Journal of Spectroscopy
Volume 2017 (2017), Article ID 6359107, 6 pages
https://doi.org/10.1155/2017/6359107

Research Article

Characterization of an Atmospheric-Pressure Argon Plasma Generated by 915 MHz Microwaves Using Optical Emission Spectroscopy

Robert Miotk,¹ Bartosz Hrycak,¹ Mariusz Jasiński,¹ and Jerzy Mizeraczyk²

¹The Institute of Fluid Flow Machinery, Polish Academy of Sciences, Fiszera 14, 80-231 Gdansk, Poland
²Department of Marine Electronics, Gdynia Maritime University, Morska 81-87, 81-225 Gdynia, Poland

Correspondence should be addressed to Robert Miotk; rmiotk@imp.gda.pl

Received 30 August 2017; Accepted 16 October 2017; Published 1 December 2017

Academic Editor: Nikša Krstulović

Copyright © 2017 Robert Miotk et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Abstract.

The paper presents the investigations of an atmospheric-pressure argon plasma generated at 915 MHz microwaves using the optical emission spectroscopy (OES). The 915 MHz microwave plasma was inducted and sustained in a waveguide-supplied coaxial-line-based nozzleless microwave plasma source. The aim of presented investigations was to estimate parameters of the generated plasma, that is, excitation temperature of electrons Texc, temperature of plasma gas Tg, and concentration of electrons ne. Assuming that excited levels of argon atoms are in local thermodynamic equilibrium, Boltzmann method allowed in determining the Texc temperature in the range of 8100–11000 K. The temperature of plasma gas Tg was estimated by comparing the simulated spectra of the OH radical to the measured one in LIFBASE program. The obtained Tg temperature ranged in 1200–2800 K. Using a method based on Stark broadening of the Hβ line, the concentration of electrons ne was determined in the range from 1.4 × 10¹⁵ to 1.7 × 10¹⁵ cm⁻³, depending on the power absorbed by the microwave plasma.

1. Introduction

The atmospheric-pressure microwave plasma sources (MPSs) found many different physical and technical applications such as decomposition of gaseous pollutants [1–4], deposition thin layers in nanosensors [5, 6], medicine for bacteria inactivation [7], and production of hydrogen via conversion of hydrocarbons or other hydrogen carriers [8–12].

Since in process of the gas treatment by the plasma, the temperature of plasma gas and concentration of electrons play an important role; therefore, the knowledge of these basic parameters is crucial for understanding the chemical kinetics and its optimization.

In this work, an optical emission spectroscopy (OES) [13–17] method has been used for diagnosing the microwave argon plasma. The plasma was induced by microwaves at a frequency of 915 MHz in waveguide-supplied coaxial-line-based nozzleless MPS [1]. The presented device allows the generation of so-called cold plasma which is classified as a partial local thermodynamic equilibrium (PLTE) plasma [13, 14, 18–20].

2. Experiment

In Figure 1(a), a photo of the MPS is shown, whereas a draft of an experimental setup is presented in Figure 1(b). The MPS is supplied via a standard waveguide WR 975 and ended by a movable plunger which allows for an effective transfer of the microwave power from the electric field to the plasma.

(a)

(b)

Figure 1: (a) Photo of the microwave plasma source and (b) the experimental setup used for the spectroscopic investigations.

Inside the used MPS, a quartz tube is placed. In the tube, two gas flows are formed. The first one is the axial flow (processed gas), and the second one is the swirl flow (cooling gas). In the axial flow, the processed gas is introduced into the quartz tube through the inner electrode. In the swirl flow, the cooling gas is delivered into the MPS by four inlets located tangentially to the quartz tube wall [1]. This resulted in a vortex (swirl) flow inside the quartz tube. In this type of the MPS, plasma in a form of flame occurs inside the quartz tube at the tip of the inner electrode. The additional swirl flow stabilized the discharge in the center of the quartz tube and protects the quartz wall from overheating [1]. Below the MPS waveguide, the quartz tube is surrounded by a metal cylinder with a vertical slit for the observation of the generated discharge.

