CP620, Shock Compression of Condensed Matter - 2001 edited by M. D. Furnish, N. N. Thadhani, and Y. Horie © 2002 American Institute of Physics 0-7354-0068-7/02/$ 19.00 EMISSION SPECTROSCOPY APPLIED TO SHOCK TO DETONATION TRANSITION IN NITROMETHANE Viviane Bouyer1'2, Gerard Baudin2, Christian Le Gallic2, Philippe Herve1 ^aboratoire d'Energetique et d'Economic d'Energie, Paris X University, I Chemin Desvallieres, 92410 Ville d 'Avray, France, viviane. bouyer@cva. u-parisl O.fr 2 DGA/DCE/Centre d'Etudes de Gramat(CEG), 46500 Gramat, France, [email protected] Abstract. The objective of this work is to clarify the mechanism of shock to detonation of nitromethane by time-resolved emission spectroscopy. This paper presents the experiments performed in the spectral range 0.3-0.85 jim. Experimental results provide several radiance values depending on wavelength and time that we compared to measurements of pyrometry previously performed. Determination of the temperature profile is treated from the resolution of the equation of radiative transfer by an inversion method. The case of the steady state detonation is considered here. INTRODUCTION around 3000-4000K and pressure between 1030 GPa complicates the problem. To improve knowledge of shock to detonation transition (SDT) of homogeneous high explosives, especially nitromethane (NM), temperature profiles are one of the parameters required. Optical techniques as pyrometry are often used to determine the NM detonation temperature (1). One of the most successful techniques today is the six-wavelength pyrometer developed at CEG (2)(3)(4). These means are based on the assumption of a surface emissivity. To obtain more information on the optical properties of condensed matter, spectroscopy techniques are widely used (5)(6)(7). This context and the fact that the different media involved in the SDT are likely semitransparent brings us to set up a time-resolved emission spectroscopy technique that enables a continuous measurement of the radiation emitted during the detonation of NM with a 1 ns time resolution. This paper presents the study of the visible range, where the NM in liquid state is transparent. From the radiance values obtained versus time and wavelength, we aim at determining profiles temperature by resolving the equation of radiative transfer. The fact that emissive media are made of gaseous compressed species at temperature EXPERIMENTAL CONFIGURATION One interesting property of NM for optical studies is its semi-transparence. Figure 1 shows the NM spectrum in the 0.6-3 |tim range. In the visible range 0.4-0.6 jam, NM is transparent (2). 10080SS .1 .22 « 6040200 wavelength pm FIGURE 1. Transmission spectrum of the NM for a thickness of 15 mm measured by a FT-IR Fourier Spectrometer The experiments consist in plane shock impacts on explosive targets at 8.6 GPa, under conditions of one-dimensional strain. A single stage powder gun 1223 propels the projectile on the target at a velocity of 1940 m/s to initiate the detonation (Fig. 2). The NM is in a polyethylene chamber of 15 to 25 mm depth, closed by a copper transfer plate. An optical probe collects the thermal radiation emitted during the detonation through a lithium fluoride (LiF) window. This radiation is transmitted to the spectroscopy system by an optical fiber. A Jobin Yvon Triax 180 spectrometer spectrally disperses the light beam. The dispersion is 33.5 nm/mm at 565 nm. A multianode photomultiplier tube (16 channels/ Hamamatsu R5900U-01-L16) is used to detect the signal in the spectral range [0.3-0.85 jim]. Its response time is 0.6 ns. Complementary measurement techniques are used: a polarization electrode records the shock entrance, the superdetonation and the detonation, piezo-electric pins measure the shock and detonation velocities. Projectile Opt&al probe that propagates until the interaction with the LiF window at 4.5 1 2 3 4 6 5 time us FIGURE 3. Results of one experiment at 8.6 GPa on a 25 mm NM target RADIANCE PROFILE ANALYSIS Analysis of one experiment at 8.6 GPa Optical fibre Changes in radiance depending on wavelength have been studied for different typical moments of the SDT (Fig. 4). From the formation of the superdetonation, a discontinuity appears between 0.65 and 0.75 urn It remains until the end of the propagation of the detonation wave. Coneave j Pholomuitiplier ^ 3.0x10 - & 2.5x1 06- e * 1 o 0 « f «** 