Measurements of evaporated aluminium concentration on self-absorbed spectral lines

In the paper we discuss the experimental results of powerful plasma-stream interaction with aluminum target at the presence of the magnetic field. The plasma streams are generated by a quasi-stationary plasma accelerator (QSPA Kh- 50). Such experiments performed with QSPA facility during last years...

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Published in:Вопросы атомной науки и техники
Date:2002
Main Authors: Lobko, A.K., Trubchaninov, S.A., Tsarenko, A.V.
Format: Article
Language:English
Published: Національний науковий центр «Харківський фізико-технічний інститут» НАН України 2002
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Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/79289
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Cite this:Measurements of evaporated aluminium concentration on self-absorbed spectral lines / A.K. Lobko, S.A. Trubchaninov, A.V. Tsarenko // Вопросы атомной науки и техники. — 2002. — № 5. — С. 151-153. — Бібліогр.: 5 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Lobko, A.K.
Trubchaninov, S.A.
Tsarenko, A.V.
author_facet Lobko, A.K.
Trubchaninov, S.A.
Tsarenko, A.V.
citation_txt Measurements of evaporated aluminium concentration on self-absorbed spectral lines / A.K. Lobko, S.A. Trubchaninov, A.V. Tsarenko // Вопросы атомной науки и техники. — 2002. — № 5. — С. 151-153. — Бібліогр.: 5 назв. — англ.
collection DSpace DC
container_title Вопросы атомной науки и техники
description In the paper we discuss the experimental results of powerful plasma-stream interaction with aluminum target at the presence of the magnetic field. The plasma streams are generated by a quasi-stationary plasma accelerator (QSPA Kh- 50). Such experiments performed with QSPA facility during last years [1-3] are of great interest for current disruption simulation in ITER tokamak and testing divertor materials. Some experimental series in our activity were devoted to the problem of mass losses of target under the high power plasma stream irradiation. This work presents the spectral method of determination of the evaporated material quantities in plasma-target interaction experiments. The distinctive feature of the offered work is follows – all spectral measurements were carried out using aluminum spectral lines only. There are two mechanisms of mass losses – evaporation and splashing melt layer. We succeeded in the evaluation of the evaporation mechanism contribution to the mass defect for aluminum target.
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fulltext MEASUREMENTS OF EVAPORATED ALUMINIUM CONCENTRATION ON SELF-ABSORBED SPECTRAL LINES A.K. Lobko, S.A.Trubchaninov, A.V.Tsarenko Institute of Plasma Physics of the National Science Center “Kharkov Institute of Physics and Technology”, 61108, Kharkov, Akademicheskaya Str., 1, Ukraine In the paper we discuss the experimental results of powerful plasma-stream interaction with aluminum target at the presence of the magnetic field. The plasma streams are generated by a quasi-stationary plasma accelerator (QSPA Kh- 50). Such experiments performed with QSPA facility during last years [1-3] are of great interest for current disruption simulation in ITER tokamak and testing divertor materials. Some experimental series in our activity were devoted to the problem of mass losses of target under the high power plasma stream irradiation. This work presents the spectral method of determination of the evaporated material quantities in plasma-target interaction experiments. The distinctive feature of the offered work is follows – all spectral measurements were carried out using aluminum spectral lines only. There are two mechanisms of mass losses – evaporation and splashing melt layer. We succeeded in the evaluation of the evaporation mechanism contribution to the mass defect for aluminum target. PACS: 52.40.Hf; 52.70.Kz INTRODUCTION The problem of the interaction of powerful plasma streams with materials presents a large interest for many physical and technical areas. Especially, it concerns the materials of the candidates on manufacturing ITER divertor plates. Erosion of the divertor plates material during a tokamak disruption event restricts the divertor plates lifetime and presents an important problem of ITER fusion technology. So the present work was done in the frame of ITER tasks and it was aimed at investigations of plasma-target interaction under conditions simulating disruption in ITER. The dense shielding layer that consists of ionized vapors of target material is formed during interaction of high power plasma stream with the target. The main part of the energy of the stream is absorbed and radiated in the shielding layer that comes to the screening effect. The screening effect is amplified in the presence of the magnetic field [2]. The main aim of the present work is determination of the evaporated material quantities using spectral technique. EXPERIMENTAL SETUP AND DIAGNOSTIC FACILITIES Experiments were carried out on installation QSPA Kh-50. Detail descriptions of the installation, experimental conditions, diagnostic facility (including spectroscopy) are adduced in series of publications [1-3]. It is necessary to point basic characteristics of plasma stream – power density ~ 10 MW/cm2 (it is so called “soft” regime of QSPA), plasma stream duration ~ 150 μs and diameter of the stream ~ 10 cm. The spectral diagnostic technique elements and its assignment: − diffractive spectrograph DFS-452 (resolution – 0.3 Ǻ, dispersion – 8 Ǻ/mm) - integral spectra registration of plasma radiation; − monochromator MDR-23 (resolution – 0.5 Ǻ, dispersion – 13 Ǻ/mm). Monochromator with the electron-optical converter (EOC) serves for receiving optical spectra with the temporary and spatial resolution. The monochromator was coupled with the photomultiplier for the registration of separate spectral lines. Signals from the photo multiplier were recorded with the help of oscillograph C8-17; − photo diodes - monitoring of the integral plasma radiation, plasma velocity measurements; − micro photometer IFO-451 – spectral data processing The optical technique in details is described in [4]. The scheme of experiment is presented in Fig.1. Aluminum target (diameter – 12 cm) was located perpendicularly to the plasma stream. Spectral measurements were performed in two sections (horizontal and vertical) as shown in Fig.1. DIAGNOSTIC PROCEDURE Some intensive spectral lines of aluminum were registered by the help of photomultiplier for the definition of luminescence time of spectral lines. The examples of oscillograms are represented in Fig.2. They were received as follows: the upper line is a radiation of a spectral line Al III (5696 Ǻ), and lower one – integral radiation of plasma on the photodiode. It is visible, that the luminescence time of aluminum in a shielding layer makes 50 μs, and in the ambient plasma stream this time is almost twice less (20 μs). Problems of Atomic Science and Technology. 2002. № 5. Series: Plasma Physics (8). P. 151-153 151 H=0.57T Streamline plasma Plasma stream Vacuum chamber Diagnostic Cross sections Al target ∅ 12cm Target plasma Fig.1 Scheme of experiment 0 10 20 30 40 50 60 70 0,1 1 10 Al II (559.3nm) Al II (358.7nm) N e, 10 17 c m -3 L, mm Fig. 3. Plasma electron density a) b) Fig.2. Upper line - radiation of Al III (λ=569.6nm) 50μs/cell; Lower line - integral radiation: a) in front of the target(1-2 cm) b) behind the target (1-2cm) The determination of plasma electron density was carried out on the base of Stark broadening measurements of spectral lines Al II after exception of a measured contour Doppler and instrumental broadening with using the Foigts contour method. Such lines of Al II: 5593Ǻ, 3900Ǻ, 3587Ǻ, 2816Ǻ and 2631Ǻ were used. The Fig.3 presents radial distribution of plasma electron density depending on the distance from the target. Differences in the density values may be explained by self-absorption of multiplet – λ=3587 Ǻ and considerable error under reconstruction the Stark broadening. In the consequent evaluations of Te and aluminum concentration we used data, obtained from Al II 5593 Ǻ. The electron temperature was determined from the ratio of intensities of spectral lines of Al II (5593 Ǻ, 3900 Ǻ, 3587 Ǻ, 2816 Ǻ, 2631 Ǻ) and Al III (5722 Ǻ, 5696 Ǻ, 4512 Ǻ, 3612 Ǻ, 3601 Ǻ). The average value of the electron temperature in a plasma shield is equal 1.9-2.1 eV. The analysis of experimental data – intensities and profiles lines - shows that some spectral lines of Al II (3587Ǻ, 2816Ǻ) and Al III (3601Ǻ, 3612 Ǻ) are self- absorbed. It is possible to calculate optical thickness using proportion of the true width of spectral line to experimentally measured one. Particularly, the measured half width (Δλ=1.1Ǻ) of Al II spectral line 3p 1P0 – 4s 1S (λ=2816Å) significantly exceed its calculated value for the optically thin plasma - Δλ≈0.15÷0.2Ǻ. Calculations of contour parameters for λ=2816Ǻ Al II, namely Doppler and Stark contributions, were executed by Foigt function technique using Ne data from Stark broadening of λ=5593Ǻ as standard. All necessary data are available for these procedures in [4]. Thus, we may obtain the value of optical thickness – τ, using the well-known formula for the Lorenz contour, counting the Stark broadening mechanism as a dominant: ( ) 1 -exp1 2ln − + = ∆ ∆ τ τ λ λ L (1) Here ∆λ - observed half width, ∆λL - half width for the optically thin plasma. For example, optical thickness (λ=2816Å) for the near target region amounts to τ ~ 20÷ 30. Somewhat different technique was used for the determination of optical thickness for the Al III spectral multiplet 3d2D – 4p2P0 – λ=3601.6 Ǻ and λ=3612 Ǻ. It is common knowledge that intensities proportion for components of spectral multiplets is defined by gf proportion only, and is independent of Ne, Te in the case of neglible optical thickness (usually values of Te considerably larger than fine structure of corresponding terms). Generally differences of λ for multiplets are neglible also. Equally it is concerned to τ, because of the same broadening parameters. Distortion of the “atomic” line intensities ratio indicates on a large optical thickness. We have possibility to evaluate τ in such a way: ( ) ( )α τ τ -exp1 -exp1 − −=R (2) Where R – observed ratio intensities; α – “atomic” ratio between gf; τ – optical thickness for center of strongest line. When τ → ∞ (Plank limit), R →1; given τ → 0, R → α – optically transparent plasma. In the Eq. 2) the matter concerns brightness in a center of line, the whole intensity distort too, but slightly complex. For the mentioned above Al III multiplet, R is equal to 1.3 (region behind target), under α ~ 2. We have the value τ ~2 for the spectral line λ=3601.6 Ǻ. There is necessary to mark that the ratio intensities is more “sensitive“ to optical thickness in comparison with line shapes. Namely, distortions of contour are observable under the significant values of optical thickness - τ »1. 152 0 5 10 15 20 25 30 35 40 45 1,2 1,6 2,0 2,4 2,8 Al III(559.6nm)/II(559.3nm) Al III(361.2nm)/II(358.7nm) T e, eV L - distance from the target, mm Fig.4. The electron temperature distribution The information about τ permits us to determine the quantity of evaporated Al in the shielding layer and in the ambient plasma stream. We may use the following relation:             −⋅⋅⋅ ∆ ⋅⋅⋅= ∗− eT LNfk ε λ λτ -exp110 2 20 (3) Where ∆λ[nm] – half width for optically transparent plasma; λ[nm] – wavelength; f – absorption oscillator force; L[cm] – geometrical thickness of luminescence layer; N*[cm-3] (for Al in our case) – population on lower exciting level of corresponding transition; ε[eV] – photon energy; Te[eV] – the electron temperature; k – coefficient depending on contour type k=5.6 for Lorenz type and k=8.2 for Gauss type. Under the commensurable contributions of both broadening mechanisms one may take k=7. For the determination N* from Eq.(3) we used values Te presented on Fig.4. There are some differences in finding ∆λ – half width for optically transparent plasma. For the λ=2816 Ǻ (the near target region) we have taken theoretically calculated half width by setting ion temperature of Al – Ti=Te≈2eV. In the case of λ=3601.6 Ǻ the measured and corrected ∆λ according to Eq.(1) have been used. For L in front of target we used geometric size – 12cm. Value L behind of target was determined from the spectra in vertical cross section (Fig.1), as the doubled thickness of ambient stream. Further the concentrations of Al I – Al IV and the whole (sum on ionization states) density of Al have been calculated using well-known Saha-Boltzmann correlations, taking into account statistical sums. Application of these correlations is wholly justified because of large values of Ne at that significant magnitudes of τ for resonance lines just promote the LTE conditions. All atomic data, constants, parameters of ions (ionization and excitation potentials, statistical weights, oscillator forces, Stark broadening parameters, etc.) that are necessary in this case are present at [4,5]. Fig.5 demonstrates results of the calculation of whole density of aluminum along with Ne and Ne Al= ΣzAlz (Alz – partial concentration of corresponding ion) – part of the electron density, caused by the evaporated aluminum. These data have been used for the evaluation of mass losses taking into account velocity of the ambient flow and geometry of the experiment. All main results of measurements and calculations are submitted in the Table. NAl is regarded as a full quantity of evaporated Al atoms in the shielding layer or in the ambient stream, M – mass loss, t – lifetime of Al in front of or behind of target. One can see that the most part of the evaporated material is pressed out from the shielding layer and passed away with the ambient flow. The values of mass loss obtained in such a way are in a good agreement with direct measurements of mass defect by weighing. Table. Near the target 