5 Surface Wave Plasma Sources Michel Moisan,
1.0
Joette Margot and Zenon Zakrzewski
INTRODUCTION
As a first approach to presenting surface wave (SW) plasma sources, let us consider their distinctive features with respect to the other plasma sources described in the book:
1. The discharge can be sustained far away from the active zone of the field applicator. This is because the electric field supporting the discharge is provided by a wave that carries away the power from the applicator. It is an electromagnetic surface wave whose sole guiding structure is the plasma column that it sustains and the dielectric tube enclosing it.[lj-[3j This is, thus, a non-eumbersome method for producing long plasma columns; plasma columns up to 6 meters in length have been achieved in our laboratory while launching the wave with a field applicator that surrounded the discharge tube over a few centimeters in length only.f4][5j 2. The range ofthe applied field frequency f = m121r is the broadest of all kinds of high frequency (HF) sustained plasma sources. We have succeeded in realizing HF power transfer to the discharge efficiently from approximately 10 MHz to 10 GHz[6j and, with impaired coupling efficiency, down to 200 kHz.[7] This frequency range includes radiofrequencies (RF) and the lower part of the microwave
191
192 High Density Plasma Sources frequency spectrum; we use the term high frequencies to designate RF as well as microwave frequencies. An interesting aspect ofthis frequency flexibility is the possibility ofacting on the electron energy distribution function (EEDF) to optimize a given plasma process.Pl
3. The gas pressure range is extremely large. On the one hand, one can operate SW discharges in the sub-mtorr range under electron cyclotron resonance (ECR) conditions, [9] while, on the other hand, it is possible to sustain a stable plasma of a few millimeters diameter at pressures at least a few times atmospheric pressure.U''l
4. The range ofplasma density, n, is very large. At reduced pressure and with f in the few MHz range, n can be as low as 10 8 cm', [7] while at atmospheric pressure it can exceed 10 15 cm-3 . [I OI A related parameter is the degree ofionization a., i.e. the plasma density relative to the initial neutral atom concentration. Under ECR conditions, for example withf = 2.45 GHzwheren can reach up to a few 1012 cm', a, ranges approximately from O.1-10%, whereas in the abovementioned atmospheric pressure case, it is smaller than 10-4. The higher n, the higher the rate of plasma processes dependingon ions or on neutral particles (e.g., atoms, radicals) when the latter are obtained through electron collisions.Pl Large a i values favor the existence ofa Maxwellian EED F. Compared to other RF and microwave plasma sources, SW discharges are undoubtedly the most flexible ones. They also are efficient discharges since very little HF power is lost in the impedance matching circuit. Moreover, as far as theory is concerned, SW discharges are the most completely modeled HF discharges; this provides insight into HF discharges in general since, to a first approximation, the local plasma properties of SW discharges are the same as in all RF and microwave discharges under given discharge conditions (discharge tube shape and dimensions, nature and pressure of the gas, frequency f and, eventually, intensity of the static magnetic field), and for a given HF power density deposited in the plasma. The advantages of SW discharges are thus to be found in their flexibility, coupling efficiency and reproducibility, and in their advanced modeling. This chapter is organized as follows. Section 2 provides a summary ofthe wave and plasma properties ofSW sustained plasma columns. Section 3
Surface Wave Plasma Sources
193
reviews the essential parts composing a SW plasma source while Sec. 4 describes a family of efficient SW launchers for such plasma sources. Section 5 dwells on three typical experimental arrangements and, finally, Sec. 6 is a brief summary recalling the advantages of SW plasma sources.
2.0
SUMMARY OF THE MAIN PROPERTIES OF SW SUSTAINED PLASMA COLUMNS
2.1
Nonionizing Surface Waves Along a Plasma Medium
We start by presenting the properties of electromagnetic surface waves in general. A bounded plasma may support such waves which are guided along the boundary surface, their energy flux being concentrated in the vicinity ofthis surface, hence their name.[1l][12] As a rule, the plasma is contained within a cylindrical dielectric tube, which is sometimes placed coaxially inside a metal enclosure; however, the metal-free configuration is the one most often used. In the latter case, the field intensity decays radially in free space in a quasi-exponential fashion, as shown from experiment in Fig. 1.[13] We consider first nonionizing waves and an axially uniform plasma to better evidence later on the specific characteristics of surface waves when they sustain discharges.
1l-25.2m-1
E
-0.5
"E :::J
CP
.2:
'6
g
....
-1.0
N~
0>
.5!
-1.5
5
9
RADIAL POSITIQN (em)
Figure 1. Natural logarithm of the squared intensity of the wave electric field radial component outside the plasma tube as a function of radial position from the axis, for a m = 0 surface wave sustained discharge ei f> 900 MHz; the tube outer wall radial position is indicated by an arrow. The points are experimental while the full line is fitted from theory, yielding the value of the axial phase coefficient fl. Measurements are performed at 300 mm from the wave launcher in argon at 250 mtorr, in a tube of26 and 30 mm i.d. and 0.d.l 13]
194 High Density Plasma Sources In a cylindrical configuration, the possible modes of propagation of surface waves are defined by their field intensity dependence upon the azimuthal angle ¢. This field intensity in the case ofuniform media varies as exp U(OJt- pz+ m¢) - az] for traveling waves wherej= -Y:f, tis time, z is the axial coordinate, p is the axial phase coefficient (p = 21l/A where A is the SW wavelength along the z axis) and a is the axial attenuation coefficientl while m is the integer defining the mode of propagation. In the absence ofa static magnetic field applied to the plasma, the dispersion equation for the Iml ~ I modes is exactly the same for the positive and negative values of a given Iml. These two waves are thus degenerate, i.e., their phase and attenuation characteristics are identical. Experiments show that they are excited simultaneously since their mixing leads, in the azimuthal direction, to a standing wave pattern. [14] This is shown in Fig. 2 for the Iml = I mode, where the squared intensity ofthe radial component ofthe wave electric field has been recorded as a function of ¢.tt
",/2" = 2A5GHz Argon: 200 mtorr
R= 13mm
=
Ro 15mm
m=1
~
"'w
m=O
OL-_-'-_-'-_-'-_----'-_ __'__--"""""'_-'-_~_ __'___~_~_ ___' 270
300
330
o
30
60
90
120
ISO
180
210
240
270
AZIMUTHAL ANGLE, 4> (deg)
Figure 2. Observed azimuthal distribution of the squared intensity of the wave electric field radial component, for a surface wave plasma column sustained either in the m = 0 or m = I mode in a cylindrical discharge tube of inner and outer radii Rand R o.l 14]
t It is only in the case where the media are perfectly lossless that the wave propagates completely along the z axis and without attenuation. Otherwise, in a plasma, the higher the collision frequency, the more the direction of wave propagation, and that of the power flux, point towards the normal to the axis of the plasma column.Usl Nonetheless, it is the axial phase coefficient p that one readily measures. tt Although Figs. I and 2 concern SW sustained discharges, the features that they illustrate are common to both ionizing and nonionizing surface waves.
Surface Wave Plasma Sources
195
.Surface wave propagation in a plasma is usually characterized by the so-called phase diagram or phase characteristic. This is a plot of fJ versus mlmp where m is fixed and the angular plasma frequency mp = (ne 2Ime &o) 1I2 varies, in contrast with a dispersion diagram in which it is to that varies and mp is constant (e/m; is the electron charge-to-mass ratio and &0 is the free-space permittivity). Figure 3 shows an example ofthe phase characteristic ofthe azimuthally symmetric (m = 0) surface wave, where the effective collision frequency for momentum transfer, v, is set to zero. In actual fact, as long as v 2 « m2 , i.e., under low pressure conditions, the phase characteristic is unaffected by the presence ofcollisions. Note that aiko; = (1 + &g)-1I2 is the limiting value when fJ ~ co (wave resonance), where &g is the tube relative permittivity; this sets the minimum density nD below which the wave no longer propagates. Numerically, Eq.(l) wherefis expressed in MHz (as an example, the value of &g is 3.78 for fused silica). For some tube dimensions and values off, the phase characteristic may show a slight overshoot before tending toward the asymptotic value expressed by Eq. 1, leading to n values slightly lower than nD . When vim grows past a certain value, experiment shows that the minimum density for wave propagation then increases with respect to nD .f3j In short, from the above (i) measuring fJ can be a way of determining n; (ii) the higher f, the higher nD . Figure 4 shows the attenuation characteristic ofthe wave corresponding to the phase characteristic in Fig. 3. Under such low pressure conditions, a satisfactory analytical expression for «(fi) is
Eq. (2)
where R is the inner radius of the discharge tube and
Eq. (3)
n(z) =
2 rR R2 J n(r,z)rdr o
196 High Density Plasma Sources is the cross-section average electron density.t Here B(OJ,R) has to be determined by fitting Eq. 2 to the attenuation coefficient calculated for a given OJ and a given R. The value of n depends onf, on the nature ofthe gas and is approximately proportional to its pressure p. Note that Eq. 2 implies that ii > nD and so nD defines the minimum density for surface wave propagation; it also shows that a( n) increases with decreasing n.
.5
----1 / ~
-------------.-=.-:.;--:.;.-;:..;:--......._ - j
.4
.3
&
8
8
.2 co/ 21t = 2.45 GHz R =5mm
.1
Ro = 6mm £g = 4
0 0
.5
pR
1.5
2
2.5
Figure 3. Calculated phase characteristic of the azimuthally symmetric (m = 0 mode) surface wave propagating over a cylindrical plasma column of inner and outer radii R and R o , assuming the influence of collisions to be negligible. The dashed line corresponds to wave resonance (fJ ~ 00) conditions and it depends on the relative permittivity eg of the discharge tube.Isl
t Plasma columns are, in general, nonuniform radially. Considering positive column plasmas, Trivelpiecel'>J has used a perturbation-like calculation to show that this type of nonuniformity has little influence on the propagation and attenuation characteristics of surface waves provided fJR < 1, i.e., n(r) in the corresponding equations can be simply replaced by ii. Using this time a self-consistent model for surface-wave sustained plasmas, Sa et aIJ l 6) have shown that the radial nonuniformity of the plasma has some, though limited, influence on the wave characteristics whatever the value of fJ for f= 433 MHz andR = 38 mm whereas there is no influence at all atf= 2.45 GHz andR = 1.5 mm.
Surface Wave Plasma Sources
197
- - NUMERICAL CALC. - - - - - - ANALYTICAL APPROX.
-E 2
_>-
--
10-9
Ie ~
co / 21t = 2.45 GHz
10-10
10-11
,
R = 5mm
""
RO = 6mm Eg=4 '--
10-1
-'-
.....L
'--
102
...l
103
Figure 4. Calculated normalized attenuation coefficient ofthe azimuthally symmetric (m == 0 mode) surface wave as a function ofthe cross-section average electron density 'if, under the same conditions as for the phase characteristic ofFig. 3. The plasma is assumed to be weakly collisional, namely (vl@)2 « 1 where v is the effective collision frequency for momentum transfer, nD the density at SW resonance and nc the critical density (@p == @). The analytical approximation is that ofEq. 2)6)
Another useful parameter for describing surface wave propagation is the characteristic impedance ~ of the plasma column (considered as a waveguiding structure) as seen by the wave. In the case of a weakly attenuated wave, R; can be assumed real. This resistance is instrumental in explaining the energy transfer from the wave launcher to the excited wave. We define it as Eq. (4) with
Eq. (5)
198 High Density Plasma Sources where EJr) is the radial component ofthe wave's electric field strength and P is the total (i.e., including all media) power flux of the wave at z. Recall that the characteristic impedance for any wave other than the transverse electric and magnetic (TEM) waves cannot be uniquely defined. The m = 0 mode surface wave is a transverse magnetic (TM) wave while the m ~ 1 mode surface waves are combinations of TM and transverse electric (TE) waves.£14] We have used expressions (4) and (5) because they account for the power carried away by the wave in the equivalent circuit of the plasma source (Sec. 3.3).t Figure 5 shows a typical example ofthe dependence of R; on ii. Note that for electron density values exceeding a few times nD, the plasma impedance seen at the launcher's is nearly independent of ii. When sustaining a plasma with surface waves (see below), the stability of R w with respect to variations of n may be important for certain applications such as analytical chemistry, as it ensures that the impedance matching of the plasma source with the HF generator remains unaffected under varying discharge conditions. ""' E s:
200
0 "'; 180 £l'
160
u.i U 140 Z
< 0
w 120
c..
