Pierre Auger Computing

Located in western Argentina, the Pierre Auger Observatory is studying
extensive cosmic ray air showers over an area of 3,000 square kilometers. These
showers are generated by particles with far higher energies than any ground-based accelerator can reach, and they continue to challenge our
understanding. The strategy behind the design of the Pierre Auger
Observatory is to study showers through detecting not only the
particles, with an array of 1600 water Cherenkov detectors, but also
the fluorescence light, using four stations, each with six telescopes
overlooking the particle detectors.
The Computing Division supports the Pierre Auger experiment in the
following areas:
1. Maintenance and support of the augerd1.fnal.gov data server
This server, along with the Fermilab BlueArc disk server, holds a copy
of the raw and reconstructed data taken by the experiment, as the
North America data mirror. We are currently "rsync"ed to the computing
center in Lyon, France. This server also acts as the database server
for Offline calibration and monitoring. Database scripts are running
daily to update tables from a few expert sites, such as Karlsruhe,
Germany, Boston and Colorado.
2. Support desktop system for analysis
The Auger group at Fermilab
is actively participating in the study of systematics associated with
the determination of the total cross section measurement of
proton-nucleus at energies exceeding the LHC energy, by a factor ~300.
We are also involved with the study of (putative) anisotropy in
Galactic Center and other point like sources.
More Information: Pierre Auger Observatory Home
Send comments about this page via the suggestion form
Last updated by cdweb on 04/29/2008
|