Science.gov

Sample records for radio science conference

  1. Lunar & Planetary Science Conference.

    ERIC Educational Resources Information Center

    Warner, Jeffrey L.; And Others

    1982-01-01

    Summaries of different topics discussed at the Lunar and Planetary Science Conference are presented to provide updated information to nonplanetologists. Some topics include Venus, isotopes, chondrites, creation science, cosmic dust, cratering, moons and rings, igneous rocks, and lunar soil. (DC)

  2. The 1992 World Administrative Radio Conference: Technology and Policy Implications

    NASA Astrophysics Data System (ADS)

    1993-05-01

    As the 20th century draws to a close, new radio technologies and services are poised to change the ways we communicate. Radio waves already make possible a wide range of services considered commonplace--AM and FM radio broadcasting, television, cellular telephones, remote garage-door openers, and baby monitors. Advances in radio technology are giving birth to even more new products and services, including pocket-sized telephones that may allow people to make and receive calls anywhere in the world, high-definition televisions (HDTV) with superior quality pictures and sound, and static-free digital radios. The 1992 World Administrative Radio Conference (WARC-92) authorized frequencies for many of these new radio communication services, and granted additional frequencies for many existing services, including international broadcasting, satellite-based mobile communications, and communications in space. The effects of these changes will be felt well into the 21st century as countries around the world develop and deploy new communications systems to serve the needs of consumers, businesses, and governments. For the United States, the decisions made at the conference will critically affect how we develop new radio technologies and applications, how competitive this country will be in radio communications equipment and services, and how effectively the United States can exercise its role as a leader in world radio communication policymaking. This study of the outcomes and implications of WARC-92 was requested by the House Committee on Energy and Commerce and the Senate Committee on Commerce, Science, and Transportation. OTA was asked to evaluate the success of U.S. proposals at the conference, discuss the implications of the decisions made for U.S. technology and policy development, and identify options for improving U.S. participation in future world radio communication conferences.

  3. What Is the World Administrative Radio Conference?

    ERIC Educational Resources Information Center

    Howkins, John

    1979-01-01

    Describes the issues and interests to be discussed at the World Administrative Radio Conference in September, 1979. Includes definitions of principles for the use of the frequency spectrum, rights and duties of users, reallocation of frequency bands, and the need for principles to guide international cooperation. (JMF)

  4. CONFERENCES AND SYMPOSIA: Seventy years of the Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Waves Propagation (IZMIRAN) (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 25 November 2009)

    NASA Astrophysics Data System (ADS)

    2010-08-01

    A scientific session of the Physical Sciences Division of the Russian Academy of Sciences dedicated to the 70th anniversary of the Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences (IZMIRAN) (Troitsk, Moscow region) was held in the conference hall of IZMIRAN on 25 November 2009. The following reports were put on the session agenda posted on the web site www.gpad.ac.ru of the Physical Sciences Division, RAS: (1) Gurevich A V (Lebedev Physical Institute RAS, Moscow) "The role of cosmic rays and runaway electron breakdown in atmospheric lightning discharges"; (2) Aleksandrov E B (Ioffe Physical Technical Institute, RAS, St. Petersburg) "Advances in quantum magnetometry for geomagnetic research"; (3) Dorman L I (IZMIRAN, Troitsk, Moscow region, CR & SWC, Israel) "Cosmic ray variations and space weather"; (4) Mareev E A (Institute of Applied Physics, RAS, Nizhnii Novgorod) "Global electric circuit research: achievements and prospects"; (5) Tereshchenko E D, Safargaleev V V (Polar Geophysical Institute, Kola Research Center, RAS, Murmansk) "Geophysical research in Spitsbergen Archipelago: status and prospects"; (6) Gulyaev Yu V, Armand N A, Efimov A I, Matyugov S S, Pavelyev A G, Savich N A, Samoznaev L N, Smirnov V V, Yakovlev O I (Kotel'nikov Institute of Radio Engineering and Electronics RAS, Fryazino Branch, Fryazino, Moscow region) "Results of solar wind and planetary ionosphere research using radiophysical methods"; (7) Kunitsyn V E (Lomonosov Moscow State University, Moscow) "Satellite radio probing and the radio tomography of the ionosphere"; (8) Kuznetsov V D (IZMIRAN, Troitsk, Moscow region) "Space Research at the Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences." Papers based on reports 2-8 are published below. The main contents of report 1 are reproduced in A V Gurevich's review, "Nonlinear effects in the ionosphere" [Phys. Usp. 50

  5. Conference OKs science budgets

    NASA Astrophysics Data System (ADS)

    With the budget process all but complete for next fiscal year, the National Science Foundation and the National Aeronautics and Space Administration observers were saying that science had not done that badly in Congress, for an election year. NSF got half the budget increase it requested, NASA two-thirds. The Space Station did well, at the expense of environmental and social programs, which are funded by Congress from the same pot of money as NASA and NSF.A House-Senate conference finished work on a $59 billion appropriations bill for the Department of Housing and Urban Development and independent agencies, including EPA, NASA, and NSF, in early August. The House and Senate then quickly passed the measure before their recess; the President is expected to sign it soon. Included in the Fiscal Year 1989 spending bill are $1,885 billion for NSF, a 9.8% increase over FY 1988, and $10.7 billion for NASA, 18.5% more than the year before.

  6. NASA Microgravity Materials Science Conference

    NASA Technical Reports Server (NTRS)

    Szofran, Frank R. (Compiler); McCauley, D. (Compiler); Walker, C. (Compiler)

    1996-01-01

    The Microgravity Materials Science Conference was held June 10-11, 1996 at the Von Braun Civic Center in Huntsville, AL. It was organized by the Microgravity Materials Science Discipline Working Group, sponsored by the Microgravity Science and Applications Division at NASA Headquarters, and hosted by the NASA Marshall Space Flight Center and the Alliance for Microgravity Materials Science and Applications (AMMSA). It was the second NASA conference of this type in the microgravity materials science discipline. The microgravity science program sponsored approximately 80 investigations and 69 principal investigators in FY96, all of whom made oral or poster presentations at this conference. The conference's purpose was to inform the materials science community of research opportunities in reduced gravity in preparation for a NASA Research Announcement (NRA) scheduled for release in late 1996 by the Microgravity Science and Applications Division at NASA Headquarters. The conference was aimed at materials science researchers from academia, industry, and government. A tour of the MSFC microgravity research facilities was held on June 12, 1996. This volume is comprised of the research reports submitted by the principal investigators after the conference and presentations made by various NASA microgravity science managers.

  7. 2002 Microgravity Materials Science Conference

    NASA Technical Reports Server (NTRS)

    Gillies, Donald (Editor); Ramachandran, Narayanan (Editor); Murphy, Karen (Editor); McCauley, Dannah (Editor); Bennett, Nancy (Editor)

    2003-01-01

    The 2002 Microgravity Materials Science Conference was held June 25-26, 2002, at the Von Braun Center, Huntsville, Alabama. Organized by the Microgravity Materials Science Discipline Working Group, sponsored by the Physical Sciences Research Division, NASA Headquarters, and hosted by NASA Marshall Space Flight Center and member institutions under the Cooperative Research in Biology and Materials Science (CORBAMS) agreement, the conference provided a forum to review the current research and activities in materials science, discuss the envisioned long-term goals, highlight new crosscutting research areas of particular interest to the Physical Sciences Research Division, and inform the materials science community of research opportunities in reduced gravity. An abstracts book was published and distributed at the conference to the approximately 240 people attending, who represented industry, academia, and other NASA Centers. This CD-ROM proceedings is comprised of the research reports submitted by the Principal Investigators in the Microgravity Materials Science program.

  8. NASA Microgravity Materials Science Conference

    NASA Technical Reports Server (NTRS)

    Gillies, D. C. (Compiler); McCauley, D. E. (Compiler)

    1999-01-01

    The Microgravity Materials Science Conference was held July 14-16, 1998 at the Von Braun Center in Huntsville, AL. It was organized by the Microgravity Materials Science Discipline Working Group, sponsored by the Microgravity Research Division at NASA Headquarters, and hosted by the NASA Marshall Space Flight Center and the Alliance for Microgravity Materials Science and Applications. It was the third NASA conference of this type in the microgravity materials science discipline. The microgravity science program sponsored approximately 125 investigations and 100 principal investigators in FY98, almost all of whom made oral or poster presentations at this conference. The conference's purpose was to inform the materials science community of research opportunities in reduced gravity in preparation for a NASA Research Announcement scheduled for release in late 1998 by the Microgravity Research Division at NASA Headquarters. The conference was aimed at materials science researchers from academia, industry, and government. A tour of the Marshall Space Flight Center microgravity research facilities was held on July 16, 1998. This volume is comprised of the research reports submitted by the principal investigators after the conference.

  9. Inaugural AGU Science Policy Conference

    NASA Astrophysics Data System (ADS)

    Uhlenbrock, Kristan

    2012-01-01

    AGU will present its inaugural Science Policy Conference, 30 April to 3 May 2012, at the Ronald Reagan Building and International Trade Center, located in downtown Washington, D. C. This conference will bring together leading scientists, policy makers, industry professionals, press, and other stakeholders to discuss natural hazards, natural resources, oceans, and Arctic science and the role these sciences play in serving communities. To bridge the science and policy fields, AGU plans to host this conference every 2 years and focus on the applications of Earth and space sciences to serve local and national communities. "Our nation faces a myriad of challenges such as the sustainability of our natural resources, current and future energy needs, and the ability to mitigate and adapt to natural and manmade hazards," said Michael McPhaden, president of AGU. "It is essential that policies to address these challenges be built on a solid foundation of credible scientific knowledge."

  10. Rosetta Radio Science Investigations (RSI)

    NASA Astrophysics Data System (ADS)

    Pätzold, Martin; Häusler, Bernd; Aksnes, Kaare; Anderson, John D.; Asmar, Sami W.; Barriot, Jean-Pierre; Bird, Michael K.; Boehnhardt, Hermann; Eidel, Werner; Grün, Eberhardt; Ip, Wing H.; Marouf, Essam; Morley, Trevor; Neubauer, Fritz M.; Rickman, Hans; Thomas, Nicolas; Tsurutani, Bruce T.; Wallis, Max K.; Wickramasinghe, N. C.; Mysen, Eirik; Olson, Oystein; Remus, Stefan; Tellmann, Silvia; Andert, Thomas; Carone, Ludmila; Fels, Markus; Stanzel, Christina; Audenrieth-Kersten, Iris; Gahr, Alexander; Müller, Anna-Liane; Stupar, Dusan; Walter, Christina

    2007-02-01

    The Rosetta spacecraft has been successfully launched on 2nd March 2004 to its new target comet 67 P/Churyumov-Gerasimenko. The science objectives of the Rosetta Radio Science Investigations (RSI) experiment address fundamental aspects of cometary physics such as the mass and bulk density of the nucleus, its gravity field, its interplanetary orbit perturbed by nongravitational forces, its size and shape, its internal structure, the composition and roughness of the nucleus surface, the abundance of large dust grains, the plasma content in the coma and the combined dust and gas mass flux. The masses of two asteroids, Steins and Lutetia, shall be determined during flybys in 2008 and 2010, respectively. Secondary objectives are the radio sounding of the solar corona during the superior conjunctions of the spacecraft with the Sun during the cruise phase. The radio carrier links of the spacecraft Telemetry, Tracking and Command (TT&C) subsystem between the orbiter and the Earth will be used for these investigations. An Ultrastable oscillator (USO) connected to both transponders of the radio subsystem serves as a stable frequency reference source for both radio downlinks at X-band (8.4 GHz) and S-band (2.3 GHz) in the one-way mode. The simultaneous and coherent dual-frequency downlinks via the High Gain Antenna (HGA) permit separation of contributions from the classical Doppler shift and the dispersive media effects caused by the motion of the spacecraft with respect to the Earth and the propagation of the signals through the dispersive media, respectively. The investigation relies on the observation of the phase, amplitude, polarization and propagation times of radio signals transmitted from the spacecraft and received with ground station antennas on Earth. The radio signals are affected by the medium through which the signals propagate (atmospheres, ionospheres, interplanetary medium, solar corona), by the gravitational influence of the planet on the spacecraft and

  11. e-POP Radio Science Using Amateur Radio Transmissions

    NASA Astrophysics Data System (ADS)

    Frissell, N. A.; Perry, G. W.; Miller, E. S.; Shovkoplyas, A.; Moses, M. L.; James, H. G.; Yau, A. W.

    2015-12-01

    A major component of the enhanced Polar Outflow Probe (e-POP) Radio Receiver Instrument (RRI) mission is to utilize artificially generated radio emissions to study High Frequency (HF) radio wave propagation in the ionosphere. In the North American and European sectors, communications between amateur radio operators are a persistent and abundant source source of HF transmissions. We present the results of HF radio wave propagation experiments using amateur radio transmissions as an HF source for e-POP RRI. We detail how a distributed and autonomously operated amateur radio network can be leveraged to study HF radio wave propagation as well as the structuring and dynamics of the ionosphere over a large geographic region. In one case, the sudden disappearance of nearly two-dozen amateur radio HF sources located in the midwestern United States was used to detect a enhancement in foF2 in that same region. We compare our results to those from other more conventional radio instruments and models of the ionosphere to demonstrate the scientific merit of incorporating amateur radio networks for radio science at HF.

  12. Rosetta Radio Science Investigations (RSI)

    NASA Astrophysics Data System (ADS)

    Tellmann, Silvia; Pätzold, M.; Häusler, B.; Bird, M. K.

    2006-09-01

    In March 2004 the ROSETTA spacecraft started its journey to the comet P/Churyumov-Gerasimenko. The very ambitious mission will escort the comet for several months in 2015 as it heads towards the sun. The ROSETTA Radio Science Experiment (RSI) uses the radio carrier links of the spacecraft Telemetry, Tracking and Command subsystem at X-band and S-band. The spacecraft is specially equipped with an Ultra-Stable Oscillator (USO) that stabilizes the radio links for a significant improvement of the sensitivity and accuracy of the measurement. RSI is interested in dispersive frequency shifts due to the propagation of the radio signals through ionized media as well as non-dispersive frequency shifts caused by other perturbing forces acting on the spacecraft (gravity field, gas and dust mass flux from the comet). These observations will allow the investigation of the comet's nucleus, its size and shape and the lower harmonics of its gravity field, and the dielectric properties of its surface. In addition the electron content of the cometary coma and the abundance of large dust grains can be determined. The mass and bulk density of the asteroid will be determined during the flyby at asteroid Lutetia in 2010 First results from the commissioning phase and regularly performed measurements allow to assess the sensitivity of the experiment and the ageing of the USO quartz oscillator. These results are compared with the coherent two-way-measurements also recorded during commissioning. Between March and May 2006 ROSETTA moved into superior conjunction with the Sun. This allowed the investigation of the solar corona to derive electron density profiles in the structured corona, solar wind speed and to detect, identify and describe the spatial and temporal evolution of the shockfronts of coronal mass ejections.

  13. Social sciences conference on AIDS.

    PubMed

    1997-03-01

    This paper reports on the 1996 South African Universities Social Sciences Conference on AIDS held in Mmambatho, Northwest Province, South Africa. The conference was attended with a strong contingent from Botswana, Lesotho, Malawi, Namibia, South Africa, Swaziland, Zambia, and Zimbabwe. In the conference, various papers explored the needs of, and programmatic responses to women, orphaned children, university students, communities, youth private enterprise, the informal sector, and policy and socioeconomic concerns at a broader level. In addition, several papers specifically discussed the situation of women and AIDS, as well as relevant policy issues. A recommendation was made for governments to coordinate their efforts, with a call for increased openness at all levels rather than facing the epidemic individually. In this respect, the conference noted that the media could play a much more decisive role. This report also highlights the major comments made during the conference and some of the key issues that were raised in each of the following areas: 1) awareness and prevention, 2) children, 3) women, and 4) household costs.

  14. World Administrative Radio Conference. Issues for US International Spectrum Policy

    NASA Astrophysics Data System (ADS)

    1991-11-01

    U.S. preparations for the 1992 World Administrative Radio Conference to be held in Spain, February 1992 are examined. WARC-92 will attempt to reassign radio frequencies internationally in order to take advantage of new radio-based technologies and applications, such as digital audio broadcasting, high definition television, and personal communications services, while still accommodating the needs of existing users and services. The impacts of the realignment will be felt throughout the U.S. economy and around the world, and the agreements reached at WARC-92 will influence the development of radio-based systems and services well into the next century.

  15. Radio Science Measurements with Suppressed Carrier

    NASA Technical Reports Server (NTRS)

    Asmar, Sami; Divsalar, Dariush; Oudrhiri, Kamal

    2013-01-01

    Radio Science started when it became apparent with early Solar missions that occultations by planetary atmospheres would affect the quality of radio communications. Since then the atmospheric properties and other aspects of planetary science, solar science, and fundamental physics were studied by scientists. Radio Science data was always extracted from a received pure residual carrier (without data modulation). For some missions, it is very desirable to obtain Radio Science data from a suppressed carrier modulation. In this paper we propose a method to extract Radio Science data when a coded suppressed carrier modulation is used in deep space communications. Type of modulation can be BPSK, QPSK, OQPSK, MPSK or even GMSK. However we concentrate mostly on BPSK modulation. The proposed method for suppressed carrier simply tries to wipe out data that acts as an interference for Radio Science measurements. In order to measure the estimation errors in amplitude and phase of the Radio Science data we use Cramer-Rao bound (CRB). The CRB for the suppressed carrier modulation with non-ideal data wiping is then compared with residual carrier modulation under the same noise condition. The method of derivation of CRB for non-ideal data wiping is an innovative method that presented here. Some numerical results are provided for coded system.

  16. The Different Wavelengths of Radio Science

    NASA Technical Reports Server (NTRS)

    Malecha, Jessica L.

    2005-01-01

    Radio Science covers many different avenues. This summer I attempted to work in each of the different avenues to learn the full range of subjects covered by Radio Science. I began my summer by traveling to Greece for the 3rd International Planetary Probe Workshop (IPPW-3). I went as a co-author of the Doppler Wind Experiment (DWE) team paper. My first job when I returned from Greece was to update the Radio Science activities webpage. I then used Fast Fourier Transforms (FFT) to find radio signals in recorded Radio Science experimental data and determine frequencies and powers. I read about and ran Fortran code being used to determine wind measurements on Huygens. I formatted and revised the abstracts and data lengths for the DVD data sets. By performing these tasks, I also learned the Unix operating system as well as a small amount of shell programming.

  17. Radio interferometry: Techniques for Geodesy. [conference

    NASA Technical Reports Server (NTRS)

    1980-01-01

    Progress in the development and application of radio interferometry as a tool for geophysical research is reported and discussed. Among the topics reviewed are: Surveys of is the Seventies, Movements, Terrestrial and Celestial, Degrees Kelvin and Degrees of Phase, the Mark 3 VLBI System, Waves of the Future and other Emissions, and Adherence and Coherence in Networks, and Plans.

  18. Major Issues of the World Administrative Radio Conference 1979.

    ERIC Educational Resources Information Center

    Ullah, Ifram

    In preparation for the 1979 World Administrative Radio Conference (WARC), this paper lists some of the issues on which WARC participants will focus. These issues include the expansion of the shortwave spectrum and the formulation of more equitable, more efficient procedures by which broadcasters are awarded high-frequency shortwave bands; ways to…

  19. Euro3D Science Conference

    NASA Astrophysics Data System (ADS)

    Walsh, J. R.

    2004-02-01

    The Euro3D RTN is an EU funded Research Training Network to foster the exploitation of 3D spectroscopy in Europe. 3D spectroscopy is a general term for spectroscopy of an area of the sky and derives its name from its two spatial + one spectral dimensions. There are an increasing number of instruments which use integral field devices to achieve spectroscopy of an area of the sky, either using lens arrays, optical fibres or image slicers, to pack spectra of multiple pixels on the sky (``spaxels'') onto a 2D detector. On account of the large volume of data and the special methods required to reduce and analyse 3D data, there are only a few centres of expertise and these are mostly involved with instrument developments. There is a perceived lack of expertise in 3D spectroscopy spread though the astronomical community and its use in the armoury of the observational astronomer is viewed as being highly specialised. For precisely this reason the Euro3D RTN was proposed to train young researchers in this area and develop user tools to widen the experience with this particular type of data in Europe. The Euro3D RTN is coordinated by Martin M. Roth (Astrophysikalisches Institut Potsdam) and has been running since July 2002. The first Euro3D science conference was held in Cambridge, UK from 22 to 23 May 2003. The main emphasis of the conference was, in keeping with the RTN, to expose the work of the young post-docs who are funded by the RTN. In addition the team members from the eleven European institutes involved in Euro3D also presented instrumental and observational developments. The conference was organized by Andy Bunker and held at the Institute of Astronomy. There were over thirty participants and 26 talks covered the whole range of application of 3D techniques. The science ranged from Galactic planetary nebulae and globular clusters to kinematics of nearby galaxies out to objects at high redshift. Several talks were devoted to reporting recent observations with newly

  20. Information Content in Radio Waves: Student Investigations in Radio Science

    NASA Astrophysics Data System (ADS)

    Jacobs, K.; Scaduto, T.

    2013-12-01

    We describe an inquiry-based instructional unit on information content in radio waves, created in the summer of 2013 as part of a MIT Haystack Observatory (Westford, MA) NSF Research Experiences for Teachers (RET) program. This topic is current and highly relevant, addressing science and technical aspects from radio astronomy, geodesy, and atmospheric research areas as well as Next Generation Science Standards (NGSS). Projects and activities range from simple classroom demonstrations and group investigations, to long term research projects incorporating data acquisition from both student-built instrumentation as well as online databases. Each of the core lessons is applied to one of the primary research centers at Haystack through an inquiry project that builds on previously developed units through the MIT Haystack RET program. In radio astronomy, students investigate the application of a simple and inexpensive software defined radio chip (RTL-SDR) for use in systems implementing a small and very small radio telescope (SRT and VSRT). Both of these systems allow students to explore fundamental principles of radio waves and interferometry as applied to radio astronomy. In ionospheric research, students track solar storms from the initial coronal mass ejection (using Solar Dynamics Observatory images) to the resulting variability in total electron density concentrations using data from the community standard Madrigal distributed database system maintained by MIT Haystack. Finally, students get to explore very long-baseline interferometry as it is used in geodetic studies by measuring crustal plate displacements over time. Alignment to NextGen standards is provided for each lesson and activity with emphasis on HS-PS4 'Waves and Their Applications in Technologies for Information Transfer'.

  1. Enhancing GLAST Science Through Complementary Radio Observations

    NASA Astrophysics Data System (ADS)

    Ulvestad, James S.

    2006-12-01

    Radio astronomical observations with state-of-the-art instrumentation will be critical for achieving the maximum science return from the GLAST mission. Radio nterferometers with baselines of thousands of kilometers, such as the Very Long Baseline Array (VLBA), will provide sub-milliarcsecond imaging of GLAST blazars. High-frequency VLBA imaging, repeatable at intervals of days to weeks, will image the region where gamma-ray flares occur in blazars and help determine the location of the gamma-ray emission. Multi-frequency arcsecond-scale imaging with interferometers having baselines of one to tens of kilometers, particularly the Very Large Array, will provide efficient discrimination among the candidates for unidentified gamma-ray sources. Pulsar timing with single-dish radio telescopes such as the Green Bank Telescope will enable accurate registration of gamma-ray photons with pulsar ephemerides for studies of the pulsar emission mechanisms. Along with these contemporaneous radio/GLAST observing programs, we will discuss briefly some of the recent radio programs that have been conducted in preparation for GLAST launch. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.

  2. Microgravity Materials Science Conference 2000. Volume 3

    NASA Technical Reports Server (NTRS)

    Ramachandran, Narayanan; Bennett, Nancy; McCauley, Dannah; Murphy, Karen; Poindexter, Samantha

    2001-01-01

    This is Volume 3 of 3 of the 2000 Microgravity Materials Science Conference that was held June 6-8 at the Von Braun Center, Huntsville, Alabama. It was organized by the Microgravity Materials Science Discipline Working Group, sponsored by the Microgravity Research Division (MRD) at NASA Headquarters, and hosted by NASA Marshall Space Flight Center and the Alliance for Microgravity Materials Science and Applications (AMMSA). It was the fourth NASA conference of this type in the Microgravity materials science discipline. The microgravity science program sponsored 200 investigators, all of whom made oral or poster presentations at this conference- In addition, posters and exhibits covering NASA microgravity facilities, advanced technology development projects sponsored by the NASA Microgravity Research Division at NASA Headquarters, and commercial interests were exhibited. The purpose of the conference was to inform the materials science community of research opportunities in reduced gravity and to highlight the Spring 2001 release of the NASA Research Announcement (NRA) to solicit proposals for future investigations. It also served to review the current research and activities in material,, science, to discuss the envisioned long-term goals. and to highlight new crosscutting research areas of particular interest to MRD. The conference was aimed at materials science researchers from academia, industry, and government. A workshop on in situ resource utilization (ISRU) was held in conjunction with the conference with the goal of evaluating and prioritizing processing issues in Lunar and Martian type environments. The workshop participation included invited speakers and investigators currently funded in the material science program under the Human Exploration and Development of Space (HEDS) initiative. The conference featured a plenary session every day with an invited speaker that was followed by three parallel breakout sessions in subdisciplines. Attendance was close

  3. Microgravity Materials Science Conference 2000. Volume 2

    NASA Technical Reports Server (NTRS)

    Ramachandran, Narayanan (Editor); Bennett, Nancy (Editor); McCauley, Dannah (Editor); Murphy, Karen (Editor); Poindexter, Samantha (Editor)

    2001-01-01

    This is Volume 2 of 3 of the 2000 Microgravity Materials Science Conference that was held June 6-8 at the Von Braun Center, Huntsville, Alabama. It was organized by the Microgravity Materials Science Discipline Working Group, sponsored by the Microgravity Research Division (MRD) at NASA Headquarters, and hosted by NASA Marshall Space Flight Center and the Alliance for Microgravity Materials Science and Applications (AMMSA). It was the fourth NASA conference of this type in the Microgravity materials science discipline. The microgravity science program sponsored approx. 200 investigators, all of whom made oral or poster presentations at this conference- In addition, posters and exhibits covering NASA microgravity facilities, advanced technology development projects sponsored by the NASA Microgravity Research Division at NASA Headquarters, and commercial interests were exhibited. The purpose of the conference %%,its to inform the materials science community of research opportunities in reduced gravity and to highlight the Spring 2001 release of the NASA Research Announcement (NRA) to solicit proposals for future investigations. It also served to review the current research and activities in material,, science, to discuss the envisioned long-term goals. and to highlight new crosscutting research areas of particular interest to MRD. The conference was aimed at materials science researchers from academia, industry, and government. A workshop on in situ resource utilization (ISRU) was held in conjunction with the conference with the goal of evaluating and prioritizing processing issues in Lunar and Martian type environments. The workshop participation included invited speakers and investigators currently funded in the material science program under the Human Exploration and Development of Space (HEDS) initiative. The conference featured a plenary session every day with an invited speaker that was followed by three parallel breakout sessions in subdisciplines. Attendance

  4. Microgravity Materials Science Conference 2000. Volume 1

    NASA Technical Reports Server (NTRS)

    Ramachandran, Narayanan (Editor); Bennett, Nancy (Editor); McCauley, Dannah (Editor); Murphy, Karen (Editor); Poindexter, Samantha (Editor)

    2001-01-01

    This is Volume 1 of 3 of the 2000 Microgravity Material Science Conference that was held June 6-8 at the Von Braun Center, Huntsville, Alabama. It was organized by the Microgravity Materials Science Discipline Working Group, sponsored by the Microgravity Research Division (MRD) at NASA Headquarters, and hosted by NASA Marshall Space Flight Center and the Alliance for Microgravity Materials Science and Applications (AMMSA). It was the fourth NASA conference of this type in the microgravity materials science discipline. The microgravity science program sponsored approx. 200 investigators, all of whom made oral or poster presentations at this conference. In addition, posters and exhibits covering NASA microgravity facilities, advanced technology development projects sponsored by the NASA Microgravity Research Division at NASA Headquarters, and commercial interests were exhibited. The purpose of the conference was to inform the materials science community of research opportunities in reduced gravity and to highlight the Spring 2001 release of the NASA Research Announcement (NRA) to solicit proposals for future investigations. It also served to review the current research and activities in materials science, to discuss the envisioned long-term goals. and to highlight new crosscutting research areas of particular interest to MRD. The conference was aimed at materials science researchers from academia, industry, and government. A workshop on in situ resource utilization (ISRU) was held in conjunction with the conference with the goal of evaluating and prioritizing processing issues in Lunar and Martian type environments. The workshop participation included invited speakers and investigators currently funded in the material science program under the Human Exploration and Development of Space (HEDS) initiative. The conference featured a plenary session every day with an invited speaker that was followed by three parallel breakout sessions in subdisciplines. Attendance was

  5. IEEE International conference on plasma science: Conference record--Abstracts

    SciTech Connect

    Not Available

    1993-01-01

    The conference covered the following topics: basic plasma physics; vacuum electronics; gaseous and electrical gas discharges; laser-produced plasma; space plasmas; computational plasma science; plasma diagnostics; electron, ion and plasma sources; intense electron and ion beams; intense beam microwaves; fast wave M/W devices; microwave-plasma interactions; magnetic fusion; MHD; plasma focus; ultrafast z-pinches and x-ray lasers; plasma processing; fast-opening switches; EM and ETH launchers; solid-state plasmas and switches; plasmas for lighting; ball lightning and spherical plasma configurations; and environmental/energy issues. Separate abstracts were prepared for 379 items in this conference.

  6. Math/science education action conference report

    SciTech Connect

    Not Available

    1990-05-01

    On October 8--10, 1989, the US Department of Energy, the Lawrence Hall of Science, and the Lawrence Berkeley Laboratory sponsored a Math/Science Education Action Conference in Berkeley, California. The conference was co-chaired by Admiral James D. Watkins, Secretary of Energy, and Dr. Glenn T. Seaborg Chairman of the Lawrence Hall of Science. Nearly 250 scientists, educators, business executives, and government leaders came together to develop a concrete plan of action for restructuring and revitalizing mathematics and science education. Their target was to improve education for an entire cohort of children--the Class of 2007, the children born this school year--and their governing principle was one of collaboration, both between Federal agencies, and between public and private sectors. The report of the conference co-chairmen and participants is provided in this document. 41 figs.

  7. Apollo 11 Lunar Science Conference

    ERIC Educational Resources Information Center

    Cochran, Wendell

    1970-01-01

    Report of a conference called to discuss the findings of 142 scientists from their investigations of samples of lunar rock and soil brought back by the Apollo 11 mission. Significant findings reported include the age and composition of the lunar samples, and the absence of water and organic matter. Much discussed was the origin and structure of…

  8. Bridging Science and Policy: The AGU Science Policy Conference

    NASA Astrophysics Data System (ADS)

    Hankin, E. R.; Uhlenbrock, K.; Landau, E. A.

    2013-12-01

    In recent years, science has become inextricably linked to the political process. As such, it is more important now than ever for science to forge a better relationship with politics, for the health of both science and society. To help meet this need, the American Geophysical Union (AGU) strives to engage its members, shape policy, and inform society about the excitement of Earth and space science and its role in developing solutions for the sustainability of the planet. In June 2013, AGU held its second annual Science Policy Conference in Washington, D.C. The goal of the conference is to provide a new forum for diverse discussions and viewpoints on the challenges and opportunities of science policy, with a focus on applications of Earth and space science that serve local, national, and international communities. The meeting brought together more than 300 scientists, policy makers, industry professionals, members of the press, and other stakeholders to discuss the topics concerning the Arctic, climate change, oceans, energy, technology and infrastructure, and natural hazards science as they relate to challenges impacting society. Sessions such as 'The Water-Energy Nexus,' 'Potential for Megadisasters,' 'The Changing Ocean and Impacts on Human Health,' and 'Drowning and Drought: Agricultural Impacts of Climate Change' are examples of some of the intriguing and timely science policy issues addressed at the conference. The findings from the conference were used to develop a summary report. The report highlights key facts and figures to be used as a resource in discussions with policy makers and other stakeholders regarding the conference topics. This presentation will discuss the goals and outcomes of the conference and how the event represents one of the many ways AGU is approaching its 'Science and Society' priority objective as part of the Union's strategic plan; namely by increasing the effectiveness and recognition of AGU among policy makers as an authoritative

  9. A Versatile Planetary Radio Science Microreceiver

    NASA Technical Reports Server (NTRS)

    Fry, Craig D.; Rosenberg, T. J.

    1999-01-01

    We have developed a low-power. programmable radio "microreceiver" that combines the functionality of two science instruments: a Relative Ionospheric Opacity Meter (riometer) and a swept-frequency, VTF/HF radio spectrometer. The radio receiver, calibration noise source, data acquisition and processing, and command and control functions are all contained on a single circuit board. This design is suitable for miniaturizing as a complete flight instrument. Several of the subsystems were implemented in a field-programmable gate array (FPGA), including the receiver detector, the control logic, and the data acquisition and processing blocks. Considerable efforts were made to reduce the power consumption of the instrument, and eliminate or minimize RF noise and spurious emissions generated by the receiver's digital circuitry. A prototype instrument was deployed at McMurdo Station, Antarctica, and operated in parallel with a traditional riometer instrument for approximately three weeks. The attached paper (accepted for publication by Radio Science) describes in detail the microreceiver theory of operation, performance specifications and test results.

  10. International Conference on Applied Sciences (ICAS2013)

    NASA Astrophysics Data System (ADS)

    Lemle, Ludovic Dan; Jiang, Yiwen

    2014-03-01

    The International Conference on Applied Sciences (ICAS2013) took place in Wuhan, P R China from 26-27 October 2013 at the Military Economics Academy. The conference is regularly organized, alternately in Romania and in P R China, by ''Politehnica'' University of Timişoara, Romania, and Military Economics Academy of Wuhan, P R China, with the aim to serve as a platform for the exchange of information between various areas of applied sciences, and to promote the communication between the scientists of different nations, countries and continents. The conference has been organized for the first time in 15-16 June 2012 at the Engineering Faculty of Hunedoara, Romania. The topics of the conference covered a comprehensive spectrum of issues: Economical sciences Engineering sciences Fundamental sciences Medical sciences The conference gathered qualified researchers whose expertise can be used to develop new engineering knowledge that has applicability potential in economics, defense, medicine, etc. The number of registered participants was nearly 90 from 5 countries. During the two days of the conference 4 invited and 36 oral talks were delivered. A few of the speakers deserve a special mention: Mircea Octavian Popoviciu, Academy of Romanian Scientist — Timişoara Branch, Correlations between mechanical properties and cavitation erosion resistance for stainless steels with 12% chromium and variable contents of nickel; Carmen Eleonora Hărău, ''Politehnica'' University of Timişoara, SWOT analysis of Romania's integration in EU; Ding Hui, Military Economics Academy of Wuhan, Design and engineering analysis of material procurement mobile operation platform; Serban Rosu, University of Medicine and Pharmacy ''Victor Babeş'' Timişoara, Cervical and facial infections — a real life threat, among others. Based on the work presented at the conference, 14 selected papers are included in this volume of IOP Conference Series: Materials Science and Engineering. These papers

  11. Radio-science performance analysis software

    NASA Technical Reports Server (NTRS)

    Morabito, D. D.; Asmar, S. W.

    1995-01-01

    The Radio Science Systems Group (RSSG) provides various support functions for several flight project radio-science teams. Among these support functions are uplink and sequence planning, real-time operations monitoring and support, data validation, archiving and distribution functions, and data processing and analysis. This article describes the support functions that encompass radio-science data performance analysis. The primary tool used by the RSSG to fulfill this support function is the STBLTY program set. STBLTY is used to reconstruct observable frequencies and calculate model frequencies, frequency residuals, frequency stability in terms of Allan deviation, reconstructed phase, frequency and phase power spectral density, and frequency drift rates. In the case of one-way data, using an ultrastable oscillator (USO) as a frequency reference, the program set computes the spacecraft transmitted frequency and maintains a database containing the in-flight history of the USO measurements. The program set also produces graphical displays. Some examples and discussions on operating the program set on Galileo and Ulysses data will be presented.

  12. Radio Science from an Optical Communications Signal

    NASA Technical Reports Server (NTRS)

    Moision, Bruce; Asmar, Sami; Oudrhiri, Kamal

    2013-01-01

    NASA is currently developing the capability to deploy deep space optical communications links. This creates the opportunity to utilize the optical link to obtain range, doppler, and signal intensity estimates. These may, in turn, be used to complement or extend the capabilities of current radio science. In this paper we illustrate the achievable precision in estimating range, doppler, and received signal intensity of an non-coherent optical link (the current state-of-the-art for a deep-space link). We provide a joint estimation algorithm with performance close to the bound. We draw comparisons to estimates based on a coherent radio frequency signal, illustrating that large gains in either precision or observation time are possible with an optical link.

  13. 78 FR 10180 - Annual Computational Science Symposium; Conference

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-02-13

    ... HUMAN SERVICES Food and Drug Administration Annual Computational Science Symposium; Conference AGENCY... public conference entitled ``The FDA/PhUSE Annual Computational Science Symposium.'' The purpose of the conference is to help the broader community align and share experiences to advance computational science....

  14. 77 FR 4568 - Annual Computational Science Symposium; Public Conference

    Federal Register 2010, 2011, 2012, 2013, 2014

    2012-01-30

    ... HUMAN SERVICES Food and Drug Administration Annual Computational Science Symposium; Public Conference... announcing a public conference entitled ``The FDA/PhUSE Annual Computational Science Symposium.'' The purpose... computational science. At the conference, which will bring together FDA, industry, and academia, FDA will...

  15. An Overview of Cassini Radio Science

    NASA Astrophysics Data System (ADS)

    Kliore, A.; Rappaport, N.; Anabtawi, A.; Asmar, S.; Armstrong, J.; Barbinis, E.; Goltz, G.; Johnston, D.; Fleischman, D.; Rochblatt, D.; Anderson, J.; Marouf, E.; Wong, K.; Thomson, F.; Flasar, F. M.; Schinder, P.; French, R.; McGhee, C.; Mohammed, P.; Steffes, P.; Nagy, A.; Iess, L.; Tortora, P.; Ambrosini, R.; Flamini, E.

    2005-08-01

    The Cassini spacecraft, which has been in orbit about Saturn for over a year, is the first Radio Science platform to provide three downlink frequencies. In addition to the X-band telemetry link (3,56 cm w.l.), two other frequencies, S-band (13.04 cm), and Ka-band (0.94 cm) are available. This, plus the high SNR (>50 dBHz at X-band) afforded by the 4 m diameter s/c high gain antenna in combination with the excellent low noise receivers of the DSN, as well as overall system stabilities of 1 x 10-13 when referenced to the on-board ultra-stable oscillator (USO) in one-way operation, and 1 x 10-15 for a two-way link, make Cassini an unprecedented instrument of radio science. In addition to Gravitational Wave Search and Solar Conjunction experiments conducted during the cruise phase, the orbital tour phase of the mission has as its main radio science objectives: a) determination of the masses and gravity fields of Saturn's icy satellites, Titan, and Saturn through two-way tracking during fly-bys. To date, the masses of Phoebe, Iapetus, Dione and Enceladus have been measured, and will be reported here. b) Measurement of the structure and other properties of Saturn's rings through three-band occultation. Several near-diametric occultations at a high ring opening angle have been completed, and the results will be presented here. c) Measurement of the vertical structure of the atmosphere and ionosphere of Saturn. The same series of occultations have provided nearly equatorial occultations, and the results on the atmosphere structure, the ionosphere, and the abundances of microwave-absorbing gases in Saturn's atmosphere will be described here. In the remaining years of the Cassini mission, these results will be expanded to include the atmosphere, ionosphere, surface, and gravity field of Titan, the gravity field and masses of Saturn and the remaining icy satellites, and the completion of the Saturn objectives described above. The Cassini Radio Science Team wishes to express

  16. SIAM Conference on Computational Science and Engineering

    SciTech Connect

    2003-01-01

    The Second SIAM Conference on Computational Science and Engineering was held in San Diego from February 10-12, 2003. Total conference attendance was 553. This is a 23% increase in attendance over the first conference. The focus of this conference was to draw attention to the tremendous range of major computational efforts on large problems in science and engineering, to promote the interdisciplinary culture required to meet these large-scale challenges, and to encourage the training of the next generation of computational scientists. Computational Science & Engineering (CS&E) is now widely accepted, along with theory and experiment, as a crucial third mode of scientific investigation and engineering design. Aerospace, automotive, biological, chemical, semiconductor, and other industrial sectors now rely on simulation for technical decision support. For federal agencies also, CS&E has become an essential support for decisions on resources, transportation, and defense. CS&E is, by nature, interdisciplinary. It grows out of physical applications and it depends on computer architecture, but at its heart are powerful numerical algorithms and sophisticated computer science techniques. From an applied mathematics perspective, much of CS&E has involved analysis, but the future surely includes optimization and design, especially in the presence of uncertainty. Another mathematical frontier is the assimilation of very large data sets through such techniques as adaptive multi-resolution, automated feature search, and low-dimensional parameterization. The themes of the 2003 conference included, but were not limited to: Advanced Discretization Methods; Computational Biology and Bioinformatics; Computational Chemistry and Chemical Engineering; Computational Earth and Atmospheric Sciences; Computational Electromagnetics; Computational Fluid Dynamics; Computational Medicine and Bioengineering; Computational Physics and Astrophysics; Computational Solid Mechanics and Materials; CS

  17. Planned BepiColombo Radio Science Investigations

    NASA Astrophysics Data System (ADS)

    Asmar, Sami; Iess, Luciano; Dehant, Veronique; Milani, Andrea; Tortora, Paolo

    The BepiColombo mission to Mercury has defined the investigations of the planetary interiors as well as tests of the theory of general relativity among its science objectives. Both of these objectives can be achieved using the tools and instrumentation of Radio Science. The investigations will provide detailed mapping of Mercury's gravity field, along with temporal variations due to tides, and important information about its deep internal structure. The global gravitational field along with the rotation state of the planet would enable improved constrains of whether the solid surface is decoupled from the inner core. The addition of altimetry enables the geophysical study of the crust, mantle, and impact basins. The global orbital solutions, obtained from precise radio metric data will lead to very accurate tests of General Relativity and other metric theories of gravity. The classical tests of the solar gravitational deflection and the precession of perihelion could significantly improve the measurement of several post-Newtonian parameters to levels nearing detection of possible violations of General Relativity. In spite of the uncertainty of the theoretical scenarios, the motivations for further tests of gravitational theories are stronger then ever: string theory, new cosmological observations, the hypotheses of dark matter and dark energy, all point to the need for a new and more profound understanding of the universe and its laws, including the laws of gravity. In order to achieve the scientific objectives in geophysics and fundamental physics, suitable radio frequency instrumentation for the Doppler and ranging observables for the spacecraft as well as ground stations. The target ranging accuracy of approximately 20 cm require the capability of transmitting and receiving at multiple frequencies to reduce plasma noise as well as larger modulation bandwidths. This paper describes experiments for probing space-time in the solar system with the Bepi

  18. The Deep Space Network: An instrument for radio science research

    NASA Technical Reports Server (NTRS)

    Renzetti, N. A.

    1981-01-01

    Doppler and ranging data routinely generated at the Deep Space Stations of the California Institute of Technology-Jet Propulsion Laboratory Deep Space Network serve as an excellent source of radio science information. Important radio science experiments based on Deep Space Network generated radio metric data have included confirmation of Einstein's Theory of Relativity, measurement of the masses and gravitational harmonics of the planets out to Saturn, and measurement of electron density distribution and turbulence in the solar corona. In response to an increased level of radio science requirements, the Deep Space Network chose in 1976 to implement a new radio science system, which was completed in late 1978. Key features include (1) highly phase stable open loop receivers, (2) reduction of recorded data bandwidth through use of programmed local oscillators, and (3) real time digitization and recording on computer compatible tape.

  19. Amateur Planetary Radio Data Archived for Science and Education: Radio Jove

    NASA Astrophysics Data System (ADS)

    Thieman, J.; Cecconi, B.; Sky, J.; Garcia, L. N.; King, T. A.; Higgins, C. A.; Fung, S. F.

    2015-12-01

    The Radio Jove Project is a hands-on educational activity in which students, teachers, and the general public build simple radio telescopes, usually from a kit, to observe single frequency decameter wavelength radio emissions from Jupiter, the Sun, the galaxy, and the Earth usually with simple dipole antennas. Some of the amateur observers have upgraded their receivers to spectrographs and their antennas have become more sophisticated as well. The data records compare favorably to more sophisticated professional radio telescopes such as the Long Wavelength Array (LWA) and the Nancay Decametric Array. Since these data are often carefully calibrated and recorded around the clock in widely scattered locations they represent a valuable database useful not only to amateur radio astronomers but to the professional science community as well. Some interesting phenomena have been noted in the data that are of interest to the professionals familiar with such records. The continuous monitoring of radio emissions from Jupiter could serve as useful "ground truth" data during the coming Juno mission's radio observations of Jupiter. Radio Jove has long maintained an archive for thousands of Radio Jove observations, but the database was intended for use by the Radio Jove participants only. Now, increased scientific interest in the use of these data has resulted in several proposals to translate the data into a science community data format standard and store the data in professional archives. Progress is being made in translating Radio Jove data to the Common Data Format (CDF) and also in generating new observations in that format as well. Metadata describing the Radio Jove data would follow the Space Physics Archive Search and Extract (SPASE) standard. The proposed archive to be used for long term preservation would be the Planetary Data System (PDS). Data sharing would be achieved through the PDS and the Paris Astronomical Data Centre (PADC) and the Virtual Wave Observatory (VWO

  20. DSN radio science system description and requirements. [for satellite radio astronomy experiments

    NASA Technical Reports Server (NTRS)

    Mulhall, B. D. L.

    1977-01-01

    The data system created to collect the functions performed by the Deep Space Network in support of spacecraft radio science experiments is described. Some of the major functional requirements presently being considered for the system are delineated.

  1. The Radio Jove Project: Citizen Science Contributes to Jupiter Decametric Radio Research

    NASA Astrophysics Data System (ADS)

    Thieman, J.; Higgins, C. A.; Sky, J.; Cecconi, B.; Garcia, L. N.

    2014-12-01

    The Radio Jove Project is a hands-on educational activity in which students, teachers, and the general public build a simple radio telescope, usually from a kit, to observe single frequency decameter wavelength radio emissions from Jupiter, the Sun, the galaxy, and the Earth. Regular monitoring of Jupiter and solar radio storms is typical, and Radio Jove amateur observations have improved in their scientific utility. Some observers have upgraded their equipment to make spectroscopic observations in the frequency band from 15-30 MHz. These observations can be particularly useful when made in conjunction with professional telescopes such as the Long Wavelength Array (LWA), the Nancay Decametric Array, the Ukrainian UTR-2 Radio Telescope, etc. The coming Juno mission to Jupiter will observe the radio emissions while in orbit at Jupiter and will benefit from the Earth-based perspective provided by frequent monitoring of the emissions. With these goals in mind work is now underway to provide simple methods of archiving the Radio Jove observations for use by the amateur and professional radio science community in scientifically useful and easily analyzed formats. The data will be ingested to both Radio Jove specific databases and to archives containing a variety of "waves" data. Methods are being developed to assure the scientific validity of contributed data such as certification of the observers. Amateur scientists have made overwhelming contributions to optical astronomy and we believe the same is possible within the radio astronomy community as well.

  2. PREFACE: International Conference on Applied Sciences (ICAS2014)

    NASA Astrophysics Data System (ADS)

    Lemle, Ludovic Dan; Jiang, Yiwen

    2015-06-01

    The International Conference on Applied Sciences (ICAS2014) took place in Hunedoara, Romania from 2-4 October 2014 at the Engineering Faculty of Hunedoara. The conference takes place alternately in Romania and in P.R. China and is organized by "Politehnica" University of Timisoara, Romania, and Military Economics Academy of Wuhan, P.R. China, with the aim to serve as a platform for exchange of information between various areas of applied sciences and to promote the communication between scientists of different nations, countries and continents. The topics of the conference covered a comprehensive spectrum of issues: 1. Economical Sciences 2. Engineering Sciences 3. Fundamental Sciences 4. Medical Sciences The conference gathered qualified researchers whose expertise can be used to develop new engineering knowledge that has the potential for application in economics, defense, medicine, etc. There were nearly 100 registered participants from six countries, and four invited and 56 oral talks were delivered during the two days of the conference. Based on the work presented at the conference, selected papers are included in this volume of IOP Conference Series: Materials Science and Engineering. These papers present new research in the various fields of Materials Engineering, Mechanical Engineering, Computer Engineering, and Mathematical Engineering. It is our great pleasure to present this volume of IOP Conference Series: Materials Science and Engineering to the scientific community to promote further research in these areas. We sincerely hope that the papers published in this volume will contribute to the advancement of knowledge in their respective fields.

  3. RIKEN Radio Isotope Beam Factory: Japanese Flagship for Nuclear Science

    NASA Astrophysics Data System (ADS)

    En'yo, Hideto

    2015-11-01

    Recent activities at the RIKEN Radio Isotope Beam Factory (RIBF) are reported together with its history and future prospects. RIBF is the Japanese flagship for nuclear science, and at this moment is the world flagship machine.

  4. Radiofrequency use and management. Impacts from the World Administrative Radio Conference of 1979

    NASA Astrophysics Data System (ADS)

    1982-01-01

    The impacts on the United States of key decisions taken at the general World Administrative Radio Conference (WARC-79) and options for preparation and participation in future international telecommunication conferences were evaluated. Congressional concern for the adequacy of existing machinery and procedures for U.S. policymaking and preparation for such conferences were reflected. WARC-79 and related international conferences demonstrate that contention for access to the radio spectrum and its important collateral element, the geostationary orbit for communication satellites, presents new and urgent challenges to vital U.S. national interests. Given the complexities of spectrum management in a changing world environment and the increased importance of telecommunications to both developed and developing nations, it is unlikely that traditional U.S. approaches to these issues are sufficient to protect vital U.S. interests in the future. Problems require strategies not yet developed or tested.

  5. Editorial: Special Issue (SI): International Conference on Science Education (ICSE)

    NASA Astrophysics Data System (ADS)

    Liu, Xiufeng; Zhang, BaoHui

    2014-04-01

    In the context of science education globalization, the International Conference on Science Education was held in Nanjing, China, in October 2012. The purpose of this conference was to provide a forum for science education researchers from China and from the rest of the world to exchange research ideas and best practices in science education. A call for papers for a special issue of the Journal of Science Education and Technology was made to all conference participants, and a set of six articles was resulted from a standard peer review process. This set of six articles provides a snapshot of research in China and in some other countries, and represents a dialogue between Chinese science education researchers and science education researchers from other countries. We call for more exchange and collaboration in science education between China and the rest of the world.

  6. Radio Sounding Science at High Powers

    NASA Technical Reports Server (NTRS)

    Green, J. L.; Reinisch, B. W.; Song, P.; Fung, S. F.; Benson, R. F.; Taylor, W. W. L.; Cooper, J. F.; Garcia, L.; Markus, T.; Gallagher, D. L.

    2004-01-01

    Future space missions like the Jupiter Icy Moons Orbiter (JIMO) planned to orbit Callisto, Ganymede, and Europa can fully utilize a variable power radio sounder instrument. Radio sounding at 1 kHz to 10 MHz at medium power levels (10 W to kW) will provide long-range magnetospheric sounding (several Jovian radii) like those first pioneered by the radio plasma imager instrument on IMAGE at low power (less than l0 W) and much shorter distances (less than 5 R(sub E)). A radio sounder orbiting a Jovian icy moon would be able to globally measure time-variable electron densities in the moon ionosphere and the local magnetospheric environment. Near-spacecraft resonance and guided echoes respectively allow measurements of local field magnitude and local field line geometry, perturbed both by direct magnetospheric interactions and by induced components from subsurface oceans. JIMO would allow radio sounding transmissions at much higher powers (approx. 10 kW) making subsurface sounding of the Jovian icy moons possible at frequencies above the ionosphere peak plasma frequency. Subsurface variations in dielectric properties, can be probed for detection of dense and solid-liquid phase boundaries associated with oceans and related structures in overlying ice crusts.

  7. The Radio Meteor Zoo: a citizen science project

    NASA Astrophysics Data System (ADS)

    Calders, S.; Verbeeck, C.; Lamy, H.; Martínez Picar, A.

    2016-01-01

    Scientists from the BRAMS radio meteor network have started a citizen science project called Radio Meteor Zoo in collaboration with Zooniverse in order to identify meteor reflections in BRAMS spectrograms. First, a small-scale version of the Radio Meteor Zoo was carried out with a sample of meteor identifications in 12 spectrograms by 35 volunteers. Results are presented here and allowed us to define a method that reliably detects meteor reflections based on the identifications by the volunteers. It turns out that, if each spectrogram is inspected by 10 volunteers, hit and false detection percentages of 95% respectively 6% are expected. The Radio Meteor Zoo is online at https://www.zooniverse.org/projects/zooniverse/radio-meteor-zoo. Citizen scientists are kindly invited to inspect spectrograms.

  8. Undergraduate Teaching in the Animal Sciences, Proceedings of a Conference.

    ERIC Educational Resources Information Center

    Commission on Education in Agriculture and Natural Resources, Washington, DC.

    The proceedings of a conference which reviewed the content of undergraduate animal science curricula, content of courses in the animal sciences, and methods and materials used in undergraduate teaching in the animal sciences are presented in this bulletin. These individual papers are included: Trends in Animal Agriculture and the Future of…

  9. The First URTNA Conference on Educational Radio and Television, Algiers: 2nd - 9th October 1969

    ERIC Educational Resources Information Center

    Kirby, Brian

    1969-01-01

    Discussed are the conference's "three main aspects: (a) defining the role of radio and television in rural areas at both school and adult levels; (b) studying the adaptation of programme method and content in the rural context; (c) examining the training of broadcasters for educational purposes. (Author/LS)

  10. PREFACE: Tsukuba International Conference on Materials Science 2013

    NASA Astrophysics Data System (ADS)

    Kijima, Masashi; Ohshima, Kenichi; Kojima, Seiji; Nagasaki, Yukio; Miyazaki, Shuichi; Kim, Hee Young; Kadowaki, Kazuo; Kashiwagi, Takanari; Nakamura, Junji; Yamamoto, Yohei; Goto, Hiromasa

    2014-03-01

    Tsukuba International Conference on Materials Science (TICMS) was held from 28th August to 6th September, 2013 for the celebration of 40th year anniversary of the University of Tsukuba. The conference was organized by the Division of Materials Science, in cooperation with the Graduate School of Pure and Applied Sciences, and Tsukuba Research Center for Interdisciplinary Materials Science. The purpose of the conference was to provide a unique forum for researchers and students working in various fields of materials science, which have been progressing so rapidly that no single society could cover. The conference consists of following seven workshops to cover various fields. The organizing committee believed that the conference gave all participants new insights into the widespread development of materials science and enhanced the circulation, among them, of information released at the conference. The organizers are grateful for the financial support from University of Tsukuba. This volume contains 25 selected papers from invited and contributed papers, all of which have been screened on the basis of the standard review process of the program committee. The editors express their thanks to those authors who contributed the papers published in this proceedings, which reflects the scientific value of the conference. Nov. 20, 2013 Seiji Kojima, Prof. Dr. Chair, Division of Materials Science Chair, Doctoral Program in Materials Science TICMS 2013 (http://www.ticonfms.tsukuba.ac.jp/) Workshop list The 13th Japan-Korea Joint Workshop on Materials Science Summer School of Biomaterials Science The Japan-Korea Joint Workshop on Shape Memory and Superelastic Technologies The 2nd Workshop on THz Radiation from Intrinsic Josephson Junctions The 3rd German-Japan Nanoworkshop TICMS and IWP Joint Workshop on Conjugated Polymers International Workshop on Science and Patents (IWP) 2013

  11. Planeta Vivo Radio: a 365 chapter story between science and radio

    NASA Astrophysics Data System (ADS)

    Calvo, David; Villalba, Eustaquio; Rodríguez, Fátima; Álvarez, Domingo; Pérez, Nemesio M.

    2016-04-01

    PLANETA VIVO RADIO (http://www.planetavivoradio.es/) is a joint effort of the Spanish National Public Radio in the Canary Islands (RNE-Canarias) and Instituto Volcanológico de Canarias (INVOLCAN) to broadcast scientific and technological advances related to Earth Sciences and the Earth Planet. This initiative was born in a very special year, 2008, the International Year of the Planet Earth, and is actually co-financed by the Parque Científico y Tecnológico de Tenerife (PCTT) and co-financed by the PROCIVMAC project. This 50 minutes weekly radio program broadcast scientists' interviews and scientific/technological reports related to the state of the art of several topics of scientific and social interest in addition to a weekly report of natural hazards that have occurred in the Earth Planet during the last week turning "PLANETAVIVORADIO" as a milestone of the Earth Sciences for the society. Since that moment, Planeta Vivo Radio has been broadcasted through 365 weeks in a continuous way. Several modifications have been added to the program, being divided today into eight different parts, a mix with interviews, reports, ephemerals, bios, agenda and the review to the most prominent natural hazards occurring through the last seven days. Since October 2015, Planeta Vivo Radio is the longest science radio program ever broadcasted in the Canary Islands.

  12. Puerto Ricans in Science and Biomedicine: Report of a Conference.

    ERIC Educational Resources Information Center

    American Association for the Advancement of Science, Washington, DC.

    Twelve divisions and institutes of the National Institutes of Health (NIH) cosponsored this conference to examine the barriers to participation of Puerto Ricans in the United States to careers in science and biomedicine. Areas addressed during the conference included: (1) perspectives from the NIH; (2) historical and modern perspectives of…

  13. A Deep Space Network Portable Radio Science Receiver

    NASA Technical Reports Server (NTRS)

    Jongeling, Andre P.; Sigman, Elliott H.; Chandra, Kumar; Trinh, Joseph T.; Navarro, Robert; Rogstad, Stephen P.; Goodhart, Charles E.; Proctor, Robert C.; Finley, Susan G.; White, Leslie A.

    2009-01-01

    The Radio Science Receiver (RSR) is an open-loop receiver installed in NASA s Deep Space Network (DSN), which digitally filters and records intermediate-frequency (IF) analog signals. The RSR is an important tool for the Cassini Project, which uses it to measure perturbations of the radio-frequency wave as it travels between the spacecraft and the ground stations, allowing highly detailed study of the composition of the rings, atmosphere, and surface of Saturn and its satellites.

  14. Impact of the 1985 Space World Administrative Radio Conference on frequency/orbit planning and use

    NASA Technical Reports Server (NTRS)

    Miller, E. F.

    1986-01-01

    The 1985 World Administrative Radio Conference (WARC-ORB-85) was held to determine which space radio services should be planned and which planning methods should be used. The second session of this Conference (WARC-ORB-88) will meet to develop the required plans. This paper presents the results of WARC-ORB-85, assesses the impact of those decisions, and identifies the intersessional work to be conducted by administrations and the CCIR (Consultative Committee on International Radio). The major decisions of WARC-ORB-85 were: (1) the restriction of additional planning to the fixed satellite service at identified frequencies; and (2) the selection of a planning method consisting of two parts (a) an allotment plan, and (b) improved procedures. The paper also discusses WARC-ORB-85 decisions relative to the Region 2 broadcast satellite service plans at 12 GHz, feederlink planning for Regions 1 and 3 broadcast satellites at 12 GHz, and sound broadcast satellite service.

  15. Remote Radio Sounding Science for JIMO

    NASA Technical Reports Server (NTRS)

    Green, J. L.; Reinisch, B. W.; Song, P.; Fung, S. F.; Benson, R. F.; Taylor, W. W.; Cooper, J. F.; Garcia, L.; Gallagher, D.

    2003-01-01

    Radio sounding of the Earth's top side ionosphere and magnetosphere is a proven technique from geospace missions such as the International Satellites for Ionospheric Studies (ISIS) and the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE). Application of this technique to the Jupiter Icy Moons Orbiter (JIMO) mission will provide unique remote sensing observations of the plasma and magnetic field environments, and the subsurface conductivities, of Europa, Ganymede, and Callisto. Spatial structures of ionospheric plasma above the moon surfaces vary in response to magnetic field perturbations from (1) magnetospheric plasma flows, (2) ionospheric currents from ionization of sputtered surface material, and (3) induced electric currents in salty subsurface oceans. Radio sounding at 3 kHz to 10 MHz can provide globally-determined electron densities necessary for the extraction of the oceanic current signals and supplements in-situ plasma and magnetic field measurements. Subsurface variations in conductivity, can be investigated by radio sounding from 10 MHz to 40 MHz allowing the determination of the presence of dense and solid-liquid phase boundaries associated with oceans and related structures in overlying ice crusts.

  16. AGU Science Policy Conference: 2012 Recap and 2013 Preview

    NASA Astrophysics Data System (ADS)

    Hankin, E. R.; Landau, E. A.; Uhlenbrock, K. M.

    2012-12-01

    In recent years, science has become inextricably linked to the political process. As such, it is more important now than ever for science to forge a better relationship with politics, for the health of both science and society. To help meet this need, the American Geophysical Union (AGU) strives to engage its members, shape policy, and inform society about the excitement of Earth and space science and its role in developing solutions for the sustainability of the planet. In the spring of 2012, AGU held its inaugural Science Policy Conference in Washington, D.C. The goal of this new conference is to ensure diverse discussions and viewpoints on the challenges and opportunities of Earth and space science policy. The meeting brought together more than 300 scientists, policymakers, industry professionals, members of the press, and other stakeholders to discuss Arctic, oceans, natural resources, and natural hazards science as they relate to challenges impacting society. Sessions such as Hydraulic Fracturing, Mitigation and Resiliency to Severe Weather, Governance and Security in the Arctic, and Ocean Acidification are examples of some of the intriguing science policy issues addressed at the conference. The AGU Science Policy Conference will be an annual spring event in Washington, D.C.

  17. IMPROVING SCIENCE EDUCATION. REPORT OF A NATIONAL CONFERENCE OF SCIENCE SUPERVISORS (JUNE 14-17, 1966).

    ERIC Educational Resources Information Center

    PILTZ, ALBERT; STIEDLE, WALTER

    PROCEEDINGS OF A CONFERENCE FOR STATE SCIENCE SUPERVISORS ARE SUMMARIZED. MAJOR SPEECHES ARE CONCERNED WITH (1) STATE LEADERSHIP IN SCIENCE, (2) LEARNING THEORY, (3) THE AMERICAN ASSOCIATION FOR THE ADVANCEMENT OF SCIENCE ELEMENTARY SCIENCE PROGRAM, (4) OUTDOOR SCIENCE EDUCATION, (5) TITLE III OF THE NATIONAL DEFENSE EDUCATION ACT, (6) TITLES I,…

  18. MPS Internships in Public Science Education: Sensing the Radio Sky

    NASA Astrophysics Data System (ADS)

    Blake, Melvin; Castelaz, M. W.; Moffett, D.; Walsh, L.; LaFratta, M.

    2006-12-01

    The intent of the “Sensing the Radio Sky” program is to teach high school students the concepts and relevance of radio astronomy through presentations in STARLAB portable planetariums. The two year program began in the summer of 2004 and was completed in December 2006. The program involved a team of 12 undergraduate physics and multimedia majors and four faculty mentors from Furman University, University of North Carolina-Asheville and Pisgah Astronomical Research Institute (PARI). One component of the program is the development and production of a projection cylinder for the portable STARLAB planetariums. The cylinder gives a thorough view of the Milky Way and of several other celestial sources in radio wavelengths, yet these images are difficult to perceive without prior knowledge of radio astronomy. Consequently, the Radio Sky team created a multimedia presentation to accompany the cylinder. This multimedia component contains six informative lessons on radio astronomy assembled by the physics interns and numerous illustrations and animations created by the multimedia interns. The cylinder and multimedia components complement each other and provide a unique, thorough, and highly intelligible perspective on radio astronomy. The final draft is complete and will be sent to Learning Technologies, Inc., for marketing to owners of STARLAB planetariums throughout the world. We acknowledge support from the NSF Internship in Public Science Education Program grant number 0324729.

