SH049
Parker Solar Probe: One Step Closer to the Sun III Posters

Wednesday, 16 December 2020: 04:00-20:59
Poster
Primary Convener:  Robert B Decker, Johns Hopkins Applied Physics Laboratory, Laurel, United States
Conveners:  Adam Szabo1, Tatiana Niembro Hernandez2 and Kristoff W Paulson2, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States(2)Smithsonian Astrophysical Observatory, Cambridge, MA, United States
Primary Liaison:  Robert B Decker, The Johns Hopkins University. Applied Physics Laboratory, Laurel, MD, United States
Chairs:  Tatiana Niembro Hernandez, UNAM National Autonomous University of Mexico, Fac. de Ciencias, Mexico City, Mexico and Kristoff W Paulson, University of New Hampshire, Chelmsford, MA, United States
OSPA Liaison:  Kristoff W Paulson, University of New Hampshire, Chelmsford, MA, United States
 
Prediction of the In Situ Coronal Mass Ejection Rate for Solar Cycle 25: Implications for Parker Solar Probe In Situ Observations (674073)
Christian Moestl1,2, Andreas Weiss2,3, Martin Reiss4, Rachel Bailey4, Ute Amerstorfer4, Tanja Amerstorfer4, Jürgen Hinterreiter4,5, Maike Bauer4,5, Scott William McIntosh6, Noé Lugaz7 and David Stansby8, (1)Austrian Academy of Sciences, Vienna, Austria, (2)Graz University of Technology, Institute of Geodesy, Graz, Austria, (3)Austrian Academy of Sciences, Space Research Institute, Vienna, Austria, (4)Austrian Academy of Sciences, Space Research Institute, Graz, Austria, (5)University of Graz, Institute of Physics, Graz, Austria, (6)High Altitude Observatory, Boulder, CO, United States, (7)University of New Hampshire, Durham, United States, (8)Imperial College London, London, SW7, United Kingdom
 
On the location of the Solar Alfvén Point and the imminent crossing by Parker Solar Probe (769722)
Michael Louis Stevens1, Anthony W Case1, Kelly E Korreck1, Tatiana Niembro Hernandez1, Kristoff W Paulson2, Justin Christophe Kasper3, Davin Larson4, Roberto Livi4, Phyllis L Whittlesey4, Keith Goetz5, Peter Harvey4, Robert J MacDowall6, Kristopher G. Klein7, Stuart Bale8, Marc Pulupa4, David Malaspina9, John W Bonnell10, Thierry Dudok de Wit11, Michel Moncuquet12, Robert Colby Allen13 and Samuel Timothy Badman14, (1)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (4)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (5)University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States, (6)NASA/Goddard Space Flight Center, Greenbelt, United States, (7)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (8)University of California, Berkeley, Berkeley, CA, United States, (9)University of Colorado, Astrophysical and Planetary Sciences Department, Boulder, CO, United States, (10)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (11)LPC2E, CNRS and University of Orléans, Orléans, France, (12)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, (13)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (14)University of Oxford, Oxford, United Kingdom
 
The Shape and Motions of the Heliospheric Current Sheet Close to the Sun (685492)
Adam Szabo1, Shaela I Jones1, Justin Christophe Kasper2, Charles Nickolos Arge1, Stuart D Bale3, Michael Louis Stevens4, Anthony W Case4, Davin E Larson5, Phyllis L Whittlesey6, Marc Pulupa6, Robert J MacDowall7 and Andriy Koval1, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (3)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (4)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (5)Space Sciences Laboratory, Berkeley, CA, United States, (6)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (7)NASA/Goddard Space Flight Center, Greenbelt, United States
 
Corotating Interaction Regions observed between Solar Orbiter and Parker Solar Probe (729428)
Robert Colby Allen1, George C Ho1, Glenn M Mason1, Javier Rodriguez-Pacheco2, Robert F Wimmer-Schweingruber3, David J McComas4, Eric R Christian5, Nathan Schwadron6, Matthew E Hill1, Mark E Wiedenbeck7, Ralph L McNutt Jr8, Nour E. Raouafi9 and David Lario10, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)University of Alcalá, Space Research Group, Alcalá de Henares, Spain, (3)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (4)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (5)NASA GSFC, Greenbelt, MD, United States, (6)University of New Hampshire, Durham, NH, United States, (7)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (8)Johns Hopkins Univ/APL, Laurel, MD, United States, (9)Johns Hopkins University, Baltimore, MD, United States, (10)The Johns Hopkins University, Laurel, MD, United States
 
