ARTICLE IN PRESS International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 Contents lists available at ScienceDirect International Journal of Rock Mechanics & Mining Sciences journal homepage: www.elsevier.com/locate/ijrmms Fissure formation and subsurface subsidence in a coalbed fire Taku S. Ide a,, David Pollard b, Franklin M. Orr Jra a b Department of Energy Resources and Engineering, Stanford University, Stanford, CA 94305, USA Department of Geological and Environmental Sciences, Stanford University, Stanford, CA 94305, USA a r t i c l e in fo abstract Article history: Received 1 January 2009 Received in revised form 26 April 2009 Accepted 11 May 2009 Available online 25 June 2009 Coalbed fires are uncontrolled subsurface fires that occur around the world. These fires are believed to be significant contributors to annual CO2 emissions. Although many of these fires have been burning for decades, researchers have only recently begun to investigate physical mechanisms that control fire behavior. One aspect of fire behavior that is poorly characterized is the relationship between subsurface combustion and surface fissures. At the surface above many fires, long, wide fissures are observed. At a coalbed fire near Durango, Colorado, these fissures form systematic orthogonal patterns that align with regional joints in the Upper Cretaceous Fruitland Formation. Understanding the mechanisms that form these fissures is important, as the fissures are believed to play vital roles in sustaining the combustion in the subsurface. In some of the coalbed fire simulation models available today, these fissures are treated as fixed boundary conditions. We argue, using data collected, field observations and simulation result, that there exists a relationship between the location and magnitude of subsidence caused by the fire and the opening of fissures. The results presented suggest that fissures are believed to open when subsurface subsidence gives rise to tensile stresses around pre-existing joints. & 2009 Published by Elsevier Ltd. Keywords: Coalbed fire Coal fire Subsidence Pre-existing joints Fissures Numerical modeling CO2 1. Introduction Uncontrolled subsurface fires in coalbeds account for significant releases of CO2 to the atmosphere. One of the world’s largest active coalbed fires has been documented in Wuda, China [1], where the estimated annual loss of coal is around 200,000 t, equivalent to a yearly emission of 1.5 Mt of CO2 [2]. Coalbed fires are burning in many locations in China, Indonesia, India, and the United States [3]. They can be started naturally by forest fires that burn near an outcrop, by lightning strikes, by human activities, or by spontaneous exothermic reactions of pyrites [4]. Forest fires in Indonesia in 1997 and 1998 ignited hundreds of coal fires at outcrops [5]. A subsurface fire near Centralia, Pennsylvania, was started in May of 1962 when the local government decided to burn an unregulated trash dump in an abandoned strip mine to reduce trash volume and control rodents. The fire ignited an anthracite outcrop, eventually connected to and spread through underground tunnels, and has been burning since. Fissures created by the coal fire emit assorted hot gases, some of which are toxic. A combination of subsidence and emissions from fissures has caused the town of Centralia to be abandoned [4,6]. The particular fire examined in this study, called the North Coalbed Fire, to distinguish it from other active fires in the region, Corresponding author. E-mail address: [email protected] (T.S. Ide). 1365-1609/$ - see front matter & 2009 Published by Elsevier Ltd. doi:10.1016/j.ijrmms.2009.05.007 was discovered in 1998 on the Southern Ute Indian Reservation when sets of fissures that are orthogonal to each other—similar to those at other coal fires around the world—appeared at the surface [7]. Anecdotal evidence provided by local Southern Ute Tribe members [8] suggests that the fire may have been smoldering for decades prior to the reported date of discovery. The fire continues to burn today. The research effort described here is an attempt to understand whether coal combustion followed by subsurface subsidence can produce fissures with systematic patterns at the surface. Subsidence can occur when a burned coalseam loses its structural integrity and collapses under the weight of the overburden. Understanding the formation of fissures is important, as they appear to foreshadow the direction of the combustion front propagation and may play a key role in sustaining the underground fire. First, we summarize the San Juan Basin geology, highlighting key features in the NW section of the basin, where the coalbed fire is located. Second, we characterize the geological features and the surface anomalies in the vicinity of North Coalbed Fire. Surface topography, images of fissures overlying the coalbed fire, and measurements of fissure orientations are presented. We also outline the process of mapping features over the North Coalbed Fire and describe how they were combined with the subsurface information obtained from the wells drilled in the area. In the third section, the field data and previous geological surveys of the area are used to suggest how subsidence can open pre-existing joints in the area, leading to the formation of surface fissures over ARTICLE IN PRESS 82 T.S. Ide et al. / International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 the combustion region. Finally, we model this phenomenon using a simple boundary element numerical code, and explore relationships among key variables that contrast subsidence activities and surface deformation. The results and the limitations of applicability of this simulation model are discussed. 