A fully autonomous data center for the space-borne hard X-ray Compton polarimeter POLAR developed at PSI
Hualin Xiao, Wojtek Hajdas, Radaslow Marcinkowski

TL;DR
This paper describes the design and implementation of a fully autonomous data center at PSI for processing, storing, and analyzing the large volume of data generated by the space-borne POLAR X-ray polarimeter, enabling efficient space data management.
Contribution
It introduces a novel fully automated data center specifically developed for the POLAR space mission, integrating hardware and software for real-time data processing and alerting.
Findings
Successful handling of up to 50 GB daily telemetry data
Implementation of automated data processing and alerting systems
Enhanced data management for space-borne X-ray polarimetry
Abstract
POLAR is a space-borne hard X-ray Compton polarimeter built by a collaboration of institutes from Switzerland, China and Poland. Precise detection of the polarization can be a powerful tool to unveil emission mechanisms of e.g. Gamma-Ray Bursts (GRB) or Solar Flares (SF). POLAR is equipped with an array of 1600 scintillator bars dimensioned for precise measurements of the polarization of hard X-rays in the energy range from 50 keV to 500 keV. The instrument was launched into space on September 15th, 2016 on-board the Chinese Space Laboratory TG-2 for up to 3 years long observation period. Telemetry data from its operation in space may reach up tp 50 GB daily. To store and process such a huge amount of data both dedicated hardware and specialized software are required. Moreover, constant data inflow also requires a fully automated and safeguarded data processing. For this purpose, a…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsParticle Detector Development and Performance · Gamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena
