Title of article
CME–flare association during the 23rd solar cycle Original Research Article
Author/Authors
A. Mahrous، نويسنده , , M. Shaltout، نويسنده , , M.M. Beheary، نويسنده , , R. Mawad، نويسنده , , M. Youssef، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2009
Pages
4
From page
1032
To page
1035
Abstract
The relation between coronal mass ejections (CMEs) and solar flares are statistically studied. More than 10,000 CME events observed by SOHO/LASCO during the period 1996–2005 have been analyzed. The soft X-ray flux measurements provided by the Geostationary Operational Environmental Satellite (GOES), recorded more than 20,000 flares in the same time period. The data is filtered under certain temporal and spatial conditions to select the CME–flare associated events. The results show that CME–flare associated events are triggered with a lift-off time within the range 0.4–1.0 h. We list a set of 41 CME–flare associated events satisfying the temporal and spatial conditions. The listed events show a good correlation between the CME energy and the X-ray flux of the CME–flare associated events with correlation coefficient of 0.76.
Keywords
Solar flares , Solar wind , Coronal mass ejections
Journal title
Advances in Space Research
Serial Year
2009
Journal title
Advances in Space Research
Record number
1132596
Link To Document