IceCube experience using XRootD-based Origins with GPU workflows in PNRP

¹ University of Wisconsin–Madison, Madison, WI 53715, USA
² University of California San Diego, La Jolla, CA 92093, USA
³ University of Nebraska-Lincoln, Lincoln, NE 68588, USA

^* Corresponding author: david.schultz@icecube.wisc.edu

Published online: 6 May 2024

Abstract

The IceCube Neutrino Observatory is a cubic kilometer neutrino telescope located at the geographic South Pole. Understanding detector systematic effects is a continuous process. This requires the Monte Carlo simulation to be updated periodically to quantify potential changes and improvements in science results with more detailed modeling of the systematic effects. IceCube’s largest systematic effect comes from the optical properties of the ice the detector is embedded in. Over the last few years there have been considerable improvements in the understanding of the ice, which require a significant processing campaign to update the simulation. IceCube normally stores the results in a central storage system at the University of Wisconsin–Madison, but it ran out of disk space in 2022. The Prototype National Research Platform (PNRP) project thus offered to provide both GPU compute and storage capacity to IceCube in support of this activity. The storage access was provided via XRootD-based OSDF Origins, a first for IceCube computing. We report on the overall experience using PNRP resources, with both successes and pain points.