SH029
Fundamental Physics of the Solar Corona and Inner Heliosphere IV Posters

Friday, 11 December 2020: 04:00-20:59
Poster
Primary Convener:  Chadi S Salem, University of California Berkeley, Berkeley, CA, United States
Conveners:  Marco C M 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 Can, Spain
Primary Liaison:  Chadi S Salem, University of California, Berkeley, CA, United States
Chairs:  Chadi S Salem, University of California, Berkeley, CA, United States, Olga Panasenco, Advanced Heliophysics, Pasadena, CA, United States and Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States
OSPA Liaison:  Chadi S Salem, University of California, Berkeley, CA, United States
 
A Kinetic Simulation of Ponderomotive Interactions Between Reflecting Coronal Alfvén Waves and Particles (708566)
Kendra Bergstedt1, Jonathan Jara-Almonte2 and Hantao Ji2, (1)Princeton University, Princeton, NJ, United States, (2)Princeton Plasma Physics Laboratory, Princeton, NJ, United States
 
The Role of Gurevich Ion Acceleration in Heating the Solar Corona (661054)
Claudio vita-Finzi, Natural History Museum of London, London, United Kingdom
 
Accelerating and Supersonic Density Disturbances in Solar Polar Plumes (671594)
Il-Hyun Cho1, Yong-Jae Moon2, Valeri M Nakariakov3, Jin-Yi Lee4, Dae Jung Yu5, Kyung-Suk F Cho6, Vasyl Yurchyshyn7 and Harim Lee4, (1)Kyung Hee University, Astronomy and Space Science, Yongin-si, South Korea, (2)School of Space Research, Kyung Hee University, Yongin, South Korea, (3)University of Warwick, Physics, Coventry, United Kingdom, (4)Kyung Hee University, Yongin, Korea, Republic of (South), (5)Kyung Hee University, Yongin-si, South Korea, (6)KASI, Daejeon, South Korea, (7)Big Bear Solar Observatory, Big Bear City, CA, United States
 
Proton Core Behaviour inside Magnetic Field Switchbacks (671794)
Thomas Woolley1, Lorenzo Matteini2, Timothy Simon Horbury3, Stuart Bale2,4, Lloyd David Woodham5, Ronan Laker5, Benjamin L Alterman6, John W Bonnell7, Anthony W Case8, Justin Christophe Kasper8,9, Kristopher G. Klein10, Mihailo Martinovic11,12 and Michael Louis Stevens8, (1)Imperial College London, Department of Physics, London, United Kingdom, (2)Imperial College London, Physics, London, United Kingdom, (3)Imperial College London, Physics, London, SW7, United Kingdom, (4)University of California, Berkeley, Berkeley, CA, United States, (5)Imperial College London, Department of Physics, London, SW7, United Kingdom, (6)Southwest Research Institute, San Antonio, MI, United States, (7)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (8)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (9)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (10)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (11)Paris Observatory Meudon, Meudon, France, (12)University of Arizona, Lunar and Planetary Laboratory, Tucson, United States
 
Free energy available to microinstabilities in the solar wind (673589)
Emily Rose Lichko and Kristopher G. Klein, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States
 
Effect of Higher Radial Harmonics in Sausage Oscillations in Coronal Loops (673803)
Daye Lim, Kyung Hee University, Astronomy and Space Science, Yongin, Korea, Republic of (South), Valeri M Nakariakov, University of Warwick, Physics, Coventry, United Kingdom, Yong-Jae Moon, School of Space Research, Kyung Hee University, Yongin, South Korea, Dae Jung Yu, Kyung Hee University, Yongin-si, South Korea and Il-Hyun Cho, Kyung Hee University, Astronomy and Space Science, Yongin-si, South Korea
 
Spicule Jets in the Solar Atmosphere Modeled with Resistive MHD and Thermal Conduction (674965)
José Juan Juan González, CONACyT - Servicio de Clima Espacial Mexico - Laboratorio Nacional de Clima Espacial, SCiESMEX – LANCE, Instituto de Geofísica, Unidad Michoacán, UNAM, Morelia, MH, Mexico, Francisco Guzmán, Universidad Michoacana de San Nicolás de Hidalgo, Instituto de Física y Matemáticas, Morelia, MH, Mexico, Viktor Fedun, The University of Sheffield, Sheffield, United Kingdom and Gary Verth, University of Sheffield, School of Mathematics and Statistics, Sheffield, S10, United Kingdom
 
Formation of Unique Magnetic Structures Observed in the Inner Heliosphere: from Braids to Knots (676465)
Ilan Roth, University of California at Berkeley, Space Sciences, Berkeley, CA, United States
 
Simulating the FIP Effect in Coronal Loops Using a Multi-Species Kinetic-Fluid Model (680287)
Nicolas Poirier1, Michael Lavarra1, Alexis P Rouillard2, Mikel Indurain1, Pierre-Louis Blelly1, Rui Pinto2 and Victor Réville1, (1)IRAP, Toulouse, France, (2)IRAP/CNRS, Toulouse, France
 
