<?xml version="1.0" encoding="utf-8" standalone="yes"?>
<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom">
	<channel>
		<title>Ink on UV Light Zone</title>
		<link>http://uv-light-zone.com/en/tags/ink/</link>
		<description>Recent content in Ink on UV Light Zone</description>
		<generator>Hugo</generator>
		<language>en-us</language>
		
		
		
		
			<lastBuildDate>Fri, 19 Jun 2026 10:34:26 +0800</lastBuildDate>
		
			<atom:link href="http://uv-light-zone.com/en/tags/ink/index.xml" rel="self" type="application/rss+xml" />
			<item>
				<title>Gallium halide lamp for curing ink</title>
				<link>http://uv-light-zone.com/en/posts/gallium-halide-lamp-for-curing-ink/</link>
				<pubDate>Fri, 19 Jun 2026 10:34:26 +0800</pubDate>
				<guid>http://uv-light-zone.com/en/posts/gallium-halide-lamp-for-curing-ink/</guid>
				<description>&lt;p&gt;&lt;img src=&#34;http://uv-light-zone.com/images/a340ed1f2aa85198d59ebbbb11cc1cc2.png&#34; alt=&#34;Gallium halide lamp for curing ink&#34;&gt;&lt;/p&gt;&#xA;&lt;p&gt;Out on the press, thick-build ink layers can look good right off the &lt;a href=&#34;https://o-yate.net&#34;&gt;blanket&lt;/a&gt;—until the top skins over while the bottom stays soft. That latent tack is what gives you blocking, edge distortion, and the inevitable rework.&#xA;It&amp;rsquo;s physics, plain and simple. With conventional UV, most of the energy gets &lt;a href=&#34;https://o-yate.com&#34;&gt;absorbed&lt;/a&gt; near the surface, so the base never gets enough photoinitiator activation. &lt;a href=&#34;https://henruite.com&#34;&gt;Gallium&lt;/a&gt; halide lamps shift the balance by pushing more output into the longer wavelengths—385nm and 405nm—where absorption is lower and penetration is higher.&#xA;The whole play is about spectral control. Gallium halide chemistry lets you tune the emission to deliver higher irradiance in the 385–405nm band, while still holding onto the short-wave energy you need for surface cure. That pushes photon flux deeper into the ink column, so you can get through-cure even on heavy deposits.&#xA;In practice, you end up with more peak irradiance at the substrate plane and curing energy density that stays consistent through the build—not just in the first few microns.&#xA;And that translates straight to throughput and yield. On thick-build screen and flexo work, full cross-linking from bottom to top cuts down on inter-layer adhesion headaches and post-cure blocking. You can run &lt;a href=&#34;https://goldisgood.com&#34;&gt;faster&lt;/a&gt; without fighting surface skinning, and you trim scrap from incomplete cure.&#xA;Gallium halide lamps also run cooler than standard high-pressure mercury systems, which helps keep the curing window stable—especially on heat-sensitive substrates.&#xA;If you&amp;rsquo;re spec&amp;rsquo;ing these, match the lamp spectrum to the ink&amp;rsquo;s photoinitiator package: 365nm for surface response, 385–405nm for depth. Make sure the reflector geometry and the dichroic coating on the housing are right for your setup, so you don&amp;rsquo;t bleed irradiance.&#xA;Expect output to decay over lamp life, so plan replacement intervals to keep energy density inside the ink window. And don&amp;rsquo;t overlook ozone management and cooling airflow—skimp on airflow and you&amp;rsquo;ll shorten lamp life and drift the spectral profile.&lt;/p&gt;</description>
			</item>
	</channel>
</rss>