  19. Observability of Rembrandt scarp with Mercury Radio Science Experiment

    NASA Astrophysics Data System (ADS)

    Junior Mariani, Mirco; Marabucci, Manuela; Di Achille, Gaetano

    2015-04-01

    The radio science experiment of the ESA mission BepiColombo (MORE, Mercury Orbiter Radio science Experiment) is devoted to the estimation of Mercury's gravity field with unprecedented accuracy, by means of highly stable, multi-frequency radio links in X and Ka band, provided by the Ka band transponder (KaT) on-board the Mercury Planetary Orbiter (MPO). The estimation of gravity field coefficients and planetary tidal deformation with radio science experiment will provide fundamental constraints for modelling planet interior, but additional analysis can be carried out in order to verify whether radio science can give a significant contribution in the study of other physical phenomena, like for example crustal thickening due to tectonic phenomena. This paper reports on the observability of Mercury scarps and crustal thickening with the Mercury Orbiter Radio science experiment, exploiting the extremely precise radio observables (range rate accuracies of 3 micron/s at 1000 s integration time at nearly all elongation angles, and range observables accuracies of 20 cm two-way). One of the largest surface structures of Mercury's surface is the Rembrandt scarp, which can be modeled with a length of 1000 km, an average width of 300 km and a height of 5 km, assuming a flat-ramp-flat tectonic geometry for its enucleation. In general, a surface structure can be observed with radio science if the variation in velocity due to the change in the gravitational potential is larger than the accuracy of the signal at an integration time equal to the interaction time between the spacecraft and the structure, e.g. about 100s for the Rembrandt scarp. Based on our simualtions, the gravity anomalies associated to the Rembrandt scarp can potentially produce effects on the spacecraft orbit that are significantly higher than the expected noise. Therefore, there is an excellent chance that the density contrast generated by the crustal thickness along the Rembrandt scarp will be measurable to a

  20. PREFACE: The International Conference on Science of Friction

    NASA Astrophysics Data System (ADS)

    Miura, Kouji; Matsukawa, Hiroshi

    2007-07-01

    The first international conference on the science of friction in Japan was held at Irago, Aichi on 9-13 September 2007. The conference focused on the elementary process of friction phenomena from the atomic and molecular scale view. Topics covered in the conference are shown below.:

  21. Superlubricity and friction
  22. Electronic and phononic contributions to friction
  23. Friction on the atomic and molecular scales
  24. van der Waals friction and Casimir force
  25. Molecular motor and friction
  26. Friction and adhesion in soft matter systems
  27. Wear and crack on the nanoscale
  28. Theoretical studies on the atomic scale friction and energy dissipation
  29. Friction and chaos
  30. Mechanical properties of nanoscale contacts
  31. Friction of powder
  32. The number of participants in the conference was approximately 100, registered from 11 countries. 48 oral and 29 poster talks were presented at the conference. This volume of Journal of Physics: Conference Series includes 23 papers devoted to the above topics of friction. The successful organization of the conference was made possible by the contribution of the members of the Organizing Committee and International Advisory Committee. The conference was made possible thanks to the financial support from Aichi University of Education and the Taihokogyo Tribology Research Foundation (TTRF), and moreover thanks to the approval societies of The Physical Society of Japan, The Surface Science Society of Japan, The Japanese Society of Tribologists and Toyota Physical and Chemical Research Institute. The details of the conference are available at http://www.science-of-friction.com . Finally we want to thank the speakers for the high quality of their talks and all participants for coming to Irago, Japan and actively contributing to the conference. Kouji Miura and Hiroshi Matsukawa Editors

  1. NSF Internships in Public Science Education: Sensing the Radio Sky

    NASA Astrophysics Data System (ADS)

    Hund, L.; Boltuch, D.; Fultz, C.; Buck, S.; Smith, T.; Harris, R.; Moffett, D.; LaFratta, M.; Walsh, L.; Castelaz, M. W.

    2005-12-01

    The intent of the "Sensing the Radio Sky" project is to teach high school students the concepts and relevance of radio astronomy through presentations in STARLAB portable planetariums. The two year project began in the summer of 2004. A total of twelve interns and four faculty mentors from Furman University and UNCA have participated at the Pisgah Astronomical Research Institute to develop the Radio Sky project. The project united physics and multimedia majors and allowed these students to apply their knowledge of different disciplines to a common goal. One component of the project is the development and production of a cylinder to be displayed in portable STARLAB planetariums. The cylinder gives a thorough view of the Milky Way and of several other celestial sources in radio wavelengths, yet these images are difficult to perceive without prior knowledge of radio astronomy. Consequently, the Radio Sky team created a multimedia presentation to accompany the cylinder. This multimedia component contains six informative lessons on radio astronomy assembled by the physics interns and numerous illustrations and animations created by the multimedia interns. The cylinder and multimedia components complement each other and provide a unique, thorough, and highly intelligible perspective on radio astronomy. The project is near completion and the final draft will be sent to Learning Technologies, Inc., for marketing to owners of STARLAB planetariums throughout the world. The development of the Radio Sky project has also provided a template for potential similar projects that examine our universe in different wavelengths, such as gamma ray, x-ray, and infrared. We acknowledge support from the NSF Internship in Public Science Education Program grant number 0324729.

  2. Thank you to 2015 reviewers of Radio Science

    NASA Astrophysics Data System (ADS)

    Wilkinson, Phil; Salous, Sana

    2016-04-01

    On behalf of Radio Science, AGU, and the scientific community, the editors and associate editors would like to thank everybody who reviewed manuscripts for Radio Science in 2015. Peer review is widely accepted as an indispensable part of science. The hours spent reading and commenting on manuscripts not only improve the manuscripts themselves, but also ensure the scientific rigor of future research in our field. These contributions are vital. Many of those listed below went further and reviewed three or more manuscripts for our journal, and they are indicated in italics. Overall, reviewers contributed 591 individual reviews of 282 manuscripts. Thank you once again to all our reviewers for contributing your valuable time to this essential task. We look forward to a 2016 of exciting advances in our field and communicating those advances to our community and to the broader public.

  3. FOREWORD: Proceedings of the Nordic Conference on Surface Science

    NASA Astrophysics Data System (ADS)

    Pessa, V. M.; Nieminen, R. M.

    1983-01-01

    The present issue of Physica Scripta contains the Proceedings of the Nordic Conference on Surface Science. This meeting was held in Tampere, Finland 18-20 August, 1982. The original motivation for the conference was to bring together the various Nordic research groups engaged in surface science and related activities. However, soon after the initial announcement the conference attracted considerable interest also beyond the Nordic area, and it eventually obtained a truly international character: more than half of the 150 participants came from non-Nordic countries. At least to some extent this reflects the high international esteem of surface physics and chemistry in the Nordic area, which hosts some of the strongest research centers in this exciting and important branch of science. The conference provided an opportunity to exchange information in this rapidly moving field, to establish new contacts and strengthen old ones. It showed that there certainly is scope for increased collaboration between various groups, both within the Nordic countries and also more internationally. The opinion was expressed by several participants that this conference was a particularly successful one, both in scientific content and in format. It is the hope of the organizers of the Nordic Conference on Surface Science that this would serve as an incentive to consider having this kind of meetings on a more or less regular basis, as an established event in the Nordic surface science community. The cross-disciplinary nature of surface science is clearly reflected in these proceedings. The topics discussed range from those close to more traditional condensed matter spectroscopy through physical chemistry to biology. The formidable array of sophisticated techniques developed for surface investigations is given ample attention, but nevertheless the proceedings also show the trend towards more problem-oriented instead of technique-oriented emphasis. The proceedings are organized in accordance

  4. Visions for a sustainable world: A conference on science, technology and social responsibility. Conference report

    SciTech Connect

    Not Available

    1992-12-31

    This report summarizes the organization, activities, and outcomes of Student Pugwash USA`s 1992 International Conference, Visions for a Sustainable World: A Conference on Science, Technology and Social Responsibility. The conference was held June 14--20, 1992 at Emory University, and brought together 94 students and over 65 experts from industry, academe, and government. The conference addressed issues ranging from global environmental cooperation to the social impacts of the Human Genome Project to minority concerns in the sciences. It provided a valuable forum for talented students and professionals to engage in critical dialogue on many interdisciplinary issues at the juncture of science, technology and society. The conference challenged students -- the world`s future scientists, engineers, and political leaders -- to think broadly about global problems and to devise policy options that are viable and innovative. The success of the conference in stimulating interest, understanding, and enthusiasm about interdisciplinary global issues is clearly evident from both the participants` feedback and their continued involvement in Student Pugwash USA programs. Six working groups met each morning. The working group themes included: environmental challenges for developing countries; energy options: their social and environmental impact; health care in developing countries; changing dynamics of peace and global security; educating for the socially responsible use of technology; ethics and the use of genetic information. The conference was specifically designed to include mechanisms for ensuring its long-term impact. Participants were encouraged to focus on their individual role in helping resolve global issues. This was achieved through each participant`s development of a Personal Plan of Action, a plan which mapped out activities the student could undertake after the conference to continue the dialogue and work towards the resolution of global and local problems.

  5. PREFACE: International Conference on Applied Sciences 2015 (ICAS2015)

    NASA Astrophysics Data System (ADS)

    Lemle, Ludovic Dan; Jiang, Yiwen

    2016-02-01

    The International Conference on Applied Sciences ICAS2015 took place in Wuhan, China on June 3-5, 2015 at the Military Economics Academy of Wuhan. The conference is regularly organized, alternatively in Romania and in P.R. China, by Politehnica University of Timişoara, Romania, and Military Economics Academy of Wuhan, P.R. China, with the joint aims to serve as a platform for exchange of information between various areas of applied sciences, and to promote the communication between the scientists of different nations, countries and continents. The topics of the conference cover a comprehensive spectrum of issues from: >Economical Sciences and Defense: Management Sciences, Business Management, Financial Management, Logistics, Human Resources, Crisis Management, Risk Management, Quality Control, Analysis and Prediction, Government Expenditure, Computational Methods in Economics, Military Sciences, National Security, and others... >Fundamental Sciences and Engineering: Interdisciplinary applications of physics, Numerical approximation and analysis, Computational Methods in Engineering, Metallic Materials, Composite Materials, Metal Alloys, Metallurgy, Heat Transfer, Mechanical Engineering, Mechatronics, Reliability, Electrical Engineering, Circuits and Systems, Signal Processing, Software Engineering, Data Bases, Modeling and Simulation, and others... The conference gathered qualified researchers whose expertise can be used to develop new engineering knowledge that has applicability potential in Engineering, Economics, Defense, etc. The number of participants was 120 from 11 countries (China, Romania, Taiwan, Korea, Denmark, France, Italy, Spain, USA, Jamaica, and Bosnia and Herzegovina). During the three days of the conference four invited and 67 oral talks were delivered. Based on the work presented at the conference, 38 selected papers have been included in this volume of IOP Conference Series: Materials Science and Engineering. These papers present new research

  6. Reflections on a Career in Radio Science

    NASA Astrophysics Data System (ADS)

    Peden, Irene C.

    2006-12-01

    Why would a WWII-generation teenager select an engineering career? Dr. Peden outlines the background, motivations and patterns of personal interest that led to her choice in the wartime “climate” of that period, including the influence of teachers and parents. She remembers experiencing the need to undertake graduate studies 10 years later, and recalls why she chose an academic career. She later became a leader in campus and national efforts to improve the professional climate for women, and will comment on the variation s in campus attitudes toward diversity over the years. Finally, she offers her thoughts on the special challenges for faculty that are presented by student views of their own responsibilities and roles in engineering education, and reflects on the impact of these factors on the science/mathematics/engineering “pipeline” .

  7. The United Nations Conference on Science and Technology for Development.

    PubMed

    Kaplan, M M

    1979-12-01

    Despite a long gestation period in preparation for the United Nations Conference on Science and Technology for Development (UNCSTD) and overall expenditures estimated at some $50 million for this Vienna held conference, there were no dramatic results. The Conference faced trying to reach some compromise agreement on the following main points: 1) a global information system, and governing principles for the transfer of technology; 2) institutional arrangements, particularly within the United Nations system, which would ensure a high status for an Intergovernmental Committee on Science and Technology for development; and 3) automatically renewable financing to be supplied primarily by the industrialized countries to implement the Plan of Action. Arguments concerning these points occupied 2 committees for 10 working days of the conference. The outcome of negotiations on these identified points included the following: 1) minimal progress in facilitating access to industrial information, and to patent rights and transfer of technology in general; 2) the proposed Intergovernmental Committee on Science and Technology for Development will be open to all interested countries and will report to the United Nations General Assembly through ECOSOC; 3) coordination of the post-conference program of the Plan of Action will be centered in the office of Director-General for Development and International Economic Cooperation at the United Nations; 4) $250 million was named as the target for the first 2 years of operation; and 5) groups of experts will be convened on an ad hoc basis to advise on various matters.

  8. The Third Annual NASA Science Internet User Working Group Conference

    NASA Technical Reports Server (NTRS)

    Lev, Brian S. (Editor); Gary, J. Patrick (Editor)

    1993-01-01

    The NASA Science Internet (NSI) User Support Office (USO) sponsored the Third Annual NSI User Working Group (NSIUWG) Conference March 30 through April 3, 1992, in Greenbelt, MD. Approximately 130 NSI users attended to learn more about the NSI, hear from projects which use NSI, and receive updates about new networking technologies and services. This report contains material relevant to the conference; copies of the agenda, meeting summaries, presentations, and descriptions of exhibitors. Plenary sessions featured a variety of speakers, including NSI project management, scientists, and NSI user project managers whose projects and applications effectively use NSI, and notable citizens of the larger Internet community. The conference also included exhibits of advanced networking applications; tutorials on internetworking, computer security, and networking technologies; and user subgroup meetings on the future direction of the conference, networking, and user services and applications.

  9. Digital signal processing in the radio science stability analyzer

    NASA Technical Reports Server (NTRS)

    Greenhall, C. A.

    1995-01-01

    The Telecommunications Division has built a stability analyzer for testing Deep Space Network installations during flight radio science experiments. The low-frequency part of the analyzer operates by digitizing wave signals with bandwidths between 80 Hz and 45 kHz. Processed outputs include spectra of signal, phase, amplitude, and differential phase; time series of the same quantities; and Allan deviation of phase and differential phase. This article documents the digital signal-processing methods programmed into the analyzer.

  10. PREFACE: 6th European Thermal Sciences Conference (Eurotherm 2012)

    NASA Astrophysics Data System (ADS)

    Petit, Daniel; Le Niliot, Christophe

    2012-11-01

    About EUROTHERM The aim of the EUROTHERM Committee (www.eurothermcommittee.eu) is to promote and foster European cooperation in Thermal Sciences and Heat Transfer by gathering together scientists and engineers working in specialized areas. The Committee consists of members representing and appointed by national bodies in the EU countries. The current President of EUROTHERM is Professor Anton van Steenhoven from the University of Eindhoven (The Netherlands). The Committee organizes and coordinates European scientific events such as the EUROTHERM Seminars (about 4 per year) and the European Thermal Sciences Conference (every 4 years). About the conference This sixth in the series of European Thermal Sciences Conferences (www.eurotherm2012.com) took place in France, in the Conference Centre of Poitiers, Futuroscope. We address special thanks to the 225 reviewers, coming from different European countries, who have evaluated these papers. We also thank the scientific committee, consisting of some EUROTHERM Committee members together with other internationally recognized experts. Their role has been to manage the evaluation of abstracts and the papers selection process as co-coordinators for specific topics. This conference is the joint effort of two laboratories: the PPRIME Institute in Poitiers and the IUSTI laboratory in Marseille. It could not be organized without the efficient help of our secretaries and our technician for the IT support. This volume of Journal of Physics: Conference Series includes 180 articles presented at the conference. Professor Daniel PETIT Chairman, PPRIME Poitiers, France Institut P'(UPR CNRS 3346) ENSMA 1 av. Clément Ader - BP40109 86961 Futuroscope-Chasseneuil France daniel.petit@ensma.fr Professor Christophe LE NILIOT Co-chairman, IUSTI Marseille, France Laboratoire IUSTI UMR CNRS 6595 Technopôle de Chateau-Gombert 5, rue Enrico Fermi 13 453 MARSEILLE CEDEX 13 France christophe.leniliot@polytech.univ-mrs.fr

  11. Proceedings of the eighteenth lunar and planetary science conference

    SciTech Connect

    Ryder, G. )

    1988-01-01

    This book contains the Proceedings of the 18th Lunar and Planetary Science Conference. Topics covered include: Petrogensis and chemistry of lunar samples; geology and petrogensis of the Apollo 15 landing site; Lunar geology and applications; and Extraterrestrial grains: observations and theories.

  12. The First International Conference on Mars Polar Science and Exploration

    NASA Technical Reports Server (NTRS)

    1998-01-01

    This volume contains abstracts of articles that have been accepted for presentation at the First International Conference on Mars Polar Science and Exploration. Articles about the geology of the Martian Polar regions were presented, and analogs from Earth's geology were also presented. Presentations also were given about the probable contents of the Martian polar caps

  13. Sea Changes in Social Science Education: Woods Hole 2000. The Social Science Education Consortium Conference Series.

    ERIC Educational Resources Information Center

    White, Charles S., Ed.

    The agenda for the Social Science Education Consortium conference at Woods Hole (Massachusetts) was designed to continue a tradition of examining scholarship relative to the social sciences in K-12 education. The content focus for this volume, is political science, economics, and sociology. Following a "Foreword" (Matthew T. Downey; Joseph P.…

  14. The History of Radio Astronomy and the National Radio Astronomy Observatory: Evolution Toward Big Science

    NASA Astrophysics Data System (ADS)

    Malphrus, Benjamin Kevin

    1990-01-01

    The purpose of this study is to examine the sequence of events that led to the establishment of the NRAO, the construction and development of instrumentation and the contributions and discovery events and to relate the significance of these events to the evolution of the sciences of radio astronomy and cosmology. After an overview of the resources, a brief discussion of the early days of the science is given to set the stage for an examination of events that led to the establishment of the NRAO. The developmental and construction phases of the major instruments including the 85-foot Tatel telescope, the 300-foot telescope, the 140-foot telescope, and the Green Bank lnterferometer are examined. The technical evolution of these instruments is traced and their relevance to scientific programs and discovery events is discussed. The history is told in narrative format that is interspersed with technical and scientific explanations. Through the use of original data technical and scientific information of historical concern is provided to elucidate major developments and events. An interpretive discussion of selected programs, events and technological developments that epitomize the contributions of the NRAO to the science of radio astronomy is provided. Scientific programs conducted with the NRAO instruments that were significant to galactic and extragalactic astronomy are presented. NRAO research programs presented include continuum and source surveys, mapping, a high precision verification of general relativity, and SETI programs. Cosmic phenomena investigated in these programs include galactic and extragalactic HI and HII, emission nebula, supernova remnants, cosmic masers, giant molecular clouds, radio stars, normal and radio galaxies, and quasars. Modern NRAO instruments including the VLA and VLBA and their scientific programs are presented in the final chapter as well as plans for future NRAO instruments such as the GBT.

  15. International Conference on Materials Science and Technology (ICMST 2012)

    NASA Astrophysics Data System (ADS)

    Joseph, Ginson P.

    2015-02-01

    FROM THE CONVENOR'S DESK The Department of Physics, St. Thomas College Pala, is highly privileged to organize an International Conference on Materials Science and Technology (ICMST 2012) during 10-14 June 2012, and as Convenor of the conference it is with legitimate pride and immense gratitude to God that I remember the most enthusiastic responses received for this from scientists all over the world. In a time of tremendous revolutionary changes in Materials Science and Technology, it is quite in keeping with the tradition of a pioneering institute that St. Thomas College is, to have risen to the occasion to make this conference a reality. We have no doubt that this proved to be a historic event, a real breakthrough, not only for us the organizers but also for all the participants. A conference of this kind provides a nonpareil, a distinctly outstanding platform for the scholars, researchers and the scientists to discuss and share ideas with delegates from all over the world. This had been most fruitful to the participants in identifying new collaborations and strengthening existing relations. That experts of diverse disciplines from across the world were sitting under one roof for five days, exchanging views and sharing findings, was a speciality of this conference. The event has evoked excellent responses from all segments of the Materials Science community worldwide. 600 renowned scholars from 28 countries participated in this. We were uniquely honoured to have Prof. C.N.R. Rao, Chairman, Scientific Advisory Council to the Prime Minister of India, to inaugurate this conference. May I take this opportunity to thank all those who have contributed their valuable share, diverse in tone and nature, in the making of this conference. My whole hearted gratitude is due to the international and national members of the advisory committee for their valuable guidance and involvement. I place on record my heartfelt gratitude to our sponsors. I am sure that this conference has

  16. Numerical arc segmentation algorithm for a radio conference: A software tool for communication satellite systems planning

    NASA Technical Reports Server (NTRS)

    Whyte, W. A.; Heyward, A. O.; Ponchak, D. S.; Spence, R. L.; Zuzek, J. E.

    1988-01-01

    The Numerical Arc Segmentation Algorithm for a Radio Conference (NASARC) provides a method of generating predetermined arc segments for use in the development of an allotment planning procedure to be carried out at the 1988 World Administrative Radio Conference (WARC) on the Use of the Geostationary Satellite Orbit and the Planning of Space Services Utilizing It. Through careful selection of the predetermined arc (PDA) for each administration, flexibility can be increased in terms of choice of system technical characteristics and specific orbit location while reducing the need for coordination among administrations. The NASARC software determines pairwise compatibility between all possible service areas at discrete arc locations. NASARC then exhaustively enumerates groups of administrations whose satellites can be closely located in orbit, and finds the arc segment over which each such compatible group exists. From the set of all possible compatible groupings, groups and their associated arc segments are selected using a heuristic procedure such that a PDA is identified for each administration. Various aspects of the NASARC concept and how the software accomplishes specific features of allotment planning are discussed.

  17. "Adventures in Science": Casting Scientifically Talented Youth as National Resources on American Radio, 1942-1958

    ERIC Educational Resources Information Center

    Terzian, Sevan G.

    2008-01-01

    From 1942 to 1958, a national weekly programme on CBS radio and presented by Science Service, Inc. devoted 37 of its broadcasts to profiling American high school students' achievements in science talent searches, clubs and fairs. These "Adventures in Science" radio programmes cast scientifically talented youth as potential contributors to national…

  18. Twenty-Third Lunar and Planetary Science Conference

    NASA Technical Reports Server (NTRS)

    1992-01-01

    Presented here is a collection of papers from the Twenty-Third Lunar and Planetary Science Conference that were chosen for having the greatest potential interest for the general reading public. The presentations avoid jargon and unnecessarily complex terms. Topics covered include electron microscopy studies of a circumstellar rock, the fractal analysis of lava flows, volcanic activity on Venus, the isotopic signature of recent solar wind nitrogen, and the implications of impact crater distribution on Venus.

  19. Second International Conference on Mars Polar Science and Exploration

    NASA Technical Reports Server (NTRS)

    2000-01-01

    This volume contains abstracts that were presented at the Second International Conference on Mars Polar Science and Exploration, August 21-25, 2000. The abstracts of the presentations given are listed. Presentations were given on the advances in technology, data analysis of past and current missions, and new instruments destined for Mars. Particular attention was paid to the polar regions and what they reveal about Mars.

  20. The fourth International Conference on Information Science and Cloud Computing

    NASA Astrophysics Data System (ADS)

    This book comprises the papers accepted by the fourth International Conference on Information Science and Cloud Computing (ISCC), which was held from 18-19 December, 2015 in Guangzhou, China. It has 70 papers divided into four parts. The first part focuses on Information Theory with 20 papers; the second part emphasizes Machine Learning also containing 21 papers; in the third part, there are 21 papers as well in the area of Control Science; and the last part with 8 papers is dedicated to Cloud Science. Each part can be used as an excellent reference by engineers, researchers and students who need to build a knowledge base of the most current advances and state-of-practice in the topics covered by the ISCC conference. Special thanks go to Professor Deyu Qi, General Chair of ISCC 2015, for his leadership in supervising the organization of the entire conference; Professor Tinghuai Ma, Program Chair, and members of program committee for evaluating all the submissions and ensuring the selection of only the highest quality papers; and the authors for sharing their ideas, results and insights. We sincerely hope that you enjoy reading papers included in this book.

  1. Conference peeks into the past and future of ocean science

    NASA Astrophysics Data System (ADS)

    Showstack, Randy

    During the past 50 fifty years, oceanographic research in the United States has birthed many landmark discoveries and programs that have changed our perception of the seas, how they work, and how mankind interacts with them. During these decades, ocean science also drifted through the Cold War as a frequent and strategic partner with the military, and then largely was weaned away from that source of funding as the National Science Foundation (NSF) became perhaps the principle supporter for the science.Speakers at a NSF conference held in Washington, D.C. in October reviewed some of these achievements, as well as anecdotal remembrances of programs, priorities, and personalities that have shaped ocean sciences over the past five decades, since NSF was founded in 1950. Speakers also peeked into the future of oceanography and significant affects it has on climate, coastal processes, human health, and other societal concerns.

  2. Science Education Future. Proceedings of the Arctic Science Conference (39th, Fairbanks, Alaska, October 7-10, 1988).

    ERIC Educational Resources Information Center

    American Association for the Advancement of Science, Fairbanks, AK. Arctic Div.

    This catalog includes abstracts of each of the papers delivered at the Arctic Science Conference. The conference was divided into the following symposia: (1) "Biochemistry and Molecular Biology"; (2) "An Update of Alaskan Science and Discovery"; (3) "Science Education for the Public"; (4) "Hubbard Glacier, Russell Fjord and Situk River Studies";…

  3. Lunar Radio Telescopes: A Staged Approach for Lunar Science, Heliophysics, Astrobiology, Cosmology, and Exploration

    NASA Technical Reports Server (NTRS)

    Lazio, Joseph; Bowman, Judd D.; Burns, Jack O.; Farrell, W. M.; Jones, D. L.; Kasper, J. C.; MacDowall, R. J.; Stewart, K. P.; Weiler, K.

    2012-01-01

    Observations with radio telescopes address key problems in cosmology, astrobiology, heliophysics, and planetary science including the first light in the Universe (Cosmic Dawn), magnetic fields of extrasolar planets, particle acceleration mechanisms, and the lunar ionosphere. The Moon is a unique science platform because it allows access to radio frequencies that do not penetrate the Earth's ionosphere and because its far side is shielded from intense terrestrial emissions. The instrument packages and infrastructure needed for radio telescopes can be transported and deployed as part of Exploration activities, and the resulting science measurements may inform Exploration (e.g., measurements of lunar surface charging). An illustrative roadmap for the staged deployment of lunar radio telescopes

  4. Planetary data system requirements: Multi-mission radio science requirements for the 1978 to 1988 era

    NASA Technical Reports Server (NTRS)

    Howard, H. T. (Editor)

    1979-01-01

    The functional and performance requirements for support of multimission radio science are established. The classes of radio science investigation are described and the needed data is discussed. This document is for a sliding ten year period and will be iterated as the mission set evolves.

  5. Initial Results of Radio Science in Akatsuki mission

    NASA Astrophysics Data System (ADS)

    Imamura, Takeshi; Ando, Hiroki; Akatsuki Radio Science Team

    2016-10-01

    The Radio Science experiment (RS) in the Akatsuki mission of JAXA aims to determine the vertical structure of the Venus atmosphere, thereby complementing the imaging observations by onboard instruments. The physical quantities to be retrieved are the vertical distributions of the atmospheric temperature, the electron density, the sulfuric acid vapor density, and small-scale density fluctuations. The uniqueness of Akatsuki RS is quasi-simultaneous observations with multi-band cameras dedicated to meteorological study; the cameras can observe the locations probed by RS a short time before or after the occultations. An ultra-stable oscillator (USO) provides a stable reference frequency, which is used for the X-band downlink signal. The signal traverses the Venusian atmosphere near the limb and reaches the ground station, where it is sampled using an open-loop recording system. In the first radio occultation season of March-July, 2016, we plan 8 Venus occultation experiments in total (6 experiments have been done successfully till June). The temperature profiles cover the altitude region of 40-90 km, which enables studies of vertical coupling among different altitude levels and studies of the cloud system. Another target of Akatsuki RS is solar corona. During solar conjunction periods, the downlink signal that traverses the solar corona is recorded at the ground station. The data yields information on the solar wind velocity, plasma density fluctuations, and magnetic field fluctuations from Faraday rotation measurement. In the solar conjunction period of May-June, 2016, 11 occultation experiments were conducted.

  6. South Australian Science Teachers Association Conference and Science Fair, Salisbury Teachers College, July 1971.

    ERIC Educational Resources Information Center

    1971

    The major papers presented at the 1971 conference of the South Australian Science Teachers Association are included in this pamphlet. Scientists from industry, research institutions, and the police forensic laboratory, and practicing teachers presented papers which included descriptions of modern scientific techniques, discussions of the role of…

  7. The Social Science Teacher. 1972. Collected Conference Papers: Social Science Concepts Classroom Methods.

    ERIC Educational Resources Information Center

    Noble, Pat, Ed.; And Others

    Papers in this publication are collected from a conference on social science concepts and classroom methods which focused on the theories of Jerome Bruner. The first article, entitled "Jerome Bruner," outlines four of Bruner's themes--structure, readiness, intuition, and interest--which relate to cognitive learning. Three papers--"Socialization"…

  8. Physiology and applied sciences in Nepal: 1st annual conference

    PubMed Central

    2014-01-01

    With the increasing number of medical schools in Nepal, there is an expected increase in the number of Nepalese physiologists. The first medical school was established in the 1970s. We report here about the first annual conference of Nepalese physiologists on 27-28 September 2013 organized by the Department of Clinical Physiology of the Nepalese Army Institute of Health Sciences (NAIHS) and Kathmandu University School of Medical Sciences (KUMS). Nepalese physiologists are trying to form their own physiological society. In this regard, NAIHS and KUMS have played an important role to bring physiologists from different parts of Nepal involved in teaching, learning, and research activities in medical schools. There were a number of foreign invitees (India, Israel, Italy, Japan, and Sweden). There were plenary presentations on the topics that are relevant in Nepal, e.g., high-altitude physiology and wilderness medicine. The final session of the conference was an open session meeting of Nepalese physiologists. There was an open interaction about establishing Nepalese Physiological Society. After much deliberation, there was an agreement to register the society in Kathmandu with the current ad hoc committee which will elect the first executive body of the society. PMID:24580838

  9. The Deep Space Network as an instrument for radio science research

    NASA Technical Reports Server (NTRS)

    Asmar, S. W.; Renzetti, N. A.

    1993-01-01

    Radio science experiments use radio links between spacecraft and sensor instrumentation that is implemented in the Deep Space Network. The deep space communication complexes along with the telecommunications subsystem on board the spacecraft constitute the major elements of the radio science instrumentation. Investigators examine small changes in the phase and/or amplitude of the radio signal propagating from a spacecraft to study the atmospheric and ionospheric structure of planets and satellites, planetary gravitational fields, shapes, masses, planetary rings, ephemerides of planets, solar corona, magnetic fields, cometary comae, and such aspects of the theory of general relativity as gravitational waves and gravitational redshift.

  10. The Exeter Conference on Secondary School Science Education (Exeter, New Hampshire, June 15-22, 1980).

    ERIC Educational Resources Information Center

    Brinckerhoff, Richard F.; Compton, Charles A.

    In June, 1980, 38 secondary school science teachers and 10 specialists met at Phillips Exeter Academy to discuss the state of science education. Conference participants agreed that a crisis in science education exists. Events appear to indicate that the public is telling science teachers that what they are offering in the name of science education…

  11. Allerton Invitational Conference on Education for Health Sciences Librarianship. Proceedings of a Conference (Monticello, Illinois, April 2-4, 1979).

    ERIC Educational Resources Information Center

    Berk, Robert A., Ed.

    The conference described in this report had five objectives: to examine the existing curricula for medical librarianship in accredited library school programs; to examine trends in post-master's training programs for health sciences librarianship; to explore the relationship between graduate education for health sciences librarianship and the…

  12. Taking the Plunge: Next Steps in Engaged Learning: Project Kaleidoscope-Connecticut Conference of Independent Colleges Conference for Science Educators.

    PubMed

    Frederick, Jennifer

    2010-09-01

    College and university science educators from across Connecticut gathered at Yale's West Campus in April 2010 for a Project Kaleidoscope (PKAL) program entitled "Taking the Plunge: Next Steps in Engaged Learning." Funded by the National Science Foundation (NSF) and co-sponsored by the Connecticut Conference of Independent Colleges (CCIC) and Yale's McDougal Graduate Teaching Center, the event was the latest in a PKAL series of one-day conferences aimed at equipping science, technology, engineering, and math (STEM) instructors with effective approaches to engaging students and training future scientists.

  13. Radio science requirements and the end-to-end ranging system

    NASA Technical Reports Server (NTRS)

    Berman, A. L.

    1978-01-01

    Radio science ranging requirements negotiated between past and present flight projects and the DSN have generally focused on just the DSS and spacecraft hardware. All elements in the end-to-end system are analyzed and considered in terms of the error hierarchy. The end-to-end system is defined and examined as it applies to the generation of radio science ranging requirements. The variability of the performance levels of the system elements is emphasized with respect to the radio science experiment being performed and the DSN-spacecraft frequency band configuration.

  14. Using Twitter to communicate conservation science from a professional conference.

    PubMed

    Bombaci, Sara P; Farr, Cooper M; Gallo, H Travis; Mangan, Anna M; Stinson, Lani T; Kaushik, Monica; Pejchar, Liba

    2016-02-01

    Scientists are increasingly using Twitter as a tool for communicating science. Twitter can promote scholarly discussion, disseminate research rapidly, and extend and diversify the scope of audiences reached. However, scientists also caution that if Twitter does not accurately convey science due to the inherent brevity of this media, misinformation could cascade quickly through social media. Data on whether Twitter effectively communicates conservation science and the types of user groups receiving these tweets are lacking. To address these knowledge gaps, we examined live tweeting as a means of communicating conservation science at the 2013 International Congress for Conservation Biology (ICCB). We quantified and compared the user groups sending and reading live tweets. We also surveyed presenters to determine their intended audiences, which we compared with the actual audiences reached through live tweeting. We also asked presenters how effectively tweets conveyed their research findings. Twitter reached 14 more professional audience categories relative to those attending and live tweeting at ICCB. However, the groups often reached through live tweeting were not the presenters' intended audiences. Policy makers and government and non-governmental organizations were rarely reached (0%, 4%, and 6% of audience, respectively), despite the intent of the presenters. Plenary talks were tweeted about 6.9 times more than all other oral or poster presentations combined. Over half the presenters believed the tweets about their talks were effective. Ineffective tweets were perceived as vague or missing the presenters' main message. We recommend that presenters who want their science to be communicated accurately and broadly through Twitter should provide Twitter-friendly summaries that incorporate relevant hashtags and usernames. Our results suggest that Twitter can be used to effectively communicate speakers' findings to diverse audiences beyond conference walls.

  15. Using Twitter to communicate conservation science from a professional conference.

    PubMed

    Bombaci, Sara P; Farr, Cooper M; Gallo, H Travis; Mangan, Anna M; Stinson, Lani T; Kaushik, Monica; Pejchar, Liba

    2016-02-01

    Scientists are increasingly using Twitter as a tool for communicating science. Twitter can promote scholarly discussion, disseminate research rapidly, and extend and diversify the scope of audiences reached. However, scientists also caution that if Twitter does not accurately convey science due to the inherent brevity of this media, misinformation could cascade quickly through social media. Data on whether Twitter effectively communicates conservation science and the types of user groups receiving these tweets are lacking. To address these knowledge gaps, we examined live tweeting as a means of communicating conservation science at the 2013 International Congress for Conservation Biology (ICCB). We quantified and compared the user groups sending and reading live tweets. We also surveyed presenters to determine their intended audiences, which we compared with the actual audiences reached through live tweeting. We also asked presenters how effectively tweets conveyed their research findings. Twitter reached 14 more professional audience categories relative to those attending and live tweeting at ICCB. However, the groups often reached through live tweeting were not the presenters' intended audiences. Policy makers and government and non-governmental organizations were rarely reached (0%, 4%, and 6% of audience, respectively), despite the intent of the presenters. Plenary talks were tweeted about 6.9 times more than all other oral or poster presentations combined. Over half the presenters believed the tweets about their talks were effective. Ineffective tweets were perceived as vague or missing the presenters' main message. We recommend that presenters who want their science to be communicated accurately and broadly through Twitter should provide Twitter-friendly summaries that incorporate relevant hashtags and usernames. Our results suggest that Twitter can be used to effectively communicate speakers' findings to diverse audiences beyond conference walls. PMID

  16. Development of Radio Astronomy at Centre for Basic Space Science Observatory, Nsukka Nigeria

    NASA Astrophysics Data System (ADS)

    Aliyu, Nasiru; Okere, Bonaventure I.; Lanre, Daniyan O.; Ezechi, Nwachukwu E.

    2015-08-01

    Radio telescopes for research, teaching and learning at Centre for Basic Space Science (CBSS) observatory are currently in place of development. A small parabolic radio telescope with diameter of 3.0 m working at 1420 MHz is already available for general purpose of radio astronomical observations. In addition, a Radio Jove telescope with dual dipole antenna working at 20 MHz and Sudden Ionospheric Disturbance (SID) monitor working at 24 KHz are also available. It is suitable to monitor daily solar burst, solar flares as well as Jupiter decametric emission. More over, CBSS radio interferometers are now under construction. It consists of non-tracking Radio Jove array and SID monitor as well as two radio telescope tracking interferometers. The latter is planned to utilize up to 4 antennas. Multi frequency receivers are made available at 24 KHz, 20 and 1420 MHz and will be used for VLBI in the near future.

  17. IEEE conference record -- Abstracts: 1996 IEEE international conference on plasma science

    SciTech Connect

    1996-12-31

    This meeting covered the following topics: space plasmas; non-equilibrium plasma processing; computer simulation of vacuum power tubes; vacuum microelectronics; microwave systems; basic phenomena in partially ionized gases -- gaseous electronics, electrical discharges; ball lightning/spherical plasma configuration; plasma diagnostics; plasmas for lighting; dense plasma focus; intense ion and electron beams; plasma, ion, and electron sources; flat panel displays; fast z-pinches and x-ray lasers; environmental/energy issues in plasma science; thermal plasma processing; computational plasma physics; magnetic confinement fusion; microwave-plasma interactions; space plasma engineering; EM and ETH launchers; fast wave devices; intense beam microwaves; slow wave devices; space plasma measurements; basic phenomena in fully ionized plasma -- waves, instabilities, plasma theory, etc; plasma closing switches; fast opening switches; and laser-produced plasma. Separate abstracts were prepared for most papers in this conference.

  18. Toward Excellence in Science Education. Proceedings of Annual Curriculum Update Conference (June 18-23, 1982).

    ERIC Educational Resources Information Center

    Iowa Univ., Iowa City. Science Education Center.

    The National Science Teachers Association (NSTA) Horizons Committee met in Iowa City (Iowa) before the 1982 Curriculum Update Conference. The committee was charged with planning a new future of science education. The thinking of the members of the Horizons Committee provided the framework for the 1982 conference. These proceedings represent a…

  19. Radio science receiver support of the Mars Exploration Rover Landings

    NASA Technical Reports Server (NTRS)

    Johnston, Douglas; Asmar, Sami; Chang, Christine; Estabrook, Polly; Finely, Sue; Pham, Timothy; Satorius, Edgar

    2004-01-01

    The low power levels of the communication signals during the Entry Descent and Landing (EDL) sequences of the Mars rovers prevented the transmission of telemetry at X-band signal to inform the mission operations center of the health and progress of the spacecraft. As an altemative, a series of tones were sent to indicate basic spacecraft conditions and execution of critical events. An open-loop receiver designed for Radio Science experiments was used to acquire the signal during this time. The receiver recorded over a 100 Khz bandwidth to identify the presence of the carrier and tones. The data were fed in real-time to a processing unit which detected the carrier and the frequency separation of the tones from the carrier, in order to determine which event has occurred. Up to 256 different tones were possible. During the actual events, all tones were identified, and the carrier was tracked down to the surface, and for the second rover, through the bouncing which followed, and finally, while stopped on the surface, found the carrier and tones which indicated the spacecraft was alive. In order to identify the tones, the ground receivers had to be able to respond to the bevy of events occurring in the relatively short timespan of EDL.

  20. Ka-Band Transponder for Deep-Space Radio Science

    NASA Technical Reports Server (NTRS)

    Dennis, Matthew S.; Mysoor, Narayan R.; Folkner, William M.; Mendoza, Ricardo; Venkatesan, Jaikrishna

    2008-01-01

    A one-page document describes a Ka-band transponder being developed for use in deep-space radio science. The transponder receives in the Deep Space Network (DSN) uplink frequency band of 34.2 to 34.7 GHz, transmits in the 31.8- to 32.3 GHz DSN downlink band, and performs regenerative ranging on a DSN standard 4-MHz ranging tone subcarrier phase-modulated onto the uplink carrier signal. A primary consideration in this development is reduction in size, relative to other such transponders. The transponder design is all-analog, chosen to minimize not only the size but also the number of parts and the design time and, thus, the cost. The receiver features two stages of frequency down-conversion. The receiver locks onto the uplink carrier signal. The exciter signal for the transmitter is derived from the same source as that used to generate the first-stage local-oscillator signal. The ranging-tone subcarrier is down-converted along with the carrier to the second intermediate frequency, where the 4-MHz tone is demodulated from the composite signal and fed into a ranging-tone-tracking loop, which regenerates the tone. The regenerated tone is linearly phase-modulated onto the downlink carrier.

  1. The 26th IEEE international conference on plasma science

    SciTech Connect

    1999-07-01

    Some of the sessions covered by this conference are: Basic Processes in Fully and Partially Ionized Plasmas; Slow Wave Devices; Laser-Produced Plasma; Non-Equilibrium Plasma Processing; Space Plasmas and Partially Ionized Gases; Microwave Plasmas; Inertial Confinement Fusion; Plasma Diagnostics; Computational Plasma Physics; Microwave Systems; Laser Produced Plasmas and Dense Plasma Focus; Intense Electron and Ion Beams; Fast Wave Devices; Spherical Configurations and Ball Lightning; Thermal Plasma Chemistry and Processing and Environmental Issues in Plasma Science; Plasma, Ion, and Electron Sources; Fast Wave Devices and Intense Beams; Fast Z-pinches and X-ray Lasers; Plasma Opening Switches; Plasma for Lighting; Intense Beams; Vacuum Microwaves; Magnetic Fusion Energy; and Plasma Thrusters and Arcs. Separate abstracts were prepared for some of the papers in this volume.

  2. Biotech 2011 conference Zurich University of applied sciences.

    PubMed

    Demuth, Caspar

    2011-01-01

    More than 160 experts from industry and academia came together this September for the Biotech 2011 at the Zurich University of Applied Sciences (ZHAW) in Wädenswil. As one of the main topics, the conference addressed innovations in sensor technology, where new measurement principles and methods have helped to enhance robustness and user friendliness. Another main emphasis of Biotech 2011 was the application of sensors and related analytical techniques in bioprocesses. In this area, the sensor industry needs to meet the challenges introduced by the increasing use of single-use bioreactors. With its strong focus on sensor applications, Biotech 2011 successfully promoted interaction between professionals in academic and industrial research as well as with experts who apply sensors in biopharmaceutical production.

  3. Numerical Arc Segmentation Algorithm for a Radio Conference-NASARC (version 4.0) technical manual

    NASA Technical Reports Server (NTRS)

    Whyte, Wayne A., Jr.; Heyward, Ann O.; Ponchak, Denise S.; Spence, Rodney L.; Zuzek, John E.

    1988-01-01

    The information contained in the NASARC (Version 4.0) Technical Manual and NASARC (Version 4.0) User's Manual relates to the Numerical Arc Segmentation Algorithm for a Radio Conference (NASARC) software development through November 1, 1988. The Technical Manual describes the NASARC concept and the algorithms used to implement the concept. The User's Manual provides information on computer system considerations, installation instructions, description of input files, and program operation instructions. Significant revisions were incorporated in the Version 4.0 software over prior versions. These revisions have further enhanced the modeling capabilities of the NASARC procedure and provide improved arrangements of predetermined arcs within the geostationary orbits. Array dimensions within the software were structured to fit within the currently available 12 megabyte memory capacity of the International Frequency Registration Board (IFRB) computer facility. A piecewise approach to predetermined arc generation in NASARC (Version 4.0) allows worldwide planning problem scenarios to be accommodated within computer run time and memory constraints with enhanced likelihood and ease of solution.

  4. Numerical Arc Segmentation Algorithm for a Radio Conference (NASARC), version 4.0: User's manual

    NASA Technical Reports Server (NTRS)

    Whyte, Wayne A., Jr.; Heyward, Ann O.; Ponchak, Denise S.; Spence, Rodney L.; Zuzek, John E.

    1988-01-01

    The information in the NASARC (Version 4.0) Technical Manual (NASA-TM-101453) and NASARC (Version 4.0) User's Manual (NASA-TM-101454) relates to the state of Numerical Arc Segmentation Algorithm for a Radio Conference (NASARC) software development through November 1, 1988. The Technical Manual describes the NASARC concept and the algorithms used to implement the concept. The User's Manual provides information on computer system considerations, installation instructions, description of input files, and program operation instructions. Significant revisions were incorporated in the Version 4.0 software over prior versions. These revisions have further enhanced the modeling capabilities of the NASARC procedure and provide improved arrangements of predetermined arcs within the geostationary orbit. Array dimensions within the software were structured to fit within the currently available 12-megabyte memory capacity of the International Frequency Registration Board (IFRB) computer facility. A piecewise approach to predetermined arc generation in NASARC (Version 4.) allows worldwide planning problem scenarios to be accommodated within computer run time and memory constraints with enhanced likelihood and ease of solution.

  5. Numerical Arc Segmentation Algorithm for a Radio Conference-NASARC, Version 2.0: User's Manual

    NASA Technical Reports Server (NTRS)

    Whyte, Wayne A., Jr.; Heyward, Ann O.; Ponchak, Denise S.; Spence, Rodney L.; Zuzek, John E.

    1987-01-01

    The information contained in the NASARC (Version 2.0) Technical Manual (NASA TM-100160) and the NASARC (Version 2.0) User's Manual (NASA TM-100161) relates to the state of the Numerical Arc Segmentation Algorithm for a Radio Conference (NASARC) software development through October 16, 1987. The technical manual describes the NASARC concept and the algorithms which are used to implement it. The User's Manual provides information on computer system considerations, installation instructions, description of input files, and program operation instructions. Significant revisions have been incorporated in the Version 2.0 software over prior versions. These revisions have enhanced the modeling capabilities of the NASARC procedure while greatly reducing the computer run time and memory requirements. Array dimensions within the software have been structured to fit into the currently available 6-megabyte memory capacity of the International Frequency Registration Board (IFRB) computer facility. A piecewise approach to predetermined arc generation in NASARC (Version 2.0) allows worldwide scenarios to be accommodated within these memory constraints while at the same time reducing computer run time.

  6. Numerical arc segmentation algorithm for a radio conference-NASARC (version 2.0) technical manual

    NASA Technical Reports Server (NTRS)

    Whyte, Wayne A., Jr.; Heyward, Ann O.; Ponchak, Denise S.; Spence, Rodney L.; Zuzek, John E.

    1987-01-01

    The information contained in the NASARC (Version 2.0) Technical Manual (NASA TM-100160) and NASARC (Version 2.0) User's Manual (NASA TM-100161) relates to the state of NASARC software development through October 16, 1987. The Technical Manual describes the Numerical Arc Segmentation Algorithm for a Radio Conference (NASARC) concept and the algorithms used to implement the concept. The User's Manual provides information on computer system considerations, installation instructions, description of input files, and program operating instructions. Significant revisions have been incorporated in the Version 2.0 software. These revisions have enhanced the modeling capabilities of the NASARC procedure while greatly reducing the computer run time and memory requirements. Array dimensions within the software have been structured to fit within the currently available 6-megabyte memory capacity of the International Frequency Registration Board (IFRB) computer facility. A piecewise approach to predetermined arc generation in NASARC (Version 2.0) allows worldwide scenarios to be accommodated within these memory constraints while at the same time effecting an overall reduction in computer run time.

  7. An Overview of Recent Results from the Cassini Radio and Plasma Wave Science Investigation

    NASA Astrophysics Data System (ADS)

    Gurnett, D.; Kurth, W.; Hospodarsky, G.; Persoon, A.; Averkamp, T.; Cecconi, B.; Lecacheux, A.; Zarka, P.; Canu, P.; Cornilleau-Wehrlin, N.; Galopeau, P.; Roux, A.; Harvey, C.; Louarn, P.; Bostrom, R.; Gustafsson, G.; Wahlund, J.-E.; Desch, M.; Farrell, W.; Kaiser, M.; Kellogg, P.; Goetz, K.; Fischer, G.; Ladreiter, H.-P.; Rucker, H.; Alleyne, H.; Pedersen, A.

    2005-08-01

    The Radio and Plasma Wave Science (RPWS) investigation on the Cassini spacecraft provides measurements of radio emissions, plasma waves, and thermal plasma parameters in the vicinity of Saturn. This paper gives an overview of recent results from the RPWS. These include the most recent measurements of the rotational modulation period of radio emissions from Saturn (Saturn Kilometric Radiation), of impulsive radio bursts from atmospheric lightning (Saturn Electrostatic Discharges), of the distribution of small dust particles near the ring plane, and of the distribution and origin of plasma in the inner regions of the Saturnian system and near Titan.

  8. Trends in Performance and Characteristics of Ultra-Stable Oscillators for Deep Space Radio Science Experiments

    NASA Technical Reports Server (NTRS)

    Asmar, Sami

    1997-01-01

    Telecommunication systems of spacecraft on deep space missions also function as instruments for Radio Science experiments. Radio scientists utilize the telecommunication links between spacecraft and Earth to examine very small changes in the phase/frequency, amplitude, and/or polarization of radio signals to investigate a host of physical phenomena in the solar system. Several missions augmented the radio communication system with an Ultra-Stable Oscillator (USO) in order to provide a highly stable reference signal for oneway downlink. This configuration is used in order to enable better investigations of the atmospheres of the planets occulting the line-of-sight to the spacecraft; one-way communication was required and the transponders' built-in auxiliary oscillators were neither sufficiently stable nor spectrally pure for the occultation experiments. Since Radio Science instrumentation is distributed between the spacecraft and the ground stations, the Deep Space Network (DSN) is also equipped to function as a world-class instrument for Radio Science research. For a detailed account of Radio Science experiments, methodology, key discoveries, and the DSN's historical contribution to the field, see Asmar and Renzetti (1993). The tools of Radio Science can be and have also been utilized in addressing several mission engineering challenges; e.g., characterization of spacecraft nutation and anomalous motion, antenna calibrations, and communications during surface landing phases. Since the first quartz USO was flown on Voyager, the technology has advanced significantly, affording future missions higher sensitivity in reconstructing the temperature pressure profiles of the atmospheres under study as well as other physical phenomena of interest to Radio Science. This paper surveys the trends in stability and spectral purity performance, design characteristics including size and mass, as well as cost and history of these clocks in space.

  9. National conference on environmental remediation science and technology: Abstracts

    SciTech Connect

    1998-12-31

    This conference was held September 8--10, 1998 in Greensboro, North Carolina. The purpose of this conference was to provide a multidisciplinary forum for exchange of state-of-the-art information on methods and site characterization technologies for environmental monitoring and remedial action planning of hazardous materials. This report contains the abstracts of sixty-one papers presented at the conference.

  10. News Conference: Serbia hosts teachers' seminar Resources: Teachers TV website closes for business Festival: Science takes to the stage in Denmark Research: How noise affects learning in secondary schools CERN: CERN visit inspires new teaching ideas Education: PLS aims to improve perception of science for school students Conference: Scientix conference discusses challenges in science education

    NASA Astrophysics Data System (ADS)

    2011-07-01

    Conference: Serbia hosts teachers' seminar Resources: Teachers TV website closes for business Festival: Science takes to the stage in Denmark Research: How noise affects learning in secondary schools CERN: CERN visit inspires new teaching ideas Education: PLS aims to improve perception of science for school students Conference: Scientix conference discusses challenges in science education

  11. Voyager radio science observations of neptune and triton.

    PubMed

    Tyler, G L; Sweetnam, D N; Anderson, J D; Borutzki, S E; Campbell, J K; Eshleman, V R; Gresh, D L; Gurrola, E M; Hinson, D P; Kawashima, N; Kursinski, E R; Levy, G S; Lindal, G F; Lyons, J R; Marouf, E A; Rosen, P A; Simpson, R A; Wood, G E

    1989-12-15

    The Voyager 2 encounter with the Neptune system included radio science investigations of the masses and densities of Neptune and Triton, the low-order gravitational harmonics of Neptune, the vertical structures of the atmospheres and ionospheres of Neptune and Triton, the composition of the atmosphere of Neptune, and characteristics of ring material. Demanding experimental requirements were met successfully, and study of the large store of collected data has begun. The initial search of the data revealed no detectable effects of ring material with optical depth tau [unknown] 0.01. Preliminary representative results include the following: 1.0243 x 10(26) and 2.141 x 10(22) kilograms for the masses of Neptune and Triton; 1640 and 2054 kilograms per cubic meter for their respective densities; 1355 +/- 7 kilometers, provisionally, for the radius of Triton; and J(2) = 3411 +/- 10(x 10(-6)) and J(4) = -26(+12)(-20)(x10(-6)) for Neptune's gravity field (J>(2) and J(4) are harmonic coefficients of the gravity field). The equatorial and polar radii of Neptune are 24,764 +/- 20 and 24,340 +/- 30 kllometers, respectively, at the 10(5)-pascal (1 bar) pressure level. Neptune's atmosphere was probed to a pressure level of about 5 x 10(5) pascals, and effects of a methane cloud region and probable ammonia absorption below the cloud are evident in the data. Results for the mixing ratios of helium and ammonia are still being investigated; the methane abundance below the clouds is at least 1 percent by volume. Derived temperature-pressure profiles to 1.2 x 10(5) pascals and 78 kelvins (K) show a lapse rate corresponding to "frozen" equilibrium of the para- and ortho-hydrogen states. Neptune's ionosphere exhibits an extended topside at a temperature of 950 +/- 160 K if H(+) is the dominant ion, and narrow ionization layers of the type previously seen at the other three giant planets. Triton has a dense ionosphere with a peak electron concentration of 46 x 10(9) per cubic meter at an

  12. Voyager radio science observations of neptune and triton.

    PubMed

    Tyler, G L; Sweetnam, D N; Anderson, J D; Borutzki, S E; Campbell, J K; Eshleman, V R; Gresh, D L; Gurrola, E M; Hinson, D P; Kawashima, N; Kursinski, E R; Levy, G S; Lindal, G F; Lyons, J R; Marouf, E A; Rosen, P A; Simpson, R A; Wood, G E

    1989-12-15

    The Voyager 2 encounter with the Neptune system included radio science investigations of the masses and densities of Neptune and Triton, the low-order gravitational harmonics of Neptune, the vertical structures of the atmospheres and ionospheres of Neptune and Triton, the composition of the atmosphere of Neptune, and characteristics of ring material. Demanding experimental requirements were met successfully, and study of the large store of collected data has begun. The initial search of the data revealed no detectable effects of ring material with optical depth tau [unknown] 0.01. Preliminary representative results include the following: 1.0243 x 10(26) and 2.141 x 10(22) kilograms for the masses of Neptune and Triton; 1640 and 2054 kilograms per cubic meter for their respective densities; 1355 +/- 7 kilometers, provisionally, for the radius of Triton; and J(2) = 3411 +/- 10(x 10(-6)) and J(4) = -26(+12)(-20)(x10(-6)) for Neptune's gravity field (J>(2) and J(4) are harmonic coefficients of the gravity field). The equatorial and polar radii of Neptune are 24,764 +/- 20 and 24,340 +/- 30 kllometers, respectively, at the 10(5)-pascal (1 bar) pressure level. Neptune's atmosphere was probed to a pressure level of about 5 x 10(5) pascals, and effects of a methane cloud region and probable ammonia absorption below the cloud are evident in the data. Results for the mixing ratios of helium and ammonia are still being investigated; the methane abundance below the clouds is at least 1 percent by volume. Derived temperature-pressure profiles to 1.2 x 10(5) pascals and 78 kelvins (K) show a lapse rate corresponding to "frozen" equilibrium of the para- and ortho-hydrogen states. Neptune's ionosphere exhibits an extended topside at a temperature of 950 +/- 160 K if H(+) is the dominant ion, and narrow ionization layers of the type previously seen at the other three giant planets. Triton has a dense ionosphere with a peak electron concentration of 46 x 10(9) per cubic meter at an

  13. Proceedings of the Plutonium Futures ? The Science 2006 Conference

    SciTech Connect

    Fluss, M; Hobart, D; Allan, P; Jarvinen, G

    2007-07-12

    Plutonium Futures--The Science 2006 provided opportunities to examine present knowledge of the chemical and physical properties of plutonium and other actinides in complex media and materials; to discuss the current and emerging science (chemistry, physics, materials science, nuclear science, and environmental effects) of plutonium and actinides relevant to enhancing global nuclear security; and to exchange ideas. This international conference also provided a forum for illustrating and enhancing capabilities and interests, and assessing issues in these areas. U.S. and international scientists, engineers, faculty, and students from universities, national laboratories, and DOE's nuclear complex were encouraged to participate and make technical contributions. The Conference ran from Sunday, July 9th through Thursday, July 13th. A popular aspect of the conference was the opening tutorial session on Sunday afternoon intended for students and scientists new to the area of plutonium research. The tutorial was well attended by novices and veterans alike, and featured such diverse topics as; plutonium metallurgy, plutonium in the environment, and international arms control and nonproliferation. Two plenary lectures began each morning and each afternoon session and highlighted the breakout sessions on coordination/organometallic chemistry, solid-state physics, environmental chemistry, materials science, separations and reprocessing, advanced fuels and waste forms, phase transformations, solution and gas-phase chemistry, compounds and complexes, electronic structure and physical properties, and more. Chemistry Highlights--Among the many chemistry highlights presented in this proceedings are the overview of concepts and philosophies on inert nuclear fuel matrices and concerns about the ever-increasing amounts of minor actinides and plutonium generated in the fuel cycle. The various ideas involve multiple reduction schemes for these materials, suggesting fuels for 'burning' or

  14. Results from the Mars Climate Sounder and Intercomparison of Data with Radio Science

    NASA Astrophysics Data System (ADS)

    McCleese, D. J.; Schofield, J. T.; Hinson, D. P.; Abdou, W. A.; Kleinboehl, A.; Kass, D. M.

    2012-12-01

    The Mars Climate Sounder (MCS) on MRO has obtained a record of the vertical structure of Martian atmospheric temperature, dust, and water ice clouds extending more than 3 Mars years (MY 28-MY 31). When added to the data set acquired by the highly successful Thermal Emission Spectrometer (TES) on MGS, a nearly continuous climate record now exists of sufficient duration (>7 Mars years) to study dominant modes of the atmospheric circulation and interannual variability. New insight into the vertical structure of dust and condensates has changed our perception of the role of aerosols and their variability in driving the global circulation. Recent work by Kleinböhl, et al (this conference) utilizes MCS coverage of local time of day to observe and model semi-diurnal tides. In this paper we discuss the robustness of inferences drawn from MCS data, our efforts to validate the observations, and explore the continuity of the data with previous and concurrent measurements. Comparison of profiles of temperature from MCS and MRO Radio Science (RS) are particularly useful because the two measurement techniques are based on different physical principles. Radio occultations sound the limb of Mars with an X-band radio signal (~4 cm wavelength), using measurements of refractive bending to derive profiles of density, temperature, and pressure versus radius. This is a physically independent mechanism from the thermal emission measurements of MCS and, unlike MCS, RS is insensitive to dust and aerosol. Also, RS investigations were conducted on both MGS and MRO providing a means of comparing the non-overlapping TES and MCS observations. On MRO, RS profiles are obtained roughly once per day on ingress occultations only. RS temperature measurements extend from 0-40 km with a vertical resolution of about 1 km, and are particularly accurate in the lower half of this range. MCS obtains temperatures from 0-80 km, and is able to use its two-axis articulation to make simultaneous and coincident

  15. 11th National Conference on Science, Policy, and the Environment: Our Changing Oceans

    SciTech Connect

    Peter Saundry

    2012-04-17

    On January 19-21, 2011, The National Council for Science and the Environment (NCSE) successfully convened its 11th National Conference on Science, Policy and the Environment: Our Changing Oceans in Washington, DC at the Ronald Reagan Building and International Trade Center. Over 1,247 participants attended the conference, representing federal, state and local governments, university and colleges across the US, civil society organizations, the business community, and international entities. In addition, the conference was webcast to an audience across several states. The conference provided a forum to examine the profound changes our ocean will undergo over the next 25-50 years and share various perspectives on the new research, tools, and policy initiatives to protect and sustain our ocean. Conference highlights and recommendations are available to the public on NCSE's conference website, www.OurChangingOceans.org.

  16. State-Controlled Multimedia Education for All? Science Programs in Early German Radio

    ERIC Educational Resources Information Center

    Schirrmacher, Arne

    2012-01-01

    While science education and popularization by means of print media developed in quite similar forms in many nations, the advent of radio resulted in initiatives to bring science on the air that were rather heterogeneous from country to country. The German case stands out with respect to quantity, variety and ambition, and also for its special…

  17. Producing a Radio Show about Psychological Science: The Story of "Psychological Frontiers"

    ERIC Educational Resources Information Center

    Stark, Emily; Sachau, Daniel; Albertson, Dawn N.

    2012-01-01

    The authors describe the development of a campus-based radio show about psychological science. The authors' goals in creating the show were to inform the public about the science of psychology and to create a teaching and learning resource for faculty members and students. The show, "Psychological Frontiers," airs twice a week and consists of…

  18. The Five-hundred-meter Aperture Spherical radio Telescope project and its early science opportunities

    NASA Astrophysics Data System (ADS)

    Li, Di; Nan, Rendong; Pan, Zhichen

    2013-03-01

    The National Astronomical Observatories, Chinese Academy of Science (NAOC), has started building the largest antenna in the world. Known as FAST, the Five-hundred-meter Aperture Spherical radio Telescope is a Chinese mega-science project funded by the National Development and Reform Commission (NDRC). FAST also represents part of Chinese contribution to the international efforts to build the square kilometer array (SKA). Upon its finishing around September of 2016, FAST will be the most sensitive single-dish radio telescope in the low frequency radio bands between 70 MHz and 3 GHz. The design specifications of FAST, its expected capabilities, and its main scientific aspirations were described in an overview paper by Nan et al. (2011). In this paper, we briefly review the design and the key science goals of FAST, speculate the likely limitations at the initial stages of FAST operation, and discuss the opportunities for astronomical discoveries in the so-called early science phase.

  19. A Comparison of the Methodological Quality of Articles in Computer Science Education Journals and Conference Proceedings

    ERIC Educational Resources Information Center

    Randolph, Justus J.; Julnes, George; Bednarik, Roman; Sutinen, Erkki

    2007-01-01

    In this study we empirically investigate the claim that articles published in computer science education journals are more methodologically sound than articles published in computer science education conference proceedings. A random sample of 352 articles was selected from those articles published in major computer science education forums between…

  20. Proceedings of the Redesign in Science Education Conference (RISE) (Columbus, OH, October 20-21, 2000).

    ERIC Educational Resources Information Center

    Beeth, Michael E., Ed.; Kwon, Hyeoksoon, Ed.; Lee, Gyoungho, Ed.

