A high-precision interpolation method for pulsed radio signals from cosmic-ray air showers

التفاصيل البيبلوغرافية
العنوان: A high-precision interpolation method for pulsed radio signals from cosmic-ray air showers
المؤلفون: Corstanje, A., Buitink, S., Desmet, M., Falcke, H., Hare, B. M., Hörandel, J. R., Huege, T., Jhansi, V. B., Karastathis, N., Krampah, G. K., Mitra, P., Mulrey, K., Nelles, A., Nivedita, K., Pandya, H., Scholten, O., Terveer, K., Thoudam, S., Trinh, G., ter Veen, S.
المصدر: JINST 18 P09005, 2023
سنة النشر: 2023
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics - Instrumentation and Methods for Astrophysics
الوصف: Analysis of radio signals from cosmic-ray induced air showers has been shown to be a reliable method to extract shower parameters such as primary energy and depth of shower maximum. The required detailed air shower simulations take 1 to 3 days of CPU time per shower for a few hundred antennas. With nearly $60,000$ antennas envisioned to be used for air shower studies at the Square Kilometre Array (SKA), simulating all of these would come at unreasonable costs. We present an interpolation algorithm to reconstruct the full pulse time series at any position in the radio footprint, from a set of antennas simulated on a polar grid. Relying on Fourier series representations and cubic splines, it significantly improves on existing linear methods. We show that simulating about 200 antennas is sufficient for high-precision analysis in the SKA era, including e.g. interferometry which relies on accurate pulse shapes and timings. We therefore propose the interpolation algorithm and its implementation as a useful extension of radio simulation codes, to limit computational effort while retaining accuracy.
Comment: 21 pages, 14 figures. Accepted for publication in JINST (Journal of Instrumentation)
نوع الوثيقة: Working Paper
DOI: 10.1088/1748-0221/18/09/P09005
URL الوصول: http://arxiv.org/abs/2306.13514
رقم الأكسشن: edsarx.2306.13514
قاعدة البيانات: arXiv
الوصف
DOI:10.1088/1748-0221/18/09/P09005