2. San Juan Basin geology The San Juan Basin is an asymmetric, coal bearing basin that covers approximately 16,800–19,400 km2, stretching approximately 145 km west–east and 160 km north–south [9,10]. It is located near the Four Corners, and spans across northwest New Mexico and southwest Colorado as shown in Fig. 1. The basin is well characterized due to the abundance of both coal and coalbed methane resources in the Upper Cretaceous Fruitland Formation (Fig. 2). One study has estimated that a coalbed methane reserve of nearly 1.4 1012 m3 (50 1012 ft3) adsorbed onto 219 109 Mt of coal that underlies the San Juan Basin [9]. The flat Central Basin is bounded by several key geologic features, which are described in detail in previous geologic surveys of the area [9,10,11]. The western and northwestern regions of the basin are circumscribed by the Defiance and the Hogback monoclines, respectively, and the Nacimiento uplift borders the basin on the east side [11]. As shown in Fig. 1, the North Coalbed Fire is located along the Hogback Monocline in the northwestern portion of the basin. The Hogback monocline is believed to have formed either due to the shortening of the Cretaceous strata that induced a right-lateral strike-slip motion along the western and eastern margins during the Laramide orogeny [11], or through reactivation of western dipping thrust faults underlying the Hogback monocline that Fig. 2. Stratigraphic columns representative of the San Juan Basin (left) and the top 25 m of the lithology over the North Coalbed Fire (right). Over the coalbed fire, formations above the blue dotted line have been removed due to weathering. Stratigraphic column on left adapted from Molenaar, 1977. (Figure not drawn to scale.) [For interpretation of the references to color in this figure legend, the reader is referred to the webversion of this article.] Fig. 1. San Juan Basin and its characteristic geologic features. The North Coalbed Fire location is highlighted in the box in the northwestern corner of the basin along the Hogback Monocline. The green area denotes outcrops of Pictured Cliffs sandstone. Figure reproduced from [11]. [For interpretation of the references to color in this figure legend, the reader is referred to the webversion of this article.] resulted in the uplift [12]. In the former view, the shortening can be attributed to the Zuni uplift thrusting northward and north northeastward into the San Juan Basin from the south, and the San Juan uplift indenting southward into the basin [11]. Today, only the forelimb of the Hogback Monocline is exposed and some of the formation members of the Upper Cretaceous are exposed on the western side of the basin. Along the northern perimeter of the Basin, including areas affected by the North Coalbed Fire, thick coalseams crop out along the Hogback monocline [13]. Formations that make up the Upper Cretaceous rocks in the San Juan Basin are described by Molenaar [14]. The Fruitland Formation, which includes the coalbed fire, and adjacent geologic units are depicted in the stratigraphic column in Fig. 2. The left column is representative of the entire San Juan Basin. The right column shows the top 25 m of rock found directly over the North Coalbed Fire. Above the coalbed fire, formations above the dotted line—the Kirtland Shale and most of the Fruitland Formation—have been removed by weathering and erosion. The Kirtland Shale and the Fruitland Formation lie atop of the Pictured Cliffs (PC) Sandstone, which was deposited as regressive marine sands [15] parallel to the shoreline stretching northwest–southeast [10]. The Fruitland Formation is a mixture of mudstones, siltstones, carbonaceous shales and coals deposited landward and parallel to this shoreline [10]. Coalseams in the Fruitland Formation are often referred to as Lower Coal, Middle Coal and Upper Coal, and the thickest, most continuous coalbeds are found in the Lower ARTICLE IN PRESS T.S. Ide et al. / International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 Coal Zone in the northeastern region of the San Juan Basin [16]. The Lower Coal is burning at the North Coalbed Fire. At the North Coalbed Fire, 14 boreholes were drilled in 2007 over an area of 600 200 m. The high density of boreholes allowed reliable subsurface correlations to be made at the site. Both the PC and the Fruitland Formation rise in a step-like fashion from the southwest to the northeast with respect to the isochronously deposited Huerfanito Bed in the Lewis shale, representing a migrating regression–transgression cycle over 1.2 million years [16,17]. The deposition pattern suggests that the subsurface correlation along the shoreline in the northwest– southeast direction is warranted, as this is the trend of the long axis of most coal deposits [18]. The echelon geometry of coal deposits can make subsurface correlations difficult in the transverse direction [18], but it has been shown that Fruitland Formation coalbed correlation was possible when well-logs spaced less than 4 km apart were obtained [17,18]. The San Juan Basin contains several sets of natural fractures that have been extensively mapped and documented. Previous studies have offered various explanations for fracture formations, which are summarized in [11]. Ruf suggests that the fractures formed due to post-Laramide extension [19], while Taylor and Huffman describe a Proterozoic crystalline basement with reactivated faults that may have influenced the orientations of the fractures in overlying strata [20]. Lorenz and Cooper suggest that the orientations of the fractures are most influenced by the 83 formation of tectonic features such as the San Juan uplift and the Zuni uplift (cf. Fig. 1) during the Laramide Orogeny [11]. Despite the competing explanations of the origins of the fractures, orientation measurements in various parts of the San Juan Basin are consistent across many studies. The earliest fracture orientation study of the San Juan Basin concluded from aerial photography that northeast (N10E to N60E) and northwest (N15W to N75W) trends occurred most frequently [21–24]. Their findings are generally supported by more recent measurements [11,12,15,19,25]. The most relevant study for the North Coalbed Fire was carried out by Condon [15], who presents joint orientations and coal strikes found within the Southern Ute Indian Reservation. His findings are discussed in detail in the ensuing section, and they are compared to the fissure orientations that were measured over the North Coalbed Fire. 3. North Coalbed Fire A satellite image of the area bounded by the red dotted box in Fig. 1 is shown in Fig. 3a. The dotted rectangle