SH008
Fundamental Physics of the Solar Corona and Inner Heliosphere

Session ID#: 81546

Session Description:
The inner heliosphere provides a natural laboratory to understand how magnetized plasmas are heated, accelerated and structured over a wide range of time and spatial scales. This session explores the many facets of physical processes involved in the origins of the turbulent,  super-Alfvénic wind filling the heliosphere: what are the sources of different wind types and their connection to coronal structures? How do distribution functions evolve? What are the roles of turbulence and wave-particle interactions in heating and acceleration? How is the energization associated with structures, such as shocks, current sheets and magnetic reconnection. This session welcomes theoretical, numerical simulation, and observational papers, including contributions stemming from the initial Parker Solar Probe exploration inside the orbit of Mercury, together with theoretical developments and new challenges inspired by such observations.
Index Terms:

2164 Solar wind plasma [INTERPLANETARY PHYSICS]
2169 Solar wind sources [INTERPLANETARY PHYSICS]
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7863 Turbulence [SPACE PLASMA PHYSICS]

Primary Convener:  Chadi S Salem, University of California Berkeley, Berkeley, CA, United States
Conveners:  Marco Velli, University of California Los Angeles, Los Angeles, CA, United States, Olga Panasenco, Advanced Heliophysics, Pasadena, CA, United States and Yannis Zouganelis, European Space Agency, ESAC, Villanueva de la Canada, Spain
Primary Liaison:  Chadi S Salem, University of California, Berkeley, CA, United States
 
The Solar Wind Electron Halo as Produced by Electron Beams Originating in Nanoflares: Beam Density Dependence (485674)
Haihong Che1, Melvyn L Goldstein2, Chadi S Salem3 and Adolfo F. Vinas1, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)NASA Goddard SFC, Greenbelt, MD, United States, (3)University of California, Berkeley, CA, United States
 
Kinetic physics everywhere in the inner heliosphere: Evidence from the FIELDS instrument on Parker Solar Probe (Invited) (486810)
Stuart D Bale1, Marc Pulupa1, Keith Goetz2, John W Bonnell1, Trevor A Bowen3, Anthony W Case4, Cynthia A Cattell5, Christopher H K Chen6, James Frederick Drake7, Thierry Dudok de Wit8, Katherine Goodrich9, Peter Harvey10, Justin Christophe Kasper11, Paul J Kellogg2, Kelly E Korreck12, Vladimir Krasnoselskikh8, Davin E Larson13, Roberto Livi3, Robert J MacDowall14, Milan Maksimovic15, David Malaspina16, Alfred Mallet17, Michael McManus18, Michel Moncuquet19, Michael Louis Stevens20, Phyllis L Whittlesey3, John R Wygant2 and the PSP FIELDS and SWEAP teams, (1)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)University of Minnesota, Minneapolis, MN, United States, (3)University of California Berkeley, Berkeley, CA, United States, (4)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (5)University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States, (6)Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom, (7)University of Maryland College Park, College Park, MD, United States, (8)LPC2E, CNRS and University of Orléans, Orléans, France, (9)University of Colorado Boulder, Boulder, CO, United States, (10)Space Sciences Laboratory, Berkeley, United States, (11)University of Michigan, Ann Arbor, MI, United States, (12)Smithsonian Observatory, Cambridge, MA, United States, (13)Space Sciences Laboratory, Berkeley, CA, United States, (14)NASA/Goddard Space Flight Center, Greenbelt, United States, (15)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, Meudon, France, (16)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (17)University of California Berkeley, Walnut CREEK, CA, United States, (18)U.S. EPA, Cincinnati, United States, (19)LESIA-CNRS, Meudon Cedex, France, (20)Smithsonian Astrophysics Observatory, Cambridge, MA, United States
 
