Positive and negative feedback of microwave (MW) ECR (electron cyclotron resonance) discharges in cross magnetic field were manipulated by a three-stub coaxial tuner. Unstable ECR discharges in the positive feedback region, such as the self-mode transition between the ordinary (O)-wave mode and extraordinary (X) one, inverse hysteresis, and oscillation, were investigated using a time-resolved MW power meter, high speed camera, and thermocouple. In the positive feedback region, the self-O → X wave mode discharge transition can be driven under the “hot” wall condition, while the counterpart, namely the self-X → O wave mode transition, is observable for the “cold” wall; the inverse hysteresis and oscillation take place at low and moderate gas flow rates, respectively. The mechanism underlying the self-mode transitions and instabilities is the discharge shift due to the gas heating effect. For MW ECR discharges to become stable, as indicated in previous experiments, they should be mismatched in the negative feedback region.
I. INTRODUCTION
Microwave (MW) ECR (electron cyclotron resonance) plasma sources have been applied widely in important application fields such as advanced micro-manufacturing,1–3 powerful ion sources,4,5 and long-life electric thrusters.6–10 However, operation of ECR plasma sources is sometimes intractable due to the presence of discontinuous discharge modes, hysteresis loops, and oscillations.11–22 Existing investigations about theses ECR-discharge instabilities have been concentrated on influencing parameters or factors such as MW power, gas pressure, and gas species.11–14,16,18,20,21 In comparison, works on the effects of impedance matching networks are scanty.15,17,19,22 Minomo et al. suggested that unstable ECR discharges could be stabilized by keeping the reflection coefficient of incident MWs at a nonzero value.15 Asmussen and Mak also found that stable ECR plasmas could be produced by operating in a slight mismatch condition.17 Angra et al. reported that unstable ECR plasmas were highly sensitive to the three-stub-tuner’s configuration.19 As in Refs. 15 and 17, Muguira et al. also confirmed the conclusion that unstable ECR plasmas could be stabilized by manipulating an automatic triple-stub tuner.22 Although an impedance matching network was confirmed to play a stabilizing role in unstable MW ECR discharges, the underlying mechanism has not been explicated. Positive and negative feedback regions were proposed in radio-frequency (RF) inductive and capacitive discharges to explain effects of an impedance matching network on different evolutions of discharge-mode transitions or voltage waveforms.23,24 However, it is unclear that whether the concept of positive and negative feedback regions suggested in RF discharges is also applicable to MW ECR ones.
Of various ECR ion thrusters, the engine with a cross-magnetic-field is attractive due to its higher ion extraction current.6,9 In such a magnetic field configuration, the low electron-density discharge is sustained by ordinary (O) wave ionization in the front of the rod antenna, where the calculated MW electric field is parallel with the static magnetic field.9 In the high electron-density regime, the ionization region shifts to the upstream ECR layer, where the calculated MW electric field has the component perpendicular to the static magnetic field, In this case, the plasma is produced mainly by X-mode waves. Discharges between O and X wave modes are not continuous, but can transit abruptly.9 As in previous unstable ECR-discharges, the O ↔ X wave mode discharge transitions in the cross-magnetic-field are affected by discharge power and gas pressure (or flow rate),9 but the influence of other control parameters or components such as an impedance matching network remains veiled.
In this paper, further investigations are addressed to the effects of an impedance matching network on O ↔ X wave mode ECR discharge transitions under different gas-flow-rate (or pressure) regions and wall conditions. Mechanisms underlying the reversed self-mode transition, inverse hysteresis, and oscillation are discussed.
II. EXPERIMENT APPARATUS
The experimental system for the ECR discharge in the cross-magnetic-field is shown in Fig. 1, details of which were described in Ref. 9. The ECR plasma source was installed in a large vacuum chamber with a diameter of 51.0 cm and a length of 66.0 cm. The chamber was evacuated by a turbo molecular pump (1000 L/S) and a rotary one (14 L/S). The Xe gas flow rate was monitored with a mass flow controller (MFC) and used to control the gas pressure in the small ECR discharge chamber. A MW power generator (MPG) was used to produce the 2.45 GHz MW. The produced MW was injected into the ECR discharge chamber via a MW power meter (MPM, Bird Technologies 7022), a three-stub coaxial tuner (TSCT), a direct current block (DCB) and a molybdenum rod-antenna. The screen grid (SG) and accelerator grid (AG) were not biased to extract ion in discharges of this paper. A K-type thin film thermocouple (not shown in Fig. 1) was stuck on the outside surface of the ECR plasma chamber to measure the wall temperature. The magnetic field in the ECR plasma chamber is the same as that described in Ref. 9. Sizes of the key components of the ECR plasma source are listed in Table I.
Schematic of experimental system. MPG: MW Power Generator, MPM: Microwave Power Meter, TSCT: Three-Stub Coaxial Tuner, DCB: Direct Current Block, SG: Screen Grid, AG: Accelerator Grid. The plasma source and the vacuum chamber are not plotted to scale; the former is smaller than one tenth of the latter.
