Solar mini-dimmings can be detect in the Extreme Ultra-Violet coronal eruptions. Here, sequences of 171_A images taken by Solar Dynamic Observatory/Atmospheric Imaging Assembaly on 13 June 2010 are used. In this special day, both of coronal mass ejection and prominence were observed. The average velocities and accelerations of 500 mini-dimmings which were detected using on feature based classifier (Alipour et al 2012) [1] are studied. The large number of mini-dimmings shows positive accelerations in the beginning times as similar as Coronal Mass Ejections. On the the start time of prominence eruptions, the number of mini-dimmings is increased to a maximum values. There is a positive correlation between the kinematics of mini-dimmings and both CME and prominences. This study can be extended to understand the exact relationship of CMEs and mini-dimmings.
Alipour, N., & Safari, H. (2014). Solar Mini-Dimming Kinematics and Their Positive Correlations with Coronal Mass Ejections and Prominence. Iranian Journal of Astronomy and Astrophysics, 1(1), 57-63. doi: 10.22128/ijaa.2014.5
MLA
Nasibe Alipour; Hossein Safari. "Solar Mini-Dimming Kinematics and Their Positive Correlations with Coronal Mass Ejections and Prominence", Iranian Journal of Astronomy and Astrophysics, 1, 1, 2014, 57-63. doi: 10.22128/ijaa.2014.5
HARVARD
Alipour, N., Safari, H. (2014). 'Solar Mini-Dimming Kinematics and Their Positive Correlations with Coronal Mass Ejections and Prominence', Iranian Journal of Astronomy and Astrophysics, 1(1), pp. 57-63. doi: 10.22128/ijaa.2014.5
VANCOUVER
Alipour, N., Safari, H. Solar Mini-Dimming Kinematics and Their Positive Correlations with Coronal Mass Ejections and Prominence. Iranian Journal of Astronomy and Astrophysics, 2014; 1(1): 57-63. doi: 10.22128/ijaa.2014.5
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