depicts the region where surface anomalies associated with the North Coalbed Fire are observed. The lack of vegetation over the fire can be attributed to several factors: a surface forest fire, death of vegetation due to toxic combustion fumes emanating from the subsurface, and intentional tree removal to prevent future forest fires. The North Fig. 3. (a) A satellite image over the North Coalbed Fire. The red dotted box outlines the region affected by the underlying fire. A cross-section line A–A0 is used in Fig. 3b. Satellite image is provided by Googlemaps. (b) Cross-section A–A0 showing surface topography and representative subsurface stratigraphy in the vicinity of the North Coalbed Fire. The coalbed fire is located near the coal outcrop inside of the red dotted box. Kl ¼ Lewis Shale, Kp ¼ Pictured Cliffs Sandstone, Kf ¼ Fruitland Formation, Kkl ¼ Kirtland Shale. [For interpretation of the references to color in this figure legend, the reader is referred to the webversion of this article.] ARTICLE IN PRESS 84 T.S. Ide et al. / International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 coalbed fire is contained between latitude N3710105700 and N371020 2400 and longitude W1081060 3600 and W1081060 1800 , and has an aerial extent of approximately 600 200 m. There are signs of coalbed fires underlying the bare patch of land south southwest of the North Coalbed Fire, but only minor surface deformation is observed; thus this area is not included in the surveys. The lack of vegetation there is interpreted as largely due to surface forest fires. A cross-section, A–A0 is drawn (Fig. 3b) by superimposing a USGS geological survey map over the satellite image in Fig. 3a. The cross-section line is roughly perpendicular to the strike of the Hogback monocline. The cross-section shows that the Fruitland Formation crops out along the Hogback Monocline limb (cf. Fig. 1). To the northwest of the Hogback, only the Lewis Shale—containing the Huerfanito Bentonite Bed—is observed. The region affected by the coalbed fire is located near the coal outcrop along the Hogback, and is circumscribed by the dotted box. In this region, the local topography slopes between 51 and 91 to the southeast, and the coal layer dips 61–151 in the same direction [15]. Both the surface topography and the coalseam flatten towards the southeast in the direction of the Central Basin (cf. Fig. 1). The continuous and low permeability Kirtland Shale Formation, which is absent over the North Coalbed Fire, caps the Fruitland Formation to the southeast. Many fissures are exposed on the surface overlying the North Coalbed Fire. The fissures are distinguished from regional joint sets in the same strata because fissures typically have widths on a decimeter scale, whereas joints have apertures less than 0.5 cm [15]. Some of these fissures emit high temperature combustion gases, indicative of the active fire below, while others are at ambient temperature. Four types of fissures have been observed. Examples are shown in Fig. 4: gaping fissures, plateau/offset fissure, molehill/buckling fissures, and narrow fissures. The gaping fissure in Fig. 4a is wide enough for an adult to climb inside. Typical gaping fissures are 0.15–0.3 m wide at the surface and are often wider below the soil level. Based on observations made inside of the gaping fissure in Fig. 4a, many fissures may be connected to each other in the subsurface. Gaping fissures are at ambient temperatures. The surface sediment layers do not show significant rotation around the edges of the fissure. Rather, the fissure appears to have been pulled apart from either side. Fig. 4b is an example of a plateau fissure. Plateau fissures have similar apertures at the surface as gaping fissures but fissures of this type show significant displacement and surface sediment layer rotation on one side of the fissure. The other side of the fissure does not show much displacement. Fig. 4c shows an example of a molehill fissure, where surface layers of sedimentary rock are rotated to form an apex. At molehill fissures with visible fractures at the surface, combustion gases with temperatures as high as 290 1C (550 1F) have been recorded. The temperatures at the fissures were measured using a thermal gun, Raynger 3i Series, made by Raytek. Fig. 4d is an example of a narrow fissure. Many narrow fissures are located in the northern most portion of the field, and these emit the hottest exhaust gases recorded in the field at about 1000 1C. Both the molehill and narrow fissures are about 0.15 m in width. All of the fissures appear to be opening Mode I fractures [26], as displacements are dominantly orthogonal to the fracture surfaces. Orientations of the fissures are systematic, and they often form orthogonal patterns at the surface. The directions and the lengths of 165 fissures are represented on a rose diagram in Fig. 5. Their lengths have been made dimensionless with respect to the longest fissure in the field, which is 75 m. The diagram shows that there are three main fissure directions over the North Coalbed Fire and that the longest and most frequently occurring fissures, F1, have azimuths approximately in the N50E direction. The next most prominent set, F2, strikes in the N35W direction, roughly perpendicular to the first set. The third set, F3, is directed towards the North, and these have similar lengths to the N35W set. The fissures frequently occur together in approximately orthogonal pairs, including members of the N50E and N35W sets. The azimuths of the fissures were compared with observations of joint orientations reported in Condon, 1988. Condon measured 1600 joints and coal cleats at 37 different outcrop locations on the Southern Ute Indian Reservation. Of the 37 measurement stations, eight are located along the Hogback Monocline and are spaced approximately 2 km apart. Most of his measurements were for fractures found in formations of the Upper Cretaceous, the majority of which are in the Kirtland Shale, Fruitland Formation and the Pictured Cliffs Sandstone. Four dominant joint sets, labeled J1–J4, were described. Their stereonets are reproduced in Fig. 6. A comparison of Figs. 5 and 6 shows that F1 