SH43A:
Connection of Solar Events with the Variability of Space Environments II Posters

Session ID#: 3254

Thursday, 18 December 2014: 1:40 PM-6:00 PM
Poster Hall (Moscone_South)
Chairs:  Fang Shen, National Space Science Center, CAS, Beijing, China, Alexis P Rouillard, IRAP, Toulouse, France, Xue Shang Feng, NSSC National Space Science Center, CAS, Beijing, China and Seiji Yashiro, Catholic University of America, Washington, DC, United States
Primary Convener:  Chin-Chun Wu, Naval Research Lab DC, Washington, DC, United States
Co-conveners:  Kan Liou, JHU/Applied Physics Lab, Laurel, MD, United States, Simon P Plunkett, Naval Research Lab, Washington, DC, United States and Shi Tsan Wu, University of Alabama in Huntsville, Huntsville, AL, United States
Co-Sponsor(s):
  • SA - SPA-Aeronomy
  • SM - SPA-Magnetospheric Physics
Index Terms:

2788 Magnetic storms and substorms [MAGNETOSPHERIC PHYSICS]
7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7851 Shock waves [SPACE PLASMA PHYSICS]
7924 Forecasting [SPACE WEATHER]
Virtual Option?: No

Abstracts Submitted to this Session:

 
Comparisons of characteristics of magnetic clouds and cloud-like structures during 1995-2012 (12399)
Ronald P Lepping, NASA Goddard Space Flight Center, Emeritus, Greenbelt, MD, United States, Chin-Chun Wu, Naval Research Lab DC, Washington, DC, United States and Kan Liou, JHU/Applied Physics Lab, Laurel, MD, United States
 
An Unusual Heliospheric Plasma Sheet Crossing at 1 AU  (12486)
Chin-Chun Wu1, Kan Liou2, Angelos Vourlidas1,2, Ronald P Lepping3, Yi-Ming Wang4, Simon P Plunkett1, Dennis G Socker5 and Shi Tsan Wu6, (1)Naval Research Lab DC, Washington, DC, United States, (2)JHU/Applied Physics Lab, Laurel, MD, United States, (3)NASA Goddard Space Flight Center, Emeritus, Greenbelt, MD, United States, (4)US Naval Research Laboratory, Washington, United States, (5)US Naval Research Laboratory, Washington, DC, United States, (6)University of Alabama in Huntsville, Huntsville, AL, United States
 
Severe to Extreme Solar Storms: Magnetic Field Complexity and Warnings (17666)
Henrik Lundstedt, IRF Swedish Institute of Space Physics Lund, Lund, Sweden
 
Characteristics of solar wind density depletions during solar cycles 23 and 24 (21320)
Keunchan Park1, Jeongwoo Lee1, Suyeon Oh2 and Yu Yi3, (1)Chungnam National University, Daejeon, Korea, Republic of (South), (2)Chonnam National University, Gwangju, Korea, Republic of (South), (3)Chungnam National University, Astronomy and Space Science, Daejeon, South Korea
 
Full Halo Coronal Mass Ejections: Arrival at the Earth (14496)
Chenglong Shen1, Yuming Wang2, Zonghao Pan3, Bin Miao3, Pinzhong Ye3 and Shui Wang2, (1)University Science & Technology of China, Hefei, Anhui, China, (2)University of Science and Technology of China, Hefei, China, (3)USTC University of Science and Technology of China, Hefei, China
 
Coronal shocks properties and their associations with energetic particle events measured near 1AU. (12370)
Alexis P Rouillard, IRAP, Toulouse, France, Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Allan J Tylka, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Chee Keong Ng, George Mason University Fairfax, Fairfax, VA, United States and Christina Cohen, California Institute of Technology, Pasadena, CA, United States
 
Study of Quasi-Homologous Coronal Mass Ejections from Super Active Regions in Solar Cycle 23 (5743)
Lijuan Liu1, Yuming Wang1, Chenglong Shen1, Rui Liu1, Pinzhong Ye1, Shui Wang1 and CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, (1)USTC University of Science and Technology of China, Hefei, China
 
A reexamination of long-duration radial IMF events (14936)
Gilbert Pi1, Jih-Hong Shue2, Chi-Kuang Chao3, Zdenek Nemecek4, Jana Safrankova4 and chia-Hsien Lin1, (1)Institute of Space Science National Central University, Jhongli, Taiwan, (2)National Central University, Department of Space Science and Engineering, Taoyuan, Taiwan, (3)Institute of Space Science and Engineering, National Central University, Taoyuan City, Taiwan, (4)Charles University, Prague, 180, Czech Republic
 
Interaction of magnetic clouds with the Earth’s environment: effects due to the terrestrial bow shock (15323)
Dominique Fontaine, Lucile Turc and Philippe Savoini, LPP - CNRS - Ecole polytechnique - UPMC, Palaiseau, France
 
Multi-Spacecraft Observations of Interplanetary Shocks Near Earth (22492)
Primoz Kajdic, European Space Agency, Villanueva De La Can, Spain, Xochitl Blanco-Cano, Instituto de Geofísica Universidad Nacional Autónoma de México, Mexico City, Mexico and Benoit Lavraud, Laboratoire d'astrophysique de Bordeaux, Pessac, France
 
Global MHD Simulation of the Coronal Mass Ejection on 2011 March 7: from Chromosphere to 1 AU (19211)
Meng Jin1,2, Ward Manchester3, Bart van der Holst3, Igor Sokolov3, Gabor Toth3, Angelos Vourlidas4, Curt A de Koning5 and Tamas I Gombosi3, (1)SETI Institute, Mountain View, United States, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)University of Colorado at Boulder, Boulder, CO, United States
 
Could the Collision of CMEs in the Heliosphere be Super-Elastic? (ii) Influence of the Initial Speed of CMEs on Their Collision Process (11214)
Fang Shen, National Space Science Center, CAS, Beijing, China, Yuming Wang, University of Science and Technology of China, Hefei, China, Chenglong Shen, University Science & Technology of China, Hefei, Anhui, China and Xue Shang Feng, CSSAR, Beijing, China
 
Real­-Time Ensemble Forecasting of Coronal Mass Ejections Using the Wsa-Enlil+Cone Model (8209)
M. Leila Mays1,2, Aleksandre Taktakishvili2,3, Antti A Pulkkinen4, Dusan Odstrcil5, Peter J MacNeice2, Lutz Rastaetter2, Jack A LaSota6 and the CCMC/SWRC team, (1)NASA/GSFC, CCMC, Greenbelt, MD, United States, (2)NASA Goddard Space Flight Center, Community Coordinated Modeling Center, Greenbelt, MD, United States, (3)Catholic University of America, Washington, United States, (4)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, (5)George Mason University, Fairfax, United States, (6)University of Illinois at Urbana Champaign, Urbana, IL, United States
 
Evolution of Three Geoeffective Shock-CME pairs in September 2011 (23065)
Shi Tsan Wu1, Kan Liou2, Chin-Chun Wu3, Angelos Vourlidas4, Simon P Plunkett5, Murray Dryer, Ph.D.1, Dennis G Socker6 and Brian E Wood5, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)JHU/Applied Physics Lab, Laurel, MD, United States, (3)Naval Research Lab DC, Washington, DC, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)Naval Research Lab, Washington, DC, United States, (6)Naval Research Laboratory, Washington, DC, United States
 
Squeezing of Particle Distributions by Expanding Magnetic Turbulence and Space Weather Variability (12171)
Paisan Tooprakai1,2, David J Ruffolo1,3, Achara Seripienlert1,4, Piyanate Chuychai1,5 and Prof. William H Matthaeus6, (1)Thailand Center of Excellence in Physics, CME, Ministry of Education, Bangkok, 10400, Thailand, (2)Department of Physics, Faculty of Science, Chulalongkorn University, Bangkok, 10330, Thailand, (3)Department of Physics, Faculty of Science, Mahidol University, Bangkok, Thailand, (4)Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand, (5)School of Science, Mae Fah Luang University, Chiang Rai, 57100, Thailand, (6)Bartol Research Institute and Department of Physics and Astronomy, University of Delaware, Newark, DE, United States
 
