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		<title>Vs on UV Curing Link</title>
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			<lastBuildDate>Fri, 26 Jun 2026 10:10:02 +0800</lastBuildDate>
		
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				<title>UV mercury lamp vs UV LED curing</title>
				<link>http://uv-curing-link.com/en/posts/uv-mercury-lamp-vs-uv-led-curing/</link>
				<pubDate>Fri, 26 Jun 2026 10:10:02 +0800</pubDate>
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				<description>&lt;p&gt;&lt;img src=&#34;http://uv-curing-link.com/images/58ac68eed98c0bc28c2c79d6b4e2c369.png&#34; alt=&#34;UV mercury lamp vs UV LED curing&#34;&gt;&lt;/p&gt;&#xA;&lt;p&gt;Out on the press floor, UV cure performance often comes down to one detail people overlook: reflector geometry. If the lamp isn’t throwing a stable, high-density spot onto the substrate, you end up chasing cure with more power—and still seeing pinholes, adhesion loss, and web drift from heat. It isn’t just about mercury lamp versus LED. It’s about how the whole optical train shapes what actually lands on the sheet.&#xA;What matters in real terms is peak irradiance at the surface and the delivered energy density in mJ/cm². Mercury vapor lamps give you a broad spectral output, with strong peaks at 365 nm, plus 254 nm and 436 nm. That breadth can help when your photoinitiators have multiple absorption bands, but it also dumps energy outside the photoinitiator window. LEDs are narrowband—365 nm, 385 nm, or 405 nm—so you can match the &lt;a href=&#34;https://goldisgood.com&#34;&gt;spectrum&lt;/a&gt; more precisely and run cooler, but you can lose peak irradiance unless the array is dense and thermally managed. Either way, the reflector sets the effective spot size and the &lt;a href=&#34;https://henruite.com&#34;&gt;uniformity&lt;/a&gt; profile.&#xA;A parabolic contour concentrates flux, sure—but if the tolerances aren’t tight and the dichroic coating isn’t tuned to the dominant wavelength, stray IR and UV eat into yield and beat up the optics and substrate.&#xA;Here’s the practical payoff: when reflector geometry is dialed, you get more photon utilization, which raises effective power density without throwing more watts at the problem. That means faster line speeds, &lt;a href=&#34;https://o-yate.com&#34;&gt;lower&lt;/a&gt; energy draw, and fewer lamp changes. With mercury systems, the reflector has to be ozone-free and run cool to keep spectral output stable. With LED systems, the reflector has to work cleanly with the collimation optics to keep that narrow emission intact and prevent cross-talk between emitters.&#xA;Alignment matters—a lot. A 0.5-degree mis-angle is enough to skew the irradiance profile and show up as cure bands. Mercury lamps need stable ballast and solid quartz integrity. LED arrays need active cooling to hold output steady.&#xA;Plan on using a spectral radiometer to baseline the system, and confirm that the delivered energy density actually matches the ink chemistry at your press speed.&lt;/p&gt;</description>
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