Green coronal intensity enhancements and their relation to the underlying photospheric/chromospheric activity

Details Green coronal intensity enhancements and their relation to the underlying photospheric/chromospheric activity Green coronal intensity enhancements and their relation to the underlying photospheric/chromospheric activity

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999soph..188...99r&link_type=abstract

Solar Physics, v. 188, Issue 1, p. 99-113 (1999).

Physics

3

Scientific paper

Analysis of the photospheric and chromospheric activity at the sites of enhanced 5303 Å coronal intensity revealed some important aspects of their association. We have examined the daily maps of 5303 Å coronal line intensity of Lomnický Štít for the low sunspot activity years 1985 and 1986 in association with the cotemporal daily maps of sunspots, plages and Stanford magnetograms and identified strong field gradients at the sites of enhanced intensity regions. We found that the peak intensity does not depend on the strength of the underlying magnetic field though the coronal intensity-enhanced feature is almost sure to occur at the locations of sunspots with strong magnetic fields and at the locations of plages having larger areas.

Affiliated with

Also associated with

No associations

Rating

Green coronal intensity enhancements and their relation to the underlying photospheric/chromospheric activity 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 Green coronal intensity enhancements and their relation to the underlying photospheric/chromospheric activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Green coronal intensity enhancements and their relation to the underlying photospheric/chromospheric activity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1017879