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Full Case Study

Coupled Simulation of Underground Coal Gasification (UCG) Using CMG STARS

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Underground Coal Gasification transforms coal into energy underground, but doing so safely and efficiently requires understanding one of the most complex coupled subsurface processes in energy engineering.ย 

It is an in-situ process that converts coal into syngas by injecting oxidants into a coal seam and producing combustible gases through a network of high-temperature chemical reactions.

In this study, CMG STARS was used to develop a fully coupled thermal-hydro-mechanical-chemical (THMC) model of UCG, capturing the evolution of the gasification cavity, chemical reactions, composition of produced syngas, production behavior, and subsidence.

Outcome: The model demonstrates how coupled simulation can predict cavity growth, gas production, and geomechanical deformation, providing critical insights for safe and efficient UCG operations.ย 

What is Underground Coal Gasification (UCG)?

UCG is a process where coal is converted into gas underground, rather than being mined and processed at the surface.

The process involves:

  1. Injecting oxidants (air, oxygen, steam) into a coal seamย 
  2. Initiating combustion and gasification reactionsย 
  3. Producing syngas (CO, Hโ‚‚, CHโ‚„, COโ‚‚) through a production wellย 

How It Differs from Conventional Reservoir Processes?

Unlike oil & gas production:

  • Solid coal is converted into gas in-situ
  • A cavity is created and grows over timeย 
  • Rock structure and stress conditions evolve dynamicallyย 

This makes UCG not just a flow problem, but a reactive, deforming system.ย 

Why UCG is Complex to Model?

UCG is one of the most complex subsurface processes to simulate because it requires simultaneous coupling of multiple physical domains.

1. Chemical Reactions and Kinetics

UCG involves multiple reactions, including:

  • combustionย 
  • steam gasificationย 
  • methanationย 
  • pyrolysisย 

Example (Pyrolysis: from the model below):

Coal ๐Ÿกช Char + CO + COโ‚‚ + Hโ‚‚ + CHโ‚„ย 

Despite the interdependencies among the reactions, each reaction has:

  • different activation energiesย 
  • temperature dependenciesย 
  • competing pathways

2. Extreme Thermal Conditions

  • Temperatures can exceed 1000ยฐC locallyย 
  • Strong heat gradients developย 
  • Heat drives reaction ratesย 

3. Complex Fluid Transport

  • Gas flows through evolving porous media with dynamically changing structure
  • Permeability and porosity vary significantly over time
  • Composition changes continuously, particularly during the early stages of the cavity formation
  • Multiphase flow may occur if tar is formed, although this is rare and generally not significantย 

4. Evolving Geometry (Cavity Growth)

  • Coal consumption significantly increases pore volume and, consequently, porosity over time. This alters gas-phase flow behavior, transitioning it from Darcy flow to non-Darcy and potentially turbulent flow.
  • Collapse of coal and char from the roof and sidewalls of the cavity changes flow paths and gas mixing within the cavity, which can indirectly affect reaction efficiency.

ย This implies that the treatment of coal seams in the UCG process is fundamentally different from that of conventional oil and gas reservoirs, where the available pore volume for fluids changes far less significantly.

5. Coupled Geomechanics

As the cavity grows:

  • overburden stress redistributesย 
  • subsidence occursย 
  • fracture patterns may changeย 

This directly impacts:

  • permeability and porosity
  • flow pathwaysย 
  • operational safety

Solution: CMG STARS Offers a Fully Coupled Approach

CMG STARS enables:

  • thermal simulation (high-temperature processes)ย 
  • chemical reactions and kineticsย 
  • solid-solid (coal ๐Ÿกช char) and solid-gas (char ๐Ÿกช gas)ย  conversionย 
  • multiphase flowย 
  • dynamic porosity/permeability evolutionย 
  • coupled geomechanics (subsidence, stress)ย 

This makes it uniquely suited for UCG modeling.

Operational Context: Model Overview

From the simulation setup:

  • Grid: 50 ร— 50 ร— 12ย 
  • Block size: 0.5 m ร— 0.5 m ร— 0.5 mย 
  • Wells: 1 injector and 1 producerย 
  • Perforations: Layer 10ย 
  • Initial porosity: ~8%ย 

Initial Conditions

  • Temperature: ~60ยฐCย 
  • Pressure: ~11.5 MPaย 
  • Water saturation: ~0.70ย 
  • Coal concentration: ~12,700 gmol/mยณย 

Reactions Modeled

The simulation includes:

  • pyrolysisย 
  • combustionย 
  • gasification reactionsย 

With full kinetic parameters:

  • activation energyย 
  • frequency factorsย 

This enables realistic gas composition prediction. The key step in modeling UCG reactions in STARS is representing the pyrolysis process as accurately as possible, in which coal is consumed to produce char that subsequently combusts and generates the required in-situ heat. In addition, this process produces significant quantities of gaseous species that serve as reactants in subsequent gasification and combustion reactions. Leveraging coal elemental analysis to derive realistic stoichiometric coefficients for the pyrolysis reaction is therefore of critical importance.

