Spaceflight a British Interplanetary Society Publication
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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 -
APSCC Monthly E-Newsletter JUNE 2017
APSCC Monthly e-Newsletter JUNE 2017 The Asia-Pacific Satellite Communications Council (APSCC) e-Newsletter is produced on a monthly basis as part of APSCC’s information services for members and professionals in the satellite industry. Subscribe to the APSCC monthly newsletter and be updated with the latest satellite industry news as well as APSCC activities! To renew your subscription, please visit www.apscc.or.kr/sub4_5.asp. To unsubscribe, send an email to [email protected] with a title “Unsubscribe.” News in this issue has been collected from 1 May to 31 May. INSIDE APSCC APSCC 2017 Satellite Conference & Exhibition, 10-12 October, Tokyo, Japan The APSCC Satellite Conference and Exhibition is Asia’s must-attend executive conference for the satellite and space industry, where business leaders come together to gain market insight, strike partnerships and conclude major deals. Celebrating its 20th annual event APSCC 2017 #SATECHexplorer will incorporate industry veterans and new players through the 3-day of in-depth conference program to reach out to a broader audience. Join APSCC 2017 and expand your business network while hearing from a broad range of thought-provoking panels and speakers representing visionary ideas and years of business experience in the industry. For more information, please visit www.apscc2017.com SATELLITE BUSINESS Comtech EF Data Announces Deployments Valued at $1.6 Million of Heights Networking Products in Asia May 1, 2017 - Comtech Telecommunications Corp. announced that three different customers of Comtech EF Data Corp., which is part of Comtech's Commercial Solutions segment, have installed, accepted and are now using the industry-leading Heights Networking Platform to support their business needs. -
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. -
(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 -
Analysis, Optimization & Construction of a Micro-Satellite for the Study Of
University of Patras School of Engineering Mechanical Engineering & Aeronautics Department Applied Mechanics and Vibrations Laboratory Ph.D. Dissertation Design, Analysis and Optimization of a Micro-Satellite for the Study of Lower Thermosphere and Re-Entry conditions Andreas G. Ampatzoglou Dipl. Ing. Mechanical & Aeronautics Patras, 2017 Page 1 Ph.D. Dissertation Andreas G. Ampatzoglou This page has been left blank intentionally Page 1 Ph.D. Dissertation Andreas G. Ampatzoglou This thesis is dedicated to my father Sky is not the limit, when there are footprints on the moon! Paul Brandt Page 2 Ph.D. Dissertation Andreas G. Ampatzoglou This page has been left blank intentionally Page 3 Ph.D. Dissertation Andreas G. Ampatzoglou Examination Committee 1. Professor Vassilis Kostopoulos (Thesis supervisor) Mechanical Engineering and Aeronautics Department, University of Patras, Greece 2. Professor Dimosthenis Polyzos (Thesis advisor) Mechanical Engineering and Aeronautics Department, University of Patras, Greece 3. Professor Nick Anifantis (Thesis advisor) Mechanical Engineering and Aeronautics Department, University of Patras, Greece 4. Professor Antonis Tsourdos School of Aerospace, Transport and Manufacturing, Cranfield University, UK 5. Professor Theodoros Loutas Mechanical Engineering and Aeronautics Department, University of Patras, Greece 6. Professor Antonis Tzes Electrical and Computer Engineering Department, University of Patras, Greece 7. Professor Ioannis Daglis Physics Department, National and Kapodistrian University of Athens, Greece Page 4 Ph.D. Dissertation Andreas G. Ampatzoglou Page 5 Ph.D. Dissertation Andreas G. Ampatzoglou Acknowledgements As this thesis is a collection of works of a collection of people contributing to this final manuscript, I would like to talk a little about all these different people and their role in making this possible. -
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. -
Spaceflight Affects Neuronal Morphology and Alters Transcellular Degradation of Neuronal Debris in Adult Caenorhabditis Elegans
SPACEFLIGHT AFFECTS NEURONAL MORPHOLOGY AND ALTERS TRANSCELLULAR DEGRADATION OF NEURONAL DEBRIS IN ADULT CAENORHABDITIS ELEGANS The Texas Tech community has made this publication openly available. Please share how this access benefits you. Your story matters to us. Citation Ricardo Laranjeiro, Girish Harinath, Amelia K. Pollard, Christopher J. Gaffney, Colleen S. Deane, Siva A. Vanapalli, Timothy Etheridge, Nathaniel J. Szewczyk, Monica Driscoll, Spaceflight affects neuronal morphology and alters transcellular degradation of neuronal debris in adult Caenorhabditis elegans, iScience, Volume 24, Issue 2, 2021, https://doi.org/10.1016/j.isci.2021.102105. Citable Link https://hdl.handle.net/2346/87737 Terms of Use CC BY 4.0 Title page template design credit to Harvard DASH. iScience ll OPEN ACCESS Article Spaceflight affects neuronal morphology and alters transcellular degradation of neuronal debris in adult Caenorhabditis elegans Ricardo Laranjeiro, Girish Harinath, Amelia K. Pollard, ..., Timothy Etheridge, Nathaniel J. Szewczyk, Monica Driscoll ricardo_laranjeiro@hotmail. com HIGHLIGHTS Spaceflight induces morphological remodeling of adult neurons in C. elegans Hyperbranching is a common response of adult neurons to spaceflight Neuronal debris accumulates in the hypodermis of proteo- stressed space-flown animals Laranjeiro et al., iScience 24, 102105 February 19, 2021 ª 2021 The Author(s). https://doi.org/10.1016/ j.isci.2021.102105 iScience ll OPEN ACCESS Article Spaceflight affects neuronal morphology and alters transcellular degradation of neuronal debris in adult Caenorhabditis elegans Ricardo Laranjeiro,1,7,* Girish Harinath,1 Amelia K. Pollard,2 Christopher J. Gaffney,3,4 Colleen S. Deane,3 Siva A. Vanapalli,5 Timothy Etheridge,3 Nathaniel J. Szewczyk,2,6 and Monica Driscoll1 SUMMARY Extended space travel is a goal of government space agencies and private com- panies. -
