The document discusses the Bohr-Sommerfeld atomic model, which extends Bohr's original atomic theory to explain the fine structures of hydrogen's spectral lines through elliptical electron orbits and relativistic corrections. It highlights the limitations of Bohr’s model, such as its inability to account for spectral line splitting due to electric and magnetic fields, and introduces Sommerfeld's concepts such as azimuthal quantum numbers and modified energy equations. The analysis includes the derivation of allowed electron transitions leading to the hydrogen alpha spectral line and its fine structure, showcasing Sommerfeld's contributions to atomic theory.