SH016
Fundamental Plasma Physics and Turbulence Energy Transfer: From MHD to Kinetic Scales III Posters

Wednesday, 9 December 2020: 04:00-20:59
Poster
Primary Convener:  William H Matthaeus, University of Delaware, Department of Physics and Astronomy, Newark, DE, United States
Conveners:  Luca Sorriso-Valvo, CNR-ISTP, Bari, Italy; CNR National Research Council, Rome, Italy, Tulasi N Parashar, Victoria University of Wellington, Wellington, New Zealand and Yan Yang, Southern University of Science and Technology, Shenzhen, China
Primary Liaison:  William H Matthaeus, University of Delaware, Department of Physics and Astronomy, Newark, DE, United States
Chairs:  William H Matthaeus, University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, Luca Sorriso-Valvo, ISTP-CNR, Bari, Bari, Italy, Tulasi N Parashar, Victoria University of Wellington, Wellington, New Zealand and Yan Yang, Southern University of Science and Technology, Shenzhen, China
OSPA Liaison:  Yan Yang, Southern University of Science and Technology, Shenzhen, China
 
Karman-Howarth-Monin equation for compressible Hall MHD turbulence (740095)
Petr Hellinger1, Emanuele Papini2, Andrea Verdini3, Simone Landi2, Luca Franci4 and Lorenzo Matteini5, (1)Astronomical Institute, CAS, Ondrejov/Prague, Czech Republic, (2)Università degli Studi di Firenze, Florence, Italy, (3)Università di Firenze, Dipartimento di Fisica e Astronomia, Firenze, Italy, (4)Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom, (5)Imperial College London, Department of Physics, London, United Kingdom
 
Particle-in-cell Simulations of Kinetic Range Plasma Turbulence: Does Microinstability Growth Lead to Intermittency? (670489)
Stephen Peter Gary, Space Science Institute, Boulder, CO, United States, Chen Cui, University of Southern California, Los Angeles, CA, United States and Joseph Wang, University of Southern California, Department of Astronautical Engineering, Los Angeles, CA, United States
 
Four-Dimensional Frequency-Wavenumber Spectra from Hybrid Kinetic Simulations of Quasi-Perpendicular Turbulence (676913)
Bernard John Vasquez, University of New Hampshire, Durham, NH, United States and Sergei A Markovskii, Univ New Hampshire, Durham, NH, United States
 
Scalable simulations of 3D LTSTMR with a novel plasma statistical physics algorithm (680327)
Bojing Zhu, Chinese Academy of Sciences, Beijing, China, Huihong Cheng, Key Laboratory of Computational Geodynamics, Chinese Academy of Sciences, Beijing, China and David A Yuen, Univ of Minnesota, Minneapolis, MN, United States
 
Observations of Low-Frequency Waves Excited by Newborn Interstellar Pickup He+ as Seen by the Juno Spacecraft (680383)
Sydney Neuman1,2, Charles William Smith3, Matthew R Argall3, Colin Joyce4, Philip A Isenberg5, Bernard John Vasquez3, Nathan Schwadron3, Maciej Bzowski6 and Marzena A. Kubiak6, (1)University of New Hampshire Main Campus, Department of Physics and Institute for the Study of Earth, Oceans and Space, Durham, NH, United States, (2)Rensselaer Polytechnic Institute, Materials Science and Engineering Department, Troy, NY, United States, (3)University of New Hampshire, Durham, NH, United States, (4)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (5)Univ New Hampshire, Durham, NH, United States, (6)Space Research Centre Polish Academy of Sciences, Warsaw, Poland
 
Statistical Survey of Collisionless Dissipation in the Terrestrial Magnetosheath (710692)
Yanwen Wang1, Riddhi Bandyopadhyay2, Rohit Chhiber3,4, Alexandros Chasapis5 and William H Matthaeus3, (1)University of Delaware, Newark, DE, United States, (2)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (3)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (4)NASA Goddard Space Flight Center, Greenbelt, DE, United States, (5)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States
 
Feasibility of Ion-cyclotron Resonant Heating in the Solar Wind (718184)
Roberto Navarro, Univ. Concepcion, Departamento de Física, Concepcion, Chile, Victor Munoz, Universidad de Chile, Santiago, Chile, Juan Alejandro Valdivia, University of Chile, Department of Physics, Faculty of Sciences, Santiago, Chile and Pablo S Moya, University of Chile, Santiago, Chile
 
