GD1.2

The radiogenic Pb isotope compositions of basalts from the Samoan hotspot suggest various mantle endmembers contribute compositionally distinct material to lavas erupted at different islands [1]. Basalts from the Samoan islands sample contributions from all of the classical mantle endmembers, including extreme EM II and high ³He/⁴He components, as well as dilute contributions from the HIMU, EM I, and DM components. Here, we present multiple sulfur isotope data on sulfide extracted from subaerial and submarine whole rocks associated with several Samoan volcanoes—Malumalu, Malutut, Upolu, Savaii, and Tutuila—that sample the full range of geochemical heterogeneity at Samoa and allow for an assessment of the S-isotope compositions associated with the different mantle components sampled by the Samoan hotspot. We observe variable S concentrations (10-1000 ppm) and δ³⁴S values (-0.29‰ to +4.84‰ ± 0.3, 2σ). The variable S concentrations likely reflect weathering, sulfide segregation and degassing processes. The range in δ³⁴S reflects mixing between the primitive mantle and recycled components, and isotope fractionations associated with degassing. The majority of samples reveal Δ³³S within uncertainty of Δ³³S=0 ‰ ± 0.008, suggesting Δ³³S is relatively well mixed within the Samoan mantle plume. Important exceptions to this observation include: (1) a negative Δ³³S (-0.018‰ ±0.008, 2σ) from a rejuvenated basalt on Upolu island (associated with a diluted EM I component) and (2) a previously documented small (but resolvable) Δ³³S values (up to +0.027±0.016) associated with the Vai Trend (associated with a diluted HIMU component) [2]. The variability we observed in Δ³³S is interpreted to reflect contributions of sulfur of different origins and likely multiple crustal protoliths. Δ³⁶S vs. Δ³³S relationships suggest all recycled S is of post-Archean origin. The heterogeneous S isotope values and distinct isotopic compositions associated with the various compositional trends confirms a prior hypothesis; unique crustal materials are heterogeneously delivered to the Samoan mantle plume and compositionally influence the individual groups of islands.

[1] Jackson et al. (2014), Nature; [2] Dottin et al. (2020), EPSL

How to cite: Dottin, J., Labidi, J., Jackson, M., and Farquhar, J.: Sulfur isotope evidence of geochemical zonation of the Samoan mantle plume, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-6416, https://doi.org/10.5194/egusphere-egu21-6416, 2021.

Basaltic rocks generated by upwelling mantle plumes display a range of trace element and isotope compositions indicative of strong heterogeneity in deep material brought to Earth surface.  Helium isotopes are an unrivalled tracer of the deep mantle in plume-derived basalts.  It is frequently difficult to identify the composition of the deep mantle component as He isotopes rarely correlate with incompatible trace element and radiogenic isotope tracers. It is supposed that this is due to the high He concentration of the deep mantle compared to degassed/enriched mantle reservoirs dominating the He in mixtures, although this is far from widely accepted.  The modern Afar plume is natural laboratory for testing the prevailing paradigm.

The ³He/⁴He of basalt glasses from 26°N to 11°N along the Red Sea spreading axis increases systematically from 7.9 to 15 R_a. Strong along-rift relationships between ³He/⁴He and incompatible trace element ratios are consistent with a binary mixture between moderately enriched shallow asthenospheric mantle in the north and plume mantle evident in basalts from the Gulf of Tadjoura, Djibouti (the Ramad enriched component of Barrat et al. 1990).  The high-³He/⁴He basalts have trace element-isotopic compositions that are similar, but not identical, to the high ³He/⁴He (22 R_a) high Ti (HT2) flood basalts erupted during the initial phase of the Afar plume volcanism (Rogers et al. in press). This suggests that the deep mantle component in the modern Afar plume has a HIMU-like composition. From the hyperbolic ³He/⁴He-K/Th-Rb/La mixing relationships we determine that the upwelling deep mantle has 3-5 times higher He concentration than the asthenosphere mantle beneath the northern Red Sea.

Barrat et al. 1990.  Earth and Planetary Science Letters 101, 233-247.

How to cite: Stuart, F., Balci, U., and Barrat, J.-A.: Defining the composition of the deep mantle and the primordial He inventory of the Afar plume, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-10891, https://doi.org/10.5194/egusphere-egu21-10891, 2021.

