Published July 28, 2006
| Version v1
Journal article
Stabilization of Wave Formation on a Contact Boundary of Metal Layers at an Oblique Impact during Kelvin - Helmholtz Instability Development
Creators
- 1. Russian Federal Nuclear Center All-Russian Scientific Research Institute of Experimental Physics, Sarov, 607190 (Russian Federation)
Description
The elimination effect of disturbances and mutual mixing on a contact boundaries of metal layers at oblique impact during Kelvin - Helmholtz instability development was established and investigated. Thin layers of metal coatings (Δ∼30 μm) reduce amplitude of disturbance realization in 10 - 100 times and eliminate mutual mixing of contacting materials (eliminate the formation of a welded point). The foils of the same materials and thicknesses are not characterized by the same strong stabilizing properties. This stabilizing effect is explained by physical properties of a metal coating as a whole. Thermophysical limits for coating layers are pointed out
Additional details
Identifiers
- DOI
- 10.1063/1.2263580;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 845
- Journal Issue
- 1
- Journal Page Range
- p. 1375-1378
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- American Physical Society Topical Group conference on shock compression of condensed matter
- Dates
- 31 Jul - 5 Aug 2005
- Place
- Baltimore, MD (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38043227
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; S36: MATERIALS SCIENCE;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- AMPLITUDES; BOUNDARY LAYERS; COATINGS; DISTURBANCES; FOILS; HELMHOLTZ INSTABILITY; METALS; MIXING; PHASE STABILITY; STABILIZATION; THICKNESS; THIN FILMS
- Descriptors DEC
- DIMENSIONS; ELEMENTS; FILMS; INSTABILITY; LAYERS; PLASMA INSTABILITY; PLASMA MACROINSTABILITIES; STABILITY
Optional Information
- Notes
- (c) 2006 American Institute of Physics