Published January 12, 2004
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Final Report. Hydrodynamics by high-energy-density plasma flow and hydrodynamics and radiative hydrodynamics with astrophysical application
Description
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
Availability note (English)
Available from INIS in electronic form; Also available from OSTI as DE00820683; PURL: https://www.osti.gov/servlets/purl/820683-ak7VI9/native/
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The record is publicly accessible, but files are restricted to users with access.
Additional details
Identifiers
Publishing Information
- Imprint Pagination
- 33 p.
- Report number
- INIS-US--0196
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 35022563
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- DESIGN; HYDRODYNAMICS; MICHIGAN; PERFORMANCE; PLASMA; RADIATIONS; SHOCK WAVES; SUPERNOVAE
- Descriptors DEC
- BINARY STARS; DEVELOPED COUNTRIES; ERUPTIVE VARIABLE STARS; FLUID MECHANICS; MECHANICS; NORTH AMERICA; STARS; USA; VARIABLE STARS
Optional Information
- Contract/Grant/Project number
- FG03-99DP00284
- Funding organization
- USDOE Office of Defense Programs (DP) (United States)