Symmetrical double convex quartz lens (50 mm in diameter, focal length 75 mm) was used to focus light emitted by the microwave plasma. Additionally to collimate the emitted light, two diaphragms with pinholes of 1 mm in diameter were placed. In these investigations, the spectrum of the microwave plasma was measured by McPherson model 209 spectrometer, equipped with double-pass scanning monochromator. The used spectrograph is equipped with sensitivity-calibrated iCCD camera and diffraction grating 1200 grooves/mm.

Using Hg I lines λ = 365.02 nm, 435.84 nm, and 546.07 nm emitted from low-pressure calibration Hg-Ne lamp, the instrumental line broadening has been determined. The obtained values of was about 0.07 nm.

3. Results

During the experiment, the nitrogen was used as a cooling gas with constant flow rate of 50 NL/min. The investigations were performed with argon as processed gas with flow rate equal to 50 NL/min. The power absorbed by the microwave plasma PA was calculated as a difference between power incident PI and power reflected PR in the MPS [1]. The PI and PR were directly measured using a directional coupler. In these investigations, the power PA was changed from 2 to 4 kW.

The spectra were recorded 15 mm below the tip of the inner electrode. In our measurements, we focused on the range of emission spectra from 300–600 nm. An example of the recorded spectra is shown in Figure 2. To detect emission spectral lines of the H or the OH radicals, a small addition of H₂O vapour (H₂O—0.1 kg/h, H₂O vapour temperature was equal to 400°C) was added to the process gas flow.

Figure 2: Measured emission spectra of argon plasma (with a small amount of H₂O vapour) with selected argon 4p–4s and 5p–4s transition lines for Boltzmann plot method. Absorbed microwave power PA = 3 kW and argon flow rate Q = 50 l/min.

In performed investigations, we assumed that microwave plasma at atmospheric pressure is generally in partial local thermodynamic equilibrium [13, 14, 18–20]. This assumption allowed us to use the Boltzmann plot method to determine the Texc [14, 15]. Five transition lines of argon (see Figure 2) were selected to determine the Texc. Selected argon lines with the parameters for the Boltzmann plot method were presented in Table 1. An example of Boltzmann plot is shown in Figure 3. Conformity of a straight line with experimental points indicates balance in the excited states of argon atoms. The obtained Texc was in the range of 8100–11000 K, as shown in Figure 4. The estimated Texc temperature increased with increasing the absorbed microwave power PA.

Table 1: Parameters of selected argon emission lines used to determine the excitation temperature of the electrons Texc. n/m: energy levels upper/lower, respectively; λnm: wavelength of transition n → m, Anm: Einstein coefficient for transition n → m, : statistical weight of the upper level n. En is the energy of the upper level n.

l.p.
λnm (nm)
Transition
Anm (10⁷ s⁻¹)

En (cm⁻¹)

1
427.75
5p → 4s
0.0797
3
117,151

2
430.01
0.0377
5
116,999

3
434.51
0.0297
5
118,407

4
518.77
5d → 4p
0.1380
5
123,372

5
603.21
0.1400
9
122,036

Figure 3: Example of Boltzmann plot for determination of the Texc. Inm—intensity of the recorded emission line from transition n → m, microwave power absorbed PA = 3 kW, and argon flow rate Q = 50 l/min.

Figure 4: Electron excitation temperature as a function of absorbed microwave power PA.

It is widely accepted that in the microwave discharges, the rotational temperature of the OH radical Trot corresponds to the translational temperature of heavy particles in the plasma (temperature of plasma gas Tg) [16, 17]. To obtain the molecule rotational temperature, the OH band was used. This band is very sensitive against the changes of the rotational temperature [16]. After measuring the OH spectrum, we simulated this band in the LIFBASE program [21]. This program allows calculating the emitted spectrum of plasma radiation of various gases at individually given rotational and vibrational temperatures. In this program, the simulated OH band was fitted to the experimental one (Figure 5). A good agreement has been found. Spectrum simulations were performed for Gaussian line shapes with a FWHM value equal to 0.07 nm. The obtained gas temperature Tg ranged from 1200 to 2800 K (Figure 6).

Figure 5: Comparison of the measured and simulated in LIFBASE emission spectra of OH band. Absorbed microwave power PA = 3 kW and argon flow rate Q = 50 l/min.