Sharp Alfvenic Impulses in the Near-Sun Solar Wind: Properties and Possible Origins (Invited) (487042)
Timothy Simon Horbury1, Lorenzo Matteini2, Thomas Woolley3, Ronan Laker4, Denise Perrone5, David Stansby6, Marco Velli7, Benjamin D G Chandran8, Stuart D Bale9, Justin Christophe Kasper10, Michael Louis Stevens11, Marc Pulupa9, Kelly E Korreck12, Davin E Larson13, Roberto Livi14, Phyllis L Whittlesey14, David Malaspina15, John W Bonnell9, Peter Harvey9, Keith Goetz16, Thierry Dudok de Wit17, Robert J. MacDowall18 and The Parker Solar Probe FIELDS and SWEAP instrument teams, (1)Imperial College, London, United Kingdom, (2)Observatoire De Paris, LESIA, Meudon, FRANCE, (3)Imperial College London, London, United Kingdom, (4)Imperial College London, Physics, London, United Kingdom, (5)Universita' della Calabria, Rende, Italy, (6)Imperial College London, London, SW7, United Kingdom, (7)University of California Los Angeles, Los Angeles, CA, United States, (8)University of New Hampshire, Durham, NH, United States, (9)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (10)University of Michigan, Ann Arbor, MI, United States, (11)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (12)Smithsonian Observatory, Cambridge, MA, United States, (13)Space Sciences Laboratory, Berkeley, CA, United States, (14)University of California Berkeley, Berkeley, CA, United States, (15)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (16)University of Minnesota, Minneapolis, MN, United States, (17)LPC2E, CNRS and University of Orléans, Orléans, France, (18)NASA Goddard SFC, Greenbelt, MD, United States
 
Do High Speed Streams from Coronal Holes Typically Have Distinct Core and Boundary Regions? (498781)
Kevin Delano, University of Texas at San Antonio, San Antonio, TX, United States, Heather Alison Elliott, Southwest Research Institute San Antonio, San Antonio, TX, United States, Susan T Lepri, University of Michigan, Ann Arbor, MI, United States and Stephen A Fuselier, Southwest Research Institute, San Antonio, TX, United States
 
Automated Analysis of Transition Region Plasma Characteristics Under Hot Coronal Footpoints (502545)
Shane Atwood, Marika McCarthy and Charles C Kankelborg, Montana State University, Bozeman, MT, United States
 
New theory of magnetic pumping as applied to spacecraft observations of particle heating (502688)
Emily Rose Lichko1, Jan Egedal1 and William S Daughton2, (1)University of Wisconsin Madison, Madison, WI, United States, (2)MS-F699, Plasma Theory and App, Los Alamos, NM, United States
 
Turbulence, Cross-Helicity, and delta|B| Evolution in the Inner Heliosphere (505864)
D Aaron Roberts, NASA Goddard Space Flight Center, Code 672, Greenbelt, MD, United States and Vadim Roytershteyn, Space Science Institute, Boulder, CO, United States
 
Temperature-anisotropy-driven instabilities and electron and ion energy budget in the expanding solar wind: fully-kinetic Expanding Box Model simulations with EB-iPic3D (506914)
Maria Elena Innocenti, NASA Jet Propulsion Laboratory, Pasadena, CA, United States, Anna Tenerani, California Institute of Technology, Pasadena, CA, United States, Elisabetta Boella, Lancaster University, Physics Department, Lancaster, United Kingdom and Marco Velli, University of California Los Angeles, Los Angeles, CA, United States
 
Perpendicular Ion Heating by Cyclotron Resonant Dissipation of Turbulently Generated Kinetic Alfvén Waves in the Solar Wind (506964)
Philip A Isenberg, University of New Hampshire, Durham, NH, United States and Bernard John Vasquez, University of New Hampshire Main Campus, Durham, NH, United States
 
The Correlation Between The Enhanced Sulfur Abundance in Slow Solar Winds and The Magnetic Field Geometry of Their Source Regions (507138)
Natsuha Kuroda, University Corporation for Atmospheric Research, Boulder, CO, United States and J. M. Laming, Naval Research Laboratory, Washington, DC, United States
 
