L.; Smith, S. P.; Kinsey, J. E.; Grierson, B. A.; Chrystal, C.

    2014-05-15

    The Trapped Gyro-Landau Fluid (TGLF) quasi-linear model [G. M. Staebler, et al., Phys. Plasmas 12, 102508 (2005)], which is calibrated to nonlinear gyrokinetic turbulence simulations, is now able to predict the electron density, electron and ion temperatures, and ion toroidal rotation simultaneously for internal transport barrier (ITB) discharges. This is a strong validation of gyrokinetic theory of ITBs, requiring multiple instabilities responsible for transport in different channels at different scales. The mystery of transport inside the ITB is that momentum and particle transport is far above the predicted neoclassical levels in apparent contradiction with the expectation from the theory of suppression of turbulence by E×B velocity shear. The success of TGLF in predicting ITB transport is due to the inclusion of ion gyro-radius scale modes that become dominant at high E×B velocity shear and to improvements to TGLF that allow momentum transport from gyrokinetic turbulence to be faithfully modeled.

  3. Homocystinuria, a possible solution of the Akhenaten's mystery.

    PubMed

    Cavka, Mislav; Kelava, Tomislav; Cavka, Vlatka; Busi?, Zeljko; Oluji?, Boris; Brkljaci?, Boris

    2010-03-01

    Pharaoh Amenophis IV (Amenhotep IV), also known as Akhenaten, is the most mysterious person in Egyptian history and he still remains the object of academic argues. This revolutionary king introduced a new concept in Egyptian religion and arts. It is still unexplained if images of him and his family were just an artistic outbreak from old Egyptian canon or an excellent paleopathological study. Several pathologic conditions were proposed to explain his appearance but neither is completely acceptable. We propose a different disease that he could have suffered of homocystinuria--lack of cysthationine-synthase. Our conclusion is that in comparison with up to date most convincing theory, that he was suffering of Marfan syndrome, our theory equally well explains his physical appearance but is better in explaining affecting and unaffecting of his relatives. This is the only theory about Akhenaten's disease that could be checked in the near future. PMID:20402329

  4. K2P potassium channels, mysterious and paradoxically exciting.

    PubMed

    Goldstein, Steve A N

    2011-08-01

    New evidence reveals that the common electrolyte disorder hypokalemia can induce K2P1 channels that are normally selective for K+ to break the rules and conduct Na+. This defiant behavior leads to paradoxical depolarization of many cells in the heart, increasing the risk for lethal arrhythmia. The new research resolves a mystery uncovered 50 years ago and bestows an array of new riddles. Here, I discuss how K2P1 might achieve this alchemy--through stable residence of the K+ selectivity filter in a Na+-conductive state between its open and C-inactive configurations--and predict that other K+ channels and environmental stimuli will be discovered to produce the same excitatory misconduct. PMID:21868351

  5. The Carbon Tetrachloride (CCl4) Budget: Mystery or Not

    NASA Technical Reports Server (NTRS)

    Liang, Qing; Newman, Paul A.; Daniel, John S.; Reimann, Stefan; Hall, Bradley; Dutton, Geoff; Kuijpers, Lambert J. M.

    2014-01-01

    Carbon tetrachloride (CCl4) is a major anthropogenic ozone-depleting substance and greenhouse gas and has been regulated under the Montreal Protocol. However, atmospheric observations show a very slow decline in CCl4 concentrations, inconsistent with the nearly zero emissions estimate based on the UNEP reported production and feedstock usage in recent years. It is now apparent that there are either unidentified industrial leakages, an unknown production source of CCl4, or large legacy emissions from CCl4 contaminated sites. In this paper we use a global chemistry climate model to assess the budget mystery of atmospheric CCl4. We explore various factors that affect the global trend and the gradient between the Northern and Southern hemispheres or interhemispheric gradient (IHG): emissions, emission hemispheric partitioning, and lifetime variations. We find a present-day emission of 30-50 Gg per yr and a total lifetime 25 - 36 years are necessary to reconcile both the observed CCl4 global trend and IHG.

  6. Turkish Primary Students' Perceptions about Scientist and What Factors Affecting the Image of the Scientists

    ERIC Educational Resources Information Center

    Turkmen, Hakan

    2008-01-01

    Students' views of science and scientists have been widely studied. The purpose of this study is to analyze image of scientist from drawn picture of scientists using The Draw-a-Scientist Test (DAST) by 5th grade students and to analyze where this image comes from students minds in changing Turkish educational perspective. Two hundred eighty seven…

  7. Enigma of Runaway Stars Solved

    NASA Astrophysics Data System (ADS)

    1997-01-01

    Supernova Propels Companion Star through Interstellar Space The following success story is a classical illustration of scientific progress through concerted interplay of observation and theory. It concerns a 35-year old mystery which has now been solved by means of exciting observations of a strange double star. An added touch is the successive involvement of astronomers connected to the European Southern Observatory. For many years, astronomers have been puzzled by the fact that, among the thousands of very young, hot and heavy stars which have been observed in the Milky Way, there are some that move with exceptionally high velocities. In some cases, motions well above 100 km/sec, or ten times more than normal for such stars, have been measured. How is this possible? Which mechanism is responsible for the large amounts of energy needed to move such heavy bodies at such high speeds? Could it be that these stars are accelerated during the powerful explosion of a companion star as a supernova? Such a scenario was proposed in 1961 by Adriaan Blaauw [1], but until now, observational proof has been lacking. Now, however, strong supporting evidence for this mechanism has become available from observations obtained at the ESO La Silla observatory. The mysterious runaway stars OB-runaway stars [2] are heavy stars that travel through interstellar space with an anomalously high velocity. They have been known for several decades, but it has always been a problem to explain their high velocities. Although most OB-runaway stars are located at distances of several thousands of lightyears, their high velocity results in a measurable change in position on sky photos taken several years apart. The velocity component in the direction of the Earth can be measured very accurately from a spectrogram. From a combination of such observations, it is possible to measure the space velocity of OB-runaways. Bow shocks reveal runaway stars It has also been found that some OB-runaways display bow shocks of compressed matter, which look very much like the bow wave around a boat crossing the ocean. They are of the same physical nature as a bow shock created by a jet-fighter in the air. The explanation is similar: when an OB-runaway star plows through the interstellar medium (a very thin mixture of gas and dust particles) with supersonic velocity [3], interstellar matter is swept up in a bow shock. Stars of low velocity do not create bow shocks. Thus, the detection of a bow shock around a particular OB star indicates that it must have a supersonic velocity, thereby securely identifying it as a runaway star, even if its velocity has not been measured directly. Runaway stars come from stellar groups When a star's direction of motion in space is known, it is possible to reconstruct its previous path and, even more interestingly, to find the place where the star originally came from. It turns out that the paths of many OB-runaways can be traced back to socalled OB-associations , that is groups of 10 to 100 OB-type stars which are located in the spiral arms of our galaxy. About fifty OB-associations are known in the Milky Way. In fact, the majority of all known OB stars are members of an OB-association. Therefore, it is not very surprising that OB-runaway stars should also originate from OB-associations. This is also how they got their name: at some moment, they apparently left the association in which they were formed. The ejection mechanism But why were the OB-runaway stars kicked out of the OB-association and how did they achieve such high speeds? One possibility is that some OB stars in an OB-association are ejected due to strong gravitational effects at the time of close encounters between the members of the group. Complicated computer simulations show that this is in principle possible. Nevertheless, since many years, most astronomers think that a more likely scenario is that of violent supernova explosions, first proposed in 1961 by Adriaan Blaauw. Stellar evolution theory predicts that all OB stars will end their life in a supernova explosion. The he

  8. Solving Symbolic Equations with PRESS 

    E-print Network

    Sterling, L.; Bundy, Alan; Byrd, L.; O'Keefe, R.; Silver, B.

    1982-01-01

    We outline a program, PRESS (PRolog Equation Solving System) for solving symbolic, transcendental, non-differential equations. The methods used for solving equations are described, together with the service facilities. The ...

  9. Electric Current Solves Mazes

    ERIC Educational Resources Information Center

    Ayrinhac, Simon

    2014-01-01

    We present in this work a demonstration of the maze-solving problem with electricity. Electric current flowing in a maze as a printed circuit produces Joule heating and the right way is instantaneously revealed with infrared thermal imaging. The basic properties of electric current can be discussed in this context, with this challenging question:…

  10. [Problem Solving Activities.

    ERIC Educational Resources Information Center

    Wisconsin Univ. - Stout, Menomonie. Center for Vocational, Technical and Adult Education.

    The teacher directed problem solving activities package contains 17 units: Future Community Design, Let's Build an Elevator, Let's Construct a Catapult, Let's Design a Recreational Game, Let's Make a Hand Fishing Reel, Let's Make a Wall Hanging, Let's Make a Yo-Yo, Marooned in the Past, Metrication, Mousetrap Vehicles, The Multi System…

  11. Problem Solving in Electricity.

    ERIC Educational Resources Information Center

    Caillot, Michel; Chalouhi, Elias

    Two studies were conducted to describe how students perform direct current (D-C) circuit problems. It was hypothesized that problem solving in the electricity domain depends largely on good visual processing of the circuit diagram and that this processing depends on the ability to recognize when two or more electrical components are in series or…

  12. On Solving Linear Recurrences

    ERIC Educational Resources Information Center

    Dobbs, David E.

    2013-01-01

    A direct method is given for solving first-order linear recurrences with constant coefficients. The limiting value of that solution is studied as "n to infinity." This classroom note could serve as enrichment material for the typical introductory course on discrete mathematics that follows a calculus course.

  13. Universal Design Problem Solving

    ERIC Educational Resources Information Center

    Sterling, Mary C.

    2004-01-01

    Universal design is made up of four elements: accessibility, adaptability, aesthetics, and affordability. This article addresses the concept of universal design problem solving through experiential learning for an interior design studio course in postsecondary education. Students' experiences with clients over age 55 promoted an understanding of…

  14. Problem Solving by Design

    ERIC Educational Resources Information Center

    Capobianco, Brenda M.; Tyrie, Nancy

    2009-01-01

    In a unique school-university partnership, methods students collaborated with fifth graders to use the engineering design process to build their problem-solving skills. By placing the problem in the context of a client having particular needs, the problem took on a real-world appeal that students found intriguing and inviting. In this article, the…

  15. Solving Problems in Genetics

    ERIC Educational Resources Information Center

    Aznar, Mercedes Martinez; Orcajo, Teresa Ibanez

    2005-01-01

    A teaching unit on genetics and human inheritance using problem-solving methodology was undertaken with fourth-level Spanish Secondary Education students (15 year olds). The goal was to study certain aspects of the students' learning process (concepts, procedures and attitude) when using this methodology in the school environment. The change…

  16. Solving problems with technology

    E-print Network

    California at Santa Barbara, University of

    Solving problems with technology: Computer Science! by: Saiph and Veronika #12;What is Computer in UNAM #12;Saiph's research I create computer models, conduct interviews and surveys to understand how people use technology. I use the knowledge to create interactive interfaces that enrich the online

  17. Data Scientist Training for Librarians

    NASA Astrophysics Data System (ADS)

    Erdmann, C.

    2015-04-01

    Recent studies suggest that there will be a shortfall in the near future of skilled talent available to help take advantage of big data in organizations. Meanwhile, government initiatives have encouraged the research community to share their data more openly, raising new challenges for researchers. Librarians can assist in this new data-driven environment. Data Scientist Training for Librarians (or Data Savvy Librarians) is an experimental course being offered by the Harvard Library to train librarians to respond to the growing data needs of their communities. In the course, librarians familiarize themselves with the research data lifecycle, working hands-on with the latest tools for extracting, wrangling, storing, analyzing, and visualizing data. By experiencing the research data lifecycle themselves, and becoming data savvy and embracing the data science culture, librarians can begin to imagine how their services might be transformed.

  18. Professional Societies of Minority Scientists

    NASA Astrophysics Data System (ADS)

    Stassun, K. G.

    2003-12-01

    This session will highlight professional organizations that serve minorities in physics, astronomy, and space science, such as the National Society of Black Physicists (NSBP), the National Society of Hispanic Physicists (NSHP), and the Society for the Advancement of Chicanos and Native Americans in Science (SACNAS). These organizations represent and serve minority colleagues and students at both majority and minority-serving institutions. A panel of representatives from these organizations---as well as AAS members who are presently working with them---will discuss these groups' activities and will offer suggestions for how AAS members can better connect with their constituencies. The panel will also include representatives from APS and NASA who will discuss programmatic efforts being developed in partnership with these groups to better engage minority scientists in the research enterprise. Specific funding opportunities will also be presented, including support for minority outreach, undergraduate scholarships, and research grants.

  19. Involving Scientists in Education and Public Outreach

    NASA Astrophysics Data System (ADS)

    Peticolas, L. M.

    2009-12-01

    There are many potential barriers for scientists' involvement in education and public outreach. At the Center for Science Education at the Space Sciences Laboratory at the University of California at Berkeley, we regularly work with scientists at a variety of levels in education and outreach. We have provided links to scientists and other education programs, such as Project ASTRO. We have brought scientists in to help in reviewing products for a variety of our programs, such as K-12 school curriculum. We have worked with scientists to present at different types of education and outreach venues, from teacher workshops to community events. We have worked collaboratively with scientists on education and outreach programs, developing programs as a team, such as the THEMIS high school magnetometer program. We have featured scientists in podcasts for the International Year of Astronomy. And we have supported scientists in writing their own education and public outreach proposals. I will present several of these ways in which we have engaged scientists in our programs and have supported scientists in their own efforts in education and public outreach. And will present responses I have received about this support, the challenges we have encountered, and the successes as well.

  20. Universities Earth System Scientists Program

    NASA Technical Reports Server (NTRS)

    Estes, John E.

    1995-01-01

    This document constitutes the final technical report for the National Aeronautics and Space Administration (NASA) Grant NAGW-3172. This grant was instituted to provide for the conduct of research under the Universities Space Research Association's (USRA's) Universities Earth System Scientist Program (UESSP) for the Office of Mission to Planet Earth (OMTPE) at NASA Headquarters. USRA was tasked with the following requirements in support of the Universities Earth System Scientists Programs: (1) Bring to OMTPE fundamental scientific and technical expertise not currently resident at NASA Headquarters covering the broad spectrum of Earth science disciplines; (2) Conduct basic research in order to help establish the state of the science and technological readiness, related to NASA issues and requirements, for the following, near-term, scientific uncertainties, and data/information needs in the areas of global climate change, clouds and radiative balance, sources and sinks of greenhouse gases and the processes that control them, solid earth, oceans, polar ice sheets, land-surface hydrology, ecological dynamics, biological diversity, and sustainable development; (3) Evaluate the scientific state-of-the-field in key selected areas and to assist in the definition of new research thrusts for missions, including those that would incorporate the long-term strategy of the U.S. Global Change Research Program (USGCRP). This will, in part, be accomplished by study and evaluation of the basic science needs of the community as they are used to drive the development and maintenance of a global-scale observing system, the focused research studies, and the implementation of an integrated program of modeling, prediction, and assessment; and (4) Produce specific recommendations and alternative strategies for OMTPE that can serve as a basis for interagency and national and international policy on issues related to Earth sciences.

  1. Using Scientists and Real-World Scenarios in Professional Development for Middle School Science Teachers

    ERIC Educational Resources Information Center

    Morrison, Judith A.; Estes, Jeffrey C.