Schematic of experimental system. MPG: MW Power Generator, MPM: Microwave Power Meter, TSCT: Three-Stub Coaxial Tuner, DCB: Direct Current Block, SG: Screen Grid, AG: Accelerator Grid. The plasma source and the vacuum chamber are not plotted to scale; the former is smaller than one tenth of the latter.
Sizes for key components of plasma source in mm.
Parameter . | Value . |
---|---|
Diameter of rod antenna | 3.0 |
Length of rod antenna | 9.0 |
Gap between rod antenna’s front end and screen grid | 5.0 |
Inner diameter of source chamber | 21.0 |
Length of the source chamber | 14.0 |
Parameter . | Value . |
---|---|
Diameter of rod antenna | 3.0 |
Length of rod antenna | 9.0 |
Gap between rod antenna’s front end and screen grid | 5.0 |
Inner diameter of source chamber | 21.0 |
Length of the source chamber | 14.0 |
To capture dynamic images of oscillating discharges, a high-speed camera (Phantom, V1610) was installed outside the observation window of the large vacuum chamber. The camera was set at a frame rate of 10 000 fps (frames per second) with a pix resolution of 265 × 265 pixels and an exposure time of 99.498 µs. The camera at the above setting could only record 101 033 images over 10.1 s due to the limitation of the camera’s internal storage capacity. The recorded images were converted to 8-bit grayscale (0 to 255 scale) files by the image processing software Image J,25 in order to enable quantitative analysis of investigated discharges.
Shown in Fig. 2 is the schematic of the three-stub coaxial tuner, which consists of three identical coaxial branch-lines connected in parallel with each other. The lengths of the inner conducts underneath the sliding piston (see Fig. 2) can be changed by moving the pistons, thus achieving the good impedance matching. The length li (i = 1, 2, and 3), as denoted in Fig. 2, cannot be measured directly, but determined indirectly by measuring di (i = 1, 2, and 3), namely the length of the inner conductor outside the coaxial branch-line. At the minimal di (denoted as dimin, refer to the illustration for coaxial branch-line 3 in Fig. 2), the sliding piston is moved to the furthest downward position, under which its bottom surface is flushed with that of the external conductor. When dimin is known, li is calculated by di-dimin. For discharges in this paper, only coaxial branch-lines 1 and 2 were tuned, while the sliding piston of coaxial branch-line 3 was fixed at the most downward position, i.e., l3 = 0.0 mm.
Schematic of three-stub coaxial tuner. The red and blue parts denote respectively the sliding pistons and the inner conductors of the coaxial lines. The green arrow denotes the injected MW.
Schematic of three-stub coaxial tuner. The red and blue parts denote respectively the sliding pistons and the inner conductors of the coaxial lines. The green arrow denotes the injected MW.
III. EXPERIMENTAL RESULTS AND DISCUSSION
A. Different feedback regions and discharge transitions
The impedance-matching experiment was first conducted under the conditions that the amplifier gain (Ag) of the MW power generator was kept constant and the Xe gas was not introduced into the ECR plasma chamber, aiming to prevent gas breakdown. The reflected MW power was minimized to a low level by adjusting branch-lines 1 and 2. Simultaneously, the delivered MW power (Pw), calculated as the difference between the incident MW power and the reflected one, achieved its maximum. The minimal reflected MW-power was attained at d2 = 2.38 cm (refer to Fig. 2 for the denotation). This length was also fixed so that only d1 could be adjusted to change Pw. The obtained Pw against d1 is shown in Fig. 3(a), where the curve is asymmetric with respect to the value of d1 at the maximal Pw. The corresponding value of d1 is named as d1m for a concise description. Worth noting is that the asymmetric curve in Fig. 3(a) is not consistent with the symmetric one achieved in the RF regime without discharge (refer to Fig. 4 in Ref. 24). Considering that Fig. 4 in Ref. 24 was plotted against the capacitance of the tuning capacitor in the impedance matching network, Fig. 3(a) is replotted by substituting d1 with Zin1 calculated from Eq. (1). As expected, the obtained curve of Pw vs Xin1 [see Fig. 3(b)] becomes symmetric with respect to the location of the maximal Pw, indicating that the aforementioned two kinds of impedance matching networks have a common feature, regardless of the differences in both hardware structure and operation frequency.
Delivered MW power against d1 (a) and Xin1 (b) in the absence of discharge. d1 is the length of inner conductor outside coaxial branch-line 1 and Xin1 is defined in Eq. (1).
Delivered MW power against d1 (a) and Xin1 (b) in the absence of discharge. d1 is the length of inner conductor outside coaxial branch-line 1 and Xin1 is defined in Eq. (1).
