Applications of antenna-level buffering
A. Nelles, J.D. Bray, C.W. James (SKA Focus Group: High Energy Cosmic, Particles)

TL;DR
This paper discusses how antenna-level buffering in SKA-LOW enables scientific research and engineering tasks like calibration, RFI localization, and hardware diagnostics, based on experiences with various radio telescopes.
Contribution
It introduces the practical applications of antenna-level buffering in radio astronomy, highlighting its benefits for calibration, RFI detection, and hardware troubleshooting.
Findings
Antenna-level buffers aid in antenna calibration.
Buffers help localize radio frequency interference.
They assist in diagnosing hardware issues.
Abstract
The purpose of this document is to discuss applications of the antenna-level buffering capability being implemented in SKA-LOW. In addition to their scientific motivation -- to detect and study cosmic rays interacting in the atmosphere -- these buffers provide access to low-level data for engineering and development work. Experience has shown that antenna-level buffered data can assist with antenna calibration, localising RFI, and diagnosing fundamental hardware problems. In this document, we describe several of these applications, with close reference to experience with LOFAR, ACTA, Parkes, and the OVRO-LWA.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsRadio Astronomy Observations and Technology · Astrophysics and Cosmic Phenomena · Scientific Research and Discoveries