corresponds to J3, F2 to J4, and F3 to J2 based on similarities between the fissure orientations and joint orientations. Typically, the joints occur in pairs—a J1–J2 pair and a J3–J4 pair—much like the fissures F1 and F2 that form orthogonal pairs above the North Coalbed Fire. Condon classifies the J1–J4 joints as extension joints, due to the lack of features such as slickenside striations that would suggest lateral shear movement and the presence of plumose structures, arrest lines, and twist hackle features that indicate extension joints [15]. Whereas J1, J2 and J3 are stratigraphically continuous through multiple beds, J4 fractures only cut through the sandstone in interbedded sequences of sandstone and shale. Their orientation ranges are as follows: J1 (N4E–N23E), J2 (N72W–N83W), J3 (N41E–N64E) and J4, (N24W–N49W). Joints J1, J2, and J3 have exposed lengths of roughly 1–5 m, and are spaced 0.15–6 m. J4 exposed lengths are less than 2 m, and the spacings are more inconsistent [15]. The fissures above the North Coalbed Fire were mapped using a pack-mounted GPS receiver in order to place them with respect to the topography of North Coalbed Fire site. In addition, the GPS was used to digitize the topography and to mark the locations of boreholes that have been drilled in the area. The GPS device used in the survey was a Trimble ProXH, and the points recorded had better than 1 m accuracy, with most having better than 0.5 m accuracy after differential correction. Fig. 7a shows the digitized representation of the surface overlying the North Coalbed Fire. The contour map approximately represents the region bounded by the red dotted box in Figs. 1 and 3a. The left edge of this map traces the contact line between the Fruitland Formation and the Pictured Cliffs Sandstone (cf. Figs. 3a and b). The dominant N50E trending fissures are nearly parallel to the local strike of the Hogback Monocline. The black lines represent narrow fissures that have been grouted using a specialized concrete produced by Goodson and Associates [7]. The concrete was injected into identified openings in 2000 in an attempt to smother the fire. Boreholes were drilled around the grouted fissures, and thermocouples were installed to allow monitoring of temperature changes. These boreholes are shown as open white triangles in Fig. 7a. Although the attempt to extinguish the fire was not successful, the driller’s logs from 2000 provide valuable insight into the subsurface. This particular extinguishing method failed mainly because it was not possible to locate and fill all existing fissures in the region. Fourteen additional boreholes were drilled in 2007. These boreholes are marked with solid triangles in Fig. 7. For these new boreholes, driller’s logs were obtained, and most of the boreholes were logged using caliper, density and gamma ray logs. In one of the boreholes, borehole 7, an 80 ft core was obtained. ARTICLE IN PRESS T.S. Ide et al. / International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 85 Fig. 4. (a) A gaping fissure with an adult inside, (b) a plateau fissure, (c) a molehill fissure with a 0.15 m aperture at the apex, and (d) a narrow fissure venting exhaust gases exceeding 900 1C. The surface information in Fig. 7a can be related to the subsurface information by creating a cross-section along the line A–A00 . This cross-section shows that the depth to coal is approximately 20 m. The cross-section is approximately perpendicular to the prominent N50E fissures. Any boreholes or fissures that lie close to this line are plotted along with the surface topography in Fig. 7b. Where available, a combination of driller’s-logs and well-logs were used to identify the depths and thicknesses of void, ash and coalseams at each intersecting well. If data were missing at a well, lithologies below it are left blank in Fig. 7b. Fissures that intersect the cross-section line A–A00 are represented using red circles. It is worth noting that in borehole 11, no signs of coal combustion were apparent. The last set of fissures occurs up dip of borehole 11, and there are no fissures down dip of this borehole. A black line in Fig. 7b connects the bottom of the coal seam. 4. Formation of fissures—a conceptual model We hypothesize that fissures are created from pre-existing fractures in the overlying sandstone and shale that widen when subsidence occurs. Subsidence results when the burned coal loses structural integrity and collapses under the weight of the overburden. In Fig. 7b, the occurrences of surface fissures coincide with regions where void and ash were encountered during drilling. For example, borehole 4 (solid triangle, Fig. 7b) located near the peak of the topography contains only ash and ARTICLE IN PRESS 86 T.S. Ide et al. / International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 Fig. 5. A rose diagram showing the orientation and the lengths of the fissures found above the North Coalbed Fire. The characteristic length scale is 100 m. Fig. 6. (Bottom) Four stereonets reproduced from Condon, 1988. (a) J1 joint, (b) J2 joint, (c) J3 joint, and (d) J4 joint. coal. The lack of a void in this well suggests that subsidence occurred, and thus both the ash and void are fully compacted. Fissures located between boreholes 4 and 5 may have resulted from this subsidence. Similarly, some of the void space may have been compacted at well 5, causing a fissure to open-up down dip of this borehole. The notion of subsurface compaction leading to surface deformation and fracturing is not new. It is explored in Whittaker and Reddish’s work on subsidence related to long-wall coal mining [27]. They describe surface profiles associated with various subsurface subsidence configurations. Their work is based on examples from various long-wall coal mining sites and includes field observations, experimental, and numerical results. In long-wall mining, the excavation front advances much like we envision the combustion front may move through the coalseam in a coalbed fire. Fig. 8 is a conceptual model of subsidence near a long-wall mining process [27]. Here, tensile fractures develop in strata immediately overlying the collapse. This figure can be also be