After the discharge was ignited by introducing 0.15 sccm Xe gas, coaxial branch-line 1 was re-adjusted under the fixed d2 and Ag. The measurement of Pw and record of image used in Fig. 4 and Figs. 5–11 were conducted at 5 min after the variation of Pw, in order to eliminate the effect of the irregular change in gas temperature. The obtained curves of Pw vs l1 and Xin1 are shown in Fig. 4. At the presence of plasma, the curve of Pw vs l1 in Fig. 4(a) is generally similar to what is shown in Fig. 3(a), but the curve of Pw vs Xin1 in Fig. 4(b) still remains asymmetric. Specifically, Pw varies with Xin1 more slowly and rapidly at the left and right sides of the maximal Pw, respectively. This feature is also the same as that defined in terms of positive and negative feedback regions in the RF discharges.23,24 The equivalent circuit to explain the feedback effect in MW ECR discharges is not as simple as in the unmagnetized RF cases. In magnetized MW discharges under the cross-magnetic field, there exist EPR (electron plasma resonance) and X-wave ECR,8,9 neither of which can be described by a simple equivalent circuit. Despite of the great discrepancy between MW ECR and RF discharges, the net power against the impedance of the tuning component in the impedance match network displays the similar characteristic. Accordingly, the left and right regions in Fig. 4 can be also regarded as positive and negative feedback regions in our MW ECR discharges.
Delivered MW power against d1 (a) and Xin1 (b) at presence of discharge under a fixed Ag and Xe gas flow rate of 0.15 sccm. Ag is the amplifier gain of the MW power generator. Meanings of d1 and Xin1 are described in the legend of Fig. 3. The dashed lines denote the separatrixes for the positive and negative feedback regions.
Delivered MW power against d1 (a) and Xin1 (b) at presence of discharge under a fixed Ag and Xe gas flow rate of 0.15 sccm. Ag is the amplifier gain of the MW power generator. Meanings of d1 and Xin1 are described in the legend of Fig. 3. The dashed lines denote the separatrixes for the positive and negative feedback regions.
Delivered MW power against d1 at presence of discharge. Ag in this figure is higher than that in Fig. 4. The Xe gas flow rate is 0.15 sccm.
Delivered MW power against d1 at presence of discharge. Ag in this figure is higher than that in Fig. 4. The Xe gas flow rate is 0.15 sccm.
Variation of d1max with Pwmax at the separatrix of negative and positive feedback regions. Pwmax is varied by adjusting Ag at the Xe gas flow rate of 0.15 sccm.
Variation of d1max with Pwmax at the separatrix of negative and positive feedback regions. Pwmax is varied by adjusting Ag at the Xe gas flow rate of 0.15 sccm.
Variation of d1max at the separatrix of negative and positive feedback regions with Xe gas flow rate at a fixed Ag.
Variation of d1max at the separatrix of negative and positive feedback regions with Xe gas flow rate at a fixed Ag.
Total gray value against delivered MW power in discharges operated in positive feedback region. Ag is the same for all the discharges. The ramping-up and -down of Pw are achieved by tuning coaxial branch-line 1, while the other two are fixed. The width of the hysteresis loop is defined to be ΔPwuhl = Pw1 − Pw2, here Pw1 and Pw2 are denoted in (a) and (c).
Total gray value against delivered MW power in discharges operated in positive feedback region. Ag is the same for all the discharges. The ramping-up and -down of Pw are achieved by tuning coaxial branch-line 1, while the other two are fixed. The width of the hysteresis loop is defined to be ΔPwuhl = Pw1 − Pw2, here Pw1 and Pw2 are denoted in (a) and (c).
Variation of width of hysteresis loop (ΔPwhl) with gas flow rate. ΔPwhl is defined to be Pw1-Pw2. Pw1 and Pw2 are denoted in Fig. 8. Ag was unchanged in all the discharges, and the three coaxial branch lines were adjusted and then fixed in the positive feedback region.
Variation of width of hysteresis loop (ΔPwhl) with gas flow rate. ΔPwhl is defined to be Pw1-Pw2. Pw1 and Pw2 are denoted in Fig. 8. Ag was unchanged in all the discharges, and the three coaxial branch lines were adjusted and then fixed in the positive feedback region.
Width of inverse hysteresis-loop (ΔPwhl) against d1 under Xe flow rate of 0.15 sccm.
Width of inverse hysteresis-loop (ΔPwhl) against d1 under Xe flow rate of 0.15 sccm.
Width of normal hysteresis-loop (ΔPwhl) against d1 under Xe flow rate of 0.55 sccm.
Width of normal hysteresis-loop (ΔPwhl) against d1 under Xe flow rate of 0.55 sccm.