Key Results

1. Gas Production Behavior

The simulation shows:

  • rapid increase in gas productionย 
  • stabilization as cavity developsย 
  • eventual decline as coal is consumedย 

Figure 1: Simulated gas production showing rapid initial increase as gasification reactions intensify, followed by stabilization and eventual decline as coal is consumed and the cavity evolves.

Insight

Gas production is directly linked to:

  • reaction front movementย 
  • available coal volumeย 
  • evolving flow pathways connecting the injection points (cavities) to production perforation

Gas production strategies must account for reaction front progression and cavity evolution to avoid premature decline.

2. Cavity Growth and Porosity Evolution

After ~90 days:

  • significant increase in porosity near injection zoneย 
  • formation of a clear gasification cavityย 

Figure 2: Shows the formation and expansion of the gasification cavity between injector and producer wells. Increased porosity highlights regions where coal has been consumed and converted into gas.

Insight

The cavity is not uniform. It evolves based on:

  • heat distributionย 
  • reaction kineticsย 
  • flow direction, for example, rapidly developing upward as gas components rise within the cavityย 
  • Gas component residence time, which is influenced by the production rate and the degree of cavity-producer connectivityย 

3. Temperature Front Propagation

Pyrolysis and char combustion reactions occur mainly along the cavity boundaries. However, due to the tendency of gas flow toward the production perforation, the high-temperature front is typically oriented in that direction and gradually advances toward the producer over time.

Figure 3: Shows temperature profiles at different times showing the advancement of the high-temperature reaction zone. Thermal gradients define the active gasification region and control reaction kinetics and gas generation.

Insight

  • High-temperature zones define exothermic reaction regionsย 
  • Heat transfer, mainly due to gas convection flow, controls reaction progressionย 
  • ย Thermal breakthrough, characterized by high temperatures at the production perforations, dictates production behaviorย 

4. Coal-to-Char Conversion

Results show:

  • conversion of coal near injection zone at early time and at the cavity boundary at later time
  • formation of char due to pyrolysis process
  • progression toward producerย 

Figure 4: Distribution of coal and char at the end of injection, showing progressive consumption of coal near the injector and transformation into char as reactions advance toward the producer.

Insight

Reaction zones migrate dynamically, altering:

  • material compositionย 
  • flow propertiesย 
  • gas yield

5. Geomechanical Response and Subsidence

Simulation shows:

  • measurable subsidence after 90 daysย 
  • stress redistribution across reservoirย 

Figure 5: 3D visualization of subsidence resulting from coal removal and cavity expansion, highlighting the spatial extent of geomechanical deformation.\

Figure 6: Integrated view of pressure distribution and vertical displacement, demonstrating the interaction between fluid flow, reaction progression, and geomechanical deformation.

Insight

Geomechanics directly affects:

  • structural integrityย 
  • flow pathwaysย 
  • operational safetyย 

Subsidence prediction is critical for ensuring well integrity and minimizing surface impact.

Why This Matters

This case demonstrates that UCG is not just about maximizing gas production.

It requires understanding:

  • where the cavity will growย 
  • how reactions evolve spatiallyย 
  • how the reservoir deformsย 
  • how production changes over timeย 

Key Takeaways

  • UCG is a fully coupled thermal-hydro-mechanical-chemical (THMC) processย 
  • Cavity growth (resulting from reactions) and subsidence (resulting from material deformation) must be modeled togetherย 
  • Gas production depends on type and rate of injected oxidants, reaction kinetics, and heat distributionย 
  • Flow behavior evolves as coal is consumedย 
  • CMG STARS enables end-to-end modeling of all governing physicsย 

Best Practices for UCG Modeling

  • Include reaction kinetics, not just simplified conversionsย 
  • Model cavity growth dynamicallyย 
  • Incorporate geomechanical effects for safety and accuracyย 
  • Perform time-dependent simulations to capture system evolutionย 

Conclusion

Underground Coal Gasification is one of the most complex subsurface processes to model, requiring the integration of chemical reactions, fluid flow, heat transfer, and geomechanics.

This study demonstrates that CMG STARS provides a unified framework to simulate these coupled processes, enabling accurate prediction of gas production, cavity evolution, and subsurface deformation.

By capturing the full system behavior, engineers can move beyond simplified assumptions and make more informed decisions about UCG design, operation, and safety.

About This Resource

Reference#:ย https://doi.org/10.1016/j.fuel.2013.07.091

Year: 2026

Software: STARS

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