That same year Otto Stern proposed an experiment carried out later called the Stern–Gerlach experiment in which silver atoms in a magnetic field were deflected in opposite directions of distribution. This pre-1925 period marked the old quantum theory built upon the Bohr-Sommerfeld model of the atom with its classical elliptical electron orbits. During the period between 1916 and 1925, much progress was being made concerning the arrangement of electrons in the periodic table. In order to explain the Zeeman effect in the Bohr atom, Sommerfeld proposed that electrons would be based on three 'quantum numbers', n, k, and m, that described the size of the orbit, the shape of the orbit, and the direction in which the orbit was pointing. Irving Langmuir had explained in his 1919 paper regarding electrons in their shells, "Rydberg has pointed out that these numbers are obtained from the series N = 2 ( 1 + 2 2 + 2 2 + 3 2 + 3 2 + 4 2 ) . The factor two suggests a fundamental two-fold symmetry for all stable atoms." This 2 n 2 configuration was adopted by Edmund Stoner, in October 1924 in his paper 'The Distribution of Electrons Among Atomic Levels' published in the Philosophical Magazine. Wolfgang Pauli hypothesized that this required a fourth quantum number with a two-valuedness.