skip to content

The Godwin Laboratory for Palaeoclimate Research

 

Wed 04 Mar 14:00: From Mantle Convection to Seismic Observations – and Back?: The Impact of Tomographic Resolution and Mineralogical Uncertainty on Reconstructed Mantle Evolution

http://talks.cam.ac.uk/show/rss/15125 - Thu, 12/02/2026 - 12:02
From Mantle Convection to Seismic Observations – and Back?: The Impact of Tomographic Resolution and Mineralogical Uncertainty on Reconstructed Mantle Evolution

Understanding the structure and evolution of Earth’s mantle is fundamental for constraining plate-driving forces, lithospheric stresses, and the long-term behaviour of the geodynamo. While the present-day thermodynamic state of the mantle can be estimated from seismic tomography and high-pressure mineral physics, putting tight constraints on temperature and chemical heterogeneity based on seismic observations still remains a major challenge. Geodynamic simulations, by contrast, provide theoretical predictions for mantle evolution. However, their quality depends on how well input parameters are known, and they are only meaningful when rigorously tested through geodynamic–tomographic comparisons or, ideally, by comparing secondary predictions to a broad range of Earth observations. In this talk, I will discuss recent developments and potential future directions aimed at providing a quantitative, physically consistent link between temperatures predicted by mantle circulation models (MCMs) and the wealth of information contained in seismic recordings. For example, using global 3-D seismic wavefield simulations and full-coupling free-oscillation calculations for the MCM -derived structures, synthetic traveltime residuals and seismic spectra can be computed that accurately capture the various non-linearities in the relation to the underlying temperatures. A critical component in this context is the effect of mineral anelasticity, and it is particularly important to account for the associated uncertainties when comparing synthetic and real data. In addition to this forward approach, geodynamic adjoint inverse modelling can be used to retrodict mantle flow back in geologic time starting from the present-day state derived from tomographic images. Key challenges therein include determining the resolution and uncertainty of the tomography used and how they affect adjoint-state reconstructions, as well as assessing how accurately temperatures can be recovered using uncertain mineralogical information. Addressing the scale discrepancy between fluid dynamic predictions and seismically imaged structures is crucial, as validating reconstructed mantle flow involves surface topography calculations that are highly sensitive to the tomographic input. To improve future retrodictions, we conducted synthetic experiments illustrating the challenges of integrating tomographic and geodynamic models. Using a reference MCM as the “true” structure, we employed the linear SOLA Backus–Gilbert framework to explore spatially optimised averaging kernels and noise-related uncertainties, proposing a workflow to identify ideal SOLA parameters for next-generation adjoint models. Furthermore, synthetic closed-loop experiments demonstrate that tomographic damping, spatial blurring, and simplified mineralogies cause substantial deviations from “true” temperatures, especially near phase transitions. When such temperatures are used to prescribe buoyancy in geodynamic simulations, the errors will amplify non-linearly, potentially activating incorrect phase transitions and significantly altering reconstructed flow trajectories.

Add to your calendar or Include in your list

Wed 18 Feb 14:00: From icequakes to earthquakes: Using seismology across the scales to understand Antarctica’s glacial and subglacial environment

http://talks.cam.ac.uk/show/rss/15125 - Wed, 11/02/2026 - 11:36
From icequakes to earthquakes: Using seismology across the scales to understand Antarctica’s glacial and subglacial environment

Seismic waves, generated both within the ice and by distant earthquakes, provide a unique window into some of the most inaccessible environments on Earth. In this way, cryoseismology, a rapidly evolving branch of seismology, offers a wide and exciting range of opportunities to study the glacial and subglacial environments of polar and mountain regions. Such observations are invaluable to our understanding of the cryosphere and for constraining how ice sheets will respond to a warming world. In this talk, I will present results from two studies that demonstrate how cryoseismology can be used to improve our understandings of the Antarctic Ice Sheet. Starting small, an array of accelerometers and geophones deployed on the Larsen C Ice Shelf in 2022 detected 108 icequakes originating from within the ice shelf. Correlations between icequake explosivity and tidal phase suggest that this micro-seismicity is predominantly driven by tidal infiltration and circulation of seawater in the ice. In combination with radar data, this novel observation provides new insight into how rifting, which eventually leads to the calving of large tabular icebergs such as A68 , can be controlled by the internal structure of ice shelves, with important implications for their long-term stability. At the other end of the scale, the growing number of seismic deployments across Antarctica has enabled the use of teleseismic earthquakes to investigate the continent’s lithospheric structure. These data, however, also record information about the basal conditions of the Antarctic Ice Sheet. By building on established receiver function and P-wave coda autocorrelation methods, both the extent of subglacial sediment and the presence of subglacial till can be constrained. Rutford Ice Stream provides an ideal natural laboratory for testing this approach, with complementary radar, active-source seismic, and drilling data allowing the seismic signatures of subglacial till to be robustly validated. This proof of concept is then extended across Antarctica, where mapping the distribution of this deformable till can inform ice sheet models and reduce uncertainties in the consequent sea-level rise predictions.