    This document contains the papers presented at the Redesign in Science Education (RISE) Conference. Papers include: (1) "A Model Development Concept (MDC) for Education: A Framework for Change" (C. K. Barsky, K. G. Wilson, and B. Daviss); (2) "Teaching Science Everyday" (K. L. Scott); (3) "Science Teacher Licensure Requirements in Ohio" (P.…

  1. Proceedings of the International Conference e-Learning 2014. Multi Conference on Computer Science and Information Systems (Lisbon, Portugal, July 15-19, 2014)

    ERIC Educational Resources Information Center

    Baptista Nunes, Miguel, Ed.; McPherson, Maggie, Ed.

    2014-01-01

    These proceedings contain the papers of the International Conference e-Learning 2014, which was organised by the International Association for Development of the Information Society and is part of the Multi Conference on Computer Science and Information Systems (Lisbon, Portugal July 15-19, 2014). The e-Learning 2014 conference aims to address the…

  2. Proceedings of the New England Conference on Ocean Science Education, Woods Hole, Massachusetts, May 1966.

    ERIC Educational Resources Information Center

    Mangelsdorf, Frederick E.; And Others

    Reported are the papers presented at the New England Conference on Ocean Science Education. The purpose of the conference was to bring together prominent oceanographers and New England educators at the primary and secondary level to discuss current progress in oceanographic research and to relate this progress to the needs of schools for materials…

  3. Organization by Gordon Research Conferences of the 2012 Plasma Processing Science Conference 22-27 July 2012

    SciTech Connect

    Chang, Jane

    2012-07-27

    The 2012 Gordon Research Conference on Plasma Processing Science will feature a comprehensive program that will highlight the most cutting edge scientific advances in plasma science and technology as well as explore the applications of this nonequilibrium medium in possible approaches relative to many grand societal challenges. Fundamental science sessions will focus on plasma kinetics and chemistry, plasma surface interactions, and recent trends in plasma generation and multi-phase plasmas. Application sessions will explore the impact of plasma technology in renewable energy, the production of fuels from renewable feedstocks and carbon dioxide neutral solar fuels (from carbon dioxide and water), and plasma-enabled medicine and sterilization.

  4. Radio Frequency Interference Mitigation Strategies: Summary of the E. & F. White Conference held in Sydney, Australia, December 1999

    NASA Astrophysics Data System (ADS)

    Bell, Jon F.; Ekers, Ron D.; Bunton, John D.

    2000-12-01

    The E. & F. White Conference held in Sydney in December 1999 brought together expertise on a range of interference mitigation techniques from CSIRO, Australian and international industry and universities. Key goals were to enhance the understanding of techniques and their inter-relationship, to increase awareness of advanced technologies such as software radios and photonics, and to foster a cooperative approach to the development of interference mitigation techniques. The foremost application in mind was the square kilometre array (SKA) and the need to find ways to develop a hierarchical scheme for removing unwanted signals from astronomical data. This paper gives an overview of the topics discussed at the conference and summarises some of the key ideas and results that were presented.

  5. Proceedings of the twentieth Hawaii international conference on system sciences

    SciTech Connect

    Shriver, B.D.

    1987-01-01

    This book presents the papers given at a conference which considered parallel processing. Topics covered at the conference included the implementation of LISP on Cray computers, executive codes, a programming language for the DADO parallel machine, parallel algorithms, multiprocessor algorithms, functional parallel languages, distributed processing systems, compiler technology, and issues in distributed data base systems.

  6. International Conference on Bio-Medical Instrumentation and related Engineering and Physical Sciences (BIOMEP 2015)

    NASA Astrophysics Data System (ADS)

    2015-09-01

    The International Conference on Bio-Medical Instrumentation and related Engineering and Physical Sciences (BIOMEP 2015) took place in the Technological Educational Institute (TEI) of Athens, Greece on June 18-20, 2015 and was organized by the Department of Biomedical Engineering. The scope of the conference was to provide a forum on the latest developments in Biomedical Instrumentation and related principles of Physical and Engineering sciences. Scientists and engineers from academic, industrial and health disciplines were invited to participate in the Conference and to contribute both in the promotion and dissemination of the scientific knowledge.

  7. Essays on Creativity and Science. Proceedings of the Creativity and Science Conference (Honolulu, Hawaii, March 23-24, 1985).

    ERIC Educational Resources Information Center

    DeLuca, Diana Macintyre, Ed.

    Essays focusing on creativity in the humanities and sciences are contained in this proceedings of the Creativity and Science Conference. The presentors, who represented many academic disciplines, agreed that creativity is as essential to the scientist as to the humanist and that one can prepare for it but not instruct or be instructed in achieving…

  8. PREFACE: International Conference on High Pressure Science and Technology, Joint AIRAPT-22 & HPCJ-50

    NASA Astrophysics Data System (ADS)

    Viña, Luis; Tejedor, Carlos; Calleja, José M.

    2010-01-01

    The International Joint AIRAPT-22 & HPCJ-50 Conference was held in Odaiba, Tokyo, on 26-31 July 2009. About 480 scientists from 24 countries attended the conference and 464 papers, including 3 plenary lectures, 39 invited talks, and 156 oral presentations, were presented. It is my great pleasure to present this proceedings volume, which is based on the high quality scientific works presented at the conference. The International AIRAPT conference has been held every two years in various countries around the world since 1965, while High Pressure Conference of Japan (HPCJ) has been held annually since 1959 in various Japanese cities. Pressure is a fundamental parameter to control the property of matter. As a result, both AIRAPT and HPCJ have become highly multidisciplinary, and cover Physics, Chemistry, Materials Science, Earth and Planetary Sciences, Biosciences, Food Science, and Technology. Although each discipline has a unique target, they all have high-pressure research in common. This proceedings volume includes about 200 papers of state-of-the-art studies from numerous fields. I hope this proceedings volume provides excellent pieces of information in various fields to further advance high-pressure research. Conference logo Takehiko Yagi Conference Chairman Institute for Solid State Physics The University of Tokyo 7 December 2009 Conference photograph Participants at the conference venue, Tokyo International Exchange Center, Odaiba, Tokyo, Japan. Editor in Chief TAKEMURA Kenichi National Institute for Materials Science, Japan Editorial board Tadashi KONDO Osaka University, Japan Hitoshi MATSUKI The University of Tokushima, Japan Nobuyuki MATUBAYASI Kyoto University, Japan Yoshihisa MORI Okayama University of Science, Japan Osamu OHTAKA Osaka University, Japan Chihiro SEKINE Muroran Institute of Technology, Japan

  9. Parkes radio science system design and testing for Voyager Neptune encounter

    NASA Technical Reports Server (NTRS)

    Rebold, T. A.; Weese, J. F.

    1989-01-01

    The Radio Science System installed at Parkes, Australia for the Voyager Neptune encounter was specified to meet the same stringent requirements that were imposed upon the Deep Space Network Radio Science System. The system design and test methodology employed to meet these requirements at Parkes are described, and data showing the measured performance of the system are presented. The results indicate that the system operates with a comfortable margin on the requirements. There was a minor problem with frequency-dependent spurious signals which could not be fixed before the encounter. Test results characterizing these spurious signals are included.

  10. Proceedings of the 38th Lunar and Planetary Science Conference

    NASA Technical Reports Server (NTRS)

    2007-01-01

    The sessions in the conference include: Titan, Mars Volcanism, Mars Polar Layered Deposits, Early Solar System Isotopes, SPECIAL SESSION: Mars Reconnaissance Orbiter: New Ways of Studying the Red Planet, Achondrites: Exploring Oxygen Isotopes and Parent-Body Processes, Solar System Formation and Evolution, SPECIAL SESSION: SMART-1, . Impact Cratering: Observations and Experiments, SPECIAL SESSION: Volcanism and Tectonism on Saturnian Satellites, Solar Nebula Composition, Mars Fluvial Geomorphology, Asteroid Observations: Spectra, Mostly, Mars Sediments and Geochemistry: View from the Surface, Mars Tectonics and Crustal Dichotomy, Stardust: Wild-2 Revealed, Impact Cratering from Observations and Interpretations, Mars Sediments and Geochemistry: The Map View, Chondrules and Their Formation, Enceladus, Asteroids and Deep Impact: Structure, Dynamics, and Experiments, Mars Surface Process and Evolution, Martian Meteorites: Nakhlites, Experiments, and the Great Shergottite Age Debate, Stardust: Mainly Mineralogy, Astrobiology, Wind-Surface Interactions on Mars and Earth, Icy Satellite Surfaces, Venus, Lunar Remote Sensing, Space Weathering, and Impact Effects, Interplanetary Dust/Genesis, Mars Cratering: Counts and Catastrophes?, Chondrites: Secondary Processes, Mars Sediments and Geochemistry: Atmosphere, Soils, Brines, and Minerals, Lunar Interior and Differentiation, Mars Magnetics and Atmosphere: Core to Ionosphere, Metal-rich Chondrites, Organics in Chondrites, Lunar Impacts and Meteorites, Presolar/Solar Grains, Topics for Print Only papers are: Outer Planets/Satellites, Early Solar System, Interplanetary Dust, Comets and Kuiper Belt Objects, Asteroids and Meteoroids, Chondrites, Achondrites, Meteorite Related, Mars Reconnaissance Orbiter, Mars, Astrobiology, Planetary Differentiation, Impacts, Mercury, Lunar Samples and Modeling, Venus, Missions and Instruments, Global Warming, Education and Public Outreach, Poster sessions are: Asteroids/Kuiper Belt Objects

  11. Proceedings of the 40th Lunar and Planetary Science Conference

    NASA Technical Reports Server (NTRS)

    2009-01-01

    The 40th Lunar and Planetary Science Conference included sessions on: Phoenix: Exploration of the Martian Arctic; Origin and Early Evolution of the Moon; Comet Wild 2: Mineralogy and More; Astrobiology: Meteorites, Microbes, Hydrous Habitats, and Irradiated Ices; Phoenix: Soil, Chemistry, and Habitability; Planetary Differentiation; Presolar Grains: Structures and Origins; SPECIAL SESSION: Venus Atmosphere: Venus Express and Future Missions; Mars Polar Caps: Past and Present; SPECIAL SESSION: Lunar Missions: Results from Kaguya, Chang'e-1, and Chandrayaan-1, Part I; 5 Early Nebula Processes and Models; SPECIAL SESSION: Icy Satellites of Jupiter and Saturn: Cosmic Gymnasts; Mars: Ground Ice and Climate Change; SPECIAL SESSION: Lunar Missions: Results from Kaguya, Chang'e-1, and Chandrayaan-1, Part II; Chondrite Parent-Body Processes; SPECIAL SESSION: Icy Satellites of Jupiter and Saturn: Salubrious Surfaces; SNC Meteorites; Ancient Martian Crust: Primary Mineralogy and Aqueous Alteration; SPECIAL SESSION: Messenger at Mercury: A Global Perspective on the Innermost Planet; CAIs and Chondrules: Records of Early Solar System Processes; Small Bodies: Shapes of Things to Come; Sulfur on Mars: Rocks, Soils, and Cycling Processes; Mercury: Evolution and Tectonics; Venus Geology, Volcanism, Tectonics, and Resurfacing; Asteroid-Meteorite Connections; Impacts I: Models and Experiments; Solar Wind and Genesis: Measurements and Interpretation; Mars: Aqueous Processes; Magmatic Volatiles and Eruptive Conditions of Lunar Basalts; Comparative Planetology; Interstellar Matter: Origins and Relationships; Impacts II: Craters and Ejecta Mars: Tectonics and Dynamics; Mars Analogs I: Geological; Exploring the Diversity of Lunar Lithologies with Sample Analyses and Remote Sensing; Chondrite Accretion and Early History; Science Instruments for the Mars Science Lander; . Martian Gullies: Morphology and Origins; Mars: Dunes, Dust, and Wind; Mars: Volcanism; Early Solar System Chronology

  12. Conference on Geospatial Approaches to Cancer Control and Population Sciences

    Cancer.gov

    The purpose of this conference is to bring together a community of researchers across the cancer control continuum using geospatial tools, models and approaches to address cancer prevention and control.

  13. Unified Science - Premises and Prospects. Proceedings of the Annual Conference of the Federation for Unified Science Education (FUSE) (8th, Columbus, Ohio, May 2-5, 1974).

    ERIC Educational Resources Information Center

    Showalter, Victor, Ed.; And Others

    Included in this record of the proceedings of the eighth annual conference of the Federation for Unified Science Education (FUSE) are texts of major presentations, panel discussions, and contributed papers. Other activities of the conference are also reported. (CP)

  14. IFLA General Conference, 1984. Special Libraries Division. Section on Social Science Libraries. Papers.

    ERIC Educational Resources Information Center

    International Federation of Library Associations, The Hague (Netherlands).

    The two papers in this document on social science libraries were presented at the 1984 IFLA general conference. In "Library and Continuing Education with Implications for Developing Countries: A Research Essay," David R. Bender (United States) examines factors impacting upon the skills necessary for effective librarianship in the social sciences,…

  15. Third International Conference on Inverse Design Concepts and Optimization in Engineering Sciences (ICIDES-3)

    NASA Technical Reports Server (NTRS)

    Dulikravich, George S. (Editor)

    1991-01-01

    Papers from the Third International Conference on Inverse Design Concepts and Optimization in Engineering Sciences (ICIDES) are presented. The papers discuss current research in the general field of inverse, semi-inverse, and direct design and optimization in engineering sciences. The rapid growth of this relatively new field is due to the availability of faster and larger computing machines.

  16. Annual Science Education Conference (9th, Murdoch University, Perth, Western Australia, September 23, 1983).

    ERIC Educational Resources Information Center

    Western Australia Science Education Association.

    This proceedings contains the texts of 14 science education research studies which were presented at the 1983 Western Australia Science Education Conference. They include: "Students' Understanding of Chemical Equilibrium: A Report of Research in Progress" (Patrick J. Garnett, Mark W. Hackling); "Measuring the Learning Environment in Elementary and…

  17. PREFACE The International Conference on Science of Friction 2010 (ICSF2010)

    NASA Astrophysics Data System (ADS)

    Miura, Kouji; Matsukawa, Hiroshi

    2010-11-01

    The second international conference on science of friction in Japan was held at Ise-Shima, Mie on 13-18 September 2010. The conference focused on the elementary process of friction phenomena from atomic and molecular scale view. Topics covered at the conference were: Superlubricity and friction Electronic and phononic contributions to friction Friction on the atomic and molecular scales van der Waals friction and Casimir force Molecular motor and friction Friction and adhesion in soft matter system Wear and crack on the nanocsale Theoretical studies on the atomic scale friction and energy dissipatin Friction and Chaos Mechanical properties of nanoscale contacts Friction of powder The number of participants in the conference was approximately 85, registered from 8 countries. 40 oral and 16 poster talks were presented at the conference. This volume of Journal of Physics: Conference Series includes 19 papers devoted to the topics of friction. The successful organization of the conference was made possible by the contribution of the members of the organizing Committee. The conference was made possible thanks to the financial support from Aichi University of Education, and moreover thanks to the approval societies of The Physical Society of Japan, The surface Science Society of Japan and The Japanese Society of Tribologists. The details of the conference are available on http://www.science-of-friction.com/2010/. Finally we would like to thank the speakers for the high quality of their talks and all participants for coming to Ise-Shima, Japan and actively contributing to the conference. Kouji Miura and Hiroshi Matsukawa Editors

  18. A review of decametric radio astronomy - Instruments and science

    NASA Technical Reports Server (NTRS)

    Erickson, W. C.; Cane, H. V.

    1987-01-01

    The techniques and instruments used in Galactic and extragalactic radio astronomy at dkm wavelengths are surveyed, and typical results are summarized. Consideration is given to the large specialized phased arrays used for early surveys, the use of wideband elements to increase frequency agility, experimental VLBI observations, and limitations on ground-based observations below about 10 MHz (where the proposed LF Space Array, with resolution 0.5-5 arcmin, could make a major contribution). Observations discussed cover the Galactic center, the Galactic background radiation, SNRs, compact Galactic sources, the ISM, and large extragalactic sources.

  19. Radio frequency science considerations. [technology utilization of telecommunications system

    NASA Technical Reports Server (NTRS)

    Croft, T. A.

    1974-01-01

    Use of the 400 MHz telecommunications system to obtain scientific information, to provide backup information for the experiments flown, and to obtain measurements which aid in designing future probes is considered. Recommended objectives of such a program are summarized and include: measure 400 MHz amplitude to determine adsorption and perhaps scintillation (if data rate permits); measure noise strength near 400 MHz to reexamine 400 MHz choice and to observe thermal, cosmic, and local synchrotron noise trends; probe VSWR sensing to monitor integrity of system, icing, and possible plasma effects; after the probe is finished, have the bus radio occultation in the same region where the probe fell to evaluate the occultation.

  20. Developing Open Loop Radio Science Facility for YH-1 Martian Mission

    NASA Astrophysics Data System (ADS)

    Ping, Jinsong; Jian, Nianchuan; Shi, Xian; Yan, Jianguo; Wang, Mingyuan; Zhang, Sujun; Shang, Kun; Huang, Qian; Wang, Guangli; Qiu, Shi

    The first Chinese martian orbiter, Yinghuo-1, is planned to be launched together with the Rassian Phobos-Grunt sampling return mission next year. Open loop radio tracking technique will be applied for s/c tracking and radio science study. A team from Shanghai Astronomical Observatory of CAS has been involved to develop the open loop radio science techniques. They simulated the OD by considering the VLBI and One-way tracking technique; they are developing the DOR/DOD and one-way tracking system; also, they are developing the s/c to ground occultation facilities to study the Martian atmosphere. Using the data released by PDS (http://pds.jpl.nasa.gov) and other resources, they are learning the experiences of deep space tracking and exploration, step by step.

  1. Mars observer radio science (MORS) observations in polar regions

    NASA Technical Reports Server (NTRS)

    Simpson, Richard A.

    1992-01-01

    MORS observations will focus on two major areas of study: (1) the gravity field of Mars and its interpretation in terms of internal structure and history and (2) the structure of the atmosphere, with emphasis on both temperature-pressure profiles of the background atmosphere and small scale inhomogeneities resulting from turbulence. Scattering of cm wavelength radio signals from Mars' surface at highly oblique angles will also be studied during the primary mission; nongrazing scattering experiments may be possible during an extended mission. During the MORS primary mission, measurements of the spacecraft distance and velocity with respect to Earth based tracking stations will be used to develop models of the global gravity field. The improvement in knowledge of the gravity field will be especially evident in polar regions. The spatial and temporal coverage of atmospheric radio occultation measurements are determined by the geometry of the spacecraft orbit and the direction to the Earth. Profiles of atmospheric temperature and pressure will extend from the surface to altitudes of 50 to 70 km.

  2. FOREWORD: 9th Curtin University of Technology Science and Engineering International Conference 2014 (CUTSE2014)

    NASA Astrophysics Data System (ADS)

    Chieng Chen, Vincent Lee

    2015-04-01

    A very warm welcome to all participants of the 9th Curtin University Technology, Science and Engineering (CUTSE) Conference 2014. This annual conference dates back to 2006 when the first Curtin University of Technology Science and Engineering (CUTSE) Conference was held in Curtin University, Miri Sarawak. CUTSE Conference was initially intended for Curtin's undergraduates such that they are able to experience the presentation of their work in a conference environment. As time passes and following the urge of knowledge dissemination, CUTSE Conference is hence open to public. This year the Department of Mechanical Engineering has been given the honour to organize the 9th CUTSE Conference. It has been a pleasure to watch CUTSE grow from strength to strength over the years. This year, our theme is "Discovering, Innovating and Engineering". We hope that it is in this spirit that CUTSE participants may align their respective work, such that we all aim for a greater and better implementation of "Discovering, Innovating and Engineering". The 9th CUTSE Conference 2014 is an excellent avenue for researchers, engineers, scientists, academicians, professionals from industry and students to share their research findings and initiate further collaborations in their respective fields. Parallel sessions in Mechanical, Electrical, Computer, Civil and Chemical engineering as well as the sciences will be hosted over a period of two days. Each year, the conference attracts participation from a number of countries in addition to Malaysia and Australia. In addition, student participants will get the opportunity to present their research projects and gain valuable feedback from industry professionals. This year the Conference will be organised by the Department of Mechanical Engineering of Curtin Sarawak's School of Engineering and Science in collaboration with The Institute of Engineers Malaysia, Miri Branch. On behalf of the organizing committee, I would like to thank this year

  3. Open-loop radio science with a suppressed-carrier signal

    NASA Technical Reports Server (NTRS)

    Greenhall, C. A.

    1980-01-01

    When a suppressed-carrier signal is squared, the carrier reappears in doubled form. An open-loop receiver can be used to deliver a recording of a band-limited waveform containing this carrier, whose amplitude and phase can be tracked by the radio science experimenter.

  4. Ultra-Stable Oscillators for Probe Radio Science Investigations

    NASA Technical Reports Server (NTRS)

    Asmar, Sami

    2012-01-01

    An Ultra-Stable Oscillator (USO) is: A frequency reference, and A clock It is stable, small, and sensitive. It is a science and an art form. It is flown on spacecraft/probes. It]is utilized at ground stations alone or as a cleanup loop. It eliminates lock-up time on uplink for occultation egress & effect of media on uplink signal. It has enabled significant planetary science investigations.

  5. Proceedings of the 40th Lunar and Planetary Science Conference

    NASA Technical Reports Server (NTRS)

    2009-01-01

    The 40th Lunar and Planetary Science Conference included sessions on: Phoenix: Exploration of the Martian Arctic; Origin and Early Evolution of the Moon; Comet Wild 2: Mineralogy and More; Astrobiology: Meteorites, Microbes, Hydrous Habitats, and Irradiated Ices; Phoenix: Soil, Chemistry, and Habitability; Planetary Differentiation; Presolar Grains: Structures and Origins; SPECIAL SESSION: Venus Atmosphere: Venus Express and Future Missions; Mars Polar Caps: Past and Present; SPECIAL SESSION: Lunar Missions: Results from Kaguya, Chang'e-1, and Chandrayaan-1, Part I; 5 Early Nebula Processes and Models; SPECIAL SESSION: Icy Satellites of Jupiter and Saturn: Cosmic Gymnasts; Mars: Ground Ice and Climate Change; SPECIAL SESSION: Lunar Missions: Results from Kaguya, Chang'e-1, and Chandrayaan-1, Part II; Chondrite Parent-Body Processes; SPECIAL SESSION: Icy Satellites of Jupiter and Saturn: Salubrious Surfaces; SNC Meteorites; Ancient Martian Crust: Primary Mineralogy and Aqueous Alteration; SPECIAL SESSION: Messenger at Mercury: A Global Perspective on the Innermost Planet; CAIs and Chondrules: Records of Early Solar System Processes; Small Bodies: Shapes of Things to Come; Sulfur on Mars: Rocks, Soils, and Cycling Processes; Mercury: Evolution and Tectonics; Venus Geology, Volcanism, Tectonics, and Resurfacing; Asteroid-Meteorite Connections; Impacts I: Models and Experiments; Solar Wind and Genesis: Measurements and Interpretation; Mars: Aqueous Processes; Magmatic Volatiles and Eruptive Conditions of Lunar Basalts; Comparative Planetology; Interstellar Matter: Origins and Relationships; Impacts II: Craters and Ejecta Mars: Tectonics and Dynamics; Mars Analogs I: Geological; Exploring the Diversity of Lunar Lithologies with Sample Analyses and Remote Sensing; Chondrite Accretion and Early History; Science Instruments for the Mars Science Lander; . Martian Gullies: Morphology and Origins; Mars: Dunes, Dust, and Wind; Mars: Volcanism; Early Solar System Chronology

  6. PREFACE: 1st Conference on Light and Particle Beams in Materials Science 2013 (LPBMS2013)

    NASA Astrophysics Data System (ADS)

    Kumai, Reiji; Murakami, Youichi

    2014-04-01

    From 29-31 August 2013, the 1st International Conference on Light and Particle Beams in Materials Science, LPBMS 2013, took place in the Tsukuba International Congress Center in the city of Tsukuba, Japan. The conference was a continuation of the international series Synchrotron Radiation in Materials Science (SRMS), which started in 1994. The last one, SRMS-7, was held in Oxford UK 11-14 July 2010, where the International Advisory Committee (IAC) recommended the conference be enlarged to incorporate Materials Research from Neutron, Muon, and Slow Positron Sources, as well as the science emerging from Synchrotron Light Sources. The conference brought together contributions from academics and industrial researchers with a diverse background and experience from the physics, chemistry and engineering communities. The topics covered in the LPBMS2013 include strongly correlated electron systems, magnetism and magnetic materials, soft matter, interface and surface defects, catalysts, biomaterials, and ceramics. In the 3-day scientific program, the conference consisted of 9 plenary talks, 33 invited talks, 20 oral presentations, and 126 poster presentations. We are pleased to publish the proceedings of the LPBMS2013 in this volume of Journal of Physics: Conference Series. This volume contains 58 papers representing the work that was presented and discussed at the conference. We hope that this volume will promote further development of this interdisciplinary materials research emerging from synchrotron light, neutron, muon, and slow positron sciences. Finally, we would like to thank the International Advisory Committee (Chair: Professor G N Greaves), sponsors, all the participants and contributors for making possible this international meeting of researchers. Reiji Kumai & Youichi Murakami Conference photograph Details of the program and organizing committees are available in the pdf

  7. Marine Science and the 1974 Law of the Sea Conference

    ERIC Educational Resources Information Center

    Knauss, John A.

    1974-01-01

    More intensive and varied use of the oceans and their resources requires a more comprehensive legal regime than previously. Three years of preparatory work have been completed for the Law of the Sea Conference. It appears that the coastal nations will gain some form of jurisdiction over fisheries and mineral resources off their shores. (RH)

  8. 1st International Nuclear Science and Technology Conference 2014 (INST2014)

    NASA Astrophysics Data System (ADS)

    2015-04-01

    Nuclear technology has played an important role in many aspects of our lives, including agriculture, energy, materials, medicine, environment, forensics, healthcare, and frontier research. The International Nuclear Science and Technology Conference (INST) aims to bring together scientists, engineers, academics, and students to share knowledge and experiences about all aspects of nuclear sciences. INST has evolved from a series of national conferences in Thailand called Nuclear Science and Technology (NST) Conference, which has been held for 11 times, the first being in 1986. INST2014 was held in August 2014 and hosted by Thailand Institute of Nuclear Technology (TINT). The theme was "Driving the future with nuclear technology". The conference working language was English. The proceedings were peer reviewed and considered for publication. The topics covered in the conference were: • Agricultural and food applications [AGR] • Environmental applications [ENV] • Radiation processing and industrial applications [IND] • Medical and nutritional applications [MED] • Nuclear physics and engineering [PHY] • Nuclear and radiation safety [SAF] • Other related topics [OTH] • Device and instrument presentation [DEV] Awards for outstanding oral and poster presentations will be given to qualified students who present their work during the conference.

  9. Literature and the Sea. Proceedings of a Conference Held at the Marine Science Center, Newport, Oregon, May 8, 1976.

    ERIC Educational Resources Information Center

    Astro, Richard, Ed.

    This document is a collection of eight papers presented at a conference held at the Marine Science Center, Newport, Oregon, May 8, 1976. The conference concluded a course offered jointly by the School of Oceanography and the Department of English at Oregon State University. The conference had two purposes: (1) focus on the relationship between…

  10. Engineering and science highlights of the KAT-7 radio telescope

    NASA Astrophysics Data System (ADS)

    Foley, A. R.; Alberts, T.; Armstrong, R. P.; Barta, A.; Bauermeister, E. F.; Bester, H.; Blose, S.; Booth, R. S.; Botha, D. H.; Buchner, S. J.; Carignan, C.; Cheetham, T.; Cloete, K.; Coreejes, G.; Crida, R. C.; Cross, S. D.; Curtolo, F.; Dikgale, A.; de Villiers, M. S.; du Toit, L. J.; Esterhuyse, S. W. P.; Fanaroff, B.; Fender, R. P.; Fijalkowski, M.; Fourie, D.; Frank, B.; George, D.; Gibbs, P.; Goedhart, S.; Grobbelaar, J.; Gumede, S. C.; Herselman, P.; Hess, K. M.; Hoek, N.; Horrell, J.; Jonas, J. L.; Jordaan, J. D. B.; Julie, R.; Kapp, F.; Kotzé, P.; Kusel, T.; Langman, A.; Lehmensiek, R.; Liebenberg, D.; Liebenberg, I. J. V.; Loots, A.; Lord, R. T.; Lucero, D. M.; Ludick, J.; Macfarlane, P.; Madlavana, M.; Magnus, L.; Magozore, C.; Malan, J. A.; Manley, J. R.; Marais, L.; Marais, N.; Marais, S. J.; Maree, M.; Martens, A.; Mokone, O.; Moss, V.; Mthembu, S.; New, W.; Nicholson, G. D.; van Niekerk, P. C.; Oozeer, N.; Passmoor, S. S.; Peens-Hough, A.; Pińska, A. B.; Prozesky, P.; Rajan, S.; Ratcliffe, S.; Renil, R.; Richter, L. L.; Rosekrans, D.; Rust, A.; Schröder, A. C.; Schwardt, L. C.; Seranyane, S.; Serylak, M.; Shepherd, D. S.; Siebrits, R.; Sofeya, L.; Spann, R.; Springbok, R.; Swart, P. S.; Thondikulam, Venkatasubramani L.; Theron, I. P.; Tiplady, A.; Toruvanda, O.; Tshongweni, S.; van den Heever, L.; van der Merwe, C.; van Rooyen, R.; Wakhaba, S.; Walker, A. L.; Welz, M.; Williams, L.; Wolleben, M.; Woudt, P. A.; Young, N. J.; Zwart, J. T. L.

    2016-08-01

    The construction of the seven-dish Karoo Array Telescope (KAT-7) array in the Karoo region of the Northern Cape in South Africa was intended primarily as an engineering prototype for technologies and techniques applicable to the MeerKAT telescope. This paper looks at the main engineering and scientific highlights from this effort, and discusses their applicability to both MeerKAT and other next-generation radio telescopes. In particular, we found that the composite dish surface works well, but it becomes complicated to fabricate for a dish lacking circular symmetry; the Stirling cycle cryogenic system with ion pump to achieve vacuum works but demands much higher maintenance than an equivalent Gifford-McMahon cycle system; the ROACH (Reconfigurable Open Architecture Computing Hardware)-based correlator with SPEAD (Streaming Protocol for Exchanging Astronomical Data) protocol data transfer works very well and KATCP (Karoo Array Telescope Control Protocol) control protocol has proven very flexible and convenient. KAT-7 has also been used for scientific observations where it has a niche in mapping low surface-brightness continuum sources, some extended H I haloes and OH masers in star-forming regions. It can also be used to monitor continuum source variability, observe pulsars, and make Very Long Baseline Interferometry observations.

  11. Mercury's gravity, tides, and spin from MESSENGER radio science data

    NASA Astrophysics Data System (ADS)

    Verma, Ashok Kumar; Margot, Jean-Luc

    2016-09-01

    We analyze radio tracking data obtained during 1311 orbits of the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft in the period March 2011 to April 2014. A least squares minimization of the residuals between observed and computed values of two-way range and Doppler allows us to solve for a model describing Mercury's gravity, tidal response, and spin state. We use a spherical harmonic representation of the gravity field to degree and order 40 and report error bars corresponding to 10 times the formal uncertainties of the fit. Our estimate of the product of Mercury's mass and the gravitational constant, GM = (22031.87404 ± 9×10-4) km3 s-2, is in excellent agreement with published results. Our solution for the geophysically important second-degree coefficients (C¯2,0=-2.25100×10-5±1.3×10-9, C¯2,2=1.24973×10-5±1.2×10-9) confirms previous estimates to better than 0.4% and, therefore, inferences about Mercury's moment of inertia and interior structure. Our estimate of the tidal Love number k2 = 0.464 ± 0.023 indicates that Mercury's mantle may be hotter and weaker than previously thought. Our spin state solution suggests that gravity-based estimates of Mercury's spin axis orientation are marginally consistent with previous measurements of the orientation of the crust.

  12. The Fifteenth International Conference on the Science and Application of Nanotubes (NT14)

    SciTech Connect

    cronin, stephen

    2015-01-06

    The Fifteenth International Conference on the Science and Application of Nanotubes (NT14) was held at the University of Southern California in Los Angeles, California on June 2-6, 2014. NT14 upheld the NT tradition of presenting the latest results in the science and applications of nanotubes and related materials in plenary sessions. Emphasis was given to convivial poster sessions and student participation. Over 225 participants attended the conference, including students, post-docs, faculty, and members from industry. A total of 45 talks were presented, as well as 157 posters.

  13. Perspectives of women of color in science-based education and careers. Summary of the conference on diversity in science

    SciTech Connect

    1998-12-01

    Research on inequality or stratification in science and engineering tends to concentrate on black/white or male/female difference; very few studies have discussions of both race and gender. Consequently, very little is known about the exact course that women of color take in science-based education and employment or about the course that steers them out of science-based careers. Questions abound: What are the environmental factors that affect the choices in education and science-based careers of women of color? What has influenced women of color who currently are in science-based careers? Is critical mass important and, if so, what are the keys to increasing it? What recommendations can be made to colleges and universities, faculty members, employers, the federal government, women of color themselves, and to improve the conditions and numbers of women of color in science-based careers? These questions prompted the National Research Council`s Committee on Women in Science and Engineering (CWSE) to convene a conference on Diversity in Science: Perspectives on the Retention of Minority Women in Science, Engineering, and Health-Care Professions, held on October 21--23, 1995. Confronting the problem of the lack of knowledge about the journey of women of color in science-based education and career, the conference offered opportunities for these women to describe the paths that they have taken and to identify strategies for success. Their perspectives ground this report. For purposes of this document, women of color include women in the following racial or ethnic groups: Hispanics, African-Americans, Asian and Pacific Islanders, and American Indians and Alaskan Natives. Science-based careers include those in the physical sciences and mathematics, life sciences, social sciences, and engineering.

  14. TheRadio Science Experiment VeRa onboard ESA's Venus Express (VEX) Spacecraft

    NASA Astrophysics Data System (ADS)

    Haeusler, Bernd; Paetzold, M.; Bird, M. K.; Simpson, R. A.; Tyler, L. G.; Dehant, V.; Imamura, T.; Tellmann, S.; Mattei, R.

    2006-09-01

    The VEX spacecraft was successfully injected into the Venus orbit on April 11, 2006. VeRa is an active radio sounding instrument which will measure atmospheric/ionospheric temperature and density profiles, sound with bistatic radar experiments the surface of the planet, will measure its gravity anomalies and investigate also the structure of the corona by analyzing radio carrier signals received on ground in the S- and X-frequency bands. The radio science instrument VeRa is equipped with an ultrastable oscillator (USO) which will be used especially for atmospheric sounding and bistatic radar experiments as frequency reference in the OneWay transmission mode. We will present the current status of the experiment, the results of the commissioning tests and first scientific results.

  15. The Gravity Field of Mars From MGS, Mars Odyssey, and MRO Radio Science

    NASA Technical Reports Server (NTRS)

    Genova, Antonio; Goossens, Sander; Lemoine, Frank G.; Mazarico, Erwan; Smith, David E.; Zuber, Maria T.

    2015-01-01

    The Mars Global Surveyor (MGS), Mars Odyssey (ODY), and Mars Reconnaissance Orbiter (MRO) missions have enabled NASA to conduct reconnaissance and exploration of Mars from orbit for sixteen consecutive years. These radio systems on these spacecraft enabled radio science in orbit around Mars to improve the knowledge of the static structure of the Martian gravitational field. The continuity of the radio tracking data, which cover more than a solar cycle, also provides useful information to characterize the temporal variability of the gravity field, relevant to the planet's internal dynamics and the structure and dynamics of the atmosphere [1]. MGS operated for more than 7 years, between 1999 and 2006, in a frozen sun-synchronous, near-circular, polar orbit with the periapsis at approximately 370 km altitude. ODY and MRO have been orbiting Mars in two separate sun-synchronous orbits at different local times and altitudes. ODY began its mapping phase in 2002 with the periapis at approximately 390 km altitude and 4-5pm Local Solar Time (LST), whereas the MRO science mission started in November 2006 with the periapis at approximately 255 km altitude and 3pm LST. The 16 years of radio tracking data provide useful information on the atmospheric density in the Martian upper atmosphere. We used ODY and MRO radio data to recover the long-term periodicity of the major atmospheric constituents -- CO2, O, and He -- at the orbit altitudes of these two spacecraft [2]. The improved atmospheric model provides a better prediction of the annual and semi-annual variability of the dominant species. Therefore, the inclusion of the recovered model leads to improved orbit determination and an improved gravity field model of Mars with MGS, ODY, and MRO radio tracking data.

  16. Adapting Science to Social Needs: Knowledge, Institutions, People Into Action. Proceedings of a Workshop Conference on Problem-Oriented Research.

    ERIC Educational Resources Information Center

    Scribner, Richard A., Ed.; Chalk, Rosemary A., Ed.

    This document contains the proceedings of a workshop conference sponsored by the American Association for the Advancement of Science (AAAS) held at the Institute of Man and Science in Rensselaerville, New York, in May 1976. The proceedings include presented papers, discussions, and comments of the participants. The conference had two sets of…

  17. 75 FR 3243 - NIH State-of-the-Science Conference: Preventing Alzheimer's Disease and Cognitive Decline; Notice

    Federal Register 2010, 2011, 2012, 2013, 2014

    2010-01-20

    ... HUMAN SERVICES National Institutes of Health NIH State-of-the-Science Conference: Preventing Alzheimer's... the ``NIH State-of-the-Science Conference: Preventing Alzheimer's Disease and Cognitive Decline'' to... state of cognitive impairment or into various forms of dementia, including Alzheimer's disease....

  18. Sixteenth Lunar and Planetary Science Conference. Press abstracts

    NASA Technical Reports Server (NTRS)

    1985-01-01

    A broad range of topics concerned with lunar and planetary science are discussed. Topics among those included are, the sun, the planets, comets, meteorities, asteroids, satellites, space exploration, and the significance of these to Earth.

  19. 75th anniversary of the N V Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences (IZMIRAN) (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 25 February 2015)

    NASA Astrophysics Data System (ADS)

    2015-06-01

    A scientific session of the Physical Sciences Division of the Russian Academy of Sciences (RAS) celebrating the 75th anniversary of the N V Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation of the RAS (IZMIRAN) was held in the IZMIRAN conference hall on 25 February 2015. The agenda of the session announced on the website http://www.gpad.ac.ru of the RAS Physical Sciences Division contained the following reports: (1) Kuznetsov V D (IZMIRAN, Moscow) "N V Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences (IZMIRAN) yesterday, today, and tomorrow"; (2) Gvishiani A D (Geophysical Center, Moscow) "Studies of the terrestrial magnetic field and the network of Russian magnetic laboratories"; (3) Sokoloff D D (Faculty of Physics, Lomonosov Moscow State University, Moscow) "Magnetic dynamo questions"; (4) Petrukovich A A (Space Research Institute, RAS, Moscow) "Some aspects of magnetosphere-ionosphere relations"; (5) Lukin D S (Moscow Institute of Physics and Technology (State University), Dolgoprudnyi, Moscow region) "Current problems of ionospheric radio wave propagation"; (6) Safargaleev V V (Polar Geophysical Institute, Kola Scientific Center, RAS, Murmansk), Sergienko T I (Swedish Institute of Space Physics (IRF), Sweden), Kozlovskii A E (Sodankyl \\ddot a Geophysical Observatory, Finland), Safargaleev A V (St. Petersburg State University, St. Petersburg), Kotikov A L (St. Petersburg Branch of IZMIRAN, St. Petersburg) "Magnetic and optical measurements and signatures of reconnection in the cusp and vicinity"; (7) Kuznetsov V D (IZMIRAN, Moscow) "Space solar research: achievements and prospects". Papers written on the basis of oral reports 1, 3, 4, 6, and 7 are given below. • N V Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences (IZMIRAN) yesterday, today, tomorrow, V D Kuznetsov Physics-Uspekhi, 2015

  20. Report on a Boston University Conference December 7-8, 2012 on "How Can the History and Philosophy of Science Contribute to Contemporary US Science Teaching?"

    ERIC Educational Resources Information Center

    Garik, Peter; Benétreau-Dupin, Yann

    2014-01-01

    This is an editorial report on the outcomes of an international conference sponsored by a grant from the National Science Foundation (NSF) (REESE-1205273) to the School of Education at Boston University and the Center for Philosophy and History of Science at Boston University for a conference titled: "How Can the History and Philosophy of…

  1. Undergraduate Education in the Plant and Soil Sciences, Proceedings of a Conference.

    ERIC Educational Resources Information Center

    Commission on Education in Agriculture and Natural Resources, Washington, DC.

    The proceedings of the 1967 Conference on Undergraduate Teaching in the Plant and Soil Sciences are presented in this publication. Seven individual presentations and reports from ten working groups review the adequacy and effectiveness of courses and curricula for undergraduate students; discuss instructional materials, methods, and equipment that…

  2. IFLA General Conference, 1986. Special Libraries Division. Section: Social Science Libraries. Papers.

    ERIC Educational Resources Information Center

    International Federation of Library Associations and Institutions, The Hague (Netherlands).

    Papers on social science libraries presented at the 1986 International Federation of Library Associations (IFLA) conference include: (1) "Efforts at Computerization in Nigerian Libraries--A State of Development Review" (A. Olugboyega Banjo, Nigeria); (2) "The Information Activities of the National Library of Economics in the Federal Republic of…

  3. Conference of the Society for Literature and Science. Proceedings (Atlanta, Georgia, October 10-13, 1996).

    ERIC Educational Resources Information Center

    Perkowitz, Sidney, Ed.

    The papers contained in these proceedings from the 1996 Society for Literature and Science Conference are organized into sections based on theme. Some of these themes are: (1) Secularizing Enlightenment; (2) Eugenics and the Politics of Knowledge; (3) Reading the Discourses of Psychology; (4) Women and Medicine; (5) The Rhetoric of Public Health;…

  4. Impact of an In-Class Biochemistry Mini-Conference on Students' Perception of Science

    ERIC Educational Resources Information Center

    Gerczei, Timea

    2016-01-01

    The work presented here is the summary of a 3 year study that aimed to uncover how students' perception of science changes with the chance to participate in a mini-conference that is incorporated into the biochemistry lecture course. Students were asked to work in groups of 2 or 3 and research a topic that is related to the material covered in…

  5. Conference on Education for Information Science--Strategies for Change in Library School Programs.

    ERIC Educational Resources Information Center

    Klempner, Irving M., Ed.

    1978-01-01

    This proceedings of a conference at the School of Library and Information Science at SUNY-Albany includes two presentations on diagnostics and strategies for change, from the faculty viewpoint and from the administrative viewpoint; three papers on curricular changes and paradigms; and comments by a three-member reactor panel. (MBR)

  6. Open Conference on Information Science in Canada, Proceedings (1st, Montebello, Quebec, May 14 & 15, 1973).

    ERIC Educational Resources Information Center

    Mauerhoff, Georg R., Comp.

    The papers presented at the first Canadian conference on information science are presented in this volume. Six presentations were given under the general topic of research: Research into Privacy and Data Banks, Communications Knowledge Software Industry for Canada, Census Data Access and Statistical Information Management, Communication System…

  7. IFLA General Conference, 1985. Division on Special Libraries. Section on Biological and Medical Science Libraries. Papers.

    ERIC Educational Resources Information Center

    International Federation of Library Associations, The Hague (Netherlands).

    Papers on biological and medical science libraries which were presented at the 1985 International Federation of Library Associations (IFLA) conference include: (1) "The International Programs of the National Library of Medicine" (Lois Ann Colaianni, United States); (2) "Information Needs for International Health. A CDC (Centers for Disease…

  8. IFLA General Conference, 1985. Division on Special Libraries. Section on Science and Technology Libraries. Papers.

    ERIC Educational Resources Information Center

    International Federation of Library Associations, The Hague (Netherlands).

    Papers on science and technology libraries which were presented at the 1985 International Federation of Library Associations (IFLA) conference include: (1) "UAP (Universal Availability of Publications) and User Training for Categories of Grey Literature" (Dieter Schmidmaier, Mining Academy Freiberg, East Germany); (2) "Resource Sharing in Science…

  9. IFLA General Conference, 1984. Special Libraries Division. Section on Science and Technology Libraries. Papers.

    ERIC Educational Resources Information Center

    International Federation of Library Associations, The Hague (Netherlands).

    Papers on scientific/technical information and libraries presented at the 1984 IFLA general conference include: (1) "Library Ethics and the Special Library Network in Science and Technology" (Dieter Schmidmaier, East Germany); (2) "The Dissemination of Patent Information by Libraries: An Example Demonstrating the Necessity of Libraries in the…

  10. News Festival: Science on stage deadline approaches Conference: Welsh conference attracts teachers Data: New phase of CERN openlab tackles exascale IT challenges for science Meeting: German Physical Society holds its physics education spring meeting Conference: Association offers golden opportunity in Norway Competition: So what's the right answer then?

    NASA Astrophysics Data System (ADS)

    2012-07-01

    Festival: Science on stage deadline approaches Conference: Welsh conference attracts teachers Data: New phase of CERN openlab tackles exascale IT challenges for science Meeting: German Physical Society holds its physics education spring meeting Conference: Association offers golden opportunity in Norway Competition: So what's the right answer then?

  11. Precise Pointing for Radio Science Occultations and Radar Mapping During the Cassini Mission at Saturn

    NASA Technical Reports Server (NTRS)

    Burk, Thomas A.

    2015-01-01

    This paper discusses the implementation challenges and lessons learned from radar and radio science pointing observations during the Cassini mission at Saturn. Implementation of the precise desired pointing reveals key issues in the ground system, the flight system, and the pointing paradigm itself. To achieve accurate pointing on some observations, specific workarounds had to be implemented and folded into the sequence development process. Underlying Cassini's pointing system is a remarkable construct known as Inertial Vector Propagation.

  12. IEEE conference record -- abstracts: 1995 IEEE international conference on plasma science

    SciTech Connect

    1995-12-31

    Topics covered at this meeting are: computational plasma physics; slow wave devices; basic phenomena in fully ionized plasmas; microwave-plasma interactions; space plasmas; fast wave devices; plasma processing; plasma, ion, and electron sources; vacuum microelectronics; basic phenomena in partially ionized gases; microwave systems; plasma diagnostics; magnetic fusion theory/experiment; fast opening switches; laser-produced plasmas; dense plasma focus; intense ion and electron beams; plasmas for lighting; fast z-pinches and x-ray lasers; intense beam microwaves; ball lightning/spherical plasma configuration; environmental plasma science; EM and ETH launchers; and environmental/energy issues in plasma science. Separate abstracts were prepared for most of the individual papers.

  13. PREFACE: 23rd International Conference on High Pressure Science and Technology (AIRAPT-23)

    NASA Astrophysics Data System (ADS)

    Gupta, Satish C.

    2012-07-01

    The 23rd AIRAPT International Conference on High Pressure Science and Technology was held at Bhabha Atomic Research Centre, Mumbai, from 25-30 September 2011. This conference is part of the series of AIRAPT International Conferences which are held biennially. AIRAPT is an acronym for the French title which translates as 'International Association for the Advancement of High Pressure Science and Technology'. This was the second time the AIRAPT Conference was organized in India. The first was held 20 years ago at the National Aeronautical Laboratory, Bangalore in 1991. The 23rd Conference covered many important topics in the area of both static and dynamic high pressures including theoretical and experimental investigations on the response of materials under high pressures, new developments using neutron and synchrotron sources, investigations on superconductivity under high pressure, studies of geophysical and planetary sciences, biosciences, and the synthesis of new materials. The conference program included Bridgman award lecture, Jemieson award lecture, seven plenary talks, 85 invited talks, 83 oral presentations and about 195 posters. In all there were 372 presentations. 285 scientists from 19 countries participated in the conference. The countries represented included Austria, Canada, China, Estonia, France, Germany, India, Israel, Italy, Japan, Nepal, New Zealand, Poland, Russia, South Korea, Spain, Sweden, Switzerland, Turkey, UK, Ukraine and USA. Many new developments were presented, for example, measurement techniques using the new generation synchrotron sources, more powerful neutron sources and much brighter laser sources; integration of gas-gun with synchrotron source; the achievement of multi-megabar pressures in shock-less dynamic compressions; and capabilities to synthesize centimeter size diamonds with better quality. All these developments have opened up new opportunities for understanding the physics of materials under high pressures. I would like

  14. Determination of Enceladus' gravity field from Cassini radio science data

    NASA Astrophysics Data System (ADS)

    Parisi, Marzia; Iess, Luciano; Ducci, Marco

    2014-05-01

    ., Science 311, 1393 (2006).

  15. PREFACE: 2013 International Conference on Science & Engineering in Mathematics, Chemistry and Physics (ScieTech 2013)

    NASA Astrophysics Data System (ADS)

    Lumban Gaol, Ford

    2013-03-01

    The 2013 International Conference on Science and Engineering in Mathematics, Chemistry and Physics (ScieTech 2013), was held at the Aston Rasuna Hotel, Jakarta, Indonesia, on 24-25 January 2013. The ScieTech 2013 conference aims to bring together scholars, leading researchers and experts from diverse backgrounds and applications areas. Special emphasis is placed on promoting interaction between the theoretical, experimental, and applied communities, so that a high level exchange is achieved in new and emerging areas within mathematics, chemistry and physics, all areas of sciences and applied mathematics. We would like to thank the invited and plenary speakers as well as all in the Technical Program Committee who have reviewed the papers and developed a very interesting Conference Program. This year, we received 197 papers and, after rigorous review, 67 papers were accepted. The participants come from 21 countries. There are 6 (six) Plenary and Invited Speakers. It is an honour to present this volume of Journal of Physics: Conference Series and we thank the authors for their enthusiastic and high-grade contributions. Finally, we would like to thank the conference chairmen, the members of the steering committee, the organizing committee, the organizing secretariat and the financial support from the conference sponsors that allowed ScieTech 2013 be be sucyh a success. The Editors of the ScieTech 2013 Proceedings Dr Ford Lumban Gaol Dr Hoga Saragih Tumpal Pandiangan Dr Mohamed Bououdina The PDF also contains the abstracts of the Invited and Plenary talks, and some photographs taken during the conference.

  16. 2014 International Conference on Science & Engineering in Mathematics, Chemistry and Physics (ScieTech 2014)

    NASA Astrophysics Data System (ADS)

    2014-04-01

    2014 International Conference on Science & Engineering in Mathematics, Chemistry and Physics (ScieTech 2014), was held at the Media Hotel, Jakarta, Indonesia, on 13-14 January 2014. The ScieTech 2014 conference is aimed to bring together researchers, engineers and scientists in the domain of interest from around the world. ScieTech 2014 is placed on promoting interaction between the theoretical, experimental, and applied communities, so that a high level exchange is achieved in new and emerging areas within Mathematics, Chemistry and Physics. We would like to express our sincere gratitude to all in the Technical Program Committee who have reviewed the papers and developed a very interesting Conference Program as well as the invited and plenary speakers. This year, we received 187 papers and after rigorous review, 50 papers were accepted. The participants come from 16 countries. There are 5 (Five) Paralell Sessions and Four Keynote Speakers. It is an honour to present this volume of Journal of Physics: Conference Series (JPCS) and we deeply thank the authors for their enthusiastic and high-grade contributions. Finally, we would like to thank the conference chairmen, the members of the steering committee, the organizing committee, the organizing secretariat and the financial support from the conference sponsors that allowed the success of ScieTech 2014. The Editors of the Scietech 2014 Proceedings: Dr. Ford Lumban Gaol Dr. Benfano Soewito Dr. P.N. Gajjar

  17. Press abstracts of the 21st Lunar and Planetary Science Conference

    NASA Technical Reports Server (NTRS)

    1990-01-01

    The Program Committee for the Twenty-fisrt Lunar and Planetary Science Conference has chosen these contributions as having the greatest potential interest for the general public. The papers in this collection were written for general presentation, avoiding jargon and unnecessarily complex terms. More technical abstracts will be found in Lunar and Planetary Science XXI. Representative titles are: Ancient Ocean-Land-Atmosphere Interactions on Mars: Global Model and Geological Evidence; Oxygen Isotopic Compositions of Ordinary Chondrites and Their Chondrules; Exposure Ages and Collisional History of L-Chondrite Parent Bodies; Models of Solar-Powered Geysers on Triton; and Search for Life: A Science Rationale for a Permanent Base on Mars.

  18. Proceedings of the 39th Lunar and Planetary Science Conference

    NASA Technical Reports Server (NTRS)

    2008-01-01

    Sessions with oral presentations include: A SPECIAL SESSION: MESSENGER at Mercury, Mars: Pingos, Polygons, and Other Puzzles, Solar Wind and Genesis: Measurements and Interpretation, Asteroids, Comets, and Small Bodies, Mars: Ice On the Ground and In the Ground, SPECIAL SESSION: Results from Kaguya (SELENE) Mission to the Moon, Outer Planet Satellites: Not Titan, Not Enceladus, SPECIAL SESSION: Lunar Science: Past, Present, and Future, Mars: North Pole, South Pole - Structure and Evolution, Refractory Inclusions, Impact Events: Modeling, Experiments, and Observations, Mars Sedimentary Processes from Victoria Crater to the Columbia Hills, Formation and Alteration of Carbonaceous Chondrites, New Achondrite GRA 06128/GRA 06129 - Origins Unknown, The Science Behind Lunar Missions, Mars Volcanics and Tectonics, From Dust to Planets (Planetary Formation and Planetesimals):When, Where, and Kaboom! Astrobiology: Biosignatures, Impacts, Habitability, Excavating a Comet, Mars Interior Dynamics to Exterior Impacts, Achondrites, Lunar Remote Sensing, Mars Aeolian Processes and Gully Formation Mechanisms, Solar Nebula Shake and Bake: Mixing and Isotopes, Lunar Geophysics, Meteorites from Mars: Shergottite and Nakhlite Invasion, Mars Fluvial Geomorphology, Chondrules and Chondrule Formation, Lunar Samples: Chronology, Geochemistry, and Petrology, Enceladus, Venus: Resurfacing and Topography (with Pancakes!), Overview of the Lunar Reconnaissance Orbiter Mission, Mars Sulfates, Phyllosilicates, and Their Aqueous Sources, Ordinary and Enstatite Chondrites, Impact Calibration and Effects, Comparative Planetology, Analogs: Environments and Materials, Mars: The Orbital View of Sediments and Aqueous Mineralogy, Planetary Differentiation, Titan, Presolar Grains: Still More Isotopes Out of This World, Poster sessions include: Education and Public Outreach Programs, Early Solar System and Planet Formation, Solar Wind and Genesis, Asteroids, Comets, and Small Bodies, Carbonaceous

  19. PREFACE: 4th Global Conference on Materials Science and Engineering (CMSE 2015)

    NASA Astrophysics Data System (ADS)

    Ruda, H. E.; Khotsianovsky, A.

    2015-12-01

    IOP Conference Series: Materials Science and Engineering is publishing a volume of conference proceedings that contains a selection of papers presented at the 4th Global Conference on Materials Science and Engineering (CMSE 2015), which is an annual event that started in 2012. CMSE 2015, technically supported by the Institute of Applied Physics and Materials Engineering of University of Macau, organized by Wuhan Advance Materials Society, was successfully held at the University of Macau-new campus located on Hengqin Island from August 3rd-6th, 2015. It aims to bring together leading academic scientists, researchers and scholars to exchange and share their experience and research results on all aspects of Materials Science and Engineering, and to discuss the practical challenges encountered and the solutions adopted. Macau, one of the two special administrative regions of the People's Republic of China, where East meets West, turned out to be an ideal meeting place for domestic and overseas participants of this annual international conference. The conference program included keynote presentations, special sessions, oral and poster contributions. From several hundred submissions, 52 of the most promising and mainstream, IOP-relevant, contributions were included in this volume. The submissions present original ideas or results of general significance, supported by clear reasoning, compelling evidence and methods, theories and practices relevant to the research. The authors state clearly the problems and the significance of their research to theory and practice. Being a successful conference, this event gathered more than 200 qualified and high-level researchers and experts from over 40 countries, including 10 keynote speakers from 6 countries, which created a good platform for worldwide researchers and engineers to enjoy the academic communication. Taking advantage of this opportunity, we would like to thank all participants of this conference, and particularly the

  20. Taking the initiative: A leadership conference for women in science and engineering

    NASA Technical Reports Server (NTRS)

    1994-01-01

    The conference sprang from discussions on the current climate that women face in science, mathematics, engineering, and technology. The conference (and this document) is a beginning, not a culmination, of women's learning leadership skills. Conferees were active, articulate, energetic, and ready to learn leadership qualities, some of which seem universal, others that appear to require skills in specific fields. After the introduction, the workshops and presentations are arranged under vision and direction, barriers, alignment and communication, and motivation and inspiration. Some statistics are presented on women degrees and employment in various fields.

  1. Taking the initiative. A leadership conference for women in science and engineering

    SciTech Connect

    1994-12-31

    The conference sprang from discussions on the current climate that women face in science, mathematics, engineering, and technology. The conference (and this document) is a beginning, not a culmination, of women`s learning leadership skills. Conferees were active, articulate, energetic, and ready to learn leadership qualities, some of which seem universal, others that appear to require skills in specific fields. After the introduction, the workshops and presentations are arranged under vision and direction, barriers, alignment and communication, and motivation and inspiration. Some statistics are presented on women degrees and employment in various fields.

  2. Application of high stability oscillators to radio science experiments using deep space probes

    NASA Technical Reports Server (NTRS)

    Kursinski, Emil R.

    1990-01-01

    The microwave telecommunication links between the earth and deep space probes have long been used to conduct radio science experiments which take advantage of the phase coherency and stability of these links. These experiments measure changes in the phase delay of the signals to infer electrical, magnetic and gravitational properties of the solar system environment and beyond through which the spacecraft and radio signals pass. The precision oscillators, from which the phase of the microwave signals are derived, play a key role in the stability of these links and therefore the sensitivity of these measurements. These experiments have become a driving force behind recent and future improvements in the Deep Space Network and spacecraft oscillators and frequency and time distribution systems. Three such experiments which are key to these improvements are briefly discussed and relationship between their sensitivity and the signal phase stability is described. The first is the remote sensing of planetary atmospheres by occultation in which the radio signal passes through the atmosphere and is refracted causing the signal pathlength to change from which the pressure and the temperature of the atmosphere can be derived. The second experiment is determination of the opacity of planetary rings by passage of the radio signals through the rings. The third experiment is the research for very low frequency gravitational radiation. The fractional frequency variation of the signal is comparable to the spatial strain amplitude the system is capable of detecting. A summary of past results and future possibilities for these experiments are presented.

  3. Radio Frequency Interference: Projects and Activities Developed for the High School Earth Science, Astronomy, and Physics Classroom

    NASA Astrophysics Data System (ADS)

    Dunn, S. K.; Brown, J.

    2003-12-01

    Radio Frequency Interference: Projects and Activities Developed for the High School Earth Science, Astronomy, and Physics Classroom Susan Dunn Tewksbury Memorial High School Jason Brown Tyngsboro High School Preethi Pratap MIT Haystack Observatory The Research Experiences for Teachers (RET) program, funded by the NSF, brings teachers into research environments to interact with scientists and translate the experience into the classroom. We will describe a RET experience at the MIT Haystack Observatory which involved using an AR3000A communications receiver and a discone antenna as the basis for an Earth Science, Astronomy, and Physics classroom unit. The projects and activities in this unit were developed to help foster student learning and understanding of radio astronomy, the electromagnetic spectrum, wave dynamics, signal propagation, meteor detection, and radio frequency interference. Additionally, this RET project utilizes the SEARFE (Students Examining Australia???s Radio Frequency Environment) software developed for use with the AR3000A communications receiver to scan and monitor frequencies across the radio bandwidth to determine areas of low and high usage in the radio spectrum. Classroom activities include Scanning Protected Radio Astronomy Bandwidths, Investigating the Radio Environment, Time Variation of Signal Strength, Signal Strength vs. Location Studies, Detecting Meteors using the AR300A Receiver, Mapping the RFI Environment of Your School, AM Radio Interference, and Signal Propagation Effects. The primary focus of the unit???s activities is to address the Massachusetts State Science Frameworks for electromagnetic radiation, waves, cosmology, and matter and energy in the Earth system and foster an understanding of how everyday communications devices may cause radio frequency interference with sensitive radio astronomy equipment. The projects and activities in the unit will be used in the classroom, amended, and the results of the classroom

  4. 13th ERS Lung Science Conference. The most important take home messages: News from the Underground.

    PubMed

    Bikov, Andras; Boots, Agnes; Bjerg, Anders; Jacinto, Tiago; Olland, Anne; Skoczyński, Szymon

    2015-06-01

    The 13th ERS Lung Science Conference (LSC) was organised to bring academics together from all over the world to present and discuss the latest developments regarding lung infection and immunity. The conference took place in breathtaking Estoril, Portugal; however, it wasn't the beautiful surroundings that were our main motivation to attend, but instead the scientific merit of the conference and the chance to create new scientific collaborations. The scientific programme [1] was packed with the most up-to-date content in the field of lung infection and immunity and included some of the top researchers within this exciting area. Moreover, the convenient size of the LSC offered the opportunity to renew and intensify friendships and collaborations. In particular, for researchers at the start of their career, this is a great feature and we therefore warmly recommend the LSC to ERS Juniors Members!

  5. The radio science experiment with BepiColombo mission to Mercury .

    NASA Astrophysics Data System (ADS)

    Schettino, G.; Di Ruzza, S.; De Marchi, F.; Cicalò, S.; Tommei, G.; Milani, A.

    BepiColombo is a joint ESA/JAXA mission to Mercury with challenging objectives regarding geophysics, geodesy and fundamental physics. The Mercury Orbiter Radio science Experiment (MORE) is one of the on-board experiments, including three different but linked experiments: gravimetry, rotation and relativity. Using radio observables (range and range-rate) performed with very accurate tracking from ground stations, together with optical observations from the on-board high resolution camera (SIMBIO-SYS) and accelerometer readings from the on-board accelerometer (ISA), MORE will be able to measure with unprecedented accuracy the global gravity field of Mercury and the rotation state of the planet. In this work we present the results of a numerical full-cycle simulation of the gravimetry and rotation experiments of MORE: we discuss the accuracies which can be achieved, focussing in particular on the possible benefits from the use of optical observations in support to the tracking measurements.

  6. Longitudinal effects of college type and selectivity on degrees conferred upon undergraduate females in physical science, life science, math and computer science, and social science

    NASA Astrophysics Data System (ADS)

    Stevens, Stacy Mckimm

    There has been much research to suggest that a single-sex college experience for female undergraduate students can increase self-confidence and leadership ability during the college years and beyond. The results of previous studies also suggest that these students achieve in the workforce and enter graduate school at higher rates than their female peers graduating from coeducational institutions. However, some researchers have questioned these findings, suggesting that it is the selectivity level of the colleges rather than the comprised gender of the students that causes these differences. The purpose of this study was to justify the continuation of single-sex educational opportunities for females at the post-secondary level by examining the effects that college selectivity, college type, and time have on the rate of undergraduate females pursuing majors in non-traditional fields. The study examined the percentage of physical science, life science, math and computer science, and social science degrees conferred upon females graduating from women's colleges from 1985-2001, as compared to those at comparable coeducational colleges. Sampling for this study consisted of 42 liberal arts women's (n = 21) and coeducational (n = 21) colleges. Variables included the type of college, the selectivity level of the college, and the effect of time on the percentage of female graduates. Doubly multivariate repeated measures analysis of variance testing revealed significant main effects for college selectivity on social science graduates, and time on both life science and math and computer science graduates. Significant interaction was also found between the college type and time on social science graduates, as well as the college type, selectivity level, and time on math and computer science graduates. Implications of the results and suggestions for further research are discussed.