Figure 6: Measured rotational temperatures of the OH radical as a function of absorbed microwave power PA.

By using the method based on Stark broadening of the hydrogen Hβ line, the concentrations of electrons ne in the plasma were determined [13–15, 17]. The introduction of water vapour caused the emergence of emission lines of hydrogen Hβ, Hδ, and Hγ. In our work, we focus only on the Hβ (486.13 nm) line. The Hδ and Hγ lines were hardly noticeable or partially overlapped by the argon lines. Therefore, these two lines were not used to determine the concentration of electrons ne.

The shape of the recorded Hβ line is affected by several different mechanisms of broadening (instrumental , Van der Waals , Stark , resonance , Doppler , and natural ) which result to a Voigt profile [13–15]. In order to obtain the FWHM of Hβ line in investigations to the measured profile, the Voigt function was fitted. The fitting was performed using the Origin software [22].

The Doppler broadening is a result of atoms’ random motions in the plasma. This effect can be calculated from [15, 23]

where is the wavelength, is the temperature of the emitter in Kelvins, is the mass of the emitter in a.m.u. In this work, was assumed equal to the temperature of plasma gas . The Van der Waals broadening is the effects of dipolar interaction between excited the atoms and the neutral ground state atom [14]. The broadening can be estimated from [23]

where is the pressure and is the Boltzmann constant. Determination of plasma gas temperature allows to estimate values of Van der Waals and Doppler broadening effect. Using the above formulas, the values of and broadening of the Hβ line were calculated. The obtained value of was equal to 0.003 nm while ΔλW = 0.02 nm, respectively. In the tested range of the absorbed microwave power PA, determined values were constant. In the presented work, resonance and natural broadening have been omitted due to low FWHM values in comparison to the other effects [13–15].

Taking into account the estimated values of , , and and obtained value FWHM of Hβ line, the Stark broadening was calculated [15, 23]. In the experiment, we observed a linear relationship between the estimated value of Stark broadening of Hβ line and the absorbed microwave power PA by the plasma. In calculation of the ne, a Gig-Card theory [24] was used. The measured concentration of electrons ne ranged from 1.4 × 10¹⁵ to 1.7 × 10¹⁵ cm⁻³ (Figure 7). The values of the electron concentration indicate that the balance between electrons and heavy particles as a result of collisions cannot be achieved. Thus, the plasma cannot be described by a single temperature.

Figure 7: The concentration of electrons as a function of absorbed microwave power PA.

Adopting a classical ideal gas model and using the measured concentration of electrons, we estimated that the ionization degree in plasma was about ~10⁻⁴. This indicates that ionization degree is too low to thermalize the electron energy distribution function. Therefore, there may be a lack of balance between the basic state and the excited states of argon atoms in plasma. This cause that the measured temperatures could be overestimated. In measurements, we record the radiation from the excited states, which are the result of collisions, while the basic states remain neutral.

4. Conclusions

The investigations of an atmospheric-pressure argon plasma generated at 915 MHz microwaves using optical emission spectroscopy (OES) are presented in this work. These investigations yielded the excitation temperature of electrons Texc, the gas temperature Tg, and the concentration of electrons ne in the generated argon plasma. In the tested range of the absorbed microwave power PA by the plasma, we observed an increase in the excitation temperature Texc, the gas temperature Tg, and the concentration of electrons ne. These results indicate that appropriate selection of the gases and the operating parameters of the MPS (central and the additional flow rate, absorbed microwave power) enables in obtaining the plasma with desired parameters. It should also be mentioned that the investigated MPS works very stable with various processing gases (argon, nitrogen, air, and carbon dioxide) at high flow rates and absorbed microwave power by the plasma can be changed in a wide range. Thus, the above properties make the presented MPS an attractive tool for different gas processing at high flow rates.

Conflicts of Interest

The authors declare that they have no conflicts of interest.

Acknowledgments

The authors are grateful to the National Science Centre (Program no. 2013/11/N/ST8/00802) and the Foundation for Polish Science (FNP Program START no. 53.2017) for the financial support of this work.

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