~
U
100
i=
80
ii w
60
R .. Smm
40
Ro .. 6mm
ill / 21t.. 2.45 GHz
II)
I-
~<
:l:
U
Eg
20
= 3.78
0 0
2
4
6
8
10
ELECTRON DENSITY (10 12 cm- 3) Figure 5. Calculated characteristic impedance R; of the plasma column as seen by a rn = 0 mode surface wave, as a function of the cross-section average electron density. The plasma is assumed to be weakly collisional and nD is then the minimum density for wave propagation.l'"
t lntroducing the axial electric field component E, instead of E; in Eq. (5) leads to an imaginary U value since it corresponds to a power flow being transverse to the axis.
Surface Wave Plasma Sources 2.2
199
Surface Waves When They Sustain a Plasma
A surface wave carrying sufficient power flux can sustain the plasma column along which it propagates. Under purely traveling wave conditions, the electron density then steadily decreases away from the launcher because the power flux of the wave decreases axially as power is gradually transferred to the discharge: the plasma column is axially nonuniform. As a result, one can infer from Fig. 3 that the value of f3 can be a rapidly increasing function of axial position z. Nonetheless, the wave phase characteristic can be used locally at position z, as if the column extended uniformly in the axial direction on both sides of this point, provided the WKB condition is verified. It reads here
Eq. (6)
1 dil(z) (Z ) -----«/3 il(z) dz
In this case, the wave phase increases progressively as
s: /3(z')dz' In contrast to nonionizing surface waves, surface waves sustaining a plasma propagate in a mode that is very little dependent upon the azimuthal configuration of the wave launcher.U'tl their mode selection relies essentially on the value of the product JR. When this value is less than approximately 2 GHz em, one can sustain a plasma only with the m = 0 SW. WhenJR is increased starting from 2 GHz ern, one can achieve the discharge with the m = 1 mode, first over a narrow operating domain, then over a broader range and more easily than with the m = 0 wave and, finally, the m = 0 mode plasma can no longer be obtained. With increasingfR, the preceding situation repeats with the m = 2 wave relative to the m = 1 mode plasma, and so on. The axial nonuniformity of the SW plasma column can be a shortcoming in some applications, but there are possible remedies to this situation. One of them is to have the wave reflected at the end of the discharge tubel'?' or on some staggered dielectric obstacle.F" Another solution is to place a wave launcher at each end ofthe plasma tube, the two axial gradients canceling out. These launchers must be supplied from two
200 High Density Plasma Sources separate, non-phase-related HF power generators to avoid forming standing waves, [19] which would lead to spatially periodic variations of plasma density along the column. [20]
2.3
Properties of SW Sustained Plasma Columns
Axial Properties. The effects resulting from increasing the HF power incident on the field applicator are specific to SW discharges: • The length of the plasma column increases (provided the discharge tube allows it) • The axial gradient of n is barely affected • The additional plasma length connects to the high density side of the column
This can be seen in Fig. 6. Consider, for example, the curve atf= 100 MHz and the increase of input power from 36 to 58 W. The plasma column initially sustained at 36 W remains unchanged when the power is increased; it becomes the tail of the higher power plasma column. On account of this, the axial properties of SW plasma columns are better described when they are referred to the end of the column rather than to the launcher. Notice in the figure that dii/dz does not vary in general with axial position, except here atf= 27 MHz where the slope takes on two slightly different values.l-U The observed linear decrease of n as a function of z can be obtained analytically from theory for a weakly collisional plasma.£22]t The axial gradient of n can actually be cast as an electrodynamic similarity law upon ( vf/R) which expresses the discharge conditions (as defined in the introduction; here p is represented by its action on v), namely
Eq. (7)
dYi =
dz
_c(Yf) R
where C = 7.3 x 10-3 whenfis in MHz, R in em and dii/dz in crrr". Recall that Eq. (7) is valid under low pressure conditions; at higher pressures (including atmospheric pressure), this dependence is only qualitatively obeyed.
t Typically with argon gas, the plasma is considered to be weakly collisional at pressures below 20-30 mtorr for f = 360 MHz and below 200 mtorr for f = 2.45 GHz.
Surface Wave Plasma Sources
..,
E 0
+
1.5
0
~
en Z
2R-6,Acm 2Ro=7.1 em
+
0
1.0
W
Argon: 30 mtorr + 200 MHz 0100 MHz .. 50 MHz o 27 MHz +'\
a
-,•
z
0
-,
0: 0-
U
w ~ w
201
0.5
400
300
200
100
0
AXIAL DISTANCE FROM THE END OFTHE COLUMN, z (em)
Figure 6. Axial distribution of electron density if along a m = 0 SW discharge, at various wave frequencies. The arrow shows the position of the wave launcher's gap from the end of the plasma column at the indicated power Po applied to iU 21j
Radial Properties. Radial Distribution of n. There is very little experimental data on n(r) in SW plasmas. This is because the usual local density diagnostics imply inserting in the discharge probes that usually strongly disturb the SW field, hence the plasma. [20] We thus tum to theory for information. Consider the case where charged particles are mainly lost through diffusion to the wall: the radial profilel of electron density is determined by two factors: (i) the global movement ofthese particles toward the wall, which depends essentially on the vessel configuration and dimensions; (ii) the radial variation ofthe ionization rate. In the specific case of SW discharges where the wave electric field intensity E (and consequently the ionization rate) increases with radial position, Ferreira's modeling[23] shows that n(r)/n(O) is flatter than the Bessel function J o (2.4 r/R), which applies when E is sufficiently radially uniform as in the positive column plasma of a DC discharge.
t The terms profile and distribution are used to designate n(r)/n(O) and n(r) respectively.
202 High Density Plasma Sources Radial Distribution of Excited Atom Density. The radial density distribution nir) of atoms excited in a given state j in SW discharges vary significantly withj R, P (discharge conditions) and n. Two types of radial profiles are observed depending on whether we are considering atoms in a radiative state (once excited, these atoms emit a photon well before suffering a collision) or in long-lived states, which can be metastable (these atoms lose energy through collisions) or resonant energy levels (photons are trapped in the plasma).£24] Figure 7 shows a three-dimensional presentation of the radial density profile of atoms in a given radiative state as a function of ii; whatever j nj increases with 11. In the positive column plasma, whatever ii, the maximum of nir) is at the tube axis while, with SW plasmas, this maximum moves toward the wall with increasingf, and as a result, nir) also broadens.F'I In summary from Ref. 25: (i) for givenp andf, the higher ii, the more convex (curved outward) are the profiles; (ii) for givenp and ii, with increasingj, the profiles become flatter or even concave; (iii) for given nand f but varying p, there is no general trend, except for p :::: I torr; then the radial extent of nj reduces with increasing p. This contraction of the profile is discussed in the next paragraph. .....,------;;;.....,..;:--------,1.0
E zC: O-
;:;;~ ~LO
~ ...... 0.5 w _
w< >...., ~~ ~;:;;
wZ
0.0
~w
Z
-I
Figure 7. Experimental three-dimensional plots showing the emission intensity from an argon optically thin line, as a function of the radial position and cross-section average electron density (p = 150 mtorr). (a) Positive-column plasma; SW-produced plasma at a frequency of (b) 200 MHz, (c) 600 MHz, and (d) 900 MHz )25] (Cant'd)
Surface Wave Plasma Sources
203
E
1.0
ZC
O~
en~
~Il)
<
::2:-
0.5w w....,
~~
:5 en
( b)
wZ
Q::W
0.0
l-
Z
5
10
-1
Figure 7. (Cont'd)
-1----:::;;:~~7.?:n:;>=;:'-----__,1.0 Z
E
c O-
0.5
::2:W
-<
~...,
~~
(c)
\--_-.1°. 0 W Z
....
~w
Z 16
12
I \()
~,
-1
Figure 7. (Cont'd)
:~)
\<;)C~
204 High Density Plasma Sources
E
1.0 Z c
O-
U;~
~ll)
~
<... ~~
0.5 w
w...,
~U;
(d)
wZ
0.0 ~~ 18 Z
6 -1
1
Figure 7. (Cont'd)
The radial contraction of the plasma column glow shows up at pressures above approximately one torr, whatever f and ii; this effect increases with p. When preaches 50-100 torr (the exact value ofp at which this occurs depends on R, on the nature of the gas, mostly its thermal conductivity, and its flow rate), the discharge glow breaks into .small diameter bright filaments which rotate and move around randomly[1O][26] This constricted filament effect is observed in DC arc discharges as well as in HF discharges.F" it is related to the setting of a radial gradient of gas temperature (due to a finite thermal conductivity) as p is increased. [28] Owing to this, achieving a stable and reproducible discharge requires reducing R until only one plasma filament is present in the discharge tube and well-centered radially. For example, at atmospheric pressure in argon and withf= 915 MHz, the diameter ofthe plasma filament does not exceed 2 mm at powers below 700 W (it grows with the HF power density); we find that 2R should not be larger than 6 or 8 mm to achieve a single filament discharge.U''l Figure 8 shows the measured radial density distribution of the 3P2 metastable and 1P 1 resonant state atoms in neon in a SW discharge at f = 900 MHz and, for comparison, in the positive column plasma of a DC discharge. [29] We observe that: (i) the radial density distributions are flatter in the SW plasma; (N) the maximum nj value attained as a function of r does
Surface Wave Plasma Sources
205
not differ markedly in both types of discharges-it is slightly higher for the 3P2 level in the positive column plasma whereas it is the opposite with the 'P, level. A similar behavior is observed in argon;[29] (iii) as a rule, the SW plasma has a larger cross-section density ii (11j is defined as n in Eq. 3). In the particular case ofFig. 8, 11j (3P2) and 11j (ip]) are 2.5 and 5.2 times larger respectively in the SW plasma relatively to the positive column plasma. A similar advantage is also reported for the 2 3Sand 2 ]S metastable atoms in helium.[29] This effect is due to the radial increase of E toward the wall in SW discharges. As far as applications are concerned, a larger cross-section average density of metastable atoms could increase the throughput of species produced by Penning power transfer while, in the case of resonant state atoms, a larger value of nj close to the wall could be (but this is still under discussion) beneficial for UV lampsPH30]- [32]
2
,,
,
0'"
,p 1011
I
9
"
"l
E 0 ....,
~
,I I
I I
W
I
c
,,
-SURFACEWAVEPLASMA ~ ---- POSITIVE COLUMN PLASMA '.
