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Oxidation state and volatile element evolution during equilibrium planetary accretion: The case study for mars and vesta

Earth and Planetary Science Letters - Wed, 08/26/2026 - 07:47

Publication date: 15 October 2026

Source: Earth and Planetary Science Letters, Volume 692

Author(s): Fabrice Gaillard, Yves Marrocchi, Gregory Rogerie, Mohamed A. Bouhifd, Camille Bernard, Mathieu Roskosz

Temperature-dependent kinetics and saturation of OH formation during solar wind proton implantation

Earth and Planetary Science Letters - Wed, 08/26/2026 - 07:47

Publication date: 15 October 2026

Source: Earth and Planetary Science Letters, Volume 692

Author(s): Qi-ao Chen, Wen Yu, Hao Yan, Tian Zhang, Hong Tang, Xiongyao Li

Cave-based chronology of valley incision in the glaciated Northern Carpathians

Earth and Planetary Science Letters - Wed, 08/26/2026 - 07:47

Publication date: 15 October 2026

Source: Earth and Planetary Science Letters, Volume 692

Author(s): Jacek Szczygieł, Gregory D Hoke, Artur Sobczyk, Helena Hercman, Lee B. Corbett, Jason Drebber, Alan J. Hidy, Paul R. Bierman, Marc W. Caffee

Modelling ductile strain localization with evolutive stochastic rheologies

Earth and Planetary Science Letters - Wed, 08/26/2026 - 07:47

Publication date: 15 October 2026

Source: Earth and Planetary Science Letters, Volume 692

Author(s): Andréa Tommasi, Felipe Sáez-Leiva, Lilou Zeller, Michel Peyret, Riad Hassani, Maurine Montagnat

The dynamical surface of Phobos: A morphodynamic atlas

Earth and Planetary Science Letters - Wed, 08/26/2026 - 07:47

Publication date: 15 October 2026

Source: Earth and Planetary Science Letters, Volume 692

Author(s): Isabel Herreros, Sébastien Charnoz

Microcline reveals how a common mineral surface triggers ice formation in clouds

Phys.org: Earth science - Tue, 08/25/2026 - 21:40
Pure water freezes only at around -38°C (-36°F). Tiny mineral dust particles act as so-called ice nucleators—crystallization seeds on which ice crystals form. A research team at Bielefeld University and the University of Vienna, in cooperation with researchers at the University of Helsinki, has now demonstrated for the first time at the molecular scale why the mineral microcline is particularly effective at forming ice in clouds. The study, published in published in the journal Nature Communications, provides a new explanation for processes that influence climate and precipitation worldwide.

Finding the world's highest late Middle Pleistocene marine deposits

Phys.org: Earth science - Tue, 08/25/2026 - 21:00
Selma Sarı and an international group of colleagues investigated the TOL-1 section in the Mut Basin (southern Türkiye), while documenting the world's highest known Late Middle Pleistocene (MIS 7) marine deposits, preserved at 1,177 m (3,860 feet) above mean sea level on the southern margin of the Central Anatolian Plateau.

Could 12 inches of rain hit New York City? AI maps plausible rare storms

Phys.org: Earth science - Tue, 08/25/2026 - 18:40
Can a city's seawall stand up to a blockbuster storm? Will a region's power grid hold against record-breaking heat? And can a town's firefighting resources contain a major wildfire?

Satellite analysis tracks carbon cost of coastal erosion

Phys.org: Earth science - Tue, 08/25/2026 - 17:00
From Texas to Maine, coastal wetlands and marshes are releasing more than 1.45 billion pounds (660,000 metric tons) of carbon into the ocean each year, according to new research supported by NASA. Coastal marshes, like forests and tundra, store large amounts of carbon in their plants and soil, but changes caused by storms, rising seas and human development can affect how that carbon is stored and transported.

Extreme Heat and Extreme Cold Drive an Increase in Fatal Overdoses

EOS - Tue, 08/25/2026 - 13:18

Anomalously high and low temperatures affect human habits in myriad ways—forcing us inside, disrupting our sleep, and even exacerbating mental health conditions.

Temperature extremes seem to affect drug use and overdose deaths, too. A new study published in Drug and Alcohol Dependence shows that both extreme heat and extreme cold may cause an uptick in fatal overdoses. The study adds to a limited but growing field of research on temperature and drug use and could help communities better prevent overdoses, especially as climate change makes our weather more volatile.

Fatal overdoses are “something we need to pay attention to in the future” as extreme temperature events affect more people.