Add to your calendar or Include in your list

Tue 24 Feb 12:00: Melting of unconstrained particles

http://talks.cam.ac.uk/show/rss/15125 - Wed, 11/02/2026 - 08:56
Melting of unconstrained particles

What do ice cubes in a cocktail have in common with butter on a pan? And what can both tell us about the physics of melting? Through controlled experiments we explored the melting dynamics of (nearly) unconstrained systems, and compared our results with direct numerical simulations and analytical predictions, and show that two idealised systems at the extremes of Reynolds number (i.e., lubrication approximation, and fully developed isotropic turbulence) can provide useful insights for complex, inaccessible phenomena.

Add to your calendar or Include in your list

Wed 11 Feb 14:00: What triggering can teach us on faults, fluids and slow slip

http://talks.cam.ac.uk/show/rss/15125 - Tue, 10/02/2026 - 13:25
What triggering can teach us on faults, fluids and slow slip

It is now well known that large earthquakes can trigger a wide range of slip events, from slow to fast, on active faults at very large distances. I will discuss instances of triggering following the 2023 Kahramanmaraş earthquakes in Turkiye, all pointing the finger on the role of fluids and granular dynamics using geodetic data and seismological records.

Add to your calendar or Include in your list

Tue 24 Feb 12:00: TBC

http://talks.cam.ac.uk/show/rss/15125 - Tue, 10/02/2026 - 08:58
TBC

Abstract not available

Add to your calendar or Include in your list

Wed 25 Feb 14:00: Exploring upper mantle flow with seismic anisotropy and mantle circulation models

http://talks.cam.ac.uk/show/rss/15125 - Tue, 10/02/2026 - 00:27
Exploring upper mantle flow with seismic anisotropy and mantle circulation models

Plate tectonics, and its familiar dynamic consequences including earthquakes, volcanoes, and even the surface topography, are intrinsically linked to convection in the silicate mantle below. Mantle convection is a complex thermochemical process by which hot material rises from the deep Earth to the surface via upwellings like plumes, and cold material is returned to the deep via subduction. Tomographic images of seismic velocity provide a snapshot of the thermochemical state of the mantle at the present day, but do not directly constrain dynamic processes such as deformation. Seismic anisotropy, the variation of seismic wave speed with direction, emerges as a result of the long-wavelength ordering of smaller features (such as crystals, fractures, or melt inclusions) and thus can give information about processes such as deformation and flow. Recent advances in seismic tomography have provided a global picture of anisotropy throughout the mantle, but quantitatively interpreting these for mantle flow requires models. The NERC -funded MC2 project has focused on building a large suite of mantle circulation models (MCMs) – convection simulations constrained by models of the Earth’s plate motion over the last 1 billion years – exploring a range of different parameters of mantle convection. It is providing a framework to compare these models to a broad spectrum of observations (seismic, geodynamic, geochemical, and geomagnetic). In this talk, I will outline how we are using these models to predict the seismic anisotropy resulting from the flow in the upper mantle in these models and comparing it to tomographic models of radial anisotropy. These comparisons demonstrate the influence of parameters including the radial viscosity profile of the shallow mantle and the core-mantle boundary temperature on the resulting anisotropy. The models we produce show a consistent discrepancy with the tomographic images at around 100 km below mid-ocean ridges, suggesting that the anisotropy observed here for the Earth cannot be explained by solely by the lattice preferred orientation of olivine. The most plausible alternative explanation for these signatures is the presence of deep melt below the ridges.

Add to your calendar or Include in your list

Wed 11 Mar 14:00: Seismotectonics of the Sumatra-Andaman region: insights from block modelling, high-resolution seismicity and seismic imaging

http://talks.cam.ac.uk/show/rss/15125 - Thu, 05/02/2026 - 11:16
Seismotectonics of the Sumatra-Andaman region: insights from block modelling, high-resolution seismicity and seismic imaging

Convergence of the Indo-Australian and Eurasian plates along the Sunda subduction zone generates large earthquakes and tsunamis, exemplified by the 2004 Mw9.2 event. The subduction zone is a classic example of slip partitioning, where oblique convergence is partitioned between the megathrust and upper plate strike-slip faults. Upper plate faults are highly active, but their location and slip rates offshore are not well known. Additionally, the distribution of locked and creeping areas along the fault systems is not well resolved.

