Acta Polytechnica Acta Polytechnica 53(2):193–196, 2013 © Czech Technical University in Prague, 2013 available online at http://ctn.cvut.cz/ap/ HIGH-SPEED MONITORING OF DUST PARTICLES IN ITER ELMs SIMULATION EXPERIMENTS WITH QSPA KH-50 Vadym A. Makhlaja,∗, Igor E. Garkushaa, Nikolay N. Aksenova, Alexander A. Chuviloa, Igor S. Landmanb a Institute of Plasma Physics of the NSC KIPT, 61108 Kharkov, Ukraine b Karlsruhe Institute of Technology (KIT), IHM, 76344 Karlsruhe, Germany ∗ corresponding author: makhlay@kipt.kharkov.ua Abstract. Dust generation under powerful plasma stream impacts has been studied in ITER ELM simulation experiments with QSPA Kh-50 plasma accelerator. Repetitive plasma exposures of tungsten have been performed by 0.25 ms plasma pulses and the heat load varied in the range (0.1 ÷ 1.1) MJ m−2. Main characteristics of dust particles such as a number of ejected particles, their velocity, angular distribution and start time from the surface are investigated. Dust particles have not been observed under heat load below the cracking threshold. Quantity of dust particles rises with increasing heat load. Average velocities of dust particles are found to be strongly dependent on their start time from the surface after beginning of plasma-surface interaction. Maximal velocity achieved a few tens of meters per second. Keywords: ITER, ELMs simulation experiments, QSPA, plasma-surface interaction, tungsten dust. 1. Introduction The anticipated regime of the tokamak ITER is the ELMy H-mode. The edge localized modes (ELMs) of plasma instabilities, intrinsic for H-mode, produce short periodic pulses of heat flux at the divertor armor. Tungsten is the most suitable material for the ITER divertor. It should withstand both the stationary and transient heat fluxes demonstrating tolerably erosion rate. The drawbacks of tungsten as plasma-facing material are W brittleness and damage effects related with brittle destruction as well as the melt layer ero- sion [11]. Tungsten cracking leads to generation of the dust, which can contaminate and radiatively cool the core plasma [7, 4]. The dust particles produced during tungsten cracking and the droplets ejected from the melt layer under the action of giant ELMs and disruptions are critical issues for ITER performance that require comprehensive experimental studies. There are three main approaches to experimental dust study in fusion plasmas: (i) collection of dust particles resulted from transient events, (ii) laser scat- tering by the dust grain sand and (iii) dust monitoring with fast cameras [6]. Observations with fast cameras can track the trajectories of the grains in the chamber during the discharge (with trajectory reconstruction), giving the magnitude of dust speed. It can also provide information on grain–wall collisions, some peculiar fea- tures of dust dynamics in fusion reactor, the amount of visible dust grains in vacuum chamber during oper- ation in different discharges and regimes [6]. The ITER energy fluxes to the divertor are not achievable in existing tokamaks. For this reason sim- ulation experiments of ITER transients have been carried out with other plasma devices [7, 4, 5]. In particular, the quasi-stationary plasma acceler- ators (QSPA) can reproduce energy densities (0.2 ÷ 2 MJ m−2) and pulse duration (0.1 ÷ 0.5 ms) of ITER ELMs [7, 4]. Therefore, QSPA can be applied for in- vestigation of material response to the expected heat loads [4, 5, 3]. This paper presents the results of QSPA Kh-50 experiments on high-power interactions with material surfaces and behavior of tungsten dust under pulsed energy loads typical for ITER Type I ELMs. 2. Experimental setup The quasi-steady-state plasma accelerator QSPA Kh-50 is the largest and most powerful device of this kind [4, 12]. QSPA Kh-50 consists of two stages. The first one is used for plasma production and pre- acceleration. The main second stage is a coaxial sys- tem of shaped active electrodes with magnetically screened elements, supplied from independent power sources. The hydrogen plasma streams, generated by QSPA Kh-50, are injected into the magnetic sys- tem of 1.6 m in length and 0.44 m in inner diameter with a magnetic field of up to 0.54 T in diagnostic chamber (2.3 m from acceleretor) where the target has been installed [3, 12]. Plasma parameters were varied both by changing dynamics and the amount of gas filled in the accelerator channel and by the vari- ation of the working voltage of capacitor battery of the accelerating channel. The main