SH53A:
Large-Scale Interplanetary Structures: Sources, Evolution, Space Weather Effects, and Solar Cycle Variations Posters

Submit an Abstract to this Session



Session ID#: 23872

Session Description:
Since 1994, WIND, ACE and other satellites have continuously recorded the in-situ solar wind magnetic field and plasma parameters near the Earth for about two solar cycles. Using these measurements, different large-scale interplanetary structures, such as interplanetary coronal mass ejections (ICMEs), stream interaction regions (SIRs), shocks and also their mixed structures, have been reported and studied. Now, it is well accepted that these structures are the main causes of geospace environmental disturbances. Most discussions about the large-scale interplanetary structures focused on the following issues: (1) their solar or interplanetary sources; (2) the propagation and interaction between these structures; (3) the evolution of interplanetary structures and their variations with solar cycle; (4) the space weather effect of these phenomena. This session will exhibit and discuss the recent advances in understanding these issues, especially the progress on the interaction between multiple interplanetary structures and the variation of these structures with solar cycles.
Primary Convener:  Chenglong Shen, University Science & Technology of China, Hefei, Anhui, China
Conveners:  Lan Jian, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Nat Gopalswamy, NASA Goddard SFC, Greenbelt, United States and Bingxian Luo, NSSC National Space Science Center, Haidian, Beijing, China
Chairs:  Lan Jian, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Bingxian Luo, NSSC National Space Science Center, Haidian, Beijing, China
OSPA Liaison:  Chenglong Shen, University Science & Technology of China, Hefei, Anhui, China
Index Terms:

2101 Coronal mass ejections [INTERPLANETARY PHYSICS]
2102 Corotating streams [INTERPLANETARY PHYSICS]
2111 Ejecta, driver gases, and magnetic clouds [INTERPLANETARY PHYSICS]
2162 Solar cycle variations [INTERPLANETARY PHYSICS]

Abstracts Submitted to this Session:

Tracking Energetics of a CME Core in the Low Solar Corona (301010)
Manan Kocher, University of Michigan Ann Arbor, Ann Arbor, MI, United States, Enrico Landi, University of Michigan, Ann Arbor, MI, United States and Susan T Lepri, University of Michigan, Ann Arbor, United States
Predicting ICME properties at 1AU (278119)
Alisson Dal Lago, Carlos Roberto Braga, Amanda Lucia Mesquita and Rafael Rodrigues Souza De Mendonça, INPE National Institute for Space Research, Sao Jose dos Campos, Brazil
Why a geoeffective CME was missed by SOHO LASCO? (251708)
Yutian Chi1, Jie Zhang2, Chenglong Shen3, Phillip Hess4, Li Feng5, Yuming Wang3 and Wageesh Mishra1, (1)University of Science and Technology of China, Hefei, China, (2)George Mason University, Department of Physics and Astronomy, Fairfax, United States, (3)USTC University of Science and Technology of China, Hefei, China, (4)George Mason University Fairfax, Fairfax, United States, (5)Max Planck Institute for Solar System Research, Goettingen, Germany
Variations of Helium Parameters within ICMEs (257372)
Jana Safrankova, Charles University, Prague, 180, Czech Republic, Tereza Durovcova, Charles University, Prague, Czech Republic and Zdenek Nemecek, Charles University, Faculty of Mathematics and Physics, Prague, 180, Czech Republic
Numerical simulations of the solar wind transients in terms of the spacecraft position (258191)
Ricardo F. González1, Tatiana Niembro Hernandez2, Alejandro Lara1 and Jorge Cantó Illa3, (1)National Autonomous University of Mexico, Ciudad DE Armería, Mexico, (2)Universidad Nacional Autonoma de Mexico, Mexico City, Mexico, (3)National Autonomous of Mexico, Astronomy, Mexico City, Mexico
CME Simulations with Boundary Conditions Derived from Multiple Viewpoints of STEREO (287665)
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
Lessons Learned from 10 Years of STEREO Solar Wind Observations (274774)
Lan Jian, University of Maryland, College Park, College Park, MD, United States; NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, Christopher T Russell, University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, CA, United States, Janet G Luhmann, Space Sciences Laboratory, University of California Berkeley, Berkeley, United States and Antoinette Broe Galvin, University of New Hampshire, Durham, NH, United States
Comparing Temporally-Separated Solar Wind Structures at 1 AU (STEREO A and OMNI) (258968)
Antoinette Broe Galvin, University of New Hampshire, Durham, United States, Charles J Farrugia, New hampshire university, Durham, NH, United States and Lan Jian, University of Maryland, College Park, College Park, MD, United States
High-speed Solar Wind Stream Forecast Based on Coronal Hole Index Derived from Solar EUV Images (230773)
Jiancun Gong, Bingxian Luo, Xuan Bu and Siqing Liu, National Space Science Center, CAS, Beijing, China
Relationship between coronal holes and high speed streams at L1: arrival times, durations, and intensities (230804)
Bingxian Luo, Xuan Bu, Siqing Liu and Jiancun Gong, National Space Science Center, CAS, Beijing, China
Studying Solar Wind Properties Around CIRs and Their Effects on GCR Modulation (296024)
Keyvan Ghanbari, University of Alabama in Huntsville, Space Science, Huntsville, AL, United States and Vladimir A Florinski, University of Alabama, Huntsville, United States
The geoeffectiveness of CIRs and ICMEs (295133)
Chenglong Shen, University of Science and Technology of China, Hefei, China, Yutian Chi, University of Science and Technology of China, Anhui, China and Yuming Wang, USTC University of Science and Technology of China, Hefei, China
Relative Contributions of Coronal Mass Ejections and High-speed Streams to the Long-term Variation of Annual Geomagnetic Activity: Solar Cycle Variation and Latitudinal Differences (279860)
Lauri Holappa, University of Oulu, Space Physics and Astronomy Research Unit, Oulu, Finland and Kalevi Mursula, University of Oulu, ReSoLVE Centre of Excellence, Space Climate Research Unit, Oulu, Finland
The seesaw space, a vector space to identify and characterize large-scale structures at 1 AU (227658)
Tatiana Niembro Hernandez, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico and Alejandro Lara, National Autonomous University of Mexico, Ciudad DE Armería, Mexico
Dependence of the Interplanetary Magnetic Field on Heliocentric Distance between 0.3 and 1.7 AU from MESSENGER, ACE and MAVEN data (267482)
Cedar Hanneson, University of Alberta, Edmonton, AB, Canada, Catherine Johnson, Planetary Science Institute, Tucson, United States and Manar Al Asad, University of British Columbia, Department of Earth, Ocean and Atmospheric Sciences, Vancouver, BC, Canada
Cosmic Ray Modulation and Radiation Dose of Aircrews During Possible Grand Minimum (273083)
Shoko Miyake, National Institute of Technology (KOSEN), Ibaraki College, Ibaraki, Japan, Ryuho Kataoka, NIPR National Institute of Polar Research, Tokyo, Japan; The Graduate University for Advanced Studies, SOKENDAI, Kanagawa, Japan, Tatsuhiko Sato, Japan Atomic Energy Agency, Tokai, Japan, Shinsuke Imada, Nagoya University, ISEE, Nagoya, Japan, Hiroko Miyahara, Musashino Art University, Kodaira-city, Japan, Daikou Shiota, National Institute of Information and Communications Technology, Tokyo, Japan, Tomoaki Matsumoto, Hosei University, Tokyo, Japan and Haruka Ueno, Japan Aerospace Exploration Agency, Tokyo, Japan

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