Quaternary Intraplate volcanoes are sparsely distributed in Northeast Asia including Northeast China and Korean Peninsula and roles of the stagnant Pacific plate in the volcanoes have been studied. Recent geochemical studies suggest that the hydrated mantle in the mantle transition zone was incorporated in the wet plumes that were generated from the hydrated layer atop the stagnant slab, and the ascending wet plumes experienced partial melting in the shallow asthenosphere. To quantitatively evaluate the incorporation of the mantle in the transition zone into the wet plumes and their partial melting in the asthenosphere, we conducted a series of two-dimensional thermochemical numerical models by including the olivine-wadsleyite phase transition at the 410km discontinuity. The buoyancy is controlled by temperature, bound-water content and mineral phase. Viscosity reduction by the bound-water is added to the temperature-dependent viscosity. Particle tracers are used to track the incorporation of the mantle in the transition zone into the wet plumes. We vary the Clapeyron slope of the phase transition and water distributions in the mantle transition zone and hydrated layer of the stagnant slab to evaluate their effects on the behavior of the wet plumes. Results show that multiple wet plumes generated from atop the stagnant slab incorporate the hydrated mantle in the transition zone. Due to the endothermic phase transition at the 410 km discontinuity, the ascending wet plumes are retarded and laterally migrated beneath the 410 km discontinuity for several million years, and enter the overlying asthenosphere as merged large wet plumes. The ascending merged wet plumes laterally spread beneath the thermal lithosphere and experience partial melting, consistent with the interpretation based on the geochemical studies. The spacing of the merged wet plumes (~440 km) caused by the phase transition at the 410 km discontinuity is consistent with the sparse volcano distribution in Northeast China and Korean Peninsula.

How to cite: Kim, H., Lee, Y., Kim, D., and Lee, C.: Behaviors of Wet Plume Controlled by Olivine-Wadsleyite Phase Transition and Water Distribution, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-1944, https://doi.org/10.5194/egusphere-egu21-1944, 2021.

Approximately 90% of all magmatism on Earth can be explained through plate tectonics; the remainder is associated with intraplate volcanism. In large part, this intraplate volcanism can be attributed to mantle plumes, yet this does not represent all known examples. A number of hypotheses have been proposed to explain non-plume related intraplate volcanism. One geodynamically viable theory through the process of small-scale convection associated with lithospheric instabilities evolving into edge driven convection (EDC) in regions which possess large variations in lithospheric thickness. One such intraplate volcanic example that may be explained by this process is the Cameroon Volcanic Line, which forms a linear chain of non-age progressive volcanoes that straddle the African continental lithosphere and the Atlantic oceanic lithosphere.

In this study we compute numerical models utilising mantle convection modelling software ‘ASPECT’, to investigate the initiation, evolution and potential of melt generation as a result of EDC through geological time, applying these models to the Cameroon Volcanic Line. Our preliminary modelling results suggest that episodic intraplate melting events can indeed be generated through edge-driven convection. But in order to do so, mantle temperatures need to be higher than average to produce sufficient melt from a typical upper mantle source. We therefore investigate the possibility that more enriched mantle lithosphere, destabilised by the assembly and breakup of Pangaea, could flow into the source region of the Cameroon volcanism, allowing the production of similar quantities of melt with less elevated mantle temperatures. We present results on how lithospheric development, evolution and stability, as well as supercontinent cycles can influence intraplate volcanism.

How to cite: Likely, M., van Hunen, J., Kirstein, L., Fitton, G., Kalnins, L., Jenkins, J., and Negredo, A.: Connecting mantle flow below passive margins and intraplate melt generation: an application to the Cameroon Volcanic Line., EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-8489, https://doi.org/10.5194/egusphere-egu21-8489, 2021.

The amount of water stored as OH-defects in nominally anhydrous minerals in the deep mantle is poorly constrained and its direct quantification can only be accessed by the analysis of mantle xenoliths. While the vast majority of xenoliths are peridotites and minor pyroxenites, some very rare xenoliths found in kimberlite pipes display an eclogitic mineral assemblage. We investigated three eclogite xenoliths from the 128 m.y. old Robert Victor kimberlite from South Africa that display an assemblage of garnet and omphacite with two samples showing additional kyanite, suggesting low-pressure gabbroic rock as protolith. Thermobarometry estimations based on Fe-Mg partitioning between garnet and pyroxene gives temperatures of 1100-1250 °C. When projected on the cratonic geotherm (Griffin & O’Reilly 2007) an equilibrium depth of 200-210 km is obtained, confirming that these rocks come from the lithosphere-asthenosphere boundary. Therefore these fragments might be key witnesses to understand the deep cycling of water in the mantle.