In practical operation, d1 is a convenient control-parameter in manipulating the stub tuner. For this reason, we selected di in plotting figures other than Figs. 3 and 4. Shown in Fig. 5 is the curve of Pw vs d1 obtained when Ag is increased above a threshold higher than that in Fig. 4. The curve in the negative feedback region is qualitatively identical to the counterpart in Fig. 4(a), namely the discharge evolves continuously with l1 or Pw. In the positive feedback region of Fig. 5, however, the discharge becomes discontinuously. This discontinuity was attributed in Ref. 9 to the abrupt discharge-transition from the ordinary (O) wave mode existing in the low Pw region to the extraordinary (X) mode appearing in the moderate Pw region. The investigation in Ref. 9 was primarily focused on the effect of gas flow rate (gas pressure), while the influence of impedance matching was unexplored. For discharges in Fig. 5, other external control-parameters are unchanged except the manipulation of the impedance matching network. Therefore, the effect of the impedance matching network is the cause for the continuous and discontinuous discharge-transitions in the negative and positive feedback regions. The O ↔ X wave-mode transitions are intrinsically driven by Pw, and thus can occur in either the positive or the negative feedback region. However, the O ↔ X wave-mode transitions are governed by not only the discharge but also the impedance matching network that is interacting with the internal discharge. To obtain an easy description, the elucidation of the interaction is started below with the simple result in Fig. 3(b), where the interaction does not exist.
The maximal Pw in Fig. 3(b) requires both Xin = −Xs and Rin = Rs, i.e., the impedance of the load equals the conjugate impedance of the power generator. When d1 or Xin is increased in the left or right side of d1m, Pw respectively approaches to and shifts away from its maximum as a result of the deviation from the impedance-matching state for the maximal Pw. The reason for selecting coaxial branch-lines 1 as the tuner is that the reflected power is more sensitive to changing d1. Compared with the Γ-shaped impedance matching network used widely in radio-frequency (RF) plasma sources, the role of coaxial branch-line 1 in Fig. 2 is analogy to that of the tuning capacitor in series with RF plasmas. In the absence of plasmas including ECR ones, discharge circuits are linear. The adjustment of coaxial branch-line 1 results in a significant variation in the reactance of the linear load. In other words, Xin varies greatly when d1 is tuned. With the changing Xin, Pw or Us varies accordingly. Rs and Xs are the electric parameters of the power source and almost constant. From the above, Pw in Eq. (2) is strongly affected by Xin during the tuning of coaxial branch-line 1 in the absence of nonlinear ECR discharges. Consequently, the curve of Pw vs Xin1 in Fig. 3(b) is symmetric with respect to the maximal Pw achieved at Xin = −Xs.
After the discharge is ignited, the understanding about the behaviors of Pw becomes difficult due to the presence of nonlinear ECR plasmas that can be also regarded as a part of the load’s resistance and reactance in Eq. (2). Accordingly, the quantitative analysis about the influence of varying plasma-impedance on Pw is not an easy task.6 For this reason, a qualitative discussion is conducted below.
In both negative and positive feedback regions (see Fig. 4), the variation of the load impedance at the presence of a discharge has two contributions: (1) the direct change in the impedance of the adjusted coaxial branch-line; (2) the induced change in the plasma impedance as a result of the varied Pw. In the negative feedback region, the above two contributions counteract each other, leading to the reduced net variation in Xin1 or Zin1, as evidenced by the lower absolute-slope of the Pw-Xin1 curve. When the variation in Pw is suppressed, the larger change of Pw required by a discontinuous discharge-transition is prohibited, and thus, a continuous discharge-transition is the natural consequence. In the positive feedback region, however, the above situation is inversed: the influence of tuning the coaxial branch-line on Pw is augmented by the simultaneously induced change in the plasma impedance, boosting Pw to vary more steeply with Zin1, as shown by the curve at the right side of d1max in Fig. 4. The large variation of Pw due to changes in parameters such as d1 or Zin1 can allow the discharge to transit across the wide power-gap between the O ↔ X wave modes in a discontinuous manner. In the low Pw (electron density) region, where only the O-wave mode exists,9 discharges also evolve continuously in the positive feedback region [see Fig. 4(b)]. Results in Figs. 4 and 5 indicate that the presence of the discontinuous discharge-transition requires both the eternal matching condition and the internal discharge mode.
B. Separatrix of negative and positive feedback regions
Comparing the locations of d1max in Figs. 4(a) and 5, i.e., separatrixes of the negative and positive feedback regions, one can find that d1max is not constant but varies with Ag. To quantify the relationship between d1max and Ag, Ag is substituted by the maximal Pw at the separatrix, i.e., Pwmax. The curve of d1max vs Pwmax obtained at 0.15 sccm of Xe is shown in Fig. 6.
The most remarkable is that d1max rises with the increasing Pwmax. As the Xe gas flow rate is varied under a constant Ag, the obtained d1max (see Fig. 7) increases with the increasing gas flow rate, but the curve deviates from the quasi-linearity as shown in Fig. 6. The above results suggest that, as Ag or the gas flow rate is varied at a fixed d1, the discharge can shift between the positive and negative feedback regions. Therefore, care must be taken for each discharge to ascertain its characteristic feedback region.
