SH31C:
Preparing for Solar Probe Plus and Solar Orbiter: A Coordinated Science from the Corona to the Inner Heliosphere II Posters


Session ID#: 8726

Session Description:
Understanding coronal heating and solar wind acceleration, unveiling the mechanisms of coronal mass ejections and energetic particle acceleration, linking the magnetic field evolution from the solar interior to its consequences in terms of solar variability and space weather are at the core of heliophysics exploration in the next decade with Solar Probe Plus and Solar Orbiter.  Coordinating science with advanced instrumentation on multiple spacecraft, assets at Earth and beyond, as well as sophisticated modeling of basic plasma physical processes on multiple scales will be key to understand the origins of the solar wind and heliosphere and its evolution from the sun. This session encourages contributions covering observations, data analysis and theoretical developments that combine data from different sources and advanced modeling to understand the dynamics of the solar atmosphere from the base of the corona into the inner heliosphere.
Primary Convener:  Kelly E Korreck, Smithsonian Astrophysical Observatory, Cambridge, United States
Conveners:  Yannis Zouganelis, European Space Agency, ESAC, Villanueva De La Can, Spain, Nicola Justine Fox, Johns Hopkins Univ Applied Phy, Laurel, United States and Nathan Schwadron, University of New Hampshire, Durham, United States
Chairs:  Nathan Schwadron, University of New Hampshire, Durham, United States and Nicola Justine Fox, Johns Hopkins University Applied Physics Laboratory, Laurel, United States
OSPA Liaison:  Kelly E Korreck, Smithsonian Astrophysical Observatory, Cambridge, MA, United States
Index Terms:

7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7534 Radio emissions [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7829 Kinetic waves and instabilities [SPACE PLASMA PHYSICS]
7845 Particle acceleration [SPACE PLASMA PHYSICS]

Abstracts Submitted to this Session:

