SH51D:
Large-Scale Interplanetary Structures and Their Space Weather Effects I Posters


Submit an Abstract to this Session


Session ID#: 50410

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, Heliophysics Science Division, Greenbelt, MD, United States
Primary Liaison:  Chenglong Shen, University Science & Technology of China, Hefei, Anhui, China
Chairs:  Chenglong Shen, University Science & Technology of China, Hefei, Anhui, China and Fang Shen, National Space Science Center, CAS, Beijing, China
OSPA Liaison:  Lan Jian, NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States
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:

What causes CME travel time estimation errors: their kinematic measurements in the corona or the limited understanding of the forces in their IP propagation? (413293)
Carlos Roberto Braga1, Angelos Vourlidas2, Alisson Dal Lago3, Rafael Rodrigues Souza de Mendonça4, Ezequiel Echer1, Laura Balmaceda5 and RyunYoung Kwon6, (1)INPE National Institute for Space Research, Sao Jose dos Campos, Brazil, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (3)National Institute for Space Research (INPE), São José dos Campos - SP, Brazil, (4)National Institute for Space Research and State Key Laboratory of Space Weather, Chinese Academy of Sciences, São José dos Campos, Brazil, (5)George Mason University, Fairfax, United States, (6)George Mason University Fairfax, Fairfax, VA, United States
Three-dimensional MHD simulation of solar wind using a new boundary treatment: Comparison with in-situ data at Earth (361969)
Fang Shen1, Zicai Yang2, Jie Zhang3, Wenwen Wei2 and Xueshang Feng2, (1)National Space Science Center, CAS, Beijing, China, (2)National Space Science Center, Beijing, China, (3)George Mason University, Department of Physics and Astronomy, Fairfax, United States
Evolution of ICME structure in the inner heliosphere: a parametric study (378343)
Elena Provornikova1, Viacheslav G Merkin1, Sarah E Gibson2, Anna V Malanushenko3, Charles Nickolos Arge4 and Angelos Vourlidas1, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States, (3)High Altitude Observatory, Boulder, United States, (4)NASA Goddard Space Flight Center, Greenbelt, MD, United States
2.5D Numerical simulations of ICMES up to 1AU. (368061)
Skralan Hosteaux1, Emmanuel Chané1 and Stefaan Poedts2, (1)KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium, (2)KU Leuven, Centre for mathematical Plasma-Astrophysics, Department of Mathematics, Leuven, Belgium
Modeling the Thermodynamic State of a Coronal Mass Ejection (CME) Using Its Kinematics in the Heliosphere (402023)
Wageesh Mishra and Yuming Wang, University of Science and Technology of China, Hefei, China
Observation-based Sun-to-Earth simulations of geo-effective Coronal Mass Ejections with EUHFORIA (374103)
Camilla Scolini1,2, Francesco P. Zuccarello1, Stefaan Poedts3, Luciano Rodriguez4, Marilena Mierla4,5, Christine Verbeke1, Jens Pomoell6, Joachim Raeder7 and William D Cramer7, (1)KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium, (2)Royal Observatory of Belgium, Brussels, Belgium, (3)KU Leuven, Centre for mathematical Plasma-Astrophysics, Department of Mathematics, Leuven, Belgium, (4)SIDC, Royal Observatory of Belgium, Brussels, Belgium, (5)Institute of Geodynamics of the Romanian Academy, Bucharest, Romania, (6)University of Helsinki, Helsinki, Finland, (7)University of New Hampshire, Durham, NH, United States
Sun to Earth MHD simulation of a CME model constrained by observed mass, speed, and poloidal flux (387451)
Talwinder Singh, Georgia State University, Atlanta, GA, United States, Mehmet Sarp Yalim, University of Alabama in Huntsville, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States and Nikolai V Pogorelov, University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States
Why the Shock-ICME Complex Structure Is Important: Learning from the Early 2017 September CMEs (387587)