New Scientist's
PHOTO ESSAY MISSION ICARUS The Parker Solar Probe is about to take us closer to the sun than ever before. It’s an audacious mission that will test technology – and the nerves of the scientists behind it – to the limit Interviews by Richard Webb. Photos by Michael Soluri 31 March 2018 | NewScientist | 37 180331_F_Probe_roughcm.indd 37 03/04/2018 16:08 PHOTO ESSAY PHOTO ESSAY Our sun is no serene orb. Every now particles were moving very freely Previous page: The Parker Solar Above: A silver blanket covering the The solar wind doesn’t just break front surface, and we had to make and then its fiery surface turns from sun to Earth. Around the same Probe being tested at the Goddard probe will protect its instruments away from the sun, it carries the sun’s sure there would only be 30 watts explosive, sending matter, energy time, astronomers were noting that Space Flight Center in Maryland from the sun. One of its two solar magnetic field with it somehow. on the back side. There are some and magnetism whirling into the comet tails always pointed away panels will attach to the pair of Whatever state the field is in, whatever high-temperature metals that could surrounding vacuum. from the sun, and that, too, was very Above: A mock-up of the mounts at the bottom of the shot direction, however strong it is, it is make the protective shield, but they In 1859, a particularly violent difficult to explain. instrument that will observe frozen into the solar wind. That’s what are too heavy to launch. -
A Laboratory Model for the Parker Spiral and Magnetized Stellar Winds
ARTICLES https://doi.org/10.1038/s41567-019-0592-7 A laboratory model for the Parker spiral and magnetized stellar winds Ethan E. Peterson 1*, Douglass A. Endrizzi 1, Matthew Beidler2,3, Kyle J. Bunkers 1, Michael Clark1, Jan Egedal1, Ken Flanagan 1, Karsten J. McCollam1, Jason Milhone 1, Joseph Olson 1, Carl R. Sovinec 2, Roger Waleffe 1, John Wallace1 and Cary B. Forest1 Many rotating stars have magnetic fields that interact with the winds they produce. The Sun is no exception. The interaction between the Sun’s magnetic field and the solar wind gives rise to the heliospheric magnetic field—a spiralling magnetic struc- ture, known as the Parker spiral, which pervades the Solar System. This magnetic field is critical for governing plasma processes that source the solar wind. Here, we report the creation of a laboratory model of the Parker spiral system based on a rapidly rotating plasma magnetosphere and the measurement of its global structure and dynamic behaviour. This laboratory system exhibits regions where the plasma flows evolve in a similar manner to many magnetized stellar winds. We observe the advec- tion of the magnetic field into an Archimedean spiral and the ejection of quasi-periodic plasma blobs into the stellar outflow, which mimics the observed plasmoids that fuel the slow solar wind. This process involves magnetic reconnection and can be modelled numerically by the inclusion of two-fluid effects in the simulation. The Parker spiral system mimicked in the labora- tory can be used for studying solar wind dynamics in a complementary fashion to conventional space missions such as NASA’s Parker Solar Probe mission. -
Debris Mitigation, Assembly, Integration, and Test, in the Context of the Istsat-1 Project
Debris Mitigation, Assembly, Integration, and Test, in the context of the ISTsat-1 project Paulo Luís Granja Macedo Thesis to obtain the Master of Science Degree in Aerospace Engineering Supervisors: Prof. Paulo Jorge Soares Gil Prof. Agostinho Rui Alves da Fonseca Examination Committee Chairperson: Prof. José Fernando Alves da Silva Supervisor: Prof. Paulo Jorge Soares Gil Member of the Committee: Prof. Elsa Maria Pires Henriques November 2018 ii Dedicado ao meu Pai, Mae˜ e Irma˜ iii iv Acknowledgments I want to thank my supervisors, Professor Paulo Gil and Professor Agostinho Fonseca, for guiding me thorough the project. I also want to thank the ISTsat-1 team members, both professors and students, for giving me the opportunity to be part of such a great project and for the availability they had for my questions. The project would not happen if we did not have the University help and the ESA initiative Fly Your Satellite. I want to thank both organizations, that provided and will keep providing financial support, development rooms, test facilities and expertise in Space related matters. I want to thank all the other people that helped me through this phase, my fiends and girlfriend, thank you. Tambem´ quero agradecer aos meus pais e irma,˜ que me ajudaram em tudo o que foi preciso para chegar a este dia, sem eles nao˜ seria poss´ıvel. Obrigado. v vi Resumo O ISTsat-1 e´ um CubeSat desenvolvido por estudantes e professores do Instituto Superior Tecnico´ (IST), com a ajuda de um programa da ESA chamado Fly Your Satellite (FYS). O objectivo principal e´ educar estudantes em cienciaˆ e tecnologia espacial.