Science Data Management Plan
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Program Book Update
15th Annual International Astrophysics Conference Cape Coral, FL – April 3-8, 2016 AGENDA SUNDAY, APRIL 3 5:00 PM – 8:00 PM Registration – Tarpon Terrace 6:00 PM – 9:00 PM Welcome Reception - Tarpon Terrace MONDAY, APRIL 4 7:00 AM - 5:00 PM Registration – Grandville Ballroom 8:00 AM – 6:00 PM GENERAL SESSION – Grandville Ballroom CHAIR: Zank 7:45 AM - 8:00 AM GARY ZANK WELCOME 8:00 AM - 8:25 AM Chen, Bin Particle Acceleration by a Solar Flare Termination Shock 8:25 AM - 8:50 AM Bucik, Radoslav Large-scale Coronal Waves in 3He-rich Solar Energetic Particle Events Element Abundances and Source Plasma Temperatures of 8:50 AM - 9:15 AM Reames, Donald Solar Energetic Particles 9:15 AM - 9:40 AM Manchester, Ward Simulating CME-Driven Shocks and Implications for SEPs STEREO and ACE SEP Science- Transforming Space Weather 9:40 AM - 10:05 AM Luhmann, Janet Prospects 10:05 AM - 10:30 AM Morning Break - Ballroom Foyer CHAIR: Zirnstein 11 years of ENA imaging with Cassini/INCA and in-situ ion Voyager1 & 10:30 AM - 10:55 AM Krimigis, Stamatios 2/LECP measurements Investigating the Heliospheric Boundary at Energies down to 10eV with 10:55 AM - 11:20 AM Wurz, Peter Neutral Atom Imaging by IBEX. In-situ and Remote Sensing Studies of Solar Wind Origin and 11:20 AM - 11:45 AM Landi, Enrico Acceleration The Sun’s Dynamic Influence on the Outer Heliosphere, the Heliosheath, 11:45 AM - 12:10 PM Intriligator, Devrie and the Local Interstellar Medium 12:10 PM – 1:30 PM Lunch Break – Ballroom Foyer CHAIR: Fichtner 1:30 PM - 1:55 PM McNutt, Ralph Making Interstellar -
Spaceflight a British Interplanetary Society Publication
SpaceFlight A British Interplanetary Society publication Volume 61 No.2 February 2019 £5.25 Sun-skimmer phones home Rolex in space Skyrora soars ESA uploads 02> to the ISS 634089 From polar platform 770038 to free-flier 9 CONTENTS Features 18 Satellites, lightning trackers and space robots Space historian Gerard van de Haar FBIS has researched the plethora of European payloads carried to the International Space Station by SpaceX Dragon capsules. He describes the wide range of scientific and technical experiments 4 supporting a wide range of research initiatives. Letter from the Editor 24 In search of a role Without specific planning, this Former scientist and spacecraft engineer Dr Bob issue responds to an influx of Parkinson MBE, FBIS takes us back to the news about unmanned space vehicles departing, dying out and origins of the International Space Station and arriving at their intended explains his own role in helping to bring about a destinations. Pretty exciting stuff British contribution – only to see it migrate to an – except the dying bit because it unmanned environmental monitoring platform. appears that Opportunity, roving around Mars for more than 14 30 Shake, rattle and Rolex 18 years, has finally succumbed to a On the 100th anniversary of the company’s birth, global dust storm. Philip Corneille traces the international story Some 12 pages of this issue are behind a range of Rolex watches used by concerned with aspects of the astronauts and cosmonauts in training and in International Space Station, now well into its stride as a research space, plus one that made it to the Moon. -
Aphelion) 25/02/04 16:20 Page 1
SORTIE (Aphelion) 25/02/04 16:20 Page 1 Aphelion™ IMAGE PROCESSING AND IMAGE ANALYSIS SOFTWARE TO FACE NEW CHALLENGES ORGANIZATIONS ALREADY USING APHELION™ 3M (USA) Halliburton (USA) Procter & Gamble (USA & Europe) Arcelor (Europe) Hewlett-Packard (UK) Queen’s College (UK) Boeing Aerospace (USA) Hitachi (Japan) Rolls Royce (UK) CEA (France) Hoya (Japan) SNECMA Moteurs (France) CNRS (France) Joint Research Center (Europe) Thales (France) CSIRO (Australia) Kawasaki Heavy Industry (Japan) Toshiba (Japan) Corning (France) Kodak Industrie (France) Université de Lausanne (Switzerland) Dako (USA) Lilly (USA) Université de Liège (Belgium) Dornier (Germany) Lockheed Martin (USA) University of Massachusetts (USA) EADS (France) Mitsubishi (Japan) Unilever (UK) Ecole de Technologie Supérieure (Canada) Nikon (Japan) US Navy (USA) FedEx (USA) Nissan (Japan) Volvo Aero Corporation (Sweden) FAO, Defence Research Establishment (Sweden) Pechiney (France) Xerox (USA) Ford (USA) Peugeot-Citroën (France) Framatome (France) Philips (France) Aphelion IMAGE PROCESSING IMAGE PROCESSING AND IMAGE ANALYSIS SOFTWARE TO FACE NEW CHALLENGE AND IMAGE ANALYSIS SOFTWARE TO FACE NEW CHALLENGES PRODUCT DISTRIBUTION Licensing: Single-user license & site license for end-users Run-time licenses for OEMs Downloadable from web Standard package: APHELION™ Developer includes all the standard libraries available as DLLs & ActiveX components, development capabilities, and the graphical user interface BIOLOGY / COSMETICS / GEOLOGY INSPECTION / MATERIALS SCIENCE Optional modules: 3D Image Processing METROLOGY 3D Image Display OBJECT RECOGNITION Recognition Toolkit VisionTutor, a computer vision course including extensive exercises PHARMACOLOGY / QUALITY CONTROL / REMOTE SENSING / ROBOTICS Interface to a wide variety of frame grabber boards SECURITY / TRACKING Twain interface to control scanners and digital cameras Video media interface Interface to control microscope stages ActiveX components: Extensive Image Processing libraries for automated applications. -
Letter to Dr. Nicola Fox, Heliophysics Division Director of NASA
Michael W. Liemohn • Professor July 30, 2020 Dr. Nicola Fox, Heliophysics Division Director National Aeronautics and Space Administration Heliophysics Division 300 E Street, SW Washington, DC 20546-0001 Dear Dr. Fox: The Heliophysics Advisory Committee (HPAC), an advisory committee to the Heliophysics Division (HPD) of the National Aeronautics and Space Administration (NASA), convened on 30 June through 1 July 2020, virtually through Webex. The undersigned served as Chair for the meeting with the support of Dr. Janet Kozyra, HPAC Designated Federal Officer (DFO), of NASA-HPD. This letter summarizes the meeting outcomes, including our findings and recommendations. All of the members of HPAC participated. Specifically, the membership of HPAC is as follows: Vassilis Angelopoulos (University of California, Los Angeles), Rebecca Bishop (The Aerospace Corporation), Paul Cassak (West Virginia University), Darko Filipi (BizTek International LLC), Lindsay Glesener (University of Minnesota), Larisa Goncharenko (Massachusetts Institute of Technology (MIT) Haystack Observatory), George Ho (Johns Hopkins University Applied Physics Laboratory), Lynn Kistler (University of New Hampshire), James Klimchuk (NASA Goddard Space Flight Center), Tomoko Matsuo (University of Colorado Boulder), William H. Matthaeus (University of Delaware), Mari Paz Miralles (Smithsonian Astrophysical Observatory), Cora Randall (University of Colorado, Boulder), and me. The meeting opened with you giving an overview of the state of HPD. We were pleased to hear about HPD’s successful recent launch of Solar Orbiter and the healthy status of all of the Heliophysics division missions. This includes the HERMES payload on the Gateway and plans for a request for information regarding community input for instrumentation and spacecraft related to NASA’s return to the moon. -
A Journey of Exploration to the Polar Regions of a Star: Probing the Solar
Experimental Astronomy manuscript No. (will be inserted by the editor) A journey of exploration to the polar regions of a star: probing the solar poles and the heliosphere from high helio-latitude Louise Harra · Vincenzo Andretta · Thierry Appourchaux · Fr´ed´eric Baudin · Luis Bellot-Rubio · Aaron C. Birch · Patrick Boumier · Robert H. Cameron · Matts Carlsson · Thierry Corbard · Jackie Davies · Andrew Fazakerley · Silvano Fineschi · Wolfgang Finsterle · Laurent Gizon · Richard Harrison · Donald M. Hassler · John Leibacher · Paulett Liewer · Malcolm Macdonald · Milan Maksimovic · Neil Murphy · Giampiero Naletto · Giuseppina Nigro · Christopher Owen · Valent´ın Mart´ınez-Pillet · Pierre Rochus · Marco Romoli · Takashi Sekii · Daniele Spadaro · Astrid Veronig · W. Schmutz Received: date / Accepted: date L. Harra PMOD/WRC, Dorfstrasse 33, CH-7260 Davos Dorf and ETH-Z¨urich, Z¨urich, Switzerland E-mail: [email protected]; ORCID: 0000-0001-9457-6200 V. Andretta INAF, Osservatorio Astronomico di Capodimonte, Naples, Italy E-mail: vin- [email protected]; ORCID: 0000-0003-1962-9741 T. Appourchaux Institut d’Astrophysique Spatiale, CNRS, Universit´e Paris–Saclay, France; E-mail: [email protected]; ORCID: 0000-0002-1790-1951 F. Baudin Institut d’Astrophysique Spatiale, CNRS, Universit´e Paris–Saclay, France; E-mail: [email protected]; ORCID: 0000-0001-6213-6382 L. Bellot Rubio Inst. de Astrofisica de Andaluc´ıa, Granada Spain A.C. Birch Max-Planck-Institut f¨ur Sonnensystemforschung, 37077 G¨ottingen, Germany; E-mail: arXiv:2104.10876v1 [astro-ph.SR] 22 Apr 2021 [email protected]; ORCID: 0000-0001-6612-3861 P. Boumier Institut d’Astrophysique Spatiale, CNRS, Universit´e Paris–Saclay, France; E-mail: 2 Louise Harra et al. -
(ISIS): Design of the Energetic Particle Investigation
Space Sci Rev (2016) 204:187–256 DOI 10.1007/s11214-014-0059-1 Integrated Science Investigation of the Sun (ISIS): Design of the Energetic Particle Investigation D.J. McComas · N. Alexander · N. Angold · S. Bale · C. Beebe · B. Birdwell · M. Boyle · J.M. Burgum · J.A. Burnham · E.R. Christian · W.R. Cook · S.A. Cooper · A.C. Cummings · A.J. Davis · M.I. Desai · J. Dickinson · G. Dirks · D.H. Do · N. Fox · J. Giacalone · R.E. Gold · R.S. Gurnee · J.R. Hayes · M.E. Hill · J.C. Kasper · B. Kecman · J. Klemic · S.M. Krimigis · A.W. Labrador · R.S. Layman · R.A. Leske · S. Livi · W.H. Matthaeus · R.L. McNutt Jr · R.A. Mewaldt · D.G. Mitchell · K.S. Nelson · C. Parker · J.S. Rankin · E.C. Roelof · N.A. Schwadron · H. Seifert · S. Shuman · M.R. Stokes · E.C. Stone · J.D. Vandegriff · M. Velli · T.T. von Rosenvinge · S.E. Weidner · M.E. Wiedenbeck · P. Wilson IV Received: 21 February 2014 / Accepted: 16 June 2014 / Published online: 5 July 2014 © The Author(s) 2014. This article is published with open access at Springerlink.com Abstract The Integrated Science Investigation of the Sun (ISIS) is a complete science in- vestigation on the Solar Probe Plus (SPP) mission, which flies to within nine solar radii of the Sun’s surface. ISIS comprises a two-instrument suite to measure energetic parti- D.J. McComas (B) · N. Alexander · N. Angold · C. Beebe · B. Birdwell · M.I. Desai · J. Dickinson · G. Dirks · S. Livi · S.E. Weidner · P. -
Solar Probe Plus (SPP)
Pre-decisional – For NASA Internal Use Only Solar Probe Plus (SPP) Committee on Solar and Space Physics 5 October 2016 Joe Smith Program Executive NASA Headquarters 5 October 2016 1 Solar Probe Plus (SPP) Overview Using in-situ measurements made closer to the Sun than by any previous spacecraft, SPP will determine the mechanisms that produce the fast and slow solar winds, coronal heating, and the transport of energetic particles. Solar Probe Plus will fly to less than 10 solar radii (Rs) of the Sun, having “walked in” from 35 Rs over 24 orbits. Milestones • Sponsor: NASA/GSFC LWS Pre-Phase A: 07/2008 – 11/2009 • LWS Program Manager – Nick Chrissotimos GSFC • LWS Deputy Program Manager – Mark Goans, GSFC Phase A: 12/2009 – 01/2012 • Project Manager – Andy Driesman, APL Phase B: 02/2012 – 03/2014 • Project Scientist – Nicky Fox, APL Phase C/D: 03/2014 – 09/2018 • Spacecraft Development/Operations – APL LRD: 31 July 2018 • Investigations selected by AO: • FIELDS – University of California Phase E: 10/2018 – 09/2025 • ISIS – Princeton University/SwRI • SWEAP – Smithsonian Astrophysical Obs Management Commitment: $1,366M • WISPR – Naval Research Laboratory Category 1, Risk Classification B • HelioOrigins – Jet Propulsion Laboratory 5 October 2016 Solar Probe Plus CSSP 2 50 years into the space age and we still don’t understand the corona and solar wind . The concept for a “Solar Probe” dates back to “Simpson’s Committee” of the Space Science Board (National Academy of Sciences, 24 October 1958) ‒ The need for extraordinary knowledge of Sun from remote observations, theory, and modeling to answer the questions: – Why is the solar corona so much hotter than the photosphere? – How is the solar wind accelerated? . -
