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Front. Phys. 11(4), 114209 (2016)
DOI 10.1007/s11467-016-0581-6
Research article
The role of microwaves in the enhancement of
laser-induced plasma emission
Ali Khumaeni1,†
, Katsuaki Akaoka2
, Masabumi Miyabe2
, Ikuo Wakaida2
1
Department of Physics, Faculty of Science and Mathematics, Diponegoro University,
Tembalang, Semarang 50275, Indonesia
2
Fuel Debris Analysis Group, Collaborative Laboratories for Advanced Decommissioning Science (CLADS),
Japan Atomic Energy Agency, Tokai-mura, Ibaraki-ken 311-1195, Japan
Corresponding author. E-mail: †
khumaeni@fisika.undip.ac.id
Received November 13, 2015; accepted February 20, 2016
We studied experimentally the effect of microwaves (MWs) on the enhancement of plasma emission
achieved by laser-induced breakdown spectroscopy (LIBS). A laser plasma was generated on a calcium
oxide pellet by a Nd:YAG laser (5 mJ, 532 nm, 8 ns) in reduced-pressure argon surrounding gas. A
MW radiation (400 W) was injected into the laser plasma via a loop antenna placed immediately above
the laser plasma to enhance the plasma emission. The results confirmed that when the electromagnetic
field was introduced into the laser plasma region by the MWs, the lifetime of the plasma was extended
from 50 to 500 µs, similar to the MW duration. Furthermore, the plasma temperature and electron
density increased to approximately 10900 K and 1.5×1018
cm−3
, respectively and the size of the plasma
emission was extended to 15 mm in diameter. As a result, the emission intensity of Ca lines obtained
using LIBS with MWs was enhanced by approximately 200 times compared to the case of LIBS without
MWs.
Keywords laser-induced breakdown spectroscopy, LIBS, microwave-assisted laser-induced breakdown
spectroscopy, MA-LIBS, enhancement of laser plasma emission
PACS numbers 42.62.Fi, 95.75.Fg, 42.55.-f, 42.62.-b, 87.50.S-
1 Introduction
Laser-induced breakdown spectroscopy (LIBS) is one of
the most powerful analytical methods for spectrochemi-
cal analysis. In LIBS, a Nd:YAG laser is usually focused
onto a sample target to generate a luminous plasma [1, 2].
The elemental composition of the target can be obtained
by analyzing the atomic emission from the plasma. The
appealing advantages of LIBS are the use of unprocessed
samples, the possibility of in-situ analysis, and the capa-
bility of micro-area analysis [3]. For these reasons, LIBS
has been successfully implemented for elemental analy-
sis in various fields, such as the environmental field [4,
5], the metal industries [6–8], and nuclear power plants
[9]. LIBS has also been used for calcium detection; cal-
cium analysis is known to be necessary in various ap-
plications, including soil analysis, the coal industry, and
environmental. Bustamante et al. performed Ca analy-
sis in soil using LIBS [10]. Maravelaki-Kalaitzaki et al.
employed LIBS for the characterization of encrustation
on marble [11]. Body and Chadwick conducted research
on coal analysis using LIBS [12]. Although LIBS has nu-
merous applications, it suffers from reduced sensitivity
compared to other spectroscopic methods.
To overcome this drawback, efforts have been made
by many LIBS groups to develop the double-pulse LIBS
technique (DP-LIBS) [13–15], which can be effectively
used for the improvement of the analytical capabilities
of single-pulse LIBS (SP-LIBS). DP-LIBS obtains signif-
icant increases in the signal-to-noise ratio (S/N) and the
emission intensity compared to SP-LIBS. The enhance-
ment in line emission intensity achieved by double-pulse
excitation is believed to be due to the increased ablated
mass, higher plasma temperature, and longer plasma du-
ration [16].
Other methods aimed at enhancing the emission inten-
sity have been developed by coupling microwave (MW)
and laser systems, which is known as MW-assisted LIBS
(MA-LIBS). Envimetrics and Liu et al. used MWs to
enhance the plasma emission of metal samples [17, 18].
Kearton et al. and Liu et al. reported intensity enhance-
© Higher Education Press and Springer-Verlag Berlin Heidelberg 2016
Research article
Fig. 1 Experimental setup used in this work.
ments obtained by using laser-assisted MW spectroscopy
(LAMPS) [19, 20]. Ikeda et al. used MWs to extend the
lifetime of plasma emission to the order of a millisecond
[21]. However, these methods required the use of waveg-
uides and microwave cavities.
For the convenient application of MWs, we developed
a method of MA-LIBS coupled with a loop antenna for
the enhancement of LIBS emission. In this method, a lu-
minous plasma is generated by a low-energy pulsed laser
at a local point, where an electromagnetic field is pro-
duced by localized MW radiation. The MWs are applied
through a loop antenna via a coaxial cable to enhance the
plasma emission. We must emphasize that this method is
especially suitable for practical application because the
antenna is very flexible and can access the sample via
the coaxial cable, which is combined with a fiber sys-
tem. Thus, the technique is highly applicable to mate-
rial analysis in the field. In contrast, previously proposed
MA-LIBS methods required waveguides and microwave
cavities, which is inconvenient for practical applications
because the sample must be placed in a special chamber
connected to the MW source.
