cuFFS: A GPU-accelerated code for Fast Faraday Rotation Measure Synthesis
S. S. Sridhar, G. Heald, and J. M. van der Hulst

TL;DR
cuFFS is a GPU-accelerated software that significantly speeds up Faraday Rotation Measure synthesis, enabling efficient processing of large astronomical datasets from modern radio telescopes.
Contribution
This paper introduces cuFFS, a GPU-based implementation of RM synthesis that achieves up to 100x speedup over CPU versions, optimizing large-scale polarization data analysis.
Findings
Achieves up to two orders of magnitude speedup over CPU implementations.
Supports faster HDFITS format to mitigate disk I/O bottlenecks.
Demonstrates effectiveness on large datasets from LOFAR, MWA, and SKA.
Abstract
Rotation measure (RM) synthesis is a widely used polarization processing algorithm for reconstructing polarized structures along the line of sight. Performing RM synthesis on large datasets produced by telescopes like LOFAR can be computationally intensive as the computational cost is proportional to the product of the number of input frequency channels, the number of output Faraday depth values to be evaluated and the number of lines of sight present in the data cube. The required computational cost is likely to get worse due to the planned large area sky surveys with telescopes like the Low Frequency Array (LOFAR), the Murchison Widefield Array (MWA), and eventually the Square Kilometre Array (SKA). The massively parallel General Purpose Graphical Processing Units (GPGPUs) can be used to execute some of the computationally intensive astronomical image processing algorithms including…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Geophysics and Gravity Measurements · Adaptive optics and wavefront sensing