Propagation of Alfvén waves and evolution of turbulence in the expanding solar wind with the presence of stream interaction (507927)
Chen Shi, University of California Los Angeles, Earth, Planetary and Space Sciences, Los Angeles, CA, United States, Marco Velli, University of California Los Angeles, Los Angeles, CA, United States, Anna Tenerani, California Institute of Technology, Pasadena, CA, United States and Victor Réville, IRAP, Toulouse, France; University of California Los Angeles, Los Angeles, United States
 
Ion acoustic waves and solar wind heating (508950)
Paul J Kellogg, Retired, Washington, DC, United States
 
Study of High-Temperature Emission in the Solar Corona (512361)
Mahboubeh Asgari-Targhi, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States and Alisdair R Davey, Smithsonian Astrophysical Observatory, Cambridge, MA, United States
 
Simulations of Thermal Nonequilibrium in Raining Null-Point Topologies (516761)
Emily Irene Mason, Catholic University of America, Washington, DC, United States, Spiro K Antiochos, NASA GSFC, Silver Spring, MD, United States and Nicholeen M Viall, NASA GSFC, Greenbelt, MD, United States
 
Reflection-driven MHD turbulence in the solar atmosphere and solar wind (518763)
Benjamin D G Chandran, University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States and Jean Carlos Perez, Florida Institute of Technology, Melbourne, FL, United States
 
Evidence for Solar Coronal Heating by Nanoflares Based on Coordinated EUV Spectra Observed with the EUNIS Sounding Rocket and Hinode/EIS (519365)
Jeffrey W Brosius, Catholic University of America, Washington, DC, United States, Adrian Nigel Daw, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Enrico Landi, University of Michigan, Ann Arbor, MI, United States
 
Linear and nonlinear evolution of jets and microstreams in the solar wind (519684)
Jason Derr, University of Texas at Austin, Austin, TX, United States, Anna Tenerani, California Institute of Technology, Pasadena, CA, United States and Marco Velli, University of California Los Angeles, Los Angeles, CA, United States
 
Proton-Alpha Temperature Relaxation and Preferential Heating in the Corona: a Ulysses Case Study. (524014)
Wenyi Sun, University of Science and Technology of China, Hefei, China, Chen Shi, Peking University, Beijing, China, Marco Velli, University of California Los Angeles, Los Angeles, CA, United States and Anna Tenerani, California Institute of Technology, Pasadena, CA, United States
 
Statistics of Energetic Particles in the first Parker Solar Probe Orbit: Correlations and Association with Magnetic Structures (524681)
William H Matthaeus1, Riddhi Bandyopadhyay2, Tulasi Parashar1, Alexandros Chasapis3, Rohit Chhiber1, David J Ruffolo4, Ramiz A Qudsi5, David J McComas6, Eric R Christian7, Jamey R Szalay6, Colin Joyce6, Melvyn L. Goldstein8, Bennett Maruca2, Joe Giacalone9, Nathan Schwadron10, Donald G Mitchell11, Mark E Wiedenbeck12, Ralph L McNutt Jr13, Stuart Bale14, John W Bonnell15, Thierry Dudok de Wit16, Keith Goetz17, Peter Harvey18, Robert J MacDowall19, David Malaspina20, Marc Pulupa15, Justin Christophe Kasper21, Kelly E Korreck22, Anthony W Case23, Michael Stevens24, Phyllis L Whittlesey25, Davin E Larson26, Roberto Livi25, Marco Velli27 and Nour Raouafi11, (1)University of Delaware, Newark, DE, United States, (2)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (3)Laboratory for Atmospheric and Space Physics, Boulder, United States, (4)Mahidol University, Department of Physics, Faculty of Science, Bangkok, Thailand, (5)University of Delaware, Department of Physics & Astronomy, Newark, DE, United States, (6)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (7)NASA GSFC, Greenbelt, MD, United States, (8)Space Science Institute, Baltimore, MD, United States, (9)University of Arizona, Tucson, AZ, United States, (10)University of New Hampshire, Durham, NH, United States, (11)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (12)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (13)Johns Hopkins Univ/APL, Laurel, MD, United States, (14)University of California, Berkeley, Berkeley, CA, United States, (15)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (16)LPC2E, CNRS and University of Orléans, Orléans, France, (17)University of Minnesota, Minneapolis, MN, United States, (18)Space Sciences Laboratory, Berkeley, United States, (19)NASA/Goddard Space Flight Center, Greenbelt, United States, (20)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (21)University of Michigan, Ann Arbor, MI, United States, (22)Smithsonian Observatory, Cambridge, MA, United States, (23)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (24)Royal Holloway University of London, Egham, TW20, United Kingdom, (25)University of California Berkeley, Berkeley, CA, United States, (26)Space Sciences Laboratory, Berkeley, CA, United States, (27)University of California Los Angeles, Los Angeles, CA, United States
 
