I12-JEEP: Joint Engineering, Environmental and Processing
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Barbara
Bonechi
,
Fabio
Arzilli
,
Margherita
Polacci
,
Alessandro
Fabbrizio
,
Giuseppe
La Spina
,
Eleni
Michailidou
,
Elisa
Biagioli
,
Richard A.
Brooker
,
Jean-Louis
Hazemann
,
Robert C.
Atwood
,
Danilo
Di Genova
,
Sumith
Abeykoon
,
David A.
Neave
,
Renat R.
Almeev
,
Mike
Burton
Diamond Proposal Number(s):
[31529]
Open Access
Abstract: Crystallisation kinetics play a fundamental role in controlling conduit dynamics and eruptive style. The degree of superheating is critical in controlling crystallisation kinetics; however, its effect is still debated and has an unclear impact on eruption dynamics. Here, we investigate how superheating influences clinopyroxene nucleation in tephritic magmas from the 2021 Tajogaite eruption (La Palma, Spain) through both in situ and ex situ view experiments. Our findings show that superheating delays nucleation by dissolving pre-existing nuclei, thereby inhibiting crystallisation upon return to subliquidus conditions. Using a numerical model, we investigate how different nucleation delays resulting from different degrees of superheating affect magma ascent dynamics. Depending on the initial thermodynamic conditions and on the pre-eruptive history of magma, an increased nucleation delay can significantly reduce crystal content during ascent, lowering magma viscosity and affecting eruptive style. These findings highlight the critical role of pre-eruptive thermal histories in controlling eruptive style, and provide constraints for refining experimental protocols and numerical models, with direct implications for improving volcanic hazard assessment and eruption forecasting.
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Jun 2026
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Jeanne
Caumartin
,
Karim
Benzerara
,
Robin
Havas
,
Christophe
Thomazo
,
Neha
Mehta
,
Vladimir
Betancourt
,
Luis Carlos
Colocho Hurtarte
,
Marine
Cotte
,
Imène
Estève
,
Didier
Jézéquel
,
Electra
Kotopoulou
,
Pierre
Sans-Jofre
,
Rosaluz
Tavera
,
Purificaciόn
Lόpez-Garcίa
Abstract: Recently, carbonate microbialites were discovered in Lake Alchichica, Mexico, forming below the oxycline (down to 40 m depth), under seasonally anoxic conditions, while conspicuous microbialites also grow at shallower depths under continuously oxic conditions. Here, we investigated sulfur (S) speciation in these microbialites at submicrometer resolution using synchrotron-based X-ray absorption near-edge structure (XANES) spectroscopy, complemented by laboratory X-ray fluorescence (XRF) mapping, scanning electron microscopy (SEM) and energy dispersive X-ray spectrometry (EDXS). Our findings revealed that S is pervasive in both shallow and deep microbialites. However, S speciation varied with depth: while carbonate-associated sulfates (CAS) and organic S compounds were present at all depths, more reduced S species were enriched in the aragonitic layers of deep microbialites, particularly in association with remnants of biogenic structures. These variations in S speciation suggest that deep Alchichica microbialites continue to accrete during seasonal anoxia. Moreover, our results indicate that S speciation in modern microbialites is influenced by ambient redox conditions. By documenting the processes affecting S speciation in a modern microbialitic system, this study provides a framework for future investigations into ancient microbialites that formed under sulfidic conditions.
