Statistical Analysis of Decimetric Radio Bursts, Flares, and Coronal Mass Ejections

Details Statistical Analysis of Decimetric Radio Bursts, Flares, and Coronal Mass Ejections Statistical Analysis of Decimetric Radio Bursts, Flares, and Coronal Mass Ejections

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009soph..257..113m&link_type=abstract

Solar Physics, Volume 257, Issue 1, pp.113-124

Physics

Sun: Solar Activity, Sun: Radio Bursts

Scientific paper

A statistical analysis of decimetric radio bursts (RBs), X-ray flares and coronal mass ejections (CMEs) is carried out. We consider all radio bursts recorded by the Cracow Solar Radio Telescope from the beginning of 1996 until the end of 2004. It is found that the decimetric radio bursts are associated and strongly correlated with X-ray flares. Correlation coefficients between RBs durations and the maximal fluxes of the radio bursts and flares are found to be 0.60 and 0.87, respectively. We also demonstrated that a significant population of the decimetric radio bursts are associated with CMEs. The correlation coefficient between the maximal radio flux density multiplied by the duration of the RBs versus velocity multiplied by width of CMEs is found to be 0.55.

Affiliated with

Also associated with

No associations

Rating

Statistical Analysis of Decimetric Radio Bursts, Flares, and Coronal Mass Ejections does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Statistical Analysis of Decimetric Radio Bursts, Flares, and Coronal Mass Ejections, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Statistical Analysis of Decimetric Radio Bursts, Flares, and Coronal Mass Ejections will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-860333