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dc.contributor.authorJiang, Guilin
dc.contributor.authorHusseini, Ghaleb
dc.contributor.authorBaxter, Larry L.
dc.contributor.authorLinford, Matthew R.
dc.date.accessioned2021-03-04T07:44:21Z
dc.date.available2021-03-04T07:44:21Z
dc.date.issued2005
dc.identifier.citationJiang, G., Husseini, G. A., Baxter, L. L., & Linford, M. R. (2004). Analysis of Grain Screenings by X-ray Photoelectron Spectroscopy. Surface Science Spectra, 11(1), 97-104. https://doi.org/10.1116/11.20040802en_US
dc.identifier.issn1055-5269
dc.identifier.urihttp://hdl.handle.net/11073/21341
dc.description.abstractDetermining the chemical structure and composition of biomass fuels using x-ray photoelectron spectroscopy (XPS) can provide fundamental knowledge of their structures that is useful in understanding and predicting their combustion behavior. Grain screenings are an example of an agricultural residue (byproduct of food and feed production) of potential interest for biomass combustion. The XPS spectra of grain screenings provide both its elemental composition and indications of its bonding. Traditional fuel analyses of this fuel are also provided. These include: ultimate analysis — the elemental composition of the overall fuel (C, H, N, S, and O); chlorine analysis — reported here as part of the ultimate analysis but formally a separate procedure; proximate analysis — the proximate composition of the fuel (moisture, fixed carbon, volatiles, and ash); heating value — the specific heat of combustion; ash chemistry analysis — an elemental analysis of the ash content, expressed as oxides (which does not imply that they occur as oxides in the fuel). These data are summarized with the XPS spectra.en_US
dc.language.isoen_USen_US
dc.publisherAmerican Vacuum Societyen_US
dc.relation.urihttps://doi.org/10.1116/11.20040802en_US
dc.subjectBiomassen_US
dc.subjectGrain screeningsen_US
dc.subjectXPSen_US
dc.subjectFuelen_US
dc.titleAnalysis of Grain Screenings by X-ray Photoelectron Spectroscopyen_US
dc.typePeer-Revieweden_US
dc.typeArticleen_US
dc.typePublished versionen_US
dc.identifier.doi10.1116/11.20040802


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