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By Harkins W.D., Ewing D.T.

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618 eV. to data of Angel and Samson (1988). to data of Henke et al . (1993). a df/dE b Fitted c Fitted spanned by the resonances should yield the correct oscillator strength, despite experimental broadening. 16. 687 eV)–280 eV Alternative values of the photoabsorption cross section in this continuum region are given by Angel and Samson (1988) and Henke et al . (1993). 687 and 150 eV. At higher energies, the cross sections of Angel and Samson are ∼15% lower, but they merge at 270–280 eV. 16. Their differences are quite small compared to the total sums.

Angel and Samson (1988). j Using Henke et al . (1993). k Wettlaufer and Glass (1972). l Saha (1993). m Werner and Meyer (1976). n Allison et al . (1972). o Kelly (1969). p Fraga et al . (1976). q M¨ uller (1996). r Bunge et al . (1993). s Zeiss et al . (1977). i Using See text. 618 eV. to data of Angel and Samson (1988). to data of Henke et al . (1993). a df/dE b Fitted c Fitted spanned by the resonances should yield the correct oscillator strength, despite experimental broadening. 16. 687 eV)–280 eV Alternative values of the photoabsorption cross section in this continuum region are given by Angel and Samson (1988) and Henke et al .

07. 0 o From Bunge et al . (1993). p Zeiss et al . (1977). i Using cross sections of Samson and Angel (1990), or alternatively the compilation of Henke et al . (1993). 11. The good agreement provides internal support for the cross sections used here. 5341 eV. Le Dourneuf et al . (1979). Samson and Angel (1990). 5 Pre-K edge resonances Although these have not been observed for atomic nitrogen, Zhadenov et al . (1987) argue that they should appear more analogous to corresponding structures in N2 than those in NH3 .

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An Apparent High Pressure Due to Adsorption, the Heat of Adsorption, and the Density of Gas-M[...]co by Harkins W.D., Ewing D.T.


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