An algorithm for the detection of low frequency solar radio burst

Background: In this work, we develop a simple algorithm which detect major solar flares reliably and the amount of false detection cases was limited. The radio frequencies below 1000 MHz are allocated for various services. However, this frequency range also has interesting scientific aspects. The Sun is very active also these frequencies, e.g. well-known solar II and III type bursts appear in these frequencies. It is challenging to separate interference signals from real solar radio burst since these signals have quite often similar features.