  7. PREFACE: 1st International Conference in Applied Physics and Materials Science

    NASA Astrophysics Data System (ADS)

    2015-06-01

    We are delighted to come up with thirty two (32) contributed research papers in these proceedings, focusing on Materials Science and Applied Physics as an output of the 2013 International Conference in Applied Physics and Materials Science (ICAMS2013) held on October 22-24, 2013 at the Ateneo de Davao University, Davao City, Philippines. The conference was set to provide a high level of international forum and had brought together leading academic scientists, industry professionals, researchers and scholars from universities, industries and government agencies who have shared their experiences, research results and discussed the practical challenges encountered and the solutions adopted as well as the advances in the fields of Applied Physics and Materials Science. This conference has provided a wide opportunity to establish multidisciplinary collaborations with local and foreign experts. ICAMS2013, held concurrently with 15th Samahang Pisika ng Visayas at Mindanao (SPVM) National Physics Conference and 2013 International Meeting for Complex Systems, was organized by the Samahang Pisika ng Visayas at Mindanao (Physics Society of Visayas and Mindanao) based in MSU-Iligan Institute of Technology, Iligan City, Philippines. The international flavor of converging budding researchers and experts on Materials Science and Applied Physics was the first to be organized in the 19 years of SPVM operation in the Philippines. We highlighted ICAMS2013 gathering by the motivating presence of Dr. Stuart Parkin, a British Physicist, as one of our conference's plenary speakers. Equal measures of gratitude were also due to all other plenary speakers, Dr. Elizabeth Taylor of Institute of Physics (IOP) in London, Dr. Surya Raghu of Advanced Fluidics in Maryland, USA and Prof. Hitoshi Miyata of Niigata University, Japan, Prof. Djulia Onggo of Institut Teknologi Bandung, Indonesia, and Dr. Hironori Katagiri of Nagaoka National College of Technology, Japan. The warm hospitality of the host

  8. NSSDC Conference on Mass Storage Systems and Technologies for Space and Earth Science Applications, volume 3

    NASA Technical Reports Server (NTRS)

    Kobler, Ben (Editor); Hariharan, P. C. (Editor); Blasso, L. G. (Editor)

    1992-01-01

    This report contains copies of nearly all of the technical papers and viewgraphs presented at the National Space Science Data Center (NSSDC) Conference on Mass Storage Systems and Technologies for Space and Earth Science Applications. This conference served as a broad forum for the discussion of a number of important issues in the field of mass storage systems. Topics include magnetic disk and tape technologies, optical disk and tape, software storage and file management systems, and experiences with the use of a large, distributed storage system. The technical presentations describe, among other things, integrated mass storage systems that are expected to be available commercially. Also included is a series of presentations from Federal Government organizations and research institutions covering their mass storage requirements for the 1990s.

  9. Report on a Boston University Conference December 7-8, 2012 on How Can the History and Philosophy of Science Contribute to Contemporary US Science Teaching?

    NASA Astrophysics Data System (ADS)

    Garik, Peter; Benétreau-Dupin, Yann

    2014-09-01

    This is an editorial report on the outcomes of an international conference sponsored by a grant from the National Science Foundation (NSF) (REESE-1205273) to the School of Education at Boston University and the Center for Philosophy and History of Science at Boston University for a conference titled: How Can the History and Philosophy of Science Contribute to Contemporary US Science Teaching? The presentations of the conference speakers and the reports of the working groups are reviewed. Multiple themes emerged for K-16 education from the perspective of the history and philosophy of science. Key ones were that: students need to understand that central to science is argumentation, criticism, and analysis; students should be educated to appreciate science as part of our culture; students should be educated to be science literate; what is meant by the nature of science as discussed in much of the science education literature must be broadened to accommodate a science literacy that includes preparation for socioscientific issues; teaching for science literacy requires the development of new assessment tools; and, it is difficult to change what science teachers do in their classrooms. The principal conclusions drawn by the editors are that: to prepare students to be citizens in a participatory democracy, science education must be embedded in a liberal arts education; science teachers alone cannot be expected to prepare students to be scientifically literate; and, to educate students for scientific literacy will require a new curriculum that is coordinated across the humanities, history/social studies, and science classrooms.

  10. Improved spacecraft tracking and navigation using a Portable Radio Science Receiver

    NASA Astrophysics Data System (ADS)

    Soriano, M.; Jacobs, C.; Navarro, R.; Naudet, C.; Rogstad, S.; White, L.; Finley, S.; Goodhart, C.; Sigman, E.; Trinh, J.; Garcia, J. L.; Garcia-Miro, C.; Mercolino, M.; Madde, R.

    The Portable Radio Science Receiver (PRSR) is a suitcase-sized open-loop digital receiver designed to be small and easy to transport so that it can be deployed quickly and easily anywhere in the world. The PRSR digitizes, down-converts, and filters using custom hardware, firmware, and software. Up to 16 channels can be independently configured and recorded with a total data rate of up to 256 Mbps. The design and implementation of the system's hardware, firmware, and software is described. To minimize costs and time to deployment, our design leveraged elements of the hardware, firmware, and software designs from the existing full-sized operational (non-portable) Radio Science Receivers (RSR) and Wideband VLBI Science Receivers (WVSR), which have successfully supported flagship NASA deep space missions at all Deep Space Network (DSN) sites. We discuss a demonstration of the PRSR using VLBI, with one part per billion angular resolution: 1 nano-radian / 200 μ as. This is the highest resolution astronomical instrument ever operated solely from the Southern Hemisphere. Preliminary results from two sites are presented, including the European Space Agency (ESA) sites at Cebreros, Spain and Malargü e, Argentina. Malargü e's South American location is of special interest because it greatly improves the geometric coverage for spacecraft navigation in the Southern Hemisphere and will for the first time provide coverage to the 1/4 of the range of declination that has been excluded from reference frame work at Ka-band.

  11. Improved Spacecraft Tracking and Navigation Using a Portable Radio Science Receiver

    NASA Technical Reports Server (NTRS)

    Soriano, Melissa; Jacobs, Christopher; Navarro, Robert; Naudet, Charles; Rogstad, Stephen; White, Leslie; Finley, Susan; Goodhart, Charles; Sigman, Elliott; Trinh, Joseph

    2013-01-01

    The Portable Radio Science Receiver (PRSR) is a suitcase-sized open-loop digital receiver designed to be small and easy to transport so that it can be deployed quickly and easily anywhere in the world. The PRSR digitizes, downconverts, and filters using custom hardware, firmware, and software. Up to 16 channels can be independently configured and recorded with a total data rate of up to 256 Mbps. The design and implementation of the system's hardware, firmware, and software is described. To minimize costs and time to deployment, our design leveraged elements of the hardware, firmware, and software designs from the existing full-sized operational (non-portable) Radio Science Receivers (RSR) and Wideband VLBI Science Receivers (WVSR), which have successfully supported flagship NASA deep space missions at all Deep Space Network (DSN) sites. We discuss a demonstration of the PRSR using VLBI, with one part per billion angular resolution: 1 nano-radian / 200 ?as synthesized beam. This is the highest resolution astronomical instrument ever operated solely from the Southern Hemisphere. Preliminary results from two sites are presented, including the European Space Agency (ESA) sites at Cebreros, Spain and Malargue, Argentina. Malargue's South American location is of special interest because it greatly improves the geometric coverage for spacecraft navigation in the Southern Hemisphere and will for the first time provide coverage to the 1/4 of the range of declination that has been excluded from reference frame work at Ka-band.

  12. Improved Spacecraft Tracking and Navigation Using a Portable Radio Science Receiver

    NASA Astrophysics Data System (ADS)

    Soriano, M.; Jacobs, Christopher S.; Navarro, Robert; Naudet, C.; Rogstad, S.; White, L.; Finley, S.; Goodhart, C.; Sigman, E.; Trinh, J.; Lobo-Garcia, J.; García-Miró, C.; Mercolino, M.; Maddè, R.

    2013-05-01

    The Portable Radio Science Receiver (PRSR) is a suitcase-sized open-loop digital receiver designed to be small and easy to transport so that it can be deployed quickly and easily anywhere in the world. The PRSR digitizes, downconverts, and filters using custom hardware, firmware, and software. Up to 16 channels can be independently configured and recorded with a total data rate of up to 256 Mbps. The design and implementation of the system's hardware, firmware, and software is described. To minimize costs and time to deployment, our design leveraged elements of the hardware, firmware, and software designs from the existing full-sized operational (non-portable) Radio Science Receivers (RSR) and Wideband VLBI Science Receivers (WVSR), which have successfully supported flagship NASA deep space missions at all Deep Space Network (DSN) sites. We discuss a demonstration of the PRSR using VLBI, with one part per billion angular resolution: 1 nano-radian / 200 μas. This is the highest resolution astronomical instrument ever operated solely from the Southern Hemisphere. Preliminary results from two sites are presented, including the European Space Agency (ESA) sites at Cebreros, Spain and Malargüe, Argentina. Malargüe's South American location is of special interest because it greatly improves the geometric coverage for spacecraft navigation in the Southern Hemisphere and will for the first time provide coverage to the 1/4 of the range of declination that has been excluded from reference frame work at Ka-band.

  13. Conference of the Society for Literature and Science. Proceedings (Los Angeles, California, November 2-5, 1995).

    ERIC Educational Resources Information Center

    Labinger, Jay, Ed.

    The papers contained in this proceedings from the 1995 Society for Literature and Science Conference are organized into sections with the following themes: (1) Metaphor and Science; (2) The Technological Invasion of the Living Space; (3) Autobiographies and Biographies of Scientists; (4) Science and 19th Century Literature; (5) Visions of the…

  14. Proceedings of the Klamath Basin Science Conference, Medford, Oregon, February 1-5, 2010

    USGS Publications Warehouse

    Thorsteinson, Lyman; VanderKooi, Scott; Duffy, Walter

    2011-01-01

    This report presents the proceedings of the Klamath Basin Science Conference (February 2010). A primary purpose of the meeting was to inform and update Klamath Basin stakeholders about areas of scientific progress and accomplishment during the last 5 years. Secondary conference objectives focused on the identification of outstanding information needs and science priorities as they relate to whole watershed management, restoration ecology, and possible reintroduction of Pacific salmon associated with the Klamath Basin Restoration Agreement (KBRA). Information presented in plenary, technical, breakout, and poster sessions has been assembled into chapters that reflect the organization, major themes, and content of the conference. Chapter 1 reviews the major environmental issues and resource management and other stakeholder needs of the basin. Importantly, this assessment of information needs included the possibility of large-scale restoration projects in the future and lessons learned from a case study in South Florida. Other chapters (2-6) summarize information about key components of the Klamath Basin, support conceptual modeling of the aquatic ecosystem (Chapter 7), and synthesize our impressions of the most pressing science priorities for management and restoration. A wealth of information was presented at the conference and this has been captured in chapters addressing environmental setting and human development of the basin, hydrology, watershed processes, fishery resources, and potential effects from climate change. The final chapter (8) culminates in a discussion of many specific research priorities that relate to and bookend the broader management needs and restoration goals identified in Chapter 1. In many instances, the conferees emphasized long-term and process-oriented approaches to watershed science in the basin as planning moves forward.

  15. Overview of Cassini radio science at Saturn, Titan, and the icy satellites

    NASA Astrophysics Data System (ADS)

    Kliore, A. J.; Ambrosini, R.; Armstrong, J. W.; Flasar, F. M.; French, R. G.; Iess, L.; Marouf, E. A..; Nagy, A. F.; Rappaport, N. J.; Tortora, P.; Jpl/Dsn Radio Science Support Team

    The Cassini spacecraft which has been in orbit about Saturn for over two years is the first Radio Science platform to provide three downlink frequencies In addition to the X-band telemetry link 3 56 cm w l two other frequencies S-band 13 04 cm and Ka-band 0 94 cm are available This plus the high SNR 50 dBHz at X-band afforded by the 4 m diameter s c high gain antenna in combination with the excellent low noise receivers of the DSN as well as overall system stabilities of 1 part in 10 13 when referenced to the on-board ultra-stable oscillator USO in one-way operation and 1 part inx 10 15 for a two-way link make Cassini an unprecedented instrument of radio science The orbital tour phase of the mission has the following main radio science objectives a determination of the masses and gravity fields of Saturn s icy satellites Titan and Saturn through two-way tracking during fly-bys To date the masses of Phoebe Iapetus Dione Enceladus Rhea and Titan have been measured and will be reported here b Measurement of the structure and other properties of Saturn s rings through three-band occultation Seven near-diametric occultations at a high ring opening angle have been completed and the results will be presented here c Measurement of the vertical structure of the atmosphere and ionosphere of Saturn The same series of occultations have provided nearly equatorial observations of the atmosphere structure and the ionosphere and the results will be described here d Measurement of the vertical structure of

  16. Research in Science Education, Volume 1990. Selected Refereed Papers from the Annual Conference of the Australasian Science Education Research Association (21st, Perth, Western Australia, July 1990).

    ERIC Educational Resources Information Center

    Gardner, Paul L., Ed.

    1990-01-01

    This book contains selected refereed papers from the 21st Annual Conference of the Australasian Science Education Research Association. The papers are as follows: "A Learning Model for Science Education: Developing Teaching Strategies" (Appleton); "Researching Balance between Cognition and Affect in Science Teaching" (Baird et al.); "Toward a…

  17. UNDERGRADUATE EDUCATION IN THE BIOLOGICAL SCIENCES FOR STUDENTS IN AGRICULTURE AND NATURAL RESOURCES, PROCEEDINGS OF A CONFERENCE.

    ERIC Educational Resources Information Center

    National Academy of Sciences - National Research Council, Washington, DC.

    REPORTED ARE THE PROCEEDINGS OF A 1966 CONFERENCE WHICH DEALT WITH UNDERGRADUATE EDUCATIONAL NEEDS FOR STUDENTS IN AGRICULTURE AND NATURAL RESOURCES. THE 167 EDUCATORS (MOSTLY DEANS AND DIRECTORS OF RESIDENT INSTRUCTION) WHO PARTICIPATED IN THE CONFERENCE REPRESENTED AGRICULTURE, RENEWABLE NATURAL RESOURCES, THE BIOLOGICAL SCIENCES, AND…

  18. Undergraduate Education in the Sciences for Students in Agriculture and Natural Resources. Summary of Proceedings of Regional Conferences.

    ERIC Educational Resources Information Center

    Commission on Education in Agriculture and Natural Resources, Washington, DC.

    Following a national conference entitled, "Undergraduate Education in the Biological Sciences for Students in Agriculture and Natural Resources," four regional conferences ensued, bringing together teaching faculty members from agriculture, forestry, other natural resource areas, and biology. The papers presented at these regional meetings are…

  19. Proceedings of the Fourth International Conference on Mars Polar Science and Exploration

    NASA Technical Reports Server (NTRS)

    2006-01-01

    Sessions in this conference include: Mars polar geology and glaciology; Mars and terrestrial radar investigations; Observations, nature, and evolution of the Martian seasonal polar caps; Mars' residual south polar cap; Climate change, ice core analysis, and the redistribution of volatiles on Mars; errestrial Mars analog environments; The Phoenix Scout mission and the nature of the near-polar environment; Moderated Discussion: Key Issues Regarding Phoenix Scout Mission and the nature of the near-polar environment; Panel Discussion: Key Issues in Mars Polar Science and Exploration; Mars Reconnaissance Orbiter investigations of the Martian polar regions and climate; Mars Polar Scout Mission concepts; and Panel Discussion: New perspectives on Mars polar science and exploration

  20. PREFACE: 6th Vacuum and Surface Sciences Conference of Asia and Australia (VASSCAA-6)

    NASA Astrophysics Data System (ADS)

    Ahsan Bhatti, Javaid; Hussain, Talib; Khan, Wakil

    2013-06-01

    The Vacuum and Surface Sciences Conference of Asia and Australia (VASSCAA) conference series has been organized to create a new forum in Asia and Australia to discuss vacuum, surface and related sciences, techniques and applications. The conference series is officially endorsed by the International Union for Vacuum Science, Technique and Application (IUVSTA). The International Steering Committee of VASSCAA is comprised of Vacuum Societies in seven countries: Australia, China, India, Iran, Japan, South Korea and Pakistan. VASSCAA-1 was organized by the Vacuum Society of Japan in 1999 in Tokyo, Japan. VASSCAA-2 was held in 2002 in Hong Kong, VASSCAA-3 in Singapore in 2005. VASSCAA-4 was held in Matsue, Japan in 2008 and VASSCAA-5 in 2010 in Beijing, China. The 6th Vacuum and Surface Sciences Conference of Asia and Australia (VASSCAA-6) was held from 9-13 October 2012 in the beautiful city of Islamabad, Pakistan. The venue of the conference was the Pak-China Friendship Centre, Islamabad. More than six hundred local delgates and around seventy delegates from different countries participated in this mega event. These delegates included scientists, researchers, engineers, professors, plant operators, designers, vendors, industrialists, businessmen and students from various research organizations, technical institutions, universities, industries and companies from Pakistan and abroad. The focal point of the event was to enhance cooperation between Pakistan and the international community in the fields of vacuum, surface science and other applied technologies. At VASSCAA-6 85 oral presentations were delivered by local and foreign speakers. These were divided into different sessions according to their fields. A poster session was organized at which over 70 researchers and students displayed their posters. The best three posters won prizes. In parallel to the main conference sessions four technical short courses were held. The participants showed keen interest in all these

  1. The Venus Neutral Atmosphere from the Radio Science Experiment VeRa on Venus Express

    NASA Astrophysics Data System (ADS)

    Tellmann, S.; Haeusler, B.; Paetzold, M.; Bird, M. K.; Tyler, G. L.

    2008-12-01

    The Venus Express Radio Science Experiment VeRa is sounding the Venus neutral atmosphere and ionosphere using the spacecraft radio subsystem in the oneway radio link mode at X-band (8.4 GHz) and S- band (2.3 GHz). An Ultrastable Oscillator (USO) provides a high quality onboard frequency reference source for the derivation of electron density profiles in the ionosphere and profiles of pressure, temperature and neutral number density of the neutral atmosphere. Radial profiles of neutral number density derived from the occultations cover the altitude range 40 to 90 km, which are converted to vertical profiles of temperature and pressure. The polar orbit of Venus Express provides the opportunity to study the atmosphere at all planetocentric latitudes under varying illumination conditions. Five occultation seasons could be covered so far during the Venus Express mission resulting in a data set of more than 150 profiles of the neutral atmosphere. The thermal structure is investigated with regard to the latitudinal and temporal variability. A distinct cold collar region could be observed on both hemispheres. The tropopause altitude increases in this latitude region while the tropopause temperature shows a strong decrease. Profiles of static stability are found to be latitude-dependent and nearly adiabatic in the middle cloud region.

  2. Summaries of Conference Papers, Theme 1, Research Findings. International Conference on Evaluation and Research in Educational Television and Radio (Milton Keynes, England, April 9-13, 1976).

    ERIC Educational Resources Information Center

    Open Univ., Walton, Bletchley, Bucks (England).

    Educational television and radio research and evaluation findings are the subject of 25 papers summarized in this document. Seven papers deal with evaluation of research projects in educational television and radio. Four papers on adult education and two on educational technology in teacher training are also summarized. Research in teaching with…

  3. The Venus Neutral Atmosphere from the Radio Science Experiment VeRa on Venus Express

    NASA Astrophysics Data System (ADS)

    Tellmann, Silvia; Haeusler, Bernd; Paetzold, Martin; Bird, Michael; Tyler, G. L.; Andert, Thomas; Remus, Stefan

    The Venus Express Radio Science Experiment VeRa performs regular radio-sounding experi-ments in the Venus neutral atmosphere and ionosphere using the spacecraft radio subsystem in the one-way radio mode at X-band (8.4 GHz) and S-band (2.3 GHz). An Ultra-Stable Oscilla-tor (USO) provides a high quality on-board frequency reference for refractivity measurements, from which electron density profiles in the ionosphere and profiles of pressure, temperature and neutral number density of the neutral atmosphere are derived. Radial profiles of neutral number density from the atmospheric-induced Doppler shift during the occultations cover the altitude range 40-90 km. These are then used to derive vertical profiles of temperature and pressure. The polar orbit of Venus Express provides the opportunity to study the troposphere and meso-sphere at all planetocentric latitudes under varying illumination conditions. Seven occultation seasons have occurred thus far during the Venus Express mission, resulting in a data set with more than 320 neutral atmospheric profiles. The thermal structure is investigated with regard to the latitudinal and temporal variability. The Venus mesosphere shows a high variability resulting from atmospheric waves and turbulence. Profiles of atmospheric static stability are found to be latitude dependent and nearly adiabatic in the middle cloud region. Abrupt changes in the static stability can occur at the boundaries of the middle cloud layer, the vertical dis-tribution of which shows a distinct latitudinal dependence. Correlations of wave activity with the static stability profile will be investigated

  4. The Martian Neutral Atmosphere from the Radio Science Experiment MaRS on Mars Express

    NASA Astrophysics Data System (ADS)

    Tellmann, S.; Pätzold, M.; Häusler, B.; Tyler, G. L.; Hinson, D. P.

    2008-09-01

    The Radio Science Experiment MaRS on Mars Express is sounding the Martian atmosphere and ionosphere using the spacecraft radio signals at Xband and S-band in Earth occultation geometry. MaRS relies on the observation of the phase, amplitude, polarisation and propagation times of radio signals transmitted from the spacecraft and received on Earth. The signals are affected by the different dispersive media through which they propagate (atmospheres, ionospheres, interplanetary medium, solar corona), by gravitational influences of planets and by the classical Doppler shift resulting from the relative motion of spacecraft, Earth and Mars. A simultaneous and coherent dual-frequency downlink at X- and S-band via the Spacecraft's High Gain Antenna (HGA) is required to separate effects of dispersive media from the classical Doppler shift. The bending of the radio carrier ray paths in the Martian atmosphere prior to the occultation of the spacecraft by the planetary disc as seen from the Earth is used to derive vertical profiles of density, pressure and temperature. The bending is caused by atmospheric refractivity and vertical density and temperature profiles can be retrieved assuming hydrostatic equilibrium and ideal gas law. The elliptical orbit of Mars Express allows to investigate a large range of local times and locations and can therefore be used to study latitudinal, diurnal and seasonal variations. The data set retrieved since March 2004 is quite complementary to the Mars Global Surveyor profiles with regard to the local times and the geographical distribution of the measurements. This presentation will compare the MaRS results with model data and data from other Mars missions.

  5. The Deep Space Atomic Clock: Ushering in a New Paradigm for Radio Navigation and Science

    NASA Technical Reports Server (NTRS)

    Ely, Todd; Seubert, Jill; Prestage, John; Tjoelker, Robert

    2013-01-01

    The Deep Space Atomic Clock (DSAC) mission will demonstrate the on-orbit performance of a high-accuracy, high-stability miniaturized mercury ion atomic clock during a year-long experiment in Low Earth Orbit. DSAC's timing error requirement provides the frequency stability necessary to perform deep space navigation based solely on one-way radiometric tracking data. Compared to a two-way tracking paradigm, DSAC-enabled one-way tracking will benefit navigation and radio science by increasing the quantity and quality of tracking data. Additionally, DSAC also enables fully-autonomous onboard navigation useful for time-sensitive situations. The technology behind the mercury ion atomic clock and a DSAC mission overview are presented. Example deep space applications of DSAC, including navigation of a Mars orbiter and Europa flyby gravity science, highlight the benefits of DSAC-enabled one-way Doppler tracking.

  6. Radio science investigations by VeRa onboard the Venus Express spacecraft

    NASA Astrophysics Data System (ADS)

    Häusler, B.; Pätzold, M.; Tyler, G. L.; Simpson, R. A.; Bird, M. K.; Dehant, V.; Barriot, J.-P.; Eidel, W.; Mattei, R.; Remus, S.; Selle, J.; Tellmann, S.; Imamura, T.

    2006-11-01

    The Venus Express Radio Science Experiment (VeRa) uses radio signals at wavelengths of 3.6 and 13 cm ("X"- and "S"-band, respectively) to investigate the Venus surface, neutral atmosphere, ionosphere, and gravity field, as well as the interplanetary medium. An ultrastable oscillator (USO) provides a high quality onboard reference frequency source; instrumentation on Earth is used to record amplitude, phase, propagation time, and polarization of the received signals. Simultaneous, coherent measurements at the two wavelengths allow separation of dispersive media effects from classical Doppler shift. VeRa science objectives include the following: Determination of neutral atmospheric structure from the cloud deck (approximately 40 km altitude) to 100 km altitude from vertical profiles of neutral mass density, temperature, and pressure as a function of local time and season. Within the atmospheric structure, search for, and if detected, study of the vertical structure of localized buoyancy waves, and the presence and properties of planetary waves. Study of the H 2SO 4 vapor absorbing layer in the atmosphere by variations in signal intensity and application of this information to tracing atmospheric motions. Scintillation effects caused by radio wave diffraction within the atmosphere can also provide information on small-scale atmospheric turbulence. Investigation of ionospheric structure from approximately 80 km to the ionopause (<600 km), allowing study of the interaction between solar wind plasma and the Venus atmosphere. Observation of forward-scattered surface echoes obliquely reflected from selected high-elevation targets with anomalous radar properties (such as Maxwell Montes). More generally, such bistatic radar measurements provide information on the roughness and density of the surface material on scales of centimeters to meters. Detection of gravity anomalies, thereby providing insight into the properties of the Venus crust and lithosphere. Measurement of the

  7. Improved spacecraft radio science using an on-board atomic clock: Application to gravitational wave searches

    SciTech Connect

    Tinto, Massimo; Dick, George J.; Prestage, John D.; Armstrong, J. W.

    2009-05-15

    Recent advances in space-qualified atomic clocks (low-mass, low power-consumption, frequency stability comparable to that of ground-based clocks) can enable interplanetary spacecraft radio science experiments at unprecedented Doppler sensitivities. The addition of an on-board digital receiver would allow the up- and down-link Doppler frequencies to be measured separately. Such separate, high-quality measurements allow optimal data combinations that suppress the currently leading noise sources: phase scintillation noise from the Earth's atmosphere and Doppler noise caused by mechanical vibrations of the ground antenna. Here we provide a general expression for the optimal combination of ground and on-board Doppler data and compute the sensitivity such a system would have to low-frequency gravitational waves (GWs). Assuming a plasma scintillation noise calibration comparable to that already demonstrated with the multilink CASSINI radio system, the space-clock/digital-receiver instrumentation enhancements would give GW strain sensitivity of 3.7x10{sup -14} Hz{sup -1/2} for randomly polarized, monochromatic GW signals isotropically distributed over the celestial sphere, over a two-decade ({approx}0.0001-0.01 Hz) region of the low-frequency band. This is about an order of magnitude better than currently achieved with traditional two-way coherent Doppler experiments. The utility of optimally combining simultaneous up- and down-link observations is not limited to GW searches. The Doppler tracking technique discussed here could be performed at minimal incremental cost to improve also other radio science experiments (i.e., tests of relativistic gravity, planetary and satellite gravity field measurements, atmospheric and ring occultations) on future interplanetary missions.

  8. News Conference: Brecon hosts 10th teacher's conference Summer school: Science summer school heads to Crete Award: The Corti Science Prize Radioactivity: Scottish beach is no beta off Workshop: Heureka project promotes teaching Experiments: Spanish project proves that learning science can be exciting Lecture: IOP schools lecture journeys from x-rays to antimatter Correction to the news item 'Delegates experience universality' Forthcoming events

    NASA Astrophysics Data System (ADS)

    2012-01-01

    Conference: Brecon hosts 10th teacher's conference Summer school: Science summer school heads to Crete Award: The Corti Science Prize Radioactivity: Scottish beach is no beta off Workshop: Heureka project promotes teaching Experiments: Spanish project proves that learning science can be exciting Lecture: IOP schools lecture journeys from x-rays to antimatter Correction to the news item 'Delegates experience universality' Forthcoming events

  9. NSSDC Conference on Mass Storage Systems and Technologies for Space and Earth Science Applications, volume 2

    NASA Technical Reports Server (NTRS)

    Kobler, Ben (Editor); Hariharan, P. C. (Editor); Blasso, L. G. (Editor)

    1992-01-01

    This report contains copies of nearly all of the technical papers and viewgraphs presented at the NSSDC Conference on Mass Storage Systems and Technologies for Space and Earth Science Application. This conference served as a broad forum for the discussion of a number of important issues in the field of mass storage systems. Topics include the following: magnetic disk and tape technologies; optical disk and tape; software storage and file management systems; and experiences with the use of a large, distributed storage system. The technical presentations describe, among other things, integrated mass storage systems that are expected to be available commercially. Also included is a series of presentations from Federal Government organizations and research institutions covering their mass storage requirements for the 1990's.

  10. PREFACE: IC-MSQUARE 2012: International Conference on Mathematical Modelling in Physical Sciences

    NASA Astrophysics Data System (ADS)

    Kosmas, Theocharis; Vagenas, Elias; Vlachos, Dimitrios

    2013-02-01

    The first International Conference on Mathematical Modelling in Physical Sciences (IC-MSQUARE) took place in Budapest, Hungary, from Monday 3 to Friday 7 September 2012. The conference was attended by more than 130 participants, and hosted about 290 oral, poster and virtual papers by more than 460 pre-registered authors. The first IC-MSQUARE consisted of different and diverging workshops and thus covered various research fields in which mathematical modelling is used, such as theoretical/mathematical physics, neutrino physics, non-integrable systems, dynamical systems, computational nanoscience, biological physics, computational biomechanics, complex networks, stochastic modelling, fractional statistics, DNA dynamics, and macroeconomics. The scientific program was rather heavy since after the Keynote and Invited Talks in the morning, two parallel sessions ran every day. However, according to all attendees, the program was excellent with a high level of talks and the scientific environment was fruitful; thus all attendees had a creative time. The mounting question is whether this occurred accidentally, or whether IC-MSQUARE is a necessity in the field of physical and mathematical modelling. For all of us working in the field, the existing and established conferences in this particular field suffer from two distinguished and recognized drawbacks: the first is the increasing orientation, while the second refers to the extreme specialization of the meetings. Therefore, a conference which aims to promote the knowledge and development of high-quality research in mathematical fields concerned with applications of other scientific fields as well as modern technological trends in physics, chemistry, biology, medicine, economics, sociology, environmental sciences etc., appears to be a necessity. This is the key role that IC-MSQUARE will play. We would like to thank the Keynote Speaker and the Invited Speakers for their significant contributions to IC-MSQUARE. We would also

  11. Information in the Language Sciences: Proceedings of the Conference Held at Warrenton, Virginia, March 4-6, 1966.

    ERIC Educational Resources Information Center

    Freeman, Robert R., Ed.; And Others

    This collection of 22 papers from the Conference on Information in the Language Sciences held in Warrenton, Va., in 1966, sponsored by the Center for Applied Linguistics, stresses three themes: general trends, information needs of the languages sciences, and system design. Discussions attempt to formulate modern rational approaches to the complex…

  12. Presented Papers of the European Division Mathematics & Science Conference (1st, Heidelberg, West Germany, February 28-March 2, 1986).

    ERIC Educational Resources Information Center

    Maryland Univ., College Park. Univ. Coll.

    This document contains the papers presented at a conference designed to provide a forum to discuss the European Division mathematics and science program and to allow an opportunity for professional development. Papers on approaches to teaching specific topics in the Maryland mathematics and science curriculum, as well as on other aspects of…

  13. 75 FR 2552 - NIH State-of-the-Science Conference: Enhancing Use and Quality of Colorectal Cancer Screening

    Federal Register 2010, 2011, 2012, 2013, 2014

    2010-01-15

    ... From the Federal Register Online via the Government Publishing Office DEPARTMENT OF HEALTH AND HUMAN SERVICES National Institutes of Health NIH State-of-the-Science Conference: Enhancing Use and Quality of Colorectal Cancer Screening Notice is hereby given by the National Institutes of Health (NIH) of the ``NIH State-of-the-Science...

  14. Developing Talent in Mathematics, Science and Technology: A Conference on Academic Talent (Durham, North Carolina, March 28-30, 1988).

    ERIC Educational Resources Information Center

    Dreyden, Julia I., Ed.; And Others

    An introductory chapter, "Contemporary Issues in Gifted Education" by Julia Dreyden and Shelagh Gallagher, summarizes National Science Foundation policy concerning development of new science and mathematics curricula and the work of the Talent Identification Program. Major conference papers and responses are then presented: "Developing Academic…

  15. First Rosetta Radio Science Bistatic Radar Observations of 67P/Churyumov-Gerasimenko

    NASA Astrophysics Data System (ADS)

    Andert, Thomas P.; Remus, Stefan; Simpson, Richard A.; Pätzold, Martin; Asmar, Sami W.; Kahan, Daniel S.; Bird, Mike K.; Häusler, Bernd; Tellmann, Silvia

    2015-04-01

    The Rosetta spacecraft was successfully inserted on 6th August 2014 into orbit around comet 67P/Churyumov-Gerasimenko. In September Rosetta was placed into bound orbits with an initial distance of 30 km and a decreasing distance until the end October. After lander delivery, bound orbits were maintained again at 20 km and 30 km. One of the objectives of the Rosetta Radio Science Investigations (RSI) is to address the dielectric properties, small-scale roughness, and rotational state of the nucleus of the comet, which can be determined by means of a surface scattering experiment, also known as Bistatic Radar. The radio subsystem transmitter located on board the Rosetta spacecraft beams right circularly polarized radio signals at two wavelengths -3.6 cm (X-Band) and 13 cm (S-Band) - toward the nucleus surface. Part of the impinging radiation is then scattered toward a receiver at a ground station on Earth and recorded. On September 29th, 2014 the first Bistatic Radar experiment ever at a comet was successfully conducted. The distance between 67P/Churyumov-Gerasimenko and Rosetta was 20 km and both right circularly polarized (RCP) and left circularly polarized (LCP) reflected signals from the comet's surface in X-Band were detected during the experiment at the Goldstone complex of the NASA Deep Space Network. The ultra-stable oscillator (USO) on board Rosetta served during the experiment as a very stable reference frequency source. The direct and reflected signal were separated during the experiment by only a fraction of 1 Hz. The extreme stability of the USO allowed a detection and separation of the weak signals even on the required long integration times. Five additional Bistatic Radar experiments were conducted successfully between mid-October and mid-December 2014 with the 70-m DSN ground stations in Goldstone and Canberra at different distances to the comet (10 km, 20 km and 30 km) and reflected signals were observed in each case.

  16. 4th Annual Conference for African-American Researchers in the Mathematical Sciences (CAARMS4). Preliminary Program

    SciTech Connect

    Tapia, Richard

    1998-06-01

    In June, The Center for Research on Parallel Computation (CRPC), an NSF-funded Science and Technology Center, hosted the 4th Annual Conference for African-American Reserachers in the Mathematical Sciences (CAARMS4) at Rice University. The main goal of this conference was to highlight current work by African-American researchers and graduate students in mathematics. This conference strengthened the mathematical sciences by encouraging the increased participation of African-American and underrepresented groups into the field, facilitating working relationships between them and helping to cultivate their careers. In addition to the talks there was a graduate student poster session and tutorials on topics in mathematics and computer science. These talks, presentations, and discussions brought a broader perspective to the critical issues involving minority participation in mathematics.

  17. Science and Technology in Asian Development. Conference on the Application of Science and Technology to the Development of Asia (New Delhi, India, August, 1968).

    ERIC Educational Resources Information Center

    United Nations Educational, Scientific, and Cultural Organization, Paris (France).

    The conclusions reached by commissions established by the Conference on the Application of Science and Technology to the Development of Asia, convened by UNESCO in 1968, are presented after brief descriptions of the present status of applied science and technology in 19 Asian countries. One commission studied social, economic, and cultural factors…

  18. Mars Express 10 years at Mars: Observations by the Mars Express Radio Science Experiment (MaRS)

    NASA Astrophysics Data System (ADS)

    Pätzold, M.; Häusler, B.; Tyler, G. L.; Andert, T.; Asmar, S. W.; Bird, M. K.; Dehant, V.; Hinson, D. P.; Rosenblatt, P.; Simpson, R. A.; Tellmann, S.; Withers, P.; Beuthe, M.; Efimov, A. I.; Hahn, M.; Kahan, D.; Le Maistre, S.; Oschlisniok, J.; Peter, K.; Remus, S.

    2016-08-01

    The Mars Express spacecraft is operating in Mars orbit since early 2004. The Mars Express Radio Science Experiment (MaRS) employs the spacecraft and ground station radio systems (i) to conduct radio occultations of the atmosphere and ionosphere to obtain vertical profiles of temperature, pressure, neutral number densities and electron density, (ii) to conduct bistatic radar experiments to obtain information on the dielectric and scattering properties of the surface, (iii) to investigate the structure and variation of the crust and lithosphere in selected target areas, (iv) to determine the mass, bulk and internal structure of the moon Phobos, and (v) to track the MEX radio signals during superior solar conjunction to study the morphology of coronal mass ejections (CMEs). Here we report observations, results and discoveries made in the Mars environment between 2004 and 2014 over almost an entire solar cycle.

  19. Testing General Relativity with the Radio Science Experiment of the BepiColombo mission to Mercury

    NASA Astrophysics Data System (ADS)

    Schettino, Giulia; Tommei, Giacomo

    2016-09-01

    The relativity experiment is part of the Mercury Orbiter Radio science Experiment (MORE) on-board the ESA/JAXA BepiColombo mission to Mercury. Thanks to very precise radio tracking from the Earth and accelerometer, it will be possible to perform an accurate test of General Relativity, by constraining a number of post-Newtonian and related parameters with an unprecedented level of accuracy. The Celestial Mechanics Group of the University of Pisa developed a new dedicated software, ORBIT14, to perform the simulations and to determine simultaneously all the parameters of interest within a global least squares fit. After highlighting some critical issues, we report on the results of a full set of simulations, carried out in the most up-to-date mission scenario. For each parameter we discuss the achievable accuracy, in terms of a formal analysis through the covariance matrix and, furthermore, by the introduction of an alternative, more representative, estimation of the errors. We show that, for example, an accuracy of some parts in 10^-6 for the Eddington parameter β and of 10^-5 for the Nordtvedt parameter η can be attained, while accuracies at the level of 5×10^-7 and 1×10^-7 can be achieved for the preferred frames parameters α1 and α2, respectively.

  20. Radio science ground data system for the Voyager-Neptune encounter, part 1

    NASA Technical Reports Server (NTRS)

    Kursinski, E. R.; Asmar, S. W.

    1991-01-01

    The Voyager radio science experiments at Neptune required the creation of a ground data system array that includes a Deep Space Network complex, the Parkes Radio Observatory, and the Usuda deep space tracking station. The performance requirements were based on experience with the previous Voyager encounters, as well as the scientific goals at Neptune. The requirements were stricter than those of the Uranus encounter because of the need to avoid the phase-stability problems experienced during that encounter and because the spacecraft flyby was faster and closer to the planet than previous encounters. The primary requirement on the instrument was to recover the phase and amplitude of the S- and X-band (2.3 and 8.4 GHz) signals under the dynamic conditions encountered during the occultations. The primary receiver type for the measurements was open loop with high phase-noise and frequency stability performance. The receiver filter bandwidth was predetermined based on the spacecraft's trajectory and frequency uncertainties.

  1. ALMA Science Verification Data: Millimeter Continuum Polarimetry of the Bright Radio Quasar 3C 286

    NASA Astrophysics Data System (ADS)

    Nagai, H.; Nakanishi, K.; Paladino, R.; Hull, C. L. H.; Cortes, P.; Moellenbrock, G.; Fomalont, E.; Asada, K.; Hada, K.

    2016-06-01

    We present full-polarization observations of the compact, steep-spectrum radio quasar 3C 286 made with the Atacama Large Millimeter and Submillimeter Array (ALMA) at 1.3 mm. These are the first full-polarization ALMA observations, which were obtained in the framework of Science Verification. A bright core and a south-west component are detected in the total intensity image, similar to previous centimeter images. Polarized emission is also detected toward both components. The fractional polarization of the core is about 17%; this is higher than the fractional polarization at centimeter wavelengths, suggesting that the magnetic field is even more ordered in the millimeter radio core than it is further downstream in the jet. The observed polarization position angle (or electric vector position angle (EVPA)) in the core is ˜39◦, which confirms the trend that the EVPA slowly increases from centimeter to millimeter wavelengths. With the aid of multi-frequency VLBI observations, we argue that this EVPA change is associated with the frequency-dependent core position. We also report a serendipitous detection of a sub-mJy source in the field of view, which is likely to be a submillimeter galaxy.

  2. Global Navigation Satellite System Radio Occultation: Processing Algorithms, Science Applications, and COSMIC-2 Mission Status

    NASA Astrophysics Data System (ADS)

    Schreiner, W. S.; Sokolovskiy, S. V.; Kuo, Y. H.; Weiss, J.; Braun, J.; Hunt, D.; Pedatella, N. M.; Yue, X.; Ho, S. P.; Zeng, Z.; Wee, T. K.; Vanhove, T.

    2015-12-01

    Global Navigation Satellite System (GNSS) Radio Occultation (RO) data are becoming a benchmark dataset of the international global observing system. The high vertical resolution, precision, and accuracy of retrieved atmospheric profiles makes GNSS RO ideal for weather and space weather specification and forecasting, climate change research and detection, and ground-based and satellite instrument validation. With a GNSS receiver on board a low-Earth orbiting (LEO) satellite, the amplitude and phase of the radio frequency (RF) signals transmitted from GNSS satellites can be measured very precisely as the ray tangent point descends from ~100 km altitude to the surface. With proper algorithms and observational modeling, vertical profiles of bending angle are derived. Profiles of refractivity, and subsequently pressure, temperature and humidity can be derived with additional a priori information. This presentation will first provide an overview of GNSS RO data processing algorithms and then present recent research results from challenging regions such as the upper stratosphere and the lower troposphere. Additional research results from science application studies using RO data will also be discussed. Finally, a status update of the COSMIC-2 mission due to launch in Sept 2016 will be presented.

  3. ALMA Science Verification Data: Millimeter Continuum Polarimetry of the Bright Radio Quasar 3C 286

    NASA Astrophysics Data System (ADS)

    Nagai, H.; Nakanishi, K.; Paladino, R.; Hull, C. L. H.; Cortes, P.; Moellenbrock, G.; Fomalont, E.; Asada, K.; Hada, K.

    2016-06-01

    We present full-polarization observations of the compact, steep-spectrum radio quasar 3C 286 made with the Atacama Large Millimeter and Submillimeter Array (ALMA) at 1.3 mm. These are the first full-polarization ALMA observations, which were obtained in the framework of Science Verification. A bright core and a south–west component are detected in the total intensity image, similar to previous centimeter images. Polarized emission is also detected toward both components. The fractional polarization of the core is about 17%; this is higher than the fractional polarization at centimeter wavelengths, suggesting that the magnetic field is even more ordered in the millimeter radio core than it is further downstream in the jet. The observed polarization position angle (or electric vector position angle (EVPA)) in the core is ˜39◦, which confirms the trend that the EVPA slowly increases from centimeter to millimeter wavelengths. With the aid of multi-frequency VLBI observations, we argue that this EVPA change is associated with the frequency-dependent core position. We also report a serendipitous detection of a sub-mJy source in the field of view, which is likely to be a submillimeter galaxy.

  4. Mars Global Surveyor Radio Science Electron Density Profiles: Interannual Variability and Implications for the Neutral Atmosphere

    NASA Technical Reports Server (NTRS)

    Bougher, S. W.; Engel, S.; Hinson, D. P.; Murphy, J. R.

    2003-01-01

    The Mars Global Surveyor (MGS) Radio Science (RS) experiment employs an ultrastable oscillator aboard the spacecraft. The signal from the oscillator to Earth is refracted by the Martian ionosphere, allowing retrieval of electron density profiles versus radius and geopotential. The present analysis is carried out on five sets of occultation measurements: (1) four obtained near northern summer solstice (Ls = 74-116, near aphelion) at high northern latitudes (64.7-77.6N), and (2) one set of profiles approaching equinox conditions (Ls = 135- 146) at high southern latitudes (64.7-69.1S). Electron density profiles (95 to 200 km) are examined over a narrow range of solar zenith angles (76.5-86.9 degrees) for local true solar times of (1) 3-4 hours and (2) 12.1 hours. Variations spanning 1-Martian year are specifically examined in the Northern hemisphere.

  5. Italian Spring Accelerometer (ISA): A fundamental support to BepiColombo Radio Science Experiments

    NASA Astrophysics Data System (ADS)

    Iafolla, V.; Fiorenza, E.; Lefevre, C.; Morbidini, A.; Nozzoli, S.; Peron, R.; Persichini, M.; Reale, A.; Santoli, F.

    2010-01-01

    The Radio Science Experiments of the BepiColombo mission will enable substantial improvement of the knowledge of Mercury's orbit and rotation, and the relativistic dynamics in the solar system. A fundamental support to the spacecraft tracking data will be given by the Italian Spring Accelerometer (ISA). This is a three-axis accelerometer devoted to the measurement of the non-gravitational perturbations acting on the Mercury Planetary Orbiter (MPO), whose knowledge is important in order to fully exploit the quality of the tracking data. The intrinsic noise level of the instrument that will be onboard MPO, 10-9m/s2/√{Hz} in the 3×10-5 to 10-1Hz frequency range, guarantees the fulfilment of the RSE requirements. The main scientific and technological features of the instrument are discussed, together with its current error budget, experimental activities and foreseen calibration strategies.

  6. Surface Science Laboratory for Studying the Surfaces of Superconducting Radio Frequency Cavities

    SciTech Connect

    Andy Wu

    2003-09-01

    A Surface Science Laboratory (SSL) has been established at JLab to study surfaces relevant to superconducting radio frequency (SRF) cavities. Current operational facilities include a scanning electron microscope equipped with energy dispersive x-ray analysis, a secondary ion mass spectrometry, a metallographic optical microscope, a transmission electron microscope, a high precision and large scan area 3-D profilometer, a scanning field emission microscope, and a fully equipped sample preparation room. A scanning Auger microscope is being commissioned, and will be available for routine usage soon. Results from typical examples of the R&D projects on SRF cavities that were supported in the past through the use of the facilities in the SSL will be briefly reported.

  7. Precise radio Doppler and interferometric tracking of spacecraft in service of planetary science

    NASA Astrophysics Data System (ADS)

    Duev, Dmitry; PRIDE team

    2016-10-01

    The Planetary Radio Interferometry and Doppler Experiments (PRIDE) project is designed as a multi-purpose, multidisciplinary enhancement of the space missions science return by means of Doppler and phase-referenced Very Long Baseline Interferometry (VLBI) tracking of spacecraft. These measurements can be used in a multitude of scientific applications, both fundamental and applied, where an accurate estimate of the spacecraft state vector is essential. In particular, the gravitational field of planetary moons can be sampled with close spacecraft flybys, allowing to probe the moons' interior.In this presentation, we will describe the principles of PRIDE data collection, processing, and analysis. We will present the results of demonstrational observations of a Phobos flyby conducted by ESA's Mars Express spacecraft.

  8. The Weather Guys - Discussing Science via regular Radio and Newspaper Appearances

    NASA Astrophysics Data System (ADS)

    Ackerman, S. A.; Martin, J. E.

    2013-12-01

    The University of Wisconsin has described the value of outreach through its Wisconsin Idea. Simply put it states that the boundaries of the university are the boundaries of the state. In addition to their research, teaching, and administration duties, they have routinely reached out to share their science with various public groups. Since 1998, Profs Jon Martin and Steve Ackerman, have be regular quests on the Larry Meiller show on Wisconsin Public Radio IDEAS Network. The format of the show is a live call-in show. They air as guests the last Monday of every month. The show is also web-cast live (http://www.wpr.org/), enabling questions to be called in on phone or sent via email. Archives can be found at http://www.wpr.org/webcasting/audioarchives_display.cfm?Code=mlr In 2008 they were asked to do a Q&A column for the regional Madison paper: The Wisconsin State Journal (WSJ). This is a weekly column that addresses readers questions in about 250 words. Example columns can be found in the WSJ e-book: http://www.amazon.com/Ask-Weather-Guys-2010-ebook/dp/B00AY4VMZE These two activities have earned them the nickname The Weather Guys, resulting in various speaking invitations including master gardener clubs and a Science Pub sponsored by Nova. Overall, these activities have been beneficial to our careers, earning name recognition across the University and throughout the state. They also provide learning opportunities for us through experiences described by the public. We will discuss our motivation and experiences in doing this live show and the weekly column, presenting personal stories of successful and less-successful communication attempts. A nearly complete archive exists or the live radio show and we will present an analysis of the type of questions asked and the more common, and less common, topics. The Weather Guys, an image developed by and for the Why?Files (http://whyfiles.org

  9. PREFACE: The fifth International Conference on Inertial Fusion Sciences and Applications (IFSA2007)

    NASA Astrophysics Data System (ADS)

    Azechi, Hiroshi; Hammel, Bruce; Gauthier, Jean-Claude

    2008-06-01

    The Fifth International Conference on Inertial Fusion Sciences and Applications (IFSA 2007) was held on 9-14 September 2007 at Kobe International Conference Center in Kobe, Japan. The host organizations for this conference were Osaka University and the Institute of Laser Engineering (ILE) at Osaka University; and co-organized by the Institute Lasers and Plasmas (ILP) in France, the Commissariatá l'Energie Atomique (CEA), Lawrence Livermore National Laboratory (LLNL), National Institute for Fusion Science (NIFS) in Japan, and Kansai Photon Science Institute (KPSI), Japan Atomic Energy Agency (JAEA). The conference objective was to review the state of the art of research in inertial fusion sciences and applications since the last conference held in Biarritz, France, in 2005. 470 abstracts were accepted, and 448 persons from 18 countries attended the conference. These Proceedings contain 287 of the papers presented at IFSA 2007. This collection of papers represents the manuscripts submitted to and passing the peer review process. The program was organized with some specific features: The reviews of influential programs appeared both at the very beginning and at the very end of the Conference to attract attendance throughout the Conference. Each poster session had the same time period as a single oral session, thereby avoiding overlap with oral talks. The everyday program was structured to be as similar as possible so the attendees could easily recognize the program. With a goal of achieving inertial fusion ignition and burn propagation in the laboratory, researchers presented the exciting advances in both traditional hot spot ignition and fast ignition approach, including status report of USA's National Ignition Facility (NIF), French Laser Magajoule (LMJ), Japanese Fast Ignition Realization Experiment (FIREX), and European High Power laser Energy Research (HiPER). A particular emphasis of the meeting was that the `physics of inertial fusion' category was dominated

  10. Phenylketonuria Scientific Review Conference: state of the science and future research needs.

    PubMed

    Camp, Kathryn M; Parisi, Melissa A; Acosta, Phyllis B; Berry, Gerard T; Bilder, Deborah A; Blau, Nenad; Bodamer, Olaf A; Brosco, Jeffrey P; Brown, Christine S; Burlina, Alberto B; Burton, Barbara K; Chang, Christine S; Coates, Paul M; Cunningham, Amy C; Dobrowolski, Steven F; Ferguson, John H; Franklin, Thomas D; Frazier, Dianne M; Grange, Dorothy K; Greene, Carol L; Groft, Stephen C; Harding, Cary O; Howell, R Rodney; Huntington, Kathleen L; Hyatt-Knorr, Henrietta D; Jevaji, Indira P; Levy, Harvey L; Lichter-Konecki, Uta; Lindegren, Mary Lou; Lloyd-Puryear, Michele A; Matalon, Kimberlee; MacDonald, Anita; McPheeters, Melissa L; Mitchell, John J; Mofidi, Shideh; Moseley, Kathryn D; Mueller, Christine M; Mulberg, Andrew E; Nerurkar, Lata S; Ogata, Beth N; Pariser, Anne R; Prasad, Suyash; Pridjian, Gabriella; Rasmussen, Sonja A; Reddy, Uma M; Rohr, Frances J; Singh, Rani H; Sirrs, Sandra M; Stremer, Stephanie E; Tagle, Danilo A; Thompson, Susan M; Urv, Tiina K; Utz, Jeanine R; van Spronsen, Francjan; Vockley, Jerry; Waisbren, Susan E; Weglicki, Linda S; White, Desirée A; Whitley, Chester B; Wilfond, Benjamin S; Yannicelli, Steven; Young, Justin M

    2014-06-01

    New developments in the treatment and management of phenylketonuria (PKU) as well as advances in molecular testing have emerged since the National Institutes of Health 2000 PKU Consensus Statement was released. An NIH State-of-the-Science Conference was convened in 2012 to address new findings, particularly the use of the medication sapropterin to treat some individuals with PKU, and to develop a research agenda. Prior to the 2012 conference, five working groups of experts and public members met over a 1-year period. The working groups addressed the following: long-term outcomes and management across the lifespan; PKU and pregnancy; diet control and management; pharmacologic interventions; and molecular testing, new technologies, and epidemiologic considerations. In a parallel and independent activity, an Evidence-based Practice Center supported by the Agency for Healthcare Research and Quality conducted a systematic review of adjuvant treatments for PKU; its conclusions were presented at the conference. The conference included the findings of the working groups, panel discussions from industry and international perspectives, and presentations on topics such as emerging treatments for PKU, transitioning to adult care, and the U.S. Food and Drug Administration regulatory perspective. Over 85 experts participated in the conference through information gathering and/or as presenters during the conference, and they reached several important conclusions. The most serious neurological impairments in PKU are preventable with current dietary treatment approaches. However, a variety of more subtle physical, cognitive, and behavioral consequences of even well-controlled PKU are now recognized. The best outcomes in maternal PKU occur when blood phenylalanine (Phe) concentrations are maintained between 120 and 360 μmol/L before and during pregnancy. The dietary management treatment goal for individuals with PKU is a blood Phe concentration between 120 and 360 μmol/L. The use

  11. Phenylketonuria Scientific Review Conference: state of the science and future research needs.

    PubMed

    Camp, Kathryn M; Parisi, Melissa A; Acosta, Phyllis B; Berry, Gerard T; Bilder, Deborah A; Blau, Nenad; Bodamer, Olaf A; Brosco, Jeffrey P; Brown, Christine S; Burlina, Alberto B; Burton, Barbara K; Chang, Christine S; Coates, Paul M; Cunningham, Amy C; Dobrowolski, Steven F; Ferguson, John H; Franklin, Thomas D; Frazier, Dianne M; Grange, Dorothy K; Greene, Carol L; Groft, Stephen C; Harding, Cary O; Howell, R Rodney; Huntington, Kathleen L; Hyatt-Knorr, Henrietta D; Jevaji, Indira P; Levy, Harvey L; Lichter-Konecki, Uta; Lindegren, Mary Lou; Lloyd-Puryear, Michele A; Matalon, Kimberlee; MacDonald, Anita; McPheeters, Melissa L; Mitchell, John J; Mofidi, Shideh; Moseley, Kathryn D; Mueller, Christine M; Mulberg, Andrew E; Nerurkar, Lata S; Ogata, Beth N; Pariser, Anne R; Prasad, Suyash; Pridjian, Gabriella; Rasmussen, Sonja A; Reddy, Uma M; Rohr, Frances J; Singh, Rani H; Sirrs, Sandra M; Stremer, Stephanie E; Tagle, Danilo A; Thompson, Susan M; Urv, Tiina K; Utz, Jeanine R; van Spronsen, Francjan; Vockley, Jerry; Waisbren, Susan E; Weglicki, Linda S; White, Desirée A; Whitley, Chester B; Wilfond, Benjamin S; Yannicelli, Steven; Young, Justin M

    2014-06-01

    New developments in the treatment and management of phenylketonuria (PKU) as well as advances in molecular testing have emerged since the National Institutes of Health 2000 PKU Consensus Statement was released. An NIH State-of-the-Science Conference was convened in 2012 to address new findings, particularly the use of the medication sapropterin to treat some individuals with PKU, and to develop a research agenda. Prior to the 2012 conference, five working groups of experts and public members met over a 1-year period. The working groups addressed the following: long-term outcomes and management across the lifespan; PKU and pregnancy; diet control and management; pharmacologic interventions; and molecular testing, new technologies, and epidemiologic considerations. In a parallel and independent activity, an Evidence-based Practice Center supported by the Agency for Healthcare Research and Quality conducted a systematic review of adjuvant treatments for PKU; its conclusions were presented at the conference. The conference included the findings of the working groups, panel discussions from industry and international perspectives, and presentations on topics such as emerging treatments for PKU, transitioning to adult care, and the U.S. Food and Drug Administration regulatory perspective. Over 85 experts participated in the conference through information gathering and/or as presenters during the conference, and they reached several important conclusions. The most serious neurological impairments in PKU are preventable with current dietary treatment approaches. However, a variety of more subtle physical, cognitive, and behavioral consequences of even well-controlled PKU are now recognized. The best outcomes in maternal PKU occur when blood phenylalanine (Phe) concentrations are maintained between 120 and 360 μmol/L before and during pregnancy. The dietary management treatment goal for individuals with PKU is a blood Phe concentration between 120 and 360 μmol/L. The use

  12. Mars' gravity field and upper atmosphere with MGS, Mars Odyssey, and MRO radio science data

    NASA Astrophysics Data System (ADS)

    Genova, Antonio; Goossens, Sander J.; Lemoine, Frank G.; Mazarico, Erwan; Smith, David E.; Zuber, Maria T.

    2015-04-01

    The Mars exploration program conducted by NASA during the last decade has enabled continuous observations of the planet from orbit with three different missions: the Mars Global Surveyor (MGS), Mars Odyssey (ODY), and the Mars Reconnaissance Orbiter (MRO). These spacecraft were equipped with on board instrumentation dedicated to collect radio tracking data in the X-band. The analysis of these data has provided a high-resolution gravity field model of Mars. MGS and ODY were inserted into two separate frozen sun-synchronous, near-circular, polar orbits with different local times, with their periapsis altitude at ~370 km and ~390 km, respectively. MGS was in orbit around Mars between 1999 and 2006, whereas ODY has been orbiting the planet since January 2002. Using the radio science data of these two spacecraft, gravity models with a maximum resolution of degree and order 95 in spherical harmonics (spatial resolution of 112 km) have been determined. MRO has been orbiting Mars since August 2006 in a frozen sun-synchronous orbit with a periapsis at 255 km altitude. Therefore, its radio data helped significantly improve Mars' gravity field model, up to degree and order 110 (spatial resolution of 96 km). However, mismodeling of the atmospheric drag, which is the strongest non-conservative force acting on the spacecraft at MRO's low altitude, compromises the estimation of the temporal variations of the gravity field zonal harmonics that provide crucial information on the seasonal mass of carbon dioxide in the polar caps. For this reason, we implemented the Drag Temperature Model (DTM)-Mars model (Bruinsma and Lemoine 2002) into our Precise Orbit Determination (POD) program GEODYN-II. We estimated key model parameters to adequately reproduce variations in temperatures and (partial) density along the spacecraft trajectories. Our new model allows us to directly estimate the long-term periodicity of the major constituents at MGS, ODY, and MRO altitudes (~255-450 km). In this

  13. PARTICIPANT SUPPORT FOR THE 2010 GORDON RESEARCH CONFERENCE ON PLASMA PROCESSING SCIENCE (JULY 11-16,2010)

    SciTech Connect

    Uwe Kortshagen

    2011-06-14

    The 2010 Gordon Research Conference on Plasma Processing Science will feature a comprehensive program that will highlight the most cutting edge scientific advances in low temperature plasma science and will explore the applications of low temperature plasma technology relative to many grand societal challenges. Fundamental science sessions will focus on plasma kinetics, plasma surface interactions, and recent trends in plasma generation and multi-phase plasmas. Application sessions will explore the impact of plasma technology in renewable energy and the production of fuels from renewable feedstocks, plasma-enabled medicine and sterilization, and environmental remediation and waste treatment. The conference will bring together in an informal atmosphere leaders in the field with junior investigators and graduate students. The special format of the Gordon Conferences, with programmed discussion sessions and ample time for informal gatherings in the afternoons and evenings, will provide for a fertile atmosphere of brainstorming and creative thinking among the attendees.

  14. Ike 101: The Dwight D. Eisenhower Program for Mathematics and Science Education National Conference (Arlington, Virginia, November 17-22, 1991).

    ERIC Educational Resources Information Center

    Triangle Coalition for Science and Technology Education, College Park, MD.

    A conference was held to discuss educational issues related to mathematics and science education. This document reports the proceedings of the conference by summarizing the comments of several of the conference speakers. The speakers and topics discussed included: (1) Senator Mark Hatfield and Congressman Thomas Sawyer on the perspective of…

  15. The Red Radio Ring: a gravitationally lensed hyperluminous infrared radio galaxy at z = 2.553 discovered through the citizen science project SPACE WARPS

    NASA Astrophysics Data System (ADS)

    Geach, J. E.; More, A.; Verma, A.; Marshall, P. J.; Jackson, N.; Belles, P.-E.; Beswick, R.; Baeten, E.; Chavez, M.; Cornen, C.; Cox, B. E.; Erben, T.; Erickson, N. J.; Garrington, S.; Harrison, P. A.; Harrington, K.; Hughes, D. H.; Ivison, R. J.; Jordan, C.; Lin, Y.-T.; Leauthaud, A.; Lintott, C.; Lynn, S.; Kapadia, A.; Kneib, J.-P.; Macmillan, C.; Makler, M.; Miller, G.; Montaña, A.; Mujica, R.; Muxlow, T.; Narayanan, G.; O'Briain, D.; O'Brien, T.; Oguri, M.; Paget, E.; Parrish, M.; Ross, N. P.; Rozo, E.; Rusu, Cristian E.; Rykoff, E. S.; Sanchez-Argüelles, D.; Simpson, R.; Snyder, C.; Schloerb, F. P.; Tecza, M.; Wang, W.-H.; Van Waerbeke, L.; Wilcox, J.; Viero, M.; Wilson, G. W.; Yun, M. S.; Zeballos, M.

    2015-09-01

    We report the discovery of a gravitationally lensed hyperluminous infrared galaxy (intrinsic LIR ≈ 1013 L⊙) with strong radio emission (intrinsic L1.4 GHz ≈ 1025 W Hz-1) at z = 2.553. The source was identified in the citizen science project SPACE WARPS through the visual inspection of tens of thousands of iJKs colour composite images of luminous red galaxies (LRGs), groups and clusters of galaxies and quasars. Appearing as a partial Einstein ring (re ≈ 3 arcsec) around an LRG at z = 0.2, the galaxy is extremely bright in the sub-millimetre for a cosmological source, with the thermal dust emission approaching 1 Jy at peak. The redshift of the lensed galaxy is determined through the detection of the CO(3→2) molecular emission line with the Large Millimetre Telescope's Redshift Search Receiver and through [O III] and Hα line detections in the near-infrared from Subaru/Infrared Camera and Spectrograph. We have resolved the radio emission with high-resolution (300-400 mas) eMERLIN L-band and Very Large Array C-band imaging. These observations are used in combination with the near-infrared imaging to construct a lens model, which indicates a lensing magnification of μ ≈ 10. The source reconstruction appears to support a radio morphology comprised of a compact (<250 pc) core and more extended component, perhaps indicative of an active nucleus and jet or lobe.

  16. A Rooftop Radio Observatory: A New Method for Teaching Science Fundamentals to Advanced Undergraduates

    NASA Astrophysics Data System (ADS)

    Frank, C.; Cudaback, D.; Heiles, C.; Treffers, R.; Hancox, C.; Millan, R.; Parthasarathy, R.

