Specific Process Knowledge/Thin film deposition/Deposition of Silicon Oxide/SiO2 disk and granule source tests in Temescal October 2026
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This page is written by Evgeniy Shkondin @DTU Nanolab if nothing else is stated.
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SiO2 disk and granule source tests in E-Beam Evaporator (10-pockets), October 2026
Experimental work and documentation: Evgeniy Shkondin, DTU Nanolab. Rikke M. Nielsen was present during Run 1 (22 October 2026). Run 2 (23 October 2026) was carried out by Evgeniy Shkondin alone. Report updated on 27 October 2026.
Service and target loading: Henrik Nielsen (DTU Nanolab)
Photographs and schematics: Evgeniy Shkondin / DTU Nanolab. The power and rate plots are reconstructed from the instrument recordings. Both runs used a HULA (high uniformity lift-off assembly) holder; film thicknesses were determined by Cauchy-model ellipsometry.
Overview
Two source-loading configurations were tested in the E-Beam Evaporator (10-pockets) on 22 and 23 October 2026. Each run used four solid, circular SiO2 disks in a graphite liner and a nominal thickness setpoint of 600 nm at 1 Å/s. Run 1 used the disks alone. Run 2 used new disks with SiO2 granules between the stack and liner wall. Both runs used a HULA (high uniformity lift-off assembly) holder.
The disks alone developed a narrow cavity that penetrated the entire stack. Adding granules and changing to a horizontal figure-eight sweep produced a more manageable deposition: repeated small rate spikes persisted, but the run finished without the major instability or growing liner-exposure concern described for Run 1. The deepest penetration stopped at the interface between the third and fourth disks.
| Outcome | Run 1: disks | Run 2: disks + granules |
|---|---|---|
| Deposition date | 22 October 2026 | 23 October 2026 |
| People present | Evgeniy Shkondin; Rikke M. Nielsen | Evgeniy Shkondin |
| Thickness setpoint | 600 nm | 600 nm |
| Cauchy-model thickness | 665 nm | 668 nm |
| Sweep program | #2: small circle | #7: horizontal figure-eight |
| Peak recorded deposition power | 6.9% | 6.9% |
| Final source condition | Full-stack breakthrough | Penetration through the first three disks |
| Source mass change | 1.55 g loss | Not recorded |
The report follows the experimental sequence using source photographs, schematics, visual observations, and instrument recordings. The power curves retain the recorded values without smoothing. Run 1 heating-timer pauses (caused by a recipe condition that issues an alarm message after 30 min of continuous heat; the value is corrected to 300 min for Run2) are excluded from the main comparison and are separate from source instability. These exploratory tests document source behavior and provide a basis for further process development.
Test design and recorded settings
The tests examined source erosion and sweep behaviour over a nominal 600 nm deposition. Four disks were stacked in the graphite liner. Before Run 2, a new stack was loaded and surrounded by SiO2 granules. A HULA (high uniformity lift-off assembly) holder was used in both runs. The source specifications below are taken from the material package labels.
| Source | Company | Dimensions | Labelled purity |
|---|---|---|---|
| Disks | ScoTech | 21 mm diameter × 5 mm thick | 99.99% (4N) |
| Granulate | Umicore Thin Film Products AG | 1.5-3.5 mm | 99.99% |
Common tooling-file and deposition settings
| Parameter | Recorded value |
|---|---|
| Tooling factor / density / Z-ratio | 78.5 / 2.648 g/cm3 / 1 |
| Control gain | 8.0 (Å/s)/% power |
| Control TC / control DT | 0.1 s / 0.1 s |
| Maximum allowed power | 10% |
| O2 flow setting | 5% |
| Rate | 1 Å/s |
| Thickness setpoint | 600 nm |
Conditions that differed between runs
| Parameter | Run 1 | Run 2 |
|---|---|---|
| Substrate temperature setting | 190 °C | Room temperature (RT) |
| Source loading | Four disks alone | Four new disks + surrounding granules |
| Sweep geometry | Small circle (#2) | Horizontal figure-eight (#7) |
| Reported sweep parameters | 15% amplitude; 2 Hz | Snapshot: 35% on both axes; 1 Hz / 2 Hz |
Note. Density is a controller input, not measured film density. O2 = 5% is the instrument setting, not gas composition or partial pressure. Run 2 was reported as RT/unheated, but its logged thermocouple temperature rose from 22.0 to 61.6 °C during deposition. The TC channel is not an independent sample-surface temperature measurement. Power is recorded as a percent of full scale.
Source loading, sweep geometry, and the temperature condition changed together, so this is not a single-variable comparison. The logs also show different rise/soak settings, including soak-2 levels of 2.8% in Run 1 and 5.0% in Run 2. Thickness milestones refer to the QCM indication.
Run 1: solid disks alone
Run 1 was carried out on 22 October 2026 by Evgeniy Shkondin (DTU Nanolab), with Rikke M. Nielsen present. Initiating evaporation from solid disks required more power than the established granulate process, so the tooling-file limit was raised to 10%. The figure-eight sweep appeared to extend beyond the disks. Small-circle program #2 was therefore selected, with 15% amplitude and a 2 Hz frequency.
| Stage / indicated thickness | Observation and reconstruction from the log |
|---|---|
| Startup to about 30 nm | Recorded power reached 6.9% near 1.3 nm and remained about 6.7% at 20 nm. The main power decrease began after the first approximately 30 nm. |
| About 30-90 nm | Power fell sharply, with local medians of 5.8% at 40 nm and 2.8% at 60 nm. Oscillations followed. A central hole was visible near 70 nm; the log contains brief QCM-rate peaks up to 9.6 Å/s. |
| After about 120 nm | The beam was shifted slightly off centre. Power stabilized around 2.6-2.7%, then gradually increased. |
| Around 270 / 400 nm | Recorded power was approximately 3.5% / 3.9%, consistent with the approximate written milestones. |
| About 500 nm to completion | The cavity began to glow and liner exposure was suspected. The beam was shifted again, with uncertain benefit. A late recorded transient near 587-589 nm occurred before completion at about 600 nm. |
Ellipsometry using a Cauchy model for SiO2 gave a thickness of 665 nm for the transparent film. Inspection after venting confirmed breakthrough through the full disk stack and no graphite-liner damage. Typical visible rate fluctuations were 0.6-2.2 Å/s; the recording captures larger brief excursions.

