SH51A:
Evolution and Dynamics of Turbulence in the Heliosphere I Posters

Friday, 19 December 2014: 8:00 AM-12:20 PM
Chairs:  Kareem Osman1, Minping Wan2, William H Matthaeus2 and Khurom Hussain Kiyani1, (1)University of Warwick, Coventry, CV4, United Kingdom(2)University of Delaware, Newark, DE, United States
Primary Conveners:  Kareem Osman, University of Warwick, Coventry, CV4, United Kingdom
Co-conveners:  Khurom Hussain Kiyani1, William H Matthaeus2 and Minping Wan2, (1)University of Warwick, Coventry, CV4, United Kingdom(2)University of Delaware, Newark, DE, United States
OSPA Liaisons:  Kareem Osman, University of Warwick, Coventry, CV4, United Kingdom

Abstracts Submitted to this Session:

 
Twins: A New Mission to Solve the Problem of Turbulence and Energy Dissipation at Electron Scales in the Solar Wind
Fouad Sahraoui, Laboratoire de Physique des Plasmas, Saint-Maur Des Fossés Cedex, France
 
M⁴ - a mission candidate for ESA M4
Andris Vaivads, IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden and Alessandro Retino, CNRS, Paris Cedex 16, France
 
The Effects of Ion Kinetic Instabilities on the Three-Dimensional Reconnection of Ion-Scale Current Sheets in the Solar Wind
David Burgess, Queen Mary, University of London, London, United Kingdom, Peter Gingell, Queen Mary, University of London, London, E1, United Kingdom and Lorenzo Matteini, Imperial College London, London, United Kingdom
 
Alfvénic Turbulence and Kinetic Instabilities in the Expanding Solar Wind: Two-Dimensional Hybrid Simulations
Lorenzo Matteini1, Petr Hellinger2, Simone Landi3, Luca Franci3, Andrea Verdini3,4 and Pavel M. Travnicek2,5, (1)Imperial College London, London, United Kingdom, (2)Astronomical Institute, AS CR, Prague, Czech Republic, (3)Università di Firenze, Dipartimento di Fisica e Astronomia, Firenze, Italy, (4)Royal Observatory of Belgium, Brussels, Belgium, (5)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
 
Electron and Ion Heating By Whistler Turbulence: Three-Dimensional Particle-in-Cell Simulations
Randall Scott Hughes1, S Peter Gary2 and Joseph Wang1, (1)University of Southern California, Los Angeles, CA, United States, (2)Los Alamos National Laboratory, Los Alamos, NM, United States
 
Forward and Inverse Cascades of Whistler Turbulence: Three-Dimensional Particle-in-Cell Simulations
S Peter Gary, Los Alamos National Laboratory, Los Alamos, NM, United States, Ouliang Chang, Univ. of Southern California, Foster City, CA, United States; Oracle Corp., Redwood Shores, CA, United States and Joseph Wang, University of Southern California, Los Angeles, CA, United States
 
Dissipation Model for Solar Wind Turbulence by Kinetic Alfvén Waves at Electron Scales
Anne Rita Schreiner and Joachim Saur, University of Cologne, Cologne, Germany
 
The anisotropic nature of the intermittent turbulence spectra in the solar wind
Chuan-Yi Tu1, Xin Wang1, Jiansen He1, Eckart Marsch2 and Linghua Wang1, (1)Peking University, Beijing, China, (2)University of Kiel, Kiel, Germany
 
Exploring Plasma Turbulence in the Kronian Magnetosheath Using Cassini Data
Lina Hadid1, Fouad Sahraoui2, Khurom Hussain Kiyani3, Ronan Modolo4, Alessandro Retino5, Patrick Canu5, Adam Masters6 and Michele Karen Dougherty7, (1)Ecole Polytechnique, Palaiseau Cedex, France, (2)Laboratoire de Physique des Plasmas, Saint-Maur Des Fossés Cedex, France, (3)University of Warwick, Coventry, CV4, United Kingdom, (4)UVSQ / LATMOS-IPSL/CNRS-INSU, Guyancourt, France, (5)Laboratoire de Physique des Plasmas, Palaiseau, France, (6)Imperial College London, London, SW7, United Kingdom, (7)Imperial College London, Blackett Laboratory, London, United Kingdom
 
