<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Journal_article | James R. Beattie</title><link>https://astro-beattie.com/publication_types/journal_article/</link><atom:link href="https://astro-beattie.com/publication_types/journal_article/index.xml" rel="self" type="application/rss+xml"/><description>Journal_article</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Sat, 01 Nov 2025 00:00:00 +0000</lastBuildDate><image><url>https://astro-beattie.com/media/icon_hu58f049e2f3dec21651e29209817604b1_360074_512x512_fill_lanczos_center_3.png</url><title>Journal_article</title><link>https://astro-beattie.com/publication_types/journal_article/</link></image><item><title>Conservation of magnetic-helicity fluctuations due to spatial decorrelation of fluxes in decaying MHD turbulence</title><link>https://astro-beattie.com/publication/hosking_invariant/</link><pubDate>Sat, 01 Nov 2025 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/hosking_invariant/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>The growth of magnetic energy during the nonlinear phase of the subsonic and supersonic small-scale dynamo</title><link>https://astro-beattie.com/publication/nonlinear_dynamo/</link><pubDate>Mon, 15 Sep 2025 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/nonlinear_dynamo/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>Cosmic ray and plasma coupling for isothermal supersonic turbulence in the magnetized interstellar medium</title><link>https://astro-beattie.com/publication/cosmic_ray_diff_3/</link><pubDate>Wed, 04 Jun 2025 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/cosmic_ray_diff_3/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>Fundamental MHD scales -- II: the kinematic phase of the supersonic small-scale dynamo</title><link>https://astro-beattie.com/publication/fundamental_scales_2/</link><pubDate>Fri, 31 Jan 2025 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/fundamental_scales_2/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>Growth or Decay - I: universality of the turbulent dynamo saturation</title><link>https://astro-beattie.com/publication/g_or_d_1/</link><pubDate>Fri, 01 Sep 2023 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/g_or_d_1/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>Turbulent diffusion of streaming cosmic rays in compressible, partially ionized plasma</title><link>https://astro-beattie.com/publication/cosmic_ray_diff_2/</link><pubDate>Wed, 01 Feb 2023 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/cosmic_ray_diff_2/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>The density distribution and physical origins of intermittency in supersonic, highly magnetized turbulence with diverse modes of driving</title><link>https://astro-beattie.com/publication/pdf_intermittent/</link><pubDate>Thu, 01 Dec 2022 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/pdf_intermittent/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>Availability, outage, and capacity of spatially correlated, Australasian free-space optical networks</title><link>https://astro-beattie.com/publication/ground_station/</link><pubDate>Tue, 01 Nov 2022 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/ground_station/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>Energy balance and Alfvén Mach numbers in compressible magnetohydrodynamic turbulence with a large-scale magnetic field</title><link>https://astro-beattie.com/publication/energy_balance/</link><pubDate>Sat, 01 Oct 2022 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/energy_balance/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>Magnetized compressible turbulence with a fluctuation dynamo and Reynolds numbers over a million</title><link>https://astro-beattie.com/publication/cosmic_ray_diff_1/</link><pubDate>Sat, 01 Oct 2022 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/cosmic_ray_diff_1/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>Fundamental scales in the kinematic phase of the turbulent dynamo</title><link>https://astro-beattie.com/publication/fundamental_scales_1/</link><pubDate>Fri, 01 Jul 2022 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/fundamental_scales_1/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>A multishock model for the density variance of anisotropic, highly magnetized, supersonic turbulence</title><link>https://astro-beattie.com/publication/aniso_dens_var/</link><pubDate>Thu, 01 Jul 2021 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/aniso_dens_var/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>Magnetic field fluctuations in anisotropic, supersonic turbulence</title><link>https://astro-beattie.com/publication/b_field_fluctuations/</link><pubDate>Thu, 01 Oct 2020 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/b_field_fluctuations/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>Filaments and striations: anisotropies in observed, supersonic, highly magnetized turbulent clouds</title><link>https://astro-beattie.com/publication/aniso_dens/</link><pubDate>Sat, 01 Feb 2020 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/aniso_dens/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>The relation between the turbulent Mach number and observed fractal dimensions of turbulent clouds</title><link>https://astro-beattie.com/publication/fractal_2/</link><pubDate>Sun, 01 Sep 2019 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/fractal_2/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item><item><title>The relation between the true and observed fractal dimensions of turbulent clouds</title><link>https://astro-beattie.com/publication/fractal_1/</link><pubDate>Thu, 01 Aug 2019 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/fractal_1/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
&lt;span class="pr-3 pt-1 text-primary-600 dark:text-primary-300">
&lt;svg height="24" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 24 24">&lt;path fill="none" stroke="currentColor" stroke-linecap="round" stroke-linejoin="round" stroke-width="1.5" d="m11.25 11.25l.041-.02a.75.75 0 0 1 1.063.852l-.708 2.836a.75.75 0 0 0 1.063.853l.041-.021M21 12a9 9 0 1 1-18 0a9 9 0 0 1 18 0m-9-3.75h.008v.008H12z"/>&lt;/svg>
&lt;/span>
&lt;span class="dark:text-neutral-300">Create your slides in Markdown - click the &lt;em>Slides&lt;/em> button to check out the example.&lt;/span>
&lt;/div>
Add the publication's **full text** or **supplementary notes** here. You can use rich formatting such as including [code, math, and images](https://docs.hugoblox.com/content/writing-markdown-latex/). --></description></item></channel></rss>