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

Session ID#: 3409

Tuesday, 16 December 2014: 8:00 AM-12:20 PM
Poster Hall (Moscone_South)
Chairs:  Kelly E Korreck, Smithsonian Astrophysical Observatory, Cambridge, United States and Nathan Schwadron, University of New Hampshire, Durham, United States
Primary Convener:  Marco C M Velli, Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States
Co-conveners:  Nathan Schwadron, University of New Hampshire, Durham, United States, Kelly E Korreck, Smithsonian Astrophysical Observatory, Cambridge, United States and Yannis Zouganelis, European Space Agency, ESAC, Villanueva De La Can, Spain
OSPA Liaison:  Kelly E Korreck, Smithsonian Astrophysical Observatory, Cambridge, United States
Index Terms:

2134 Interplanetary magnetic fields [INTERPLANETARY PHYSICS]
2199 General or miscellaneous [INTERPLANETARY PHYSICS]
7599 General or miscellaneous [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7999 General or miscellaneous [SPACE WEATHER]
Virtual Option?: No

Abstracts Submitted to this Session:

 
Global Multi-Fluid Solar Corona and Inner Heliosphere Model for Solar Probe Plus and Solar Orbite (3789)
Bart van der Holst1, Igor Sokolov1, Gabor Toth1,2 and Tamas I Gombosi1,2, (1)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (2)University of Michigan, Ann Arbor, MI, United States
 
Solar Probe Plus: A NASA Mission to Touch the Sun (10537)
Nicola Justine Fox, Johns Hopkins Univ Applied Phy, Laurel, United States, Marco C M Velli, Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, Justin Christophe Kasper, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, David J McComas, Southwest Research Institute San Antonio, San Antonio, TX, United States, Russell A. Howard, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Stuart D Bale, University of California Berkeley, Space Sciences Laboratory, 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 (5319)
Timothy Simon Horbury, Imperial College London, Department of Physics, London, SW7, United Kingdom and Lorenzo Matteini, Observatoire De Paris, LESIA, Meudon, FRANCE
 
3D Visualization of Solar Data: Preparing for Solar Orbiter and Solar Probe Plus (12390)
Daniel Mueller1, Simon Felix2, Stefan Meier2, Andre Csillaghy2, Bogdan Nicula3, Freek Verstringe3, Bram Bourgoignie3, David Berghmans4 and Piers Jiggens5, (1)European Space Agency, ESAC, Villanueva De La Can, Spain, (2)University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland, (3)Royal Observatory of Belgium, Solar Influences Data Analysis Center, Brussels, Belgium, (4)Royal Observatory of Belgium, Brussels, Belgium, (5)European Space Agency, ESTEC, Noordwijk, Netherlands
 
The Energetic Particle Detector (EPD) for Solar Orbiter – Sensor Status and Calibration (4323)
Robert F Wimmer-Schweingruber1, Javier Rodriguez-Pacheco2, Glenn M Mason3, Cesar Martin-Garcia4, Manuel Prieto2, Stephan I Boettcher1, Shrinivasrao R. Kulkarni1, Lauri Panitzsch5, Sebastian Sanchez6, George C Ho7, Jan Kohler8, Raul Gomez-Herrero9, Juan Jose Blanco10 and Solar Orbiter EPD Team, (1)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (2)University of Alcalá, Space Research Group, Alcalá de Henares, Spain, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (4)IEAP, University of Kiel, Kiel, Germany, (5)now at OHB Systems, Bremen, Germany, (6)University of Alcala, Alcala de Henares, Spain, (7)southwest Research Institute, San Antonio, United States, (8)University of Kiel, Kiel, Germany, (9)University of Alcala, Space Research Group, Alcala de Henares, Spain, (10)University of Alcala, Alcala de Henarez, Spain
 
Implications of the S-Web for the Corona and Inner Heliosphere (8904)
Spiro K Antiochos, NASA GSFC, Greenbelt, United States
 
Synthetic White-light Imagery for the Wide-field Imager for Solar Probe Plus (WISPR) (18882)
Paulett Creyke Liewer1, Yubo Su1, Angelos Vourlidas2, Arnaud F Thernisien3, Russell A. 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 (25375)
Phyllis L Whittlesey1, Anthony W Case2, Justin Christophe Kasper3, Kenneth H Wright Jr1, Benjamin L Alterman4, Jonathan W Cirtain5, Jay Bookbinder6, Kelly E Korreck7 and Michael Louis Stevens2, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (4)Southwest Research Institute, Space Science and Engineering, San Antonio, United States, (5)NASA Marshall Space Flight Center, Huntsville, AL, United States, (6)Smithsonian Astrophysical Obse, Cambridge, MA, United States, (7)Smithsonian Astrophysical Observatory, Cambridge, United States
 
