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The complex magnetic-resonance spectrum of oxygen gas is observed at 9340 Mc/sec in magnetic fields up to 9000 oersted. Some 40 lines are resolved. A partial analysis of the spectrum is made with the help of Henry's recent Zeeman theory of O₂. Other lines are identified by the temperature dependence of the relative intensities. Line widths are measured by several techniques and range from 0. 6 to 4 Mc/sec/mm Hg at room temperature. The temperature and pressure dependence of the line widths are investigated.
Beringer et al. (1951) studied this question.
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