TY - JOUR
T1 - Association between Tornadoes and Instability of Hosting Prominences
AU - Mghebrishvili, Irakli
AU - Zaqarashvili, Teimuraz B.
AU - Kukhianidze, Vasil
AU - Kuridze, David
AU - Tsiklauri, David
AU - Shergelashvili, Bidzina M.
AU - Poedts, Stefaan
PY - 2018/7/11
Y1 - 2018/7/11
N2 - We studied the dynamics of all prominence tornadoes detected by the Solar Dynamics Observatory/Atmospheric Imaging Assembly from 2011 January 01 to December 31. In total, 361 events were identified during the whole year, but only 166 tornadoes were traced until the end of their lifetime. Out of 166 tornadoes, 80 (48%) triggered CMEs in hosting prominences, 83 (50%) caused failed coronal mass ejections (CMEs) or strong internal motion in the prominences, and only 3 (2%) finished their lifetimes without any observed activity. Therefore, almost all prominence tornadoes lead to the destabilization of their hosting prominences and half of them trigger CMEs. Consequently, prominence tornadoes may be used as precursors for CMEs and hence for space weather predictions
AB - We studied the dynamics of all prominence tornadoes detected by the Solar Dynamics Observatory/Atmospheric Imaging Assembly from 2011 January 01 to December 31. In total, 361 events were identified during the whole year, but only 166 tornadoes were traced until the end of their lifetime. Out of 166 tornadoes, 80 (48%) triggered CMEs in hosting prominences, 83 (50%) caused failed coronal mass ejections (CMEs) or strong internal motion in the prominences, and only 3 (2%) finished their lifetimes without any observed activity. Therefore, almost all prominence tornadoes lead to the destabilization of their hosting prominences and half of them trigger CMEs. Consequently, prominence tornadoes may be used as precursors for CMEs and hence for space weather predictions
KW - Sun: atmosphere
KW - Sun: filaments, prominences
KW - Sun: oscillations
U2 - 10.3847/1538-4357/aac823
DO - 10.3847/1538-4357/aac823
M3 - Article
SN - 0004-637X
VL - 861
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 112
ER -