SH53A
Evolution of Solar Wind Transients through the Heliosphere and Associated Space Weather Effects II Posters

Friday, 18 December 2015: 13:40-18:00
Poster Hall (Moscone South)
Primary Conveners:  Ying D. Liu, NSSC National Space Science Center, CAS, Beijing, China
Conveners:  Noé Lugaz, University of New Hampshire Main Campus, Durham, NH, United States, Neel Savani, George Mason University Fairfax, Fairfax, VA, United States and Lan Jian, University of Maryland College Park, College Park, MD, United States
Chairs:  Noé Lugaz, University of New Hampshire, Durham, NH, United States and Neel Savani, NASA Goddard Space Flight Center, Greenbelt, MD, United States; University of Maryland Baltimore County, Baltimore, MD, United States
OSPA Liaisons:  Ying D. Liu, NSSC National Space Science Center, CAS, Beijing, China
 
The role of active region coronal magnetic fi eld in determining coronal mass ejection propagation direction (60252)
Rui Wang1, Ying D. Liu1, Xinghua Dai2, Zhongwei Yang1, Chong Huang3 and Hu Huidong1, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China, (3)Institute of Space Sciences and School of Space Science and Physics, Shandong University, Weihai, China
 
Low Solar Wind Density Causing the Fast Coronal Mass Ejection from 23 July 2012 (58698)
Manuela Temmer, University of Graz, Graz, Austria and Nariaki Nitta, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
 
On Streamer-Blowout CMEs That Aren’t Really CMEs: How the Corona Makes Slow Flux Rope-Like ICMEs Without an Explosive Release of Free Magnetic Energy (84630)
Benjamin J Lynch1, Sophie Masson2, Yan Li1, C Richard DeVore2, Janet G Luhmann1 and Spiro K Antiochos3, (1)University of California Berkeley, Berkeley, CA, United States, (2)NASA GSFC, Greenbelt, MD, United States, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Coincidence of Heliospheric Current Sheet and Stream Interface: Implications for the Origin and Evolution of the Solar Wind (67852)
Jia Huang1, Yong Liu1, Berndt Klecker2 and Yao Chen3, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)Max Planck Institut for Extraterrestrial Physics, Garching, Germany, (3)Shandong Univ. at Weihai, Weihai, Shandong, China
 
At What Distance are CME Deflections Determined? (61035)
Christina Kay and Merav Opher, Boston University, Boston, MA, United States
 
Using ForeCAT to constrain the initial parameters of the 2010 August 14 CME in the low corona. (63832)
Vivek Anand Pisharody, Cornell University, Ithaca, NY, United States
 
Comparison of Analytical Models of Propagation of CMEs and its Validation Using Type II Radio Bursts Observations (64787)
Carlos Arturo Perez Alanis, Ernesto Aguilar-Rodriguez and Pedro Corona Romero, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico
 
Radio emission before, during and after the interaction between two coronal mass ejections in the interplanetary medium (86382)
Tatiana Niembro1, Alejandro Lara1, Alejandro Raga1 and Ricardo González2, (1)Universidad Nacional Autonoma de Mexico, Mexico City, Mexico, (2)Instituto de Radioastronomía y Astrofísica, UNAM, Morelia, Michoacán, Mexico
 
Understanding the Nature of Collision of CMEs in the Heliosphere (62459)
Wageesh Mishra and Yuming Wang, University of Science and Technology of China, Hefei, China
 
First Results on Visualization and Verification of the STEREO Heliospheric Imager CME Catalogue with In Situ Data from the Heliophysics System Observatory (66910)
Christian Moestl1,2, Tanja Rollett2, Peter D Boakes1, Alexey Isavnin3, Jackie A Davies4, Jason Byrne4, David Barnes5,6, Simon W Good7, Christopher H Perry4, Manuel Kubicka2, Richard Anthony Harrison4, Emilia Kilpua8, Robert J Forsyth7 and Volker Bothmer9, (1)University of Graz, Institute of Physics, Graz, Austria, (2)Space Research Institute, Austrian Academy of Sciences, Graz, Austria, (3)University of Helsinki, Department of Physics, Helsinki, Finland, (4)Rutherford Appleton Laboratory, Didcot, United Kingdom, (5)Rutherford Appleton Laboratory, Didcot, OX11, United Kingdom, (6)University College London, London, United Kingdom, (7)Imperial College London, London, United Kingdom, (8)University of Helsinki, Helsinki, Finland, (9)University of Göttingen, Göttingen, Germany
 
Modelling the force balance of magnetic flux ropes between the Sun and 1AU: application to space weather predictions (79879)
Michael Lavarra, IRAP, Toulouse, France
 
Ensemble Modeling within the WSA-Enlil Solar Wind Model (74051)
Michele D Cash, CIRES, Boulder, CO, United States, Victor J Pizzo, NOAA Boulder, Boulder, CO, United States, Curt A de Koning, University of Colorado at Boulder, Boulder, CO, United States, Douglas Alan Biesecker, NOAA Boulder, SWPC, Boulder, CO, United States and Dusan Odstrcil, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Interplanetary Coronal Mass Ejections from MESSENGER Orbital Observations at Mercury  (75979)
Reka Moldovan Winslow1, Noé Lugaz1, Lydia C Philpott2, Nathan Schwadron3, Charles J Farrugia1, Brian J Anderson4 and Charles William Smith1, (1)University of New Hampshire Main Campus, Durham, NH, United States, (2)University of British Columbia, Department of Earth, Ocean and Atmospheric Sciences, Vancouver, BC, Canada, (3)University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States, (4)Johns Hopkins University, Baltimore, MD, United States
 
