SM13A:
Imaging the Global Dynamics of the Solar Wind-Magnetosphere Interaction II Posters

Submit an Abstract to this Session



Session ID#: 25183

Session Description:
Recent years have seen a host of novel imaging techniques employed to define the state and dynamics of the global solar wind-magnetosphere interaction, and their ability to validate the predictions of global simulations for the solar wind’s interaction with various obstacles within the heliosphere including Venus, Mars, comets, and the Earth. This session is devoted to reviewing the information that can be learned from past, present, and potential future heliophysics, planetary, and astrophysics missions, using global numerical simulations to define the expected images, and describing future imaging techniques. Presentations describing results from previous/current missions, simulations, techniques and ideas for future missions are welcome.
Primary Convener:  Yaireska M Collado-Vega, NASA Goddard Space Flight Center, Moon to Mars Space Weather Analysis Office, Greenbelt, MD, United States
Conveners:  Harald U Frey, University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, Dennis Lee Gallagher, NASA Marshall Space Flight Center, Huntsville, AL, United States and Simon Wing, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Chairs:  Dennis Lee Gallagher, NASA Marshall Space Flight Center, Huntsville, AL, United States, Harald U Frey, University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, Simon Wing, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Yaireska M Collado-Vega, NASA Goddard Space Flight Center, Moon to Mars Space Weather Analysis Office, Greenbelt, MD, United States
OSPA Liaison:  Yaireska M Collado-Vega, NASA Goddard Space Flight Center, Moon to Mars Space Weather Analysis Office, Greenbelt, MD, United States

Cross-Listed:
  • P - Planetary Sciences
  • SH - SPA-Solar and Heliospheric Physics
Index Terms:

2723 Magnetic reconnection [MAGNETOSPHERIC PHYSICS]
2740 Magnetospheric configuration and dynamics [MAGNETOSPHERIC PHYSICS]
2756 Planetary magnetospheres [MAGNETOSPHERIC PHYSICS]
2794 Instruments and techniques [MAGNETOSPHERIC PHYSICS]

Abstracts Submitted to this Session:

Locating the Magnetopause in X-ray Observations (289937)
Kip D Kuntz, Johns Hopkins University, Baltimore, United States
Data-Model Comparisons of Storm-Time Ion Dynamics Using TWINS ENA Images and the Space Weather Modeling Framework (229730)
Amy M Keesee, University of New Hampshire, Physics and Space Science Center, Durham, United States, Yu Huang, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China, Raluca Ilie, University of Illinois at Urbana Champaign, Electrical and Computer Engineering, Urbana, United States, Earl Scime, West Virginia Univ, Morgantown, WV, United States and Michael Warren Liemohn, University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
Boundary Detection in Three Dimensions With Application to the SMILE mission (281159)
Anders Moller Jorgensen1, Tianran Sun2, Chi Wang3, Lei Dai4, Steven Sembay5, Fei Wei2, Yihong Guo2 and Xu Ronglan2, (1)New Mexico Institute of Mining and Technology, Electrical Engineering Department, Socorro, NM, United States, (2)NSSC National Space Science Center, CAS, Beijing, China, (3)NSSC, CAS, Beijing, China, (4)CAS Chinese Academy of Sciences, National Space Science Center, Beijng, China, (5)University of Leicester, Leicester, United Kingdom
What Solar Wind Conditions Lead to the Generation of the Different Types of Poleward-Moving Auroral Forms? (300419)
Gerard J Fasel1, Alex Booth2, Ashley Golla3, David Cook2, Juliet Elise Mills2, Simone Raeth2, Jennifer Lau4, Kaseba Chibwe2, Fred Sigernes5 and Dag A Lorentzen6, (1)Pepperdine University, Natural Science, Malibu, CA, United States, (2)Pepperdine University, Malibu, CA, United States, (3)State College, PA, United States, (4)Pepperdine University, natural science department, Malibu, CA, United States, (5)University Centre in Svalbard, Longyearbyen, Norway, (6)UNIS, Longyearbyen, Norway
Storm-Time Ring Current Ion Distributions Deduced from the IMAGE/HENA Observations (291305)
Syau-Yun Wang Hsieh1, Pontus C. Brandt1, Robert Demajistre2 and Grant Killian Stephens1, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Johns Hopkins Applied Physics Laboratory, Laurel, United States
Twisting of Earth's Neutral Sheet and its Response to Changes in the IMF By Component (255115)
Nathan Case, Lancaster University, Department of Physics, Lancaster, United Kingdom, Adrian Grocott, Lancaster University, Physics Department, Lancaster, United Kingdom, Carley Martin, Lancaster University, Lancaster, United Kingdom, Stein Haaland, University Centre in Svalbard, IFT, Longyearbyen, Norway and Tsugunobu Nagai, ISAS/JAXA, Sagamihara, Japan
Magnetosphere and ionosphere response to a positive-negative pulse pair of solar wind dynamic pressure (251303)
Anmin Tian, Shandong University at Weihai, Institute of Space Science, Weihai, China and Alex W Degeling, Shandong University at Weihai, Weihai, China
Does the Magnetosphere go to Sleep? (270543)
Michael Hesse1, Therese Moretto Jorgensen1,2, Eigil A Friis-Christensen3, Masha Kuznetsova4, Nikolai Ostgaard5, Paul Tenfjord6 and Hermann J Opgenoorth7, (1)University of Bergen, Bergen, Norway, (2)National Science Foundation, Arlington, VA, United States, (3)DTU, Kongens Lyngby, Denmark, (4)NASA Goddard Space Flight Center, Community Coordinated Modeling Center, Greenbelt, United States, (5)University of Bergen, Department of Physics and Technology, Bergen, Norway, (6)University of Bergen, Birkeland Centre for Space Science, Bergen, Norway, (7)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden

See more of: SPA-Magnetospheric Physics