used to illustrate an empirical relationship presented in their work, which shows that the ratio of the length of coal excavated (L) to the depth (d) of excavation must typically exceed 1.4 for maximum subsidence to occur [27]. Adjacent unmined parts of the coalseam and a natural arch that develops above the coal removal site may be capable of supporting most of overburden when L/d is less than 1.4 [27]. There are two key differences between their study and the work presented in this paper. First, the North Coalbed Fire is burning 20 m below the surface, whereas longwall mining typically occurs at much greater depths [27]. Second, pre-existing vertical joints and their response to subsurface compaction are not discussed by Whittaker and Reddish [27]. Previous studies of coalbed fires have also suggested that subsurface subsidence leads to the formation of fissures at the surface [28–40]. Fig. 9 is from one such study of a Coalbed Fire in China, where subsidence apparently played a significant role in opening surface fissures indicated by the arrows. Most of these studies did not examine whether fissures resulted from the widening of pre-existing joints in the region. In Chen’s work [29], it is shown that fissure orientations coincide with joint orientations in the sandstones overlying the coalbed fire in Ruqigou, China. In this study, however, relationships between variables such as the location and magnitude of subsidence and the widths of surface fissures were not established [29]. In a coalbed fire combustion simulation model presented by Huang [41], the fissures were modeled as fixed boundary conditions, through which exhaust gases can escape and fresh oxygen can enter, irrespective of the location of the combustion front. Similarly, in the numerical model of Wessling et al. [40], mechanical processes such as subsidence and fissure openings were not considered. By establishing a first order relationship between combustion front location and fissure opening width as a function of governing variables such as depth, length of collapse, proximity of pre-existing fissures, and the stiffness of the overburden rock, we hope to aid future numerical modeling of coalbed fires. Observations at an outcrop about 1 km north of the North Coalbed Fire shows how subsurface subsidence can cause preexisting fractures to open at the surface. This outcrop exposes a fossilized coalbed fire, subsidence, extension fractures and fissures. At the outcrop, shown in Fig. 10a, a coalseam is overlain by 10 m of sandstone, shale, and siltstone. A person 1.5 m tall standing to the right is used as a scale. There are two prominent features at the outcrop: the fissure that runs down the middle of the outcrop, and the deformed ash layer towards the bottom of the outcrop. The fissure down the middle of the photograph is labeled as Fissure 2, and this fissure has an opening of around 0.5 m at the surface. When the coalseam was consumed by a combustion front moving from the right to left, we suggest the ash deformed by compaction under the weight of the overburden. The maximum collapse recorded at the outcrop is 1.5 m. Features at this outcrop such as Fissure 2 and the subsided ash layer were mapped using a laser rangefinder produced by LaserCraft Inc. [42]. The digitized version of the outcrop is ARTICLE IN PRESS T.S. Ide et al. / International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 87 Fig. 7. (a) A contour map of the North Coalbed Fire site, fissures and wells created using a pack-mounted GPS. Red lines are gaping fissures, green lines are plateau/offset fissures, magenta lines are molehill/buckling fissures, and blue lines are narrow fissures. The cross-section is created along A–A00 . (b) A cross-section of the North Coalbed Fire site along A–A00 . Red circles indicate locations of fissures that intersect the line. Numbers above the surface represent borehole numbers. [For interpretation of the references to color in this figure legend, the reader is referred to the webversion of this article.] Fig. 8. A conceptual model of subsidence associated with long wall mining. Tensile stress fractures associated with the collapse are shown. L signifies the length of coal excavated, and the d the depth below the surface of the seam being mined [27]. Fig. 9. A picture of a subsided area and fissures nearby (indicated by arrows) in a coalbed fire at the Wuda Syncline, Inner Mongolia Autonomous Region, China. (Courtesy of Chris Hecker, ITC, 2008.) juxtaposed next to the photo of the outcrop in Fig. 10b. Note how the tabular coalseam is deformed due to the collapse of the ash layer. Above the collapse, opening fractures, much like those depicted in Fig. 8, were observed. In addition, four fissures with more modest openings were mapped over the collapse. In subsequent sections, when we compare numerical solutions to our measurements at this outcrop, we assume that Fissure 2 in Fig. 10b widened largely due to the collapse of the combusted coal layer and that the weathering process to expose the outcrop did not significantly enhance the opening. ARTICLE IN PRESS 88 T.S. Ide et al. / International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 Fig. 10. (Left) A picture of an outcrop near the North Coalbed Fire with an exposed fossilized coalbed fire, subsidence and associated surface fissures; (right) Some features from the same outcrop mapped using a Laser Range Finder. The major features are depicted using thicker lines. 