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Davies, Roy C.1, John A Howell2, Stephen Flint1, Claus Diessel3, Ron Boyd3
(1) University of Liverpool, Liverpool, United Kingdom
(2) University of Bergen, Bergen, Norway
(3) University of Newcastle, Callaghan, Australia

ABSTRACT: Identifying High Resolution Records of Base-Level and Climate Change Using Coal Previous HitSeamNext Hit Micro-Stratigraphy

Coal seams are highly sensitive indicators of changes in accommodation and organic productivity. Changes in inorganic mineral and inertinite content enable sub-parasequence scale base-level changes to be identified and correlated over tens of kilometres of depositional dip. Similarly, changes in vitrinite to inertinite ratios record high frequency climatic cycles, which can be detected through spectral analysis of coal Previous HitseamNext Hit data.
Detailed petrographic analysis of over 300 samples from the Sunnyside coal Previous HitseamNext Hit of the Cretaceous Blackhawk Formation in Eastern Utah has enabled us to identify an extremely high-resolution record of base-level change throughout the formation of the Previous HitseamNext Hit. Laterally extensive coal Previous HitseamNext Hit splits that open out basinward into packages of shallow-marine sediments enable us to integrate this record with changes in marine base-level observed in the laterally equivalent shallow-marine strata. This integration between marine and non-marine records is central to understanding sequence stratigraphic expressions in non-marine systems.
Using various spectral analysis techniques it is possible to detect cyclic variations in the vitrinite to inertinite ratios through the Previous HitseamTop, the most significant of these occur at approximately 0.6 m-1 and 5.0 m-1 in a 2.5 metre thick section. The exact duration of these cycles is difficult to determine as peat accumulation rates are not constant and removal of peat due to wild fires and erosion may occur during excessively dry periods. However, based on estimates of 60 Ka – 120 Ka for the Sunnyside coal to form, they may correspond to obliquity (41 Ka) and hemi-precession (~ 10 Ka) respectively.

 

AAPG Search and Discovery Article #90026©2004 AAPG Annual Meeting, Dallas, Texas, April 18-21, 2004.