SH012
Fundamental Physics of the Solar Corona and Inner Heliosphere

Session ID#: 157259

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: How do magnetic structure and local processes at the sources in the solar atmosphere determine different wind types? How do distribution functions evolve, from the thermal population to energetic particle acceleration? What are the roles of turbulence and wave-particle interactions in heating and acceleration of the solar corona and wind? How is the energization associated with structures, such as switchbacks, shocks, compression regions, current sheets and magnetic reconnection?

Now in its eighth year, this session welcomes theoretical, numerical simulation, and observational papers, including contributions stemming from Parker Solar Probe, Solar Orbiter, BepiColombo and the whole Heliophysics System Observatory, as well as developments and new challenges inspired by such observations.

Index Terms:

2159 Plasma waves and turbulence [INTERPLANETARY PHYSICS]
2164 Solar wind plasma [INTERPLANETARY PHYSICS]
2169 Solar wind sources [INTERPLANETARY PHYSICS]
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]


Primary Convener:  Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States
Conveners:  Chadi S Salem, University of California, Berkeley, CA, United States, Olga Panasenco, Advanced Heliophysics Inc., Pasadena, United States and Yannis Zouganelis, European Space Agency, Villanueva De La Can, Spain
Student/Early Career Convener:  Chen Shi, University of California, Los Angeles, Los Angeles, United States
 
Radial Evolution and Acceleration of the Solar Wind (Invited) (1049081)
Jasper S Halekas1, Phyllis L Whittlesey2, Davin E Larson3, Milan Maksimovic4, Roberto Livi2, Matthieu Berthomier5, Justin Christophe Kasper6, Anthony W Case7, Michael Louis Stevens7, Stuart D Bale8, Robert J MacDowall9 and Marc Pulupa10, (1)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (2)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (3)Space Sciences Laboratory, Berkeley, United States, (4)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, (5)LPP, Ecole Polytechnique, UPMC, Paris, France, (6)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (7)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (8)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (9)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (10)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States
 
Dispersive and kinetic effects at switchbacks boundaries (Invited) (1050381)
Anna Tenerani1, Carlos A Gonzalez1, Lorenzo Matteini2, Chen Shi3 and Marco C M Velli4, (1)University of Texas at Austin, Austin, United States, (2)Imperial College London, Department of Physics, London, United Kingdom, (3)University of California, Los Angeles, Los Angeles, United States, (4)Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States
 
What Produces the Transition Region of the Quiet Sun? (1051692)
Paul Song, University of Massachusetts Lowell, Lowell, MA, United States and Jiannan Tu, Space Science Laboratory, Lowell, MA, United States
 
Overview and Classification of Solar Wind Instabilities in the Inner Heliosphere (1057017)
Mihailo Martinović, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, Kristopher G Klein, University of Arizona, Tucson, AZ, United States, Tereza Durovcova, Charles University, Prague, Czech Republic and Ben Alterman, Southwest Research Institute, San Antonio, United States
 
Association of intermittency with electron heating in the near-Sun solar wind (1059802)
Camryn Phillips, Princeton, New Jersey, UNITED STATES, Riddhi Bandyopadhyay, Princeton University, Department of Astrophysics, Princeton, NJ, United States, David J McComas, Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States and Stuart D Bale, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
 
A Self-Consistent Kinetic Model of the Solar Wind (1062738)
Patrick Kilian, Space Science Institute Boulder, Boulder, CO, United States, Vadim Roytershteyn, Space Science Institute, Boulder, NM, United States and Jack D Scudder, Space Science Institute, Boulder, United States
 
X-ray heating of the quiescent solar corona (1065389)
Vishal Upendran1, Durgesh Tripathi1, N. P. S. Mithun2, Santosh V Vadawale2 and Aveek Sarkar2, (1)Inter University Centre for Astronomy and Astrophysics (IUCAA), Pune, India, (2)Physical Research Laboratory, Ahmedabad, India
 