In the negative feedback region where mode transitions tend to be continuous (see Fig. 5), ECR discharges are relatively stable. At the boundary between the negative and positive feedback regions, the reflection coefficient of incident MW achieves its minimum. However, ECR discharges under this condition are less stable than those in the negative feedback region. For this reason, investigators in Refs. 15, 17, and 22 operated their ECR discharges at the mismatch state, which is believed to be lied in the negative feedback region.
C. Normal and inverse hysteresis-loops
Variations in plasma parameters with discharge power, such as electron density and electron temperature, are important to understand characteristics of plasma sources. In this paper, electron density and electron temperature are not measured. As a monitoring signal of ECR discharges, the total gray (Gt) values of images captured from discharges in the positive feedback region are extracted using Image J software.25,26 At three typical Xe gas flow rates, the obtained Gt-values against the increasing and decreasing Pw are shown in Fig. 8.
In the ramping-up stage of Pw at 0.55 sccm [see Fig. 8(a)], the Gt-value jumps from the lower branch of the curve at a critical Pw to Pw1 of the upper branch. In the ramping-down stage of the upper branch, the Gt-value reverts to the lower branch at Pw2. The fact of Pw2 being lower than Pw1 indicates that the observed hysteresis is normal. At the moderate gas flow rate [see Fig. 8(b)], the hysteresis-loop almost disappears. As the gas flow rate decreases to 0.15 sccm [see Fig. 8(c)], Pw2 exceeds Pw1, indicating that the hysteresis loop becomes inverse or abnormal.
In order to gain more insight, the power difference ΔPwhl (=Pw1 − Pw2) is defined as the width of the hysteresis loop to evaluate the evolution of the hysteresis. The obtained ΔPwhl against gas flow rate is shown in Fig. 9. For the inverse hysteresis appearing in the low gas-flow-rate region, the loop width ΔPwhl is negative. As the gas flow rate increases to around 0.22 sccm, ΔPwhl reduces to zero. The zero loop-width is maintained until the gas flow rate exceeds 0.38 sccm. After ΔPwhl becomes positive, it varies at a smaller rate than that in the low gas-flow-rate region. On the lower branches of curves shown in Fig. 8, the hysteresis loops also exists, and thus the corresponding loop-width can be defined. The dependence of this loop-width on gas flow rate is qualitatively similar to that shown in Fig. 9.
In the moderate gas-flow-rate region of Fig. 9, as denoted by the two green lines, the two loop-widths defined above become sufficiently narrow that discharges are subject to small variations of discharge parameters. The triggered oscillations will be discussed in Subsection III E.
The inverse hysteresis-loop shown in Fig. 8(c) was ever observed in two RF inductively coupled plasma (ICP) sources.27 The appearance of such loops in MW ECR and RF inductive discharges requires a common condition, namely they exist in small-sized plasma sources operated in low pressure region. This suggests that there exists a same mechanism underlying the inverse hysteresis. Lee and Chung ascribed the inverse hysteresis to the evolution of electron energy distribution (EEDF).27 However, the effect of EEDF is not the cause to produce the inverse H → E mode transition because such an evolution even exists in the Faraday-shielded RF ICPs,28,29 where no discharge mode transition occurs. Zhao and Ding suggested a consistent explanation on the inverse hysteresis:30 electron density is reduced with decreased neutral density due to gas temperature rise resulted from the slow wall gas-heating.31 During the ramping-up phase of Pw in the X-wave mode discharge (see Fig. 8), the wall temperature rises to a high level. The subsequent ramping-down of Pw is carried out at a time rate of change that is not sufficiently low. Consequently, the temperature of the wall overheated in the high-Pw X-wave mode discharge cannot immediately follow the decreasing Pw, and thus, are higher compared with that at Pw in the ramping-up phase. At a constant gas flow rate, the neutral density is reduced in the ramping-down phase due to the increased gas temperature. In low gas pressure (gas flow rate) region [see Fig. 8(c)], the reduction in neutral density is relatively large. Accordingly, at 0.15 sccm, the X-wave mode discharge transits to the O-one at Pw2 that is higher than Pw1, forming the inverse hysteresis-loop.
D. Effect of impedance matching on width of hysteresis loop
Results from Figs. 4 and 5 are obtained by changing d1 in discharges operated in the feedback region. The effect of d1 on the width of hysteresis loop (ΔPwhl) can be investigated by varying Pw under different d1 values. The obtained curves of ΔPwhl vs d1 under different gas flow rates are shown in Figs. 10 and 11. For the inverse hysteresis (see Fig. 10), the absolute loop-width rises with the increasing d1. In the case of the normal hysteresis (see Fig. 11), the curve shape is seemingly opposite to that shown in Fig. 9, but the behavior is essentially the same, i.e., the width of the normal hysteresis-loop also rises with the increasing d1.
