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The Invisible Brake: Near‑Surface Cooling Stalls Giant Dyke Swarms  

EOS - Tue, 11/18/2025 - 14:00
Editors’ Highlights are summaries of recent papers by AGU’s journal editors. Source: Journal of Geophysical Research: Solid Earth

Giant dyke swarms are networks of long, sheet-like cracks in Earth’s crust that carry molten rock (magma) sideways for hundreds of kilometers. In a new study, Foschi and Cartwright [2025] use shallow, laterally injected sills—thin, horizontal sheets of solidified magma—as natural pressure gauges to reconstruct magma pressure along a 660 kilometers dyke from the Mull volcanic center.

The authors run large Monte Carlo simulations (many randomized model runs) to account for uncertainty and find that magma pressure remained high enough that eruption at the surface should have been possible in many places. Despite that, the dykes did not erupt, and the paper shows the classic ideas of neutral buoyancy (where magma stops rising because it becomes the same density as the surrounding rock) or simple mechanical blockage do not explain this. Instead, field evidence and the pressure reconstructions point to near‑surface cooling by groundwater: when hot magma meets cold water or wet sediment it cools, becomes more viscous (thicker), and stalls before reaching the surface.

This finding matters because it changes how we think about long‑range magma transport and eruption risk: strong subsurface cooling can prevent eruptions even when subsurface pressures are high. The sill‑piezometer approach also offers a practical method for constraining magma pressure in other volcanic systems, improving models of where and how magma moves underground.

Citation: Foschi, M., & Cartwright, J. A. (2025). Constraints on magma pressure distribution during long range lateral propagation of giant radial dyke swarms. Journal of Geophysical Research: Solid Earth, 130, e2025JB031995. https://doi.org/10.1029/2025JB031995

—Nikolai Bagdassarov, Associate Editor, JGR: Solid Earth

Text © 2025. The authors. CC BY-NC-ND 3.0
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Andes glaciers will fail to buffer megadroughts by century's end, study suggests

Phys.org: Earth science - Tue, 11/18/2025 - 10:00
In light of the ongoing fifteen-year megadrought in Chile, an international team of researchers, including Francesca Pellicciotti from the Institute of Science and Technology Austria (ISTA), addressed a bold future scenario. Their findings: by the end of the century, the considerably worn-out glaciers will not be able to buffer a similar megadrought. They call for coordinated global climate policies to develop effective water management strategies. The results are published in Communications Earth & Environment.

Antarctic ice loss linked to 'storms' at ocean's subsurface

Phys.org: Earth science - Tue, 11/18/2025 - 10:00
Researchers at the University of California, Irvine and NASA's Jet Propulsion Laboratory have identified stormlike circulation patterns beneath the Antarctic ice shelves that are causing aggressive melting, with major implications for global sea level rise projections.

Weather behind past heat waves could return far deadlier

Phys.org: Earth science - Tue, 11/18/2025 - 10:00
The weather patterns that produced some of Europe's most extreme heat waves over the past three decades could prove far more lethal if they strike in today's hotter climate, pushing weekly deaths toward levels seen during the COVID pandemic, according to a study in Nature Climate Change.

Early Triassic sediments reveal Earth's hidden wildfire past

Phys.org: Earth science - Tue, 11/18/2025 - 00:00
An international team of scientists, including a senior researcher at Heriot-Watt University in Edinburgh, Scotland, has uncovered new evidence of ancient wildfires that reshapes our understanding of Earth's turbulent Early Triassic epoch, about 250 million years ago.

Seismic Structure Beneath Western Pacific and Adjacent Regions from Seismic Full-Waveform Inversion