Analysis of Solar Wind Ejecta Observed by the Wide-field Imager (WISPR) on Parker Solar Probe (767752)
Paulett Creyke Liewer, NASA Jet Propulsion Laboratory, Pasadena, CA, United States, Jiong Qiu, Montana State University, Physics Department, Bozeman, MT, United States, Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Jeffrey R Hall, Jet Propulsion Laboratory, Pasadena, CA, United States, Paulo Penteado, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States and Russell A. Howard, U.S. Naval Research Laboratory, Washington, DC, United States
 
Small-scale Magnetic Flux Ropes in the First Two Parker Solar Probe Encounters (752797)
Yu Chen1, Qiang Hu1,2, Lingling Zhao2, Justin Christophe Kasper3, Stuart D Bale4, Kelly E Korreck5, Anthony W Case5, Michael Louis Stevens5, John W Bonnell4, Keith Goetz6, Peter Harvey4, Kristopher G. Klein7, Davin Larson4, Roberto Livi4, Robert J MacDowall8, David Malaspina9, Marc Pulupa4 and Phyllis L Whittlesey4, (1)University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States, (2)Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (4)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (5)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (6)University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States, (7)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (8)NASA/Goddard Space Flight Center, Greenbelt, United States, (9)University of Colorado, Astrophysical and Planetary Sciences Department, Boulder, CO, United States
 
Investigation of a prominent solar wind structure observed by PSP on June 13, 2020 (758680)
Tatiana Niembro Hernandez1, Michael Louis Stevens1, Kelly E Korreck1, Kristoff W Paulson2, Teresa Nieves-Chinchilla3, Adam Szabo3, Laura Antonia Balmaceda4, Angelos Vourlidas5, Timothy Simon Horbury6, Janet G Luhmann7, Anthony W Case1, Justin Christophe Kasper8, Davin E Larson9, Roberto Livi10, Ali Rahmati7, Jia Huang8, Phyllis L Whittlesey10, Stuart D Bale7, Marc Pulupa10, David Malaspina11, John W Bonnell12, Peter Harvey13, Keith Goetz14, Thierry Dudok de Wit15, Robert J MacDowall16 and Andriy Koval3, (1)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (4)NASA Goddard Space Flight Center, Greenbelt, United States, (5)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (6)Imperial College London, Department of Physics, London, SW7, United Kingdom, (7)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (8)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (9)Space Sciences Laboratory, Berkeley, CA, United States, (10)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (11)University of Colorado, Astrophysical and Planetary Sciences Department, Boulder, CO, United States, (12)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (13)Space Sciences Laboratory, Berkeley, United States, (14)University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States, (15)LPC2E, CNRS and University of Orléans, Orléans, France, (16)NASA/Goddard Space Flight Center, Greenbelt, United States
 
Searching for Weak Stream Interactions in the Inner Heliosphere Using the Parker Solar Probe (774547)
Christopher Mark Bert1, Justin Christophe Kasper1, Anthony W Case2, Kelly E Korreck2, Davin E Larson3, Roberto Livi4, Michael Louis Stevens2, Phyllis L Whittlesey4, Stuart D Bale5, Marc Pulupa4, Robert J MacDowall6, Robert Colby Allen7 and Jia Huang1, (1)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (2)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (3)Space Sciences Laboratory, Berkeley, CA, United States, (4)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (5)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (6)NASA/Goddard Space Flight Center, Greenbelt, United States, (7)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
 
The Dust Environment in the Inner Heliosphere (668201)
Russell A. Howard1, Guillermo Stenborg2, Phillip Hess1, Brendan Gallagher2 and Arnaud Thernisien1, (1)US Naval Research Laboratory, Washington, DC, United States, (2)US Naval Research Laboratory, Space Science Division, Washington, DC, United States
 
