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Title: Final Report

Abstract

OAK-B135 This is the final report from the project Hydrodynamics by High-Energy-Density Plasma Flow and Hydrodynamics and Radiation Hydrodynamics with Astrophysical Applications. This project supported a group at the University of Michigan in the invention, design, performance, and analysis of experiments using high-energy-density research facilities. The experiments explored compressible nonlinear hydrodynamics, in particular at decelerating interfaces, and the radiation hydrodynamics of strong shock waves. It has application to supernovae, astrophysical jets, shock-cloud interactions, and radiative shock waves.

Authors:
Publication Date:
Research Org.:
University of Michigan (US)
Sponsoring Org.:
USDOE Office of Defense Programs (DP) (US)
OSTI Identifier:
820683
Report Number(s):
1
TRN: US0400410
DOE Contract Number:  
FG03-99DP00284
Resource Type:
Technical Report
Resource Relation:
Other Information: PBD: 12 Jan 2004
Country of Publication:
United States
Language:
English
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY; 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; DESIGN; HYDRODYNAMICS; MICHIGAN; PERFORMANCE; PLASMA; RADIATIONS; SHOCK WAVES; SUPERNOVAE; RADIATION HYDRODYNAMICS; HIGH ENERGY DENSITY PHYSICS

Citation Formats

R Paul Drake. Final Report. United States: N. p., 2004. Web. doi:10.2172/820683.
R Paul Drake. Final Report. United States. doi:10.2172/820683.
R Paul Drake. Mon . "Final Report". United States. doi:10.2172/820683. https://www.osti.gov/servlets/purl/820683.
@article{osti_820683,
title = {Final Report},
author = {R Paul Drake},
abstractNote = {OAK-B135 This is the final report from the project Hydrodynamics by High-Energy-Density Plasma Flow and Hydrodynamics and Radiation Hydrodynamics with Astrophysical Applications. This project supported a group at the University of Michigan in the invention, design, performance, and analysis of experiments using high-energy-density research facilities. The experiments explored compressible nonlinear hydrodynamics, in particular at decelerating interfaces, and the radiation hydrodynamics of strong shock waves. It has application to supernovae, astrophysical jets, shock-cloud interactions, and radiative shock waves.},
doi = {10.2172/820683},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Mon Jan 12 00:00:00 EST 2004},
month = {Mon Jan 12 00:00:00 EST 2004}
}

Technical Report:

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