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An investigation of the causal relationship between sunspot groups and coronal mass ejections (CMEs)
; Gani Caglar Coban - Canakkale Onsekiz Mart University, Turkey; Huseyin Huseyin Cavus - Canakkale Onsekiz Mart University, Turkey
The initiation of Coronal mass ejections (CMEs) is one of the major solar events that has not been fully modelled yet. The causal relationship between the sunspot groups and the CMEs can be uncovered by identifying the sunspot groups that are present at the base of the large scale magnetic loops that can distort or undergo magnetic reconnection which as a consequence result in CMEs. For this purpose, NASA’s SOHO mission’s Large Angle and Spectroscopic Coronagraph (LASCO) and magnetic doppler imager (MDI) along with Solar Dynamics Observatory’s (SDO) Helioseismic and Magnetic Imager (HMI) can be used to identify these sunspot groups with respect to their respective CMEs. The relationship between the parameters of these identified sunspot groups with respect to the CMEs reveals the causal relationship between these two solar phenomena. In this study we have identified these sunspot groups and related them to the CMEs with the help of a custom written code. Moreover, a machine learning technique using K-means for classification is being developed to find these causal relationships in the identified sunspot groups with their respective CMEs. This study in this manner can provide insight into the initiation of the CMEs.
16 July 2020
Abstract submission opens:
16 July 2020
European Space Weather Medals:
6 September 2020
25 September 2020
Registration deadline: [extended]
10 October 2020
Abstract submission deadline:
4 September 2020