1.5x106- FIGURE 2. Experimental device. fo ^ cf ^ 2.0x1 0 6 E Data acquisition system 4 o m o' 9 » i I S- 1.0x106- ^ s | 5.0x1 0 5 - EXPERIMENTAL RESULTS 1 1 ii 8 0 S wi « 0* ^S •o* * 0 0 • 1» 0.0- We analyzed one of our experiments carried out at 8.6 GPa on a 25 mm thick NM target. Figure 3 represents the radiance signals for different wavelengths versus time. Only 6 measurements among 16 are represented. The spectral resolution is 28 nm and time resolution is 20 ns after filtering through noise. These measurements, with the piezoelectric pins and electrode signals clearly show the different phases of the SDT as described by Chaiken (8): a first jump at 1.65 jis characterizes the formation of the superdetonation, which overtakes the initial shock wave at a second jump at 2.15 u.s. A strong detonation is then formed and gradually decays into an overdriven steady state detonation O '• ;:, i a 2- A" *&^' ^ A 0.4 0.5 ° ^ * * 0.6 *' 0.7 *' ^ A 0.8 wavelength pm FIGURE 4. Radiance profiles at different times: a) after shock entrance (0.3 us), b) before the superdetonation formation (1.2 us), c) superdetonation formation (1.65 us), d) 1.9 us, e) catch up of the shock wave (2.15 us), f) strong detonation (2.45 us), g) overdriven steady state detonation (3.8 to 4.4 us). Radiance values were averaged around the given time value. One interpretation for this discontinuity may be gaseous H2O produced during the SDT: the H2O spectrum shows absorption lines between 0.65 and 0.75 jim. Another interpretation could be given from Gruzdkov and Gupta works (6). They measured the emission spectrum between 0.4 and 0.75 jim of NM 1224 shocked at 16.7 GPa under a stepwise loading process, and a peak appeared at 0.65 um. They explained it as luminescence from reaction products, maybe NO2. Determination of the temperature from the equation of radiative transfer By using inversion methods, it should be possible to determine the temperature profiles during the SDT from the equation of radiative transfer (ERT). In this paragraph, we will only present the ERT and compare the detonation temperatures obtained from pyrometry and spectroscopy results. Comparison with previous pyrometry measurements In 1998, a time-resolved six-wavelength pyrometer was developed at CEG (4). The same experiments on NM had been carried out with this device so we can compare our results to those obtained by pyrometry (Fig. 5). However, the comparison is limited to the overdriven detonation phase because we do not obtain the same time of apparition of the superdetonation and detonation. Radiative transfer for a semitransparent medium Given a semitransparent medium at a temperature T, with an absorption coefficient K^ and a thickness (x*-x0), the ERT gives the spectral intensity transmitted and emitted by the medium along the detonation axis as: 2,5x106^ 2,0x106- (1) (0 I 1,5x106- x* \K,(x')L°,(T)exp\ ^ 1,0x1065 5,0x10 1 0,0- X0 x* \-K,(x)dx\dx' \Xr ) Applying (1) to the SDT, different media are involved: neat NM, shocked NM, reaction products and detonation products. The two parameters T and KX are unknown except for neat NM. The difficulty lies in the knowledge of the media involved. If thermochemical codes give the main present chemical species, a model giving their absorption properties at the pressure and temperature encountered during the SDT does not exist. Therefore, the resolution of (1) by mathematical methods will require suitable absorption models. 6 wavelength pyrometer measurements emission spectroscopy measurements Planck curve at 3570 K 0,4 0,5 0,6 0,7 0,8 0,9 1,0 1,1 1,2 1,3 1,4 1,5 1,6 wavelength um FIGURE 5. Radiance profiles obtained by pyrometry and spectroscopy during the steady state detonation, x error bars represent the spectral resolution. The spectroscopy technique gives more information than the pyrometry technique because of the greater number of detectors and of the better spectral resolution (28 nm against 40 to 100 nm). Thus, the discontinuity can not be recorded by pyrometry. Consequently, the exploitation of the only six radiance values can give approached results, in particular for the temperature. Moreover, the black or grey body assumption often used when determining the temperature of the overdriven detonation may be questioned from these results. As shown on Fig. 5, emission spectroscopy measurements do not match with the Planck curve. Further