SH43B:
Solar Sources and Heliospheric Consequences of Coronal Mass Ejections in Solar Cycle 24 II Posters

Session ID#: 1895

Thursday, 18 December 2014: 1:40 PM-6:00 PM
Poster Hall (Moscone_South)
Chairs:  Ying D. Liu, NSSC National Space Science Center, CAS, Beijing, China, Noé Lugaz, University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States and Neel Savani, George Mason University Fairfax, Fairfax, VA, United States
Primary Convener:  Ying D. Liu, NSSC National Space Science Center, CAS, Beijing, China
Co-conveners:  Noé Lugaz, University of New Hampshire, Durham, United States, Benoit Lavraud, LAB, Toulouse, France and Neel Savani, Naval Research Laboratory, Washington, DC, United States
OSPA Liaison:  Neel Savani, George Mason University Fairfax, Fairfax, VA, United States
Co-Sponsor(s):
  • SM - SPA-Magnetospheric Physics
Index Terms:

2111 Ejecta, driver gases, and magnetic clouds [INTERPLANETARY PHYSICS]
2114 Energetic particles [INTERPLANETARY PHYSICS]
7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7954 Magnetic storms [SPACE WEATHER]
Virtual Option?: No

Abstracts Submitted to this Session:

 
25 MeV Solar Proton Events in Cycle 24 and Previous Cycles (2175)
Ian G Richardson, University of Maryland College Park, NASA Goddard Space Flight Center, Greenbelt, United States; University of Maryland College Park, Department of Astronomy, College Park, MD, United States, Hilary V Cane, University of Tasmania, Mathematics and Physics, Hobart, Australia and Tycho T von Rosenvinge, NASA Goddard SFC, Greenbelt, United States
 
Energetic Particle Anisotropies Observed By Stereo/LET in the 23 July 2012 Solar Particle Event (6195)
Richard A Leske1, Alan C Cummings1, Christina Cohen1, Richard Mewaldt1, Allan Wayne Labrador1, Edward C Stone1, Mark E Wiedenbeck2, Eric R Christian3 and Tycho T von Rosenvinge3, (1)California Institute of Technology, Pasadena, CA, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (3)NASA GSFC, Greenbelt, MD, United States
 
A Comparison of Fe-Rich Solar Energetic Particle Events from Cycle 24 to Those of Cycle 23 (4923)
Christina Cohen, California Institute of Technology, Pasadena, CA, United States, Richard Mewaldt, Caltech, Pasadena, CA, United States, Glenn M Mason, Johns Hopkins University Applied Physics Laboratory, Laurel, United States and Mark E Wiedenbeck, NASA Jet Propulsion Laboratory, Pasadena, CA, United States
 
Preliminary Results on Simulations of Ground Level Enhancements (GLEs) detected by The High Altitude Water Cherenkov Observatory (HAWC) (17316)
Olivia Enriquez Rivera1, Alejandro Lara1 and HAWC Collaboration, (1)Universidad Nacional Autonoma de Mexico, Mexico City, Mexico
 
GLE and the NON-GLE Solar Events Observed by AMS-02 in Solar Cycle 24 (15177)
Cristina Consolandi1, Veronica Bindi2, Claudio Corti3 and Kathryn Whitman1, (1)University of Hawaii at Manoa, Honolulu, HI, United States, (2)University of Hawaii at Manoa, Physics and Astronomy, Honolulu, HI, United States, (3)Community Coordinated Modeling Center, Physics and Astronomy, Silver Spring, United States
 
Proton Intensity Spectra during the May 17th, 2012 and January 6th, 2014 Solar Energetic Particle Events - Measurement Capabilities of the Electron Proton Helium Telescope on Board SOHO (8392)
Patrick Kühl1, Sasha Banjac2, Nina Dresing1, Raul Gomez-Herrero3, Bernd Heber2, Andreas Klassen2 and Christoph Terasa1, (1)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (2)University of Kiel, Kiel, Germany, (3)University of Alcala, Space Research Group, Alcala de Henares, Spain
 
Simulations of Solar Energetic Particles Response to Interplanetary Coronal Mass Ejections in the Gradual Events (7022)
Yang Wang and Gang Qin, NSSC National Space Science Center, CAS, Beijing, China
 
Possible Role of Coronal Streamer as Magnetically-closed Structure in Shock-induced Energetic Electrons and Metric Type II Radio Bursts (15163)
Xiangliang Kong1, Yao Chen1, Fan Guo2 and Gang Li3, (1)Shandong University at Weihai, Weihai, China, (2)Los Alamos National Lab, Los Alamos, NM, United States, (3)University of Alabama in Huntsville, Department of Space Sciences and CSPAR, Huntsville, AL, United States
 
A Solar type-II radio burst from CME-coronal ray interaction: simultaneous radio and EUV imaging (20161)
Yao Chen1, Guohui Du1, Li Feng2, Shiwei Feng1, Xiangliang Kong1, Fan Guo3, Bing Wang1 and Gang Li4, (1)Shandong University at Weihai, Weihai, China, (2)Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China, (3)Los Alamos National Lab, Los Alamos, NM, United States, (4)University of Alabama in Huntsville, Department of Space Sciences and CSPAR, Huntsville, AL, United States
 
DIRECT OBSERVATIONS OF MAGNETIC FLUX ROPE FORMATION DURING A SOLAR CORONAL MASS EJECTION (15231)
Hongqiang Song1, Jie Zhang2, Yao Chen1 and Xin Cheng3, (1)Shandong University at Weihai, Weihai, China, (2)George Mason University, Department of Physics and Astronomy, Fairfax, United States, (3)Nanjing University, Nanjing, China
 
