SPE Journal
Volume 16,
Number 3,
September 2011,
pp. 524-536
Summary
One method to access unconventional, heavy-oil resources is to apply in-situ
combustion (ISC) to oxidize in place a small fraction of the hydrocarbon,
thereby providing heat and pressure that enhances recovery. ISC is also
attractive because it provides the opportunity to upgrade oil in situ by
increasing the API gravity and decreasing, for instance, sulfur content.
Despite a considerable literature on ISC dynamics, the propagation of a
combustion front through porous media has never been visualized directly. We
use X-ray computed tomography (CT) to monitor ISC movement, displacement-front
shape, and thickness in a 1-m-long "combustion" tube. Temperature-profile
history, liquid production, and effluent gas data are also obtained. Tests
employ an 8.65°API heavy crude oil and representative sand. The general trend
of saturation profiles is defined through spatially and temporally varying CT
numbers. The role of initial oil and water saturations is examined by packing
the combustion tube with either multiple samples with different saturations or
by filling it with a uniform sample. Our work quantifies that ISC fronts
display instabilities on a fine scale (cm). ISC reactions appear to add to
front instability in comparison to inert gas advance. The pressure gradients
during ISC appear to influence grain arrangement for loose packing. These grain
arrangements cause combustion-front fingering, suggesting that the
geomechanical state is relevant to combustion. These new data advance the
knowledge base significantly by providing a data set for benchmarking of ISC
simulations.
© 2011. Society of Petroleum Engineers
View full textPDF
(
2,801 KB
)
History
- Original manuscript received:
5 September 2010
- Meeting paper published:
21 September 2010
- Revised manuscript received:
19 November 2010
- Manuscript approved:
25 November 2010
- Published online:
9 June 2011
- Version of record:
15 September 2011