Abstracts Details


First Name * : Nur Amira
Last Name * : Mohd Norsham
Affiliation * : Universiti Teknologi MARA
Abstract Type * : Poster
Title * : An Analysis on the Formation of Solar Radio Burst Type II, III and IV by Using e-CALLISTO and Space Weather Data
Author(s) * : Nur Amira Mohd Norsham, Zety Sharizat Hamidi
Abstract Session * : Solar flares and coronal mass ejections
Abstract * : 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 between these three types of solar radio burst can be studied. The necessary data were collected from the free online websites which include the Space Weather and e-CALLISTO Website. 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. From all the data collected on 30th March 2018 and 31st March 2018, it shows that even the Sun is not active (in terms of the production of the sunspot), we can still get the data which indicates that the sun, somehow, is active for the production of the flares and Coronal Mass Ejection.