SH51B:
Fundamental Physics of the Solar Corona and Inner Heliosphere II Posters
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Session ID#: 12438
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 and Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States
Chairs: Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States and Chadi S Salem, SSL, University of California Berkeley, Berkeley, United States
OSPA Liaison: Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States
Abstracts Submitted to this Session:
Peter H Yoon, University of Maryland College Park, Institute for Physical Science and Technology, College Park, United States
Rudolf von Steiger, International Space Science Institute, Bern, Switzerland and Thomas Zurbuchen, University of Michigan Ann Arbor, Ann Arbor, MI, United States
Verena Heidrich-Meisner1, Thies Peleikis2, Martin Alexander Kruse II2, Robert F Wimmer-Schweingruber1 and Lars Berger1, (1)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (2)University of Kiel, Kiel, Germany
Lina Hadid, Laboratoire de Physique des Plasmas, LPP, CNRS-Ecole Polytechnique-UPMC-Université Paris-Sud, F-91128 Palaiseau, France, Palaiseau, France, Fouad Sahraoui, Laboratoire de Physique des Plasmas, Saint-Maur Des Fossés Cedex, France, Sébastien Galtier, Laboratoire de Physique des Plasmas, Palaiseau, France and Supratik Banerjee, Universitat zu Koln, Institut fur Geophysik und Meteorologie, Pohligstrasse 3, 50969 Koln, Germany, Koln, Germany
Joel Pavan, UFPEL Federal University of Pelotas, Pelotas, Brazil and Adolfo F. Vinas, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Maria Elena Innocenti, Katholieke Universiteit Leuven, Department of Mathematics, Leuven, Belgium, Wei Jiang, School of Physics, Huazhong University of Science and Technology, Wuhan, China, Wuhan, China, Giovanni Lapenta, KU Leuven, Mathematics, Leuven, Belgium and Stefano Markidis, KTH Royal Institute of Technology, Stockholm, Sweden
Kyunghwan Dokgo1, Helen H Kaang2, Kyoung W Min1 and Cheongrim Choi3, (1)KAIST Korea Advanced Institute of Science and Technology, Daejeon, Korea, Republic of (South), (2)NFRI National Fusion Research Institute, Daejeon, Korea, Republic of (South), (3)Chungbuk National University, Cheongju, Korea, Republic of (South)
Nils Peter Janitzek1, Lars Berger2, Christian Drews2 and Robert F Wimmer-Schweingruber2, (1)University of Kiel, Kiel, Germany, (2)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany
D Aaron Roberts, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Yuan-Kuen Ko, US Naval Research Laboratory, Space Science Division, Washington, DC, United States and Susan T Lepri, University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
Kelly E Korreck1, Anthony W Case1, Michael Louis Stevens1, Justin Christophe Kasper2, Phyllis L Whittlesey3, Davin E Larson4, Roberto Livi5 and Jasper S Halekas6, (1)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (2)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (3)University of Alabama in Huntsville, Huntsville, AL, United States, (4)Space Sciences Laboratory, Berkeley, United States, (5)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (6)University of Iowa, Iowa City, IA, United States
Jiansen He1, Wenzhi Ruan2, Lei Zhang3, Christian Vocks4, Eckart Marsch5, Chuanyi Tu5, Hardi Peter6 and Linghua Wang2, (1)Peking University, School of Earth and Space Sciences, Beijing, China, (2)Peking University, Institute of Space Physics and Applied Technology, Beijing, China, (3)NSSC National Space Science Center, CAS, Beijing, China, (4)Leibniz Institute for Astrophysics Potsdam, Potsdam, Germany, (5)University of Kiel, Kiel, Germany, (6)Max Planck Institute for Solar System Research, Göttingen, Germany
Lars K. S. Daldorff1, James A Klimchuk2 and Kalman Joshua Knizhnik2, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States
Alejandro Lara1, Cynthia Lopez-Portella2, Andrea Borgazzi2, Juan Carlos Gonzalez2 and Tatiana Niembro Hernandez3, (1)National Autonomous University of Mexico, Ciudad DE Armería, Mexico, (2)Universidad Nacional Autonoma de Mexico, Instituto de Geofisica, Mexico City, Mexico, (3)Universidad Nacional Autonoma de Mexico, Mexico City, Mexico
John T Steinberg, Los Alamos National Laboratory, Los Alamos, NM, United States, Yuguang Tong, University of California Berkeley, Berkeley, CA, United States and Joseph Borovsky, Space Science Institute Los Alamos, Los Alamos, NM, United States
Anna Tenerani, University of Texas at Austin, Austin, TX, United States and Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States
Mahboubeh Asgari-Targhi and Adriaan A. van Ballegooijen, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
Chen Shi, Auburn University, Department of Physics, Auburn, United States, Anna Tenerani, University of Texas at Austin, Austin, TX, United States and Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States
