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You are seeing Ask web results for abundance ratio of isotopes because there was not a match on Dictionary.com.
Nitrogen Isotope Abundance Ratio Determination Using. Molecular Emission Spectrometry. Robert J. Eierman' and Edward H. Piepmeier* ...
pubs.acs.org/doi/abs/10.1021/ac00125a026
This paper presents a generalization of the previously reported matched abundance-ratio cascades for multicomponent isotope separation. ...
linkinghub.elsevier.com/retrieve/pii/0009250963800160
Determination of the 36Ar/38Ar isotopic abundance ratio of the solar wind using SOHO/CELIAS/MTOF. James M. Weygand Corresponding Author Contact Information ...
linkinghub.elsevier.com/retrieve/pii/S0016703701007402
The Abundance Ratio of the Isotopes of Lithium. A. Keith Brewer Bureau of Chemistry and Soils, U. S. Department of Agriculture, Washington, D. C. ...
link.aps.org/doi/10.1103/PhysRev.47.571.2
This yields a value of 92.2+/-3.7 for the C12/C13 abundance ratio of the carbon isotopes in good agreement with the value reported by Vaughan, Williams and ...
adsabs.harvard.edu/abs/1937PhRv...52..472B
A New Determination of the C^{12}/C^{13} Isotopic Abundance Ratio in the Solar Photosphere. Authors: Herzberg, Luise; Delbouille, L.; Roland, G. ...
adsabs.harvard.edu/full/1967ApJ...147..697H
The measurement data of the isotopic abundance ratio of natural uranium are shown in table 2. By analysis of variance for the data shown in table 2, ...
www.springerlink.com/index/FK745206560210K6.pdf
Generally, stable environmental isotopes are measured as ratios of the two most abundant isotopes of a given element. The absolute abundance ratio of isotopes is not usually measured in natural waters because it requires sophisticated mass spectrometric technique.
www.wileywater.com/Contributor/Sample_1.htm
The relative abundances of the mass spectra 1 – 16 are given in Table 2. In the electron ionization mass spectra all of the studied compounds are observed the corresponding molecular ions, where the abundance ratio of the isotopes of selenenium is characteristic [4].
www.mdpi.net/ecsoc-5/d0008/d0008.htm
This study also serves to investigate whether the 2090 Å line is free of line-blends, so as to be useful for future studies with improved instrumentation of the abundance ratio between the two boron isotopes 10 and 11. This ratio is also sensitive to which mechanism(s) were important in the early galactic production...
www.astro.uu.se/~be/boron.html
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