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:  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 Olga Panasenco, Advanced Heliophysics Inc., Pasadena, United States
OSPA Liaison:  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:

Modeling Plasmas with a Kappa Electron Energy Distribution (58968)
Michael Hahn and Daniel Wolf Savin, Columbia University, New York, United States
A Low Beta and Exact Kinetic Equilibrium for a 1D Nonlinear Force-Free field (60265)
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
Compressive Solar-Wind Turbulence and Anisotropy-Driven Micro-Instabilities (60516)
Daniel Verscharen, University College London, London, United Kingdom and Benjamin D G Chandran, University of New Hampshire Main Campus, Durham, NH, United States
Energy Balance in Magnetic Loops of the Quiet Sun (61946)
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
Solar Minima Comparative Analysis Using EUV Tomography (62155)
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
Multi-Species Instability Thresholds in the Solar Wind (62666)
Christopher H K Chen, Queen Mary University of London, Department of Physics and Astronomy, London, United Kingdom
Self-consistent particle-in-cell simulations of fundamental and harmonic radio plasma emission mechanisms (63287)
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
Relative Heating of Heavy Ions Observed at 1 AU with ACE/SWICS (64689)
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
Differential flow: Locally Generated or Coronal Artifact? (64749)
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
Pitch Angle Scattering of Solar Flare Electrons in the Interplanetary Medium: Observations and Modelling (65243)
Benjamin Alcock1, Eduard Kontar1 and Neus Agueda2, (1)University of Glasgow, Glasgow, G12, United Kingdom, (2)University of Barcelona, Barcelona, Spain
Modeling electron density, temperature distribution in the solar corona based on solar surface magnetic field observations (65722)
Jenny Marcela Rodríguez, Luis Eduardo A 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
Effects of density fluctuations on nonlinear evolution of low-frequency Alfven waves in solar wind plasmas (65911)
Yasuhiro Nariyuki and Jungjoon Seough, University of Toyama, Toyama, Japan
Research of fast Magnetoacoustic Wave in Solar Atmosphere (66810)
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
A Mechanism for Helium-3 Abundance Enhancements in Solar Flares (70676)
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
A Unified Scenario for the Solar Wind Phenomenon (73569)
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
Observational Characteristics of Langmuir Turbulence Associated with Solar Type III Radio Bursts (74726)
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
High Resolution Simulations of Tearing and Flux-Rope Formation in Active Region Jets (74914)
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 GSFC, Greenbelt, United States
Solar Wind Magnetic Fluctuations and Electron Non-Thermal Temperature Anisotropy: Survey of Wind-SWE-VEIS Observations (75579)
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)University of Chile, Department of Physics, Santiago, Chile
Non-gyrotropic pressure anisotropy induced by velocity shear. (78496)
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
 Anomalous Ion Charge State Behavior In Interplanetary Coronal Mass Ejections (80495)
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
Numerical Modeling of Supra-Arcade Downflows (81271)
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

See more of: SPA-Solar and Heliospheric Physics