The Propagation of Solar Energetic Particles as Observed by the Stereo Spacecraft and Near Earth (30813)
Tycho T von Rosenvinge1, Ian G Richardson2, Hilary V Cane3, Eric R Christian1, Alan C Cummings4, Christina Cohen4, Richard A Leske4, Richard Mewaldt4, Edward C Stone4 and Mark E Wiedenbeck5, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)University of Maryland College Park, NASA Goddard Space Flight Center, Greenbelt, United States, (3)University of Tasmania, Mathematics and Physics, Hobart, Australia, (4)California Institute of Technology, Pasadena, CA, United States, (5)Jet Propulsion Laboratory, Pasadena, CA, United States
 
Magnetic reconnection at the solar wind current sheets as a possible cause of strahl electrons acceleration and SEP dropouts (31136)
Olga Khabarova, IZMIRAN RAS, Moscow, Russia and Valentina V Zharkova, Northumbria University, MPEE, Newcastle-Upon-Tyne, United Kingdom
 
Persistent Energetic Ion Outbursts from the Sun (21059)
Radoslav Bucik, Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, Davina Innes, Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany and Glenn M Mason, Johns Hopkins University Applied Physics Laboratory, Laurel, United States
 
Q/A Dependence on Shock Geometry Using Multi-Spacecraft Observations (30836)
Lulu Zhao1, Gang Li2, Glenn M Mason3, Christina Cohen4, Robert W Ebert5, Richard A. Mewaldt4 and Ian G Richardson6, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)University of Alabama in Huntsville, Department of Space Sciences and CSPAR, Huntsville, AL, United States, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (4)California Institute of Technology, Pasadena, CA, United States, (5)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (6)University of Maryland College Park, NASA Goddard Space Flight Center, Greenbelt, United States
 
A searching of past large Solar Proton Event by measuring carbon-14 content in tree-rings (14846)
Fusa Miyake1, Kimiaki Masuda2, Masataka Hakozaki2, Toshio Nakamura3 and Katsuhiko Kimura4, (1)Nagoya University, ISEE, Nagoya, Japan, (2)Nagoya University, Nagoya, Japan, (3)Nagoya University, Graduate School of Enviromentasl Studies, Nagoya, Japan, (4)Fukushima University, Fukushima, Japan
 
Association Rate of Major Sep Events As a Function of CME Speed and Source Longitude (8270)
Seiji Yashiro1,2, Nat Gopalswamy2, Sachiko Akiyama3,4, Pertti A Makela1,3 and Hong Xie1,3, (1)Catholic University of America, Washington, DC, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)NASA Goddard Space Flight Center, Greenbelt, United States, (4)Catholic University of America, Washington, United States
 
Solar Energetic Particle Acceleration in the Solar Corona with Simulated Field Line Random Walk and Wave Generation (30375)
Aaron Douglas Arthur1,2 and Jakobus Albertus le Roux2, (1)Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States, (2)University of Alabama in Huntsville, Huntsville, AL, United States
 
The Solar Energetic Particle Event on 2013 April 11: An Investigation of the Solar Origin of its Longitudinal Widespread (22072)
David Lario, The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Nour E Raouafi, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Ryun Young Kwon, George Mason University Fairfax, School of Physics, Astronomy and Computational Sciences, Fairfax, VA, United States, Jie Zhang, George Mason University, Department of Physics and Astronomy, Fairfax, VA, United States, Raul Gomez-Herrero, University of Alcala, Space Research Group, Alcala de Henares, Spain, Nina Dresing, University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany and Pete Riley, Predictive Science Inc., San Diego, CA, United States
 
Transport of Solar Energetic Particles across the Parker field direction due to field line meandering (15730)
Timo LM Laitinen1, Andreas Kopp2, Frederic Effenberger3, Silvia Dalla1 and Michael S Marsh1, (1)Univ. of Central Lancashire, Preston, United Kingdom, (2)University of Kiel, Kiel, Germany, (3)Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany
 
High Energy Particle Events in Solar Cycles 23 and 24 (30429)
Neeharika Thakur1,2, Nat Gopalswamy1, Pertti A Makela2,3, Seiji Yashiro1,2, Sachiko Akiyama3,4 and Hong Xie2,3, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Catholic University of America, Washington, DC, United States, (3)NASA Goddard Space Flight Center, Greenbelt, United States, (4)Catholic University of America, Washington, United States