Royal Astronomical Society Annual Report and Accounts 31 December
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Mars, the First Results from the Cassini-Huygens Probe Which Landed on Titan and Robotic Space Missions
OH 404 new.qxd 20/02/2006 11:49 Page 1 OpenHouse Newspaper for staff of The Open University Issue number 404 Jan - Feb 2006 Military Coup by Peter Taylor-Whiffen THOUSANDS of members of the Armed Forces will be numbers are expected to increase by a total of 400 studying Open University MBA courses after the OU learners across all three defence services within five signed a 22-year deal to provide courses for the years. military. A Ministry of Defence statement said: “Individuals at The university will work in partnership with Cranfield all levels from the Royal Navy, Army, Royal Air Force and University to deliver postgraduate education to military the Civil Service will benefit from this investment and the personnel through the Ministry of Defence’s Defence higher level education and training it provides for.” College of Management and Technology (DCMT) – and it’s And Defence Minister Don Touhig added: “We expect expected at least 400 servicemen and women will sign up our Armed Forces to operate in an increasingly complex every year. and demanding environment. We can’t ask this of our “It’s very good news indeed,” said the OU’s Head of Service personnel, and the civilians who support them, Strategic Partnerships, Edmund Dixon. “It’s the reward unless we invest in their ongoing training and for a lot of hard work tendering and then further development. impressing the MoD when we made a shortlist.” “This contract provides access to the very best Cranfield has worked with the DCMT, at Shrivenham, postgraduate education and the flexibility to help equip Wiltshire for many years but its previous contract ended our people to meet these challenges.” last year and other universities were invited to apply. -
1 1/4/18 Dr. Stefi Alison Baum Dean, Faculty of Science Professor, Dept
RESUME – DR. STEFI BAUM, 1/4/18 Dr. Stefi Alison Baum Dean, Faculty of Science Professor, Dept. of Physics and Astronomy University of Manitoba Winnipeg, MB, Canada Email [email protected] cell phone 204-297-0698 EDUCATION B.A. Physics, cum laude June 1980 Harvard University, Cambridge, MA Co-Captain Varsity Women’s Lacrosse and Co-Captain Varsity Women’s Soccer PhD Astronomy Dec 1987 University of Maryland, College Park, MD POST-DEGREE EDUCATION Center for Higher Education Research and Development • The Senior University Administrators Course, Niagara-on-the-Lake, 2015 University of Wisconsin-Madison, Fluno Center, Executive Education, 2013 • Fundraising and Development for Nonprofits Harvard University, Graduate School of Education, 2012 • Performance Assessment in Higher Education Peabody Fellow, Vanderbilt Peabody Professional Institute, 2011 • Higher Education Management Pardee RAND Graduate School, 2009, New Security Challenges Harvard-MIT-Tufts Program on Negotiation, Executive Ed Series, 2007 • Program on Negotiation for Senior Executives • Dealing with Difficult People and Difficult Situations American Council on Education, 2005, Chairing the Academic Department MIT-Sloan Executive Series, 2002, 2003, 2005: • System Dynamics for Senior Managers • Managing Technical Professionals and Organizations • The Innovative Organization United States Foreign Service Institute, 2004, Global Issues Coursera Courses Completed - 2013 • Leading Innovative Change in Organizations, Vanderbilt University • Synapses, Neurons and Brains, Hebrew University of Jerusalem • What a Plant Knows, Tel Aviv University, (audit) • Epigenetic Control of Gene Expression, University of Melborne, (audit) • A Brief History of Humankind, Hebrew University (audit) • Surviving Disruptive Technologies, University of Maryland, (audit) 1 EXPERTISE Over 25 years of leadership in highly interdisciplinary research and educational environments, including higher education, not for profits, and government agencies. -