Spontaneous Generation of Alfvén Waves during three-dimensional Magnetic Reconnection in the Solar Corona (1070489)
Liping Yang1, Jiansen He2, Xueshang Feng3, Fan Guo4 and Hui Li4, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)Peking University, Beijing, China, (3)National Space Science Center, Beijing, China, (4)Los Alamos National Lab, Los Alamos, NM, United States
 
A two-fluid slow solar wind model with proton temperature anisotropy and Alfven-wave turbulence (1070657)
Hwanhee Lee1, Jungjoon Seough2, Bo Li3, Yeon-Han Kim4 and Kyung-Suk F Cho4, (1)KASI Korea Astronomy and Space Science Institute, Space Weather Research Group, Daejeon, Korea, Republic of (South), (2)KASI Korea Astronomy and Space Science Institute, Daejeon, Korea, Republic of (South), (3)Shandong University at Weihai, Weihai, China, (4)KASI Korea Astronomy and Space Science Institute, Space Weather Research Group, Daejeon, South Korea
 
What Alpha to Proton Ratio Variations During Periodic Mesoscale Solar Wind Structures Tell Us About Solar Wind Plasma Release. (1072395)
Larry Kepko, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Nicholeen M Viall, NASA GSFC, Greenbelt, MD, United States
 
The Baseline Solar Wind (1073865)
Milan Maksimovic, CNRS, Paris Cedex 16, France, Dakeyo Jean-Baptiste, LESIA, Observatoire de Paris, Meudon, France, Stuart D Bale, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, Pascal Demoulin, LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, Jasper S Halekas, University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States and Yannis Zouganelis, European Space Agency, Villanueva De La Can, Spain
 
Interchange reconnection within coronal holes powers the fast solarwind: Suprathermal ion flows and bursty magnetic fields modulated by the network magnetic field. (1076938)
Stuart D Bale, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, James Frederick Drake, University of Maryland College Park, College Park, MD, United States, Michael McManus, SSL/UC Berkeley, Berkely, United States, Mihir Indrajit Desai, Southwest Research Institute, San Antonio, United States, Davin E Larson, Space Sciences Laboratory, Berkeley, United States, Marc Swisdak, University of Maryland, College Park, United States, Nour E. Raouafi, Johns Hopkins University, Baltimore, United States, Samuel Timothy Badman, University of Oxford, Oxford, United Kingdom, Tai D. Phan, SSL, Berkeley, Berkeley, United States, Marco C M Velli, Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, David J McComas, Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, Christina Cohen, Caltech, Pasadena, United States, Donald G Mitchell, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Justin Christophe Kasper, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States
 
Expansion and Size Effects on Switchback Stability in 3D (1078924)
Maile Marriott, University of Texas at Austin, Austin, TX, United States and Anna Tenerani, University of Texas at Austin, Austin, United States
 
Statistical Analysis of Whistler Waves in Pristine Solar Wind at 1 AU (1079796)
Yutong Du, University of California Berkeley, Physics, Berkeley, United States, Ivan Vasko, Space Science Lab, UC berkeley, Berkeley, United States, Anton Artemyev, University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, United States and Forrest Mozer, University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
 
Signatures of Quasilinear Cyclotron Resonance in the Inner Heliosphere (1085052)
Trevor Bowen1, Benjamin D G Chandran2, Jonathan Squire3, Michael McManus4, Davin Larson1, Stuart D Bale5, Jaye Verniero6, Kristopher G Klein7 and Alfred Mallet8, (1)University of California Berkeley, Berkeley, CA, United States, (2)University of New Hampshire, Durham, NH, United States, (3)University of Otago, Dunedin, New Zealand, (4)SSL/UC Berkeley, Berkely, United States, (5)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (6)NASA/GSFC, Greenbelt, United States, (7)University of Arizona, Tucson, AZ, United States, (8)University of California, Berkeley, Space Sciences Laboratory, Berkeley, United States
 
Theoretical prediction of ion scale waves observed in the inner heliosphere (1085135)
Jungjoon Seough, KASI Korea Astronomy and Space Science Institute, Daejeon, Korea, Republic of (South), Peter H Yoon, Univ Maryland, College Park, MD, United States and Yasuhiro Nariyuki, University of Toyama, Toyama, Japan
 