Global MHD Modeling of the Solar Corona and Solar Wind with Turbulent Transport and Heating: Comparisons with Parker Solar Probe Observations (687831)
Arcadi V. Usmanov1,2, Rohit Chhiber1,2, William H Matthaeus1, Melvyn L Goldstein3 and Riddhi Bandyopadhyay4, (1)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (2)NASA Goddard Space Flight Center, Greenbelt, DE, United States, (3)University of Maryland Baltimore County, Baltimore, MD, United States, (4)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States
 
Observed Turbulent Properties of Spherically Polarized Alfvénic States (761491)
Trevor Bowen1, Samuel Timothy Badman1, Stuart D Bale2, Benjamin D G Chandran3, Christopher H K Chen4, Thierry Dudok de Wit5, Timothy Simon Horbury6, Justin Christophe Kasper7, Kristopher G. Klein8, Davin Larson9, Alfred Mallet10, Lorenzo Matteini11, Michael McManus2, Anna Tenerani12, Marco C M Velli13 and J. L. Verniero2, (1)University of California Berkeley, Berkeley, CA, United States, (2)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)University of New Hampshire, Durham, NH, United States, (4)Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom, (5)LPC2E, CNRS and University of Orléans, Orléans, France, (6)Imperial College London, Department of Physics, London, SW7, United Kingdom, (7)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (8)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (9)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (10)University of California Berkeley, Walnut CREEK, CA, United States, (11)Imperial College London, Department of Physics, London, United Kingdom, (12)University of Texas, Austin, TX, United States, (13)University of California Los Angeles, Los Angeles, CA, United States
 
Parker Solar Probe Observations of Ion Velocity-Space Diffusion Associated with Ion-Scale Right-Hand Polarized Waves (762069)
J. L. Verniero1, Benjamin D G Chandran2, Davin E Larson3, Ali Rahmati1, Michael McManus1, Roberto Livi4, Phyllis L Whittlesey4, Kristopher G. Klein5, Justin Christophe Kasper6, Ben Alterman7, Trevor A Bowen8, John W Bonnell9 and SWEAP/FIELDS Team, (1)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)University of New Hampshire, Durham, NH, United States, (3)Space Sciences Laboratory, Berkeley, CA, United States, (4)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (5)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (6)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (7)Southwest Research Institute, San Antonio, United States, (8)University of California Berkeley, Berkeley, CA, United States, (9)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
 
Parker Solar Probe Proton Beams and Waves: Observations and Modeling (697031)
Leon Ofman1,2, Lan Jian2 and Scott A Boardsen3,4, (1)Catholic University of America, Washington, DC, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)University of Maryland Baltimore County, Goddard Planetary Heliophysics Institute, Baltimore, MD, United States, (4)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States
 
Examining Ion-Scale Wave Properties in the Inner Heliosphere Observed by Parker Solar Probe (703787)
Stephanie Colon1,2, Kristoff W Paulson3, Tatiana Niembro Hernandez4, Mary Eby5, Anthony W Case3, Michael Louis Stevens3, Kelly E Korreck3, Justin Christophe Kasper6 and Stuart D Bale7, (1)University of Puerto Rico Rio Piedras Campus, San Juan, PR, United States, (2)Center for Astrophysics | Harvard-Smithsonian, Cambridge, United States, (3)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (4)UNAM National Autonomous University of Mexico, Fac. de Ciencias, Mexico City, Mexico, (5)Texas Lutheran University, Seguin, TX, United States, (6)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (7)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
 
Ion-Scale Waves With Rising Frequency Tones Observed by Parker Solar Probe (763969)
Kristoff W Paulson1, Tatiana Niembro Hernandez2, Michael Louis Stevens1, Anthony W Case1, J. L. Verniero3, Trevor A Bowen4, Kelly E Korreck1, Roberto Livi5, Davin E Larson6, Justin Christophe Kasper7 and Stuart D Bale3, (1)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (3)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (4)University of California Berkeley, Berkeley, CA, United States, (5)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (6)Space Sciences Laboratory, Berkeley, CA, United States, (7)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
 
