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Causes of Solder Dross Formation in Wave Soldering: Two-Way Improvement of Solder Bar and Process

A
Paste separation means the powder and flux system have split, with the top of the jar thinner and powder settled at the bottom. Mild separation can be restored to homogeneity by proper stirring, and the paste can be used if viscosity checks out. Severe separation that does not remix even after stirring, with heavy powder settling and caking, means the rheological system has failed — the paste must not be used. Separation usually comes from fluctuating storage temperature or overlong storage. Before each use, inspect appearance and stir-check; discard any abnormal batch.

When we encounter an abnormal increase in wave soldering dross, we often first suspect incomplete Flux volatilization or a clogged wave nozzle. However, to truly identify the root cause, we must simultaneously compare the coupling response of tin bar composition fluctuations with conveyor speed, preheat temperature, and wave height. For example, a customer using 99.99% purity tin bars at a conveyor speed of 1.2 m/min and wave height of 8 mm produced an average of 180 g of dross per day. After switching to 99.3% antimony-containing tin bars, the dross amount soared to 320 g, and the dross appeared loose and porous. This indicates that impurity elements not only accelerate oxidation but also alter the density and peeling behavior of the oxide film.

Differences in tin bar purity directly affect the regeneration rate and adhesion of the oxide film. At 255°C in the molten state, the oxide film thickness of 99.99% tin bars remains stable at 8–12 nm. In contrast, due to the catalytic effect of copper and iron impurities, the oxide film of 99.3% lead-containing tin bars reaches over 25 nm in thickness within 4 hours at the same temperature, accompanied by a large amount of hard FeSn₂ inclusions. These inclusions make the oxide film more prone to shattering into flaky dross under wave disturbance, rather than being continuously carried away by the scraper. If the nitrogen protection intensity is reduced from 500 L/min to 300 L/min, the dross amount of 99.99% tin bars only increases by 12%, while that of 99.3% tin bars surges by 67%. This proves that low-purity tin bars are far more sensitive to atmosphere control than high-purity models.

The impact of conveyor speed changes on different tin bars exhibits a non-linear inflection point. When the conveyor speed is increased from 0.8 m/min to 1.0 m/min, the dross amount of 99.99% tin bars slightly increases by 9%, while that of 99.3% tin bars jumps by 31%. This is because the oxide film can still partially self-repair in the low-speed range; once the critical shear stress is exceeded, the impurity-enriched regions peel off first. When the wave height is adjusted from 6 mm to 10 mm, the dross amount of high-purity tin bars only increases by 15% due to their good melt fluidity and uniform surface tension. However, for antimony-containing tin bars, the dross amount surges by 44% due to intensified segregation, and the proportion of tin beads in the dross rises from 11% to 29%. This indicates that increasing the height amplifies the interface instability effect caused by compositional non-uniformity.

The matching between preheat temperature settings and tin bars is extremely strong. With 99.99% tin bars preheated at 120°C, the flux is fully activated with minimal residual solvent, resulting in weak water vapor impact in the wave zone and fine dross that is easy to scrape off. However, for 99.3% tin bars at the same temperature, due to delayed pyrolysis of impurities and rosin complexes, the optimal activation point is only reached at 135°C. If the process is forced to run with parameters for high-purity tin bars, undecomposed flux will enter the wave and cause explosive boiling, directly tearing the oxide film and entraining metal particles to form clumpy dross. After a factory uniformly increased the preheat temperature from 120°C to 135°C, the daily dross amount of 99.3% tin bars decreased by 22%, but that of 99.99% tin bars increased by 18% due to premature flux carbonization. This shows that higher preheat temperature is not always better; it must be locked to match the thermal response characteristics of the tin bars.

The adaptability of scraper material and angle to different dross morphologies varies significantly. Carbon steel scrapers perform stably when handling the thin, dense dross produced by 99.99% tin bars, but are prone to edge chipping when facing the hard, blocky dross generated by 99.3% tin bars. After switching to SKD11 quenched scrapers, the service life was extended by 3.2 times. When the scraper rake angle is increased from 5° to 8°, the dross removal rate of high-purity tin bars improves by 14%. However, for antimony-containing tin bars, due to the high brittleness of the dross, increasing the rake angle instead leads to discontinuous scraping and a 9% rise in dross residue. This indicates that mechanical peeling parameters must be dynamically adjusted according to the physical characteristics of the dross, rather than applying a one-size-fits-all approach.

Considering the overall line changeover cost and maintenance pressure, small-batch, high-reliability products must use 99.99% tin bars with full nitrogen protection (≥500 L/min), conveyor speed ≤1.1 m/min, wave height 7–8 mm, and preheat at 120°C. Under these conditions, the dross amount can be controlled within 150 g per shift. For medium-to-large batch consumer boards where cost is a concern, 99.3% antimony-containing tin bars may be selected, but the scraper material must be upgraded simultaneously, the preheat temperature increased to 135°C, and nitrogen flow maintained at no less than 400 L/min. Otherwise, the risk of uncontrolled dross generation is extremely high. Mixing the two types of tin bars under nitrogen-free conditions is strictly prohibited, as cross-contamination of residual dross will rapidly degrade the oxide film quality of high-purity tin bars. A factory once experienced a doubling of dross amount for 99.99% tin bars within two weeks due to this issue.

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