SH21B:
Coordinated Science from the Corona to the Inner Heliosphere in Preparation for Solar Probe Plus and Solar Orbiter I Posters

Tuesday, 16 December 2014: 8:00 AM-12:20 PM
Chairs:  Kelly E Korreck, Smithsonian Observatory, Cambridge, MA, United States and Nathan Schwadron, University of New Hampshire, Durham, NH, United States
Primary Conveners:  Marco M C Velli, Calif Inst of Tech-JPL, Pasadena, CA, United States
Co-conveners:  Nathan Schwadron, University of New Hampshire, Durham, NH, United States, Kelly E Korreck, Smithsonian Observatory, Cambridge, MA, United States and Yannis Zouganelis, European Space Agency, Villanueva De La Can, Spain
OSPA Liaisons:  Kelly E Korreck, Smithsonian Observatory, Cambridge, MA, United States

Abstracts Submitted to this Session:

 
Global Multi-Fluid Solar Corona and Inner Heliosphere Model for Solar Probe Plus and Solar Orbite
Bart van der Holst1, Igor Sokolov1, Gabor Toth1,2 and Tamas I Gombosi1,3, (1)University of Michigan, Ann Arbor, MI, United States, (2)Univ Michigan, Ann Arbor, MI, United States, (3)Univ of Michigan, Ann Arbor, MI, United States
 
Solar Probe Plus: A NASA Mission to Touch the Sun
Nicola Justine Fox, Johns Hopkins Univ Applied Phy, Laurel, MD, United States, Marco M C Velli, Calif Inst of Tech-JPL, Pasadena, CA, United States, Justin Christophe Kasper, University of Michigan, Ann Arbor, MI, United States, David J McComas, Southwest Research Institute San Antonio, San Antonio, TX, United States, Russell Howard, U.S. Naval Research Laboratory, Washington, DC, United States, Stuart D Bale, University of California Berkeley, Berkeley, CA, United States and Robert B Decker, Johns Hopkins Applied Physics Laboratory, Laurel, United States
 
Alfvenic Fluctuations in the Inner Heliosphere: Implications for Solar Orbiter and Solar Probe Plus
Timothy Simon Horbury, Imperial College London, London, SW7, United Kingdom and Lorenzo Matteini, Imperial College London, London, United Kingdom
 
3D Visualization of Solar Data: Preparing for Solar Orbiter and Solar Probe Plus
Daniel Mueller1, Simon Felix2, Stefan Meier2, Andre Csillaghy2, Bogdan Nicula3, Freek Verstringe3, Bram Bourgoignie3, David Berghmans3 and Piers Jiggens4, (1)European Space Agency, ESTEC, Villanueva De La Can, Spain, (2)University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland, (3)Royal Observatory of Belgium, Brussels, Belgium, (4)European Space Agency, ESTEC, Noordwijk, Netherlands
 
The Energetic Particle Detector (EPD) for Solar Orbiter – Sensor Status and Calibration
R F Wimmer-Schweingruber1, Javier Rodriguez-Pacheco2, Glenn M Mason3, Cesar Martin-Garcia1, Manuel Prieto2, Stephan I Böttcher1, Shrinivasrao R. Kulkarni1, Lauri Panitzsch1, Sebastian Sanchez2, George C Ho2, Jan Kohler1, Raul Gomez-Herrero2 and Juan Jose Blanco2, (1)University of Kiel, Kiel, Germany, (2)University of Alcala, Alcala de Henarez, Spain, (3)JHU / APL, Laurel, MD, United States
 
Implications of the S-Web for the Corona and Inner Heliosphere
Spiro K Antiochos, NASA GSFC, Silver Spring, MD, United States
 
Synthetic White-light Imagery for the Wide-field Imager for Solar Probe Plus (WISPR)
Paulett Creyke Liewer1, Yubo Su1, Angelos Vourlidas2, Arnaud F Thernisien3, Russell Howard2, Jeffrey R Hall1 and Eric DeJong1, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Naval Research Laboratory, Washington, DC, United States, (3)George Mason University Fairfax, Fairfax, VA, United States
 
Testing the Solar Probe Cup, An Instrument Designed to Touch the Sun
Phyllis L Whittlesey1, Anthony W Case2, Justin Christophe Kasper3, Kenneth H Wright Jr1, Ben Alterman3, Jonathan W Cirtain4, Jay Bookbinder5, Kelly E Korreck6 and Michael Louis Stevens7, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (3)University of Michigan, Ann Arbor, MI, United States, (4)NASA Marshall Space Flight Center, Huntsville, AL, United States, (5)Smithsonian Astrophysical Obse, Cambridge, MA, United States, (6)Smithsonian Observatory, Cambridge, MA, United States, (7)Smithsonian Astrophysics Observatory, Cambridge, MA, United States
 
Numerical Techniques for Removing Instrumental Noise in the Solar Probe Plus/FIELDS Search Coil Magnetometer
Trevor A Bowen1, Stuart D Bale1, Davin E Larson2, Thierry Dudok de Wit3 and Robert J. MacDowall4, (1)University of California Berkeley, Berkeley, CA, United States, (2)Space Sciences Laboratory, Berkeley, CA, United States, (3)University of Orleans, Orleans, France, (4)NASA Goddard SFC, Greenbelt, MD, United States
 
