SH41A:
Multiwavelength Observations and Modeling of Solar Flares: Magnetic Structures, Particle Acceleration, and Atmospheric Response Posters
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Session ID#: 23501
Session Description:
Solar flares are highly dynamic processes that can release significant amounts of thermal and non-thermal energy. How the energy is transported along the solar atmosphere and deposited in different layers as well as the relation between wave-heating, thermal, and non-thermal processes is still largely unknown. Similarly, the role of magnetic field topological structures and dynamic processes in the energy budget and energy release processes of a flare remain topics of discussion. High quality multi-wavelength and spectroscopic information with unprecedented spatial and temporal resolution from space and ground-based telescopes (e.g., RHESSI, MinXSS, IRIS, SDO, Hinode, NuSTAR, NoRH, and OVSA) together with advanced simulations can constrain the energy input and dissipation during a flare. The emission at each wavelength is associated with physical processes in different atmospheric layers. Studying the atmospheric response, thermal and non-thermal emissions, and magnetic field evolution are keys to understand the flare heating mechanism and energetic particle production.
Primary Convener: Frederic Effenberger, Bay Area Environmental Research Institute, NASA Research Park, Moffet Field, CA, United States; International Space Science Institute, Bern, Switzerland
Conveners: Fatima Rubio da Costa, Stanford University, Department of Physics, Stanford, CA, United States, Xudong Sun, Stanford University, Stanford, CA, United States and Lucia Kleint, University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland
Chairs: Frederic Effenberger, International Space Science Institute, Bern, Switzerland and Xudong Sun, Stanford University, Stanford, CA, United States
OSPA Liaison: Fatima Rubio da Costa, Stanford University, Department of Physics, Stanford, CA, United States
Index Terms:
7514 Energetic particles [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7519 Flares [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7554 X-rays, gamma rays, and neutrinos [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
Abstracts Submitted to this Session:
Ryan O Milligan1,2, Jack Ireland3, Bernhard Fleck4, Hugh S Hudson5, Lyndsay Fletcher1 and Brian R Dennis6, (1)University of Glasgow, Glasgow, G12, United Kingdom, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)ADNET Systems Inc. Greenbelt, Greenbelt, MD, United States, (4)European Space Agency, Villanueva De La Can, Spain, (5)Space Sciences Laboratory, Berkeley, CA, United States, (6)NASA GSFC, Greenbelt, MD, United States
Jeffrey W Brosius, Catholic University of America, Washington, DC, United States and Andrew R Inglis, Catholic University of America, Washington, United States
Vanessa Polito, Bay Area Environmental Research Institue, Moffett Field, United States, Paola Testa, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States and Joel C Allred, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Iain G Hannah, University of Glasgow, Glasgow, United Kingdom, Lucia Kleint, University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland, Sam Krucker, Space Sciences Laboratory, Berkeley, United States, Lindsay Glesener, University of Minnesota Twin Cities, Minneapolis, United States and Brian Grefenstette, California Institute of Technology, Pasadena, United States
Juliana Therese Vievering1, Lindsay Glesener2, P. S. Athiray3, Daniel Ryan4, Sam Krucker5, Steven Christe6, Juan Camilo Buitrago-Casas5, Andrew R Inglis7 and Sophie Musset8, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)University of Minnesota, Minneapolis, United States, (3)University of Alabama in Huntsville, Huntsville, AL, United States, (4)NASA GSFC, Solar Physics Lab, Greenbelt, MD, United States, (5)Space Sciences Laboratory, Berkeley, United States, (6)NASA GSFC, Solar Physics Lab, Greenbelt, United States, (7)Catholic University of America, Washington, United States, (8)ESTEC, Noordwijk, Netherlands
P. S. Athiray1, Lindsay Glesener2, Juliana Therese Vievering3, Daniel Ryan4, Steven Christe5, Andrew R Inglis6, Juan Camilo Buitrago-Casas7, Sophie Musset8 and Sam Krucker7, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)University of Minnesota Twin Cities, Minneapolis, United States, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (4)NASA GSFC, Solar Physics Lab, Greenbelt, MD, United States, (5)NASA GSFC, Solar Physics Lab, Greenbelt, United States, (6)Catholic University of America, Washington, United States, (7)Space Sciences Laboratory, Berkeley, United States, (8)ESTEC, Noordwijk, Netherlands
Frederic Effenberger, International Space Science Institute, Bern, Switzerland; Bay Area Environmental Research Institute, NASA Research Park, Moffet Field, CA, United States, Sam Krucker, Space Sciences Laboratory, Berkeley, United States and Fatima Rubio da Costa, Stanford University, Department of Physics, Stanford, CA, United States
Fatima Rubio da Costa, Stanford University, Department of Physics, Stanford, CA, United States, Frederic Effenberger, Bay Area Environmental Research Institute, NASA Research Park, Moffet Field, CA, United States and Lucia Kleint, University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland
Sujin Kim, Korea Astronomy and Space Science Institute, Daejeon, South Korea, Vasyl Yurchyshyn, Big Bear Solar Observatory, Big Bear City, CA, United States and Chaowei Jiang, Chinese Academy of Sciences, SIGMA Weather Group, State Key Laboratory of Space Weather, National Space Science Center, Beijing, China
Kanya Kusano1, Johan Muhamad1, Naoyuki Ishiguro2, Tomoya Iju2, Yuki Asahi2 and Yuta Mizuno2, (1)Nagoya University, ISEE, Nagoya, Japan, (2)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan
Adam Kobelski, University of Alabama in Huntsville, Huntsville, United States, Sabrina L Savage, NASA Marshall Space Flight Center, Huntsville, United States and David Malaspina, Univ Colorado, Boulder, CO, United States
Natsuha Kuroda1, Dale E Gary2, Haimin Wang2, Gregory D Fleishman2, Gelu M Nita2 and Ju Jing3, (1)George Mason University Fairfax, Fairfax, United States, (2)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States, (3)New Jersey Institute of Technology, Physics, Newark, United States
Masumi Shimojo, National Astronomical Observatory of Japan, Mitaka, Japan, Hugh S Hudson, Space Sciences Laboratory, Berkeley, CA, United States, Stephen M White, Air Force Research Laboratory Albuquerque, Albuquerque, NM, United States, Tim Bastian, National Radio Astronomy Observatory, Charlottesville, VA, United States and Kazumasa Iwai, Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan
Dale E Gary1, Bin Chen2, Gelu M Nita2, Gregory D Fleishman1, Sijie Yu2, Stephen M White3, Gordon J Hurford4 and James M McTiernan4, (1)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States, (2)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Edison, NJ, United States, (3)AFRL, Kirtland AFB, NM, United States, (4)Space Sciences Laboratory, Berkeley, CA, United States
Kyoko Watanabe, National Defense Academy of Japan, Yokosuka, Japan and S Masuda, Nagoya University, Institute for the Space and Earth Environment, Nagoya, Japan
Meng Jin1, Chun Ming Mark Cheung2, Marc L DeRosa1, Nariaki Nitta3 and Karel Schrijver4, (1)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (2)CSIRO Astronomy and Space Science Geraldton, Perth, Australia, (3)Lockheed Martin Advanced Technology Center, Palo Alto, United States, (4)Lockheed Martin Adv Techn Ctr, Palo Alto, CA, United States