Fatal overdoses are “something we need to pay attention to in the future” as extreme temperature events affect more people, said Thanh Lu, a research economist at RTI International, a science and policy research institute, and lead author of the new study. (Although there is significant debate about the role of climate change in the occurrence of extreme cold events, there is scientific consensus that climate change is increasing the frequency and intensity of extreme heat waves.)

Though there is little research in the space, the study confirms previous findings indicating a link between heat and overdoses, said Raminta Daniulaityte, a population health researcher at Arizona State University who was not involved in the new study.

Hot and Cold

To further study the link between extreme temperatures and fatal overdoses, Lu and the research team compared cause-of-death data from 1999 to 2021 from the National Center for Health Statistics to county-level weather data from NOAA’s Global Historical Climatology Network. They analyzed how many fatal overdoses occurred when a person would have been experiencing extreme temperatures relative to a typical day in that county in each month.

They found that annual fatal overdoses increased with temperature extremes. For example, one day above 90°F (32°C) relative to days in the 70°F (21°C) to 80°F (27°C) range led to a 0.2% increase in overdoses. Similarly anomalous extreme low temperatures led to a similar increase in overdoses. According to the analysis, in 2021, temperatures likely drove 1,431 of the year’s 107,000 fatal overdoses.

Despite the link, the overall impact of extreme temperatures on total overdoses was still small, with temperature driving about 1% of the total annual fatal overdoses that the team studied.

Researchers also found that the types, not just the number, of overdoses varied with temperature; opioid-related overdoses occurred more at extreme low temperatures, while stimulant-related overdoses were more correlated with extreme high temperatures. The results align with what Daniulaityte sees in her research in the Phoenix area, where afternoon temperatures in the summer frequently exceed 110°F (43°C). In particular, her research shows a significant relationship between the impacts of heat and overdoses from stimulants, she said.

Extreme temperatures likely drive overdoses in two main ways, Lu said: First, substance use can decrease the body’s ability to cope with extreme heat and extreme cold, making some of the effects of substances, like altered heart rate and weakened breathing, more likely to lead to a fatality. Second, extreme temperatures can affect economic or employment opportunities, decreases in which are known to increase overdoses.

“We were not able to examine or tease out what mechanism, specifically, is a key driver,” Lu said. However, moderately high and low temperatures had a small effect on fatal overdoses, too, indicating that heat and cold can drive overdoses even when it’s not too hot or too cold to go outside or go to work. This means the physiological effects of extreme temperatures likely play an important role, she said.

Daniulaityte said scientists see more consistent links between heat and stimulant-related overdoses than opioid-related overdoses. “We need more data” on how heat affects opioid-related overdoses, she said.

Prevention in a Warming World

The overall impact of extreme temperatures on total overdoses was small in the study, and the researchers did not explicitly link the increase in fatal overdoses to climate change. Still, extreme temperature may become more of a factor in overdose deaths as the climate continues to warm, Lu said.

“People who will be impacted first will be people who experience multiple vulnerabilities.”

Mitigating the effects of extreme temperatures on overdose deaths could look like providing more cooling and warming centers for unhoused people who use drugs or increasing communities’ supplies of naloxone (a medication that reverses an opioid overdose) when extreme temperatures are expected, Lu said. Policymakers should pay equal attention to the effects of both extreme cold and extreme hot weather on overdoses, she said.

Daniulaityte emphasized that increased risk for overdoses is just another way that climate change harms the most vulnerable members of society. “We see the risks [of overdoses] significantly higher for people who are experiencing housing instability and poor access to health services,” she said.

“People who will be impacted first will be people who experience multiple vulnerabilities.”

—Grace van Deelen (@gvd.bsky.social), Staff Writer

Citation: van Deelen, G. (2026), Extreme heat and extreme cold drive an increase in fatal overdoses, Eos, 107, https://doi.org/10.1029/2026EO260270. Published on 25 August 2026. Text © 2026. The authors. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

The Magnetic Face of Plasma Irregularities on Mars

EOS - Tue, 08/25/2026 - 12:00
Editors’ Highlights are summaries of recent papers by AGU’s journal editors. Source: AGU Advances

Plasma density irregularities are small-scale ripples in the ionized gas surrounding the Earth and other planets – some no larger than a hundred-meter city block in length. They can affect the propagation of radio waves by steering, trapping, or scattering specific portions of a radio signal, and thereby impact satellite communications and navigation in a complex manner – GPS navigation being a good example on Earth.

