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elopment and commissioning of a completely new facilitywith such requirements is economically unwarranted and time-consuming, the global n analysis goals are achievable when all types of existing detectors are merged into a worldwide network. The idea to use the instruments in operation is based on a novel trigger algorithm: in parallel to looking for neighbour surface detectors receiving the signal simultaneously, one should also look for spatially i solated stations clustered in a small time window. On the other hand, CREDO strategy is also aimed at an active engagem ent of a large number of participants, who will contribute to the project by using common electronic devices (e.g., smartphones), capable of detecting cosmic rays. It will help not only in expanding the geographical spread of
CREDO, but also in managing a large manpowernecessary for a more efficient crowd-sourced pattern recognition scheme to identify and classify SPS. A worldwidenetwork of cosmic-ray detectors could not only become a unique tool to study fundamental physics, it will also
provide a number of other opportunities, including space-weather or geophysics studies. Among the latter one hasto list the potential to predict earthquakes by monitoring the rate of low energy cosmic-ray events. The diversity of goals motivates us to advertise this concept across the astroparticle physics community. <ref>https://arxiv.org/pdf/1709.05230.pdf</ref><ref>http://inspirehep.net/record/1623988/plots</ref><ref>https://icd.desy.de/e49245/</ref><ref>http://www.intibs.pl/en/seminars/current-seminars/seminar/1002.html</ref><ref>http://www.oa.uj.edu.pl/2017czastki/homola.pdf</ref>
== Application credo ==
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