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Lookup NU author(s): Dr Richard Tyson
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A reanalysis of both published and unpublished datasets shows that good and useful statistical relationships often exist between whole-rock hydrogen indices and the nature of the kerogen assemblage determined with light microscopy. The best regression results are reviewed, presented and compared, and the potential reasons for occasional poor results discussed. The most important parameters for predicting the hydrogen index (HI) of immature distal marine and lacustrine sediments are the percentage of plankton- or bacterially-derived amorphous organic matter (AOM, especially when normalised to a palynomorph-free basis) and the visual intensity of autofluorescence of the AOM matrix under blue light excitation. Correct discrimination of AOM and consistent visual assessment of fluorescence intensity are thus essential. The best statistical relationships were obtained using the newly defined fluorescence scale index, which integrates directly the abundance and preservation of the AOM; on average, this parameter explains 70-80% of the observed variation in whole-rock HI and enables HI prediction to within 100 mgHC/gTOC. This study emphasises the considerable preservation-dependent variation in the hydrocarbon generating potential of AOM. © 2005 Elsevier Ltd. All rights reserved.
Author(s): Tyson RV
Publication type: Review
Publication status: Published
Journal: Organic Geochemistry
Year: 2006
Volume: 37
Issue: 1
Pages: 45-63
Print publication date: 01/01/2006
ISSN (print): 0146-6380
ISSN (electronic): 1873-5290
URL: http://dx.doi.org/10.1016/j.orggeochem.2005.08.018
DOI: 10.1016/j.orggeochem.2005.08.018