Numerical Techniques for Removing Instrumental Noise in the Solar Probe Plus/FIELDS Search Coil Magnetometer (18243)
Trevor Bowen1, Stuart D Bale1, Davin E Larson2, Thierry Dudok de Wit3 and Robert J. MacDowall4, (1)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (3)LPC2E, CNRS and University of Orléans, Orléans, France, (4)NASA Goddard SFC, Greenbelt, MD, United States
 
The Form of Proton Energy Spectra from Self-Consistent Simulations of the Coronal Shock Acceleration (21213)
Alexandr N. Afanasiev1, Rami O Vainio1 and Markus C Battarbee2, (1)University of Turku, Department of Physics and Astronomy, Turku, Finland, (2)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. (26392)
Michel Moncuquet1, Yannis Zouganelis2, Nicole Meyer-Vernet3, Karine Issautier4, Arnaud Zaslavsky5, Milan Maksimovic3, Gaetan LE CHAT6 and Mihailo Martinovic6, (1)Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, LESIA, Meudon, France, (2)European Space Agency, ESAC, Villanueva De La Can, Spain, (3)CNRS, Observatoire de Paris, LESIA, Meudon, France, (4)LIRA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, (5)University Pierre and Marie Curie Paris VI, LESIA - Observatoire de Paris, Paris, France, (6)Paris Observatory Meudon, LESIA, Meudon, France
 
Photoelectron and Secondary Electron Dynamics Around the Solar Probe Plus Spacecraft (18528)
Yohei Miyake, Kobe University, Graduate School of System Informatics, Kobe, Japan and Hideyuki Usui, Kobe University, Kobe, Japan
 
Automated tracing of open-field coronal structures for an optimized large-scale magnetic field reconstruction (27734)
Vadim Uritsky, Joseph M Davila and Shaela I Jones, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Instant: An Innovative L5 Small Mission Concept for Coordinated Science with Solar Orbiter and Solar Probe Plus (6850)
Benoit Lavraud1, Ying D. Liu2, Richard Anthony Harrison3, William Liu2, F Auchere4, Weiqun Gan5, Philippe L Lamy6, Lidong Xia7, Jonathan P Eastwood8, Robert F Wimmer-Schweingruber9, Qiugang Zong10, Pierre Leon Rochus11, Milan Maksimovic12, Manuela Temmer13, C Philippe Escoubet14, K Emilia J Kilpua15, Alexis P Rouillard16, Jackie A Davies17, Jean-Claude Vial18, Nat Gopalswamy19, Stuart D Bale20, Gang Li21, Timothy A Howard22 and Craig E DeForest22, (1)Laboratoire d'astrophysique de Bordeaux, Pessac, France, (2)NSSC National Space Science Center, CAS, Beijing, China, (3)United Kingdom Research and Innovation - Science & Technology Facilities Council - Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom, (4)Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, Orsay, France, (5)Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China, (6)Lab Astrophysique Marseille, Marseilles Cedex 13, France, (7)Shandong Univ. at Weihai, Weihai, China, (8)Imperial College London, Physics, London, United Kingdom, (9)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (10)Peking University, Institute of Space Physics and Applied Technology, Beijing, China, (11)Centre Spatial de Liege, Liege, Belgium, (12)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, Meudon, France, Meudon, France, (13)University of Graz, Institute of Physics, Graz, Austria, (14)ESTEC, Noordwijk, 2201, Netherlands, (15)University of Helsinki, Department of Physics, Helsinki, Finland, (16)Université Toulouse III - Paul Sabatier, Observatoire Midi–Pyrénées, CNRS, CNES, IRAP, Toulouse, France, (17)United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom, (18)IAS Institut d'Astrophysique Spatiale, Orsay Cedex, France, (19)NASA Goddard SFC, Greenbelt, United States, (20)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (21)University of Alabama in Huntsville, Department of Space Sciences and CSPAR, Huntsville, AL, United States, (22)Southwest Research Institute Boulder, Boulder, CO, United States
 
Properties of Mlso MK3 White-Light CMEs from 1989-1996 (8102)
O C St Cyr, NASA GSFC, Greenbelt, MD, United States, Quincy Allen Allen Flint, NASA Goddard Space Flight Center, Code 670, Greenbelt, MD, United States, Hong Xie, NASA/GSFC, Greenbelt, United States, David F Webb, Boston College, ISR, Chestnut Hill, MA, United States, Joan Burkepile, National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States and Alice R Lecinski, NCAR, Boulder, CO, United States
 
Fast solar wind measurements from the Bright Monitor of the Solar Wind instrument on Spektr-R (12077)
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, 180, Czech Republic, (3)Inst Space Research, Moscow, Russia, (4)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (5)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (6)MIT, Cambridge, MA, United States
 
Software Development for Jointly Analyzing Thermal-Ion Measurements from Multiple In-Situ Instruments (26471)
Bennett Maruca, University of California Berkeley, Berkeley, CA, United States, Michael Louis Stevens, Smithsonian Astrophysical Observatory, Cambridge, MA, United States, Justin Christophe Kasper, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States and Kelly E Korreck, Smithsonian Astrophysical Observatory, Cambridge, United States
 