On the properties of the Electron Heat Flux and Thermal Force in the Solar Wind at 1AU: New Insights from Wind Observations (527808)
Chadi S Salem, University of California Berkeley, Berkeley, CA, United States, Marc Pulupa, University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States and Jack D Scudder, Univ of Iowa, Iowa City, IA, United States
 
Electron-Langmuir wave resonance in 3D and implications for the evolution of electron distributions in the heliosphere. (529312)
James Harding, University of Sydney, School of Physics, Sydney, NSW, Australia, Iver Cairns, University of Sydney, Sydney, Australia and Donald B Melrose, University of Sydney, SIfA, School of Physics, Sydney, Australia
 
Dependency of Plasma Emission on Plasma-to-Cyclotron Frequency Ratio: Particle-In-Cell Simulation (530991)
Sang-Yun Lee, KAIST Korea Advanced Institute of Science and Technology, Daejeon, Korea, Republic of (South), Peter H Yoon, University of Maryland, IPST, College Park, MD, United States and Ensang Lee, Dept. of Astronomy and Space Science, Kyung Hee University, Yongin, Gyeonggi, South Korea
 
Probing Fine Spatial, Temporal and Spectral Structures of Extremely Quiet Radio Sun (533225)
Rohit Sharma, University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland and Divya Oberoi, MIT Haystack Observatory, Westford, MA, United States
 
Validating the Alfven Wave Solar Atmosphere (AWSoM) Model from the Low Corona to 1 AU (539677)
Nishtha Sachdeva1, Bart van der Holst1, Ward Manchester1, Gabor Toth1, Diego Gustavo Lloveras2, Alberto M Vásquez3, Philippe Lamy4, Bernard V Jackson5 and Carl J Henney6, (1)University of Michigan, Ann Arbor, MI, United States, (2)University of Buenos Aires, Physics, Buenos Aires, Argentina, (3)Instituto de Astronoma y Fsica del Espacio, Buenos Aires, Argentina, (4)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (5)Univ California San Diego, Center for Astrophysics and Space Sciences, La Jolla, CA, United States, (6)Air Force Research Laboratory Kirtland AFB, Kirtland AFB, NM, United States
 
The role of Alfvén wave dynamics in the large scale properties of the solar wind: comparing 3D MHD simulation and PSP data (546039)
Victor Réville1,2, Marco Velli3, Olga Panasenco4, Anna Tenerani5, Chen Shi6, Alexis P Rouillard7, Stuart D Bale8, Justin Christophe Kasper9, Samuel Timothy Badman10, Kelly E Korreck11, Marc Pulupa8, John W Bonnell8, Anthony W Case12, Davin E Larson13, Roberto Livi10, Michael Louis Stevens14, Phyllis L Whittlesey10, David Malaspina15, Peter Harvey16, Keith Goetz17, Thierry Dudok de Wit18 and Robert J MacDowall19, (1)University of California Los Angeles, Los Angeles, United States, (2)IRAP, Toulouse, France, (3)University of California Los Angeles, Los Angeles, CA, United States, (4)Advanced Heliophysics, Pasadena, CA, United States, (5)University of Texas at Austin, Austin, TX, United States, (6)University of California Los Angeles, Earth, Planetary and Space Sciences, Los Angeles, CA, United States, (7)IRAP/CNRS, Toulouse, France, (8)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (9)University of Michigan, Ann Arbor, MI, United States, (10)University of California Berkeley, Berkeley, CA, United States, (11)Smithsonian Observatory, Cambridge, MA, United States, (12)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (13)Space Sciences Laboratory, Berkeley, CA, United States, (14)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (15)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (16)Space Sciences Laboratory, Berkeley, United States, (17)University of Minnesota, Minneapolis, MN, United States, (18)LPC2E, CNRS and University of Orléans, Orléans, France, (19)NASA/Goddard Space Flight Center, Greenbelt, United States
 
Numerical simulations of the evolution of magnetic field kinks in the solar wind (547610)
Anna Tenerani1, Marco Velli2, Victor Réville3, Chen Shi4, Stuart D Bale5, Justin Christophe Kasper6, Michael Louis Stevens7, Anthony W Case8, Kelly E Korreck9, Davin E Larson10, Roberto Livi11, Kristopher G. Klein12, Phyllis L Whittlesey11, Marc Pulupa5, David Malaspina13, John W Bonnell5, Peter Harvey14, Keith Goetz15, Thierry Dudok de Wit16 and Robert J. MacDowall17, (1)University of Texas at Austin, Austin, TX, United States, (2)University of California Los Angeles, Los Angeles, CA, United States, (3)IRAP, Toulouse, France, (4)Peking University, Beijing, China, (5)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (6)University of Michigan, Ann Arbor, MI, United States, (7)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (8)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (9)Smithsonian Observatory, Cambridge, MA, United States, (10)Space Sciences Laboratory, Berkeley, CA, United States, (11)University of California Berkeley, Berkeley, CA, United States, (12)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (13)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (14)Space Sciences Laboratory, Berkeley, United States, (15)University of Minnesota, Minneapolis, MN, United States, (16)LPC2E, CNRS and University of Orléans, Orléans, France, (17)NASA Goddard SFC, Greenbelt, MD, United States
 
Kinetic models of current sheets in the solar wind (550062)
Thomas Neukirch, University of St Andrews, St Andrews, KY16, United Kingdom, Ivan Vasko, University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, Anton Artemyev, University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, CA, United States and Oliver Allanson, University of Reading, Meteorology, Reading, United Kingdom
 
The Onset and Development of 3D Magnetic Reconnection in the Solar Corona: New Insights (550826)
James A Klimchuk1, Lars K. S. Daldorff2, James Edward Leake1 and Kalman Joshua Knizhnik3, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Catholic University of America, Washington, DC, United States, (3)US Naval Research Laboratory, Washington, DC, United States
 
Mechanisms of generation and statistical properties of whistler waves in the solar wind (551709)
Ivan Vasko1, Yuguang Tong2, Stuart Bale3, Anton Artemyev4, Forrest Mozer2 and Vladimir Krasnoselskikh5, (1)Space Science Lab, UC Berkeley, Berkeley, CA, United States, (2)University of California Berkeley, Berkeley, CA, United States, (3)University of California, Berkeley, Berkeley, CA, United States, (4)University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, CA, United States, (5)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Orléans Cedex 2, France
 
The Onset and Development of 3D Magnetic Reconnection in the Solar Corona: Important Physical Details (552788)
Lars K. S. Daldorff, Catholic University of America, Washington, DC, United States, James Edward Leake, NASA Goddard Space Flight Center, Greenbelt, MD, United States, James A Klimchuk, NASA GSFC, Solar Physics Lab, Greenbelt, MD, United States and Kalman Joshua Knizhnik, US Naval Research Laboratory, Washington, DC, United States
 