    2007-01-01

    Middle school science teachers were involved in a problem-solving experience presented and guided by research scientists. Data on the teachers' perspectives about this professional development and any impact it may have had on their teaching practices were collected through interviews, surveys, and classroom observations. The findings show that…

  2. How Long Has Grandpa Been Dead and Other Forensic Mysteries

    SciTech Connect

    Baden, Michael

    2006-05-17

    Was the baby born alive? Can a child's brain really be shaken hard enough to cause death? Was the body dead before going into the water? Does a lightening strike cause any unique changes in the body? Why are hair and maggots becoming so important to the forensic scientist? Let's talk.

  3. How Long Has Grandpa Been Dead and Other Forensic Mysteries

    ScienceCinema

    Baden, Michael [MD, New York Police, New York, New York, United States

    2009-09-01

    Was the baby born alive? Can a child's brain really be shaken hard enough to cause death? Was the body dead before going into the water? Does a lightening strike cause any unique changes in the body? Why are hair and maggots becoming so important to the forensic scientist? Let's talk.

  4. Scientists Toast the Discovery of Vinyl Alcohol in Interstellar Space

    NASA Astrophysics Data System (ADS)

    2001-10-01

    Astronomers using the National Science Foundation's 12 Meter Telescope at Kitt Peak, AZ, have discovered the complex organic molecule vinyl alcohol in an interstellar cloud of dust and gas near the center of the Milky Way Galaxy. The discovery of this long-sought compound could reveal tantalizing clues to the mysterious origin of complex organic molecules in space. Vinyl Alcohol and its fellow isomers "The discovery of vinyl alcohol is significant," said Barry Turner, a scientist at the National Radio Astronomy Observatory (NRAO) in Charlottesville, Va., "because it gives us an important tool for understanding the formation of complex organic compounds in interstellar space. It may also help us better understand how life might arise elsewhere in the Cosmos." Vinyl alcohol is an important intermediary in many organic chemistry reactions on Earth, and the last of the three stable members of the C2H4O group of isomers (molecules with the same atoms, but in different arrangements) to be discovered in interstellar space. Turner and his colleague A. J. Apponi of the University of Arizona's Steward Observatory in Tucson detected the vinyl alcohol in Sagittarius B -- a massive molecular cloud located some 26,000 light-years from Earth near the center of our Galaxy. The astronomers were able to detect the specific radio signature of vinyl alcohol during the observational period of May and June of 2001. Their results have been accepted for publication in the Astrophysical Journal Letters. Of the approximately 125 molecules detected in interstellar space, scientists believe that most are formed by gas-phase chemistry, in which smaller molecules (and occasionally atoms) manage to "lock horns" when they collide in space. This process, though efficient at creating simple molecules, cannot explain how vinyl alcohol and other complex chemicals are formed in detectable amounts. For many years now, scientists have been searching for the right mechanism to explain how the building blocks for vinyl alcohol and other chemicals are able to form the necessary chemical bonds to make larger molecules - those containing as many as six or more atoms. "It has been an ongoing quest to understand exactly how these more complex molecules form and become distributed throughout the interstellar medium," said Turner. Since the 1970s, scientists have speculated that molecules could form on the microscopic dust grains in interstellar clouds. These dust grains are thought to trap the fast-moving molecules. The surface of these grains would then act as a catalyst, similar to a car's catalytic converter, and enable the chemical reactions that form vinyl alcohol and the other complex molecules. The problem with this theory, however, is that the newly formed molecules would remain trapped on the dust grains at the low temperature characteristic of most of interstellar space, and the energy necessary to "knock them off" would also be strong enough to break the chemical bonds that formed them. "This last process has not been well understood," explained Turner. "The current theory explains well how molecules like vinyl alcohol could form, but it doesn't address how these new molecules are liberated from the grains where they are born." To better understand how this might be accomplished, the scientists considered the volatile and highly energetic region of space where these molecules were detected. Turner and others speculate that since this cloud lies near an area of young, energetic star formation, the energy from these stars could evaporate the icy surface layers of the grains. This would liberate the molecules from their chilly nurseries, depositing them into interstellar space where they can be detected by sensitive radio antennas on Earth. Astronomers are able to detect the faint radio signals that these molecules emit as they jump between quantum energy states in the act of rotating or vibrating. Turner cautions, however, that even though this discovery has shed new light on how certain h

  5. Genetic Mystery of Behcet's Disease Unfolds Along the Ancient Silk Road

    MedlinePLUS

    ... mystery of Behcet’s disease unfolds along the ancient Silk Road NIH researchers identify new gene variants associated with ... found predominantly in people with ancestors along the Silk Road. For nearly 2,000 years, traders used this ...

  6. How Things Work. Mystery Glow-Ball: When Is a Battery Not a Battery?

    ERIC Educational Resources Information Center

    Crane, H. Richard, Ed.

    1989-01-01

    Examines the working mechanism of a commercial "Mystery Glow-Ball" by analyzing its electronic circuitry. Finds that the advertising for the ball is wrong; energy actually came from inserting a battery. (YP)

  7. On Classical Analogs of Quantum Schwarzschild and Reissner-Nordstrom Black Holes. Solving the "Mystery of log(3)"

    E-print Network

    Victor Berezin

    2010-01-22

    The model is built in which the main global properties of classical and quasi-classical black holes become local. These are the event horizon, "no-hair", temperature and entropy. Our construction is based on the features of a quantum collapse, discovered while studying some quantum black hole models. But it is purely classical, and this allows to use the Einstein equations and classical (local) thermodynamics and explain in this way the "log(3)" - puzzle.

  8. PREFACE: FAIRNESS 2014: FAIR Next Generation ScientistS 2014

    NASA Astrophysics Data System (ADS)

    2015-04-01

    FAIRNESS 2014 was the third edition in a series of workshops designed to bring together excellent international young scientists with research interests focused on physics at FAIR (Facility for Antiproton and Ion Research) and was held on September 22-27 2014 in Vietri sul Mare, Italy. The topics of the workshops cover a wide range of aspects in both theoretical developments and current experimental status, concentrated around the four scientific pillars of FAIR. FAIR is a new accelerator complex with brand new experimental facilities, that is currently being built next to the existing GSI Helmholtzzentrum for Schwerionenforschung close to Darmstadt, Germany. The spirit of the conference is to bring together young scientists, e.g. advanced PhD students and postdocs and young researchers without permanent position to present their work, to foster active informal discussions and build up of networks. Every participant in the meeting with the exception of the organizers gives an oral presentation, and all sessions are followed by an hour long discussion period. During the talks, questions are anonymously collected in a box to stimulate discussions. The broad physics program at FAIR is reflected in the wide range of topics covered by the workshop: • Physics of hot and dense nuclear matter, QCD phase transitions and critical point • Nuclear structure, astrophysics and reactions • Hadron Spectroscopy, Hadrons in matter and Hypernuclei • New developments in atomic and plasma physics • Special emphasis is put on the experiments CBM, HADES, PANDA, NUSTAR, APPA and related experiments For each of these different areas one invited speaker was selected to give a longer introductory presentation. The write-ups of the talks presented at FAIRNESS 2014 are the content of this issue of Journal of Physics: Conference Series and have been refereed according to the IOP standard for peer review. This issue constitutes therefore a collection of the forefront of research that is dedicated to the physics at FAIR. February 2015, Organizers of FAIRNESS 2014: Marco Destefanis, Tetyana Galatyuk, Fernando Montes, Diana Nicmorus, Hannah Petersen, Claudia Ratti, Laura Tolos, and Sascha Vogel. Support for holding the conference was provided by: Conference photograph

  9. Modelling biological complexity: a physical scientist's perspective

    PubMed Central

    Coveney, Peter V; Fowler, Philip W

    2005-01-01

    We discuss the modern approaches of complexity and self-organization to understanding dynamical systems and how these concepts can inform current interest in systems biology. From the perspective of a physical scientist, it is especially interesting to examine how the differing weights given to philosophies of science in the physical and biological sciences impact the application of the study of complexity. We briefly describe how the dynamics of the heart and circadian rhythms, canonical examples of systems biology, are modelled by sets of nonlinear coupled differential equations, which have to be solved numerically. A major difficulty with this approach is that all the parameters within these equations are not usually known. Coupled models that include biomolecular detail could help solve this problem. Coupling models across large ranges of length- and time-scales is central to describing complex systems and therefore to biology. Such coupling may be performed in at least two different ways, which we refer to as hierarchical and hybrid multiscale modelling. While limited progress has been made in the former case, the latter is only beginning to be addressed systematically. These modelling methods are expected to bring numerous benefits to biology, for example, the properties of a system could be studied over a wider range of length- and time-scales, a key aim of systems biology. Multiscale models couple behaviour at the molecular biological level to that at the cellular level, thereby providing a route for calculating many unknown parameters as well as investigating the effects at, for example, the cellular level, of small changes at the biomolecular level, such as a genetic mutation or the presence of a drug. The modelling and simulation of biomolecular systems is itself very computationally intensive; we describe a recently developed hybrid continuum-molecular model, HybridMD, and its associated molecular insertion algorithm, which point the way towards the integration of molecular and more coarse-grained representations of matter. The scope of such integrative approaches to complex systems research is circumscribed by the computational resources available. Computational grids should provide a step jump in the scale of these resources; we describe the tools that RealityGrid, a major UK e-Science project, has developed together with our experience of deploying complex models on nascent grids. We also discuss the prospects for mathematical approaches to reducing the dimensionality of complex networks in the search for universal systems-level properties, illustrating our approach with a description of the origin of life according to the RNA world view. PMID:16849185

  10. What Is the (ethical) Role of Scientists?

    NASA Astrophysics Data System (ADS)

    Oreskes, N.

    2014-12-01

    Many scientists are reluctant to speak out on issues of broad societal importance for fear that doing so crosses into territory that is not the scientists' domain. Others fear that scientists lose credibility when they address ethical and moral issues. A related concern is that discussing social or ethical questions runs the risk of politicizing science. Yet history shows that in the past, scientists often have spoken out on broad issues of societal concern, often (although not always) effectively. This paper explores the conditions under which scientists may be effective spokesmen and women on ethical and moral choices, and suggests some criteria by which scientists might decide when and whether it is appropriate for them to speak out beyond the circles of other technical experts.

  11. Best practices in bioinformatics training for life scientists

    PubMed Central

    Blicher, Thomas; Bongcam-Rudloff, Erik; Brazas, Michelle D.; Brooksbank, Cath; Budd, Aidan; De Las Rivas, Javier; Dreyer, Jacqueline; Fernandes, Pedro L.; van Gelder, Celia; Jacob, Joachim; Jimenez, Rafael C.; Loveland, Jane; Moran, Federico; Mulder, Nicola; Nyrönen, Tommi; Rother, Kristian; Schneider, Maria Victoria; Attwood, Teresa K.

    2013-01-01

    The mountains of data thrusting from the new landscape of modern high-throughput biology are irrevocably changing biomedical research and creating a near-insatiable demand for training in data management and manipulation and data mining and analysis. Among life scientists, from clinicians to environmental researchers, a common theme is the need not just to use, and gain familiarity with, bioinformatics tools and resources but also to understand their underlying fundamental theoretical and practical concepts. Providing bioinformatics training to empower life scientists to handle and analyse their data efficiently, and progress their research, is a challenge across the globe. Delivering good training goes beyond traditional lectures and resource-centric demos, using interactivity, problem-solving exercises and cooperative learning to substantially enhance training quality and learning outcomes. In this context, this article discusses various pragmatic criteria for identifying training needs and learning objectives, for selecting suitable trainees and trainers, for developing and maintaining training skills and evaluating training quality. Adherence to these criteria may help not only to guide course organizers and trainers on the path towards bioinformatics training excellence but, importantly, also to improve the training experience for life scientists. PMID:23803301

  12. The benefits of mystery in nature on attention: assessing the impacts of presentation duration

    PubMed Central

    Szolosi, Andrew M.; Watson, Jason M.; Ruddell, Edward J.

    2014-01-01

    Although research has provided prodigious evidence in support of the cognitive benefits that natural settings have over urban settings, all nature is not equal. Within nature, natural settings that contain mystery are often among the most preferred nature scenes. With the prospect of acquiring new information, scenes of this type could more effectively elicit a person's sense of fascination, enabling that person to rest the more effortful forms of attention. The present study examined the direct cognitive benefits that mystery in nature has on attention. Settings of this sort presumably evoke a form of attention that is undemanding or effortless. In order to investigate that notion, participants (n = 144) completed a Recognition Memory Task (RMT) that evaluated recognition performance based on the presence of mystery and presentation duration (300 ms, 1 s, 5 s, and 10 s). Results revealed that with additional viewing time, images perceived high in mystery achieved greater improvements in recognition performance when compared to those images perceived low in mystery. Tests for mediation showed that the effect mystery had on recognition performance occurred through perceptions of fascination. Implications of these and other findings are discussed in the context of Attention Restoration Theory. PMID:25505441

  13. Identifying Future Scientists: Predicting Persistence into Research Training

    PubMed Central

    2007-01-01

    This study used semistructured interviews and grounded theory to look for characteristics among college undergraduates that predicted persistence into Ph.D. and M.D./Ph.D. training. Participants in the summer undergraduate and postbaccalaureate research programs at the Mayo Clinic College of Medicine were interviewed at the start, near the end, and 8–12 months after their research experience. Of more than 200 themes considered, five characteristics predicted those students who went on to Ph.D. and M.D./Ph.D. training or to M.D. training intending to do research: 1) Curiosity to discover the unknown, 2) Enjoyment of problem solving, 3) A high level of independence, 4) The desire to help others indirectly through research, and 5) A flexible, minimally structured approach to the future. Web-based surveys with different students confirmed the high frequency of curiosity and/or problem solving as the primary reason students planned research careers. No evidence was found for differences among men, women, and minority and nonminority students. Although these results seem logical compared with successful scientists, their constancy, predictive capabilities, and sharp contrast to students who chose clinical medicine were striking. These results provide important insights into selection and motivation of potential biomedical scientists and the early experiences that will motivate them toward research careers. PMID:18056303

  14. Clinician-scientist trainee: a German perspective.

    PubMed

    Bossé, Dominick; Milger, Katrin; Morty, Rory E

    2011-01-01

    Clinician-scientists are particularly well positioned to bring basic science findings to the patient's bedside; the ultimate objective of basic research in the health sciences. Concerns have recently been raised about the decreasing workforce of clinician-scientists in both the United States of America and in Canada; however, little is known about clinician-scientists elsewhere around the globe. The purpose of this article is two-fold: 1) to feature clinician-scientist training in Germany; and 2) to provide a comparison with the Canadian system. In a question/answer interview, Rory E. Morty, director of a leading clinician-scientist training program in Germany, and Katrin Milger, a physician and graduate from that program, draw a picture of clinician-scientist training and career opportunities in Germany, outlining the place of clinician-scientists in the German medical system, the advantages and drawbacks of this training, and government initiatives to promote training and career development of clinician-scientists. The interview is followed by a discussion comparing the German and Canadian clinician-scientist development programs, focusing on barriers to trainee recruitment and career progress, and efforts to eliminate the barriers encountered along this very demanding but also very rewarding career path. PMID:22129920

  15. Mad City Mystery: Developing Scientific Argumentation Skills with a Place-based Augmented Reality Game on Handheld Computers

    NASA Astrophysics Data System (ADS)

    Squire, Kurt D.; Jan, Mingfong

    2007-02-01

    While the knowledge economy has reshaped the world, schools lag behind in producing appropriate learning for this social change. Science education needs to prepare students for a future world in which multiple representations are the norm and adults are required to "think like scientists." Location-based augmented reality games offer an opportunity to create a "post-progressive" pedagogy in which students are not only immersed in authentic scientific inquiry, but also required to perform in adult scientific discourses. This cross-case comparison as a component of a design-based research study investigates three cases (roughly 28 students total) where an Augmented Reality curriculum, Mad City Mystery, was used to support learning in environmental science. We investigate whether augmented reality games on handhelds can be used to engage students in scientific thinking (particularly argumentation), how game structures affect students' thinking, the impact of role playing on learning, and the role of the physical environment in shaping learning. We argue that such games hold potential for engaging students in meaningful scientific argumentation. Through game play, players are required to develop narrative accounts of scientific phenomena, a process that requires them to develop and argue scientific explanations. We argue that specific game features scaffold this thinking process, creating supports for student thinking non-existent in most inquiry-based learning environments.