"
9
I
6,,
I
I
2
lP
Q"
,
1010
0...... ,,
1 .IT'-o- , 0-
,, ct,
, \
,'D
~
I
,, ,,
0
p' I
5
,
0\
I I
,P
,
q,
r
\
3 -R
.,
,
... '" '0 c: C
,,
0,
I
0/
5
Z
~
,,
I
~
\ 0"
3P2
I
-R/2
a
R/2
R
RADIAL POSITION
Figure 8. Measured density of atoms in the 3P2 metastable and 'P, resonant states in neon, as a function of radial position in a SW-produced plasma (j"= 900 MHz) and in a positive-column plasma, in the same discharge tube (R = 13 mm), at the same gas pressure (p = 400 mtorr). The density of excited atoms has been maximized by varying the discharge current or the HF power. The column length is 150 mm.[29]
206 High Density Plasma Sources Azimuthal Density Distribution of Excited Atoms in a Radiative State. The azimuthal nonunifonnity ofthe wave electric field intensity that exists when Iml ~ I (see Fig. 2) reflects on nlr). Figure 9 shows nlr)/nlO) at two values ofthe azimuthal angle ¢ thatare 90° apart. At!=4 MHz(R = 13 mm), we observe that nlr, ¢) = nir, ¢+ 90°), which agrees with the fact that only the m = 0 SW plasma can be sustained at such a low frequency (Sec. 2.2). In contrast, atf= 2.45 GHz (R = 13 mm), the discharge is achieved in the present case with the Iml = I mode surface wave; there is then a maximum of excited atom density close to the wall at some angle ¢max while at ¢min = ¢max + 90°, nlr) is flat and assumes smaller values than at ¢max' Figure 9 also confirms the fact noted from Fig. 7 that the radial profile of excited atom density broadens with increasingj, provided psi torr.
>
t(/)
Z W
t-
Z'(i;'
10~1
AI I 549.6nm f=2.45GHz,m=1
-:= ZC::
O~
-(i)-=
(/)~
:E
10-2
w w
,
Z
.....
,
,, , ,
I
10-3 -1
-0.5
0
0.5
r/ R Figure 9. Observed radial profile of a thin line emission intensity in argon at 0.2 torr, from a 26 mm diameter plasma column at two frequency values. At 4 MHz, the radial recordings made at two azimuthal angles 90° apart indicate an azimuthally synunetric mode of propagation. At 2450 MHz, the fact that the two azimuthal profiles are different suggest a Iml = I mode wave. ,pmax (~) corresponds to the maximum field-intensity angular direction, whereas ,pmin, (- - -) 90° apart, relates to the minimum field intensity.Pl
Surface Wave Plasma Sources 2.4
207
Range of Discharge Conditions
The discharge conditions designate the operator-set parameters, excluding HF power, as defined in the introduction. The domain offrequency, j over which one can sustain a discharge with the m= 0 and Iml ~ 1 mode surface waves has been examined in Sec. 2.2. As for the domain of pressure, p, and discharge tube radius, R, we need to distinguish discharges with and without an applied static magnetic field. Range of p and R Values Without an Applied Static Magnetic Field. Besides its role upon wave mode selection through the productfR, R sets the minimum and maximum gas pressures of SW discharges: 1. The minimum pressure is defined as the pressure below which the discharge goes off. We have measured it in argon gas that was flowing to reduce contamination due to wall outgassing; the flow rate was nonetheless low (5 0.5 seem) to minimize the axial gradient ofpressure (particularly with the smaller diameter tube). The results are shown in Table 1. Different operating frequencies were used (9.5, 200, 465, 1000 and 2450 MHz) with the 25 rom i.d. tube; the observed variations of minimum pressure appeared to be within experimental error and not correlated with f The minimum pressure did not depend significantly on the HF power used (up to 180 W for f 5200 MHz and f = 2450 MHz, and up to 60 W for 465 and 1000 MHz). The plasma column was generally very short at minimum pressure with the HF power level used, which means that it was not always clear that the discharge was sustained by a fully developedsurface wave, eventhough the column length increased with HF power. The values shown in Table 1 are smaller than those that we have reported earlier[241 where the gas was stagnant. The minimum pressure values for the small and intermediate tubes in Table 1are much smaller than in DC glow discharges where pR minimum for argon is 0.22 mtorr em. [331 Recall that, in general, the minimum pressure for striking the discharge is higher than the minimum pressure considered here. 2. The maximum pressure is that above which the discharge is no longer stable and reproducible (see Sec. 2.3 on that subject). The larger R, the lower the maximum p value, as shown in Table 1.
208 High Density Plasma Sources Table 1. Pressure Range for a Stable SW Discharge in Argon Gas as a Function of the Discharge Tube Diameter
2R (mm)
3.5
Minimum pressure (torr) 3 ±l
x
10-4
Maximum pressure (torr) ~5000
(maximum tested value) 2.5 125
5 ±3 7
x
x
10-5
10-5
-20 ~0.35
Range of p, R, and B o Values When Applying an Axially Directed Static Magnetic Field. When below a certain gas pressure, we observe that a discharge can only be struck in the presence of a static magnetic field. At f = 2.45 GHz, in a cylindrical discharge vessel we can initiate a plasma at pR products as low as 7.5 x 10-4 torr em, provided an axially directed magnetic field ofsufficient intensity B ois applied to the discharge. Although this can be obtained with Boas low as 400 G, the best impedance match of the plasma source with the microwave generator occurs at B o ~ 960 G in our uniform field configuration (see Sec. 5.3).t This magnetic field intensity value is higher than that required theoretically for ECR in a cold plasma.Pf Above this optimum B o value, it is still possible to sustain plasma but its density and the microwave reflected power fluctuate. Considering the relatively larger range of the above operating Bo values compared to common ECR discharges, we conclude that we can achieve a magnetized SW plasma well below and above ECR conditions.
t The fact that this optimum power match is limited to a narrow range of Bo suggests that the discharge is then sustained resonantly.
Surface Wave Plasma Sources 3.0
209
ESSENTIAL ELEMENTS AND GENERAL FEATURES OF SW PLASMA SOURCES
So far, we have considered surface waves as they already sustain a plasma column, passing in silence over their launching. In this section, we shall describe devices that convert efficiently HF power into surface wave power flow. A SW plasma source includes as essential elements a wave launcher (composed ofthe HF field applicator and of its impedance matching network) and a dielectric discharge tube, as shown in Fig. lOa. We briefly review the role of these elements before going into details in the following sections.
WAVE LAUNCHER
,,: , ,, ,
··
FEED LINE
···
: IMPEDANCE: FIELD : : MATCHING: APPLICATOR j NETWORK: //
DIELECTRIC DISCHARGE VESSEL AND PLASMA: WAVEGUIDING STRUCTURE
oj
INPUT PLANE
· ··:, ·
~J
COLUMN END WAVE EXCITATION • : - PLANE(z=O)
.
P(z)
rp,
bj Po=P(O) =PA
Figure 10. (a) Essential elements of a SW plasma source and (b) power flow within it.
~,
PR , Ps, and ~ denote respectively the power incident in the feed line, the power reflected at the launcher input, the power radiated as space wave, and the power absorbed in the plasma. P(z) is the axial power flux of the surface wave, decreasing from Po at the launcher to almost zero at the end of the column.tsl
210 High Density Plasma Sources In a SW plasma source, the HF field applicator provides the electromagnetic field configuration required to excite a wave guided by the plasma column-discharge tube structure. As we see below, the field distribution for launching an m = 0 mode wave can be achieved efficiently using a ring shaped gap formed by two conducting surfaces (see Fig. 12 in Sec. 3.1). The function of the impedance matching network is to optimize the HF power transfer from the generator to the plasma. Both the field applicator and the matching network are essential in launching efficiently the surface wave; as we will see, these two elements of the wave launcher are not necessarily physically separated. As a rule, an efficient and well-eontrolled HF plasma source requires additional elements inserted between the generator and the launcher, as shown in Fig. 11. These are two directional couplers and a power meter, which provide the power l} incident on the wave launcher and the power PR reflected from it; a tuner and a circulator improve the power coupling efficiency and the stability of the plasma source respectively. These auxiliary components are typical elements of microwave networks; for details and operating procedures, see for example, Hubert et al.(3 5 ) and microwave text books.
CIRCULATOR
TUNER
I
·· ·· ·:
I
·
I
:
r r
I
I
·
TO MATCHED LOAD
I
· · I I
I
:.. I
FEED LINE
TO POWER METER
I I I I
·• ·•• · __ .: I
r
FIELD APPLICATOR
I I
I
Figure 11. Set of auxiliary elements to improve power transfer and stability in an HF plasma source. The insertion sequence of the elements must be observed.I'"l
Surface Wave Plasma Sources 3.1
211
Wave-Launching Aperture
Figure 12 shows the most common type of wave-launching aperture for sustaining a plasma column with a surface wave. This gap-type aperture consists of a cylindrical conducting sleeve surrounding the dielectric discharge tube (or a dielectric-material link to the discharge tube), and a thin conducting plate placed perpendicularly to the tube axis and positioned a few millimeters away from it. The launcher establishes in the gap region a high intensity electric field that excites the surface wave. With a proper design, very little of the power leaving the gap is emitted as space (nonguided) wave, [12] almost all ofit being transformed into a surface wave flow composed of two oppositely directed waves."
CONDUCTING SLEEVE THIN CONDUCTING FRONT PLATE
Figure 12. Elements forming the launching gap used for exciting m = 0 mode surface waves. This field-shaping structure consists of a cylindrical conducting tube (sleeve) surrounding the discharge tube (or a dielectric-material link to the discharge tube) and a thin (s 0.5 mm ) conducting plate perpendicular to the tube. When using a tight-fitting sleeve around the dielectric tube, the propagation of the wave excited at the gap towards the sleeve is nearly choked; this usually gives rise to a longer plasma column on the other side of the gap, where the discharge tube is surrounded by air. The arrows show approximately the electric field Iines.H
t As with any antenna, reactive energy is stored in the electromagnetic field at and in the
vicinity of the gap, and furthermore, here some power is dissipated in the plasma slab delimited by the gap interstice (more in Sec. 3.3). We shall neglect these losses further on.
