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Handbook for Methane Control in Mining - AMMSA

Handbook for Methane Control in Mining - AMMSA

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12LAYERING OF METHANE AT THE MINE ROOFThe density of methane is roughly half that of air, so methane released at the m<strong>in</strong>e roof may <strong>for</strong>ma buoyant layer that does not readily mix <strong>in</strong>to the ventilation air stream. Such layers have beenthe source of many m<strong>in</strong>e explosions, 17 so it is important to understand the circumstances that ledto the <strong>for</strong>mation of methane roof layers and the methods used to dissipate them.Creedy and Phillips [1997] have written athorough summary of methane layer<strong>in</strong>g andits implications <strong>for</strong> South African m<strong>in</strong>es.Detect<strong>in</strong>g methane layers. <strong>Methane</strong> layers are largely a result of <strong>in</strong>adequate ventilation. Ra<strong>in</strong>e[1960] asserted that a measurement of ventilation velocity is of most practical importance. Hefound that under conditions of “normal firedamp emission,” 18 an air velocity of 100 ft/m<strong>in</strong> measuredat the roof was enough to prevent layer<strong>in</strong>g. 19 Most current-day estimates of the necessaryvelocity are close to this value. 20An alternative approach to estimat<strong>in</strong>g the air velocity required to prevent layer<strong>in</strong>g is to use a“layer<strong>in</strong>g number,” devised by Bakke and Leach [1962]. The layer<strong>in</strong>g number is a dimensionlessnumber expressed as—L =U37 ⋅3where L is the layer<strong>in</strong>g number, U is the air velocity <strong>in</strong> feet per m<strong>in</strong>ute, V is the methane releaserate <strong>in</strong> cubic feet per m<strong>in</strong>ute, and W is the entry width <strong>in</strong> feet. In layer<strong>in</strong>g experiments conductedby Bakke and Leach, methane was released at a s<strong>in</strong>gle po<strong>in</strong>t at the m<strong>in</strong>e roof, and the air velocitynecessary to dilute the layer was measured. They found that mix<strong>in</strong>g by turbulence began atlayer<strong>in</strong>g numbers larger than 2, but that a layer<strong>in</strong>g number of 5 was necessary <strong>for</strong> adequate dilution.21 Compared to the 100-ft/m<strong>in</strong> criterion, the layer<strong>in</strong>g number concept is more difficult toapply because the methane release rate V is usually not known.VW17 For example, the 1993 Middelbult coal m<strong>in</strong>e explosion <strong>in</strong> Secunda, South Africa, was attributed to a methanelayer [Davies et al. 2000].18 The phrase “normal firedamp emission” was not further def<strong>in</strong>ed. However, it is clear that at abnormally high gasfeeds, higher velocities are required. In a laboratory study, Bakke and Leach [1962] found that 230 ft/m<strong>in</strong> air velocitywas required to disperse a layer generated by a release of 12 ft 3 /m<strong>in</strong> of methane.19 The 100 ft/m<strong>in</strong> applies only to horizontal entries. Higher velocities are suggested <strong>for</strong> <strong>in</strong>cl<strong>in</strong>ed entries [Bakke andLeach 1965].20 For example, McPherson [2002] suggests 0.4 m/sec, or about 80 ft/m<strong>in</strong>.21 At high methane emission rates, the layer<strong>in</strong>g number suggests that velocities higher than 100 ft/m<strong>in</strong> are necessaryto prevent layer<strong>in</strong>g. For example, <strong>for</strong> a methane emission rate of 16 ft/m<strong>in</strong> <strong>in</strong> a 16-ft-wide entry, the velocityrequired to prevent layer<strong>in</strong>g is 185 ft/m<strong>in</strong>.

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