SH41B:
The Connections between Coronal Shock Wave Dynamics and Early SEP Production II Posters

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Session ID#: 12822

Session Description:
Recent remote observations have shown that sufficiently fast coronal mass ejections can drive shock waves very low in the solar atmosphere. Collisionless shocks are known to produce solar energetic particles (SEPs), but it is presently not known to what energies they accelerate particles efficiently and how that efficiency varies in time and location. Coronal and chromospheric signatures of shocks, including radio bursts, EUV waves, Moreton waves and their connections with the global coronal magnetic field determine the dynamics of the shock waves in the corona. X-ray and gamma-ray emissions are additional signatures of particle acceleration, while flare acceleration may also contribute to SEPs. We encourage presentations that use remote and in-situ observations, simulations, and theory to unravel the connections between coronal shocks and SEP production, explore the parameter space of coronal shocks and the contribution of alternative acceleration processes into the production of SEP events.
Primary Convener:  David Lario, The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Conveners:  Iver Hugh Cairns, University of Sydney, School of Physics, Sydney, NSW, Australia and Nariaki Nitta, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Chairs:  David Lario, The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Iver Hugh Cairns, University of Sydney, School of Physics, Sydney, NSW, Australia and Nariaki Nitta, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
OSPA Liaison:  David Lario, The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Index Terms:

7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7514 Energetic particles [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]

Abstracts Submitted to this Session:

Type II and Type III Radio Emissions and Their Association with Solar Energetic Particles (156527)
Hilary V Cane, University of Tasmania, Mathematics and Physics, Hobart, Australia and Ian G Richardson, University of Maryland College Park, Department of Astronomy, College Park, MD, United States
Connectivity Between Solar Energetic Particle Observations and Their Solar Sources: The Event on 14 August 2010 (153147)
Pertti A Makela1, David Lario2, Ryun Young Kwon3, Nour E. Raouafi4, Barbara J Thompson5, Ian G Richardson6, Tycho T von Rosenvinge7, Hong Xie1, M. Leila Mays8, Neeharika Thakur5, Hazel M Bain9, Ming Zhang10, Lulu Zhao10, Prof. William H Matthaeus11, Athanasios Papaioannou12 and Pete Riley13, (1)Catholic University of America, Washington, DC, United States, (2)The Johns Hopkins University. Applied Physics Laboratory, Laurel, MD, United States, (3)George Mason University Fairfax, School of Physics, Astronomy and Computational Sciences, Fairfax, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (6)University of Maryland College Park, Department of Astronomy, College Park, MD, United States, (7)NASA Goddard SFC, Greenbelt, United States, (8)NASA GSFC, Greenbelt, MD, United States, (9)University of California Berkeley, Berkeley, CA, United States, (10)Florida Institute of Technology, Melbourne, FL, United States, (11)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (12)National Observatory of Athens, Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing, Athens, Greece, (13)Predictive Science Inc., San Diego, CA, United States
The Connection Between the Longitudinal Extent of SEP Events and the Properties of Coronal Shocks (148673)
David Lario, The 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, United States, Nour E. Raouafi, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Pete Riley, Predictive Science Inc., San Diego, CA, United States
Coronal Disturbances and the Early Evolution of SEP Events (169082)
Nariaki Nitta, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Lan Jian, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Raul Gomez-Herrero, Universidad de Alcalá, Space Research Group, Alcalá de Henares, Spain
Solar Energetic Particle Events and CME Accelerations in the Low Corona: MLSO Observations (162188)
O C St Cyr, NASA GSFC, Greenbelt, MD, United States, Stephen W Kahler, Kirtland Air Force Base, Kirtland AFB, NM, United States, Ian G Richardson, University of Maryland College Park, Department of Astronomy, College Park, MD, United States, Hilary V Cane, University of Tasmania, Mathematics and Physics, Hobart, Australia, Hong Xie, Catholic University of America, Washington DC, United States and Joan Burkepile, National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States
Comparison on the CME-shock Acceleration of Three Widespread SEPs during Solar Cycle 24 (152318)
Hong Xie, Catholic University of America, Washington, DC, United States, Pertti Makela, Catholic University of America, Washington DC, United States, O C St Cyr, NASA GSFC, Greenbelt, MD, United States and Nat Gopalswamy, NASA Goddard SFC, Greenbelt, United States
A study of SEPs using both STEREO spacecraft. (182708)
Luis Preisser, National Autonomous University of Mexico, Ciudad DE Armería, Mexico, Xochitl Blanco-Cano, Instituto de Geofísica Universidad Nacional Autónoma de México, Mexico City, Mexico and Primoz Kajdic, National Autonomous University of Mexico, Ciudad de Mexico, Mexico
The Relationship Between SEP Events, Type-III Radio Bursts, and Coronal Mass Ejections at the Maximum of Solar Sunspot Cycle 24 (180498)
Richard R Fisher, Goddard Spaceflight Center, Code670, Greenbelt,MD, MD, United States and Bryan Komei Yamashiro, University of Hawaii at Manoa, Institute for Astronomy, Honolulu, HI, United States
On the Origin of Long-duration Solar Gamma-ray Flares and Their Connection with SEPs (141778)
Valerie Bernstein, Villanova University, Villanova, PA, United States, Lisa M Winter, Atmospheric and Environmental Research Inc. Superior, Superior, CO, United States, Edward W Cliver, National Solar Observatory, Tucson, AZ, United States, Nicola Omodei, Stanford University, Stanford, CA, United States and Melissa Pesce-Rollins, INFN-Pisa, Pisa, Italy
Deriving the properties of coronal pressure fronts in 3-D: particle acceleration, time dependent magnetic connectivity with solar surface and link with long lasting gamma ray emission in three far side Coronal Mass Ejections (180020)
Illya Plotnikov and Alexis P Rouillard, IRAP, Toulouse, France
GOES X-class flares released during the Peak of SC-24 (151472)
Ahmed Abdel Hady II, Cairo University, Giza, Egypt

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