The energy levels, lifetimes, oscillator strengths, and transition probabilities of N II lines have been reported in this thesis. We have used the Hartree-Fock (HF) and Multiconfiguration Hartree-Fock (MCHF) methods in our calculations. The relativistic operators mass correction, one-body Darwin term, spin-orbit interaction, and spin-other-orbit have been included in the Breit-Pauli Hamiltonian in our calculations of atomic parameters of singly-ionized nitrogen. We considered 70 levels of the 2s2 2p2, 2s2 2p3, 2s2 2p 3p, 2s2 2p 3s, 2s2 2p 4p, 2s2 2p 3d, 2s2 2p 4s, and 2s2 2p 4d configurations of N II. Our results have been compared with other available calculations and measurements, and generally a good agreement is found.