Rucio is a software framework that provides functionality to organize, manage, and access large volumes of scientific data using customisable policies. The data can be spread across globally distributed locations and across heterogeneous data centers, uniting different storage and network technologies as a single federated entity. Rucio offers advanced features such as distributed data recovery or adaptive replication, and is highly scalable, modular, and extensible. Rucio has been originally developed to meet the requirements of the high-energy physics experiment ATLAS, and is continuously extended to support LHC experiments and other diverse scientific communities.
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Important Travel Advisory: In particular, we’d like to ask you to connect remotely if you are traveling from, transiting through or have visited in the last 14 days, the following countries:
We sincerely apologize for the inconvenience this will cause. |
For the 3nd Rucio Community Workshop we will meet at the Fermilab LPC (LHC Physics Center), close to Chicago, USA. The Workshop will be devoted to the information exchange between the Rucio developers, service administrators and the various interested communities in order to collect feedback and requirements.
On Monday March 9th there will be a WLCG DOMA Face to Face meeting at Fermilab.
On Thursday/Friday March 12-13, directly after the workshop, there will be a Rucio Coding Camp for Rucio developers and people interested in Rucio development.
We set up a mailing list to which you can subscribe and where we will send more details about the program in the coming weeks.
We also created a Slack channel dedicated to the workshop discussion on the Rucio Slack workspace (Invitation Link). Join #workshop.
All participants must follow Fermilab's code of conduct:
http://directorate-docdb.fnal.gov/cgi-bin/RetrieveFile?docid=174
We would really appreciate if you could fill the following participants feedback form whether you attended this workshop live or offline, it will help us improve the LPC events offering:
