<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>https://pub023.cs.technik.fhnw.ch/wiki/index.php?action=history&amp;feed=atom&amp;title=STIX_flare_processing_pipeline</id>
	<title>STIX flare processing pipeline - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://pub023.cs.technik.fhnw.ch/wiki/index.php?action=history&amp;feed=atom&amp;title=STIX_flare_processing_pipeline"/>
	<link rel="alternate" type="text/html" href="https://pub023.cs.technik.fhnw.ch/wiki/index.php?title=STIX_flare_processing_pipeline&amp;action=history"/>
	<updated>2026-05-01T20:18:13Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.31.1</generator>
	<entry>
		<id>https://pub023.cs.technik.fhnw.ch/wiki/index.php?title=STIX_flare_processing_pipeline&amp;diff=15835&amp;oldid=prev</id>
		<title>Hualin: Created page with &quot;Solar flare processing pipeline   Select  L1 bulk science data from the database.  For each selected flare * Check if  peak counts above a given value (e.g. 600) using the fla...&quot;</title>
		<link rel="alternate" type="text/html" href="https://pub023.cs.technik.fhnw.ch/wiki/index.php?title=STIX_flare_processing_pipeline&amp;diff=15835&amp;oldid=prev"/>
		<updated>2021-08-19T09:38:47Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;Solar flare processing pipeline   Select  L1 bulk science data from the database.  For each selected flare * Check if  peak counts above a given value (e.g. 600) using the fla...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;Solar flare processing pipeline&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Select  L1 bulk science data from the database.  For each selected flare&lt;br /&gt;
* Check if  peak counts above a given value (e.g. 600) using the flare list database. Skip faint flares &lt;br /&gt;
* Use GOES LC to determine the GOES class, write the GOES LC to a png file, store the GOES class in the flare list database  &lt;br /&gt;
* Select background from database and do background selection&lt;br /&gt;
* Determine flare location, store location information in the database   &lt;br /&gt;
* Background subtraction for spectrograms &amp;amp; energy spectra&lt;br /&gt;
* Spectral analysis with sunspex, store results (to be done in the future …)&lt;br /&gt;
* Calculate ephemeris &amp;amp; viewing angles using spice kernel &lt;br /&gt;
* Reconstruct flare images (to be done in the future)&lt;br /&gt;
* Prepare simultaneous observation plots&lt;br /&gt;
** Create EUI image,  AIA images for the flare&lt;br /&gt;
** EPD plots&lt;br /&gt;
** Radio&lt;br /&gt;
** ...&lt;br /&gt;
 &lt;br /&gt;
&lt;br /&gt;
Results can be displayed on web pages &lt;br /&gt;
Group flares by GOES classes, dates&lt;br /&gt;
Results can be also retrieved using sdcpy&lt;/div&gt;</summary>
		<author><name>Hualin</name></author>
		
	</entry>
</feed>