2544 IEEE TRANSACTIONS ON PLASMA SCIENCE, VOL. 39, NO. 11, NOVEMBER 2011
Optical Observation of Nitrogen Propagation in
Argon Plasma
Daisuke Ogawa, Matthew J. Goeckner, and Lawrence J. Overzet
Abstract—While the gas flow patterns in reactors can be visual-
ized using models, it has proven that it is difficult to measure them.
This paper shows that the gas flow pattern for pulsed injection of
nitrogen gas into argon plasma can be readily seen in the optical
emission intensity. As N
2
enters the Ar plasma, N
2
molecules
cause increased optical emission intensity by the Penning effect.
This allows one to measure the N
2
propagation. In this paper, we
present the pictures with the measurement details and analysis.
Index Terms—Argon, emission, image analysis, nitrogen, optical
imaging, optical spectroscopy, plasma measurements, pressure
effects, spraying, velocity measurement.
L
ARGE gas flow rates and fast-pulsed injection of gases at
large flow rates are finding increasing importance in de-
vice processing, particularly in microelectromechanical-system
etching. The large flow rates and the quick switching between
gases must be also accompanied by great processing uniformity
over large areas. This undoubtedly requires a very uniform gas
distribution (or gas flow pattern). While the gas flow pattern
can be visualized by modeling, it has thus far proven to be
remarkably difficult to measure. In this paper, we show the
gas flow pattern for nitrogen injection into argon plasma using
time-resolved measurements of the optical emission intensity
pattern. Such a method can be used to measure flow patterns in
reactors for comparison with models.
In order to take the series of time-resolved total emis-
sion intensity pictures shown in Figs. 1 and 2, we used an
intensified charge-coupled device (ICCD) camera (Princeton
Instruments–ITEA/CCD-576GRBEM). The ICCD gate time
was set at 0.2 ms, and each picture comes from an average
of over 16 N
2
injections. To obtain the change in emission
caused by the arrival of the N
2
molecules, the pictures were
subtracted, pixel by pixel, from the intensities measured just
before N
2
arrived at t =2 ms. White–green indicates a region
where the emission increased, dark-blue–black indicates that
the emission decreased, and blue indicates that the emission
remained constant. All pictures have the same color scale.
We visualized the gas propagation in plasma by inject-
ing gases through an automotive fuel injector (Denso 23209-
0D040) into a 120-mtorr capacitively coupled Ar plasma.
For this initial discharge, the flow rate was 15 standard cu-
bic centimeters per minute (SCCM), and the RF power was
10 W at 13.56 MHz. The injector was located 3
′′
above
the plasma region, at the top of a six-way 4(1/2)
′′
cross.
The injected gas causes the chamber pressure to rise to
Manuscript received November 29, 2010; revised June 3, 2011; accepted
June 4, 2011. Date of publication July 18, 2011; date of current version
November 9, 2011. This work is supported by the Department of Energy under
Grant DE-SC0001355.
The authors are with The University of Texas at Dallas, Richardson,
TX 75080 USA (e-mail: goeckner@utdallas.edu; overzet@utdallas.edu).
Digital Object Identifier 10.1109/TPS.2011.2159625
∼180 mtorr, 60 ms after the injector opened. The equivalent gas
flow rate was 240 SCCM, the reactor was 2.5 L, and the pump
speed was 3.6 L/s. The injector opened at ∼3 ms, resulting in
a pressure wave arriving at the plasma at ∼3.2 ms. The plasma
was driven by the RF electrode, observed at the bottom of the
circular window in the pictures. This is most noticeable by the
increased optical emission occurring just above it. Although
the net plasma power can vary as the gas flows in, it was found
to remain constant at ∼10 W during the time period shown in
Figs. 1 and 2.
Fig. 1 shows the results of the Ar gas injection into the Ar
plasma for comparison with the N
2
results. The Ar injection
only increased the emission just above the RF electrode surface
once the pressure wave arrived [see Fig. 1(b) and (c)]. In
addition, the emission decreased in the region just above the
brightened line. This is all consistent with the sheath thinning
as the pressure increases and the electron mean free path
decreases. The emission increases more on the right-hand side
of each picture, which is consistent with the orientation of the
injection.
As shown in Fig. 2, the injection of N
2
into the Ar plasma
gives a markedly different emission pattern from that with
the Ar injection, allowing one to see how N
2
fills the reactor
volume temporally. Here, there is an emission increase that
propagates from the top to the bottom on the right-hand side.
It takes ∼0.4 ms for N
2
to traverse from top to bottom in
these pictures indicating speed ∼160 m/s (one-third the thermal
velocity of N
2
). Furthermore, time-resolved optical emission
spectra, taken under experimental conditions similar to those
used in Fig. 2, showed that the propagation observed in Fig. 2
was indeed caused by N
2
. Lines from both the first negative
system of N
2
(427 nm; C
3
Π
u
− B
3
Π
g
, v
′
− v
′′
; 1–5) [1] and
the second positive system of N
+
2
(427.8 nm; B
2
σ
+
u
− X
2
σ
+
g
,
v
′
− v
′′
; 0–1) [1] increased as N
2
arrived [2]. Furthermore, an
Ar emission line (415.9 nm; 3p
6
− 1s
5
) [3] decreased at the
same time [2]. Therefore, the increased emission was from N
2
,
and the implication is that Ar metastables and Ar
+
cause that
increase in emission via excitation reactions [4], [5] of N
2
.
Finally, the N
2
addition affects the plasma near the RF
electrode nearly immediately. The emission just above the RF
electrode well decreases before the N
2
gas arrives. The black
region indicates a significant reduction in emission in the main
body of the plasma that occurs well before the N
2
gas arrives
and continues on the left-hand side even after the N
2
gas
reaches the RF electrode. As such, it seems that this decrease
cannot be explained by any chemical interaction, such as the
increased emission at the right, but must be rather related to a
plasma impedance change or other far-reaching and fast effects.
In conclusion, we have followed the N
2
propagation in argon
plasma by a change in emission. The increased emission ap-
pears to have been caused by Penning excitation and ionization
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