parameters of QSPA plasma streams were as follows: ion impact energy about 0.4 ÷ 0.6 keV, the maximum plasma pressure 3.2 bar, and the plasma stream diameter about 18 cm. The surface energy loads measured with a thermocouple calorimeters were varied in the range 193 http://ctn.cvut.cz/ap/ Vadym A. Makhlaj et al. Acta Polytechnica Figure 1. High speed imaging of plasma interac- tion with tungsten target: t = 1.2 ms after the start of plasma-surface interaction, texp = 1.2 ms; a) Qsurf = 0.45 MJ m−2, b) Qsurf = 0.6 MJ m−2, c) Qsurf = 0.75 MJ m−2. of (0.1 ÷ 1.1) MJm−2 [3]. The plasma pulse shape was approximately triangular, and the pulse duration was about 0.25 ms. In previous experiments it was demonstrated that tungsten cracking and melting thresholds under QSPA Kh-50 exposures corresponded to 0.3 MJ m−2 and 0.6 MJ m−2 respectively. The evaporation onset is es- timated as 1.1 MJ m−2 [4, 3]. The targets made of pure tungsten of sizes 5 × 5 × 0.5 cm3 and 12 × 8 × 0.1 cm3 have been used for these experiments. Observations of plasma in- teractions with exposed surfaces, the dust particle dynamics and the droplets monitoring have been per- formed with a high-speed 10 bit CMOS pco.1200 s digital camera PCO AG (exposure time from 1 µs to 1 s, spectral range from 290 to 1100 nm). In general, the applied measurement scheme for droplets monitoring was similar to one used in [4, 5, 3]. As an example, Fig. 1 shows camera frames registered with the same exposure for differ- ent plasma heat loads. Camera frames corresponding to different time moments during one plasma pulse are presented in Fig. 2. Dynamics of particles ejected from exposed surfaces has been analyzed from the series of camera frames. This is the main difference of applied scheme from the experiments described in [5]. Velocities of ejected tungsten dust particles/droplets have been evaluated from the lengths of their traces done coluring selected frame. The moment when the particle was released from the target surface could be calculated also. Tem- poral distributions of quantity and velocity of ero- sion products were obtained for different heat loads to the exposed tungsten surfaces. The observed region in front of target was 8 cm due to feature of a design the diagnostic vacuum chamber of QSPA Kh-50. Therefore, the particles with veloc- ity higher than 35 m/s were able to fly away of ob- served region during of 2.2 ms. Taking into account Figure 2. High speed images of plasma interaction with inclined (35◦ to plasma jet) tungsten target, a) t = 1.16 ms and b) t = 9.06 ms after the start of plasma-surface interaction, Qsurf = 0.75 MJ m−2, texp = 0.25 ms. these circumstance, the special pulsed system was used for synchronization of the camera registration start and the beginning the plasma-surface interac- tion. This allows improvement of temporal resolution for applied registration system in comparison with that described in [5]. The exposure was not exceed 1.5 ms. Particles were also registered after plasma im- pact for more than 9 ms (Fig. 2b). The total recording time achieved 50 ms. 3. Experimental results The irradiation of tungsten surface with QSPA Kh-50 plasma heat load below the cracking threshold (0.3 MJ m−2) does not trigger the generation of ero- sion products. At the heat load above the cracking threshold but below melting threshold only several dust particles traces have been registered (Fig. 1a). 194 vol. 53 no. 2/2013 High-Speed Monitoring of Dust Particles Elastic energy stored in stressed tungsten surface layer should be the motive force for the cracking process with following acceleration of separated solid particles in this case [10]. Further increase of heat load leads to the surface melting and results in splashing of eroded material (Fig. 1b). Number of ejected particles rises with in- creasing heat load due to growing thickness of melted layer. Quantity of particles ejected from irradiated surface increases more than twice as a consequence of heat load elevation from 0.6 MJ m−2 to 0.75 MJ m−2 only. The majority of W particles are ejected from the exposed surface 0.2 ms after beginning of plasma– surface interaction (Fig. 3). Velocity of registered tungsten particles achieves 25 m/s for earlier instants. For the later moments, ve- locity decreases to several m/s [3, 9]. Maximal velocity only weakly depends on the heat load. The maximum of particles with high velocities (i.e. ejected from surface before t = 0.4 ms) is clearly detected on cam- era frame at 1.2 ms after beginning of