Chenglong Shen1, Yuming Wang1, Yutian Chi2 and Mengjiao Xu3, (1)University of Science and Technology of China, Hefei, China, (2)University of Science and Technology of China, Anhui, China, (3)USTC University of Science and Technology of China, ESS, Hefei, China
Classifying Counterstreaming Suprathermal Electrons and Investigating their Correlation with Interplanetary Coronal Mass Ejections and their Observed In-Situ Substructure (466027)
Alicia Kathryn Petersen, University of Michigan Ann Arbor, Climate and Space Sciences, Ann Arbor, MI, United States, Susan T Lepri, University of Michigan, Ann Arbor, United States and Michael Warren Liemohn, University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
Suprathermal Electrons Bidirectionality Study inside Magnetic Clouds Observed by STEREO (2007-2014) (465554)
Fernando Carcaboso1, Raul Gomez-Herrero2, Miguel A. UAH Hidalgo3, Francisco Espinosa Lara2, Ignacio Cernuda4 and Javier Rodriguez-Pacheco5, (1)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, (2)University of Alcala, Space Research Group, Alcala de Henares, Spain, (3)University of Alcalá, Madrid, Spain, (4)University of Alcala, Alcala de Henares, Spain, (5)University of Alcalá, Space Research Group, Alcalá de Henares, Spain
Dependence of Interplanetary Coronal Mass Ejection Magnetic Properties on Their Solar Sources (366361)
Sanchita Pal, George Mason University, Fairfax, United States and Dibyendu Nandy, Indian Institute of Science Education and Research Kolkata, Center of Excellence in Space Sciences India and Department of Physical Sciences, Kolkata, India
Tracking and Validating ICMEs Propagating Towards Mars using STEREO Heliospheric Imagers Combined with Forbush Decreases Detected by MSL/RAD (433039)
Johan Lauritz Freiherr von Forstner, University of Kiel, Institute of Experimental and Applied Physics, Kiel, Germany, Jingnan Guo, University of Science and Technology of China, School of Earth and Space Sciences, Hefei, China, Robert F Wimmer-Schweingruber, University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, Manuela Temmer, University of Graz, Institute of Physics, Graz, Austria, Christian Moestl, Institute of Physics, University of Graz, Graz, Austria and The MSL/RAD Scientific Team
Evolution of a coronal mass ejection from the Sun to Saturn (431196)
Dr. Erika Palmerio1, K Emilia J Kilpua2, Andrei Zhukov3, David Barnes4, Marilena Mierla5, Olivier G Witasse6, Teresa Nieves-Chinchilla7, Beatriz Sanchez-Cano8, Christian Moestl9, Luciano Rodriguez5, Elias Roussos10, Jingnan Guo11, Adam Masters12, Alexey Isavnin13, Gabrielle Provan14, Neel Savani15 and Lucile Turc16, (1)Predictive Science Inc., San Diego, CA, United States, (2)University of Helsinki, Department of Physics, Helsinki, Finland, (3)SIDC, Royal Observatory of Belgium, Brussels, Belgium, (4)United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom, (5)SIDC, Royal Observatory of Belgium, Uccle, Belgium, (6)European Space Agency, ESTEC, Villanueva De La Can, Spain, (7)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, (8)University of Leicester, Leicester, LE1, United Kingdom, (9)Institute of Physics, University of Graz, Graz, Austria, (10)Max Planck Institute for Solar System Research, Göttingen, Germany, (11)University of Science and Technology of China, School of Earth and Space Sciences, Hefei, China, (12)Imperial College London, Blackett Laboratory, London, United Kingdom, (13)Katholieke Universiteit Leuven, Leuven, Belgium, (14)University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, (15)University of Maryland Baltimore County, Baltimore, MD, United States, (16)LPP - CNRS - Ecole polytechnique - UPMC, Palaiseau, France
The Internal Structure of ICMEs: Heavy Ion Composition and the Associated Magnetic Field (392378)
Yuan-Kuen Ko, US Naval Research Laboratory, Space Science Division, Washington, DC, United States, Teresa Nieves-Chinchilla, NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, Neel Savani, University of Maryland Baltimore County, Baltimore, MD, United States, Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and John Martin Laming, Naval Research Laboratory, Washington, United States