In this study, the effect of MWs on the enhancement
of laser plasma emission was studied by measuring time-
resolved emission spectra obtained with (MA-LIBS) and
without MWs (LIBS). Pelletized calcium oxide (CaO)
powder was used as the sample.
2 Experimental setup
The basic experimental setup used in this work is shown
in Fig. 1. A Q-switched Nd:YAG laser (Quanta-Ray,
Spectra Physics, 532 nm, 8 ns) was directly focused onto
a sample surface through a quartz window (200 mm) to
generate a plasma. The laser energy was fixed at 5 mJ.
The plasma emission was enhanced by intensified MWs
produced via a loop antenna; the antenna was shaped as
a loop with a diameter of 3 mm. MWs were generated us-
ing a magnetron at a frequency of 2.45 GHz (MUEGGE
MG0500D-215TC, 400 W, 0–1 ms). The MW impedance
could be experimentally adjusted for the plasma genera-
tion by a three-stub tuner. The Nd:YAG laser and MWs
were operated in the synchronization mode and a delay
time of 10 µs was used for the Nd:YAG laser bombard-
ment relatively to the MW generation to obtain MWs
with good stability.
The sample used in the study was a calcium oxide
(CaO) pellet, which has relatively simple spectral lines.
During the experiment, the sample was placed in a metal
chamber equipped with windows, on which a fine-plated
gold mesh (lattice constant of 80 µm and wire diameter
of 30 µm) was attached. The experiment was performed
in reduced-pressure Ar surrounding gas (0.6 kPa).
The emission spectrum was obtained by using an in-
tensified charge-coupled device (ICCD) camera (Andor,
iStar) through a high-resolution echelle spectrometer
(LTB ARYELLE) with a resolution of 50 pm. The light
emission of the laser plasma was collected by an optical
fiber positioned at approximately 80◦
relatively to the
laser axis (Fig. 1). The plasma radiation from the sam-
ple surface for the LIBS and MA-LIBS cases was imaged
at one end of the fiber using a quartz lens (f = 100 mm).
To study the dynamics of plasma expansion, an ICCD
114209-2
Ali Khumaeni, et al., Front. Phys. 11(4), 114209 (2016)
Research article
camera (Andor, iStar) was used. The plasma emission
was imaged by using a quartz lens placed in the ICCD.
3 Results and discussion
To determine the optimum emission intensity of Ca lines
in laser-induced plasma with and without MWs, the spa-
tial distribution of the time-integrated emission intensity
of Ca was measured. Figure 2 displays the emission in-
tensities of Ca II 393.3 nm and Ca I 422.6 nm, measured
perpendicularly to the sample surface. The figure shows
that the time-integrated emissions of Ca II and Ca I are
distributed up to 10 mm and 5 mm from the sample sur-
face in the case of MA-LIBS and LIBS, respectively. In
the MA-LIBS case, the optimum emission intensity of
Ca ions was located at 4 mm to 7 mm from the sam-
ple surface, and in the case of LIBS, at 2 mm. It must
be mentioned that the position of the loop antenna was
3 mm above the sample surface. In the experiment, the
laser beam was focused on the sample surface after pass-
ing through the inner side of the antenna. It is assumed
that the optimum intensity was obtained at 4 to 7 mm
because the electromagnetic field was optimum in the in-
terior of the loop antenna. Based on this result, we used
5 mm and 2 mm heights from the sample surface for the
data acquisition in MA-LIBS and LIBS, respectively.
Figure 3 shows the emission spectra of calcium ac-
quired from the CaO sample using MA-LIBS and LIBS.
The gated delay time was 2 µs and the gated width was
600 µs. The laser energy was set at 5 mJ and the mi-
crowave input power was 400 W. The spectra were ac-
cumulated for the duration of 10 laser shots. The laser
beam focused on a new point of the moving sample sur-
face to avoid shot-to-shot fluctuation. For a comparison
between the MA-LIBS and LIBS cases, the experimen-
tal conditions were the same. Figure 3(a) shows that the
Ca ionic lines at 393.3 nm and 396.8 nm can be clearly
Fig. 2 Spatial distribution of Ca II 393.3 nm and Ca I 422.6
nm taken from the calcium oxide sample by using LIBS with
and without microwave.
Fig. 3 Emission spectra of (a) Ca II at 393.3 nm and 396.8
nm, and (b) Ca I 422.6 nm taken from the calcium oxide sam-
ple by using LIBS with microwave and without microwave.