Geophysical Journal International - Tue, 11/18/2025 - 00:00
SummaryA comprehensive full-waveform inversion model of the seismic velocity, covering nearly the entire tectonic domain of the western Pacific (FWP24) is developed using an optimized many-core version of SPECFEM3D_GLOBE on the New Generation Sunway supercomputer. Taking the global adjoint tomography model GLAD-M25 as the initial model, the three-component seismograms from 1 228 earthquakes recorded at 3 687 stations are employed in iterative gradient-based inversions for three period bands: 40-100 s, 17-40 s, and 10-60 s. A total of 36 iterations are carried out using the conjugate gradient method to update the velocities of horizontally and vertically polarized P-waves and S-waves (Vph, Vpv, Vsh, and Vsv) in the FWP24 model. This process systematically reduces the phase difference between the synthetic and observed seismograms within the phase measurements. Compared with existing region inversion results, the FWP24 model realizes a wider, more continuous, and higher-resolution inversion range, including all subduction zones in the western Pacific (e.g. Kurile-Japan, Izu-Bonin-Mariana, New-Britain-Solomon, New-Hebrides, and Tonga-Kermadec). Furthermore, compared to the initial model, FWP24 reveals more detailed structures particularly in oceanic regions around the Philippine Sea Plate, the Caroline Sea Plate and the Ontong-Java Plateau by applying more seismic data.

Inference of the S- to P-wave velocity anomalies ratio and its uncertainty with an application to South-East Asia

Geophysical Journal International - Tue, 11/18/2025 - 00:00
SummaryThe ratio R of shear-wave to compressional-wave velocity variations (dlnVs/dlnVp) is a useful physical parameter to study the thermochemical properties of the Earth’s interior. Several approaches have been employed to estimate R (or its inverse 1/R), but they either assume the same local resolution in models of dlnVs and dlnVp or assume the same ray paths for S- and P-phases, while excluding valuable data and overlooking uncertainties. We overcome these issues by characterizing both dlnVs and dlnVp through the Backus-Gilbert based SOLA method to obtain R including its uncertainties. This approach enables us to ensure that dlnVs and dlnVp share the same local resolution, making it possible to compute their ratio through division. In addition, SOLA provides uncertainties on dlnVs and dlnVp, which we propagate into our estimates of R using the Hinkley distribution for dlnVs/dlnVp. When resembling a Gaussian, the Hinkley distribution provides Gaussian uncertainties for R, enabling us to interpret tomographic features as for instance in terms of slab morphology or partial melt with greater confidence. To illustrate our new approach, we use a data set of P- and S-phase onset-time residuals from ISC to infer the velocity anomalies and the ratio R (or 1/R) in South-East Asia between 100 and 800 km depth. As the SOLA method is driven by data uncertainties, we reassess the provided ISC uncertainties using a statistical approach before developing models of dlnVs and dlnVp with their uncertainties. Based on our quantitative model estimates, we argue that a large velocity anomaly below the Sumatra slab, with a value of R over 2.5, is resolved given our data and their uncertainties. However, in contrast to previous work, we do not find evidence for a slab hole under Java. Our proposed approach to obtain R with uncertainties using the Hinkley distribution can be applied to a large range of tomographic imaging settings.

Geomagnetic reversals and excursions as an outcome of non-equilibrium bulk turbulence in the Earth’s core

Geophysical Journal International - Tue, 11/18/2025 - 00:00
SummaryWe investigate the effect of statistically non-stationary turbulence in the Earth’s outer core on the effective turbulent electromotive force generated by the convectively driven flow of liquid iron and the evolution characteristics of the geomagnetic field. The non-stationarity means that interactions of distinct waves are crucial, and the effect of beat induces a slow time variation of the large-scale electromotive force. This provides an attractive and fairly simple physical mechanism for the random appearance of short-lived geomagnetic excursions and reversals separating long periods of relatively stable field, through non-synchronized evolution of the amplifying α-effect and turbulent diffusion. This implies rare and random appearance of simultaneous suppression of the α-effect and enhancement of diffusion which leads to a sudden magnetic energy drop, i.e. an excursion. The turbulent field of what is termed MAR waves (Magnetic-Archemedean-Rossby) is analysed. The dispersion relation and structure of such waves involving the joint effect of the Lorentz, buoyancy, and Coriolis forces together with curvature of the core-mantle boundary are obtained and utilized for estimation of the non-stationary electromotive force in the core. The solutions for the large-scale dipole possess an Earth-like behaviour, magnitude, and timescales, and the physical mechanism of the process, including identification of two dynamically important parameters, is discussed. Similar ideas concerning the dynamics of waves within the so-called Stratified Ocean at the top of the Core (SOC) were considered in the recent work Mizerski (2025). The SOC is an important but thin, strongly stratified layer near the core-mantle boundary, and here, the possibility of global non-equilibrium dynamo mechanisms is analysed. It is possible that the surface and bulk mechanisms coexist in the core, both adding to the complexity of the observed picture of reversal occurrences.