212 High Density Plasma Sources 3.2
Efficiency of a SW Plasma Source
The efficiency 17 of an HF plasma source is the fraction ofthe power delivered at the source input that is absorbed into the plasma. It is an important parameter: the higher the efficiency, the more plasma volume or plasma density is obtained, while the occurrence of power losses in parts of the setup other than the plasma column can damage components. In a SW plasma source, there are three causes of power loss: power reflection at the launcher input, losses in the dielectric and metallic parts of the launcher and in the dielectric tube, and power radiation into the surrounding space through space waves. By a careful design of the wave launcher, the first two types of power loss, namely losses in the impedance matching network and in the field applicator can be kept low compared to the power PA absorbed into the plasma. We disregard these losses henceforth but, on practical grounds, regular checks should be made that it is really the case. We analyze the efficiency of SW plasma sources using the notion of coupling and launching efficiencies developed in connection with terrestrial surface waves.P'" and we refer to the power flow in Fig. lOb. The coupling efficiency accounts for the fraction ofHF power not entering the plasma as a result of reflection at the feed-line launcher interface and thus Eq. (8) The launching efficiency accounts for the power not entering the plasma because it is radiated as a space wave carrying power Ps . Assuming that the power from the launcher that is transformed into SW power flow is fullyf absorbed in the plasma (power P.4) , the launching efficiency is Eq. (9) As a rule, space-wave radiation can be kept at a very low level by proper design of the launcher and guiding structure (for example, the diameter of the gap elements should be as close as possible to the tube outer diameter).
t This assumption generally applies with the m = 0 mode but only under certain conditions with higher modes. For example, with the m = 1 mode plasma and when the jR product is not much larger than 2 GHz ern, a significant part of the power flux remains past the column endJl4]
Surface Wave Plasma Sources
213
The overall efficiencyofthe SW plasma source can now be written as Eq. (10) Neglecting Ps compared to ~, we finally have Eq. (II) This value can be measured directly in the feed line using standard reflectometer techniques.P'" 3.3
Impedance Matching in SW Plasma Sources
As seen from Eq. 11, the efficiency of the plasma source essentially depends on the possibility of reducing the reflected power at the launcher input. This can be done by using an impedance matching network. Such a system consists either of intrinsic tuning means (i.e., means incorporated into the applicator structure) or of external tuning elements. To achieve an optimum match, we need to know the influence ofthe various components of the plasma source on its input impedance. This can be provided by an equivalent circuit analysis. Equivalent Circuit of a SW Plasma Source. The various elements of an equivalent circuit represent HF energy storage and dissipation processes occurring in different parts of the system. [36] This representation method yields the electrodynamic characteristics of the plasma source without having to solve a full set of electromagnetic field equations. In this context, the plasma source is ultimately a lossy termination to the feed line. Gap Impedance. Figure 13 shows the circuit elements accounting for the impedance Zg seen at the gap when a SW discharge is sustained, which we call, in short, the gap impedance. The resistances Rwl and RW2 are the characteristic impedances of the plasma column (Sec. 2.1) as seen by waves 1 and 2, which propagate in opposite directions away from the gap; these resistances are related to the power carried away by the waves. The capacitances C w1 and Cw2 represent energy storage within the near-field region of the applicator when launching a wave. To account for energy dissipation and energy storage in the gap region itself, we use Zp and Z; to describe these processes in the plasma and outside it, respectively. The resulting gap impedance varies with the chosen reference plane in the launcher structure (see Sec. 4 for examples).
214 High Density Plasma Sources
CONDUCTING SURFACES GAP • TUBE WALL
PLASMA TUBE AXIS
of WAVE 2 ,
WAVE 1
bf
Figure 13. (a) Approximate electric field distribution in the gap region where a surface wave is launched in both directions; (b) corresponding equivalent circuit elements representing power transport (R,.) and reactive energy storage (Cw ) , power dissipation [Re(L;,), Re(Z.)] and energy storage [lm(Zp), Im(Z.)] within the gap region in the plasma and outside it respectively; Re and 1m denote the real and imaginary parts of a complex number. The resulting impedance Zg is called the gap impedancels)
Surface Wave Plasma Sources
215
Launcher Impedance. The whole wave launcher can be represented as a two-port network (quadrupole) inserted between the feed line of characteristic impedance Zo and the gap impedance Zg, as shown in Fig. 14a. Figure 14b is the T-configuration, one possible general form of the quadrupole (we will see specific quadrupoles for given wave launchers in Sec. 4). Since we neglect energy loss within the launcher, the quadrupole is lossless and all its impedances are imaginary. Figure 14c shows that the input impedance of the quadrupole is actually the load presented to the feed line by the plasma source. To relate this impedance to the source efficiency 1], we shall turn below to standard methods oftransmission line analysis. In this case, it is customary to use impedances normalized with respect to Zo, which is a real quantity, yielding Eq. (12)
z
= Z/Zo = R/ Zo + jXlZo = r + jx
or their reciprocal values, the normalized admittances, Eq. (13)
y
= ZrlZ = GZo + jBZo = g + jb
Conditions for Impedance Matching. The quantity that characterizes both the impedance mismatch ofa transmission line and the wave reflection level within it, is the reflection coefficient
Eq. (14)
The squared absolute value of this coefficient is equal to the fraction of the incident wave power that is reflected at the launcher input, Eq. (15) Considering that there are no losses within the launcher and no power radiation into space, Eqs. (11) and (15) yield the overall efficiency of the plasma source as Eq. (16)
1] =
1 -IIfJ2
216 High Density Plasma Sources
·· ··· ····
LAUNCHER INPUT --: PLANE
GAP INPUT PLANE
·· ·· ·· ·
-: I I I
I I
oj
WAVE LAUNCHER
bl
cJ
Figure 14. (a) The wave launcher as a two-port network inserted between the feed line of impedance Zo and the gap impedance Zg; (b) its equivalent T-circuit, and (c) the equivalent one-port termination ZL representing the plasma source impedance.H
A variable load impedance will absorb the maximum of power from the generator when it is equal to the complex conjugate of the output impedance of the generator (conjugate impedance matching). However, there is no reflected wave in the feed line only when GL = O. The latter condition calls for the termination ofthe feed line with an impedance equal to Zo (image impedance matching). In most practical plasma sources, a circulator (the input and output impedances of which are equal to Zo) is inserted between the generator and the launcher input (Fig. 11), mainly to avoid unstable operation. In this configuration, the generator is thus
Surface Wave Plasma Sources
217
terminated with Zo and the impedance seen from the launcher input towards the generator also equals Zo. The corresponding perfect match conditions at the launcher input are then Eq. (17) or, in terms of admittances, Eq. (18) Clearly the above conditions require that at least two of the equivalent circuit elements be variable. In practical terms, the wave launcher should be equipped with at least two independent tuning means; however, over a narrow domain of discharge conditions (e.g., under fixed frequency operation), a well-designed launcher can ensure close to zero reflected power with only one tuning element. [38]
3.4
Discharge Vessels
Using surface waves to generate plasma provides more flexibility in terms of discharge vessel shape and volume than any other type of discharge. The reasons are that: (i) the wave follows the interface between the plasma and its contiguous dielectric medium; then when the discharge tube configuration or dimensions are modified, provided this is done smoothly along the interface, the wave will continue to propagate, filling with plasma the whole cross-section of the tube; (ii) the plasma column length increases with increasing power delivered to the launcher. To achieve a surface-wave sustained plasma, part of the discharge vessel must go into the launcher aperture (or be connected to it by a dielectric link). The tube wall must be made of a dielectric material (e.g., fused silica, glass, ceramic), preferably not too lossy (loss tangent < 10-3 at the frequency ofoperation) to avoid HF power heating. The tube then heats mainly by diffusing particles and photons. This heating can be particularly detrimental to that part of the discharge tube enclosed within the field applicator, which reduces heat transport from the tube to the outside. With gap-type launchers, the gap opening can be used for directing compressed air onto the discharge tube. The specific design of the plasma vessel depends, of course, on its application. Figure 15 shows some vessel configurations particularly
218 High Density Plasma Sources suitable for surface-wave discharges. The simplest and most commonly used one is the straight cylindrical tube (Fig. 15a). Other tube configurations generally lead to reflection of the surface wave and excitation of a space wave at the discontinuity; the importance of these phenomena increases with the abruptness of the changes in configuration or dimensions. Consider the T-shaped vessel in Fig. 15b, with the wave launcher located at the base of the T. [391 It yields a plasma column that extends symmetrically on both sides of the junction: the electron density decreases away from the junction with the same axial gradient on each side; raising the input power increases the plasma length symmetrically. Space wave radiation is excited at the junction. To achieve surface-wave discharges with diameters that are large relative to available launcher apertures (which is the case, for example, when using standard-waveguide based systems), we recommend the configuration shown schematically in Fig. 15c. The large or useful section of the discharge tube is tapered down at one end to a size that can be accommodated by the launcher aperture. This design bypasses two limitations related to sustaining large diameter plasmas with surface waves: (i) the efficient operation ofsome launchers (e.g., surfaguidel'PI) requires that their aperture not exceed a given fraction of the free-space wavelength; (it) a perfect azimuthal uniformity of the plasma density requires the selective excitation ofthe m = 0 mode wave (recall Fig. 9).t As mentioned in Sec. 2.2, it is not possible to excite a m = 0 mode wave whenjR 2 2 GHz cm; however, one can launch the m = 0 mode wave in a "small" tube (fR ~ 2 GHz em) and have it propagate in a "large" tube by using a tapered transition to connect both tubes. Returning to Fig. 15c, the excited surface wave reaches the large-diameter section of the tube via a conical transition, the length of which is the result of a compromise: if it is too short, the reflected wave power is excessive, whereas if it is too long, too much power is expended in creating plasma outside the useful region. Figure 15d shows a discharge vessel intended for systems using an afterglow (remote) plasma for surface processing. The chemically reactive particles are generated within the HF field zone and from there on, they flow into the reaction chamber. Note that by increasing HF power to the launcher, the length of the plasma column increases and so does the residence time of particles in the discharge zone.
t However, in the presence of an applied static magnetic field, the m = 1 and m =-1 are no longer degenerate, i.e., there is no standing wave in the azimuthal direction. The plasma is then always azimuthally uniform.
Surface Wave Plasma Sources
219
WAVE LAUNCHER
PLASMA
a
PLASMA
b
TUBE
WAVE LAUNCHER
PLASMA
c
WAVE LAUNCHER REACTION CHAMBER
d GAS INLET _TO PUMP
AFTERGLOW PLASMA
Figure 15. Examplesof vesselsused in SW plasmasources: (a) straight cylindrical tube, (b) symmetric T-tube, (c) tapered tube, and (d) reactionchamber using an afterglowplasma.l''l
220 High Density Plasma Sources
4.0
A FAMILY OF EFFICIENT SW LAUNCHERS FOR SUSTAINING PLASMA COLUMNS
Various devices, some ofthem quite ingenious, were used in the 60's for launching surface waves over positive column plasmas as a diagnostic means, mainly to determine electron density (see Ref. 11 for a review). These nonionizing waves required HF power ofthe order of 100 mW; little effort was paid to come up with an efficient launcher whereas mode selection was deemed important. Designing a SW launcher for sustaining a plasma column implies a different approach because: 1. The launcher must be efficient. Not only HF power is costly but most of all, reflected power and power losses in the field applicator and impedance matching network can damage components and yield a non-reproducible plasma 2. The azimuthal symmetry of the launched wave is almost independent of the azimuthal configuration of the field applicator; t it is essentiallydeterminedby the discharge stability criterion expressed by the jR product (Sec. 2.2). Nonetheless, a priori, the launching efficiency is maximum when the allowed (in terms of the jR product) SW mode is excited with the corresponding mode launcher 3. The gap impedance Zg depends on the discharge conditions, which thus act on the plasma source impedance. Thus, for stable operation with respect to changes in discharge conditions, the impedance of the plasma source seen at the generator input must not reflect these changes too strongly. This is mainly a matter of characteristic impedance ~ and matching network configuration (see Sees. 2.1 and 4.3, respectively) 4. Significant HF radiation can flow into the surroundings, especially when the plasma source is not properly operated: improper use includes tube diameter not fitting closely the aperture of the launcher, azimuthal symmetry of the aperture not corresponding to the excited wave mode, discontinuities in
t The fact that a field applicator with an azimuthally symmetric aperture can excite a m = 1mode SW discharge can be explained by noting that: (i) all wave modes are present at the aperture because of the inherent electromagnetic discontinuity; (ii) the HF power feeding of the aperture of the SW launchers that we use is not azimuthally symmetric.I'f this reinforces the available amplitude of Iml ~ 1 modes at the aperture.