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May 2026
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I18-Microfocus Spectroscopy
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Diamond Proposal Number(s):
[36021]
Open Access
Abstract: Sulfur isotopes in mantle plume-derived magmas show heterogeneities attributed to recycling of material from the Earth's surface. The sedimentary sulfur isotope record exhibits dramatic temporal variations over Earth history, raising the question of whether its secular evolution is echoed in mantle plume-derived magmas. We present new secondary ion mass spectrometry and X-ray absorption near-edge structure measurements of δ34S and Fe3+/ΣFe in naturally glassy melt inclusions from the 2.7 Ga Belingwe komatiites. We find that δ34S of Belingwe melt inclusions is relatively homogeneous (+3.2 ± 0.9) and elevated relative to the depleted upper mantle. We evaluate explanations for elevated magmatic δ34S including degassing, sulfide fractionation, assimilation, subduction-like processes, and mantle recycling. We find no evidence for significant sulfur isotope fractionation via degassing or sulfide saturation. The elevated δ34S in the Belingwe komatiites could reflect late-stage assimilation of sediments or seawater. Alternatively, Belingwe komatiites may have formed in a subduction-like setting, as modern arcs display a bias toward positive δ34S. However, we find these scenarios less favorable. Instead, our preferred interpretation is that elevated δ34S was supplied to the komatiite mantle source via recycled lithologies such as sediments, altered oceanic crust, and/or pyroxenite. Combined with δ34S data from mantle plume-derived magmas spanning a wide age range, our results resemble the secular evolution of δ34S in surface reservoirs. We suggest that the δ34S record in mantle plume-derived magmas may echo secular evolution in the surficial sulfur reservoir with a delay of several hundred million years, linking Earth's surface and interior sulfur cycles.
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May 2026
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I13-2-Diamond Manchester Imaging
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Diamond Proposal Number(s):
[30455]
Abstract: Tracking carbon dioxide (CO2) flow and its consequent effects in subsurface rocks has received considerable attention in geological carbon sequestration. However, existing research on CO2 flow in reservoir-caprock systems with well-developed pores and microfractures is limited, and our understanding of its mechanisms remains incomplete. Here, we present the first observation of gaseous and supercritical CO2 (scCO2) behavior within a reservoir-caprock couplet using high-resolution synchrotron X-ray imaging. We found that high-speed gaseous CO2 flow reshaped part of the fracture framework but did not induce additional secondary fractures. High-speed scCO2 caused significant fracturing, connecting natural fractures in shale with newly developed secondary branches and creating larger pore spaces in sandstone. Consequently, the simulated permeability increased by approximately 2.6-fold in shale and 8.6-fold in sandstone. The concentrated strains around the main fracture in shale and the web-like strain patterns along granular mineral boundaries in sandstone highlight the distinct modes of scCO2 action during its passage through the reservoir-caprock system. This work provides new insights into the complex reservoir-caprock system and offers practical guidelines for fluid injection and production activities.
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Apr 2026
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I12-JEEP: Joint Engineering, Environmental and Processing
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Diamond Proposal Number(s):
[22517]
Open Access
Abstract: Seismic wave speed monitoring is important for the non-destructive evaluation of material properties in response to external forcing. Coda wave interferometry (CWI) uses travel time perturbations in multiply-scattered seismic wave trains – the seismic coda – to detect subtle perturbations in bulk wave speed. However, conventional body-wave CWI cannot separate the coupled contributions of P and S waves, which are sensitive to different material properties. We introduce energy partitioning inversion which decouples these modes by combining a scattering model with CWI measurements within non-equipartitioned coda windows. We applied this methodology to repeated ultrasonic pulse surveys during two laboratory loading experiments on Clashach sandstone: a dynamic experiment (constant strain rate until brittle failure) and a quasi-static experiment (modulating stress to maintain constant acoustic emission rate and slow down the failure process). Relative travel time perturbations and their full covariance between all pairs of surveys were measured across multiple coda windows and inverted for a single perturbation profile using a least-squares method to minimise the variance of the profile. Using an isotropic point scatterer model to predict mode partitioning with respect to the coda lapse time, we invert travel time perturbations for the scattering mean free path travel time and relative P and S wave speed perturbations via Markov-chain Monte Carlo inversion to quantify uncertainty. P and S wave speed perturbations were resolved with 95 % credible intervals of 0.025 % and 0.008 %, respectively. During the quasi-static experiment the temporal resolution was sufficient to capture a quasi-linear decrease in P and S wave speeds by ~ 50 % and ~ 14%, respectively, from peak to failure. The peak P and S wave speed perturbations were ~ 33% lower and ~ 75% higher, respectively, compared to those found in the dynamic experiment. These results demonstrate that CWI and energy partitioning inversion enables the robust, uncertainty-quantified evaluation of separate relative bulk P and S wave speed perturbations in strongly-scattering media.
