Difference between revisions of "STIX data center"

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(Flare detection)
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The 4-10 keV light curves are used for flare detection.  
 
The 4-10 keV light curves are used for flare detection.  
 
4-sec time bins are first rebinned to 1-min time bins in order to  
 
4-sec time bins are first rebinned to 1-min time bins in order to  
smooth light curves. Then  
+
smooth light curves. Then the smoothed light curves are used
 
+
to search for peaks.
 
+
A flare is considered being detected if a
 
+
peak satisfies several conditions as follows:
 +
* The peak counts is above 2 sigma of the background.
  
 
== Source code ==
 
== Source code ==

Revision as of 07:57, 6 July 2021

This page is still under construction.

STIX data center is a virtual server hosted at FHNW.

1 STIX Data Center tasks

Its tasks include

  • Process STIX raw data & produce high level data products
  • Monitor Data quality and instrument health status
  • Provide data products and data browsing tools for the Solar Physics Community
  • Support STIX operations
  • Data archiving

2 STIX data center architecture

The data flow at STIX data center is shown in the picture below:

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Data processing SW mainly written in python. NoSQL DB (MongoDB) used to stored telemetry packets, file metadata and configurations

3 Key Algorithms

3.1 Offline flare location solution

3.2 Flare detection

The 4-10 keV light curves are used for flare detection. 4-sec time bins are first rebinned to 1-min time bins in order to smooth light curves. Then the smoothed light curves are used to search for peaks. A flare is considered being detected if a peak satisfies several conditions as follows:

  • The peak counts is above 2 sigma of the background.

4 Source code

The source code can be found at:

5 Developers