Coronal mass ejections associated with LDE flares of slow rise phase

Details Coronal mass ejections associated with LDE flares of slow rise phase Coronal mass ejections associated with LDE flares of slow rise phase

2011-04-05

arxiv.org/abs/1104.0846v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Accepted for publication in Central European Astrophysical Bulletin

Scientific paper

It is well known, that there is temporal relationship between CMEs and associated flares. The duration of the acceleration phase is related to the duration of the rise phase of a flare. We investigated CMEs associated with long duration flares of slow rise phase (slow LDE). These CMEs are characterized by high velocity (v>1000 km/s) during the propagation phase and low average acceleration during the main, prolongated, acceleration phase. The CMEs are accelerated until the height $> 5 R_\odot$, which is higher value than in typical impulsive CMEs. CMEs associated with slow LDEs have characteristics of both classes of CMEs, i.e. CMEs associated with flares and CMEs associated with eruptive prominences.

Affiliated with

Also associated with

No associations

Rating

Coronal mass ejections associated with LDE flares of slow rise phase 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 Coronal mass ejections associated with LDE flares of slow rise phase, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Coronal mass ejections associated with LDE flares of slow rise phase will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-321423