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

Session ID#: 1576

Friday, 19 December 2014: 8:00 AM-12:20 PM
Poster Hall (Moscone_South)
Chairs:  Kareem Osman1, Minping Wan2, Prof. William H Matthaeus3 and Khurom Hussain Kiyani1, (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:

 
Twins: A New Mission to Solve the Problem of Turbulence and Energy Dissipation at Electron Scales in the Solar Wind (10053)
Fouad Sahraoui, Laboratoire de Physique des Plasmas, Palaiseau, France
 
M⁴ - a mission candidate for ESA M4 (29018)
Andris Vaivads, Royal Institute of Technology, KTH, Space and Plasma Physics, Stockholm, Sweden, Alessandro Retino, CNRS, Paris Cedex 16, France and M⁴ team
 
The Effects of Ion Kinetic Instabilities on the Three-Dimensional Reconnection of Ion-Scale Current Sheets in the Solar Wind (10453)
David Burgess, Queen Mary, University of London, London, United Kingdom, Peter Gingell, Queen Mary, University of London, London, E1, United Kingdom and Lorenzo Matteini, Observatoire De Paris, LESIA, Meudon, FRANCE
 
Alfvénic Turbulence and Kinetic Instabilities in the Expanding Solar Wind: Two-Dimensional Hybrid Simulations (13806)
Lorenzo Matteini1, Petr Hellinger2, Simone Landi3, Luca Franci4, Andrea Verdini5,6 and Pavel M. Travnicek2,7, (1)Observatoire De Paris, LESIA, Meudon, FRANCE, (2)Astronomical Institute, AS CR, Prague, Czech Republic, (3)Università degli Studi di Firenze, Florence, Italy, (4)Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom, (5)Università di Firenze, Dipartimento di Fisica e Astronomia, Firenze, Italy, (6)Royal Observatory of Belgium, Brussels, Belgium, (7)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
 
Electron and Ion Heating By Whistler Turbulence: Three-Dimensional Particle-in-Cell Simulations (7540)
Randall Scott Hughes, University of Southern California, Los Angeles, CA, United States, Stephen Peter Gary, Los Alamos National Laboratory, Los Alamos, NM, United States and Joseph Wang, University of Southern California, Department of Astronautical Engineering, Los Angeles, United States
 
Forward and Inverse Cascades of Whistler Turbulence: Three-Dimensional Particle-in-Cell Simulations (28451)
Stephen 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, Department of Astronautical Engineering, Los Angeles, United States
 
Dissipation Model for Solar Wind Turbulence by Kinetic Alfvén Waves at Electron Scales (14987)
Anne Schreiner, University of Cologne, Institute of Geophysics and Meteorology, Cologne, Germany and Joachim Saur, University of Cologne, Cologne, Germany
 
The anisotropic nature of the intermittent turbulence spectra in the solar wind (15169)
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 (6838)
Lina Hadid1, Fouad Sahraoui2, Khurom Hussain Kiyani3, Ronan Modolo4, Alessandro Retino5, Patrick Canu2, Adam Masters6 and Michele Karen Dougherty7, (1)Ecole Polytechnique, LPP-CNRS, Palaiseau Cedex, France, (2)Laboratoire de Physique des Plasmas, Palaiseau, France, (3)University of Warwick, Coventry, CV4, United Kingdom, (4)LATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, Guyancourt, France, (5)Laboratoire de Physique des Plasmas, CNRS/Sorbonne Université/Univ. Paris Saclay/Obs. de Paris/ Ecole Polytechnique, Institut Polytechnique de Paris, Palaiseau, France, (6)Imperial College London, Department of Physics, London, United Kingdom, (7)Imperial College London, London, United Kingdom
 
Statistical Study of Magnetic Field Spectra Around Ion Scales: STEREO Observations. (25485)
Sonny Lion, Observatoire de Paris, PSL, CNRS, LESIA, Meudon, France, Olga Alexandrova, Observatoire de Paris, LESIA, Meudon, France, Arnaud Zaslavsky, Paris Observatory Meudon, Meudon, France, Filippo G E Pantellini, CNRS, Observatoire de Paris, LESIA, Meudon, France, Milan Maksimovic, LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, Meudon, France, Meudon, France and Andre Mangeney, LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France
 
Solar Wind MHD Turbulence in Coronal Hole and Streamer Belt wind (27562)
Junxiang Hu, NASA Goddard Space Flight Center, Code 671, Greenbelt, United States, Gang Li, University of Alabama in Huntsville, Department of Space Sciences and CSPAR, Huntsville, AL, United States and Bin Miao, USTC University of Science and Technology of China, Hefei, China
 
Large eddy simulations of MHD Turbulence (31756)
Dr. Rohit Chhiber, BSc (Honours), MSc, PhD1, Minping Wan2, Arcadi V. Usmanov3, Prof. William H Matthaeus3 and Melvyn L Goldstein4, (1)University of Delaware, Department of Physics and Astronomy, Newark, United States, (2)University of Delaware, Newark, United States, (3)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (4)Space Science Institute Boulder, Boulder, United States
 
Intermittency and Alignment in Strong Reduced Magnetohydrodynamic Turbulence (9060)
Benjamin D G Chandran1, Alexander A Schekochihin2 and Alfred Mallet2,3, (1)University of New Hampshire, Durham, United States, (2)University of Oxford, Oxford, United Kingdom, (3)University of New Hampshire, Durham, NH, United States
 
LAGRANGIAN MAPPING APPROACH TO GENERATE INTERMITTENCY AND ITS APPLICATION IN PLASMA TURBULENCE (31757)
Prachanda Subedi1, Prof. William H Matthaeus2, Jeffrey Tessein1, Dr. Rohit Chhiber, BSc (Honours), MSc, PhD3 and Minping Wan4, (1)University of Delaware, Newark, DE, United States, (2)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (3)University of Delaware, Department of Physics and Astronomy, Newark, United States, (4)University of Delaware, Newark, United States
 
Dynamical Field Line Connectivity in Magnetic Turbulence (14410)
David J Ruffolo, Mahidol University, Bangkok, Thailand and Prof. 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 (5830)
Michael von Papen and Joachim Saur, University of Cologne, Cologne, Germany
 
Are There Natural Categories of Solar Wind? (13881)
D Aaron Roberts, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Tamara Sipes, Curemetrix, Ranch Santa Fe, CA, United States and Homayoun Karimabadi, Analytics Ventures, San Diego, CA, United States
 
The isotropic nature of the background turbulence spectra in the solar wind (15103)
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 (15925)
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 (18742)
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 (20865)
Renier Adriaan Burger1, Amore E Nel1 and Nicholas Eugene Engelbrecht2, (1)North-West University, Mahikeng, South Africa, (2)North-West University, Potchefstroom, South Africa
 
Anisotropy of the cascade in MHD turbulence (22299)
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 Prof. Wolf-Christian Muller, Technische Universität Berlin, Plasma-Astrophysics, Berlin, Germany
 
Stochastic perpendicular ion heating in Hall MHD (28278)
Qian Xia, Northumbria University, Newcastle-Upon-Tyne, United Kingdom, Stanislav Boldyrev, University of Wisconsin Madison, Madison, WI, United States and Benjamin D G Chandran, University of New Hampshire, Durham, United States