Anisotropy of Magnetic Field and Velocity Fluctuations in the Solar Wind (722123)
Jana Safrankova1, Zdenek Nemecek2, Frantisek Nemec2, Victor Montagud-Camps2, Daniel Verscharen3,4 and Tereza Durovcova2, (1)Charles University, Prague, 180, Czech Republic, (2)Charles University, Prague, Czech Republic, (3)University of New Hampshire, Space Science Center, Durham, United States, (4)University College London, Mullard Space Science Laboratory, Dorking, United Kingdom
 
Hybrid Formulation of Fully- and Gyrokinetic Hamiltonian Field Theory for Space and Laboratory Plasma (724160)
Felipe Nathan de Oliveira Lopes1, Karen Pommois2, Aleksandr Mustonen2, Simon Lautenbach3, Florian Allmann-Rahn3, Rainer Grauer3 and Daniel Told2, (1)Max Planck Institute for Plasma Physics, Greifswald, Germany, (2)Max Planck Institute for Plasma Physics, Munich, Germany, (3)Ruhr University Bochum, Bochum, Germany
 
Comparison of basis functions defined on infinite interval for pseudo-spectral Vlasov solvers (726294)
Taiki Jikei, University of Tokyo, Bunkyo-ku, Japan and Takanobu Amano, The University of Tokyo, Bunkyo-ku, Japan
 
Inverse and direct energy cascades in two-dimensional β-plane magnetohydrodynamic turbulence (726580)
Timofey Zinyakov, Space Research Institute of the Russian Academy of Sciences, Moscow, Russia and Arakel Petrosyan, Space Research Institute RAS, Moscow, Russia
 
Magnetic Field Intermittency Statistics in the Expanding Solar Wind: Parker Solar Probe (Encounters 1-3), Helios 1 (0.3 to 1AU), and Voyager 1 (1 to 10AU) (739437)
Manuel Enrique Cuesta1, Tulasi Parashar2, Riddhi Bandyopadhyay3, Rohit Chhiber1,4 and William H Matthaeus1, (1)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (2)Victoria University of Wellington, Wellington, New Zealand, (3)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (4)NASA Goddard Space Flight Center, Greenbelt, DE, United States
 
Solar Wind Turbulence from 1 to 45 AU (740614)
Zackary Bradley Pine1, Charles William Smith2, Sophia Hollick3, Matthew R Argall2, Bernard John Vasquez2, Philip A Isenberg4, Nathan Schwadron2, Colin Joyce5, Justyna M Sokol6, Maciej Bzowski7, Megan L. McLaurin8, Kathleen E Hamilton9 and Robert James Leamon10, (1)Boston University, Boston, MA, United States, (2)University of New Hampshire, Durham, NH, United States, (3)Providence, RI, United States, (4)Univ New Hampshire, Durham, NH, United States, (5)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (6)Space Research Center Polish Academy of Sciences, Warszawa, Poland, (7)Space Research Centre Polish Academy of Sciences, Warsaw, Poland, (8)Wolters Kluwer, Waltham, MA, United States, (9)Oak Ridge National Laboratory, Quantum Computing Institute, Oak Ridge, TN, United States, (10)NASA Headquarters, Washington, DC, United States
 
von Karman Correlation Similarity in Solar Wind Magnetic Turbulence: Comparison of near-Sun (below 0.17 AU) observations from Parker Solar Probe with ACE measurements at 1 AU (754141)
Sohom Roy1, Rohit Chhiber2,3, Maria Emilia Ruiz4, Sergio Dasso4, Minping Wan1 and William H Matthaeus2, (1)University of Delaware, Newark, DE, United States, (2)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (3)NASA Goddard Space Flight Center, Greenbelt, DE, United States, (4)University of Buenos Aires, Buenos Aires, Argentina
 
Relative heating of ions and electrons in the young solar wind due to turbulent dissipation mediated via Landau damping (761839)
Niranjana Shankarappa1, Kristopher G. Klein2, Mihailo Martinovic2, Emily Rose Lichko2, Justin Christophe Kasper3, Jia Huang3, Anthony W Case4, Michael Louis Stevens4, Kelly E Korreck4, Stuart D Bale5 and Gregory G Howes6, (1)University of Arizona, Department of Physics, Tucson, AZ, United States, (2)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (4)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (5)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (6)Department of Physics and Astronomy, University of Iowa, Iowa City, IA, United States
 
How Pickup Ions Generate Turbulence in the Inner Heliosheath: A Multi-Fluid Approach (763251)
Bertalan Zieger, Boston University, Boston, MA, United States, Merav Opher, Boston University, Astronomy, Boston, MA, United States, Gabor Toth, University of Michigan, Department of Climate and Space, Center for Space Environment Modeling, Ann Arbor, MI, United States and Vladimir A Florinski, University of Alabama, Huntsville, AL, United States