ATOMIC TRANSITION-PROBABILITIES IN TI-I

We report the measurement of 92 branching fractions and atomic transit ion probabilities in Ti I. High-current, hollow cathode spectra record ed using the Fourier transform spectrometer at the National Solar Obse rvatory are used to determine the branching fractions. An absolute sca le is established using recently reported radiative lifetimes from tim e-resolved laser induced fluorescence measurements. These 92 lines are connected to high-lying, even parity levels in neutral Ti. Most of ou r transition probabilities are accurate to better than +/- 10%.