Formation of the CL I line at 1351 A in the solar chromosphere

Details Formation of the CL I line at 1351 A in the solar chromosphere Formation of the CL I line at 1351 A in the solar chromosphere

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...266..882s&link_type=abstract

Astrophysical Journal, Part 1, vol. 266, Mar. 15, 1983, p. 882-888.

Astronomy and Astrophysics

Astrophysics

26

Chlorine, Chromosphere, Line Spectra, Solar Atmosphere, Solar Spectra, Ultraviolet Spectra, Fine Structure, Fluorescence, Solar Flares

Scientific paper

The formation of the multiplet containing the Cl I 1351 A line is investigated due to the unusual brightness of this line. It is determined that this line is formed via a fluorescence effect driven by the 1335 A line of C II. Non-LTE calculations including this effect are found to agree with the observed line intensity. It is shown that the 1347 and 1363 A lines of Cl I do not benefit from this effect and they are predicted to be approximately 100 times weaker.

Affiliated with

Also associated with

No associations

Rating

Formation of the CL I line at 1351 A in the solar chromosphere 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 Formation of the CL I line at 1351 A in the solar chromosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Formation of the CL I line at 1351 A in the solar chromosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1465971