Quantifying K, U, and Th contents of marine sediments using shipboard natural gamma radiation spectra measured on DV JOIDES Resolution

dc.contributor.author De Vleeschouwer, David
dc.contributor.author Dunlea, Ann G.
dc.contributor.author Auer, Gerald
dc.contributor.author Anderson, Chloe H.
dc.contributor.author Brumsack, Hans-Jürgen
dc.contributor.author de Loach, Aaron
dc.contributor.author Gurnis, Michael
dc.contributor.author Huh, Youngsook
dc.contributor.author Ishiwa, Takeshige
dc.contributor.author Jang, Kwangchul
dc.contributor.author Kominz, Michelle A.
dc.contributor.author März, Christian
dc.contributor.author Schnetger, Bernhard
dc.contributor.author Murray, Richard W.
dc.contributor.author Pälike, Heiko
dc.contributor.author Expedition 356 Shipboard Scientists
dc.date.accessioned 2017-05-09T18:51:28Z
dc.date.available 2017-05-09T18:51:28Z
dc.date.issued 2017-03-21
dc.description © The Author(s), 2017. This article is distributed under the terms of the Creative Commons Attribution License. The definitive version was published in Geochemistry, Geophysics, Geosystems 18 (2017): 1053–1064, doi:10.1002/2016GC006715. en_US
dc.description.abstract During International Ocean Discovery Program (IODP) expeditions, shipboard-generated data provide the first insights into the cored sequences. The natural gamma radiation (NGR) of the recovered material, for example, is routinely measured on the ocean drilling research vessel DV JOIDES Resolution. At present, only total NGR counts are readily available as shipboard data, although full NGR spectra (counts as a function of gamma-ray energy level) are produced and archived. These spectra contain unexploited information, as one can estimate the sedimentary contents of potassium (K), thorium (Th), and uranium (U) from the characteristic gamma-ray energies of isotopes in the 40K, 232Th, and 238U radioactive decay series. Dunlea et al. (2013) quantified K, Th, and U contents in sediment from the South Pacific Gyre by integrating counts over specific energy levels of the NGR spectrum. However, the algorithm used in their study is unavailable to the wider scientific community due to commercial proprietary reasons. Here, we present a new MATLAB algorithm for the quantification of NGR spectra that is transparent and accessible to future NGR users. We demonstrate the algorithm's performance by comparing its results to shore-based inductively coupled plasma-mass spectrometry (ICP-MS), inductively coupled plasma-emission spectrometry (ICP-ES), and quantitative wavelength-dispersive X-ray fluorescence (XRF) analyses. Samples for these comparisons come from eleven sites (U1341, U1343, U1366-U1369, U1414, U1428-U1430, and U1463) cored in two oceans during five expeditions. In short, our algorithm rapidly produces detailed high-quality information on sediment properties during IODP expeditions at no extra cost. en_US
dc.identifier.citation Geochemistry, Geophysics, Geosystems 18 (2017): 1053–1064 en_US
dc.identifier.doi 10.1002/2016GC006715
dc.identifier.uri https://hdl.handle.net/1912/8969
dc.language.iso en en_US
dc.publisher John Wiley & Sons en_US
dc.relation.uri https://doi.org/10.1002/2016GC006715
dc.rights Attribution-NonCommercial-NoDerivatives 4.0 International *
dc.rights.uri http://creativecommons.org/licenses/by-nc-nd/4.0/ *
dc.subject IODP en_US
dc.subject Physical properties en_US
dc.subject Natural gamma radiation en_US
dc.subject Downhole logging en_US
dc.title Quantifying K, U, and Th contents of marine sediments using shipboard natural gamma radiation spectra measured on DV JOIDES Resolution en_US
dc.type Article en_US
dspace.entity.type Publication
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