plasma-surface interaction (Fig. 3). For the later moments of obser- vation [9], they leave a zone of observation. Therefore, the number of such particles decreases. The quantity of particles with velocity of 10 m/s changes weakly during 5 ms. As follows from [3], under perpendicular plasma im- pacts droplets are ejected primarily with small angles to the normal (i.e. towards impact plasma, see Fig. 1c). Nevertheless, rather large angles of ejection, up to 80◦ have been observed also. Analysis of droplet traces from consecutive images shows the influence of gravi- tational force on droplets with larger mass and smaller velocity values. Due to gravitation the resulting an- gular distribution of droplets became non-symmetric. The high speed imaging of QSPA Kh-50 plasma interaction with the inclined tungsten target is pre- sented in Fig. 2. For this case, the angular distribu- tion of ejected droplets is also non-symmetric (Fig. 4). The maximal number of particles has been registered at angle (35 ÷ 40)◦ to the normal. Such particles flying towards the plasma impact, i.e., in upstream direction. However, quite large number of droplets turns to the downstream direction due to the influ- ence of gravitational force and plasma stream pressure. It should be mentioned that the impacting energy den- sity to the exposed surface depends on the plasma incidence angle to the target [8, 2]. A non-uniform distribution of the heat load along the target surface (for instance, due to formation of non-uniform shield- ing layer) can also cause a non-symmetric angular distribution of ejected droplets. For heat load exceeding the melting threshold, the flying particles can be originated from melt surface due to Kelvin–Helmholtz or Rayleigh–Taylor insta- bilities [1]. Analysis of obtained experimental results and comparison with the results of numerical simu- lations [10, 9] allows conclusion that the generation of tungsten particles in the form of droplets may occur Figure 3. Amount of dust particles versus delay from start for different heat loads to target surface; a) Qsurf = 0.6 MJ m−2, b) Qsurf = 0.75 MJ m−2. only during the plasma pulse and (as latest) few tens microseconds after the pulse end. Other particles may be exclusively solid dust that is generated due to elas- tic energy stored in stressed re-solidified tungsten surface layer. It is interesting to compare the results of QSPA Kh-50 plasma exposures with performed ex- periments on erosion product monitoring in QSPA-T facility [3, 1]. Similar velocity of erosion products and the energy threshold of particles appearing have been observed. However, in our experiments with inclined irradiation the droplets are primarily ejected at small angles to the plasma jet. The reason for somewhat different results obtained in mentioned devices can be much larger plasma pressure and output electric currents in QSPA-T. 4. Summary The results of erosion products monitoring from tung- sten targets exposed to ITER ELM-like surface heat load at QSPA Kh-50 have been discussed. Plasma en- ergy load to the target surfaces achieved 0.75 MJ m−2 and caused a pronounced surface melting. The erosion products for tungsten targets have been registered with a high-speed digital camera both under normal and inclined plasma irradiation. Distributions of the particles in dependence on their start time from the target surface have been obtained for different heat loads. The number of particles grows signifi- cantly with increasing heat load. Erosion products have been observed with CCD camera only under 195 Vadym A. Makhlaj et al. Acta Polytechnica Figure 4. The angular distribution of ejected droplets for inclined (35◦ to plasma jet) plasma irradiation. heat load exceeding the cracking threshold. Maximal velocity of tungsten particles may achieve few tens of m/s. The main erosion mechanisms are found to be droplet ejection from the melt and solid dust origina- tion during the brittle destruction of exposed tungsten surfaces due to the thermo-stress. For energy load below 0.75 MJ m−2, the start time of ejected particles from the surface is only weakly depended on the heat load value. The measurement scheme applied in QSPA Kh-50 can be effectively used for investigations of dust dy- namics in near-surface plasma in simulation studies of plasma interaction with ITER divertor surfaces. References [1] B. Bazylev, et al. Experimental and theoretical investigation of droplet emission from tungsten melt layer. 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