Statistical Study of Magnetic Field Spectra Around Ion Scales: STEREO Observations.
Sonny Lion1, Olga Alexandrova2, Arnaud Zaslavsky1, Filippo G E Pantellini3, Milan Maksimovic4 and Andre Mangeney2, (1)Paris Observatory Meudon, Meudon, France, (2)Paris Observatory, Paris, France, (3)CNRS, Observatoire de Paris, LESIA, Meudon, France, (4)CNRS, Paris Cedex 16, France
 
Solar Wind MHD Turbulence in Coronal Hole and Streamer Belt wind
Junxiang Hu1, Gang Li1 and Bin Miao2, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)USTC University of Science and Technology of China, Hefei, China
 
Large eddy simulations of MHD Turbulence
Rohit Chhiber1, Minping Wan1, Arcadi V. Usmanov1, William H Matthaeus1 and Melvyn L Goldstein2, (1)University of Delaware, Newark, DE, United States, (2)NASA Goddard SFC, Greenbelt, MD, United States
 
Intermittency and Alignment in Strong Reduced Magnetohydrodynamic Turbulence
Benjamin D G Chandran1, Alexander A Schekochihin2 and Alfred Mallet1,2, (1)University of New Hampshire, Durham, NH, United States, (2)University of Oxford, Oxford, United Kingdom
 
LAGRANGIAN MAPPING APPROACH TO GENERATE INTERMITTENCY AND ITS APPLICATION IN PLASMA TURBULENCE
Prachanda Subedi, William H Matthaeus, Jeffrey Tessein, Rohit Chhiber and Minping Wan, University of Delaware, Newark, DE, United States
 
Dynamical Field Line Connectivity in Magnetic Turbulence
David J Ruffolo, Mahidol University, Bangkok, Thailand and William H Matthaeus, Bartol Research Institute and Department of Physics and Astronomy, University of Delaware, Newark, DE, United States
 
Evaluation of Reduced Power Spectra from Three-Dimensional k-Space
Michael von Papen and Joachim Saur, University of Cologne, Cologne, Germany
 
Are There Natural Categories of Solar Wind?
D Aaron Roberts, NASA Goddard Space Flight Center, Code 670, Greenbelt, MD, United States, Tamara Sipes, Curemetrix, Ranch Santa Fe, CA, United States and Homayoun Karimabadi, SciberQuest, Del Mar, CA, United States
 
The isotropic nature of the background turbulence spectra in the solar wind
Xin Wang1, Chuan-Yi Tu1, Jiansen He1, Eckart Marsch2 and Linghua Wang1, (1)Peking University, Beijing, China, (2)University of Kiel, Kiel, Germany
 
Three Dimensional Probability Distributions of the Interplanetary Magnetic Field
John J Podesta, Space Science Institute, Center for Space Plasma Physics, Boulder, CO, United States
 
Strength of Linear and Nonlinear Accelerations in MHD Turbulence: Global versus Local Measures
Sanjoy Ghosh, Johns Hopkins University, Laurel, MD, United States and Tulasi Parashar, University of Delaware, Newark, DE, United States
 
Solar-cycle dependence of a model turbulence spectrum using IMP and ACE observations over 38 years
Renier Adriaan Burger, Amore E Nel and Nicholas Eugene Engelbrecht, North-West University, Mahikeng, South Africa
 
Anisotropy of the cascade in MHD turbulence
Andrea Verdini, Università di Firenze, Dipartimento di Fisica e Astronomia, Firenze, Italy; Royal Observatory of Belgium, Brussels, Belgium, Roland Grappin, LUTH, Observatoire de Paris and LPP, Ecole Polytechnique, Paris, France, Petr Hellinger, Astronomical Institute AS CR, Prague, Czech Republic, Simone Landi, University of Florence, Florence, Italy and Wolf-Christian Muller, Technical University Berlin, Berlin, Germany
 
Stochastic perpendicular ion heating in Hall MHD
Qian Xia1, Stanislav Boldyrev1 and Benjamin D G Chandran2, (1)University of Wisconsin Madison, Madison, WI, United States, (2)University of New Hampshire, Durham, NH, United States