In this talk, I’ll share initial results from two studies investigating this tectonic system. We first use earthquake and GPS data to resolve fault slip rates through block modelling. We find several new features of the tectonic system, including the separation of the forearc into two independent blocks and a rapid slip rate of the Andaman-Nicobar fault in the Andaman Sea. Second, to better understand the geometry and behaviour of the Great Sumatran Fault in Northern Sumatra, we deployed 130 seismic nodes primarily for microseismicity detection and subsurface imaging. Our ~18 months of data reveal pronounced differences in seismicity along the fault. One segment appears to be creeping, with abundant shallow microseismicity and repeating earthquakes, while the other appears to have a locked upper crust.

Add to your calendar or Include in your list

Tue 17 Feb 12:00: Iron rain and iron snow in planetary interiors: insights from fluids experiments

http://talks.cam.ac.uk/show/rss/15125 - Wed, 04/02/2026 - 10:39
Iron rain and iron snow in planetary interiors: insights from fluids experiments

At a late stage of its accretion, the Earth experienced high-energy planetary impacts. Following each collision, the metal core of the impactor sank as millimetric drops into a molten silicate magma ocean — the so-called “iron rain”. The efficiency of chemical equilibration between metal and silicates controlled the initial temperature and composition of the Earth. Current parameterizations of the equilibration efficiency neglect the influence of planetary rotation after impact.

In a different planetary context, the icy moon Ganymede sustains an intrinsic magnetic field, likely generated by fluid motions in its iron-rich liquid core. Core evolution models suggest solidification proceeds from the outer boundary inward, producing dense, pure iron crystals that sink and remelt at greater depth. This process, referred to as “iron snow”, is thought to drive core dynamics that feed the magnetic field. Yet, it is commonly modeled as purely fluid convection, neglecting the presence and properties of solid particles.

Add to your calendar or Include in your list

Tue 03 Mar 12:00: Sulphur stories from the land, sulfur stories from the sea

http://talks.cam.ac.uk/show/rss/15125 - Tue, 03/02/2026 - 14:04
Sulphur stories from the land, sulfur stories from the sea

The sulfur cycle is one of the main contributors to the control of O2 and CO2 atmospheric levels during Earth’s history. It interacts with both the carbon and oxygen cycles during weathering on land and diagenesis in the ocean. It is thus paramount to reconstruct accurately its variations in the past. To do so, sulfur isotope ratios in carbonates are an increasingly used archive, though major questions remains about (1) how sulfur isotope ratios are recorded in carbonate, (2) how well they are preserved and (3) what they mean.

I will present recent progress about how sulfate is incorporated in carbonates and a few examples of paleoenvironmental investigations, both on land and in the ocean. In continental environments, carbonates help retrace the origin of sulfur and understand the role of sulfuric acid in diagenetical processes. In oceanic sediments, reliably reconstructing past sulfur isotope ratios of seawater from carbonates will help to unpack various steps of diagenetic alteration and thus collect key information about the activity of microorganisms in deep ocean sediments.

Add to your calendar or Include in your list

Mon 23 Feb 13:00: Constraining Carbon in Earth’s Mantle

http://talks.cam.ac.uk/show/rss/15125 - Tue, 03/02/2026 - 13:44
Constraining Carbon in Earth’s Mantle

In situ carbon isotopes are a powerful but under-utilised tracer of mantle processes, in part due to analytical challenges and lack of reference materials. In this talk, I present a new SIMS method for concurrently measuring carbon isotopes and carbon concentration in basaltic glass, enabling improved precision at low carbon concentrations and high spatial resolution. Applying this method to olivine-hosted melt inclusions, I first describe recent work constraining the convecting upper mantle, which yields a more positive and more tightly defined δ13C value than previously assumed, along with a lower organic burial fraction of carbon. I then present results from the Icelandic primordial mantle reservoir sampled at Miðfell, revealing anomalously heavy carbon isotopic compositions coupled with depleted incompatible element concentrations, potentially linking early core formation to modern mantle heterogeneity. Together, these results refine the mantle carbon baseline and deep carbon cycle and demonstrate how melt inclusions retain isotopic memory of Earth’s interior processes.

