Stark broadening and transition probability ratios in the Mg I spectrum

Details Stark broadening and transition probability ratios in the Mg I spectrum Stark broadening and transition probability ratios in the Mg I spectrum

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...425..361d&link_type=abstract

Astronomy and Astrophysics, v.425, p.361-365 (2004)

Astronomy and Astrophysics

Astrophysics

5

Atomic Data, Line: Profiles

Scientific paper

Stark widths (W) and shifts (d) of the six astrophysically important 285.212, 383.230, 383.829, 516.732, 517.268, and 518.360 nm neutral magnesium (Mg I) spectral lines in the 3s2 1S-3p1P0, 3p3P0-3d 3D and 3p3P0-4s3S transitions have been measured in laboratory helium plasma at about 50 000 K electron temperature and 1 × 1023 m-3 electron density. They represent the first measured values and, also, the first experimental W and d data in the mentioned transitions. Using the relative line intensity ratios of the lines in the mentioned transitions we have obtained the ratios of corresponding transition probability values (Einstein's A values). They represent the first experimental data based on the analysis of the Mg I emission spectral lines. We have found agreement with theoretical transition probability ratios tabulated by NIST.

Affiliated with

Also associated with

No associations

Rating

Stark broadening and transition probability ratios in the Mg I spectrum 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 Stark broadening and transition probability ratios in the Mg I spectrum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stark broadening and transition probability ratios in the Mg I spectrum will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-894974