5. Numerical modeling Numerical models were employed to examine whether preexisting joints could pull open to form fissures when subjected to the stresses due to the overburden weight and those induced by a subsurface collapse. The mechanical effects of subsurface subsidence on the jointed strata overlying the coal were modeled using a Boundary Element Method (BEM) formulation for a line source of displacement discontinuity in an elastic half-plane. This problem formulation is an adaptation of the displacement discontinuity method [43]. The BEM code is a modified version of Martel’s Matlab BEM code [44], which in turn is based on the original Fortran code presented in Crouch and Starfield [43]. Several key assumptions are made in this model, including an elastic homogeneous medium with a reduced stiffness coefficient, infinitesimal strain, a state of plane strain, and a flat traction free surface. The rock above the collapsing coalseam is modeled using a reduced stiffness coefficient in place of explicitly modeling each fracture and joint in the overburden. The use of reduced stiffness coefficients compared to the values measured in experiments is justified in the previous literature on fractured rock deformation [45,46]. Hooke’s Law is used to relate stress and strain, while the infinitesimal strain assumption dismisses higher order displacement derivative terms in the relationship between strain and displacement [47]. The infinitesimal strain assumption admits the use of the method of superposition, which is used to calculate stress and displacement distributions in the domain and to create a half-plane surface. The plane strain assumption restricts any displacement perpendicular to the plane of the model [43]. Finally, a flat surface is modeled rather than the actual topography over the coalbed fire outcrop for simplification. Although these assumptions lead to a model that, at best, approximates the deformation of jointed rock over a coalbed fire, it nevertheless helps to build an intuitive understanding between subsidence and fissure opening, which has not been explored in today’s coalbed fire modeling literature [36,40,41]. In the BEM code, discretized horizontal elements are used to model the coalseam, and discretized vertical traction free elements are used to model pre-existing joints in the overburden. The infinite plane is transformed into a half-plane by introducing the principle of superposition to create a traction free boundary condition along the x-axis [43]. Stress boundary conditions are perturbed along the horizontal elements to simulate a collapse as Fig. 11. Definitions of variables and dimensionless groups used in the BEM model. E and szz have units of MPa, while fd, fl, a and d have units of m. the coal burns, and the elastic domain is deformed as a result of this perturbation. Stresses and displacements that arise at any point in the domain can be calculated by combining the contribution of stresses and displacements from each element [43]. The stress distribution in the elastic material is a function of the location and orientation of the boundary elements and the boundary conditions on them. Fig. 11 defines the variables and applicable dimensionless groups used in this modeling. E is Young’s modulus, and szz is the normal compressive stress defined along the horizontal elements to simulate the downward pressure due to the overburden. These variables both have units of stress (MPa). All other variables have units of length (m), and they are defined as follows: fd is the height of the vertical fracture, fl is the distance between the vertical fracture and the edge of the horizontal collapse, d is the depth, and a is the horizontal length of the collapse. We first introduce a domain with no vertical joints in order to illustrate the stress distribution that arises as a result of collapse of a continuous overburden. We then introduce a vertical fracture, and compare how it reacts to a subsidence event when located in regions of induced tensile stress. This is followed by a sensitivity analysis to demonstrate the behavior of vertical joints with respect to various model variables. Finally, a BEM model is constructed from the outcrop mapped using the laser range finder (cf. Fig. 10b), and simulation results are compared to field observations. In the first example, a 12 m horizontal line of elements that is located 10 m below the surface is deformed by applying a uniform ARTICLE IN PRESS T.S. Ide et al. / International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 compressive stress of 0.25 MPa, which is exerted by the weight of the overlying rock. The elastic modulus of the overburden is 10 MPa, and a maximum compaction of 1.5 m is induced at the horizontal elements. Fig. 12 depicts the distribution of the horizontal component of normal stress, sxx, in response to the inward directed displacement discontinuity on the horizontal elements. The sign of sxx at the surface is indicated by the words tensile (+) and compression (). The blue solid line along the bottom of the figure indicates the horizontal elements subject to subsurface subsidence. We suggest that this inward directed relative motion is similar to what would occur as compaction of the coalseam developed during burning. Directly above the elements at the surface sxx is compressive. The greatest concentrations of surface tensile stresses emanate diagonally upward from the ends of the line of collapse. A modification to the first simulation investigates the effects of the collapse on traction free vertical joints. The setting and the parameter values are the same as the first simulation (cf. Fig. 12), except vertical elements are introduced to simulate the joint. The vertical elements are placed at x ¼ 12 m, where tensile stresses found in the first case (cf. Fig. 12). Fig. 13 shows the model geometry and the resulting normal horizontal stress (sxx) distributions when a horizontal collapse occurs near the vertical fracture. A comparison of Figs. 12 and 13 shows that if a vertical joint exists off to the side of the compaction zone, sxx relaxes and becomes less tensile as the joint opens. Figs. 14 compares the horizontal displacements between the two cases discussed in this section, the model without vertical fracture and the model with the vertical fracture. The horizontal 89 displacements at the surface have been made dimensionless by the maximum vertical subsidence induced along the horizontal elements. Here a positive displacement signifies a movement to the right, and a negative displacement indicates a movement to the left. Horizontal surface displacements are continuous when there are no vertical fractures since the domain is modeled as an elastic medium. In contrast, surface displacements are perturbed during the subsidence when a fracture is located within the tensile region. The right side of the fracture—the edge closer to the