Abstract:
This study investigated a natural analogue for CO
2 leakage near the Green River, Utah, aiming to understand the influence of various factors on CO
2 leakage and to reliably predict underground CO
2 behavior after injection for geologic CO
2 sequestration. Advective, diffusive, and eruptive characteristics of CO
2 leakage were assessed via a soil CO
2 flux survey and numerical modeling. The field results show anomalous CO
2 fluxes (> 10 g m
-2 d
-1) along the faults, particularly adjacent to CO
2-driven cold springs and geysers (e.g., 36,259 g m
-2 d
-1 at Crystal Geyser), ancient travertines (e.g., 5,917 g m
-2 d
-1), joint zones in sandstone (e.g., 120 g m
-2 d
-1), and brine discharge zones (e.g., 5,515 g m
-2 d
-1). Combined to similar isotopic ratios of gas and progressive evolution of brine chemistry at springs and geysers, a gradual decrease of soil CO
2 flux from the Little Grand Wash (LGW; ~36,259 g m
-2 d
-1) to Salt Wash (SW; ~1,428 g m
-2 d
-1) fault zones reveals the same CO
2 origin and potential southward transport of CO
2 over 10-20 km. The numerical simulations overtly exhibit lateral transport of free CO
2 and CO
2-rich brine from the LGW to SW fault zones through the regional aquifers (e.g., Entrada, Navajo, Kayenta, Wingate, White Rim). CO
2 travels predominantly as an aqueous phase (X
co2=~0.045) as previously suggested, giving rise to the convective instability that further accelerates CO
2 dissolution. While the buoyant free CO
2 always tends to ascend, a fraction of dense CO
2-rich brine flows laterally into the aquifer and mixes with the formation fluids during upward migration along the fault. The fault always enhances advective CO
2 transport regardless of its permeability (k). However, only the low-k fault scenario engenders development of CO
2 anticlinal trap within the shallow aquifers (Entrada and Navajo), concentrating high CO
2 fluxes (~1,273 g m
-2 d
-1) within the northern footwall of the LGW fault similar to the field. Moreover, eruptive CO
2 leakage at a well (Crystal Geyser) solely appears under the presence of anticlinal trap. Thus, it can be concluded that the LGW fault is likely low-permeable, 0.01 md ≤ k
h <0.1 md and 0.5 md ≤ k
v < 1 md, which could be used as a good starting point for other studies and further improved.