Pregled bibliografske jedinice broj: 478832
Timing relationship between CME and the prominence events (kinematics of the three part structure)
Timing relationship between CME and the prominence events (kinematics of the three part structure) // Proceedings of International Symposium Forges 2008, Forecasting of the Radiation and Geomegnetic Storms by networks of particle detectors, Nor Amberd, Armenia, 29 September- October 3, 2008 / A. Chilingarian (ur.).
Erevan: Cosmic Ray Division, Alikhanyan Physics Institute, 2009. str. 23-27 (poster, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
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Naslov
Timing relationship between CME and the prominence events (kinematics of the three part structure)
Autori
Maričić, Darije ; Vršnak, Bojan ; Roša, Dragan
Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni
Izvornik
Proceedings of International Symposium Forges 2008, Forecasting of the Radiation and Geomegnetic Storms by networks of particle detectors, Nor Amberd, Armenia, 29 September- October 3, 2008
/ A. Chilingarian - Erevan : Cosmic Ray Division, Alikhanyan Physics Institute, 2009, 23-27
ISBN
99941-0-165-X
Skup
Forges 2008, Forecasting of the Radiation and Geomegnetic Storms by networks of particle detectors
Mjesto i datum
Amberd, Armenija, 29.09.2008. - 03.10.2008
Vrsta sudjelovanja
Poster
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
Sun: Coronal mass ejection (CMEs)
Sažetak
We present a statistical analysis of the relationship between the acceleration of the leading edge of coronal mass ejections (CMEs) and eruptive prominences (EPs). We study the main acceleration phase of 18 CMEs in which kinematics was measured from the pre-eruption stage up to the post-acceleration phase using the data provided by the Extreme Ultraviolet Imaging Telescope, the Mark-IV K-coronameter of the Mauna Loa Solar Observatory, and the Large Angle and Spectrometric Coronagraph. We find a distinct correlation between the duration of the leading edge acceleration phase and prominence acceleration phase. In the majority of events (78%) the acceleration phase of the leading edge is very closely synchronized with the acceleration of the prominence (±20 min). However, in two events acceleration of the leading edge started earlier than the acceleration of the prominence (>50 min), and in two events prominence acceleration started earlier than the acceleration of the leading edge (>40 min).
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
007-0000000-1362 - Eruptivni procesi u Sunčevoj atmosferi
Ustanove:
Geodetski fakultet, Zagreb