Radiation Belt Storm Probes Launch
National Aeronautics and Space Administration PRESS KIT | AUGUST 2012 Radiation Belt Storm Probes Launch www.nasa.gov Table of Contents Radiation Belt Storm Probes Launch ....................................................................................................................... 1 Media Contacts ........................................................................................................................................................ 4 Media Services Information ..................................................................................................................................... 5 NASA’s Radiation Belt Storm Probes ...................................................................................................................... 6 Mission Quick Facts ................................................................................................................................................. 7 Spacecraft Quick Facts ............................................................................................................................................ 8 Spacecraft Details ...................................................................................................................................................10 Mission Overview ...................................................................................................................................................11 RBSP General Science Objectives ........................................................................................................................12 -
[,T,;O1\[ WI':ST,'!':'{J\]\I ACADEMY, Fiaufrvilt,E, Ni:':W Ijkunetwlc'r
PI' 'CIP/\I Ui" CHf: MOUNT 111,[,T,;o1\[ WI':ST,'!':'{J\]\I ACADEMY, fIAUfrVILT,E, Ni:':W IJKUNEtWlC'R. THE PROVIN.CIAL WESLEYAN AL ANACK, 1880: Containing all necessary Astronomical Calculation~; p.. ep~red with ~rQat care for this special ohject; toge~her with a large amount of General Intelligence, Railway, Telegraph and POBt Office Regulations, Religious Statistical Iuformation, with many other matters of PUBLIC AND PROVINCIAL INTEREST, INCLUDING A. HALIFAX BUSINESS CITY DIRECTORY. Prepared expressly for this work; maki-ng it well calcl\latcd for a large circulation as a popular and useful VOLUME II. .iJALIFAX, N. S: PUBLISHED UNDER THE SAN"CTION OF THE EASTERN BRITISH A~lERICAN CONFERENCE. 2 rROVINCIAL WESLEYAN PREFACE. TIIE Publishers of the" Provincial Wesleyan Al.manack" cannot omit the opportunity (in publishing the second yolume) of thanking the public for the very cordial reception givcn to their publication of last year. The most encouraging testimonials have been received from every quarter approving their labors,-a most gratifying proof of which was found in the rapid sale of this Annual last year-the whole edition being exhausted in two months from first· date of issue. A discerning public ,,-ill perceive in evcry page of the present volume the evidences of thought and labor, with a laudable anxiety to secure general approbation. The arrangement of the different departments will be fouud much more complete-a great deal of new matter, not llitherto fOlmd in such a publication, has b.een introduced. Eyery portion has been most carefully revised up to the date of publication. -
David J. Mccomas - Refereed Publications
David J. McComas - Refereed Publications 1982 1. McComas, D.J. and S.J. Bame, Radially Uniform Electron Source, Rev. of Sci. Instrum., 53, 1490-1491, 1982. 2. Feldman, W.C., S.J. Bame, S.P. Gary, J.T. Gosling, D.J. McComas, M.F. Thomsen, G. Paschmann, N. Sckopke, M.M. Hoppe, C.T. Russell, Electron Heating Within the Earth's Bowshock, Phys. Rev. Lett., 49, 199-201,1982. 1983 3. Feldman, W.C., R.C. Anderson, S.J. Bame, S.P. Gary, J.T. Gosling, D.J. McComas, M.F. Thomsen, G. Paschmann, M.M. Hoppe, Electron Velocity Distributions Near the Earth's Bowshock, J. Geophys. Res., 88, 96-110, 1983. 