Title :
The relation between solar radio burst types II, III and IV due to solar activities
Author :
N. Ramli;Z. S. Hamidi;Z. Z. Abidin;S. N. Shahar
Author_Institution :
Department of Physics, Faculty of Science, University Malaya, 50603 Kuala Lumpur, Malaysia
Abstract :
Solar radio burst becoming an interesting topic among solar physicists in order to study the Space Weather condition. It generally originate at the same level as solar flare, Coronal Mass Ejection (CME) and shock at solar atmosphere which the Sun project the radio energy into the interstellar medium. In this study, the relation between solar radio burst type II, III and IV due to active region AR2157 and AR2158 was investigate. This study was carried out using the data from e-Callisto and was detected that solar radio burst type II, type III and type IV occurred on 10th September 2014 from 17:28 UT until 17:45 UT. The solar burst emission is associated with X1.6 class solar flare which occurred at sunspot AR2157 and AR2158 at 17:21 UT were observed from NOAA. We also compared with other events such as CME and geomagnetic storm that is potentially associated with this three bursts to show their importance role on space weather studies.
Keywords :
"Sun","Storms","Earth","US Government agencies","Plasmas","Time-frequency analysis"
Conference_Titel :
Space Science and Communication (IconSpace), 2015 International Conference on
Electronic_ISBN :
2165-431X
DOI :
10.1109/IconSpace.2015.7283756