Data management at the Oulu cosmic ray station
|Author:||Poluianov, Stepan1,2; Usoskin, Ilya1,2; Ibragimov, Askar3|
1Sodankylä Geophysical Observatory, University of Oulu, Finland
2Space Physics and Astronomy Research Unit, University of Oulu, Finland
3Independent researcher, Helsinki, Finland
|Online Access:||PDF Full Text (PDF, 0.6 MB)|
|Persistent link:|| http://urn.fi/urn:nbn:fi-fe2021062339690
|Publish Date:|| 2021-06-23
With the recent electronics upgrade of Antarctic neutron monitors (NMs) DOMC and DOMB in 2019, the Oulu cosmic ray station (Sodankylä Geophysical Observatory, Finland) receives a significantly larger amount of data than before. This has led to a need for an important upgrade of the configuration of servers working at the station. The new configuration has three types of servers: a web-server, a datamaster server and data acquisition machines. The web-server provides a user interface for services of the station: the main website, the GLE database and other services. The datamaster is the main server, which stores all data in raw files and a database. Data acquisition machines are computers that directly receive data from the instruments and send the files farther to the datamaster server. This work describes technical details of the cosmic ray station setup providing reliable and secure data acquisition, handling and publication.
Cosmic ray studies with neutron detectors
|Volume:||2021 : 1|
|Pages:||205 - 207|
Proceedings of NMDB@Home 2020
NMDB@Home : virtual symposium on cosmic ray studies with neutron detector
|Type of Publication:||
B3 Article in conference proceedings
|Field of Science:||
115 Astronomy and space science
The work was partly supported by FINNARP and Academy of Finland (projects 264378 CRIPA, 304435 CRIPA-X, ReSoLVE and 321882 ESPERA).
|Academy of Finland Grant Number:||
264378 (Academy of Finland Funding decision)
304435 (Academy of Finland Funding decision)
321882 (Academy of Finland Funding decision)
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