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

Thursday, 18 December 2014: 1:40 PM-6:00 PM
Chairs:  Fang Shen, CSSAR, 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

Abstracts Submitted to this Session:

 
Comparisons of characteristics of magnetic clouds and cloud-like structures during 1995-2012
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 
Chin-Chun Wu1, Kan Liou2, Angelos Vourlidas1,2, Ronald P Lepping3, Y.-M. Wang1, Simon P Plunkett1, Dennis G Socker1 and Shi Tsan Wu4, (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)University of Alabama in Huntsville, Huntsville, AL, United States
 
Severe to Extreme Solar Storms: Magnetic Field Complexity and Warnings
Henrik Lundstedt, IRF Swedish Institute of Space Physics Lund, Lund, Sweden
 
Characteristics of solar wind density depletions during solar cycles 23 and 24
Keunchan Park1, Jeongwoo Lee1, Suyeon Oh2 and Yu Yi1, (1)Chungnam National University, Daejeon, South Korea, (2)Chonnam National University, Gwangju, South Korea
 
Full Halo Coronal Mass Ejections: Arrival at the Earth
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.
Alexis P Rouillard, IRAP, Toulouse, France, Angelos Vourlidas, Naval Research Laboratory, Alexandria, VA, United States, Allan J Tylka, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Chee Keong Ng, George Mason University Fairfax, Washington, DC, United States and Christina MS Cohen, California Institute of Technology, Pasadena, CA, United States
 
Study of Quasi-Homologous Coronal Mass Ejections from Super Active Regions in Solar Cycle 23
Lijuan Liu, Yuming Wang, Chenglong Shen, Rui Liu, Pinzhong Ye and Shui Wang, USTC University of Science and Technology of China, Hefei, China
 
A reexamination of long-duration radial IMF events
Gilbert Pi1, Jih-Hong Shue1, Chi-Kuang Chao1, Zdenek Nemecek2, Jana Safrankova2 and chia-Hsien Lin1, (1)Institute of Space Science National Central University, Jhongli, Taiwan, (2)Charles University, Prague, Czech Republic
 
Interaction of magnetic clouds with the Earth’s environment: effects due to the terrestrial bow shock
Dominique Fontaine, Lucile Turc and Philippe Savoini, LPP - CNRS - Ecole polytechnique - UPMC, Palaiseau, France
 
Multi-Spacecraft Observations of Interplanetary Shocks Near Earth
Primoz Kajdic, European Space Agency, Villanueva De La Can, Spain, Xochitl Blanco-Cano, UNAM, Mexico, Mexico and Benoit Lavraud, IRAP, Toulouse, France
 
Global MHD Simulation of the Coronal Mass Ejection on 2011 March 7: from Chromosphere to 1 AU
Meng Jin1,2, Ward Manchester1, Bart van der Holst1, Igor Sokolov1, Gabor Toth3, Angelos Vourlidas4, Curt A de Koning5 and Tamas I Gombosi6, (1)University of Michigan, Ann Arbor, MI, United States, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (3)Univ Michigan, Ann Arbor, MI, United States, (4)Naval Research Laboratory, Alexandria, VA, United States, (5)University of Colorado at Boulder, Boulder, CO, United States, (6)Univ of Michigan, Ann Arbor, MI, 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
Fang Shen1, Yuming Wang2, Chenglong Shen3 and Xue Shang Feng1, (1)CSSAR, Beijing, China, (2)University of Science and Technology of China, Hefei, China, (3)University Science & Technology of China, Hefei, Anhui, China
 
Real­-Time Ensemble Forecasting of Coronal Mass Ejections Using the Wsa-Enlil+Cone Model
M. Leila Mays1,2, Aleksandre Taktakishvili1,2, Antti A Pulkkinen1, Dusan Odstrcil3, Peter J MacNeice1, Lutz Rastaetter1 and Jack A LaSota4, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Catholic University of America, Washington, DC, United States, (3)George Mason University Fairfax, Computational and Data Sciences, Fairfax, VA, United States, (4)University of Illinois at Urbana Champaign, Urbana, IL, United States
 