This study focuses on the H₂O quantification in the three rock-forming minerals using Fourier transform infrared spectroscopy (FTIR). Omphacite contains 50-250 ppm H₂O, kyanite contains 40-60 ppm H₂O and garnet of only one eclogite contains 40 ppm H₂O. Garnet and omphacite with the highest OH content are enriched in Ca.

The use of advanced mapping and profiling techniques enabled the investigation of the spatial repartition of the OH component in these minerals. High-resolution mapping (5.6 µm) of kyanite reveals diffusive gain of OH at the rim of the crystal that is interpreted as hydration during interaction with the kimberlitic melt. The OH plateau in the core of kyanite must therefore have been acquired previously, suggesting that this is residual OH that has been transported by subduction to the lithosphere-asthenosphere boundary by a once hydrated gabbroic protolith. Our results have implications for the retention of hydrogen over long timescale at the lithosphere-asthenosphere boundary and suggest that the deep cycling of water has been running since Archean times.

Griffin, W. L., & O'Reilly, S. Y. (2007). Cratonic lithospheric mantle: is anything subducted?. Episodes, 30(1), 43-53.

How to cite: Reynes, J. and Hermann, J.: Eclogite xenoliths document water cycling at the lithosphere-asthenosphere boundary, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-5932, https://doi.org/10.5194/egusphere-egu21-5932, 2021.

Estimating the fluxes and speciation of volatiles during the existence of a global magma ocean is fundamental for understanding the cooling history of the early Earth and for quantifying the volatile budget of the present day. Using first-principles molecular dynamics, we predict the vaporization rate of carbon and hydrogen at the interface between the magma ocean and the hot dense atmosphere, just after the Moon-forming impact. The concentration of carbon and the oxidation state of the melts affect the speciation of the vaporized carbon molecules (e.g., the ratio of carbon dioxide to carbon monoxide), but do not appear to affect the overall volatility of carbon. We find that carbon is rapidly devolatilized even under pressure, while hydrogen remains mostly dissolved in the melt during the devolatilization process of carbon. Thus, in the early stages of the global magma ocean, significantly more carbon than hydrogen would have been released into the atmosphere, and it is only after the atmospheric pressure decreased, that much of the hydrogen devolatilized from the melt. At temperatures of 5000 K (and above), we predict that bubbles in the magma ocean contained a significant fraction of silicate vapor, increasing with decreasing depths with the growth of the bubbles, affecting the transport and rheological properties of the magma ocean. As the temperature cooled, the silicate species condensed back into the magma ocean, leaving highly volatile atmophile species, such as CO₂ and H₂O, as the dominant species in the atmosphere. Due to the greenhouse nature of CO₂, its concentration in the atmosphere would have had a considerable effect on the cooling rate of the early Earth.

How to cite: Solomatova, N. and Caracas, R.: The vaporization behavior of carbon and hydrogen from the early global magma ocean, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-10847, https://doi.org/10.5194/egusphere-egu21-10847, 2021.

We evaluate the equilibrium concentration of a thermally convecting suspension that is cooled from above and in which
solid crystals are self-consistently generated in the thermal boundary layer near the top. In a previous study (Patočka et
al., 2020), we investigated the settling rate of solid particles suspended in a highly vigorous (Ra = 10⁸ , 10¹⁰, and 10¹² ),
finite Prandtl number (Pr = 10, 50) convection. In this follow-up study we additionally employ the model of crystal
generation and growth of Jarvis and Woods (1994), instead of using particles with a predefined size and density that are
uniformly injected into the carrier fluid.