Determining the significance of CME evolutionary effects during interplanetary propagation for Bz forecasting (82480)
Neel Savani, George Mason University Fairfax, Fairfax, VA, United States
 
Plasma and Magnetic Field Characteristics of Coronal Mass Ejections in Relation to Geomagnetic Storm Intensity and Variability (60201)
Ying D. Liu1, Hu Huidong1, Rui Wang1, Zhongwei Yang1, Zhu Bei1, Liu A. Yi1, Janet G Luhmann2 and John D Richardson3, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)University of California Berkeley, Berkeley, CA, United States, (3)MIT, Cambridge, MA, United States
 
Multipoint Data Analysis of the Poloidal Motion inside a Magnetic Cloud (63338)
A Ke Zhao, University of Science and Technology of China, Hefei, China
 
Multispacecraft study of interplanetary shocks at 1 AU.  (70997)
Xochitl Blanco-Cano, UNAM, Mexico, Mexico
 
STEREO Observations of Small Transients in the Solar Wind at 1 AU (2007-2014) and Comparison with Near – Earth Results from Wind (1995 - 2014) (78764)
Wenyuan Yu1, Charles J Farrugia1, Antoinette Broe Galvin2, Noé Lugaz1, Janet G Luhmann3 and Kristin Simunac4, (1)University of New Hampshire Main Campus, Durham, NH, United States, (2)Univ of New Hampshire, Durham, NH, United States, (3)University of California Berkeley, Berkeley, CA, United States, (4)Organization Not Listed, Washington, DC, United States
 
Multi-spacecraft Characterization of Current Sheet Crossings in the Dynamic Solar Wind (82635)
Natalie D. Foster1,2, Michael Louis Stevens3, Douglas Alan Biesecker4, Anthony W Case3, Justin Christophe Kasper5, Andriy Koval6 and Adam Szabo6, (1)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (2)University of Florida, Astronomy, Gainesville, FL, United States, (3)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (4)NOAA Boulder, SWPC, Boulder, CO, United States, (5)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Investigating the Solar Energetic Particle (SEP) Events Occurred During Solar Cycle 24 (63599)
Rashmi Rawat1, Ezequiel Echer2 and Walter D Gonzalez2, (1)Inst Nac Pesquisas Espaciais, sao jose dos campos, SP, Brazil, (2)INPE National Institute for Space Research, Sao Jose dos Campos, Brazil
 
Modeling Extreme Solar Energetic Particle Acceleration with Self-Consistent Wave Generation (76213)
Aaron Douglas Arthur, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States; University of Alabama in Huntsville, Huntsville, AL, United States
 
Particle Acceleration Affected by the Evolving Velocity Structures in the Solar Wind (72022)
Ken Tsubouchi, Tokyo Institute of Technology, Tokyo, Japan
 
Abundance and Source Population of Suprathermal Heavy Ions in Corotating Interaction Regions (71559)
Rachael Jo Jensema1, Mihir Indrajit Desai2, Thomas W Broiles2 and Maher A Dayeh2, (1)Southwest Research Institute San Antonio, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, TX, United States
 
Forbush Effects on the Martian Surface and Earth’s Poles (81698)
Arik Posner1, Jingnan Guo2, Bernd Heber2, R F Wimmer-Schweingruber2, Cary Zeitlin3,4, Yihua Zheng5, Peter J MacNeice5, Dusan Odstrcil5, Lutz Rastaetter5, Christian T Steigies6, John P Andrews3, Jan Kristoffer Appel2, Rudolf Beaujean6, Lars Berger2, Stephan I Böttcher2, David E Brinza7, Mark Bullock3, Soenke Burmeister2, Francis Cucinotta8, Nina Dresing2, Christian Drews2, Bent Ehresmann3, Michael E Epperly9, Don Hassler3, Konstantin Herbst2, Myung-Hee Y Kim10, Jan Kohler2, Patrick Kühl2, Henning Lohf2, Cesar Martin-Garcia2, Reinhold Müller-Mellin2, Kerry Neal3, Scot CR Rafkin3, Gunther Reitz11, Kelly D Smith9, Yvette Tyler9 and Gerald weigle II12, (1)NASA Headquarters, Washington, DC, United States, (2)University of Kiel, Kiel, Germany, (3)Southwest Research Institute Boulder, Boulder, CO, United States, (4)NASA Johnson Space Center, Houston, TX, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (6)Christian-Albrechts-Universität zu Kiel, Kiel, Germany, (7)Jet Propulsion Laboratory, Pasadena, CA, United States, (8)University of Nevada Las Vegas, Las Vegas, NV, United States, (9)Southwest Research Institute, San Antonio, TX, United States, (10)Organization Not Listed, Washington, DC, United States, (11)DLR, Cologne, Germany, (12)Big Head Endian, San Antonio, TX, United States
 
Heliospheric and Geomagnetic Modulation of Galactic Cosmic Ray under Quiet and disturbed interplanetary conditions during Solar cycle 20-23. (62664)
Florence Darlene Kalu, University of Nigeria, Nsukka, Nigeria
 
Impact of pickup ions on the shock front nonstationarity andenergy dissipation of the heliospheric termination shock:Two-dimensional full particle simulations and comparison withVoyager 2 observations (60245)
Zhongwei Yang1, Ying Liu1, John D Richardson2, Quanming Lu3, Can Huang4 and Rui Wang1, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)MIT, Cambridge, MA, United States, (3)USTC University of Science and Technology of China, Hefei, China, (4)University of Science and Technology of China, Hefei, China
 
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