Evolution of Three Geoeffective Shock-CME pairs in September 2011
Shi Tsan Wu1, Kan Liou2, Chin-Chun Wu3, Angelos Vourlidas4, Simon P Plunkett5, Murray Dryer, Ph.D.1, Dennis G Socker6 and Brian Erland 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)Naval Research Laboratory, Alexandria, VA, 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
Paisan Tooprakai1,2, David J Ruffolo2,3, Achara Seripienlert2,3, Piyanate Chuychai2,4 and William H Matthaeus5, (1)Department of Physics, Faculty of Science, Chulalongkorn University, Bangkok, 10330, Thailand, (2)Thailand Center of Excellence in Physics, CME, Ministry of Education, Bangkok, 10400, Thailand, (3)Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand, (4)School of Science, Mae Fah Luang University, Chiang Rai, 57100, Thailand, (5)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
Tycho T von Rosenvinge1, Ian G Richardson1, Hilary V Cane2, Eric R Christian1, Alan C Cummings3, Christina MS Cohen3, Richard A Leske3, Richard A Mewaldt3, Edward C Stone3 and Mark E Wiedenbeck4, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)University of Tasmania, Hobart, TAS, Australia, (3)California Institute of Technology, Pasadena, CA, United States, (4)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
Olga Khabarova, IZMIRAN RAS, Moscow, Russia and Valentina V Zharkova, Northumbria University, Newcastle-Upon-Tyne, NE1, United Kingdom
 
Persistent Energetic Ion Outbursts from the Sun
Radoslav Bucik1, Davina Innes1 and Glenn M Mason2, (1)Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany, (2)JHU / APL, Laurel, MD, United States
 
Q/A Dependence on Shock Geometry Using Multi-Spacecraft Observations
Lulu Zhao1, Gang Li1, Glenn M Mason2, Christina MS Cohen3, Robert W Ebert4, Richard A. Mewaldt3 and Ian G Richardson5, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)JHU / APL, Laurel, MD, United States, (3)California Institute of Technology, Pasadena, CA, United States, (4)Southwest Research Institute, San Antonio, TX, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
A searching of past large Solar Proton Event by measuring carbon-14 content in tree-rings
Fusa Miyake1, Kimiaki Masuda1, Masataka Hakozaki1, Toshio Nakamura1 and Katsuhiko Kimura2, (1)Nagoya University, Nagoya, Japan, (2)Fukushima University, Fukushima, Japan
 
Association Rate of Major Sep Events As a Function of CME Speed and Source Longitude
Seiji Yashiro1,2, Nat Gopalswamy2, Sachiko Akiyama1,2, Pertti A Makela1,2 and Hong Xie1,2, (1)Catholic University of America, Washington, DC, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Solar Energetic Particle Acceleration in the Solar Corona with Simulated Field Line Random Walk and Wave Generation
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
David Lario1, Nour-Eddine Raouafi2, Ryun Young Kwon3, Jie Zhang3, Raul Gomez-Herrero4, Nina Dresing5 and Pete Riley6, (1)The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (3)George Mason University Fairfax, School of Physics, Astronomy and Computational Sciences, Fairfax, VA, United States, (4)University of Alcala, Alcala de Henarez, Spain, (5)University of Kiel, Kiel, Germany, (6)Predictive Science Inc., San Diego, CA, United States
 
Transport of Solar Energetic Particles across the Parker field direction due to field line meandering
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)University of Waikato, Hamilton, New Zealand
 
High Energy Particle Events in Solar Cycles 23 and 24
Neeharika Thakur1,2, Nat Gopalswamy1, Pertti A Makela1,2, Seiji Yashiro1,2, Sachiko Akiyama1,2 and Hong Xie1,2, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Catholic University of America, Washington, DC, United States