1. Introduction
Since the late seventies numerous studies have pointed to high carbon dioxide emissions in tectonically active regions frequently hosting geothermal systems [1,2,3]. High-temperature geothermal systems form in active magmatic regions, where a large amount of heat is lost from the Earth’s interior. The heat and mass transfer from a cooling magmatic intrusion to the groundwater drives fluid convection, boiling, and steam separation [4]. In the low-permeability and high-temperature ductile rocks hosting the intrusion, the heat transfer is dominated by conduction. Contrarily, convection dominates heat transfer in the permeable rocks of geothermal systems. The boiling of the convecting liquids produces a vapor-dominated phase with a significant amount of CO2, which flows towards the surface. Consequently, geothermal regions represent prevalent emitters of both geogenic CO2 and heat [5,6,7,8,9].
In these areas, CO2 is either emitted in the atmosphere through focused fumarolic vents, boiling pools, and areas of diffuse soil degassing [10,11,12], or dissolved in groundwater [13,14]. In the late 1990s, Kerrick et al. [5] developed a methodology based on convective heat flow measurements to estimate the relative flux of CO2 from geothermal systems. Subsequently, the development of techniques for measuring CO2 fluxes from volcanic and geothermal soil, such as the accumulation chamber [15] and eddy covariance [16], enabled the convective heat flow to be estimated by applying the reverse approach.
The aim of this study was to synthesize in a unique document the principles and results of CO2-based techniques for the estimation of heat flow, referring to published and unpublished cases. In detail we will show how the measurement of soil CO2 degassing can be used to compute both the thermal emission from the hot soils of hydrothermal sites and the total heat associated with the convection of geothermal liquids. The published results obtained at Latera caldera (Italy) are presented and discussed together with those obtained from unpublished CO2 flux measurements performed at the Torre Alfina geothermal area (Italy). These cases show that CO2 flux measurements find useful applications in geothermal prospecting because they allow one to cheaply estimate the natural advective-convective heat flow.
Finally, we re-elaborated the published data of a regional investigation on the aquifers of the central Apennine (Italy) [17] computing, aquifer by aquifer, the total deeply derived CO2 emission and the geothermal heat flow from these hundreds of square kilometers wide areas. The results, supported by the CO2 concentrations and enthalpies of geothermal fluids of the region, indicate the presence of a geothermal source particularly rich in CO2 in central Italy.
2. Geothermal Heat Flow from the Diffuse Emission of CO2
According to [5], in geothermal systems heat and CO2 are transferred from depth to the surface through the convection of geothermal liquids (Figure 1). Based on this conceptual model, Kerrick et al. [5] used the heat flow measured at the surface to calculate the CO2 emission from the Taupo geothermal zone (New Zealand). Assuming the same conceptual model, in reverse the measured emission of CO2 can be used to compute the thermal energy of the upflowing geothermal fluids.
Considering that the CO2 flow towards the surface (QCO2 in kg s−1) is sustained by the depressurization and boiling of the geothermal liquid during its upflow (Figure 1), the mass flow rate of the liquid (QL in kg s−1) and the associated thermal energy (QH in MW) can be computed, rearranging the original relation of [5] as:
QL = QCO2/(mCO2 × 0.044)(1)
QH = 10−3 × QL × HL(2)
where HL (in kJ kg−1) is the original enthalpy of the liquid, mCO2 (in mol kg−1) is the original CO2 concentration, and 0.044 is the factor to convert moles to kg. During the boiling of the upflowing liquid, the original energy is divided into a fraction associated with the residual liquid, which is possibly discharged by thermal springs or returned into the system with the descending columns of convective cells (Qres and QH,res in Figure 1), and a fraction transported toward the surface by the separated vapor. This ascending vapor-dominated phase condenses near the surface heating the soil, whereas the low-soluble CO2 is emitted in the atmosphere.According to this model, geothermal areas often host sites characterized by emissions of hydrothermal CO2 from hot soils (steaming ground), which extend over their fumarolic fields. To measure the heat flow from these hot soils, several techniques have been developed since the 1950s [18] (and references therein). In these pioneer works, the heat flow is calculated by measuring soil temperatures at fixed depths and using empirical relations derived from long, time-consuming heat flow measurements with suitable calorimeters. For example, Fridriksson et al. [10] following [18], proposed that qs = 5.2 × 10−6 × t154, where qs is the heat flow (in W m−2) and t15 is the soil temperature (in °C) at a depth of 15 cm. However, this method is not generally valid because the empirically derived relation depends on local conditions, such as soil thermal conductivity and ambient temperature.