Annual Report to Industry Canada Covering The
Annual Report to Industry Canada Covering the Objectives, Activities and Finances for the period August 1, 2008 to July 31, 2009 and Statement of Objectives for Next Year and the Future Perimeter Institute for Theoretical Physics 31 Caroline Street North Waterloo, Ontario N2L 2Y5 Table of Contents Pages Period A. August 1, 2008 to July 31, 2009 Objectives, Activities and Finances 2-52 Statement of Objectives, Introduction Objectives 1-12 with Related Activities and Achievements Financial Statements, Expenditures, Criteria and Investment Strategy Period B. August 1, 2009 and Beyond Statement of Objectives for Next Year and Future 53-54 1 Statement of Objectives Introduction In 2008-9, the Institute achieved many important objectives of its mandate, which is to advance pure research in specific areas of theoretical physics, and to provide high quality outreach programs that educate and inspire the Canadian public, particularly young people, about the importance of basic research, discovery and innovation. Full details are provided in the body of the report below, but it is worth highlighting several major milestones. These include: In October 2008, Prof. Neil Turok officially became Director of Perimeter Institute. Dr. Turok brings outstanding credentials both as a scientist and as a visionary leader, with the ability and ambition to position PI among the best theoretical physics research institutes in the world. Throughout the last year, Perimeter Institute‘s growing reputation and targeted recruitment activities led to an increased number of scientific visitors, and rapid growth of its research community. Chart 1. Growth of PI scientific staff and associated researchers since inception, 2001-2009. -
Understanding Cosmic Acceleration: Connecting Theory and Observation
Understanding Cosmic Acceleration V(!) ! E Hivon Hiranya Peiris Hubble Fellow/ Enrico Fermi Fellow University of Chicago #OMPOSITIONOFAND+ECosmic HistoryY%VENTS$ UR/ INGTHE%CosmicVOLUTIONOFTHE5 MysteryNIVERSE presentpresent energy energy Y density "7totTOT = 1(k=0)K density DAR RADIATION KENER dark energy YDENSIT DARK G (73%) DARKMATTER Y G ENERGY dark matter DARK MA(23.6%)TTER TIONOFENER WHITEWELLUNDERSTOOD DARKNESSPROPORTIONALTOPOORUNDERSTANDING BARYONS BARbaryonsYONS AC (4.4%) FR !42 !33 !22 !16 !12 Fractional Energy Density 10 s 10 s 10 s 10 s 10 s 1 sec 380 kyr 14 Gyr ~1015 GeV SCALEFACTimeTOR ~1 MeV ~0.2 MeV 4IME TS TS TS TS TS TSEC TKYR T'YR Y Y Planck GUT Y T=100 TeV nucleosynthesis Y IES TION TS EOUT DIAL ORS TIONS G TION TION Z T Energy THESIS symmetry (ILC XA 100) MA EN EE WNOF ESTHESIS V IMOR GENERATEOBSERVABLE IT OR ELER ALTHEOR TIONS EF SIGNATURESINTHE#-" EAKSYMMETR EIONIZA INOFR Y% OMBINA R E6 EAKDO #X ONASYMMETR SIC W '54SYMMETR IMELINEOF EFFWR Y Y EC TUR O NUCLEOSYN ), * +E R 4 PLANCKENER Generation BR TR TURBA UC PH Cosmic Microwave NEUTR OUSTICOSCILLA BAR TIONOFPR ER A AC STR of primordial ELEC non-linear growth of P 44 LIMITOFACC Background Emitted perturbations perturbations: GENER ES carries signature of signature on CMB TUR GENERATIONOFGRAVITYWAVES INITIALDENSITYPERTURBATIONS acoustic#-"%MITT oscillationsED NON LINEARSTR andUCTUR EIMPARTS #!0-!0OBSERVES#-" ANDINITIALDENSITYPERTURBATIONS GROWIMPARTINGFLUCTUATIONS CARIESSIGNATUREOFACOUSTIC SIGNATUREON#-"THROUGH *throughEFFWRITESUPANDGR weakADUATES WHICHSEEDSTRUCTUREFORMATION -
Martian Methane: Rocky Birth, Then Gone with the Wind?
