301:
Coupling Processes in Geospace During Enhanced Solar Wind Driving I Posters


Session ID#: 40525

Session Description:
Geospace is a highly coupled system that involves inter-regional and cross-scale interaction processes. Those processes are particularly evident during disturbed conditions driven by enhanced solar wind driving and explosive release of magnetotail energy, which results in storms and substorms. To achieve system-level understanding of the terrestrial space environment, it is essential to understand plasma and energy transport by particles and fields to/from neighboring domains in the magnetosphere-ionosphere-thermosphere system. Examples of those can be found in magnetopause processes, plasma circulation (plume, patches and outflow), particle injection/energization/precipitation, fast flow channels, wave-particle interaction, and field-aligned currents. It is critical to utilize growing capability of observations by multi-satellites and ground-based network such as the Heliophysics/Geospace System Observatory, as well as global/multi-scale simulations, for advancing community's understanding of Geospace dynamics.

This session solicits presentations on a wide range of coupling processes in the Earth's magnetosphere, ionosphere and thermosphere system; including solar wind-magnetosphere interaction, tail-inner magnetosphere interaction, magnetosphere-ionosphere-thermosphere coupling, and global magnetospheric processes. Observations in space and ground, simulations and theory are invited. Recent progresses, future planning and discussion on open questions are welcome.

Primary Convener:  Yukitoshi Nishimura, Boston University, Boston, MA, United States
Conveners:  Christine Gabrielse, The Aerospace Corporation, El Segundo, United States and Ying Zou, Boston University, Boston, MA, United States
Index Terms:

2736 Magnetosphere/ionosphere interactions [MAGNETOSPHERIC PHYSICS]
2744 Magnetotail [MAGNETOSPHERIC PHYSICS]
2784 Solar wind/magnetosphere interactions [MAGNETOSPHERIC PHYSICS]
2788 Magnetic storms and substorms [MAGNETOSPHERIC PHYSICS]

Abstracts Submitted to this Session:

 
301.078
The Magnetosphere of the Earth under Sub‐Alfvénic Solar Wind Conditions as Observed on 24 and 25 May 2002 (335263)
Emmanuel Chané1, Joachim Saur2, Joachim Raeder3, Fritz M. Neubauer2 and Stefaan Poedts4, (1)Katholieke Universiteit Leuven, Leuven, Belgium, (2)University of Cologne, Cologne, Germany, (3)University of New Hampshire, Space Science Center, Durham, United States, (4)KU Leuven, Centre for mathematical Plasma-Astrophysics, Department of Mathematics, Leuven, Belgium
 
301.080
Faux Magnetopause Crossings and How to Recognize Them (334232)
Yi Qi, University of California, Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, United States, Cong Zhao, Univ. of Sci. & Tech. of China, Hefei, China, Una Gaylin Schneck, UCLA, Earth Planetary And Space Sciences, Los Angeles, United States, Hairong Lai, Sun Yat-Sen University, Guangzhou, China and Christopher T Russell, University of California Los Angeles, Los Angeles, CA, United States
 
301.081
Magnetosphere-ionosphere responses to foreshock and magnetosheath transients (335069)
Yukitoshi Nishimura, Boston University, Boston, MA, United States, Boyi Wang, University of California, Los Angeles, Departments of Atmospheric and Oceanic Sciences, Los Angeles, United States, Ying Zou, The University of Alabama in Huntsville, Huntsville, United States, Eric Donovan, University of Calgary, Physics and Astronomy, Calgary, AB, Canada, Vassilis Angelopoulos, University of California, Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, United States, Joran Moen, University Centre in Svalbard, Longyearbyen, Norway, Lasse Boy Novock Clausen, University of Oslo, Department of Physics, Oslo, Norway and Tsutomu Nagatsuma, NICT National Institute of Information and Communications Technology, Tokyo, Japan
 
301.082
Statistical Properties of Meso-scale Plasma Flows in the Nightside High-latitude Ionosphere (335775)
Christine Gabrielse, The Aerospace Corporation, El Segundo, United States, Yukitoshi Nishimura, University of California Los Angeles, Los Angeles, CA, United States; Boston University, Boston, MA, United States, Larry R Lyons, University of California Los Angeles, Department of Atmospheric and Oceanic Sciences, Los Angeles, CA, United States, Bea Gallardo-Lacourt, University of Calgary, Calgary, AB, Canada, Yue Deng, University of Texas at Arlington, Arlington, TX, United States and Kathryn A McWilliams, University of Saskatchewan, Saskatoon, SK, Canada
 
301.083
Ionospheric Polar Cap Patches Observed in Antarctic Summer using Swarm (333933)
Alex Chartier, Johns Hopkins University, Applied Physics Laboratory, Laurel, United States
 
301.084
Prediction of entry paths of solar wind ions into the inner magnetosphere using a toy model (335841)
Hadi Madanian1, J. Douglas Patterson2, Grant Stephens3, Donald G Mitchell4, Jerry Wayne Manweiler2 and Louis J Lanzerotti5, (1)Epex Scientific, Richmond, United States, (2)Fundamental Technologies, LLC, Lawrence, KS, United States, (3)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)New Jersey Inst Tech, Newark, United States
 
301.085
The detection of ultra-relativistic electrons in low Earth orbit by the LYRA instrument on board the PROBA2 satellite (334911)
Athanassios Katsiyannis, Observatoire Royal de Belgique, Brussel, Belgium, Marie Dominique, Royal Observatory of Belgium, Brussels, Belgium, Viviane Pierrard, Royal Belgian Institute for Space Aeronomy, Brussels, Belgium and Graciela Lopez Rosson, Royal Belgian Institute for Space Aeronomy, Space Physics, Brussels, Belgium
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