Surface Wave Plasma Sources
221
the discharge tube configuration or dimensions. On account of such radiation in the room, it may be required to enclose the plasma source with an adequate electromagnetic shielding to maintain radiation leakage below the maximum permissible exposure (see Sec. 5). To avoid interference with communication and broadcasting systems, only ISM approved frequencies t should be used . We have developed a whole family of efficient SW launchers such that their individual domain ofoperating frequencies overlap to cover the 10 MHz-I0 GHz range. One can thus elect the appropriate launcher according to the frequency required to optimize a given plasma process or to the frequency of available HF generators. The field shaping function of these launchers is provided by a circular gap (Fig. 12), and, essentially, they are intended to be m = 0 wave launchers. Their efficiency is optimized by impedance tuning means, the type ofwhich depends on the value off At the lowest frequencies, our matching network consists oflumped elements in the form of standard inductances, L, and capacitances, C. With increasing frequency, we tum to distributed reactances, first as obtained from coaxial line elements, then as a mix ofcoaxial and waveguide line components. The power handling capability of these launchers depends on both the field applicator (mainly gap arcing limitation) and the matching network components. With the lumped LC match box that we have tested, which uses air capacitors but water-cooled inductance coils, it is limited to approximately 1 kW. In the mid-frequency range, when using standard coaxial cables that mate with N or HN type connectors, the power limitation comes from losses in the dielectric material which increase withf[35] Finally, at GHz frequencies, waveguides may be used, which have larger power handling capability, to supply power to the launchers. For instance, at 2.45 GHz, the power limit with common coaxial cables is approximately 400-500 W,f35] while waveguide supplied systems can support many kW. We shall now describe three wave launchers of the aforementioned family as typical examples: the LC Ro-box (lumped element impedance network), the surfatron (a coaxial structure fed by a coaxial cable) and the waveguide-surfatron (a mixed coaxial-waveguide structure fed by a waveguide). They should suffice to evidence the essential features of SW plasma sources operating over different frequency domains. For more t World wide frequencies designated for industrial, scientific and medical (ISM) applications above I MHz are: 6.78,13.56,27.12,40.68 MHz and 2.45,5.80 GHz, ... )4IJ
222 High Density Plasma Sources details on these launchers or for a description of launchers such as the stub Ro-box[5] and the sur!aguide,[47j the reader is referred to the original publications.
4.1
LC Ro-box
This launcher operates efficiently between approximately 10 and 100 MHz, which is the lowest frequency band of our SW plasma sources. Because of this low frequency, the electron density under traveling wave conditions is the lowest, typically 108_1010 electrons/em' for 0.02
t This remark applies to all gap-type SW launchers: typical thickness of the front plate is 0.2-0.5 mm.
tt At higher frequencies, a high intensity field at the launching gap can be obtained with no rear gap, because the total length is + 4,(see Sec. 4.2) of the intrinsic coaxial line ofthe launcher is approximately 1..0 /4 where 1..0 is the free-space wavelength.
Surface Wave Plasma Sources
223
N-TYPE CONNECTOR
ALUMINIUM
/-~~~
BRASS TEFLON
Figure 16. Example of a Ro-box field applicator to be used with an LC matching network: D) = 8 nun, D 2 = 50 nun; launching gap width GL = 2 nun, field-arresting gap width ~ = 3 rnm.Pl
The equivalent circuit of this field applicator (Fig. 17a) is composed of an inductance L b , related mainly to the wire connecting its inner tube (sleeve) with the central pin of the coaxial cable connector, and a capacitance Cb that takes into account the energy stored in the electric field within the field applicator. Impedance Matching Network. HF power is supplied to the field applicator via a matching network represented as a two-port network in Fig. 17a. Impedance matching can generally be achieved with two independently variable tuning elements. These elements can be arranged as in Fig. 17b (configuration I) or as in Fig. 17c (configuration II»)42) The parameter Z~ is the impedance seen at the input connector (or in general, at a given reference plane; note the use of the mark' for this purpose) due to the gap impedance Zg combined with the impedances related to L b and C b . Equivalent Circuit. The normalized input impedances ZL (or admittance YL) of the plasma source for the above two matching network configurations can then be calculated.
224 High Density Plasma Sources
LAUNCHER
INPUT PLANE
.
: ZL
. .:,------...,
o
:---
:-GAP
o o o o o
o
LC
a
NETWORK
POWER GENERATOR, FEED LINE
IMPEDANCE MATCHING NETWORK
FIELD :APPLICATOR 0 0 0 0 0 0 0 0
·· ··
Zo
0
Xl
z:9
b
z'9
c
Figure 17. (a) Equivalent circuit of a SW plasma source using an LC Ro-box; (b) configuration I (high impedance plasma source) and (c) configuration II (low impedance plasma source) of the LC tuning elements in the impedance matching network.ls-l
Surface Wave Plasma Sources Configuration I, (X2 = 0, i.e., Z22 - Z12 =
225
°
in Fig. 14):
Eq. (19)
where, for example, b ~ = bg + jwCb , assuming that the influence of L b is negligible at low frequencies (recall from Sec. 3.3 that ZglZo = rg + jXg and ZOIZg = gg + j bg, and Xi = X/Zo)· Configuration II, (Xl
°
= 0, i.e., Z11 - Z12 = in Fig. 14):
Eq. (20)
Frequency Tuning Response. The Ro-box field applicator module can be utilized with two types of matching networks: an LC network, yielding the LC Ro-box system described above, or the HF power can be fed to the aperture through a tunable capacitive coupler (as in a surfatron, Sec. 4.2) and further tuning provided by a coaxial stub, hence the name stub Robox in this case.Pl The Ro-box field applicator module operates over a very large range of frequency. Its upper frequency limit increases with decreasing tube diameter. For example, with R = 15 mm, it is approximately 1200 MHz while with R = 4 mm, it goes up to 2.45 GHz; when employing this field applicator with an LC matching network, it is not efficient to use it above 200 MHz. As for the lower frequency limit, it is around 10 MHz when using air coils as inductances (for still lower frequencies, ferrite loaded coils should be used). Figure 18 shows the HF power reflected at the launcher input at constant incident power as a function of frequency, the so-ealledfrequency characteristic, for an LC Ro-box plasma source. It uses configuration II for the matching network at two fixed values of X 2 while X 3 is adjusted at each frequency for minimum reflected power. We observe that: (i) for a given X 2 , there exists a frequency at which the system can be perfectly matched; (ii) the lower the frequency at which zero reflected power is
226 High Density Plasma Sources required, the sharper is the tuning process. Recall that, as a rule, the broader the tuning, the less affected is the power matching with respect to changes in the discharge conditions and hence the more stable is the discharge. One may find experimentally that employing the matching configuration I instead ofIl (i.e., reversing input and output ofthe matching network) facilitates tuning. To understand this result, one has to realize that configurations I and II yield a perfect match (PR = 0) for two different domains of Z~: configuration I requires S I ("high impedance" plasma source), while configuration II demands r~ s 1 ("low impedance" plasma source). These two conditions are not compatible in general, except when r~ < < x~ and < < in which case either structure can be used to match the plasma source. t An example ofpractical realization ofan LC Ro-box plasma source is given in Sec. 5.2.
s;
b;,
s;
40 Argon: 100 mtorr
,.. :>!! 0
30
R
+ x~l)
~
w
:: 0 0-
= 15mm
20
0
x~) o
0
w .....
0
X(l) (2) < 2
w
.~
w
10
~
0 35
40
45
50
FREQUENCY (MHz) Figure 18. Observed frequency characteristics for an LC Ro-box plasma source. The matching network uses configuration IT (Fig. 17c), at two fixed values of A] while A; is adjusted at each frequency for minimum reflected power. The applicator dimensions are (refer to Fig. 16): D J = 30 mm, D2 = 75 mm, and its axial length is 65 mm.H
t Although as a rule rg andxg are smaller than unity, the corresponding impedance values seen at the plasma source input (denoted by the mark ") can be made "high" or "low" depending on the actual configuration ofthe wave launcher (see further in relation with Fig. 25).
Surface Wave Plasma Sources 4.2
227
Surfatron
This was the first SW launcher ofthe present family to be developedl'"! and it is still the most widely known. The term surfatron plasma is even used by some authors to designate SW sustained plasmas. It is best suited for frequencies above 500 MHz. Its overall axial length being usually more than A0I8 (Ao is the free-space wavelength), it is therefore less cumbersome to use Ro-box systems at lower frequencies. Its upper frequency limit can be as high as 2.45 GHz provided R ~ 4 mm (this is the case for the surfatron described in Sec. 5.1). The surfatron is an integrated wave launcher in the sense that a single unit performs both the field shaping and impedance matching functions. Figure 19 shows schematically a cross-section of this device in an axial plane. In terms ofHF circuit, it is a coaxial line ofcharacteristic impedance Zos and length ts + t b , terminated by a short circuit at one end and by a circular gap at the other, and supplied from a coaxial feed line via a capacitive coupler.
COAXIAL CABLE CONNECTOR "<,
Zo
INPUT PLANE
SPRING CONTACT
PLUNGJ
CAPACITIVE
LAUNCHING GAP
COUPLER'\.
~~1RfRo ............................................................................ , :::Ll.
-j
les
~ts
,
.~.
!
<, TOBE WAll
tb-1
Figure 19. Axial cross-section of a surfatron showing the field shaping structure (the coaxial line of length (b terminated by the launching gap) and the intrinsic tuning means (capacitive coupler and plunger) (after Ref. 38).
228 High Density Plasma Sources Field Shaping. SW excitation is provided by a circular gap, as in a Ro-box. Impedance Matching. HF power is supplied to the launcher via a commercial coaxial feed line terminated by an adjustable capacitive coupler (details in Sec. 5.1), which constitutes one tuning means. The second tuning means is the plunger position, which defines the length ts of the shortcircuited intrinsic coaxial line with respect to the coupler axis (Fig. 19); when limiting operation of the surfatron to a narrow frequency band, low (but generally nonzero) values of PRJ!} can nonetheless be secured with a fixed ts (see below with Fig. 22), yielding a lower cost and easier to build device. Equivalent Circuit. Figure 20a shows the equivalent circuit of the surfatron. (In this circuit and in the next one, the distributed elements are represented by bold lines). This circuit can be reduced, as shown in Fig. 20b, to that ofconfiguration I ofthe LC Ro-box (Fig. 17b). Thus, the input impedance of the surfatron is given by Eq. (19) with Eq. (21) Eq. (22) where Z~ , the gap impedance at the reference plane, is here taken at the input plane (see Fig. 19). Varying t s can be used to determine the real part of the input impedance (although it affects both parts) while varying C; through the insertion depth of the coupler (Fig. 19) affects only its imaginary part. Tuning and Frequency Characteristics. For a given rL , PR is minimum when xL = 0 (Sec. 3.3). This condition can be met by adjusting the coupler's capacitance Ce , provided the associated inductance L, is large enough. [38] An important feature which can be seen from Eqs. (19) and (21) is that, for given discharge conditions, there is only one setting of the capacitive coupler that yields XL = 0; tuning is thus simple and unambiguous. The surfatron should always be operated with XL = O. Assuming that the surfatron's coupler is always set such that XL = 0, we refer to the dependence of PR/p/ upon the plunger position ts (at constant frequency) and upon the frequency ofoperation (at constant ts ) as the tuning characteristics and the frequency characteristics of the surfatron, respectively. Examples ofthese characteristic curves are shown in Figs. 21 and 22, respectively. The existence of one or two zeroes of power means that s; s 1.£38] Note the large range of low (s 10%) reflected power in
Surface Wave Plasma Sources
229
terms of either ts or f, which ensures stability of the discharge. However, whenfis increased to higher values, the tuning characteristics narrow; past a certain value fm' one can no longer find a ts value yielding zero reflected power,[38] andfm is then considered as the maximum frequency ofoperation of the surfatron; above fm' the minimum reflected power that one can achieve increases continuously with f.
