High-resolution observations of tungsten liner collapse and early jet formation
Abstract
High-resolution photography of collapsing tungsten-lined shaped charges has revealed surface texturing both similar to and strikingly different from that previously observed during copper liner collapse. The behavior of three types of tungsten-lined shaped charges, with different liner designs and high explosives but with similar tungsten processing, were characterized by image-converter camera and fast- framing camera photography, and flash x-ray radiography. 120-mm- diameter, trumpet-shaped Octol charges produced surface blistering near the base of the tungsten liner, probably due to inhomogeneities near the liner-explosive interface resulting from cast loading. 148- mm-diameter, quasi-conical LX-14 charges produced smooth shocked- surface texture similar to that observed in conical, copper-lined LX- 14 (Viper) charges. 81-mm-diameter, conical LX-20 charges produced severe radial texturing throughout the collapsing tungsten liner, which transitioned to azimuthal banding on the jet surface. For each type of charge, obscuring debris from the tungsten jet tip prevented clear imaging of the jet surface at late time. 8 refs., 6 figs., 2 tabs.
- Authors:
- Publication Date:
- Research Org.:
- Lawrence Livermore National Lab., CA (United States)
- Sponsoring Org.:
- USDOE, Washington, DC (United States); Department of Defense, Washington, DC (United States)
- OSTI Identifier:
- 281679
- Report Number(s):
- UCRL-JC-123067; CONF-960982-3
ON: DE96013877
- DOE Contract Number:
- W-7405-ENG-48
- Resource Type:
- Technical Report
- Resource Relation:
- Conference: 16. international symposium on ballistics, San Francisco, CA (United States), 23-28 Sep 1996; Other Information: PBD: Jul 1996
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 45 MILITARY TECHNOLOGY, WEAPONRY, AND NATIONAL DEFENSE; SHAPED CHARGES; LINERS; FAILURES; TUNGSTEN; JETS; C CODES; EXPERIMENTAL DATA; THEORETICAL DATA
Citation Formats
Winer, K.A., Breithaupt, R.D., Muelder, S.A., and Baum, D.W. High-resolution observations of tungsten liner collapse and early jet formation. United States: N. p., 1996.
Web. doi:10.2172/281679.
Winer, K.A., Breithaupt, R.D., Muelder, S.A., & Baum, D.W. High-resolution observations of tungsten liner collapse and early jet formation. United States. doi:10.2172/281679.
Winer, K.A., Breithaupt, R.D., Muelder, S.A., and Baum, D.W. Mon .
"High-resolution observations of tungsten liner collapse and early jet formation". United States.
doi:10.2172/281679. https://www.osti.gov/servlets/purl/281679.
@article{osti_281679,
title = {High-resolution observations of tungsten liner collapse and early jet formation},
author = {Winer, K.A. and Breithaupt, R.D. and Muelder, S.A. and Baum, D.W.},
abstractNote = {High-resolution photography of collapsing tungsten-lined shaped charges has revealed surface texturing both similar to and strikingly different from that previously observed during copper liner collapse. The behavior of three types of tungsten-lined shaped charges, with different liner designs and high explosives but with similar tungsten processing, were characterized by image-converter camera and fast- framing camera photography, and flash x-ray radiography. 120-mm- diameter, trumpet-shaped Octol charges produced surface blistering near the base of the tungsten liner, probably due to inhomogeneities near the liner-explosive interface resulting from cast loading. 148- mm-diameter, quasi-conical LX-14 charges produced smooth shocked- surface texture similar to that observed in conical, copper-lined LX- 14 (Viper) charges. 81-mm-diameter, conical LX-20 charges produced severe radial texturing throughout the collapsing tungsten liner, which transitioned to azimuthal banding on the jet surface. For each type of charge, obscuring debris from the tungsten jet tip prevented clear imaging of the jet surface at late time. 8 refs., 6 figs., 2 tabs.},
doi = {10.2172/281679},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Mon Jul 01 00:00:00 EDT 1996},
month = {Mon Jul 01 00:00:00 EDT 1996}
}
-
Irradiation of tungsten with metallic diatomic molecular ions: atomic-resolution observations of depleted zones
Direct evidence, on an atomic scale, is presented for the enhancement of damage production per projectile ion in diatomic metallic molecular ion (dimer) irradiations of tungsten as compared to monatomic metallic ion (monomer) irradiations. Irradiations were performed in situ at less than or equal to 10 K, in a field-ion microscope, employing 20 keV Ag/sup +/ or W/sup +/ monomer ions and the results are compared with 40 keV W/sub 2//sup +/ or Ag/sub 2//sup +/ dimer ion bombardments; the average energy per ion was 20 keV. First, in the near-surface region the depleted zones produced by the W/sub 2//supmore » -
Fabry-Perot measurements and analysis of TOW-2A liner collapse and jet formation
A TOW-2A 146 mm shaped charge was fired and observed with five beam Fabry-Perot laser velocimetry. The liner collapse velocities were measured at five lines of sight covering the outer half of the liner. A record of 8-10 {mu}s in length was obtained for each sight line The velocity records at late time differ for each location, reflecting the varying charge-to-mass ratio as the end of the liner is approached. The results were analyzed with the CALE-2D hydrodynamic simulation code. The calculations reproduce the jump-off times, the shapes of the velocity jumps and the late time velocity asymptotes, but theymore » -
High-resolution imaging of early-time imprinting using normal-incidence multilayer mirrors. Final report
A normal-incidence multilayer mirror telescope was designed, fabricated, and tested. The telescope consisted of a primary mirror and a secondary mirror in a Cassegrain optical configuration. The mirrors had multilayer coatings that efficiently reflected the soft x-ray radiation in a narrow bandpass centered at a wavelength of 48 {angstrom}. The telescope was taken to the Laboratory for Laser Energetics (LLE) on October 28, 1996. The telescope was mounted in a TIM instrument module on the OMEGA target chamber. The focusing and alignment of the mirrors were checked and optimized. Images were recorded on x-ray film on October 30. Images weremore »