Large Scale Structure of the Solar Wind, Poynting Flux, and Ion Energy Flow between 35 and 130 Solar Radii. (554882)
John R Wygant1, Forrest Mozer2, Stuart D Bale3, Marc Pulupa3, Samuel Timothy Badman4, John W Bonnell3, David Malaspina5, Robert J MacDowall6, Peter Harvey7, Keith Goetz8, Justin Christophe Kasper9, Michael Louis Stevens10, Kelly E Korreck11, Katherine Goodrich12, Aaron W Breneman13, Davin E Larson14, Phyllis L Whittlesey2, Anthony W Case15, Cynthia A Cattell16, Vladimir Krasnoselskikh17, Thierry Dudok de Wit17, Christopher Carew Chaston18 and Oleksiy V Agapitov19, (1)University of Minnesota Twin Cities, Minneapolis, MN, United States, (2)University of California Berkeley, Berkeley, CA, United States, (3)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (4)University of Oxford, Oxford, United Kingdom, (5)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (6)NASA/Goddard Space Flight Center, Greenbelt, United States, (7)Space Sciences Laboratory, Berkeley, United States, (8)University of Minnesota, Minneapolis, MN, United States, (9)University of Michigan, Ann Arbor, MI, United States, (10)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (11)Smithsonian Observatory, Cambridge, MA, United States, (12)University of Colorado Boulder, Boulder, CO, United States, (13)The University of Minnesota, Minneapolis, MN, United States, (14)Space Sciences Laboratory, Berkeley, CA, United States, (15)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (16)University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States, (17)LPC2E, CNRS and University of Orléans, Orléans, France, (18)Univ California Berkeley, Berkeley, CA, United States, (19)Space Science Laboratory, UCB, Berkeley, CA, United States
 
Modeling the Steady Solar Wind with an Observationally Driven Fluxon Coronal Magnetic Field (555192)
Chris Lowder, Derek A Lamb and Craig DeForest, Southwest Research Institute, Boulder, CO, United States
 
The Thermal Force: Omnipresent Coulomb Friction and Neglected Player in Internal Energy Redistribution in the Solar Wind (556372)
Jack D Scudder, University of Iowa, Iowa City, IA, United States
 
The Radial Dependence of Proton-scale Magnetic Spectral Break During PSP Encounter 2 (569036)
Die Duan1,2, Trevor A Bowen3, Christopher H K Chen4, Jiansen He5, Alfred Mallet6,7, Stuart D Bale8, Daniel Vech9, Marc Pulupa8, David Malaspina10, John W Bonnell8, Peter Harvey11, Keith Goetz12, Thierry Dudok de Wit13, Robert J MacDowall14, Justin Christophe Kasper15, Anthony W Case16, Kelly E Korreck17, Davin E Larson18, Roberto Livi3, Michael Louis Stevens19 and Phyllis L Whittlesey3, (1)Peking University, School of Earth and Space Sciences, Beijing, China, (2)Space Science Laboratory, UCB, Berkeley, United States, (3)University of California Berkeley, Berkeley, CA, United States, (4)Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom, (5)Peking University, Beijing, China, (6)University of New Hampshire, Durham, NH, United States, (7)Space Science Laboratory, UCB, Berkeley, CA, United States, (8)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (9)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (10)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (11)Space Sciences Laboratory, Berkeley, United States, (12)University of Minnesota, Minneapolis, MN, United States, (13)LPC2E, CNRS and University of Orléans, Orléans, France, (14)NASA/Goddard Space Flight Center, Greenbelt, United States, (15)University of Michigan, Ann Arbor, MI, United States, (16)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (17)Smithsonian Observatory, Cambridge, MA, United States, (18)Space Sciences Laboratory, Berkeley, CA, United States, (19)Smithsonian Astrophysics Observatory, Cambridge, MA, United States
 
