SH12B:
Synergies Amidst the Magnetic Environment of Solar Eruptions I

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Session ID#: 15859

Session Description:
Space weather events are driven by eruptive activity originating on the Sun. The plasma dynamics and radiation signatures depend on the magnetic field configuration in the lower solar atmosphere, whereas the magnetic environment in the intervening heliospheric volume determines its geo-effectiveness. This session focuses on the complex magnetic environment from the Sun to 1 AU, knowledge of which is crucial to understanding and forecasting solar eruptions and their impact on Earth. We invite contributions that preferably combine (theoretical and observational) knowledge taken from two or more of the following themes: the energy budget and stability of solar active region field; the predicability of CME productiveness of solar flares; the special magnetic topology responsible for SEP and gamma-ray production; the remote-sensing and in-situ magnetic signatures of flux ropes; or the mapping of magnetic field from the interplanetary space to the Sun.
Primary Convener:  Xudong Sun, Stanford University, Stanford, United States
Conveners:  Xin Cheng, Nanjing University, Nanjing, China and Marc L DeRosa, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Chairs:  Marc L DeRosa, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Xin Cheng, Nanjing University, Nanjing, China and Xudong Sun, Stanford University, Stanford, United States
OSPA Liaison:  Xudong Sun, Stanford University, Stanford, United States
Index Terms:

7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7529 Photosphere [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]

Abstracts Submitted to this Session:

Bernhard Kliem, University of Potsdam, Institute of Physics and Astronomy, Potsdam, Germany
Jiajia Liu1, Yuming Wang1, Robert Erdelyi2, Rui Liu1, Scott William McIntosh3, Tingyu Gou1, Jun Chen1, Kai Liu1, Lijuan Liu4 and Zonghao Pan1, (1)University of Science and Technology of China, Hefei, China, (2)University of Sheffield, School of Mathematics and Statistics, Sheffield, United Kingdom, (3)High Altitude Observatory, Boulder, United States, (4)Sun Yat-Sen University, School of Atmospheric Sciences, Guangzhou, China
Jens Pomoell1, Erkka Lumme1, K Emilia J Kilpua2, Christine Verbeke3, Stefaan Poedts3, Erika Palmerio1 and Alexey Isavnin2, (1)University of Helsinki, Department of Physics, Helsinki, Finland, (2)University of Helsinki, Helsinki, Finland, (3)Centre for Mathematical Plasma-Astrophysics, KU Leuven, Belgium
Chaowei Jiang, Chinese Academy of Sciences, SIGMA Weather Group, State Key Laboratory of Space Weather, National Space Science Center, Beijing, China, S. T. Wu, The University of Alabama in Huntsville, Huntsville, AL, United States, Vasyl Yurchyshyn, Big Bear Solar Observatory, Big Bear City, CA, United States, Haimin Wang, New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States, Xue Shang Feng, State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China;, Beijing, China and Qiang Hu, University of Alabama in Huntsville, Department of Space Science, Huntsville, United States
Cooper Downs1, Viacheslav S. Titov1, Qiu Jiong2, Dr. Tibor Torok3, Jon Linker1 and Zoran Mikic1, (1)Predictive Science Inc., San Diego, CA, United States, (2)Montana State University, Physics Department, Bozeman, MT, United States, (3)Predictive Science Inc., San Diego, United States
Jason Earl Kooi, Naval Research Laboratory, Washington, United States, Steven R. Spangler, University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States and Namir E Kassim, US Naval Research Laboratory, Washington, DC, United States
Janet G Luhmann1, Christina O Lee1, Shannon Curry2, Dr. Takuya Hara3, Jasper S Halekas4, Yan Li5, Chuanfei Dong6, Yingjuan Ma7, Robert J Lillis6, Patrick A Dunn8, Jacob Gruesbeck9, Jared R Espley10, Dave A Brain11, John E P Connerney12, Davin E Larson3, Bruce M Jakosky13 and Christopher T Russell14, (1)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (2)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (3)Space Sciences Laboratory, Berkeley, United States, (4)University of Iowa, Iowa City, IA, United States, (5)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (6)University of California Berkeley, Berkeley, CA, United States, (7)University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, United States, (8)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (9)NASA GSFC, Greenbelt, United States, (10)NASA Goddard Space Flight Center, Greenbelt, United States, (11)University of Colorado at Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (12)Space Research Corporation, Annapolis, United States, (13)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (14)University of California, IGPP/EPSS, Los Angeles, CA, United States