SH23B:
Waves, Instabilities, and Turbulence in Magnetized Plasma Structures I
Submit an Abstract to this Session
Session ID#: 61308
Session Description:
Excitation of plasma waves, instabilities, and turbulence have been manifested in remote and in-situ space observations on a wide range of spatio-temporal scales. A few examples of these phenomena include Alfven and kink waves in chromospheric and coronal structures, acoustic modes in photosphere and convection zone, turbulence and kinetic waves in the solar wind. Laboratory experiments have made vital contributions in developing models that can accurately predict propagation and damping of plasma waves and instabilities. Improvements and validation of theoretical/numerical models for solar plasma can help us fully utilize diagnostic capabilities of these waves and understand their role in energy transport. This session invites participation of space observers, modelers, and plasma physicists working in this broad area of research. Contributions based on recent (SDO, Hinode, IRIS, WIND, ACE, Helios, Cluster, and MMS) and planning for next generation observational facilities (DKIST, EST, Solar-Orbiter, and Parker Solar Probe) are especially welcome.
Primary Convener: Shreekrishna Tripathi, University of California Los Angeles, Los Angeles, United States
Conveners: Gary Paul Zank, Univ of Alabama, Huntsville, Huntsville, United States and Leon Ofman, NASA GSFC/CUA, Greenbelt, United States
Primary Liaison: Shreekrishna Tripathi, University of California Los Angeles, Los Angeles, United States
Chairs: Leon Ofman, NASA GSFC/CUA, Greenbelt, United States and Shreekrishna Tripathi, University of California Los Angeles, Los Angeles, United States
OSPA Liaison: Shreekrishna Tripathi, University of California Los Angeles, Los Angeles, United States
Cross-Listed:
Abstracts Submitted to this Session:
Michael Hahn, Columbia University, New York, United States
Paul Murray Bellan and Magnus Albert Haw, California Institute of Technology, Pasadena, CA, United States
Lloyd David Woodham1, Robert T Wicks2,3, Daniel Verscharen4,5 and Christopher John Owen2, (1)Imperial College, London, United Kingdom, (2)University College London, Mullard Space Science Laboratory, London, United Kingdom, (3)University College London, Institute for Risk and Disaster Reduction, London, United Kingdom, (4)University of New Hampshire, Space Science Center, Durham, United States, (5)University College London, Mullard Space Science Laboratory, Dorking, United Kingdom
Gary Verth, University of Sheffield, School of Mathematical and Physical Sciences, Sheffield, United Kingdom, Wernher Brevis, Pontificia Universidad Catolica de Chile, Santiago, Chile, Cristian R Escauriaza, Pontifical Catholic University of Chile, Hydraulic and Environmental Engineering, Santiago, Chile, Viktor Fedun, The University of Sheffield, School of Electrical and Electronic Engineering, Sheffield, United Kingdom, David B Jess, Queen's University Belfast, School of Mathematics and Physics, Belfast, United Kingdom, Marco Stangalini, Italian Space Agency, Roma, Italy and Anwar Ali Aldhafeeri, University of Sheffield, Sheffield, S10, United Kingdom
Tongjiang Wang, Catholic University of America and NASA GSFC, Washington, United States; NASA GSFC, Greenbelt, United States, Stephen J. Bradshaw, Rice University, Department of Physics and Astronomy, Houston, United States, Leon Ofman, NASA GSFC/CUA, Greenbelt, United States; Catholic University of America, Physics, Washington, DC, United States and Brian R Dennis, NASA GSFC, Greenbelt, MD, United States
Prof. Kristopher Gregory Klein, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, Daniel Verscharen, University College London, Mullard Space Science Laboratory, Dorking, United Kingdom, Michael Louis Stevens, Smithsonian Astrophysical Observatory, Cambridge, MA, United States, Benjamin L. Alterman, Southwest Research Institute, Space Science and Engineering, San Antonio, United States, Daniel Vech, University of Michigan Ann Arbor, Ann Arbor, MI, United States and Justin Christophe Kasper, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States
Bennett Maruca1, Alexandros Chasapis2, S. Peter Gary3, Riddhi Bandyopadhyay4, Dr. Rohit Chhiber, BSc (Honours), MSc, PhD5, Tulasi Parashar6, Prof. William H Matthaeus1, Michael A. Shay1, James L Burch7, Thomas Earle Moore8, Craig J Pollock9, Barbara L Giles9, William R Paterson10, John C Dorelli11, Daniel J Gershman9, Roy B Torbert12, Christopher T Russell13 and Robert J Strangeway14, (1)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (2)University of Delaware, Physics and Astronomy, Newark, United States, (3)Space Science Institute Boulder, Boulder, CO, United States, (4)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (5)University of Delaware, Department of Physics and Astronomy, Newark, United States, (6)University of Delaware, Newark, DE, United States, (7)Southwest Research Institute, San Antonio, United States, (8)NASA Goddard Space Flight Ctr, Greenbelt, United States, (9)NASA Goddard Space Flight Center, Greenbelt, United States, (10)NASA Goddard Space Flight Center, Geospace Physics Laboratory, Greenbelt, MD, United States, (11)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (12)University of New Hampshire, Durham, United States, (13)University of California Los Angeles, Los Angeles, United States, (14)University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, United States
Vadim Roytershteyn1, Gian Luca Delzanno2 and Oleksandr Koshkarov2, (1)Space Science Institute Boulder, Boulder, United States, (2)Los Alamos National Laboratory, Los Alamos, NM, United States