More recently Chiodini et al. [6,19] proposed an approach based on the measurement of the diffuse emission of hydrothermal CO2 from hot soils. In this approach the equivalent amount of steam that condenses in the subsurface (Qcond in kg s−1) and the associated heat release (QH,cond in MW) is computed using the following equations:
Qcond = QCO2 × RH2O/CO2(3)
QH,cond = 10−3 × Qcond × (HV, Tcond − HL, Tamb)(4)
where RH2O/CO2 is the H2O/CO2 weight ratio of the original (precondensation) vapor phase, and HV, Tcond and HL, Tamb are the enthalpies of the steam at the condensation temperature (2676 kJ kg−1 for a condensation temperature of 100 °C; [20]) and of the liquid at the ambient temperature (83.9 kJ kg−1 for an ambient temperature of 20 °C; [20]), respectively. These equations are solved assuming a RH2O/CO2 equal to that of the fumaroles located in the zone degassing CO2 [6].In the next sections we present and discuss the results obtained in different hydrothermal areas where QCO2 is used for the estimation of QH,cond and QH.
2.1. Thermal Energy Release from Soils Heated by Steam Condensation (QH,cond)
The approach based on the application of Equations (3) and (4) is strongly supported by the spatial correspondence between hot soils and CO2 emissions, which frequently characterize the hydrothermal areas of active volcanoes and geothermal sites. Figure 2 shows, e.g., the map of CO2 fluxes and soil temperature (at 10 cm of depth) of the Solfatara di Pozzuoli (Campi Flegrei caldera, Italy), where this approach was first tested in 1998 [19]. These maps, as well as those reported in the following figures, were elaborated using the sequential Gaussian simulations (sGs; [21]) method. Equations (3) and (4) were solved with the measured QCO2 (17.6 kg s−1) and RH2O/CO2 (2.2) obtaining the energy released by steam condensation from the Solfatara di Pozzuoli (QH,cond~100 MW, [19]). This thermal energy was released from an area of ~0.5 km2 (Table 1) and constituted the main part of the total energetic budget of the Campi Flegrei caldera. In fact, it was much higher than (i) the conductive heat flux over the ~100 km2 of the entire caldera, (ii) the energy of the earthquakes, and (iii) the energy associated with ground deformation [19]. Subsequently, this method was applied to many geothermal sites in the world. Some examples and their relative references are reported in Table 1, where the acronym DDS (Diffuse Degassing Structure) indicates the areas diffusively emitting the hydrothermal, deeply derived CO2. The cases reported in Table 1 were selected based on the availability of (i) detailed CO2 flux surveys, (ii) estimation of the deeply derived emission (note that in the literature often is reported the total emission but not that related to the deep source), and (iii) the composition of the fumaroles located in the area.
2.2. Thermal Energy of Convective Geothermal Liquid (QH)
In Table 2 we report some results of the method for the estimation of the total thermal energy QH involved in the convective generation of gas emissions (Figure 1) using published [10,12,25] and unpublished data. Equations (1) and (2) were solved assuming HL and mCO2 of the hottest geothermal well as representative of the original convecting liquid. The computations completed at Latera caldera and Torre Alfina starting from the CO2 emission measurements are then described in detail in the following sections. Latera and Torre Alfina are two geothermal systems located in the Quaternary volcanic region of central Italy [31] (and references therein) which emit a low-temperature and dry gas phase, dominated by CO2. We use published measurements of the diffuse CO2 emission at Latera [12], while, in the case of Torre Alfina we use unpublished data.
2.2.1. CO2 Emission and Convective Heat Release from the Latera Caldera
Results of a detailed investigation of the CO2 degassing from the Latera caldera [12] are here synthesized and discussed. The Latera geothermal system is hosted in permeable Mesozoic carbonates covered by impermeable flysch layers and volcanic products (see [12] for a detailed geological setting). Surface manifestations of the active fluid circulation consist of CO2-rich shallow groundwaters, areas of strong soil diffuse CO2 emission, and low-temperature (from 19 °C to 31 °C) CO2-rich gas vents. The CO2 emission was quantified and mapped through 930 flux measurements performed with the accumulation chamber over an area of ~10.8 km2 (Figure 3; [12]). The CO2 flux map shows a NE-SW band of high CO2 emission (Latera DDS), corresponding to the structural high hosting the geothermal reservoir [12,32,33]. Notably, the productive wells of Latera (L3/3D, L2 and L4 in Figure 3) are located in this anomalous band.