Whistler wave properties during PSP’s encounter 1 - First results from SCM cross-spectral data (721860)
Clara Froment1, Vladimir Krasnoselskikh2, Oleksiy V Agapitov3, Thierry Dudok de Wit4, David Malaspina5, Vamsee Krishna Jagarlamudi4, Matthieu Kretzschmar6, Andrea Larosa2, Stuart D Bale7, John W Bonnell8, Anthony W Case9, Keith Goetz10, Justin Christophe Kasper11, Kelly E Korreck9, Davin E Larson12, Roberto Livi13, Robert J. MacDowall14, Michel Moncuquet15, Forrest Mozer16, Marc Pulupa13, Claire Revillet6, Michael Louis Stevens9 and Phyllis L Whittlesey13, (1)LPC2E, CNRS/University of Orléans/CNES, Orléans, France, (2)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Orléans Cedex 2, France, (3)Space Science Laboratory, UCB, Berkeley, CA, United States, (4)LPC2E, CNRS and University of Orléans, Orléans, France, (5)University of Colorado, Astrophysical and Planetary Sciences Department, Boulder, CO, United States, (6)CNRS and University of Orléans, LPC2E, Orléans, France, (7)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (8)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (9)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (10)University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States, (11)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (12)Space Sciences Laboratory, Berkeley, CA, United States, (13)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (14)NASA Goddard SFC, Greenbelt, MD, United States, (15)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, (16)University of California, Berkeley, Berkeley, CA, United States
 
Whistler Waves in the Inner Heliosphere (682279)
Brent Page1, Stuart Bale2, Trevor A Bowen3, Thierry Dudok de Wit4, Katherine Goodrich1, David Malaspina5 and Marc Pulupa6, (1)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)University of California, Berkeley, Berkeley, CA, United States, (3)University of California Berkeley, Berkeley, CA, United States, (4)LPC2E, CNRS and University of Orléans, Orléans, France, (5)University of Colorado, Astrophysical and Planetary Sciences Department, Boulder, CO, United States, (6)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States
 
Magnetic switchbacks: on the sensitivity of the statistical results with the chosen methodology (690726)
Naïs Fargette1, Benoit Lavraud2, Alexis P Rouillard2, Nicolas Poirier1, Marit Oieroset3, Tai Phan4, Rui Pinto2, Athanasios Kouloumvakos1, Jonathan P Eastwood5, Jasper S Halekas6, Justin Christophe Kasper7, Jia Huang7, Stuart Bale8, Matthieu Berthomier9, Anthony W Case10, Kelly E Korreck10, Davin E Larson11, Philippe Louarn12, David Malaspina13, Marc Pulupa14, Michael Louis Stevens10, Phyllis L Whittlesey14 and Keith Goetz15, (1)IRAP, Toulouse, France, (2)IRAP/CNRS, Toulouse, France, (3)Univ California, Berkeley, CA, United States, (4)University of California Berkeley, Berkeley, United States, (5)Imperial College London, Physics, London, SW7, United Kingdom, (6)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (7)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (8)University of California, Berkeley, Berkeley, CA, United States, (9)LPP, Ecole Polytechnique, UPMC, Paris, France, (10)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (11)Space Sciences Laboratory, Berkeley, CA, United States, (12)IRAP, CNRS, Toulouse, France, (13)University of Colorado, Astrophysical and Planetary Sciences Department, Boulder, CO, United States, (14)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (15)University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States
 
Magnetic Field Dropouts at near-Sun Switchback Boundaries: A Superposed Epoch Analysis (691909)
William M Farrell, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Robert J MacDowall, NASA/Goddard Space Flight Center, Greenbelt, United States, Jacob Gruesbeck, University of Maryland College Park, College Park, MD, United States, Stuart Bale, University of California, Berkeley, Berkeley, CA, United States and Justin Christophe Kasper, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
 