We perform a series of numerical experiments of particle-laden thermal convection in 2D and 3D Cartesian geometry
using the freely available code CH4 (Calzavarini, 2019). Starting from a purely liquid phase, the solid fraction gradually
grows until an equilibrium is reached in which the generation of the solid phase balances the loss of crystals due to
sedimentation at the bottom of the fluid. For a range of predefined density contrasts of the solid phase with respect to
the density of the fluid (ρ_p /ρ_f = [0, 2]), we measure the time it takes to reach such equilibrium. Both this time and
the equilibrium concentration depend on the average settling rate of the particles and are thus non-trival to compute for
particle types that interact with the large-scale circulation of the fluid (see Patočka et al., 2020).

We apply our results to the cooling of a large volume of magma, spanning from a large magma chamber up to a
global magma ocean. Preliminary results indicate that, as long as particle re-entrainment is not a dominant process, the
separation of crystals from the fluid is an efficient process. Fractional crystallization is thus expected and the suspended
solid fraction is typically small, prohibiting phenomena in which the feedback of crystals on the fluid begins to govern the
physics of the system (e.g. Sparks et al, 1993).

References
Patočka V., Calzavarini E., and Tosi N.(2020). Settling of inertial particles in turbulent Rayleigh-Bénard convection.
Physical Review Fluids, 26(4) 883-889.

Jarvis, R. A. and Woods, A. W.(1994). The nucleation, growth and settling of crystals from a turbulently convecting
fluid. J. Fluid. Mech, 273 83-107.

Sparks, R., Huppert, H., Koyaguchi, T. et al (1993). Origin of modal and rhythmic igneous layering by sedimentation in
a convecting magma chamber. Nature, 361, 246-249.

Calzavarini, E (2019). Eulerian–Lagrangian fluid dynamics platform: The ch4-project. Software Impacts, 1, 100002.

How to cite: Patocka, V., Tosi, N., and Calzavarini, E.: A numerical study of the nucleation, growth and settling of crystals from a turbulent convecting fluid, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-14371, https://doi.org/10.5194/egusphere-egu21-14371, 2021.

The existence of a high pressure ice layer between the silicate core and the liquid ocean in large icy moons and ocean worlds is usually seen as a barrier to habitability, preventing the compounds needed for life to flow into the ocean. More recently, three studies from Choblet et al [1] and Kalousová et al [2, 3] challenged that hypothesis and showed that, in certain conditions, exchanges were possible between the core and the ocean, allowing transport of salts toward the ocean. Here, we consider an effect not taken into account in these previous studies: the possibility of mass exchange between the ice and ocean layers by phase change. Convective stresses in the solid create a topography of the interface which can be erased by melting and freezing if flow on the liquid side is efficient. This effect is included in a convection model as a phase change boundary condition, allowing a non-zero vertical velocity at the surface of the HP ice layer, which has a significant impact on the flow dynamics and enables exchanges with the ocean by fusion and crystallization of the ice at the top interface, even without partial melting in the bulk of the ice layer. These exchanges are directly linked to the melting capacity of the ice at the interface between the HP ice layer and the core, depending on the Rayleigh number and the efficiency of convection. Then, considering this new condition at the interface between the HP ice layer and the liquid ocean, we propose a scaling of the bottom temperature and the vertical velocity. Applied to a specific celestial body, as Ganymede or Titan, it would be the first step to conclude about its habitability.

References:

[1] G. Choblet, G. Tobie, C. Sotin, K. Kalousová, O. Grasset (2017). Heat transport in the high-pressure ice mantle of large icy moons. Icarus, 285, 252-262

[2] K. Kalousová, C. Sotin, G. Choblet, G. Tobie, O. Grasset (2018). Two-phase convection in Ganymede’s high-pressure ice layer — Implications for its geological evolution. Icarus, 299, 133-147

[3] K.Kalousová, C. Sotin (2018). Melting in High-Pressure Ice Layers of Large Ocean Worlds—Implications for Volatiles Transport. Geophys. Res. Lett., 45, 8096-8103.

How to cite: Lebec, L., Labrosse, S., Morison, A., and Tackley, P.: Scaling of convection in high-Pressure ice layers of large icy moons and implications for habitability, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-12691, https://doi.org/10.5194/egusphere-egu21-12691, 2021.