The Form of Proton Energy Spectra from Self-Consistent Simulations of the Coronal Shock Acceleration
Alexandr N. Afanasiev, Rami O Vainio and Markus C Battarbee, University of Turku, Turku, Finland
 
Probing the inner heliosphere and corona with electric antennas: quasi-thermal noise spectroscopy on Solar Orbiter and Solar Probe Plus.
Michel Moncuquet1, Yannis Zouganelis2, Nicole Meyer-Vernet1, Karine Issautier1, Arnaud Zaslavsky3, Milan Maksimovic1, Gaetan LE CHAT4 and Mihailo Martinovic4, (1)CNRS, Observatoire de Paris, LESIA, Meudon, France, (2)European Space Agency, Villanueva De La Can, Spain, (3)University Pierre and Marie Curie Paris VI, LESIA - Observatoire de Paris, Paris, France, (4)Paris Observatory Meudon, LESIA, Meudon, France
 
Photoelectron and Secondary Electron Dynamics Around the Solar Probe Plus Spacecraft
Yohei Miyake and Hideyuki Usui, Kobe University, Kobe, Japan
 
Automated tracing of open-field coronal structures for an optimized large-scale magnetic field reconstruction
Vadim M Uritsky1, Joseph M Davila2 and Shaela I Jones1, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)NASA Goddard SFC, Greenbelt, MD, United States
 
Instant: An Innovative L5 Small Mission Concept for Coordinated Science with Solar Orbiter and Solar Probe Plus
Benoit Lavraud1, Ying D. Liu2, Richard Anthony Harrison3, William Liu2, Frederic Auchere4, Weiqun Gan5, Philippe L Lamy6, Lidong Xia7, Jonathan P Eastwood8, R F Wimmer-Schweingruber9, Qiugang Zong10, Pierre Rochus11, Milan Maksimovic12, Manuela Temmer13, C Philippe Escoubet14, Emilia Kilpua15, Alexis P Rouillard16, Jackie A Davies17, Jean-Claude Vial4, Nat Gopalswamy18, Stuart D Bale19, Gang Li20, Timothy A Howard21 and Craig E DeForest22, (1)IRAP, Toulouse, France, (2)NSSC National Space Science Center, CAS, Beijing, China, (3)Rutherford Appleton Laboratory, Didcot, OX11, United Kingdom, (4)IAS Institut d'Astrophysique Spatiale, Orsay Cedex, France, (5)Purple Mountain Observatory, Nanjing, China, (6)Lab Astrophysique Marseille, Marseilles Cedex 13, France, (7)Shandong Univ. at Weihai, Weihai, China, (8)Imperial College London, London, United Kingdom, (9)University of Kiel, Kiel, Germany, (10)Peking University, Beijing, China, (11)Centre Spatial de Liege, Liege, Belgium, (12)CNRS, Paris Cedex 16, France, (13)University of Graz, Graz, Austria, (14)ESTEC, Noordwijk, 2201, Netherlands, (15)University of Helsinki, Helsinki, Finland, (16)IRAP/CNRS, Toulouse, France, (17)Rutherford Appleton Laboratory, Didcot, United Kingdom, (18)NASA Goddard SFC, Greenbelt, MD, United States, (19)University of California Berkeley, Berkeley, CA, United States, (20)University of Alabama in Huntsville, Huntsville, AL, United States, (21)Southwest Research Institute Boulder, Boulder, CO, United States, (22)Southwest Research Institute, Boulder, CO, United States
 
Properties of Mlso MK3 White-Light CMEs from 1989-1996
O C St Cyr1, Quincy Flint1, Hong Xie2, David F Webb3, Joan Burkepile4 and Alice R Lecinski4, (1)NASA Goddard Space Flight Center, Code 670, Greenbelt, MD, United States, (2)NASA/GSFC, Greenbelt, MD, United States, (3)Boston College, Chestnut Hill, MA, United States, (4)NCAR, Boulder, CO, United States
 
Fast solar wind measurements from the Bright Monitor of the Solar Wind instrument on Spektr-R
Jean-Louis Zerbo1, Jana Safrankova2, Zdenek Nemecek2, Georgy N Zastenker3, Justin Christophe Kasper4, Michael Louis Stevens5 and John D Richardson6, (1)Massachusetts Institute of Technology, Cambridge, MA, United States, (2)Charles University, Prague, Czech Republic, (3)Inst Space Research, Moscow, Russia, (4)University of Michigan, Ann Arbor, MI, United States, (5)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (6)MIT, Cambridge, MA, United States
 
Software Development for Jointly Analyzing Thermal-Ion Measurements from Multiple In-Situ Instruments
Bennett Maruca, University of California Berkeley, Berkeley, CA, United States, Michael Louis Stevens, Smithsonian Astrophysics Observatory, Cambridge, MA, United States, Justin Christophe Kasper, University of Michigan, Ann Arbor, MI, United States and Kelly E Korreck, Smithsonian Observatory, Cambridge, MA, United States
 