E. Self-mode-transition
Self-mode-transitions are believed to occur automatically in various discharges. But as far as we know, there have been only two specific investigations on this topic. One is the E → H mode transition in the RF inductively coupled plasma (ICP),32 and the other is the undetermined mode transition in MW ECR plasma.33 Recently, the slow wall gas-heating was proposed as the cause for the observed long drift toward the self-E → H mode transition point.30 The H → E mode transition is the counterpart of the E → H mode transition and has also been extensively investigated. However, no self-H → E mode transition has been reported. The E and H modes in RF ICPs correspond respectively to the O- and X-wave modes in our ECR plasmas. The arising question is that whether the self-O → X wave mode transition, especially the self-X → O one, can occur in our ECR discharges.
1. Self-O → X wave mode transition during cooling down of hot wall
The first experiment is to confirm the self-O → X wave mode transition. According to the requirement for triggering the self-E → H mode transition in the RF ICP,32 the chamber wall of the ECR plasma source was first pre-heated in the “hot” 3.5-W X-mode discharge for 30 min, and then, the discharge was switched from the X-wave mode to the O-wave mode in the vicinity of the O → X wave mode-transition point. Henceforth, the temperature of the chamber’s external surface was monitored by the thermocouple described in Sec. II. Owing to the slow variation of the external wall temperature, the voltage standing wave ratio (VSWR) recorded by the MW power meter could be also monitored synchronously. The obtained time-evolutions of both the wall temperature and VSWR at 0.15 and 0.55 sccm are shown respectively in Figs. 12 and 13.
Time evolutions of VSWR (a) and wall temperature (b) in 0.15 sccm discharges under hot wall condition. The classification of region I, II, and III is described in the text.
Time evolutions of VSWR (a) and wall temperature (b) in 0.15 sccm discharges under hot wall condition. The classification of region I, II, and III is described in the text.
Time evolutions of VSWR (a) and wall temperature (b) in 0.55 sccm discharges under hot wall condition. The classification of region I, II, and III is described in the text.
Time evolutions of VSWR (a) and wall temperature (b) in 0.55 sccm discharges under hot wall condition. The classification of region I, II, and III is described in the text.
The time evolution of VSWR in Fig. 12(a) can be divided into three characteristic regions: (1) region I where the overall VSWR drops with time at a small rate of change; (2) region II, in which the VSWR oscillates irregularly with a very small amplitude; (3) region III, the domain immediately after the step fall of the VSWR due to the self-O → X wave mode transition. After entering region III of the X-mode discharge, the VSWR ceases to oscillate immediately, implying that the discharge stability is recovered.
As argued in Ref. 30, the wall temperature in Fig. 12(b) does decrease before the self-O → X wave-mode transition. This outcome is natural because the wall overheated in the “hot” X-mode discharge is cooled slowly down in the “cold” O-wave mode discharge with a low Pw. As a result of the reduced wall gas-heating in regions I and II (see Fig. 12 and refer to Ref. 30), the gas temperature and neutral density drops and rises, respectively. In the low-pressure region where the electron-neutral collision is weak, the rising neutral-density causes the increasing electron density.34 In this way, the O-wave mode discharge automatically shifts slowly toward to the O → X wave mode transition point, as evidenced by the slow drop in the VSWR signifying the discharge state. After the self-O → X wave mode transition, Pw increases steeply and the wall temperature starts to rise. The reason for which is that, as the discharge enters the X-mode region with a relatively high-Pw, the power deposited onto the chamber wall becomes larger than that transmitted from the wall.
At 0.55 sccm, the time evolution of VSWR in Fig. 13(a) is also characterized by the three regions in Fig. 12(a), but there exist the following two differences: (1) the oscillating amplitude of VSWR in region II of Fig. 13(a) is larger than the counterpart in Fig. 12(a); (2) the self-O → X wave mode transition at 0.55 sccm takes place in a shorter time-interval than that at 0.15 sccm. In other words, the former discharge-transition develops faster than the later one. The behind reason is the gas pressure or gas flow rate. During the self-mode-transition, electron density varies spontaneously, the change rate of which is determined by ionization rate that subsequently depends on gas pressure or gas flow rate. In the 0.55-sccm case where the gas pressure is relatively higher, the larger ionization-rate can drive a faster self-mode-transition. The large oscillating amplitude in region II at 0.55-sccm [see Fig. 13(a)] is also related to the gas pressure, details of which will be discussed in Subsection III F.
