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Handbook for Methane Control in Mining - AMMSA

Handbook for Methane Control in Mining - AMMSA

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100Vertical methane dra<strong>in</strong>age boreholes drilled from the surface usually require both dewater<strong>in</strong>g andhydraulic fractur<strong>in</strong>g <strong>for</strong> maximum effectiveness. Horizontal, cross-measure, or vertical undergrounddegasification boreholes may also need to remove water to effectively produce gas.These methane dra<strong>in</strong>age systems are fully expla<strong>in</strong>ed and referenced by Diamond [1994].Gas-bear<strong>in</strong>g paleochannel deposits oradjacent coalbeds may require surface orcross-measure methane dra<strong>in</strong>age boreholes.Coalbeds and other adjacent gas source beds. Historical m<strong>in</strong><strong>in</strong>g experience and research haveshown that coalbeds adjacent to the m<strong>in</strong>ed seam can contribute significant quantities of methanegas <strong>in</strong>to active work<strong>in</strong>gs [F<strong>in</strong>f<strong>in</strong>ger and Cervik 1979; Ayruni 1984; Diamond et al. 1992].Degasification of these coalbeds may be accomplished through vertical or directional boreholesdrilled from the surface. Occasionally, <strong>in</strong>-m<strong>in</strong>e vertical, cross-measure, or directional boreholesare used to reduce potentially explosive accumulations of gas [F<strong>in</strong>f<strong>in</strong>ger and Cervik 1979;Ayruni 1984; Diamond 1994].In addition to nearby coalbeds, other adjacent strata may also be significant gas reservoirs andcontribute unexpected emissions <strong>in</strong>to m<strong>in</strong>e work<strong>in</strong>gs. Shales and siltstones rich <strong>in</strong> organic matteroften conta<strong>in</strong> significant quantities of methane gas [Darton 1915; Johnson and Flores 1998].Although these <strong>for</strong>mations may have a large gas storage capacity, permeability is usually verylow. Thus, these rocks may not release gas until m<strong>in</strong><strong>in</strong>g-<strong>in</strong>duced fractures <strong>in</strong>crease their permeabilityand provide a pathway <strong>for</strong> gas migration to the m<strong>in</strong>e work<strong>in</strong>gs. In study<strong>in</strong>g the gas contentof U.K. coalbeds, Creedy [1988] concluded that although the gas contents and porosities ofthese rocks are low, a well-developed jo<strong>in</strong>t or fracture system could facilitate gas release fromthese strata. There<strong>for</strong>e, it may be assumed that if certa<strong>in</strong> organic-rich rocks adjacent to m<strong>in</strong>edcoalbeds have sufficient gas content, migration via jo<strong>in</strong>ts or fractures <strong>in</strong>to the work<strong>in</strong>gs couldgenerate hazardous explosive conditions. <strong>Methane</strong> dra<strong>in</strong>age methods similar to those discussedpreviously <strong>for</strong> adjacent coalbeds are usually appropriate <strong>for</strong> adjacent noncoal gas-bear<strong>in</strong>g strataas well.Large- and small-scale structural fault<strong>in</strong>g. For this discussion, large-scale faults are looselydef<strong>in</strong>ed as hav<strong>in</strong>g tectonically activated and structurally mappable features, with lengths greaterthan 500 m (1,640 ft) and vertical movement of at least 10–20 m (33–66 ft). Small-scale faultsare dist<strong>in</strong>guished from large-scale faults by their limited extent both horizontally and vertically.Faults may have a profound effect on gas emissions <strong>in</strong>to m<strong>in</strong>e work<strong>in</strong>gs and may also be associatedwith outbursts and blowers. Usually, the presence of large-scale fault<strong>in</strong>g is known fromregional geologic mapp<strong>in</strong>g and/or exploration boreholes. In certa<strong>in</strong> cases, these large faults mayact as barriers to gas flow, especially if they conta<strong>in</strong> impermeable fault gouge or the displacementcauses impermeable rock above or below the m<strong>in</strong>ed coalbed to abut aga<strong>in</strong>st it [Diamond1982]. In these situations, large volumes of gas can be trapped beh<strong>in</strong>d the fault at pressureshigher than that of the m<strong>in</strong>e atmosphere. If m<strong>in</strong>e development proceeds through the fault byramp<strong>in</strong>g upward or downward <strong>in</strong>to the displaced, high-pressure coalbed gas reservoir, the potential<strong>for</strong> sudden, excess gas emissions must be addressed.

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