SH21A:
Fundamental Physics of the Solar Corona and Inner Heliosphere III Posters


Session ID#: 8813

Session Description:
The solar corona and solar wind provide a complex laboratory where magnetic fields guide and energize the plasma. Structured over an incredibly wide range of time and spatial scales, the coronal plasma is heated and accelerated to give the turbulent, super-Alfvénic wind observed in the heliosphere. This session is open to exploring the many facets of the physical processes involved in heliospheric origins: from the sources of different wind types and their connection to coronal structures, to the micro-physics of distribution functions, anisotropies, to the role of turbulence and wave-particle interactions in heating and acceleration, to the energization associated with structures, such as shocks, current sheets and magnetic reconnection. What specific observables can be derived from models, what fundamental observations should drive theoretical developments, in preparation for the decade of inner heliospheric and coronal exploration with Solar Orbiter and Solar Probe Plus? Solicited contributions include theoretical, numerical simulation, and observational papers.
Primary Convener:  Chadi S Salem, University of California Berkeley, Berkeley, CA, United States
Conveners:  Dr. Olga Panasenco, Advanced Heliophysics Inc., Pasadena, United States and Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States
Chairs:  Chadi S Salem, University of California Berkeley, Berkeley, CA, United States and Dr. Olga Panasenco, Advanced Heliophysics Inc., Pasadena, United States
OSPA Liaison:  Dr. Olga Panasenco, Advanced Heliophysics Inc., Pasadena, United States
Index Terms:

2164 Solar wind plasma [INTERPLANETARY PHYSICS]
2169 Solar wind sources [INTERPLANETARY PHYSICS]
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]

Abstracts Submitted to this Session:

Michael Hahn and Daniel Wolf Savin, Columbia University, New York, United States
Oliver Allanson, University of St Andrews, School of Mathematics & Statistics, St Andrews, United Kingdom, Thomas Neukirch, University of St Andrews, St Andrews, KY16, United Kingdom, Fiona Wilson, University of St Andrews, St Andrews, United Kingdom and Sascha Troscheit, University of Waterloo, Department of Pure Mathematics, Waterloo, ON, Canada
Daniel Verscharen, University of New Hampshire Main Campus, Durham, United States and Benjamin D G Chandran, University of New Hampshire Main Campus, Durham, NH, United States
Cecilia Mac Cormack1, Bart van der Holst2, Federico A Nuevo3,4, Alberto M Vásquez3,5, Marcelo Lopez-Fuentes3, Richard A Frazin2, Enrico Landi2 and Cristina H Mandrini3,4, (1)Catholic University of America. NASA Goddard Space Flight Center, Greenbelt, United States, (2)University of Michigan Ann Arbor, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (3)Instituto de Astronomía y Física del Espacio, Buenos Aires, Argentina, (4)University of Buenos Aires, Physics, Buenos Aires, Argentina, (5)National University of Tres de Febrero, Department of Science and Technology, Buenos Aires, Argentina
Diego Gustavo Lloveras1, Bart van der Holst2, Alberto M Vásquez3,4, Federico Nuevo3 and Richard A Frazin2, (1)University of Buenos Aires, Physics, Buenos Aires, Argentina, (2)University of Michigan Ann Arbor, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (3)Instituto de Astronomía y Física del Espacio, Buenos Aires, Argentina, (4)National University of Tres de Febrero, Department of Science and Technology, Buenos Aires, Argentina
Christopher H K Chen, Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
David Tsiklauri, Queen Mary, University of London, London, United Kingdom and Jonathan O. Thurgood, Northumbria University, Department of Mathematics and Information Sciences, Newcastle-Upon-Tyne, United Kingdom
Patrick Tracy1, Justin Christophe Kasper2, Thomas Zurbuchen1, Jim M Raines2 and Jason A Gilbert2, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
Benjamin L. Alterman1, Justin Christophe Kasper2, Michael Louis Stevens3, Adam Szabo4 and Andriy Koval4, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (3)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (4)NASA Goddard Space Flight Center, Greenbelt, MD, United States
Benjamin Alcock1, Eduard Kontar1 and Neus Agueda2, (1)University of Glasgow, Glasgow, G12, United Kingdom, (2)University of Barcelona, Barcelona, Spain
Jenny Marcela Rodríguez, Luis Vieira, Alisson Dal Lago, Tardelli Ronan Coelho Stekel, Joaquim E R Costa and Tereza S. N. Pinto, National Institute for Space Research (INPE), São José dos Campos - SP, Brazil
Yasuhiro Nariyuki and Jungjoon Seough, University of Toyama, Toyama, Japan
Nigang Liu, CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China, Hefei, China
Nicholas Bradley McGreivy1, Marc Swisdak1, James Frederick Drake1 and Stephen Peter Gary2, (1)University of Maryland College Park, College Park, MD, United States, (2)Los Alamos National Laboratory, Los Alamos, NM, United States
Mark Stakhiv, University of Michigan Ann Arbor, Ann Arbor, MI, United States, Susan T Lepri, University of Michigan, Ann Arbor, United States and Enrico Landi, University of Michigan Ann Arbor, Departament of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
Thejappa Golla, University of Maryland College Park, College Park, MD, United States and Robert J. MacDowall, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Peter Fraser Wyper, University of Durham, Durham, United Kingdom, C Richard DeVore, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Judith T Karpen, NASA Goddard Space Flight Center, Code 674, Greenbelt, MD, United States
Mark L Adrian1, Adolfo F. Vinas2, Pablo S Moya3 and Deirdre E Wendel2, (1)Auburn University, Physics Department, Auburn, AL, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)NASA Goddard Space Flight Center, Heliophysics Division, Geospace Physics Laboratory, Mail Code 673, Greenbelt, MD, United States
Daniele Del Sarto, University of Lorraine Nancy, Institut Jean Lamour UMR 7198 CNRS, Nancy Cedex, France, Francesco Pegoraro, University of Pisa, Physics Department, Pisa, Italy, Francesco Califano, University of Pisa, Pisa, Italy and Anna Tenerani, University of Texas at Austin, Austin, TX, United States
Manan Kocher1, Susan T Lepri2, Enrico Landi3 and Liang Zhao2, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Michigan, Ann Arbor, United States, (3)University of Michigan Ann Arbor, Departament of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
Yi-Min Huang1, Amitava Bhattacharjee1, Lijia Guo2 and Davina Innes3, (1)Princeton University, Princeton, NJ, United States, (2)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (3)JHU / APL, Laurel, MD, United States