·: :,
,,, ,
··
LAUNCHER INPUT PLANE
: - COUPLER AXIS
.:-GAP a
POWER GENERATOR, FEED LINE
Zo
b
z'9
Figure 20. (a) Equivalent circuit of the surfatron (distributed elements are represented by bold lines); (b) reduced equivalent circuit showing the tuning elements and the gap impedance at the coupler's axis (matching configuration 1).142 ]
230 High Density Plasma Sources
f
CALC. (g ~
-
15
= 950 MHz
o
MEAS.
~
0 ......,
~
w
3:
-C
10
0 0a
I j
:-I
W
=0.66, b~ = 1.04 )
t-
~~~ 33
I I I
i I
J,--J $ i
I
65
I~
i
9
r-
O
W .....
u-
w
5
~
o 20
40
60
POSITION OF PLUNGER
80
t s (mm )
Figure 21. Measured and calculated tuning characteristics of the surfatron when sustaining a plasma column. The theoretical curve is obtained from the equivalent circuit of the surfatron (Fig. 20a), which yields the values of g~ and b~ from the two ts positions at which we observe zero reflected power. The insert shows the approximate dimensions of the launcher parts. [38J
Surface Wave Plasma Sources
--
231
20
:0.!! l :l'
w 15
3:
0 Q.
a
w .... U w .... u..
10
w
l:l'
5
600
800
1000
1200
FREQUENCY (MHz) Figure 22. Measured and calculated frequency characteristics of the surfatron when sustaining a plasma column. Fitting from the equivalent circuit equation yields g~ = 0.66 and b~ = 1.04. Launcher dimensions as in Fig. 2I.!38]
4.3
Waveguide Surfatron
This waveguide-based device should not be used much below one GHz because the large cross-section dimensions of any waveguide operating below that frequency would be cumbersome even in a research laboratory and also because the waveguide hardware for such low frequencies is costly and not readily available. This SW launcher is particularly recommended for operation with large tube diameters! and with high microwave power levels (6 kW testedj.F"
t Large diameter means here approaching or somewhat exceeding the free-space wavelength; at 2.45 GHz, Ao '" 122 mm. Indeed, most of the microwave-produced plasma columns that we are aware of at this frequency are less than 20 mm in diameter. We have achieved an 80-mm diameter plasma with a WR-430 waveguide (wide wall width 109 mm); still larger diameter plasmas can be realized at this frequency but with an hybrid version of the waveguide surfatron (Sec. 5.3).
232 High Density Plasma Sources The structure ofthis launcher consists of waveguide and coaxial line elements, as shown in Fig. 23. Microwave power is supplied by the generator to a rectangular waveguide section that is terminated, past the launching aperture, by a movable short circuit in the form of a waveguide plunger. A coaxial line section is attached perpendicularly to the wide wall of the waveguide, and its inner conductor extends into the waveguide as a sleeve around the discharge tube, forming a circular launching gap in the immediate vicinity ofthe opposite wall. The other end ofthis coaxial line is terminated by a movable short circuit (a coaxial plunger) located at a distance to from the waveguide wall (Fig. 23b).
ROD FOR MOVING COAXIAL PLUNGER
STANDARD RECTANGULAR WAVEGUIDE THINNER WALL _~--------,-;~ POWER INPUT _
WAVEGUIDE MOVABLE SHORT
a
Figure 23. (a) Overall view ofthe waveguide surfatron; (b) simplified sketch showing its internal design (after Ref. 43). (Cont'd next page.)
Surface Wave Plasma Sources
COAXIAL
COAXIAL
PLUNGER
SECTION
WAVEGUIDE SECTION
POWER INPUT
7
METAL SLEEVE
233
WAVEGUIDE PLUNGER
LAUNCHING[-L GAP
b
/ DISCHARGE TUBE
2 RO
Figure 23. (Cont'd)
Field Shaping. SW excitation is provided by a circular gap, as in Fig. 12. The gap width is usually fixed at 3-4 nun (or slightly larger to avoid arcing when operating at the kW power level). The waveguide wall around the aperture is thinned down from the outside to 0.5 nun over a circular area centered on the aperture and having a diameter close to the waveguide width (Fig. 23a). Impedance Matching. The coaxial and waveguide elements of the launcher structure serve as a wave mode converter (from the TE IO mode in the rectangular waveguide to the TEM mode in the coaxial section terminated by the field shaping structure) and as an impedance transformer. Such an impedance matching system is particularly suitable to match a low impedance load on the coaxial side of it to the characteristic impedance of the feed waveguide. Tuning the waveguide plunger position tw (Fig. 23b) for minimum reflected power is equivalent to adjusting C; with the capacitive coupler in a surfatron (it brings XL to zero) while the coaxial plunger position to plays the same role as that of ts in a surfatron, hence the name waveguide surfatron.
234 High Density Plasma Sources Equivalent Circuit. When the outer diameter of the coaxial section is small compared with the width of the waveguide, a simple equivalent circuit ofthe launcher can be constructed: all the impedances can be related to a single reference plane, coincident with the axis ofthe coaxial section. [43] Figure 24a shows such a circuit; the two distributed elements represent the short circuited coaxial and waveguide lines, of characteristic impedances Zoe and Zo and adjustable lengths tc and tw respectively, and Z, accounts for the conducting sleeve going across the waveguide. This equivalent circuit can be reduced to the matching configuration II (Fig. 17c), as shown in Fig. Then in Eq. (20) for YL, we have 24b where Z; = Zg +
z;
Eq. (23)
Eq. (24)
REFERENCE :--- ZL PLANE -: ,------, SHORT CIRCUITED COAXIAL LINE
POWER GENERATOR, FEED GUIDE
Zo
. S~Z~~~J~~U~;~~ ~ :
-,
SLEEVE
,
C?x,~z, . , ,,
b
''
Figure 24. (a) Equivalent circuit of the waveguide surfatron; (b) equivalent circuit reduced to the tuning elements and gap impedance seen at the coupler axis: matching network configuration II. The reference plane is perpendicular to the waveguide axis and runs along the tube axis.[42]
Surface Wave Plasma Sources
235
Tuning Characteristic. It represents here the dependence of PRIPJ on t ~ with tw being always tuned for minimum reflected power. Figure 25 shows a set ofcalculated tuning characteristics for the waveguide surfatron, illustrating the influence of Z~ = r~ +jx~, the gap impedance seen at the reference plane and including Z9' As a rule, we experimentally get values of r~ S 0.01 but it is possible to implement a section ofa coaxial line between the gap and the waveguide wall that acts as an impedance transformer.If-l Then, one can obtain larger values of r~, yielding flatter tuning characteristics as shown in Fig. 25, thereby achieving a plasma source much less dependent on discharge conditions. As a rule, some HF power is lost in such transformers.
'00
z
! ! ~
80
'00
r~_05
~
~ ~ ~
eo so
»: .32'
80
!
80
<1.15
loll -c
t
z
~.o
<, ~.05
005
0.1$
025
80
r~.2
~.o
80
" )
20
.32'
<1.15
~.05
10''0
r~ =0.5
r~,",o.s
x~ = ·0.5
~.O
0,15
02'
10''0
60
o
OJ
et Ii'
005
\ 20
"'-
.-/\1 z=-"--':0'7,5--::,;::--~----o<:::""'...lLJ 0.05 0.0$ 0.15 0,25
) 0.15
0-25
10''0
Figure 25. Set of calculated tuning characteristics for the waveguide surfatron, showing the influence of the real and imaginary parts of the gap impedance seen at the reference plane (Fig. 24). Clearly there exist values of Z~ = r~ +jX~ that ensure low reflected power at the waveguide surfatron input over a large portion of the tuning characteristic.I-"
5.0
TYPICAL EXPERIMENTAL ARRANGEMENTS
In the previous sections, we have presented the theory and general design principles of SW plasma sources. This section provides a detailed practical description of three kinds of SW plasma sources as examples of how to construct and operate them correctly.
236 High Density Plasma Sources Caution. Personnel must be aware that exposure to microwave energy radiated from the wave launcher and the plasma column as well as from the HF generator can be detrimental to their health. According to IEEE, [44] for "cognizant individuals" (notion ofcontrolled environmentlr'l), the maximum permissible exposure in the HF range of interest to us is as given in Table 2. To maintain RF and microwave radiations below the maximum permissible level, the plasma source should be periodically inspected and checked with a calibrated HF radiation monitor. One should also keep up with publications on the hazards of RF and microwave radiation.
Table 2. Maximum Permissible Exposure in a Controlled Environment. I44]
5.1
Frequency Range (MHz)
Power Density (E field, H field) (mW/cm 2)
3-30
900/f2, 10000/f2
30-100
1.0, 10000/f2
100-300
1.0
300-3000
1/300
Atmospheric Pressure Microwave Discharges with a Surfatron
The device presented is widely spread among analytical chemists dealing with atomic spectrometry. The sample to be analyzed is sent through an argon or helium plasma in order to dissociate its molecules, then excite and ionize the resulting atoms and finally detect these atoms through optical emission spectroscopy or mass spectrometry.l45]-[63] Recall from Sec. 2.3 that SW discharges at atmospheric pressure are stable and reproducible provided that they are achieved in a tube with a maximum inner diameter of 6-8 mm. The surfatron described below is intended for operation at the fixed ISM frequency of 2.45 GHz; a movable plunger is required because the impedance matching conditions for argon and helium are significantly different at powers below 100-200 W (this is related to variations in the resistance ~, Sec. 2.1).
Surface Wave Plasma Sources
237
Description of the Wave Launcher. Figure 26 shows two crosssectional drawings ofthe device developed by the Groupe de Physique des Plasmas at Universite de Montreal. The numbers refer to the following elements: (1) Wave launching interstice (gap)-typically 2 mm wide. (2) Front plate ofthe field shaping section-thickness: 0.5 mm. (3) Inner conducting tube (sleeve)-made of aluminium, it is anodized (Al Z03) on its non-threaded portion to reduce the possibility of its arcing with the coupler's plate (4). The central part ofthe front plate (2) is also anodized for similar reasons. (4) Plate of the capacitive coupler-round copper plate with a curvature equal to the radius of the outside diameter of the sleeve plus I or 2 mm; the coupler's axis is at 10 mm from the front plate (2). (5) Spring contacts for the capacitive coupler-it ensures that the semirigid coaxial cable constituting the coupler's feed is in good electrical contact with the body ofthe surfatron. (6) Knurled wheel to move the coupler's assembly radially. (7) Chimney preventing the coupler's semirigid cable from being stressed or bent, which would interfere with a swift and precise radial displacement of the coupler assembly. (8) Guide-pin to prevent the semirigid coaxial cable from rotating when moving the coupler's plate radially. (9) Clamping nut holding the coupler semirigid cable in placeit allows a coarse radial adjustment of the coupler's plate position with respect to the surfatron sleeve. In this way, the capacitive coupler can be used on surfatrons of different body diameters.
(10) Semirigid cable-0.250" (6.35 mm) or 0.325" (8.25 mm). (11) N-type (female) connector to mate with the microwave coaxial cable feed. (12) Strip of metal-it serves together with screw (13) to pry the threadings in the surfatron body in order to obtain a better electrical contact, avoiding arcing in the threaded portion when operating at powers> 100 watts.
