The EOSC-Synergy cloud services implementation for the Latin American Giant Observatory (LAGO)
| Autor: | Rubio-Montero, Antonio Juan, Pagán-Muñoz, Raúl, Mayo-García, Rafael, Pardo-Diaz, Alfonso, Sidelnik, Iván, Asorey, Hernán |
|---|---|
| Rok vydání: | 2021 |
| Předmět: | |
| Zdroj: | in Proceedings of 37th International Cosmic Ray Conference - PoS(ICRC2021) (Berlin, Germany - Online: Sissa Medialab), 261, https://pos.sissa.it/395/261 (2021) |
| Druh dokumentu: | Working Paper |
| DOI: | 10.22323/1.395.0261 |
| Popis: | The Latin American Giant Observatory (LAGO) is a distributed cosmic ray observatory at a regional scale in Latin America, by deploying a large network of Water Cherenkov detectors (WCD) and other astroparticle detectors in a wide range of latitudes from Antarctica to M\'exico, and altitudes from sea level to more than 5500 m a.s.l. Detectors telemetry, atmospherics conditions and flux of secondary particles at the ground are measured with extreme detail at each LAGO site by using our own-designed hardware and firmware (ACQUA). To combine and analyse all these data, LAGO developed ANNA, our data analysis framework. Additionally, ARTI, a complete framework of simulations designed to simulate the expected signals at our detectors coming from primary cosmic rays entering the Earth atmosphere, allowing a precise characterization of the sites in realistic atmospheric, geomagnetic and detector conditions. As the measured and synthetic data started to flow, we are facing challenging scenarios given a large amount of data emerging, performed on a diversity of detectors and computing architectures and e-infrastructures. These data need to be transferred, analyzed, catalogued, preserved, and provided for internal and public access and data-mining under an open e-science environment. In this work, we present the implementation of ARTI at the EOSC-Synergy cloud-based services as the first example of LAGO' frameworks that will follow the FAIR principles for provenance, data curation and re-using of data. For this, we calculate the flux of secondary particles expected in up to 1 week at detector level for all the 26 LAGO, and the 1-year flux of high energy secondaries expected at the ANDES Underground Laboratory and other sites. Therefore, we show how this development can help not only LAGO but other data-intensive cosmic rays observatories, muography experiments and underground laboratories. Comment: [30Dic21. No changes in the paper. Corrected mistake in ArXiv' metadata: swapping given name order: Juan Antonio Rubio-Montero -> Antonio Juan Rubio-Montero] |
| Databáze: | arXiv |
| Externí odkaz: |
|