observed with very low background emission intensity
both in the MA-LIBS and the LIBS spectra. It must be
noted that, compared to LIBS, a significant intensity en-
hancement was obtained for the Ca ions at 393.3 nm and
396.8 nm when the MWs were employed. The enhance-
ment factor for the Ca II 393.3 nm line is approximately
200 times; this was defined as the ratio between the MA-
LIBS intensity and the LIBS intensity after subtracting
the background emission. A different result was obtained
for the case of the neutral emission intensity of Ca, as
shown in Fig. 3(b). Namely, the enhancement factor for
the Ca neutral emission intensity at 422.6 nm is signif-
icantly lower (approximately 10 times higher intensity
achieved by MA-LIBS than by LIBS). The background
emission is almost the same for LIBS with and without
MWs, which suggests that the signal-to-background ra-
tio (S/B ratio) is effectively enhanced when the MWs
were applied. The mechanism of laser plasma enhance-
ment by using MWs coupled with a loop antenna can
be described as follows: a laser plasma is generated by
a pulsed laser on a sample target near the center of the
antenna, where a locally intensified electromagnetic field
is produced. After several microseconds of plasma gener-
ation, the electron density of the laser plasma decreases,
Ali Khumaeni, et al., Front. Phys. 11(4), 114209 (2016)
114209-3
Research article
especially at the outer layer of the plasma region, and
the electrons absorb the MW radiation. The electrons
are then accelerated and provide kinetic energy to ex-
cite the atoms and ions by multiple collisions between
electrons–atoms and electrons–ions. The plasma emis-
sion can be sustained for a long time because of the long
MW duration, from several hundreds of microseconds to
milliseconds. As a result, the plasma emission intensity
is enhanced owing to the increased integration time. The
interaction between laser plasma and MWs via a charged
species like electrons is consistent with the observation
of the enhancement factor difference between Ca ions
and atoms. Because of the Coulombic interaction, the
kinetic energy can be more effectively transferred to the
ions than to the neutral atoms. It must also be noted that
an experiment using DP-LIBS and LIBS reported in our
previous work [22] achieved a 25-fold signal intensity en-
hancement for DP-LIBS compared to LIBS in a Gd2O3
sample. This enhancement factor for DP-LIBS is signifi-
cantly lower than the present result, namely, an enhance-
ment factor of approximately 200 achieved by MA-LIBS
in a CaO sample. This could be attributed to the longer
lifetime of plasma emission in MA-LIBS, which results in
a larger integration time compared to that of DP-LIBS.
As a result, the total emission intensity in MA-LIBS is
much higher than in DP-LIBS. To determine the cause
of the emission intensity enhancement in the MA-LIBS
method, the time-resolved emission of plasma was ob-
served.
Figure 4 shows the emission intensity of the Ca II 393.3
nm and Ca I 422.6 nm lines as a function of delay time.
The plasma emission was measured with delays of 0–5 µs
after the end of the YAG laser irradiation. We observe
that in the MA-LIBS case, the emission intensities for
both Ca ions and Ca atoms exhibit long lifetimes of ap-
proximately 500 µs. The intensity of ionic Ca sharply in-
creases with time to form a peak at approximately 10 µs
and subsequently decreases; the intensity of Ca I reaches
a peak at 10 µs. It must be noted that the intensity en-
hancement of Ca II is much higher than that of Ca I.
At 5 µs, the MW radiation has been effectively absorbed
by the laser plasma, enhancing the plasma emission as
described above. The optimum intensity enhancement in
the case of MA-LIBS occurs at 10 µs, which may indi-
cate the delay time for which the absorption of the MWs
by the laser plasma is optimum. Compared to the case
of LIBS, which has a short plasma emission lifetime of
approximately 50 µs, the emission obtained with MA-
LIBS has considerably longer lifetime and higher emis-
sion intensity. As a consequence of the prolonged plasma
lifetime and higher time-resolved emission intensity, the
integrated emission intensity of Ca is enhanced. The re-
sults verified that the MW radiation significantly con-
tributes to the enhancement of the laser-induced plasma
emission.
Fig. 4 Time-resolved emission profiles of Ca II 393.3 nm
and Ca I 422.6 nm taken from the calcium oxide sample by
using LIBS with and without microwave.
To understand the role of MWs in the enhancement of
laser plasma emission, the plasma temperature and elec-
tron density in the laser plasma with and without MWs
were also investigated. Selected lines and the correspond-
ing spectroscopic data from the NIST database were used
to determine the plasma temperature and electron den-
sity [23]. The lines of Ca II 315.9 nm, Ca II 317.9 nm,
Ca II 318.1 nm, Ca II 370.6 nm, Ca II 393.4 nm, and Ca
II 396.8 nm were employed to calculate the plasma tem-
perature. These lines and their spectroscopic parameters,
obtained from the NIST atomic database, are shown in
Table 1.
To determine the plasma temperature, we assume that
local thermodynamic equilibrium (LTE) is achieved [24,
25]. Examples of the Boltzmann plots of selected lines
acquired with MA-LIBS and LIBS at 10 µs delay time
are shown in Fig. 5(a). The slope of the curve yields a
plasma temperature of approximately 10 900 K for the
MA-LIBS and 9300 K for the LIBS data. The increased
plasma temperature in the MA-LIBS case may be due
to the effect of reheating by MW radiation, as in the
case of pulsed-LIBS [26]. The introduction of the MWs
into the laser plasma accelerates the electrons. Thus, the
multiple collisions of electrons increase, resulting in the
increase of plasma temperature. Figure 5(b) shows the
Table 1 Wavelength, upper level energy, upper level de-
generacy, and transition probability for the ionic Ca emission
lines used in this study.
Elements
Wavelength
(nm)
Upper level
energy (eV)
Upper level
degeneracy
Transition
probability
(s−1)
Ca II 315.9 7.0472 4 3.1 × 108
Ca II 317.9 7.0496 6 3.6 × 108
Ca II 318.1 7.0471 4 5.8 × 107
Ca II 370.6 6.4679 2 8.8 × 107
Ca II 373.7 6.4679 2 1.7 × 108
Ca II 393.4 3.1509 4 1.5 × 108
Ca II 396.8 3.1233 2 1.4 × 108
114209-4
Ali Khumaeni, et al., Front. Phys. 11(4), 114209 (2016)
Research article
Fig. 5 (a) Boltzmann plot made from the analysis of Ca II
lines, considering the intensities at 0.6 kPa of argon surround-
ing gas. The continuous line represents the result of a linear
best fit. (b) Plasma temperature dependence of MA-LIBS on
a delay time.
estimated plasma temperature in the MA-LIBS data as
a function of delay time. The time duration of each point
plotted in the graph is 5 µs. At 5 µs, the plasma tem-
perature is 10 500 K; it increases to 10 900 K at 10 µs,
and slowly decreases to approximately 7700 K at 100
µs. We assume that the high temperature at the initial
plasma emission is due to the high electron density in the
plasma region. With increasing time, the electron den-
sity decreases while the MWs continue supplying elec-
tromagnetic radiation in the plasma region, resulting in
multiple collisions between electrons, atoms, and ions.
The increase in plasma temperature is attributed to the
MW duration. Namely, multiple electron collisions in the
MW-assisted laser plasma occur continuously while the
MW radiation is applied in the laser plasma region.
The high plasma temperature and long lifetime of
the plasma emission observed in the MW-assisted laser
plasma are due to the influence of MWs. The increased
plasma temperature is attributed to the MW duration.
Namely, multiple electron collisions in the MW-assisted
laser plasma occur continuously while the MW radiation
is applied in the laser plasma region.
The electron density of the laser plasma obtained with
and without MWs was also investigated. The full width
at half maximum (FWHM) of the line, ∆λ1/2, is related
to the electron density Ne by the expression [27]:
∆λ1/2 = 2w
(
Ne
1016
)
+ 0.35A
(
Ne
1016
)1
4
×x(1 − 1.2N
−1/3
D )w
(
Ne
1016
)
, (1)
where w is the electron impact width parameter, A the
ion broadening parameter, and ND the number of par-
ticles in the Debye sphere. For a plasma in LTE, Stark
broadening is predominantly determined by the electron
impact. Because the perturbations caused by ions are
negligible compared with those of electrons, the electron
density related to the FWHM of the Stark-broadened
line ∆λ1/2 is described by the following equation [25]:
∆λ1/2 = 2w
(
Ne
1016
)
, (2)
where Ne is the electron number density (cm−3
), w is the
electron impact width parameter. The measured FWHM
is then corrected by subtracting the contribution of the
instrumental line broadening (0.05 nm). By using the Ca
II 396.8 nm line and Eqs. (1) and (2), we estimated that
the electron densities of the laser plasma induced at 0.6
kPa with and without MWs were 1.5 × 1018
cm−3
and
7.6 × 1017
cm−3
, respectively. From the known electron
density and plasma temperature, we can confirm that
the LTE assumption is valid by applying the McWhirter
criterion, which provides the lower limit of the electron
density [28]:
Ne ≥ 1.6x1012
Te1/2
∆E3
, (3)
where ∆E (eV) is the largest energy transition for which
the condition holds and Te(K) is the plasma tempera-
ture. In this work, we used ∆E = 3.9 eV for Ca and T =
10 900 K, which is the highest temperature obtained by
MA-LIBS. Thus, the lower limit of the electron density is
approximately 9.9 × 1015
cm−3
. In both MA-LIBS and
LIBS, the electron density in the plasma is much higher
than 9.9 × 1015
cm−3
. Thus, the McWhirter criterion
is fulfilled, verifying that the plasma at 5 mm from the
sample surface was in LTE conditions.
4 Conclusions
We conducted a study on the effect of MW radiation
on the enhancement of plasma emission in LIBS. In this
work, MWs were introduced into a laser plasma through
a loop antenna to enhance the LIBS emission. The re-
sults revealed that the optical emission intensity, plasma
lifetime, electron temperature, and density were strongly
influenced by the MWs. When the MWs were injected,
the lifetime of plasma emission obtained by LIBS (ap-
proximately 50 µs) was extended to approximately 500
Ali Khumaeni, et al., Front. Phys. 11(4), 114209 (2016)
114209-5
Research article
µs throughout the MW duration, the LIBS plasma tem-
perature increased from 9300 K to 10 900 K, the electron
density from 7.6 × 1017
cm−3
to 1.5 × 1018
cm−3
, and
the plasma size expanded to 15 mm. As a consequence
of these phenomena, the plasma emission can effectively
be enhanced by using MWs and the emission intensity of
Ca achieved by LIBS was increased by approximately 200
times. The final goal of the proposed method is its prac-
tical application (remote and in-situ analysis) in solid
material analysis. The MA-LIBS method using a loop an-
tenna is very suitable for practical applications because
the antenna is very flexible and can access the sample
by using a fiber system. Thus, it is highly applicable to
material analysis in the field. In contrast, previously pro-
posed MA-LIBS methods required waveguides and MW
cavities, which is inconvenient for practical applications
because the sample must be placed in a special chamber
connected to the MW source.
References and notes
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Ali Khumaeni, et al., Front. Phys. 11(4), 114209 (2016)
114209-7

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1. the role of microwaves in lips (frontiers of physics if 2.4)

  • 1. Front. Phys. 11(4), 114209 (2016) DOI 10.1007/s11467-016-0581-6 Research article The role of microwaves in the enhancement of laser-induced plasma emission Ali Khumaeni1,† , Katsuaki Akaoka2 , Masabumi Miyabe2 , Ikuo Wakaida2 1 Department of Physics, Faculty of Science and Mathematics, Diponegoro University, Tembalang, Semarang 50275, Indonesia 2 Fuel Debris Analysis Group, Collaborative Laboratories for Advanced Decommissioning Science (CLADS), Japan Atomic Energy Agency, Tokai-mura, Ibaraki-ken 311-1195, Japan Corresponding author. E-mail: † khumaeni@fisika.undip.ac.id Received November 13, 2015; accepted February 20, 2016 We studied experimentally the effect of microwaves (MWs) on the enhancement of plasma emission achieved by laser-induced breakdown spectroscopy (LIBS). A laser plasma was generated on a calcium oxide pellet by a Nd:YAG laser (5 mJ, 532 nm, 8 ns) in reduced-pressure argon surrounding gas. A MW radiation (400 W) was injected into the laser plasma via a loop antenna placed immediately above the laser plasma to enhance the plasma emission. The results confirmed that when the electromagnetic field was introduced into the laser plasma region by the MWs, the lifetime of the plasma was extended from 50 to 500 µs, similar to the MW duration. Furthermore, the plasma temperature and electron density increased to approximately 10900 K and 1.5×1018 cm−3 , respectively and the size of the plasma emission was extended to 15 mm in diameter. As a result, the emission intensity of Ca lines obtained using LIBS with MWs was enhanced by approximately 200 times compared to the case of LIBS without MWs. Keywords laser-induced breakdown spectroscopy, LIBS, microwave-assisted laser-induced breakdown spectroscopy, MA-LIBS, enhancement of laser plasma emission PACS numbers 42.62.Fi, 95.75.Fg, 42.55.-f, 42.62.-b, 87.50.S- 1 Introduction Laser-induced breakdown spectroscopy (LIBS) is one of the most powerful analytical methods for spectrochemi- cal analysis. In LIBS, a Nd:YAG laser is usually focused onto a sample target to generate a luminous plasma [1, 2]. The elemental composition of the target can be obtained by analyzing the atomic emission from the plasma. The appealing advantages of LIBS are the use of unprocessed samples, the possibility of in-situ analysis, and the capa- bility of micro-area analysis [3]. For these reasons, LIBS has been successfully implemented for elemental analy- sis in various fields, such as the environmental field [4, 5], the metal industries [6–8], and nuclear power plants [9]. LIBS has also been used for calcium detection; cal- cium analysis is known to be necessary in various ap- plications, including soil analysis, the coal industry, and environmental. Bustamante et al. performed Ca analy- sis in soil using LIBS [10]. Maravelaki-Kalaitzaki et al. employed LIBS for the characterization of encrustation on marble [11]. Body and Chadwick conducted research on coal analysis using LIBS [12]. Although LIBS has nu- merous applications, it suffers from reduced sensitivity compared to other spectroscopic methods. To overcome this drawback, efforts have been made by many LIBS groups to develop the double-pulse LIBS technique (DP-LIBS) [13–15], which can be effectively used for the improvement of the analytical capabilities of single-pulse LIBS (SP-LIBS). DP-LIBS obtains signif- icant increases in the signal-to-noise ratio (S/N) and the emission intensity compared to SP-LIBS. The enhance- ment in line emission intensity achieved by double-pulse excitation is believed to be due to the increased ablated mass, higher plasma temperature, and longer plasma du- ration [16]. Other methods aimed at enhancing the emission inten- sity have been developed by coupling microwave (MW) and laser systems, which is known as MW-assisted LIBS (MA-LIBS). Envimetrics and Liu et al. used MWs to enhance the plasma emission of metal samples [17, 18]. Kearton et al. and Liu et al. reported intensity enhance- © Higher Education Press and Springer-Verlag Berlin Heidelberg 2016
  • 2. Research article Fig. 1 Experimental setup used in this work. ments obtained by using laser-assisted MW spectroscopy (LAMPS) [19, 20]. Ikeda et al. used MWs to extend the lifetime of plasma emission to the order of a millisecond [21]. However, these methods required the use of waveg- uides and microwave cavities. For the convenient application of MWs, we developed a method of MA-LIBS coupled with a loop antenna for the enhancement of LIBS emission. In this method, a lu- minous plasma is generated by a low-energy pulsed laser at a local point, where an electromagnetic field is pro- duced by localized MW radiation. The MWs are applied through a loop antenna via a coaxial cable to enhance the plasma emission. We must emphasize that this method is especially suitable for practical application because the antenna is very flexible and can access the sample via the coaxial cable, which is combined with a fiber sys- tem. Thus, the technique is highly applicable to mate- rial analysis in the field. In contrast, previously proposed MA-LIBS methods required waveguides and microwave cavities, which is inconvenient for practical applications because the sample must be placed in a special chamber connected to the MW source. In this study, the effect of MWs on the enhancement of laser plasma emission was studied by measuring time- resolved emission spectra obtained with (MA-LIBS) and without MWs (LIBS). Pelletized calcium oxide (CaO) powder was used as the sample. 