Chairs: Ian G Richardson, University of Maryland College Park, NASA Goddard Space Flight Center, Greenbelt, United States, Leif Svalgaard, Stanford University, Stanford, CA, United States and Fatima Rubio da Costa, Stanford University, Department of Physics, Stanford, CA, United States
Primary Convener: Ian G Richardson, University of Maryland College Park, NASA Goddard Space Flight Center, Greenbelt, United States
Co-conveners: Robyn M Millan, Dartmouth College, Department of Physics and Astronomy, Hanover, United States and Larry J Paxton, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
OSPA Liaison: Ian G Richardson, University of Maryland College Park, NASA Goddard Space Flight Center, Greenbelt, United States
Does There Exist a Relationship Between Acoustic and White-Light Emission in Hard-X ray Solar Flares? (27366)
Juan Camilo Buitrago-Casas, Space Sciences Laboratory, Berkeley, CA, United States, Juan Carlos Martinez Oliveros, University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, Lindsay Glesener, University of Minnesota Twin Cities, Minneapolis, United States, Sam Krucker, Space Sciences Laboratory, Berkeley, United States and Benjamin Calvo-Mozo, Universidad Nacional de Colombia, Observatorio Astronómico Nacional, Bogota, Colombia
Statistical Study of Coronal Hard X-ray Source Heights and Fluxes (27402)
Lindsay Glesener1, Mitsuo Oka2, Sam Krucker3,4 and Hugh S Hudson2,5, (1)University of Minnesota Twin Cities, Minneapolis, United States, (2)Space Sciences Laboratory, Berkeley, CA, United States, (3)Space Sciences Laboratory, Berkeley, United States, (4)FHNW, Windisch, Switzerland, (5)University of Glasgow, Glasgow, United Kingdom
First High-resolution Spectroscopic Observations by IRIS of a Fast, Helical Prominence Eruption Associated with a Coronal Mass Ejection (28069)
Wei Liu1, Bart De Pontieu2, Takenori J. Okamoto3, Jean-Claude Vial4, Alan M Title2, Patrick Antolin5, Thomas E Berger6 and Han Uitenbroek7, (1)University of California Riverside, Riverside, CA, United States, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (3)Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, Yoshinodai, Sagamihara, Japan, (4)IAS Institut d'Astrophysique Spatiale, Orsay Cedex, France, (5)Department of Mathematics, Physics and Electrical Engineering, Northumbria University, Newcastle Upon Tyne, United Kingdom, (6)National Center for Atmospheric Research, High Altitude Observatory, Boulder, United States, (7)National Solar Observatory, Tucson, AZ, United States
Harnessing AIA Diffraction Patterns to Determine Flare Footpoint Temperatures (30905)
Hazel M Bain, University of California Berkeley, Berkeley, CA, United States, Richard A Schwartz, American University, Washington, DC, United States, Gabriele Torre, Catholic University of America, Washington, DC, United States, Sam Krucker, Space Sciences Laboratory, Berkeley, United States and Claire L Raftery, University Corporation for Atmospheric Research, Boulder, CO, United States
