Time variability of coronal funnels

Details Time variability of coronal funnels Time variability of coronal funnels

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.505..215b&link_type=abstract

In: SOLMAG 2002. Proceedings of the Magnetic Coupling of the Solar Atmosphere Euroconference and IAU Colloquium 188, 11 - 15 Jun

Computer Science

Sun: Chromosphere, Sun: Corona, Sun: Transition Region, Sun: Uv Radiation

Scientific paper

Transition region spectra from the network are commonly composed by two components: a narrow one from smaller loops and a broad tail component that can be interpreted as originating from coronal funnels. We present a time series analysis of tail components for one network region. A comparison of fitted spectra obtained by applying running means with full time resolution spectra shows that typical explosive events are not responsible for the observed tail components. The correlation between core and tail intensities on time-scales of minutes is not significant.

Affiliated with

Also associated with

No associations

Rating

Time variability of coronal funnels 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 Time variability of coronal funnels, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Time variability of coronal funnels will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1422473