Radiative lifetimes of 22 levels in Rh I and of 35 levels in Ta I are
reported. The lifetimes are measured with the use of time-resolved
laser-induced fluorescence on an atomic beam. The Rh I lifetimes resolve
the discrepancy between the spectroscopically determined solar
abundance of Rh and the abundance of Rh determined from chondritic
meteorites.
Journal
Title
PHYSICAL REVIEW A,VOLUME 27, NUMBER 2,FEBRUARY 1983