SH33A:
Plasma Properties of the Solar Corona and Solar Wind: Sources Versus Evolution II Posters

Session ID#: 3127

Wednesday, 17 December 2014: 1:40 PM-6:00 PM
Poster Hall (Moscone_South)
Chairs:  Chadi S Salem, University of California, Berkeley, United States and Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States
Primary Convener:  Chadi S Salem, University of California, Berkeley, United States
Co-conveners:  Marco C M Velli, Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States and Roberto Lionello, Predictive Science Inc., San Diego, United States
OSPA Liaison:  Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States
Index Terms:

2164 Solar wind plasma [INTERPLANETARY PHYSICS]
2169 Solar wind sources [INTERPLANETARY PHYSICS]
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7511 Coronal holes [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
Virtual Option?: No

Abstracts Submitted to this Session:

 
Heliospheric Tomography from IPS Data at 140 MHz (19137)
Julio Cesar Mejia-Ambriz, University of California San Diego, La Jolla, CA, United States; Universidad Nacional Autonoma de Mexico, Mexico City, Mexico, Bernard V Jackson, University of California, San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, Americo Gonzalez-Esparza, Universidad Nacional Autonoma de Mexico, Instituto de Geofisica, Unidad Michoacan, Morelia, Mexico and Andrew Buffington, University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States
 
Validation of Coronal and Heliospheric Models for Quasi-Steady Solar Wind: WSA-Enlil, MAS-Enlil, SWMF, and IPS Tomography Models (18422)
Lan Jian1,2, Peter J MacNeice3, Aleksandre Taktakishvili3,4, Rebekah M Evans1,5, Dusan Odstrcil1,6, Charles Nickolos Arge7, Bernard V Jackson8, Hsiu-Shan Yu9, Pete Riley10 and Igor Sokolov11, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)University of Maryland, College Park, College Park, MD, United States, (3)NASA Goddard Space Flight Center, Community Coordinated Modeling Center, Greenbelt, MD, United States, (4)Catholic University of America, Washington, United States, (5)George Mason University Fairfax, Fairfax, VA, United States, (6)George Mason University Fairfax, Physics and Astronomy, Fairfax, VA, United States, (7)NASA Goddard Space Flight Center, Greenbelt, United States, (8)University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (9)Univ California San Diego, La Jolla, CA, United States, (10)Predictive Science Inc., San Diego, CA, United States, (11)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States
 
Modeling the heating and the acceleration of the fast solar wind ion (26445)
Leon Ofman, Catholic University of America, Physics, Washington, DC, United States and Adolfo F. Vinas, NASA Goddard Space Flight Center, Heliophysics Division, Geospace Physics Laboratory, Mail Code 673, Greenbelt, MD, United States
 
A Nonlinear Model for Dynamics in the Expanding Accelerating Solar Wind (26405)
Anna Tenerani, California Institute of Technology, Pasadena, CA, United States and Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States
 
Pseudostreamers: Formation, Magnetic Topology and Plasma Properties (29806)
Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States and Marco C M Velli, University of California Los Angeles, Earth Planetary and Space Sciences, Los Angeles, United States
 
Coronal Hole Boundaries as Source Regions of a Steady Slow Solar Wind: Global Modeling of Charge State Composition and Sun-to-Earth Observations (32120)
Rona Oran1, Enrico Landi2, Bart van der Holst3, Susan T Lepri4, Ward Manchester3, Richard A Frazin5, Federico Nuevo6, Alberto M Vásquez6, Igor Sokolov7 and Tamas I Gombosi3, (1)Univ of Michigan--AOSS, Ann Arbor, United States, (2)University of Michigan, Ann Arbor, MI, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (4)University of Michigan, Ann Arbor, United States, (5)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (6)Instituto de Astronoma y Fsica del Espacio, Buenos Aires, Argentina, (7)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, United States
 
Global Variation of the Coronal Electron Density with Solar Cycle and its Comparison with 3D MHD Modeling (30587)
Nelson Leslie Reginald, NASA GSFC, Greenbelt, United States, Tongjiang Wang, Catholic University of America and NASA GSFC, Washington, United States and Joseph M Davila, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
How Well Does the S-Web Theory Predict In-Situ Observations of the Slow Solar Wind? (24169)
Aleida Katherine Higginson, University of Michigan, AOSS, Ann Arbor, United States, Spiro K Antiochos, NASA GSFC, Greenbelt, United States, Jon Linker, Predictive Science Inc., San Diego, CA, United States and Thomas Zurbuchen, University of Michigan Ann Arbor, Ann Arbor, MI, United States
 
