Bursts of Explosive Events in the Solar Network

Details Bursts of Explosive Events in the Solar Network Bursts of Explosive Events in the Solar Network

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997soph..175..341i&link_type=abstract

Solar Physics, Volume 175, Issue 2, pp.341-348

Physics

47

Scientific paper

Observations of the quiet-Sun network in the UV emission line Siiv 1393 Å over a time period of two hours are presented. Bursts of explosive events, highly Doppler-shifted emission, seem to be sporadically emitted from the brighter regions of the network lanes. Individual events have typical lifetimes of ≈ 1 6 min and come in bursts of up to 30 min. The most spectacular burst in this dataset, shown in the accompanying movie, lasts ≈ 30 min and shows a wide variety of line profiles with both red and blue shifts ≈180 km s1. There appears to be no characteristic form or evolutionary pattern to the line profiles in either the individual events or series of events. There are about twice as many blue shifts as red shifts.

Affiliated with

Also associated with

No associations

Rating

Bursts of Explosive Events in the Solar Network 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 Bursts of Explosive Events in the Solar Network, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bursts of Explosive Events in the Solar Network will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1158050