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Apr 2026
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I18-Microfocus Spectroscopy
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Y.
Moussallam
,
G.
Georgeais
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S.
Ding
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J.-L.
Devidal
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B.
Scaillet
,
C.
Oppenheimer
,
A.
Burgisser
,
E. F.
Rose-Koga
,
K. T.
Kogan
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N.
Peters
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A.
Peccia
,
P.
Samaniego
,
N.
Métrich
,
P.
Robidoux
,
M.
Kawaguchi
Diamond Proposal Number(s):
[36021]
Open Access
Abstract: Arc magmas have long been considered significantly more oxidised than their ocean island and mid-ocean ridge counterparts, a characteristic widely attributed to infusion of the mantle wedge by fluids from subducted lithologies. However, here we show that at comparable degree of differentiation and sulfur content, arc magmas have comparable oxidation state to ocean island magmas. Our study is based on measurements of Fe3+/∑Fe along with major and volatile elements in olivine and plagioclase hosted melt inclusions and matrix glasses from eleven volcanic systems located in arc settings worldwide. Accounting for fractional crystallisation (to MgO = 6 wt. %) we find that all systems lie on a reducing trend accompanying sulfur degassing, from QFM +0.9 (±0.2, 1σ) when S > 2000 ppm to QFM −0.2 (±0.6, 1σ) when S < 100 ppm (where QFM stands for the Quartz-Fayalite-Magnetite buffer). These findings reconcile the observed discrepancy between the oxidation states of xenoliths in arc magmas and gas emissions from arc volcanoes. We further show that fractional crystallisation influences the redox evolution of arc magmas to a comparable extent as, and sometimes counteracting, sulfur degassing.
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Apr 2026
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I12-JEEP: Joint Engineering, Environmental and Processing
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Michael
Chandler
,
Xun
Li
,
Alexis
Cartwright-Taylor
,
Ian
Butler
,
Damien
Freitas
,
Birhanmeskel
Woldemichael
,
Alexander
Liptak
,
Robert
Atwood
,
Ian
Main
,
Maria-Daphne
Mangriotis
,
Andrew
Curtis
,
Florian
Fusseis
,
Mark
Chapman
Open Access
Abstract: The partition of strain between seismic and aseismic processes, notably brittle creep, is highly variable in both tectonic and induced seismicity settings. The two processes have a complicated relationship, with brittle creep generally being associated with more distributed deformation and dynamic rupture with strain localisation. While the overall macroscopic strain behaviour during this process is reasonably well established, the mechanisms by which localised damage regions develop, interact, and ultimately coalesce to form localised fault zones remain under active investigation. The recent development of in-situ X-ray tomography during rock deformation experiments enables direct, time‑resolved, three‑dimensional interrogation of these processes at sub-grain scale.
Here, brittle creep was induced in a water-saturated sample of heavily cemented Clashach sandstone under triaxial conditions (σ3 = 20 MPa, Ppore = 5 MPa) using the University of Edinburgh’s “Stór Mjölnir” deformation rig (Cartwright-Taylor et al., 2022). This triaxial rig is equipped with piezoelectric transducers to monitor acoustic emissions and seismic velocity change, and was mounted on synchrotron beamline I12 at Diamond Light Source, UK. In-situ X-ray microtomography was conducted throughout the creep process with a voxel edge length of 7.91 μm, comfortably smaller than the average grain diameter of ≅ 300 μm. These coupled datasets allow for simultaneous monitoring of changes in seismic velocity, acoustic emissions, macroscopic and grain-scale strains as the sample creeps (Cartwright-Taylor et al., 2022, Mangriotis et al., 2025).