238 High Density Plasma Sources (13) Butterfly screw used with (12). (14) Discharge tube (fused silica)-minimum inner diameter tested: 0.5 mm, wall thickness tested: 0.5 to 4 mm. For a watercooled small bore tube, see Ref 63. (15) Wheel for adjusting the gap width (typically 2 mm). (16) Wheel for adjusting the plunger axial position fixing the length (s' (17) Surfatron main body. (18) Compressed air input for external cooling of the discharge tube-dry air must be used to avoid damaging the threadings. (19) Ring holding the gap thin plate (2) in position. Operating Instructions. The discharge tube must be a low-loss high temperature-resistant dielectric such as fused silica or high purity ceramic. It must fit as closely as possible the inner diameter of the sleeve (3); for example, with a 6.5 mm i.d. sleeve, we recommend using a 6 mm o.d. discharge tube. It is advisable to always have dry, oil-free compressed air flowing through (18) to provide external cooling of the discharge tube when it encloses an atmospheric pressure discharge. Water cooling ofthe surfatron body is required in the present case when operating above 150 watts. Striking the Plasma for the First Time. When initiating operation of the plasma source at atmospheric pressure, one should begin with argon (or any other easy to ionize gas) and set its flow in the range 300-600 seem (mild laminar flow). The coupler plate (4) radial position is initially adjusted with the knurled wheel (6) so it barely touches the sleeve, which means it rests approximately at 0.5-1 mm from it. The plunger is positioned with (16) so that (s :::::: 6-10 mm. The microwave generator, connected to (11) via an appropriate coaxial cable, [35] is switched on at approximately 100 W while either bringing a Tesla coil (spark generator) in front of the open end of the discharge tube or introducing into it a small wire (which will glow), to provide initial ionization at the gap level. Once the discharge is on, we adjust the capacitive coupler with the knurled wheel (6) for maximum plasma length. Then, we tune the plunger with (16) looking again for maximum plasma length. This procedure is repeated until there are no further improvements in the tuning. As a rule, one should arrive at a PRJP/ value less than 10%, as shown in Fig. 27.
~
11
D ~ ~
~
St,
~
~ ~
~
~l:::l
19
Physique des Plasmas - Universite de Montreal
I o
I 1
I 2
I 3
~
I
I
;::
4
Scm
~
Figure 26. Cross-sectional drawings of a surfatron intended for operation at 2.45 GHz with small bore discharge tubes. This device is well-suited for stable discharges at atmospheric pressures in gases as different as argon, hydrogen, and helium.
~
~
'C
240 High Density Plasma Sources
+ 4.5 mm diameter sleeve ;
40
*
6.5 mm diameter sleeve
Ill:
w
:1:
30
0
a.. C
w .... ow
20
w
10
.......
Ill:
2
4
6
8
10
12
POSITION OF PLUNGER,
14
ts
16
18
20
(mm)
Figure 27. Tuning characteristics of the surfatron described in Fig. 26 for a discharge in argon at atmospheric pressure and with 100 watts of incident power at 2.45 GHz. The two curves are for 4 and 6 mm o.d. tubes (sleeve of 4.5 and 6.5 mm i.d respectively); the gap width is 2 mm.
Striking the Plasma with Hard-to-Ionize Gases such as Helium or Nitrogen. Once the surfatron has been tuned for argon, we can use one of the two following procedures to strike a hard-to-ionize gas without damaging the surfatron and the microwave generator: 1. Mixing of the hard-to-ionize gas with argon-this gas is initially mixed with a large flow ofargon and the concentration of the latter is gradually reduced as the coupler and plunger are continuously tuned for minimum reflected power. Tuning begins to be really affected when almost no argon is flowing 2. Striking the discharge directly with the hard gas-a circulator must then be inserted between the HF generator and the surfatron to avoid damaging the feed cable and the generator. The plunger is initially set for a low power argon discharge, namely at 30-50 watts of incident power. Then, the hard-toionize gas alone is sent at a flow rate of 300-600 seem with 150-200 W of incident power; the coupler is tuned while activating the Tesla coil at the open end ofthe tube so that a stream of ionized gas reaches the gap. Faraday Cage. A small diameter Faraday cage can be attached to the front plate ring (19). It should be long enough to enclose not only the plasma column but also the dielectric tube. Otherwise, microwave radiation may be directed along the discharge tube outside the cage.
Surface Wave Plasma Sources 5.2
241
A Broadband (10-100 MHz) RF Plasma Source with an LC Ro-Box
The Ro-box field applicator is simple to construct: dimensions are not critical and there are no movable parts. The main difficulty arises with the LC impedance matching network which should provide low reflected power, little heating ofthe matching network and reproducible tuning. The matching network described below was found to be efficient between 10 and 100 MHz in argon and helium discharges: (i) at reduced pressure (0.01 S psi torr) in a 26 mm i.d., 30 mm o.d. Pyrex tube; (it) at atmospheric pressure with 2, 4, and 6 mm i.d. fused silica tubes. Ro-Box Field Applicator. Dimensions are given with reference to Fig. 16. For the small diameter discharge tube, these are D 1 = 9 mm, D 2 = 30 mm and GA = 5 mm while for the 30 mm o.d. tube, D 1 = 31.5 mm, D 2 = 77 mm and GA = 6 mm. The launching gap front plate is 0.5 mm thick. As a rule, the various parts ofthe applicator are made of aluminium. AN-type (HN for higher power) female bulkhead connector is used and mounted as shown in Fig. 16. LC Matching Network. Figure 28a shows the circuit used; it corresponds to network matching configuration II in Fig. 17. The components are: C/ Continuously variablecapacitor(commercial), 32-241 pF (4500 V breakdown voltage). Ci Continuously variable capacitor (commercial), 13-74 pF (4500 V breakdown voltage). L / Three-taps inductance (laboratory made), approximately 110 nH/tum. It consists ofthree turns nominally of 1" (25.4 mm) diameter made with a II4" (6.3 mm) o.d. copper tubing. L 2: Continuously variable inductance (commercial), 4.4 mH with 12 turns.
All these components lay in a metallic box and are connected together by copper strips-I/l6" (1.6 mm) thick, II2" (12.7 mm) wide. No forced air and water cooling was used; the limit of input power was 150 W at reduced pressure while, at atmospheric pressure, with helium, it was 100 W. We also built matching networks that used water cooling of the inductances and worked up to 500 W. We initially tried employing an amateur radio matching network, which is shown in Fig. 28b. We could not match the plasma source satisfactorily with it; clearly this matching network does not mate correctly with the low impedances presented by the present Ro-box plasma source.
242 High Density Plasma Sources
L2 af I I I I I I I
,. ,, ,
c1 L]
C2
Z'9
I I
Z'9
Figure 28. (a) Elements and configuration (II in Fig. I7c) of the LC matching network of the Ro-box in the range 10-100 MHz (see text for actual values); (b) elements and configuration of the amateur radio matching network tested unsuccessfully with the Robox; note that it cannot be reduced to configuration I or II.
Operating Procedure. The HF power feeding arrangement includes the components shown in Fig. 11. When no circulator is available, one may need to replace it with a high power 3 dB attenuator in the feed line, which reduces the interaction between the plasma source and the generator. Before striking the plasma, one sets C j so P j is maximized on the directional power measuring line. Then, the discharge is struck, and C 2 and L 2 adjusted for maximum plasma length, and C, retuned until a maximum plasma length is obtained with a satisfactory reflected power level.
Surface Wave Plasma Sources 5.3
243
A Millitorr and Sub-Millitorr Magnetized Plasma Source Sustained by Surface Waves
As indicated in Sec. 2.4, when applying a static magnetic field of the appropriate intensity, it is possible to achieve a SW discharge at gas pressures as low as 0.1 mtorr in argon at 2.45 GHz. We present below the magnetized SW sustained plasma source and the associated reactor that we have been developing for anisotropic etching experiments. Description of the System. The wave launcher employed is an unconventional version of the waveguide surfatron of Sec. 4.3 because of its "overgrown" coaxial section. The reason for using such a variant is that there is no standard rectangular waveguide for connecting to a microwave generator at 2.45 GHz that would have a wide wall large enough to accommodate a tube of 150 mm o.d., as required by the present reactor design. The launching gap section of this wave launcher is shown in Fig. 29; it is similar to that ofa surfatron. Microwave power is supplied via a WR-284 waveguide, perpendicularly to the field applicator body, close to the gap as shown in Fig. 29, while a movable waveguide plunger is located opposite to it. As shown in Fig. 30, the fused silica discharge tube extends a few centimeters past the wave launching gap before entering a larger diameter (280 mm), 700 mm long steel chamber (reactor) where the substrates to be processed are placed. Both the SW plasma source and the reactor are submitted to a uniform (12 coils), axially directed static magnetic field, the intensity of which can attain 1400 gauss (0.14 T). Operating Conditions. The coaxial and waveguide plungers are set so that the reflected power is near zero and the plasma viewed axially from the reactor end is as homogeneous as possible azimuthally. This requires some minimum microwave power, typically 300-400 W for argon. The plasma glow has then a donut shape, i.e., its luminosity is maximum close to the discharge tube periphery. Such a radial profile of luminosity has been reported earlier with classical ECR discharges and is also typical of large diameter SW sustained plasmas in absence ofmagnetic field, because of the increase of the average electron energy with radius (Sec. 2.3).
244 High Density Plasma Sources
ISIDE· VIEwl
I~I~ ~
L
~
'----r:1l'7T---=r-::----=-.....,..!.r-
~
LAUNCHING GAP
ANODIZ;;-{ ROD TO MOVE COAXIAl PLUNGER
IFRONT VIEWI WR-284 SECTION
~
MICROWAVE INPUT
ALUMINIUM
Y/////.
BRASS
,0'/,;'/,;/
~
WR-284 WAVEGUIDE PLUNGER
TEFLON
Figure 29. Field applicator and coaxial tuning system of a SW launcher sustaining plasma with diameters that exceed the width of the largest standard rectangular waveguide at 2.45 GHz. The inner diameter of the applicator sleeve is 154 mm for a 150 mm o.d. discharge tube. This wave launcher uses a waveguide plunger (not shown) as its second tuning means. The waveguide feed and plunger are of the WR-284 type (72 x 34 mm inside dimensions).
12 Solenoids Wave Launcher
Metallic Vessel (280 rnrn LD.)
•
,'£;:~!m;,~"'~:~~~iifrii!~:~r:i:I~~I~·
II .--.
Gas
InJe/~~I~~;m:j: ~ Probe
O62
Source :..
- - - .. Reactor
1200
.,.i
To Pump
.-,
Wafer Holder (water cooled)
..
~
~
~
~
...
~
~
850 r
o
.
25 Axial position (em)
~
80
Figure 30. Sketch of our magnetized SW plasma source and associated reactor for plasma etching. The axially directed static magnetic field is uniform starting from the launching gap up to 600 mm away from it in the reactor.
i
~
t:
a~ ~ tJl
246 High Density Plasma Sources The discharge can be operated in a broad range ofgas pressure. For example, in argon, we have been successful in sustaining plasma from 0.1 mtorr to 20 mtOIT. As noted in Sec. 2.4, magnetized SW discharges have a larger Bo operating domain than conventional ECR systems. More specifically, at the lower end of the pressure range, we find that a minimum B o value is required at the above-mentioned microwave power level; in argon, it is typically 700 gauss. Though we have not tested this possibility, we feel that it should be possible to decrease this minimum Bo value by increasing the wave power. We have also observed that plasma can be sustained at magnetic field intensities higher than for ECR, although above a certain B o value the discharge becomes unstable (above 1 kgauss in argon). Finally, we find that the operating values given above depend somehow on the gas used. Confinement of the Plasma Glow in the Reactor Chamber. Confinement ofthe plasma by the magnetic field can be observed visually in the reactor region: as the plasma enters the reactor, its diameter remains approximately the same as that of the discharge tube, here 15 em.