The Structure and Origin of Switchbacks: Parker Solar Probe Observations (700450)
Jia Huang1, Justin Christophe Kasper2, Lennard A Fisk3, Michael McManus4, J. L. Verniero4, Davin E Larson5, Roberto Livi6, Bennett Maruca7, Ramiz A Qudsi8, Mihailo Martinović9, Kristopher G. Klein9, Daniel Vech10, Mojtaba Akhavan-Tafti11, Michael Louis Stevens12, Anthony W Case12, Kelly E Korreck12, Stuart D Bale4, Phyllis L Whittlesey6, Marc Pulupa6, Thierry Dudok de Wit13, David Malaspina14, Benoit Lavraud15 and Naïs Fargette16, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (3)Univ Michigan, Ann Arbor, MI, United States, (4)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (5)Space Sciences Laboratory, Berkeley, CA, United States, (6)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (7)Center for Astrophysics, Berkeley, CA, United States, (8)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (9)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (10)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (11)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (12)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (13)LPC2E, CNRS and University of Orléans, Orléans, France, (14)University of Colorado, Astrophysical and Planetary Sciences Department, Boulder, CO, United States, (15)IRAP/CNRS, Toulouse, France, (16)IRAP, Toulouse, France
 
Behavior of energetic particles in magnetic switchbacks observed by ISOIS in early PSP orbits (773109)
William H Matthaeus, University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, Riddhi Bandyopadhyay, Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States and ISOIS Suite team on PSP
 
Small Electron Events Observed by Parker Solar Probe/ISʘIS During Encounter 2 (741852)
J. Grant Mitchell1,2, Georgia Adair de Nolfo2, Matthew E Hill3, Eric R Christian4, David J McComas5, Nathan Schwadron6, Mark E Wiedenbeck7, Stuart D Bale8, Anthony W Case9, Christina Cohen10, Colin Joyce5, Justin Christophe Kasper11, Allan Wayne Labrador12, Richard A Leske13, Robert J MacDowall14, Richard Mewaldt15, Donald G Mitchell3, Marc Pulupa16, Ian G Richardson17, Michael Louis Stevens9 and Jamey R Szalay5, (1)George Washington University, Department of Physics, Washington, DC, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (4)NASA GSFC, Greenbelt, MD, United States, (5)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (6)University of New Hampshire, Durham, NH, United States, (7)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (8)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (9)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (10)Caltech, Pasadena, CA, United States, (11)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (12)Mail Code 290-17, Pasadena, CA, United States, (13)CALTECH, Pasadena, CA, United States, (14)NASA/Goddard Space Flight Center, Greenbelt, United States, (15)California Institute of Technology, Pasadena, CA, United States, (16)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (17)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States
 
Observations and Statistics of Secondary Alpha Populations in the Inner Heliosphere (767875)
Michael McManus1, Davin E Larson2, Stuart D Bale1, J. L. Verniero1, Roberto Livi3, Ali Rahmati1, Phyllis L Whittlesey3, Trevor A Bowen4, Bennett Maruca5, Justin Christophe Kasper6, Anthony W Case7, Michael Louis Stevens7, Lorenzo Matteini8, Kristopher G. Klein9 and Kelly E Korreck7, (1)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)Space Sciences Laboratory, Berkeley, CA, United States, (3)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (4)University of California Berkeley, Berkeley, CA, United States, (5)Center for Astrophysics, Berkeley, CA, United States, (6)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (7)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (8)Imperial College London, Department of Physics, London, United Kingdom, (9)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States
 
Modeling the Transport Process of a Pair of Solar Energetic Particle Events Observed by Parker Solar Probe Near Perihelion (773623)
Lulu Zhao, Florida Institute of Technology, Department of Physics and Space Sciences, Melbourne, FL, United States, Ming Zhang, Florida Institute of Technology, Melbourne, FL, United States and David Lario, The Johns Hopkins University, Laurel, MD, United States
 
A Solar Coronal Hole and Fast Solar Wind Turbulence Model and First Orbit Parker Solar Probe (PSP) Observations (745733)
Laxman Adhikari, University of Alabama in Huntsville, Huntsville, AL, United States, Gary Paul Zank, Univ of Alabama, Huntsville, Huntsville, AL, United States and Lingling Zhao, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States
 
Comparison of the Alfven Wave Solar atmosphere Model (AWSoM) with Parker Solar Probe Observations (750041)
Bart van der Holst, University of Michigan Ann Arbor, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, Benjamin D G Chandran, University of New Hampshire, Durham, NH, United States and Justin Christophe Kasper, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States