    1996-05-01

    This paper reports on an innovative teaching style for the instruction of advanced undergraduates in experimental science fundamentals. Working under the belief that a complete education includes both theoretical work and ``hands-on'' laboratory experience, a radio observatory has been created on top of the U. C. Berkeley Astronomy Department building. Class work with this observatory give students an understanding of: (1) components of a radio telescope system, (2) system operation and trouble-shooting, (3) observation strategies, (4) data collection and reduction, and (5) presentation and visualization of results. Our antenna consists of a two meter tall pyramidal horn optimized to observe the 21 cm atomic hydrogen transition. The receiver consists of a double-heterodyning system with a PC to sample and Fourier transform the signal and generate a power spectrum. System components were constructed by students with guidance from faculty members. Students using this system obtain power spectra representing the Doppler shifted HI line, as a function of galactic coordinate. Students derive results including basic galactic structure and rotation and mass curves. Further technical information is presented in the accompanying poster paper. Close contact between students and equipment is essential for successful comprehension of fundamental concepts. The system is constructed such that most components can be individually examined or assembled on a bench-top in a configuration the student wishes to explore. We believe that systems which perform real astronomy can be duplicated by other universities. The small scale of the antenna as well as the strength of the HI line require a small allocation of resources to implement an observation system. The ``hands-on'' approach compliments theoretical course work, in addition to providing practical experience for students who may not be inclined towards graduate school. Finally, this educational technique is exportable and

  17. Observations of Mars Neutral Atmosphere during the Polar Night by the Mars Express Radio Science Experiment

    NASA Astrophysics Data System (ADS)

    Tyler, G. L.; Pätzold, M.; Tellmann, S.; Häusler, B.; Hinson, D. P.

    2006-09-01

    The Radio Science Experiment on Mars Express (MaRS) sounds the Martian atmophere and ionosphere making use of spacecraft radio signals at 3.6 and 13 cm-wavelength and an Earth-Mars occultation geometry. Vertical profiles of pressure, temperature, and density in the neutral atmosphere are obtained with an altitude resolution of only a few hundred meters. The elliptical orbit of Mars Express permits examination of a large range of local times and locations and therefore can be used to investigate latitudinal, diurnal, and seasonal variations of Mars atmosphere. Daytime atmospheric profiles collected from both hemispheres since March 2004 allow us to study the development of the atmosphere in the early morning and the polar night. The second occultation season, December 2004, produced 32 profiles located in the southern polar latitudes at an average solar longitude of about 130°. Approximately 30 profiles obtained during the fourth occultation season, July 2005-April 2006, provide data on the north polar region at latitudes above 70° and a solar longitude of about 271°. The polar night at 75° north shows a 142-145 K isothermal atmosphere up to an altitude of 40 km, which is at or close to the condensation line of CO2. A similar behavior is observed during the southern polar night at 80° south, but with a significant warming at longitudes passing through Hellas. Model calculations of a Martian General Circulation Model (GCM) developed by the Laboratoire de Météorologie Dynamique de C.N.R.S. (LMD) support the interpretation of the observed atmospheric phenomena. The MaRS investigation is funded by the DLR Grant 50QP9909 and by the NASA Mars Program.

  18. An International Workshop on Primary Science. Report on the Primary Science Workshop Held after the Conference in Science and Technology Education and Future Human Needs (Bangalore, India, August 1985).

    ERIC Educational Resources Information Center

    Harlen, Wynne, Comp.

    A conference on science and technology and future human needs was attended by over 300 science educators from 64 countries. Educators with particular interest in primary science and technology education extended their stay for an additional seminar. This report highlights the events of that seminar. Contents include: (1) recent and on-going work…

  19. News Competition: School team launches a rocket Conference: Norway focuses on physics teaching Science on Stage: Canadian science acts take to the stage Particle Physics: Teachers get a surprise at CERN Teaching: Exploring how students learn physics University: Oxford opens doors to science teachers Lasers: Lasers shine light on meeting Science Fair: Malawi promotes science education

    NASA Astrophysics Data System (ADS)

    2010-11-01

    Competition: School team launches a rocket Conference: Norway focuses on physics teaching Science on Stage: Canadian science acts take to the stage Particle Physics: Teachers get a surprise at CERN Teaching: Exploring how students learn physics University: Oxford opens doors to science teachers Lasers: Lasers shine light on meeting Science Fair: Malawi promotes science education

  20. 2010 IEEE Nuclear Science Symposium, Medical Imaging Conference, and Room Temperature Semiconductor Detectors Workshop

    NASA Astrophysics Data System (ADS)

    The Nuclear Science Symposium (NSS) offers an outstanding opportunity for scientists and engineers interested or actively working in the fields of nuclear science, radiation instrumentation, software and their applications, to meet and discuss with colleagues from around the world. The program emphasizes the latest developments in technology and instrumentation and their implementation in experiments for space sciences, accelerators, other radiation environments, and homeland security. The Medical Imaging Conference (MIC) is the foremost international scientific meeting on the physics, engineering and mathematical aspects of nuclear medicine based imaging. As the field develops, multi-modality approaches are becoming more and more important. The content of the MIC reflects this, with a growing emphasis on the methodologies of X-ray, optical and MR imaging as they relate to nuclear imaging techniques. In addition, specialized topics will be addressed in the Short Courses and Workshops programs. The Workshop on Room-Temperature Semiconductor Detectors (RTSD) represents the largest forum of scientists and engineers developing new semiconductor radiation detectors and imaging arrays. Room-temperature solid-state radiation detectors for X-ray, gamma-ray, and neutron radiation are finding increasing applications in such diverse fields as medicine, homeland security, astrophysics and environmental remediation. The objective of this workshop is to provide a forum for discussion of the state of the art of material development for semiconductor, scintillator, and organic materials for detection, materials characterization, device fabrication and technology, electronics and applications.

  1. PREFACE: 4th International Conference on Mathematical Modeling in Physical Sciences (IC-MSquare2015)

    NASA Astrophysics Data System (ADS)

    Vlachos, Dimitrios; Vagenas, Elias C.

    2015-09-01

    The 4th International Conference on Mathematical Modeling in Physical Sciences (IC-MSQUARE) took place in Mykonos, Greece, from Friday 5th June to Monday 8th June 2015. The Conference was attended by more than 150 participants and hosted about 200 oral, poster, and virtual presentations. There were more than 600 pre-registered authors. The 4th IC-MSQUARE consisted of different and diverging workshops and thus covered various research fields where Mathematical Modeling is used, such as Theoretical/Mathematical Physics, Neutrino Physics, Non-Integrable Systems, Dynamical Systems, Computational Nanoscience, Biological Physics, Computational Biomechanics, Complex Networks, Stochastic Modeling, Fractional Statistics, DNA Dynamics, Macroeconomics etc. The scientific program was rather intense as after the Keynote and Invited Talks in the morning, three parallel oral and one poster session were running every day. However, according to all attendees, the program was excellent with a high quality of talks creating an innovative and productive scientific environment for all attendees. We would like to thank the Keynote Speaker and the Invited Speakers for their significant contribution to IC-MSQUARE. We also would like to thank the Members of the International Advisory and Scientific Committees as well as the Members of the Organizing Committee.

  2. PREFACE: 3rd International Conference on Mathematical Modeling in Physical Sciences (IC-MSQUARE 2014)

    NASA Astrophysics Data System (ADS)

    2015-01-01

    The third International Conference on Mathematical Modeling in Physical Sciences (IC-MSQUARE) took place at Madrid, Spain, from Thursday 28 to Sunday 31 August 2014. The Conference was attended by more than 200 participants and hosted about 350 oral, poster, and virtual presentations. More than 600 pre-registered authors were also counted. The third IC-MSQUARE consisted of different and diverging workshops and thus covered various research fields where Mathematical Modeling is used, such as Theoretical/Mathematical Physics, Neutrino Physics, Non-Integrable Systems, Dynamical Systems, Computational Nanoscience, Biological Physics, Computational Biomechanics, Complex Networks, Stochastic Modeling, Fractional Statistics, DNA Dynamics, Macroeconomics etc. The scientific program was rather heavy since after the Keynote and Invited Talks in the morning, three parallel oral sessions and one poster session were running every day. However, according to all attendees, the program was excellent with high level of talks and the scientific environment was fruitful, thus all attendees had a creative time. We would like to thank the Keynote Speaker and the Invited Speakers for their significant contribution to IC-MSQUARE. We also would like to thank the Members of the International Advisory and Scientific Committees as well as the Members of the Organizing Committee.

  3. PREFACE: 2nd International Conference on Mathematical Modeling in Physical Sciences 2013 (IC-MSQUARE 2013)

    NASA Astrophysics Data System (ADS)

    2014-03-01

    The second International Conference on Mathematical Modeling in Physical Sciences (IC-MSQUARE) took place at Prague, Czech Republic, from Sunday 1 September to Thursday 5 September 2013. The Conference was attended by more than 280 participants and hosted about 400 oral, poster, and virtual presentations while counted more than 600 pre-registered authors. The second IC-MSQUARE consisted of different and diverging workshops and thus covered various research fields where Mathematical Modeling is used, such as Theoretical/Mathematical Physics, Neutrino Physics, Non-Integrable Systems, Dynamical Systems, Computational Nanoscience, Biological Physics, Computational Biomechanics, Complex Networks, Stochastic Modeling, Fractional Statistics, DNA Dynamics, Macroeconomics. The scientific program was rather heavy since after the Keynote and Invited Talks in the morning, three parallel sessions were running every day. However, according to all attendees, the program was excellent with high level of talks and the scientific environment was fruitful, thus all attendees had a creative time. We would like to thank the Keynote Speaker and the Invited Speakers for their significant contribution to IC-MSQUARE. We also would like to thank the Members of the International Advisory and Scientific Committees as well as the Members of the Organizing Committee. Further information on the editors, speakers and committees is available in the attached pdf.

  4. Science preparedness and science response: perspectives on the dynamics of preparedness conference.

    PubMed

    Lant, Timothy; Lurie, Nicole

    2013-01-01

    The ability of the scientific modeling community to meaningfully contribute to postevent response activities during public health emergencies was the direct result of a discrete set of preparedness activities as well as advances in theory and technology. Scientists and decision-makers have recognized the value of developing scientific tools (e.g. models, data sets, communities of practice) to prepare them to be able to respond quickly--in a manner similar to preparedness activities by first-responders and emergency managers. Computational models have matured in their ability to better inform response plans by modeling human behaviors and complex systems. We advocate for further development of science preparedness activities as deliberate actions taken in advance of an unpredicted event (or an event with unknown consequences) to increase the scientific tools and evidence-base available to decision makers and the whole-of-community to limit adverse outcomes.

  5. Proceedings of the Annual International Conference of the Association for the Education of Teachers in Science (Seattle, Washington, January 11-14, 1996).

    ERIC Educational Resources Information Center

    Rubba, Peter A. Ed.; And Others

    These conference proceedings include papers presented and summaries of presentations made at the 1996 Annual International Conference of the Association for the Education of Teachers in Science (AETS). Topics include: English-as-a-Second Language (ESL) Strategies in science methods courses; writing strategies; action research and equity issues;…

  6. Spectral Calibration Requirements of Radio Interferometers for Epoch of Reionisation Science with the SKA

    NASA Astrophysics Data System (ADS)

    Trott, Cathryn M.; Wayth, Randall B.

    2016-05-01

    Spectral features introduced by instrumental chromaticity of radio interferometers have the potential to negatively impact the ability to perform Epoch of Reionisation and Cosmic Dawn (EoR/CD) science. We describe instrument calibration choices that influence the spectral characteristics of the science data, and assess their impact on EoR/CD statistical and tomographic experiments. Principally, we consider the intrinsic spectral response of the antennas, embedded within a complete frequency-dependent primary beam response, and instrument sampling. The analysis is applied to the proposed SKA1-Low EoR/CD experiments. We provide tolerances on the smoothness of the SKA station primary beam bandpass, to meet the scientific goals of statistical and tomographic (imaging) of EoR/CD programs. Two calibration strategies are tested: (1) fitting of each fine channel independently, and (2) fitting of an nth-order polynomial for each ~ 1 MHz coarse channel with (n+1)th-order residuals (n = 2, 3, 4). Strategy (1) leads to uncorrelated power in the 2D power spectrum proportional to the thermal noise power, thereby reducing the overall sensitivity. Strategy (2) leads to correlated residuals from the fitting, and residual signal power with (n+1)th-order curvature. For the residual power to be less than the thermal noise, the fractional amplitude of a fourth-order term in the bandpass across a single coarse channel must be < 2.5% (50 MHz), < 0.5% (150 MHz), < 0.8% (200 MHz). The tomographic experiment places constraints on phase residuals in the bandpass. We find that the root-mean-square variability over all stations of the change in phase across any fine channel (4.578 kHz) should not exceed 0.2 degrees.

  7. A Decade of Cassini Radio Science Observations of the Saturn System

    NASA Astrophysics Data System (ADS)

    French, R.; Armstrong, J.; Flasar, M.; Iess, L.; Kliore, A.; Marouf, E.; McGhee, C.; Nagy, A.; Rappaport, N.; Schinder, P.; Tortora, P.; Anabtawi, A.; Asmar, S.; Barbinis, E.; Fleischmann, D.; Kahan, D.

    2014-04-01

    The Cassini Radio Science Subsystem (RSS) on board the Cassini spacecraft has returned a wealth ofinformation about the Saturn system during its first decade of observations. The instrumentation is quite versatile, operating in up to three wavelengths simultaneously (S, X, and Ka bands), and tied to a very stable frequency standard either on board or uplinked to the spacecraft from a maser-controlled transmitter as part of the Deep Space Network. Over the course of the mission so far, dozens of occultations by Saturn's rings have been observed, revealing the detailed structure and scattering properties of the rings at sub-km resolution. A companion set of atmospheric occultations by Saturn and Titan have provided detailed vertical profiles of the temperature of the neutral atmosphere and the electron density of the ionosphere, spanning a range of latitudes and a significant fraction of a Saturn season. Operatin in a bistatic mode, the RSS instrument has transmitted signals to the surface of Titan at the specular point such that the reflected signal is received on the earth, revealing the dielectric properties of Titan's surface. Finally, exquisitely accurate measurements of the gravitationally induced Dopper shift of the RSS transmitted signal have provided measurements of the gravitations fields and probes of the internal structure of several of Saturn's major satellites, most notably indicating the presence of sub-surface oceans on both Titan and Enceladus. During the upcoming three-year finale of the Cassini mission, highlights of the remaining RSS science objectives include high- SNR measurements of the rings at their most favorable geometry of the entire Cassini orbital tour, and a set of close orbital fly-bys of Saturn itself, enabling the determination of the planet's gravitational field to an accuracy comparable to that expected for the Juno mission to Jupiter.

  8. Panel discussion--NASA Russia agreement/Earth applications. Summary of the panel discussion during the 1994 Life Support and Biosphere Science (LSB Science) Conference

    PubMed

    Huff, W

    1994-01-01

    The panel at the Life Support and Biosphere (LSB) Science conference resulted in a discussion of the current issues facing this industry today. As the LSB Science industry looks to future space missions, joint Russian missions and Earth applications several quandaries arise, such as funding future work, developing practical workable standards and applying these systems to Earth applications. The panel members addressed these quandaries with some insightful comments.

  9. Panel discussion--NASA Russia agreement/Earth applications. Summary of the panel discussion during the 1994 Life Support and Biosphere Science (LSB Science) Conference

    PubMed

    Huff, W

    1994-01-01

    The panel at the Life Support and Biosphere (LSB) Science conference resulted in a discussion of the current issues facing this industry today. As the LSB Science industry looks to future space missions, joint Russian missions and Earth applications several quandaries arise, such as funding future work, developing practical workable standards and applying these systems to Earth applications. The panel members addressed these quandaries with some insightful comments. PMID:11538721

  10. Education in Library and Information Science. Proceedings of the International Conference (Dubrovnik, Yugoslavia, May 21-26, 1984).

    ERIC Educational Resources Information Center

    Mihel, Ivan, Ed.; Tudor-Silovic, Neva, Ed.

    1984-01-01

    An international conference attended by 59 participants from 12 countries was organized to present Yugoslavia as a case study to the international audience, to bring to the Yugoslav audience a variety of international experiences in library and information science education and training, and to acquaint participants with some of the new…

  11. The Science of Enhanced Student Engagement and Employability: Introducing the Psychology Stream of the Inaugural HEA STEM Conference

    ERIC Educational Resources Information Center

    Hulme, Julie; Taylor, Jacqui; Davies, Mark N. O.; Banister, Peter

    2012-01-01

    The Higher Education Academy (HEA) is committed to enhancing the quality of learning and teaching for all university students in the UK, and the inaugural conference for the Science, Technology, Engineering and Mathematics (STEM) subjects, held in April 2012 at Imperial College, London, aimed to showcase research and evidence-based educational…

  12. Classroom Assessment in Mathematics: Views from a National Science Foundation Working Conference (Greensboro, North Carolina, May 16-18, 1997).

    ERIC Educational Resources Information Center

    Bright, George W., Ed.; Joyner, Jeane M., Ed.

    This document presents papers from a National Science Foundation (NSF) working conference to identify research issues and implementation strategies that support quality classroom assessment. Papers include: (1) "Understanding and Improving Classroom Assessment: Summary of Issues Raised" (George W. Bright and Jeane M. Joyner); (2) "Recommendations…

  13. IFLA General Conference, 1985. Division on Special Libraries. Section on Social Science Libraries and Geography and Map Libraries. Papers.

    ERIC Educational Resources Information Center

    International Federation of Library Associations, The Hague (Netherlands).

    Papers presented on social science and map and geography libraries at the 1985 International Federation of Library Associations (IFLA) conference include: (1) "Information for the Developing World: NTIS's (National Technical Information Service) Role in Information Transfer to Developing Countries" (Joseph F. Caponio, United States); (2)…

  14. PROCEEDINGS OF THE CONFERENCE ON THE CHANGING IDENTITY OF GRADUATE EARTH SCIENCE EDUCATION (ATLANTA, JANUARY 25-26, 1965).

    ERIC Educational Resources Information Center

    WEAVER, CHARLES E.

    DISCUSSED ARE THE CHANGING IDENTITY OF GRADUATE EARTH SCIENCE EDUCATION, THE FACTORS WHICH PRECIPITATED THESE CHANGES, AND THE RESULTING PROBLEMS. THE CONFERENCE PARTICIPANTS INCLUDED EARTH SCIENTISTS WITH DIVERSE SCIENTIFIC BACKGROUNDS FROM A BROAD GEOGRAPHICAL AREA. SPECIFIC TOPICS COVERED INCLUDED--(1) PRESENT DEVELOPMENTS AND FUTURE OF EARTH…

  15. On the Juno radio science experiment: models, algorithms and sensitivity analysis

    NASA Astrophysics Data System (ADS)

    Tommei, G.; Dimare, L.; Serra, D.; Milani, A.

    2015-01-01

    Juno is a NASA mission launched in 2011 with the goal of studying Jupiter. The probe will arrive to the planet in 2016 and will be placed for one year in a polar high-eccentric orbit to study the composition of the planet, the gravity and the magnetic field. The Italian Space Agency (ASI) provided the radio science instrument KaT (Ka-Band Translator) used for the gravity experiment, which has the goal of studying the Jupiter's deep structure by mapping the planet's gravity: such instrument takes advantage of synergies with a similar tool in development for BepiColombo, the ESA cornerstone mission to Mercury. The Celestial Mechanics Group of the University of Pisa, being part of the Juno Italian team, is developing an orbit determination and parameters estimation software for processing the real data independently from NASA software ODP. This paper has a twofold goal: first, to tell about the development of this software highlighting the models used, secondly, to perform a sensitivity analysis on the parameters of interest to the mission.

  16. Stability measurements of the radio science system at the 34-m high-efficiency antennas

    NASA Technical Reports Server (NTRS)

    Pham, T. T.; Breidenthal, J. C.; Peng, T. K.; Abbate, S. F.; Rockwell, S. T.

    1993-01-01

    From 1991 to 1993 the fractional frequency stability of the operational Radio Science System was measured at DSS's 15, 45, and 65. These stations are designed to have the most stable uplink and downlink equipment in the Deep Space Network (DSN). Some measurements were performed when the antenna was moving and the frequency was ramped. The stability, including contributions of all elements in the station except for the antenna and the hydrogen maser, was measured to be 0.3 to 1.3 x 10(exp -15) when the frequency was fixed, and 0.6 to 6.0 x 10(exp -15) when the frequency was ramped (sample interval, 1000 sec). Only one measurement out of fifteen exceeded specification. In all other cases, when previous measurements on the antenna and the hydrogen maser were added, a total system stability requirement of 5.0 x 10(exp -15) as met. In addition, ambient temperature was found to cause phase variation in the measurements at a rate of 5.5 deg of phase per deg C.

  17. A Decade of Cassini Radio Science so Far, and Three Spectacular Years Ahead

    NASA Astrophysics Data System (ADS)

    French, R. G.; Armstrong, J. W.; Flasar, F. M.; Iess, L.; Kliore, A. J.; Marouf, E. A.; McGhee-French, C.; Nagy, A. F.; Rappaport, N. J.; Schinder, P. J.; Tortora, P.; Anabtawi, A.; Asmar, S. W.; Barbinis, E.; Fleischman, D. U.; Kahan, D. S.

    2014-12-01

    Over the past decade, the Cassini RSS (Radio Science Subsystem) instrument has provided fundamental new insights into many aspects of the Saturn system. Taking advantage of the capability to use up to three simultaneous wavelengths (Ka, X, and S bands), a series of occultation experiments of Titan and Saturn have provided detailed vertical profiles of the atmospheric and ionospheric structure, exhibiting seasonal and regional variability. Gravity experiments, conducted during close flybys of Saturn's moons, have yielded information about their internal structure, including evidence of sub-surface oceans on Titan and Enceladus. From dozens of ring occultation experiements, the radial structure, scattering properties, and particle sizes of the rings have been measured to high precision, enabling detailed comparative studies of ring dynamics and orbital characteristics. Recent bistatic observations of Titan, in which the transmitted signal reflects off of the specular point and is received on Earth, have traversed the northern polar regions, crossing the boundaries between seas and land, showing that the surface of the seas is remarkably smooth, and providing information about the dielectric properties of the liquids and surface materials. The best is yet to come, during the final three years of the Cassini mission, when the RSS instrument will observe the rings in a series of occultation measurements at their most favorable geometry of the entire Cassini mission, and a companion set of close fly-bys of Saturn will provide the first detailed determination of Saturn's gravitational field.

  18. Improving Science Instruction for Students with Disabilities: Proceedings. Working Conference on Science for Persons with Disabilities (Anaheim, California, March 28-29, 1994).

    ERIC Educational Resources Information Center

    Stefanich, Greg P.; Egelston-Dodd, Judy, Ed.

    This proceedings report includes papers presented at a conference on teaching science to students with disabilities. In the first paper, "Family Pedigrees: A Model Lesson Illustrating Strategies for Teaching Students with Disabilities in a Mainstreamed High School Biology Class" (Kathleen Ball and Edward C. Keller, Jr.), strategies are described…

  19. CONFERENCES AND SYMPOSIA Commemoration of the 85th birthday of S I Syrovatskii(Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 26 May 2010)

    NASA Astrophysics Data System (ADS)

    2010-12-01

    A scientific session of the Physical Sciences Division, Russian Academy of Sciences (RAS), was held on 26 May 2010 at the conference hall of the Lebedev Physical Institute, RAS. The session was devoted to the 85th birthday of S I Syrovatskii. The program announced on the web page of the RAS Physical Sciences Division (www.gpad.ac.ru) contained the following reports: (1) Zelenyi L M (Space Research Institute, RAS, Moscow) "Current sheets and reconnection in the geomagnetic tail"; (2) Frank A G (Prokhorov General Physics Institute, RAS, Moscow) "Dynamics of current sheets as the cause of flare events in magnetized plasmas"; (3) Kuznetsov V D (Pushkov Institute of Terrestrial Magnetism, the Ionosphere, and Radio Wave Propagation, RAS, Troitsk, Moscow region) "Space research on the Sun"; (4) Somov B V (Shternberg Astronomical Institute, Lomonosov Moscow State University, Moscow) "Strong shock waves and extreme plasma states"; (5) Zybin K P (Lebedev Physical Institute, RAS, Moscow) "Structure functions for developed turbulence"; (6) Ptuskin V S (Pushkov Institute of Terrestrial Magnetism, the Ionosphere, and Radio Wave Propagation, RAS, Troitsk, Moscow region) "The origin of cosmic rays." Papers based on reports 1-4 and 6 are published in what follows. • Metastability of current sheets, L M Zelenyi, A V Artemyev, Kh V Malova, A A Petrukovich, R Nakamura Physics-Uspekhi, 2010, Volume 53, Number 9, Pages 933-941 • Dynamics of current sheets underlying flare-type events in magnetized plasmas, A G Frank Physics-Uspekhi, 2010, Volume 53, Number 9, Pages 941-947 • Space research of the Sun, V D Kuznetsov Physics-Uspekhi, 2010, Volume 53, Number 9, Pages 947-954 • Magnetic reconnection in solar flares, B V Somov Physics-Uspekhi, 2010, Volume 53, Number 9, Pages 954-958 • The origin of cosmic rays, V S Ptuskin Physics-Uspekhi, 2010, Volume 53, Number 9, Pages 958-961

  20. The Albany Two-Way Radio Conferences, 1955-1981: a retrospective look at a program providing interactive continuing medical education at a distance.

    PubMed

    Tulgan, Henry

    2014-01-01

    Despite early widespread recognition of the necessity of continuing medical education (CME) for practicing physicians and surgeons, medical schools and national medical organizations were slow to mobilize to address the need. One pioneering program, developed by the Albany Medical College in New York, not only provided CME, but did so in a live distance education format that allowed for interaction between the participants and the faculty presenters. The Albany Program commenced in 1955 using what was then state-of-the-art technology; it exemplified principles and practices that can be seen as the precursors for the distance education approaches used to reach physicians today. This short article describes the contributions of the Albany Two-Way Radio Conferences and places them in the context of developments in national organizations and policies in the 20th century.

  1. 2011 X-Ray Science Gordon Research Conference (August 7-12, 2011, Colby, College. Waterville, ME)

    SciTech Connect

    Gregory Stephenson

    2011-08-12

    The 2011 Gordon Research Conference on X-ray Science will feature forefront x-ray-based science enabled by the rapid improvements in synchrotron and x-ray laser sources. Across the world, x-ray sources are playing an increasingly important role in physics, materials, chemistry, and biology, expanding into ever broadening areas of science and engineering. With the first hard x-ray free electron laser source beginning operation and with other advanced x-ray sources operational and planned, it is a very exciting and pivotal time for exchange ideas about the future of x-ray science and applications. The Conference will provide the forum for this interaction. An international cast of speakers will illuminate sessions on ultrafast science, coherence, imaging, in situ studies, extreme conditions, new developments in optics, sources, and detectors, inelastic scattering, nanoscience, life science, and energy sciences. The Conference will bring together investigators at the forefront of these areas, and will provide a venue for young scientists entering a career in x-ray research to present their research in poster format, hold discussions in a friendly setting, and exchange ideas with leaders in the field. Some poster presenters will be selected for short talks. The collegial atmosphere of this Conference, with ample time for discussion as well as opportunities for informal gatherings in the afternoons and evenings, will provide an avenue for scientists from different disciplines to exchange ideas about forefront x-ray techniques and will promote cross-fertilization between the various research areas represented.

  2. Proceedings of the Annual International Conference of the Association for the Education of Teachers in Science (Minneapolis, MN, January 8-11, 1998).

    ERIC Educational Resources Information Center

    Rubba, Peter A., Ed.; Rye, James A., Ed.

    The 40 papers from this international conference addressed the major theme of facilitating science literacy for all teachers and students. Papers include the following: (1) "Confronting the Gender Gap in Science and Mathematics: The Sisters in Science Program" (P. Hammrich); (2) Teaching Instructional Materials for Science Educators with a CD-ROM…

  3. Seventy Years of Radio Science, Technology, Standards, and Measurement at the National Bureau of Standards

    NASA Astrophysics Data System (ADS)

    Gillmor, C. Stewart

    This large volume describes all the forms of radio research done at the National Bureau of Standards (now, National Institute of Standards and Technology) from its founding in 1901 until about 1980. The volume truly reflects its subtitle; it describes in great detail research in radio propagation and all its connections with geophysics and geospace, but also radio as instrument for discovery and application in meteorology, navigation, and in standards of measurement and testing in electronics.The book is a bit unwieldy and some of its chapters will be of most interest to former NBS employees. For example, there is a lengthy chapter on the transfer of radio research work from Washington, D.C, to Boulder, Colo., in the early 1950s, complete with photostat of the quit claim deed to NBS from the Boulder Chamber of Commerce. On the other hand, radio research developed and flourished in this country in the early days at industrial (Bell Telephone, General Electric, Westinghouse) and government (NBS, Naval Research Laboratory) labs more than in academia, and it is very interesting to learn how the labs interacted and to read details of the organizational structure. I can attest personally to the great difficulties in locating materials concerning radio history. While we have numerous volumes devoted to certain popular radio heroes, little is available concerning government radio pioneers such as L. W. Austin, who directed the U.S. Navy's radio research for many years while situated physically at the Bureau of Standards, or J. H. Dellinger, long-time chief of the Radio Section and head spokesman on radio for the U.S. government until the 1930s.

  4. Radio Astronomy at the Byurakan Astrophysical Observatory, the Institute of Radio Physics and Electronics of the Academy of Sciences of the Armenian SSR and Other Armenian Organisations

    NASA Astrophysics Data System (ADS)

    Sanamian, V. A.

    The establishment and development of radio astronomy in Armenia is described in detail. Information about the radio telescopes of the Byurakan Astrophysical Observatory (BAO) is summarised. The main results of radio-astronomy studies carried out by BAO staff are described, including a number that used large Soviet and foreign radio telescopes, primarily studies of active galaxies.

  5. Definition phase of Grand Tour missions/radio science investigations study for outer planets missions

    NASA Technical Reports Server (NTRS)

    Tyler, G. L.

    1972-01-01

    Scientific instrumentation for satellite communication and radio tracking systems in the outer planet exploration mission is discussed. Mission planning considers observations of planetary and satellite-masses, -atmospheres, -magnetic fields, -surfaces, -gravitational fields, solar wind composition, planetary radio emissions, and tests of general relativity in time delay and ray bending experiments.

  6. Amateur Radio in Space: A Teacher's Guide with Activities in Science, Mathematics, and Technology.

    ERIC Educational Resources Information Center

    Peck, Sandy; White, Rosalie

    This educator's guide contains background information on the Space Amateur Radio EXperiment (SAREX) designed to facilitate communication between astronauts in orbit and students on the ground. Through SAREX, astronauts make scheduled and unscheduled amateur radio contacts from the Shuttle orbiter with schools selected through a proposal process…

  7. Methods and successes of New York University workshops for science graduate students and post-docs in science writing for general audiences (readers and radio listeners)

    NASA Astrophysics Data System (ADS)

    Hall, S. S.

    2012-12-01

    Scientists and science administrators often stress the importance of communication to the general public, but rarely develop educational infrastructures to achieve this goal. Since 2009, the Arthur L. Carter Journalism Institute at New York University has offered a series of basic and advanced writing workshops for graduate students and post-docs in NYU's eight scientific divisions (neuroscience, psychology, physics, biology, chemistry, mathematics, anthropology, and computer science). The basic methodology of the NYU approach will be described, along with successful examples of both written and radio work by students that have been either published or broadcast by general interest journalism outlets.

  8. Learning radio astronomy by doing radio astronomy

    NASA Astrophysics Data System (ADS)

    Vaquerizo Gallego, J. A.

    2011-11-01

    PARTNeR (Proyecto Académico con el Radio Telescopio de NASA en Robledo, Academic Project with the NASA Radio Telescope at Robledo) is an educational program that allows high school and undergraduate students to control a 34 meter radio telescope and conduct radio astronomical observations via the internet. High-school teachers who join the project take a course to learn about the science of radio astronomy and how to use the antenna as an educational resource. Also, teachers are provided with learning activities they can do with their students and focused on the classroom implementation of the project within an interdisciplinary framework. PARTNeR provides students with firsthand experience in radio astronomy science. Thus, remote radio astronomical observations allow students to learn with a first rate scientific equipment the basics of radio astronomy research, aiming to arouse scientific careers and positive attitudes toward science. In this contribution we show the current observational programs and some recent results.

  9. From Research to Radio: How to Talk to a Science Reporter

    NASA Astrophysics Data System (ADS)

    Bentley, M. C.

    2006-12-01

    While there can be misunderstanding between scientists and journalists in communicating scientific research and, in particular, the realities of climate change, the communication gulf is wider between scientists/journalists and the public. Scientists may not be aware just how a journalist decides when and how to report on scientific research so that it might have an impact on the audience since these considerations are not those made when writing a paper for scientists' peers - or, in turn, how scientists can work with reporters to communicate more effectively the significance of their work. For example, polls have shown that while the majority of the American public is aware of climate change, they feel no urgency about it, or feel helpless as to how to respond. A newspaper article that includes new research into increased melt of Artic glaciers, that also includes the relevance the changes have to the individual living outside the Arctic, and how the public might take action, may help scientists break through the psychological barrier that prevents the public from absorbing the consequences of a changing climate. It is also important that scientists describe their research in language that a lay public can understand, without the jargon familiar only to scientists within a particular circle of research. In this talk I will describe my experience reporting on science and climate change for the BBC as to what frustrations reporters have in interviewing scientists, what misconceptions scientists may have about how journalism work, and what scientists should keep in mind when talking to reporters so that both groups can work together to communicate more effectively to the public. I will include audio examples from my radio work, whose concepts are relevant also to other media.

  10. STEM on the radio

    NASA Astrophysics Data System (ADS)

    Showstack, Randy

    2011-10-01

    Looking for an Internet radio station focusing on programing about science, technology, engineering, and math (STEM)? The U.S. National Science Foundation (NSF) announced on 26 September the launch of Science360 Radio, which it says is the first Internet radio stream dedicated to STEM programing. Science360 includes more than 100 radio shows and podcasts that are available on the Web as well as on iPhone and Android devices. The shows originate from a variety of sources, including NSF, other U.S. government agencies, science organizations, universities, and media outlets. For more information, see http://science360.gov/files/.

  11. Abstracts of Presented Papers and the Proceedings of the Association for Education of Teachers in Science--North Central Region and Society for College Science Teachers Conference (Indianapolis, Indiana, October 29-30, 1986).

    ERIC Educational Resources Information Center

    Foster, Gerald Wm., Ed.

    This document contains the abstracts of the presentations made at this conference. Topics of presentations included: (1) linking research and science teaching using community resources; (2) planning science teacher workshops; (3) school-related recycling programs; (4) improving student attitudes toward science; (5) rural science teaching; (6)…

  12. News Conference: Take a hold of Hands-on Science Meeting: Prize-winning physics-education talks are a highlight of the DPG spring meeting in Jena Event: Abstracts flow in for ICPE-EPEC 2013 Schools: A new Schools Physics Partnership in Oxfordshire Conference: 18th MPTL is forum for multimedia in education Meeting: Pursuing playful science with Science on Stage Forthcoming events

    NASA Astrophysics Data System (ADS)

    2013-03-01

    Conference: Take a hold of Hands-on Science Meeting: Prize-winning physics-education talks are a highlight of the DPG spring meeting in Jena Event: Abstracts flow in for ICPE-EPEC 2013 Schools: A new Schools Physics Partnership in Oxfordshire Conference: 18th MPTL is forum for multimedia in education Meeting: Pursuing playful science with Science on Stage Forthcoming events

  13. Lunar and Planetary Science Conference, 21st, Houston, TX, Mar. 12-16, 1990, Proceedings

    SciTech Connect

    Ryder, G.; Sharpton, V.L.

    1991-01-01

    The present conference on lunar and planetary science discusses the geology and geophysics of Venus; the lunar highlands and regolith; magmatic processes of the moon and meteorites; remote sensing of the moon and Mars; chondrites, cosmic dust, and comets; ammonia-water mixtures; and the evolution of volcanism, tectonics, and volatiles on Mars. Attention is given to volcanism on Venus, pristine moon rocks, the search for Crisium Basin ejecta, Apollo 14 glasses, lunar anorthosites, the sources of mineral fragments in impact melts 15445 and 15455, and argon adsorption in the lunar atmosphere. Also discussed are high-pressure experiments on magnesian eucrite compositions, the early results of thermal diffusion in metal-sulfide liquids, preliminary results of imaging spectroscopy of the Humorum Basin region of the moon, high-resolution UV-visible spectroscopy of lunar red spots, and a radar-echo model for Mars. Other topics addressed include nitrogen isotopic signatures in the Acapulco Meteorite, tridymite and maghemite formation in an Fe-SiO smoke, and the enigma of mottled terrain on Mars.

  14. Radio Jove: Jupiter Radio Astronomy for Citizens

    NASA Astrophysics Data System (ADS)

    Higgins, Charles; Thieman, J. R.; Flagg, R.; Reyes, F. J.; Sky, J.; Greenman, W.; Brown, J.; Typinski, D.; Ashcraft, T.; Mount, A.

    2014-01-01

    Radio JOVE is a hands-on educational activity that brings the radio sounds of the Sun, Jupiter, the Milky Way Galaxy, and terrestrial radio noise to students, teachers, and the general public. Participants may build a simple radio telescope kit, make scientific observations, and interact with professional radio observatories in real-time over the Internet. Our website (http://radiojove.gsfc.nasa.gov) includes science information, construction manuals, observing guides, and education resources for teachers and students. Radio Jove is continually expanding its participants with over 1800 kits sold to more than 70 countries worldwide. Recently some of our most dedicated observers have upgraded their Radio Jove antennas to semi-professional observatories. We have spectrographs and wide band antennas, some with 8 MHz bandwidth and some with dual polarization capabilities. In an effort to add to the science literature, these observers are coordinating their efforts to pursue some basic questions about Jupiter’s radio emissions (radio source locations, spectral structure, long term changes, etc.). We can compare signal and ionosphere variations using the many Radio Jove observers at different locations. Observers are also working with members of the Long Wavelength Array Station 1 (LWA1) radio telescope to coordinate observations of Jupiter; Radio Jove is planning to make coordinated observations while the Juno Mission is active beginning in 2015. The Radio Jove program is overviewed, its hardware and software are highlighted, recent sample observations are shown, and we demonstrate that we are capable of real citizen science.

  15. Resonance and Radio

    ERIC Educational Resources Information Center

    Starrett, Malin J.

    2008-01-01

    The science and technology of radio receives little attention in contemporary education. This article discusses ways to explore the basic operating principles of radio. (Contains 4 figures, 3 footnotes, and 2 notes.)

  16. New ITU ``Handbook on Radio Astronomy'' Gives Support to Protection Efforts

    NASA Astrophysics Data System (ADS)

    Davis, Michael M.

    1994-12-01

    A complex international structure exists for the administration of the radio spectrum, now widely viewed as an increasingly valuable natural resource. Radio astronomy was first officially recognized as a radio communications service at the World Administrative Radio Conference of 1959. At that time the IAU, URSI and COSPAR set up under ICSU the Inter-Union Commission for the Allocation of Frequencies for Radio Astronomy and Space Science (IUCAF) to represent scientific usage of the spectrum. Radio astronomers work through their national agencies or IUCAF to get their concerns considered by the International Telecommunications Union (ITU), or included on the agenda of a World Radio Conference. In addition to IUCAF, National and Regional committees such as the US Committee on Radio Frequencies (CORF) and the European Committee on Radio Astronomy Frequencies (CRAF) facilitate a united participation by radio astronomers. It is essential that the unique requirements of the passive services be clearly documented and readily accessible to professional spectrum managers more attuned to the requirements of government and commercial transmitting services. The ITU Radio-communications Sector is supporting this effort by the publication of ``Handbook on Radio Astronomy''. This document, prepared by an international team of radio astronomers experienced in frequency management, describes the characteristics of the radio astronomy service, the preferred frequency bands for radio astronomy use, and the extreme sensitivity and resulting vulnerability of radio astronomy observations to interference. It defines sharing criteria, harmful interference limits, and the threat of unwanted emissions from broad band (spread spectrum) modulation. Copies of the ITU ``Handbook on Radio Astronomy'' should be in every engineering and astronomy library, and the material it provides can usefully be included in college and graduate level courses. The Handbook is available in both English and

  17. News Teaching Support: New schools network launched Competition: Observatory throws open doors to a select few Festival: Granada to host 10th Ciencia en Acción Centenary: Science Museum celebrates 100 years Award: Queen's birthday honour for science communicator Teacher Training: Training goes where it's needed Conference: Physics gets creative in Christchurch Conference: Conference is packed with ideas Poster Campaign: Bus passengers learn about universe Forthcoming events

    NASA Astrophysics Data System (ADS)

    2009-09-01

    Teaching Support: New schools network launched Competition: Observatory throws open doors to a select few Festival: Granada to host 10th Ciencia en Acción Centenary: Science Museum celebrates 100 years Award: Queen's birthday honour for science communicator Teacher Training: Training goes where it's needed Conference: Physics gets creative in Christchurch Conference: Conference is packed with ideas Poster Campaign: Bus passengers learn about universe Forthcoming events

  18. The Calm Methane Northern Seas of Titan from Cassini Radio Science Observations

    NASA Astrophysics Data System (ADS)

    Marouf, Essam A.; French, Richard G.; Wong, Kwok; Anabtawi, Aseel; Schinder, Paul J.; Cassini Radio Science Team

    2016-10-01

    We report on results from 3 bistatic scattering observations of Titan northern seas conducted by the Cassini spacecraft in 2014 ( flybys T101, T102, and T106). The onboard Radio Science instrument transmits 3 sinusoidal signals of 0.94, 3.6, and 13 cm wavelengths. The spacecraft is continuously maneuvered to point in incidence direction so that mirror-like reflections from Titan's surface are observed at the ground stations of the NASA Deep Space Network. The corresponding ground-track in all 3 cases crossed different regions of Kraken Mare, and in the case of T101 also crossed Ligeia Mare. A nearly pure sinusoidal reflected signal was clearly detectable in the observed echoes spectra over surface regions identified in the Cassini RADAR images as potential liquid regions. Weaker quasi-specular echoes were also evident over some intermediate dry land and near sea shores. Cassini transmits right-circularly-polarized (RCP) signals and both the RCP and LCP echo components are observed. Their spectral shape, bandwidth, and total power are the observables used to infer/constrain physical surface properties. Presented results are limited to the 3.6 cm wavelength signal which has the largest SNR. The remarkably preserved sinusoidal echo spectral shape and the little detectable Doppler broadening strongly suggest surface that is smooth on scales large compared to 3.6 cm. If long wavelength gravity waves are present, they must be very subtle. The measured RCP/LCP echo power ratio provides direct measurement of the surface dielectric constant and is diagnostic of the liquid composition. The power ratio measurements eliminate possible significant ethane contribution and strongly imply predominantly liquid methane and nitrogen composition. Carefully calibrated measurements of the absolute echo power and the inferred dielectric constant constrain the presence of any capillary waves of wavelength << 3.6 cm. The latter affect wave coherence across the Fresnel region, reducing the

  19. Proceedings of a Conference on a National Information System in the Mathematical Sciences (Harrison House, Glen Cove, New York, January 18-20, 1970).

    ERIC Educational Resources Information Center

    Phelps, C. Russell, Ed.

    The purpose of this conference was to consider ways of developing a system of improved information services for the mathematical sciences and for the interfaces with related scientific fields. Conference memebrs investigated the achievements, coverage, and technology of existing information services and systems in the fields of engineering,…

  20. Proceedings of the Annual Conference of the Western Australian Science Education Association (19th, Perth, Western Australia, Australia, November 18, 1994).

    ERIC Educational Resources Information Center

    Rennie, Leonie J., Ed.

    The Western Australian Science Education Association is an informal group which meets annually for a conference. This document contains the proceedings of the 1994 conference. Papers included were: (1) "Relationship Between Cognitive Style and Students' Proportional Reasoning Ability" (Ayo Akatugba); (2) "Alternative Modes of Instruction in…

  1. PREFACE: 3rd International Conference on Science & Engineering in Mathematics, Chemistry and Physics 2015 (ScieTech 2015)

    NASA Astrophysics Data System (ADS)

    Gaol, F. L.

    2015-06-01

    The 3rd International Conference on Science & Engineering in Mathematics, Chemistry and Physics 2015 (ScieTech 2015), was held at The Westin Resort Nusa Dua, Bali on 31 January - 1 February 2015. The ScieTech 2015 conference is aimed to bring together researchers, engineers and scientists from around the world. ScieTech 2015 is placed on promoting interaction between the theoretical, experimental, and applied communities, so that a high level exchange is achieved in new and emerging areas within mathematics, chemistry and physics. As we already know that science and technology have brought tremendous benefits for human civilization. People are becoming healthier, wealthier, better educated, more peaceful, increasingly connected, and living longer. Of course, science and technology provide many answers to global challenges, but we will face more complex problems in the next decade due to increasing world population, limitation of energy, and climate change. Therefore, researchers should be more active in conducting research that enables collaboration between one and the others. Interdisciplinary cooperation is absolutely necessary in order to create a smart system for solving the global problems. We need a global and general long-term view of the future with long-range goals for solving complex problems in next decade. Therefore the conference was held to be a forum for researchers from different disciplines to start collaborating and conducting research that provides a solution to the global issues. The theme of ScieTech 2015 was ''The interdisciplinary Application between Mathematics, Chemistry and Physics to enhance the Quality of Life''. We would like to express our sincere gratitude to all in the Technical Program Committee who have reviewed the papers and developed a very interesting conference program as well as the invited and plenary speakers. This year, we received 197 papers and after rigorous review, 59 papers were accepted. The participants came from 19

  2. PREFACE: 3rd International Conference on Geological, Geographical, Aerospace and Earth Science 2015 (AeroEarth 2015)

    NASA Astrophysics Data System (ADS)

    Gaol, F. L.

    2016-02-01

    The 3rd International Conferences on Geological, Geographical, Aerospaces and Earth Sciences 2015 (AeroEarth 2015), was held at The DoubleTree Hilton, Jakarta, Indonesia during 26 - 27 September 2015. The 1st AeoroEarth was held succefully in Jakarta in 2013. The success continued to The 2nd AeroEarth 2014 that was held in Kuta Bali, Indonesia. The publications were published by EES IOP in http://iopscience.iop.org/1755-1315/19/1 and http://iopscience.iop.org/1755-1315/23/1 respectively. The AeroEarth 2015 conference aims to bring together researchers, engineers and scientists from around the world. Through research and development, Earth's scientists have the power to preserve the planet's different resource domains by providing expert opinion and information about the forces which make life possible on Earth. The theme of AeroEarth 2015 is ''Earth and Aerospace Sciences : Challenges and Opportunities'' Earth provides resources and the exact conditions to make life possible. However, with the advent of technology and industrialization, the Earth's resources are being pushed to the brink of depletion. Non-sustainable industrial practices are not only endangering the supply of the Earth's natural resources, but are also putting burden on life itself by bringing about pollution and climate change. A major role of earth science scholars is to examine the delicate balance between the Earth's resources and the growing demands of industrialization. Through research and development, earth scientists have the power to preserve the planet's different resource domains by providing expert opinion and information about the forces which make life possible on Earth. We would like to express our sincere gratitude to all in the Technical Program Committee who have reviewed the papers and developed a very interesting Conference Program as well as the invited and plenary speakers. This year, we received 78 papers and after rigorous review, 18 papers were accepted. The participants

  3. The structure of the Venus neutral atmosphere from the Radio Science Experiment VeRa on Venus Express

    NASA Astrophysics Data System (ADS)

    Tellmann, Silvia; Bird, Mike; Verweyen, Alice; Haeusler, Bernd; Paetzold, Martin; Tyler, G. L.

    The Venus Express Radio Science Experiment VeRa uses one-way radio signals at X-band and S-band for the sounding of the Venus neutral atmosphere and ionosphere. An Ultrastable Oscillator (USO) provides a high quality onboard frequency reference source for this one-way radio link. Simultaneous, coherent measurements at two wavelengths allow separation of dispersive media effects from the classical Doppler shift. Electron density profiles of the ionosphere and profiles of pressure, temperature and neutral number density of the neutral atmosphere can be derived via an Abel transform with an altitude resolution of only a few hundred metres in the altitude range between about 40 and 100 km. Three occultation seasons could be covered during the nominal mission of Venus Express resulting in a data set of about 140 profiles of the neutral atmosphere. Another three occultation seasons are planned during the extended mission. The polar orbit of Venus Express provides the opportunity to study the atmosphere at all planetocentric latitudes under varying illumination conditions. Day-night and latitudinal variations of the thermal structure, the high variability of the atmosphere above the troposphere and signal absorption effects caused by the H2SO4 vapour can be investigated with the resulting data set.

  4. The Structure of the Venus Neutral Atmosphere from the Radio Science Experiment VeRa on Venus Express

    NASA Astrophysics Data System (ADS)

    Tellmann, S.; Häusler, B.; Pätzold, M.; Bird, M.; Tyler, G. L.

    2007-08-01

    The Venus Express Radio Science Experiment VeRa uses one-way radio signals at X-band and S-band for the sounding of the Venus neutral atmosphere and ionosphere. An Ultrastable Oscillator (USO) provides a high quality onboard frequency reference source for this dual-frequency one-way radio link. Simultaneous, coherent measurements at two wavelengths allow separation of dispersive media effects from the classical Doppler shift. Electron density profiles of the ionosphere and profiles of pressure, temperature and neutral number density of the neutral atmosphere can be derived via an Abel transform with an altitude resolution of only a few hundred metres from the cloud deck to ~ 100 km. Two occultation seasons took place in the first year of observation. A total number of 42 profiles occultation experiments were conducted. The polar orbit of Venus Express provides the opportunity to study the atmosphere at all planetocentric latitudes under varying illumination conditions. Special attention will be given to day-night variations of the atmospheric structure and the temperature distribution at high polar latitudes on both hemispheres ("cold collar region") and signal absorption effects caused by the H2SO4 vapour.

  5. The Structure of the Venus Neutral Atmosphere from the Radio Science Experiment VeRa on Venus Express

    NASA Astrophysics Data System (ADS)

    Tellmann, S. A.; Häusler, B.; Pätzold, M.; Bird, M. K.; Tyler, G. L.

    2007-12-01

    The Venus Express Radio Science Experiment VeRa is sounding the Venus neutral atmosphere and ionosphere using the spacecraft radio subsystem in the oneway radio link mode. An Ultrastable Oscillator (USO) provides a high quality onboard frequency reference source for the derivation of electron density profiles in the ionosphere and profiles of pressure, temperature and neutral number density of the neutral atmosphere. The measurement configuration allows an altitude resolution of only a few hundred metres from the cloud deck at about 40 km to approximately 100 km. Three occultation seasons could be covered in the first two years of the Venus Express mission resulting in a data set of about 140 profiles of the neutral atmosphere. The polar orbit of Venus Express provides the opportunity to study the atmosphere at all planetocentric latitudes under varying illumination conditions. Special attention will be given to day-night variations of the thermal structure and the temperature distribution at high polar latitudes on both hemispheres ("cold collar region") and signal absorption effects caused by the H2SO4 vapour.

  6. Sulfuric acid vapor in the atmosphere of Venus as observed by the Venus Express Radio Science experiment VeRa

    NASA Astrophysics Data System (ADS)

    Oschlisniok, Janusz; Pätzold, Martin; Häusler, Bernd; Tellmann, Silvia; Bird, Mike; Andert, Tom

    2016-04-01

    The cloud deck within Venus' atmosphere, which covers the entire planet between approx. 50 and 70 km altitude, consists mostly of liquid and gaseous sulfuric acid. The gaseous part increases strongly just below the main clouds and builds an approx. 15 km thick haze layer of H2SO4. This region is responsible for a strong absorption of radio waves as seen in VeRa radio science observations. The amount of the absorption, which is used to derive the abundance of gaseous sulfuric acid, depends on the signal frequency. VeRa probed the atmosphere of Venus between 2006 and 2015 with radio signals at 13 cm (S-band) and 3.6 cm (X-band) wavelengths. We present H2SO4 profiles derived from S-band and X-band absorption during the first occultation season in 2006. The comparison of the H2SO4 profiles derived from both frequency bands provides a reliable picture of the H2SO4 abundance. Distinct differences in the S- and X-band profiles may give a clue to increased SO2 abundances. The derived VeRa results shall be compared with results provided by other experiments onboard Venus Express as well as with previous missions.

  7. The New Horizons Radio Science Experiment: Performance and Measurements of Pluto's Atmospheric Structure, Surface Pressure, and Surface Temperature

    NASA Astrophysics Data System (ADS)

    Linscott, I.; Hinson, D. P.; Bird, M. K.; Stern, A.; Weaver, H. A., Jr.; Olkin, C.; Young, L. A.; Ennico Smith, K.

    2015-12-01

    The New Horizons (NH) spacecraft payload contained the Radio Science Experiment (REX) for determining key characteristics of Pluto and Charon during the July 14, 2015, flyby of the Pluto/Charon system. The REX flight equipment augments the NH X-band radio transceiver by providing a high precision, narrow band recording of high power uplink transmissions from Earth stations, as well as a record of broadband radiometric power. This presentation will review the performance and initial results of two high- priority observations. First, REX received two pair of 20-kW signals, one pair per polarization, transmitted from the DSN at 4.2-cm wavelength during a diametric radio occultation by Pluto. REX recorded these uplink signals and determined precise measurement of the surface pressure, the temperature structure of the lower atmosphere, and the surface radius of Pluto. The ingress portion of one polarization was played back from the spacecraft in July and processed to obtain the pressure and temperature structure of Pluto's atmosphere. Second, REX measured the thermal emission from Pluto at 4.2- cm wavelength during two linear scans across the disk at close range when both the dayside and the night side are visible. Both scans extend from limb to limb with a resolution of one-tenth Pluto's disk and temperature resolution of 0.1 K. Occultation and radiometric temperature results presented here will encompass additional data scheduled for playback in September.

  8. Exploring the Proposition of a Joint Conference between State Science, and Technology and Engineering Education Associations

    ERIC Educational Resources Information Center

    Love, Tyler S.; Loveland, Thomas

    2014-01-01

    In this article the authors collected numerous forms of data to better understand the perceptions of a joint conference from the various stakeholders. From the detailed survey and interview responses, the researchers found that administrators/supervisors had fewer reservations in regards to holding a joint conference. One reason for this may due…

  9. IEEE Transactions on Nuclear Science. Volume NS-30, no. 4, part 2: 1983 Particle Accelerator Conference

    NASA Astrophysics Data System (ADS)

    Shea, R. F.

    1983-08-01

    This second part of the conference proceedings on particle accelerators completes the two part set. Abstracts of individual items from the conference were prepared separately for the data base. Topics include: reactor technology, particle accelerators, cryogenics, superconductors, spin dynamics and plasma physics.

  10. Building on Family Strengths: Research and Services in Support of Children and Their Families. Proceedings of the Building on Family Strengths Annual Conference (14th, Portland, Oregon, May 31-June 2, 2007) and State of the Science Report

    ERIC Educational Resources Information Center

    Swart, Sandra, Ed.; Friesen, Barbara, Ed.; Holman, Ariel, Ed.; Aue, Nicole, Ed.

    2009-01-01

    The State of the Science conference was held in May, 2007 as part of the ongoing series of national conferences, "Building on Family Strengths," conducted by the Research and Training Center on Family Support and Children's Mental Health at Portland State University. The theme of this State-of-the Science conference was "Effective services for all…

  11. PREFACE: The 2nd International Conference on Geological, Geographical, Aerospace and Earth Sciences 2014 (AeroEarth 2014)

    NASA Astrophysics Data System (ADS)

    Lumban Gaol, Ford; Soewito, Benfano

    2015-01-01

    The 2nd International Conference on Geological, Geographical, Aerospace and Earth Sciences 2014 (AeroEarth 2014), was held at Discovery Kartika Plaza Hotel, Kuta, Bali, Indonesia during 11 - 12 October 2014. The AeroEarth 2014 conference aims to bring together researchers and engineers from around the world. Through research and development, earth scientists have the power to preserve the planet's different resource domains by providing expert opinion and information about the forces which make life possible on Earth. Earth provides resources and the exact conditions to make life possible. However, with the advent of technology and industrialization, the Earth's resources are being pushed to the brink of depletion. Non-sustainable industrial practices are not only endangering the supply of the Earth's natural resources, but are also putting burden on life itself by bringing about pollution and climate change. A major role of earth science scholars is to examine the delicate balance between the Earth's resources and the growing demands of industrialization. Through research and development, earth scientists have the power to preserve the planet's different resource domains by providing expert opinion and information about the forces which make life possible on Earth. We would like to express our sincere gratitude to all in the Technical Program Committee who have reviewed the papers and developed a very interesting Conference Program as well as the invited and plenary speakers. This year, we received 98 papers and after rigorous review, 17 papers were accepted. The participants come from eight countries. There are four Parallel Sessions and two invited Speakers. It is an honour to present this volume of IOP Conference Series: Earth and Environmental Science (EES) and we deeply thank the authors for their enthusiastic and high-grade contributions. Finally, we would like to thank the conference chairmen, the members of the steering committee, the organizing committee

  12. The Conference on Corporate Interference with Science and Health: fracking, food and wireless: genesis, rationale, and results.

    PubMed

    Kopald, Deborah E

    2013-01-01

    A number of serious environmental health hazards created by under-regulated/unregulated industries have morphed into public health crises around the world. The Conference on Corporate Interference with Science and Health (the Conference) was held to examine this trend in three economically significant industries: fracking, food, and wireless. The Conference provided an overview of the structures of these three industries and the history of standard-setting therein, identified the sources of environmental exposures created by these industries, and surveyed the health consequences of these exposures and the policies that have resulted in them. It then examined corporate influence on the setting of these policies and the production of scientific studies and interpretation of their results. The Conference also analyzed the general influence of corporations on the political system and the relationship of this conflict of interest to the aforementioned topics. The concluding discussion focused on what solutions could be implemented to improve public health, including what institutional changes are necessary to promote public awareness and change policy.

  13. Report on the 10th anniversary of international drug discovery science and technology conference, 8 - 10 november 2012, nanjing, china.

    PubMed

    Everett, Jeremy R

    2013-03-01

    The 10th Anniversary of International Drug Discovery Science and Technology (IDDST) Conference was held in Nanjing, China from 8 to 10 November 2012. The conference ran in parallel with the 2nd Annual Symposium of Drug Delivery Systems. Over 400 delegates from both conferences came together for the Opening Ceremony and Keynote Addresses but otherwise pursued separate paths in the huge facilities of the Nanjing International Expo Centre. The IDDST was arranged into 19 separate Chapters covering drug discovery biology, target validation, chemistry, rational drug design, pharmacology and toxicology, drug screening technology, 'omics' technologies, analytical, automation and enabling technologies, informatics, stem cells and regenerative medicine, bioprocessing, generics, biosimilars and biologicals and seven disease areas: cancer, CNS, respiratory and inflammation, autoimmune, emerging infectious, bone and orphan diseases. There were also two sessions of a 'Bench to Bedside to Business' Program and a Chinese Scientist programme. In each period of the IDDST conference, up to seven sessions were running in parallel. This Meeting Highlight samples just a fraction of the content of this large meeting. The talks included have as a link, the use of new approaches to drug discovery. Many other excellent talks could have been highlighted and the author has necessarily had to be selective.

  14. Translating Science into Survival: Report on the Inaugural International Cancer Immunotherapy Conference.

    PubMed

    Hubbard-Lucey, Vanessa M; Tontonoz, Matthew J

    2016-01-01

    The inaugural International Cancer Immunotherapy Conference, cohosted by the Cancer Research Institute (CRI), the American Association for Cancer Research (AACR), the Association for Cancer Immunotherapy (CIMT), and the European Academy of Tumor Immunology (EATI), was held in New York City on September 16–19, 2015. The conference brought together nearly 1,400 scientists, clinicians, regulators, patient advocates, and other stakeholders to discuss the latest scientific developments in cancer immunology and immunotherapy, as well as the regulatory hurdles facing new drug development. This conference report summarizes the main themes that emerged during the 4-day meeting.

  15. PREFACE: 11th Asia-Pacific Conference on Plasma Science and Technology (APCPST-11) and 25th Symposium on Plasma Science for Materials (SPSM-25)

    NASA Astrophysics Data System (ADS)

    Watanabe, Takayuki; Kaneko, Toshio; Sekine, Makoto; Tanaka, Yasunori

    2013-06-01

    The 11th Asia-Pacific Conference on Plasma Science and Technology (APCPST-11) was held in Kyoto, Japan on 2-5 October 2012 with the 25th Symposium on Plasma Science for Materials (SPSM-25). SPSM has been held annually since 1988 under the sponsorship of The 153rd Committee on Plasma Materials Science, Japan Society for the Promotion of Science (JSPS). This symposium is one of the major activities of the Committee, which is organized by researchers in academia and industry for the purpose of advancing intersectional scientific information exchange and discussion of science and technology of plasma materials processing. APCPST and SPSM are jointly held biennially to survey the current status of low temperature and thermal plasma physics and chemistry for industrial applications. The whole area of plasma processing was covered from fundamentals to applications. Previous meetings were held in China, Japan, Korea, and Australia, attended by scientists from the Asia-Pacific and other countries. The joint conference was organized in plenary lectures, invited, contributed oral presentations and poster sessions. At this meeting, we had 386 participants from 10 countries and 398 presentations, including 26 invited presentations. This year, we arranged special topical sessions that covered green innovation, life innovation, and technical reports from industry. This conference seeks to bring the plasma community together and to create a forum for discussing the latest developments and issues, the challenges ahead in the field of plasma research and applications among engineers and scientists in Asia, the Pacific Rim, as well as Europe. This volume presents 44 papers that were selected via a strict peer-review process from full papers submitted for the proceedings of the conference. The topics range from the basic physics and chemistry of plasma processing to a broad variety of materials processing and environmental applications. This volume offers an overview of recent

  16. Continued development of the radio science technique as a tool for planetary and solar system exploration

    NASA Technical Reports Server (NTRS)

    1983-01-01

    A possible alternative to a spacecraft monostatic radar system for surface studies of Titan is introduced. The results of a short study of the characteristics of a bistatic radar investigation of Titan's surface, presented in terms of the Voyager 1 flyby and a proposed Galileo orbiter of Saturn are outlined. The critical factors which need to be addressed in order to optimize the radio occultation technique for the study of clouds and cloud regions in planetary atmospheres are outlined. Potential improvements in the techniques for measuring small-scale structures in planetary atmospheres and ionospheres are addressed. The development of a technique for vastly improving the radial resolution from the radio occultation measurements of the rings of Saturn is discussed.

  17. IFLA General Conference, 1987. Division of Special Libraries. Biological and Medical Science Libraries Section. Social Science Libraries Section. Papers.

    ERIC Educational Resources Information Center

    International Federation of Library Associations, The Hague (Netherlands).

    Six of the nine papers in this collection focus on biological and medical science libraries; the remaining three are concerned with social science libraries. The papers on biological and medical science libraries appear first in this list: (1) "Standards for Medical and Health Care Libraries: Canada" (Jan Greenwood, Canada); (2) "Standards for…

  18. The Venus Ionosphere as seen by the Radio Science Experiment on Venera-15 and Venera-16

    NASA Astrophysics Data System (ADS)

    Gavrik, Anatoly; Gavrik, Yury; Kopnina, Tatiana; Bondarenko, Michael

    This report presents reprocessed results of the radio occultation experiments in the Venus ionosphere carried out by Venera-15, -16 spacecraft in 1983-1984. High stability and coherence of two monochromatic signals (at 1 and 4 GHz) allowed for better precision in determining the influence of atmosphere and ionosphere on radio wave propagation. As a result the existence of the adiabatic invariant in radio occultation was observed experimentally and explained theoretically. The fact that the adiabatic invariant was maintained as the ray moved from plasma to neutral medium let us identify interdependent oscillations of both neutral and ionized medium in the stratified system of atmosphere/ionosphere. In the data provided by the Venera-15, -16 occultation experiments, periodic perturbations of medium density were discovered near the lower boundary of the day ionosphere on Venus, whose level exceeds random variations. Periodic oscillations in electron concentration on the vertical scale of 5-10 km at altitudes between 90 and 115 km were detected. Iterative solution of the forward occultation problem helped to determine electron concentration profiles in the lower ionosphere, describing its layered structure. This report shows that Venus Express occultation data provided by ESA confirms the existence of the adiabatic invariant, which offers means to extract information about the layered structure of the Venusian ionosphere. The work is partially supported by the RAS Presidium Program 22.