Modeling magnetic switchbacks (1085868)
Bahaeddine Gannouni1, Victor Réville1, Alexis P Rouillard1 and Kévin Dalmasse2, (1)Université Toulouse III - Paul Sabatier, Observatoire Midi–Pyrénées, CNRS, CNES, IRAP, Toulouse, France, (2)University of Toulouse, Toulouse, France
 
Results from Coronal Sounding Experiments Conducted by Indian Mars Orbiter Mission (MOM) during Mars-Solar Conjunctions of 2015 and 2021 (1086235)
Richa Naja Jain1, R. K. Choudhary2, Anil Bhardwaj3, Umang Parikh4, Bijoy K. Dai4 and Roopa M.V.4, (1)Space Physics Laboratory, Vikram Sarabhai Space Center, Trivandrum, India, (2)Space Physics Laboratory, Trivandrum, India, (3)Physical Research Laboratory, Ahmedabad, India, (4)Indian Space Research Organization Satellite center, Bangalore, India
 
Switchbacks, microstreams and broadband turbulence in the solar wind (1087942)
Timothy Simon Horbury1, Stuart D Bale2, Ronan Laker1, Lorenzo Matteini3, Lloyd David Woodham4, Thomas Woolley1, Davin E Larson5, Michael McManus6, Nour E. Raouafi7, Marco C M Velli8, Stefano A Livi9, Andrei Fedorov10, Philippe Louarn10, Christopher John Owen11 and Justin Christophe Kasper12, (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)Imperial College, London, United Kingdom, (5)Space Sciences Laboratory, Berkeley, United States, (6)SSL/UC Berkeley, Berkely, United States, (7)Johns Hopkins University, Baltimore, United States, (8)Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, (9)SwRI, San Antonio, TX, United States, (10)IRAP, CNRS, Toulouse, France, (11)University College London, Mullard Space Science Laboratory, Dorking, United Kingdom, (12)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States
 
Implication of line tied magnetic field on magnetic reconnection in the closed corona (1088295)
Lars K. S. Daldorff, Catholic University of America, Washington, DC, United States, James Edward Leake, US Naval Research Laboratory, Washington, United States and James A Klimchuk, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Propagation and Evolution of MHD Waves in Fast and Slow Solar Wind in Inner Heliosphere (1089543)
Jiansen He1, Liping Yang2, Die Duan2, Xingyu Zhu2 and Chuanpeng Hou2, (1)Peking University, School of Earth and Space Sciences, Beijing, China, (2)Peking University, Beijing, China
 
What drives the formation of the solar wind from coronal streamers? (1089939)
Samantha Wallace, NASA Postdoctoral Program / GSFC, Greenbelt, United States, Nicholeen M Viall, NASA GSFC, Greenbelt, MD, United States, Charles Nickolos Arge, NASA Goddard Space Flight Center, Greenbelt, United States and Aleida Katherine Higginson, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
The Response of the Corona and of the Heliosphere to Realistic Photospheric Magnetic Flux Evolution (1092548)
Roberto Lionello1, Cooper Downs1, Jon Linker1, Emily Irene Mason2, Pete Riley3, Viacheslav S. Titov1, Ronald M. Caplan1 and Marc L DeRosa4, (1)Predictive Science Inc., San Diego, CA, United States, (2)Predictive Science Inc., San Diego, United States, (3)Predictive Science, Inc., San Diego, United States, (4)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
 
Kinetic Model of Fast Solar Wind Generation and Heating by Kinetic Alfvén Wave Turbulence (1092803)
Philip A Isenberg, University of New Hampshire, Durham, United States and Bernard John Vasquez, University of New Hampshire, Durham, NH, United States
 
Parametric Instability of Alfvén Waves with Electron Landau-Fluid Closure (1095655)
Simon Lautenbach, Carlos A Gonzalez and Anna Tenerani, University of Texas at Austin, Austin, United States
 