NASA’s Mars Atmosphere and Volatile Evolution (MAVEN) satellite recently revealed that the plasma density irregularities in the Mars ionosphere are electromagnetic in nature, in contrast to the electrostatic nature in the terrestrial ionosphere: the variations in density are accompanied by changes in the magnetic field.

Using numerical simulations to investigate how these irregularities form and evolve, Jiang et al. [2026] find that electromagnetic Rayleigh-Taylor instability (RTI) – a special kind of plasma instability caused by gravity – can induce their formation in the nighttime Mars ionosphere. The magnetic field variations would reach the level of 1 nano-Tesla for plasma density variations up to 70% of the background density.

In addition to improving our understanding of the physical processes shaping the Mars ionosphere, these findings suggest that electromagnetic Rayleigh-Taylor instabilities may also be applicable on other weakly magnetized planets or satellites in the solar system.

Citation: Jiang, K., Lei, J., & Yan, M. (2026). Beyond the electrostatic approach: Numerical simulations of Martian ionospheric irregularities. AGU Advances, 7, e2026AV002327. https://doi.org/10.1029/2026AV002327

—Andrew Yau, Editor, AGU Advances

Text © 2026. The authors. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

Tides can vary by almost a meter across a single bay, four decades of satellite images reveal

Phys.org: Earth science - Tue, 08/25/2026 - 09:00
Tide levels can vary by almost a meter across a single bay, according to a new study that uses decades of satellite images to measure tides at the scale of individual beaches.

Characterizing differences in seismicity clustering and background rates between Hawaii and California

Geophysical Journal International - Tue, 08/25/2026 - 00:00
SummaryThe statistics of earthquake populations are governed by stress changes and event interactions at various scales which promote non-linear event cascades and seismicity clustering. Earthquake clustering in space and time is observed in both tectonic and volcanically dominated regions; however, notable differences exist for instance during eruptive sequences. Here, we characterize seismicity statistics in California and Hawaii and quantify differences in background rates and clustering. We compare three statistical approaches, i.e, i) Reasenberg declustering, ii) Gamma distribution fit, and iii) Nearest Neighbor Clustering which are applied to seismicity in Hawaii, southern California, and ETAS catalogs with known clustering characteristics. Tests with ETAS-catalogs suggest that background rate variations are more consistently resolvable using the Nearest Neighbor and Gamma distribution algorithm without requiring parameter adjustments to the specific study area. The Nearest Neighbor method tends to overestimate background rates, whereas the Gamma distribution algorithm shows systematic underestimation, suggesting that an ensemble model can improve the performance over any single method. Uncertainties in background rate estimates based on small magnitude events (e.g., M≥2.5) are high, in particular for the Reasenberg method, which overpredicts true rates by up to a factor of 4, and extrapolations to larger magnitudes need to be treated cautiously. Our analysis shows that the combination of the three approaches generates new insights into the processes that govern seismicity clustering. The analysis of southern California seismicity produces consistent results between the different methods, and the distribution of background seismicity rates is indistinguishable from Poissonian rates at magnitudes above 3.5. Conversely, the seismicity in Hawaii exhibits notable non-Poissonian background rate changes. Results from the Nearest Neighbor clustering analysis suggest notable differences between tectonic and volcano seismicity, including background rate changes and more pronounced spatiotemporal clustering around active volcanoes. Hawaiian seismicity is characterized by more localized spatial-temporal clustering, in particular during the 2018 eruption. This difference may be a result of magmatic, hydrothermal and eruptive processes, which make volcanic areas susceptible to stress perturbations and earthquake triggering at small scales.

Probabilistic imaging of sedimentary basins using spatial clustering of magnetotelluric model ensembles change-points

Geophysical Journal International - Tue, 08/25/2026 - 00:00
SummaryMapping the internal structure of sedimentary basins, including the depth to basement, is valuable for a variety of geological applications, particularly the identification of natural resources such as groundwater and minerals, or of the geological structures associated with them. The magnetotelluric (MT) method has proven to be a reliable technique for imaging complete sedimentary sequences, especially in areas where thick sedimentary cover makes imaging challenging. However, due to the high regularisation required by MT inversion procedures, it is limited in its ability to precisely locate geological interfaces, which is crucial for exploration. Building on previous work where we imaged the basement using interface probabilities derived from 1D probabilistic inversion of MT data, we present a new method which allows for the simultaneous classification of multiple interfaces across an entire survey, incorporating constraints on the spatial relationships between models. As a result, we obtain spatially consistent model ensembles and classified interfaces corresponding to transitions between layers of consistent electrical resistivity. This classification effectively reduces the size of the model ensemble, decreasing uncertainty in the estimated depth of the interfaces of interest. We apply this method to the Eucla sedimentary basin in Western Australia, analysing 550 MT sites distributed across 12 profiles. The ensemble clustering clearly identifies three interfaces which are consistent with the sedimentary succession expected from this basin. The results show great consistency across all the survey, providing valuable insights into the geological setting of the area. This research demonstrates the capability to reliably image the structure of a sedimentary basin using MT, within a workflow that integrates probabilistic inversion and model ensemble classification.

