SH21A:
Collisionless Shock Waves in Astrophysical Plasmas I Posters

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Session ID#: 12637

Session Description:
Collisionless shocks are ubiquitous in heliospheric and astrophysical plasmas, producing a wide range of phenomena from microscopic energy dissipation to macroscopic foreshocks filled with suprathermal shock accelerated particles.  This session is meant to be general so as to include all topics that are specific to collisionless shock waves in astrophysical plasmas, including but not limited to interplanetary shocks and planetary bow shocks.  Therefore, we invite presentations that focus on shock-related processes from both theory/simulation and observational work.
Primary Convener:  Lynn B Wilson III, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Conveners:  Drew L Turner, The Aerospace Corporation, El Segundo, CA, United States and Adnane Osmane, Aalto University, Aalto, Finland
Chairs:  Lynn B Wilson III, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Adnane Osmane, Aalto University, Aalto, Finland
OSPA Liaison:  Lynn B Wilson III, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Index Terms:

7829 Kinetic waves and instabilities [SPACE PLASMA PHYSICS]
7845 Particle acceleration [SPACE PLASMA PHYSICS]
7851 Shock waves [SPACE PLASMA PHYSICS]
7867 Wave/particle interactions [SPACE PLASMA PHYSICS]

Abstracts Submitted to this Session:

