SH31B:
Plasma Properties of the Solar Corona and Solar Wind: Sources Versus Evolution I

Session ID#: 4417

Wednesday, 17 December 2014: 8:00 AM-10:00 AM
2011 (Moscone West)
Chairs:  Chadi S Salem, University of California, Berkeley, United States and Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States
Primary Convener:  Chadi S Salem, University of California, Berkeley, United States
Co-conveners:  Marco C M Velli, Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States and Roberto Lionello, Predictive Science Inc., San Diego, United States
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]
7511 Coronal holes [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
Virtual Option?: No

Abstracts Submitted to this Session:

A Versatile 4-Plasma Categorization Scheme for the Solar Wind: Exploring the Statistical Properties of Plasmas of Different Origins (20080)
Joseph Borovsky, Space Science Institute, Los Alamos, United States and Fei Xu, NUIST Nanjing University of Information Science and Technology, Nanjing, China
Plasma Properties of Pseudostreamers and Associated Solar Wind Streams (8794)
Mari Paz Miralles, Center for Astrophysics, Harvard & Smithsonian, Cambridge, United States, Steven R Cranmer, University of Colorado, Boulder, United States and Guillermo Stenborg, US Naval Research Laboratory, Space Science Division, Washington, DC, United States
Investigation of Solar Wind Source Regions by Using Ulysses/SWICS/SWOOPS Composition Data and a Potential Field Source Surface Model to map in situ Measurements back onto the Photosphere (22637)
Thies Peleikis1, Martin Alexander Kruse II1, Lars Berger2, Christian Drews3, Robert F Wimmer-Schweingruber3, David J McComas4 and George Gloeckler5, (1)University of Kiel, Kiel, Germany, (2)Kiel University, Kiel, Germany, (3)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (4)Southwest Research Institute San Antonio, San Antonio, TX, United States, (5)Univ Michigan, Ann Arbor, MI, United States
Characterizing a Model of Coronal Heating and Solar Wind Acceleration Based on Wave Turbulence. (Invited) (5549)
Cooper Downs1, Roberto Lionello1, Zoran Mikic1, Jon Linker1 and Marco C M Velli2, (1)Predictive Science Inc., San Diego, CA, United States, (2)University of California Los Angeles, Los Angeles, CA, United States
Interchange Reconnection and Slow Solar Wind Formation at the boundaries of open field regions in the Solar Corona (Invited) (5023)
Antonio F Rappazzo, UCLA, Earth, Planetary and Space Sciences, Pasadena, CA, United States, Prof. William H Matthaeus, University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, David J Ruffolo, Mahidol University, Bangkok, Thailand, Sergio Servidio, Universita' della Calabria, Rende, Italy and Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States
Visco-resistive tearing in thin current sheets. (29753)
Marco C M Velli, University of California Los Angeles, Earth Planetary and Space Sciences, Los Angeles, United States, Anna Tenerani, California Institute of Technology, Pasadena, CA, United States, Antonio F Rappazzo, UCLA, Earth, Planetary and Space Sciences, Pasadena, CA, United States and Fulvia Pucci, University of Rome Tor Vergata, Rome, Italy
On the Dependence of Solar Wind Speed on Local Magnetic Field Orientation in Highly Alfvénic Streams (Invited) (5708)
Lorenzo Matteini, Observatoire De Paris, LESIA, Meudon, FRANCE, Timothy Simon Horbury, Imperial College London, Department of Physics, London, SW7, United Kingdom, Marcia Neugebauer, University of Arizona, Tucson, AZ, United States and Bruce E Goldstein, NASA Jet Propulsion Laboratory, Pasadena, CA, United States
Alpha-Particle/Proton Differential Flow in the Solar Wind: Implications for Plasma Heating, Azimuthal Flow, and the Parker Spiral Magnetic Field (13825)
Daniel Verscharen, University College London, Mullard Space Science Laboratory, London, United Kingdom, Sofiane Bourouaine, University of New Hampshire, Durham, NH, United States and Benjamin D G Chandran, University of New Hampshire, Durham, United States