Complex conductivity of the Toarcian claystone at Tournemire (Southern France)

Geophysical Journal International - Tue, 08/25/2026 - 00:00
SummaryThe Tournemire Underground Research Laboratory (URL) operated by ASNR (Autorité de Sûreté Nucléaire et de Radioprotection) is a French test site specifically developed to study and comprehend the confinement properties of low-porosity claystone formations. More specifically, this site allows developing an improved knowledge of the transport properties of the Toarcian (Early Jurassic) shale formation. This claystone shares indeed similar characteristics to the Callovo-Oxfordian claystone formation encountered at the Meuse/Haute-Marne underground research laboratory operated by ANDRA (Agence Nationale pour la gestion des Déchets RAdioactifs) to study the feasibility of the long-tern storage of nuclear wastes. In the present study, 18 rock samples of the Toarcian formation are used to study (i) the induced polarization properties of this formation at full water saturation and (ii) the desiccation of this claystone by looking at the evolution of the complex conductivity spectra with the decrease of the water saturation in the frequency range 1 mHz-45 kHz. In this second set of experiments, the complex conductivity spectra are fitted with a double Cole Cole complex conductivity model. We then obtain the values of the first and second Archie’s exponents and estimates of both surface conductivity and normalized chargeability. We also test relationships between the surface conductivity, the normalized chargeability, the quadrature conductivity, and both the cation exchange capacity and water content of these clay-rocks. Furthermore, the laboratory data are favorably explained by the so-called Dynamic Stern Layer (DSL) model developed in the last decade. In order to test this new knowledge in field conditions, an in situ experiment is performed in a gallery of the Tournemire URL to test the ability of the method to image the damage zone around a 80-cm hole drilled normal to the gallery axis. For this purpose, a set of 5 wells equipped with a total of 240 non-polarizing electrodes is successfully used to get both electrical conductivity and normalized chargeability tomograms, which are in turn used to image the water content around the main hole. The results are analysed in terms of stress distribution including the effect of plasticity.

Why marine heat waves and acidification strike together

Phys.org: Earth science - Mon, 08/24/2026 - 22:40
Marine heat waves and extreme ocean acidification events are each damaging on their own. But when both stressors hit simultaneously, their individual effects can be exacerbated.

How atmospheric dryness limits increases in typhoon rainfall

Phys.org: Earth science - Mon, 08/24/2026 - 21:10
Under global warming, scientists have widely expected tropical cyclones (including typhoons and hurricanes) to bring more intense and frequent rainfall. The underlying physics seems intuitive: Rising temperatures allow the atmosphere to hold more moisture, which, combined with intensifying storms, should theoretically trigger more destructive downpours. However, when researchers analyze climate model projections, they encounter a puzzling phenomenon.

Climate Model Benchmarking: Building Trust and Advancing Science

EOS - Mon, 08/24/2026 - 17:27
Editors’ Vox is a blog from AGU’s Publications Department.

As climate models become more advanced and complex, it is increasingly important to evaluate model performance with respect to observations. A new article in Reviews of Geophysics explores climate model evaluation and benchmarking efforts in the scientific community. Here, we asked the authors to give an overview of climate modeling, how scientists evaluate models, and what challenges remain.

When did scientists first start developing climate models?

While today’s climate models are comprised of millions of lines of code and need to be run on large supercomputers, climate modeling started over a century ago. Lewis Fry Richardson published his 1922 book ‘Weather Predication by Numerical Process’, outlining his idea to forecast the weather using differential equations. It took him six weeks to derive an eight-hour forecast by hand. It wasn’t until 1950 when the first computerized weather forecast was run at Princeton University, led by Jule G. Charney. Six years later, Norman Phillips published a paper titled ‘The general circulation of the atmosphere: a numerical experiment’, in which he details the first General Circulation Model (GCM) of the atmosphere.