The total CO2 emission computed from the map resulted in 497 t d−1, including both the geothermal and biogenic flux contributions. The mean soil biogenic production, which was characterized using a subset of measurements performed in an area far from the main degassing zones (red contour in Figure 3), resulted in 15.7 g m−2 d−1. Removing the biogenic CO2 contribution, the deep CO2 emission from Latera resulted in 328 t d−1 [12]. Then, integrating this large-scale survey with the results of a detailed CO2 flux campaign focused on the biggest gas manifestation in Latera, that is the Puzzolaie area, these authors concluded that the total deep CO2 emission accounted for ~350 t d−1 (4.05 kg s−1).
The total thermal energy involved in the convective upflow and boiling of the geothermal liquids was calculated with Equations (1) and (2), using the published T-mCO2 data of the hottest geothermal liquid (Latera 3D well, T = 238 °C, mCO2 = 0.73 mol kg−1; [34,35]). The geothermal fluid upflow rate (QL), feeding the CO2 emission of 4.05 kg s−1, resulted in 126 kg s−1 and the correspondent thermal energy (QH) in 130 MW.
2.2.2. CO2 Emission and Convective Heat Release from Torre Alfina, Italy
The Torre Alfina system consists of both a geothermal liquid water reservoir with temperatures between 125 and 150 °C and an overlying gas-cap, mainly CO2, at a pressure of about 40 bars [36], located at ~400 m of depth. Similarly to Latera, the reservoir is hosted in a structural high of the Mesozoic carbonate formations overlaid by flysch impermeable layers and by quaternary volcanic products [36,37]. The area above the geothermal system is characterized by high pCO2 groundwaters circulating in the volcanic products [38], CO2-rich gas vents, and areas with visible soil CO2 emissions. Soil CO2 diffuse degassing was investigated with the accumulation chamber method [15] in 2009–2010. This survey consisted of (i) 917 CO2 flux measurements performed in the main CO2 emission area located southward of the Torre Alfina village (named “Le Solfonare” by [39]; Figure 4), (ii) 119 measurements in a peripheral area with slightly high flux values (named “small degassing area”), and (iii) 262 measurements of low CO2 flux randomly distributed in a larger area and specifically performed to quantify the background soil CO2 emissions (Table S1, Supplementary Material).
The CO2 flux map of Le Solfonare, constructed with the sGs method [21], highlights a main NNW-SSE degassing structure and weaker anomalies located eastward (Figure 4). In total, these two anomalous zones emit 104.7 t d−1 of CO2, which become 107.0 t d−1 summing the 2.3 t d−1 released by the small degassing area. This value includes both the geothermal CO2 and the background emission due to the biologic activity in the soil. To separate these two contributions, we applied the GSA (Graphic Statistic Approach described in [15] and in [21]), which is based on the Sinclair’s partitioning method of lognormal polymodal distribution of data [40]. The CO2 flux measurements are reported in the log-probability plot of Figure 5 (grey points), where, for comparison, are also reported the 262 background values as a separated data set (blue points). The distribution of the CO2 fluxes is explainable by the overlapping of the background population (defined only with the blue points) and two other lognormal populations of higher fluxes, representing the deep CO2 contribution (Table 3). Based on the statistical parameters of the Population 1, we estimate an average background CO2 emission of 14.2 g m−2 d−1 which, interestingly, is very similar to the CO2 background flux of Latera, closely located to Torre Alfina and characterized by a similar type of vegetation and use of soil. Considering this background CO2 emission we estimate the total deep CO2 emission at 91.9 t d−1 (1.06 kg s−1). We assume that 35 g m−2 d−1 (95th percentile of Population 1) reflects the threshold value above which the gas emission is totally geogenic-derived. This value is used to delimitate the structures degassing deeply derived CO2 (Torre Alfina DDS, white contour in Figure 4).
The thermal energy involved in the upflow of the geothermal liquid of the Torre Alfina system was computed with Equations (1) and (2), considering temperature and mCO2 data of the wells reported in [34]. Among these data we selected the maximum temperature (150 °C) at which corresponds a mCO2 equal to 0.33 mol kg−1. Considering the CO2 diffuse emission of 1.06 kg s−1, we estimated a geothermal fluid upflow (QL) equal to 73.2 kg s−1 and an associated thermal energy (QH) equal to 46 MW.