2 Experimental setup The basic experimental setup used in this work is shown in Fig. 1. A Q-switched Nd:YAG laser (Quanta-Ray, Spectra Physics, 532 nm, 8 ns) was directly focused onto a sample surface through a quartz window (200 mm) to generate a plasma. The laser energy was fixed at 5 mJ. The plasma emission was enhanced by intensified MWs produced via a loop antenna; the antenna was shaped as a loop with a diameter of 3 mm. MWs were generated us- ing a magnetron at a frequency of 2.45 GHz (MUEGGE MG0500D-215TC, 400 W, 0–1 ms). The MW impedance could be experimentally adjusted for the plasma genera- tion by a three-stub tuner. The Nd:YAG laser and MWs were operated in the synchronization mode and a delay time of 10 µs was used for the Nd:YAG laser bombard- ment relatively to the MW generation to obtain MWs with good stability. The sample used in the study was a calcium oxide (CaO) pellet, which has relatively simple spectral lines. During the experiment, the sample was placed in a metal chamber equipped with windows, on which a fine-plated gold mesh (lattice constant of 80 µm and wire diameter of 30 µm) was attached. The experiment was performed in reduced-pressure Ar surrounding gas (0.6 kPa). The emission spectrum was obtained by using an in- tensified charge-coupled device (ICCD) camera (Andor, iStar) through a high-resolution echelle spectrometer (LTB ARYELLE) with a resolution of 50 pm. The light emission of the laser plasma was collected by an optical fiber positioned at approximately 80◦ relatively to the laser axis (Fig. 1). The plasma radiation from the sam- ple surface for the LIBS and MA-LIBS cases was imaged at one end of the fiber using a quartz lens (f = 100 mm). To study the dynamics of plasma expansion, an ICCD 114209-2 Ali Khumaeni, et al., Front. Phys. 11(4), 114209 (2016)
  • 3. Research article camera (Andor, iStar) was used. The plasma emission was imaged by using a quartz lens placed in the ICCD. 3 Results and discussion To determine the optimum emission intensity of Ca lines in laser-induced plasma with and without MWs, the spa- tial distribution of the time-integrated emission intensity of Ca was measured. Figure 2 displays the emission in- tensities of Ca II 393.3 nm and Ca I 422.6 nm, measured perpendicularly to the sample surface. The figure shows that the time-integrated emissions of Ca II and Ca I are distributed up to 10 mm and 5 mm from the sample sur- face in the case of MA-LIBS and LIBS, respectively. In the MA-LIBS case, the optimum emission intensity of Ca ions was located at 4 mm to 7 mm from the sam- ple surface, and in the case of LIBS, at 2 mm. It must be mentioned that the position of the loop antenna was 3 mm above the sample surface. In the experiment, the laser beam was focused on the sample surface after pass- ing through the inner side of the antenna. It is assumed that the optimum intensity was obtained at 4 to 7 mm because the electromagnetic field was optimum in the in- terior of the loop antenna. Based on this result, we used 5 mm and 2 mm heights from the sample surface for the data acquisition in MA-LIBS and LIBS, respectively. Figure 3 shows the emission spectra of calcium ac- quired from the CaO sample using MA-LIBS and LIBS. The gated delay time was 2 µs and the gated width was 600 µs. The laser energy was set at 5 mJ and the mi- crowave input power was 400 W. The spectra were ac- cumulated for the duration of 10 laser shots. The laser beam focused on a new point of the moving sample sur- face to avoid shot-to-shot fluctuation. For a comparison between the MA-LIBS and LIBS cases, the experimen- tal conditions were the same. Figure 3(a) shows that the Ca ionic lines at 393.3 nm and 396.8 nm can be clearly Fig. 2 Spatial distribution of Ca II 393.3 nm and Ca I 422.6 nm taken from the calcium oxide sample by using LIBS with and without microwave. Fig. 3 Emission spectra of (a) Ca II at 393.3 nm and 396.8 nm, and (b) Ca I 422.6 nm taken from the calcium oxide sam- ple by using LIBS with microwave and without microwave. observed with very low background emission intensity both in the MA-LIBS and the LIBS spectra. It must be noted that, compared to LIBS, a significant intensity en- hancement was obtained for the Ca ions at 393.3 nm and 396.8 nm when the MWs were employed. The enhance- ment factor for the Ca II 393.3 nm line is approximately 200 times; this was defined as the ratio between the MA- LIBS intensity and the LIBS intensity after subtracting the background emission. A different result was obtained for the case of the neutral emission intensity of Ca, as shown in Fig. 3(b). Namely, the enhancement factor for the Ca neutral emission intensity at 422.6 nm is signif- icantly lower (approximately 10 times higher intensity achieved by MA-LIBS than by LIBS). The background emission is almost the same for LIBS with and without MWs, which suggests that the signal-to-background ra- tio (S/B ratio) is effectively enhanced when the MWs were applied. The mechanism of laser plasma enhance- ment by using MWs coupled with a loop antenna can be described as follows: a laser plasma is generated by a pulsed laser on a sample target near the center of the antenna, where a locally intensified electromagnetic field is produced. After several microseconds of plasma gener- ation, the electron density of the laser plasma decreases, Ali Khumaeni, et al., Front. Phys. 11(4), 114209 (2016) 114209-3
