SH53A:
Fundamental Physics of the Solar Corona and Inner Heliosphere II


Submit an Abstract to this Session


Session ID#: 61412

Session Description:
The solar corona and wind provide a natural laboratory where magnetic fields guide and energize the plasma. Structured over a wide range of time and spatial scales, the coronal plasma is heated and accelerated giving rise to the turbulent, super-Alfvénic wind filling the heliosphere. With the launch of Parker Solar Probe, inner heliospheric research should reach a new level of understanding. This session explores 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 derived from models, what fundamental observations from Parker Solar Probe and Solar Orbiter should drive theoretical developments? 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 Yannis Zouganelis, European Space Agency, Villanueva De La Can, Spain
Primary Liaison:  Chadi S Salem, University of California, Berkeley, United States
Chairs:  Chadi S Salem, University of California, Berkeley, United States and Yannis Zouganelis, European Space Agency, Villanueva De La Can, Spain
OSPA Liaison:  Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, 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:

A new generation of numerical models and tools for Parker Solar Probe and Solar Orbiter (Invited) (376956)
Alexis P Rouillard, IRAP, Toulouse, France
Wave propagation within 3D MHD simulations of the heliosphere (451685)
Victor Réville1, Chen Shi2, Marco C M Velli1, Roger K Ulrich3 and Tham V Tran4, (1)University of California Los Angeles, Los Angeles, CA, United States, (2)Auburn University, Department of Physics, Auburn, United States, (3)UCLA, Department of Physics and Astronomy, Los Angeles, United States, (4)University of California at Los Angeles, Physics and Astronomy, Los Angeles, CA, United States
Three-dimensional, magnetohydrodynamic simulation of the solar wind acceleration from the coronal base to 0.1 au (400857)
Munehito Shoda, The University of Tokyo, Department of Earth and Planetary Science, Bunkyo-ku, Japan, Takeru Ken Suzuki, University of Tokyo, Tokyo, Japan, Mahboubeh Asgari-Targhi, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States and Takaaki Yokoyama, University of Tokyo, Department of Earth and Planetary Science, Bunkyo-ku, Japan
On the evolution of reflection-driven Alfven turbulence from the photosphere to 40 solar radii: Simulations, theory and future Parker Solar Probe observations. (465528)
Jean Carlos Perez, Florida Institute of Technology, Melbourne, FL, United States and Benjamin D G Chandran, University of New Hampshire, Durham, United States
Particle Heating and Energy Partition in Low-$\beta$ Guide Field Reconnection with Kinetic Riemann Simulations (449420)
Qile Zhang1, James Frederick Drake1 and Marc Swisdak2, (1)University of Maryland College Park, College Park, MD, United States, (2)University of Maryland, College Park, United States
Generation of constant-B states in high-β plasmas. (436395)
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
The Multi-Scale Nature of the Solar Wind (368237)
Daniel Verscharen, University College London, Mullard Space Science Laboratory, Dorking, United Kingdom; University of New Hampshire, Space Science Center, Durham, United States, Prof. Kristopher Gregory Klein, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States and Bennett Maruca, University of Delaware, Department of Physics and Astronomy, Newark, DE, United States
A Non-Perturbative Description for the Heat Flux in the Corona and Solar Wind (443064)
Jack D Scudder, University of Iowa, Iowa City, IA, United States, Vadim Roytershteyn, Space Science Institute Boulder, Boulder, United States and Chadi S Salem, University of California, Berkeley, United States

See more of: SPA-Solar and Heliospheric Physics