3. Enthalpy and CO2 Mass Balances of Regional Aquifers
In the previous section we combined surface measurements of the CO2 flux with the enthalpy and CO2 content of deep liquids to calculate the heat release and the thermal energy of the geothermal fluids exsolving CO2. When the upflowing fluids dissolve in aquifers, we do not need any direct information about the deep fluids to estimate the heat flux and the amount of injected CO2, as they can be calculated through the carbon mass and enthalpy balances of groundwaters.
This approach was used in central Italy [17] where the comparison of the CO2 flux map [42] with the conductive heat flux map [43] points out that the area of anomalous CO2 degassing extends eastward beyond the thermal anomaly (Figure 6). The heat flux shows in fact a sharp decrease from values higher than 100 mW m−2, typical of the Tyrrhenian side, to values lower than 50 mW m−2 in the area of the regional aquifers of the Apennine chain. Here, the large amounts of infiltrating waters that circulate in the permeable carbonate formations possibly cools the crust and causes the low conductive heat flux measured in the area [17,44].
To investigate the heat transfer in this area, Chiodini et al. [17] applied carbon mass and enthalpy balances to 46 springs of high-flow rate located in 11 large carbonate aquifers (Figure 6b). The carbon mass balance of the springs allowed [17] to differentiate the components contributing to the total dissolved inorganic carbon (TDIC), i.e., the carbon deriving from carbonate minerals dissolution (Ccarb) and that from sources external to the aquifers (Cext).
The diagram of δ13Cext vs. Cext (Figure 7) highlights two groups of waters: one characterized by low Cext (mean = 2.3 mmol L−1) and light carbon isotope compositions (δ13Cext from −10‰ to −25‰; blue points), the other by higher Cext (mean = 12.7 mmol L−1) and heavier carbon isotope compositions (δ13Cext from −10‰ to −5‰; magenta points). The first group reflects normal groundwaters with Cext deriving from a mixture of atmospheric CO2 and carbon produced by biogenic sources present in the soil of the recharge areas. The second group forms by the addition of an isotopically heavier carbon (δ13C ~ −1.5‰) source to normal groundwaters. This heavier carbon source is ascribed to the deeply derived CO2 typically emitted from this region, where the numerous and large natural gas emissions of central Italy show a mean δ13C value of about −1.5‰ [45]. The mass flow rate of Cext (QCO2 in kg s−1) in each aquifer is computed by multiplying its concentration by the discharge rate of the structure and the CO2 flux by dividing QCO2 by the surface area of the aquifer.
The enthalpy balance was performed using the method of [46], based on the temperature difference between the recharge water and the water discharged from the spring (ΔT). This is expressible as:
ΔT = Ts − Tr = (Hf × A)/(ρw × Cw × q) + Δz × (g/Cw)(5)
where Ts and Tr are the temperatures of discharge (springs) and recharge water, respectively, Hf is the geothermal heat flux (W m−2), ρw (kg m−3) and Cw (J kg−1 K−1) are the density and the heat capacity of the liquid water, q is the spring volumetric flow rate (m3 s−1), A is the surface area (m2) of the hydrogeological basin of the spring, Δz (m) is the difference between the average elevation of the recharge area and the elevation of the spring, and g is the gravitational acceleration (m s−2) (see [17] for further details on the computation of the different parameters).The results of both carbon mass and enthalpy balances for each aquifer are synthesized in Table 4. The total heat flow rate from each aquifer (QH) was computed by multiplying the mean heat flux Hf by the surface area of the aquifer. The mean values of the CO2 fluxes and Hf of the aquifers are also reported in the map of Figure 6b. This map shows that the aquifers located in the northern and eastern sector of the study area are characterized by both low CO2 fluxes and low Hf, close to values reported for the same area by the conductive heat flux map of Italy (Figure 6b). Conversely, all the other aquifers have much higher Hf values (from 180 to 370 mW m−2) up to one order of magnitude higher than the conductive heat flux. These high Hf values are observed on the Tyrrhenian side and gently decrease moving eastward. Practically, the thermal anomaly characterizing the Tyrrhenian sector of central Italy is considerably wider and extends toward the east including a large portion of the central Apennine, similarly to the deeply derived CO2 emission (Figure 6a).
CO2 and Heat Flows in Central Italy
The heat flow (QH) computed for the 11 hydrogeological structures is plotted against the CO2 mass flow rate (QCO2) in Figure 8 where, for comparison, are also reported relevant data relative to the geothermal systems of central Italy and of other zones of the Earth.
