'Shock speed' presentation slideshows

Gas Dynamics, Lecture 7 (Shocks & Point Explosions) see: astro.ru.nl/~achterb/

Prof. dr. A. Achterberg, Astronomical Dept. , IMAPP, Radboud Universiteit. Gas Dynamics, Lecture 7 (Shocks & Point Explosions) see: www.astro.ru.nl/~achterb/. Summary of shock physics. Shocks occur in supersonic flows; Shocks are sudden jumps in velocity, density and pressure;

796 views • 60 slides

Shock focusing and Converging Geometries - in the context of the VTF validation

Shock focusing and Converging Geometries - in the context of the VTF validation. D.J.Hill. S.I. meeting - June 2, 2005. Outline. History and motivation Center validation experiment: (P.Dimotakis A.Lam) Converging wedge, 3 Phases Review of experiment to date Preliminary 2D calculations

227 views • 22 slides

SPEED EVOLUTION OF CME/SHOCKS USING MULTI-SPACECRAFT OBSERVATIONS OF TYPE II RADIO BURSTS.

300 views • 21 slides

Shock focusing and Converging Geometries - in the context of the VTF validation

220 views • 20 slides

Radio Bursts

Radio Bursts. Energy Release. Confined. Eruptive. X-ray, Microwave bursts, ? -rays ( Sunward electrons , ions) Shocks, CMEs (outward electrons), SEPs. X-ray, Microwave bursts, ? -rays (Sunward electrons , ions). Radio bursts are due to accelerated electrons from ~1 keV to >1 MeV

526 views • 19 slides

SEP Source Regions

Progress Toward Measurements of Suprathermal Proton Seed Particle Populations J. Raymond, J. Kohl, A. Panasyuk, L. Gardner, and S. Cranmer Harvard-Smithsonian Center for Astrophysics. SEP Source Regions.

281 views • 18 slides

Some open questions in the study of WDM/HEDM using laser driven shock

Some open questions in the study of WDM/HEDM using laser driven shock. Andrew Ng University of British Columbia, Canada. IBD HEDP Workshop, Pleasanton, CA, June 22-24, 2010. Peter Celliers, UBC Luiz Da Silva, UBC Andrew Forsman, UBC Dean Parfeniuk, UBC Jim Waterman, UBC Guang Xu, UBC.

339 views • 18 slides

Supernova Remnants

Supernova Remnants. Shell-type versus Crab-like Phases of shell-type SNR. Shell-type SNR. Shell-type SNR: X-ray, radio, and optical emission come from a shell. X-rays are usually thermal, but can have non-thermal components. Shell is expanding.

254 views • 15 slides

Supernova Remnants

Supernova Remnants. Shell-type versus Crab-like Phases of shell-type SNR. Shell-type SNR. Shell-type SNR: X-ray, radio, and optical emission come from a shell. X-rays are usually thermal, but can have non-thermal components. Shell is expanding.

169 views • 15 slides