Physics of the Solar Transition Region (1096033)
Spiro K Antiochos, University of Michigan Ann Arbor, Ann Arbor, United States, Costis Gontikakis, RCAAM of the Academy of Athens, Athens, Greece and Peter R Young, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Interchange Reconnection within Coronal Holes Powers the Fast Solar Wind: Connecting Parker Solar Probe Observations and Simulations to Coronal Reconnection Dynamics (1097006)
James Frederick Drake, University of Maryland College Park, College Park, MD, United States, Stuart D Bale, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, Michael McManus, SSL/UC Berkeley, Berkely, United States, Mihir Indrajit Desai, Southwest Research Institute, San Antonio, United States, Davin E Larson, Space Sciences Laboratory, Berkeley, United States, Marc Swisdak, University of Maryland, College Park, United States, Nour E. Raouafi, Johns Hopkins University, Baltimore, United States, Samuel Timothy Badman, University of Oxford, Oxford, United Kingdom, Tai D. Phan, SSL, Berkeley, Berkeley, United States, Marco C M Velli, Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, David J McComas, Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, Christina Cohen, Caltech, Pasadena, United States, Donald G Mitchell, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Olga Panasenco, Advanced Heliophysics Inc., Pasadena, United States and Justin Christophe Kasper, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States
 
Evolution of Lower Frequency Breaks of Alfvenic Turbulence in the Inner Heliosphere, Observed by Parker Solar Probe and Solar Orbiter (1103189)
Zesen Huang1, Nikos Sioulas2, Chen Shi2, Marco C M Velli3 and Anna Tenerani4, (1)University of California Los Angeles, Los Angeles, CA, United States, (2)University of California, Los Angeles, Los Angeles, United States, (3)Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, (4)University of Texas at Austin, Austin, United States
 
Investigating the Effect of Source Terms in the Corona with COCONUT (1104700)
Tinatin Baratashvili1, Barbara Perri2, Michaela Brchnelova3, Andrea Lani3 and Stefaan Poedts4, (1)Katholieke Universiteit Leuven, Leuven, Belgium, (2)KU Leuven, Leuven, Belgium, (3)KU Leuven, Centre for mathematical Plasma-Astrophysics, Department of Mathematics, Leuven, Belgium, (4)KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium
 
The interplay between magnetic switchbacks and solar wind turbulence in the inner Heliosphere (1105860)
Andrea Larosa, Queen Mary, University of London, School of Physics and Astronomy, London, United Kingdom and Christopher H K Chen, Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
 
On Magnetic Clouds Associated with Hot Magnetic Flux Ropes and Filament Flux Ropes (1108226)
Hong Xie1, Nat Gopalswamy2, Sachiko Akiyama3, Seiji Yashiro4 and Pertti Makela1, (1)Catholic University of America, Washington, DC, United States, (2)NASA Goddard SFC, Greenbelt, MD, United States, (3)NASA/GSFC, Grrenbelt, MD, United States, (4)Catholic University of America, Washington DC, United States
 
Hydrodynamic Modeling of Quiet-Sun Coronal Loops (1109182)
Cecilia Mac Cormack1, Marcelo Lopez-Fuentes1, Cristina H Mandrini1, Diego Lloveras1, Alberto M Vásquez2 and Teresa Nieves-Chinchilla3, (1)Instituto de Astronomía y Física del Espacio, Buenos Aires, Argentina, (2)Instituto de Astronoma y Fsica del Espacio, Buenos Aires, Argentina, (3)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States
 
Parker Solar Probe Observations of Turbulence in the Near-Sun Solar Wind and Solar Corona (1117101)
Christopher H K Chen, Queen Mary University of London, London, United Kingdom and PSP FIELDS & SWEAP Teams
 
Magnetic field spectral evolution in the inner heliosphere: from Parker Solar Probe to Solar Orbiter. (1125000)
Nikos Sioulas1, Zesen Huang1, Chen Shi2, Marco C M Velli3, Anna Tenerani4 and FIELDS, SPC & SPAN Teams PSP, SWA & MAG Teams SolO, (1)University of California Los Angeles, Los Angeles, CA, United States, (2)University of California, Los Angeles, Los Angeles, United States, (3)Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, (4)University of Texas at Austin, Austin, United States
 
