Helical Magnetic Structure Of EUV Polar Plumes

Details Helical Magnetic Structure Of EUV Polar Plumes Helical Magnetic Structure Of EUV Polar Plumes

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.446..675v&link_type=abstract

8th SOHO Workshop: Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona. Proceedings of the Conference hel

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The results of an analysis of joint CDS of SOHO and SXT of Yohkoh observations of a decaying post-flare loop system are presented. The SXT images were used to explain some peculiar structural features visible in the examined CDS raster, resulting from the rapid evolution of the observed system and from the way the CDS rasters are built. The SXT data was also used to determine the time evolution of the temperature and the emission measure of the hot part of the system during its decay. The CDS data, with a very good temperature coverage, contains a density sensitive line pair of Fe XIV which was used for electron density analysis and a temperature sensitive line pair of Fe XVI and Si XII which was used to study the temperature structure of the loop system. From the integrated intensities of selected lines the emission measures were calculated. From these measurements we estimated the filling factor of the loop system in Fe XIV line.

Affiliated with

Also associated with

No associations

Rating

Helical Magnetic Structure Of EUV Polar Plumes 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 Helical Magnetic Structure Of EUV Polar Plumes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Helical Magnetic Structure Of EUV Polar Plumes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1084968