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

Thursday, 18 December 2014: 1:40 PM-6:00 PM
Chairs:  Ying D. Liu, NSSC National Space Science Center, CAS, Beijing, China, Noé Lugaz, University of New Hampshire Main Campus, Durham, NH, United States, Benoit Lavraud, IRAP, Toulouse, France and Neel Savani, George Mason University Fairfax, Fairfax, VA, United States
Primary Conveners:  Ying D. Liu, NSSC National Space Science Center, CAS, Beijing, China
Co-conveners:  Noé Lugaz, University of New Hampshire, Durham, NH, United States, Benoit Lavraud, IRAP/CNRS, Toulouse, France and Neel Savani, Naval Research Laboratory, Washington, DC, United States
OSPA Liaisons:  Neel Savani, George Mason University Fairfax, Fairfax, VA, United States

Abstracts Submitted to this Session:

 
25 MeV Solar Proton Events in Cycle 24 and Previous Cycles
Ian G Richardson, NASA Goddard Space Flight Center, Greenbelt, MD, United States; University of Maryland College Park, CRESST and Department of Astronomy, College Park, MD, United States, Hilary V Cane, University of Tasmania, Hobart, TAS, Australia and Tycho T von Rosenvinge, NASA Goddard SFC, Greenbelt, MD, United States
 
Energetic Particle Anisotropies Observed By Stereo/LET in the 23 July 2012 Solar Particle Event
Richard A Leske1, Alan C Cummings1, Christina MS Cohen1, Richard A 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
Christina MS Cohen, California Institute of Technology, Pasadena, CA, United States, Richard A Mewaldt, Caltech, Pasadena, CA, United States, Glenn M Mason, JHU / APL, Laurel, MD, United States and Mark E Wiedenbeck, NASA Jet Propulsion Laboratory, Pasadena, CA, United States
 
2012 May 17th GLE: New Views of a GLE with PAMELA
Georgia Adair de Nolfo1, M. Boezio2, U. Bravar3, A. Bruno4, Eric R Christian1, M. Martucci5, M. Mergè5, M. Mocchiutti2, R. Munini6, M. Ricci7, James M Ryan3, S. Stochaj8 and N. Thakur1, (1)NASA Goddard Space Flight Ctr, Greenbelt, MD, United States, (2)Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Trieste, Italy, (3)Space Science Center, University of New Hampshire, Durham, NH, United States, (4)Universita' di Bari, Bari, Italy, (5)Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Frascati and Universita' di Roma Tor Vergata, Roma, Italy, (6)Istituto Nazionale di Fisica Nucleare, Sezione di Trieste and Universita' degli studi di Trieste, Trieste, Italy, (7)Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Frascati, Frascati, Italy, (8)Electrical and Computer Engineering, New Mexico State University, Las Cruces, NM, United States
 
Preliminary Results on Simulations of Ground Level Enhancements (GLEs) detected by The High Altitude Water Cherenkov Observatory (HAWC)
Olivia Enriquez Rivera and Alejandro Lara, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico
 
GLE and the NON-GLE Solar Events Observed by AMS-02 in Solar Cycle 24
Cristina Consolandi1, Veronica Bindi2, Claudio Corti2 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
 
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
Patrick Kühl1, Sasha Banjac1, Nina Dresing1, Raul Gomez-Herrero2, Bernd Heber1, Andreas Klassen1 and Christoph Terasa1, (1)University of Kiel, Kiel, Germany, (2)University of Alcala, Alcala de Henarez, Spain
 
Developing a forecast model of solar proton flux profiles for well-connected events
Eun-Young Ji, Yong-Jae Moon and Jinhye Park, Kyung Hee University, Yongin, South Korea
 
Simulations of Solar Energetic Particles Response to Interplanetary Coronal Mass Ejections in the Gradual Events
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
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, Huntsville, AL, United States
 
A Solar type-II radio burst from CME-coronal ray interaction: simultaneous radio and EUV imaging
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, Nanjing, China, (3)Los Alamos National Lab, Los Alamos, NM, United States, (4)University of Alabama in Huntsville, Huntsville, AL, United States
 
What Do EUV Dimmings Tell Us About CME Topology?
Barbara J Thompson, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Marc L DeRosa, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Richard R Fisher, Goddard Spaceflight Center, Code670, Greenbelt,MD, MD, United States, Larisza D Krista, NOAA/SWPC, Boulder, CO, United States, Ryun Young Kwon, George Mason University Fairfax, School of Physics, astronomy and Computational Sciences, Fairfax, VA, United States, James P Mason, University of Colorado at Boulder, Boulder, CO, United States, M. Leila Mays, NASA/GSFC, Greenbelt, MD, United States, Nariaki Nitta, Lockheed Martin Adv Tech, Lockheed Martin STAR Labs, Palo Alto, CA, United States, Neel Savani, George Mason University Fairfax, Fairfax, VA, United States and Matthew John West, Royal Observatory of Belgium, Brussels, Belgium
 
