Solar flares with and without SOHO/LASCO coronal mass ejections and type II shocks

Details Solar flares with and without SOHO/LASCO coronal mass ejections and type II shocks Solar flares with and without SOHO/LASCO coronal mass ejections and type II shocks

2010-09-19

arxiv.org/abs/1009.3636v1

2006AdSpR..38.1007H

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Advances in Space Research, Volume 38, Issue 5, p. 1007-1010

Scientific paper

10.1016/j.asr.2005.11.003

We analyse of a set of radio rich (accompanied by type IV or II bursts) solar flares and their association with SOHO/LASCO Coronal Mass Ejections in the period 1998 2000. The intensity, impulsiveness and energetics of these events are investigated. We find that, on the average, flares associated both with type IIs and CMEs are more impulsive and more energetic than flares associated with type IIs only (without CME reported), as well as flares accompanied by type IV continua but not type II shocks. From the last two classes, flares with type II bursts (without CMEs reported) are the shortest in duration and the most impulsive.

Affiliated with

Also associated with

No associations

Rating

Solar flares with and without SOHO/LASCO coronal mass ejections and type II shocks 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 Solar flares with and without SOHO/LASCO coronal mass ejections and type II shocks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar flares with and without SOHO/LASCO coronal mass ejections and type II shocks will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-408772