SH31A:
Approaching Kappa Distributions: Statistical Background, Theoretical Developments, and Applications in Space Plasma Physics I Posters


Session ID#: 8618

Session Description:
Kappa distributions have become increasingly widespread across space plasma physics with the publication rate following, remarkably, an exponential growth. A breakthrough in the field came with the connection of kappa distributions with the solid statistical framework of non-extensive statistical mechanics, a generalization of the classical Boltzmann-Maxwell theory. Thereafter, numerous analyses were developed: Thermodynamics (temperature, pressure, kappa, entropy); positional distribution (when the potential is non-zero); multi-particle distribution, etc. These are followed by a plethora of applications in space plasmas throughout the heliosphere, planetary/cometary magnetospheres, and beyond. We welcome abstracts reporting on the progress of: (i) Theory of kappa distributions and non-extensive statistical mechanics; (ii) Effects of kappa distributions on plasma processes, e.g., linear/nonlinear waves, instabilities, shocks, with emphasis on the Rankine–Hugoniot conditions; (iii) Identification of mechanisms responsible for generating kappa distributions; (iv) Data analyses/ MHD simulations that involve kappa distributions, e.g., particle acceleration, circulation inside planetary magnetospheres, modeling of heliospheric boundaries.
Primary Convener:  George Livadiotis, Southwest Research Institute San Antonio, San Antonio, TX, United States
Conveners:  Peter H Yoon, University of Maryland College Park, College Park, MD, United States and Kostas Dialynas, Office for Space Research and Technology, Academy of Athens, Athens, Greece
Chairs:  George Livadiotis, Southwest Research Institute, San Antonio, TX, United States and Peter H Yoon, University of Maryland College Park, College Park, MD, United States
OSPA Liaison:  Peter H Yoon, University of Maryland College Park, College Park, MD, United States

Cross-Listed:
  • NG - Nonlinear Geophysics
  • P - Planetary Sciences
  • S - Seismology
  • SM - SPA-Magnetospheric Physics
Index Terms:

2756 Planetary magnetospheres [MAGNETOSPHERIC PHYSICS]
7827 Kinetic and MHD theory [SPACE PLASMA PHYSICS]
7845 Particle acceleration [SPACE PLASMA PHYSICS]
7851 Shock waves [SPACE PLASMA PHYSICS]

Abstracts Submitted to this Session:

