2016/06/07 by Jakub Kákona, Jakub Kakona, Kakona, Jakub +5
Computer Science · Physics and Astronomy · #Computational Physics and Python Applications #FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #astro-ph.IM
paper · pdf · doi:10.48550/arxiv.1606.02052
this article supersedes 2015pimo.conf..157K
arxiv created 2016/06/07 · openalex publication_date 2016/06/07 · arxiv updated 2016/06/08 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Most of the meteor radioastronomical radars are backscatter radars which cover only a small area of the atmosphere. Therefore a daytime meteor flux models are based on sparse data collected by only a few radar systems. To solve this issue, a radar system with a wide coverage is required. We present a new approach of open-source multi-static radio meteor detection system which could be distributed over a large area. This feature allows us to detect meteor events taking place over a larger area as well and gather more uniform data about meteor flux and possibly about meteor trajectories.