SH23D:
Preparing for Parker Solar Probe and Solar Orbiter: A Coordinated Science from the Corona to the Inner Heliosphere Posters

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Session ID#: 22026

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 the Parker Solar Probe and Solar Orbiter. While each mission will achieve its own important science objectives, taken together they will be capable of doing simultaneous and synergized observations to best address these questions. This session focuses on opportunities and capabilities for coordinated science studies with advanced instrumentation on multiple spacecraft, assets at Earth and beyond, and sophisticated modeling of basic plasma physical processes on multiple scales that will be key to understand the dynamics of the solar atmosphere from the base of the corona into the heliosphere, the origins of the solar wind and its evolution from the sun.
Primary Convener:  Kelly E Korreck, Smithsonian Astrophysical Observatory, Cambridge, MA, United States
Conveners:  Nicola Justine Fox, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Nathan Schwadron, University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States and Yannis Zouganelis, European Space Agency, ESAC, Villanueva De La Can, Spain
Chairs:  Kelly E Korreck, Smithsonian Astrophysical Observatory, Cambridge, MA, United States, Nicola Justine Fox, Johns Hopkins University Applied Physics Laboratory, Laurel, United States and Yannis Zouganelis, European Space Agency, ESAC, Villanueva De La Can, Spain
OSPA Liaison:  Kelly E Korreck, Smithsonian Astrophysical Observatory, Cambridge, MA, United States
Index Terms:

7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7514 Energetic particles [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7845 Particle acceleration [SPACE PLASMA PHYSICS]

Abstracts Submitted to this Session:

CDPP supporting tools to Solar Orbiter and Parker Solar Probe data exploitation (214116)
Vincent N Genot1, Baptiste Cecconi2, Nicolas Dufourg3, Michel Gangloff4, Nicolas André5, Myriam Bouchemit6, Christian Jacquey1, Frederic Pitout7, Alexis P Rouillard1, Jourdane Nathanaël1, Benoit Lavraud8, Joelle Durand3, Chihiro Tao9, Eric Buchlin10 and Olivier G Witasse11, (1)IRAP, Toulouse, France, (2)Observatoire de Paris, PSL, CNRS, LIRA, Meudon, France, (3)CNES, Toulouse, France, (4)CNRS, Toulouse, France, (5)IRAP, CNRS, Toulouse, France, (6)IRAP / CNRS / UPS, PEPS, Toulouse, France, (7)IRAP, CNES/CNRS/Toulouse University, Toulouse, France., Toulouse, France, (8)Laboratoire d'astrophysique de Bordeaux, Pessac, France, (9)NICT National Institute of Information and Communications Technology, Tokyo, Japan, (10)Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, Orsay, France, (11)European Space Agency, ESTEC, Villanueva De La Can, Spain
SPADER – Science Planning Analysis and Data Estimation Resource for the NASA Parker Solar Probe Mission (279995)
Douglas J Rodgers1,2, Nicola Justine Fox3, Martha Bolz Kusterer2, F. Scott Turner2 and Alayna B Woleslagle2, (1)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, United States
A New Approach to Study Stochastic Heating in the Solar Wind with Implications for Parker Solar Probe and Solar Orbiter (218550)
Daniel Vech, University of Michigan Ann Arbor, Ann Arbor, MI, United States, Prof. Kristopher Gregory Klein, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States and Justin Christophe Kasper, Smithsonian Astrophysical Observatory, Cambridge, MA, United States
The Solar Orbiter Heliospheric Imager (SoloHI) for the Solar Orbiter Mission (232747)
Robin C Colaninno1, Russell A. Howard2, Simon P Plunkett3, Arnaud F Thernisien4, Dennis Wang3, Nathan Rich5, Clarence Korendyke1, Dennis G Socker1, Mark Linton6, Donald R McMullin7, Angelos Vourlidas8, Paulett Creyke Liewer9, Eric De Jong9, Marco C M Velli10, Zoran Mikic11, Volker Bothmer12, Lamy Philippe13 and Michael T. Carter5, (1)US Naval Research Laboratory, Washington, DC, United States, (2)Naval Research Laboratory, Washington, DC, United States, (3)Naval Research Lab, Washington, DC, United States, (4)George Mason University Fairfax, Fairfax, VA, United States, (5)US Naval Research Laboratory, Washington, United States, (6)US Naval Research Laboratory, Space Science Division, Washington, DC, United States, (7)Space Systems Research Corp, Alexandria, VA, United States, (8)Applied Physics Laboratory Johns Hopkins, Space Department, Laurel, MD, United States, (9)Jet Propulsion Laboratory, Pasadena, CA, United States, (10)University of California Los Angeles, Los Angeles, CA, United States, (11)Predictive Science Inc., San Diego, CA, United States, (12)University of Göttingen, Göttingen, Germany, (13)Laboratoire d'Astrophysique de Marseille, Marseille, France
Investigations of Wind/WAVES Dust Impacts (232992)
O C St Cyr, NASA GSFC, Greenbelt, MD, United States, Lynn B Wilson III, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Keighley Rockcliffe, Rensselaer Polytechnic Institute, Troy, NY, United States, Alyssa Christine Mills, University of Maryland College Park, College Park, MD, United States, Teresa Nieves-Chinchilla, Catholic University of America, Washington, United States, Mark L Adrian, Auburn University, Physics Department, Auburn, AL, United States and David Malaspina, Univ Colorado, Boulder, CO, United States
Numerical Preparations Toward Identifying Heating Mechanisms using Distributions Function Measurements from SWEAP and Parker Solar Probe. (244730)
Prof. Kristopher Gregory Klein, University of Michigan Ann Arbor, Ann Arbor, MI, United States, Justin Christophe Kasper, University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, Gregory G Howes, Department of Physics and Astronomy, University of Iowa, Department of Physics and Astronomy, Iowa City, United States, Davin E Larson, Space Sciences Laboratory, Berkeley, United States, Francesco Valentini, University della Calabria, Rende, Italy, Phyllis L Whittlesey, Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, Roberto Livi, University of California Berkeley, Berkeley, CA, United States and Anthony W Case, Smithsonian Astrophysical Observatory, Cambridge, MA, United States
The variable nature of the solar wind (247936)
Hsiu-Shan Yu1, Bernard V Jackson2, Andrew Buffington2 and P. Paul Hick2, (1)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (2)University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States
The Energy Spectrum of the Solar Wind Core (249878)
Andrew P Walsh1, Sergio Toledo Redondo2, Pedro Osuna3, Yannis Zouganelis1, Arnaud Masson4, Anik De Groof3, Denise Perrone5, Owen Wyn Roberts6 and Matt Taylor1, (1)European Space Agency, Villanueva De La Can, Spain, (2)European Space Astronomy Centre, Madrid, Spain, (3)European Space Agency, ESAC, Madrid, Spain, (4)ESA, Villanueva De La Canada, Spain, (5)European Space Agency, ESAC, Villanueva De La Cañada, Spain, (6)Austrian Academy of Sciences, Vienna, Austria
3D Visualization of Solar Data: Preparing for Solar Orbiter and Parker Solar Probe (253321)
Daniel Mueller1, Bogdan Nicula2, Simon Felix3, Freek Verstringe2, Bram Bourgoignie2, Andre Csillaghy4, David Berghmans5, Piers Jiggens6, Jack Ireland7 and Bernhard Fleck8, (1)European Space Agency, ESTEC, Villanueva De La Can, Spain, (2)Royal Observatory of Belgium, Solar Influences Data Analysis Center, Brussels, Belgium, (3)FHNW, Institute of 4D Technologies, Windisch, Switzerland, (4)University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland, (5)Royal Observatory of Belgium, Brussels, Belgium, (6)European Space Agency, ESTEC, Noordwijk, Netherlands, (7)ADNET Systems Inc. Greenbelt, Greenbelt, MD, United States, (8)European Space Agency, Villanueva De La Can, Spain
Calibration Results and Anticipated Science Ops for the Parker Solar Probe's SWEAP/SPAN-Electron Analyzers (256967)
Phyllis L Whittlesey1, Davin E Larson2, Roberto Livi3, Robert Abiad4, Christopher Parker5, Jasper S Halekas6, Justin Christophe Kasper7 and Kelly E Korreck7, (1)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (2)Space Sciences Laboratory, Berkeley, United States, (3)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (4)University of California, Berkeley / SSL, Berkeley, CA, United States, (5)Magic Leap, Sunnyvale, CA, United States, (6)University of California Berkeley, Berkeley, CA, United States, (7)Smithsonian Astrophysical Observatory, Cambridge, MA, United States
ASHI: An All Sky Heliospheric Imager for Viewing Thomson-Scattered Light (259193)