Statistical Analysis of the Radial Evolution of the Solar Winds between 0.1 and 1 au, and their Semi-empirical Iso-poly Fluid Modeling (1125087)
Jean-Baptiste Dakeyo1, Milan Maksimovic2, Pascal Demoulin2, Jasper S Halekas3 and Michael Louis Stevens4, (1)IRAP, Observatoire Midi-Pyrénées, LESIA, Observatoire de Paris, CNRS, Chaville, France, (2)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, (3)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (4)Smithsonian Astrophysical Observatory, Cambridge, MA, United States
 
Properties of Alfvénic Switchbacks in the Expanding Solar Wind: Three-dimensional Numerical Simulations (1126120)
Zade Johnston1, Jonathan Squire1, Alfred Mallet2 and Romain Meyrand1, (1)University of Otago, Dunedin, New Zealand, (2)University of California Berkeley, Berkeley, CA, United States
 
Properties of the Corona and Inner Heliosphere with Multi-instrument Observations of Pseudostreamers and Helmet-Streamers (1134570)
Mari Paz Miralles, Center for Astrophysics | Harvard & Smithsonian, Cambridge, United States and Steven R Cranmer, University of Colorado, Boulder, CO, United States
 
A fragmented and extended Alfven critical zone in the young solar wind (1138293)
William H Matthaeus1, Rohit Chhiber1, Arcadi V. Usmanov1, Riddhi Bandyopadhyay2, Melvyn L Goldstein3 and Steven R Cranmer4, (1)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (2)Princeton University, Department of Astrophysics, Princeton, NJ, United States, (3)University of Maryland Baltimore County, Baltimore, MD, United States, (4)University of Colorado, Boulder, CO, United States
 
Fe Ion Heating Across a Shock Observed by Solar Orbiter’s Heavy Ion Sensor (1138976)
B L L Alterman1, Stefano A Livi2, Susan T Lepri3, Jim M Raines3, Ryan M. Dewey4, Christopher John Owen5, Sarah A. Spitzer6, Domenico Trotta7, Philippe Louarn8, Roberto Bruno9, Andrei Fedorov8, George C Ho10, Antoinette Broe Galvin11, Frederic Allegrini12, Keiichi Ogasawara1, Peter Wurz13, Yeimy Rivera4, Christopher Mark Bert4, Timothy Simon Horbury14, Kylie Sullivan15, Heli Hietala16, Milan Maksimovic17, Andrew P Dimmock18, Yuri Khotyaintsev19, Virginia Angelini20, Ed Fauchon-Jones21 and Lynn M Kistler22, (1)Southwest Research Institute, San Antonio, TX, United States, (2)SwRI, San Antonio, TX, United States, (3)University of Michigan, Ann Arbor, MI, United States, (4)University of Michigan, Ann Arbor, United States, (5)University College London, Mullard Space Science Laboratory, Dorking, United Kingdom, (6)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (7)Imperial College London, Department of Physics, The Blackett Laboratory, London, United Kingdom, (8)IRAP, CNRS, Toulouse, France, (9)IAPS-INAF, Rome, Italy, (10)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (11)Univ of New Hampshire, Durham, NH, United States, (12)Southwest Research Institute San Antonio, San Antonio, TX, United States, (13)University of Bern, Physics Institute, Space Research and Planetary Sciences, Bern, Switzerland, (14)Imperial College London, Department of Physics, London, SW7, United Kingdom, (15)Southwest Research Institute, San Antonio, United States, (16)Queen Mary University of London, London, United Kingdom, (17)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, (18)Aalto University, Aalto, Finland, (19)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (20)Imperial College London, Department of Physics, London, United Kingdom, (21)Imperial College London, London, United Kingdom, (22)Univ New Hampshire, Durham, NH, United States
 
