Abstract

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.

Keywords

solar radio burst, radio frequencies, separate interference signals, solar flares