Potential Contaminant Pathways from Hydraulically Fractured Shale Aquifers
Potential Contaminant Pathways from Hydraulically Fractured Shale Aquifers
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DOI:
10.1111/j.1745-6584.2012.00990.x
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发表时间:
2012-11
期刊:
影响因子:
2.6
通讯作者:
J. Saiers;E. Barth
中科院分区:
文献类型:
--
作者:
J. Saiers;E. Barth
In a recent article, T. Myers used MODFLOW to examine the impacts of hydraulic fracturing of the Marcellus Shale (“the Marcellus”) on groundwater flow patterns. Myers’ model includes a layer representing the Marcellus, a 1500-m overburden of sandstone and one highpermeability “fracture” connecting the Marcellus directly to the surface. Myers conducts steady-state and transient groundwater flow simulations for scenarios without and with injection into a horizontal well (to approximate conditions during hydraulic stimulation of the shale layer), and he examines the sensitivity of the model calculations to changes in hydraulic conductivity of the shale and overlying sandstone. His results suggest the flow system would reach a new equilibrium in 3 to 6 years following hydraulic fracturing, and he concludes that the hydrologic stress of hydraulic fracturing could allow for advective transport of frac fluids and formation water to drinkingwater aquifers in less than 10 years (Myers 2012). We recognize models represent only approximations of reality, but Myers’ modeling framework neglects critical hydrologic processes, misrepresents physical conditions that drive groundwater flow, and is underpinned by simplifications that are too severe and unnecessary. Owing to these shortcomings, Myers’ findings should not be interpreted as reasonable predictions of the response of groundwater flow and contaminant migration to hydraulic fracturing. In the paragraphs below, we elaborate on the deficiencies of Myers’ model and suggest alternative approaches that could improve descriptions of groundwater flow and solute transport during and following hydraulic stimulation of the Marcellus. Myers assumes that groundwater flow occurs exclusively through water-filled void spaces, when, in fact, the void spaces of the Marcellus and some overlying