DIRECT OBSERVATIONS OF MAGNETIC FLUX ROPE FORMATION DURING A SOLAR CORONAL MASS EJECTION
Hongqiang Song1, Jie Zhang2, Yao Chen1 and Xin Cheng3, (1)Shandong University at Weihai, Weihai, China, (2)George Mason Univ, Fairfax, VA, United States, (3)Nanjing University, Nanjing, China
 
Microwave Signatures in the Pre-impulsive Phase of a Solar Flare
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, Huntsville, AL, United States
 
Early Evolution of An Energetic Coronal Mass Ejection
Rui Liu, Yuming Wang and Chenglong Shen, University of Science and Technology of China, Hefei, China
 
The relationship between CME momenta and magnetic forces
Yan Li, Benjamin J Lynch, Brian T Welsch and David John Bercik, 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
Benjamin J Lynch1, Maria Kazachenko1, Yan Li1, Alysha Reinard2 and Tamitha Lynne Mulligan3, (1)University of California Berkeley, Berkeley, CA, United States, (2)NOAA Boulder, SWPC, Boulder, CO, United States, (3)Aerospace Corporation Los Angeles, Los Angeles, CA, United States
 
The possible trigger mechanism of the solar eruption in 2012 July 12
Rui Wang, NSSC National Space Science Center, CAS, Beijing, China
 
The Interaction of Two Coronal-Mass Ejections: Particle-in-cell simulation
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
Christina Kay1, Luiz F. G. dos Santos2 and Merav Opher1, (1)Boston University, Boston, MA, United States, (2)Universidade de Brasilia, Physics, Brasilia, Brazil
 
Propagation of the 2012 March Coronal Mass Ejections from the Sun to Heliopause
Ying D. Liu, NSSC National Space Science Center, CAS, Beijing, China, John D Richardson, MIT, Cambridge, MA, United States, Chi Wang, CSSAR, CAS, Beijing, China and Janet G Luhmann, University of California Berkeley, Berkeley, CA, United States
 
Rotation of a Magnetic Cloud: MESSENGER and STEREO-B Observations
Simon W Good, Imperial College London, London, SW7, United Kingdom and Robert J Forsyth, Imperial College London, London, United Kingdom
 
Forecasting the magnetic vectors within a CME at L1 by using solar observations.
Neel Savani1, Angelos Vourlidas2, Adam Szabo3, M. Leila Mays4, Rebekah M Evans5, Barbara J Thompson3, Ian G Richardson3, Antti A Pulkkinen3 and Teresa Nieves-Chinchilla3, (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/GSFC, Greenbelt, MD, United States, (5)NASA GSFC/ORAU, Greenbelt, MD, United States
 
The HELCATS Project: Characterising the Evolution of Coronal Mass Ejections Observed During Solar Cycle 24
Richard Anthony Harrison1, Jackie A Davies2, Christopher H Perry2, Mario Mark Bisi1, Christian Moestl3, Alexis P Rouillard4, Volker Bothmer5, Luciano Rodriguez6, Jonathan P Eastwood7, Emilia Kilpua8, Peter Gallagher9 and Dusan Odstrcil10, (1)Rutherford Appleton Laboratory, Didcot, OX11, United Kingdom, (2)Rutherford Appleton Laboratory, Didcot, United Kingdom, (3)University of Graz, Space Research Institute, Austrian Academy of Sciences, Graz, Austria, (4)IRAP, Toulouse, France, (5)University of Göttingen, Göttingen, Germany, (6)Royal Observatory of Belgium, Brussels, Belgium, (7)Imperial College London, London, United Kingdom, (8)University of Helsinki, Helsinki, Finland, (9)Trinity College Dublin, Dublin, Ireland, (10)George Mason University Fairfax, Computational and Data Sciences, Fairfax, VA, United States
 
Observations of Interplanetary Coronal Mass Ejections and its Geoeffectiveness During 1996-2013
Yutian Chi, Chenglong Shen and Yuming Wang, University of Science and Technology of China, Hefei, China
 
Shocks Propagating Through Coronal Mass Ejections
Noé Lugaz, Charles J Farrugia, Charles William Smith and Kristoff W Paulson, University of New Hampshire Main Campus, Durham, NH, United States
 
3D Numerical Study of Typical CME Event: The 2010-04-03 Event
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
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