4. Bame, S.J., R.C. Anderson, J.R. Asbridge, D.N. Baker, W.C. Feldman, J.T. Gosling, E.W. Hones, Jr., D.J. McComas, R.D. Zwickl, Plasma Regimes in the Deep Geomagnetic Tail: ISEE-3, Geophys. Res. Lett., 10, 912-915, 1983. 1984 5. McComas, D.J. and S.J. Bame, Channel Multiplier Compatible MaterialsLifetime Tests, Rev. Sci. Inst., 55, 463-467, 1984. 6. Hones, Jr., E.W., D.N. Baker, S.J. Bame, W.C. Feldman, J.T. Gosling, D.J. McComas, R.D. Zwickl, J.A. Slavin., E.J. Smith, B.T. Tsurutani, Structure of the Magnetotail at 220RE its Response to Geomagnetic Activity, Geophys. Res. Lett., 11, 5-7, 1984. 7. Baker, D.N., S.J. Bame, W.C. Feldman, J.T. Gosling, P.R. Higbie, E.W. Hones, Jr., D.J. McComas, R.D. Zwickl, Correlated Dynamical Changes in the Near Earth and Distant Magnetotail Regions: ISEE-3, J. -
WISPR (Wide Field Imager for Solar Probe Plus)
WISPR (Wide Field Imager for Solar Probe Plus) V. Bothmer, R. A. Howard (WISPR PI), A. Vourlidas 22 May 2015 Solar Probe Plus A NASA Mission to Touch the Sun HELCATS First Annual Open Workshop What is Solar Probe Plus (SPP) . Goes to the last unexplored region of the solar system and enter the solar corona as close as 9.86 Rs . Will answer fundamental questions of Heliophysics: The heating of the solar corona The origin, structure and evolution of the solar wind Origin of solar energetic particles . Investigations: FIELDS: measurements of magnetic fields, AC/DC electric fields SWEAP: measurements of flux of electrons, protons and alphas ISIS: measurement of solar energetic particles WISPR: measurement of coronal structures Observatory Scientist HELCATS First Annual Open Workshop SPP Mission Scenario – Observations from 0.25 AU to 9.86 RS HELCATS First Annual Open Workshop 3 SPP Near Sun Perihel Passages Number of Perihel passages < 30 RS (0.14 AU): • First Perihel at 35 RS (0.16 AU) after 88 days • 24 Perihel-passages over the time periofd of 7 years after launch in July 2018 • 1000 hrs of measurements at distances < 20 RS Ref.: NASA STDT HELCATS First Annual Open Workshop 4 Solar Probe Plus Encounter Portion of the Orbit 9.86 Rs HELCATS First Annual Open Workshop Figure 4.2 – Encounter Pass Geometry and Timeline The Deep Space Network (DSN) will be used to communicate with the SPP observatory and collect data required for navigation. Mission operations will be conducted at APL from a single Mission Operations Center (MOC), located at the Johns Hopkins University Applied Physics Laboratory (JHU/APL) in Laurel, Maryland. -
Parker Solar Probe Project Scientist JHU/Applied Physics Laboratory Parker Solar Probe
The Coolest, Hottest Mission under the Sun!! Dr. Nicola J. Fox Parker Solar Probe Project Scientist JHU/Applied Physics Laboratory Parker Solar Probe A NASA Mission to Touch the Sun We are PARKER SOLAR PROBE! Parker, meet Parker December 12, 2017 Parker Solar Probe– Fall AGU 2017 Why haven’t we gone to the Sun yet? It took the same technological leap from a rotary phone to an iPhone X for Parker Solar Probe to become a reality December 12, 2017 Parker Solar Probe– Fall AGU 2017 Parker Solar Probe Science . To determine the structure and dynamics of the Sun’s coronal magnetic field, understand how the solar corona and wind are heated and accelerated, and determine what mechanisms accelerate and transport energetic particles. Detailed Science Objectives • Trace the flow of energy that heats and accelerates the solar corona and solar wind. • Determine the structure and dynamics of the plasma and magnetic fields at the sources of the solar wind. • Explore mechanisms that accelerate and transport energetic particles. November 16, 2017 Parker Solar Probe Mission Briefing Modeling: Providing the missing piece . In-situ data from within 0.25 AU will be available Manchester 2014 shortly after each orbit for ingestion into the coronal, solar wind and global heliospheric models . PSP would also benefit invaluably from knowing the mapping between the spacecraft and the solar surface though each orbit . Global simulations of CMEs would provide critical context when we fly through CMEs . Contact [email protected] or [email protected] Baker