  19. Onboard Signal Processing: Wave of the Future for Planetary Radio Science?

    NASA Technical Reports Server (NTRS)

    Marouf, E. A.

    1993-01-01

    Future spacecraft-based radio observations of planetary surfaces, rings, and atmospheres could significantly benefit from recent technological advances in real-time digital signal processing (DSP) hardware. Traditionally, the radio observations have been carried out in a 'down link' configuration in which about 20-W spacecraft transmitted RF power illuminates the target of interest and the perturbed signal is collected at an Earth receiving station. The down link configuration was dictated by the large throughput of received data, corresponding to a relatively large recording band width (about 50 kHz) needed to capture the coherent and scattered signal components in the presence of trajectory, ephemeris, and measurement uncertainties. An alternative 'up link' configuration in which powerful Earth-based radio transmitters (20-200 kW) are used to illuminate the target and data are recorded on board a spacecraft could enhance the measurements' signal-to-noise ratio by a factor of about 1000, allowing a quantum leap in scientific capabilities. Various aspects of alternative signal processing technologies are discussed.

  20. XVII International AIDS Conference: From Evidence to Action - Social, behavioural and economic science and policy and political science

    PubMed Central

    2009-01-01

    AIDS 2008 firmly established stigma and discrimination as fundamental priorities in the push for universal access to HIV prevention, treatment, care and support. Conference sessions and discussions reinforced the tangible negative effects of stigma on national legislation and policies. A strong theme throughout the conference was the need to replace prevention interventions that focus exclusively on individual behaviour change or biomedical prevention interventions with "combination prevention" approaches that address both individual and structural factors that increase vulnerability to HIV infection. Several high-level sessions addressed various aspects of the debate over "vertical" (disease-specific) versus "horizontal" (health systems) funding. The majority of evidence presented at the conference suggests that HIV investments strengthen health systems through the establishment of clinical and laboratory infrastructure, strengthened supply and procurement systems, improvements in health care worker training, and increased community engagement. Human rights were a focal point at the conference; several presentations emphasized the importance of securing human rights to achieve universal access goals, including workplace discrimination, travel restrictions, gender inequality, and the criminalization of homosexuality, drug use, sex work, and HIV transmission and/or exposure. PMID:19811671

  1. Broadening Participation in Science, Technology and Medicine: Proceedings of the Annual Technological Literacy Conference (6th, Washington, D.C., February 1-3, 1991).

    ERIC Educational Resources Information Center

    Cheek, Dennis W., Ed.

    This document contains the text of 50 papers presented at a national conference that focused on the relationships among science, technology, and society (STS). Most of the papers presented featured one of five major thematic areas around which the National Association for Science, Technology and Society is organized: education and information;…

  2. Proceedings of the Annual International Conference of the Association for the Education of Teachers in Science (Charlotte, North Carolina, January 10-13, 2002).

    ERIC Educational Resources Information Center

    Rubba, Peter A., Ed.; Rye, James A., Ed.; DiBiase, Warren J., Ed.; Crawford, Barbara A., Ed.

    This document contains the proceedings of the 2002 Annual International Conference of the Association for the Education of Teachers in Science which was held in Charlotte, North Carolina, January 10-13, 2002. Papers include: (1) "Teaching Science Methods Courses with Web-Enhanced Activities" (Alec M. Bodzin); (2) "How Is Your Lawnmower Working?…

  3. Proceedings of the Nordic Conference on Science and Technology Education: The Challenge of the Future (Karlslunde Strand, Denmark, May 8-12, 1985).

    ERIC Educational Resources Information Center

    Thulstrup, Erik W., Ed.

    The Nordic Conference of 1985 was convened for the purpose of fostering cooperation between science and technology educators within different fields and at different levels, with approximately 40 science and technology educators from Finland, Norway, Sweden, Denmark, India, the United States, and Yugoslavia participating. This report contains 27…

  4. MSaTERs: Mathematics, Science, and Technology Educators & Researchers of The Ohio State University. Proceedings of the Annual Spring Conference (3rd, Columbus, OH, May 15, 1999).

    ERIC Educational Resources Information Center

    Costner, Kelly M., Ed.; Reed, Michelle K., Ed.

    The Mathematics, Science, and Technology Educators and Researchers of The Ohio State University (MSaTERs-OSU) is a student organization that grew out of the former OSU Council of Teachers of Mathematics (OSU-CTM). Papers from the third annual conference include: (1) "Gender, Ethnicity, and Science" (Terry Arambula-Greenfield); (2) "Assessment: The…

  5. Science, Technology and the Liberal Arts: Report on a National Conference Held at Lehigh University (Bethlehem, Pennsylvania, April 1-3, 1984).

    ERIC Educational Resources Information Center

    Cutcliffe, Stephen H.; Goldman, Steven L.

    This conference was designed to provide information on the development and implementation of seven undergraduate science courses primarily for non-science majors at Lehigh University, to examine what ought to be the objectives of courses such as these in the liberal arts curriculum, and to describe parallel efforts with similar educational…

  6. Minitrack on data and knowledge base issues in genomics at the 27th Hawaii International Conference on system sciences

    SciTech Connect

    1995-05-01

    This report is a summary of the proceedings from the Minitrack on Data and Knowledge Base Issues in Genomics at the 27th Hawaii International Conference on System Science, January 4 - 7, 1994. The minitrack was organized by Dong-Guk Shin (University of Connecticut) and Francois Rechenmann (INRIA, France). Support was jointly provided by the NSF, NIH and DOE. The minitrack included, after rigorous review, ten full papers and four extended abstracts in the following five different research subareas of genome informatics: data modeling and management, sequence analysis, graphical user interface, interoperation in a heterogenous computing environment, and system integration in a knowledge-based approach.

  7. 2nd Radio and Antenna Days of the Indian Ocean (RADIO 2014)

    NASA Astrophysics Data System (ADS)

    2014-10-01

    It was an honor and a great pleasure for all those involved in its organization to welcome the participants to the ''Radio and Antenna Days of the Indian Ocean'' (RADIO 2014) international conference that was held from 7th to 10th April 2014 at the Sugar Beach Resort, Wolmar, Flic-en-Flac, Mauritius. RADIO 2014 is the second of a series of conferences organized in the Indian Ocean region. The aim of the conference is to discuss recent developments, theories and practical applications covering the whole scope of radio-frequency engineering, including radio waves, antennas, propagation, and electromagnetic compatibility. The RADIO international conference emerged following discussions with engineers and scientists from the countries of the Indian Ocean as well as from other parts of the world and a need was felt for the organization of such an event in this region. Following numerous requests, the Island of Mauritius, worldwide known for its white sandy beaches and pleasant tropical atmosphere, was again chosen for the organization of the 2nd RADIO international conference. The conference was organized by the Radio Society, Mauritius and the Local Organizing Committee consisted of scientists from SUPELEC, France, the University of Mauritius, and the University of Technology, Mauritius. We would like to take the opportunity to thank all people, institutions and companies that made the event such a success. We are grateful to our gold sponsors CST and FEKO as well as URSI for their generous support which enabled us to partially support one PhD student and two scientists to attend the conference. We would also like to thank IEEE-APS and URSI for providing technical co-sponsorship. More than hundred and thirty abstracts were submitted to the conference. They were peer-reviewed by an international scientific committee and, based on the reviews, either accepted, eventually after revision, or rejected. RADIO 2014 brought together participants from twenty countries spanning

  8. Biomedical Conferences

    NASA Technical Reports Server (NTRS)

    1976-01-01

    As a result of Biomedical Conferences, Vivo Metric Systems Co. has produced cardiac electrodes based on NASA technology. Frequently in science, one highly specialized discipline is unaware of relevant advances made in other areas. In an attempt to familiarize researchers in a variety of disciplines with medical problems and needs, NASA has sponsored conferences that bring together university scientists, practicing physicians and manufacturers of medical instruments.

  9. From the History of Conferences on the Machine and Mechanism Science

    NASA Astrophysics Data System (ADS)

    Wojnarowski, J.

    2016-08-01

    In the course of the past sixty years of the Polish Committee for the Theory of Machines and Mechanisms (PC TMM) 24 scientific and didactic conferences have been held. The subject matter of these conferences, generally organized every other year, comprised problems of the classification, analysis and synthesis of mechanisms, the dynamics of machine systems, investigations concerning self-excited vibrations, the stability of the systems, the control of machines and biomechanics. The numbers of submitted papers as well as the number of participants substantiate the need of organizing such conferences, their importance and the activity of the Polish Committee of TMM for the purpose of creating a platform for the presentation and discussion of new research methods in the domain of mechanisms, machines, biomechanics and mechatronics.

  10. JP Morgan Hambrecht & Quist - 19th Annual Healthcare Conference. Gilead Sciences, American Home Products and Curis.

    PubMed

    Hookes, J

    2001-03-01

    The 19th Annual JP Morgan H and Q Healthcare Conference provided yet another fascinating opportunity to meet with, and hear presentations by, a number of representatives of wellestablished Big Pharma companies, biotech start-up companies and the healthcare service and healthcare 'dot.com' industries. The conference was hosted by JP Morgan H and Q, part of the newly formed JP Morgan - the wholesale banking group of JP Morgan Chase and Co - which led-managed 13 IPOs in the healthcare industry in 2000. This year, the conference was attended by over 5000 delegates, and in excess of 270 company presentations in six parallel sessions were made to members of the healthcare industries, the media and the investment community. PMID:16025374

  11. Recovery of Europa's geophysical attributes with the radio science component of a Europa Multiple-Flyby Mission

    NASA Astrophysics Data System (ADS)

    Verma, Ashok Kumar; Margot, Jean-Luc

    2016-10-01

    NASA has approved the development of a multiple-flyby mission to Jupiter's satellite Europa. Important science questions about Europa's interior structure and sub-surface ocean can be addressed by measuring Europa's gravity field, tidal Love number, and spin state. The mission's radio science investigation will rely on tracking the Doppler shift between the spacecraft and Deep Space Network (DSN) antennas. Here, we simulate the X-band two-way coherent Doppler link between the spacecraft and DSN antennas to evaluate the precision with which geophysical parameters can be recovered. We use the project's 15F10 reference trajectory and simulate Doppler measurements within ±2 h of the spacecraft's closest approach to Europa for each one of 42 flybys. After adding noise to the simulated observables, we solve for Europa's GM, degree and order 2 gravity coefficients (J2 and C22), tidal love number k2, pole position (right ascension and declination), and spin rate. The results of our simulations show that the precision in the recovery of geophysical parameters is sufficient to answer questions related to the presence of a global ocean in some tracking scenarios but not in others. We compare our results to an independent analysis by the Europa Mission Gravity Science Working Group (GSWG, 2016).

  12. Voyager 2 radio science observations of the uranian system: atmosphere, rings, and satellites.

    PubMed

    Tyler, G L; Sweetnam, D N; Anderson, J D; Campbell, J K; Eshleman, V R; Hinson, D P; Levy, G S; Lindal, G F; Marouf, E A; Simpson, R A

    1986-07-01

    Voyager 2 radio occultation measurements of the Uranian atmosphere were obtained between 2 and 7 degrees south latitude. Initial atmospheric temperature profiles extend from pressures of 10 to 900 millibars over a height range of about 100 kilometers. Comparison of radio and infrared results yields mole fractions near the tropopause of 0.85 and 0.15 +/- 0.05 for molecular hydrogen and helium, respectively, if no other components are present; for this composition the tropopause is at about 52 kelvins and 110 millibars. Distinctive features in the signal intensity measurements for pressures above 900 millibars strongly favor model atmospheres that include a cloud deck of methane ice. Modeling of the intensity measurements for the cloud region and below indicates that the cloud base is near 1,300 millibars and 81 kelvins and yields an initial methane mole fraction of about 0.02 for the deep atmosphere. Scintillations in signal intensity indicate small-scale stucture throughout the stratosphere and upper troposphere. As judged from data obtained during occultation ingress, the ionosphere consists of a multilayer structure that includes two distinct layers at 2,000 and 3,500 kilometers above the 100-millibar level and an extended topside that may reach altitudes of 10,000 kilometers or more. Occultation measurements of the nine previously known rings at wavelengths of 3.6 and 13 centimeters show characteristic values of optical depth between about 0.8 and 8; the maxim value occurs in the outer region of the in ring, near its periapsis. Forward-scattered signals from this ring have properties that differ from those of any of Saturn's rings, and they are inconsistent with a discrete scattering object or local (three-dimensional) assemblies of orbiting objects. These signals suggest a new kdnd of planetary ring feature characterized by highly ordered cylindrical substructures of radial scale on the order of meters and azimuthal scale of kilometers or more. From radio data

  13. NSSDC Conference on Mass Storage Systems and Technologies for Space and Earth Science Applications, volume 1

    NASA Technical Reports Server (NTRS)

    Kobler, Benjamin (Editor); Hariharan, P. C. (Editor); Blasso, L. G. (Editor)

    1992-01-01

    Papers and viewgraphs from the conference are presented. This conference served as a broad forum for the discussion of a number of important issues in the field of mass storage systems. Topics include magnetic disk and tape technologies, optical disks and tape, software storage and file management systems, and experiences with the use of a large, distributed storage system. The technical presentations describe, among other things, integrated mass storage systems that are expected to be available commercially. Also included is a series of presentations from Federal Government organizations and research institutions covering their mass storage requirements for the 1990's.

  14. DSS 43 antenna gain analysis for Voyager Uranus encounter: 8.45-GHz radio science data correction

    NASA Technical Reports Server (NTRS)

    Slobin, S. D.; Imbriale, W. A.

    1987-01-01

    A malfunction of the Deep Space Network (DSN) 64-meter antenna in Australia forced the antenna to operate with a mispositioned subreflector during the Voyager Uranus encounter period (January 24, 1986). Because of changing main reflector shape and quadripod position as a function of elevation angle, the antenna gain and pointing were not as expected, and the 8.45 GHz received signal level changed during the pass. The study described here used the Geometrical Theory of Diffraction (GTD) analysis to determine actual antenna gain and pointing during that period in an attempt to reconstruct the radio science data. It is found that the 1.4 dB of signal variation can be accounted for by antenna geometry changes and pointing error. Suggested modifications to the values measured during the pass are presented. Additionally, an extremely useful tool for the analysis of gravity deformed reflectors was developed for use in future antenna design and analysis projects.

  15. Proceedings of the NSSDC Conference on Mass Storage Systems and Technologies for Space and Earth Science Applications

    NASA Technical Reports Server (NTRS)

    Blackwell, Kim; Blasso, Len (Editor); Lipscomb, Ann (Editor)

    1991-01-01

    The proceedings of the National Space Science Data Center Conference on Mass Storage Systems and Technologies for Space and Earth Science Applications held July 23 through 25, 1991 at the NASA/Goddard Space Flight Center are presented. The program includes a keynote address, invited technical papers, and selected technical presentations to provide a broad forum for the discussion of a number of important issues in the field of mass storage systems. Topics include magnetic disk and tape technologies, optical disk and tape, software storage and file management systems, and experiences with the use of a large, distributed storage system. The technical presentations describe integrated mass storage systems that are expected to be available commercially. Also included is a series of presentations from Federal Government organizations and research institutions covering their mass storage requirements for the 1990's.

  16. Science Literacy Project for Mid-Career Public Radio Producers, Reporters, Editors and News Directors

    SciTech Connect

    Scott, Bari

    2012-12-01

    SoundVision held a post-workshop teleconference for our 2011 graduates (as we have done for all participants) to consolidate what they'd learned during the workshop. To maximize the Science Literacy Project's impact after it ends, we strengthened and reinforced our alumni's vibrant networking infrastructure so they can continue to connect and support each other, and updated our archive system to ensure all of our science and science journalism resources and presentations will be easy to access and use over time.

  17. Support for GCTE-LUCC open Science Conference on global change. Final report for period September 15, 1997, - September 14, 1998

    SciTech Connect

    Pitelka, L.F.

    1999-02-01

    The Global Change and Terrestrial Ecosystems (GCTE) core project of the International Geosphere-Biosphere Program (IGBP) and the Land-Use/Cover Change (LUCC) core project of IGBP and the International Human Dimensions Program (IHDP) held a major open Science Conference in Barcelona, Spain, on 14-18 March 1998. At the Conference, scientists presented the most recent research findings from these two international projects, explored emerging cross-cutting linkages between the projects, and highlighted the importance of the regional approach to global change research. This grant from the U.S. Department of Energy, Office of Biological and Environmental Research, provided support for the Conference by contributing to the production of conference literature and by supporting the participation of U.S. scientists in the Conference.

  18. Inverse theory resolution analysis in planning radio science gravity investigations of icy moons

    NASA Astrophysics Data System (ADS)

    Ganse, A.; Vance, S.

    2014-12-01

    The nature of an icy satellite's interior relates fundamentally to its composition, thermal structure, formation and evolution history, and prospects for supporting life. Gravity measurements via radio Doppler information during spacecraft flybys constitute an important tool to infer gross interior structure. Liquid water and ice layers have previously been inferred for the interiors of Jupiter's icy satellites Europa, Ganymede, and Callisto on the basis of magnetic field measurements by the Galileo probe. On Europa and Callisto induced magnetic field signatures measured by the Galileo probe provided strong evidence for an ionic aqueous ocean. Among the chief goals of the proposed Europa Clipper mission in returning to Europa is characterizing the structure of the moon's icy shell. A geophysical inverse theory resolution analysis can be calculated at the pre-measurement mission planning stage, contributing planning considerations from the point of view of the search for mass anomalies in the ice shell (meteorites or diapiric upwellings) or near the H2O/rock interface (seamounts). The analysis allows us to assess the location-varying resolution of an icy moon's interior density anomaly distribution that can be estimated from radio Doppler measurements. It considers the tradeoff between the resolution of the estimated density anomaly distribution and its estimation uncertainty, and investigates issues in distinguishing between ocean anomalies (e.g., seamounts) and mass anomalies within or near the surface of the ice layer. We apply the resolution analysis to proposed Europa Clipper trajectories and past Galileo spacecraft trajectories about Europa and Ganymede.

  19. Conference Report: Advancing the Science of Developmental Neurotoxicity (DNT) Testing for Better Safety Evaluation

    EPA Science Inventory

    1. Introduction The 3rd International Conference on Alternatives for Developmental Neurotoxicity Testing (DNT3), organized by the European Centre for the Validation of Alternative Methods (ECVAM), the Joint Research Centre of the European Commission, was held from May 10 -13, 20...

  20. The Twenty-Fifth Lunar and Planetary Science Conference. Part 1: A-G

    NASA Technical Reports Server (NTRS)

    1994-01-01

    Papers from the conference are presented, and the topics covered include the following: planetary geology, meteorites, planetary composition, meteoritic composition, planetary craters, lunar craters, meteorite craters, petrology, petrography, volcanology, planetary crusts, geochronology, geomorphism, mineralogy, lithology, planetary atmospheres, impact melts, volcanoes, planetary evolution, tectonics, planetary mapping, asteroids, comets, lunar soil, lunar rocks, lunar geology, metamorphism, chemical composition, meteorite craters, and planetary mantles.

  1. PREFACE: International Conference on Advancement in Science and Technology 2012 (iCAST): Contemporary Mathematics, Mathematical Physics and their Applications

    NASA Astrophysics Data System (ADS)

    Ganikhodjaev, Nasir; Mukhamedov, Farrukh; Hee, Pah Chin

    2013-04-01

    The 4th International Conference on the Advancement of Science and Technology 2012 (iCAST 2012), with theme 'Contemporary Mathematics, Mathematical Physics and their Applications', took place in Kuantan, Malaysia, from Wednesday 7 to Friday 9 November 2012. The conference was attended by more than 100 participants, and hosted about 160 oral and poster papers by more than 140 pre-registered authors. The key topics of the 4th iCAST 2012 include Pure Mathematics, Applied Mathematics, Theoretical/Mathematical Physics, Dynamical Systems, Statistics and Financial Mathematics. The scientific program was rather full since after the Keynote and Invited Talks in the morning, four parallel sessions ran every day. However, according to all attendees, the program was excellent with a high level of talks and the scientific environment was fruitful; thus all attendees had a creative time. The conference aimed to promote the knowledge and development of high-quality research in mathematical fields concerned with the application of other scientific fields as well as modern technological trends in physics, chemistry, biology, medicine, economics, sociology and environmental sciences. We would like to thank the Keynote and the Invited Speakers for their significant contributions to 4th iCAST 2012. We would also like to thank the members of the International Scientific Committee and the members of the Organizing Committee. We cannot end without expressing our many thanks to International Islamic University Malaysia and our sponsors for their financial support . This volume presents selected papers which have been peer-reviewed. The editors hope that it may be useful and fruitful for scholars, researchers, and advanced technical members of the industrial laboratory facilities for developing new tools and products. Guest Editors Nasir Ganikhodjaev, Farrukh Mukhamedov and Pah Chin Hee The PDF contains the committee lists, board list and biographies of the plenary speakers.

  2. News Astronomy: Science and beauty combined Africa: Physics technicians offer valuable skills Conference: ESERA2013 brings researchers together in Cyprus Physics Olympiad: UK team bring home more medals from the Physics Olympics in Copenhagen Physics Tournament: IOC backs Shrewsbury to host IYPT 2014 Conference: MPTL18 looks at the latest multimedia developments Workshop: The selective absorption of light Science on Stage: Illuminating Science Education in London in 2015

    NASA Astrophysics Data System (ADS)

    2013-11-01

    Astronomy: Science and beauty combined Africa: Physics technicians offer valuable skills Conference: ESERA2013 brings researchers together in Cyprus Physics Olympiad: UK team bring home more medals from the Physics Olympics in Copenhagen Physics Tournament: IOC backs Shrewsbury to host IYPT 2014 Conference: MPTL18 looks at the latest multimedia developments Workshop: The selective absorption of light Science on Stage: Illuminating Science Education in London in 2015

  3. Earth Science and Public Health: Proceedings of the Second National Conference on USGS Health-Related Research

    USGS Publications Warehouse

    Buxton, Herbert T.; Griffin, Dale W.; Pierce, Brenda S.

    2007-01-01

    health scientists and earth scientists can lead to improved solutions for existing and emerging environmental health problems. This report summarizes the presentations and discussions held at the Second National Conference on USGS Health-Related Research, held at the USGS national headquarters in Reston, Virginia. The report presents 68 abstracts of technical presentations made at the conference and summaries of six topical breakout sessions. The abstracts cover a broad range of issues and demonstrate connections between human health and the quality and condition of our environment and wildlife. The summaries of the topical breakout sessions present ideas for advancing interdisciplinary science in areas of earth science and human health.

  4. Radio science investigations of the saturn system with voyager 1: preliminary results.

    PubMed

    Tyler, G L; Eshleman, V R; Anderson, J D; Levy, G S; Lindal, G F; Wood, G E; Croft, T A

    1981-04-10

    Voyager 1 radio occultation measurements of Titan's equatorial atmosphere successfully probed to the surface, which is provisionally placed at a radius of 2570 kilometers. Derived scale heights plus other experimental and theoretical results indicate that molecular nitrogen is the predominant atmospheric constituent. The surface pressure and temperature appear to be about 1.6 bars and 93 K, respectively. The main clouds are probably methane ice, although some condensation of nitrogen cannot be ruled out. Solar abundance arguments suggest and the measurements allow large quantities of surface methane near its triple-point temperature, so that the three phases of methane could play roles in the atmosphere and on the surface of Titan similar to those of water on Earth. Radio occultation measurements of Saturn's atmosphere near 75 degrees south latitude reached a maximum pressure of 1.4 bars, where the temperature is about 156 K. The minimum temperature is about 91 K near the 60-millibar pressure level. The measured part of the polar ionosphere of Saturn has a peak electron concentration of 2.3 x 10(4) per cubic centimeter at an altitude of 2500 kilometers above the 1-bar level in the atmosphere, and a plasma scale height at the top of the ionosphere of 560 kilometers. Attenuation of monochromatic radiation at a wavelength of 3.6 centimeters propagating obliquely through Saturn's rings is consistent with traditional values for the normal optical depth of the rings, but the near-forward scattering of this radiation by the rings indicates effective scattering particles with larger than expected diameters of 10, 8, and 2 meters in the A ring, the outer Cassini division, and the C ring, respectively. Preliminary analysis of the radio tracking data yields new values for the masses of Rhea and Titan of 4.4 +/- 0.3 x 10(-6) and 236.64 +/- 0.08 x 10(-6) times the mass of Saturn. Corresponding values for the mean densities of these objects are 1.33 +/- 0.10 and about 1.89 grams

  5. Science Education on the Internet: Conference for Developers of OnLine Curricula ''Learning Strategies for Science Education Websites''

    SciTech Connect

    Gesteland,Raymond F.; Dart, Dorothy S.; Logan,Jennifer; Stark, Louisa

    2000-09-01

    Internet-based science education programs are coming of age. Educators now look seriously to the Internet as a source of accessible classroom materials, and they are finding many high-quality online science programs. Beyond providing solid curriculum, these programs have many advantages. They provide materials that are far more current than what textbooks offer and are more accessible to disadvantaged and rural population. Students can engage in inquiry-based learning online through interactive and virtual activities, accessing databases, tracking nature occurrences in real time, joining online science communities and conversing with scientists.

  6. Radio Galaxies.

    ERIC Educational Resources Information Center

    Downes, Ann

    1986-01-01

    Provides background information on radio galaxies. Topic areas addressed include: what produces the radio emission; radio telescopes; locating radio galaxies; how distances to radio galaxies are found; physics of radio galaxies; computer simulations of radio galaxies; and the evolution of radio galaxies with cosmic time. (JN)

  7. Research in Science Education, Volume 5. Proceedings of the Annual Conference of the Australian Science Education Research Association (6th, Flinders University, Bedford Park, South Australia, May 19-21, 1975).

    ERIC Educational Resources Information Center

    Lucas, A. M., Ed.; Power, Colin, N., Ed.

    This volume contains papers presented at the sixth Annual Conference of the Australian Science Education Research Association (ASERA) held at Flinders University in May, 1975. Paper topics include: pupil learning and classroom climate, teacher structuring behavior, the Australian Science Education Project (ASEP), cognitive preference and…

  8. SCIENCE FOR THE ACADEMICALLY TALENTED STUDENT IN THE SECONDARY SCHOOL, REPORT OF A CONFERENCE SPONSORED JOINTLY BY THE NATIONAL EDUCATION ASSOCIATION PROJECT ON THE ACADEMICALLY TALENTED STUDENT AND THE NATIONAL SCIENCE TEACHERS ASSOCIATION.

    ERIC Educational Resources Information Center

    DONALDSON, ROBERT R.

    RESULTS OF A JOINT NATIONAL EDUCATION ASSOCIATION-NATIONAL SCIENCE TEACHERS ASSOCIATION CONFERENCE ON SCIENCE FOR ACADEMICALLY TALENTED STUDENTS ARE REPORTED. MAJOR TOPICS DISCUSSED ARE (1) THE IDENTIFICATION OF THE TALENTED STUDENT, (2) GUIDELINES FOR THE SELECTION OF COURSE CONTENT, (3) TEACHING METHODS, AND (4) DESIRABLE QUALITIES AND…

  9. FOREWORD: Radio and Antenna Days of the Indian Ocean (RADIO 2012)

    NASA Astrophysics Data System (ADS)

    Monebhurrun, Vikass; Lesselier, Dominique

    2013-04-01

    It was an honor and a great pleasure for all those involved in its organization to welcome the participants to the 'Radio and Antenna Days of the Indian Ocean' (RADIO 2012) international conference that was held from 24th to 27th September 2012 at the Sugar Beach Resort, Wolmar, Flic-en-Flac, Mauritius. RADIO 2012 is the first of a series of conferences that is to be regularly organized in the Indian Ocean region. The aim is to discuss recent developments, theories and practical applications covering the whole scope of radio-frequency engineering, including radio waves, antennas, propagation, and electromagnetic compatibility. Following discussions with engineers and scientists from the countries of the Indian Ocean as well as from other parts of the world, a need was felt for the organization of such an international event in this region. The Island of Mauritius, worldwide known for its white sandy beaches and pleasant tropical atmosphere, provided an excellent environment for the organization of the 1st RADIO international conference. The Local Organizing Committee consisted of scientists from SUPELEC, the University of Mauritius, and the University of Technology, Mauritius. Various members of staff of the University of Mauritius provided help for the organization of the conference. The International Union of Radio Science (URSI) made available technical and financial sponsorship for partial support of young scientists. A number of companies also supported RADIO 2012 ('Platinum': GSMA, ICTA & MMF, 'Gold': CST & FEKO). The event itself was organized in a premier hotel on Mauritius. In this foreword, we would like to take the opportunity again to thank all the people, institutions and companies that made the event such a success. More than 120 abstracts were submitted to the conference and were peer-reviewed by an international scientific committee. RADIO 2012 overall featured six oral sessions, one poster session and two workshops. Three internationally recognized

  10. Multiple signal propagation at the tropopause of the Venusian atmosphere: new insights from the Radio Science Experiment (VeRa) onboard Venus Express

    NASA Astrophysics Data System (ADS)

    Herrmann, Maren; Oschlisniok, Janusz; Remus, Stefan; Tellmann, Silvia; Häusler, Bernd; Pätzold, Martin

    2016-10-01

    The rapid change of the refractive index over a short altitude range in a planetary atmosphere can lead to multi-path effects when sounding the atmosphere with radio waves. The Radio Science Experiment (VeRa) [1,2] onboard Venus Express sounded the Venusian atmosphere from 90 km downward to 40 km altitude[3,4]. More than 800 profiles of temperature, pressure and neutral number density could be retrieved which cover almost all local times and latitudes. A specially developed analysis method based on the VeRa open loop receiving technique deciphers the multi-path effect and identifies an inversion layer near the tropopause at an altitude of about 60km. This layer is of particular interest - it separates the stratified troposphere from the highly variable mesosphere and can be a likely location for the formation of gravity waves [5]. The new retrieval method shows an inversion layer up to 15 K colder than commonly thought. Local time and latitude dependence including the influence of the spacecraft trajectory on this effect will be discussed. These results will contribute to a consistent picture of the Venus' thermal atmosphere structure and therefore help to improve atmospheric models.[1] Häusler, B. et al: 'Radio science investigations by VeRa onboard the Venus Express spacecraft' Planetary and Space Science 54, 2006[2] Häusler, B. et al, 'Venus Atmospheric, Ionospheric, Surface and Interplanetery Radio-Wave Propagation Studies with the VeRa Radio Science experiment' Eur. Space Agencys, Spec. Publ., ESA SP 1295, 2007[3] Pätzold, M. et al: 'The structure of Venus' middle atmosphere and ionosphere', Nature 450, 2007[4] Tellmann, S. et al : 'Structure of the Venus neutral atmosphere as observed by the Radio Science experiment VeRa on Venus Express', Journal of Geophysical Research 114, 2009[5] Tellmann, S. et al: 'Small-scale temperature fluctuations seen by the VeRa Radio Science Experiment on Venus Express' Icarus 221, 2012.

  11. The Future Scientists and Engineers Conferences: Using Community Resources to Enhance the Science Fair

    ERIC Educational Resources Information Center

    Sinsel, Jennifer

    2008-01-01

    Conference attendees arrive at the registration desk at 9:00 a.m. sharp, eager to start their day. While standing in line, they talk excitedly about the sessions they've chosen to see, the original investigation they'll be presenting, off-site field trips for which they've registered, and the businesses scheduled to have booths in the Exhibitor's…

  12. Twenty-Fourth Lunar and Planetary Science Conference. Part 3: N-Z

    SciTech Connect

    Not Available

    1993-01-01

    Papers from the conference are presented, and the topics covered include the following: planetary geology, meteorites, planetary composition, meteoritic composition, planetary craters, lunar craters, meteorite craters, petrology, petrography, volcanology, planetary crusts, geochronology, geomorphism, mineralogy, lithology, planetary atmospheres, impact melts, K-T Boundary Layer, volcanoes, planetary evolution, tectonics, planetary mapping, asteroids, comets, lunar soil, lunar rocks, lunar geology, metamorphism, chemical composition, meteorite craters, planetary mantles, and space exploration. Separate abstracts have been prepared for articles from this report.

  13. Twenty-Fourth Lunar and Planetary Science Conference. Part 3: N-Z

    NASA Technical Reports Server (NTRS)

    1993-01-01

    Papers from the conference are presented, and the topics covered include the following: planetary geology, meteorites, planetary composition, meteoritic composition, planetary craters, lunar craters, meteorite craters, petrology, petrography, volcanology, planetary crusts, geochronology, geomorphism, mineralogy, lithology, planetary atmospheres, impact melts, K-T Boundary Layer, volcanoes, planetary evolution, tectonics, planetary mapping, asteroids, comets, lunar soil, lunar rocks, lunar geology, metamorphism, chemical composition, meteorite craters, planetary mantles, and space exploration.

  14. Proceedings of the precollege-university partnerships for science and mathematics education conference

    SciTech Connect

    Not Available

    1992-08-01

    In April of 1992 in Atlanta, Georgia, nearly 50 elementary and secondary educators and about 100 postsecondary educators convened to explore their common interests in the conference on precollege-university partnerships. This report summarizes the remarks and conclusions of speakers, panelists, and of attendees gathered in regional work groups. During the course of the conference, attendees heard from federal agencies and foundations which fund education-related projects and learned of their enthusiastic support of partnerships. In our national need to manage education and training resources wisely, these funding agents see partnership benefits such as renewed excitement for teaching at all levels, effective and technologically up-to-date in-service training, more and better-prepared high school graduates entering colleges, and a general enhancement of understanding among educators at all levels of teaching. As an added benefit, the partnership concept promotes discussion and understanding in an atmosphere of respect, appreciation, and self-esteem. Several hours of the conference were devoted to panels addressing five questions important to education coalitions. The panelists represented a wide variety of teaching levels, geographic locations, educational experiences, and ethnic groups.

  15. Radio-induced alteration in cordierite - Implications for petrology, gemmology and materials science

    NASA Astrophysics Data System (ADS)

    Krickl, R.; Nasdala, L.; Grambole, D.; Kaindl, R.

    2009-04-01

    Cordierite is a common metamorphic and magmatic mineral, which is used as petrologic tool for reconstructing the history of its host rock. Further applications include cordierite gemstones and the use of synthetic analogs in ceramics. Cordierite is stable over a wide temperature and pressure range and relatively resistant to chemical alteration; however, its properties can be significantly changed upon the impact of external irradiation. In the course of a comprehensive study, natural radiohaloes in cordierite (a widespread feature caused by the impact of alpha-particles originating from radioactive inclusions) as well as artificial analogs produced by implantation of 8.8 MeV He2+ ions were investigated using modern micro-techniques. Additional irradiation experiments were performed using O6+ ions, electrons and gamma-rays. Ion irradiation causes yellow colouration that is strongly pleochroic, and fades at higher doses. The possibility of radiation-treatment for enhancing the quality of gem-cordierite is discussed. While samples remain crystalline up to doses of 1016 He2+/cm2, the same material is fully amorphised when irradiated with the same dose of 30 MeV O6+ ions. These different observations may help to estimate the performance assessment of cordierite-ceramics in radiated environments. A very important result concerning the petrological use of cordierite is the radio-induced transformation of channel constituents: Inside the irradiated areas the vibrational bands of CO2 decrease in intensity, whereas two new bands appear at 2135 cm-1 (both IR- and Raman-active; cf. Nasdala et al., 2006) and 1550 cm-1 (only Raman-activ). They are assigned to stretching vibrations of carbon monoxide and molecular oxygen, respectively, thus indicating a radio-chemical transformation 2CO2 → 2CO + O2 in alpha-irradiated cordierite. This study yields the first spectroscopic evidence for the irradiation-induced formation of molecular oxygen in cordierite. Polarised vibrational

  16. Promoting Better Conditions for Women and Science in Mexico with Regional Conferences

    NASA Astrophysics Data System (ADS)

    Martínez, Amalia; Meza-Montes, Lilia

    2009-04-01

    We report on two main activities of the Working Group Women in Physics of the Mexican Physical Society: "Latin American Women in Exact and Life Sciences," held in Mexico City in May 2006; and the annual "Participation of Women in Science" event. We also update information on the status of female researchers.

  17. PREFACE: Selected papers from the Fourth Topical Conference on Nanoscale Science and Engineering of the American Institute of Chemical Engineers

    NASA Astrophysics Data System (ADS)

    Wong, Michael S.; Lee, Gil U.

    2005-07-01

    This special issue of Nanotechnology contains research papers contributed by the participants of the Fourth Topical Conference on Nanoscale Science and Engineering at the Annual Meeting of the American Institute of Chemical Engineers (AIChE), which was held in Austin, Texas, USA, 7-12 November, 2004. This conference saw 284 oral presentations from institutions around the world, which is the highest number for this topical conference series to date. These presentations were organized into 64 sessions, covering the range of nanotechnology subject areas in which chemical engineers are currently engaged. These sessions included the following areas. • Fundamentals: thermodynamics at the nanoscale; applications of nanostructured fluids; transport properties in nanophase and nanoscale systems; molecular modelling methods; self and directed assembly at the nanoscale; nanofabrication and nanoscale processing; manipulation of nanophases by external fields; nanoscale systems; adsorption and transport in carbon nanotubes; nanotribology; making the transition from materials and phenomena to new technologies; operation of micro-and nano-systems. • Materials: nanoparticle synthesis and stabilization; nanoscale structure in polymers; nanotemplating of polymers; synthesis of carbon nanotubes and nanotube-based materials; nanowires; nanoparticle assemblies and superlattices; nanoelectronic materials; self-assembly of templated inorganic materials; nanostructured hybrid organic/inorganic materials; gas phase synthesis of nanoparticles; multicomponent structured particles; nano energetic materials; liquid-phase synthesis of nanoparticles. • Energy: synthesis and characterization of nanostructured catalytic materials; nanomaterials and devices for energy applications. • Biotechnology: nanobiotechnology; nanotechnology for the biotechnology and pharmaceuticals industries; nanotechnology and nanobiotechnology for sensors; advances in biomaterials, bionanotechnology, biomimetic

  18. CONFERENCES AND SYMPOSIA Spintronics(Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 3 February 2010)

    NASA Astrophysics Data System (ADS)

    2010-10-01

    A scientific session of the Physical Sciences Division of the Russian Academy of Sciences (RAS) was held on 3 February 2010 at the Conference Hall of the P N Lebedev Physical Institute, RAS. The following reports were put on the session agenda posted on the website www.gpad.ac.ru of the Physical Sciences Division, RAS: (1) Ustinov V V (Institute of Metal Physics, Ural Branch, RAS, Ekaterinburg) "Metallic nanospintronics"; (2) Kusrayev Yu G (Ioffe Physical-Technical Institute, RAS, St. Petersburg) "Spin-related phenomena in semiconductors; physics and applications"; (3) Tarasenko S A (Ioffe Physical-Technical Institute, RAS, St. Petersburg) "Spin photocurrents in semiconductors"; (4) Averkiev N S, Golub L E (Ioffe Physical-Technical Institute, RAS, St. Petersburg) "Spin relaxation in quantum semiconductor heterostructures". Papers written on the basis of reports 2-4 are given below. • Spin phenomena in semiconductors: physics and applications, Yu G Kusrayev Physics-Uspekhi, 2010, Volume 53, Number 7, Pages 725-738 • Spin photocurrents in semiconductors, S A Tarasenko Physics-Uspekhi, 2010, Volume 53, Number 7, Pages 739-742 • Spin relaxation anisotropy in two-dimensional semiconductors, N S Averkiev Physics-Uspekhi, 2010, Volume 53, Number 7, Pages 742-745

  19. Lunar and Planetary Science Conference, 13th, Houston, TX, March 15-19, 1982, Proceedings. Part 2

    NASA Technical Reports Server (NTRS)

    Boynton, W. V. (Editor); Ahrens, T. J.

    1983-01-01

    The second part of the proceedings of the Thirteenth Lunar and Planetary Science Conference considers sedimentary processes and crustal cycling on Venus, a model for the formation of the earth's core, evidence of resurfacing in the lunar nearside highlands, the geology of Tethys, thermal stresses in planetary elastic lithospheres, the petrology and comparative thermal and mechanical histories of clasts in breccia 62236, lunar paleointensity data and its implications for the origin of lunar magnetism, and a model for the accumulation of solar wind radiation damage effects in lunar dust grains. Also discussed are fluid inclusions in stony meteorites, nuclear track and compositional studies of olivines in CI and CM chondrites, the impact of an asteroid or comet in the ocean and the extinction of terrestrial life, cooling rates for glass-containing lunar compositions, and the homogeneity of lava flows.

  20. Solar Wind Nine: Proceedings of the Ninth International Solar Wind Conference. Proceedings

    SciTech Connect

    Habbal, S.R.; Esser, R.; Hollweg, J.V.; Isenberg, P.A.

    1999-06-01

    These proceedings represent papers presented at the 9th Solar Wind International Conference, held in Nantucket, Massachusetts, USA, in October, 1998. The Conference was attended by 235 scientists from 25 countries. The aim of the Conference was to integrate theory, modeling, in situ measurements, and remote sensing observations of the solar wind. The Conference succeeded in accomplishing that, as is evident from the papers presented. The topics discussed included coronal plasma and streamers, small scale magnetic structure, dynamics of large scale structure, coronal mass ejection, waves and turbulence, the outer heliosphere, magnetohydrodynamics radio tracking, bursts and shock waves, and galactic cosmic rays. At the beginning of the Conference, a historical overview was presented by E. N. Parker, the predictor of solar wind forty years ago. There were 188 papers presented at the conference, out of which 15 have been abstracted for the Energy,Science and Technology database.(AIP)

  1. CONFERENCES AND SYMPOSIA: Nanoplasmonics and metamaterials(Scientific session of the Division of Physical Sciences, Russian Academy of Sciences, 27 April 2009)

    NASA Astrophysics Data System (ADS)

    Tikhodeev, Sergei G.; Shubina, Tat'yana V.; Ivanov, Sergei V.; Toropov, Aleksei A.; Kop'ev, Petr S.; Kurin, Vladislav V.; Lagarkov, Andrei N.; Sarychev, Andrei K.; Gippius, Nikolai A.

    2009-09-01

    On 27 April 2009, in the conference hall of the Lebedev Physical Institute, Russian Academy of Sciences, a scientific session of the Division of Physical Sciences of the Russian Academy of Sciences devoted to the problem of nanoplasmonics and metamaterials took place. The following reports were presented at the session: (1) Tikhodeev S G, Gippius N A (Prokhorov Institute of General Physics, Russian Academy of Sciences, Moscow) "Plasmon-polariton effects in nanostructured metal-dielectric photonic crystals and metamaterials"; (2) Shubina T V, Ivanov S V, Toropov A A, Kop'ev P S (Ioffe Physicotechnical Institute, Russian Academy of Sciences, St. Petersburg) "Plasmon effects in In(Ga)N-based nanostructures"; (3) Kurin V V (Institute of Physics of Microstructures, Russian Academy of Sciences, Nizhnii Novgorod) "Resonance scattering of light in nanostructured metallic and ferromagnetic films"; (4) Lagarkov A N , Sarychev A K (Institute of Theoretical and Applied Electrodynamics, Joint Institute of High Temperatures, Russian Academy of Sciences, Moscow) "Active optical metamaterials"; (5) Gippius N A, Tikhodeev S G (Prokhorov Institute of General Physics, Russian Academy of Sciences, Moscow) "Application of the scattering matrix method for calculating the optical properties of metamaterials." Summaries of reports 1-3 and 5 and of an article written on the basis of report 4 are given below. • Plasmon-polariton effects in nanostructured metal-dielectric photonic crystals and metamaterials, S G Tikhodeev, N A Gippius Physics-Uspekhi, 2009, Volume 52, Number 9, Pages 945-949 • Plasmon effects in In(Ga)N-based nanostructures, T V Shubina, S V Ivanov, A A Toropov, P S Kop'ev Physics-Uspekhi, 2009, Volume 52, Number 9, Pages 949-953 • Resonance scattering of light in nanostructured metallic and ferromagnetic films, V V Kurin Physics-Uspekhi, 2009, Volume 52, Number 9, Pages 953-959 • Superresolution and enhancement in metamaterials, A N Lagarkov, A K Sarychev, V N

  2. National Association for Research in Science Teaching Annual Conference (64th, Lake Geneva, Wisconsin, April 7-10, 1991). Abstracts of Presented Papers.

    ERIC Educational Resources Information Center

    National Association for Research in Science Teaching.

    Abstracts of most of the papers, symposia, discussion groups, round tables, and poster sessions presented at the 64th conference of the National Association for Research in Science Teaching (NARST) are provided. Subject areas addressed are as follows: teacher knowledge, cognitive development, conceptual change, curriculum issues, reform in science…

  3. The National Institutes of Health (NIH) State-of-the-Science Conference on Preventing Violence and Related Health-Risking Social Behaviors in Adolescents--A Commentary

    ERIC Educational Resources Information Center

    Johnson, Robert L.

    2006-01-01

    Although youth in the United States remain substantially more violent than adolescents and young adults in most industrial countries, the National Institutes of Health's (NIH) State-of-the-Science Conference on Preventing Violence and Related Health-Risking Social Behaviors in Adolescents identified many reasons for optimism about our capacity to…

  4. Technological Literacy. Proceedings of the National Science, Technology and Society (STS) Conference (3rd, Washington, DC, February 5-7, 1987).

    ERIC Educational Resources Information Center

    Waks, Leonard J., Ed.

    1987-01-01

    This document contains the text of 71 papers presented at a national conference dealing with the relationships among science, technology and society (STS) with particular emphasis on technological literacy. Topics include: (1) emerging ideas and challenges; (2) STS in developing countries; (3) STS and government; (4) frameworks and concepts in STS…

  5. Delivering Academic Excellence to Culturally Diverse Populations (Language Development through Math/Science Activities). Conference Proceedings (Saddle Brook, New Jersey, December 7-8, 1984).

    ERIC Educational Resources Information Center

    Bilotta, Cynthia, Ed.

    This document includes the proceedings of a conference that made the following points about American society now and in the future: (1) racial changes in demographics require preparing urban minority students for entrance into scientific and technological fields; (2) the science/mathematics education movement of the late 1950s into the 1970s has…

  6. MSaTERs: Mathematics, Science, and Technology Educators and Researchers of The Ohio State University. Proceedings of the Annual Spring Conference (2nd, May 16, 1998, Columbus, OH).

    ERIC Educational Resources Information Center

    Reed, Michelle K., Ed.; Costner, Kelly M., Ed.

    The Mathematics, Science, and Technology Educators and Researchers of The Ohio State University (MSaTERS-OSU) is a newly formed student organization. Papers from the conference include: (1) "Was the Geometry Course, The Nature of Proof, Taught by Harold Pascoe Fawcett the Best Course Ever Taught in Secondary School?" (Frederick Flener); (2) "A…

  7. MSaTERs: Mathematics, Science, and Technology Educators & Researchers of The Ohio State University. Proceedings of the Annual Spring Conference (4th, Columbus, Ohio, May 6, 2000).

    ERIC Educational Resources Information Center

    Costner, Kelly M., Ed.; Herman, Marlena F., Ed.

    The Mathematics, Science, and Technology Educators and Researchers of The Ohio State University (MSaTERs-OSU) is a student organization that grew out of the former Ohio State University Council of Teachers of Mathematics (OSU-CTM). Papers from the fourth annual conference include: (1) "Technology Education Curriculum Models in Michigan Secondary…

  8. MSaTERs: Mathematics, Science, and Technology Educators & Researchers of The Ohio State University. Proceedings of the Annual Spring Conference (5th, Columbus, Ohio, May 5, 2001).

    ERIC Educational Resources Information Center

    Herman, Marlena F., Ed.

    The Mathematics, Science, and Technology Educators and Researchers of The Ohio State University (MSaTERs-OSU) is a student organization that grew out of the former Ohio State University Council of Teachers of Mathematics (OSU-CTM). Papers from the fifth annual conference include: (1) "Models of the Structure of Matter: Why Should We Care about…

  9. In Search of Gender Free Paradigms for Computer Science Education. [Proceedings of a Preconference Research Workshop at the National Educational Computing Conference (Nashville, Tennessee, June 24, 1990).

    ERIC Educational Resources Information Center

    Martin, C. Dianne, Ed.; Murchie-Beyma, Eric, Ed.

    This monograph includes nine papers delivered at a National Educational Computing Conference (NECC) preconference workshop, and a previously unpublished paper on gender and attitudes. The papers, which are presented in four categories, are: (1) "Report on the Workshop: In Search of Gender Free Paradigms for Computer Science Education" (C. Dianne…

  10. Science and Technology Education for Civic and Professional Life: The Undergraduate Years. A Report of the Wingspread Conference (Racine, Wisconsin, June 1-3, 1982).

    ERIC Educational Resources Information Center

    American Association for the Advancement of Science, Washington, DC.

    The failure of colleges and universities to ensure that all undergraduates become scientifically and technologically educated was addressed at the 1982 Wingspread Conference. Representatives of education, business, government, and other professions considered the place of science and technology education within liberal education and formulated a…

  11. Proceedings of the Annual International Conference of the Association for the Education of Teachers in Science (Costa Mesa, California, January 18-21, 2001).

    ERIC Educational Resources Information Center

    Rubba, Peter A., Ed.; Rye, James A., Ed.; DiBiase, Warren J., Ed.; Crawford, Barbara A., Ed.

    This document contains the proceedings of the 2001 Annual International Conference of the Association for the Education of Teachers in Science which was held in Costa Mesa, California, January 18-21, 2001. Papers include: (1) "An Elementary Preservice Teacher's Search for Solutions about the Evolution-Divine Creation Question: The Story of Tracy"…

  12. First Cassini Radio Science Bistatic Scattering Observation of Titan's Northern Seas

    NASA Astrophysics Data System (ADS)

    Marouf, E. A.; Kliore, A. J.; Rappaport, N. J.; French, R. G.; Schinder, P. J.; Anabtawi, A.; Wong, K. K.; Armstrong, J. W.; Asmar, S. W.; Flasar, F. M.; Iess, L.; McGhee-French, C.; Nagy, A. F.; Tortora, P.; Barbinis, E.; Buccino, D.; Kahan, D. S.

    2014-12-01

    On May 17, 2014, the Cassini spacecraft completed its 101 flyby of Saturn's satellite Titan. Mirror-like (quasi-specular) reflections of radio signals transmitted by Cassini were observed on the Earth (bistatic scattering geometry). Three right circularly polarized (RCP) sinusoidal signals were transmitted (wavelength = 0.94, 3.6, and 13 cm). Both the RCP and LCP surface reflections were observed at the Canberra, Australia, complex of the NASA Deep Space Network. The signals probed the region extending from about (lat, long) = (79°N, 315°W) to about (74°N, 232°W). For the first time, two major Titan northern seas, the Ligeia Mare and the Kraken Mare, were probed. Clearly detectable RCP and LCP echo components were observed over both seas at all 3 wavelengths. The echoes were intermittent over the region in between the two seas. The echoes from the seas have narrowband spectra well modeled as pure sinusoids, suggesting very smooth surfaces over > ~1 cm scales. Over shorelines and river like channels the measured spectra reveal a second distinct broadband component, likely reflection from a rough bottom solid interface. Modeling the narrowband echo components as sinusoids, we estimate the RCP and LCP echo power profiles over the observation period. High resolution power profiles (several seconds time average; 0.2 to 2 km along the ground track) reveal remarkable structural detail. The statistical measurement uncertainty improves significantly when the resolution is degraded to about 1 m time average (3 to 30 km). Comparison of the 1 m power profiles with theoretical predictions computed assuming absent surface waves (negligible roughness) reveals excellent agreement with reflections from liquid hydrocarbons. The small statistical uncertainty promises to strongly constrain the liquid composition (ethane vs methane dominance). In principle, the measured RCP/LCP power ratio removes dependence on roughness and enables determination of the dielectric constant

  13. Stationary Planetary Waves in the Mars Winter Atmosphere as seen by the Radio Science Experiment MaRS on Mars Express

    NASA Astrophysics Data System (ADS)

    Tellmann, Silvia; Pätzold, Martin; Häusler, Bernd; Tyler, Leonard G.; Hinson, David P.

    2015-11-01

    Stationary (Rossby) Waves are excited by the interaction of the zonally varying topography with the strong eastward winter jets. They lead to distinctive longitudinal temperature variations which contribute significantly to the asymmetry of the seasonal polar CO2 ice caps and are also important for the dust redistribution in the planetary atmosphere.Radio Science profiles from the Mars Express Radio Science Experiment MaRS at northern and southern high latitudes are used to gain insight into winter stationary wave structures on both hemispheres.Mars Global Surveyor (MGS) radio occultation measurements from the same season and year with their exceptionally good longitudinal and temporal coverage can be used to estimate the influence of transient eddies. Transient waves are especially important in the northern winter hemisphere.Wave number 2 stationary waves, driven by topography, are dominant in the northern winter latitudes while the wave number 1 wave is the most significant wave number during southern winter. The wave amplitudes peak around winter solstice on both hemispheres.Radio occultation measurements provide the unique opportunity to determine simultaneous measurements of temperature and geopotential height structures. Assuming geostrophic balance, these measurements can be used to determine meridional winds and eddy heat fluxes which provide further insight into the contribution of stationary waves to the heat exchange between the poles and the lower latitudes.

  14. USL NASA/RECON project presentations at the 1985 ACM Computer Science Conference: Abstracts and visuals

    NASA Technical Reports Server (NTRS)

    Dominick, Wayne D. (Editor); Chum, Frank Y.; Gallagher, Suzy; Granier, Martin; Hall, Philip P.; Moreau, Dennis R.; Triantafyllopoulos, Spiros

    1985-01-01

    This Working Paper Series entry represents the abstracts and visuals associated with presentations delivered by six USL NASA/RECON research team members at the above named conference. The presentations highlight various aspects of NASA contract activities pursued by the participants as they relate to individual research projects. The titles of the six presentations are as follows: (1) The Specification and Design of a Distributed Workstation; (2) An Innovative, Multidisciplinary Educational Program in Interactive Information Storage and Retrieval; (3) Critical Comparative Analysis of the Major Commercial IS and R Systems; (4) Design Criteria for a PC-Based Common User Interface to Remote Information Systems; (5) The Design of an Object-Oriented Graphics Interface; and (6) Knowledge-Based Information Retrieval: Techniques and Applications.

  15. About Clinicopathological Conference and Its' Practice in the School of Medical Sciences, USM.

    PubMed

    Hassan, Shahid

    2006-07-01

    The clinicopathological conference, popularly known as CPC primarily relies on case method of teaching medicine. It is a teaching tool that illustrates the logical, measured consideration of a differential diagnosis used to evaluate patients. The process involves case presentation, diagnostic data, discussion of differential diagnosis, logically narrowing the list to few selected probable diagnoses and eventually reaching a final diagnosis and its brief discussion. The idea was first practiced in Boston, back in 1900 by a Harvard internist, Dr. Richard C. Cabot who practiced this as an informal discussion session in his private office. Dr. Cabot incepted this from a resident, who in turn had received the idea from a roommate, primarily a law student.

  16. The ionospheres of Saturn and Titan from Cassini Radio Science observations

    NASA Astrophysics Data System (ADS)

    Kliore, Arvydas; Nagy, Andrew

    Since @005, the NASA Cassini orbiter has produced 13 profiles of the electron density in the ionosphere of Titan at latitudes from near-equatorial to near polar (Kliore, A.J., et al, J. Geophys. Res.-space Phys.s, ( 2008), 113, A09317, DOI: 10.1029/2007JA012965; Kliore, A. J., et et al., J. Geophys. Res.-space Phys.(2011), 116. A11318, DOI: 10.1029/2011JA016694 ). Most of these profiles had a “normal” and fairly uniform appearance, with a main peak near 1,200 km. altitude and a peak density of about 1-2 x103 cm-3 with no peaks above the main peak. The other three observations have a “disturbed” appearance, with the main peak density of about 3 x 103 cm-3 , with several minor peaks above and below the main peak. It is probable, that these effects are due to the enhanced precipitation of energetic particles from Saturn’s magnetosphere. The planned acquisition of several more ionosphere profiles in 2014 and 2015 may cast more light on the nature of this phenomenon. In that same period, 62 profiles of the electron density in the Saturn ionosphere. In 2005, when the ring opening angle was near maximum, they obscured most of the limb of Saturn, and the near equatorial regions were available for radio occultations, and 12 near-equatorial profiles were obtained (Nagy, A.F., et al, J. Geophys. Res.-Space Phys., ( 2006), 111 ,Issue A6). During the rest of the Cassini Prime mission, 20 additional profiles were obtained at mid- and high latitudes (Kliore, A. J., et al., J. Geophys. Res.-space Phys., (20090, 114,A04215, DOI:10.1029/2008JA013900 ). In the Cassini Extended mission, 24 more profiles were obtained, mostly at low and near-equatorial latitudes during the Equinox mission in 2009-2011, and a final set of 15 observations were obtained in 2012 and 2013 during the Solstice mission, including several at high Northern and Southern latitudes. These are the last possible observations, because the increasing ring opening angle will again obscure the limb of Saturn

  17. The Twenty-Fifth Lunar and Planetary Science Conference. Part 2: H-O

    SciTech Connect

    Not Available

    1994-01-01

    Various papers on lunar and planetary science are presented, covering such topics as: planetary geology, lunar geology, meteorites, shock loads, cometary collisions, planetary mapping, planetary atmospheres, chondrites, chondrules, planetary surfaces, impact craters, lava flow, achondrites, geochemistry, stratigraphy, micrometeorites, tectonics, mineralogy, petrology, geomorphology, and volcanology. Separate abstracts have been prepared for papers from this report.

  18. Proceedings of the Second Annual NASA Science Internet User Working Group Conference

    NASA Technical Reports Server (NTRS)

    Jackson, Lenore A. (Editor); Gary, J. Patrick (Editor)

    1991-01-01

    Copies of the agenda, list of attendees, meeting summaries, and all presentations and exhibit material are contained. Included are plenary sessions, exhibits of advanced networking applications, and user subgroup meetings on NASA Science Internet policy, networking, security, and user services and applications topics.

  19. The Twenty-Fifth Lunar and Planetary Science Conference. Part 3: P-Z

    SciTech Connect

    Not Available

    1994-01-01

    Various papers on lunar and planetary science are presented, covering such topics as: impact craters, tektites, lunar geology, lava flow, geodynamics, chondrites, planetary geology, planetary surfaces, volcanology, tectonics, topography, regolith, metamorphic rock, geomorphology, lunar soil, geochemistry, petrology, cometary collisions, geochronology, weathering, and meteoritic composition. Separate abstracts have been prepared for articles from this report.

  20. The Twenty-Fifth Lunar and Planetary Science Conference. Part 3: P-Z

    NASA Technical Reports Server (NTRS)

    1994-01-01

    Various papers on lunar and planetary science are presented, covering such topics as: impact craters, tektites, lunar geology, lava flow, geodynamics, chondrites, planetary geology, planetary surfaces, volcanology, tectonics, topography, regolith, metamorphic rock, geomorphology, lunar soil, geochemistry, petrology, cometary collisions, geochronology, weathering, and meteoritic composition.

  1. The Twenty-Fifth Lunar and Planetary Science Conference. Part 2: H-O

    NASA Technical Reports Server (NTRS)

    1994-01-01

    Various papers on lunar and planetary science are presented, covering such topics as: planetary geology, lunar geology, meteorites, shock loads, cometary collisions, planetary mapping, planetary atmospheres, chondrites, chondrules, planetary surfaces, impact craters, lava flow, achondrites, geochemistry, stratigraphy, micrometeorites, tectonics, mineralogy, petrology, geomorphology, and volcanology.

  2. IFLA General Conference, 1987. Division of Special Libraries. Science and Technology Libraries Section. Papers.

    ERIC Educational Resources Information Center

    International Federation of Library Associations, The Hague (Netherlands).

    The six papers in this collection focus on science and technology libraries: (1) "Human Aspects of Electronically-Stored Information: The Library User" (A. J. Meadows, United Kingdom); (2) "Untersuchung Menschlicher Aspekte bei den Elektronisch Gespeicherten Informationen: Ansichten des Leiters eines Bibliothekskollektives = Human Aspects of…

  3. MST 1: Proceedings of a conference on the integration of mathematics, science and technology in precollege education

    SciTech Connect

    Swyler, K.

    1995-11-01

    Example MST activities examined here show: (1) an inquiry-driven learning stimulus, involving (2) the synthesis of concepts in math, science and technology, through (3) the application of the scientific method and engineering problem solving/test protocols, and provoking (4) a stimulus for further exploration. A semi-exploratory learning approach offered background aimed at enabling participants to take meaningful courses of investigation; this approach must be balanced by maintaining contact with framework content standards. On the whole, the philosophy underlying the MST learning approach--as envisioned in the draft NYS Framework, and embodied in the example activities--is strongly endorsed. This endorsement is broad-based: those represented include teachers of mathematics, science, and technology, and school district administrators--in roughly equal numbers. Discussion centers not on whether the MST approach should be pursued, but on what is involved in doing it. Teams of conference participants were given time to plan or extend MST initiatives in their own districts. Outlines of the initiatives proposed by ten of the teams are disseminated herein.

  4. National Reports on the State of Social Science Information and Documentation in 16 European Countries. Reports Presented to the ECSSID General Conference (European Cooperation in Social Science Information and Documentation, 4th, Athens, Greece, October 21-23, 1984).

    ERIC Educational Resources Information Center

    Saelen, Kirsti Thesen, Ed.

    Papers presented at the fourth European Cooperation in Social Science Information and Documentation (ECSSID) General Conference provide information on developments in the field in 16 European countries. According to the general outlines provided for these reports, the presentations focus on developments after 1977, thus supplementing information…

  5. Year of the Oceans: Science of Information Handling. [Proceedings of the] Annual Conference of the International Association of Marine Science Libraries and Information Centers (10th, Woods Hole, Massachusetts, October 2-5, 1984).

    ERIC Educational Resources Information Center

    Grundy, R. L., Ed.; Ford, R. T., Ed.

    International Association of Marine Science Libraries and Information Centers (IAMSLIC) conferences provide a format for libraries and information specialists to discuss common interests and concerns so that services and information can be made available to scientists, administrators, engineers, educators and students in the discipline of marine…

  6. How do Medical Societies Select Science for Conference Presentation? How Should They?

    PubMed Central

    Kuczmarski, Thomas M.; Raja, Ali S.; Pallin, Daniel J.

    2015-01-01

    Introduction Nothing has been published to describe the practices of medical societies in choosing abstracts for presentations at their annual meetings. We surveyed medical societies to determine their practices, and also present a theoretical analysis of the topic. Methods We contacted a convenience sample of large U.S. medical conferences, and determined their approach to choosing abstracts. We obtained information from web sites, telephone, and email. Our theoretical analysis compares values-based and empirical approaches for scoring system development. Results We contacted 32 societies and obtained data on 28 (response rate 88%). We excluded one upon learning that research was not presented at its annual meeting, leaving 27 for analysis. Only 2 (7%) made their abstract scoring process available to submitters. Reviews were blinded in most societies (21;78%), and all but one asked reviewers to recuse themselves for conflict of interest (96%). All required ≥3 reviewers. Of the 24 providing information on how scores were generated, 21 (88%) reported using a single gestalt score, and three used a combined score created from pooled domain-specific sub-scores. We present a framework for societies to use in choosing abstracts, and demonstrate its application in the development of a new scoring system. Conclusions Most medical societies use subjective, gestalt methods to select research for presentation at their annual meetings and do not disclose to submitters the details of how abstracts are chosen. We present a new scoring system that is transparent to submitters and reviewers alike with an accompanying statement of values and ground rules. We discuss the challenges faced in selecting abstracts for a large scientific meeting and share the values and practical considerations that undergird the new system. PMID:26265966

  7. International Radio Regulations Resulting from WARC 1979.

    ERIC Educational Resources Information Center

    Berrada, Abderrazak

    The main features of international regulations on radio communications of the International Telecommunication Union are summarized and the possible effects on these regulations of the World Administrative Radio Conference of 1979 (WARC-79) are discussed in this paper. It is noted that while the international radio regulations are regarded as…

  8. AINSE Plasma Science and Technology Conference and Elizabeth and Frederick White Workshop on Fundamental Problems in the Physics of Magnetically Confined Plasmas: Conference handbook

    NASA Astrophysics Data System (ADS)

    The handbook contains abstracts of papers and posters presented at the conference. The main topics relate to plasma physics and fusion, plasma processing and uses as well as specific fusion devices and experiments. Eighty-four out of ninety-two presentations were considered to be in the INIS subject scope and have been separately indexed.

