'Bow shock' diaporamas de présentation

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Cosmic Jets

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Stellar jets (I) History; Properties from observations

Stellar jets (I) History; Properties from observations. Highly collimated jets (ejected gas; supersonic velocities) are observed in many classes of astrophysical objects, both stellar and extragalactic (Livio, 2009): Stellar Extragalactic Young Stellar Objects Active Galactic Nuclei

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Mach Cone Studies with 3D Hydrodynamics

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S.S. Rossolenko 1,2 , E.E. Antonova 1,2 , I.P. Kirpichev 2,1 , Yu.I. Yermolaev 2

Interaction of the solar wind with the magnetosphere of the Earth and the formation of magnetospheric boundary layers. S.S. Rossolenko 1,2 , E.E. Antonova 1,2 , I.P. Kirpichev 2,1 , Yu.I. Yermolaev 2 1. Skobeltsyn Institute of Nuclear Physics Moscow State University, Moscow, Russia

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Multipoint Study of Solar Wind at Solar Minimum

Multipoint Study of Solar Wind at Solar Minimum. Lan K. Jian, Christopher T. Russell IGPP, UCLA STEREO SWG Caltech Nov.14, 2007. Interplanetary Shock Genesis at 1 AU Due to Stream Interaction. STEREO A. STEREO B. STEREO A. STEREO B. Wind. Shock normal:

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MEL 715 : GAS DYNAMICS

MEL 715 : GAS DYNAMICS . P M V Subbarao Associate Professor Mechanical Engineering Department I I T Delhi. A Passion of Doing Adventures lead to a Hi-Fi Science and Technology!!!. The Shocking News. People had dreamed of flying for many years. A Shocking News ?#$?%?

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MESSENGER First Flyby Magnetospheric Results J. A. Slavin and the MESSENGER Team

MESSENGER First Flyby Magnetospheric Results J. A. Slavin and the MESSENGER Team BepiColombo SERENA Team Meeting Santa Fe, New Mexico 11 May 2008. Mariner 10 View of Magnetosphere.

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Measuring the electric potential at the bow shock

Measuring the electric potential at the bow shock. Group A: Tutor: S. Bale Crew: L. Xie L. Yang B. Engavale W.-L. Teh W.-L. Shi X.-G. Zhang. Introduction Data and Analysis Techniques Present result Work to be done.

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The Movement of Charged Particles in a Magnetic Field

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M. Pick, D. Maia, S.J. Wang, A. Lecacheux, D. Haggery, S. E. Hawkins COSPAR 2002

Solar Origin of energetic particle events Near-relativistic impulsive electron events observed at 1 AU. M. Pick, D. Maia, S.J. Wang, A. Lecacheux, D. Haggery, S. E. Hawkins COSPAR 2002. CONTEXT. Association with radio type III bursts (Lin, 1981) In-situ observations IP type III 2-20 KeV

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Universal Heliophysical Processes George Siscoe Boston University

Universal Heliophysical Processes George Siscoe Boston University. 50 years exploring has led to a watershed between exploration and consolidation adolescence and maturity space physics and heliophysics What heliophysics is not

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Van Allen Probes, NOAA, and Ground Observations of a Pc 1 Wave Event Extending 12 Hours in MLT

Van Allen Probes, NOAA, and Ground Observations of a Pc 1 Wave Event Extending 12 Hours in MLT. Mark Engebretson 1 , Jennifer Posch 1 , John Wygant 2 , Craig Kletzing 3 , Geoffrey Reeves 4 , Kjellmar Oksavik 5 , and Tero Raita 6

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Shocks

Shocks. Condensation of water vapour into droplets at the sonic shock. Supersonic shock v bullet = 1.5 v sound. EF2245 Space Physics 2009. Solar wind termination shock. Bow shock in front of magnetosphere. Shocks in space. Bow shock at young star LL Ori. Supernova remnants (SNR).

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Transverse instability of Alfven wave : Cluster observations and heuristic explication.

Summer school - Chalkidiki September 23-28 2003. Transverse instability of Alfven wave : Cluster observations and heuristic explication. Olga Alexandrova LESIA, Observatoire de Paris, France. Earth Bow Shock. B. For :.

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Numerical Investigation of Supersonic Flow Over a Blunt Body

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CRL. Winter. CRL. RAL England. PREPROCESSOR. Summer. Summer. Winter. RAL. Outside User System. CRL Japan. Summer. Summer. Winter. SEC. Summer. Z-axis. RAL. Ingest/ Queue. ACE Instrument Algorithms. Physical Units. DMS. Operations Center. NOAA. ISRO India. RAL

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2. Results

Abstract

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