Statistical study of CMEs, lateral overexpansion and SEP events (CROSBI ID 698703)
Prilog sa skupa u zborniku | sažetak izlaganja sa skupa | međunarodna recenzija
Podaci o odgovornosti
Alexandros Adamis ; Astrid Veronig ; Tatiana Podladchikova ; Karin Dissauer ; Rositsa Miteva ; Jingnan Guo ; Mateja Dumbović ; Manuela Temmer ; Kamen Kozarev ; Jasmina Magdalenic ; Veronika Haberle
engleski
Statistical study of CMEs, lateral overexpansion and SEP events
We present a statistical study on the early evolution of coronal mass ejections (CMEs), to better understand the effect of CME (over)- expansion and how it relates to the production of Solar Energetic Particle (SEP) events. We study the kinematic CME characteristics in terms of their radial and lateral expansion, from their early evolution in the Sun’s atmosphere as observed in EUV imagers and coronagraphs. The data covers 72 CMEs that occurred in the time range July 2010 to September 2012, where the twin STEREO spacecraft where in quasi-quadrature to the Sun-Earth line. From the STEREO point-of-view, the CMEs under study were observed close to the limb. We calculated the radial and lateral height (width) versus time profiles and derived the corresponding peak and mean velocities, accelerations and angular expansion rates, with particular emphasis on the role of potential lateral overexpansion in the early CME evolution. We find high correlations between the radial and lateral CME velocities and accelerations. CMEs which are associated to SEPs tend to be located at the high value end of the distributions of velocities, widths and expansion rates compared to non-SEP associated events.
coronal mass ejections, solar energetic particles, space weather
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Podaci o prilogu
1-1.
2020.
objavljeno
Podaci o matičnoj publikaciji
Podaci o skupu
European Space Weather Symposium
poster
02.11.2020-06.11.2020
online