An Analysis on the Formation of Solar Radio Burst Type II, III and IV by Using e-CALLISTO, IUGONET and Space Weather Data

• Published in: Journal of Physics: Conference Series
• Main Author: Norsham N.A.M.; Hamidi Z.S.
• Format: Conference paper
• Language: English
• Published: Institute of Physics Publishing 2019
• Online Access: https://www.scopus.com/inward/record.uri?eid=2-s2.0-85073608502&doi=10.1088%2f1742-6596%2f1298%2f1%2f012018&partnerID=40&md5=8f1b5fa7c69aa7004f71c0f568e061e8

The study of the radio solar burst data on 30th March 2018 and 31st March 2018 are essential for the understanding of type II, type III and type IV nature. Through this paper, the relationship of these three types of solar radio burst can be studied. The necessary data were collected from the free online websites which includes the Space Weather Website, e-CALLISTO and IUGONET metadata database. From this study, the occurrence of solar radio burst type II, III, and IV showed that there was the production of solar flares and Coronal Mass Ejections (CMEs) where it contributed to the geomagnetic disturbances to the Earth. On 30th March 2018, the Sun produced C-class flares with C4 value while the next day, the sun had B1 solar flares' event. The planetary K-index for both days were 2 (30th March 2018) and 3 (31st March 2018) respectively. © Published under licence by IOP Publishing Ltd.