SH51A:
Particle Acceleration and Transport at the Sun and in the Inner Heliosphere I
Submit an Abstract to this Session
Session ID#: 61249
Session Description:
An important topic of solar and heliospheric physics is to understand the acceleration and transport of nonthermal particles. Such studies in the inner heliosphere encompasses a variety of processes leading to the formation of solar wind suprathermal particles, solar energetic particles, energetic particles from Corotating Interaction Regions, etc. However, many details of the acceleration and transport process of these energetic particles still remain unknown. Particle acceleration processes include magnetic reconnection, wave-particle interactions, collisionless shock waves, etc., and particle transport processes include adiabatic cooling, parallel and perpendicular diffusion, random walk of magnetic field lines, etc. This session invites contributions that discuss space-borne and ground-based observations, and theory/modeling of the processes pertaining to particle acceleration and transport at the Sun and in the inner heliosphere.
Primary Convener: Linghua Wang, Peking University, Institute of Space Physics and Applied Technology, Beijing, China
Conveners: Gang Li, University of Alabama in Huntsville, Huntsville, United States, Richard Mewaldt, Caltech, Pasadena, CA, United States and Robert F Wimmer-Schweingruber, University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany
Primary Liaison: Gang Li, University of Alabama in Huntsville, Huntsville, United States
Chairs: Linghua Wang, Peking University, Institute of Space Physics and Applied Technology, Beijing, China and Richard Mewaldt, Caltech, Pasadena, CA, United States
OSPA Liaison: Linghua Wang, Peking University, Institute of Space Physics and Applied Technology, Beijing, China
Abstracts Submitted to this Session:
Mihir Indrajit Desai, Southwest Research Institute, San Antonio, TX, United States and Integrated Science Investigation of the Sun: Energetic Particles for the Parker Solar Probe
Yihong Wu1, Alexis P Rouillard1, Athanasios Kouloumvakos1, Rami O Vainio2, Alexandr N. Afanasiev2 and Illya Plotnikov3, (1)IRAP, Toulouse, France, (2)University of Turku, Department of Physics and Astronomy, Turku, Finland, (3)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States
Georgia Adair de Nolfo1, Alessandro Bruno1, Eric R Christian2, Silvia Dalla3, Joe Giacalone4, Ian G Richardson5, James M Ryan6, Ronald J Murphy7, Gerald H Share8 and On Behalf of The PAMELA Collaboration , (1)NASA Goddard Space Flight Center, Greenbelt, United States, (2)NASA GSFC, Greenbelt, MD, United States, (3)University of Central Lancashire, Jeremiah Horrocks Institute, Preston, United Kingdom, (4)University of Arizona, Planetary Sciences, Tucson, AZ, United States, (5)University of Maryland College Park, NASA Goddard Space Flight Center, Greenbelt, United States, (6)Univ New Hampshire, Durham, NH, United States, (7)Naval Research Lab, Washington, DC, United States, (8)University of Maryland, Astronomy, Silver Spring, MD, United States
Lulu Zhao, Florida Institute of Technology, Department of Physics and Space Sciences, Melbourne, United States and Ming Zhang, Florida Institute of Technology, Melbourne, FL, United States
Joseph Lazio1, Justin Christophe Kasper2, Andrew Romero-Wolf3, Tim Bastian4, Christina Cohen5, Enrico Landi6, Ward Manchester2, Nathan Schwadron7, Igor Sokolov2, Baptiste Cecconi8, Gregg Hallinan9, Vratislav Krupar10, Milan Maksimovic11, Sofia Paraskevi Moschou12, Arnaud Zaslavsky13, Alexander Michael Hegedus14, James P Lux15, Tim L. Neilsen16 and SunRISE Science Team, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (3)Physical Insights, LLC, Kaneohe, United States, (4)Natl Radio Astron Observ, Charlottesville, VA, United States, (5)Caltech, Pasadena, United States, (6)University of Michigan, Ann Arbor, MI, United States, (7)University of New Hampshire, Durham, United States, (8)Paris Observatory Meudon, Meudon, France, (9)California Institute of Technology, Pasadena, CA, United States, (10)Universities Space Research Association Columbia, Columbia, United States, (11)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, (12)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (13)CNRS, Observatoire de Paris, LESIA, Meudon, France, (14)Lunasonde Inc., Science, Tucson, United States, (15)Jet Propulsion Laboratory, Pasadena, United States, (16)Space Dynamics Laboratory, North Logan, UT, United States
Milan Maksimovic, LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France
Joe Giacalone, University of Arizona, Planetary Sciences, Tucson, AZ, United States, David Lario, NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States and Susan T Lepri, University of Michigan, Ann Arbor, United States
Richard A Leske1, Alan C Cummings1, Richard Mewaldt2, Edward C Stone1, Tycho T von Rosenvinge3 and Mark E Wiedenbeck4, (1)California Institute of Technology, Pasadena, CA, United States, (2)Caltech, Pasadena, CA, United States, (3)NASA Goddard SFC, Greenbelt, United States, (4)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
