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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The standard flare model in three dimensions. II. Upper limit on solar flare energy · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1212.2086/</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/1212.2086/feed.xml" rel="self" type="application/rss+xml" /><item><title>The standard flare model in three dimensions. II. Upper limit on solar flare energy — mentioned by superkuh</title><link>https://news.ycombinator.com/item?id=30164385</link><guid isPermaLink="false">urn:hackerpapers:mention:1212.2086:30164385</guid><pubDate>Tue, 01 Feb 2022 16:07:00 GMT</pubDate><description>&lt;p&gt;It&amp;#x27;s pretty darn unlikely in our lifetimes. But you&amp;#x27;ll know about it yourself without anyone needing to tell you before it happens. The energy available to the initial flare and/or associated coronal mass ejection is roughly proportional to the area of the sunspot group. Before there was a &amp;quot;super&amp;quot; flare and/or CME you&amp;#x27;d see the sunspot with your unaided eyes. Check out &amp;quot;The standard flare model in three dimensions. II. Upper limit on solar flare energy&amp;quot; and the figure 4 in particular for size to energy reference. https://arxiv.org/abs/1212.2086&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1212.2086/"&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>
