The results of spectral observations of the Ae/Be star V380 Ori in the optical and near-IR ranges for 1976 to 1991, are presented. The spectra were obtained on various telescopes and spectrographs including the Main Stellar Spectrograph of the BTA six-meter telescope. For 270 bright emission lines, the intensities, equivalent widths, half-widths, radial velocities, and variability amplitudes are given.