induced subsidence—displaces towards the region of the collapse horizontal elements, while the left side does not displace as much, so the model fracture opens. This result shows how preexisting joints in tensile regions may widen to form fissures. A sensitivity study was undertaken to explore how the opening of vertical joints are influenced by the governing variables presented in Fig. 11. Four dimensionless groups are chosen to represent the relationships between the variables. P1, or E/sxx, is the ratio of Young’s modulus of the rock to the stress imposed along the horizontal elements to induce subsidence. P2, or fd/d, is the ratio of the height of the vertical fracture to the depth at which compaction occurs. P3, or a/d, is the ratio of the horizontal length of subsidence to the depth. Finally, P4, or fl/d, is the ratio of the distance between the vertical fracture and the edge of the collapsed region to the depth. These groups are plotted against a dimensionless length scale, UmaxOpening/UmaxCollapse, which relates the horizontal displacement of the joint at the surface to the maximum vertical subsurface subsidence along the horizontal elements. Here, a negative dimensionless length means that the edges of the vertical elements displace away from each other, or in Fig. 12. Subsidence along horizontal elements (blue solid line, bottom center) and resulting stress distributions in the domain. Tensile stresses emanate diagonally upwards from the edge of the horizontal elements. Colorbar in MPa. [For interpretation of the references to color in this figure legend, the reader is referred to the webversion of this article.] Fig. 13. A vertical joint located to the left of the collapsed region. Tensile stresses near the vertical joint are relaxed due to the traction free elements. Fig. 14. Horizontal displacements at the surface for cases with no fracture (solid line) and with a fracture (dotted line). The model with a fracture in the domain shows a displacement discontinuity indicating an opening. ARTICLE IN PRESS 90 T.S. Ide et al. / International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 other words, the joint opens. Simulation results show that this dimensionless length does not vary with respect to P1, and thus the following analyses are limited to demonstrating the dependence of the dimensionless length scale on P2, P3, and P4. The results presented from the sensitivity analyses can be used, on a first order basis, to estimate the location and the magnitude of the subsidence when the only the widths of the surface fissures are known. Fig. 15 is a plot of the relationship between the dimensionless opening (Umax Opening/Umax Collapse) and P4 (fl/d). Each line represents a different value of P2 (fd/d). In the following discussion, the maximum vertical subsidence length, UmaxCollapse, depth, d, and length of subsidence, a, will be fixed to simplify our analysis. As a consequence of fixing both d and a, P3, the ratio between the two variables is constant. Variables a and d are specified such that P3 ¼ 1.0. Fig. 15 shows that for a constant value of P2, or for a fixed height of the fracture, a maximum horizontal displacement at the surface is observed when P40.8. The fissure width reaches a maximum when it is located diagonally above and to the side of the zone of compaction, consistent with where a concentration of tensile stresses was observed in Fig. 12. The fissure opening decays to 0 as the vertical joint moves farther away from the region of subsidence regardless of the height of the fracture. This result is reasonable since the stresses associated with the subsidence decay with increasing distance. Fig. 15 also shows that when P2, or the height of the pre-existing joint, increases, the magnitude of the opening also increases. Based on the results, when P3 ¼ 1.0, the maximum fissure opening is observed when the pre-existing joint is located at P40.8 and is stratigraphically continuous down to the collapse horizon, or P2 ¼ 1. Fig. 16 is a similar plot. It shows how the dimensionless length scale (Umax Opening/Umax Collapse) depends on P4 (fl/d) for varying values of P3 (a/d) with both the maximum subsidence distance (UmaxCollapse) and depth (d) fixed. In addition, fd, the height of the fracture, is fixed and defined such that P2 (fd/d) is 1.0. The figure shows that for a fixed value of P3, which represents the length over which the collapse occurs, the fissure opening again depends strongly on the location of the vertical joint. The fissure opening decays to 0 far away from the subsidence and is the widest between 0.5oflo1.0 depending on the value of P3. As P3 increases, the horizontal displacement at the surface increases, which makes sense since a longer subsidence length leads to a greater tensile stress emanating upwards towards the surface. The location where the maximum fissure opening is observed moves closer to the edge of the horizontal compaction when P3 increases. In other words, the region of tensile stresses that extends upwards towards the surface lies more directly above the horizontal compaction as the length of subsidence increases when depth is constant. We investigate whether the relationship between the subsidence and fissure opening at the outcrop in Fig. 10a and b can be predicted using this numerical model. In this simulation only the most prominent fissure at the outcrop, indicated on Fig. 10b, is explicitly modeled using traction free elements. This fissure at the outcrop is slightly oblique and appears to be stratigraphically continuous down to the depth of the collapse. The bottom of this fissure is located approximately 2.5 m left of the edge of the collapsed zone. All other fissures and tensile stress fractures at the outcrop are incorporated into the model by reducing the bulk stiffness of the rock to 10 MPa, which is one to three orders of magnitude lower than published elastic moduli of various shales and sandstones. The length of subsidence is approximately 12 m at the outcrop, although the exact length is not known due to limited exposure at the outcrop. The subsidence occurs approximately 10 m below the surface. This ratio of length of collapse/ depth is