Flocculation, switchbacks, and loss of Alfvenicity: Indicators of shear-driven turbulence in the young solar wind? (571914)
David J Ruffolo1, William H Matthaeus2, Craig DeForest3, Tulasi Parashar2, Melvyn L Goldstein4,5, D Aaron Roberts6, Rohit Chhiber2, Arcadi V. Usmanov2,4, Thierry Dudok de Wit7, Riddhi Bandyopadhyay8, Alexandros Chasapis9, Bennett Maruca10, Marco C M Velli11 and Justin Christophe Kasper12, (1)Mahidol University, Department of Physics, Faculty of Science, Bangkok, Thailand, (2)University of Delaware, Newark, DE, United States, (3)Southwest Research Institute, Boulder, CO, United States, (4)NASA Goddard SFC, Greenbelt, MD, United States, (5)University of Maryland Baltimore County, Baltimore, MD, United States, (6)NASA Goddard SFC, Code 672, Greenbelt, MD, United States, (7)LPC2E, CNRS and University of Orléans, Orléans, France, (8)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (9)Laboratory for Atmospheric and Space Physics, Boulder, United States, (10)Center for Astrophysics, Berkeley, CA, United States, (11)University of California Los Angeles, Earth Planetary and Space Sciences, Los Angeles, CA, United States, (12)University of Michigan, Ann Arbor, MI, United States
 
MHD mode decomposition in the inner-heliosphere from the Parker Solar Probe (572514)
Christopher Carew Chaston1, John W Bonnell2, Stuart Bale3, Justin Christophe Kasper4, John R Wygant5, Marc Pulupa2, Phyllis L Whittlesey6, Davin E Larson7, Robert J. MacDowall8, Roberto Livi6, Chadi S Salem9, Daniel Vech10, Anthony W Case11, Keith Goetz5, Kelly E Korreck12, Peter Harvey2, David Malaspina13, Michael Louis Stevens14 and Thierry Dudok de Wit15, (1)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)University of California, Berkeley, Berkeley, CA, United States, (4)University of Michigan, Ann Arbor, MI, United States, (5)University of Minnesota, Minneapolis, MN, United States, (6)University of California Berkeley, Berkeley, CA, United States, (7)Space Sciences Laboratory, Berkeley, CA, United States, (8)NASA Goddard SFC, Greenbelt, MD, United States, (9)University of California, Berkeley, CA, United States, (10)Lawrence, KS, United States, (11)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (12)Smithsonian Observatory, Cambridge, MA, United States, (13)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (14)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (15)LPC2E, CNRS and University of Orléans, Orléans, France
 
Whistler Waves and the Halo Electron Anisotropies in the Inner Heliosphere: Helios Observations (576271)
vamsee Krishna Jagarlamudi1, Olga Alexandrova2, Laura Bercic2, Thierry Dudok de Wit3, Vladimir Krasnoselskikh3 and Milan Maksimovic2, (1)LPC2E, Orleans, France, (2)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, Meudon, France, (3)LPC2E, CNRS and University of Orléans, Orléans, France
 
Solar Wind Turbulence at Kinetic Scales in the Inner Heliosphere (582165)
Olga Alexandrova1, Vamsee Krishna Jagarlamudi2, Milan Maksimovic1, Petr Hellinger3 and Yuri Shprits4, (1)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, Meudon, France, (2)LPC2E, CNRS and University of Orléans, Orléans, France, (3)Astronomical Institute, CAS, Ondrejov/Prague, Czech Republic, (4)GFZ German Research Centre for Geosciences, Potsdam, Germany
 
Photospheric Vortices and Coronal Energy Storage And Release (591857)
Marco C M Velli, University of California Los Angeles, Earth Planetary and Space Sciences, Los Angeles, CA, United States, Franco Rappazzo, University of California Los Angeles, Los Angeles, CA, United States, Giorgio Einaudi, Berkeley Research Associates, Inc., Berkeley, CA, United States and Russell B. Dahlburg, Naval Research Laboratory, Washington, DC, United States
 