  9. News Event: UK to host Science on Stage Travel: Gaining a more global perspective on physics Event: LIYSF asks students to 'cross scientific boundaries' Competition: Young Physicists' tournament is international affair Conference: Learning in a changing world of new technologies Event: Nordic physical societies meet in Lund Conference: Tenth ESERA conference to publish ebook Meeting: Rugby meeting brings teachers together Note: Remembering John L Lewis OBE

    NASA Astrophysics Data System (ADS)

    2013-03-01

    Event: UK to host Science on Stage Travel: Gaining a more global perspective on physics Event: LIYSF asks students to 'cross scientific boundaries' Competition: Young Physicists' tournament is international affair Conference: Learning in a changing world of new technologies Event: Nordic physical societies meet in Lund Conference: Tenth ESERA conference to publish ebook Meeting: Rugby meeting brings teachers together Note: Remembering John L Lewis OBE

  10. Transforming Science and Technology: Our Future Depends on It. Volume 1 [and] Volume 2: Proceedings and Contributions to the International Gender and Science and Technology Conference (7th, Waterloo, Ontario, Canada, July 31-August 5, 1993) = Transformer les sciences et la technologie: notre avenir en depend. Volume 1 [and] Volume 2. Les soumissions a la septieme conference internationale sur l'equite des sexes en science et en technologie (du 31 juillet au 5 aout 1993).

    ERIC Educational Resources Information Center

    Haggerty, Sharon, Ed.; Holmes, Ann, Ed.

    This two-volume set of papers was produced for the seventh International Gender and Science and Technology (GASTA) Conference. Abstracts of all papers and other presentations have been translated and are published in both English and French. Papers are published in the language in which they were submitted (English or French). GASAT provides a…

  11. The Sardinia Radio Telescope

    NASA Astrophysics Data System (ADS)

    Grueff, G.; Alvito, G.; Ambrosini, R.; Bolli, P.; D'Amico, N.; Maccaferri, A.; Maccaferri, G.; Morsiani, M.; Mureddu, L.; Natale, V.; Olmi, L.; Orfei, A.; Pernechele, C.; Poma, A.; Porceddu, I.; Rossi, L.; Zacchiroli, G.

    We describe the Sardinia Radio Telescope (SRT), a new general purpose, fully steerable antenna of the National Institute for Astrophysics. The radio telescope is under construction near Cagliari (Sardinia). With its large aperture (64m diameter) and its active surface, SRT is capable of operations up to ˜100GHz, it will contribute significantly to VLBI networks and will represent a powerful single-dish radio telescope for many science fields. The radio telescope has a Gregorian optical configuration with a supplementary beam-waveguide (BWG), which provides additional focal points. The Gregorian surfaces are shaped to minimize the spill-over and standing wave. After the start of the contract for the radio telescope structural and mechanical fabrication in 2003, in the present year the foundation construction will be completed. The schedule foresees the radio telescope inauguration in late 2006.

  12. Proceedings of the U.S. Geological Survey Eighth Biennial Geographic Information Science Workshop and first The National Map Users Conference, Denver, Colorado, May 10-13, 2011

    USGS Publications Warehouse

    Sieverling, Jennifer B.; Dietterle, Jeffrey

    2014-01-01

    The U.S. Geological Survey (USGS) is sponsoring the first The National Map Users Conference in conjunction with the eighth biennial Geographic Information Science (GIS) Workshop on May 10-13, 2011, in Lakewood, Colorado. The GIS Workshop will be held at the USGS National Training Center, located on the Denver Federal Center, Lakewood, Colorado, May 10-11. The National Map Users Conference will be held directly after the GIS Workshop at the Denver Marriott West, a convention hotel in the Lakewood, Colorado area, May 12-13. The National Map is designed to serve the Nation by providing geographic data and knowledge for government, industry, and public uses. The goal of The National Map Users Conference is to enhance communications and collaboration among the communities of users of and contributors to The National Map, including USGS, Department of the Interior, and other government GIS specialists and scientists, as well as the broader geospatial community. The USGS National Geospatial Program intends the conference to serve as a forum to engage users and more fully discover and meet their needs for the products and services of The National Map. The goal of the GIS Workshop is to promote advancement of GIS and related technologies and concepts as well as the sharing of GIS knowledge within the USGS GIS community. This collaborative opportunity for multi-disciplinary GIS and associated professionals will allow attendees to present and discuss a wide variety of geospatial-related topics. The Users Conference and Workshop collaboration will bring together scientists, managers, and data users who, through presentations, posters, seminars, workshops, and informal gatherings, will share accomplishments and progress on a variety of geospatial topics. During this joint event, attendees will have the opportunity to present or demonstrate their work; to develop their knowledge by attending hands-on workshops, seminars, and presentations given by professionals from USGS and

  13. Proceedings of Lunar and Planetary Science, Volume 22; Conference, Houston, TX, Mar. 18-22, 1991

    NASA Technical Reports Server (NTRS)

    Ryder, Graham (Editor); Sharpton, Virgil L. (Editor)

    1992-01-01

    Various papers on lunar and planetary science are presented. Individual topics addressed include: analysis of Phobos Mission Gamma ray spectra from Mars, comparison of volcanic and modified landforms from Tharsis Montes on Mars, polygenetic origin of Hrad Vallis region of Mars, new evidence of lacustrine basins on Mars, flood surge through the Lunae Planum Outflow Complex on Mars, interpretation of canyon materials and flood sources on Kasei Valles on Mars, geochemistry of Manson Impact structure rocks, micrometer-sized glass spheres in Apollo 16 soil 61181, isotopic abundances in Pesyanoe of solar-type xenon, mineralogy of 12 large 'chondritic' interplanetary dust particles. Also discussed are: trace elements in chondritic stratospheric particles, evolution of isotopic signatures in lunar regolith nitrogen, pyroclastic deposits on the western limb of the moon, origin of picritic green glass magmas by polybaric fractional fusion, origin of yellow glasses associated with Apollo 15 KREEP basalt fragments, trace elements in 59 mostly highland moon rocks, mineralization on the moon, relation between diogenite cumulates and eucrite magmas.

  14. Lunar and Planetary Science Conference, 18th, Houston, TX, Mar. 16-20, 1987, Proceedings

    NASA Technical Reports Server (NTRS)

    Ryder, Graham (Editor)

    1988-01-01

    Papers on lunar and planetary science are presented, including petrogenesis and chemistry of lunar samples, geology and petrogenesis of the Apollo 15 landing site, lunar geology and applications, cratering records and cratering effects, differentiated meteorites, chondritic meteorites and asteroids, extraterrestrial grains, Venus, Mars, and icy satellites. The importance of lunar granite and KREEP in very high potassium basalt petrogenesis, indentifying parent plutonic rocks from lunar breccia and soil fragments, glasses in ancient and young Apollo 16 regolith breccias, the formation of the Imbrium basin, the chemistry and petrology of the Apennine Front, lunar mare ridges, studies of Rima Mozart, electromagnetic energy applications in lunar resource mining and construction, detecting a periodic signal in the terrestrial cratering record, and a search for water on the moon, are among the topics discussed. Other topics include the bidirectional reflectance properties of Fe-Ni meteorites, the nature and origin of C-rich ordinary chondrites and chondritic clasts, the dehydration kinetics of shocked serpentine, characteristics of Greenland Fe/Ni cosmic grains, electron microscopy of a hydrated interplanetary dust particle, trapping Ne, Ar, Kr, and Xe in Si2O3 smokes, gossans on Mars, and a model of the porous structure of icy satellites.

  15. An assessment of the determination of the tides and the rotation state of Ganymede with JUICE radio science experiment

    NASA Astrophysics Data System (ADS)

    Baland, Rose-Marie; Van Hoolst, Tim; Tobie, Gabriel; Dehant, Véronique

    2015-04-01

    Besides being the largest natural satellite known in the Solar System, Ganymede most likely also has the most differentiated internal structure of all satellites.Ganymede is thought to have an external water/ice layer subdivided into three sublayers: an outer ice shell, a global liquid water ocean, and a high pressure ice mantle. The presence of a water layer is supported by the possible detection of an induced magnetic field with the Galileo spacecraft. The metallic core is divided into a solid (inner core) and a liquid (outer core) part. Between the water/ice and the metallic layers, a rock mantle is expected. The JUpiter ICy moons Explorer (JUICE) mission led by ESA is planned to be launched in 2022. The spacecraft is expected to enter in orbit around Ganymede in september 2032. The Ganymede Tour will alternate elliptic and circular phases at different altitudes. The circular phases at altitudes of a few hundred kilometers are dedicated partly to the study of the internal structure such as the determination of the extent and composition of the ocean and of the surface ice shell. The payload of the spacecraft comprises the radio science package 3GM (Gravity and Geophysics of Jupiter and the Galilean Moons) that will be used to measure the Doppler effect on radio links between the orbiter and the Earth which will be affected by the gravity field of Ganymede. The gravity field of Ganymede is the sum of the static hydrostatic field (related to the secular Love number kf), of the periodically varying field due to tidal deformations (related to the tidal Love number k2 and the tidal dissipation factor Q), of the periodically varying field due to change in the rotation state (variations in the rotation rate and in the orientation of the rotation axis), and of the non-hydrostatic field that may be due to mass anomalies. The tidal and rotation parameters depend on the internal structure of the satellite (density, size, rheological properties of the different layers) in a

  16. News Conference: Physics brings the community together Training: CERN trains physics teachers Education: World conference fosters physics collaborations Lecture: Physics education live at ASE Prize: Physics teacher wins first Moore medal Festival: European presidents patronize Science on Stage festival Videoconference: Videoconference brings Durban closer to the classroom

    NASA Astrophysics Data System (ADS)

    2012-03-01

    Conference: Physics brings the community together Training: CERN trains physics teachers Education: World conference fosters physics collaborations Lecture: Physics education live at ASE Prize: Physics teacher wins first Moore medal Festival: European presidents patronize Science on Stage festival Videoconference: Videoconference brings Durban closer to the classroom

  17. News Conference: The Big Bangor Day Meeting Lecture: Charterhouse plays host to a physics day Festival: Science on Stage festival 2013 arrives in Poland Event: Scottish Physics Teachers' Summer School Meeting: Researchers and educators meet at Lund University Conference: Exeter marks the spot Recognition: European Physical Society uncovers an historic site Education: Initial teacher education undergoes big changes Forthcoming events

    NASA Astrophysics Data System (ADS)

    2013-09-01

    Conference: The Big Bangor Day Meeting Lecture: Charterhouse plays host to a physics day Festival: Science on Stage festival 2013 arrives in Poland Event: Scottish Physics Teachers' Summer School Meeting: Researchers and educators meet at Lund University Conference: Exeter marks the spot Recognition: European Physical Society uncovers an historic site Education: Initial teacher education undergoes big changes Forthcoming events

  18. News Expedition: Teachers go on extreme journey Summer School: Summer school inspires student Conference: Bristol plans science teaching festival Teacher Support: Make the most of your SPN support Conference: Schools can use latest physics Web Resource: Datamouse online project goes live Forthcoming Events

    NASA Astrophysics Data System (ADS)

    2010-01-01

    Expedition: Teachers go on extreme journey Summer School: Summer school inspires student Conference: Bristol plans science teaching festival Teacher Support: Make the most of your SPN support Conference: Schools can use latest physics Web Resource: Datamouse online project goes live Forthcoming Events

  19. Conference on Nuclear Energy and Science for the 21st Century: Atoms for Peace Plus Fifty - Washington, D.C., October 2003

    SciTech Connect

    Pfaltzgraff, Robert L

    2006-10-22

    This conference's focus was the peaceful uses of the atom and their implications for nuclear science, energy security, nuclear medicine and national security. The conference also provided the setting for the presentation of the prestigious Enrico Fermi Prize, a Presidential Award which recognizes the contributions of distinguished members of the scientific community for a lifetime of exceptional achievement in the science and technology of nuclear, atomic, molecular, and particle interactions and effects. An impressive group of distinguished speakers addressed various issues that included: the impact and legacy of the Eisenhower Administration’s “Atoms for Peace” concept, the current and future role of nuclear power as an energy source, the challenges of controlling and accounting for existing fissile material, and the horizons of discovery for particle or high-energy physics. The basic goal of the conference was to examine what has been accomplished over the past fifty years as well as to peer into the future to gain insights into what may occur in the fields of nuclear energy, nuclear science, nuclear medicine, and the control of nuclear materials.

  20. (Networking + Integrating) * (Systems + Society). Proceedings of the Annual Canadian Conference of Information Science (12th, Toronto, Ontario, May 14-16, 1984) = (Reseaux + Integration) * (Systemes + Societe). Comptes rendus de la conference annuelle Canadienne des sciences de l'information (12th, Toronto, Ontario, 14-16 mai, 1984).

    ERIC Educational Resources Information Center

    Canadian Association for Information Science, Ottawa (Ontario).

    Seventeen papers from the 1984 annual conference of the Canadian Association for Information Science (CAIS) are presented in four broad topic areas. The first group, which focuses on changing roles in information access, includes the keynote address by Charles Meadow, "Integrating Access to Information Utilities: Promises, Problems, and Profiles…

  1. The Radio JOVE Project

    NASA Astrophysics Data System (ADS)

    Garcia, L.; Thieman, J.; Higgins, C.

    1999-09-01

    Radio JOVE is an interactive educational activity which brings the radio sounds of Jupiter and the Sun to students, teachers, and the general public. This is accomplished through the construction of a simple radio telescope kit and the use of a real-time radio observatory on the Internet. Our website (http://radiojove.gsfc.nasa.gov/) will contain science information, instruction manuals, observing guides, and education resources for students and teachers. Our target audience is high school science classes, but subjects can be tailored to college undergraduate physics and astronomy courses or even to middle school science classes. The goals of the project are: 1) Educate people about planetary and solar radio astronomy, space physics, and the scientific method 2) Provide teachers and students with a hands-on radio astronomy exercise as a science curriculum support activity by building and using a simple radio telescope receiver/antenna kit 3) Create the first ever online radio observatory which provides real-time data for those with internet access 4) Allow interactions among participating schools by facilitating exchanges of ideas, data, and observing experiences. Our current funding will allow us to impact 100 schools by partially subsidizing their participation in the program. We expect to expand well beyond this number as publicity and general interest increase. Additional schools are welcome to fully participate, but we will not be able to subsidize their kit purchases. We hope to make a wide impact among the schools by advertising through appropriate newsletters, space grant consortia, the INSPIRE project (http://image.gsfc.nasa.gov/poetry/inspire/), electronic links, and science and education meetings. We would like to acknoledge support from the NASA/GSFC Director's Discretionary Fund, the STScI IDEAS grant program and the NASA/GSFC Space Science Data Operations Office.

  2. Basic space science for the benefit of developing countries. Proceedings. Conference, Lagos (Nigeria), 18 - 22 Oct 1993.

    NASA Astrophysics Data System (ADS)

    The following topics were dealt with: international cooperation in basic space science, education for space science, atmospheric science, planetary science, the Sun, binary stars, ground-based and space-based astronomical observations, and astrophysics and cosmology.

  3. Back to the future: science and technology directions for radio telescopes of the twenty-first century

    NASA Astrophysics Data System (ADS)

    Cordes, James M.

    2009-08-01

    The early days of radio astronomy showed incredibly diverse experimentation in ways to sample the electromagnetic spectrum at radio wavelengths. In addition to obtaining adequate sensitivity by building large collection areas, a primary goal also was to achieve sufficient angular resolution to localize radio sources for multi-wavelength identification. This led to many creative designs and the invention of aperture synthesis and VLBI. Some of the basic telescope types remain to the present day, now implemented across the entire radio spectrum from wavelengths of tens of meters to submillimeter wavelengths. In recent years, as always, there is still the drive for greater sensitivity but a primary goal is now to achieve very large fields of view to complement high resolution and frequency coverage, leading to a new phase of experimentation. This is the “back to the future” aspect of current research and development for next-generation radio telescopes. In this paper I summarize the scientific motivations for development of new technology and telescopes since about 1990 and going forward for the next decade and longer. Relevant elements include highly optimized telescope optics and feed antenna designs, innovative fabrication methods for large reflectors and dipole arrays, digital implementations, and hardware vs. software processing. The emphasis will be on meter and centimeter wavelength telescopes but I include a brief discussion of millimeter wavelengths to put the longer wavelength enterprises into perspective. I do not discuss submillimeter wavelengths because they are covered in other papers.

  4. USAAA Conference in Park City Utah: The Autism Epidemic a Mystery? Only if One Ignores All the Science

    ERIC Educational Resources Information Center

    Stoller, K. Paul

    2006-01-01

    This article is a synopsis of a presentation offered by the author at the recent United States Autism and Asperger Association Conference in Park City, Utah. During the USAAA conference, the author voices his concerns over the current autism epidemic. He opines that the failure of the medical profession and many governmental and other public…

  5. Evaluation of the 2012 18th Maternal and Child Health (MCH) Epidemiology and 22nd CityMatCH MCH Urban Leadership Conference: six month impact on science, program, and policy.

    PubMed

    Arellano, Danielle E; Goodman, David A; Howlette, Travis; Kroelinger, Charlan D; Law, Mark; Phillips, Donna; Jones, Jessica; Brantley, Mary D; Fitzgerald, Maureen

    2014-09-01

    The 18th Maternal and Child Health (MCH) Epidemiology and 22nd CityMatCH MCH Urban Leadership Conference took place in December 2012, covering MCH science, program, and policy issues. Assessing the impact of the Conference on attendees' work 6 months post-Conference provides information critical to understanding the impact and the use of new partnerships, knowledge, and skills gained during the Conference. Evaluation assessments, which included collection of quantitative and qualitative data, were administered at two time points: at Conference registration and 6 months post-Conference. The evaluation files were merged using computer IP address, linking responses from each assessment. Percentages of attendees reporting Conference impacts were calculated from quantitative data, and common themes and supporting examples were identified from qualitative data. Online registration was completed by 650 individuals. Of registrants, 30 % responded to the 6 month post-Conference assessment. Between registration and 6 month post-Conference evaluation, the distribution of respondents did not significantly differ by organizational affiliation. In the 6 months following the Conference, 65 % of respondents reported pursuing a networking interaction; 96 % shared knowledge from the Conference with co-workers and others in their agency; and 74 % utilized knowledge from the Conference to translate data into public health action. The Conference produced far-reaching impacts among Conference attendees. The Conference served as a platform for networking, knowledge sharing, and attaining skills that advance the work of attendees, with the potential of impacting organizational and workforce capacity. Increasing capacity could improve MCH programs, policies, and services, ultimately impacting the health of women, infants, and children. PMID:25107597

  6. Evaluation of the 2012 18th Maternal and Child Health (MCH) Epidemiology and 22nd CityMatCH MCH Urban Leadership Conference: six month impact on science, program, and policy.

    PubMed

    Arellano, Danielle E; Goodman, David A; Howlette, Travis; Kroelinger, Charlan D; Law, Mark; Phillips, Donna; Jones, Jessica; Brantley, Mary D; Fitzgerald, Maureen

    2014-09-01

    The 18th Maternal and Child Health (MCH) Epidemiology and 22nd CityMatCH MCH Urban Leadership Conference took place in December 2012, covering MCH science, program, and policy issues. Assessing the impact of the Conference on attendees' work 6 months post-Conference provides information critical to understanding the impact and the use of new partnerships, knowledge, and skills gained during the Conference. Evaluation assessments, which included collection of quantitative and qualitative data, were administered at two time points: at Conference registration and 6 months post-Conference. The evaluation files were merged using computer IP address, linking responses from each assessment. Percentages of attendees reporting Conference impacts were calculated from quantitative data, and common themes and supporting examples were identified from qualitative data. Online registration was completed by 650 individuals. Of registrants, 30 % responded to the 6 month post-Conference assessment. Between registration and 6 month post-Conference evaluation, the distribution of respondents did not significantly differ by organizational affiliation. In the 6 months following the Conference, 65 % of respondents reported pursuing a networking interaction; 96 % shared knowledge from the Conference with co-workers and others in their agency; and 74 % utilized knowledge from the Conference to translate data into public health action. The Conference produced far-reaching impacts among Conference attendees. The Conference served as a platform for networking, knowledge sharing, and attaining skills that advance the work of attendees, with the potential of impacting organizational and workforce capacity. Increasing capacity could improve MCH programs, policies, and services, ultimately impacting the health of women, infants, and children.

  7. Next conference

    NASA Astrophysics Data System (ADS)

    Hexemer, Alexander; Toney, Michael F.

    2010-11-01

    After the successful conference on Synchrotron Radiation in Polymer Science (SRPS) in Rolduc Abbey (the Netherlands), we are now looking forward to the next meeting in this topical series started in 1995 by H G Zachmann, one of the pioneers of the use of synchrotron radiation techniques in polymer science. Earlier meetings were held in Hamburg (1995), Sheffield (2002), Kyoto (2006), and Rolduc (2009). In September of 2012 the Synchrotron Radiation and Polymer Science V conferences will be organized in a joint effort by the SLAC National Accelerator Laboratory and Lawrence Berkeley National Laboratory. Stanford Linear Accelerator Laboratory Stanford Linear Accelerator Laboratory Advanced Light Source at LBL Advanced Light Source at LBL The conference will be organised in the heart of beautiful San Francisco. The program will consist of invited and contributed lectures divided in sessions on the use of synchrotron SAXS/WAXD, imaging and tomography, soft x-rays, x-ray spectroscopy, GISAXS and reflectivity, micro-beams and hyphenated techniques in polymer science. Poster contributions are more than welcome and will be highlighted during the poster sessions. Visits to both SLAC as well as LBL will be organised. San Francisco can easily be reached. It is served by two major international airports San Francisco International Airport and Oakland International Airport. Both are being served by most major airlines with easy connections to Europe and Asia as well as national destinations. Both also boast excellent connections to San Francisco city centre. We are looking forward to seeing you in the vibrant city by the Bay in September 2012. Golden gate bridge Alexander Hexemer Lawrence Berkeley National Laboratory, Advanced Light Source, Berkeley, CA 94720, USA Michael F Toney Stanford Synchrotron Radiation Lightsource, Menlo Pk, CA 94025, USA E-mail: ahexemer@lbl.gov, mftoney@slac.stanford.edu

  8. Proceedings of the Astrobiology Science Conference 2010. Evolution and Life: Surviving Catastrophes and Extremes on Earth and Beyond

    NASA Technical Reports Server (NTRS)

    2010-01-01

    The Program of the 2010 Astrobiology Science Conference: Evolution and Life: Surviving Catastrophes and Extremes on Earth and Beyond, included sessions on: 50 Years of Exobiology and Astrobiology: Greatest Hits; Extraterrestrial Molecular Evolution and Pre-Biological Chemistry: From the Interstellar Medium to the Solar System I; Human Exploration, Astronaut Health; Diversity in Astrobiology Research and Education; Titan: Past, Present, and Future; Energy Flow in Microbial Ecosystems; Extraterrestrial Molecular Evolution and Prebiological Chemistry: From the Interstellar Medium to the Solar System II; Astrobiology in Orbit; Astrobiology and Interdisciplinary Communication; Science from Rio Tinto: An Acidic Environment; Can We Rule Out Spontaneous Generation of RNA as the Key Step in the Origin of Life?; How Hellish Was the Hadean Earth?; Results from ASTEP and Other Astrobiology Field Campaigns I; Prebiotic Evolution: From Chemistry to Life I; Adaptation of Life in Hostile Space Environments; Extrasolar Terrestrial Planets I: Formation and Composition; Collaborative Tools and Technology for Astrobiology; Results from ASTEP and Other Astrobiology Field Campaigns II; Prebiotic Evolution: From Chemistry to Life II; Survival, Growth, and Evolution of Microrganisms in Model Extraterrestrial Environments; Extrasolar Terrestrial Planets II: Habitability and Life; Planetary Science Decadal Survey Update; Astrobiology Research Funding; Bioessential Elements Through Space and Time I; State of the Art in Life Detection; Terrestrial Evolution: Implications for the Past, Present, and Future of Life on Earth; Psychrophiles and Polar Environments; Life in Volcanic Environments: On Earth and Beyond; Geochronology and Astrobiology On and Off the Earth; Bioessential Elements Through Space and Time II; Origins and Evolution of Genetic Systems; Evolution of Advanced Life; Water-rich Asteroids and Moons: Composition and Astrobiological Potential; Impact Events and Evolution; A Warm, Wet

  9. Audiovisual heritage preservation in Earth and Space Science Informatics: Videos from Free and Open Source Software for Geospatial (FOSS4G) conferences in the TIB|AV-Portal.

    NASA Astrophysics Data System (ADS)

    Löwe, Peter; Marín Arraiza, Paloma; Plank, Margret

    2016-04-01

    The influence of Free and Open Source Software (FOSS) projects on Earth and Space Science Informatics (ESSI) continues to grow, particularly in the emerging context of Data Science or Open Science. The scientific significance and heritage of FOSS projects is only to a limited amount covered by traditional scientific journal articles: Audiovisual conference recordings contain significant information for analysis, reference and citation. In the context of data driven research, this audiovisual content needs to be accessible by effective search capabilities, enabling the content to be searched in depth and retrieved. Thereby, it is ensured that the content producers receive credit for their efforts within the respective communities. For Geoinformatics and ESSI, one distinguished driver is the OSGeo Foundation (OSGeo), founded in 2006 to support and promote the interdisciplinary collaborative development of open geospatial technologies and data. The organisational structure is based on software projects that have successfully passed the OSGeo incubation process, proving their compliance with FOSS licence models. This quality assurance is crucial for the transparent and unhindered application in (Open) Science. The main communication channels within and between the OSGeo-hosted community projects for face to face meetings are conferences on national, regional and global scale. Video recordings have been complementing the scientific proceedings since 2006. During the last decade, the growing body of OSGeo videos has been negatively affected by content loss, obsolescence of video technology and dependence on commercial video portals. Even worse, the distributed storage and lack of metadata do not guarantee concise and efficient access of the content. This limits the retrospective analysis of video content from past conferences. But, it also indicates a need for reliable, standardized, comparable audiovisual repositories for the future, as the number of OSGeo projects

  10. Interactive radio in the classroom: ten years of proven success.

    PubMed

    Imhoof, M

    1985-01-01

    Interactive instructional radio programming is an innovative, inexpensive, and highly effective educational tool. In interactive radio programming, lessons are provided by a radio instructor, but unlike other radio education programs, the instructor prompts responses from the radio audience, provides pauses for audience responses, and then supplies the correct response to the prompt. The lessons are generally supervised by a classroom teacher, and the students respond to the radio prompts either orally or in writing. The lessons encourage student participation, and the programs frequently require more than 100 audience responses for each 1/2 hour of radio programing. The US Agency for International Development's Office of Education in the Bureau for Science and Technology researched and developed the tool during the last 10 years, and conducted highly successful experimental projects with it in Kenya, Nicaragua, and the Dominican Republic. In September 1984 a conference, jointly sponsored by the agency and Kenya's Ministry of Education, Science, and Technology, was held in Nairobi to demonstrate the new tool and to encourage other countries to utilize the approach. Participants visited rural classrooms in Kenya where they had an opportunity to observe how the technique was being successfully used in Kenya's Radio Language Arts Project. In view of the successful results attained in the experimental projects of the 3 countries noted above, the conference participants recommended that the technique should immediately be integrated into the national curricula of these countries, and that the approach should be more widely used in other countries. They noted that the technique is especially appropriate for use in primary schools and in nonformal adult education programs and that the tool is especially useful for teaching mathematics and second languages. They recommended that educators in developing countries develop interactive instructional radio programs, evaluate

  11. ASE Annual Conference 2010

    ERIC Educational Resources Information Center

    McCune, Roger

    2010-01-01

    In this article, the author describes the ASE Annual Conference 2010 which was held at Nottingham after a gap of 22 years. As always, the main conference was preceded by International Day, an important event for science educators from across the world. There were two strands to the programme: (1) "What works for me?"--sharing new ideas and tried…

  12. Radio Journalism.

    ERIC Educational Resources Information Center

    Bittner, John R.; Bittner, Denise A.

    This book, a how-to-do-it guide for the novice and the professional alike, deals with several aspects of radio journalism: producing documentaries, preparing and announcing radio news, ethics and responsibility, regulation of radio journalism, and careers. It traces the history and growth of radio news, shows its impact on the public, and…

  13. PREFACE: III All-Russian Scientific and Practical Conference on Innovations in Non-Destructive Testing (SibTest 2015)

    NASA Astrophysics Data System (ADS)

    2016-01-01

    This issue of the journal is devoted to the research and studies presented at the III All-Russian Scientific and Practical Conference on Innovations in Non-Destructive Testing SibTest. The conference was held in Altai, Russia, on 27-31 July 2015. The conference brought together experts from different countries and organizations who had a great opportunity to share knowledge during oral and poster presentations and to initiate discussions on topics that are of interest to the conference attendees. The conference aimed to discuss innovative methods and the application of advanced technologies in non-destructive testing. The conference also attempted to bring together university, academic and industrial science, to expand the co-operation of scientists from different countries in research and development and the commercialization of innovative technologies in non-destructive testing. The key themes of the conference were: ultrasonic and acoustic testing; electromagnetic and thermal testing; various types of radiation non-destructive testing; passive and active testing techniques. The conference organizers are the Institute of Non-Destructive Testing, Tomsk Polytechnic University, with the assistance of the Russian Society for Non-Destructive Testing and Technical Diagnostics, Institute of Strength Physics and Materials Science, Siberian Branch of the Russian Academy of Sciences, National Research Tomsk State University, Moscow State Institute of Radio Engineering, Electronics and Automation.

  14. Proceedings of the Astrobiology Science Conference 2010. Evolution and Life: Surviving Catastrophes and Extremes on Earth and Beyond

    NASA Technical Reports Server (NTRS)

    2010-01-01

    The Program of the 2010 Astrobiology Science Conference: Evolution and Life: Surviving Catastrophes and Extremes on Earth and Beyond, included sessions on: 50 Years of Exobiology and Astrobiology: Greatest Hits; Extraterrestrial Molecular Evolution and Pre-Biological Chemistry: From the Interstellar Medium to the Solar System I; Human Exploration, Astronaut Health; Diversity in Astrobiology Research and Education; Titan: Past, Present, and Future; Energy Flow in Microbial Ecosystems; Extraterrestrial Molecular Evolution and Prebiological Chemistry: From the Interstellar Medium to the Solar System II; Astrobiology in Orbit; Astrobiology and Interdisciplinary Communication; Science from Rio Tinto: An Acidic Environment; Can We Rule Out Spontaneous Generation of RNA as the Key Step in the Origin of Life?; How Hellish Was the Hadean Earth?; Results from ASTEP and Other Astrobiology Field Campaigns I; Prebiotic Evolution: From Chemistry to Life I; Adaptation of Life in Hostile Space Environments; Extrasolar Terrestrial Planets I: Formation and Composition; Collaborative Tools and Technology for Astrobiology; Results from ASTEP and Other Astrobiology Field Campaigns II; Prebiotic Evolution: From Chemistry to Life II; Survival, Growth, and Evolution of Microrganisms in Model Extraterrestrial Environments; Extrasolar Terrestrial Planets II: Habitability and Life; Planetary Science Decadal Survey Update; Astrobiology Research Funding; Bioessential Elements Through Space and Time I; State of the Art in Life Detection; Terrestrial Evolution: Implications for the Past, Present, and Future of Life on Earth; Psychrophiles and Polar Environments; Life in Volcanic Environments: On Earth and Beyond; Geochronology and Astrobiology On and Off the Earth; Bioessential Elements Through Space and Time II; Origins and Evolution of Genetic Systems; Evolution of Advanced Life; Water-rich Asteroids and Moons: Composition and Astrobiological Potential; Impact Events and Evolution; A Warm, Wet

  15. CONFERENCE NOTE: Conference on Precision Electromagnetic Measurements

    NASA Astrophysics Data System (ADS)

    1991-01-01

    The next Conference on Precision Electromagnetic Measurements (CPEM), will be held from 9 to 12 June 1992 at the Centre des Nouvelles Industries et Technologies (CNIT), La Défense, Paris, France. This conference, which is held every two years and whose importance and high level, confirmed by thirty years' experience, are recognized throughout the world, can be considered as a forum in which scientists, metrologists and professionals will have the opportunity to present and compare their research results on fundamental constants, standards and new techniques of precision measurement in the electromagnetic domain. Topics The following topics are regarded as the most appropriate for this conference: realization of units and fundamental constants d.c. a.c. and high voltage time and frequency radio-frequency and microwaves dielectrics, antennas, fields lasers, fibre optics advanced instrumentation, cryoelectronics. There will also be a session on international cooperation. Conference Language The conference language will be English. No translation will be provided. Organizers Société des Electriciens et des Electroniciens (SEE). Bureau National de Métrologie (BNM) Sponsors Institute of Electrical and Electronics Engineers (IEEE) Instrumentation & Measurement Society Union Radio Scientifique Internationale United States National Institute of Standards and Technology Centre National d'Etudes des Télécommunications Mouvement Français pour la Qualité, Section Métrologie Comité National Français de Radioélectricité Scientifique Contact Jean Zara, CPEM 92 publicity, Bureau National de Métrologie, 22, rue Monge, 75005 Paris Tel.: (33) 1 46 34 48 16, Fax: (33) 1 46 34 48 63

  16. Third Lunar Science Conference.

    NASA Technical Reports Server (NTRS)

    Burlingame, A.; Burnett, D.; Doe, B.; Gault, D.; Haskin, L.; Schnoes, H.; Heymann, D.; Melson, W.; Papike, J.; Tilling, R.

    1972-01-01

    Discussion of the nature and properties of lunar rock as deduced from the examination of Apollo lunar rock samples. The topics include the lunar crust, the Fra Mauro formation, the interior of the moon, lunar chronology, surface processes, and earth-moon environment.

  17. Aerospace century XXI: Space sciences, applications, and commercial developments; Proceedings of the Thirty-third Annual AAS International Conference, Boulder, CO, Oct. 26-29, 1986

    SciTech Connect

    Morgenthaler, G.W.; Koster, J.N.

    1987-01-01

    Papers are presented on rocket UV observations of Comet Halley, a space system for microgravity research, transitioning from Spacelab to Space Station science, and assemblers and future space hardware. Also considered are spatial and temporal scales of atmospheric disturbances, Doppler radar for prediction and warning, data management for the Columbus program, communications satellites of the future, and commercial launch vehicles. Other topics include space geodesy and earthquake predictions, inverted cellular radio satellite systems, material processing in space, and potential for earth observations from the manned Space Station.

  18. Conference Summary

    NASA Astrophysics Data System (ADS)

    Ellis, R. S.

    2008-10-01

    This first Subaru international conference has highlighted the remarkably diverse and significant contributions made using the 8.2m Subaru telescope by both Japanese astronomers and the international community. As such, it serves as a satisfying tribute to the pioneering efforts of Professors Keiichi Kodaira and Sadanori Okamura whose insight and dedication is richly rewarded. Here I try to summarize the recent impact of wide field science in extragalactic astronomy and cosmology and take a look forward to the key questions we will address in the near future.

  19. The Radio Jove Project

    NASA Technical Reports Server (NTRS)

    Thieman, J. R.

    2010-01-01

    The Radio love Project is a hands-on education and outreach project in which students, or any other interested individuals or groups build a radio telescope from a kit, operate the radio telescope, transmit the resulting signals through the internet if desired, analyze the results, and share the results with others through archives or general discussions among the observers. Radio love is intended to provide an introduction to radio astronomy for the observer. The equipment allows the user to observe radio signals from Jupiter, the Sun, the galaxy, and Earth-based radiation both natural and man-made. The project was started through a NASA Director's Discretionary Fund grant more than ten years ago. it has continued to be carried out through the dedicated efforts of a group of mainly volunteers. Dearly 1500 kits have been distributed throughout the world. Participation can also be done without building a kit. Pre-built kits are available. Users can also monitor remote radio telescopes through the internet using free downloadable software available through the radiosky.com website. There have been many stories of prize-winning projects, inspirational results, collaborative efforts, etc. We continue to build the community of observers and are always open to new thoughts about how to inspire the observers to still greater involvement in the science and technology associated with Radio Jove.

  20. Nanodust detection near 1 AU from spectral analysis of Cassini/Radio and Plasma Wave Science data

    NASA Astrophysics Data System (ADS)

    Schippers, P.; Meyer-Vernet, N.; Lecacheux, A.; Kurth, W. S.; Mitchell, D. G.; André, N.

    2014-08-01

    Nanodust grains of a few nanometers in size are produced near the Sun by collisional breakup of larger grains and picked up by the magnetized solar wind. They have so far been detected at 1 AU by only the two STEREO spacecraft. Here we analyze the spectra measured by the radio and plasma wave instrument onboard Cassini during the cruise phase close to Earth orbit; they exhibit bursty signatures similar to those observed by the same instrument in association with nanodust stream impacts on Cassini near Jupiter. The observed wave level and spectral shape reveal impacts of nanoparticles at about 300 km/s, with an average flux compatible with that observed by the radio and plasma wave instrument onboard STEREO and with the interplanetary flux models.

  1. The Roles of Science and Technology in General and Continuing Education. Proceedings of the Conference of the Association of American Colleges (Washington, District of Columbia, December 16-18, 1979).

    ERIC Educational Resources Information Center

    Association of American Colleges, Washington, DC.

    This conference focused on issues and topics related to the roles of science and technology in general and continuing education. The keynote address is entitled "Technology Transfer to the Third World: The Critical U.S. Challenge for the Eighties" (William Eilers). The section on perspectives on the public understanding of science includes the…

  2. Acquisition and Utilization of Japanese Information in Science, Technology and Commerce in Europe and USA : Report on the International Conference on Japanese Information at the University of Warwick

    NASA Astrophysics Data System (ADS)

    Miyakawa, Takayasu; Miwa, Makiko; Kanda, Toshihiko

    Report on the International Conference on Japanese Information in Science, Technology and Commerce which was organized by the British Library, being supported by NTIS and JICST, at the University of Warwick on 1-4 September 1987. Topics discussed include, US policy on Japanese information, EEC/Japan-Info Project, various private initiatives, language barrier and translation, education of Japanese language and personnel exchange programme, quality and usage of Japanese secondary materials, original document delivery, Japanese produced databases and foreign access to them, requests upon JICST and other Japanese information services.

  3. The 8th international symposium on the breast: Using next-generation science to understand the normal breast and the development of breast cancer- conference report.

    PubMed

    Gomberawalla, Ameer; Love, Susan

    2015-12-01

    Dr. Susan Love Research Foundation is committed to performing and advancing research that will lead to the discovery of what causes cancer to develop in the human breast. As part of this effort, the Foundation hosted the 8th International Symposium on the Breast in Santa Monica, Calif., Feb. 19 to Feb. 21, 2015. More than 120 forward-thinking clinical researchers, epidemiologists, pathologists, basic scientists, translational investigators, and breast cancer advocates from six countries attended this year's conference, "Using Next Generation Science to Understand the Normal Breast and the Development of Cancer." The highlights from this year's symposium are summarized in this report.

  4. [26th Conference of the Spanish Society of Quality in Healthcare: a good balance between quality, innovation, science and participation].

    PubMed

    Astier-Peña, M P; Barrasa-Villar, I; García-Mata, J R; Aranaz-Andrés, J; Enriquez-Martín, N; Vela-Marquina, M L

    2010-01-01

    The experience and learning process of preparing a scientific conference programme, organising and conducting a conference ccompletes the quality circle with the quantitative and qualitative assessment of the process and results. The transmission of this experience and learning process through this paper will improve the performance of committees of future conference venues, partners and participants and collaborators. The method for performing this evaluation is the assessment of the activities of both the scientific and organising committees of the XXVI Conference of the Spanish Society of Quality Healthcare in October 2008 in Zaragoza. The methodology evaluated the observance of the timetable and tasks assigned to the committees in the Congress Manual of the society along with the presentation of final results of the congress concerning scientific participation and overall satisfaction. There were a total of 1211 communications with a rejection rate of 9.1%. Of the total, 577 communications were presented in oral format and 544 in poster format. Aragon was the community of origin of 24% of communications. By subject areas, those of most interest were patient safety, organisational and management processes, and patient perspectives. A total of 83 participants attended 7 of the 11 workshops offered. The average attendance for each workshop was 12 people. The response rate to the assessment of workshops questionnaire was 54.2% with an average score of 4 (scale of 1 to 5). A total of 1131 people attended the conference of which 17% (193) were SECA associates. Out of a total of 1075 overall satisfaction conference questionnaires distributed there was a response rate of 9.30% (100). The scientific content was assessed with an average score of 3.6 and the organization with 3.87, both on a total score of 5 points. According to the number of abstracts received, number of conferences, level of satisfaction with the scientific program and organisation, we can conclude that

  5. Early Experience and Visual Information Processing in Perceptual and Reading Disorders; Proceedings of a Conference Held October 27-30, 1968, at Lake Mohonk, New York, in Association with the Committee on Brain Sciences, Div. of Medical Sciences, National Research Council.

    ERIC Educational Resources Information Center

    Young, Francis A., Ed.; Lindsley, Donald B., Ed.

    This book brings together papers presented at a conference on early experience and visual information processing in perceptual and reading disorders sponsored by the National Academy of Sciences. The goal of the conference was to integrate basic knowledge of structure and mechanisms of eye and brain with their function and their behavioral roles…

  6. Proceedings of the SEPACS/SU Conferences in Science Education. (Pennsylvania, September 24, 1983, and November 19, 1983).

    ERIC Educational Resources Information Center

    Grezlak, John H., Ed.

    Two conferences were organized by the Education Committee of the Southeastern Pennsylvania Section of the American Chemical Society (SEPACS) with the assistance of Shippensburg University (SU) to examine the nature and depth of the growing trend of scientific and technological illiteracy in southeastern Pennsylvania and to propose and effect…

  7. Proceedings of the U.S. Geological Survey Eighth Biennial Geographic Information Science Workshop and first The National Map Users Conference, Denver, Colorado, May 10-13, 2011

    USGS Publications Warehouse

    Sieverling, Jennifer B.; Dietterle, Jeffrey

    2014-01-01

    The U.S. Geological Survey (USGS) is sponsoring the first The National Map Users Conference in conjunction with the eighth biennial Geographic Information Science (GIS) Workshop on May 10-13, 2011, in Lakewood, Colorado. The GIS Workshop will be held at the USGS National Training Center, located on the Denver Federal Center, Lakewood, Colorado, May 10-11. The National Map Users Conference will be held directly after the GIS Workshop at the Denver Marriott West, a convention hotel in the Lakewood, Colorado area, May 12-13. The National Map is designed to serve the Nation by providing geographic data and knowledge for government, industry, and public uses. The goal of The National Map Users Conference is to enhance communications and collaboration among the communities of users of and contributors to The National Map, including USGS, Department of the Interior, and other government GIS specialists and scientists, as well as the broader geospatial community. The USGS National Geospatial Program intends the conference to serve as a forum to engage users and more fully discover and meet their needs for the products and services of The National Map. The goal of the GIS Workshop is to promote advancement of GIS and related technologies and concepts as well as the sharing of GIS knowledge within the USGS GIS community. This collaborative opportunity for multi-disciplinary GIS and associated professionals will allow attendees to present and discuss a wide variety of geospatial-related topics. The Users Conference and Workshop collaboration will bring together scientists, managers, and data users who, through presentations, posters, seminars, workshops, and informal gatherings, will share accomplishments and progress on a variety of geospatial topics. During this joint event, attendees will have the opportunity to present or demonstrate their work; to develop their knowledge by attending hands-on workshops, seminars, and presentations given by professionals from USGS and

  8. Major Conference about Astronomical Technology in Munich

    NASA Astrophysics Data System (ADS)

    2000-03-01

    Press Conference on Monday, March 27, 2000 Which are the latest astronomical discoveries made with the new 8-10 metre class astronomical telescopes? Will it be possible to construct even more powerful instruments on the ground and in space to explore the near and distant Universe at all wavelengths from gamma-rays to radio waves? Which research areas in this dynamical science are likely to achieve break-throughs with emerging new technologies? These are some of the central themes that will be discussed by more than 600 specialists from all over the world at an international conference in Munich (Germany), "Astronomical Telescopes and Instruments 2000" , beginning on Monday, March 27, 2000. During five days, the modern architecture of the new International Congress Center in the Bavarian capital will be the scene of lively exchanges about recent progress at the world's top-class astronomical research facilities and the presentation of inspired new ideas about future technological opportunities. The conference will be accompanied by numerous on-site exhibition stands by the major industries and research organisations in this wide field. This meeting is the latest in a series, organised every second year, alternatively in the USA and Europe by the International Society for Optical Engineering (SPIE) , this year with the European Southern Observatory (ESO) as co-sponsor and host institution. The conference will be opened in the morning of March 27 by the Bavarian Minister of Science, Research and Arts, Hans Zehetmair . His address will be followed by keynote speeches by Massimo Tarenghi (European Southern Observatory), James B. Breckenridge (National Science Foundation, USA), Harvey Butcher (Netherlands Foundation for Research in Astronomy) and Albrecht Ruediger (Max Planck Institut für Quantenoptik, Germany). The conference is subtitled "Power Telescopes and Instrumentation into the New Millennium" and will be attended by leading scientists and engineers from all

  9. Conference summary

    NASA Astrophysics Data System (ADS)

    Rebolo, R.

    ``Brown dwarfs come of age" was a stimulating conference attended by a large number of very active researchers, including many young students and post-docs who were largely responsible for the lively atmosphere that we enjoyed during the full meeting. Major theoretical and observational challenges currently faced in the study of brown dwarfs were reviewed. Key spectroscopic work is being conducted to determine atmospheric temperatures, surface gravities and metallicities, essential to understand the evolution of substellar objects. Research on ultracool atmospheres is extended down to temperatures typical of the atmosphere of the Earth. Characterisation of brown dwarfs at all wavelengths from X-ray to radio is ongoing and investigation of time domain phenomena reveal interesting new processes in cool atmospheres. In addition to talks on these topics, a large number of presentations addressed the formation and evolution of brown dwarfs, the lower end of the Initial Mass Function, the properties of substellar binaries, the angular momentum and disk evolution in very low-mass systems, results of large scale surveys aimed to find the lowest luminosity and coolest brown dwarfs, searches in star clusters delineating the evolution with age of the properties of brown dwarfs, binary searches and subsequent follow-up work enabling dynamical mass determinations. The excellent level of the review talks, oral and poster presentations and the work of the enthusiastic researchers that attended the meeting ensure a brilliant future for substellar research 18 years after the discovery of the first brown dwarfs.

  10. Radio science with voyager 2 at saturn: atmosphere and ionosphere and the masses of mimas, tethys, and iapetus.

    PubMed

    Tyler, G L; Eshleman, V R; Anderson, J D; Levy, G S; Lindal, G F; Wood, G E; Croft, T A

    1982-01-29

    Voyager 2 radio occultation measurements of Saturn's atmosphere probed to the 1.2-bar pressure level, where the temperature was 143 +/- 6 K and the lapse rate apparently equaled the dry adiabatic value of 0.85 K per kilometer. The tropopause at both mid-latitude occultation locations (36.5 degrees N and 31 degrees S) was at a pressure level of about 70 millibars and a temperature of approximately 82 K. The stratospheric structures were very similar with the temperature rising to about 140 K at the 1-millibar pressure level. The peak electron concentrations sensed were 1.7 x 10(4) and 0.64 x 10(4) per cubic centimeter in the predawn (31 degrees S) and late afternoon (36.5 degrees N) locations. The topside plasma scale heights were about 1000 kilometers for the late afternoon profile, and 260 kilometers for the lower portions and 1100 kilometers for the upper portions of the topside predawn ionosphere. Radio measurements of the masses of Tethys and Iapetus yield (7.55 +/- 0.90) x 10(20) and (18.8 +/- 1.2) x 10(20) kilograms respectively; the Tethys-Mimas resonance theory then provides a derived mass for Afimas of (0.455 +/- 0.054) x 10(20) kilograms. These values for Tethys and Mimas represent major increases from previously accepted ground-based values, and appear to reverse a suggested trend of increasing satellite density with orbital radius in the Saturnian system. Current results suggest the opposite trend, in which the intermediate-sized satellites of Saturn may represent several classes of objects that differ with respect to the relative amounts of water, ammonia, and methane ices incorporated at different temperatures during formation. The anomalously low density of lapetus might then be explained as resulting from a large hydrocarbon content, and its unusually dark surface markings as another manifestation of this same material.

  11. PREFACE: XVII International Scientific Conference ''RESHETNEV READINGS''

    NASA Astrophysics Data System (ADS)

    2015-01-01

    The International Scientific Conference ''RESHETNEV READINGS'' is dedicated to the memory of Mikhail Reshetnev, an outstanding scientist, chief-constructor of space-rocket systems and communication satellites. The current volume represents selected proceedings of the main conference materials which were published by XVII International Scientific Conference ''RESHETNEV READINGS'' held on November 12 - 14, 2013. Plenary sessions, round tables and forums will be attended by famous scientists, developers and designers representing the space technology sector, as well as professionals and experts in the IT industry. A number of outstanding academic figures expressed their interest in an event of such a level including Jaures Alferov, Vice-president of the Russian Academy of Sciences (RAS), Academician of RAS, Nobel laureate, Dirk Bochar, General Secretary of the European Federation of National Engineering Associates (FEANI), Prof. Yuri Gulyaev, Academician of RAS, Member of the Presidium of RAS, President of the International Union of Scientific and Engineering Associations, Director of the Institute of Radio Engineering and Electronics of RAS, as well as rectors of the largest universities in Russia, chief executives of well-known research enterprises and representatives of big businesses. We would like to thank our main sponsors such as JSC ''Reshetnev Information Satellite Systems'', JSC ''Krasnoyarsk Engineering Plant'', Central Design Bureau ''Geophysics'', Krasnoyarsk Region Authorities. These enterprises and companies are leading ones in the aerospace branch. It is a great pleasure to cooperate and train specialists for them.

  12. A Practitioner's Guide to Science-Based Prevention: A Handbook of Promising, Effective and Model Programs. 2002 Conference Edition.

    ERIC Educational Resources Information Center

    Schinke, Steven

    The importance of science-based programs is now widely acknowledged in the substance abuse prevention field. The Center for Substance Abuse Prevention (CSAP) continues its efforts on several fronts to inform the field of the existence and availability of science-based program options. It primarily does this through its National Registry of…

  13. Perspectives on U.S. Competitiveness in Science and Technology. Conference Proceedings (Washington, DC, November 8, 2006)

    ERIC Educational Resources Information Center

    Galama, Titus, Ed.; Hosek, James, Ed.

    2007-01-01

    Concern has grown that the United States is losing its competitive edge in science and technology (S&T). The factors driving this concern include globalization, the rise of science centers in developing countries such as China and India, the increasing number of foreign-born Ph.D. students in the United States, and claims of a shortage of S&T…

  14. Proceedings of the Annual Conference of the Western Australian Science Education Association (23rd, Perth, Western Australia, November 13, 1998).

    ERIC Educational Resources Information Center

    Rennie, Leonie, Ed.

    These proceedings contain reviewed and edited papers from the 23rd annual meeting of the Western Australian Science Education Association (WASEA). Papers include: (1) Using Quantitative and Qualitative Approaches to Validate a Questionnaire to Describe Science Teacher Behavior in Taiwan and Australia (Darrell Fisher, David Henderson, and…

  15. The many facets of extragalactic radio surveys: towards new scientific challenges

    NASA Astrophysics Data System (ADS)

    2015-10-01

    Radio continuum surveys are a powerful tool to detect large number of objects over a wide range of redshifts and obtain information on the intensity, polarization and distribution properties of radio sources across the sky. They are essential to answer to fundamental questions of modern astrophysics. Radio astronomy is in the midst of a transformation. Developments in high-speed digital signal processing and broad-band optical fibre links between antennas have enabled significant upgrades of the existing radio facilities (e-MERLIN, JVLA, ATCA-CABB, eEVN, APERTIF), and are leading to next-generation radio telescopes (LOFAR, MWA, ASKAP, MeerKAT). All these efforts will ultimately lead to the realization of the Square Kilometre Array (SKA), which, owing to advances in sensitivity, field-of-view, frequency range and spectral resolution, will yield transformational science in many astrophysical research fields. The purpose of this meeting is to explore new scientific perspectives offered by modern radio surveys, focusing on synergies allowed by multi-frequency, multi-resolution observations. We will bring together researchers working on wide aspects of the physics and evolution of extra-galactic radio sources, from star-forming galaxies to AGNs and clusters of galaxies, including their role as cosmological probes. The organization of this conference has been inspired by the recent celebration of the 50th anniversary of the Northern Cross Radio Telescope in Medicina (BO), whose pioneering B2 and B3 surveys provided a significant contribution to radio astronomical studies for many decades afterwards. The conference was organized by the Istituto di Radioastronomia (INAF), and was held at the CNR Research Area in Bologna, on 20-23 October 2015. This Conference has received support from the following bodies and funding agencies: National Institute for Astrophysics (INAF), ASTRON, RadioNet3 (through the European Union’s Seventh Framework Programme for research

  16. Research in Science Education, Volume 15. Selections of Papers from the Annual Conference of the Australian Science Education Research Association (16th, Rockhampton, Queensland, Australia, May 1985).

    ERIC Educational Resources Information Center

    Tisher, Richard P., Ed.

    1985-01-01

    This publication contains 24 studies which focus on: the fostering of inquiry in secondary school science laboratories; realistic expectations for traditional laboratory work; a content-based, college-level science course for all students; understanding learning at the classroom level; transitions and student task involvement; a project to…

  17. Radio wave.

    PubMed

    Elkin, V

    1992-01-01

    In developing countries with high rates of poverty and illiteracy, radio is emerging as an excellent medium for delivering information on health issues, family planning, nutrition, and agricultural development. Since radio does not require wired electricity, it can reach remote rural populations. Surveys have found that between 50-75% of poor rural households in developing countries own radios, and the majority listen to educational radio at least once a week. A program that reaches the urban poor outside of Lima, Peru, has been instrumental in controlling the spread of cholera. A Bolivian station broadcasts 8 hours of literacy, health, agricultural, and cultural programming a day to an audience of more than 2 million Aymara Indians. Small village radio stations with a broadcast range of 15 miles can be established for under US$400 and can generally achieve sustainability through local fundraising events such as raffles. In many cases, listeners have become broadcasters at their local radio stations.

  18. Radio sociology

    NASA Astrophysics Data System (ADS)

    Swenson, George W., Jr.

    1996-04-01

    A work was conducted, using radio telemetry, to locate a migrating, radio-tagged, sharp-shinned hawk. The hawk was monitored through the noise radiation it created. The hawk was found. During this study, it was found that the concentration of population corresponds with areas of increased noise temperature. Through this study, a bigger study was planned. The study would involved the relationship between a place's radiation signature and its other attributes, such as economic type, population, geographic concentration. The method of radio sociology would be used to track the sources of radio noise.

  19. Radio science with voyager at jupiter: initial voyager 2 results and a voyager 1 measure of the io torus.

    PubMed

    Eshleman, V R; Tyler, G L; Wood, G E; Lindal, G F; Anderson, J D; Levy, G S; Croft, T A

    1979-11-23

    Voyager 2 radio signals were observed essentially continuously during a grazing occultation of the spacecraft by the southern limb of Jupiter. Intensity data show a classic atmospheric occultation profile and the effects of turbulence and ionospheric focusing and defocusing. No reliable profile of the neutral atmosphere has yet been obtained, primarily because of a combination of large trajectory uncertainties and error multiplication effects associated with the grazing geometry of the Voyager 2 occultation. Analysis of the dispersive ionospheric refraction data yields preliminary profiles for the topside ionosphere at 66.7 degrees S (entry in the evening) and 50.1 degrees S (exit in the morning) that are reversed with respect to corresponding Voyager 1 profiles in terms of plasma concentration at a fixed altitude. Plasma scale heights and temperatures of 880 kilometers, 1200 K and 1040 kilometers, 1600 K were obtained for morning and evening conditions, respectively. Preliminary reduction of the pre-encounter occultation of Voyager 1 by the Io torus yields an average plasma density of about 1000 electrons per cubic centimeter.

  20. 47 CFR 1.956 - Settlement conferences.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... 47 Telecommunication 1 2011-10-01 2011-10-01 false Settlement conferences. 1.956 Section 1.956 Telecommunication FEDERAL COMMUNICATIONS COMMISSION GENERAL PRACTICE AND PROCEDURE Wireless Radio Services Applications and Proceedings Application Requirements and Procedures § 1.956 Settlement conferences....

  1. 47 CFR 76.8 - Status conference.

    Code of Federal Regulations, 2012 CFR

    2012-10-01

    ... 47 Telecommunication 4 2012-10-01 2012-10-01 false Status conference. 76.8 Section 76.8 Telecommunication FEDERAL COMMUNICATIONS COMMISSION (CONTINUED) BROADCAST RADIO SERVICES MULTICHANNEL VIDEO AND CABLE TELEVISION SERVICE General § 76.8 Status conference. (a) In any proceeding subject to the part...

  2. 47 CFR 76.8 - Status conference.

    Code of Federal Regulations, 2010 CFR

    2010-10-01

    ... 47 Telecommunication 4 2010-10-01 2010-10-01 false Status conference. 76.8 Section 76.8 Telecommunication FEDERAL COMMUNICATIONS COMMISSION (CONTINUED) BROADCAST RADIO SERVICES MULTICHANNEL VIDEO AND CABLE TELEVISION SERVICE General § 76.8 Status conference. (a) In any proceeding subject to the part...

  3. 47 CFR 76.8 - Status conference.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ... 47 Telecommunication 4 2014-10-01 2014-10-01 false Status conference. 76.8 Section 76.8 Telecommunication FEDERAL COMMUNICATIONS COMMISSION (CONTINUED) BROADCAST RADIO SERVICES MULTICHANNEL VIDEO AND CABLE TELEVISION SERVICE General § 76.8 Status conference. (a) In any proceeding subject to the part...

  4. 47 CFR 76.8 - Status conference.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ... 47 Telecommunication 4 2013-10-01 2013-10-01 false Status conference. 76.8 Section 76.8 Telecommunication FEDERAL COMMUNICATIONS COMMISSION (CONTINUED) BROADCAST RADIO SERVICES MULTICHANNEL VIDEO AND CABLE TELEVISION SERVICE General § 76.8 Status conference. (a) In any proceeding subject to the part...

  5. 47 CFR 76.8 - Status conference.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... 47 Telecommunication 4 2011-10-01 2011-10-01 false Status conference. 76.8 Section 76.8 Telecommunication FEDERAL COMMUNICATIONS COMMISSION (CONTINUED) BROADCAST RADIO SERVICES MULTICHANNEL VIDEO AND CABLE TELEVISION SERVICE General § 76.8 Status conference. (a) In any proceeding subject to the part...

  6. Radio stars.

    PubMed

    Hjellming, R M; Wade, C M

    1971-09-17

    Up to the present time six classes of radio stars have been established. The signals are almost always very faint and drastically variable. Hence their discovery has owed as much to serendipity as to the highly sophisticated equipment and techniques that have been used. When the variations are regular, as with the pulsars, this characteristic can be exploited very successfully in the search for new objects as well as in the detailed study of those that are already known. The detection of the most erratically variable radio stars, the flare stars and the x-ray stars, is primarily a matter of luck and patience. In the case of the novas, one at least knows where and oughly when to look for radio emission. A very sensitive interferometer is clearly the best instrument to use in the initial detection of a radio star. The fact that weak background sources are frequently present makes it essential to prove that the position of a radio source agrees with that of a star to within a few arc seconds. The potential of radio astronomy for the study of radio stars will not be realized until more powerful instruments than those that are available today can be utilized. So far, we have been able to see only the most luminous of the radio stars. PMID:17836594

  7. College Radio.

    ERIC Educational Resources Information Center

    Sauls, Samuel J.

    As with commercial stations, the underlying premise of the college radio station is to serve the community, whether it be the campus community or the community at large, but in unique ways often geared to underserved niches of the population. Much of college radio's charm lies in its unpredictable nature and constant mutations. The stations give…

  8. Radio Astronomy

    NASA Technical Reports Server (NTRS)

    Shaffer, R. D.; Wolken, P. R.; Niell, A. E.

    1981-01-01

    The activities of the DSN in support of Radio and Radar Astronomy Operations during September through December 1980 are described. Emphasis is on a report of an experiment selected for use of the DSN by the radio Astronomy Experiment Selection Panel: that of VLBI observations of the energetic galactic object SS-433.

  9. Radio astronomy

    NASA Technical Reports Server (NTRS)

    Wolken, P. R.; Schaffer, R. D.; Gorenstein, M. V.

    1981-01-01

    The activities of the Deep Space Network in support of Radio Astronomy Operations during April and May 1981 are reported. Work in progres in support of an experiment selected for use of the DSN by the Radio Astronomy Experiment Selection Panel, Twin Quasi-Stellar Object VLBI, is reported.

  10. Radio astronomy

    NASA Technical Reports Server (NTRS)

    Shaffer, R. D.; Wolken, P. R.; Gulkis, S.

    1981-01-01

    The activities of the Deep Space Network in support of radio astronomy operations during the first quarter of 1981 are reported. Results of the use of a low noise maser are presented, as well as updates in DSN support of experiments sanctioned by the Radio Astronomy Experiment Selection Panel.

  11. Radio astronomy

    NASA Technical Reports Server (NTRS)

    Taylor, R. M.; Manchester, R. N.

    1980-01-01

    The activities of the Deep Space Network in support of radio and radar astronomy operations during July and August 1980 are reported. A brief update on the OSS-sponsored planetary radio astronomy experiment is provided. Also included are two updates, one each from Spain and Australia on current host country activities.

  12. Radio stars.

    PubMed

    Hjellming, R M; Wade, C M

    1971-09-17

    Up to the present time six classes of radio stars have been established. The signals are almost always very faint and drastically variable. Hence their discovery has owed as much to serendipity as to the highly sophisticated equipment and techniques that have been used. When the variations are regular, as with the pulsars, this characteristic can be exploited very successfully in the search for new objects as well as in the detailed study of those that are already known. The detection of the most erratically variable radio stars, the flare stars and the x-ray stars, is primarily a matter of luck and patience. In the case of the novas, one at least knows where and oughly when to look for radio emission. A very sensitive interferometer is clearly the best instrument to use in the initial detection of a radio star. The fact that weak background sources are frequently present makes it essential to prove that the position of a radio source agrees with that of a star to within a few arc seconds. The potential of radio astronomy for the study of radio stars will not be realized until more powerful instruments than those that are available today can be utilized. So far, we have been able to see only the most luminous of the radio stars.

  13. Emerging Frameworks and Methods. Proceedings of the International Conference on Conceptions of Library and Information Science (CoLIS4) (4th, Seattle, Washington, July 21-25, 2002).

    ERIC Educational Resources Information Center

    Bruce, Harry, Ed.; Fidel, Raya, Ed.; Ingwersen, Peter, Ed.; Vakkari, Pertti, Ed.

