FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2790826642> ?p ?o ?g. }

• W2790826642 endingPage "90" @default.
• W2790826642 startingPage "78" @default.
• W2790826642 abstract "Abstract An approach to improving the documentation of weak spectral lines falling near the prominent analytical lines used in inductively coupled plasma optical emission spectrometry (ICP-OES) is described. Measurements of ICP emission spectra in the regions around several hundred prominent lines, using concentrated solutions (up to 1% w/v) of some 70 elements, and comparison of the observed spectra with both recent published work and with the output of a computer program that allows calculation of transitions between the known energy levels, show that major improvements can be made in the coverage of spectral atlases for ICP-OES, with respect to “classical” line tables. It is argued that the atomic spectral data (wavelengths, energy levels) required for the reliable identification and documentation of a large majority of the weak interfering lines of the elements detectable by ICP-OES now exist, except for most of the observed lines of the lanthanide elements. In support of this argument, examples are provided from a detailed analysis of a spectral window centered on the prominent Pb II 220.353 nm line, and from a selected line-rich spectrum (W). Shortcomings in existing analyses are illustrated with reference to selected spectral interferences due to Zr. This approach has been used to expand the spectral-line library used in commercial ICP-ES instruments (Agilent 700-ES/5100-ES). The precision of wavelength measurements is evaluated in terms of the shot-noise limit, while the absolute accuracy of wavelength measurement is characterised through comparison with a small set of precise Ritz wavelengths for Sb I, and illustrated through the identification of Zr III lines; it is further shown that fractional-pixel absolute wavelength accuracies can be achieved. Finally, problems with the wavelengths and classifications of certain Au I lines are discussed." @default.
• W2790826642 created "2018-03-29" @default.
• W2790826642 creator A5087704446 @default.
• W2790826642 date "2018-05-01" @default.
• W2790826642 modified "2023-09-27" @default.
• W2790826642 title "Improved documentation of spectral lines for inductively coupled plasma emission spectrometry" @default.
• W2790826642 cites W1832136037 @default.
• W2790826642 cites W1972014946 @default.
• W2790826642 cites W1981540271 @default.
• W2790826642 cites W1983428183 @default.
• W2790826642 cites W1988085992 @default.
• W2790826642 cites W1988884823 @default.
• W2790826642 cites W1990396593 @default.
• W2790826642 cites W1990632845 @default.
• W2790826642 cites W1994393597 @default.
• W2790826642 cites W1995944326 @default.
• W2790826642 cites W1996390365 @default.
• W2790826642 cites W1997871924 @default.
• W2790826642 cites W2000717623 @default.
• W2790826642 cites W2003241425 @default.
• W2790826642 cites W2003731483 @default.
• W2790826642 cites W2006291367 @default.
• W2790826642 cites W2007234528 @default.
• W2790826642 cites W2012911562 @default.
• W2790826642 cites W2024119544 @default.
• W2790826642 cites W2028645448 @default.
• W2790826642 cites W2030644915 @default.
• W2790826642 cites W2039575657 @default.
• W2790826642 cites W2042365716 @default.
• W2790826642 cites W2049713607 @default.
• W2790826642 cites W2050670550 @default.
• W2790826642 cites W2054540536 @default.
• W2790826642 cites W2054743395 @default.
• W2790826642 cites W2057963994 @default.
• W2790826642 cites W2059692270 @default.
• W2790826642 cites W2062713228 @default.
• W2790826642 cites W2074660134 @default.
• W2790826642 cites W2076345536 @default.
• W2790826642 cites W2077016203 @default.
• W2790826642 cites W2077344498 @default.
• W2790826642 cites W2080370497 @default.
• W2790826642 cites W2082970175 @default.
• W2790826642 cites W2089123725 @default.
• W2790826642 cites W2094452646 @default.
• W2790826642 cites W2095808512 @default.
• W2790826642 cites W2147540315 @default.
• W2790826642 cites W2170633947 @default.
• W2790826642 cites W2309836237 @default.
• W2790826642 cites W2313075695 @default.
• W2790826642 cites W2315131513 @default.
• W2790826642 cites W2316989199 @default.
• W2790826642 cites W2321244664 @default.
• W2790826642 cites W2325086053 @default.
• W2790826642 cites W2326398725 @default.
• W2790826642 cites W2326781828 @default.
• W2790826642 cites W2331681049 @default.
• W2790826642 cites W2332269231 @default.
• W2790826642 cites W235844017 @default.
• W2790826642 cites W2963764082 @default.
• W2790826642 cites W3099741247 @default.
• W2790826642 cites W3161587739 @default.
• W2790826642 cites W3161633160 @default.
• W2790826642 cites W4290706473 @default.
• W2790826642 cites W2330857455 @default.
• W2790826642 doi "https://doi.org/10.1016/j.sab.2018.02.016" @default.
• W2790826642 hasPublicationYear "2018" @default.
• W2790826642 type Work @default.
• W2790826642 sameAs 2790826642 @default.
• W2790826642 citedByCount "3" @default.
• W2790826642 countsByYear W27908266422018 @default.
• W2790826642 countsByYear W27908266422019 @default.
• W2790826642 crossrefType "journal-article" @default.
• W2790826642 hasAuthorship W2790826642A5087704446 @default.
• W2790826642 hasConcept C113196181 @default.
• W2790826642 hasConcept C120665830 @default.
• W2790826642 hasConcept C121332964 @default.
• W2790826642 hasConcept C1276947 @default.
• W2790826642 hasConcept C184779094 @default.
• W2790826642 hasConcept C185544564 @default.
• W2790826642 hasConcept C185592680 @default.
• W2790826642 hasConcept C198352243 @default.
• W2790826642 hasConcept C2524010 @default.
• W2790826642 hasConcept C30475298 @default.
• W2790826642 hasConcept C33390570 @default.
• W2790826642 hasConcept C33923547 @default.
• W2790826642 hasConcept C43617362 @default.
• W2790826642 hasConcept C4839761 @default.
• W2790826642 hasConcept C6260449 @default.
• W2790826642 hasConcept C82706917 @default.
• W2790826642 hasConcept C95974651 @default.
• W2790826642 hasConcept C96141758 @default.
• W2790826642 hasConceptScore W2790826642C113196181 @default.
• W2790826642 hasConceptScore W2790826642C120665830 @default.
• W2790826642 hasConceptScore W2790826642C121332964 @default.
• W2790826642 hasConceptScore W2790826642C1276947 @default.
• W2790826642 hasConceptScore W2790826642C184779094 @default.
• W2790826642 hasConceptScore W2790826642C185544564 @default.
• W2790826642 hasConceptScore W2790826642C185592680 @default.

• next