SH051
Turbulence and Magnetic Reconnection: What New Science Do We Learn from Parker Solar Probe? II Posters

Wednesday, 16 December 2020: 04:00-20:59
Poster
Primary Convener:  Stas Boldyrev, University of Wisconsin Madison, Madison, WI, United States
Conveners:  Vadim Roytershteyn, Space Science Institute, Boulder, CO, United States and Stuart D Bale, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
Primary Liaison:  Stas Boldyrev, University of Wisconsin Madison, Madison, WI, United States
Chairs:  Stas Boldyrev, University of Wisconsin Madison, Madison, WI, United States, Vadim Roytershteyn, Space Science Institute, Boulder, CO, United States and Stuart D Bale, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
OSPA Liaison:  Stas Boldyrev, University of Wisconsin Madison, Madison, WI, United States
 
The effect of solar observables on magnetic reconnection activity in the solar wind (737395)
Bjorn Larsen, California State University Chico, Chico, CA, United States and Stefan Eriksson, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States
 
Particle Acceleration in Electron-only Reconnection in the Low Electron Beta Regime (698298)
Cristian Vega, University of Wisconsin Madison, Physics, Madison, WI, United States, Stas Boldyrev, University of Wisconsin Madison, Madison, WI, United States, Vadim Roytershteyn, Space Science Institute, Boulder, CO, United States and Gian Luca Delzanno, Los Alamos National Laboratory, Los Alamos, NM, United States
 
Orientation and discontinuity analyses of near-Sun magnetic field switchbacks (730658)
Mojtaba Akhavan-Tafti1, Justin Christophe Kasper2, Jia Huang2 and Stuart Bale3, (1)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (2)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (3)University of California, Berkeley, Berkeley, CA, United States
 
Disentangling space-time variations in Parker Solar Probe solar wind turbulence observations (764000)
Jean Carlos Perez and Sofiane Bourouaine, Florida Institute of Technology, Aerospace, Physics and Space Sciences, Melbourne, FL, United States
 
Intermittency scaling laws in the fast solar wind and magnetohydrodynamic turbulence simulations. (770600)
Juan Carlos Carlos Palacios, Jean Carlos Perez and Sofiane Bourouaine, Florida Institute of Technology, Aerospace, Physics and Space Sciences, Melbourne, FL, United States
 
Spectral Features in Field-aligned Solar Wind Turbulence from Parker Solar Probe Observations (734239)
Lingling Zhao1, Gary Paul Zank2, Laxman Adhikari3, Masaru Nakanotani1, Daniele Telloni4 and Francesco Carbone5, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)Univ of Alabama, Huntsville, Huntsville, AL, United States, (3)Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States, (4)INAF-OATO, Turin, Italy, (5)CNR Institute of Atmospheric Pollution Research, Rende, Italy
 
Identification of Flux Ropes through Magnetic Helicity and Partial Variance of Increments (697935)
Francesco Pecora1, Sergio Servidio1, Antonella Greco1 and William H Matthaeus2, (1)Università della Calabria, Department of Physics, Rende, Italy, (2)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States
 
Energy Budget in Decaying Compressible MHD Turbulence (720982)
Yan Yang1, Minping Wan1 and William H Matthaeus2, (1)Southern University of Science and Technology, Shenzhen, China, (2)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States
 
In situ observation of three-dimensional anisotropy and scalings of space plasmas turbulence at kinetic scales (721719)
Tieyan Wang, Rutherford Appleton Laboratory, Didcot, OX11, United Kingdom, Jiansen He, Peking University, Beijing, China, Olga Alexandrova, LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, Meudon, France, Malcolm Wray Dunlop, Rutherford Appleton Laboratory, Didcot, United Kingdom and Denise Perrone, ASI, Rome, Italy
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