Shear-Driven Transition to Isotropically Turbulent Solar Wind Outside the Alfvén Critical Zone (686877)
David J Ruffolo1, William H Matthaeus2, Rohit Chhiber2,3, Arcadi V. Usmanov2,3, Yan Yang4, Riddhi Bandyopadhyay5, Tulasi Parashar2,6, Melvyn L Goldstein7, Craig DeForest8, Minping Wan4, Alexandros Chasapis9, Bennett Maruca2, Marco C M Velli10 and Justin Christophe Kasper11,12, (1)Mahidol University, Department of Physics, Faculty of Science, Bangkok, Thailand, (2)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (3)NASA Goddard Space Flight Center, Greenbelt, DE, United States, (4)Southern University of Science and Technology, Shenzhen, China, (5)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (6)Victoria University of Wellington, Wellington, New Zealand, (7)University of Maryland Baltimore County, Baltimore, MD, United States, (8)Southwest Research Institute, Boulder, CO, United States, (9)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (10)University of California Los Angeles, Los Angeles, CA, United States, (11)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (12)Smithsonian Astrophysical Observatory, Cambridge, MA, United States
 
Fe XII and Fe XIII Line Widths in a Southern Coronal Hole up to 1.5 Solar Radii (695189)
Yingjie Zhu, University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, Judit Szente, University of Michigan Ann Arbor, Ann Arbor, MI, United States and Enrico Landi, University of Michigan, Ann Arbor, MI, United States
 
Sensitivity of Solar Wind Mass Flux to Coronal Electron Temperature (696332)
David Stansby, University College London, Mullard Space Science Laboratory, London, United Kingdom, Laura Bercic, LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, Meudon, France, Lorenzo Matteini, Imperial College London, Department of Physics, London, United Kingdom, Christopher John Owen, University College London, Mullard Space Science Laboratory, Dorking, United Kingdom, Ryan French, UCL - Mullard Space Science Laboratory, Dorking, United Kingdom, Deborah Baker, University College London, London, United Kingdom and Samuel Timothy Badman, University of California Berkeley, Berkeley, CA, United States
 
Nonequilibrium properties in the plasma sheet observed on 2017 September 10 (698089)
Jin-Yi Lee, Kyung Hee University, Yongin, Korea, Republic of (South), John Raymond, Harvard Smithsonian Center for Astrophysics, Cambridge, MA, United States, Katharine Reeves, Smithsonian Institution, Cambridge, MA, United States, Chengcai Shen, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, Yuan-Kuen Ko, Naval Research Laboratory, Washington, DC, United States, Stephen W Kahler, Kirtland AFB, Albuquerque, NM, United States, Yong-Jae Moon, School of Space Research, Kyung Hee University, Yongin, South Korea and Yeon-Han Kim, Korea Ast. & Sp. Sci. Ins., Daejeon, Korea, Republic of (South)
 
Study of the relationship between the observations of electron distribution in the solar wind and interplanetary magnetic field fluctuations (701304)
Javier Silva, University of Chile, Department of Physics, Faculty of Sciences, Santiago, Chile, Pablo S Moya, University of Chile, Santiago, Chile and Adolfo F Viñas, NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States
 
Simulating Solar Maximum Conditions with the Alfven Wave Solar Atmosphere Model (AWSoM) (704040)
Nishtha Sachdeva1, Bart van der Holst2, Gabor Toth3, Ward Manchester2 and Igor Sokolov4, (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)University of Michigan, Department of Climate and Space, Center for Space Environment Modeling, Ann Arbor, MI, United States, (4)University of Michigan, Ann Arbor, MI, United States
 
Examining Some Properties of the Magnetic and Plasma Structure of the Solar Wind (706462)
Joseph Borovsky, Space Science Institute Los Alamos, Los Alamos, NM, United States
 
In-Situ Switchback Formation in the Expanding Solar Wind (715720)
Jonathan Squire1, Benjamin D G Chandran2 and Romain Meyrand1, (1)University of Otago, Dunedin, New Zealand, (2)University of New Hampshire, Durham, NH, United States
 
Analysis of time-domain correlations between EUV and in-situ observations of coronal jets (727384)
Diego de Pablos, University College London, Mullard Space Science Laboratory, Guildford, United Kingdom, Christopher John Owen, University College London, Mullard Space Science Laboratory, Dorking, United Kingdom, David Long, University College London, London, United Kingdom, Louise K Harra, Physikalisch-Meteorologisches Observatorium Davos, World Radiation Center, Davos Dorf, Switzerland, Gherardo Valori, Mullard Space Science Laboratory, Surrey, United Kingdom and Georgios Nicolaou, UTSA, Rymdcampus, San Antonio, TX, United States
 
SunRISE Mission Implementation (740723)
Andrew Romero-Wolf, NASA Jet Propulsion Laboratory, Pasadena, CA, United States, Justin Christophe Kasper, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, Joseph Lazio, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, James P Lux, Jet Propulsion Laboratory, Pasadena, United States, Tim L. Neilsen, Space Dynamics Laboratory, North Logan, UT, United States and SunRISE Science Team
 