Microwave Signatures in the Pre-impulsive Phase of a Solar Flare (19917)
Zhao Wu1, Yao Chen1, Guangli Huang2 and Gang Li3, (1)Shandong University at Weihai, Weihai, China, (2)Purple Mountain Observatory, Nanjing, China, (3)University of Alabama in Huntsville, Department of Space Sciences and CSPAR, Huntsville, AL, United States
 
Early Evolution of An Energetic Coronal Mass Ejection (12001)
Rui Liu, Yuming Wang and Chenglong Shen, University of Science and Technology of China, Hefei, China
 
The relationship between CME momenta and magnetic forces (18533)
Yan Li1, Benjamin J Lynch1, Brian T Welsch2 and David John Bercik2, (1)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)University of California Berkeley, Berkeley, CA, United States
 
Using Ionic Charge States to Investigate the Relationship Between Eruptive Flare Emission and the Heating of CME Plasma (23401)
Benjamin J Lynch1, Maria Kazachenko2, Yan Li1, Alysha Reinard3 and Tamitha Mulligan Skov4, (1)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)University of Colorado at Boulder, NSO, LASP, Boulder, CO, United States, (3)NOAA Boulder, SWPC, Boulder, CO, United States, (4)Aerospace Corporation Los Angeles, Los Angeles, CA, United States
 
The possible trigger mechanism of the solar eruption in 2012 July 12 (29700)
Rui Wang, NSSC National Space Science Center, CAS, Beijing, China
 
The Interaction of Two Coronal-Mass Ejections: Particle-in-cell simulation (29943)
Zhongwei Yang1, Ying D. Liu1, Rui Wang1 and Can Huang2, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)University of Science and Technology of China, Hefei, China
 
ForeCAT: Using CME Deflections to Constrain their Mass and the Drag (16197)
Christina Kay, Boston University, Boston, United States, Luiz F. G. dos Santos, Shell Global Solutions, Houston, United States and Merav Opher, Boston University, Astronomy, Boston, MA, United States
 
Propagation of the 2012 March Coronal Mass Ejections from the Sun to Heliopause (9150)
Ying D. Liu, NSSC National Space Science Center, CAS, Beijing, China, John D Richardson, MIT, Cambridge, MA, United States, Chi Wang, NSSC, CAS, Beijing, China and Janet G Luhmann, Space Sciences Laboratory, University of California Berkeley, Berkeley, United States
 
Rotation of a Magnetic Cloud: MESSENGER and STEREO-B Observations (11051)
Simon W Good, Imperial College London, London, SW7, United Kingdom and Robert J Forsyth, Imperial College London, Department of Physics, London, United Kingdom
 
Forecasting the magnetic vectors within a CME at L1 by using solar observations. (29362)
Neel Savani1, Angelos Vourlidas2, Adam Szabo3, M. Leila Mays4, Rebekah M Evans5, Barbara J Thompson3, Ian G Richardson6, Antti A Pulkkinen7 and Teresa Nieves-Chinchilla7, (1)George Mason University Fairfax, Fairfax, VA, United States, (2)Applied Physics Laboratory Johns Hopkins, Space Department, Laurel, MD, United States, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (4)NASA Goddard Space Flight Center, Community Coordinated Modeling Center, Greenbelt, United States, (5)NASA GSFC/ORAU, Greenbelt, MD, United States, (6)University of Maryland College Park, NASA Goddard Space Flight Center, Greenbelt, United States, (7)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States
 
The HELCATS Project: Characterising the Evolution of Coronal Mass Ejections Observed During Solar Cycle 24 (15541)
Richard Anthony Harrison, United Kingdom Research and Innovation - Science & Technology Facilities Council - Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom, Jackie A Davies, United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom, Christopher H Perry, Rutherford Appleton Laboratory, Didcot, United Kingdom, Mario Mark Bisi, STFC Rutherford Appleton Laboratory, RAL Space, Harwell Campus, Didcot, United Kingdom, Christian Moestl, Austrian Academy of Sciences, Space Research Institute, Vienna, Austria, Alexis P Rouillard, IRAP, Toulouse, France, Volker Bothmer, University of Göttingen, Göttingen, Germany, Luciano Rodriguez, Royal Observatory of Belgium, Brussels, Belgium, Jonathan P Eastwood, Imperial College London, Physics, London, United Kingdom, K Emilia J Kilpua, University of Helsinki, Department of Physics, Helsinki, Finland, Peter Gallagher, Trinity College Dublin, Dublin, Ireland and Dusan Odstrcil, George Mason University, Fairfax, United States
 
Observations of Interplanetary Coronal Mass Ejections and its Geoeffectiveness During 1996-2013 (15433)
Yutian Chi, Chenglong Shen and Yuming Wang, University of Science and Technology of China, Hefei, China
 
Shocks Propagating Through Coronal Mass Ejections (16011)
Noé Lugaz1, Charles J Farrugia2, Charles William Smith1 and Kristoff W Paulson3, (1)University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States, (2)University of New Hampshire, Durham, United States, (3)University of New Hampshire Main Campus, Durham, NH, United States
 
3D Numerical Study of Typical CME Event: The 2010-04-03 Event (20641)
Yufen Zhou, NSSC National Space Science Center, CAS, Beijing, China, Xue Shang Feng, CSSAR, Beijing, China and Xinhua Zhao, Center for Space Science and Applied Research, Beijing, China
 
New approach for the inverse boundary value problem of Laplace's equation on a rectangle: technique renovation for the Grad-Shafranov (GS) reconstruction (22910)
Huijun Li1, Xue Shang Feng2, Jie Xiang1 and Pingbing Zuo2, (1)College of Meteorology and Oceanography, PLA University of Science and Technology, Nanjing, China, (2)CSSAR, Beijing, China