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The Successive Ejection of Several Halo CMEs from NOAA AR. 652 July 2004, a Physical Study

Published online by Cambridge University Press:  03 June 2005

Shahinaz Yousef ,
Mostafa M. EL-Nazer  and
Aisha Bebars
Shahinaz Yousef
Affiliation:
Astronomy & Meteorology Dept, Faculty of Science, Cairo University, email: [email protected]
Mostafa M. EL-Nazer
Affiliation:
Astronomy & Meteorology Dept, Faculty of Science, Cairo University, email: [email protected]
Aisha Bebars
Affiliation:
National Research Institute of Astronomy and Geophysics, Cairo, Egypt
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Abstract

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Although we are on the descending branch of solar cycle 23, a very strong active region, NOAA 652, crossed the solar visible hemisphere during the second half of July 2004. Its very large sunspot was of beta- gamma- delta type. This active region was a source of numerous X-ray flares and coronal mass ejections. Being in a favorable position not far from the equator, it represented a threat to planet Earth particularly when near its central meridian passage.

Using EIT images, it was possible to locate the position of the 2004 July 25 CME ejection as dimming of several loops to the SW of AR 652. As usual, the CME lift up was accompanied by type IV burst and followed by type II burst and a proton flare.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: coronal mass ejections (CMEs)flaresparticle emission
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 145 - 146
Copyright
© 2005 International Astronomical Union