First complete record of global underground CO₂ storage released

Phys.org: Earth science - Mon, 11/17/2025 - 21:26
The first-ever audited account of the actual amounts of CO2 stored underground by CCS projects globally has been released. It was created by a new international consortium of scientists and industrial partners, including NTNU.

Resilient Distributed Coverage Control of Satellite Swarms via Local Voronoi Feedback

Publication date: Available online 13 November 2025

Source: Advances in Space Research

Author(s): Takehiro Yasuda, Mai Bando, Shinji Hokamoto

Emissions Assessment of Low Earth Orbit (LEO) Broadband Megaconstellations; Starlink, OneWeb and Kuiper

Publication date: Available online 13 November 2025

Source: Advances in Space Research

Author(s): OGUTU B. OSORO, EDWARD J. OUGHTON, ANDREW WILSON, AKHIL RAO

Rover Wheel Tribocharging in Lunar Shadowed Regions: Deriving a Speed Limit for Charge Accumulation

Publication date: Available online 13 November 2025

Source: Advances in Space Research

Author(s): W.M. Farrell, M.I. Zimmerman

TEC increment evaluation technique during X class flares using GNSS data

Publication date: Available online 13 November 2025

Source: Advances in Space Research

Author(s): V.S. Lobanova, I.A. Ryakhovsky, B.G. Gavrilov, A.I. Sapunova, Y.V. Poklad, V.M. Ermak

Designing Observer-Based Adaptive Multi-Model Predictive Attitude Control for Flexible Satellites

Publication date: Available online 12 November 2025

Source: Advances in Space Research

Author(s): Mohammad Fathi, Hossein Bolandi, Bahman Ghorbani Vaghei

Hierarchical Trajectory Planning for Multi-Conjunction Scenarios Based on Convex Corridor Decomposition

Publication date: Available online 12 November 2025

Source: Advances in Space Research

Author(s): Jikai Wang, Xue Bai

Defining Factory in Space: Comparative Analysis of Components, Features, and Functions

Publication date: Available online 12 November 2025

Source: Advances in Space Research

Author(s): Farouk Abdulhamid, Brendan P. Sullivan, Sergio Terzi

Anti-unwinding immersion and invariance adaptive control for spacecraft attitude tracking

Publication date: Available online 12 November 2025

Source: Advances in Space Research

Author(s): Xuan Peng, Fengli Dai

Integrated Modeling and Active Suppression of Multi-Source Micro-vibrations in Aerospace Vehicles

Publication date: Available online 12 November 2025

Source: Advances in Space Research

Author(s): Zimu Zhang, Qing Li, Zhaoguo Zhang, Lei Liu, Wei Li

SuperTIGER Galactic Cosmic-Ray Source Abundances for the Charge Interval <math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si51.svg" class="math"><mrow><mn>16</mn><mo>⩽</mo><mi>Z</mi><mo>⩽</mo><mn>56</mn></mrow></math>

Publication date: Available online 12 November 2025

Source: Advances in Space Research

Author(s): N.E. Osborn, N.E. Walsh, Q. Abarr, Y. Akaike, W.R. Binns, R.G. Bose, T.J. Brandt, D.L. Braun, N.W. Cannady, R.M. Crabill, P.F. Dowkontt, S.P. Fitzsimmons, T. Hams, M.H. Israel, J.F. Krizmanic, A.W. Labrador, W. Labrador, L. Lisalda, R.A. Mewaldt, J.W. Mitchell

<strong>Nonlinear Shock and Solitary Wave Structures in Nonplanar Non-Maxwellian Plasmas</strong>

Publication date: Available online 12 November 2025

Source: Advances in Space Research

Author(s): Shakir Ullah, Abdullah Alshehab, Muhammad Shohaib, Huda Alfannakh, Najeh Rekik

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