SH13B:
Sun-to-Earth Evolution and Characteristics of Geoeffective Solar Eruptions I Posters

Submit an Abstract to this Session Please know the abstract submission deadline has passed. There are no exceptions to this deadline and no new abstracts can be submitted.
You can still search the program to see your colleague�s abstract submissions as well as the sessions submitted for the 2016 Fall Meeting. The final program will be released in early October.


Session ID#: 12621

Session Description:
This session will investigate the conditions under which the most geo-effective coronal mass ejections (CMEs) form and propagate in the corona and interplanetary space. Abstracts are invited that discuss topics such as the identification and characterization of the solar source region of the eruption, preconditioning of the corona and heliosphere for CME propagation, interactions of CMEs with the ambient solar wind structures and other CMEs, transformation of the CME flux rope, and geo-effective plasma and magnetic field characteristics at the Earth. Contributions that discuss multi-point observations and modeling that address these questions are especially welcome.
Primary Convener:  Ying D. Liu, NSSC National Space Science Center, CAS, Beijing, China
Conveners:  K Emilia J Kilpua, University of Helsinki, Department of Physics, Helsinki, Finland, Noé Lugaz, University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States and Miho Janvier, Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, Orsay, France
Chairs:  K Emilia J Kilpua, University of Helsinki, Department of Physics, Helsinki, Finland, Miho Janvier, Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, Orsay, France, Ying D. Liu, NSSC National Space Science Center, CAS, Beijing, China and Noé Lugaz, University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States
OSPA Liaison:  Ying D. Liu, NSSC National Space Science Center, CAS, Beijing, China

Cross-Listed:
  • SM - SPA-Magnetospheric Physics
Index Terms:

2111 Ejecta, driver gases, and magnetic clouds [INTERPLANETARY PHYSICS]
2139 Interplanetary shocks [INTERPLANETARY PHYSICS]
7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7954 Magnetic storms [SPACE WEATHER]

Abstracts Submitted to this Session:

Magnetic Source Region Characteristics Influencing the Velocity of Solar Eruptions in the Corona (190044)
Bernhard Kliem, University of Potsdam, Institute of Physics and Astronomy, Potsdam, Germany, Georgios Chintzoglou, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Dr. Tibor Torok, Predictive Science Inc., San Diego, United States, Jie Zhang, George Mason University, Department of Physics and Astronomy, Fairfax, VA, United States and Cooper Downs, Predictive Science Inc., San Diego, CA, United States
Parametric functions of the coronal mass ejection properties close to the Sun based on numerical models (150709)
Ricardo F. González1, Tatiana Niembro Hernandez2, Alejandro Lara2 and Jorge Canto2, (1)Instituto de Radioastronomía y Astrofísica, UNAM, Morelia, Michoacán, Mexico, (2)Universidad Nacional Autonoma de Mexico, Mexico City, Mexico
The Relationship between Stealth CMEs and Coronal Holes: Origin, Interaction, and Geoeffectiveness (199691)
Tamitha Mulligan Skov, Aerospace Corporation El Segundo, El Segundo, CA, United States and Nariaki Nitta, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Sun-to-Earth Characteristics of the 2012 July 12 Coronal Mass Ejection and Associated Geo-effectiveness (127171)
Huidong Hu1,2, Ying D. Liu1,2, Rui Wang1, Christian Moestl3,4, Zhongwei Yang1 and SPODE@NSSC, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)UCAS University of Chinese Academy of Sciences, Beijing, China, (3)Space Research Institute, Austrian Academy of Sciences, Graz, Austria, (4)Institute of Physics, University of Graz, Graz, Austria
On Sun-to-Earth Propagation of Coronal Mass Ejections: II. Slow Events and Comparison with Others (148541)
Ying D. Liu1, Huidong Hu1, Chi Wang1, Janet G Luhmann2, John D Richardson3, Zhongwei Yang1 and Rui Wang1, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (3)MIT, Cambridge, MA, United States
CME Plasma Dynamics using Remote Sensing & In-situ Observations (190202)
Manan Kocher, University of Michigan Ann Arbor, Ann Arbor, MI, United States, Susan T Lepri, University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States and Enrico Landi, University of Michigan Ann Arbor, Departament of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
The ForeCAT In Situ Data Observer and the Effects of Deflection and Rotation on CME Geoeffectiveness (134047)
Christina Kay, Johns Hopkins University Applied Physics Laboratory, Laurel, United States, Nat Gopalswamy, NASA Goddard SFC, Greenbelt, United States, Alysha Reinard, NOAA Boulder, SWPC, Boulder, CO, United States, Merav Opher, Boston University, Astronomy, Boston, MA, United States and Teresa Nieves-Chinchilla, Catholic University of America, Washington, United States
Prediction and Testing of Type II Radio Emission, White Light Images, and CME Properties from the Sun to Earth (170741)
Joachim Matthias Schmidt, University of Sydney, School of Physics,, Sydney, NSW, Australia and Iver Hugh Cairns, University of Sydney, School of Physics, Sydney, NSW, Australia
Comparative Study of the December 28, 2015 – January 2, 2016 and April 7 – 11, 1997 Sun-Earth Connection Events (147990)
Daniel Benjamin Berdichevsky, Berdichevsky Daniel B, MD 20740-4111, College Park, MD, United States, Ian G Richardson, University of Maryland College Park, Department of Astronomy, College Park, MD, United States and Charles J Farrugia, University of New Hampshire, Durham, United States
Numerical study on the interaction between magnetic cloud and heliospheric current sheet (174146)
Man Zhang1 and Xue Shang Feng1,2, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China;, Beijing, China
On the Geo-effectiveness of Shocks and Sheaths (163851)
Noé Lugaz1, Charles J Farrugia2, Reka Moldovan Winslow2, K Emilia J Kilpua3, Nada A Al-Haddad2 and Pete Riley4, (1)University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States, (2)University of New Hampshire, Durham, United States, (3)University of Helsinki, Helsinki, Finland, (4)Predictive Science Inc., San Diego, CA, United States
The variation of the Geoeffectiveness of the Recurrent CIRs during their Life Period (133491)
Yutian Chi1, Chenglong Shen1, Yuming Wang2, Bingxian Luo3, Bingkun Yu4, A Ke Zhao2 and Shui Wang2, (1)University Science & Technology of China, Hefei, Anhui, China, (2)University of Science and Technology of China, Hefei, China, (3)NSSC National Space Science Center, Haidian, Beijing, China, (4)USTC University of Science and Technology of China, Hefei, China
Geoeffectiveness of Fast and Slow Solar Wind Stream Associated to SIRs During 2007-2008 (135660)
Elsa Sanchez-Garcia, National Autonomous University of Mexico, SCiESMEX, Instituto de Geofísica, Unidad Michoacán, Ciudad DE Armería, Mexico, Ernesto Aguilar-Rodriguez, Universidad Nacional Autonoma de Mexico, Instituto de Geofisica, Unidad Michoacan, Morelia, Mexico, Americo Gonzalez-Esparza, Universidad Nacional Autonoma de Mexico, LANCE, Instituto de Geofisica, Unidad Michoacan, Morelia, Mexico and Veronica Ontiveros-Hernandez, Universidad Nacional Autonoma de Mexico, SCiESMEX, Instituto de Geofísica, Unidad Michoacán, Mexico City, Mexico
Identifying large scale structures at 1 AU using fluctuations and  wavelets (136907)
Tatiana Niembro Hernandez and Alejandro Lara, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico
The Grad-Shafranov Reconstruction of Toroidal Magnetic Flux Ropes: Applications to Multi-point Events (154862)
Qiang Hu, University of Alabama in Huntsville, Department of Space Science and CSPAR, Huntsville, AL, United States

See more of: SPA-Solar and Heliospheric Physics