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BAROMETRIC AND EARTH TIDE INDUCED WATER-LEVEL CHANGES IN A RIGID SANDSTONE AQUIFER, SOUTHWESTERN INDIANA |
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As
the sun and moon pass over a point on the Earth, their gravitational
attraction generates a dilational force on the bedrock, increasing pore
space, and decreasing the potential of the water in the aquifer (a).
After the sun and moon pass, the gravitational force decreases the
aquifer (pore space) contracts, thus increasing the pore water potential
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BY: Dr. Paul Doss,
Paul Inkenbrandt, and Robert Brown
ABSTRACT
Water levels from a deep-shallow
piezometer nest in the Inglefield sandstone depict a dynamic
ground-water system. Water levels at both the 60 foot and 110 foot
depths fluctuate up to 0.5 feet in the matter of hours. Most of this
fluctuation is driven by responses to atmospheric pressure change. A
remarkable inverse correlation exists between ground-water levels and
barometric pressure. Calculated barometric efficiency for this aquifer
ranges from 0.85 to 0.94, indicating a rigid aquifer skeleton. Following
successful quantification and removal of the barometric effects on
water-level data, the residual hydrographs suggested an additional,
smaller amplitude periodicity was still present in the water-level
records. These fluctuations were hypothesized to result from Earth-tide
induced crustal deformation stresses. Evaluation of barometric-corrected
head data by a Fast Fourier Transform method identified periodicities of
water-level changes at 12.01 and 12.4 hours. These periodicities
correlate well with solar and lunar tide stressors, respectively. Other
periods that were indicated by Fourier analysis (54 day and 2.5 hour)
have not yet been interpreted and may be artifacts of the evaluated
period of record. Whereas barometric fluctuations of water levels are
driven through the well-water column and do not result from potential
changes within the aquifer, Earth-tide induced fluctuations are the
result of changes in aquifer potential. Further, these stress induced
changes are suggestive of a confined system, yet simple stratigraphy
suggests the aquifer is unconfined. Lithologic variability within the
sandstone, specifically a finer-grained and mica-rich shallow zone,
likely generates confined behavior. It is hoped that future work can
identify the source of the other observed periodicities and whether this
aquifer responds to seismic stresses associated with the Wabash Valley
Fault System.
HYDROGEOLOGIC SETTING AND CONDITIONS Schematic geologic setting of the piezometer nest
Acknowledgements
We appreciate the help of Tom Pickett for teaching us about
the physics involved and performing the Fast Fourier Transforms.
We are grateful for help from Todd Rasmussen, for
explaining the barometric influence removal process.
We thank the USI RISC program for research and travel
support to Inkenbrandt and Brown.
Thanks to William Wilding for help with statistics. We
would also like to thank the weather for working with us and
being dynamic. The sun
and moon deserve gratitude for their great mass and proximity.
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