Parallel Reconstruction of CLEO III Data
Gregory J. Sharp, Christopher D. Jones
Abstract
Reconstruction of one run of CLEO III raw data can take up to 9 days to complete using a single processor. This is an administrative nightmare, and even minor failures result in reprocessing the entire run, which wastes time, money and CPU power. We leveraged the ability of the CLEO III software infrastructure to read and write multiple file formats to perform reconstruction of a single run using several CPUs in parallel. Using the Sun Grid Engine and some Perl scripts, we assign roughly equal-sized chunks of events to different CPUs. The Raw data are read from an Objectivity/DB database, but the reconstruction output is written to a temporary file, not the database. This takes about 6 hours. Once all the chunks have been analyzed, they are gathered together in event-number order and injected into Objectivity/DB. This process takes an additional 6 to 18 hours, depending on run size. A web-based monitoring tool displays the status of reconstruction. Many benefits accrue from this process, including a dramatic increase in efficiency, a 20% increase in luminosity processed per week, more predictable and manageable processor farm load, reduction in the time to stop the processor farm from up to 9 days to less than 24 hours, superior fault tolerance, quicker feedback and repair times for bugs in the reconstruction code, and faster turn-around of early runs for data quality and software correctness checks.
Create a lesson
Related papers
First Observation of the Radiative Decay D0 γω
BESIII Collaboration, M. Ablikim, M. N. Achasov et al.
Hyperon--nucleon interactions at BESIII
Hong-Fei Shen
Measurement of electromagnetic transition form factors in two-photon collisions at BESIII
Max Lellmann
Measurement of Born cross sections of e+e- pK-Σ0 + c.c. at s = 3.5-4.9 GeV and partial wave analysis at s = 3.773 GeV
BESIII Collaboration, M. Ablikim, M. N. Achasov et al.
MoEDAL-MAPP: the first dedicated search experiment at the LHC
John R. Ellis, Nick E. Mavromatos, Vasiliki A. Mitsou et al.
Achieving a 0.49 keV threshold in the COSINE-100 dark matter experiment
J. Kim, N. Carlin, D. F. F. S. Cavalcante et al.