Difference between revisions of "STIX data center"
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=== Flare identification === | === Flare identification === | ||
− | + | 4-10 keV quick-look light curves are used for flare identification. | |
− | 4 | ||
Identifications of flares consists of several steps as follows: | Identifications of flares consists of several steps as follows: | ||
− | * Light curve smoothing. 4-sec time bins are rebinned to 1 minute time bins in order to filter spikes from the electronics and fluctuation due to statistics and the on-board integer compression; | + | * Light curve smoothing. 4-sec time bins are rebinned to 1 minute |
− | * Background estimation. The light curves acquired during sun quiet periods are | + | time bins in order to filter spikes from the electronics and fluctuation due to statistics and the on-board integer compression; |
+ | * Background estimation. The light curves acquired during sun quiet periods are selected for background estimation. | ||
* | * | ||
Revision as of 12:16, 6 July 2021
This page is still under construction.
STIX data center is a virtual server hosted at FHNW.
Contents
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:
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
4-10 keV quick-look light curves are used for flare identification. Identifications of flares consists of several steps as follows:
- Light curve smoothing. 4-sec time bins are rebinned to 1 minute
time bins in order to filter spikes from the electronics and fluctuation due to statistics and the on-board integer compression;
- Background estimation. The light curves acquired during sun quiet periods are selected for background estimation.
The smoothed light curves have time bins of 1 minute. Those during the quiet period of the sun. to calculate the background Quick-look light curves are used for flare identification.
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:
- Data processing pipeline: https://github.com/i4Ds/STIX_python_PUB023
- STIX data center web applications: https://github.com/i4Ds/STIX-data-center
5 Developers
- Data processing software & data processing pipeline developers
- Data center