  16. Mysteries of attraction: Giovanni Pico della Mirandola, astrology and desire.

    PubMed

    Rutkin, H Darrel

    2010-06-01

    Although in his later years Giovanni Pico della Mirandola (1463-1494) vehemently rejected astrology, he earlier used it in a variety of ways, but primarily to provide further evidence for positions to which he had arrived by other means. One such early use appears in his commentary on his friend Girolamo Benivieni's love poetry, the Canzone d'amore, of 1486-1487. In the passages discussed here, Pico presents an intensive Platonic natural philosophical analysis based on a deep astrologically informed understanding of human nature as he attempts to explain a perennial question, namely, why one person is attracted to a certain person (or people), and another to others. I will place this discussion of the mysteries of attraction and desire in historical perspective by tracing Pico's changing relationship to astrology during the course of his short but passionate life, and in historiographic perspective by revising Frances Yates's still influential views concerning Pico's contribution to Renaissance thought and his relationship with Marsilio Ficino. PMID:20513623

  17. [Angkor. The mystery of the dead city and Anopheles dirus].

    PubMed

    Verdrager, J

    1992-01-01

    The desertion of Angkor, which during more than five centuries was the center of a glorious civilization, has long been a matter of mystery and conjecture. The discovery of the vectorial capacity of the jungle mosquito Anopheles dirus, its epidemiological importance in the emergence and spread of multidrug resistance in Plasmodium falciparum malaria, the wiping out of large populations after transfer or deportation of non-immune Khmers into forest areas can now easily explain the desertion of Angkor. In 1431, Angkor Thom, the capital of the Khmer kingdom surrendered to the Thai conquerors. Soon afterwards, the young king left the city in search of a new capital. As a result of the population decrease large surfaces of rice fields were abandoned and reinvaded by the jungle, the typical biotope of Anopheles dirus. Severe epidemics of Plasmodium falciparum then occurred in the non-immune population with very high mortality decreasing again the number of workers and, thus, creating a vicious circle resulting in the progressive but complete desertion of Angkor. PMID:1494307

  18. The Complex World of Adolescent Literacy: Myths, Motivations, and Mysteries

    PubMed Central

    Moje, Elizabeth Birr; Overby, Melanie; Tysvaer, Nicole; Morris, Karen

    2009-01-01

    In this article, Elizabeth Birr Moje, Melanie Overby, Nicole Tysvaer, and Karen Morris challenge some of the prevailing myths about adolescents and their choices related to reading. The reading practices of youth from one urban community are examined using mixed methods in an effort to define what, how often, and why adolescents choose to read. By focusing on what features of texts youth find motivating, the authors find that reading and writing frequently occur in a range of literacy contexts outside school. However, only reading novels on a regular basis outside of school is shown to have a positive relationship to academic achievement as measured by school grades. This article describes how adolescents read texts that are embedded in social networks, allowing them to build social capital. Conclusions are framed in terms of the mysteries that remain — namely, how to build on what motivates adolescents' literacy practices in order to both promote the building of their social selves and improve their academic outcomes. PMID:19756223

  19. Fingerprinting a Mysterious Unseen Companion in the Solar Neighborhood

    NASA Astrophysics Data System (ADS)

    Jao, Wei-Chun; Henry, Todd; Subasavage, John

    2010-08-01

    We propose to use GMOS at Gemini-South to acquire a blue spectrum of a peculiar binary system discovered by the CTIOPI project. This system has the largest photocentric perturbation (~200 mas) among more than 500 systems we have observed for up to 10 years. Our red spectrum indicates that the primary is a red dwarf of type M5.0V, while our UBVRI photometry is consistent with combined light from the M5.0V star plus a cool (4500K) white dwarf secondary. However, the white dwarf has abnormally high flux at U compared to known cool white dwarfs. In addition, the GALEX mission indicates that this system has a very strong near-UV flux. Observations made via this proposal will allow us to confirm the nature of the mysterious unseen companion and model its physical properties, including its temperature and atmosphere abundance. Our continuing parallax observations and radial velocity measurements by Phoenix at Gemini-South (already scheduled) will yield a dynamical mass for a white dwarf cooler than 5000K for the first time.

  20. Movement mysteries unveiled: spatial ecology of juvenile green sea turtles

    USGS Publications Warehouse

    Shaver, Donna J.; Hart, Kristen M.; Fujisaki, Ikuko; Rubio, Cynthia; Sartain, Autumn R.

    2013-01-01

    Locations of important foraging areas are not well defined for many marine species. Unraveling these mysteries is vital to develop conservation strategies for these species, many of which are threatened or endangered. Satellite-tracking is a tool that can reveal movement patterns at both broad and fine spatial scales, in all marine environments. This chapter presents records of the longest duration track of an individual juvenile green turtle (434 days) and highest number of tracking days in any juvenile green turtle study (5483 tracking days) published to date. In this chapter, we use spatial modeling techniques to describe movements and identify foraging areas for juvenile green turtles (Chelonia mydas) captured in a developmental habitat in south Texas, USA. Some green turtles established residency in the vicinity of their capture and release site, but most used a specific habitat feature (i.e., a jettied pass) to travel between the Gulf of Mexico and a nearby bay. Still others moved southward within the Gulf of Mexico into Mexican coastal waters, likely in response to decreasing water temperatures. These movements to waters off the coast of Mexico highlight the importance of international cooperation in restoration efforts undertaken on behalf of this imperiled species.

  1. Walter sutton: physician, scientist, inventor.

    PubMed

    Ramirez, Gregory J; Hulston, Nancy J; Kovac, Anthony L

    2015-01-01

    Walter S. Sutton (1877-1916) was a physician, scientist, and inventor. Most of the work on Sutton has focused on his recognition that chromosomes carry genetic material and are the basis for Mendelian inheritance. Perhaps less well known is his work on rectal administration of ether. After Sutton's work on genetics, he completed his medical degree in 1907 and began a 2-year surgical fellowship at Roosevelt Hospital, New York City, NY, where he was introduced to the technique of rectal administration of ether. Sutton modified the work of others and documented 100 cases that were reported in his 1910 landmark paper "Anaesthesia by Colonic Absorption of Ether". Sutton had several deaths in his study, but he did not blame the rectal method. He felt that his use of rectal anesthesia was safe when administered appropriately and believed that it offered a distinct advantage over traditional pulmonary ether administration. His indications for its use included (1) head and neck surgery; (2) operations when ether absorption must be minimized due to heart, lung, or kidney problems; and (3) preoperative pulmonary complications. His contraindications included (1) cases involving alimentary tract or weakened colon; (2) laparotomies, except when the peritoneal cavity was not opened; (3) incompetent sphincter or anal fistula; (4) orthopnea; and (5) emergency cases. Sutton wrote the chapter on "Rectal Anesthesia" in one of the first comprehensive textbooks in anesthesia, James Tayloe Gwathmey's Anesthesia. Walter Sutton died of a ruptured appendix in 1916 at age 39. PMID:25748370

  2. Astrochemistry: Fullerene solves an interstellar puzzle

    NASA Astrophysics Data System (ADS)

    Ehrenfreund, Pascale; Foing, Bernard

    2015-07-01

    Laboratory measurements confirm that a 'buckyball' ion is responsible for two near-infrared absorption features found in spectra of the interstellar medium, casting light on a century-old astrochemical mystery. See Letter p.322

  3. Real Science, Real Learning: Bridging the Gap Between Scientists, Educators and Students

    NASA Astrophysics Data System (ADS)

    Lewis, Y.

    2006-05-01

    Today as never before, America needs its citizens to be literate in science and technology. Not only must we only inspire a new generation of scientists and engineers and technologists, we must foster a society capable of meeting complex, 21st-century challenges. Unfortunately, the need for creative, flexible thinkers is growing at a time when our young students are lagging in science interest and performance. Over the past 17 years, the JASON Project has worked to link real science and scientists to the classroom. This link provide viable pipeline to creating the next generation scientists and researchers. Ultimately, JASON's mission is to improve the way science is taught by enabling students to learn directly from leading scientists. Through partnerships with agencies such as NOAA and NASA, JASON creates multimedia classroom products based on current scientific research. Broadcasts of science expeditions, hosted by leading researchers, are coupled with classroom materials that include interactive computer-based simulations, video- on-demand, inquiry-based experiments and activities, and print materials for students and teachers. A "gated" Web site hosts online resources and provides a secure platform to network with scientists and other classrooms in a nationwide community of learners. Each curriculum is organized around a specific theme for a comprehensive learning experience. It may be taught as a complete package, or individual components can be selected to teach specific, standards-based concepts. Such thematic units include: Disappearing Wetlands, Mysteries of Earth and Mars, and Monster Storms. All JASON curriculum units are grounded in "inquiry-based learning." The highly interactive curriculum will enable students to access current, real-world scientific research and employ the scientific method through reflection, investigation, identification of problems, sharing of data, and forming and testing hypotheses. JASON specializes in effectively applying technology in science education by designing animated interactive visualizations that promote student understanding of complex scientific concepts and systems (Rieber, 1990, 1996). JASON's experience in utilizing the power of simulation technology has been widely recognized for its effectiveness in exciting and engaging students in science learning by independent evaluations of JASON's multimedia science curriculum (Ba et al., 2001; Goldenberg et al., 2003). The data collected indicates that JASON's science products have had a positive impact on students' science learning, have positively influenced their perceptions of scientists and of becoming scientists, and have helped diverse students grasp a deeper understanding of complex scientific content, concepts and technologies.

  4. The soul of the scientist

    SciTech Connect

    DeBakey, M.E.

    1995-12-31

    The author addresses the essense of scientific personnel as the animating and vital principle in people credited with the facilities of thought, action and emotion. Science pervades our lives and civilization. The author provides a view of the nature of science as a way of thinking and of solving problems. Science is presented as a highly organized, integrated, dynamic structure with diverse branches and widely disparate components that often combine for producing remarkable and unexpected benefits. Medical science is used to illustrate the humane goals of science. Modern medical issues and the Nation`s concern for reform in our health management systems are used to show the need for priorities and furthering the scientific education of the nation. 3 refs.

  5. Education: Mutualistic Interactions between Scientists and Children.

    ERIC Educational Resources Information Center

    Condon, Marty

    1991-01-01

    A project that introduced scientists to students and engaged students in creative scientific activities is described. Students were asked to help scientists identify patterns on the wing of a species of fruit fly. A combined research/education program is recommended. (KR)

  6. Staff Scientist Center for Nanophase Materials Sciences

    E-print Network

    Pennycook, Steve

    1 Jihua Chen Staff Scientist Center for Nanophase Materials Sciences Oak Ridge National Laboratory Scientist, Center for Nanophase Materials Sciences (CNMS), Oak Ridge National Laboratory (ORNL) 2009. Government Agency, and iii. New Meetings #12;2 2012 Session Chair, "Low-Voltage Electron Microscopy

  7. Exploring Native American Students' Perceptions of Scientists

    ERIC Educational Resources Information Center

    Laubach, Timothy A.; Crofford, Geary Don; Marek, Edmund A.

    2012-01-01

    The purpose of this descriptive study was to explore Native American (NA) students' perceptions of scientists by using the Draw-A-Scientist Test and to determine if differences in these perceptions exist between grade level, gender, and level of cultural tradition. Data were collected for students in Grades 9-12 within a NA grant off-reservation…

  8. Scientists' Views about Communication Training

    ERIC Educational Resources Information Center

    Besley, John C.; Dudo, Anthony; Storksdieck, Martin

    2015-01-01

    This study assesses how scientists think about science communication training based on the argument that such training represents an important tool in improving the quality of interactions between scientists and the public. It specifically focuses on training related to five goals, including views about training to make science messages…

  9. Scientists Like Me: Faces of Discovery

    NASA Astrophysics Data System (ADS)

    Enevoldsen, A. A. G.; Culp, S.; Trinh, A.

    2010-08-01

    During the International Year of Astronomy, Pacific Science Center is hosting a photography exhibit: Scientists Like Me: Faces of Discovery. The exhibit contains photographs of real, current astronomers and scientists working in astronomy and aerospace-related fields from many races, genders, cultural affiliations and walks of life. The photographs were taken and posters designed by Alyssa Trinh and Sarah Culp, high school interns in Discovery Corps, Pacific Science Center's youth development program. The direct contact between the scientists and the interns helps the intended audience of teachers and families personally connect with scientists. The finished posters from this exhibit are available online (http://pacificsciencecenter.org/scientists) for teachers to use in their classrooms, in addition to being displayed at Pacific Science Center and becoming part of Pacific Science Center's permanent art rotation. The objective of this project was to fill a need for representative photographs of scientists in the world community. It also met two of the goals of International Year of Astronomy: to provide a modern image of science and scientists, and to improve the gender-balanced representation of scientists at all levels and promote greater involvement by all people in scientific and engineering careers. We would like to build on the success of this project and create an annual summer internship, with different interns, focusing on creating posters for different fields of science.

  10. USGS Scientists Monitor San Juan River

    USGS Multimedia Gallery

    USGS scientists collecting water samples along the San Juan River in Farmington, New Mexico on August 8, 2015. Scientists from the USGS New Mexico Water Science Center obtained water samples from the Animas and San Juan Rivers before and after arrival of the August 5 Gold King Mine spill....

  11. Educators' Views of Collaboration with Scientists

    ERIC Educational Resources Information Center

    Kim, Chankook; Fortner, Rosanne

    2007-01-01

    This study investigated educators' views of collaboration with scientists, a baseline for COSEE Great Lakes efforts in facilitating dynamic collaborative relationships between Great Lakes researchers and educators. Three research questions guided the study: (1) how are educators in the Great Lakes region involved in collaboration with scientists,…

  12. How Middle Schoolers Draw Engineers and Scientists

    ERIC Educational Resources Information Center

    Fralick, Bethany; Kearn, Jennifer; Thompson, Stephen; Lyons, Jed

    2009-01-01

    The perceptions young students have of engineers and scientists are often populated with misconceptions and stereotypes. Although the perceptions that young people have of engineers and of scientists have been investigated separately, they have not been systematically compared. The research reported in this paper explores the question "How are…

  13. Student Pugwash Conference Probes Scientists' Individual Responsibility.

    ERIC Educational Resources Information Center

    Seltzer, Richard J.

    1985-01-01

    Students from 25 nations and senior scientists examined ethical and social dimensions of decision making about science and technology during the 1985 Student Pugwash Conference on scientists' individual responsibilities. Working groups focused on toxic wastes, military uses of space, energy and poverty, genetic engineering, and individual rights.…

  14. How Scientists Develop Competence in Visual Communication

    ERIC Educational Resources Information Center

    Ostergren, Marilyn

    2013-01-01

    Visuals (maps, charts, diagrams and illustrations) are an important tool for communication in most scientific disciplines, which means that scientists benefit from having strong visual communication skills. This dissertation examines the nature of competence in visual communication and the means by which scientists acquire this competence. This…

  15. Response: Training Doctoral Students to Be Scientists

    ERIC Educational Resources Information Center

    Pollio, David E.