0.1 cm Distance from the target 3.6 cm Behind the target 2cm Ne, cm-3 1*1017 0.45*1017 0.5*1017 Te, eV 2 2 2 NAl, cm-3 2.8*1016 1.1*1016 6.6*1015 Ne Al cm-3 5*1016 2*1016 1.3*1016 L, cm 12 12 6 S, cm2 d~4cm ~110 V~500cm3 V=Sd V=1.5*104 NAl ~1019Al ½1019Al Whole loss ~1020Al t, μs 100 100 20 M, 10-3g ~0.5 per pulse ~0.2 per pulse ~4.6 per pulse SUMMARY The described method of determination of the plasma optical thickness starting from the distorted multiplet intensities is of great interest not only for the plasma-wall interaction problems, but also for the dense plasma spectroscopy, generally. Evidently our work is a first attempt of practical work with such effect. REFERENCES 1. V.I.Tereshin, V.V. Chebotarev, et al., Disruption modeling experiments with utilizing the powerful quasistationary plasma streams, Proc. of 18th Symposium on plasma physics. Prague, 17-20 June 1997. 2. V.V.Chebotarev, V.A.Makhlaj, et al., Optical measurements of the parameters of high power plasma streams generated by quasi-steady-state plasma accelerator and propagated in a longitudinal magnetic field, Problems of Atomic Science and Technology. Series “Plasma physics” 3(3), 4(4), 1999, pp 298-300. 3. V.I.Tereshin, V.V. Chebotarev, et al., Powerful Quasi-Steady-State Plasma Accelerator for Fusion Experiments, Brazilian Journal of Physics, vol.32, N1, March, 2002. 4. Griem G. Spektroskopia plasmy, Atomizdat, Moskva 1969 (in Russian). Problems of Atomic Science and Technology. 2002. № 5. Series: Plasma Physics (8). P. 151-153 153 0 10 20 30 40 50 0,1 1 10 Ne Whole density of Al NeAl N , 1 016 c m -3 L, mm Fig. 5. Density distributions, depends on distance from the target 5. Striganov A.R., Sventicki N.S. Tablicy spektralnyh liniy, Atomizdat, Moskva 1966 (in Russian). 154
id nasplib_isofts_kiev_ua-123456789-79289
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 1562-6016
language English
last_indexed 2025-12-07T17:43:45Z
publishDate 2002
publisher Національний науковий центр «Харківський фізико-технічний інститут» НАН України
record_format dspace
spelling Lobko, A.K.
Trubchaninov, S.A.
Tsarenko, A.V.
2015-03-30T09:44:19Z
2015-03-30T09:44:19Z
2002
Measurements of evaporated aluminium concentration on self-absorbed spectral lines / A.K. Lobko, S.A. Trubchaninov, A.V. Tsarenko // Вопросы атомной науки и техники. — 2002. — № 5. — С. 151-153. — Бібліогр.: 5 назв. — англ.
1562-6016
PACS: 52.40.Hf; 52.70.Kz
https://nasplib.isofts.kiev.ua/handle/123456789/79289
In the paper we discuss the experimental results of powerful plasma-stream interaction with aluminum target at the presence of the magnetic field. The plasma streams are generated by a quasi-stationary plasma accelerator (QSPA Kh- 50). Such experiments performed with QSPA facility during last years [1-3] are of great interest for current disruption simulation in ITER tokamak and testing divertor materials. Some experimental series in our activity were devoted to the problem of mass losses of target under the high power plasma stream irradiation. This work presents the spectral method of determination of the evaporated material quantities in plasma-target interaction experiments. The distinctive feature of the offered work is follows – all spectral measurements were carried out using aluminum spectral lines only. There are two mechanisms of mass losses – evaporation and splashing melt layer. We succeeded in the evaluation of the evaporation mechanism contribution to the mass defect for aluminum target.
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Національний науковий центр «Харківський фізико-технічний інститут» НАН України
Вопросы атомной науки и техники
Plasma diagnostics
Measurements of evaporated aluminium concentration on self-absorbed spectral lines
Article
published earlier
spellingShingle Measurements of evaporated aluminium concentration on self-absorbed spectral lines
Lobko, A.K.
Trubchaninov, S.A.
Tsarenko, A.V.
Plasma diagnostics
title Measurements of evaporated aluminium concentration on self-absorbed spectral lines
title_full Measurements of evaporated aluminium concentration on self-absorbed spectral lines
title_fullStr Measurements of evaporated aluminium concentration on self-absorbed spectral lines
title_full_unstemmed Measurements of evaporated aluminium concentration on self-absorbed spectral lines
title_short Measurements of evaporated aluminium concentration on self-absorbed spectral lines
title_sort measurements of evaporated aluminium concentration on self-absorbed spectral lines
topic Plasma diagnostics
topic_facet Plasma diagnostics
url https://nasplib.isofts.kiev.ua/handle/123456789/79289
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