Electric Fields, Currents, and Magnetic Fluctuations of the Photosphere and Solar Wind (747073)
Charles Fred Driscoll, University of California San Diego, Physics, La Jolla, CA, United States
 
A Kinetic Plasma Rosetta Stone for Understanding Plasma Heating and Particle Acceleration in Space and Astrophysical Plasmas (749686)
Gregory G Howes1, Andrew J McCubbin1, Sarah A Horvath1, Peter Montag1, Collin R Brown1, Jimmy Juno2, Kristopher G. Klein3, Jason M TenBarge4 and James W R Schroeder5, (1)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (2)University of Maryland College Park, College Park, MD, United States, (3)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (4)Princeton University, Princeton, NJ, United States, (5)Wheaton College, Physics, Norton, IL, United States
 
Statistical Analysis of Orientation, Shape and Size of Switchbacks (750932)
Ronan Laker1, Timothy Simon Horbury1, Stuart D Bale2,3, Lorenzo Matteini3, Thomas Woolley3, Lloyd David Woodham4, Samuel Timothy Badman5, Marc Pulupa6, Justin Christophe Kasper7, Michael Louis Stevens8, Anthony W Case8 and Kelly E Korreck8, (1)Imperial College London, Department of Physics, London, SW7, United Kingdom, (2)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)Imperial College London, Department of Physics, London, United Kingdom, (4)University College London, Mullard Space Science Laboratory, London, United Kingdom, (5)University of Oxford, Oxford, United Kingdom, (6)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (7)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (8)Smithsonian Astrophysical Observatory, Cambridge, MA, United States
 
Hybrid simulations of large-amplitude Alfvénic fluctuations: the role of parametric instabilities in proton heating and acceleration (755066)
Carlos Gonzalez, University of Texas at Austin, Department of physics, Austin, TX, United States, Anna Tenerani, University of Texas, Austin, TX, United States, Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States and Petr Hellinger, Astronomical Institute, CAS, Ondrejov/Prague, Czech Republic
 
Sources and Evolution of the Solar Wind Seen by Parker Solar Probe (756514)
Olga Panasenco1, Marco C M Velli2, Chen Shi3, Anna Tenerani4, Victor Réville5, Samuel Timothy Badman6, Stuart D Bale7, Raffaella D'Amicis8, Keith Goetz9, Peter Harvey10, Kelly E Korreck11, Davin E Larson12, Robert J MacDowall13, Marc Pulupa14, Jasper S Halekas15, Michael B Stevens11, Roberto Livi14 and Phyllis L Whittlesey14, (1)Advanced Heliophysics, Pasadena, CA, United States, (2)University of California Los Angeles, Los Angeles, CA, United States, (3)University of California Los Angeles, Earth, Planetary and Space Sciences, Los Angeles, CA, United States, (4)University of Texas, Austin, TX, United States, (5)IRAP, Toulouse, France, (6)University of California Berkeley, Berkeley, CA, United States, (7)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (8)INAF-IAPS, Rome, Italy, (9)University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States, (10)Space Sciences Laboratory, Berkeley, United States, (11)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (12)Space Sciences Laboratory, Berkeley, CA, United States, (13)NASA/Goddard Space Flight Center, Greenbelt, United States, (14)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (15)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States
 
Electron Heating in the Solar Wind (756973)
Stas Boldyrev, Cary Forest and Jan Egedal, University of Wisconsin Madison, Madison, WI, United States
 
Comparing the best ADAPT realizations from WSA, AWSoM and AWSoM-R (759356)
Zhenguang Huang1, Igor Sokolov2, Bart van der Holst3, Gabor Toth4, Charles Nickolos Arge5, Nishtha Sachdeva3, Shaela I Jones5, Ward Manchester3 and Tamas I Gombosi4, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Michigan, Ann Arbor, MI, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (4)University of Michigan, Department of Climate and Space, Center for Space Environment Modeling, Ann Arbor, MI, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Comparing Parker Solar Probe observations with theory and simulations of reflection-driven Alfven turbulence (762277)
Jarrod Bianco1, Jean Carlos Perez2, Benjamin D G Chandran3 and Sofiane Bourouaine2, (1)Florida Institute of Technology, Melbourne, FL, United States, (2)Florida Institute of Technology, Aerospace, Physics and Space Sciences, Melbourne, FL, United States, (3)University of New Hampshire, Durham, NH, United States
 
Field-Particle Correlation Signatures of Magnetic Pumping (765139)
Peter Montag, University of Iowa, Physics and Astronomy, Iowa City, IA, United States and Gregory G Howes, Department of Physics and Astronomy, University of Iowa, Iowa City, IA, United States
 
Total eclipse spectroscopy of visible light coronal emission lines (775955)
Gabriel Domingo Muro, Aberystwyth University, Aberystwyth, SY23, United Kingdom and Huw Morgan, Aberystwyth University, Aberystwyth, United Kingdom
 
Stellar Rotation Effects on Stellar winds (776681)
Bhimsen Shivamoggi, University of Central Florida, Orlando, FL, United States