In contrast, at the lower gas flow rate of 0.15 sccm, the time evolution of wall temperature in region III of Fig. 13(b) is distinctive from that in Fig. 12(b), namely the wall temperature as well as the gas temperature in Fig. 13(b) continues dropping after the self-O → X wave mode transition. This discrepancy is originated from the differences before and after the O → X wave mode transition. As stated above, the Pw-values in the pre-heating discharges for 0.15 or 0.55 sccm Xe are both 3.5 W. This value is relatively higher than those before and after the O → X wave mode transition at 0.55 sccm [see Fig. 8(c)]. Therefore, the relatively smaller rise of Pw during the self-O → X wave mode transition at 0.55 sccm can neither elevate nor maintain the temperature of the overheated wall. Consequently, the wall is cooled down throughout the O → X wave mode transition. For the 0.15-sccm discharge, however, the pre-heating discharge power of 3.5 W is not sufficiently higher compared with those before and after the O → X wave mode transition [see Fig. 8(c)]. As a result, the rise in Pw during the self-O → X wave mode transition can reverse the cooling-down process, leading to the rise in the wall temperature.
2. Self-X → O wave mode transition during heating up of cold wall
In contrast to the overheated wall discussed above, experiments in this subsection were conducted with the initially cold wall: the plasma source was first operated in the “cold” 1.0-W O-wave mode discharge for 5.0 min, and then, the O-wave mode discharge was switched to the X-mode discharge near the X → O wave mode-transition point. The obtained time evolutions of wall temperature and VSWR at 0.15 and 0.55 sccm are shown respectively in Figs. 14 and 15. In the two cases, the corresponding time evolutions have the similar tendency, and the irregular VSWR-oscillation shown in Fig. 12 disappears throughput the transition. The self-X → O wave mode-transitions, as evidenced by the steep rises in VSWR, occur as the wall temperatures increase slowly to their respective thresholds.
Time evolutions of VSWR (a) and wall temperature (b) in 0.15 sccm discharges under cold wall condition. The classification of region I and II is described in the text.
Time evolutions of VSWR (a) and wall temperature (b) in 0.15 sccm discharges under cold wall condition. The classification of region I and II is described in the text.
Time evolutions of VSWR (a) and wall temperature (b) in 0.55 sccm discharges under cold wall condition. The classification of region I and II is described in the text.
Time evolutions of VSWR (a) and wall temperature (b) in 0.55 sccm discharges under cold wall condition. The classification of region I and II is described in the text.
The reason for the wall-temperature rise throughout the various time domains in Figs. 14 and 15 is that, Pw in the discharge preset near the X → O wave mode-transition point and that immediately after the X → O wave mode-transition are both higher than the initial discharge-power of 1.0 W. Unlike the cooling down of the overheated wall in subsection (a), electron density during the heating up of the initially cold wall decreases, which induces the required shift to the X → O wave mode transition.
As stated above, only the self-E → H mode transition was observed in the RF ICP,27 and no self-H → E mode transition has been reported. The behind reason is that, in the normal operation, the RF inductive discharge was preset at the H → E mode transition point under the condition of hot wall preheated in the H-mode discharge. In this situation, the shift required for the self-H → E mode transition is prevented during the subsequent cooling down of the hot wall. For ECR discharges in Figs. 14 and 15, the situation is reversed, namely the initially cold wall is heated up, leading to the required shift to trigger the self-X → O wave mode transition.
F. Oscillations
The observed oscillations occur in the moderate gas-flow-rate region in Fig. 9 and are characterized by irregularity, namely the oscillations are not periodic and the amplitudes are not constant. Generally, the oscillations occurring in the central zone of the moderate gas-flow-rate region are fast and have the small amplitudes. When the gas flow rate is varied toward to either the high or low value, the oscillations become slow, while the amplitudes increase. The oscillation was not investigated in the entire gas-flow-rate region, but at a typical gas flow rate of 0.4 sccm in the positive feedback region. Additionally, in order to trigger the oscillation, Pw was required to increase above a threshold.
The oscillation was monitored by the fast camera described in Sec. II. Thanking to the camera’s capability of long-time recording, images of multiple oscillating-discharges can be recorded. One of the selected scenarios is shown in Fig. 16. The naked-eye comparison between the images finds that the discharge undergoes a complete cycle. Namely the discharge starts from a low intensity [see Figs. 16(a)–16(e)], jumps to a high intensity with a long duration [see Figs. 16(f)–16(s)], and finally recovers to the initial state [see Figs. 16(t)–16(w)]. In order to quantify the above primary judgment, the Gt-value of each image in Fig. 16 is extracted sequentially and shown in Fig. 17. Obviously, the Gt-value exhibits two steep changes: the soaring up is caused by the O → X wave mode transition, while the other by the X → O one.
Discharge images selected sequentially in the entire process of one typical oscillation in discharges at Xe flow rate of 0.4 sccm.
Discharge images selected sequentially in the entire process of one typical oscillation in discharges at Xe flow rate of 0.4 sccm.