6.0
CONCLUSION
It is now an accepted fact that given the discharge conditions (nature and pressure ofthe gas, discharge vessel dimensions and material, frequency of operation and, eventually, intensity of the applied static magnetic field) and the HF power density deposited in the plasma, the plasma characteristics (electron energy distribution function, power absorbed per electron, radially averaged electric field intensity) are, to a first approximation, the same in all HF sustained discharges.Pf However, SW discharges have the advantage of the broadest operating conditions in terms of frequency, tube dimensions and shape, and gas pressure; for example they can be utilized over both the RF and microwave domains, which permits one to optimize given processes as a function of frequency (generally through changes in the electron energy distribution function). [8] A further advantage ofSW plasmas is that they are the best modeled HF plasmas, which yields a better insight into their use and operation. Finally, a major future avenue for these discharges is their operation as magnetized plasmas. The first results presented on this subject in this chapter show that these discharges are much more flexible than common ECR systems; their modeling is also highly promising.l'"
Surface Wave Plasma Sources
247
ACKNOWLEDGMENTS The work presented has been achieved thanks to the skilled technical assistance of Messieurs F. Roy, R. Lemay, R. Martel, and 1. E. Samuel. It was funded through the following agencies or programs: the Fonds pour la Formation de Chercheurs et l'Aide a la Recherche (FCAR) of the Quebec government, the France-Quebec scientific program, and the Conseil de Recherches en Sciences Naturelles et en Genie (CRSNG) of Canada.
REFERENCES 1. Tuma, D. R, Rev. Sci. Instrum., 41:1519 (1970) 2. Moisan, M., Beaudry, C., and Leprince, P., Phys. Lett. A, 50:125-126 (1974) 3. Zakrzewski, Z., Moisan, M, Glaude, V. M M, Beaudry, P., Plasma Phys., 19:77-83 (1977)
c., and
Leprince,
4. Chaker, M, and Moisan, M., J. App/. Phys., 57:91-95 (1985) 5. Moisan, M., and Zakrzewski, Z., Rev. Sci. Instrum., 58:1895-1900 (1987) 6. Moisan, M., and Zakrzewski, Z., J. Phys. D: Appl. Phys., 24:1025-1048 (1991) 7. Ricard, A, Barbeau, C., Besner, A, Hubert, J., Margot-Chaker, 1., Moisan, M., and Sauve, G., Can. J. Phys., 66:740-748 (1988) 8. Moisan, M., Barbeau, c., Claude, R, Ferreira, C. M, Margot, J., Paraszczak, 1., Sa, A B., Sauve, G., and Wertheimer, M. R, J. Vac. Sci. Techno/. B, 9:8-25 (1991) 9. Margot, 1., and Moisan, M., in Microwave Excited Plasmas, (M. Moisan and J. Pelletier, eds.), Ch. 8, Elsevier, Amsterdam (1992) 10. Moisan, M., Pantel, R, and Hubert, 1., Contrib. Plasmas Phys., 30:293-314 (1990) 11. Moisan, M, Shivarova, A, and Trivelpiece, A. W.,Plasma Phys., 24:13311400 (1992)
12. Margot, 1., and Moisan, M. ,J. Plasma Phys., 49:357-374 (1993) 13. Margot-Chaker, 1., Moisan, M., Chaker, M, Glaude V. M M, and Sauve, G., presented at the XVIII Int. Conf., Phenomena in Ionized Gases, contributed papers, 4:602-603, Adam Hilger, Bristol (1987) 14. Margot-Chaker, 1., Moisan, M., Chaker, M., Glaude, V. M. M., Lauque, P., Paraszczak, 1., and Sauve, G., J. Appl. Phys., 66:4134--4148 (1989)
248 High Density Plasma Sources 15. Trivelpiece, A. W., Slow-Wave Propagation in Plasma Waveguides, San Francisco Press, San Francisco (1967) 16. Sa, A. B., Ferreira, C. M., Pasquiers, S., Boisse-Laporte, C., Leprince, P., and Marec, J., J. Appl. Phys., 7:4147-4158 (1991) 17. Rakem, Z., Leprince, P., and Maroc, J., Rev. Physique Appliquee, 25: 125130 (1990) 18. Hajlaoui, Y., Pomathiod, L., Margot, J., and Moisan, M., Rev. Sci. Instrum., 62:2671-2678 (1991) 19. Moisan, M., Ferreira, C. M., Hajlaoui, Y., Henry, D., Hubert, J., Pantel, R., Ricard A., and Zakrzewski, Z., Rev. Physique Appliquee, 17:707-727 (1982) 20. Rogers, J, and Asmussen, J., IEEE Trans. Plasma Sci., PS-1O:11-16 (1982) 21. Chaker, M., Moisan, M., and Zakrzewski, Z., Plasma Chem. Plasma Process., 6:79-96 (1986) 22. Aliev, Y. M., Ivanova, K. M., Moisan, M., and Shivarova, A. P., Plasma Sources Sci. Technol., 2:145-152 (1993) 23. Ferreira, C. M., J. Phys. D: Appl. Phys., 16:1673 (1983) 24. Moisan, M., and Zakrzewski, Z., in Microwave Excited Plasmas, (M. Moisan and J. Pelletier, eds.), Ch. 5, Elsevier, Amsterdam (1992) 25. Margot, J., Moisan, M., and Ricard, A., Appl. Spectrosc., 45:260-271 (1991) 26. Kapitza, P. L., Sov. Phys.- JETP, 30:973 (1970) 27. Massey, J. T., and Cannon, S. M., J. Appl. Phys., 36:361-372 (1965) 28. Massey, J. T., J. Appl. Phys., 36:373 (1965) 29. Ricard, A., Moisan, M., and Hubert, J., presented at theXVIlI Int. Conf Phenomena in Ionized Gases, contributed papers, p. 741, Budapest (1985) 30. Rowley, A. T., presented at the 43rd Annual Gaseous Electronics Conf, Abstract K-36, Champaign-Urbana, Illinois (1990) 31. Levy, D., presented atthe 43rdAnnuai Gaseous Electronics Conf, Abstract GB-2, Champaign-Urbana, Illinois (1990) 32. Beneking, c., and Anderer, P., J. Phys. D: Appl. Phys., 25:1470-1482 (1992) 33. Stangeby, P. C. and Daoud, M. A., Can. J. Phys., 53:1443-1448 (1975) 34. Margot, J., Johnston, T. W., and Musil, J., in Microwave Excited Plasmas, (M. Moisan and J. Pelletier, eds.), Ch. 6, Elsevier, Amsterdam (1992) 35. Hubert, 1., Moisan, M., and Zakrzewski, Z., Spectrochim. Acta, 4IB:205215 (1986)
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36. Ferreira, C. M., Moisan, M., and Zakrzewski, Z., in Microwave Excited Plasmas, (M. Moisan and 1. Pelletier, 008.), Ch. 2, Elsevier, Amsterdam (1992) 37. Barlow, H. M., and Brown, 1., Radio Surface-Waves, Clarendon, Oxford (1962) 38. Moisan, M., Zakrzewski, Z., and Pantel, R., J. Phys. D: Appl. Phys. 12:219-237 (1979) 39. Moutoulas, C., Moisan, M., Bertrand, L., Hubert, J., Lachambre, 1. L., and Ricard, A., Appl. Phys. Lett., 46:323-325 (1985) 40. Moisan, M., Zakrzewski, Z., Pantel, R., and Leprince, P., IEEE Trans. Plasma Sci., PS-12:203-214 (1984) 41. Moisan, M. and Pelletier, 1., in Microwave Excited Plasmas, (M. Moisan and 1. Pelletier, eds.), Appendix 1.1, Elsevier, Amsterdam (1992) 42. Zakrzewski, Z., Moisan, M., and Sauve, G., in Microwave Discharges: Fundamentals and Applications, (C. M. Ferreira and M. Moisan, eds.) pp. 117-140, Plenum, New York (1993) 43. Moisan, M., Chaker, M., Zakrzewski, Z., and Paraszczak, 1., J. Phys. E: Sci. Instrum. 20:1356-1361 (1987) 44. IEEE Standard for safety levels with respect to human exposure to radio frequency electromagnetic fields, 3 kHz to 300 GHz, IEEE C95.1-1991 (revision of ANSI C, 95:1-1982), IEEE, New York (1992) 45. Hubert, J., Moisan, M., and Ricard, A., Spectrochim: Acta, 41B:205 (1979) 46. Moisan, M., Pantel, R., Hubert, 1., Bloyet, E., Leprince, P., Marec, 1., and Ricard, A., J. Microwave Power, 14:57 (1979) 47. Hanai, T., Coulombe, S., Moisan, M., and Hubert, 1., in Developments in A tomic Plasma SpectrochemicalAnalysis, (R. Barnes, ed.) London, Heyden (1981) 48. Zander, A., and Hieftje, G. M., Appl. Spectrosc., 35:357 (1981) 49. Abdallah, M. H., Coulombe, S., Merrnet, 1. M., and Hubert, 1., Spectrochim. Acta, 37B:583 (1982) 50. Chevrier, G., Hanai, T., Tran, K. C., and Hubert, 1., Can. J. Chem., 60:898 (1982) 51. Matousek, 1. P., Orr, B. 1., and Selby, M., Prog. Anal. Atom. Spectros., 7:275 (1984) 52. Deruaz, D., and Merrnet, 1. M.,Analysis, 14:707 (1986) 53. Takigawa, Y, Hanai, T., and Hubert, 1., J. High Resol. Chrom., 9:698 (1986) 54. Selby, M., and Hieftje, G. M., Spectrochim. Acta, 42B:285 (1987)
250 High Density Plasma Sources 55. Selby, M., Rezaaiyaan, R., and Hieftje, G. M., Appl. Spectrosc., 41:749 (1987) 56. Riviere, B., Mennet, 1. M., and Deruaz, D., J. Anal. Atom. Spectrosc., 2:705 (1987) 57. Galante, L. J., Selby, M., and Hieftje, G. M., Appl. Spectrosc., 42:559 (1988) 58. Besner, A., Hubert, 1., and Moisan, M., J Anal. Atom. Spectrosc., 3:863 (1988) 59. Lauzon, C., Tran, K. C., and Hubert, 1., J Anal. Atom. Spectrom., 3:901 (1988) 60. Luffer, D. R., Galante, L. J., David, P. A., NovotnyM., and Hieftje, G. M., Anal. Chem., 60:1365 (1988) 61. Galante, L. 1., Selby, M., Luffer, D. R., Hieftje, G. M., and Novotny, M., Anal. Chem., 60:1370 (1988) 62. Sing, R. L. A., Lauzon, C; Tran, K. C., and Hubert, 1., Appl. Spectrosc., 46:430 (1992) 63. Hubert, 1., Sing, R., Boudreau, D., Tran, K. C., Lauzon, C., and Moisan, M., in Microwave Discharges: Fundamentals and Applications, (C. M. Ferreira and M. Moisan, eds.), pp. 509-530, Plenum, New York (1993) 64. Zakrzewski, Z., Moisan, M., and Sauve, G., in Microwave Excited Plasmas, (M. Moisan and J. Pelletier, eds.), Ch. 4, Elsevier, Amsterdam (1992)