SH53B
Solar and Heliospheric Physics General Contributions II Posters

Friday, 18 December 2015: 13:40-18:00
Poster Hall (Moscone South)
Primary Conveners:  Todd Hoeksema, Stanford University, Stanford, CA, United States
Conveners:  Robyn M Millan, Dartmouth College, Hanover, NH, United States and Anja Stromme, SRI International Menlo Park, Menlo Park, CA, United States
Chairs:  J Todd Hoeksema, Stanford University, Stanford, CA, United States and Ruizhu Chen, Stanford University, W. W. Hansen Experimental Physics Laboratory, Stanford, CA, United States
OSPA Liaisons:  J Todd Hoeksema, Stanford University, Stanford, CA, United States
 
Vortex Identification in the Lower Solar Atmosphere (73367)
Viktor Fedun, University of Sheffield, Sheffield, S10, United Kingdom, Ioannis Giagkiozis, University of Sheffield, Sheffield, United Kingdom, Gary Verth, University of Sheffield, School of Mathematics and Statistics, Sheffield, United Kingdom and Eamon Scullion, Trinity College Dublin, Dublin, Ireland
 
Exploring the properties of Solar Prominence Tornados (76438)
Esraa Ahmad1, Navdeep Kaur Panesar2, Alphonse C Sterling3 and Ronald L Moore3, (1)University of Massachusetts Boston, Chemistry, Boston, MA, United States, (2)University of Alabama in Huntsville, Huntsville, AL, United States, (3)NASA Marshall Space Flight Center, Huntsville, AL, United States
 
Magnetic Structure and Formation of On-disk Coronal Plumes (65397)
Sarah Antonsson1, Sanjiv K Tiwari2, Ronald L Moore2 and Amy R Winebarger2, (1)University of the Pacific, Stockton, CA, United States, (2)NASA Marshall Space Flight Center, Huntsville, AL, United States
 
Investigation of the Possible Trigger Mechansims of an Erupting Prominence (67598)
Luis A. Ortiz Flores, Organization Not Listed, Washington, DC, United States
 
Dissipationless Damping of Compressive MHD Modes in Twisted Flux Tubes (72605)
Ioannis Giagkiozis, University of Sheffield, Sheffield, United Kingdom, Viktor Fedun, University of Sheffield, Sheffield, S10, United Kingdom, Gary Verth, University of Sheffield, School of Mathematics and Statistics, Sheffield, United Kingdom and Marcel L. Goossens, University of Leuven, Leuven, Belgium
 
Probing Solar Eruption by Tracking Magnetic Cavities and Filaments (76511)
Justin Rashod Johnson, Morehouse College, Atlanta, GA, United States
 
Survey of high-altitude partially erupting prominences (78615)
Holly Robin Gilbert, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Twisting/Rolling Motions and Chirality in Filament Eruptions (84848)
Sean McKillop1, Nicholas A Murphy2, Mari Paz Miralles2, Patrick McCauley1 and Yingna Su3, (1)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (2)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (3)Purple Mountain Observatory, Nanjing, China
 
Simulating the Formation and Evolution of Solar Prominences in Coronal Cavities (78021)
Chun Xia, KU Leuven, Dover, NH, United States and R. Keppens, Katholieke Universiteit Leuven, Leuven, Belgium; KU Leuven, Leuven, NH, United States
 
Morphology and Evolution of a Polar Coronal Mass Ejection (84931)
Iballa Cabello, UTN-FRM and CONICET, Mendoza, Argentina, Laura Antonia Balmaceda, INPE National Institute for Space Research, Sao Jose dos Campos, Brazil, Hebe Cremades, Organization Not Listed, Washington, DC, United States and Ivo Dohmen, Universidad Tecnológica Nacional, Facultad Regional Mendoza, Mendoza, Argentina
 
Newtonian CAFE: a new ideal MHD code to study the solar atmosphere (60566)
José Juan González, Alejandro Cruz, Fabio Lora and Francisco Guzmán, Organization Not Listed, Washington, DC, United States
 
Three-Dimensional Reconstruction of the Electron Density in the Solar Corona (67703)
Luke Walter Burnett1, Douglas W Nychka2, Sarah E Gibson2 and Kévin Dalmasse2, (1)St. Olaf College, Northfield, MN, United States, (2)National Center for Atmospheric Research, Boulder, CO, United States
 

IPS Observations at 140 MHz to Study Solar Wind Speeds and Density Fluctuations by MEXART. (64898)

Oyuki Chang, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico
 
Influence of the Solar Wind Speed on the Propagation of Coronal Mass Ejections (70680)
Seiji Yashiro1,2, Munetoshi Tokumaru3, Ken\'ichi Fujiki3, Tomoya Iju3, Sachiko Akiyama1,2, Pertti A Makela1,2 and Nat Gopalswamy2, (1)Catholic University of America, Washington, DC, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)Nagoya University, Nagoya, Japan
 