Melt transport beneath the lithosphere is elusive. With a distinct viscosity and density from the surrounding mantle, magmatic melt moves on a different time scale as the surrounding mantle. To resolve the temporal scale necessary to accurately capture melt transport in the mantle, the model simulations become numerically expensive quickly. Recent computational advances make possible two-phase numerical explorations to understand magma transport in the mantle. We review results from a suite of two-phase models applied to the mid-ocean ridges, where we varied half-spreading rate and intrinsic mantle permeability using new openly available models, with the goal of understanding melt focusing beneath mid-ocean ridges and its relevance to the lithosphere-asthenosphere boundary (LAB). Here, we highlight the importance of viscosities for the melt focusing mechanisms. In addition, magmatic porosity waves that are a natural consequence of these two-phase flow formulations. We show that these waves could explain long-period temporal variations in the seafloor bathymetry at the Southeast Indian Ridge.

How to cite: Sim, S., Spiegelman, M., Stegman, D., and Wilson, C.: Magma transport beneath mid-ocean ridges, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-5881, https://doi.org/10.5194/egusphere-egu21-5881, 2021.

The process of fractional crystallization within a magma body has an influence on the solubility and thus on the associated release of volatiles. Nevertheless, this mechanism is widely neglected in the literature. Due to cooling of an intrusion, nominally anhydrous minerals precipitate from the melt. These minerals mainly incorporate elements that are compatible with their crystal lattice. Since volatiles such as H₂O and CO₂ behave like incompatible elements, they accumulate in the remaining melt. At a certain point, the melt is saturated and the exsolution of the volatiles initiates. The solubility is determined by several parameters like the lithostatic and the partial pressure, the temperature and the melt composition. 
In this study, we investigate the effect of these parameters as well as the impact of fractional crystallization on the solubility and the related volatile release. We focus on the exsolution of H₂O and CO₂ from basaltic magma bodies within the lithosphere. To determine the fate of the accumulating volatiles, we compare the density of the developing liquid phase (volatiles and residual melt) with the density of the host rock. If the host rock has a higher density, the liquid phase will ascent either directly to the surface or to shallower levels of the crust. Furthermore, we take into account the possibility that hydrous minerals (e.g., amphibole) are precipitated during fractional crystallization or due to a reaction with the surrounding rock. 

How to cite: Vulpius, S. and Noack, L.: Effects on the solubility and the volatile release from magmatic intrusions, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-14267, https://doi.org/10.5194/egusphere-egu21-14267, 2021.

The water exchange between the Earth’s surface and the deep interior is a prime process for the geochemical evolution of our planet and its dynamics. The degassing of water from the mantle takes place through volcanism whereas mantle regassing occurs through the subduction of H₂O chemically bound to hydrous minerals. The (im)balance between degassing and regassing controls the budget of surficial liquid water over geological timescales, i.e, the long-term global sea level. Continental freeboard constraints show that the mean-sea level has remained relatively constant in the last 540 Ma (changes less than about 100 m), thus suggesting a limited imbalance. However, thermopetrological models of water fluxes at present-day subduction zones predict that regassing exceeds degassing by about 50% which, if extrapolated to the past, would have induced a drop inconsistent with the estimations of the long-term sea-level. We have made the case that these inconsistencies arise from thermodynamic predictions for the hydrated lithospheric mantle mineralogy that are poorly constrained at a high pressure (P) and temperature (T). In our study, we thus have revised the global-water flux calculations in subduction zones using petrological constraints on post-antigorite assemblages from recent laboratory experimental data on natural peridotites under high-PT conditions [e.g. Maurice et al, 2018].

We model the thermal state of all present-day mature subduction zones along with petrological modeling using the thermodynamic code Perple_X and the most updated version of the thermodynamic database of Holland and Powell [2011]. For the modeling of peridotite, we build a hybrid phase diagram that combines thermodynamic calculations at moderate PT and experimental data at high PT (> 6 GPa- 600˚C). Our updated thermopetrological model reveals that the hydrated mantle efficiently dehydrates upon the breakdown of the hydrous aluminous-phase E before reaching 250 km in all but the coldest subduction zones. Further subducting slab dehydration is expected between 300-350 km depths, regardless of its thermal state, as a result of lawsonite breakdown in the gabbroic crust. Overall, we predict that present-day global water retention in subducting plates beyond a depth of 350 km barely exceeds the estimations of mantle degassing for average thicknesses of subducting serpentinized mantle subducting at the trenches of up to 6 km. Finally, our models quantitatively support the steady-state sea level scenario over geological times.

