SH53C:
Evolution and Dynamics of Turbulence in the Heliosphere II

Session ID#: 4408

Friday, 19 December 2014: 1:40 PM-3:40 PM
2012 (Moscone West)
Chairs:  Khurom Hussain Kiyani1, Kareem Osman1, Minping Wan2 and Prof. William H Matthaeus3, (1)University of Warwick, Coventry, CV4, United Kingdom(2)University of Delaware, Newark, United States(3)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States
Primary Convener:  Kareem Osman, University of Warwick, Coventry, CV4, United Kingdom
Co-conveners:  Khurom Hussain Kiyani, University of Warwick, Coventry, CV4, United Kingdom, Prof. William H Matthaeus, University of Delaware, Department of Physics and Astronomy, Newark, DE, United States and Minping Wan, University of Delaware, Newark, United States
OSPA Liaison:  Kareem Osman, University of Warwick, Coventry, CV4, United Kingdom
Co-Sponsor(s):
  • NG - Nonlinear Geophysics
  • SM - SPA-Magnetospheric Physics
Index Terms:

2134 Interplanetary magnetic fields [INTERPLANETARY PHYSICS]
2159 Plasma waves and turbulence [INTERPLANETARY PHYSICS]
4490 Turbulence [NONLINEAR GEOPHYSICS]
7863 Turbulence [SPACE PLASMA PHYSICS]
Virtual Option?: No

Abstracts Submitted to this Session:

SH53C-01
Formation of coherent structures in kinetic simulations of collisionless turbulence (Invited) (3480)
Vadim Roytershteyn, Space Science Institute, Boulder, United States; Space Science Institute Boulder, Boulder, United States and Homayoun Karimabadi, CureMetrix, Rancho Santa Fe, CA, United States; Analytics Ventures, San Diego, CA, United States
SH53C-02
Sub-Proton Scale Magnetic Holes: Turbulence Simulations, Theory and Cluster Observations in the Earth's Plasma Sheet. (15604)
Christopher T Haynes1, David Burgess2, Enrico Camporeale3 and Torbjorn Sundberg1, (1)Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom, (2)Queen Mary University of London, Department of Physics and Astronomy, London, United Kingdom, (3)University of Colorado, Queen Mary University of London, Boulder, United States
SH53C-03
Parametric Study of Preferential Ion Heating Due to Intermittent Magnetic Fields in the Solar Wind (5315)
Leopoldo Carbajal Gomez1, Sandra C Chapman1,2, Richard O Dendy3,4 and Nicholas Wynn Watkins2,5, (1)University of Warwick, Centre for Fusion, Space and Astrophysics, Department of Physics, Coventry, CV4, United Kingdom, (2)Max Planck Institute for the Physics of Complex Systems, Dresden, Germany, (3)EURATOM/CCFE Fusion Association, Culham Science Centre, Abingdon, United Kingdom, (4)University of Warwick, Centre for Fusion, Space and Astrophysics, Department of Physics, Coventry, United Kingdom, (5)London School of Economics, London, United Kingdom
SH53C-04
Three-fluid, 3D MHD solar wind modeling with turbulence transport and eddy viscosity (Invited) (4817)
Arcadi V. Usmanov1,2, Melvyn L Goldstein3 and Prof. William H Matthaeus2, (1)NASA Goddard SFC, Greenbelt, MD, United States, (2)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (3)Space Science Institute Boulder, Boulder, United States
SH53C-05
The Mechanisms for Particle Acceleration and Heating in Multi-Island Magnetic Reconnection (Invited) (4830)
James Frederick Drake, University of California Berkeley, Berkeley, CA, United States, Joel Dahlin, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Marc Swisdak, University of Maryland, College Park, United States
SH53C-06
In Situ Observations of Ion Scale Current Sheets and Associated Electron Heating in Turbulent Space Plasmas (14228)
Alexandros Chasapis1, Alessandro Retino2, Fouad Sahraoui1, Antonella Greco3, Andris Vaivads4, Yuri V Khotyaintsev5, David J Sundkvist6 and Patrick Canu7, (1)Laboratoire de Physique des Plasmas, Saint-Maur Des Fossés Cedex, France, (2)Laboratoire de Physique des Plasmas, CNRS/Sorbonne Université/Univ. Paris Saclay/Obs. de Paris/ Ecole Polytechnique, Institut Polytechnique de Paris, Palaiseau, France, (3)Università della Calabria, Department of Physics, Rende, Italy, (4)Royal Institute of Technology, KTH, Space and Plasma Physics, Stockholm, Sweden, (5)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (6)UC Berkeley, Berkeley, CA, United States, (7)Laboratoire de Physique des Plasmas, Palaiseau, France
SH53C-07
Observation of Counter Propagating Alfven Waves with Perpendicular Polarizations and the Associated Proton Kinetics (Invited) (4589)
Jiansen He1, Zhong-Tian Pei1, Linghua Wang1, Chuan-Yi Tu1, Eckart Marsch2 and Shuo Yao3, (1)Peking University, Beijing, China, (2)University of Kiel, Kiel, Germany, (3)China University of Geosciences, Beijing, Beijing, China
SH53C-08
Three-Dimensional Iroshnikov-Kraichnan Turbulence in a Mean Magnetic Field (8406)
Prof. Wolf-Christian Muller, Technische Universität Berlin, Plasma-Astrophysics, Berlin, Germany, Roland Grappin, LUTH, Observatoire de Paris and LPP, Ecole Polytechnique, Paris, France, Andrea Verdini, LESIA, Observatoire de Paris-Meudon & LPP, Universite Paris 6/7, Paris, Paris, France and Özgur Gürcan, LPP, Ecole Polytechnique, Paris, France
See more of: SPA-Solar and Heliospheric Physics