Simplifying the Analysis of Data from Multiple Heliophysics Instruments and Missions
David Bazell and Jon Duane Vandegriff, Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States
 
Periodic Density Structures and the Origin of the Slow Solar Wind
Nicholeen M Viall, NASA GSFC, Greenbelt, MD, United States and Angelos Vourlidas, Naval Research Laboratory, Alexandria, VA, United States; Applied Physics Laboratory Johns Hopkins, Space Department, Laurel, MD, United States
 
Diffusive Shock Acceleration in Structured Solar Wind
Leon G Kocharov, University of Oulu, Sodankylä Geophysical Observatory (Oulu Unit), Oulu, Finland
 
A Comparison of the Characteristics of 3He-Rich Solar Energetic Particle Events Observed at Single and at Multiple Spacecraft
Mark E Wiedenbeck1,2, Glenn M Mason3, Andreas Klassen4, Christina MS Cohen1 and Nariaki Nitta5, (1)California Institute of Technology, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)JHU / APL, Laurel, MD, United States, (4)University of Kiel, Kiel, Germany, (5)Lockheed Martin Adv Tech, Lockheed Martin STAR Labs, Palo Alto, CA, United States
 
The Influence Gradient Drift in the Interplanetary Magnetic field (IMF) on the Spectra of Solar Energetic Protons (SEP) at Earth as a Function of Heliographic Latitude
Dakari Makin Franklin1, David Allen Falconer1 and James H Adams Jr2, (1)National Space Science and Technology Center, Huntsville, AL, United States, (2)Univ of Alabama Huntsville, Huntsville, AL, United States
 
Long-Duration Neutron Production in Solar Eruptive Events Detected with the MESSENGER Neutron Spectrometer
William C Feldman, Planetary Science Institute Tucson, Tucson, AZ, United States, David J Lawrence, Johns Hopkins University, Baltimore, MD, United States, W. Thomas Vestrand, Los Alamos National Laboratory, Los Alamos, NM, United States and Patrick N Peplowski, Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States
 
Predictions for Near Sun Turbulent Spectra from Synthetic Time Series
Kristopher Gregory Klein, Benjamin D G Chandran and Jean Carlos Perez, University of New Hampshire, Durham, NH, United States
 
Image-Optimized Coronal Magnetic Field Reconstructions
Shaela I Jones, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Joseph M Davila, NASA Goddard SFC, Greenbelt, MD, United States and Vadim M Uritsky, NASA Goddard Space Flight Cent, Greenbelt, MD, United States
 
Large-scale Mapping of Magnetic Fields between the Sun and Earth
Bo Li1, Iver Hugh Cairns2, Matthew Francis3, Graham Alan Steward3 and David Neudegg3, (1)University of Sydney, Sydney, NSW, Australia, (2)University of Sydney, Sydney, Australia, (3)IPS Radio and Space Services, Haymarket, Australia
 
Analyses of Simulated Reconnection-Driven Solar Polar Jets
Merrill A. Roberts1,2, Vadim M Uritsky2, Judith T Karpen2 and C Richard DeVore2, (1)Catholic University of America, Washington, DC, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Probing Alfvenic turbulence in numerical simulations in preparation for Solar Probe Plus
Jean Carlos Perez and Benjamin D G Chandran, University of New Hampshire, Durham, NH, United States
 
Measurements of plasma quasi-thermal noise on STEREO spacecraft and plasma temperature deduction using antenna electron shot noise model
Mihailo Martinović1, Arnaud Zaslavsky1, Milan Maksimovic2 and Yannis Zouganelis3, (1)Paris Observatory Meudon, Meudon, France, (2)CNRS, Paris Cedex 16, France, (3)European Space Agency, Villanueva De La Can, Spain
 
3D Location of Small Solar Wind Tracers
Cynthia Lopez-Portela1, Xochitl Blanco-Cano1, Olga Panasenco2 and Sarah E Gibson3, (1)Instituto de Geofisica, Universidad Nacional Autonoma de Mexico, Ciencias Espaciales, Mexico DF, Mexico, (2)Advanced Heliophysics, Pasadena, CA, United States, (3)National Center for Atmospheric Research, Boulder, CO, United States
 
Particle Acceleration in the Low Corona Over Broad Longitudes: Coupling MHD and 3D Particle Simulations
Matthew Gorby1, Nathan Schwadron2, Tibor Torok3, Cooper Downs3, Roberto Lionello4, Jon Linker3, Viacheslav S Titov3, Zoran Mikic3, Pete Riley3, Mihir Indrajit Desai5 and Maher A Dayeh5, (1)University of New Hampshire Main Campus, Durham, NH, United States, (2)University of New Hampshire, Durham, NH, United States, (3)Predictive Science Inc., San Diego, CA, United States, (4)Predictive Science Incorporate, San Diego, CA, United States, (5)Southwest Research Institute, San Antonio, TX, United States