  We study the solar photospheric abundance of singly ionized neodymium (Nd II)
using high resolution spectroscopic data obtained by Fourier transform
spectrograph (FTS). Based on the Local Thermodynamical Equilibrium (LTE)
assumption, a new value of Nd abundance is derived. We succeed to select of 51
solar Nd II lines with accurate transition probabilities measured
experimentally by Den Hartog et al. (2003) and with accurate damping parameters
are determined from literature. Relying on atomic data of Opacity Distribution
Function (ODF), we construct theoretical photospheric solar model. The mean
solar photospheric abundance obtained from all 51 Nd II lines is log
{\epsilon}Nd=1.45 +- 0.08, which is mostly similar to the meteoric value.
