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Titlebook: 30th International Symposium on Shock Waves 2; ISSW30 - Volume 2 Gabi Ben-Dor,Oren Sadot,Ozer Igra Conference proceedings 2017 Springer Int

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期刊全称30th International Symposium on Shock Waves 2
期刊简称ISSW30 - Volume 2
影响因子2023Gabi Ben-Dor,Oren Sadot,Ozer Igra
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发行地址Includes supplementary material:
图书封面Titlebook: 30th International Symposium on Shock Waves 2; ISSW30 - Volume 2 Gabi Ben-Dor,Oren Sadot,Ozer Igra Conference proceedings 2017 Springer Int
影响因子These proceedings collect the papers presented at the 30th International Symposium on Shock Waves (ISSW30), which was held in Tel-Aviv Israel from July 19 to July 24, 2015. The Symposium was organized by Ortra Ltd. The ISSW30 focused on the state of knowledge of the following areas: Nozzle Flow, Supersonic and Hypersonic Flows with Shocks, Supersonic Jets, Chemical Kinetics, Chemical Reacting Flows, Detonation, Combustion, Ignition, Shock Wave Reflection and Interaction, Shock Wave Interaction with Obstacles, Shock Wave Interaction with Porous Media, Shock Wave Interaction with Granular Media, Shock Wave Interaction with Dusty Media, Plasma, Magnetohyrdrodynamics, Re-entry to Earth Atmosphere, Shock Waves in Rarefied Gases, Shock Waves in Condensed Matter (Solids and Liquids), Shock Waves in Dense Gases, Shock Wave Focusing, Richtmyer-Meshkov Instability, Shock Boundary Layer Interaction, Multiphase Flow, Blast Waves, Facilities, Flow Visualization, and Numerical Methods. The two volumes serve as a reference for the participants of the ISSW30 and anyone interested in these fields.
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978-3-319-83152-7Springer International Publishing AG 2017
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How European Was the Revolution of 1848/49?tically motionless medium. The position of these zones at the body surface and their size strongly depend on and are controlled by the direction and value of the dipole magnetic moment. The gasdynamic streamlines bypass the separation zone following close to the magnetic lines of force. The surface
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1848: Connected or Comparable Revolutions?on systems are still open questions. In many of these systems, the background magnetic field is parallel to the jet propagation direction. Recent experiments [1] performed at the Jupiter Laser Facility investigated the effects of imposing a background magnetic field aligned with a collimated jet. Pl
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