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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Reconstruction of spectral solar irradiance since 1700 from simulated magnetograms · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1605.02039/</link><description>Collected HN comments and submissions linking this paper.</description><language>en</language><lastBuildDate>Mon, 02 Nov 2026 11:16:22 GMT</lastBuildDate><atom:link href="https://hackerpaper.kaipfister.de/p/1605.02039/feed.xml" rel="self" type="application/rss+xml" /><item><title>Reconstruction of spectral solar irradiance since 1700 from simulated magnetograms — mentioned by Merrill</title><link>https://news.ycombinator.com/item?id=21519916</link><guid isPermaLink="false">urn:hackerpapers:mention:1605.02039:21519916</guid><pubDate>Wed, 13 Nov 2019 00:37:52 GMT</pubDate><description>&lt;p&gt;The scale on the right for temperature is a change of about 2 parts per 255 degrees Kelvin. The scale on the left is about 3 parts in 1361. It&amp;#x27;s not clear whether the much smaller variation in irradiance would be expected to cause the much larger change in temperature. Seems unlikely, since the power radiated by a black body varies as the 4th power of the temperature (Stefan-Boltzman law). Relies on - &amp;quot;Reconstruction of spectral solar irradiance since 1700 from simulated magnetograms&amp;quot; https://arxiv.org/abs/1605.02039&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1605.02039/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.SR</category></item></channel></rss>
