Özet
Organic maturity is a key property for assessment of hydrocarbon potential and generation of black shales. Early Paleozoic strata are usually void of terrestrial organic matter such as vitrinite, thus evading conventional, reflectance based maturity analysis. To overcome this, graptolites in samples from the basal hot shales of the Silurian Qusaiba Formation, with known, reflectance based vitrinite equivalent maturities from 0.54 to 1.76 VRE%, were analyzed with Raman spectroscopy to establish a spectroscopic maturity scale. All samples provided spectra showing the Disorder (D) peak and the Graphite (G) peak typical for organic carbons. Systematic variation of these peaks with sample maturity is used to quantify the relationship of reflectance with the graptolites molecular condition. Several spectral properties were tested for use as maturity indicators. The most reliable maturity tracers are the variation of position of the G peak between 1570 and 1610 cm-1 and the widening band distance (Δ(G-D)) between the G peak and D peak position at 1320 to 1370 cm-1. Comparison of the mean and modal maxima of peak positions showed that the mean of G peak position and Δ(G-D) provide the best fit of Raman and optical reflectance determinations with R2 of 0.884 and 0.935, respectively. Algorithms for the calculation of vitrinite equivalent reflectance from the Raman spectral properties were developed based on best fit exponential regressions, with a linear cross correlation of the measured and calculated values at R2 = 0.9178 for the mean of Δ(G-D). Raman based maturity measurements on graptolites provide a welcome alternative method for on particles as small as 3 μm diameter.
Orijinal dil | İngilizce |
---|---|
Sayfa (başlangıç-bitiş) | 96-107 |
Sayfa sayısı | 12 |
Dergi | International Journal of Coal Geology |
Hacim | 162 |
DOI'lar | |
Yayın durumu | Yayınlandı - 15 May 2016 |
Harici olarak yayınlandı | Evet |
Bibliyografik not
Publisher Copyright:© 2016 Elsevier B.V.
Finansman
We thank the Saudi Arabian Oil Company (Saudi Aramco) and the Ministry of Petroleum and Mineral Resources for the support received for this project and the permission to publish the results. We thank Maher I. Marhoon and Khaled Arouri for their continuous interest and support in this study. Thanks are also due to technical support we received from Salman Qathami, Mahmoud Alzharani and Mohammed Alsobaie. We thank anonymous reviewers for insightful reviews that greatly helped improve the manuscript. We appreciate kind handling of the manuscript by the editor, Dr. O. Karacan.
Finansörler | Finansör numarası |
---|---|
Saudi Aramco | |
Federal Ministry of Petroleum Resources |