Difference between revisions of "STIX data center"

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(Flare identification)
(Flare identification)
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===  Flare  identification ===
 
===  Flare  identification ===
 
Quick-look light curves are used for flare identification.  Identifications of flares consists of several steps as follows:
 
Light curves are smoothed by using average filtering in order to filter spikes from the electronics and fluctuations due to the on-board integer compression.
 
Then, light curves acquired during the quiet sun periods are selected for background estimation. 
 
We take  median values and standard deviations of a certain number of data points (typically 1500 points) as the background level.
 
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 15:13, 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 identification

4 Source code

The source code can be found at:

5 Developers