Main (2000) proposed a damage mechanics model that explains the three stages of decelerating, steady-state and accelerating creep through a combination of two mechanisms: initial deceleration due to local hardening processes, with later acceleration driven by interactions between cracks. These three stages were observed in the macroscopic axial strain data and seismic velocity variation, which fit the model closely. Digital Volume Correlation was used to observe the strains within the sample throughout creep. During primary creep, these strains are predominantly dilation, with a steep positive correlation between volumetric and shear strains. These dilational strains are strongly localised around where the eventual failure-plane nucleates. As the sample transitions into secondary creep at εz ≅ 1.85%, vp reduces to around 85% of its initial value. More mixed compaction and dilation strains are observed, again localised around the eventual failure plane. A sharp burst of more widely distributed shear strain is observed at εz ≅ 1.9% as the strain transitions into tertiary creep, and vp falls to around 80% of its initial value. These strains correspond approximately to the onset of acoustic emissions. The DVC strains then revert to a largely dilational mode prior to dynamic failure. This localised combination of dilation and shear strain development, and evolution of their relative importance over time, independently validates the combination of localised hardening and crack interaction proposed by Main (2000).
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Mar 2026
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I12-JEEP: Joint Engineering, Environmental and Processing
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Xun
Li
,
Michael
Chandler
,
Alexis
Cartwright-Taylor
,
Damien
Freitas
,
Maria-Daphne
Mangriotis
,
Birhanmeskel
Woldemichael
,
Alexander
Liptak
,
Robert
Atwood
,
Mark
Chapman
,
Florian
Fusseis
,
Ian
Butler
,
Andrew
Curtis
,
Ian
Main
Open Access
Abstract: Seismic velocity at the near surface drops during ground motions due to remote earthquakes and can recover afterwards over decades. In the laboratory, seismic velocity of rock samples decreases after dynamic deformations (e.g., shaking) and gradually recovers towards the original level. These observations at different scales are referred to as slow dynamics in granular materials (e.g., rocks and concrete), but the underlying mechanisms remain debated.
We explore the physics behind seismic velocity transients during and after dynamic deformations using Stór Mjölnir — a triaxial pressure loading apparatus featuring two piezoelectric transducers mounted in the top and bottom pistons and an X-ray transparent aluminium pressure vessel that houses a cylindrical core sample of Clashach sandstone (10 mm in diameter and 25 mm in length).
We present the mechanical, acoustic, and X-ray microtomography results of two triaxial loading experiments, conducted at room temperature with a confining pressure of 20 MPa and a pore fluid pressure of 5 MPa. Both experiments involve first increasing the ram pressure at a constant strain rate of 1x10-5 s-1 until the onset of sample yielding, indicated by a deviation from the linear stress–strain curve. In the first experiment, we further hold the ram pressure constant and then abruptly reduce the pressure by 30 MPa before rapidly returning the pressure to the previous hold level; this perturbation is repeated for 32 cycles until catastrophic failure of the rock sample. In the second experiment, we apply the same cyclic loading protocol after sample yielding, except for the abrupt pressure drop of 150 MPa; the sample survives only two loading cycles before catastrophic failure. These cyclic loading protocols are designed to induce transient seismic velocity responses, which are monitored by active acoustic surveys acquired every 8 s and in-situ 3D X-ray tomography synthesised every 6 min at the beamline I12-JEEP, Diamond Light Source (Oxfordshire, UK).
We observe nearly linear relationships between the small stress perturbations (30 MPa) and corresponding seismic velocity changes, indicating minimal slow dynamics in the rock sample. In contrast, large stress perturbations (150 MPa) cause nonlinear velocity changes, although the recovery time scale is limited by the small size of the experimental sample. The time-resolved 3D X-ray volumes from both experiments show no resolvable transient structural changes in the rock samples, despite ongoing microfracture accumulation and pore enlargement driven by background creep until catastrophic failure. These results demonstrate that active seismic waves can detect nonlinear velocity transients in triaxial loading experiments, which likely originate from microstructures (e.g., grain contacts) below the X-ray imaging resolution (voxel edge length ~ 7.9 µm). These experiments also motivate further study on seismic velocity transients using our next-generation experimental apparatus that accommodates larger samples (18 mm in diameter and 45 mm in length) and six acoustic transducers. Ultimately, we aim to assess seismic velocity transients as a proxy for rocks’ susceptibility to small stress perturbations, which could provide a method to map the proximity to catastrophic failure and hence help mitigate induced seismicity associated with hydraulic fracturing.