    2012-01-01

    The purpose of this article is to begin framing doctoral training for a science of social work. This process starts by examining two seemingly simple questions: "What is a social work scientist?" and "How do we train social work scientists?" In answering the first question, some basic assumptions and concepts about what constitutes a "social work…

  16. Scientific Encounters of the Mysterious Sea. Reading Activities That Explore the Mysterious Creatures of the Deep Blue Sea. Grades 4-7.

    ERIC Educational Resources Information Center

    Embry, Lynn

    This activity book presents reading activities for grades 4-7 exploring the mysterious creatures of the deep sea. The creatures include: angel sharks; argonauts; barberfish; comb jelly; croakers; electric rays; flying fish; giganturid; lantern fish; narwhals; northern basket starfish; ocean sunfish; Portuguese man-of-war; sea cucumbers; sea…

  17. Toward an understanding of middle school students' problem-solving strategies: Establishing a foundation for teacher inquiry

    NASA Astrophysics Data System (ADS)

    Scott, Gary

    During the past decade science teachers have made increasing use of a real-world, problem-based approach to science teaching. Without theories of how and why students use knowledge to solve such problems, teachers are constrained in their ability to diagnose students' difficulties in comprehending science concepts as well as students' problems in making connections among the concepts. In this study students from two middle schools were given a "hands-on" experience in solving a real-world forensics problem based on the Lawrence's Hall of Science's Mystery Festival, "The Case of the Missing Millionaire." Following the Mystery Festival, the students went to the computer lab to solve the computer-based transfer problems created with IMMEX problem-solving software. The software includes authoring capabilities and a tracking system that records students' use of knowledge and concepts to solve problems. Data from the computer-based pathways of 495 student pairs, video-records of pairs of students problem-solving, teachers' perception of processes in their classes, and my own observations of problem-solving in action yielded the following results: (1) Twice as many 7th and 8th graders as 6th graders were successful in solving "Roger Rabbit." (2) Approximately twice as many groups correctly solving the problem used an evidence-based approach compared to groups that missed the answer. Groups correctly answering the problem used the evidence-based method, a conjecture-based approach, and a mixed approach (integration of evidence and conjecture) with approximately the same frequencies. (3) Information selection strategies, from the first item a group selected to the last, as they attempted to solve the problem was classified in one of three categories: trial and error, menu-based, and logically linked. Trial and error and menu-based were the dominant strategies. (4) In a follow-up study, 7th and 8th graders attempted to solve "Roger Rabbit" without the hands-on experience of the Mystery Festival. These students comprised a comparison group whereas the original students were designated as the experimental group. The experimental groups were 1.5 times more likely to employ a logically linked strategy for selecting information. (5) Experimental groups that correctly solved the problem were more likely to use an evidence-based approach than were the comparison groups.

  18. Analyzing Prospective Teachers' Images of Scientists Using Positive, Negative and Stereotypical Images of Scientists

    ERIC Educational Resources Information Center

    Subramaniam, Karthigeyan; Harrell, Pamela Esprivalo; Wojnowski, David

    2013-01-01

    Background and purpose: This study details the use of a conceptual framework to analyze prospective teachers' images of scientists to reveal their context-specific conceptions of scientists. The conceptual framework consists of context-specific conceptions related to positive, stereotypical and negative images of scientists as detailed in the…

  19. Solving crimes with hypnosis.

    PubMed

    Wester, William C; Hammond, D Corydon

    2011-04-01

    Following a brief review of the literature on hypnosis and memory, this paper overviews the procedures that are used in conducting forensic hypnosis interviews. Ten forensic hypnosis cases are then described. These real world cases are in stark contrast to research done in an artificial laboratory setting where the information to be recalled lacks personal relevance and was not associated with emotionally arousing situations. These cases illustrate how forensic hypnosis can result in obtaining important additional investigative leads which lead to the solving of crimes. PMID:21598840

  20. VLBA Scientists Study Birth of Sunlike Stars

    NASA Astrophysics Data System (ADS)

    1999-06-01

    Three teams of scientists have used the National Science Foundation's Very Long Baseline Array (VLBA) radio telescope to learn tantalizing new details about how Sun-like stars are formed. Young stars, still growing by drawing in nearby gas, also spew some of that material back into their surroundings, like impatient infants that eat too quickly. The VLBA observations are giving astronomers new insights on both processes -- the accretion of material by the new stars and the outflows of material from them. "For the first time, we're actually seeing what happens right down next to the star in these young systems," said Mark Claussen, of the National Radio Astronomy Observatory (NRAO) in Socorro, NM. Claussen and other researchers announced their findings at the American Astronomical Society's meeting in Chicago. Material attracted by a young star's gravitational pull forms a flat, orbiting disk, called an accretion disk, in which the material circles closer and closer to the star until finally drawn into it. At the same time, material is ejected in "jets" speeding from the poles of the accretion disk. "The VLBA is showing us the first images of the region close to the star where the material in these jets is accelerated and formed into the `beams' of the jet," Claussen said. "We don't understand the details of these processes well," Claussen said. "These VLBA research projects are beginning to help unravel the mysteries of how stars like the Sun form." The teams are observing clumps of water vapor that naturally amplify radio emissions to see details smaller than the orbit of Mercury in young stellar systems as well as track gas motions. The clumps of gas are called masers, and amplify radio emission in much the same way that a laser amplifies light emission. "These images are just fantastic," said Al Wootten of NRAO in Charlottesville, VA. The maser clumps or "spots," emitting radio waves at a specific wavelength, can be tracked as they move over time. In addition, by measuring the Doppler shift in the wavelength of these emissions, astronomers can determine the speed at which the gas is moving. In an object known as S106FIR, 2,000 light-years away in the constellation Cygnus, a team of Japanese and U.S. VLBA observers led by Ray Furuya, a graduate student from Japan's Nobeyama Radio Observatory, has tracked the motion of material outward in the jet. This object, embedded in a dense cloud of molecular gas, the material from which the star is forming, shows maser spots moving in two directions as the jets emerge from both poles of the accretion disk. "The water masers are the only way we can detect the outflow from this young star," Furuya said. The VLBA observations can discern details as small as half the distance from the Earth to the Sun. "We can see outflow on scales the size of our Solar System. We think this object is one of the youngest protostars known," Furuya said. In another object, dubbed IRAS 16293-2422, in the constellation Ophiuchus, astronomers believe the water masers clearly show the outflowing jets of a young star and may be tracing the accretion disk as well. The young star is one of a pair of stars in a binary system some 500 light-years distant. The water-vapor masers are seen around only one of the pair, however. "In this system, we see outflow in the jet and also an elliptical ring of masers that may be part of the accretion disk," said Wootten, leader of the team observing this object. "The VLBA is showing us details as small as the size of Mercury's orbit around the Sun, a great help in understanding the physics going on there," Wootten said. A team composed largely of astronomers from the Harvard-Smithsonian Center for Astrophysics in Cambridge, MA, also used the VLBA to study water masers in a young stellar object 2,500 light-years away in Cepheus. This team sees maser spots moving in opposite directions away from the young star on scales of ten times the diameter of the solar system, pr

  1. Successful scientist: What's the winning formula?

    PubMed

    Stull, April J; Ciappio, Eric D

    2014-11-01

    What does it take to become a successful scientist? This question is usually asked or thought about at some point in a young scientist's career. The early stages of a scientific career are fraught with many hardships, and achieving success can seem impossible and daunting. After encountering many obstacles, it becomes easy to focus on failures and lose sight of career goals. The journey to success can seem so simple when looked upon from the outside, but even the best scientists have endured many hardships, which are often not communicated. This educational symposium featured a diverse panel of 5 accomplished scientists representing different work environments, such as government, industry, and academia. They discussed tips on how to have a successful career journey and the key qualities of a successful scientist. Also, they revealed the secret to what's in the winning formula for success. PMID:25398744

  2. Precise Heat Control: What Every Scientist Needs to Know About Pyrolytic Techniques to Solve Real Problems

    NASA Technical Reports Server (NTRS)

    Devivar, Rodrigo

    2014-01-01

    The performance of a material is greatly influenced by its thermal and chemical properties. Analytical pyrolysis, when coupled to a GC-MS system, is a powerful technique that can unlock the thermal and chemical properties of almost any substance and provide vital information. At NASA, we depend on precise thermal analysis instrumentation for understanding aerospace travel. Our analytical techniques allow us to test materials in the laboratory prior to an actual field test; whether the field test is miles up in the sky or miles underground, the properties of any involved material must be fully studied and understood in the laboratory.

  3. Solving Differential Equations in R: Package deSolve

    EPA Science Inventory

    In this paper we present the R package deSolve to solve initial value problems (IVP) written as ordinary differential equations (ODE), differential algebraic equations (DAE) of index 0 or 1 and partial differential equations (PDE), the latter solved using the method of lines appr...

  4. THE MYSTERY OF THE COSMIC DIFFUSE ULTRAVIOLET BACKGROUND RADIATION

    SciTech Connect

    Henry, Richard Conn; Murthy, Jayant; Overduin, James; Tyler, Joshua E-mail: jmurthy@yahoo.com E-mail: 97tyler@cardinalmail.cua.edu

    2015-01-01

    The diffuse cosmic background radiation in the Galaxy Evolution Explorer far-ultraviolet (FUV, 1300-1700 Å) is deduced to originate only partially in the dust-scattered radiation of FUV-emitting stars: the source of a substantial fraction of the FUV background radiation remains a mystery. The radiation is remarkably uniform at both far northern and far southern Galactic latitudes and increases toward lower Galactic latitudes at all Galactic longitudes. We examine speculation that this might be due to interaction of the dark matter with the nuclei of the interstellar medium, but we are unable to point to a plausible mechanism for an effective interaction. We also explore the possibility that we are seeing radiation from bright FUV-emitting stars scattering from a ''second population'' of interstellar grains—grains that are small compared with FUV wavelengths. Such grains are known to exist, and they scatter with very high albedo, with an isotropic scattering pattern. However, comparison with the observed distribution (deduced from their 100 ?m emission) of grains at high Galactic latitudes shows no correlation between the grains' location and the observed FUV emission. Our modeling of the FUV scattering by small grains also shows that there must be remarkably few such ''smaller'' grains at high Galactic latitudes, both north and south; this likely means simply that there is very little interstellar dust of any kind at the Galactic poles, in agreement with Perry and Johnston. We also review our limited knowledge of the cosmic diffuse background at ultraviolet wavelengths shortward of Ly?—it could be that our ''second component'' of the diffuse FUV background persists shortward of the Lyman limit and is the cause of the reionization of the universe.

  5. Pebble Puzzle Solved

    NASA Technical Reports Server (NTRS)

    2004-01-01

    [figure removed for brevity, see original site] Figure 1 In the quest to determine if a pebble was jamming the rock abrasion tool on NASA's Mars Exploration Rover Opportunity, scientists and engineers examined this up-close, approximate true-color image of the tool. The picture was taken by the rover's panoramic camera, using filters centered at 601, 535, and 482 nanometers, at 12:47 local solar time on sol 200 (August 16, 2004).

    Colored spots have been drawn on this image corresponding to regions where panoramic camera reflectance spectra were acquired (see chart in Figure 1). Those regions are: the grinding wheel heads (yellow); the rock abrasion tool magnets (green); the supposed pebble (red); a sunlit portion of the aluminum rock abrasion tool housing (purple); and a shadowed portion of the rock abrasion tool housing (brown). These spectra demonstrated that the composition of the supposed pebble was clearly different from that of the sunlit and shadowed portions of the rock abrasion tool, while similar to that of the dust-coated rock abrasion tool magnets and grinding heads. This led the team to conclude that the object disabling the rock abrasion tool was indeed a martian pebble.

  6. No-Fault Problem Solving

    ERIC Educational Resources Information Center

    Van Orman, W. Roy

    1975-01-01

    Describes a problem solving approach for administrative personnel which attempts to put feelings aside and deal with discussion of the facts, generation of solutions, selection of a course of action and actual action to solve the problem. (EJT)

  7. Journal Article: Using Scientists and Real-World Scenarios in Professional Development for Middle School Science Teachers

    SciTech Connect

    Morrison, Judith A.; Estes, Jeffrey C.

    2007-04-01

    Middle school science teachers were involved in a problem-solving experience presented and guided by research scientists. Data on the teachers’ perspectives about this professional development and any impact it may have had on their teaching practices were collected through interviews, surveys, and classroom observations. The findings show that the professional development experience was positive, although one concern expressed by teachers was their lack of understanding of the scientists’ vocabulary. Using scientists and real-world scenarios was shown to be an effective strategy for encouraging middle school teachers to teach science as a process and help them strengthen their science content understanding.

  8. Solving Quasars (Part 1)

    SciTech Connect

    Elvis, Martin

    2003-10-29

    Quasars are a frustratingly unsolved problem in astrophysics. For 40 years quasars and AGN have presented an ever-proliferating list of diverse and confusing phenomenology from optical to X-ray wavelengths. The result has been that despite being the most powerful objects in the universe, quasars have been increasingly sidelined in astrophysics. This is unfortunate, as quasars pose major physics, as well as astrophysics puzzles, and should be important in cosmology. The problem, I believe, is not that we do not know enough physics, but rather that we do not have the right geometry. I have proposed a simple geometric and kinematic model that allows all of the quasar diversity to be understood as part of a single structure, the 'Quasar Atmosphere'. This structure suggests a natural physical interpretation, that builds on our understanding of stars (the only fully solved problem in astrophysics), and offers the prospect that we can use quasars for cosmology at last.

  9. Problem Solving, Scaffolding and Learning

    ERIC Educational Resources Information Center

    Lin, Shih-Yin

    2012-01-01

    Helping students to construct robust understanding of physics concepts and develop good solving skills is a central goal in many physics classrooms. This thesis examine students' problem solving abilities from different perspectives and explores strategies to scaffold students' learning. In studies involving analogical problem solving

  10. My path to becoming a data scientist

    NASA Astrophysics Data System (ADS)

    Strand, G.

    2013-12-01

    The choice to become a data scientist wasn't one I consciously made. I began as a student assistant working on a small data analysis package, and have evolved since then (with various diversions along the way) to become NCAR's primary global climate model data manager and global climate model data scientist. I've witnessed how data management in this area of the earth sciences has changed, from notes attached to cases for magnetic tapes containing esoteric binary data, to today's standards for data formats and metadata standards. I'll talk about how I became a data scientist and the experiences I've had in my career.

  11. The Real Life of a Data Scientist

    NASA Astrophysics Data System (ADS)

    Strand, W. G.

    2011-12-01

    The choice to become a data scientist wasn't one I consciously made. I began as a student assistant working on a small data analysis package, and have evolved since then (with various diversions along the way) to become NCAR's primary global climate model data manager and global climate model data scientist. I've witnessed how data management in this area of the earth sciences has changed, from notes attached to cases for magnetic tapes containing esoteric binary data, to today's standards for data formats and metadata standards. I'll talk about how I became a data scientist and the experiences I've had in my career.

  12. USGS Scientists in Wadi Degla, Northern Egypt

    USGS Multimedia Gallery

    USGS scientists looking at Eocene sandstones and limestones in Wadi Degla, northern Egypt. This area was studied to understand the Levant Basin Province, as both regions have similar rock formations....

  13. USGS scientists Measure Floodwaters at Morganza Spillway

    USGS Multimedia Gallery

    USGS scientist Garron Ross is interviewed by CCTV reporters about USGS streamflow information. USGS streamflow information is used by the U.S. Army Corps of Engineers to help them make informed flood management decisions....