Add to your calendar or Include in your list

Mon 09 Feb 13:00: Modelling explosive volcanic eruptions from proximal hazards to global climate disruption

http://talks.cam.ac.uk/show/rss/15125 - Tue, 03/02/2026 - 13:41
Modelling explosive volcanic eruptions from proximal hazards to global climate disruption

Explosive volcanic eruptions have critical impacts on our environment and societies including local-regional scale devastation from pyroclastic flows and tephra fallout, regional-continental scale air pollution and airspace shutdown, and global-scale cooling of Earth’s surface. I will give an overview of my group research and how it contributes to understanding and managing these impacts. First, I will discuss how volcanic plume modelling, informed by laboratory experiments and observational databases, helps us understand the relationship between eruption intensity, atmospheric conditions and the height of injection of volcanic ash and gas into the atmosphere. Second, I will discuss how numerical models ranging from reduced-complexity models to full-blown Earth System Models with interactive stratospheric aerosols can help us constrain the radiative forcing and climatic impacts of volcanic eruptions. Using ice-core, geological and satellite records, I will apply these models to discuss volcanic impacts on climate from 8,000 BC to 2100. Last, I will bring together volcanic plume, aerosol and climate modelling to interrogate how ongoing climate change driven by anthropogenic activities will affect the life cycle of volcanic stratospheric aerosols, and whether we should expect more or less volcanic cooling as Earth warms.

Add to your calendar or Include in your list

Wed 18 Feb 14:00: From icequakes to earthquakes: Using seismology across the scales to understand Antarctica’s glacial and subglacial environment

http://talks.cam.ac.uk/show/rss/15125 - Tue, 03/02/2026 - 10:54
From icequakes to earthquakes: Using seismology across the scales to understand Antarctica’s glacial and subglacial environment

Seismic waves, generated both within the ice and by distant earthquakes, provide a unique window into some of the most inaccessible environments on Earth. In this way, cryoseismology, a rapidly evolving branch of seismology, offers a wide and exciting range of opportunities to study the glacial and subglacial environments of polar and mountain regions. Such observations are invaluable to our understanding of the cryosphere and for constraining how ice sheets will respond to a warming world. In this talk, I will present results from two studies that demonstrate how cryoseismology can be used to improve our understandings of the Antarctic Ice Sheet. Starting small, an array of accelerometers and geophones deployed on the Larsen C Ice Shelf in 2022 detected 108 icequakes originating from within the ice shelf. Correlations between icequake explosivity and tidal phase suggest that this micro-seismicity is predominantly driven by tidal infiltration and circulation of seawater in the ice. In combination with radar data, this novel observation provides new insight into how rifting, which eventually leads to the calving of large tabular icebergs such as A68 , can be controlled by the internal structure of ice shelves, with important implications for their long-term stability. At the other end of the scale, the growing number of seismic deployments across Antarctica has enabled the use of teleseismic earthquakes to investigate the continent’s lithospheric structure. These data, however, also record information about the basal conditions of the Antarctic Ice Sheet. By building on established receiver function and P-wave coda autocorrelation methods, both the extent of subglacial sediment and the presence of subglacial till can be constrained. Rutford Ice Stream provides an ideal natural laboratory for testing this approach, with complementary radar, active-source seismic, and drilling data allowing the seismic signatures of subglacial till to be robustly validated. This proof of concept is then extended across Antarctica, where mapping the distribution of this deformable till can inform ice sheet models and reduce uncertainties in the consequent sea-level rise predictions.

Add to your calendar or Include in your list

Thu 12 Feb 11:30: A Stefan-Graetz problem in the kitchen: cleaning by convective dissolution

http://talks.cam.ac.uk/show/rss/15125 - Tue, 03/02/2026 - 10:28
A Stefan-Graetz problem in the kitchen: cleaning by convective dissolution

One method of removing layers of unwanted material from a surface is to contact it with a solvent in which it will dissolve. The rate of dissolution is enhanced when the solvent is flowing, which is why dishwashers spray liquid around to both contact soiled plates with the aqueous cleaning solution and  to generate falling films over the surfaces. [This is also why you should stack the dirty dishes properly!] In many cases a cleaning front develops, between soil-free and soiled regions. Modelling the front dynamics – a Stefan problem – is complicated by the rate of mass transfer being spatially non-linear – the Graetz problem. In this talk I will present recent experimental and numerical work on this topic, driven by an interest to improve the sustainability of cleaning-in-place of food processing equipment. No food will be cleaned during this talk, just lots of instant coffee.

Add to your calendar or Include in your list

Tue 24 Feb 11:30: TBC

http://talks.cam.ac.uk/show/rss/15125 - Mon, 02/02/2026 - 09:17
TBC

Abstract not available

Add to your calendar or Include in your list

Fri 20 Mar 16:00: Title to be confirmed

http://talks.cam.ac.uk/show/rss/15125 - Wed, 28/01/2026 - 09:10
Title to be confirmed

Abstract not available

Add to your calendar or Include in your list

Fri 27 Feb 16:00: Title to be confirmed

http://talks.cam.ac.uk/show/rss/15125 - Wed, 28/01/2026 - 09:07
Title to be confirmed

Abstract not available

Add to your calendar or Include in your list