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Mar 2026
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I12-JEEP: Joint Engineering, Environmental and Processing
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Diamond Proposal Number(s):
[22517]
Open Access
Abstract: Fatigue and damage accumulation in granitoids are classical, but poorly characterised, rock mechanics problems. We explore these phenomena by examining curling stone impacts. Curling stones are slid on ice and made to collide along a circumferential striking band. This well constrained scenario involves uniaxial compression of convex surfaces (i.e., Hertzian contacts). Conservatively, each stone experiences about 2900 impacts per season, over a lifespan of 10–15 years before refurbishment, providing a unique opportunity to study fatigue and damage accumulation under dynamic cyclic loading.
Here, we first determine the stress magnitudes of head-on curling stone impacts using on-ice experiments involving a high-speed camera and pressure-sensitive films. We then characterise the damage observed in aged stones using photogrammetry, microtomography, and microscopy. For high-velocity impacts (), a curling stone is locally and momentarily stressed to 300–680 MPa, exceeding its quasi-static unconfined compressive strength and exceeding the threshold for fatigue damage for repeated dynamic loadings. Curling stone impacts are dynamic in nature, as evidenced by (1) high strain rates () that lie below those of co-seismic rock pulverization; (2) ejection of rock powder during collisions and the presence of potential spalling microcracks; and (3) presence of striations on crescent-shaped fractures, which resemble mirror-mist-hackle patterns indicative of dynamic microcrack propagation. In the striking band, damage is confined to macroscopic Hertzian cone fractures and their immediate collet zones, and does not appear to extend beyond about 3–5 cm into the stones (radially). The circumferential density of cone fractures is limited to about 2–2.5 cm−1.
We propose that (1) early, high-velocity impacts initiate cone fractures up to a specific spatial density, and (2) with subsequent collisions in the same regions of the striking band, cone fractures progressively propagate and coarsen. This concentrates and channels the accumulated damage, shielding the rest of the stone from reaching critical stress levels for damage. Our findings are significant for applications where rocks are exposed to repetitive, high-stress impacts and suggest that narrow damage zones can dissipate high-impact stresses.
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Mar 2026
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I13-1-Coherence
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Emily C.
Bamber
,
Fabio
Arzilli
,
Silvia
Cipiccia
,
Darren J.
Batey
,
Giuseppe
La Spina
,
Margherita
Polacci
,
Ali
Gholinia
,
Heath
Bagshaw
,
Danilo
Di Genova
,
Richard
Brooker
,
Daniele
Giordano
,
Pedro
Valdivia
,
Mike
Burton
Open Access
Abstract: Nanoscale crystals, or ‘nanolites’, are becoming increasingly recognised in both experimental products and natural samples of volcanic eruptions, across a range of magma compositions and explosivity. Nanolites can increase magma viscosity and influence eruptive style, due to the rheological impact of the nanoparticle suspension, by inducing chemical and structural changes in the residual melt and by facilitating heterogeneous bubble nucleation. Due to their large surface area, nanolites are also prone to aggregation. However, their morphology, spatial distribution and interaction in 3D has not yet been investigated.
Here we present a 3D, nanometre-scale visualisation and quantification of nanolites within scoriae of highly explosive basaltic volcanic eruptions, obtained using X-ray ptychography, a nanoscale microscopy technique. We find that titanomagnetite nanolites aggregate, forming elongate, irregular structures in 3D. Compositional heterogeneities are also observed within the matrix glass, as extraction of Fe and Ti from the melt during nanolite crystallisation forms differentiated, Si-rich boundary layers surrounding nanolites with higher viscosity. We support our 3D nanoscale observations with images acquired using SEM and STEM, utilising multi-scale imaging methods to visualise nanolite crystallisation in basaltic magmas. We find that syn-eruptive nanolite crystallisation can increase magma viscosity through their aggregation and impact on the composition of the residual melt, increasing the potential of magma fragmentation during ascent. Our results provide insight into the nanoscale structure of volcanic products and also the driving mechanisms of highly explosive basaltic volcanic eruptions.
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Mar 2026
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