  14. The Social Responsibilities of Scientists and Science.

    ERIC Educational Resources Information Center

    Pauling, Linus

    2000-01-01

    Points out the important role of scientists in society as educators. Explains problems caused by not understanding the theory of evolution and discusses possible solutions. First published in 1966. (YDS)

  15. In Conversation With Materials Scientist Ron Zuckermann

    SciTech Connect

    Ron Zuckerman

    2009-11-18

    Nov. 11, 2009: Host Alice Egan of Berkeley Lab's Materials Sciences Division interviews scientists about their lives and work in language everyone can understand. Her guest Berkeley Lab's Ron Zuckerman, who discusses biological nanostructures and the world of peptoids.

  16. In Conversation With Materials Scientist Ron Zuckermann

    ScienceCinema

    Ron Zuckerman

    2010-01-08

    Nov. 11, 2009: Host Alice Egan of Berkeley Lab's Materials Sciences Division interviews scientists about their lives and work in language everyone can understand. Her guest Berkeley Lab's Ron Zuckerman, who discusses biological nanostructures and the world of peptoids.

  17. CGH Short Term Scientist Exchange Program (STSEP)

    Cancer.gov

    STSEP promotes collaborative research between established U.S. and foreign scientists from low, middle, and upper-middle income countries (LMICs) by supporting, in part, exchange visits of cancer researchers between U.S. and foreign laboratories.

  18. Education and Outreach: Advice to Young Scientists

    NASA Astrophysics Data System (ADS)

    Lopes, R. M. C.

    2005-08-01

    Carl Sagan set an example to all scientists when he encouraged us to reach out to the public and share the excitement of discovery and exploration. The prejudice that ensued did not deter Sagan and, with the passing of years, more and more scientists have followed his example. Although at present scientists at all ranks are encouraged by their institutions to do outreach, the balancing of a successful scientific career with teaching and outreach is often not an easy one. Young scientists, in particular, may worry about how their outreach efforts are viewed in the community and how they will find the time and energy for these efforts. This talk will offer suggestions on how to balance an active science research program with outreach activities, the many different ways to engage in education and public outreach, and how the rewards are truly priceless.

  19. Career Panel: Scientists in Science Education

    E-print Network

    Career Panel: Scientists in Science Education Presented by The Graduate School Office of STEM Specialist, Office of STEM Education Partnerships, Northwestern University emily College. Emily joined the Office of STEM Education Partnerships at Northwestern University as a Teacher

  20. A Scientist's Guide to Science Denial

    NASA Astrophysics Data System (ADS)

    Rosenau, J.

    2012-12-01

    Why are so many scientifically uncontroversial topics, from evolution and the age of the earth to climate change and vaccines, so contentious in society? The American public respects science and scientists, yet seems remarkably unaware of - or resistant to accepting - what scientists have learned about the world around us. This resistance holds back science education and undermines public policy discussions. Scientists and science communicators often react to science denial as if it were a question of scientific knowledge, and respond by trying to correct false scientific claims. Many independent lines of evidence show that science denial is not primarily about science. People reject scientific claims which seem to conflict with their personal identity - often because they believe that accepting those claims would threaten some deeply-valued cultural, political, or religious affiliation. Only by identifying, addressing, and defusing the underlying political and cultural concerns can educators, scientists, and science communicators undo the harm done by science denial.

  1. Ask a Climate Scientist - Duration: 80 seconds.

    NASA Video Gallery

    Have a question that's always confounded you about Earth's climate? Wonder why it matters that the climate is changing now if it has changed before? Or how scientists know changes seen in recent de...

  2. Research and Teaching: Fostering Collaborative Problem Solving and 21st Century Skills Using the DEEPER Scaffolding Framework

    ERIC Educational Resources Information Center

    Antonenko, Pavlo D.; Jahanzad, Farzaneh; Greenwood, Carmen

    2014-01-01

    Collaborative problem solving is an essential component of any 21st century science career. Scientists are hired, retained, and promoted for solving problems in dynamic and interdisciplinary teams. They discuss issues, explain and justify their opinions, debate, elaborate, and reflect on their collective knowledge. At the same time, both…

  3. Where on Earth...? MISR Mystery Image Quiz #6

    NASA Technical Reports Server (NTRS)

    2002-01-01

    Here's another chance to play geographical detective! This Multi-angle Imaging SpectroRadiometer (MISR) image covers an area of about 298 kilometers x 358 kilometers, and was captured by the instrument's vertical-viewing (nadir) camera on December 27, 2001. Use any reference materials you like and answer the following five questions: The large lagoon in the image is named for a particular type of bird. Name the bird. Note the sediment plume emanating from the southern end of the lagoon. Sailors in the 16th century imagined this outlet to be the mouth of a large river. What did they call the river? A series of wave-like points and curls form 'cusps' on the inner shores of the lagoon. Which ONE of the following is most responsible for the formation of these cusps? Violent storm impacts on erosion and accretion Wind and tide-driven sediment transport and circulation Tectonic folding associated with nearby mountain ridges Bathymetric effects of dredging operations True or false: Changes in regional precipitation associated with large scale atmospheric circulation patterns have no effect on the salinity of the lagoon's water. Which one of these is NOT distributed within the area covered by this image? Ruppia maritima Chelonia mydas Tapirus bairdii Microcystis aeruginosa E-mail your answers, name (initials are acceptable if you prefer), and your hometown by Tuesday, February 19, 2002 to suggestions@mail-misr.jpl.nasa.gov. Answers will be published on the MISR web site in conjunction with the next weekly image release. The names and home towns of respondents who answer all questions correctly by the deadline will also be published in the order responses were received. The first 3 people on this list who are not affiliated with NASA, JPL, or MISR and who did not win a prize in the last quiz will be sent a print of the image. A new 'Where on Earth...?' mystery appears as the MISR 'image of the week' approximately once per month. A new image of the week is released every Wednesday at noon Pacific time on the MISR home page http://www-misr.jpl.nasa.gov. The image also appears on the Atmospheric Sciences Data Center home page, http://eosweb.larc.nasa.gov, though usually with a several-hour delay. Image courtesy NASA/GSFC/LaRC/JPL, MISR Team.

  4. Social scientist's viewpoint on conflict management

    USGS Publications Warehouse

    Ertel, Madge O.

    1990-01-01

    Social scientists can bring to the conflict-management process objective, reliable information needed to resolve increasingly complex issues. Engineers need basic training in the principles of the social sciences and in strategies for public involvement. All scientists need to be sure that that the information they provide is unbiased by their own value judgments and that fair standards and open procedures govern its use.

  5. __Mysterious Multiplication 1________________________________ Ask students to calculate 25x25. Ask them to calculate 35x35, then 45x45.

    E-print Network

    Watanabe, Tad

    __Mysterious Multiplication 1________________________________ Ask students to calculate 25x25. Ask be rearranged to form a 40 by 50 rectangle, etc. #12;b a b a See also Mysterious Multiplication (2). #12;

  6. How Middle Schoolers Draw Engineers and Scientists

    NASA Astrophysics Data System (ADS)

    Fralick, Bethany; Kearn, Jennifer; Thompson, Stephen; Lyons, Jed

    2009-02-01

    The perceptions young students have of engineers and scientists are often populated with misconceptions and stereotypes. Although the perceptions that young people have of engineers and of scientists have been investigated separately, they have not been systematically compared. The research reported in this paper explores the question "How are student perceptions of engineers and scientists similar and how are they different?" Approximately 1,600 middle school students from urban and suburban schools in the southeastern United States were asked to draw either an engineer or a scientist at work. Drawings included space for the students to explain what their person was doing in the picture. A checklist to code the drawings was developed and used by two raters. This paper discusses similarities and differences in middle school perceptions of scientists and engineers. Results reveal that the students involved in this study frequently perceive scientists as working indoors conducting experiments. A large fraction of the students have no perception of engineering. Others frequently perceive engineers as working outdoors in manual labor. The findings have implications for the development and implementation of engineering outreach efforts.

  7. The Mysterious Case of the Detective as Child Hero: Sherlock Holmes, Encyclopedia Brown and Nancy Drew as Role Models?

    ERIC Educational Resources Information Center

    Sugarman, Sally

    In the mystery genre, the one characteristic that the enduring figures of Sherlock Holmes, Nancy Drew, and Encyclopedia Brown have in common is a rational mind. The source of their strength is their ability to think and think well. A study examined some typical examples of the mystery genre in young adult literature and surveyed children and…

  8. 7 CFR 91.18 - Financial interest of a scientist.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ...2011-01-01 false Financial interest of a scientist. 91.18 Section 91.18 Agriculture ...Laboratory Service § 91.18 Financial interest of a scientist. No scientist shall perform a laboratory analysis on any...

  9. 7 CFR 91.18 - Financial interest of a scientist.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ...2010-01-01 false Financial interest of a scientist. 91.18 Section 91.18 Agriculture ...Laboratory Service § 91.18 Financial interest of a scientist. No scientist shall perform a laboratory analysis on any...

  10. Environmental Scientists Find Antibiotics, Bacteria, Resistance Genes in Feedlot Dust

    E-print Network

    Rock, Chris

    Environmental Scientists Find Antibiotics, Bacteria, Resistance Genes in Feedlot Dust :: Texas Tech Today http://today.ttu.edu/2015/01/environmental-scientists-find-antibiotics-bacteria-resistance Print Email + Font - Font Environmental Scientists Find Antibiotics, Bacteria, Resistance Genes

  11. Scientists Model the Molecular Basis of Parkinson's Disease

    E-print Network

    Xu, Jinchao

    #12;Scientists Model the Molecular Basis of Parkinson's Disease Astrophysicists Discover Supernova scientists, applied mathematicians, and computer scientists gathered in Febru- ary 2008 at the invitation through the Innovative and Novel Computational Impact on Theory and Experiment (IN- CITE) program

  12. New Observations Deepen Mystery Surrounding Water Masers in Elliptical Galaxy

    NASA Astrophysics Data System (ADS)

    New observations with the National Science Foundation's Very Long Baseline Array (VLBA) radio telescope have deepened the mystery surrounding water molecules in a galaxy 65 million light- years away. The water molecules are acting as natural masers -- amplifiers of microwave radio emissions -- and these cosmic masers within the galaxy NGC 1052 are raising difficult questions for astronomers trying to explain them. Results of the new observations, which pinpoint the location of water masers in NGC 1052, were announced today at the American Astronomical Society meeting in Toronto, Ontario. The researchers are: Jim Braatz of Harvard University in Cambridge, Massachusetts, Mark Claussen and Phil Diamond of the National Radio Astronomy Observatory in Socorro, New Mexico, Andrew Wilson of the University of Maryland in College Park, Maryland, and Christian Henkel of the Max Planck Institute fur Radioastronomie in Bonn, Germany. Water masers have been detected in several other galaxies. However, most galaxies containing water "megamasers" such as those in NGC 1052 are spiral galaxies. NGC 1052 is one of only two elliptical galaxies in which water megamasers have been detected. Because ellipticals tend to have much less gas and dust than spirals, the existence of the water masers in NGC 1052 is surprising by itself, though that galaxy does have more gas and dust than the typical elliptical. Located in the constellation Cetus, NGC 1052 also has an active nucleus, believed to be powered by the gravitational energy of a supermassive black hole at its core. The new VLBA observations produced an additional mystery. In other galaxies with water megamasers, the masers are believed to lie within a disk of molecules orbiting the galaxy's central black hole. This is the case, for example, in the now-famous galaxy NGC 4258, where the movement of the orbiting disk can be traced by measuring both the Doppler shift of radio emission from the masers and by tracking the motion of individual maser "spots" as their orbital motion carries them across our line of sight. However, in NGC 1052, this does not appear to be the case. Instead of residing within a disk orbiting the possible black hole, the water masers in NGC 1052 may lie in a "jet" of material being ejected by the central engine of the active nucleus. The high-resolution VLBA observations allowed the team of researchers to locate the water masers with respect to the jet. If the masers were in a disk around a black hole, the masers would be expected to lie in a line perpendicular to the jet axis around the radio core. Two "clumps" of maser emission, each composed of several weaker features, were found instead to lie along the jet axis. "The fact that the masers don't lie transverse to the jet axis means that these masers possibly do not trace a molecular disk around a possible black hole, but could be coming from gas either in the jet material itself, or in some molecular gas just in front of the jet," said Claussen. The researchers don't yet know exactly which of the radio continuum brightness peaks represent the true core of the galaxy, but further analysis of existing data taken by other groups in conjunction with the new data will allow them to determine just where the central engine lies with respect to the jet and the water masers. The shape of the spectrum of the water masers in NGC 1052 also is different than that of the other water megamasers. Typical spectra of water masers in spiral galaxies are composed of many narrow, "spiky" features. The maser spectrum in NGC 1052 is broad and relatively smooth. Periodic monitoring of the maser emission in NGC 1052 using single-dish radio telescopes in Germany, Australia, and the United States has been performed over the past two years. In that time, the features of the maser spectrum have drifted toward longer wavelengths, presumably because of velocity changes that affected the Doppler shift of the radio waves. The overall velocity has changed by about 50 kilometers per second duri

  13. Ulysses discovers the mysteries of the sun's south pole

    NASA Astrophysics Data System (ADS)

    1994-09-01

    Scientists at ESA's space research and technology centre in Noordwijk (the Netherlands) this morning gave a very positive account of the South polar pass phase, which started in June and will be completed in November. In particular they concluded that the south polar region displayed unexpected magnetic and dynamic characteristics; this probably means that the thinking on the magnetic structure of the Sun will have to be revised. The first thing that surprised the scientists was the low cosmic radiation activity above the south pole and the remarkable apparent absence of a south magnetic pole. Richard Marsden, ESA's project scientist, explained: "We expected the Sun to have a relatively simple magnetic field, such as the Earth's or that of a magnetised iron bar. We thought we were going to find a local increase in the field's intensity. But the probe did not detect any such thing and all the evidence so far suggests that the Sun has no south magnetic pole. Could it be that the Sun has no south magnetic pole? Or is one suddenly going to appear before Ulysses completes its pass? These are some of the questions exercising the minds of the team of scientists working on the project, who are keenly looking forward to comparing these results with those that will be coming through next year when the probe passes over the Sun's north geographic pole. It is however already manifestly clear that the structure of the solar magnetic field in the southern polar region is not as predicted by the models. In particular, the instruments on board Ulysses have detected a new type of very slowly varying electromagnetic waves, with oscillation periods of 10 to 20 hours. The experts' theory is that this is due to an unexpected phenomenon that conveys the solar magnetic field into space through the solar wind. It is still far too early to say what effect these new findings are going to have on our overall understanding of the Sun and the interplanetary wind it generates. A vast volume of data running into billions of bits, all of it of great scientific value, has been acquired during the first part of this polar pass. Detailed analysis is going to take many months. However, one thing about which there is no doubt is the complexity of the phenomena observed, which involve the combined effects of the solar wind, magnetic field, electromagnetic waves and fast-moving bursts of particles. Further insights will probably be gained when Ulysses passes over the Sun's north pole in 1995 and, if the mission is extended, when it makes two further polar passes in 2000-2001, during a period of intense magnetic activity. (*) Ulysses is a joint ESA/NASA mission. ESA developed the probe and is contributing an estimated ECU 170 million up to 1995 to its in-fl operation. European research laboratories provided half of the scie instruments. NASA provided the other half of the experiments flown a radio-isotopic power generator and the launch; it is also maintain day-to-day communications with the probe via its dedicated antennas.

