• Veerendra Singh
• Lavkush Kumar

In this paper we have made a comprehensive statistical study on the CMEs associated with prominence eruptions. A total number of 576 prominence eruptions observed by Nobeyama Radioheliograph during the period January, 1996 to December, 2013. We have studied the distribution of CMEs speed, angular width and acceleration for prominence eruptions associated CMEs. The median (average) linear speed is 492 (521) km/sec. The mean angular width is 770. Majority of events is accelerating. On studying the speed-acceleration correlation for these events we found there is no correlation between them. The number variation during solar cycle of prominence activities is similar to that of sunspots. The fraction of prominence eruptions associated CMEs during the solar minimum is less than that during solar maximum. We have also studied the mass, energy and latitudinal distribution of prominence eruptions associated CMEs.

Sun; Coronal Mass Ejections; Prominence Eruptions; Solar cycle

"On Statistical Properties of CMEs Associated with Prominence Eruption", International Journal of Emerging Technologies and Innovative Research (www.jetir.org), ISSN:2349-5162, Vol.3, Issue 4, page no.1952-1958, April-2016, Available :http://www.jetir.org/papers/JETIR1701691.pdf

"On Statistical Properties of CMEs Associated with Prominence Eruption", International Journal of Emerging Technologies and Innovative Research (www.jetir.org | UGC and issn Approved), ISSN:2349-5162, Vol.3, Issue 4, page no. pp1952-1958, April-2016, Available at : http://www.jetir.org/papers/JETIR1701691.pdf