Sources of the Mid-Latitude Fast Solar Wind (17032)
Mark Stakhiv1, Enrico Landi1, Susan T Lepri2, Thomas Zurbuchen3 and Rona Oran4, (1)University of Michigan, Ann Arbor, MI, United States, (2)University of Michigan, Ann Arbor, United States, (3)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (4)Univ of Michigan--AOSS, Ann Arbor, United States
 
Elemental building blocks of the slow solar wind (29136)
Larry Kepko1, Nicholeen M Viall1 and Susan T Lepri2, (1)NASA GSFC, Greenbelt, United States, (2)University of Michigan, Ann Arbor, United States
 
Solar Wind C, N, and O Abundances and the Solar Metallicity (8393)
Rudolf von Steiger1,2, Thomas Zurbuchen3, Paul Shearer3 and Jason A Gilbert3, (1)International Space Science Institute, Bern, Switzerland, (2)University of Bern, Physikalisches Institut, Bern, Switzerland, (3)University of Michigan, Ann Arbor, MI, United States
 
Minor Ion Species in the Solar Wind As Seen with SOHO/Celias/Mtof (6821)
Verena Heidrich-Meisner1, Lars Berger2, Robert F Wimmer-Schweingruber1, Peter Wurz3, Peter A Bochsler4, Fred M Ipavich5, George Gloeckler6, Berndt Klecker7 and John Anthony Paquette7, (1)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (2)Kiel University, Kiel, Germany, (3)University of Bern, Space Research and Planetary Sciences, Bern, Switzerland, (4)University of Bern, Bern, Switzerland, (5)Univ of Maryland, College Park, MD, United States, (6)Univ Michigan, Ann Arbor, MI, United States, (7)Max Planck Institut for Extraterrestrial Physics, Garching, Germany
 
Solar Corona/Wind Composition and Origins of the Solar Wind (Invited) (5183)
Susan T Lepri1, Jason A Gilbert1, Enrico Landi1, Paul Shearer1, Rudolf von Steiger2 and Thomas Zurbuchen1, (1)University of Michigan, Ann Arbor, MI, United States, (2)International Space Science Institute, Bern, Switzerland
 
Heavy Ion Temperatures As Observed By ACE/Swics (8760)
Patrick Tracy1, Thomas Zurbuchen1, Jim M Raines2, Paul Shearer1, Justin Christophe Kasper3, Jason A Gilbert4 and Benjamin L Alterman1, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Michigan, Ann Arbor, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (4)University of Michigan, Ann Arbor, MI, United States
 
Two-Point Observations of High- and Low-Frequency Variations of Helium Abundance in the Solar Win (10113)
Jana Safrankova1, Petr Cagas2, Zdenek Nemecek1, Lubomir Prech2, Georgy N Zastenker3 and Maria Riazantseva4,5, (1)Charles University, Prague, 180, Czech Republic, (2)Charles University, Prague, Czech Republic, (3)Inst Space Research, Moscow, Russia, (4)Moscow State University, Moscow, Russia, (5)Space Research Institute of the Russian Academy of Sciences (IKI), Moscow, Russia
 
Heavy Ion Heating at Shocks in the Heliosphere (12882)
Kelly E Korreck, Smithsonian Astrophysical Observatory, Cambridge, United States, Michael Louis Stevens, Smithsonian Astrophysical Observatory, Cambridge, MA, United States, Susan T Lepri, University of Michigan, Ann Arbor, United States and Justin Christophe Kasper, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States
 
Multi-spacecraft Observations of Heavy Ion Dropouts: Physical Processes, Fractionation Rates, and Release Mechanisms (18501)
Micah J Weberg, US National Research Council of the National Academies, NRC Research Associate, Washington, DC, United States, Susan T Lepri, University of Michigan, Ann Arbor, United States and Thomas Zurbuchen, University of Michigan Ann Arbor, Ann Arbor, MI, United States
 
High-Time Resolution Measurements of Heavy Ions with SOHO/CELIAS/CTOF (15781)
Nils Peter Janitzek1, Lars Berger2, Christian Drews3, Peter A Bochsler4, Berndt Klecker5 and Robert F Wimmer-Schweingruber3, (1)University of Kiel, Kiel, Germany, (2)Kiel University, Kiel, Germany, (3)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (4)University of Bern, Bern, Switzerland, (5)Max Planck Institut for Extraterrestrial Physics, Garching, Germany
 
A Survey of Velocity Distributions of Solar Wind Ions : ACE/SWICS observations (21459)
Lars Berger, Kiel University, Kiel, Germany, Eckart Marsch, University of Kiel, Kiel, Germany and Robert F Wimmer-Schweingruber, University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany
 