Assessing the formation of CME sheaths via the interaction of solar wind fluctuations with the ejecta (1143224)
Chaitanya Prasad Sishtla1, Jens Pomoell1, K Emilia J Kilpua2, Simon Good2 and Rami O Vainio3, (1)University of Helsinki, Helsinki, Finland, (2)University of Helsinki, Department of Physics, Helsinki, Finland, (3)Univ Helsinki, Helsinki, Finland
 
Reflection-driven turbulence in the super-Alfvénic solar wind (1144225)
Romain Meyrand1, Jonathan Squire1 and Alfred Mallet2, (1)University of Otago, Dunedin, New Zealand, (2)University of California Berkeley, Berkeley, CA, United States
 
A Study of Tearing Instability Onset with Particle In Cell Simulations (1145473)
Maria Elena Innocenti1, Fulvia Pucci1,2, Elisabetta Boella3, Anna Tenerani4 and Jeremy Dargent1, (1)Ruhr University Bochum, Bochum, Germany, (2)Jet Propulsion Laboratory, Pasadena, United States, (3)Lancaster University, Physics Department, Lancaster, United Kingdom, (4)University of Texas at Austin, Austin, United States
 
EUV Diagnostics of the Kappa-Distribution in the Solar Corona Using KAPPA Package (1151230)
Elena Dzifcakova1, Jaroslav Dudík1, Juraj Lorincik2, Giulio Del Zanna3 and Alena Zemanova4, (1)Astronomical Institute of the Academy of Sciences, Prague, United States, (2)Bay Area Environmental Research Institute Moffett Field, Moffett Field, United States, (3)University of Cambridge, DAMTP, Cambridge, United Kingdom, (4)Astronomical Institute of the Academy of Sciences, Department of Solar Physics, Ondřejov, Czech Republic
 
Local proton heating at different magnetic discontinuities in the solar wind (1160097)
Carlos Gonzalez, University of Texas at Austin, Department of physics, Austin, TX, United States and Anna Tenerani, University of Texas at Austin, Austin, United States
 
The Near-Sun Turbulence Mediated by Parametric Decaying Instability of Alfvén Waves (1161309)
Zhaoming Gan1, Xiangrong Fu1, Hui Li2 and Senbei Du3, (1)New Mexico Consortium, Los Alamos, United States, (2)Los Alamos National Lab, Los Alamos, NM, United States, (3)Los Alamos National Laboratory, Los Alamos, United States
 
The Role of Drift Waves in Solar Plasma (1168677)
Michaela Brchnelova, Katholieke Universiteit Leuven, Leuven, Belgium and Stefaan Poedts, KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium
 
Understanding the Kinetic Physics of Particle Energization at Quasiperpendicular Collisionless Shocks Using the Field-Particle Correlation Technique (1172673)
Gregory G Howes1, Jimmy Juno2, Collin R Brown1, Colby C Haggerty3, Sage Constantinou4, Jason M TenBarge5, Damiano Caprioli6, Anatoly Spitkovsky7 and Lynn B Wilson III8, (1)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (2)Princeton Plasma Physics Laboratory, Princeton, United States, (3)University of Hawaii at Manoa, Astronomy, Honolulu, United States, (4)Institute for Astronomy, Honolulu, HI, United States, (5)Princeton University, Princeton, NJ, United States, (6)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (7)Princeton University, Astrophysical Sciences, Princeton, NJ, United States, (8)NASA Goddard Space Flight Center, Greenbelt, United States
 
Identifying Waves in the Solar Wind Using Convolutional Neural Networks (1174100)
Samuel Fordin, University of Delaware, Newark, DE, United States, Michael A Shay, Department of Physics and Astronomy, University of Delaware, Newark, United States, Lynn B Wilson III, NASA Goddard Space Flight Center, Greenbelt, United States and Barbara J Thompson, NASA/GSFC, Greenbelt, MD, United States
 
