Year: 2024
Type: conference-paper
Abstract: Continuous monitoring of solar radio bursts using ground spectrometers is now essential for solar researchers, particularly in predicting space weather.Type II, Type III, and Type IV solar bursts are linked to significant solar flares and coronal mass ejections (CMEs), which affect Earth's magnetosphere and human activities.Since 2002, CALLISTO spectrometers have gathered data, available at e-Callisto.org, but detecting and classifying these bursts was laborintensive.This study aims to enhance the monitoring of solar radio bursts (SRBT II, SRBT III, SRBT IV) by automating the CALLISTO system.The developed system includes three stages: burst-finder, burst-classifier, and monitoring.Tested on both pre-training and real data, it achieved 87% success in burst detection and 61% in burst classification.Results are displayed on the user-friendly website http://solar.myfik.net,providing a valuable tool for CALLISTO-based solar burst monitoring and supporting space weather forecasting research.
DOI: 10.5109/7323404
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
OpenAlex ID: W4404653654