Behavior of transition-region lines during impulsive solar flares

Details Behavior of transition-region lines during impulsive solar flares Behavior of transition-region lines during impulsive solar flares

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86..159t&link_type=abstract

(Japan Society for the Promotion of Science and National Science Foundation, U.S.-Japan Seminar on the Recent Advances in the Un

Physics

3

Chromosphere, Coronal Loops, Solar Flares, Solar Spectra, Sunspots, Energy Transfer, Solar Maximum Mission, Solar X-Rays, Ultraviolet Spectra

Scientific paper

The emissions observed in lines originating in the transition-region plasma, particularly during impulsive flares, are investigated using data collected by the Ultraviolet Spectrometer and Polarimeter on the Solar Maximum Mission. Data concerning lines from ions such as Si II, C IV, Si IV, O V, and Fe XXI are analyzed. Topics examined include the transition region away from sunspots, oscillatory motions above sunspots, the shape of the transition region, the transition region during flares, and O V and Fe XXI during flare flash phases.

Affiliated with

Also associated with

No associations

Rating

Behavior of transition-region lines during impulsive solar flares 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 Behavior of transition-region lines during impulsive solar flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Behavior of transition-region lines during impulsive solar flares will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1628960