Maurice, J., Bolfan-Casanova, N., Padrón-Navarta, J. A., Manthilake, G., Hammouda, T., Hénot, J. M., & Andrault, D. (2018). The stability of hydrous phases beyond antigorite breakdown for a magnetite-bearing natural serpentinite between 6.5 and 11 GPa. Contributions to Mineralogy and Petrology, 173(10), 86.

Holland, T. J. B., & Powell, R. (2011). An improved and extended internally consistent thermodynamic dataset for phases of petrological interest, involving a new equation of state for solids. Journal of Metamorphic Geology, 29(3), 333-383.

How to cite: Cerpa, N., Arcay, D., and Padrón-Navarta, J. A.: Limited subduction of water to mid-upper mantle depths predicted by the phase assemblages in hydrated peridotites with natural chemical composition at high-PT conditions, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-4015, https://doi.org/10.5194/egusphere-egu21-4015, 2021.

When partial melt occurs in the mantle, redistribution of trace elements between the solid mantle material and partial melt takes place. Partition coefficients play an important role when determining the amount of trace elements that get redistributed into the melt. Due to a lower density compared to surrounding solid rock, partial melt that was generated in the upper mantle will rise towards the surface, leaving the upper mantle depleted in incompatible trace elements and an enriched crust. Studies investigating trace element partitioning in the mantle typically rely on constant partition coefficients throughout the mantle, even though it is known that partition coefficients depend on pressure, temperature, and composition. Between the pressures of 0-15 GPa, partition coefficients vary by two orders of magnitude along both, solidus and liquidus. Since partition coefficients exhibit a parabolic relationship in an Onuma diagram, a similar variation is expected for all trace element partition coefficients that can be derived from the sodium partition coefficients.

In this study, we developed a thermodynamic model for sodium in clinopyroxene after Blundy et al. (1995). With the thermodynamic model results, we were able to deduce a P-T dependent equation for sodium partitioning that is applicable up to 12 GPa between the peridotite solidus and liquidus. Because sodium is an almost strain-free element in jadeite, it can be used as a reference to model partition coefficients for other elements, including heat producing elements like K, Th, and U. This gives us the opportunity to insert P-T dependent partition coefficient calculations of any trace element into mantle melting models, which will have a big impact on the accuracy of elemental redistribution calculations and therefore, if the partitioning of the heat producing elements is taken into account, also the evolution of the mantle and crust.

Blundy, J. et al. (1995): Sodium partitioning between clinopyroxene and silicate melts, J. Geophys. Res., 100, 15501-15515.

Schmidt, J.M. and Noack, L. (2021): Parameterizing a model of clinopyroxene/melt partition coefficients for sodium to higher upper mantle pressures (to be submitted)

How to cite: Schmidt, J. M. and Noack, L.: Modelling clinopyroxene/melt partition coefficients for higher upper mantle pressures , EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-12478, https://doi.org/10.5194/egusphere-egu21-12478, 2021.

CO₂ emissions from geological sources have been recognized as an important input to the global carbon cycle. In regions without active volcanism, mines provide an extraordinary opportunity to observe dynamics of geogenic degassing close to its source.

High temporal resolution of stable carbon isotopes allows to outline temporal and interdependent dynamics of geogenic CO₂ contributions. We present data from an active underground salt mine in central Germany that were collected on site with a field-deployed laser isotope spectrometer.

Throughout the 34-day measurement period, total CO₂ concentrations varied between 805 ppmV (5^th percentile) and 1370 ppmV (95^th percentile). With a 400 ppm atmospheric background concentration, an isotope mixing model enabled the separation of geogenic (16–27 %) from highly dynamic contributions from anthropogenic CO₂-sources (21–54 %). The geogenic fraction was inversely correlated to established CO₂ concentrations that were driven by anthropogenic CO₂ emissions within the mine. This indicates gradient-driven diffusion along microcracks.

Read more about this work in our open access publication in Scientific Reports at: http://rdcu.be/cblTz

How to cite: Frank, A. H., van Geldern, R., Myrttinen, A., Zimmer, M., Barth, J. A. C., and Strauch, B.: Geological CO2 contributions quantified by high-temporal resolution carbon stable isotope monitoring in a salt mine, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-13234, https://doi.org/10.5194/egusphere-egu21-13234, 2021.