Meeting Division for Planetary Sciences CAMBRIDGE,U.K.—In the medieval city where Isaac Newton worked on the gravitational laws, about 850 scientists gathered from 4 to 9 September Martian Methane: Rocky Birth, for the 37th meeting of the American Astro- Then Gone With the Wind? nomical Society’s Division for Planetary Sciences. Last year, a spectrometer on board the Euro- which would then be quickly destroyed by the concentrations of some 10 parts per bil- pean Space Agency’s Mars Express space- oxidation, ultraviolet sunlight, and possibly lion seen in the atmosphere. craft detected methane above areas of the also by electrical activity of atmospheric dust. So where does all the methane go? Given martian surface where there also appears to Atreya says basalt reacts with liquid water that methane concentrations vary widely over be subsurface ice (Science, the martian surface, it must be 1 October 2004, p. 29). Many destroyed too quickly for the gas to researchers hailed the find as pos- Methane muddle. Who’s found the right spread out evenly. The explanation sible evidence that bacteria are liv- concentration, Mars Express or Gemini may lie in the electrostatic charg- ing in the ice and producing the South (inset)? ing of dust particles, says Atreya. gas. After all, almost all the In small dust devils and larger dust methane in Earth’s atmosphere is storms, electric fields as strong as produced by living organisms. 25 kilovolts per meter could be Indeed, says planetary scientist produced. Such voltages would Sushil Atreya of the Uni- break up water molecules, and the versity of Michigan, hydroxyl molecules created would Ann Arbor, many then oxidize methane. -
Annual Review 2011/12
UCL DEPARTMENT OF PHYSICS AND ASTRONOMY PHYSICS AND ASTRONOMY 2011–12 ANNUAL REVIEW PHYSICS AND ASTRONOMY ANNUAL REVIEW 2011–12 Contents Welcome It is an honour to write this WELCOME 1 introduction standing, to misquote Newton, on the shoulders of giants. COMMUNITY FOCUS 3 Jonathan Tennyson finished his Teaching Lowdown 4 tenure as Head of Department in September 2011 and so the majority Student Accolades 4 of the material contained in this Outstanding PhD Theses Published 5 Review records achievements under his leadership. In addition, Tony Career Profiles 6 Harker is currently acting as Head of Science in Action 8 Department in many matters and will continue to do so until October 2012. Alumni Matters 9 This is due to my on-going commitments with the ATLAS experiment on the ACADEMIC SHOWCASE 11 Large Hadron Collider (LHC) at CERN. Staff Accolades 12 I currently spend a large amount of my time in Geneva and I am very grateful Academic Appointments 14 to both Tony and Jonathan, as well as to other members of staff for helping Doctor of Philosophy (PhD) 15 to make this transition a success. In Portrait of Dr Phil Jones 16 particular I would also like to thank Hilary Wigmore as Departmental Manager and Raman Prinja as the new Director of RESEARCH SPOTLIGHT 17 Teaching for their continued support. Atomic, Molecular, Optical and Position Physics (AMOPP) 19 High Energy Physics (HEP) 21 “Success in such long- Condensed Matter and term, high-impact projects Materials Physics (CMMP) 25 requires sustained vision Astrophysics (Astro) 29 and dedicated work by Biological Physics (BioP) 33 excellent scientists over Research Statistics 35 many years.” Staff Snapshot 38 Underpinning this success is the outstanding quality of scientific research and education within the Department. -
UNIVERSITY COLLEGE LONDON Understanding the Distribution Of
UNIVERSITY COLLEGE LONDON Department of Physics & Astronomy Understanding the distribution of gas in the Universe Teresita Suarez´ Noguez Thesis presented for the Degree of Doctor of Philosophy Supervisors: Examiners: Dr Andrew Pontzen Prof. Richard Ellis Prof. Hiranya V. Peiris Dr James Bolton January 25, 2018 Declaration I, Teresita Suarez´ Noguez , declare that the thesis entitled Understanding the distribution of gas in the Universe and the work presented in the thesis are both my own, and have been generated by me as the result of my own original research. I confirm the thesis is based on work done by myself jointly with others, I have made clear exactly what was done by others and what I have contributed myself. This work has not been submitted for any other degree at UCL or any other University. London, January 25, 2018 Teresita Suarez´ Noguez