SH53B:
Large-Scale Interplanetary Structures and Their Space Weather Effects II


Submit an Abstract to this Session


Session ID#: 61424

Session Description:
Large-scale interplanetary structures, such as interplanetary coronal mass ejections (ICMEs) and streaming interaction regions (SIRs), are known to be important sources of space weather events. Using remote observations from STEREO/SOHO/SDO and MHD simulations, the evolution and interaction of these large-scale plasma structures have been discussed widely in recent years. Meanwhile, the space weather effects of these structures have also been investigated using in-situ plasma and magnetic field observations, energetic particles measurements, and geomagnetic data. This session focuses on the following issues: (1) the dynamic evolution of these structures from Sun to Earth; (2) their in-situ measurement and solar cycle variation; (3) the physical processes and the remote and in-situ signatures of the interaction between these structures; (4) their space weather effects. We invite contributions covering these different topics, with a particular interest in those combining various observations and modeling techniques.
Primary Convener:  Chenglong Shen, University of Science and Technology of China, Hefei, China
Conveners:  Noé Lugaz, University of New Hampshire, Durham, NH, United States, Fang Shen, National Space Science Center, CAS, Beijing, China and Lan Jian, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Primary Liaison:  Chenglong Shen, University Science & Technology of China, Hefei, Anhui, China
Chairs:  Noé Lugaz, University of New Hampshire, Durham, United States and Lan Jian, NASA Goddard Space Flight Center, Greenbelt, MD, United States
OSPA Liaison:  Fang Shen, National Space Science Center, CAS, Beijing, China
Index Terms:

7511 Coronal holes [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7514 Energetic particles [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7954 Magnetic storms [SPACE WEATHER]

Abstracts Submitted to this Session:

Generalizing Flux Rope Evolution in the Heliosphere (418340)
Phillip Hess, US Naval Research Laboratory, Washington, United States
Reconstructing 3D Solar Wind Structures in the Inner Heliosphere from STEREO Dual Views (Invited) (347245)
Yuming Wang, University of Science and Technology of China, Hefei, China and Xiaolei Li, Auburn University, Physics, Auburn, United States
Investigating EUV Dimming/CME/ICME Events to Understand and Predict Their Source Properties and Interplanetary Effects (381506)
David F Webb, Boston College, ISR, Chestnut Hill, MA, United States, Alysha Reinard, NOAA Boulder, SWPC, Boulder, CO, United States, Dr. James Paul Mason, PhD, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Larisza D Krista, University of Colorado at Boulder, Cooperative Institute for Research in Environmental Sciences (CIRES), Boulder, United States and Barbara J Thompson, NASA GSFC, Greenbelt, United States
Interplanetary Magnetic Flux Ropes and Their Solar Sources: Implications for Flux Rope Origination (424761)
Qiang Hu, University of Alabama in Huntsville, Department of Space Science and CSPAR, Huntsville, AL, United States and Qiu Jiong, Montana State University Bozeman, Bozeman, MT, United States
More on the internal structure of Coronal Magnetic Eruptions (461799)
Nada A Al-Haddad, Catholic University of America, Washington, DC, United States, Stefaan Poedts, KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium, Teresa Nieves-Chinchilla, NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, Wenyuan Yu, Space science center, University of new hampshire, Durham, NH, Durham, United States, Noé Lugaz, University of New Hampshire, Durham, NH, United States, Charles J Farrugia, University of New Hampshire, Durham, United States and Ilia IANKOV Roussev, National Science Foundation Office of Polar Programs, Alexandria, VA, UNITED STATES
Forecasting space weather driven by coronal mass ejections and their sheath regions (Invited) (354474)
K Emilia J Kilpua1, Jens Pomoell2, Erkka Lumme2, Daniel James Price2 and Dr. Erika Palmerio3, (1)University of Helsinki, Department of Physics, Helsinki, Finland, (2)University of Helsinki, Helsinki, Finland, (3)Predictive Science Inc., San Diego, CA, United States
Launching Hydrodynamic and Magnetic CME-like Structures into the Operational Heliospheric Space Weather Models (400709)
Dusan Odstrcil1,2, Alexis P Rouillard3 and Neel Savani1,4, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)George Mason University Fairfax, Physics and Astronomy, Fairfax, VA, United States, (3)Université Toulouse III - Paul Sabatier, Observatoire Midi–Pyrénées, CNRS, CNES, IRAP, Toulouse, France, (4)University of Maryland Baltimore County, Baltimore, MD, United States
The 2017 September 10th events and their imprints at Earth, Mars and STEREO-A (406098)
Jingnan Guo1, Mateja Dumbovic2, Robert F Wimmer-Schweingruber3, Manuela Temmer4, Henning Lohf5, Yuming Wang6, Astrid Veronig4, Don Hassler7, M. Leila Mays8, Cary Zeitlin9, Bent Ehresmann7, Olivier G Witasse10, Johan Lauritz Freiherr von Forstner11, Bernd Heber5, Mats Holmström12 and Arik Posner13, (1)University of Science and Technology of China, School of Earth and Space Sciences, Hefei, China, (2)University of Zagreb, Hvar Observatory, Faculty of Geodesy, Zagreb, Croatia, (3)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (4)University of Graz, Institute of Physics, Graz, Austria, (5)University of Kiel, Kiel, Germany, (6)University of Science and Technology of China, Hefei, China, (7)Southwest Research Institute, Boulder, United States, (8)NASA Goddard Space Flight Center, Community Coordinated Modeling Center, Greenbelt, United States, (9)NASA JSC/Leidos, Houston, United States, (10)European Space Agency, ESTEC, Villanueva De La Can, Spain, (11)University of Kiel, Institute of Experimental and Applied Physics, Kiel, Germany, (12)IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden, (13)NASA Headquarters, Washington, United States

See more of: SPA-Solar and Heliospheric Physics