Rankine–Hugoniot jump conditions incorporating kappa distributions (63546)
George Livadiotis, Southwest Research Institute San Antonio, San Antonio, TX, United States
The Spectrum of Solar Wind Superhalo Electrons (67028)
Linghua Wang1, Liu Yang1, Chuan-Yi Tu2, Jiansen He2, Peter H Yoon3, Robert F Wimmer-Schweingruber4, Chadi S Salem5 and Stuart D Bale6, (1)Peking University, Institute of Space Physics and Applied Technology, Beijing, China, (2)Peking University, Beijing, China, (3)University of Maryland College Park, College Park, MD, United States, (4)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (5)University of California Berkeley, Berkeley, CA, United States, (6)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
Solar Wind Modelling: MHD And Kinetic Treatments with Kappa Distributions for the Electrons (66941)
Sofia Paraskevi Moschou1,2, Viviane Pierrard3, R. Keppens2 and Jens Pomoell4, (1)Belgian Institute for Space Aeronomy, Brussels, Belgium, (2)KULeuven, CmPA, Leuven, Belgium, (3)Royal Belgian Institute for Space Aeronomy, Brussels, Belgium, (4)University of Helsinki, Helsinki, Finland
Misestimation of plasma temperature when applying a Maxwellian distribution to space plasmas described by kappa distributions (68519)
Georgios Nicolaou, IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden and George Livadiotis, Southwest Research Institute, San Antonio, TX, United States
Charge-exchange Induced Modulation of the Heliosheath Ion Distribution Downstream of the Termination Shock (60259)
Horst Fichtner1, Hans Joerg Fahr2 and Klaus Scherer1, (1)Ruhr Universität Bochum, Bochum, Germany, (2)University of Bonn, Bonn, Germany
Ion energetics at Saturn’s magnetosphere using Cassini/MIMI measurements: A simple model for the energetic ion integral moments (68187)
Kostas Dialynas, Academy of Athens, Athens, Greece, Chris Paranicas, Applied Physics Laboratory Johns Hopkins, Laurel, United States, Elias Roussos, Max Planck Institute for Solar System Research, Göttingen, Germany, Stamatios Mike Krimigis, Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, Mark Kane, Organization Not Listed, Washington, DC, United States and Donald G Mitchell, JHU/APL, Laurel, MD, United States
Characterizing Observations of Cometary Electrons with Kappa Distributions (84551)
Thomas W Broiles1, George Livadiotis2, James L Burch3, Raymond Goldstein2, Kathleen Mandt2, Jerry Goldstein2, George B Clark4, Stephen A Fuselier3, Marilia Samara5, Thomas Cravens6, Anders I Eriksson7, Pierre Henri8, Prachet Mokashi1 and Kyung Chae2, (1)Southwest Research Institute San Antonio, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, TX, United States, (3)Southwest Research Institute, San Antonio, United States, (4)Johns Hopkins Applied Physics Laboratory, Laurel, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (6)University of Kansas, Physics and Astronomy, Lawrence, KS, United States, (7)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (8)LPC2E, CNRS, Orléans, France
Reconsideration of pressure anisotropy thresholds in the solar wind assuming bi-kappa distributions (75668)
Patrick Astfalk1, Frank Jenko2 and Tobias Görler1, (1)Max-Planck-Institute for Plasma Physics, Garching, Germany, (2)Max Planck Institute for Plasma Physics, Garching, Germany
Steady-State Model of Solar Wind Electrons and Implications for Kappa Distribution (69707)
Sunjung Kim, Kyung Hee University, Yongin, Korea, Republic of (South), Peter H Yoon, University of Maryland College Park, College Park, MD, United States and Gwang-Son Choe, Kyung Hee University, School of Space Research, Yongin, Korea, Republic of (South)
Role of turbulent transport in the evolution of the κappa distribution functions in the plasma sheet (70955)
Marina V Stepanova, University of Santiago Chile, Santiago, Chile and Elizabeth E Antonova, Lomonosov Moscow State University, Moscow, Russia
Particle accelerations and current structures of Weibel and Filamentation instabilities (64151)
Chang-Mo Ryu and Cong Tuan Huynh, POSTECH Pohang University of Science, Pohang, Korea, Republic of (South)
OBLIQUE PROPAGATION OF ION ACOUSTIC SOLITONS IN MAGNETIZED SUPERTHERMAL PLASMAS (64382)
Devanandhan Selvaraj1, T Sreeraj2, Satyavir Singh2 and Gurbax Singh Lakhina2, (1)Indian Institute of Geomagnetism, Upper Atmosphere Studies, Navi Mumbai, India, (2)Indian Institute of Geomagnetism (IIG), Navi Mumbai, India
Obliquely propagating electrostatic waves in a magnetized plasma for different types of anisotropic kappa distribution (64179)
Muhammad Fraz Bashir1, Peter H Yoon2, Ghulam Murtaza3, Darakhsan Aqeel4, Sumaira Javed4 and Madiha Zahra4, (1)COMSATS Institute of Infotmation Technology Lahore, Department of Physics, Lahore, Pakistan, (2)University of Maryland College Park, College Park, MD, United States, (3)Quaid-i-Azam University, Islamabad, Pakistan, (4)Government College University Lahore, Lahore, Pakistan
On the self-organization of magnetic field and highly diluted matter in astrophysics (79158)
Daniel Benjamin Berdichevsky, NASA Goddard Space Flight Center, Division 670, Greenbelt, MD, United States
Temporal Correlations In Natural Time Analysis and Tsallis Non Extensive Statistical Mechanics (77855)
Panayiotis Varotsos1, Nicholas V Sarlis2 and Efthimios S Skordas2, (1)National and Kapodistrian University of Athens, Solid Earth Physics Institute, Athens, Greece, (2)National and Kapodistrian University of Athens, Department of Physics, Athens, Greece

See more of: SPA-Solar and Heliospheric Physics