  14. The GLOBE International Scientist Network: Connecting Scientists and Schools to Promote Earth System Science

    NASA Astrophysics Data System (ADS)

    Tessendorf, S. A.; Andersen, T.; Mackaro, J.; Malmberg, J.; Randolph, J. G.; Wegner, K.

    2012-12-01

    The GLOBE Program has a rich history of connecting scientists and schools around the world on issues related to Earth System Science. Science teams developed the program's core science protocols, and these and other scientists use the data collected by GLOBE students, following these protocols, in their research projects. GLOBE is an international science and education program working with scientists, teachers, and students in over 110 countries around the world. GLOBE has recently initiated a focus on climate science, as well as unveiled a new technological infrastructure (website, database, online collaboration tools, etc.). These recent technological advances provide new opportunities to increase scientist participation in the program. To better facilitate scientist involvement in GLOBE, The GLOBE International Scientist Network (GISN) was developed. This network aims to connect scientists, teachers, and students around the world to promote Earth System Science. It provides a venue for scientists seeking to engage in education and outreach to connect with schools willing to collaborate, as well as to connect with one another. Via the GLOBE website, scientists in the GISN are provided a profile page to display their bio and interests, the ability to make online "friends" thereby connecting with other registered GLOBE community members (i.e. scientists, teachers), and the ability to participate in online discussions. All interested candidates' credentials are reviewed to ensure that they meet designated criteria to maintain the quality of individuals who work with GLOBE schools. The GLOBE Program Office staff scientists facilitate the network, by creating online accounts for approved new members and responding to inquiries. This presentation will provide an overview of the GISN, including how the network is maintained, the process for membership approval, and a few examples of how scientists in the network are working with GLOBE.

  15. A Great Basin-wide dry episode during the first half of the Mystery Interval? Wallace S. Broecker a,*, David McGee a

    E-print Network

    McGee, David

    A Great Basin-wide dry episode during the first half of the Mystery Interval? Wallace S. Broecker a that the deglacial Mystery Interval (14.5­12.4 14 C kyrs) has two distinct hydrologic parts in the western USA of the Mystery Interval were triggered by the IRD event recorded off Portugal at about 13.8 14 C kyrs which post

  16. Solving Sudoku with Constraint Programming

    NASA Astrophysics Data System (ADS)

    Crawford, Broderick; Castro, Carlos; Monfroy, Eric

    Constraint Programming (CP) is a powerful paradigm for modeling and solving Complex Combinatorial Problems (generally issued from Decision Making). In this work, we model the known Sudoku puzzle as a Constraint Satisfaction Problems and solve it with CP comparing the performance of different Variable and Value Selection Heuristics in its Enumeration phase. We encourage this kind of benchmark problem because it may suggest new techniques in constraint modeling and solving of complex systems, or aid the understanding of its main advantages and limits.

  17. Measuring Family Problem Solving: The Family Problem Solving Diary.

    ERIC Educational Resources Information Center

    Kieren, Dianne K.

    The development and use of the family problem-solving diary are described. The diary is one of several indicators and measures of family problem-solving behavior. It provides a record of each person's perception of day-to-day family problems (what the problem concerns, what happened, who got involved, what those involved did, how the problem…

  18. Ettore Majorana: The scientist and the man

    NASA Astrophysics Data System (ADS)

    Recami, Erasmo

    2014-12-01

    Ettore Majorana was the brightest Italian theoretical physicist of the XX century (actually, Enrico Fermi regarded him as the brightest in the world of his time, and compared him to Galileo and Newton), even if to some people Majorana is often known mainly for his mysterious disappearance, in 1938, when he was 31. In this paper, we present a panoramic view of the main scientific articles published by him, as well as their significance. We also briefly outline his life, the biographical data being based on letters, documents, testimonies discovered or collected by the author during more than four decades, and contained since 1986 in Recami's book quoted in the text. Finally, extensive information and comments are added with regard to the scientific manuscripts left unpublished by Majorana. Two pictures complete the paper.

  19. Venus's Mysterious "Aurora" Candace Gray (candaceg@nmsu.edu), Nancy Chanover, Tom Slanger, Karan

    E-print Network

    Rathbun, Julie A.

    Venus's Mysterious "Aurora" Candace Gray (candaceg@nmsu.edu), Nancy Chanover, Tom Slanger, Karan/09/2015 The Earth posses a magnetic field which funnels solar charged particles to the poles, generating aurora. The brightest aurora on Earth is the oxygen green line at 5577 Å. Venus has no magnetic field

  20. Tragic Accidents or Mysterious Murders?: A College Town Struggles to Frame Responsibility for River Drowning Deaths

    ERIC Educational Resources Information Center

    Swanson, Douglas J.

    2006-01-01

    This paper focuses on an ongoing debate in La Crosse, Wisconsin, over recent river drowning incidents involving college-aged men. While some in the community contend the deaths were tragic but unrelated, other citizens argue that the collective set of circumstances points to a series of mysterious murders--perhaps committed by a "River Killer"…

  1. Mystics in Antiquity !!"The design of the Mysteries is to lead

    E-print Network

    MacLennan, Bruce

    among men who, after beholding these rites, go down to Hades. Only for them is there life; all the rest;!! Initiation per se !! Agrarian aspect !! Sexual aspects !! Sacred myths !! Overcoming death #12;!! Mystery a particular figure or object" -- Am. Her. Dict.) #12;!! Neolithic basis !! Problem of personal fate after

  2. The Bardic Mystery and the Dew Drop in the Rose: The Poet in the Therapeutic Process.

    ERIC Educational Resources Information Center

    Reed, M. Ann

    1992-01-01

    Discusses the ancient "Bardic Mystery" and its descent into the body to let an old Self die. Analyzes the poetry of three contemporary poets to provide substantial support for the role of the poet in the therapeutic process. Connects self-discovery, transformation, and communal awareness to the healing aspects of the lyric, epic, and dramatic…

  3. Out of the Mouths of Babes: Unlocking the Mysteries of Language and Voice.

    ERIC Educational Resources Information Center

    Thurber, Christopher A.

    2003-01-01

    Summarizes three studies that have revolutionized child psychology by teaching us that children are biologically programmed to learn language; children's language development is orderly and pragmatic, but grammatically mysterious; and children's linguistic self-expression reveals some disturbing ways in which they have been socialized. Presents…

  4. Mystery of Vacuum Energy or Rise and Fall of Cosmological Constant

    E-print Network

    A. D. Dolgov

    2002-03-26

    Two sides of cosmological constant problem are discussed: a mysterious compensation of all contributions to vacuum energy with the accuracy of 100-50 orders of magnitude and a surprising equality of a constant vacuum energy density to the present-day value of time dependent cosmological energy density.

  5. The mystery of. sigma. (700)-meson exchange in. gamma. gamma. yields. pi. pi. processes

    SciTech Connect

    Ivanov, A.N.; Troitskaya, N.I. ); Nagy, M. )

    1992-07-20

    In this paper the problem of the mystery of the {sigma} (700)-meson contribution to the {gamma}, {gamma} {yields} {pi}, {pi} {gamma}, {gamma} {yields} K{bar K} scattering amplitudes at low energies is studied at the quark level within a soft-pion-constituent-quark diagram technique. The Terent'ev low-energy theorem is derived at the quark level.

  6. The Mysterious Death: An HPLC Lab Experiment. An Undergraduate Forensic Lab

    ERIC Educational Resources Information Center

    Beussman, Douglas J.

    2007-01-01

    A high-performance liquid chromatography (HPLC) laboratory experiment based on the separation of four prescription drugs (disopyramide, lidocaine, procainamide, and quinidine) is presented. The experiment is set within the forensic science context of the discovery of a patient's mysterious death where a drug overdose is suspected. Each lab group…

  7. FUNCTIONAL COMPLEXITY FAILURES AND AUTOMATION SURPRISES: THE MYSTERIOUS CASE OF CONTROLLED FLIGHT INTO STALL (CFIS)

    E-print Network

    on the flight deck of relevant information and salient cues to monitor these rare events or their effects. Third, there was no single intervention that could mitigate all of these accidents. Implications for flight deck procedures1 FUNCTIONAL COMPLEXITY FAILURES AND AUTOMATION SURPRISES: THE MYSTERIOUS CASE OF CONTROLLED FLIGHT

  8. www.geotimes.org34 Geotimes July 2007 Much of the mystery remains

    E-print Network

    van der Hilst, Robert Dirk

    that the interior layers of Earth are heterogeneous at all scales. There is much we do not know about the strucwww.geotimes.org34 Geotimes July 2007 Much of the mystery remains because direct sampling of Earth from deeper than 150 kilometers (93 miles). Such tiny distances are dwarfed by Earth's actual

  9. Why AIDS? The Mystery of How HIV Attacks the Immune System.

    ERIC Educational Resources Information Center

    Christensen, Damaris

    1999-01-01

    Reviews differing theories surrounding the mystery of how human immunodeficiency virus (HIV) attacks the immune system. Claims that understanding how HIV triggers immune-cell depletion may enable researchers to block its effects. New knowledge could reveal strategies for acquired immune deficiency syndrome (AIDS) therapies that go beyond the drugs…

  10. Totally tubular: the mystery behind function and origin of the brain ventricular system

    E-print Network

    Lowery, Laura Anne

    into the hematopoietic circulatory and lymphatic systems.(1) Control of CSF flow is thought to originate in pressureTotally tubular: the mystery behind function and origin of the brain ventricular system Laura Anne system, a series of connected cavities which are filled with cerebrospinal fluid (CSF) and surrounded

  11. Roy J. Snell is Author of 76 Mystery Stories For Boys By Lowell Saunders

    E-print Network

    Rockmore, Dan

    Roy J. Snell is Author of 76 Mystery Stories For Boys By Lowell Saunders Wheaton College Journalism to see who would take over the school--the big boys or me." Snell won and gained the respect of his Armstrong--The All American Boy." At the special request of his publisher, he wrote eight war novels

  12. Population estimate of Chinese mystery snail (Bellamya chinensis) in a Nebraska reservoir

    USGS Publications Warehouse

    Chaine, Noelle M.; Allen, Craig R.; Fricke, Kent A.; Haak, Danielle M.; Hellman, Michelle L.; Kill, Robert A.; Nemec, Kristine T.; Pope, Kevin L.; Smeenk, Nicholas A.; Stephen, Bruce J.; Uden, Daniel R.; Unstad, Kody M.; VanderHam, Ashley E.

    2012-01-01

    The Chinese mystery snail (Bellamya chinensis) is an aquatic invasive species in North America. Little is known regarding this species' impacts on freshwater ecosystems. It is be lieved that population densities can be high, yet no population estimates have been reported. We utilized a mark-recapture approach to generate a population estimate for Chinese mystery snail in Wild Plum Lake, a 6.47-ha reservoir in southeast Nebraska. We calculated, using bias-adjusted Lincoln-Petersen estimation, that there were approximately 664 adult snails within a 127 m2 transect (5.2 snails/m2). If this density was consistent throughout the littoral zone (<3 m in depth) of the reservoir, then the total adult population in this impoundment is estimated to be 253,570 snails, and the total Chinese mystery snail wet biomass is estimated to be 3,119 kg (643 kg/ha). If this density is confined to the depth sampled in this study (1.46 m), then the adult population is estimated to be 169,400 snails, and wet biomass is estimated to be 2,084 kg (643 kg/ha). Additional research is warranted to further test the utility of mark-recapture methods for aquatic snails and to better understand Chinese mystery snail distributions within reservoirs.

  13. Change and Mystery: The Grist of How's and Why's in Inquiry Indicator Chemistry

    ERIC Educational Resources Information Center

    Schlenker, Richard M.; Petrichenko, Oksana Y.

    2006-01-01

    In this activity, students mix mystery chemicals in a freezer bag to produce reactions that are unexpected. As a result, one chemical seems to disappear, the bag expands, and then the bag turns hot and cold. Participants then ask questions and design their own activities to answer their self-generated questions. The research cycle continues until…

  14. Women of Mystery: Investigating Learning Pathways of Canadian and American Female Crime Fiction Writers

    ERIC Educational Resources Information Center

    Gouthro, Patricia A.

    2014-01-01

    This article explores the learning pathways of 15 Canadian and American female crime fiction authors. Using a critical feminist perspective, it argues that despite the neoliberal rhetoric of individual choice, as in most careers, there are social-structural factors that create opportunities and barriers for women mystery writers. The article…

  15. August 27, 2013 Mysterious decline in quail population prompts the largest research project of its kind.

    E-print Network

    Rock, Chris

    August 27, 2013 Mysterious decline in quail population prompts the largest research project of its rough terrain in search of the elusive bird. Rolling Plains Quail Research Ranch (Photo courtesy quail ranch in Stonewall County , Rick Snipes starts out seeking the familiar and iconic bird call

  16. NE OF THE GREAT MYSTERIES of the human brain is how it understands and produces language.

    E-print Network

    Bellugi, Ursula

    O NE OF THE GREAT MYSTERIES of the human brain is how it understands and produces language. Until HOW DOES THE HUMAN BRAIN PROCESS LANGUAGE? NEW STUDIES OF DEAF SIGNERS HINT AT AN ANSWER COPYRIGHT have illuminated the workings of the human brain and may help neurologists treat the ills of their deaf

  17. Case Study: The Mystery of the Seven Deaths--A Case Study in Cellular Respiration

    ERIC Educational Resources Information Center

    Gazdik, Michaela

    2014-01-01

    Cellular respiration, the central component of cellular metabolism, can be a difficult concept for many students to fully understand. In this interrupted, problem-based case study, students explore the purpose of cellular respiration as they play the role of medical examiner, analyzing autopsy evidence to determine the mysterious cause of death…

  18. Did Kanner Actually Describe the First Account of Autism? The Mystery of 1938

    ERIC Educational Resources Information Center

    Fellowes, Sam

    2015-01-01

    Kanner opens his pioneering 1943 paper on autism by making a mysterious mention of the year 1938. Recent letters to the editor of this journal have disagreed over a particular interpretation--does 1938 refer to an early paper by Asperger, effectively meaning Kanner plagiarised Asperger? I argue 1938 refers to a paper by Louise Despert. This was…

  19. Scientists and Educators Working Together: Everyone Teaches, Everyone Learns

    NASA Astrophysics Data System (ADS)

    Lebofsky, Larry A.; Lebofsky, N. R.; McCarthy, D. W.; Canizo, T. L.; Schmitt, W.; Higgins, M. L.

    2013-10-01

    The primary author has been working with three of the authors (Lebofsky, McCarthy, and Cañizo) for nearly 25 years and Schmitt and Higgins for 17 and 8 years, respectively. This collaboration can be summed up with the phrase: “everyone teaches, everyone learns.” What NASA calls E/PO and educators call STEM/STEAM, requires a team effort. Exploration of the Solar System and beyond is a team effort, from research programs to space missions. The same is true for science education. Research scientists with a long-term involvement in science education have come together with science educators, classroom teachers, and informal science educators to create a powerful STEM education team. Scientists provide the science content and act as role models. Science educators provide the pedagogy and are the bridge between the scientists and the teacher. Classroom teachers and informal science educators bring their real-life experiences working in classrooms and in informal settings and can demonstrate scientists’ approaches to problem solving and make curriculum more engaging. Together, we provide activities that are grade-level appropriate, inquiry-based, tied to the literacy, math, and science standards, and connected directly to up-to-date science content and ongoing research. Our programs have included astronomy camps for youth and adults, professional development for teachers, in-school and after-school programs, family science events, and programs in libraries, science centers, and museums. What lessons have we learned? We are all professionals and can learn from each other. By engaging kids and having them participate in activities and ask questions, we can empower them to be the presenters for others, even their families. The activities highlighted on our poster represent programs and collaborations that date back more than two decades: Use models and engage the audience, do not just lecture. Connect the activity with ongoing science and get participants outside to look at the real sky: do a Moon journal, measure shadows, observe constellations, and look through a telescope—the sky is more than just string, balls, or a computer program.

