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		<title>Ozone on UV Lamp Core</title>
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			<lastBuildDate>Mon, 08 Jun 2026 08:07:38 +0800</lastBuildDate>
		
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				<title>Ozone producing UV lamp</title>
				<link>http://uv-lamp-core.com/en/posts/ozone-producing-uv-lamp/</link>
				<pubDate>Mon, 08 Jun 2026 08:07:38 +0800</pubDate>
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				<description>&lt;p&gt;&lt;img src=&#34;http://uv-lamp-core.com/images/4c9e492a67b56412ff36b4a4447cefe9.jpg&#34; alt=&#34;Ozone producing UV lamp&#34;&gt;&lt;/p&gt;&#xA;&lt;p&gt;On the art-tile line, inkjet graphics need a finish that looks and feels like fired glaze—high gloss, rock-hard, and chemical resistant. That finish isn’t a topcoat; it’s UV energy driving cross-linking. When the lamp doesn’t pull its weight, you get tack, weak solvent resistance, and a dull, patchy sheen that doesn’t pass inspection.&#xA;&lt;strong&gt;What matters, &lt;a href=&#34;https://goldisgood.com&#34;&gt;technically&lt;/a&gt;&lt;/strong&gt;&#xA;We run an ozone-producing high-pressure mercury vapor lamp because it delivers the 200–400 nm spectral punch we need, with strong output at 365 nm to break down the photoinitiator and kick off rapid cross-linking. Peak irradiance at the substrate has to clear the ink’s initiation threshold, and we measure delivered energy density in mJ/cm² to make sure the cure goes all the way through the pigmented layer—not just skin-deep. The quartz envelope and the dichroic-coated reflector are matched to keep spectral stability and uniformity across the full print width.&#xA;&lt;strong&gt;Why it fits this job&lt;/strong&gt;&#xA;Art-tile UV inks are built for a glass-like cure profile. The 365 nm output drives higher cross-linking density, so you get a surface that can be polished to a glaze-like gloss and stands up to scratches and common household solvents. The lamp’s high-intensity profile shortens dwell, so you can run higher line speeds &lt;a href=&#34;https://o-yate.net&#34;&gt;without&lt;/a&gt; cooking the substrate. In practice, that means consistent hardness tile to tile, with fewer rejects from under-cure.&#xA;Here are the things you’ve got to keep an eye on. Ozone is a byproduct of this spectral output, so the curing zone needs solid extraction and ozone decomposition filtration. Lamp output drops as hours accumulate; keep a scheduled radiometer check on the books and replace at end-of-life thresholds to hold energy density in spec. And confirm lamp length, arc gap, and reflector geometry against your &lt;a href=&#34;https://henruite.com&#34;&gt;printer&lt;/a&gt;’s UV module footprint—otherwise you’ll fight hot and cold bands across the web.&lt;/p&gt;</description>
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