Determination of intensity variations along coronal loops

Details Determination of intensity variations along coronal loops Determination of intensity variations along coronal loops

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005jastp..67.1715b&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, v. 67, iss. 17-18 [SPECIAL ISSUE], p. 1715-1719.

Physics

Scientific paper

In this work we describe dynamical features of brightenings along coronal loops using a method derived in a previous paper. We register the behavior of space and time intensity variations along a compound of coronal magnetic tubes imaged by the Transition Region and Coronal Explorer (TRACE) in the well known coronal line at 17.1 nm. The studied loops were observed in the south-west limb on October 1st, 2001. We determine a coherent behavior of the intensity along neighboring magnetic tubes. During a first time interval we register a downflow with a brightening average speed of ≈111kms and during a second time interval we detect an upward displacement of the brightening with an average speed of ≈50kms.

Affiliated with

Also associated with

No associations

Rating

Determination of intensity variations along coronal loops 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 Determination of intensity variations along coronal loops, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Determination of intensity variations along coronal loops will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1435009