Abstract
Relative perpendicular photoionization intensities for the noble gases Ne and Ar and the molecules CH4, NH3, H2O, CO, N2, and CO2 have been measured with HeI (21.2 eV), HeII (α, 40.8 eV and β, 48.4 eV) resonance lines and Zr Mζ (151 eV) and Mg Kα (1253.6 eV) soft x rays using the same instrument for all measurements. New valence shell spectra of NH3, CO, and CO2 obtained with Zr Mζ radiation are illustrated. The experimental values are compared to values calculated for each radiation by the method of Ellison [J. Chem. Phys. 61, 507 (1974)]. Reasonable success was achieved by the theory which appears to falter most seriously with the inner valence orbitals of dominant 2s atomic character. This failure is most likely due to the improper treatment of the Cooper minimum. Attempts to improve the agreement between observed and calculated relative intensities by inclusion of multiple electron processes (’’shake up’’ transitions) are discussed.

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