Radio Triangulation of Type II Bursts Associated with a CME - CME Interaction (63639)
Vratislav Krupar, Imperial College London, London, United Kingdom
 
Electron Acceleration at Coronal Shocks Propagating Through a Large-scale Streamer-like Magnetic Field (76616)
Xiangliang Kong, Shandong University at Weihai, Weihai, China
 
Polarity Comparison Between the Coronal PFSS Model Field and the Heliospheric Magnetic Field at 1 AU Over Solar Cycles 21-24 (79999)
Jennimari Sofia Koskela, Ilpo Virtanen and Kalevi Mursula, University of Oulu, Oulu, Finland
 
Measurements and an Empirical Model of the Zodiacal Brightness as Observed by the Solar Mass Ejection Imager (SMEI) (61953)
Andrew Buffington1, Mario Mark Bisi2, John M Clover1, P. Paul Hick1, Bernard V Jackson3, Thomas A Kuchar4 and Stephan D. Price4, (1)University of California San Diego, La Jolla, CA, United States, (2)Rutherford Appleton Laboratory, Didcot, United Kingdom, (3)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (4)Boston College, Chestnut Hill, MA, United States
 
Investigation of the dynamics of nanometer-size dust particles in the inner heliosphere (81730)
Leela O'brien, University of Colorado at Boulder, Boulder, CO, United States
 
IPS of the Radio Source 3C48 During the Periods of Low and High Solar Activity (79066)
Ernesto Aguilar-Rodriguez1, S. A. Tyul'bashev2, I. V. Chashei2 and E. Romero-Hernandez1, (1)Universidad Nacional Autonoma de Mexico, Mexico City, Mexico, (2)Lebedev Physical Institute, Pushchino Radio Astronomy Observatory, Moscow, Russia
 
Observations of the Flux Density of Some Interplanetary Type II and Type III Radio Bursts and Initial Comparisons With Theory (82520)
Amaal Abd-Alla Mohamed1,2, Iver Hugh Cairns3, Dean Hillan3 and Peter A Robinson4, (1)George Mason University Fairfax, Fairfax, VA, United States, (2)National research institute of Astronomy and Geophysics, Solar and Space Dept., Cairo, Egypt, (3)University of Sydney, Sydney, Australia, (4)University of Sydney, Sydney, NSW, Australia
 
A mechanism for the Fine Structures of Solar Radio Bursts Based on the Electron Cyclotron Maser Emission (86738)
ChuanBing Wang, USTC University of Science and Technology of China, Hefei, China
 
Interplanetary Coronal Mass Ejection (ICME) and Cosmic rays transmission during Forbush decreases (62643)
Kingsley Chukwudi Okpala, University of Nigeria, Nsukka, Nigeria
 
Loading relativistic Maxwell distributions in particle simulations (81184)
Seiji Zenitani, NAOJ National Astronomical Observatory of Japan, Tokyo, Japan
 
Numerical Study of the Transverse Stability of Compressive and Rarefactive Alfven Solitons (86563)
Robert Hamilton and Charles Haneberg, George Fox University, Newberg, OR, United States
 
Rotationally Asymmetric Magnetic Holes in the Solar Wind (63421)
Mark Anthony Reynolds and Harry Raphael Wheeler IV, Embry-Riddle Aeronautical University, Daytona Beach, FL, United States
 
Non-linear analysis of PESA-Lo electrostatic analyzer data and solar wind temperature anisotropies (63792)
Blagoje Zoran Djordjevic1, Bennett Maruca1, Stuart D Bale1, Lynn B Wilson III2 and Davin E Larson3, (1)University of California Berkeley, Berkeley, CA, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)Space Sciences Laboratory, Berkeley, CA, United States
 
Ion-Driven Instabilities in the Solar Wind: Wind Observations of 19 March 2005 (68673)
S Peter Gary, Los Alamos National Laboratory, Los Alamos, NM, United States, Lan Jian, University of Maryland College Park, College Park, MD, United States, Thomas W Broiles, Southwest Research Institute, San Antonio, TX, United States, Michael Louis Stevens, Smithsonian Astrophysical Observatory, Cambridge, MA, United States, John J Podesta, Space Science Institute Boulder, Center for Space Plasma Physics, Boulder, CO, United States and Justin Christophe Kasper, University of Michigan, Ann Arbor, MI, United States
 
Conservation Laws in Fluids and MHD: MultiSymplectic and Hamiltonian Approaches (72834)
Gary M Webb, University of Alabama in Huntsville, CSPAR, Huntsville, AL, United States and Qiang Hu, University of Alabama in Huntsville, Huntsville, AL, United States