Estimating Coronagraph Visibility Functions – Progress Report (63354)
O C St Cyr1, Hong Xie2, Daniel Duncan2, David F Webb3, Russell A. Howard4 and Joseph B Gurman5, (1)NASA GSFC, Greenbelt, MD, United States, (2)Catholic University of America, Washington, DC, United States, (3)Boston College, ISR, Chestnut Hill, MA, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States
Synthetic White-light Imagery for the Wide-field Imager for Solar Probe Plus (WISPR) (66525)
Paulett Creyke Liewer1, Arnaud F Thernisien2, Angelos Vourlidas3, Russell A. Howard4, Craig DeForest5, Eric DeJong1 and Anant Desai1, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Naval Research Lab, Washington, DC, United States, (3)Applied Physics Laboratory Johns Hopkins, Space Department, Laurel, MD, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)Southwest Research Institute Boulder, Boulder, United States
Distinguishing 3He and 4He with the Electron Proton Telescope (EPT) on Solar Orbiter (64447)
Sebastian Boden1, Shrinivasrao R. Kulkarni1, Jan Steinhagen2, Jan Tammen3, Cesar Martin-Garcia3, Robert F Wimmer-Schweingruber1, Stephan I Boettcher1, Lars Seimetz1, Ali Ravanbakhsh4, Robert Elftmann1, Björn Schuster2, Alexander Kulemzin2, Stefan Kolbe1, Mahesh Yedla1, Violetta Knieriem1, Jia Yu2, Jan Kohler2, Lauri Panitzsch5, Christoph Terasa1, Eckart Boehm2, Javier Rodriguez-Pacheco6, Manuel Prieto6 and Raul Gomez-Herrero7, (1)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (2)University of Kiel, Kiel, Germany, (3)IEAP, University of Kiel, Kiel, Germany, (4)IEAP, University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (5)now at OHB Systems, Bremen, Germany, (6)University of Alcalá, Space Research Group, Alcalá de Henares, Spain, (7)University of Alcala, Space Research Group, Alcala de Henares, Spain
Multi-scale Analysis of DSCOVR Data Using Wavelet Cross Correlation (63704)
Alexander Michael Hegedus1, Justin Christophe Kasper2, Michael Louis Stevens3, Benjamin L. Alterman4, Anthony W Case3, Adam Szabo5 and Andriy Koval6, (1)Lunasonde Inc., Science, Tucson, United States, (2)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (3)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (4)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (6)NASA Goddard Space Flight Center, Greenbelt, United States
Science Planning for the Solar Probe Plus NASA Mission (70292)
Martha Bolz Kusterer1, Nicola Justine Fox2, F. Scott Turner3 and Jon Duane Vandegriff1, (1)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Performance Measurements of the Flight Detector for SPICE on SolarOrbiter (74520)
William T Thompson, ADNET Systems Inc. Greenbelt, Greenbelt, MD, United States, Joseph M Davila, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Martin Caldwell, RAL Space, STFC Rutherford Appleton Laboratory, Didcot, United Kingdom and Oswald Siegmund, Sensor Sciences, LLC, Pleasant Hill, CA, United States
Developing Techniques for Spacecraft Noise Removal in Preparation for Solar Probe Plus (84973)
Trevor Bowen and Stuart D Bale, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
Quasi-thermal noise observed by CASSINI during the first flyby of Venus (66036)
Mihailo Martinović1, Arnaud Zaslavsky1, Milan Maksimovic2, Stevo Šegan3 and Marek Svetlik4, (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)Faculty of Mathematics, University of Belgrade, Department of Astronomy, Belgrade, Serbia, (4)Faculty of Mathematics, University of Belgrade, Belgrade, Serbia
The very slow solar wind in the Inner Heliosphere (69336)
Eduardo Sanchez-Diaz1, Kevin Segura1, Alexis P Rouillard1, Benoit Lavraud2, Chihiro Tao3 and Pierre-Louis Blelly4, (1)IRAP, Toulouse, France, (2)Laboratoire d'astrophysique de Bordeaux, Pessac, France, (3)NICT National Institute of Information and Communications Technology, Tokyo, Japan, (4)Université Toulouse III - Paul Sabatier, Observatoire Midi–Pyrénées, CNRS, CNES, IRAP, Toulouse, France
Compressive Acceleration of Solar Energetic Particles within Coronal Mass Ejections: Observations and Theory Relevant to the Solar Probe Plus and Solar Orbiter Missions (74765)
Edmond C Roelof, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Diagnosing the Properties of the Solar Wind using Magnetic Topology (76336)
Zoran Mikic1, Viacheslav S. Titov1, Roberto Lionello1, Cooper Downs1, Jon Linker1, Dr. Tibor Torok2 and Pete Riley1, (1)Predictive Science Inc., San Diego, CA, United States, (2)Predictive Science Inc., San Diego, United States
Thermal Plasma Measurements with the Solar Probe Cup: An Estimate of Perihelion Data (81389)
Phyllis L Whittlesey1, Jonathan W Cirtain2, Gary Paul Zank3, Justin Christophe Kasper4, Kenneth H Wright Jr1, Laxman Adhikari5, Daikou Shiota6 and Anthony W Case7, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)NASA Marshall Space Flight Center, Huntsville, AL, United States, (3)University of Alabama in Huntsville, Space Science, Huntsville, AL, United States, (4)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (5)Center for Space Plasma and Aeronomic Research, Department of Space Science, The university of Alabama in Huntsville, Huntsville, United States, (6)National Institute of Information and Communications Technology, Tokyo, Japan, (7)Smithsonian Astrophysical Observatory, Cambridge, MA, United States
Alfvenic Turbulence from the Sun to 65 Solar Radii: Numerical predictions. (82106)
Jean Carlos Perez, University of New Hampshire Main Campus, Durham, NH, United States and Benjamin D G Chandran, University of New Hampshire Main Campus, Department of Physics and Astronomy, Durham, NH, United States
Reconnection-Driven Solar Polar Jets to be Encountered by Solar Probe Plus: Simulated In Situ Measurements and Data Analysis (82130)
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
Bulk Velocity and Thermal Properties of the Solar Wind in the Inner Heliosphere (72942)
Micah J Weberg1, Jim M Raines2, Daniel J Gershman3, Susan T Lepri4 and Thomas Zurbuchen1, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (3)University of Michigan Ann Arbor, Department of Atmospheric, Oceanic and Space Sciences, Ann Arbor, MI, United States, (4)University of Michigan, Ann Arbor, United States
Using In Situ and Remote Sensing Data to Model the Plasma Flow throughout the Heliosphere (85695)
Tae K. Kim1, Nikolai V Pogorelov2, Charles Nickolos Arge3, Bernard V Jackson4, Igor Kryukov1, Periasamy K Manoharan5, Preethi Manoharan6, Derek Tropf7, Hsiu-Shan Yu8 and Gary Paul Zank9, (1)University of Alabama in Huntsville, CSPAR, Huntsville, AL, United States, (2)University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States, (3)Air Force Research Laboratory Kirtland AFB, Kirtland AFB, NM, United States, (4)University of California, San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (5)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, (6)University of Alabama in Huntsville, Huntsville, AL, United States, (7)NASA Jet Propulsion Laboratory, Washington, DC, United States, (8)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (9)University of Alabama in Huntsville, Space Science, Huntsville, AL, United States
Characterisation of small-scale heating events in the solar atmosphere from 3D MHD simulations and their potential role in coronal heating (86170)
Margit Haberreiter1, Nuno Guerreiro1, Viggo Haraldson Hansteen2 and Werner K Schmutz1, (1)PMOD WRC Physical Meteorological Observatory Davos and World Radiation Center, Davos Dorf, Switzerland, (2)Institute for Theoretical Astrophysics, University of Oslo, Oslo, Norway
Improving Heliospheric Field Models with Optimized Coronal Models (86150)
Shaela I Jones, Joseph M Davila and Vadim Uritsky, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Constraining Large-Scale Solar Magnetic Field Models with Optical Coronal Observations (86238)
Vadim Uritsky, Joseph M Davila and Shaela I Jones, NASA Goddard Space Flight Center, Greenbelt, MD, United States

See more of: SPA-Solar and Heliospheric Physics