The broadening of d-f and f-d transitions by collisions with neutral hydrogen atoms

Details The broadening of d-f and f-d transitions by collisions with neutral hydrogen atoms The broadening of d-f and f-d transitions by collisions with neutral hydrogen atoms

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mnras.296.1057b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 296, Issue 4, pp. 1057-1060.

Astronomy and Astrophysics

Astronomy

86

Atomic Data, Sun: Abundances

Scientific paper

The theory of Anstee & O'Mara for the broadening of spectral lines owing to collisions by neutral hydrogen atoms is extended to d-f and f-d transitions of neutral atoms. Width cross-sections are tabulated against effective principal quantum numbers for the upper and lower states of the transition, for a relative collision velocity of 10^4ms^-1. The cross-sections are fitted to a variation with velocity of v^-alpha, and results for the velocity parameter alpha are similarly tabulated. The data are tested by application to d-f spectral lines in the solar spectrum. The derived abundances are consistent with those for meteorites.

Affiliated with

Also associated with

No associations

Rating

The broadening of d-f and f-d transitions by collisions with neutral hydrogen atoms 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 The broadening of d-f and f-d transitions by collisions with neutral hydrogen atoms, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The broadening of d-f and f-d transitions by collisions with neutral hydrogen atoms will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1505697