  • 4. Research article especially at the outer layer of the plasma region, and the electrons absorb the MW radiation. The electrons are then accelerated and provide kinetic energy to ex- cite the atoms and ions by multiple collisions between electrons–atoms and electrons–ions. The plasma emis- sion can be sustained for a long time because of the long MW duration, from several hundreds of microseconds to milliseconds. As a result, the plasma emission intensity is enhanced owing to the increased integration time. The interaction between laser plasma and MWs via a charged species like electrons is consistent with the observation of the enhancement factor difference between Ca ions and atoms. Because of the Coulombic interaction, the kinetic energy can be more effectively transferred to the ions than to the neutral atoms. It must also be noted that an experiment using DP-LIBS and LIBS reported in our previous work [22] achieved a 25-fold signal intensity en- hancement for DP-LIBS compared to LIBS in a Gd2O3 sample. This enhancement factor for DP-LIBS is signifi- cantly lower than the present result, namely, an enhance- ment factor of approximately 200 achieved by MA-LIBS in a CaO sample. This could be attributed to the longer lifetime of plasma emission in MA-LIBS, which results in a larger integration time compared to that of DP-LIBS. As a result, the total emission intensity in MA-LIBS is much higher than in DP-LIBS. To determine the cause of the emission intensity enhancement in the MA-LIBS method, the time-resolved emission of plasma was ob- served. Figure 4 shows the emission intensity of the Ca II 393.3 nm and Ca I 422.6 nm lines as a function of delay time. The plasma emission was measured with delays of 0–5 µs after the end of the YAG laser irradiation. We observe that in the MA-LIBS case, the emission intensities for both Ca ions and Ca atoms exhibit long lifetimes of ap- proximately 500 µs. The intensity of ionic Ca sharply in- creases with time to form a peak at approximately 10 µs and subsequently decreases; the intensity of Ca I reaches a peak at 10 µs. It must be noted that the intensity en- hancement of Ca II is much higher than that of Ca I. At 5 µs, the MW radiation has been effectively absorbed by the laser plasma, enhancing the plasma emission as described above. The optimum intensity enhancement in the case of MA-LIBS occurs at 10 µs, which may indi- cate the delay time for which the absorption of the MWs by the laser plasma is optimum. Compared to the case of LIBS, which has a short plasma emission lifetime of approximately 50 µs, the emission obtained with MA- LIBS has considerably longer lifetime and higher emis- sion intensity. As a consequence of the prolonged plasma lifetime and higher time-resolved emission intensity, the integrated emission intensity of Ca is enhanced. The re- sults verified that the MW radiation significantly con- tributes to the enhancement of the laser-induced plasma emission. Fig. 4 Time-resolved emission profiles of Ca II 393.3 nm and Ca I 422.6 nm taken from the calcium oxide sample by using LIBS with and without microwave. To understand the role of MWs in the enhancement of laser plasma emission, the plasma temperature and elec- tron density in the laser plasma with and without MWs were also investigated. Selected lines and the correspond- ing spectroscopic data from the NIST database were used to determine the plasma temperature and electron den- sity [23]. The lines of Ca II 315.9 nm, Ca II 317.9 nm, Ca II 318.1 nm, Ca II 370.6 nm, Ca II 393.4 nm, and Ca II 396.8 nm were employed to calculate the plasma tem- perature. These lines and their spectroscopic parameters, obtained from the NIST atomic database, are shown in Table 1. To determine the plasma temperature, we assume that local thermodynamic equilibrium (LTE) is achieved [24, 25]. Examples of the Boltzmann plots of selected lines acquired with MA-LIBS and LIBS at 10 µs delay time are shown in Fig. 5(a). The slope of the curve yields a plasma temperature of approximately 10 900 K for the MA-LIBS and 9300 K for the LIBS data. The increased plasma temperature in the MA-LIBS case may be due to the effect of reheating by MW radiation, as in the case of pulsed-LIBS [26]. The introduction of the MWs into the laser plasma accelerates the electrons. Thus, the multiple collisions of electrons increase, resulting in the increase of plasma temperature. Figure 5(b) shows the Table 1 Wavelength, upper level energy, upper level de- generacy, and transition probability for the ionic Ca emission lines used in this study. Elements Wavelength (nm) Upper level energy (eV) Upper level degeneracy Transition probability (s−1) Ca II 315.9 7.0472 4 3.1 × 108 Ca II 317.9 7.0496 6 3.6 × 108 Ca II 318.1 7.0471 4 5.8 × 107 Ca II 370.6 6.4679 2 8.8 × 107 Ca II 373.7 6.4679 2 1.7 × 108 Ca II 393.4 3.1509 4 1.5 × 108 Ca II 396.8 3.1233 2 1.4 × 108 114209-4 Ali Khumaeni, et al., Front. Phys. 11(4), 114209 (2016)