Acceleration and heating of solar wind: polytropic solar wind model and role of Alfvén waves (1174410)
Chen Shi, University of California Los Angeles, Earth, Planetary and Space Sciences, Los Angeles, CA, United States, Marco C M Velli, Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, Nikos Sioulas, University of California, Los Angeles, Los Angeles, United States, Zesen Huang, University of Science and Technology of China, Hefei, Anhui, China and Anna Tenerani, University of Texas at Austin, Austin, United States
 
Frustrated Relaxation And Instabilities In Solar Coronal Magnetic Fields: From Coronal Structure to Solar Wind Acceleration (1177251)
Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States and Olga Panasenco, Advanced Heliophysics Inc., Pasadena, United States
 
Multifractal Properties of Intensity Signals in Solar Coronal Holes, Adjacent Quiet Sun, and Boundary Regions in the Context of the Magnetic Network (1179455)
Ana Cristina Cadavid, California State University Northridge, Northridge, CA, United States, Landon Wells, California State University Northridge, Physics and Astronomy, Northridge, United States and Mari Paz Miralles, Center for Astrophysics, Harvard & Smithsonian, Cambridge, United States
 
Switchback formation and evolution through expanding spherically polarized Alfvén waves (1182672)
Jonathan Squire1, Zade Johnston1, Romain Meyrand1 and Alfred Mallet2, (1)University of Otago, Dunedin, New Zealand, (2)University of California, Berkeley, Space Sciences Laboratory, Berkeley, United States
 
A Data-driven MHD Simulation Model for CME Generation and Propagation: Coupling of EULAG MHD with MS-FLUKSS Global Corona Model (1186533)
Mehmet Sarp Yalim1, Avijeet Prasad2, Qiang Hu3 and Nikolai V Pogorelov3, (1)University of Alabama in Huntsville, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States, (2)University of Oslo, Rosseland Center for Solar Physics, Oslo, Norway, (3)University of Alabama in Huntsville, Department of Space Science, Huntsville, United States
 
Modeling the Solar Wind During Different Phases of the Last Solar Cycle (1187182)
Zhenguang Huang1, Gabor Toth2, Nishtha Sachdeva3, Lulu Zhao4, Bart van der Holst3, Igor Sokolov5, Ward Manchester3 and Tamas I Gombosi6, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (4)Florida Institute of Technology, Department of Physics and Space Sciences, Melbourne, United States, (5)University of Michigan, Ann Arbor, MI, United States, (6)University of Michigan, Department of Climate and Space, Center for Space Environment Modeling, Ann Arbor, MI, United States
 
Laboratory Study of Arched Plasma Eruptions in a Sheared Magnetic Field (1193531)
Kamil Sklodowski1, Shreekrishna Tripathi2 and Troy Carter1, (1)University of California Los Angeles, Los Angeles, United States, (2)University of California Los Angeles, Los Angeles, CA, United States
 
Destabilization of Alfvén Waves by a Proton Beam in a Large Magnetized Plasma (1194467)
Shreekrishna Tripathi1, Walter N Gekelman2, Stephen T Vincena1, Patrick Pribyl1 and Troy Carter1, (1)University of California Los Angeles, Los Angeles, CA, United States, (2)University of California Los Angeles, Los Angeles, United States
 
Numerical Modeling of Strahl Electron Transport in the Solar Corona and Solar Wind (1195108)
Bofeng Tang1, Gary Paul Zank2 and Vladimir Kolobov1, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)Univ of Alabama, Huntsville, Huntsville, AL, United States
 
Radial Evolution and Kinetics of Ion Species: Helios Observations (1199545)
Chadi S Salem, University of California Berkeley, Berkeley, CA, United States, Thomas Woolley, Imperial College London, Department of Physics, London, SW7, United Kingdom and Lorenzo Matteini, Imperial College London, Department of Physics, London, United Kingdom
 
Mesoscale Magnetic Structure in the Solar Wind (1199850)
Jesus Gonzalez, University of California Los Angeles, Los Angeles, CA, United States, Stuart Bale, University of California, Berkeley, Berkeley, CA, United States and Marc Pulupa, Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States