Replacing the mercury lamp in a mask aligner with UV-LED
What a UV-LED conversion changes on a mask aligner, from wavelength and dose to uniformity and lamp-house cooling, and how to requalify your resists afterwards.
Replace the mercury lamp house of a mask aligner with a UV-LED source. No warm-up, no lamp changes and no mercury to handle, with intensity mapped after installation.
Most older contact and proximity aligners use a high-pressure mercury arc lamp. It works, but it has costs that a lab manager knows well: the lamp needs warm-up before the first exposure, intensity drifts as the lamp ages, lamps are changed regularly, and each one holds mercury that needs careful handling when it breaks or reaches end of life. The lamp also runs hot and needs its own power supply and cooling.
A UV-LED conversion replaces the mercury lamp house with an LED source. The source switches on when needed, drifts far less than a mercury lamp, though it still needs periodic intensity checks, and has no mercury. For teaching cleanrooms with many occasional users, the gain in day-to-day reliability is often the main reason to convert.
The mercury lamp emits strong lines at 365 nm (i-line), 405 nm (h-line) and 436 nm (g-line). A UV-LED source covers the part of that spectrum your resists need, using LEDs at or near the relevant lines; which channels are available depends on the source model. The relative intensity of each line can differ from what your mercury lamp delivered, and broadband resists may respond differently.
That means exposure doses change. After the conversion we measure intensity at the wafer plane and set exposure times from the measured dose. We then run test exposures with your resists so you can confirm resolution and sidewall profile before returning to production work. For a longer discussion, see mercury lamp to UV-LED on a mask aligner.
A typical conversion covers:
The exact scope depends on the aligner model and its configuration. Common candidates include the SUSS MA6, the SUSS MJB4 and the EVG620.
The aligner is out of service for the installation, mapping and test exposures. On a single aligner this is normally a short planned stop of a few days, depending on configuration and on how many resists you want requalified. The proposal states the planned downtime.
You receive the installed source, an intensity and uniformity map, dose recommendations from the test exposures and updated operating notes. The old lamp house is returned to you or disposed of as you choose. The upgrade applies to contact and proximity aligners in lithography.
We check the lamp house, optics, shutter and controller on site or from photos.
We propose a UV-LED source with the wavelengths your resists need and confirm it fits the optical path.
Our engineers remove the mercury lamp house, fit the LED source and connect it to the exposure controls.
We map intensity and uniformity, set the exposure dose and run test exposures with your resist.
Yes, the MA6 and similar SUSS and EVG aligners are common candidates. The survey confirms the fit for your configuration, including the optics and the exposure controller.
Usually yes. The LED spectrum differs from the mercury spectrum, so exposure times are adjusted from the measured dose and checked with test exposures on your resists.
It depends on the LEDs fitted. Sources commonly combine LEDs around 365 nm and 405 nm, with 385 nm or a channel near the g-line on some models, so the choice is made from the resists you use.
We remove it and either return it to you or dispose of the mercury lamp through a proper waste route. Keeping the old lamp house lets you revert if you ever need to.
What a UV-LED conversion changes on a mask aligner, from wavelength and dose to uniformity and lamp-house cooling, and how to requalify your resists afterwards.
Lamp house, stage, alignment optics and mask holder sizes decide what an older aligner can still do. A checklist for your inspection visit.
Tell us the tool and what you need. We scope the work and send a written offer.