Electron cooling between 0.3 and 1 AU from Helios observations (20728)
Ondrej Sebek1, Stepan Stverak1, Pavel M. Travnicek2 and Petr Hellinger1, (1)Astronomical Institute AS CR, Prague, Czech Republic, (2)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
 
Thermodynamics of Solar Wind Core, Halo and Strahl Electrons: Properties, Regulation and Constraints (27602)
Chadi S Salem1, Marc Pulupa2 and Stuart D Bale2, (1)SSL, University of California Berkeley, Berkeley, United States, (2)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
 
The Electron Heat flux in the Solar Wind: Collisionless or Collisional Dominated? (16034)
Simone Landi, University of Florence, Florence, Italy, Filippo G E Pantellini, CNRS, Observatoire de Paris, LESIA, Meudon, France and Lorenzo Matteini, Observatoire De Paris, LESIA, Meudon, FRANCE
 
Effects of electron drifts on collisionless damping of Alfvén waves (14255)
Yuguang Tong, University of California Berkeley, Berkeley, CA, United States, Stuart D Bale, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States and Christopher H K Chen, Queen Mary University of London, Department of Physics and Astronomy, London, United Kingdom
 
Role of Compressibility in the Evolution of Solar Wind Alfvénicity (5084)
Raffaella D'Amicis and Roberto Bruno, IAPS-INAF, Rome, Italy
 
Plasma Beta Dependence of Magnetic Compressibility in Solar Wind Turbulence (12684)
Bogdan Hnat, University of Warwick, Coventry, United Kingdom, Khurom Hussain Kiyani, University of Warwick, Coventry, CV4, United Kingdom, Sandra C Chapman, University of Warwick, Centre for Fusion, Space and Astrophysics, Department of Physics, Coventry, CV4, United Kingdom and Fouad Sahraoui, Laboratoire de Physique des Plasmas, Palaiseau, France
 
High-Frequency Waves Associated with Collisionless Shocks (10119)
Oleksandr Goncharov1, Zdenek Nemecek1, Jana Safrankova1, Lubomir Prech2 and Georgy N Zastenker3, (1)Charles University, Prague, 180, Czech Republic, (2)Charles University, Prague, Czech Republic, (3)Inst Space Research, Moscow, Russia
 
Kinetic Effects in Parametric Instabilities of Finite Amplitude Alfven Waves in a Drifting Multi-Species Plasma (8487)
Yana G Maneva, KU Leuven, CmPA, Dover, NH, United States, Jaime A Araneda, Univ. Concepcion, Concepcion, Chile and Stefaan Poedts, KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium
 
A Gyrokinetic Approach to Low Frequency Anisotropy-Driven Instabilities in the Solar Wind (25904)
Jay Johnson, Andrews University, Berrien Springs, United States and Peter Porazik, Princeton Plasma Physics Lab, Princeton, NJ, United States
 
Role of Parallel and Oblique Ion-Cyclotron Waves in Heating Ions in an Inhomogeneous Expanding Solar Wind Plasma (28932)
Nataly O Ozak, Weizmann Institute of Science, Rehovot, Israel, Leon Ofman, Catholic University of America, Physics, Washington, DC, United States; NASA Goddard Space Flight Center, Greenbelt, United States and Adolfo F. Vinas, NASA Goddard Space Flight Center, Heliophysics Division, Geospace Physics Laboratory, Mail Code 673, Greenbelt, MD, United States
 
Proton-Cyclotron and Firehose Instabilities in Inhomogeneous Solar Wind (3594)
Peter H Yoon, Univ Maryland, College Park, MD, United States and Jungjoon Seough, KASI Korea Astronomy and Space Science Institute, Daejeon, South Korea
 
Generation of suprathermal protons via parallel electron fire-hose instability: Particle-in-cell simulations  (28283)
Jungjoon Seough1, Peter H Yoon2, Junga Hwang1 and Khan-Hyuk Kim3, (1)KASI Korea Astronomy and Space Science Institute, Daejeon, Korea, Republic of (South), (2)Univ Maryland, College Park, MD, United States, (3)Kyung Hee University, School of Space Research, Yongin, South Korea
 
Symmetry Properties of Proton Velocity Distributions: a Vlasov Simulation Study of the Ion Cyclotron Instability (29451)
Jaime A Araneda, Univ. Concepcion, Concepcion, Chile, Rodrigo A López, University of Santiago Chile, Santiago, Chile and Adolfo F. Vinas, NASA Goddard Space Flight Center, Heliophysics Division, Geospace Physics Laboratory, Mail Code 673, Greenbelt, MD, United States