It is worth noting that all the measured or derived data from central Italy point to a source characterized by a similar and high CO2/heat ratio, which is about 0.03 kg of CO2 per MJ of geothermal heat. Specifically, the studied aquifers affected by the input of the deep CO2 have a mean CO2/heat ratio of 0.033 kg MJ−1, the two diffuse CO2 degassing areas of Torre Alfina and Latera of 0.02 and 0.03 kg MJ−1, respectively, and the geothermal wells of 0.037 kg MJ−1. These similar ratios possibly indicate the existence of a unique original fluid feeding the geothermal systems of central Italy and generating the CO2 and geothermal heat anomalies that characterize the entire Tyrrhenian sector of the region. The similar CO2/heat ratio and the large extent of the CO2 and geothermal heat flux anomalies (thousands of square kilometres) point to a deep source, i.e., the Tyrrhenian mantle wedge that in the region is located at depths of between 20 and 25 km [47,48,49]. The Tyrrhenian mantle, which is rich in fluids produced by the underlying subducted Adria slab, was in fact already recognized as the main source of the CO2 emission of the area [42,50,51,52,53]. The CO2/heat ratios measured in central Italy (~0.03 kg MJ−1) would possibly reflect the composition of the fluids emitted from a mantle anomalously enriched in CO2. Notably, the CO2/heat ratios measured or derived for the geothermal system in central Italy are very high with respect to other geothermal systems of the world. For example, they are one order of magnitude higher than those of the Taupo and Salton Trough geothermal systems, where the computations of [5] indicate a mean CO2/heat ratio of 0.003 kg MJ−1.
4. Discussion and Conclusions
The heat flux of a region is a central parameter in geothermal prospecting and it is normally measured through expensive deep drillings. This classical method allows the estimation of the conductive heat flux but not of the convective-advective heat transported by the fluids. In this study, we reviewed the methods based on the measurement of the CO2 emission for the computation of the convective-advective geothermal heat flow, both at a local (hydrothermal sites, few km2) and regional scale (100–1000 km2).
At the local scale, we first discussed the case of the Campi Flegrei caldera. Here, the CO2-based method clearly shows that the advective heat associated with the hot soils diffusively emitting CO2 at Solfatara di Pozzuoli, is by far the main term of the energetic budget of the entire caldera. Subsequently, we focused on the cases of Latera and Torre Alfina where the depressurization of the geothermal liquid, particularly rich in CO2, causes the separation of a gas phase rich in incondensable gases, which are emitted in the atmosphere by low-temperature manifestations. For these latter cases, the measured CO2 emission, together with the temperature and the CO2 concentration in the geothermal deep fluid, allowed us to compute the thermal energy associated with the original convecting geothermal liquid, which resulted in dozens to hundreds of MW (Table 2). These remarkably high values can be considered as minimum estimates of the energy potentially exploitable from a given hydrothermal system because, assuming that the natural process occurs at a steady state condition, the emitted energy equals the energy entering the system. Therefore, the measurement of the CO2 emission from hydrothermal sites is a valuable tool for geothermal prospection.
At the regional scale, we reported the case of eleven large aquifers (each of hundreds km2) located in the central Apennine. Here, CO2 and heat fluxes have been derived from carbon mass and enthalpy balances of the groundwaters by combining hydrogeological and hydrogeochemical data. Notably, the thermal anomaly of the Tyrrhenian side of Italy extends eastward in the Apennine area, where the conductive heat flow is very low. Furthermore, the ratios between the deeply derived CO2 and the heat entering the studied aquifers (CO2/heat ~0.03 kg MJ−1) are very similar to each other and comparable to those measured in the nearby geothermal fields of Tuscany and Latium (Figure 8). This finding suggests a common CO2-rich fluid source in central Italy, which is ascribed to the Tyrrhenian mantle. The typical CO2/heat ratio of central Italy is in fact one order of magnitude higher than that of other geothermal zones of the Earth (e.g., Taupo and Salton Trough geothermal systems).
This comparison introduces a further aspect linked to the study of the CO2 degassing from geothermal regions, and that is the environmental impact of carbon dioxide and other greenhouse gases (GHG) associated with geothermal power production. In most cases, the emissions of GHG are much lower than those associated with fossil fuel [8,54,55], making geothermal utilization for power production a technology with an extremely low carbon footprint. However, in central Italy and in other regions such as Turkey [56,57,58], geothermal power plants can release significant quantities of GHG into the atmosphere. Since the ratio of CO2 emissions from power plants to natural emissions is a measure of the environmental impact associated with geothermal power production [8,59], it is very important to evaluate the natural CO2 degassing rate before and during the exploitation of the geothermal resource. Besides the potentiality in the exploration phase, the measure of the CO2 emissions can thus find valuable applications in evaluating the environmental impact of geothermal exploitation.