  20. From Science to Business: Preparing Female Scientists and Engineers for Successful Transitions into Entrepreneurship--Summary of a Workshop

    ERIC Educational Resources Information Center

    Didion, Catherine Jay; Guenther, Rita S.; Gunderson, Victoria

    2012-01-01

    Scientists, engineers, and medical professionals play a vital role in building the 21st- century science and technology enterprises that will create solutions and jobs critical to solving the large, complex, and interdisciplinary problems faced by society: problems in energy, sustainability, the environment, water, food, disease, and healthcare.…

  1. The Lord of Rings - the mysterious case of the stolen rings: a critical analysis of an informal education activity

    NASA Astrophysics Data System (ADS)

    Sandrelli, S.

    2011-10-01

    "The Lord of Rings - the mysterious case of the stolen rings" is a live astronomical role-playing game for kids aged 10 -13 [1]. Its goal is to introduce them to some of the main topics of the Solar System: a) the role of gravity; b) the distribution of mass & light; c) the effects of rotation; d) the distribution of water. The game was held at several Science Festival in Italy (Perugia, Genova, Fiorano, Bologna) obtaining great success. Teams of about 6-8 members are introduced to Mr Schioppanelli, the astro-detective of the town (the name is a pun: it reminds Schiaparelli, the famous italian astronomer, and it is a slang expression meaning "ring-breaker"). Mr Schioppanelli has his office in an "gastronomical astronomical observatory", known as The Red Giant Pizzeria. Schioppanelli informs the kids that a mysterious Centaur succeded in stealing the rings of Saturn. The partecipants are appointed astro-detectives incharge and asked to find the rings by browsing around the Solar System, which is scaled so as to fit the town historical centre or a pedestrian area, going from the Sun to Saturn or beyond, depending on the actual area at disposal. Great care must be taken allowing children playing only in a car-free area of the town. At the right scaled distances, the partecipants meet characters playing as the various planets. The kids can talk to them after solving a riddle, obtaining useful informations. A special characters play as a comet, timely going in and out of the inner solar system. The teams can also talk to some shepherdmoons of the rings. They easily discover that the rings were totally destroyed by the Centaur: a real disaster! They are also suggested to gather the necessary ingredients (gravity, light, rotation, inclination, dust and water, represented by simple objects like apples, spinning tops and so on) to rebuild the rings. The kids can buy the ingredients from different planets: every planet has ingredients in quantities which are proportionate to the real physical properties of that celestial object. After collecting the ingredients, they must carry them to the "The Red Giant" and indicate their best recipe to Mr Schioppanelli. Depending on the recipe, rings can be too strict or too luminous or too fast rotating and so on. The winning group is the one which prepares the best recipe to cook the rings in the smallest amount of time. After introducing this specific (and mysterious) game, we analyze the advantage-disadvantage ratio of such an activity, which is as funny as dispersive [2]. The key expression of the whole activity is, of course, "informal education". But, as a best practice result, we organize also 1 or 2 very simple laboratories about the solar system before playing the game. One of these, called The Olmicomics, allows the pupils to understand the dimensions of the planets with respect to their distances, providing them the correct introduction to "The Lord of Rings". The pupils are simply requested to pone the planets in a correct scale on a map of the city where they live. Then we coherently calculate together dimension of the Solar System planets and the Sun, according to the scale they chose. The second activity provide the pupils hints about the physical properties of the planets, touching the points a)-d) listed above. We believe this two-faces strategy is a quite effective tool for an education suited to our target group. They really do things, touch things, use their own body as a meter to understand distances and physical properties as the gravitational force. In the meanwhile, they are also asked to think about what they are doing, to make calculation and to build a representation of the Solar System by numbers, turning it into a visual representation only after their calculation. And, finally, to play with all these conceipts.

  2. Introducing New Scientists 2012 Introducing New Scientists 2012 is published by

    E-print Network

    . Approximately 40 reached retirement age in the past five years and have been succeeded by 43 new hires.One of the most notable developments this year is that we recruited three young scientists whose focus is earth and planetary sciences,whose research is helping inform understanding of life on Earth.To help a scientist come

  3. How to Grow Project Scientists: A Systematic Approach to Developing Project Scientists

    NASA Technical Reports Server (NTRS)

    Kea, Howard

    2011-01-01

    The Project Manager is one of the key individuals that can determine the success or failure of a project. NASA is fully committed to the training and development of Project Managers across the agency to ensure that highly capable individuals are equipped with the competencies and experience to successfully lead a project. An equally critical position is that of the Project Scientist. The Project Scientist provides the scientific leadership necessary for the scientific success of a project by insuring that the mission meets or exceeds the scientific requirements. Traditionally, NASA Goddard project scientists were appointed and approved by the Center Science Director based on their knowledge, experience, and other qualifications. However the process to obtain the necessary knowledge, skills and abilities was not documented or done in a systematic way. NASA Goddard's current Science Director, Nicholas White saw the need to create a pipeline for developing new projects scientists, and appointed a team to develop a process for training potential project scientists. The team members were Dr. Harley Thronson, Chair, Dr. Howard Kea, Mr. Mark Goldman, DACUM facilitator and the late Dr. Michael VanSteenberg. The DACUM process, an occupational analysis and evaluation system, was used to produce a picture of the project scientist's duties, tasks, knowledge, and skills. The output resulted in a 3-Day introductory course detailing all the required knowledge, skills and abilities a scientist must develop over time to be qualified for selections as a Project Scientist.

  4. Images of Science and Scientists: A Study of School Teachers' Views. I. Characteristics of Scientists.

    ERIC Educational Resources Information Center

    Rampal, A.

    1992-01-01

    Examines trends in teachers' beliefs about scientists and the nature of science. Discusses teachers' questionnaire responses on the following qualities of scientists: minimum educational qualifications; creativity; temperament; stereotyped image; and personal beliefs about indigenous systems of medicine and astrology. (Contains 63 references.)…

  5. Extraordinary Cosmic Laboratory Helps Unravel Mysteries of a Galaxy's Powerful Central "Engine"

    NASA Astrophysics Data System (ADS)

    An extraordinary cosmic laboratory 21 million light-years away is providing radio astronomers their best opportunity yet to decipher the mysteries of the ultra-powerful "engines" at the hearts of many galaxies and quasars. An international research team using the National Science Foundation's Very Long Baseline Array (VLBA) and Very Large Array (VLA) radio telescopes has peered deeply into the core of the galaxy NGC 4258, learning important new information about the mysterious region from which high-speed jets of subatomic particles are ejected. The scientists announced their findings today at the American Astronomical Society meeting in Toronto, Ontario. The new research provides significant quantitative support for a theoretical model for the origin of such jets first proposed in 1979. NGC 4258 is the galaxy in which a warped disk of water molecules was discovered in 1994. That disk, observed in detail with the VLBA, was shown to be orbiting a central mass some 35 million times more massive than the Sun. That central mass, the astronomers believe, is a black hole. More recent studies of the disk and its surroundings have given astronomers their most detailed look yet at the heart of an active galactic nucleus (AGN), including the ability to pinpoint the exact center of the system, where the black hole resides. The 1994 observations provided the best evidence to date for the existence of a black hole at the heart of a galaxy. Black holes, so dense that not even light can escape their gravitational fields, have long been suspected as the driving force behind the energetic central engines of AGNs. The fortuitous existence of the molecular disk in NGC 4258 has helped astronomers use the ultrasharp radio "vision" of the continent-wide VLBA to probe with unprecedented clarity into the heart of that galaxy's central engine. The researchers are: James Herrnstein, James Moran, and Lincoln Greenhill of the Harvard-Smithsonian Center for Astrophysics; Philip Diamond of the National Radio Astronomy Observatory in Socorro, NM; Mikoto Miyoshi of Japan's Misusawa Astrogeodynamics Observatory; and Naomasa Nakai and Makoto Inoue of Japan's Nobeyama Radio Observatory. The work formed the basis of Herrnstein's Ph.D. dissertation at Harvard University. The extraordinary detail of the observations is made possible by the fact that the water molecules in the disk orbiting the black hole are amplifying microwave radio emissions in the same manner that a laser amplifies light. These natural amplifiers are called cosmic masers, and they produce bright targets for radio telescopes. Study of water masers at the center of NGC 4258 is what revealed the orbiting disk in 1994. Further studies of the water masers in NGC 4258 now have allowed the research team to deduce the exact location of the object orbited by the disk. In addition, new observations of the galaxy's center show radio emission the astronomers believe traces the inner parts of the high-speed jets. Combined, these new observations allow measurement of the distance between the black hole and the innermost observable portions of the jets. Such measurement is extremely important, because the standard theoretical model, proposed in 1979 by Roger Blandford of Caltech and Arieh Konigl of the University of Chicago, makes a clear prediction that all detected radio emission will be offset from the central engine generating the jets. The new radio observations of NGC 4258 are the first to show the exact location of the core of an AGN, and thus the first to allow measurement of the offset between the core and the detected emission closest to it. Significantly, the offset measured in NGC 4258 is fully consistent with the quantitative prediction made by the model of Blandford and Konigl. "There has been a lot of speculation about the relationship between radio jets and black holes over the years," said Herrnstein. "But this measurement precisely pins down the geometric relationship between them in this object." In addition to these measurements, the research

  6. Difficulties in Genetics Problem Solving.

    ERIC Educational Resources Information Center

    Tolman, Richard R.

    1982-01-01

    Examined problem-solving strategies of 30 high school students as they solved genetics problems. Proposes a new sequence of teaching genetics based on results: meiosis, sex chromosomes, sex determination, sex-linked traits, monohybrid and dihybrid crosses (humans), codominance (humans), and Mendel's pea experiments. (JN)

  7. Learning Impasses in Problem Solving

    NASA Technical Reports Server (NTRS)

    Hodgson, J. P. E.

    1992-01-01

    Problem Solving systems customarily use backtracking to deal with obstacles that they encounter in the course of trying to solve a problem. This paper outlines an approach in which the possible obstacles are investigated prior to the search for a solution. This provides a solution strategy that avoids backtracking.

  8. The Future Problem Solving Program.

    ERIC Educational Resources Information Center

    Crabbe, Anne B.

    1989-01-01

    Describes the Future Problem Solving Program, in which students from the U.S. and around the world are tackling some complex challenges facing society, ranging from acid rain to terrorism. The program uses a creative problem solving process developed for business and industry. A sixth-grade toxic waste cleanup project illustrates the process.…

  9. Creative Thinking and Problem Solving.

    ERIC Educational Resources Information Center

    Lacy, Grace

    The booklet considers the nature of creativity in children and examines classroom implications. Among the topics addressed are the following: theories about creativity; research; developments in brain research; the creative process; creative problem solving; the Structure of Intellect Problem Solving (SIPS) model; a rationale for creativity in the…

  10. Problem Solving vis Soap Bubbles

    ERIC Educational Resources Information Center

    Bader, William A.

    1975-01-01

    Describes the use of a scientific phenomenon related to the concept of surface tension as an intriguing vehicle to direct attention to useful problem solving techniques. The need for a definite building process in attempts to solve mathematical problems is stressed. (EB)

  11. Multiple Ways to Solve Proportions

    ERIC Educational Resources Information Center

    Ercole, Leslie K.; Frantz, Marny; Ashline, George

    2011-01-01

    When solving problems involving proportions, students may intuitively draw on strategies that connect to their understanding of fractions, decimals, and percents. These two statements--"Instruction in solving proportions should include methods that have a strong intuitive basis" and "Teachers should begin instruction with more intuitive…

  12. The Evolution of the Data Scientist.

    NASA Astrophysics Data System (ADS)

    Parsons, M. A.

    2011-12-01

    When did the data scientist come into being? The National Science Board formally defined the term in 2005. Prior to that, the term was used sporadically, but typically to refer to statisticians or analysts. Nevertheless, the data scientist function has existed for a long time. Those who performed the function were called data managers or librarians or curators. Their role with digital data was critical but ill defined and poorly understood, especially by outsiders. Today, the tem data scientist is gaining currency and the discipline is gaining prominence, but it is a very dynamic field. And while it may be better defined, the term is still poorly understood. This lack of understanding can partly be attributed to the dynamic and evolutionary nature of the field. Domain scientists have developed new expectations for technology and services that enhance their ability to handle massive and complex data and present new challenges to data scientists. In response, data scientists are redefining and adapting their role to these rapidly changing demands of data-driven science and the fourth paradigm. In this paper, I explore the recent evolution of the field of data science as a socio-technical discipline. I discuss what has changed as well as what has remained the same and how some things that seem new may be a recasting of old problems. I take the view that data science is necessarily an evolutionary field that will need to continue to adapt in response to known and unknown challenges in order to ensure a healthy data ecosystem.

  13. AGU Hosts Networking Event for Female Scientists

    NASA Astrophysics Data System (ADS)

    McEntee, Chris

    2013-01-01

    At Fall Meeting this year I had the pleasure of cohosting a new event, a Networking Reception for Early Career Female Scientists and Students, with Jane Lubchenco, under secretary of Commerce for Oceans and Atmosphere and National Oceanic and Atmospheric Administration administrator, and Marcia McNutt, director of the U.S. Geological Survey. AGU recognizes the importance of having a diverse pool of new researchers who can enrich Earth and space sciences with their skills and innovation. That's why one of our four strategic goals is to help build the global talent pool and provide early-career scientists with networking opportunities like this one.

  14. Media and the making of scientists

    NASA Astrophysics Data System (ADS)

    O'Keeffe, Moira

    This dissertation explores how scientists and science students respond to fictional, visual media about science. I consider how scientists think about images of science in relation to their own career paths from childhood onwards. I am especially interested in the possibility that entertainment media can inspire young people to learn about science. Such inspiration is badly needed, as schools are failing to provide it. Science education in the United States is in a state of crisis. Studies repeatedly find low levels of science literacy in the U.S. This bleak situation exists during a boom in the popularity of science-oriented television shows and science fiction movies. How might entertainment media play a role in helping young people engage with science? To grapple with these questions, I interviewed a total of fifty scientists and students interested in science careers, representing a variety of scientific fields and demographic backgrounds, and with varying levels of interest in science fiction. Most respondents described becoming attracted to the sciences at a young age, and many were able to identify specific sources for this interest. The fact that interest in the sciences begins early in life, demonstrates a potentially important role for fictional media in the process of inspiration, perhaps especially for children without access to real-life scientists. One key aspect to the appeal of fiction about science is how scientists are portrayed as characters. Scientists from groups traditionally under-represented in the sciences often sought out fictional characters with whom they could identify, and viewers from all backgrounds preferred well-rounded characters to the extreme stereotypes of mad or dorky scientists. Genre is another aspect of appeal. Some respondents identified a specific role for science fiction: conveying a sense of wonder. Visual media introduce viewers to the beauty of science. Special effects, in particular, allow viewers to explore the unknown. Advocates of informal science learning initiatives suggest that media can be used as a tool for teaching science content. The potential of entertainment media to provide a sense of wonder is a powerful aspect of its potential to inspire the next generation of scientists.

  15. Perspectives on Being a Data Scientist (Invited)

    NASA Astrophysics Data System (ADS)

    Narock, T. W.

