CaltechAUTHORS
  A Caltech Library Service

Pressure-Dependent, Infrared-Emitting Phenomenon in Hypervelocity Impact

Mihaly, Jonathan M. and Tandy, Jonathan D. and Rosakis, A. J. and Adams, M. A. and Pullin, D. (2015) Pressure-Dependent, Infrared-Emitting Phenomenon in Hypervelocity Impact. Journal of Applied Mechanics, 82 (1). Art. No. 011004. ISSN 0021-8936. https://resolver.caltech.edu/CaltechAUTHORS:20150320-155256012

[img] PDF - Published Version
See Usage Policy.

1995Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20150320-155256012

Abstract

A series of hypervelocity impact experiments were conducted with variable target chamber atmospheric pressure ranging from 0.9 to 21.5 Torr. Using a two-stage light-gas gun, 5.7 mg nylon 6/6 right-cylinders were accelerated to speeds ranging between 6.0 and 6.3 km/s to impact 1.5 mm thick 6061-T6 aluminum plates. Full-field images of near-IR emission (0.9 to 1.7 μm) were measured using a high-speed spectrograph system with image exposure times of 1 μs. The radial expansion of an IR-emitting impact-generated phenomenon was observed to be dependent upon the ambient target chamber atmospheric pressures. Higher chamber pressures demonstrated lower radial expansions of the subsequently measured IR-emitting region uprange of the target. Dimensional analysis, originally presented by Taylor to describe the expansion of a hemispherical blast wave, is applied to describe the observed pressure-dependence of the IR-emitting cloud expansion. Experimental results are used to empirically determine two dimensionless constants for the analysis. The maximum radial expansion of the observed IR-emitting cloud is described by the Taylor blast-wave theory, with experimental results demonstrating the characteristic nonlinear dependence on atmospheric pressure. Furthermore, the edges of the measured IR-emitting clouds are observed to expand at extreme speeds ranging from approximately 13 to 39 km/s. In each experiment, impact ejecta and debris are simultaneously observed in the visible range using an ultrahigh-speed laser shadowgraph system. For the considered experiments, ejecta and debris speeds are measured between 0.6 and 5.1 km/s. Such a disparity in observed phenomena velocities suggests the IR-emitting cloud is a distinctly different phenomenon to both the uprange ejecta and downrange debris generated during a hypervelocity impact.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1115/1.4028856 DOIArticle
http://appliedmechanics.asmedigitalcollection.asme.org/article.aspx?articleid=1919305PublisherArticle
Additional Information:© 2015 by ASME. Contributed by the Applied Mechanics Division of ASME for publication in the Journal of Applied Mechanics. Manuscript received June 2, 2014; final manuscript received October 17, 2014; accepted manuscript posted October 21, 2014; published online November 19, 2014. This material is based upon work supported by the Department of Energy National Nuclear Security Administration under Award No. DE-FC52-08NA28613. The authors would also like to thank Michael Mello for his assistance with the optomechanical design of the LSL system and Petros Arakelian for his assistance in installing the optical benches and safety feature.
Group:GALCIT
Funders:
Funding AgencyGrant Number
Department of Energy (DOE) National Nuclear Security AdministrationDE-FC52-08NA28613
Issue or Number:1
Record Number:CaltechAUTHORS:20150320-155256012
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150320-155256012
Official Citation:Mihaly JM, Tandy JD, Rosakis AJ, Adams MA, Pullin DD. Pressure-Dependent, Infrared-Emitting Phenomenon in Hypervelocity Impact. ASME. J. Appl. Mech.. 2015;82(1):011004-011004-9. doi:10.1115/1.4028856
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:55952
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:20 Mar 2015 23:36
Last Modified:03 Oct 2019 08:10

Repository Staff Only: item control page