Simplifying the Analysis of Data from Multiple Heliophysics Instruments and Missions (13326)
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 (13334)
Nicholeen M Viall, NASA GSFC, Greenbelt, United States and Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States; Applied Physics Laboratory Johns Hopkins, Space Department, Laurel, MD, United States
 
A Comparison of the Characteristics of 3He-Rich Solar Energetic Particle Events Observed at Single and at Multiple Spacecraft (7073)
Mark E Wiedenbeck1,2, Glenn M Mason3, Andreas Klassen4, Christina Cohen2 and Nariaki Nitta5, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)California Institute of Technology, Pasadena, CA, United States, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (4)University of Kiel, Kiel, Germany, (5)Lockheed Martin Advanced Technology Center, Palo Alto, 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 (12564)
Dakari Makin Franklin1, David Allen Falconer1 and James H Adams Jr2, (1)National Space Science and Technology Center, Huntsville, AL, United States, (2)Fifth Gait Technologies, Inc., Huntsville, United States
 
Long-Duration Neutron Production in Solar Eruptive Events Detected with the MESSENGER Neutron Spectrometer (13762)
William C Feldman, Planetary Science Institute, 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 (12886)
Prof. Kristopher Gregory Klein, University of New Hampshire, Durham, NH, United States, Benjamin D G Chandran, University of New Hampshire, Durham, United States and Jean Carlos Perez, Florida Institute of Technology, Aerospace, Physics and Space Sciences, Melbourne, FL, United States
 
Image-Optimized Coronal Magnetic Field Reconstructions (13262)
Shaela I Jones1, Joseph M Davila1 and Vadim Uritsky2, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)NASA GSFC / CUA, Greenbelt, United States
 
The Origin of Electron Halo in the Solar Wind Electron Velocity Distribution Function: Connection to Nanoflares in the Solar Corona (18756)
Haihong Che and Melvyn L Goldstein, University of Alabama in Huntsville, Space Science, Huntsville, United States
 
Large-scale Mapping of Magnetic Fields between the Sun and Earth (20394)
Bo Li1, Iver Hugh Cairns2, Matthew James Francis3, Graham Alan Steward3 and Dave Neudegg4, (1)University of Sydney, Sydney, NSW, Australia, (2)University of Sydney, School of Physics and ARC Training Centre for CubeSats, UAVs, and Their Applications (CUAVA), Sydney, NSW, Australia, (3)IPS Radio and Space Services, Haymarket, Australia, (4)University of Adelaide, Adelaide, Australia
 
Analyses of Simulated Reconnection-Driven Solar Polar Jets (26124)
Merrill A. Roberts1,2, Vadim Uritsky2, Judith T Karpen3 and C Richard DeVore2, (1)Catholic University of America, Washington, DC, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)NASA GSFC, Greenbelt, United States
 
Probing Alfvenic turbulence in numerical simulations in preparation for Solar Probe Plus (27968)
Jean Carlos Perez, Florida Institute of Technology, Aerospace, Physics and Space Sciences, Melbourne, FL, United States and Benjamin D G Chandran, University of New Hampshire, Durham, United States
 
Measurements of plasma quasi-thermal noise on STEREO spacecraft and plasma temperature deduction using antenna electron shot noise model (29826)
Mihailo Martinović1, Arnaud Zaslavsky1, Milan Maksimovic2 and Yannis Zouganelis3, (1)Paris Observatory Meudon, Meudon, France, (2)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, Meudon, France, Meudon, France, (3)European Space Agency, ESAC, Villanueva De La Can, Spain
 
3D Location of Small Solar Wind Tracers (29889)
Cynthia Lopez-Portela, Instituto de Geofisica, Universidad Nacional Autonoma de Mexico, Ciencias Espaciales, Mexico DF, Mexico, Xochitl Blanco-Cano, Instituto de Geofísica Universidad Nacional Autónoma de México, Mexico City, Mexico, Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States and Sarah E Gibson, National Center for Atmospheric Research, Boulder, CO, United States
 
Particle Acceleration in the Low Corona Over Broad Longitudes: Coupling MHD and 3D Particle Simulations (31333)
Matthew Gorby1, Nathan Schwadron2, Dr. Tibor Torok3, Cooper Downs4, Roberto Lionello3, Jon Linker4, Viacheslav S. Titov4, Zoran Mikic4, Pete Riley4, Mihir Indrajit Desai5 and Maher A Dayeh5, (1)University of New Hampshire Main Campus, Durham, NH, United States, (2)University of New Hampshire, Durham, United States, (3)Predictive Science Inc., San Diego, United States, (4)Predictive Science Inc., San Diego, CA, United States, (5)Southwest Research Institute, San Antonio, United States