Conceptualization, G.C.; investigation—field work, G.C., C.C., F.F., G.B. and B.L.; writing—original draft preparation, G.C., C.C., G.B. and F.F.; writing—review and editing, G.B., C.C., G.C., F.F., S.C. and L.R. All authors have read and agreed to the published version of the manuscript.
This research and the APC was funded by MIUR, grant number project no. PRIN2017-2017LMNLAW “Connect4Carbon”.
Not applicable.
Not applicable.
The original data presented in this study are available in the
The authors declare no conflict of interest. The funders had no role in the design of the study; in the collection, analyses, or interpretation of data; in the writing of the manuscript, or in the decision to publish the results.
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Figure 1. Sketch of the conceptual model of CO2 and heat transfer in a geothermal system.
Figure 2. (a) CO2 flux; (b) soil temperature maps of the Solfatara di Pozzuoli in December 1998. The two maps were realised using 200 sGs. In the figure are reported the measurement points (dots) where both CO2 flux and soil temperature were measured and the contour of Solfatara DDS (white line). The DDS has been defined as the area where over 50% of the 200 simulated CO2 fluxes are higher than 50 g m−2 d−1, which is assumed as a reasonable maximum value for CO2 production by biological activity in the soil (see [22]). CO2 flux and soil temperature data from [22]). Coordinates refer to ED 50/UTM zone 33 N.
Figure 3. Map of the CO2 diffuse degassing from Latera obtained through 100 sGs simulations (modified after [12]). In the figure are reported the measurement points (dots); the experimental variogram and the variogram model (red curve) used in the sGs (upper left inset); the contour of the Latera DDS (white line) defined as the area where over 50% of the 100 simulated CO2 flux values are higher than the biogenic CO2 flux threshold (50 g m−2 d−1 [12]); the contour of the area used to define the biogenic CO2 background flux (red line); and the location of the main vents and geothermal wells. Coordinates refer to WGS 84/UTM zone 33 N.
Figure 4. Map of the CO2 diffuse degassing from Torre Alfina obtained through 200 sGs simulations. In the figure are reported the measurement points (dots); the experimental variogram and the variogram model (red curve) used in the sGs (upper right inset); and the contour of the Torre Alfina DDS (white line) defined as the area where over 50% of the 200 simulated CO2 flux values are higher than the biogenic CO2 flux threshold (35 g m−2 d−1, see the text). Coordinates refer to WGS 84/UTM zone 33 N.
Figure 5. Probability plot of Log CO2 fluxes. The entire dataset is reported with grey points while the background CO2 fluxes are reported as blue symbols. The black lines represent the partitioned populations while the dashed red curve represents their mixture in the proportion reported in Table 3.
Figure 6. (a) CO2 flux map of central Italy (modified from [17]); (b) Conductive heat flux map of central Italy ([43] modified from [17]). The location of the investigated aquifers and springs are reported together with the mean of the CO2 flux and of the geothermal heat flux computed for each aquifer. Locations of the Latera and the Torre Alfina geothermal systems and of other geothermal wells are also shown. The area of Apennine aquifers is highlighted in both maps (dashed area).
Figure 7. 13δCext vs. Cext diagram (modified from [17]). The diagram shows the presence of two groups of water: the normal groundwater where the carbon derives from the atmospheric and biogenic CO2 (blue points) and waters generated by the addition of deeply derived CO2 to normal groundwaters (magenta point). In the figure are also reported the mean Cext and δ13Cext of the eleven investigated aquifers (open circles, numbers refer to Table 4). The grey band corresponds to the theoretical compositions computed by adding deep CO2 with a δ13C = −1.5‰ to the normal groundwaters (redrawn from [17]).
Figure 8. CO2 mass flow rates (QCO2) plotted against heat flows (QH). In the figure are reported: the results of the carbon mass and enthalpy balance of the 11 aquifers of Central Italy (open circle; numbers as in Table 4, colours as in Figure 7); the values computed for diffuse degassing areas (magenta and orange squares, see Table 2); the values of the geothermal systems of Taupo (New Zealand) and Salton Trough (USA) (from [5]; blue dots); and the QCO2/QH ratios of central Italy geothermal systems derived from deep wells data (from [34]; grey lines; see Figure 6 for the locations of the wells). The best fit of the aquifers, Torre Alfina and Latera diffuse degassing data is also shown (dashed black line).