close to the critical extraction value of 1.4 observed for collapses associated with long-wall mining operations [27]. The collapsing ash layer is modeled using tilted elements with appropriately defined stress boundary conditions. The depth where the collapse occurs is approximately 10 m, maximum subsidence is approximately 1.5 m, and a 0.5 m surface opening of the vertical fracture was observed at the outcrop. When a collapse is induced in the numerical model, tensile stresses are relaxed around the vertical fissure by opening. Fig. 17a Fig. 15. Dimensionless length vs. P4 (fl/d). Each line represents a different value of P2 (fd/d), while P3 (a/d) is kept constant at 1.0. ARTICLE IN PRESS T.S. Ide et al. / International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 91 Fig. 16. Dimensionless length vs. P4 (fl/d). Each line represents a different value of P3 (a/d), while P3 (fd/d) is kept constant at 1.0. Fig. 17. (a) Geometric representation of the two prominent features found at the outcrop (cf. Fig. 10). (b) Tensile stresses dominate around the diagonally oriented joint, which is stratigraphically continuous down to the depth of collapse. fd10 m, d10 m, a12 m, and fl2.5 m. shows the geometry of the model and Fig. 17b is the sxx stress distribution map resulting from the collapse when a downward stress of 0.25 MPa is defined along the horizontal elements. The dimensionless opening, UmaxOpening/Umax Collapse is around 0.23 when these parameters are used to simulate the fissure opening and the collapse. Alternatively, this value could have been obtained by calculating appropriate dimensionless variables, and using Fig. 16 to obtain the dimensionless length scale. Based on the model assumptions, appropriate dimensionless values are calculated as follows: P2 ¼ fd/d1, P3 ¼ a/d1.2, P4 ¼ fl/d0.25. Although this method approximates the coalseam and the traction free fracture to be horizontal and vertical, respectively, it nevertheless gives a dimensionless length scale of approximately 0.23. Both of these values are consistent with the UmaxOpening/UmaxCollapse observed at the outcrop. At the outcrop, UmaxOpening ¼ 0.5 m and UmaxCollapse ¼ 1.5 m, giving a length scale ratio of 0.3. The discrepancy is attributed to relatively simple assumptions associated with this numerical model. In future modeling efforts, these assumptions will be made more realistic. The results from the numerical simulation suggests that preexisting joints that are located above existing coalbed fires can open when they are in regions of tensile stress induced by the subsidence. Fig. 18 is a conceptual model of how the propagation of the combustion front at the North Coalbed Fire can lead to opening of fissures at the surface. The figure accounts for the local geology, geometry and the findings from the numerical investigations. In the figure, the lithology above the coalbed fire is characterized as either shales or sandstones. At the site, shales are often softer than the sandstones. In this conceptual model, the coalseam is transformed into a layer of ash as the thin combustion front propagates through the lower coal. The overlying strata ARTICLE IN PRESS 92 T.S. Ide et al. / International Journal of Rock Mechanics & Mining Sciences 47 (2010) 81–93 Fig. 18. A conceptual model depicting the mechanism of how pre-existing joints above the North Coalbed Fire open up to form a fissure. collapse, and a pre-existing joint opens up to form a surface fissure. The underlying Pictured Cliffs sandstone remains intact. Opened fissures above the fire may act as conduits that connect the surface and the coalseam. These fissures allow combustion gases to escape from the combustion zone, and enable fresh oxygen to reach the coalseam in order to keep the combustion alive. 6. Conclusions At the surface above the North Coalbed Fire, which burns along the Hogback Monocline in the San Juan Basin, numerous fissures form orthogonal patterns. Some of these fissures vent hot exhaust gases from the subsurface, an indication of a burning coalseam in the subsurface. A combination of available geologic data from previous surveys, observations and measurements from the field allows identification of a mechanism for the formation of surface fissures. The hypothesis is that pre-existing joints in the strata overlying the North Coalbed Fire widen to form fissures when the underground coalseam combusts and then compacts as its structural integrity is lost. Previous literature has suggested or described relationships between surface deformation and subsurface subsidence, but no work has established first order functional relationships between variables that govern fissure widening and subsurface subsidence in a coalbed fire. In this study, a simple BEM model was formulated to simulate the collapse of the coalseam and the opening of pre-existing vertical fractures. Results show that the aperture of the fissures at the surface depends strongly on where the vertical fracture is located with respect to the subsurface subsidence. The sensitivity analyses performed using this simulator also demonstrate the relationships amongst the governing variables defined in this study. Those relationships can be used to estimate the location and subsidence magnitude based on the fissure locations and width measured at the surface. The model was tested using a dataset obtained from a near by outcrop that showed evidences of subsidence in a combusted coalseam and an opening of a vertical fracture above. Many assumptions were made in the simple numerical simulation, and thus there is some discrepancy between the model results and measured values. Acknowledgments The authors of this paper would like to thank: Bill Flint of the Southern Ute Indian Tribe for facilitating fieldwork details and his help in securing funding; the Southern Ute Indian Tribe for their gracious hospitality, allowing us to access their land and their continued support; Jonathan Begay, Kyle Siesser and Ashley Neckowitz for their help in the field and the Stanford Global Climate and Energy Project and its contributors for their funding that made this research possible. 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