Note. A 30-minute heating allowance caused three alarms. Each resumption initiated a new rise/soak sequence before deposition continued. These timer-related interruptions are excluded from the source comparison. The recording confirms completion at approximately 600 nm.
Run 1: post-deposition evidence

The axial views reveal a relatively narrow passage through a much wider remaining body of source material. This is consistent with strongly localized erosion. Full-stack breakthrough does not mean that most of the source mass was consumed: the reported mass decreased from 15.54 g to 13.99 g, a loss of approximately 10.0%.
Run 2: disks with surrounding granules
Run 2 was carried out by Evgeniy Shkondin alone on 23 October 2026. New disks were loaded and SiO2 granules filled the surrounding space in the graphite liner. This allowed the conventional horizontal figure-eight sweep, program #7. The run was performed without substrate heating, using the same HULA holder type. The table follows visual observations through the top chamber window; the approximate surface shapes are interpreted in Figure 5.
| Indicated thickness | Power | Observation |
|---|---|---|
| Initiation | 5.9% | Reached the 1 Å/s rate setpoint. |
| 20 nm | 6.8% | Source appeared normal (stage A). |
| 40 nm | 5.7% | Power began to decrease. |
| Approaching 50 nm | Not stated | The disk edge appeared deformed and a dark region became visible (stage B). |
| 60 nm | 5.1% | Power continued to decrease. |
| 150 nm | 4.5% | Rate remained around 1 Å/s. The dark region became slightly larger. |
| 300 nm | 4.4% | Power was very stable. Rough-looking features appeared around the dark region (stage C). |
| Beyond 300 nm | Not stated | A darker spot appeared within the existing dark region, suggesting local deepening (stage D). |
| 400 nm | 4.3% | The upper disk appeared deformed and a second dark region became visible (stage E). |
| 500 nm | 4.4% | The two dark regions appeared to merge into a figure-eight-shaped region (stage F). |
Small repeated rate spikes occurred throughout the run. Surrounding granules occasionally glowed when struck by the sweeping beam. Apart from these spikes, the rate and power remained reasonably stable, and the deposition completed without significant instability or additional concern.
Ellipsometry using a Cauchy model for SiO2 gave a thickness of 668 nm for the transparent film. After venting, inspection showed penetration through the first three disks, stopping at the boundary between the third and fourth. Local cavity formation persisted, while the bottom disk remained intact.
Run 2: geometry and controller evidence


