<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Self-Supervised Learning |</title><link>https://lelain.net/tags/self-supervised-learning/</link><atom:link href="https://lelain.net/tags/self-supervised-learning/index.xml" rel="self" type="application/rss+xml"/><description>Self-Supervised Learning</description><generator>HugoBlox Kit (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Fri, 25 Sep 2026 00:00:00 +0000</lastBuildDate><image><url>https://lelain.net/media/icon.svg</url><title>Self-Supervised Learning</title><link>https://lelain.net/tags/self-supervised-learning/</link></image><item><title>Self-Supervised Representation Learning: From Spectral Foundation Models to Auroral Emission Spectra</title><link>https://lelain.net/publications/aurora-ssl/</link><pubDate>Fri, 25 Sep 2026 00:00:00 +0000</pubDate><guid>https://lelain.net/publications/aurora-ssl/</guid><description>&lt;p&gt;Preprint posted on arXiv on September 25, 2026, and submitted to IEEE ICASSP 2027. A joint work with the Royal Belgian Institute for Space Aeronomy, based on the ASIS archive of auroral spectra acquired in Skibotn, Norway.&lt;/p&gt;
&lt;p&gt;This work follows the supervised study presented at
, where a 1D Vision Transformer was trained on 719 expert-annotated spectra. Here, the unlabelled part of the archive (223,000 spectra) is used to pretrain the same architecture with a masked autoencoder, which raises the macro-AP from 77.8 to 88.5 on the same benchmark and shows that the learned representation encodes the emission-line ratios used by physicists, without being told about them.&lt;/p&gt;</description></item></channel></rss>