Ion acceleration and its effect in shock-shock interaction (133087)
Masaru Nakanotani, IRAP, CNRS - University Paul sabatier, Toulouse, France; Kyushu University, Fukuoka, Japan, Shuichi Matsukiyo, Kyushu University, International Center for Space Weather Science and Education (ICSWSE), Fukuoka, Japan, Tohru Hada, Kyushu University, Department of Advanced Environmental Science and Engineering, Faculty of Engineering Sciences, Fukuoka, Japan and Christian Xavier Mazelle, University Paul Sabatier Toulouse III, Toulouse Cedex 09, France
Ion transmission and reflection in low-Mach number shocks (134853)
Michael Gedalin, Ben-Gurion University of the Negev, Beer Sheva, Israel and Michael A Balikhin, University of Sheffield, Sheffield, S1 3JD, United Kingdom
Langmuir waveforms at interplanetary shocks: STEREO statistical analysis (127130)
Carine Briand, LESIA, Observatoire de Paris, CNRS, UPMC, UPD, Meudon, France
Shock Wave Structure Mediated by Energetic Particles (127576)
Parisa Mostafavi, Princeton University, Princeton, NJ, United States, Gary Paul Zank, University of Alabama in Huntsville, Space Science, Huntsville, AL, United States and Gary M Webb, University of Alabama in Huntsville, CSPAR, Huntsville, AL, United States
Interaction of Weibel and Synchrotron Maser Instabilities in Astrophysical Shock Precursor Waves (130486)
Masanori Iwamoto, University of Tokyo, Bunkyo-ku, Japan, Takanobu Amano, University of Tokyo, Graduate School of Science, Bunkyo-ku, Japan, Yosuke Matsumoto, Chiba University, Chiba, Japan and Masahiro Hoshino, The University of Tokyo, Tokyo, Japan
Electron Surfing Acceleration in High Mach Number Shocks (140220)
Masahiro Hoshino, The University of Tokyo, Tokyo, Japan, Takanobu Amano, University of Tokyo, Graduate School of Science, Bunkyo-ku, Japan and Yosuke Matsumoto, Chiba University, Chiba, Japan
Prolonged electron accelerations at a high-Mach-number, quasi-perpendicular shock (123319)
Yosuke Matsumoto, Chiba University, Chiba, Japan, Takanobu Amano, University of Tokyo, Graduate School of Science, Bunkyo-ku, Japan, Tsunehiko Kato, NAOJ National Astronomical Observatory of Japan, Tokyo, Japan and Masahiro Hoshino, The University of Tokyo, Tokyo, Japan
Relativistic electrons produced by transient ion foreshock phenomena (117943)
Lynn B Wilson III, NASA Goddard Space Flight Center, Greenbelt, MD, United States, David G Sibeck, NASA/GSFC, Greenbelt, United States, Drew L Turner, The Aerospace Corporation, El Segundo, CA, United States, Adnane Osmane, Aalto University, Aalto, Finland, Damiano Caprioli, Princeton University, Department of Astrophysical Sciences, Princeton, United States and Vassilis Angelopoulos, University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, CA, United States
Two Types of Whistler Instabilities in the Foot of Quasi-perpendicular Supercritical Shocks: a Poynting Flux Analysis (147491)
Laurent Muschietti1,2 and Bertrand Lembege2, (1)University of California Berkeley, SSL, Berkeley, CA, United States, (2)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France
impact of realistic plasma conditions on characteristic scales/amplitudes of macroscopic fields of quasi-perpendicular supercritical shock front. (154244)
Bertrand Lembege, LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, Zhongwei Yang, NSSC National Space Science Center, CAS, Beijing, China and Shuichi Matsukiyo, Kyushu University, International Center for Space Weather Science and Education (ICSWSE), Fukuoka, Japan
Whistler-mode Waves Upstream of Saturn (149615)
Ali H Sulaiman1, Donald A Gurnett2, Jasper S Halekas3, Japheth N Yates4, William S Kurth3 and Michele Karen Dougherty4, (1)University of Minnesota, School of Physics and Astronomy, Minneapolis, United States, (2)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (3)University of Iowa, Iowa City, IA, United States, (4)Imperial College London, London, United Kingdom
Ion dynamics at a rippled quasi-parallel shock: 2D hybrid simulations (118053)
Yufei Hao1,2, Quanming Lu1,2, Xinliang Gao1,2 and Shui Wang1,2, (1)University of Science and Technology of China, Hefei, China, (2)Collaborative Innovation Center of Astronautical Science and Technology, Hefei, China
Effect of field-aligned-beam in parallel diffusion of energetic particles in the Earth's foreshock (152808)
Shuichi Matsukiyo1, Kento Nakanishi2, Fumiko Otsuka3, Arpad Kis4, Istvan Lemperger4 and Tohru Hada5, (1)Kyushu University, International Center for Space Weather Science and Education (ICSWSE), Fukuoka, Japan, (2)Kyushu University, Fukuoka, Japan, (3)ESST Kyushu University, Fukuoka, Japan, (4)Hungarian Academy of Sciences, Budapest, Hungary, (5)Kyushu University, Department of Advanced Environmental Science and Engineering, Faculty of Engineering Sciences, Fukuoka, Japan
Nonlinear growth of magnetic pulses in the upstream of Earth's bow shock (199480)
Ensang Lee1, George K Parks2, Naiguo Lin3, Zhongwei Yang4, Ying D. Liu4, Suiyan Fu5 and Jinhy Hong6, (1)Kyung Hee University, School of Space Research, Yongin, South Korea, (2)University of California Berkeley, Berkeley, United States, (3)Univ California Berkeley, Berkeley, CA, United States, (4)NSSC National Space Science Center, CAS, Beijing, China, (5)Peking University, School of Earth and Space Sciences, Beijing, China, (6)Kyung Hee University, School of Space Research, Yongin, Korea, Republic of (South)
Mass, charge and energy dependence of solar wind interaction with Earth's bow shock (152056)
George K Parks1, Ensang Lee2, Suiyan Fu3, Ying D. Liu4, Zhongwei Yang4 and Hee-Eun Kim5, (1)University of California Berkeley, Berkeley, United States, (2)Kyung Hee University, School of Space Research, Yongin, South Korea, (3)Peking University, School of Earth and Space Sciences, Beijing, China, (4)NSSC National Space Science Center, CAS, Beijing, China, (5)Dept. of Astronomy and Space Science, Kyung Hee University, Yongin, Gyeonggi, South Korea
WAVE PHENOMENA ASSOCIATED WITH INTERPLANETARY SHOCKS (177183)
Thejappa Golla, University of Maryland College Park, College Park, MD, United States and Robert J. MacDowall, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Modeling the Earth’s ULF Foreshock: Self-consistent Monte Carlo Simulations versus Hybrid-Vlasov Simulations (175236)
Alexandr N. Afanasiev1, Rami O Vainio1, Minna Palmroth2, Yann Pfau-Kempf2, Urs Ganse2 and Markus Battarbee3, (1)University of Turku, Department of Physics and Astronomy, Turku, Finland, (2)Finnish Meteorological Institute, Helsinki, Finland, (3)Jeremiah Horrocks Institute, University of Central Lancashire, Preston, United Kingdom
Comparison of 1-D PIC simulations with GBDR and Langmuir waves observations in front of the Saturnian bow shock. (175415)
Marek Basovník1,2, David Pisa3, Miroslav Horky1, Ondrej Santolik1,2, Jan Soucek4, William S Kurth5 and Donald A Gurnett6, (1)Institute of Atmospheric Physics ACSR, Praha 4, Czech Republic, (2)Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic, (3)Institute of Atmospheric Physics ACSR, Department of Space Physics, Praha 4, Czech Republic, (4)Institute of Atmospheric Physics of the Czech Academy of Sciences, Department of Space Physics, Prague, Czech Republic, (5)University of Iowa, Iowa City, IA, United States, (6)University of Iowa, Physics and Astronomy, Iowa City, IA, United States
Determination of the dynamics of low frequency turbulence upstream and downstream of the Earth’s Bow shock using Cluster measurements (175578)
Stefanos Giagkiozis1, Simon N Walker2 and Keith Yearby2, (1)University of Sheffield, Automatic Control and Systems Engineering, Sheffield, United Kingdom, (2)University of Sheffield, Sheffield, S10, United Kingdom
Multispacecraft study of shock-flux rope interaction (158420)
Xochitl Blanco-Cano, Instituto de Geofísica Universidad Nacional Autónoma de México, Mexico City, Mexico, David Burgess, Queen Mary, University of London, London, United Kingdom, Torbjorn Sundberg, Queen Mary, University of London, London, E1, United Kingdom and Primoz Kajdic, UNAM National Autonomous University of Mexico, Department of Space Sciences, Mexico City, Mexico
Diffuse Ion Spatial Profiles Along the Magnetic Field Line and Along the Bow Shock Normal: a Comparative Study at the Earth's Quasi-Parallel Bow Shock (192732)
Arpad Kis, Institute of Earth Physics and Space Science, Sopron, Hungary, Manfred Scholer, The Max Planck Institute for Extraterrestrial Physics, Garching, Germany, Berndt Klecker, Max Planck Institut for Extraterrestrial Physics, Garching, Germany and Iannis S Dandouras, IRAP, Toulouse, France
Laboratory Observation of Laser-Driven, Supercritical Collisionless Shocks (158843)
Derek Schaeffer1, William Fox2, Dan Haberberger3, Gennady Fiksel4, Amitava Bhattacharjee5,6, D Barnak3,7, Suxing Hu8 and Kai Germaschewski9, (1)University of California Los Angeles, Physics & Astronomy, Los Angeles, CA, United States, (2)Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (3)University of Rochester, Laboratory for Laser Energetics, Rochester, NY, United States, (4)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (5)Princeton University, Princeton, NJ, United States, (6)Princeton Plasma Physics Laboratory, Princeton, United States, (7)University of Rochester, Fusion Science Center for Extreme States of Matter, Rochester, United States, (8)University of Rochester, Laboratory for Laser Energetics, Rochester, United States, (9)University of New Hampshire, Durham, NH, United States
IST, Intermediate Shocks and Magnetic Decreases (199636)
Bob Hamilton, George Fox University, Newberg, OR, United States and Zach Koontz, George Fox University, College of Engineering, Newberg, OR, United States

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