SM33B:
Imaging the Global Dynamics of the Solar Wind: Magnetosphere Interaction I Posters

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Session ID#: 17772

Session Description:
In conjunction with global simulations, global imagers provide an opportunity to define the nature of the solar wind’s interaction with a variety of heliospheric obstacles.  This session is devoted to reviewing the information that can be learned from past and present heliophysics, planetary, and astrophysics missions, using global numerical simulations to help us define the expected images, and describe future imaging techniques.  Recent years have seen a host of novel imaging techniques employed to define the state 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.  Presentations describing results from previous missions, simulations, 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:  Gerard J Fasel, Pepperdine University, Natural Science, Malibu, CA, United States, Syau-Yun Wang Hsieh, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Steven Sembay, University of Leicester, Leicester, United Kingdom
Chairs:  David G Sibeck, NASA/GSFC, Greenbelt, United States, Steven M Petrinec, Lockheed Martin Corporation, Arlington, VA, United States and Thomas Cravens, University of Kansas, Physics and Astronomy, Lawrence, KS, United States
OSPA Liaison:  Yaireska M Collado-Vega, NASA Goddard Space Flight Center, Moon to Mars Space Weather Analysis Office, Greenbelt, MD, United States
Index Terms:

2723 Magnetic reconnection [MAGNETOSPHERIC PHYSICS]
2724 Magnetopause and boundary layers [MAGNETOSPHERIC PHYSICS]
2740 Magnetospheric configuration and dynamics [MAGNETOSPHERIC PHYSICS]
2794 Instruments and techniques [MAGNETOSPHERIC PHYSICS]

Abstracts Submitted to this Session:

The SMILE Mission: Orbit Design and Observation Strategy (133107)
Jianhua Zheng1,2, Xi Zheng Yu1, Chi Wang1, Tianran Sun1, Jian Wei Han1, Denis Rebuffat3, C Philippe Escoubet3, Xiao Cheng Zhu4, Graziella Branduardi-Raymont5, Lei Li1, Fei Wei1, Lei Dai6 and Walfried Raab3, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)University of Chinese Academy of Sciences, Beijing, China, (3)European Space Research and Technology Centre, Noordwijk Zh, Netherlands, (4)ShangHai Engineering Center for Micro-satellite, ShangHai, China, (5)University College London, Mullard Space Science Laboratory, London, United Kingdom, (6)National Space Science Center, Chinese Academy of Sciences, Beijing, China
In situ plasma and magnetic field measurements of SMILE (144286)
Lei Li1, Lei Dai2, Jingdong Wang1, Aibing Zhang1, Linggao Kong1, Chi Wang1, Graziella Branduardi-Raymont3, C Philippe Escoubet4, David G Sibeck5, Jianhua Zheng1, Denis Rebuffat4 and Walfried Raab4, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)National Space Science Center, Chinese Academy of Sciences, Beijing, China, (3)University College London, Mullard Space Science Laboratory, London, United Kingdom, (4)European Space Research and Technology Centre, Noordwijk Zh, Netherlands, (5)NASA/GSFC, Greenbelt, United States
Magnetopause Surface Reconstruction from Tangent Vector Observations (138276)
Michael R Collier, NASA/GSFC, Greenbelt, MD, United States and Hyunju KIM Connor, NASA Goddard Space Flight Center, Geospace Physics Laboratory, Greenbelt, MD, United States
X-ray Magnetosheath Emission from Solar Wind Charge Exchange During Two CME Events in 2001 (156394)
Ian Carl Whittaker1, Steven Sembay2, Andrew Read1, Jennifer Alyson Carter2, Steve E Milan1 and Minna Palmroth3, (1)University of Leicester, Leicester, United Kingdom, (2)University of Leicester, Leicester, LE1, United Kingdom, (3)Finnish Meteorological Institute, Helsinki, Finland
X-ray modeling for SMILE (172169)
Tianran Sun1, Chi Wang2, Fei Wei1, Z.-Q. Liu1, Jianhua Zheng1, Xi Zheng Yu1, Steven Sembay3 and Graziella Branduardi-Raymont4, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)NSSC, CAS, Beijing, China, (3)University of Leicester, Leicester, United Kingdom, (4)University College London, Mullard Space Science Laboratory, London, United Kingdom
The STORM and CuPID soft X-ray cameras on the DXL sounding rocket mission: Employment of slumped micropore optics to image solar wind charge exchange X-ray emission in the magnetosheath. (183127)
Nicholas Thomas, NASA Goddard Space Flight Center, Greenbelt, MD, United States and The STORM and DXL Team
Selection of FUV Auroral Imagers for Satellite Missions (165742)
Craig Unick1, Eric Donovan2, Emma Spanswick2, Vadim Uritsky3 and Greg Enno2, (1)Keo Scientific Ltd., Calgary, Canada, (2)University of Calgary, Physics and Astronomy, Calgary, AB, Canada, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States
The First Light for a New Ground-based Imaging Capability of JHU/APL in Support of Auroral Science Campaigns and Missions (185510)
Syau-Yun Wang Hsieh, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, David G Sibeck, NASA/GSFC, Greenbelt, United States and Donald L Hampton, University of Alaska Fairbanks, Fairbanks, AK, United States
The Brightening History of Poleward-Moving Auroral Forms (190740)
Gerard J Fasel1, Taylor Glenn Brandt2, Ashley Rothballer2, Emma Harper2, Uni Kim2, Jacques Joubert2, Juliet Elise Mills2, Alex Booth2, Connor Nam2, Paige Grittner2, Kaseba Chibwe2, Simone Raeth2, Karin Frizzelle2, Charles Lammerding2, Rachel Lockwood2, Ben Fox2, Michael Gribble2, Fred Sigernes3, Dag A Lorentzen4, Riley Josh2 and Ashley Golla2, (1)Pepperdine University, Natural Science, Malibu, CA, United States, (2)Pepperdine University, Malibu, CA, United States, (3)University Centre in Svalbard, Longyearbyen, Norway, (4)UNIS, Longyearbyen, Norway
Reconfiguration of Reverse Convection in the Dayside Throat Region under Varying Northward IMF Conditions (191313)
Maimaitirebike Maimaiti1, J Michael Ruohoniemi2, Joseph BH Baker1, C. Robert Clauer3, Michael J Nicolls4 and Marc R Hairston5, (1)Virginia Tech, Blacksburg, VA, United States, (2)Virginia Tech, Blacksburg, United States, (3)National Institute of Aerospace, Hampton, VA, United States, (4)SRI International Menlo Park, Menlo Park, CA, United States, (5)University of Texas at Dallas, William B. Hanson Center for Space Sciences, Richardson, TX, United States

See more of: SPA-Magnetospheric Physics