Thermal energy associated with the CO2 degassing from hot soils from some geothermal/hydrothermal systems and relevant parameters for its calculation.
Volcano (DDS) | Date | DDS Extent a km2 | RH2O/CO2 | QCO2 |
Qcond |
QH,cond |
Reference |
---|---|---|---|---|---|---|---|
Campi Flegrei, Solfatara | 12/1998 | 0.454 b | 2.20 | 17.6 | 38.72 | 100.4 | [ |
Campi Flegrei, Solfatara | 07/2000 | 0.455 b | 2.27 | 17.13 | 38.88 | 100.8 | [ |
Ischia, Donna Rachele | 04/2001 | 0.058 | 147 | 0.11 | 15.48 | 40.1 | [ |
Vesuvio, cone | 04/2000 | 0.331 | 3.66 | 1.75 | 6.40 | 16.6 | [ |
Vulcano, crater | 07/1998 | 0.415 | 4.42 | 1.83 | 8.08 | 21.0 | [ |
Vulcano, PL Beach | 03/2002 | 0.018 | 5.24 | 0.22 | 1.15 | 3.0 | [ |
Pantelleria, Favara Grande | 07/2004 | 0.058 | 17.2 | 0.08 | 1.39 | 3.6 | [ |
Masaya, Comalito | 03/2003 | 0.010 | 1.60 | 0.22 | 0.35 | 0.9 | [ |
Yellowstone, Mud volcanoes | 08/2003 | 0.400 | 3.49 | 3.36 | 11.82 | 30.6 | [ |
Yellowstone (HSB) | - | 0.160 | 15.63 | 0.80 | 12.48 | 32.3 | [ |
Yellowstone (HLGB) | - | 0.040 | 250 | 0.02 | 5.79 | 15.0 | [ |
Yellowstone (CH) | 08/2014 | <0.035 c | 13.44 | 0.97 | 13.1 | 33.9 | [ |
Nisyros-Stefanos | 10/2018 | 0.086 | 36.0 | 0.19 | 7.00 | 18.1 | [ |
Nisyros-Kaminakia | 10/2018 | 0.164 | 6.90 | 0.16 | 1.08 | 2.8 | [ |
Nisyros-Polibote | 10/2018 | 0.031 | 26.0 | 0.07 | 1.68 | 4.4 | [ |
Nisyros-Phlegeton | 10/2018 | 0.053 | 21.2 | 0.04 | 0.85 | 2.2 | [ |
Nisyros Lofos | 10/2018 | 0.196 | 27.3 | 0.23 | 6.31 | 16.4 | [ |
Nisyros-Ramos | 10/2018 | 0.048 | 16.5 | 0.12 | 2.01 | 5.2 | [ |
Nisyros-NEfault | 10/2018 | 0.124 | 6.9 | 0.10 | 0.66 | 1.7 | [ |
Nisyros-SENWline | 10/2018 | 0.123 | 27.3 | 0.05 | 1.30 | 3.4 | [ |
Nisyros-NESWline | 10/2018 | 0.029 | 27.3 | 0.02 | 0.59 | 1.5 | [ |
Nisyros, all DDSs | 10/2018 | 0.825 | 6.9–36 | 1.06 | 23.40 | 60.7 | [ |
Nisyros, all DDSs | 02/2000 | 0.690 | 6.1–36 | 0.79 | 16.44 | 42.6 | [ |
Copahue-Las Máquinas | 03/2014 | <0.321 c | 15.8 | 0.43 | 6.73 | 14.9 | [ |
Copahue-Las Maquinitas I+II | 03/2014 | <0.079 c | 17.3 | 0.19 | 3.30 | 7.3 | [ |
Termas Copahue | 03/2014 | <0.576 c | 16.6 | 1.05 | 17.45 | 38.7 | [ |
Terceira-Furnas do Enxofre | 08/2014 | <0.024 c | 14.9 | 0.03 | 0.44 | 1.1 | [ |
Teide | 07/2016 | <0.560 c | 2.24 | 2.44 | 5.47 | 14.2 | [ |
Peteroa | 01/2020 | <0.08 c | 12.9 | 0.08 | 0.77 | 2.6 | [ |
a For the criteria used to define the DDS extent see the original works; b DDS extent from [
Thermal energy associated with the convection of geothermal fluids. The cases were selected based on the availability of TL and mCO2 of the original geothermal liquid.