    These proceedings are the fourth in the series of international conferences whose general aim is to provide a broad forum for critically exploring and analyzing library and information science as a discipline and as a field of research from historical, theoretical, philosophical, and empirical perspectives. The papers in this volume cover a wide…

  14. The Place of the Liberal Arts and Sciences in the Curriculum: A Renewed Commitment. Proceedings of a Conference Sponsored by the State Council of Higher Education for Virginia (Richmond, Virginia, December 17-18, 1984).

    ERIC Educational Resources Information Center

    Potter, David L., Ed.

    Proceedings of a conference on Virginia's undergraduate curriculum are presented. Attention is focused on the future of the traditional arts and sciences disciplines. Contents include: (1) a keynote address on benefits of studying the humanities, along with answers to audience questions (William H. Bennett, head of the National Endowment for the…

  15. Youth in Transition: The Challenges of Generational Change in Asia. Proceedings of the Biennial General Conference of the Association of Asian Social Science Research Councils (15th, Canberra, Australia, 2005)

    ERIC Educational Resources Information Center

    Gale, Fay, Ed.; Fahey, Stephanie, Ed.

    2005-01-01

    This book originates from a conference of the Association of Asian Social Science Research Councils and contains writings and research reports on Youth in Transition in the Asia and Pacific region. The definition of "youth" varies from country to country and ranges between the ages of 10 to 35. The publication summarizes issues in the region,…

  16. PREFACE: International Symposium on Materials Science and Innovation for Sustainable Society - Eco-Materials and Eco-Innovation for Global Sustainability - The 21st Iketani Conference 2011

    NASA Astrophysics Data System (ADS)

    Takahashi, Yasuo

    2012-08-01

    Conference logo The 21st century has been called the century of environmental revolution. Green innovations and environmentally friendly production systems based on physics, chemistry, materials science, and electronic engineering will be indispensable for ensuring renewable energy and establishing a sustainable society. In particular, production design, materials processing, and fabrication technologies such as welding and joining will be very important components of such green innovations. For these reasons, the International Symposium on Materials Science and Innovation for Sustainable Society - eco-materials and eco-innovation for global sustainability - (ECO-MATES 2011) was organized by the Joining and Welding Research Institute (JWRI) and the Center of Environmental Innovation Design for Sustainability (CEIDS), Osaka University. ECO-MATES 2011 was held at Hotel Hankyu Expo Park, Osaka, Japan from 28-30 November 2011. 435 participants from 20 countries around the world attended the symposium. 149 oral presentations including 60 invited talks and 160 posters were presented at the symposium to discuss the latest research and developments in green innovations in relation to environmental issues. The topics of the symposium covered all environmentally related fields including renewable energy, energy-materials, environment and resources, waste and biomass, power electronics, semiconductor, rare-earth metals, functional materials, organic electronics materials, electronics packaging, smart processing, joining and welding, eco-efficient processes, and green applied physics and chemistry. Therefore, 55 full papers concerning green innovations and environmentally benign production were selected and approved by the editorial board and the program committee of ECO-MATES 2011. All papers were accepted through peer review processes. I believe that all the papers have many informative contents. On behalf of the steering committee of the symposium, I would like to express

  17. News Education: Physics Education Networks meeting has global scale Competition: Competition seeks the next Brian Cox Experiment: New measurement of neutrino time-of-flight consistent with the speed of light Event: A day for all those who teach physics Conference: Students attend first Anglo-Japanese international science conference Celebration: Will 2015 be the 'Year of Light'? Teachers: Challenging our intuition in spectacular fashion: the fascinating world of quantum physics awaits Research: Science sharpens up sport Learning: Kittinger and Baumgartner: on a mission to the edge of space International: London International Youth Science Forum calls for leading young scientists Competition: Physics paralympian challenge needs inquisitive, analytical, artistic and eloquent pupils Forthcoming events

    NASA Astrophysics Data System (ADS)

    2012-05-01

    Education: Physics Education Networks meeting has global scale Competition: Competition seeks the next Brian Cox Experiment: New measurement of neutrino time-of-flight consistent with the speed of light Event: A day for all those who teach physics Conference: Students attend first Anglo-Japanese international science conference Celebration: Will 2015 be the 'Year of Light'? Teachers: Challenging our intuition in spectacular fashion: the fascinating world of quantum physics awaits Research: Science sharpens up sport Learning: Kittinger and Baumgartner: on a mission to the edge of space International: London International Youth Science Forum calls for leading young scientists Competition: Physics paralympian challenge needs inquisitive, analytical, artistic and eloquent pupils Forthcoming events

  18. ConfChem Conference on Flipped Classroom: Time-Saving Resources Aligned with Cognitive Science to Help Instructors

    ERIC Educational Resources Information Center

    Hartman, JudithAnn R.; Dahm, Donald J.; Nelson, Eric A.

    2015-01-01

    Studies in cognitive science have verified that working memory (where the brain solves problems) can manipulate nearly all elements of knowledge that can be recalled automatically from long-term memory, but only a few elements that have not previously been well memorized. Research in reading comprehension has found that "lecture notes with…

  19. Radio Telescopes

    NASA Astrophysics Data System (ADS)

    Ekers, Ron; Wilson, Thomas L.

    ``Radio Telescopes" starts with a brief historical introduction from Jansky's1931 discovery of radio emission from the Milky Way through the development ofradio telescope dishes and arrays to aperture synthesis imaging. It includessufficient basics of electromagnetic radiation to provide some understanding of thedesign and operation of radio telescopes. The criteria such as frequencyrange, sensitivity, survey speed, angular resolution, and field of view thatdetermine the design of radio telescopes are introduced. Because it is soeasy to manipulate the electromagnetic waves at radio frequencies, radiotelescopes have evolved into many different forms, sometimes with "wire"structures tuned to specific wavelengths, which look very different from anykind of classical telescope. To assist astronomers more familiar with otherwavelength domains, the appendix A.1. includes a comparison of radioand optical terminology. Some of the different types of radio telescopesincluding the filled aperture dishes, electronically steered phased arrays, andaperture synthesis radio telescopes are discussed, and there is a sectioncomparing the differences between dishes and arrays. Some of the morerecent developments including hierarchical beam forming, phased arrayfeeds, mosaicing, rotation measure synthesis, digital receivers, and longbaseline interferometers are included. The problem of increasing radiofrequency interference is discussed, and some possible mitigation strategies areoutlined.

  20. Research in Science Education. Volume 14. Selections of Papers from the Annual Conference of the Australian Science Education Research Association (15th, Victoria, Australia, May 1984).

    ERIC Educational Resources Information Center

    Tisher, Richard P., Ed.

    1984-01-01

    This publication contains studies which focus on students' science concepts and the alternative frameworks they use to interpret natural phenomena. Among the specific areas investigated are: conceptions held by Year 11 chemistry students about stoichiometry; how some 9-year-old students interpret the word "solid" to mean hard, unbreakable,…

  1. IATUL Conference 1985.

    ERIC Educational Resources Information Center

    Information Services and Use, 1985

    1985-01-01

    Summarizes presentations at conference on theme "The future of information resources for science and technology and role of libraries": industrial and commercial use of national, regional, and university resources; balance between public- and private-sector resources; local access in national and regional context; access to information in…

  2. Radio Astronomy

    NASA Technical Reports Server (NTRS)

    Wolken, P. R.; Shaffer, R. D.

    1983-01-01

    Deep Space Network (DSN) 26- and 64-meter antenna stations were utilized in support of Radio Astronomy Experiment Selection Panel experiments. Within a time span of 10 days, in May 1983 (267.75 hours total), nine RAES experiments were supported. Most of these experiments involved multifacility interferometry using Mark 3 data recording terminals and as many as six non-DSN observatories. Investigations of black holes, quasars, galaxies, and radio sources are discussed.

  3. USGS Gulf Coast Science Conference and Florida Integrated Science Center Meeting: Proceedings with Abstracts, October 20-23, 2008, Orlando, Florida

    USGS Publications Warehouse

    Edited and compiled by Lavoie, Dawn; Rosen, Barry; Sumner, Dave; Haag, Kim; Tihansky, Ann; Boynton, Betsy; Koenig, Renee

    2008-01-01

    Welcome! The USGS is the Nation's premier source of information in support of science-based decision making for resource management. We are excited to have the opportunity to bring together a diverse array of USGS scientists, managers, specialists, and others from science centers around the Gulf working on biologic, geologic, and hydrologic issues related to the Gulf of Mexico and the State of Florida. We've organized the meeting around the major themes outlined in the USGS Circular 1309, Facing Tomorrow's Challenges - U.S. Geological Survey Science in the Decade 2007-2017. USGS senior leadership will provide a panel discussion about the Gulf of Mexico and Integrated Science. Capstone talks will summarize major topics and key issues. Interactive poster sessions each evening will provide the opportunity for you to present your results and talk with your peers. We hope that discussions and interactions at this meeting will help USGS scientists working in Florida and the Gulf Coast region find common interests, forge scientific collaborations and chart a direction for the future. We hope that the meeting environment will encourage interaction, innovation and stimulate ideas among the many scientists working throughout the region. We'd like to create a community of practice across disciplines and specialties that will help us address complex scientific and societal issues. Please take advantage of this opportunity to visit with colleagues, get to know new ones, share ideas and brainstorm about future possibilities. It is our pleasure to provide this opportunity. We are glad you're here.

  4. Lunar and planetary science XXVIII; Lunar and Planetary Science Conference, 28th, Houston, TX, Mar. 17-21, 1997, Abstracts. Pt. 1 A-G

    NASA Astrophysics Data System (ADS)

    1997-01-01

    The present conference discusses such topics as density crossovers in lunar picrites, the geology of the Cassini impact basin, Mars, nanobacteria in carbonates, the properties of shocked aerogels, a chemical model of Comet Halley, lunar mascons, the impact evolution of icy regoliths, the geology of the Venera 8 landing site, the photogeologic mapping of northern Venus, HST observations of Mars, observational constraints on the rotational dynamics of Mars, and primordial magnetic field measurements from the moon. Also discussed are models of the S2 fluorescence spectra of comets, Martian crater ejecta, the heights of Venusian steep-sided domes, cloud-climate interactions on Venus, the Humorum basin geology from Clementine data, an early Amazonian lake in the Gale crater of Mars, nebular fractionations and Mn-Cr systematics, the Rock Chipper planetary surface sample collection, Mariner 10 stereo images of Mercury, remote and local stresses and Calderas on Mars, the electrostatic charging of saltating particles, SO2 detected on Callisto, the Mars Explorer Planetary Data System, an assessment of explosive venting on Europa, the sequential faulting history of the Mars Valles Marineris, a search for Martian sediments, the composition and internal structure of Europa, long-term and 'diurnal' tidal stresses on Europa, and episodic greenhouse climates on Mars.

  5. VERITAS (Venus Emissivity, Radio Science, InSAR, Topo-graphy And Spectroscopy): A Proposed Discovery Mission

    NASA Astrophysics Data System (ADS)

    Smrekar, Suzanne; Dyar, Melinda; Hensley, Scott; Helbert, Joern; VERITAS Science Team

    2016-10-01

    VERITAS addresses one of the most fundamental questions in planetary evolution: How Earth-like is Venus? These twin planets diverged down different evolutionary paths, yet Venus may hold lessons for past and future Earth, as well as for Earth-sized exoplanets. VERITAS will search for the mineralogical fingerprints of past water, follow up on the discoveries of recent volcanism and the possible young surface age, and reveal the conditions that have prevented plate tectonics from developing. Collectively these questions address how Venus ended up a sulfurous inferno while Earth became habitable.VERITAS carries the Venus Interferometric Synthetic Aperture Radar (VISAR) and the Venus Emissivity Mapper (VEM), plus a gravity science investigation.The VISAR X-band radar produces: 1) a global digital elevation model (DEM) with 250 m postings, 5 m height accuracy, 2) Synthetic aperture radar (SAR) global imaging with 30 m pixels, 3) SAR imaging at 15 m for targeted areas, and 4) surface deformation from repeat pass interferometry (RPI) at 2 mm height precision for targeted, potentially active areas. VEM [see Helbert abstract] will measure surface emissivity, look for active volcanic flows and outgassing of water over ~78% of the surface using 6 NIR surface bands within 5 atmospheric windows and 8 bands for calibration of clouds, stray light, and water vapor.VERITAS uses Ka-band uplink and downlink to create a global gravity field with 3 mgal accuracy and 145 km resolution (130 spherical harmonic degree and order or d&o) and providing a significantly higher resolution field with much more uniform resolution than that available from Magellan.VERITAS will create a rich data set of high resolution topography, imaging, spectroscopy, and gravity. These co-registered data sets will be on par with those acquired for Mercury, Mars and the Moon that have revolutionized our understanding of these bodies. VERITAS would be a valuable asset for future lander or probe missions, collecting

  6. The Official Radio and Television Institute in Spain

    ERIC Educational Resources Information Center

    Ruiz, Anibal Arias

    1976-01-01

    A description of the Official School of Radio and Television which is designed to train university graduates in the fields of journalism, the sciences of cinema, radio and television, and advertising. (JY)

  7. Goldstone-Apple Valley Radio Telescope System Theory of Operation

    NASA Technical Reports Server (NTRS)

    Stephan, George R.

    1997-01-01

    The purpose of this learning module is to enable learners to describe how the Goldstone-Apple Valley Radio Telescope (GAVRT) system functions in support of Apple Valley Science and Technology Center's (AVSTC) client schools' radio astronomy activities.

  8. Lunar and planetary science XXVIII; Lunar and Planetary Science Conference, 28th, Houston, TX, Mar. 17-21, 1997, Abstracts. Pt. 3 P-Z

    NASA Astrophysics Data System (ADS)

    1997-01-01

    The present volume on lunar and planetary science discusses density crossovers in lunar picrites, the geology of the Cassini Impact Basin on Mars, nanobacteria in carbonates, and properties of shocked aerogel. Attention is given to a chemical model of Comet Halley, the impact evolution of icy regoliths, the geology of the Venera 8 landing site, and meteoritic metal in Apollo 16 agglutinates. Other topics addressed include HST observations of Mars during 1996-1997, observational constraints on the rotational dynamics of Mars, primordial magnetic field measurements from the moon, heights of Venusian steep-sided domes, and cloud-climate interactions on Venus.

  9. Lunar and planetary science XXVIII; Lunar and Planetary Science Conference, 28th, Houston, TX, Mar. 17-21, 1997, Abstracts. Pt. 2 H-O

    NASA Astrophysics Data System (ADS)

    1997-01-01

    The present conference volume discusses the discrepancy between experimental and observational results for cumulus pyroxene in Shergotty, optical properties of water ice below 300 K, the effect of Fe on Cr redox state in spinel-saturated basalts, the application of geographic information systems to planetary research, the distribution of Th on the lunar surface, digital elevation models of the western Valles Marineris of Mars, Galileo views of Ganymede dark-floor craters, grooved terrain formation in Ganymede by tectonic resurfacing, petrogenic evolution implications of lunar mare basalt volcanism, the evolution of the early lunar crust, the stratigraphy pf mare deposits in Marginis Basin, massively parallel image processing for crater recognition, and high pressure reactions between Fe-metal and mantle silicates. Also discussed are the nebular shock wave model for chondrule formation, the rotation of Europa, the capture of cohesive hypervelocity particles by silica aerogel, magnetite in carbonaceous chondrites, the mutual gravitational influence of beyond-Neptune bodies, cometary activity and problems of celestial mechanics, possible effects of electrically charged particles in Io's volcanic plumes, the evolution of orbits at the 2:3 resonance with Neptune, estimates of material properties of fluidized ejecta blankets on Mars, an impact hypothesis for Venus Ar anomalies, the astrodynamics of new planetary systems, volcanic differentiation of Io, a geologic mapping of Venus, Mg diffusion in anorthite, catastrophic impacts and asteroid formation rates, the mystery of Callisto, Galileo's view of Io, possible origins of the Europan macula, dust grain orbital behavior around Mars, and the dynamics of the liquid masses on Titan.

  10. PREFACE: 1982 International Conference on Plasma Physics

    NASA Astrophysics Data System (ADS)

    Wilhelmsson, Hans

    1982-01-01

    second one to (3) Fusion and (4) Laboratory Plasmas. The 1982 International Conference on Plasma Physics was organized by Chalmers University of Technology. It gathered about 500 participants from 40 countries. Large delegations came from the USA, France, West Germany, Japan, the USSR, and India, the number of participants from these countries ranging from 100 to 20. Sweden had about 50 participating scientists. There were a total of about 20 from the other Scandinavian countries. The principal sponsor of the conference was IUPAP, the International Union of Pure and Applied Physics. The conference also had a number of co-sponsors like IAU, the International Astronomical Union, URSI, the International Union of Radio Science, EPS, the European Physical Society, and EURATOM-FUSION. The conference was supported by Swedish Industry and Swedish Research Boards. The previous ICPP, held in Nagoya two years ago, was the first attempt to combine two types of conferences: the Plasma Theory Conference, first held in Kiev in the Soviet Union in 1971, and the Waves and Instabilities Congress, held for the first time in Innsbruck, Austria in 1973. As a consequence of the success of the Nagoya conference it was decided by the International Organizing Committee of the ICPP that the 1982 conference should also be of the combined type. The 1982 ICPP in Göteborg was thus a Joint Conference of the Fifth Kiev International Conference in Plasma Theory and the Fifth International Congress on Waves and Instabilities in Plasmas. During the conference in Göteborg the International Organizing Committee had a meeting and it was decided that also the next International Conference on Plasma Physics will be of the combined type. It will be held in Lausanne, Switzerland in 1984. The International Organizing Committee on the 1982 International Conference on Plasma Physics comprised about 40 plasma physics scientists from all over the world, who represented various sections of plasma physics. I would

  11. Radio astronomy

    NASA Technical Reports Server (NTRS)

    Kellermann, Kenneth I.; Heeschen, David; Backer, Donald C.; Cohen, Marshall H.; Davis, Michael; Depater, Imke; Deyoung, David; Dulk, George A.; Fisher, J. R.; Goss, W. Miller

    1991-01-01

    The following subject areas are covered: (1) scientific opportunities (millimeter and sub-millimeter wavelength astronomy; meter to hectometer astronomy; the Sun, stars, pulsars, interstellar masers, and extrasolar planets; the planets, asteroids, and comets; radio galaxies, quasars, and cosmology; and challenges for radio astronomy in the 1990's); (2) recommendations for new facilities (the millimeter arrays, medium scale instruments, and small-scale projects); (3) continuing activities and maintenance, upgrading of telescopes and instrumentation; (4) long range programs and technology development; and (5) social, political, and organizational considerations.

  12. CONFERENCES AND SYMPOSIA: Nuclear physics, lasers, and medicine(Scientific session of the General Meeting of the Physical Sciences Division of the Russian Academy of Sciences, 14 December 2009)

    NASA Astrophysics Data System (ADS)

    2010-09-01

    The scientific session of the General Meeting of the Physical Sciences Division of the Russian Academy of Sciences (RAS) was held in the Conference Hall of the Lebedev Physical Institute, RAS, on 14 December 2009. The following reports were put on the session agenda posted on the web site www.gpad.ac.ru of the Physical Sciences Division, RAS: (1) Kotov Yu D (National Research Nuclear University 'Moscow Engineering Physics Institute' (MEPhI), Institute of Astrophysics, Moscow) "High-energy solar flare processes and their investigation onboard Russian satellite missions CORONAS"; (2) Pakhlov P N (Russian Federation State Scientific Center 'Alikhanov Institute for Theoretical and Experimental Physics,' Moscow) "Exotic charmonium"; (3) Shcherbakov I A (Prokhorov General Physics Institute, RAS, Moscow) "Laser and plasma technologies in medicine"; (4) Balakin V E (Center for Physics and Technology, Lebedev Physical Institute, RAS, Protvino, Moscow region) "New-generation equipment and technologies for the ray therapy of oncological diseases using a proton beam"; (5) Kravchuk L V (Institute for Nuclear Research, RAS, Moscow) "Development of nuclear physics medicine at the Institute for Nuclear Research, RAS." Papers based on reports 1, 3, and 5 are published below. The expanded content of the report by Pakhlov is presented in review form in Physics-Uspekhi 53 219 (2010). • High-energy solar flare processes and their investigation onboard Russian satellite missions CORONAS, Yu D Kotov Physics-Uspekhi, 2010, Volume 53, Number 6, Pages 619-631 • Laser physics in medicine, I A Shcherbakov Physics-Uspekhi, 2010, Volume 53, Number 6, Pages 631-635 • Development of nuclear physics medicine at the Institute for Nuclear Research, RAS, L V Kravchuk Physics-Uspekhi, 2010, Volume 53, Number 6, Pages 635-639

  13. DSMS science operations concept

    NASA Technical Reports Server (NTRS)

    Connally, M. J.; Kuiper, T. B.

    2001-01-01

    The Deep Space Mission System (DSMS) Science Operations Concept describes the vision for enabling the use of the DSMS, particularly the Deep Space Network (DSN) for direct science observations in the areas of radio astronomy, planetary radar, radio science and VLBI.

  14. A Teaching Lab in Radio Astronomy

    ERIC Educational Resources Information Center

    Smith, Kirk R.; Cudaback, David D.

    1976-01-01

    Describes a study in which participants in a summer institute for secondary science teachers performed a series of experiments with a radio telescope. Concludes that a radio astronomy teaching facility would encourage students to use their own initiative and strategy in working with the scientific concepts involved. (MLH)

  15. Principles of Radio: A Laboratory Experiment

    ERIC Educational Resources Information Center

    Kraftmakher, Yaakov

    2002-01-01

    An experiment is proposed for learning the principles of radio. A simple radio receiver illustrates amplitude modulation and demodulation, the selectivity of a receiver and the features of a directional antenna. Both normal and computerized versions of the experiment are described. The computerized experiment employs the "ScienceWorkshop"…

  16. Green Bank (National Radio Astronomical Observatory)

    NASA Astrophysics Data System (ADS)

    Murdin, P.

    2000-11-01

    Located in Green Bank, Pocahontas County, West Virginia. The site of the world's largest fully steerable radio telescope, which was under construction during 1999 and 2000. The National Radio Astronomy Observatory (NRAO) is a facility of the US National Science Foundation, and is operated under a cooperative agreement by Associated Universities, Inc. (AUI)....

  17. CONFERENCES AND SYMPOSIA: Scientific Session of the Physical Sciences Division of the Russian Academy of Sciences dedicated to the centenary of L D Landau's birth (22-23 January 2008)

    NASA Astrophysics Data System (ADS)

    Andreev, A. F.; Kagan, Yu M.; Pitaevskii, L. P.; Khalatnikov, I. M.; Kamenshchik, A. Yu; Ioffe, B. L.; Okun, L. B.; Lipatov, L. N.

    2008-06-01

    A scientific session of the Physical Sciences Division of the Russian Academy of Sciences dedicated to the centenary of L D Landau's birth was held in the Conference Hall of the Lebedev Physics Institute, Russian Academy of Sciences, on 22 and 23 January 2008. An Opening Address by A F Andreev and the following reports were presented at the session: (1) Andreev A F (Kapitza Institute of Physical Problems, Russian Academy of Sciences) "Supersolidity of quantum glasses" (2) Kagan Yu M (Russian Research Center Kurchatov Institute, Moscow) "Formation kinetics of the Bose condensate and long-range order"; (3) Pitaevskii L P (Kapitza Institute of Physical Problems, Russian Academy of Sciences; Dipartimento di Fisica, Universita di Trento and BDC Center, Trento, Italy) "Superfluid Fermi liquid in a unitary regime"; (4) Lebedev V V (Landau Institute for Theoretical Physics, Russian Academy of Sciences, Chernogolovka, Moscow Region) "Kolmogorov, Landau, and the modern theory of turbulence"; (5) Khalatnikov I M (Landau Institute for Theoretical Physics, Russian Academy of Sciences, Moscow), Kamenshchik A Yu (Landau Institute for Theoretical Physics, Russian Academy of Sciences, Moscow; Dipartimento di Fisica and Istituto Nazionale di Fisica Nucleare, Bologna, Italy) "Lev Landau and the problem of singularities in cosmology"; (6) Ioffe B L (Russian State Scientific Center Alikhanov Institute for Theoretical and Experimental Physics, Moscow) "Axial anomaly in quantum electro- and chromodynamics and the structure of the vacuum in quantum chromodynamics"; (7) Okun L B (Russian State Scientific Center Alikhanov Institute for Theoretical and Experimental Physics, Moscow) "The theory of relativity and the Pythagorean theorem"; (8) Lipatov L N (St. Petersburg Nuclear Physics Institute, Gatchina, St. Petersburg) "Bjorken and Regge asymptotics of scattering amplitudes in QCD and in supersymmetric gauge models." A brief presentation of the Opening Address by A F Andreev and reports 2

  18. Teaching radio astronomy with Affordable Small Radio Telescope (ASRT)

    NASA Astrophysics Data System (ADS)

    Joshi, Bhal Chandra

    A simple, easy to build and portable radio telescope, called Affordable Small Radio Telescope (ASRT), has been developed by the Radio Physics Laboratory (RPL), a radio astronomy teaching unit associated with the National Centre for Radio Astrophysics (TIFR) and Inter-University Centre for Astronomy and Astrophysics (IUCAA), which are two premier astronomy institutes in India. ASRT consists of off-the-shelf available Direct to Home television dishes and is easy to assemble. Our design is scalable from simple very low cost telescope to more complex yet moderately costing instrument. ASRT provides a platform for demonstrating radio physics concepts through simple hands-on experiment as well as for carrying out solar monitoring by college/University students. The presentation will highlight the concept of ASRT and the different experiments that can be carried out using it. The solar monitoring observations will be discussed along-with details of methods for calibrating these measurements. The pedagogical usefulness of ASRT in introducing undergraduatephysics students to astrophysics, measurements and analysis methods used in radio astronomy will also be discussed. Use of ASRT in the last three years in the programs of RPL, namely the annual Radio Astronomy Winter School for College students (RAWSC) and Pulsar Observing for Students (POS) is also presented. This year a new program was initiated to form a virtual group of an ASRT community, which will not only share their measurements, but also think of improving the pedagogical usefulness of ASRT by innovative experiments. This initiative is presented with the best practices drawn from our experience in using ASRT as a tool for student training in space sciences. The talk will also point out future ideas in involving a larger body of students in simple radio astronomy experiments with the ASRT, which RPL is likely to nucleate as part of its mandate.

  19. Microbicides 2006 conference

    PubMed Central

    Ramjee, Gita; Shattock, Robin; Delany, Sinead; McGowan, Ian; Morar, Neetha; Gottemoeller, Megan

    2006-01-01

    Current HIV/AIDS statistics show that women account for almost 60% of HIV infections in Sub-Saharan Africa. HIV prevention tools such as male and female condoms, abstinence and monogamy are not always feasible options for women due to various socio-economic and cultural factors. Microbicides are products designed to be inserted in the vagina or rectum prior to sex to prevent HIV acquisition. The biannual Microbicides conference took place in Cape Town, South Africa from 23–26 April 2006. The conference was held for the first time on the African continent, the region worst affected by the HIV/AIDS pandemic. The conference brought together a record number of 1,300 scientists, researchers, policy makers, healthcare workers, communities and advocates. The conference provided an opportunity for an update on microbicide research and development as well as discussions around key issues such as ethics, acceptability, access and community involvement. This report discusses the current status of microbicide research and development, encompassing basic and clinical science, social and behavioural science, and community mobilisation and advocacy activities. PMID:17038196

  20. Conference Resolution

    NASA Astrophysics Data System (ADS)

    2009-04-01

    Since the first IUPAP International Conference on Women in Physics (Paris, March 2002) and the Second Conference (Rio de Janeiro, May 2005), progress has continued in most countries and world regions to attract girls to physics and advance women into leadership roles, and many working groups have formed. The Third Conference (Seoul, October 2008), with 283 attendees from 57 countries, was dedicated to celebrating the physics achievements of women throughout the world, networking toward new international collaborations, building each participant's capacity for career success, and aiding the formation of active regional working groups to advance women in physics. Despite the progress, women remain a small minority of the physics community in most countries.

  1. PREFACE: Quark Matter 2006 Conference

    NASA Astrophysics Data System (ADS)

    Ma, Yu-Gang; Wang, En-Ke; Cai, Xu; Huang, Huan-Zhong; Wang, Xin-Nian; Zhu, Zhi-Yuan

    2007-07-01

    The Quark Matter 2006 conference was held on 14 20 November 2006 at the Shanghai Science Hall of the Shanghai Association of Sciences and Technology in Shanghai, China. It was the 19th International Conference on Ultra-Relativistic Nucleus Nucleus Collisions. The conference was organized jointly by SINAP (Shanghai Institute of Applied Physics, Chinese Academy of Sciences (CAS)) and CCNU (Central China Normal University, Wuhan). Over 600 scientists from 32 countries in five continents attended the conference. This is the first time that China has hosted such a premier conference in the field of relativistic heavy-ion collisions, an important event for the Chinese high energy nuclear physics community. About one half of the conference participants are junior scientists—a clear indication of the vigor and momentum for this field, in search of the fundamental nature of the nuclear matter at extreme conditions. Professor T D Lee, honorary chair of the conference and one of the founders of the quark matter research, delivered an opening address with his profound and philosophical remarks on the recent discovery of the nature of strongly-interacting quark-gluon-plasma (sQGP). Professor Hongjie Xu, director of SINAP, gave a welcome address to all participants on behalf of the two hosting institutions. Dr Peiwen Ji, deputy director of the Mathematics and Physics Division of the Natural Science Foundation of China (NSFC), also addressed the conference participants and congratulated them on the opening of the conference. Professor Mianheng Jiang, vice president of the Chinese Academy of Sciences (CAS), gave a concise introduction about the CAS as the premier research institution in China. He highlighted continued efforts at CAS to foster international collaborations between China and other nations. The Quark Matter 2006 conference is an example of such a successful collaboration between high energy nuclear physicists in China and other nations all over the world. The

  2. The Radio JOVE Project - Shoestring Radio Astronomy

    NASA Technical Reports Server (NTRS)

    Thieman, J.; Flagg, R.; Greenman, W.; Higgins, C.; Reyes, F.; Sky, J.

    2010-01-01

    Radio JOVE is an education and outreach project intended to give students and other interested individuals hands-on experience in learning radio astronomy. They can do this through building a radio telescope from a relatively inexpensive kit that includes the parts for a receiver and an antenna as well as software for a computer chart recorder emulator (Radio Skypipe) and other reference materials

  3. NewsMars: Express journey to Mars ASE 2003: Knocked out by meteorites Events: Sun-Earth Day ASE 2003: Fun Physics - popular as ever Appointments: Sykes to bring science to the people UK Science Education: The future's bright, the future's science ASE 2003: A grand finale for Catherine Teaching Resources: UK goes to the planets Cambridge Physics Update: Basement physics Conferences: Earth Science Teachers' Association Conference 2003 New Website: JESEI sets sail GIREP: Teacher education seminar Malaysia: Rewards for curriculum change Cambridge Physics Update: My boomerang will come back! Teaching Resources: Widening particiption through ideas and evidence with the University of Surrey Wales: First Ffiseg Events: Nuna: Solar car on tour Physics on Stage: Physics on Stage 3 embraces life Symposium: In what sense a nuclear 'debate'? Gifted and Talented: Able pupils experiencing challenging science Australia: ISS flies high Down Under

    NASA Astrophysics Data System (ADS)

    2003-03-01

    Mars: Express journey to Mars ASE 2003: Knocked out by meteorites Events: Sun-Earth Day ASE 2003: Fun Physics - popular as ever Appointments: Sykes to bring science to the people UK Science Education: The future's bright, the future's science ASE 2003: A grand finale for Catherine Teaching Resources: UK goes to the planets Cambridge Physics Update: Basement physics Conferences: Earth Science Teachers' Association Conference 2003 New Website: JESEI sets sail GIREP: Teacher education seminar Malaysia: Rewards for curriculum change Cambridge Physics Update: My boomerang will come back! Teaching Resources: Widening particiption through ideas and evidence with the University of Surrey Wales: First Ffiseg Events: Nuna: Solar car on tour Physics on Stage: Physics on Stage 3 embraces life Symposium: In what sense a nuclear 'debate'? Gifted and Talented: Able pupils experiencing challenging science Australia: ISS flies high Down Under

  4. Radio Galaxy Zoo: host galaxies and radio morphologies derived from visual inspection

    NASA Astrophysics Data System (ADS)

    Banfield, J. K.; Wong, O. I.; Willett, K. W.; Norris, R. P.; Rudnick, L.; Shabala, S. S.; Simmons, B. D.; Snyder, C.; Garon, A.; Seymour, N.; Middelberg, E.; Andernach, H.; Lintott, C. J.; Jacob, K.; Kapińska, A. D.; Mao, M. Y.; Masters, K. L.; Jarvis, M. J.; Schawinski, K.; Paget, E.; Simpson, R.; Klöckner, H.-R.; Bamford, S.; Burchell, T.; Chow, K. E.; Cotter, G.; Fortson, L.; Heywood, I.; Jones, T. W.; Kaviraj, S.; López-Sánchez, Á. R.; Maksym, W. P.; Polsterer, K.; Borden, K.; Hollow, R. P.; Whyte, L.

    2015-11-01

    We present results from the first 12 months of operation of Radio Galaxy Zoo, which upon completion will enable visual inspection of over 170 000 radio sources to determine the host galaxy of the radio emission and the radio morphology. Radio Galaxy Zoo uses 1.4 GHz radio images from both the Faint Images of the Radio Sky at Twenty Centimeters (FIRST) and the Australia Telescope Large Area Survey (ATLAS) in combination with mid-infrared images at 3.4 μm from the Wide-field Infrared Survey Explorer (WISE) and at 3.6 μm from the Spitzer Space Telescope. We present the early analysis of the WISE mid-infrared colours of the host galaxies. For images in which there is >75 per cent consensus among the Radio Galaxy Zoo cross-identifications, the project participants are as effective as the science experts at identifying the host galaxies. The majority of the identified host galaxies reside in the mid-infrared colour space dominated by elliptical galaxies, quasi-stellar objects and luminous infrared radio galaxies. We also find a distinct population of Radio Galaxy Zoo host galaxies residing in a redder mid-infrared colour space consisting of star-forming galaxies and/or dust-enhanced non-star-forming galaxies consistent with a scenario of merger-driven active galactic nuclei (AGN) formation. The completion of the full Radio Galaxy Zoo project will measure the relative populations of these hosts as a function of radio morphology and power while providing an avenue for the identification of rare and extreme radio structures. Currently, we are investigating candidates for radio galaxies with extreme morphologies, such as giant radio galaxies, late-type host galaxies with extended radio emission and hybrid morphology radio sources.

  5. Space Telecommunications Radio System STRS Cognitive Radio

    NASA Technical Reports Server (NTRS)

    Briones, Janette C.; Handler, Louis M.

    2013-01-01

    Radios today are evolving from awareness toward cognition. A software defined radio (SDR) provides the most capability for integrating autonomic decision making ability and allows the incremental evolution toward a cognitive radio. This cognitive radio technology will impact NASA space communications in areas such as spectrum utilization, interoperability, network operations, and radio resource management over a wide range of operating conditions. NASAs cognitive radio will build upon the infrastructure being developed by Space Telecommunication Radio System (STRS) SDR technology. This paper explores the feasibility of inserting cognitive capabilities in the NASA STRS architecture and the interfaces between the cognitive engine and the STRS radio. The STRS architecture defines methods that can inform the cognitive engine about the radio environment so that the cognitive engine can learn autonomously from experience, and take appropriate actions to adapt the radio operating characteristics and optimize performance.

  6. Producing Interactive Educational Radio Programs for Distance Education

    ERIC Educational Resources Information Center

    Yuzer, T. Volkan; Kurubacak, Gulsun

    2004-01-01

    It is not surprising that the interactivity affects radio and its applications. Besides, after radio began its first broadcasting, new inventions affected its development two ways: 1) the first one was the technological developments of sciences. For instance, the invention of transistors made it possible to create very small radio machines, and…

  7. INSPIRE: A VLF Radio Project for High School Students

    ERIC Educational Resources Information Center

    Marshall, Jill A.; Pine, Bill; Taylor, William W. L.

    2007-01-01

    Since 1988 the Interactive NASA Space Physics Ionospheric Radio Experiment, or INSPIRE, has given students the opportunity to build research-quality VLF radio receivers and make observations of both natural and stimulated radio waves in the atmosphere. Any high school science class is eligible to join the INSPIRE volunteer observing network and…

  8. Women in engineering conference: capitalizing on today`s challenges

    SciTech Connect

    Metz, S.S.; Martins, S.M.

    1996-06-01

    This document contains the conference proceedings of the Women in Engineering Conference: Capitalizing on Today`s Challenges, held June 1-4, 1996 in Denver, Colorado. Topics included engineering and science education, career paths, workplace issues, and affirmative action.

  9. The Radio JOVE Project - An Inexpensive Introduction to Radio Astronomy

    NASA Astrophysics Data System (ADS)

    Thieman, J. R.; Higgins, C.

    2004-12-01

    The Radio JOVE project began over six years ago as an education-centered program to inspire secondary school students' interest in space science through hands-on radio astronomy. The project was begun on small grants from the Goddard Space Flight Center Director's Discretionary Fund, the Initiative to Develop Education through Astronomy and Space Science (IDEAS) program, and the American Astronomical Society. Students build a radio receiver and antenna kit capable of receiving Jovian, solar, and galactic emissions at a frequency of 20.1 MHz. More than 600 of these kits have been distributed to students and interested observers (ages 10 through adult) in over 30 countries. For those who are not comfortable building their own kit, the Radio JOVE project has made it possible to monitor real-time data and streaming audio online from professional radio telescopes in Florida (http://jupiter.kochi-ct.jp) and Hawaii http://jupiter.wcc.hawaii.edu/newradiojove/main.html). Freely downloadable software called Radio-Skypipe (http://radiosky.com) emulates a chart recorder to monitor ones own radio telescope or the telescopes of other observers worldwide who send out their data over the Internet. Inexpensive spectrographs have been developed for the professional telescopes in Hawaii and Florida and freely downloadable spectrograph display software is available to receive this research-quality data. We believe the amateur network data to be of value to the research community and would like to have students more directly connected to ongoing research projects to enhance their interest in participating. Results of the project and plans for the future will be highlighted.

  10. PREFACE: Quark Matter 2006 Conference

    NASA Astrophysics Data System (ADS)

    Ma, Yu-Gang; Wang, En-Ke; Cai, Xu; Huang, Huan-Zhong; Wang, Xin-Nian; Zhu, Zhi-Yuan

    2007-07-01

    The Quark Matter 2006 conference was held on 14 20 November 2006 at the Shanghai Science Hall of the Shanghai Association of Sciences and Technology in Shanghai, China. It was the 19th International Conference on Ultra-Relativistic Nucleus Nucleus Collisions. The conference was organized jointly by SINAP (Shanghai Institute of Applied Physics, Chinese Academy of Sciences (CAS)) and CCNU (Central China Normal University, Wuhan). Over 600 scientists from 32 countries in five continents attended the conference. This is the first time that China has hosted such a premier conference in the field of relativistic heavy-ion collisions, an important event for the Chinese high energy nuclear physics community. About one half of the conference participants are junior scientists—a clear indication of the vigor and momentum for this field, in search of the fundamental nature of the nuclear matter at extreme conditions. Professor T D Lee, honorary chair of the conference and one of the founders of the quark matter research, delivered an opening address with his profound and philosophical remarks on the recent discovery of the nature of strongly-interacting quark-gluon-plasma (sQGP). Professor Hongjie Xu, director of SINAP, gave a welcome address to all participants on behalf of the two hosting institutions. Dr Peiwen Ji, deputy director of the Mathematics and Physics Division of the Natural Science Foundation of China (NSFC), also addressed the conference participants and congratulated them on the opening of the conference. Professor Mianheng Jiang, vice president of the Chinese Academy of Sciences (CAS), gave a concise introduction about the CAS as the premier research institution in China. He highlighted continued efforts at CAS to foster international collaborations between China and other nations. The Quark Matter 2006 conference is an example of such a successful collaboration between high energy nuclear physicists in China and other nations all over the world. The

  11. Radio Studies of Galactic Objects, Galaxies and AGNs

    NASA Astrophysics Data System (ADS)

    Han, J. L.; Sun, X. H.; Yang, J.; Wielebinski, R.

    2003-02-01

    The Sino-German Radio Astronomy Conference was held in Xi'an between July 18th and 25th 2002. This conference was also a meeting of radio astronomy in China. The partner group of Max-Plack-Institut for Radioastronomie at National Astronomical Observatories of China took the responsibility for detailed organizations. The conference was focused on "Radio studies of Galactic objects, galaxies and AGNs", with 80 partici- pants plus the 6 helpers. Most radio astronomers in China together with about 30 students enjoyed the fruitful discussions with 9 German senior scientists and 6 famous experts from other countries. In addition, the his- torical sites and culture environments specifically in Xi'an also attracted a dozen companions of delegates.

  12. Minnesota Junior College Faculty 1969 Conferences. Reports and Papers from Three Conferences on Innovation.

    ERIC Educational Resources Information Center

    Moen, Norman W., Ed.; Shaner, James P., Ed.

    Three conferences on educational innovation raised basic questions concerning goals and values for junior college students. Speakers addressed each of the conferences on problems encountered in their respective areas of humanities, social sciences, and physical sciences. The addresses are presented, along with recommendations made by the…

  13. The Future of Radio astronomy

    NASA Astrophysics Data System (ADS)

    Ekers, R. D.

    2001-12-01

    Five decades ago, astronomers finally broke free of the boundaries of light when a new science, radio astronomy, was born. This new way of "seeing" rapidly uncovered a range of unexpected objects in the cosmos. This was our first view of the non-thermal universe, and our first unobscured view of the universe. In its short life, radio astronomy has had an unequalled record of discovery, including four Nobel prizes: Big-Bang radiation, neutron stars, aperture synthesis and gravitational radiation. Radio telescopes have followed the pattern of exponential growth generally seen in flourishing areas of science and technology and there is no technical reason for this not to continue, but to do so will require a shift in technology that will set new challenges. New technologies have made it possible to construct an affordable radio telescope with collecting area of one square km the SKA. Such a telescope would be so powerful that we could expand our knowledge of the universe from the earliest stages of its formation through to planetary exploration with greatly enhanced spacecraft communications. The SKA will join the new generation of telescopes at other wavebands with the sensitivity and resolution to image the earliest phases of galaxy formation, as well as greatly extending the range of unique science accessible at radio wavelengths. We already know how to build an SKA, the issue is how to build the most cost effective SKA, and how to maximize the science we can do with it. The path we have chosen to achieve this vision is through international collaboration. Following the pattern of other successful international collaborations in science we have started this process early, and we are already benefiting from the level of innovation generated by our international interactions.

  14. Monitoring Radio Frequency Interference in Southwest Virginia

    NASA Astrophysics Data System (ADS)

    Rapp, Steve

    2010-01-01

    The radio signals received from astronomical objects are extremely weak. Because of this, radio sources are easily shrouded by interference from devices such as satellites and cell phone towers. Radio astronomy is very susceptible to this radio frequency interference (RFI). Possibly even worse than complete veiling, weaker interfering signals can contaminate the data collected by radio telescopes, possibly leading astronomers to mistaken interpretations. To help promote student awareness of the connection between radio astronomy and RFI, an inquiry-based science curriculum was developed to allow high school students to determine RFI levels in their communities. The Quiet Skies Project_the result of a collaboration between the National Aeronautics and Space Administration (NASA), the National Science Foundation (NSF), and the National Radio Astronomy Observatory (NRAO)_encourages students to collect and analyze RFI data and develop conclusions as a team. Because the project focuses on electromagnetic radiation, it is appropriate for physics, physical science, chemistry, or general science classes. My class-about 50 students from 15 southwest Virginia high schools-participated in the Quiet Skies Project and were pioneers in the use of the beta version of the Quiet Skies Detector (QSD), which is used to detect RFI. Students have been involved with the project since 2005 and have collected and shared data with NRAO. In analyzing the data they have noted some trends in RFI in Southwest Virginia.

  15. RADIO ALTIMETERS

    DOEpatents

    Bogle, R.W.

    1960-11-22

    A radio ranging device is described which utilizes a superregenerative oscillator having alternate sending and receiving phases with an intervening ranging interval between said phases, means for varying said ranging interval, means responsive to an on-range noise reduction condition for stopping said means for varying the ranging interval and indicating means coupled to the ranging interval varying means and calibrated in accordance with one-half the product of the ranging interval times the velocity of light whereby the range is indicated.

  16. Science.

    ERIC Educational Resources Information Center

    Roach, Linda E., Ed.

    This document contains the following papers on science instruction and technology: "A 3-D Journey in Space: A New Visual Cognitive Adventure" (Yoav Yair, Rachel Mintz, and Shai Litvak); "Using Collaborative Inquiry and Interactive Technologies in an Environmental Science Project for Middle School Teachers: A Description and Analysis" (Patricia…

  17. New Information Technology in Social Science Education: Viewpoints from Europe and the United States. Annual Conference of the Social Science Education Consortium (20th, Athens, Georgia, June 8-11, 1983).

    ERIC Educational Resources Information Center

    Hepburn, Mary A., Ed.

    Fourteen conference papers dealing with the effects of electronic information technology on social studies education are provided. Microcomputers received most of the attention, followed by satellite telecommunications, as the conference participants examined implications for student learning styles, student knowledge and attitudes, teacher…

  18. PREFACE: XXI Fluid Mechanics Conference

    NASA Astrophysics Data System (ADS)

    Szmyd, Janusz S.; Fornalik-Wajs, Elzbieta; Jaszczur, Marek

    2014-08-01

    This Conference Volume contains the papers presented at the 21st Fluid Mechanics Conference (XXI FMC) held at AGH - University of Science and Technology in Krakow, Poland, 15-18 June 2014, and accepted for Proceedings published in the Journal of Physics: Conference Series. The Fluid Mechanics Conferences have been taking place every two years since 1974, a total of forty years. The 21st Fluid Mechanics Conference (XXI FMC) is being organized under the auspices of the Polish Academy of Sciences, Committee of Mechanics. The goal of this conference is to provide a forum for the exposure and exchange of ideas, methods and results in fluid mechanics. Conference topics include, but are not limited to Aerodynamics, Atmospheric Science, Bio-Fluids, Combustion and Reacting Flows, Computational Fluid Dynamics, Experimental Fluid Mechanics, Flow Machinery, General Fluid Dynamics, Hydromechanics, Heat and Fluid Flow, Measurement Techniques, Micro- and Nano- Flow, Multi-Phase Flow, Non-Newtonian Fluids, Rotating and Stratified Flows, Turbulence. Within the general subjects of this conference, the Professor Janusz W. Elsner Competition for the best fluid mechanics paper presented during the Conference is organized. Authors holding a M.Sc. or a Ph.D. degree and who are not older than 35 years of age may enter the Competition. Authors with a Ph.D. degree must present individual papers; authors with a M.Sc. degree may present papers with their supervisor as coauthor, including original results of experimental, numerical or analytic research. Six state-of-the-art keynote papers were delivered by world leading experts. All contributed papers were peer reviewed. Recommendations were received from the International Scientific Committee, reviewers and the advisory board. Accordingly, of the 163 eligible extended abstracts submitted, after a review process by the International Scientific Committee, 137 papers were selected for presentation at the 21st Fluid Mechanics Conference, 68

  19. History of NAMES Conferences

    NASA Astrophysics Data System (ADS)

    Filippov, Lev

    2013-03-01

    -Russian International Centre was demonstrated. By the high standards of the reports presented, as well as by its overall organization, the second Seminar met the standards of an international conference. Reviews of state-of-the-art developments in materials science were given by leading scientists from Moscow and from the Lorraine region. The three days of the seminar were structured into four main themes: Functional Materials Coatings, Films and Surface Engineering Nanomaterials and Nanotechnologies The Environment and three Round Table discussions: Defining practical means of carrying out Franco-Russian collaborations in technology transfer and innovation Materials science ARCUS: Lorraine-Russian collaboration in materials science and the environment 32 oral and 25 poster presentations within four sections were given by a total of 110 participants. NAMES 2007, the 3rd Franco-Russian Seminar on New Achievements in Materials and Environmental Sciences, took place in Metz, France on 7-9 November 2007. The conference highlights fundamentals and development of the five main themes connected to the Lorraine-Russia ARCUS project with possible extension to other topics. The five main subjects included in the ARCUS project are: Bulk-surface-interface material sciences Nanomaterials and nanotechnologies Environment and natural resources Plasma physics—ITER project Vibrational dynamics The first, second and third NAMES conferences were financially supported by the following organizations: Ambassade de France à Moscou Communauté Urbaine du Grand Nancy Région Lorraine Conseil Général de Meurthe et Moselle Institut National Polytechnique de Lorraine Université de Metz Université Henry Poincaré CNRS ANVAR Federal Agency on Science and Innovations of the Ministry of Education and Science of the Russian Federation Moscow Committee on Science and Technologies Moscow Institute of Steel and Alloys (Technological University) The 4th conference is supported by the Ministry of Foreign Affairs of

  20. Proceedings SPIE: Conference Digest, volume 2104

    NASA Astrophysics Data System (ADS)

    Birch, James R.; Parker, Terence J.

    1993-09-01

    The Eighteenth International Conference on Infrared and Millimeter Waves was held from 6-10 Sep. 1993, at the University of Essex in Colchester, UK. The scope of the Conference covers progress in all areas of infrared and millimeter wave science and technology, and the large number of contributions (more than 300) received from more than 25 countries demonstrates the importance of the field and the need for the Conference.

  1. Conference Summary

    NASA Technical Reports Server (NTRS)

    Harrington, James L., Jr.

    2000-01-01

    Celebrations and special events were in order this year as the Minority University-Space Interdisciplinary Network (MU-SPIN) Program and NASA's Minority University Research and Education Division (MURED) both reached their 10th anniversaries. In honor of this occasion, the 2000 Annual Users' Conference held at Morris Brown College (MBC) in Atlanta, Georgia, September 11-15, 2000, was the first to be jointly hosted by MU-SPIN and MURED. It was particularly fitting that this anniversary should fall in the year 2000. The start of the new millennium propelled us to push bold new ideas and renew our commitment to minority university participation in all areas of NASA. With the theme 'Celebrating Our Tenth Year With Our Eyes on the Prize,' the conference provided a national forum for showcasing successful MU-SPIN and MURED Program (MUREP) experiences to enhance faculty/student development in areas of scientific and technical research and education. Our NASA-relevant conference agenda resulted in a record-breaking 220 registered attendees. Using feedback from past participants, we designed a track of student activities closely tailored to their interests. The resulting showcase of technical assistance and best practices set a new standard for our conferences in the years to come. This year's poster session was our largest ever, with over 50 presentations from students, faculty, and teachers. Posters covered a broad range of NASA activities from 'A Study of the Spiral Galaxy M101' to 'Network Cabling Characteristics.'

  2. IEEE conference record -- Abstracts

    SciTech Connect

    Not Available

    1994-01-01

    This conference covers the following areas: computational plasma physics; vacuum electronic; basic phenomena in fully ionized plasmas; plasma, electron, and ion sources; environmental/energy issues in plasma science; space plasmas; plasma processing; ball lightning/spherical plasma configurations; plasma processing; fast wave devices; magnetic fusion; basic phenomena in partially ionized plasma; dense plasma focus; plasma diagnostics; basic phenomena in weakly ionized gases; fast opening switches; MHD; fast z-pinches and x-ray lasers; intense ion and electron beams; laser-produced plasmas; microwave plasma interactions; EM and ETH launchers; solid state plasmas and switches; intense beam microwaves; and plasmas for lighting. Separate abstracts were prepared for 416 papers in this conference.

  3. Metabolic Engineering VII Conference

    SciTech Connect

    Kevin Korpics

    2012-12-04

    The aims of this Metabolic Engineering conference are to provide a forum for academic and industrial researchers in the field; to bring together the different scientific disciplines that contribute to the design, analysis and optimization of metabolic pathways; and to explore the role of Metabolic Engineering in the areas of health and sustainability. Presentations, both written and oral, panel discussions, and workshops will focus on both applications and techniques used for pathway engineering. Various applications including bioenergy, industrial chemicals and materials, drug targets, health, agriculture, and nutrition will be discussed. Workshops focused on technology development for mathematical and experimental techniques important for metabolic engineering applications will be held for more in depth discussion. This 2008 meeting will celebrate our conference tradition of high quality and relevance to both industrial and academic participants, with topics ranging from the frontiers of fundamental science to the practical aspects of metabolic engineering.

  4. 45 CFR 672.12 - Prehearing conference.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... Public Welfare Regulations Relating to Public Welfare (Continued) NATIONAL SCIENCE FOUNDATION ENFORCEMENT... conference appears unnecessary, the Presiding Officer, at any time before the hearing begins, shall direct... telephonic conference or direct the parties to correspond with him to accomplish any of the objectives...

  5. 45 CFR 672.12 - Prehearing conference.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ... Public Welfare Regulations Relating to Public Welfare (Continued) NATIONAL SCIENCE FOUNDATION ENFORCEMENT... conference appears unnecessary, the Presiding Officer, at any time before the hearing begins, shall direct... telephonic conference or direct the parties to correspond with him to accomplish any of the objectives...

  6. Chemical Education Conference Caters to Varied Audience.

    ERIC Educational Resources Information Center

    Worthy, Ward

    1986-01-01

    Reports on the 9th Biennial Conference on Chemical Education sponsored by the American Chemical Society. The conference theme: "Chemistry: Learning, Instructing, Presenting," was addressed by numerous sessions. Highlighted were presentations calling for an increase in process-oriented chemistry teaching, reduction of "science anxiety," and the…

  7. Conference Summary

    NASA Technical Reports Server (NTRS)

    Begelman, Mitchell C.

    1997-01-01

    At the end of three days' spirited discussion of the type 2 Seyfert galaxy NGC 1068, what do we think we understand about this object? New observations, particularly in the infrared and radio are helping to resolve old problems, while drawing attention to new ones. It appears that NGC 1068 is a relatively normal spiral galaxy in which large-scale gravitational disturbances are funneling matter into the nucleus. A collimated outflow disturbs the interstellar medium out to kiloparsec scales, but the nucleus itself is hidden behind an opaque screen. Radio observations have now pierced the screen, and suggest that at the center of it all, a 10-20 million solar mass black hole is accreting at close to its Eddington limit.

  8. Survivorship conference highlights research for survivor care

    Cancer.gov

    More than 400 leading experts in cancer survivorship convened today for a conference, Cancer Survivorship Research: Translating Science to Care, to focus on such current concerns as how obesity might not have the same effects on all cancer survivors, and

  9. Moon exploration: lunar radio observatory

    NASA Astrophysics Data System (ADS)

    Skalsky, Alexandre; Zelenyi, Lev; Rothkaehl, Hanna; Gurvits, Leonid; Sadovski, Andrei; Mogilevsky, Mikhail; Gotlib, Vladimir

    The Moon is an attractive base for fundamental scientific studies. The conducting ionosphere of Earth prevents propagation of radio emission coming from the outer space to the Earth’s surface at frequencies below a few MHz. In contrast, the Moon surrounded by a very thin atmosphere and ionosphere is a perfect site for an ultra-long-wavelength (ULW) facility for studies of cosmic radio emission at frequencies below the Earth’s ionosphere cut-off. This range of frequencies is the last unexplored window in the spectrum of the universe’s electromagnetic emission, The radio facility deployed on the Moon’s surface will be a multidisciplinary tool for addressing a wide range of scientific disciplines from cosmology to astrophysics to planetology, solar-terrestrial physics and geophysics. The Moon-based ULW observatory will be an experimental and observational facility for transformational science. One of the most intriguing objectives for the ULW science is a search for terrestrial-like planets in the exosolar systems, i.e. extra-solar planets possessing an intrinsic magnetic field and magnetospheres interacting with a stellar wind. Such the interaction generates radio emission similar to the Auroral Kilometric Radiation (AKR) of the terrestrial magnetosphere. The intrinsic magnetic field shielding the planetary surface from the cosmic radiation is one of the strong indicators of possible habitability of an exoplanet. ACKNOWLEDGMENTS: This work was supported by the PP RAS 22 grant.

  10. Reshaping Assessment Practices: Mathematics Assessment under Challenge. Proceedings from the National Conference on Assessment in the Mathematical Sciences (1st, Geelong, Victoria, Australia November 20-24, 1991).

    ERIC Educational Resources Information Center

    Stephens, Max, Ed.; Izard, John, Ed.

    The purpose of the Australian conference on mathematical assessment was to address the challenges to traditional methods of assessment that have resulted as part of the call for reform in the mathematics curriculum. The 28 papers presented were: "Who Assesses Whom and To What Purpose?" (Leone Burton; "Assessment of the Learned Structure in…

  11. Minnesota Junior College Faculty Interests and Concerns: Proceedings of a Conference of Instructors in Natural Science and Occupational Education (Minneapolis, March 24-26, 1968).

    ERIC Educational Resources Information Center

    Moen, Norman W., Ed.; Stave, Roman L., Ed.

    In this report on the third of three conferences (1968), N.C. Harris stressed the obligation of the junior college to provide high quality instruction for a great variety of students, noting the distinction between rigor and quality. He also provided charts as guidelines for several programs. Discussion groups covered (1) problems of having junior…

  12. SCIENCE ADMINISTRATION, EDUCATION, AND CAREER MOBILITY. SUMMARY OF PROCEEDINGS AND WORKING PAPERS OF THE UNIVERSITY-FEDERAL AGENCY CONFERENCE (NOVEMBER 7-9, 1965).

    ERIC Educational Resources Information Center

    RANDALL, RAYMOND L., ED.; SIMPSON, DICK W., ED.

    THE 1965 UNIVERSITY-FEDERAL AGENCY CONFERENCE FOCUSED ON THE MIDCAREER TRAINING AND EDUCATIONAL NEEDS OF FEDERAL SCIENTISTS. PARTICIPANTS REPRESENTING GOVERNMENT, INDUSTRY, AND UNIVERSITIES EXPLORED IN DEPTH THE POTENTIAL UTILITY OF CLOSER COOPERATION AMONG ALL THREE SECTORS TO PREVENT OBSOLESCENCE OF VALUABLE SKILLS AND, BY USING THE UNIQUE…

  13. African science contributes to the fight against cancer in the world: reflections after the 10th AORTIC conference, 18–22nd November 2015, Marrakesh, Morocco

    PubMed Central

    Stefan, DC

    2016-01-01

    AORTIC (OAREC), the Pan – African organization aiming to unite African scientists in the fight against cancer on the continent, held its 2015 conference in November, in Marrakesh. It was an opportunity to evaluate the progress made, to strengthen scientific collaborations and to draw the future battle lines against cancer on the continent. PMID:26913074

  14. Proceedings of the RESNA '98 Annual Conference: The State of the Arts and Science (Minneapolis, Minnesota, June 26-30, 1998). Volume 18.

    ERIC Educational Resources Information Center

    Springle, Stephen, Ed.

    This text contains papers presented at the 1998 conference of the Rehabilitation Engineering and Assistive Technology Society of North America held on June 26-30, 1998, in Minneapolis, Minnesota. Papers are divided into the following sections: (1) service delivery and public policy, including papers addressing independent literacy, integrating…

  15. Pan Pacific Microgravity Conference -- Outreach

    NASA Technical Reports Server (NTRS)

    2001-01-01

    Teachers, students, and parents listen as scientists explain what is different about the microgravity envirornment of space and why it is a valuable tool for research. This was part of the outreach session of the Pan Pacific Microgravity Conference on May 2, 2001, at the California Science Center.

  16. Space Station Freedom Utilization Conference

    NASA Technical Reports Server (NTRS)

    1992-01-01

    The topics addressed in Space Station Freedom Utilization Conference are: (1) space station freedom overview and research capabilities; (2) space station freedom research plans and opportunities; (3) life sciences research on space station freedom; (4) technology research on space station freedom; (5) microgravity research and biotechnology on space station freedom; and (6) closing plenary.

  17. Conference Abstracts: Microcomputers in Education.

    ERIC Educational Resources Information Center

    Baird, William E.

    1985-01-01

    Provides abstracts of five papers presented at the Fourth Annual Microcomputers in Education Conference. Papers considered microcomputers in science laboratories, Apple II Plus/e computer-assisted instruction in chemistry, computer solutions for space mechanics concerns, computer applications to problem solving and hypothesis testing, and…

  18. Science Education and Educational Policies

    ERIC Educational Resources Information Center

    Livermore, Arthur

    1976-01-01

    Discusses several conferences held by the American Association for the Advancement of Science (AAAS) Office of Science Education to address the question of the future of science education, particularly at the pre-college level. (MLH)

  19. FOREWORD: 13th International Workshop on Plasma-Facing Materials and Components for Fusion Applications/1st International Conference on Fusion Energy Materials Science 13th International Workshop on Plasma-Facing Materials and Components for Fusion Applications/1st International Conference on Fusion Energy Materials Science

    NASA Astrophysics Data System (ADS)

    Jacob, Wolfgang; Linsmeier, Christian; Rubel, Marek

    2011-12-01

    The 13th International Workshop on Plasma-Facing Materials and Components (PFMC-13) jointly organized with the 1st International Conference on Fusion Energy Materials Science (FEMaS-1) was held in Rosenheim (Germany) on 9-13 May 2011. PFMC-13 is a successor of the International Workshop on Carbon Materials for Fusion Applications series. Between 1985 and 2003 ten 'Carbon Workshops' were organized in Jülich, Stockholm and Hohenkammer. Then it was time for a change and redefinition of the scope of the symposium to reflect the new requirements of ITER and the ongoing evolution in the field. Under the new name (PFMC-11), the workshop was first organized in 2006 in Greifswald, Germany and PFMC-12 took place in Jülich in 2009. Initially starting in 1985 with about 40 participants as a 1.5 day workshop, the event has continuously grown to about 220 participants at PFMC-12. Due to the joint organization with FEMaS-1, PFMC-13 set a new record with more than 280 participants. The European project Fusion Energy Materials Science, FEMaS, coordinated by the Max-Planck-Institut für Plasmaphysik (IPP), organizes and stimulates cooperative research activities which involve large-scale research facilities as well as other top-level materials characterization laboratories. Five different fields are addressed: benchmarking experiments for radiation damage modelling, the application of micro-mechanical characterization methods, synchrotron and neutron radiation-based techniques and advanced nanoscopic analysis based on transmission electron microscopy. All these fields need to be exploited further by the fusion materials community for timely materials solutions for a DEMO reactor. In order to integrate these materials research fields, FEMaS acted as a co-organizer for the 2011 workshop and successfully introduced a number of participants from research labs and universities into the PFMC community. Plasma-facing materials experience particularly hostile conditions as they are

  20. Polar Gateways Arctic Circle Sunrise 2008 Conference at the Top of the World

    NASA Technical Reports Server (NTRS)

    Cooper, John F.; Kauristie, Kirsti; Weatherwax, Allan T.; Sandahl, Ingrid; Ostgaard, Nikolai; Sheehan, Glenn W.; Smith, Roger W.; Lewis, Elaine M.; Cline, Troy D.; Haines-Stiles, Geoff

    2008-01-01

    , Mars, Jupiter, Saturn, the Kuiper Belt, and the solar wind termination shock now crossed by both Voyager spacecraft. Barrow participants experienced look and feel of icy worlds like Europa by going "on the ice" during snowmobile expeditions to the near-shore sea ice and Point Barrow. Extensive educational outreach activities were conducted with the local Barrow township and North Slope Borough communities, partly through several interviews with local host Earl Finkler on Barrow's KBRW Radio, and through the NASA Digital Learning Network (DLN) "live from the top of the world" at Barrow. The Goddard robotic rover "Nunuq of the North" became a local celebrity. The complete science program and photo library, eventually also including video recordings of all main presentations, will be available at the new polargateways2008.gsfc.nasa.gov web site (old version: polargateways2008.org) with links to educational materials from the conference already accessible at sunearthday.nasa.gov/polarsunrise.