  • 5. Research article Fig. 5 (a) Boltzmann plot made from the analysis of Ca II lines, considering the intensities at 0.6 kPa of argon surround- ing gas. The continuous line represents the result of a linear best fit. (b) Plasma temperature dependence of MA-LIBS on a delay time. estimated plasma temperature in the MA-LIBS data as a function of delay time. The time duration of each point plotted in the graph is 5 µs. At 5 µs, the plasma tem- perature is 10 500 K; it increases to 10 900 K at 10 µs, and slowly decreases to approximately 7700 K at 100 µs. We assume that the high temperature at the initial plasma emission is due to the high electron density in the plasma region. With increasing time, the electron den- sity decreases while the MWs continue supplying elec- tromagnetic radiation in the plasma region, resulting in multiple collisions between electrons, atoms, and ions. The increase in plasma temperature is attributed to the MW duration. Namely, multiple electron collisions in the MW-assisted laser plasma occur continuously while the MW radiation is applied in the laser plasma region. The high plasma temperature and long lifetime of the plasma emission observed in the MW-assisted laser plasma are due to the influence of MWs. The increased plasma temperature is attributed to the MW duration. Namely, multiple electron collisions in the MW-assisted laser plasma occur continuously while the MW radiation is applied in the laser plasma region. The electron density of the laser plasma obtained with and without MWs was also investigated. The full width at half maximum (FWHM) of the line, ∆λ1/2, is related to the electron density Ne by the expression [27]: ∆λ1/2 = 2w ( Ne 1016 ) + 0.35A ( Ne 1016 )1 4 ×x(1 − 1.2N −1/3 D )w ( Ne 1016 ) , (1) where w is the electron impact width parameter, A the ion broadening parameter, and ND the number of par- ticles in the Debye sphere. For a plasma in LTE, Stark broadening is predominantly determined by the electron impact. Because the perturbations caused by ions are negligible compared with those of electrons, the electron density related to the FWHM of the Stark-broadened line ∆λ1/2 is described by the following equation [25]: ∆λ1/2 = 2w ( Ne 1016 ) , (2) where Ne is the electron number density (cm−3 ), w is the electron impact width parameter. The measured FWHM is then corrected by subtracting the contribution of the instrumental line broadening (0.05 nm). By using the Ca II 396.8 nm line and Eqs. (1) and (2), we estimated that the electron densities of the laser plasma induced at 0.6 kPa with and without MWs were 1.5 × 1018 cm−3 and 7.6 × 1017 cm−3 , respectively. From the known electron density and plasma temperature, we can confirm that the LTE assumption is valid by applying the McWhirter criterion, which provides the lower limit of the electron density [28]: Ne ≥ 1.6x1012 Te1/2 ∆E3 , (3) where ∆E (eV) is the largest energy transition for which the condition holds and Te(K) is the plasma tempera- ture. In this work, we used ∆E = 3.9 eV for Ca and T = 10 900 K, which is the highest temperature obtained by MA-LIBS. Thus, the lower limit of the electron density is approximately 9.9 × 1015 cm−3 . In both MA-LIBS and LIBS, the electron density in the plasma is much higher than 9.9 × 1015 cm−3 . Thus, the McWhirter criterion is fulfilled, verifying that the plasma at 5 mm from the sample surface was in LTE conditions. 4 Conclusions We conducted a study on the effect of MW radiation on the enhancement of plasma emission in LIBS. In this work, MWs were introduced into a laser plasma through a loop antenna to enhance the LIBS emission. The re- sults revealed that the optical emission intensity, plasma lifetime, electron temperature, and density were strongly influenced by the MWs. When the MWs were injected, the lifetime of plasma emission obtained by LIBS (ap- proximately 50 µs) was extended to approximately 500 Ali Khumaeni, et al., Front. Phys. 11(4), 114209 (2016) 114209-5
  • 6. Research article µs throughout the MW duration, the LIBS plasma tem- perature increased from 9300 K to 10 900 K, the electron density from 7.6 × 1017 cm−3 to 1.5 × 1018 cm−3 , and the plasma size expanded to 15 mm. As a consequence of these phenomena, the plasma emission can effectively be enhanced by using MWs and the emission intensity of Ca achieved by LIBS was increased by approximately 200 times. The final goal of the proposed method is its prac- tical application (remote and in-situ analysis) in solid material analysis. The MA-LIBS method using a loop an- tenna is very suitable for practical applications because the antenna is very flexible and can access the sample by using a fiber system. Thus, it is highly applicable to material analysis in the field. In contrast, previously pro- posed MA-LIBS methods required waveguides and MW cavities, which is inconvenient for practical applications because the sample must be placed in a special chamber connected to the MW source. 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