DENSITY MEASUREMENTS BY DOUBLE-LASER INTERFEROMETRY: EXPERIMENTAL TECHNIQUE M. Domingo, R. Luna, M. A. Satorre, C. Santonja. Laboratorio de Caracterizaciones de Interés Astrofísico. Escuela Politécnica Superior de Alcoy, Spain mdomingo@fis.upv.es Abstract In this work we present a technique to determine the real part of the index of refraction (n) using double laser interferometry. Keywords: Ices, index of refraction. Figure 1. Laser scheme. 2 1. Experimental procedure In our laboratory[1], we study properties of ices of astrophysical interest. They are deposited at a certain temperature ranging from 10 K until 150 K onto a Quartz Crystal Microbalance (QCMB) placed inside a high vacuum chamber (P < 10−7 mbar). In most cases the index of refraction is unknown at low temperature, in other cases, for example in mixtures of different compounds, it is even completely unknown. This work refers a technique to determine the real part of n using double laser interferometry (Figure 1)[2]. The index n is obtained from the quotient of the periods of the interference curves measured from each of the lasers (Figure 2) using the expression n = [sin2 βi2 − γ 2 sin2 βi1 /[1 − γ 2 ]](1/2) (1) To improve the sensitivity of this technique, the incidence angles α and β must be chosen in order to γ varies in the largest possible range with respect to the refraction index n (see Figure 3, left). In Figure 3 (right) can be observed that in order to obtain the best value of dγ , dn is necessary that α → 0 and β → π/2. The values of the periods are obtained using a software based in the Fourier analysis, developed by us. 4950000 laser 1 T laser 2 frequency 4947000 Frec.(Hz) Laser intensity (a.u.) 48,5 48,0 4944000 47,5 T 4941000 5040 5760 6480 7200 7920 time (s) Figure 2. Interference curves and deposition rate. Density measurements by double-laser interferometry Figure 3. Left: Dependence between γ and n for different α and β. Right: Variation of with α and β. 3 dγ dn References [1] R. Luna, M.A. Satorre, G. Blanes, C. Santonja, M. Domingo, O. Gomis (2002). Density determination of ices of astrophysiucal interest by double laser interferometry. Highlights of Spanish Astrophysics, Kluver Academic Publishers. [2] Tempelmeyer, K.E. and D.W. Mills,Jr 1968. Refractive index of carbon dioxide cryodeposit. J. Appl. Phys. 39, 2968-2969.
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