SH11B:
Fundamental Physics of the Solar Corona and Inner Heliosphere Posters
Submit an Abstract to this Session
Session ID#: 23804
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 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, SSL, University of California Berkeley, Berkeley, United States
Conveners: Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States, Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States and Prof. William H Matthaeus, University of Delaware, Department of Physics and Astronomy, Newark, DE, United States
Chairs: Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States, Chadi S Salem, University of California, Berkeley, United States, Prof. William H Matthaeus, University of Delaware, Department of Physics and Astronomy, Newark, DE, United States and Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States
OSPA Liaison: Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States
Abstracts Submitted to this Session:
Sofiane Bourouaine, Florida Institute of Technology, Aerospace, Physics and Space Sciences, Melbourne, United States and Jean Carlos Perez, Florida Institute of Technology, Melbourne, FL, United States
Yi-Min Huang1, Amitava Bhattacharjee1 and Amitava Bhattacharjee2, (1)Princeton University, Princeton, NJ, United States, (2)Princeton Plasma Physics Laboratory, Princeton, United States
Carolyn N Wendeln, University of Michigan Ann Arbor, Ann Arbor, MI, United States and Enrico Landi, University of Michigan, Ann Arbor, MI, United States
Jing Ye1,2, Jun Lin1, John C Raymond2 and Chengcai Shen2, (1)Chinese Academy of Science, Yunnan Observatories, Kunming, China, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
Ying-Dong Jia, University of California Los Angeles, Los Angeles, CA, United States, William Dean Pesnell, NASA / GSFC, Greenbelt, United States, Paul Bryans, NSF National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States, Cooper Downs, Predictive Science Inc., San Diego, CA, United States, Wei Liu, Bay Area Environmental Research Institute Palo Alto, Palo Alto, CA, United States and Steven J Schwartz, Earth and planetary and Space Sciences, Los angeles, United States
Roberto Lionello1, Pete Riley1, Dr. Tibor Torok2, Jon Linker1, Zoran Mikic1, John C Raymond3 and Chengcai Shen3, (1)Predictive Science Inc., San Diego, CA, United States, (2)Predictive Science Inc., San Diego, United States, (3)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
Yeimy Rivera1, Enrico Landi2, Susan T Lepri3 and Jason A Gilbert2, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Michigan, Ann Arbor, MI, United States, (3)University of Michigan, Ann Arbor, United States
Derek A Lamb, Southwest Research Institute, Boulder, CO, United States and Craig E. DeForest, Southwest Research Institute Boulder, Boulder, CO, United States
Chadi S Salem, SSL, University of California Berkeley, Berkeley, United States
Elizabeth (Lily) Hanson, University of California Berkeley, Berkeley, CA, United States, Chadi S Salem, University of California, Berkeley, United States, John W Bonnell, University of California, Berkeley, Space Sciences Laboratory, Berkeley, United States, Christopher Carew Chaston, University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, Stuart D Bale, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States and Forrest Mozer, University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
D Aaron Roberts, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Christopher Mark Bert1, Justin Christophe Kasper2,3, Prof. Kristopher Gregory Klein4 and Anthony W Case3, (1)University of Michigan, Ann Arbor, 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)University of Michigan Ann Arbor, Ann Arbor, MI, United States
Peter Hunana, University of Alabama in Huntsville, CSPAR, Huntsville, AL, United States, Gary Paul Zank, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States, Gary M Webb, Univ of Alabama, Huntsville, AL, United States and Laxman Adhikari, Center for Space Plasma and Aeronomic Research, Department of Space Science, The university of Alabama in Huntsville, Huntsville, United States
Alfred Mallet, University of New Hampshire Main Campus, Durham, NH, United States, Alexander A Schekochihin, University of Oxford, Oxford, United Kingdom and Benjamin D G Chandran, University of New Hampshire, Durham, United States
Chen Shi, Auburn University, Department of Physics, Auburn, United States, Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States and Anna Tenerani, University of Texas at Austin, Austin, TX, United States
Marco C M Velli, University of California Los Angeles, Earth Planetary and Space Sciences, Los Angeles, United States, Fulvia Pucci, NIFS National Institute for Fusion Science, Gifu, Japan, Anna Tenerani, California Institute of Technology, Pasadena, CA, United States, Chen Shi, Auburn University, Department of Physics, Auburn, United States, Daniele Del Sarto, University of Lorraine Nancy, Nancy Cedex, France and Antonio F Rappazzo, UCLA, Earth, Planetary and Space Sciences, Pasadena, CA, United States
Victor Réville1, Marco C M Velli1 and Sacha Brun2, (1)University of California Los Angeles, Los Angeles, CA, United States, (2)AIM, CEA, SACLAY, France
Roland Grappin, Ecole Polytechnique, LPP, Palaiseau Cedex, France, Victor Montagud-Camps, Astronomical Institute of the Academy of Sciences, Prague, Czech Republic and Andrea Verdini, University of Florence, Florence, Italy
Trevor Bowen1, Stuart D Bale1 and Samuel Timothy Badman2, (1)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)University of California Berkeley, Berkeley, CA, United States