What the controller photograph establishes
The image independently supports the stated figure-eight sweep and the presence of repeated rate deviations. Its indicated thickness of 158.1 nm and power of 4.5% are consistent with the written observation of approximately 4.5% at 150 nm. The sweep display also identifies pocket 9 at the time of the photograph.
The controller photograph shows the short-term rate trace. The instrument recording provides an approximately one-second time series for the later power and rate figures. Faster oscillations may remain unresolved at this sampling interval. The 1 Hz and 2 Hz values in the image are sweep settings, not measured spike frequencies.
Run 2: observed surface evolution

| Stage | Approximate point in run | Visual interpretation through the window |
|---|---|---|
| A | Early stage / about 20 nm | An apparently regular disk surface surrounded by granules. |
| B | Approaching 50 nm | Apparent edge deformation and the first visible dark region. |
| C | About 300 nm | A rough-looking boundary appears near the surrounding granules. |
| D | Beyond 300 nm | A darker spot within the first region suggests local deepening. |
| E | About 400 nm | A second dark region appears with further apparent upper-disk deformation. |
| F | About 500 nm | The dark regions appear to merge into a figure-eight-shaped area. |
The drawings are visual mental descriptions based on looking through the small window on top of the chamber during deposition. The actual source shape can be difficult to interpret: brightness and contrast may be misleading, and several shadowing effects can alter the appearance. The sequence therefore records perceived changes in the source. Post-run inspection established the final penetration depth independently of these in-process impressions.
Run 2: post-deposition evidence

The source retained an intact lower disk beneath a strongly reshaped upper region. Irregular material remained around the cavity and in the liner. This morphology is consistent with interaction between the disk stack and the surrounding granules, but it does not establish a mass balance or a reduction in total material consumption.
Thickness, mass and numerical comparison
The comparison combines Cauchy-model ellipsometry, source-mass measurements and instrument recordings. The logs distinguish the last DEPOSIT sample from the later final-thickness summary, written after the idle ramp. The latter includes small post-deposition changes in the QCM indication and should not be equated with extra film thickness on the sample.
| Quantity | Run 1 | Run 2 |
|---|---|---|
| Thickness setpoint | 600 nm | 600 nm |
| Last DEPOSIT sample | 599.93 nm | 600.03 nm |
| Final log summary after idle ramp | 600.7 nm | 600.5 nm |
| Ellipsometry thickness | 665 nm | 668 nm |
| Measured thickness minus setpoint | +65 nm | +68 nm |
| Relative difference from setpoint | +10.83% | +11.33% |
| Recorded total shutter-open time | 101 min 17 s | 99 min 49 s |
| Reported initial / final source mass | 15.54 / 13.99 g | Not recorded |
| Apparent source mass loss | 1.55 g (9.97%) | Not calculable |
Thickness and mass calculations
Relative thickness difference = 100 × (ellipsometry thickness − setpoint) / setpoint. The films differ by 3 nm, approximately 0.45% of their mean of 666.5 nm. Both thicknesses were obtained by fitting SiO2 with a Cauchy model. Two different experimental conditions do not establish repeatability.
Run 1 apparent source loss = 15.54 − 13.99 = 1.55 g, or 100 × 1.55 / 15.54 = 9.97%. This source mass change is not collection efficiency. No equivalent mass measurements were supplied for Run 2.
Implications for calibration
The final logged values confirm that both depositions reached the intended 600 nm range. The approximately 11% difference from ellipsometry therefore remains a calibration question (Tooling factor).
The present tooling factor may be adjusted and confirmed to the different 200-mm wafer holder that differs from HULA in geometry design and wafer placement. The HULA may require a slightly higher tooling factor.
Recorded power versus thickness

The recordings provide 6680 valid source records for Run 1 and 6170 for Run 2, mostly at approximately one-second intervals. The table gives local sample medians in ±2.5 nm windows. These summarize quantized controller values; they are not independent-replicate statistics or power calibration uncertainties.
| QCM thickness | Run 1 power | Run 2 power |
|---|---|---|
| 20 nm | 6.7% | 6.8% |
| 40 nm | 5.8% | 5.7% |
| 60 nm | 2.8% | 5.1% |
| 120 nm | 2.6% | 4.9% |
| 150 nm | 2.7% | 4.6% |
| 300 nm | 3.6% | 4.4% |
| 400 nm | 3.9% | 4.3% |
| 500 nm | 4.1% | 4.4% |
| 550 nm | 4.3% | 4.4% |
Run 1 reaches a minimum operating region near 2.5-2.7% after the early oscillations, then rises gradually towards approximately 4.5% near completion. Run 2 reaches 6.9% near 19 nm, falls towards 5%, and settles around 4.3-4.5% for much of the later deposition. The combined loading improves stability, but does not require less power at every thickness.
Early power and rate transients