    2013-12-01

    Advances in computation and data management are fundamentally changing the way geoscience research is undertaken. However, to effectively utilize these advances scientific teams must be skilled in multiple areas and have a high degree of computer literacy. The 'data scientist', a new breed of researcher that has skills in the science fundamentals as well as the computational and data sciences, can help bridge this gap. I present my own experiences in becoming a 'data scientist' highlighting what's working and what's not working in making data science routine. Additionally, I will show examples of geoscience advances made via data science collaborations.

  16. "Physics and Life" - Teachers Meet Scientists at Major EIROforum Event [

    NASA Astrophysics Data System (ADS)

    2003-11-01

    More than 400 selected delegates from 22 European countries will take part in "Physics on Stage 3" , organised by the EIROforum [1] research organisations (CERN, EFDA, EMBL, ESA, ESO, ESRF, ILL) at the ESA ESTEC site (Noordwijk, The Netherlands). It is the culmination of a year-long educational programme and is a central event during the EC-sponsored European Science and Technology Week (November 8-15, 2003). Following the vastly successful preceeding events in 2000 and 2002, the main theme this year is "Physics and Life", reflecting the decision to broaden the Physics on Stage activities to encompass more of the natural sciences within an interdisciplinary approach. As before, European teachers, scientists, curricula organisers and others connected to the national education systems in Europe will gather with the main goal of exploring solutions to stimulate the interest of young people in science, by means of exciting and innovative teaching methods and materials. The rich one-week programme has many components: spectacular and original performances by students and professional actors, intensive encounters at a central fair where each country will present the latest developments from its teaching community at their stands, workshops about a host of crucial themes related to the central mission of this programme, seminars where EIROforum scientists and experienced high school teachers get together to discuss new teaching opportunities based on the latest results from front-line research projects at Europe's leading science centres, as well as a publishers fair that will also serve as an international exchange for new educational materials. A mystery cultural event will surprise everyone with its originality. And last but not least, the annual European Science Teaching Awards - the highest distinction in this field - will be presented at the end of the meeting. "Physics on Stage" is a joint project organised by EIROforum, together with the European Physical Society (EPS) and the European Association for Astronomy Education (EAAE) . The project is funded in part by the European Commission and takes place under the auspices of the European Science and Technology Week 2003. It is directed by the EIROforum Working Group on Outreach that brings together key members of the seven organisations' respective outreach departments. The "Physics on Stage 3" festival will be opened on Monday, November 10, by His Royal Highness, Prince Johan Friso of the Netherlands. Among the distinguished guests will also be Her Excellency, Mrs. Maria van der Hoeven, the Dutch Minister of Education, Culture and Science, as well as several Directors-General of the EIROforum organisations. This "Physics on Stage 3" festival is the most visible event within a year-long programme with the very active involvement of National Committees in two dozen European countries, each of which organised national events or competitions, during which the 400 delegates to the festival were selected for their outstanding projects to promote science teaching. Among the many entries, for example, two young physicists from Germany focus on the beauty of physical phenomena, producing fractals and demonstrating the "Theremin", the only musical instrument played without being touched. In another demonstration, a team from the UK explore the nature of sound and the theme of genetics through drama, music and physical theatre. In this third international festival of physics education, biological and biochemical themes will also play a major role. As usual, the colourful centrepiece of the week is the Fair. Every country has its own stand where delegates show their new, exciting and surprising projects, innovative software, elegant experiments, etc. In this highly inspiring atmosphere, the teachers exchange practical experience and insights, learning from each other and preparing themselves to bring back to their respective countries a rich harvest of new ideas and inspiration for better teaching of science. "Physics

  17. Dr. Jeremy Martin Senior Scientist, Clean Vehicles Program

    E-print Network

    Firestone, Jeremy

    Dr. Jeremy Martin Senior Scientist, Clean Vehicles Program Union of Concerned Scientists Jeremy Martin, Senior Scientist in the Union of Concerned Scientists' Clean Vehicles Program, evaluates the impact of biofuels and fuel policy. Dr. Martin is the author of more than 15 technical publications

  18. Determining the Effectiveness of Prompts for Self-Regulated Learning in Problem-Solving Scenarios

    ERIC Educational Resources Information Center

    Ifenthaler, Dirk

    2012-01-01

    Cognitive scientists have studied internal cognitive structures, processes, and systems for decades in order to understand how they function in human learning. In order to solve challenging tasks in problem situations, learners not only have to perform cognitive activities, e.g., activating existing cognitive structures or organizing new…

  19. Studying PubMed usages in the field for complex problem solving: Implications for tool design

    PubMed Central

    Song, Jean; Tonks, Jennifer Steiner; Meng, Fan; Xuan, Weijian; Ameziane, Rafiqa

    2012-01-01

    Many recent studies on MEDLINE-based information seeking have shed light on scientists’ behaviors and associated tool innovations that may improve efficiency and effectiveness. Few if any studies, however, examine scientists’ problem-solving uses of PubMed in actual contexts of work and corresponding needs for better tool support. Addressing this gap, we conducted a field study of novice scientists (14 upper level undergraduate majors in molecular biology) as they engaged in a problem solving activity with PubMed in a laboratory setting. Findings reveal many common stages and patterns of information seeking across users as well as variations, especially variations in cognitive search styles. Based on findings, we suggest tool improvements that both confirm and qualify many results found in other recent studies. Our findings highlight the need to use results from context-rich studies to inform decisions in tool design about when to offer improved features to users. PMID:24376375

  20. Studying PubMed usages in the field for complex problem solving: Implications for tool design.

    PubMed

    Mirel, Barbara; Song, Jean; Tonks, Jennifer Steiner; Meng, Fan; Xuan, Weijian; Ameziane, Rafiqa

    2013-05-01

    Many recent studies on MEDLINE-based information seeking have shed light on scientists' behaviors and associated tool innovations that may improve efficiency and effectiveness. Few if any studies, however, examine scientists' problem-solving uses of PubMed in actual contexts of work and corresponding needs for better tool support. Addressing this gap, we conducted a field study of novice scientists (14 upper level undergraduate majors in molecular biology) as they engaged in a problem solving activity with PubMed in a laboratory setting. Findings reveal many common stages and patterns of information seeking across users as well as variations, especially variations in cognitive search styles. Based on findings, we suggest tool improvements that both confirm and qualify many results found in other recent studies. Our findings highlight the need to use results from context-rich studies to inform decisions in tool design about when to offer improved features to users. PMID:24376375

  1. Scientists Release Altantic Salmon into Beaverdam Brook

    USGS Multimedia Gallery

    USGS Tunison Lab scientists Rich Chiavelli (left) and Emily Waldt (middle) hand a bucketful of young Atlantic salmon to Dan Bishop (right) of the New York State Department of Environmental Conservation for release into Beaverdam Brook at the state's Salmon River Fish Hatchery. Thousands of you...

  2. Scientists Release Altantic Salmon into Beaverdam Brook

    USGS Multimedia Gallery

    USGS Tunison Lab scientist Emily Waldt (right) assists Dan Bishop of the New York State Department of Environmental Conservation in releasing Atlantic salmon into Beaverdam Brook at the state's Salmon River Fish Hatchery. Thousands of young Atlantic salmon are being release...

  3. Scientist Researches Way to Reduce Global Warming

    Technology Transfer Automated Retrieval System (TEKTRAN)

    For the last four years, scientists at the USDA, Agricultural Research Service, Northern Plains Agricultural Research Laboratory have been searching for alternative soil and crop management practices to reduce greenhouse gas emissions and increase carbon and nitrogen sequestration. “If we can redu...

  4. Scientists' internal models of the greenhouse effect

    NASA Astrophysics Data System (ADS)

    Libarkin, J. C.; Miller, H.; Thomas, S. R.

    2013-12-01

    A prior study utilized exploratory factor analysis to identify models underlying drawings of the greenhouse effect made by entering university freshmen. This analysis identified four archetype models of the greenhouse effect that appear within the college enrolling population. The current study collected drawings made by 144 geoscientists, from undergraduate geoscience majors through professionals. These participants scored highly on a standardized assessment of climate change understanding and expressed confidence in their understanding; many also indicated that they teach climate change in their courses. Although geoscientists held slightly more sophisticated greenhouse effect models than entering freshmen, very few held complete, explanatory models. As with freshmen, many scientists (44%) depict greenhouse gases in a layer in the atmosphere; 52% of participants depicted this or another layer as a physical barrier to escaping energy. In addition, 32% of participants indicated that incoming light from the Sun remains unchanged at Earth's surface, in alignment with a common model held by students. Finally, 3-20% of scientists depicted physical greenhouses, ozone, or holes in the atmosphere, all of which correspond to non-explanatory models commonly seen within students and represented in popular literature. For many scientists, incomplete models of the greenhouse effect are clearly enough to allow for reasoning about climate change. These data suggest that: 1) better representations about interdisciplinary concepts, such as the greenhouse effect, are needed for both scientist and public understanding; and 2) the scientific community needs to carefully consider how much understanding of a model is needed before necessary reasoning can occur.

  5. The Political Scientist as Local Campaign Consultant

    ERIC Educational Resources Information Center

    Crew, Robert E., Jr.

    2011-01-01

    During my 45 years as an academic, I have followed the admonition sometimes attributed to the legendary Jedi warrior Obi-Wan Kenobe that political scientists should "use [their] power for good and not for evil." In this spirit, I have devoted substantial portions of my career to public service by providing strategic advice and campaign management…

  6. U.S. Ethnic Scientists and Entrepreneurs

    ERIC Educational Resources Information Center

    Kerr, William R.

    2007-01-01

    Immigrants are exceptionally important for U.S. technology development, accounting for almost half of the country's Ph.D. workforce in science and engineering. Most notably, the contribution of Chinese and Indian scientists and entrepreneurs in U.S. high-technology sectors increased dramatically in the 1990s. These ethnic scientific communities…

  7. The VIVO Ontology: Enabling Networking of Scientists

    E-print Network

    Menczer, Filippo

    technologies to model scientists and provides federated search to enhance the discovery of researchers been adopted nationally and internationally, and enables the national and international federated search for finding experts. 1 Introduction The exponential growth in complexity and scope of modern

  8. RESEARCH SCIENTIST POSITION DESCRIPTION MICHAEL G. RYAN

    E-print Network

    Anderson, Charles W.

    ) Mitigation of elevated atmospheric greenhouse gases requires knowledge of carbon dynamics. (4) Management and energy with the atmosphere, sequester or release nutrients, and how these processes are regulated of the program: Ecosystem effects of mulching treatments for fuel reduction and forest restoration. The scientist

  9. Galaxy Zoo: Motivations of Citizen Scientists

    ERIC Educational Resources Information Center

    Raddick, M. Jordan; Bracey, Georgia; Gay, Pamela L.; Lintott, Chris J.; Cardamone, Carie; Murray, Phil; Schawinski, Kevin; Szalay, Alexander S.; Vandenberg, Jan

    2013-01-01

    Citizen science, in which volunteers work with professional scientists to conduct research, is expanding due to large online datasets. To plan projects, it is important to understand volunteers' motivations for participating. This paper analyzes results from an online survey of nearly 11000 volunteers in Galaxy Zoo, an astronomy citizen…

  10. Spain's Earth Scientists and the Oil Spill

    E-print Network

    Gillooly, Jamie

    Spain's Earth Scientists and the Oil Spill THE SPANISH COAST OF GALICIA IS CURRENT- ly subject to an oil spill that, given its spatial and temporal extent, could become one of the worst spills ever a third, and possibly not the last, oil wave. 2) Once the oil spill had occurred, the poor coordination

  11. USGS Scientist Inspects Streamgage During Flooding Event

    USGS Multimedia Gallery

    USGS scientist Matt Jennings inspects streamgage number  02136361 at Turkey Creek near Maryville, South Carolina, the morning of October 4, 2015. The discharge they measured was 6,000 cfs. These instruments form the backbone of our National Streamgage Network, which in turn feeds valuable info...

  12. NCI scientists identify new inflammatory syndrome

    Cancer.gov

    NCI scientists have identified a new inflammatory condition called interleukin-6 syndrome caused by Kaposi’s sarcoma-associated herpesvirus (KSHV) in some people with HIV/AIDS. This syndrome will be added to three existing types of KSHV-linked illnesses i

  13. Cautiously, Scientists Put Faith in Obama Promise

    ERIC Educational Resources Information Center

    Field, Kelly

    2009-01-01

    This article reports that academic researchers are optimistic that President Barack Obama's approach to science heralds a new era of support for their work. When Mr. Obama named his top science and technology advisers only weeks after being elected, many scientists celebrated. After eight years of an administration that many academics believed…

  14. Calling on Scientists to Fight Budget Cuts

    E-print Network

    Vermont, University of

    Calling on Scientists to Fight Budget Cuts THE FUNDING LEVELS REQUESTED BY THE Bush AdministrationMembersofCongress, including myself, are fighting to push science and technology as a priority in this and future budgets. Second, the more wars we fight, the more funds governments expend in the arms market, but we cannot argue

  15. All-in-One Python for Scientists

    E-print Network

    Delene, David J.

    to 3D Via scripting and GUI #12;Resources 2 Scientific Computing with Python - 2004 PythonPy4Science @ UND #12;#12;All-in-One Python for Scientists Enthought Python Distribution Open, NASA, NCAR, NOAA uses "Every pixel counts " #12;Resources 1 What is Python? by Wesley Chun Python 101

  16. Astrobiology from early-career scientists' perspective

    NASA Astrophysics Data System (ADS)

    Noack, Lena; Verseux, Cyprien; Serrano, Paloma; Musilova, Michaela; Nauny, Philippe; Samuels, Toby; Schwendner, Petra; Simoncini, Eugenio; Stevens, Adam

    2015-10-01

    What is astrobiology? Which fields does it comprise and what makes an astrobiologist? Ask five scientists and you may end up with six different definitions. This issue was raised at the first symposium of the European network of Astrobiology Graduates (AbGradE), held last year in Edinburgh, when discussing whether the attendees' fields of study were represented in the astrobiology community.

  17. "The Disinterested Scientist": Fact or Fiction?

    ERIC Educational Resources Information Center

    Mitroff, Ian I.

    1973-01-01

    The behavior of scientists who studied the moon rocks from the various Apollo missions was examined over a three year period. Methods of interviews ranging from discussion to written questionnaires were designed to explore issues connected with lunar missions and to focus on specific attitudes towards these issues. The central question emphasized…

  18. Yoshihiko Tamura Co-Chief Scientist

    E-print Network

    Busby, Cathy

    Peter Blum Expedition Project Manager/Staff Scientist Integrated Ocean Drilling Program Texas A be appropriately acknowledged. Citation: Tamura, Y., Busby, C., and Blum, P., 2013. Izu-Bonin-Mariana Rear Arc for Ocean Leadership, Lamont-Doherty Earth Observatory of Columbia University, and Texas A&M University

  19. MFR PAPER 1079 NMFS scientists have

    E-print Network

    MFR PAPER 1079 NMFS scientists have devised a simple method for . . . Controlling Bone Particle use of the product. A simple, rapid method for quantifying the bone content is presented. It involves machines may contain bone particles. The frequency of occurrence of parti- cles depends largely on the size

  20. Back to Article page Sailing Scientist

    E-print Network

    Shapin, Steven

    Back to Article page Sailing Scientist Steven Shapin Edmond Halley: Charting the Heavens and the odd couple is joined by a third, for here appears the name of the astronomer Edmond Halley (1656 on the Principia's title-page, your best bet is understanding Edmond Halley. For it was Halley's life that linked