Zone of Preferential Heating for Heavy Ions in the Solar Wind (600451)
Janelle Holmes, University of Michigan Ann Arbor, Ann Arbor, MI, United States, Justin Christophe Kasper, University of Michigan, Ann Arbor, MI, United States and Kristopher G. Klein, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States
 
Intermittency Statistics of the Expanding Solar Wind: Helios 1 (.3 to 1 AU) and Voyager 1 (1 to 10 AU) (601010)
Manuel Enrique Cuesta, Tulasi Parashar and William H Matthaeus, University of Delaware, Newark, DE, United States
 
Volume-filling Simulations of Coronal Loops Heated by Nanoflares (601102)
Joseph Plowman1, Will Barnes2, Stephen J. Bradshaw3, Amir Caspi4, Craig DeForest4 and James A Klimchuk5, (1)National Solar Observatory, Tucson, AZ, United States, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States, (3)Rice University, Department of Physics and Astronomy, Houston, TX, United States, (4)Southwest Research Institute, Boulder, CO, United States, (5)NASA GSFC, Solar Physics Lab, Greenbelt, MD, United States
 
Data-Driven MHD Model of Global Solar Corona and Inner Heliosphere with Nearly Incompressible MHD Turbulence Coronal Heating (606269)
Mehmet Sarp Yalim, University of Alabama in Huntsville, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States, Nikolai V Pogorelov, University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States, Gary Paul Zank, Univ of Alabama, Huntsville, Huntsville, AL, United States and Laxman Adhikari, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States
 
Comparing Coronal Hole Wave Properties and Density Profiles Derived from Indirect and Direct Observations (607489)
Micah J Weberg1, Yuan-Kuen Ko2, J. M. Laming2 and Harry Warren2, (1)US National Research Council of the National Academies, Washington, United States, (2)Naval Research Laboratory, Washington, DC, United States
 
Particle Heating and Turbulence in Low-beta Guide Field Reconnection (608107)
Qile Zhang1, James Frederick Drake1 and Marc Swisdak2, (1)University of Maryland College Park, College Park, MD, United States, (2)University of Maryland, College Park, MD, United States
 
Coronal Hole Variation from Chromosphere to Solar Wind (617539)
Paul Bryans, High Altitude Observatory, Boulder, CO, United States
 
Tracking Topological Changes in MHD Simulations using Slip-Back Mapping (622467)
Roberto Lionello, Viacheslav S. Titov, Jon Linker and Zoran Mikic, Predictive Science Inc., San Diego, CA, United States
 
Tomographic Measurements of Magnetic Free Energy in CME Source Regions (628553)
Haosheng Lin, Institute for Astronomy, Honolulu, HI, United States, Maxim Kramar, University of Hawaii at Manoa, Institute for Astronomy, Honolulu, HI, United States and Steven Tomczyk, National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States
 
What controls the thermodynamic evolution of the expanding solar wind? (628697)
Jungjoon Seough, KASI Korea Astronomy and Space Science Institute, Daejeon, Korea, Republic of (South), Peter H Yoon, University of Maryland, IPST, College Park, MD, United States and Yasuhiro Nariyuki, University of Toyama, Toyama, Japan
 
Oscillation of a Small Hα Surge in a Solar Polar Coronal Hole (628743)
Kyung-Suk F Cho, KASI Korea Astronomy and Space Science Institute, Daejeon, Korea, Republic of (South)
 
Interplay among Eruptive Processes, Global Oscillations, and Broad Spectra of Alfvén Waves in Arched Magnetized Plasmas (631882)
Shreekrishna Tripathi1, Kamil Krynski1 and Walter N Gekelman2, (1)University of California Los Angeles, Los Angeles, CA, United States, (2)UCLA, Los Angeles, CA, United States
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