Climate modeling, as a distinct field of study from weather forecasting, developed significantly throughout the 1960s, with several seminal studies being published which still underpin climate research today, culminating in the first results from a coupled atmosphere-ocean GCM, in which the atmosphere, ice, and ocean interact with each other for the first time (Manabe et al., 1975 Part 1 and Part 2).

What’s the difference between physical climate models and Earth System Models (ESMs)?

GCMs are predecessors of ESMs, which have been expanded to include more processes describing the climate system.

The difference between physical (“physics-based”) climate models (GCMs) and Earth System Models (ESMs) can be very clearly determined: GCMs are predecessors of ESMs, which have been expanded to include more processes describing the climate system. GCMs focus strictly on the physical processes and exchanges of energy and matter between the atmosphere, oceans, land surface, and sea ice. They therefore provide the means to understand the physics of the system.

ESMs are based on more comprehensive model configurations. In addition to the physical representation of the climate system, they also include processes such as interactive atmospheric chemistry, biogeochemical cycles, and marine/terrestrial ecosystems, and carbon exchange between Earth system components. These additional processes help with the realistic representation of the climate system and increase the confidence in future climate projections, but they come with increased costs in resources and time. Which configuration of climate models are used to prepare a simulation is therefore still very much dependent on the planned use of the simulation.

Why is it important to evaluate and benchmark climate models?

A diverse set of tests and diagnostics can help understand differences between models, differences caused by changes over model generations, and identify priorities for future scientific development.

Climate models are among the most important and useful scientific mechanisms to study the Earth system, and the past and future climate. Every generation of climate models brings new advances in representing processes in different components of the Earth system such as the atmosphere, oceans and land and their interactions. State-of-the-art models also include the representation of the carbon cycle across these different domains, allowing us to understand the role of carbon cycling in determining the Earth’s climate. Climate model evaluation with a wide variety of diagnostics is how we develop confidence in the fidelity with which models represent processes that affect future climate projections (IPCC AR 4). A diverse set of tests and diagnostics can help understand differences between models, differences caused by changes over model generations, and identify priorities for future scientific development.

What are some of the different ways that scientists evaluate climate model simulations?

Climate model evaluation is described as the process of comparing model simulations against observational or reanalyzes datasets. Benchmarking is the process where model simulations are evaluated with observations, reanalysis data, or with other models often resulting in a statement made about the “goodness” of the simulation or model based on a predetermined set of standards or criteria. One or more models can be compared against the same set of observations in evaluation. Some of the more basic diagnostics used in model evaluation are the comparison of climatological (average over a period of 30 years or so) means, inter-annual variability and biases often expressed as time series. Maps or spatial patterns comparing models and observations, statistical analyses such as distributions of a specific variable and portrait plots for multi-model evaluation are other approaches commonly used to evaluate models. More complex diagnostics such as water, energy or carbon budgets and cross-domain interactions (e.g. how does temperature vary with precipitation) are also used for better process-based evaluation.

The evaluation of climate model simulations can be grouped in six general approaches. Most approaches require observations and can be applied on a global or regional scale. Credit: Hassler et al. [2026], Figure 2

What are some specific model biases that have been improved due to routine assessments?

Systematic model evaluation assures scientists are frequently reminded of biases that have not been eliminated or that often recur, and it helps modeling centers identify process representations to prioritize in future model development. Biases in cloud and water vapor process representations have been reduced over the past 20 years due to the growth of detailed observations and improvements in cloud vertical distribution and parameter tuning.

The East Asian summer monsoon (EASM), which carries moisture from the Indian and Pacific Oceans to East Asia, exhibits intense interannual variability that results in severe droughts and floods. Several multi-model benchmarking studies have focused on model reproductions of the EASM, and they identified a weakened western North Pacific anticyclone as a primary cause of biases in the western Pacific subtropical high and the Meiyu-Baiu-Changma rainband.

Early efforts in evaluating land carbon cycle models identified persistent biases in the timing of the seasonal variation of vegetation growth, especially with respect to satellite-derived leaf area index (LAI), which were tied to an underestimate of carbohydrate pools carried from one growing season to the next. Land models substantially overestimated aboveground live biomass in the Amazon Basin compared to estimates from satellite observations, which researchers attributed primarily to low autotrophic respiration and excessive allocation of net primary production to wood. Improvements in model representation of vegetation processes significantly reduced these long-standing biases that have been routinely assessed through comparison with observational data for at least three decades.