Understanding the distribution of gas in the Universe Teresita Suarez´ Noguez Abstract The distribution of gas in the Universe can be observed in absorption in the spectra of quasars. However, interpreting the spectra requires comparison to physical models which map the distribution, temperatures and ionisation states of the gas. First, I focused on understanding the presence of outflowing cold gas around galaxies. I performed numerical simulations to study how outflows, launched from a central galaxy undergoing starbursts, affect the circumgalactic medium. I model an outflow as a rapidly moving bubble of gas above the disk and analyse its evolution. I sampled a distribution of parameters with a grid of two-dimensional hydrodynamical simulations –with and without– radiative cooling, assuming primordial gas composition. -
The Observatory Founded in 1877 by Sir William Christie, Astronomer Royal
The Observatory Founded in 1877 by Sir William Christie, Astronomer Royal EditEd by D. J. SticklanD R. W. ARgyle S. J. Fossey eDitors 1877–2013 W. H. m. Christie 1877–1882 P. J. d. Gething 1954–1956 E. W. maunder 1881–1887 d. W. dewhirst 1956–1957 A. m. W. downing 1885–1887 A. Hewish 1957–1961 t. lewis 1885–1887 W. R. Hindmarsh 1957–1961 and 1893–1912 b. E. J. Pagel 1961–1962 A. A. Common 1888–1892 J. E. baldwin 1961–1962 H. H. turner 1888–1897 d. mcNally 1961–1963 H. P. Hollis 1893–1912 C. A. murray 1961–1966 S. Chapman 1913–1914 P. A. Wayman 1962–1964 A. S. Eddington 1913–1919 R. V. Willstrop 1963–1966 F. J. m. Stratton 1913–1925 R. F. Griffin 1963–1985 H. Spencer Jones 1915–1923 J. b. Alexander 1964–1965 J. Jackson 1920–1927 S. V. m. Clube 1965–1966 W. m. H. Greaves 1924–1932 K. b. Gebbie 1966–1968 J. A. Carroll 1926–1931 W. Nicholson 1966–1973 G. merton 1928 d. lynden-bell 1967–1969 W. H. Steavenson 1929–1933 C. Jordan 1968–1973 H. W. Newton 1929–1936 R. G. bingham 1969–1972 R. o. Redman 1932–1935 m. V. Penston 1972–1975 R. v. d. R. Woolley 1933–1939 S. J. burnell 1973–1976 W. H. mcCrea 1935–1937 d. H. P. Jones 1973–1977 H. F. Finch 1936–1947 P. J. Andrews 1975–1983 A. d. thackeray 1938–1942 G. G. Pooley 1976–1984 G. C. mcVittie 1938–1948 R. -
High-Sensitivity Radio Astronomy
High-Sensitivity Radio Astronomy Proceedings of a meeting held at Jodrell Bank, University of Manchester January 22-26, 1996 Edited by N. Jackson R. J. Davis Jodrell Bank, Nuffield Radio Astronomy Laboratories, University of Manchester CAMBRIDGE UNIVERSITY PRESS Contents Participants xi Preface xv Foreword xvii Acknowledgements xviii Planets, stars and pulsars Longitudinal asymmetry of Jupiter's radiation belts after the encounter with comet D/Shoemaker-Levy 9 Richard Strom, Imke de Pater and Floris van der Tak 2 Pulsars at the highest radio frequencies Richard Wielebinski 6 Present and future pulsar searches F. Camilo 14 The study of stellar radio emission with very large aperture radio telescopes E.R. Seaquist 23 High-resolution. MERLIN maps of the radio emission from Nova Cygni 1992 and Nova Cassiopeiae 1993 Stewart Eyres, Richard Davis, Mike Bode and Huw Lloyd 33 Orbital motion and a model for HM Sge H.T. Kenny, A.R. Taylor, S. Kwok, S.P.S. Eyres and R.J. Davis 37 Variable sources and jets in Cepheus A V.A. Hughes 42 A radio survey of southern X-ray binary stars R.E. Spencer, A.K. Tzioumis, L.R. Ball, 5.J. Newell and V. Migenes 46 MERLIN astrometry of radio stars S.T. Garrington, R.J. Davis, L.V. Morrison and R.W. Argyle 50 High-sensitivity radio observations of the 8.665-GHz 3He+ hyperfme line emission from planetary nebulae D.S. Balser, T.M. Bania, R.T. Rood and T.L. Wilson 53 High-resolution observations of young planetary nebulae M. Bryce, A. Pedlar, T. Muxlow, P. -
List of Participants
COSMO 2014 August 25-29, 2014 International Conference on Particle Physics and Cosmology, 2014 Chicago, IL http://cosmo2014.uchicago.edu/ LIST OF PARTICIPANTS http://kicp.uchicago.edu/ http://www.nsf.gov/ http://www.kavlifoundation.org/ http://www.uchicago.edu/ The 18th annual International Conference on Particle Physics and Cosmology (COSMO 2014) will be held in Chicago on August 25 29, 2014. The meeting is being hosted by the Kavli Institute for Cosmological Physics (KICP) at the University of Chicago, and will be held at the University of Chicago's Gleacher Center in downtown Chicago. Plenary Speakers Nima Arkani-Hamed Laura Baudis Stefano Borgani Institute for Advanced Study University of Zurich