Study on the agreement between solar and interplanetary magnetic field north-south directions using 101 CME-ICME pairs (391548)
S.K. Sung1, Yong-Jae Moon2 and Jin-Yi Lee1, (1)Kyung Hee University, Yongin, Korea, Republic of (South), (2)School of Space Research, Kyung Hee University, Yongin, South Korea
Reconstruction of the near-Earth interplanetary coronal mass ejections during 1995-2015: Catalog of geometrical and physical properties (440204)
Teresa Nieves-Chinchilla, Catholic University of America, Washington, United States, Luiz Fernando Guedes dos Santos, Catholic University of America, Washington, DC, United States, Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Nada A Al-Haddad, University of New Hampshire, Durham, United States, Neel Savani, University of Maryland Baltimore County, Baltimore, MD, United States and Adam Szabo, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Thermodynamic description of the dynamics of CMEs (355130)
Alberto Flandes, Instituto de Geofísica, Universidad Nacional Autónoma de México, Mexico City, Mexico and Héctor Javier Durand-Manterola, Universidad Nacional Autónoma de México, Instituto de Geofísica, Mexico, D. F., Mexico
Revisiting Wind's Prograde Orbits During SC23 Maximum: Coronal Mass Ejections (407561)
Noé Lugaz1, Reka Moldovan Winslow2, Charles J Farrugia2, Christina O Lee3, Antoinette Broe Galvin2, Nada A Al-Haddad4, Teresa Nieves-Chinchilla5, Charles William Smith2 and Miho Janvier6, (1)University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States, (2)University of New Hampshire, Durham, United States, (3)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (4)Catholic University of America, Washington, DC, United States, (5)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, (6)Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, Orsay, France
Forecasting Periods of Strong Southward Magnetic Field Following Interplanetary Shocks (426481)
Tarik Mohammad Salman1, Noé Lugaz2, Charles J Farrugia3, Reka Moldovan Winslow3, Antoinette Broe Galvin3 and Nathan Schwadron3, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)University of New Hampshire, Durham, NH, United States, (3)University of New Hampshire, Durham, United States
Comparing Recurring Solar Wind Structures in the Previous and Current Approaches to Solar Minimum (454589)
Antoinette Broe Galvin1, Charles J Farrugia1, Lan Jian2 and Andrea Opitz3, (1)University of New Hampshire, Durham, United States, (2)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, (3)Wigner Research Centre for Physics, Institute for Particle and Nuclear Physics, Budapest, Hungary
The Coronal Hole Influence Parameter (CHIP) as an Important Parameter for Developing the Geomagnetic Storm Prediction Models (453483)
Amaal Abd-Alla Mohamed, National Research Institute of Astronomy and Geophysics, Solar and Space research Lab, Helwan, Egypt and Nat Gopalswamy, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Helium abundance profiles in the large-scale solar-wind phenomena (375360)
Yuri I Yermolaev, Irina G Lodkina, Mikhail Yu. Yermolaev, Elena E. Grigorenko, Natalia L. Borodkova, Maria Riazantseva and Liudmila Rakhmanova, Space Research Institute RAS, Moscow, Russia
Statistical Survey of Solar Wind Dynamic Pressure Pulses based on WIND Observations (456725)
Pingbing Zuo, Harbin Institute of Technology, Shenzhen, Institute of Space Science and Applied Technology, Shenzhen, China and Xueshang Feng, National Space Science Center, Beijing, China
Identifying the arrival of complex structures at 1AU using the seesaw space (468356)
Tatiana Niembro Hernandez and Alejandro Lara, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico
Enhancement of Geomagnetic Storm Intensity Due to Shock-Magnetic Cloud Interaction (424947)
Mengjiao Xu, University of Science and Technology of China, Hefei, China and Chenglong Shen, University Science & Technology of China, Hefei, Anhui, China

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