By Joseph Berkowitz
Atomic and Molecular Photoabsorption, quantity 1 describes and catalogs on hand spectral details proper to how universal gases engage with sun and different resources of electromagnetic radiation resembling x-rays, flames, and plasmas. Photoabsorption is light's aid in depth and strength while it passes via a column of fuel or liquid. This publication additionally features a huge variety of facts tables and figures which are valuable to researchers simply because they assist them decide on precisely which wavelengths to take advantage of of their experiments. The additional distinguishing element of this publication is its synthesis throughout a huge spectrum of wavelengths and compilation of knowledge for a lot of atoms and molecules.
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Extra info for Atomic and Molecular Photoabsorption: Absolute Total Cross Sections
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 .
Atomic and Molecular Photoabsorption: Absolute Total Cross Sections by Joseph Berkowitz