SH33A
Evolution, Dynamics, and Macroscopic Effects of Turbulence in the Heliosphere I Posters

Wednesday, 16 December 2015: 13:40-18:00
Poster Hall (Moscone South)
Primary Conveners:  William H Matthaeus, Department of Physics and Astronomy, University of Delaware, Newark, DE, United States
Conveners:  Melvyn L Goldstein, NASA Goddard SFC, Greenbelt, MD, United States, Sergio Servidio, Universita' della Calabria, Rende, Italy and Sean Oughton, University of Waikato, Hamilton, New Zealand
Chairs:  William H Matthaeus, University of Delaware, Newark, DE, United States, Melvyn L Goldstein, NASA Goddard SFC, Greenbelt, MD, United States and Sean Oughton, University of Waikato, Hamilton, New Zealand
OSPA Liaisons:  William H Matthaeus, Department of Physics and Astronomy, University of Delaware, Newark, DE, United States
 
The Transport of Low-Frequency Turbulence in Astrophysical Flows. II. Solutions for the Super-Alfvenic Solar Wind (63563)
Laxman Adhikari1, Gary Paul Zank2, Roberto Bruno3, Daniele Telloni4, Peter Hunana1, Raffaele Marino5 and Qiang Hu6, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)University of Alabama in Huntsville, Space Science, Huntsville, AL, United States, (3)IAPS-INAF, Rome, Italy, (4)INAF-OATO, Turin, Italy, (5)National Center for Atmospheric Research, Boulder, CO, United States, (6)University of Alabama in Huntsville, Department of Space Science and CSPAR, Huntsville, AL, United States
 
Small scale solar wind turbulence due to nonlinear Alfvén waves (67788)
Sanjay Kumar1, R P Sharma2 and Yong-Jae Moon1, (1)Kyung Hee University, Yongin, South Korea, (2)Indian Institute of Technology Delhi, Centre for Energy Studies, New Delhi, India
 
Low-Amplitude Solar Wind Turbulence: Spectral Features (67883)
Xin Wang1, Chuan-Yi Tu1, Jiansen He1, Eckart Marsch2, Linghua Wang1 and Chadi S Salem3, (1)Peking University, Beijing, China, (2)University of Kiel, Kiel, Germany, (3)University of California Berkeley, Berkeley, CA, United States
 
No evidence that solar wind turbulence can be described by the critical balance theory (67894)
Chuan-Yi Tu1, Eckart Marsch2 and Xin Wang1, (1)Peking University, Beijing, China, (2)University of Kiel, Kiel, Germany
 
Alfvénic fluctuations with power-law spectra propagating sunward within the region from L1 to the Earth's bow shock (67908)
Honghong Wu1, Xin Wang1, Linghua Wang1,2, Chuanyi Tu1,2, Jiansen He1,2 and Eckart Marsch3,4, (1)Peking University, Beijing, China, (2)Peking University, Institute of Space Physics and Applied Technology, Beijing, China, (3)University of Kiel, Kiel, Germany, (4)Institute for Experimental and Applied Physics, Kiel, Germany
 
Complexity Variations in the Interplanetary Magnetic Field between 0.4 and 5.3 AU (70774)
James M Weygand1, Margaret Kivelson1, Marco Velli1, Walter N Gekelman2, Krishan K Khurana1, Vassilis Angelopoulos3 and Raymond J Walker3, (1)University of California Los Angeles, Los Angeles, CA, United States, (2)UCLA, Los Angeles, CA, United States, (3)University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, CA, United States
 
Variance Anisotropy of Solar Wind Velocity and Magnetic Field Fluctuations (71356)
Sean Oughton1, William H Matthaeus2 and Minping Wan2, (1)University of Waikato, Hamilton, New Zealand, (2)University of Delaware, Newark, DE, United States
 
Global MHD Modeling of the Heliosphere with Turbulence Transport and Pickup Protons as Separate Fluid (71605)
Arcadi V. Usmanov1, Melvyn L Goldstein2 and William H Matthaeus1, (1)University of Delaware, Newark, DE, United States, (2)NASA Goddard SFC, Greenbelt, MD, United States
 
Parametric studies of ion and electron heating by whistler turbulence: three dimensional Particle-In-Cell simulations (75583)
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
 
Diffusion of Charged Particles in the Presence of Coherent Structures (76218)
Prachanda Subedi, University of Delaware, Newark, DE, United States
 
Alfvénic fluctuations of ICMEs and high-speed solar wind streams (80518)
Eija Irene Tanskanen, Finnish Meteorological Institute, Helsinki, Finland
 
Scaling of compressible magnetohydrodynamic turbulence in the fast solar wind (82374)
Fouad Sahraoui, Laboratoire de Physique des Plasmas, Saint-Maur Des Fossés Cedex, France
 
CGL and Landau fluid simulations of turbulence (86660)
Peter Hunana, University of Alabama in Huntsville, Huntsville, AL, United States
 
Plasma Heating During Magnetic Reconnection: Implications for Turbulent Dissipation (83084)
Michael A Shay, University of Delaware, Newark, DE, United States
 
Charge pariticle transport in the non-isotropic turbulences (84371)
Peng Sun and Jack R Jokipii, University of Arizona, Tucson, AZ, United States
 
See more of: SPA-Solar and Heliospheric Physics
<< Previous Session | Next Session >>