to this, we analyze the influence of the number and kind of radiance values on the steady state detonation temperature calculation. Case of the overdriven steady state detonation To get onto the resolution problem and to improve the comparison between the pyrometry and the spectroscopy techniques, it could be interesting to approach the case of the determination of the temperature of the overdriven steady state detonation. T is uniform (according to the Jouguet model) and equal to the semitransparent detonation products temperature Tj. K^J is only depending on the wavelength A,. Then, as the detonation wave interacts with the window, the intensity is (I is the depth of the cell): 1225 choice of the pyrometer wavelength is critical. Afterwards, emission spectroscopy will be performed in the infrared range 0.8-5 jum to characterize the functional groups of gaseous species. The determination of temperature profiles by an inversion method is not so obvious because of the absorption coefficient. Chemical species produced, N2, H2O, CO2, CO and C(s), are in such a thermodynamic state (high pressure and temperature) that it is not represented by existing absorption models (like Hitemp or Hitran data bases). Thermochemical calculations, existing detonation models will be then required to initiate the ETR resolution. But first, it is necessary to resolve the direct problem to analyze the sensitivity of the solution L(^,t) to the parameters of the chosen absorption model. (2) No accurate model for K^ is available yet that could consider the absorption window. Except for this discontinuity, calculation results can point out relevant remarks. Table 1 represents calculations of Tj and of the transmissivity r A = exp^-K^ -I) from the pyrometry measurements and from 5 and 7 values of spectroscopy measurements. TABLE 1. Determination of temperature Tj pyrometry 5 measurements of spectroscopy 7 measurements of spectroscopy Tj(K) 3570±16 3533±21 3604±36 ^=0.5 TA=06 0.01 0.66 0.02 0.38 TA=08 0.06 0.04 0.7 0.47 0.14 The three calculations give similar values. However, transmissivity values obtained from pyrometry measurements justify the hypothesis of a surface emissivity, close to black body's, whereas spectroscopy results don't confirm it. Consequently, the choice of the wavelength affects the estimation of the optical characteristic of the studied medium. ACKNOWLEDGMENTS The work described here was carried out with financial support from DGA/SPNuc, for the interest of CEA. Each impact experience was performed at Physics Explosive Laboratory of CEG with the assistance of ARES and Metrology staff. CONCLUSION REFERENCES Time-resolved emission spectroscopy performed during the detonation of NM gives radiance measurements versus time between 0.3 and 0.85 jim, with a 28 nm spectral resolution. This technique brings out more information than timeresolved six-wavelength pyrometry, which was previously used to study the SDT of the NM at CEG. Indeed, our results showed a discontinuity between 0.65 and 0.75 jam in the radiance profile, appearing from the formation of the superdetonation. We still have to explain the presence of this discontinuity. It affects the determination of the temperature; however, we resolved the equation of radiative transfer outside the discontinuity in the case of an overdriven detonation. Detonation temperatures calculated are close to the temperature obtained by pyrometry but there is a significant difference between the transmissivity. Therefore, black or grey body assumption commonly used seems doubtful and the 1. Kato Y., Mori N., Sakai H., Detonation temperature of nitromethane and some solid high explosives, in 8th Symposium on detonation, Albuquerque, NM, 1985, pp. 558-566. 2. Leal Crouzet B., Ph. D. Dissertation, University of Poitiers, France, 1998. 3. Leal Crouzet B., Baudin G., Presles H.N., Combustion and Flame 122, 463-473 (2000). 4. Leal Crouzet, Bouriannes R., Baudin G., Goutelle J.C., EPJ Applied Physics 8, 189-194 (1999). 5. Winey J. M., Gupta Y. M, J. Phys. Chem. A 101, 9333-9340(1997). 6. Gruzdkov Y. A., Gupta Y. M., J. Phys. Chem. A 102, 2322-2331 (1998). 7. Piermarini G. J., Block S., Miller P. J., J. Phys. Chem. 93,457.462(1989). 8. Chaiken R. F., The kinetic theory of detonation of high explosives, M.S Thesis, Polytechnic Inst. of Brooklyn, 1957. 1226
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