It is worth noting here that, prior to the O → X wave mode transition, the Gt-value increases slightly (see Fig. 17). This is an indicator for the discharge shift to the O → X wave mode transition point. Immediately after the O → X wave mode transition, the Gt-value undergoes an overshoot, followed by a drop until the minimum. The recovery does not last for a long time, but is interrupted by a drop in the Gt-value. When the Gt-value drops to a threshold, the X → O wave mode transition is triggered. Subsequently, the undershoot in the Gt-value occurs as a transient response of the X → O wave mode transition. Following the undershoot, the Gt-value rises, leading to another O → X wave mode transition, as described above.
G. Differences and correlation between self-mode transition and oscillation
Results in Figs. 12(a)–15(a) and 17 confirm that discharges during the self-mode transitions and oscillation are both unstable. However, they differ in the following aspects. Firstly, both occur under different conditions. The self-mode transition can be triggered as long as the preset discharge is sufficiently near the transition mode point under the condition of the cold or hot wall, regardless of the width of the hysteresis loop. The oscillation, however, can only occur in discharges whose hysteresis-loop width is sufficiently narrow. Therefore, in Fig. 9, the moderate gas-flow-rate region with a small width of the hysteresis loop is subject to oscillation. Secondly, the self-mode transitions occur between O- and X-wave-mode discharges [Figs. 12(a)–15(a)], so does the oscillation in Fig. 17. However, it is not true for all observed oscillations. In Fig. 13(a), the discharge in region II is oscillating, despite that the oscillating cannot transiently reach the O-wave mode. Thirdly, the self-mode transitions and oscillations develop in different time scales. The time required for the self-mode transition mainly depends on the gap between the preset discharge and the mode transition point. In Figs. 12–15, the so-called gaps are rather wide, so that the self-mode transitions take several minutes. If the preset discharge is sufficiently close to the mode-transition point, the self-mode transition will occur immediately. In this case, however, the monitor of the time-varying wall temperature or VSWR becomes difficult.
Despite of the above difference, the oscillation in Fig. 17 is essentially the fast self-mode transitions switching reversibly between O- and X-wave mode discharges, in which the widths of the hysteresis-loops on the lower and upper branches of the curves in Fig. 8 are sufficiently small. Therefore, the oscillation is also expected to be driven by the shift in the direct volume gas-heating as well as the indirect wall gas-hating. In view of this, the oscillation shown in Fig. 17 is explained as following. The plateau of the oscillating Gt-value in Fig. 17 is a result of the high Pw after the O-X wave mode transition. The cold wall in the O-wave mode discharge is subsequently heated up. Consequently, the electron density drops slowly with the reduced neural density, as evidenced by the decreasing Gt-value at the right side of the plateau (see Fig. 17). When electron density decreases to the threshold for the X–O wave mode transition, the X–O wave mode transition is thus triggered. In contrast, after the discharge transits into the low-Pw O-wave mode discharge, the processes described above are inversed: the neutral density along with electron density is increased as the hot wall is cooled down. The variation finally leads to the onset of the O-X wave mode transition. The above scenario is repetitive, leading to the oscillation as shown in Figs. 16 and 17. It is worth noting that, the small variation in neutral density due to gas heating can only induce a limited change in electron density, so that the oscillation occurs merely in discharges whose widths of hysteresis loops are sufficiently narrow. This requirement is merely satisfied in the moderate gas-flow-rate (gas pressure) region.
IV. CONCLUSION
Positive and negative feedback regions are confirmed in MW ECR discharges by adjusting a three-stub coaxial tuner. When mismatched in the negative feedback region, MW ECR discharges are stable, and they become unstable in the positive feedback region. Self-mode transitions from high to low electron-density discharge are achieved for the first time by presetting the discharge under cold-wall condition. The counterpart, namely self-mode transitions from low to high electron-density discharge can be triggered under hot-wall condition. Inverse hysteresis and oscillation occur respectively in the low and moderate gas-flow-rate (gas pressure) regions. Effects of wall gas-heating are suggested to explain the self-mode transition and inverse hysteresis as well as oscillation. The hysteresis is caused by the relatively-stronger wall gas-heating in the low gas-flow-rate (gas pressure) region. The observed oscillation can be regarded as the reversible mode transition between two discharge modes whose widths of hysteresis loops are sufficiently narrow in the moderate gas-flow-rate (gas pressure) region.
ACKNOWLEDGMENTS
This work was partially supported by the National Natural Science Foundation of China under Grants Nos. 11975070 and 11475040 and Open Funds for Science and Technology on Vacuum Technology and Physics Laboratory, Lanzhou Institute of Physics (Grant No. zwk1609).
AUTHOR DECLARATIONS
Conflict of Interest
The authors have no conflicts to disclose.
Author Contributions
Z. F. Ding: Conceptualization (equal); Funding acquisition (equal); Supervision (equal); Writing – original draft (equal); Writing – review & editing (equal). Y. R. Yang: Data curation (equal); Investigation (equal). S. H. Fu: Software (equal).
DATA AVAILABILITY
The data that support the findings of this study are available from the corresponding author upon reasonable request.