Name | QCO2 |
mCO2 |
TL |
HL |
QL |
QH |
---|---|---|---|---|---|---|
Reykjanes 1 | 0.156 | 0.0284 | 290 | 1289 | 125 | 161 |
Nisyros 2 | 1.060 | 0.29 | 340 | 1594 | 83.9 | 134 |
Torre Alfina | 1.064 | 0.33 | 150 | 632.2 | 73.3 | 46 |
Latera | 4.050 | 0.73 | 238 | 1028 | 126.1 | 130 |
1 data from [
Statistical parameters of the individual partitioned populations.
Population | Mean Log CO2 Flux | σ | % | Mean CO2 Flux * |
---|---|---|---|---|
1 | 1.05 | 0.30 | 33 | 14.2 (13.3–15.2) |
2 | 1.62 | 0.29 | 46 | 52.1(49.4–54.8) |
3 | 2.15 | 0.75 | 21 | 626 (441–905) |
* The mean of the CO2 flux was then estimated using a Monte Carlo simulation procedure. Between brackets are reported the 5th and 95th percentile of the mean CO2 flux values returned by the Monte Carlo simulation procedure [
Main hydrogeological parameters of the aquifers (total flow rate Q and surface area of the hydrogeological basin A) and results of the carbon mass and enthalpy balances (Hf, QH, CO2 flux, QCO2). Data are from [
N. | Name | Q |
A |
Hf |
QH |
CO2 Flux |
QCO2 |
---|---|---|---|---|---|---|---|
1 | Umbria NE | 6.73 | 399 | 23 | 9.3 | 1.74 × 109 | 0.69 |
2 | Val Nerina | 1.78 | 105 | 39 | 4.1 | 1.21 × 109 | 0.13 |
3 | Terminillo | 5.79 | 340 | 39 | 13.2 | 1.94 × 109 | 0.66 |
4 | Narnese-Amerina | 15.00 | 740 | 350 | 259.4 | 1.44 × 108 | 10.67 |
5 | Marsica N | 22.35 | 716 | 282 | 202.2 | 8.70 × 109 | 6.23 |
6 | G Sasso N | 17.95 | 793 | 176 | 139.9 | 3.98 × 109 | 3.16 |
7 | G Sasso S | 7.00 | 309 | 39 | 12.2 | 1.92 × 109 | 0.59 |
8 | Prenestini | 9.00 | 499 | 369 | 184.3 | 1.58 × 108 | 7.87 |
9 | Ernici | 18.00 | 618 | 316 | 195.5 | 7.45 × 109 | 4.60 |
10 | Marsica S | 9.80 | 411 | 224 | 91.9 | 5.46 × 109 | 2.24 |
11 | Lepini | 14.80 | 525 | 312 | 163.7 | 8.99 × 109 | 4.72 |
Supplementary Materials
The following are available online at
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Abstract
We review the methods based on the measurement of CO2 emissions for the computation of geothermal heat flow, both at a local (hydrothermal sites, a few km2) and regional scale (hundreds km2). At the local scale, we present and discuss the cases of the Latera caldera and Torre Alfina (Italy) geothermal systems. At Torre Alfina and Latera, the convection process sustains a CO2 emission of ~1 kg s−1 and ~4 kg s−1, and heat flows of 46 MW and 130 MW, respectively. At the regional scale, we discuss the case of the central Apennine (Italy), where CO2 mass and enthalpy balances of regional aquifers highlights a wide and strong thermal anomaly in an area of low conductive heat flow. Notably, the CO2/heat ratios computed for the central Apennines are very similar to those of the nearby geothermal systems of Latium and Tuscany, suggesting a common source of CO2-rich fluids ascribed to the Tyrrhenian mantle.
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1 Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Bologna, Via D. Creti 12, 40128 Bologna, Italy;
2 Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Bologna, Via D. Creti 12, 40128 Bologna, Italy;
3 Institute of Geochemistry and Petrology, ETH Zürich, Clausiusstrasse 25, 8092 Zürich, Switzerland;
4 Dipartimento di Fisica e Geologia, Università di Perugia, Via Pascoli snc, 06123 Perugia, Italy;
5 Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Napoli, Via Diocleziano 328, 80124 Napoli, Italy;