Astronomical Observatory of Trieste Kiwoon Choi Ryan Foley Wendy Freedman Institute for Basic Science (IBS) University of Illinois, Urbana-Champaign Carnegie Observatories Daniel Green Catherine Heymans Justin Khoury CITA University of Edinburgh University of Pennsylvania Will Kinney Lloyd Knox John Kovac University at Buffalo, SUNY UC Davis Harvard University Andrei Linde Nikhil Padmanabhan Hiranya Peiris Stanford University Yale University University College London Sarah Shandera Eva Silverstein Tracy Slatyer Pennsylvania State University Stanford University Massachusetts Institute of Technology Mark Trodden Neal Weiner University of Pennsylvania New York University International Steering Committee Vernon Barger Daniel Baumann John Beacom University of Wisconsin-Madison Cambridge University Ohio State University David Caldwell Jonathan Ellis -
NL#153 July/August
AAAS Publication for the members N of the Americanewsletter Astronomical Society July/August 2010, Issue 153 CONTENTS President's Column Debra Meloy Elmegreen, [email protected] 2 th From the Moon over Miami, palm trees, and a riverwalk set the perfect scene for our 216 meeting, a typically intimate summer gathering with about 800 attendees. Kudos and thanks to Kevin and Executive Office his Marvel-ous staff for another smooth and well-executed gathering. It was all the more special because of meeting jointly with the Solar Physics Division, which happens every three years. It is nice when the smaller divisions are able to overlap with the general meeting, to foster more interactions among astronomers who work in a variety of fields. Dramatic results from new 3 missions such as Herschel, Hinode and SDO, WISE, CoRot, Cassini-Huygens observations of Journals Update Titan, CMB observations from the South Pole, progress on ALMA, and solar tales from SPD Hale prize winner Marcia Neugebauer and Harvey prize winner Brian Welsch were among the many exciting presentations. 4 Three newly funded opportunities were announced: the Doxsey Award for thesis-presenting Council Actions graduate students to travel to the AAS, the Lancelot Berkeley Prize for meritorious recently published research to be presented at the AAS, and the Kavli Award to a distinguished plenary AAS speaker, as discussed elsewhere in this Newsletter. 5 I was thinking about what makes AAS meetings special. We gather for the science, of course; the general meetings provide opportunities to get a firsthand update on key advances, which help Secretary's Corner inform not only our research but also our teaching. -
MOONS of the SOLAR SYSTEM Titan Narrator
MOONS OF THE SOLAR SYSTEM Titan Narrator: There is only one moon in the whole Solar system with an atmosphere . Titan, largest moon of Saturn. Shrouded in thick haze, until recently the surface of this mysterious world remained a mystery. Professor John Zarnecki: Every time I look through the telescope and I see Titan I find it incredible to think that something we designed and built is sitting there on the surface. It landed in 2005. It's there now . it will always be there. Incredible. Dr Athena Coustenis: Titan is a very intriguing object. It has been so for centuries now, though we have been studying it for 350 years. We had never been able to glimpse through its thick atmosphere before and so with Cassini Huygens this was our chance to go there and explore this exciting new world. Clip: And lift off of the Cassini Spacecraft on a billion mile trek to Saturn. Narrrator: Launched in 1997, the Cassini Huygens spacecraft was the most ambitious mission ever sent to the outer solar system. The massive Cassini orbiter carried with it a tiny lander called Huygens. Dr Athena Coustenis: It took seven and a half years to bring the orbiter and the probe it was carrying out of the Saturnian system the Huygens probe was launched into Titan in December 2004 and made a fantastic descent January 2005 through Titan’s atmosphere, landed on the surface. I think it has been the most thrilling moment in my whole career. Professor John Zarnecki: The probe carried six instruments and one of those was ours, led by the Open University and it measured a whole range of parameters on the surface and ours was the first instrument to touch the surface when we landed Mark Leese: When we were initially designing the instrument we were told that we would get a maximum of three minutes on the surface before the probe died.