Andrew Buffington1, Bernard V Jackson2, Hsiu-Shan Yu3, P. Paul Hick2 and Mario Mark Bisi4, (1)University of California, San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (2)University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (3)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (4)United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom
Remote Sensing of the Solar Wind Density, Speed, and Temperature in the Region between the Sun and Parker Solar Probe (274815)
Joseph M Davila, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Nelson Leslie Reginald, The Catholic University of America, Washington, United States
The Wide-Field Imager for the Parker Solar Probe Mission (WISPR) (276573)
Simon P Plunkett1, Russell A. Howard1, Damien H Chua1, Nicholas A Crump2, Hillary Dennison1, Clarence Korendyke1, Mark Linton3, Nathan Rich4, Dennis G Socker1, Arnaud Thernisien5, Dennis Wang6, Angelos Vourlidas7, Rebecca Baugh8, J Peter Van Duyne8, Paulett Creyke Liewer9, Eric De Jong9, Mark T Boies10, Zoran Mikic11, Volker Bothmer12, Pierre Leon Rochus13 and Jean-Philippe Halain13, (1)US Naval Research Laboratory, Washington, DC, United States, (2)Naval Research Laboratory, Space Science Division, Washington, DC, United States, (3)US Naval Research Laboratory, Space Science Division, Washington, DC, United States, (4)US Naval Research Laboratory, Washington, United States, (5)Naval Research Laboratory, Washington, United States, (6)Space System Research Corporation, Alexandria, United States, (7)Applied Physics Laboratory Johns Hopkins, Space Department, Laurel, MD, United States, (8)Space Systems Research Corporation, Alexandria, VA, United States, (9)Jet Propulsion Laboratory, Pasadena, CA, United States, (10)Research Support Instruments, Lanham, MD, United States, (11)Predictive Science Inc., San Diego, CA, United States, (12)University of Göttingen, Göttingen, Germany, (13)Centre Spatial de Liege, Liege, Belgium
Solar Probe ANalyzer for Ions – Laboratory Performance (214902)
Roberto Livi1, Davin E Larson2, Justin Christophe Kasper3, Kelly E Korreck3 and Phyllis L Whittlesey4, (1)University of California Berkeley, Berkeley, CA, United States, (2)Space Sciences Laboratory, Berkeley, United States, (3)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (4)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States
Solar Probe Cup: Laboratory Performance (280943)
Anthony W Case1, Justin Christophe Kasper1, Kelly E Korreck1, Michael Louis Stevens1, Davin E Larson2, Kenneth H Wright Jr3, Dennis Lee Gallagher4 and Phyllis L Whittlesey5, (1)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (2)Space Sciences Laboratory, Berkeley, United States, (3)Universities Space Research Association, Huntsville, AL, United States, (4)NASA Marshall Space Flight Center, Huntsville, AL, United States, (5)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States
Correcting PSP electron measurements for the effects of spacecraft electrostatic and magnetic fields (284215)
Daniel McGinnis, University of Iowa, Iowa City, United States, Jasper S Halekas, University of California Berkeley, Berkeley, CA, United States, Davin E Larson, Space Sciences Laboratory, Berkeley, United States, Phyllis L Whittlesey, Space Sciences Laboratory, University of California Berkeley, Berkeley, United States and Justin Christophe Kasper, Smithsonian Astrophysical Observatory, Cambridge, MA, United States
Preliminary calibration results from a simple Wave/Particle correlator instrument that combines data from SPP/SWEAP and FIELDS (285463)
Davin E Larson1, Stuart D Bale2, Keith Goetz3, Roberto Livi2, Phyllis L Whittlesey4, Justin Christophe Kasper5, Prof. Kristopher Gregory Klein6 and Gregory G Howes7, (1)Space Sciences Laboratory, Berkeley, United States, (2)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States, (4)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (5)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (6)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (7)Department of Physics and Astronomy, University of Iowa, Department of Physics and Astronomy, Iowa City, United States
Data-driven Model of the ICME Propagation through the Solar Corona and Inner Heliosphere (287103)
Mehmet Sarp Yalim, University of Alabama in Huntsville, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States, Nikolai Pogorelov, The University of Alabama in Huntsville, Space Science, Huntsville, United States, Talwinder Singh, Georgia State University, Department of Physics and Astronomy, Atlanta, United States and Yang Liu, W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, United States
A Time-dependent Heliospheric Model Driven by Empirical Boundary Conditions (287336)
Tae K. Kim, The University of Alabama in Huntsville, The Center for Space Plasma and Aeronomic Research, Huntsville, United States, Charles Nickolos Arge, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Nikolai V Pogorelov, University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States
10 Years of Student Questions about the Sun and Solar Physics: Preparing Graduate Students to Work with Parker Solar Probe Data (288452)
Nicholas A Gross, Boston University, Astronomy, Boston, MA, United States, W Jeffrey Hughes, Boston University, Boston, MA, United States and Michael James Wiltberger, National Center for Atmospheric Research, Boulder, United States
Radio Remote Sensing of Coronal Mass Ejections: Implications for Parker Solar Probe and Solar Orbiter (292286)
Jason Earl Kooi, US Naval Research Laboratory, Washington, United States, Najma C Thomas, Spelman College, Department of Physics, Atlanta, GA, United States, Michael B Guy III, Morgan State University, Department of Physics and Engineering Physics, Baltimore, MD, United States and Steven R. Spangler, University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States
Analysis of Solar Coronal Holes with Synoptic Magnetogram Data (295497)
Alexander Canner, Indiana University Purdue University Indianapolis, Indianapolis, IN, United States, Tae Kwang Kim, University of Alabama in Huntsville, CSPAR, Huntsville, United States, Nikolai Pogorelov, The University of Alabama in Huntsville, Space Science, Huntsville, United States and Mehmet Sarp Yalim, University of Alabama in Huntsville, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States
The Solar Wind from Pseudostreamers and their Environs: Opportunities for Observations with Parker Solar Probe and Solar Orbiter (296743)
Olga Panasenco1, Marco C M Velli2, Aram Panasenco2 and Roberto Lionello3, (1)Advanced Heliophysics Inc., Pasadena, CA, United States, (2)University of California Los Angeles, Los Angeles, CA, United States, (3)Predictive Science Inc., San Diego, CA, United States

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