SH51A
Characteristics, Consequences, and Predictabilities of Large Solar Storms II Posters

Friday, 18 December 2015: 08:00-12:20
Poster Hall (Moscone South)
Primary Conveners:  Chin-Chun Wu, Naval Research Lab DC, Washington, DC, United States
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
Chairs:  Pingbing Zhou, Chinese Academy of science, Beijing, China and Daniel Benjamin Berdichevsky, University of the district of Columbia, Washington, DC, United States
OSPA Liaisons:  Yi Wang, Chinese Academy of science, Beijing, China
 
The Geoeffectiveness of ICMEs from 1996 to 2013 (71354)
Yutian Chi and Chenglong Shen, University Science & Technology of China, Hefei, Anhui, China
 
RELATIONSHIPs among Geomagnetic storms, interplanetary shocks, magnetic clouds, and SUNSPOT NUMBER during 1995-2012 (67631)
Ronald P Lepping, NASA Goddard Space Flight Center, Emeritus, Greenbelt, MD, United States, Chin-Chun Wu, US Naval Research Laboratory, Washington, DC, United States and Daniel Benjamin Berdichevsky, Berdichevsky Daniel B, Greenbelt, MD, United States
 
The first super geomagnetic storm of solar cycle 24: “The St. Patrick day (17 March 2015)” event (48075)
Chin-Chun Wu1, Kan Liou2, Dennis G Socker3, Russell Howard3, Bernard V Jackson4, Hsiu-Shan Yu4, Lynn Hutting5 and Simon P Plunkett6, (1)Naval Research Lab DC, Washington, DC, United States, (2)JHU/Applied Physics Lab, Laurel, MD, United States, (3)Naval Research Laboratory, Washington, DC, United States, (4)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (5)U.S. Naval Research Laboratory, Washington, DC, United States, (6)US Naval Research Laboratory, Washington, DC, United States
 
Development of a CME-associated geomagnetic storm intensity prediction tool (67000)
Jasmine M DeHart, Philander Smith College, Little Rock, AR, United States
 
3D numerical study of the propagation characteristics of a consequence of coronal mass ejections in a structured ambient solar wind (61683)
Yufen Zhou, NSSC National Space Science Center, CAS, Beijing, China
 
Characterizing Interplanetary Structures of Long-Lasting Ionospheric Storm Events (68788)
Chris Tandoi1, Ying Dong1, Zhenkang Yang1, San Peng1,2, Chigomezyo Mudala Ngwira3, M. Chantale Damas1 and Tak D Cheung4, (1)Queensborough Community College, Bayside, NY, United States, (2)CUNY City College of New York, New York, NY, United States, (3)Catholic University of America, Washington, DC, United States, (4)QCC, Bayside, NY, United States
 
Solar Corona Simulation Model With Positivity-preserving Property (69423)
Xue Shang Feng, State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100190, China;, Beijing, China
 
Modeling the Impacts of Geomagnetic Disturbances on the New York State Power Transmission System (70500)
Djibrina Ouedraogo1, Orlando Castillo1, Ahmed Mohamed2, M. Chantale Damas1, Chigomezyo Mudala Ngwira3 and CUNY Space Weather Group, (1)Queensborough Community College, Bayside, NY, United States, (2)CUNY City College of New York, Electrical Engineering, New York, NY, United States, (3)Catholic University of America, Washington, DC, United States
 
Comparative Analyses of Two Extremely Fast CMEs Induced Shocks using A H3DMHD Model (73305)
Shi Tsan Wu1, Chin-Chun Wu2, Kan Liou3, Murray Dryer, Ph.D.4 and Simon P Plunkett2, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)US Naval Research Laboratory, Washington, DC, United States, (3)JHU/Applied Physics Lab, Laurel, MD, United States, (4)NOAA Boulder, Boulder, CO, United States
 
A Comparative Study of Shock Structures for the Halloween 2003 and the 23 July 2012 CME Events (83833)
Kan Liou, JHU/Applied Physics Lab, Laurel, MD, United States and Chin-Chun Wu, US Naval Research Laboratory, Washington, DC, United States
 
Diffuse Interplanetary Radio Emission (DIRE) Accompanying Type II Radio Bursts (79370)
Tsega Berhane Teklu1, Nat Gopalswamy2, Pertti A Makela3, Seiji Yashiro3, Sachiko Akiyama4 and Hong Xie3, (1)Catholic University of America, Physics, Washinton DC, WA, United States, (2)NASA Goddard SFC, Greenbelt, MD, United States, (3)Catholic University of America, Washington, DC, United States, (4)NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
High-frequency Plasma Waves Associated with Magnetic Reconnection in the Solar Wind (77772)
Yi Wang, National Space Science Center, Chinese Academy of Sciences, beijing, China
 
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