Photospheric abundance of samarium deduced from two new ionic lines

Details Photospheric abundance of samarium deduced from two new ionic lines Photospheric abundance of samarium deduced from two new ionic lines

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...215..165y&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 215, no. 1, May 1989, p. 165-167.

Astronomy and Astrophysics

Astrophysics

2

Abundance, Line Spectra, Metal Ions, Photosphere, Samarium, Oscillator Strengths, Rare Earth Elements, Solar Spectra, Transition Probabilities

Scientific paper

Two ionic lines observed in the sun at 4068.334 and 5103.125 A and attributed to Sm have been analyzed assuming LTE. Oscillator strengths, obtained from lifetimes and branching-ratio measurements, are used for the abundance determination. Using the spectral synthesis method, the Sm abundance derived from these two lines is 0.99 + or - 0.05, in good agreement with the meteoritic value (0.97 + or - 0.03).

Affiliated with

Also associated with

No associations

Rating

Photospheric abundance of samarium deduced from two new ionic lines 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 Photospheric abundance of samarium deduced from two new ionic lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photospheric abundance of samarium deduced from two new ionic lines will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1873906