Run 1: the major drop occurs after the first 30 nm
The log refines the early chronology: power was still 6.7-6.8% around 20 nm, rather than already near 2%. It fell sharply over approximately 30-70 nm. Large fluctuations in the recorded rate accompanied the low-power oscillations. The highest recorded rate was 9.6 Å/s near 69.2 nm, followed by further large peaks around 73-77 nm.
Run 2: a smaller recorded rate excursion
Run 2 reached a maximum recorded rate of 1.7 Å/s near 39.6 nm. It then remained much closer to the 1 Å/s setpoint in the sampled record. This supports the observer’s assessment of improved stability. The logger cannot fully resolve fast spikes visible on the controller display, so these maxima are limited to the sampled data.
A late Run 1 event remains in the comparison
Near 587-589 nm, Run 1 recorded a rate excursion up to 7.8 Å/s while power fell to about 2.8%, followed by recovery. This occurred well after the final restart and is retained in the main curve. The log alone cannot assign it to beam repositioning, source reshaping or another specific cause.
Processing interpretation

Treatment of heating-timer interruptions
Run 1 was interrupted by alarms when the 30-minute heating allowance expired (corrected to 300 min for Run2). The main plots use sustained DEPOSIT phases, exclude repeated rise/soak sequences, and omit a fixed 120 s recovery interval after each restart. These exclusions are shown as gaps. Three isolated zero-power DEPOSIT-labelled records preceding restart ramps are also excluded. The initial startup is retained.
No smoothing, outlier removal or thickness rescaling is applied to the remaining points. Original record order and small reversals in the thickness indication are preserved. The package includes the unfiltered wall-clock plots and all records. Cumulative deposition-phase time is about 101.33 min for Run 1 and 99.87 min for Run 2; the separate shutter-open counters are each 3 s shorter.
Conclusions
Conclusions supported by this comparison
Four solid SiO2 disks alone, used with a small circular sweep, developed a cavity through the full source stack during the nominal 600 nm test. The recording captures strong early rate excursions and a late transient. The heating-timer pauses are a separate operational issue and are not evidence of source instability. The liner was reported undamaged.
The combination of disks, surrounding granules, and a horizontal figure-eight sweep gave more stable operation in the second test and left the fourth disk unpenetrated.
Both configurations produced transparent SiO2 films with Cauchy-model ellipsometry thicknesses close to 0.67 µm. The combined configuration is a reasonable starting point for further source optimization.
The strongest evidence supports improved deposition stability and reduced penetration depth in Run 2. Lower mass consumption was not quantified because the second charge was not weighed before and after deposition. A reliable maximum thickness requires further testing.
Note. This report records exploratory tests rather than an operating instruction. Source coverage must be assessed during deposition; the absence of damage in one run does not establish that continued operation after breakthrough is acceptable. Use the current local operating procedures and tool-responsible guidance [1, 2].
Related local documentation
[1] DTU Nanolab LabAdviser, “Temescal processing / Good to know about the Temescal”. QCM conversion, tooling calibration and source monitoring. Accessed 27 October 2026.
Open the Temescal process-control guide
[2] DTU Nanolab LabAdviser, “Evaporation of SiO2 in Temescal-2”. Related local process information, accessed 27 October 2026. Its earlier tests are separate from this comparison.
Open the related SiO2 deposition page
Scope of the comparison
The tests compare two complete source configurations: loading, sweep and temperature changed together. Exact timestamps for beam shifts, the added granulate mass and a Run 2 mass balance were not recorded. The logged TC temperature does not independently establish sample-surface temperature. Composition and contamination were not measured in these tests.
The recordings establish the power and rate histories and confirm an approximately 600 nm endpoint for each run. The timer-related Run 1 interruptions are excluded from the source-performance comparison. Proposed physical explanations remain interpretations of the recorded behaviour.