<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Article | James R. Beattie</title><link>https://astro-beattie.com/publication_types/article/</link><atom:link href="https://astro-beattie.com/publication_types/article/index.xml" rel="self" type="application/rss+xml"/><description>Article</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Wed, 20 May 2026 00:00:00 +0000</lastBuildDate><image><url>https://astro-beattie.com/media/icon_hu58f049e2f3dec21651e29209817604b1_360074_512x512_fill_lanczos_center_3.png</url><title>Article</title><link>https://astro-beattie.com/publication_types/article/</link></image><item><title>Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas</title><link>https://astro-beattie.com/publication/lab_shock_turbulence_3t/</link><pubDate>Wed, 20 May 2026 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/lab_shock_turbulence_3t/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
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