What are some of the remaining biases in climate models where additional research and development efforts are needed?

Identifying persistent biases and tracking their reductions are crucial to strengthening the utility of projections from climate and Earth system models.

A variety of biases exhibited by many climate models have been difficult to reduce or completely eliminate despite frequent model evaluation and bias characterization. Many of these have led scientists to perform extensive model tuning exercises or apply bias removal techniques to reduce the impacts of such biases. Examples include both positive and negative regional biases in precipitation, the double ITCZ (intertropical convergence zone), warming biases in the tropical troposphere, and low Arctic Sea ice sensitivity to global warming compared to observations. Identifying such persistent biases and tracking their reductions are crucial to strengthening the utility of projections from climate and Earth system models. Creating a wealth of additional model performance metrics and enhancing collections of observational data sets are required to understand the sources of these long-standing model biases.

—Birgit Hassler (birgit.hassler@dlr.de, 0000-0003-2724-709X), Deutsches Zentrum für Luft- und Raumfahrt (DLR), Germany; Forrest Hoffman (0000-0001-5802-4134), Oak Ridge National Laboratory, United States; Ranjini Swaminathan (0000-0001-5853-2673), University of Reading, United Kingdom; and Beth Dingley (0000-0002-9831-9671), European Space Agency, United Kingdom

Editor’s Note: It is the policy of AGU Publications to invite the authors of articles published in Reviews of Geophysics to write a summary for Eos Editors’ Vox.

Citation: Hassler, B., F. Hoffman, R. Swaminathan, and B. Dingley (2026), Climate model benchmarking: building trust and advancing science, Eos, 107, https://doi.org/10.1029/2026EO265032. Published on 24 August 2026. This article does not represent the opinion of AGU, Eos, or any of its affiliates. It is solely the opinion of the author(s). Text © 2026. The authors. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

Climate scientists solve monsoon puzzle and warn of risks to fisheries

Phys.org: Earth science - Mon, 08/24/2026 - 15:20
A new study has reconciled a long-standing paradox in the South Asian summer monsoon cycle. Climate scientists have discovered why geological records from land and sea have told opposite stories about monsoons throughout history and found that rising temperatures over Southern Africa reduce upwelling in the Arabian Sea, which could damage marine productivity and fisheries. The work is published in the journal Proceedings of the National Academy of Sciences.

Why Marine Heat Waves and Acidification Strike Together

EOS - Mon, 08/24/2026 - 12:12
Source: AGU Advances

Marine heat waves and extreme ocean acidification events are each damaging on their own. But when both stressors hit simultaneously, their individual effects can be exacerbated.

That threat may be best exemplified by “the Blob” of 2013–2015, during which both a marine heat wave and an ocean acidification extreme event hit the northeastern Pacific. Fisheries were closed, marine mammals were stranded, seabirds died, and sea creatures either changed their distribution or perished.

But our understanding of these compound heat-acidity ocean extreme events is limited, with more research focused on the marine heat wave component than on the acidification aspect.

Gregor and Gruber used 43 years of monthly data (1982–2024) on surface ocean temperatures and acidity to determine when, where, and why compound heat-acidity extreme events have occurred. They defined extreme events as those situations when detrended acidity and temperature exceed their 95th percentiles.

Compound ocean heat-acidity events happen more often than would be expected by chance, the authors found. In the low to midlatitudes, they occur roughly 4 times more often than compared to chance, mostly in places with permanent stratification. In these places, heat waves drive waters to be more acidic. The compound events were least common in the eastern equatorial Pacific and around the poles, where deep waters upwell to the surface. When marine heat waves strike in these upwelling regions, a warm lens (top layer of water) prevents the surfacing of the deep acidic waters, leading to unusually low acidity for the region.

A majority (73%) of compound heat-acidity extreme events in the study period were smaller than 500,000 square kilometers (193,000 square miles, roughly the size of Spain) and lasted for about a month. But a few events, like the Blob in 2015, lasted for more than a year, sometimes with long-lasting consequences.

El Niño and La Niña events are important drivers of these compound events, but the events seldom happen at the weather events’ epicenter in the equatorial Pacific. During El Niño, warmer waters create a lens that prevents upwelling, thus reducing the typical acidity of the region. And during La Niña, cold, deep waters with higher acidity upwell, resulting in only an acidification extreme. However, it is in the neighboring regions where the knock-on effect of this warming or acidity causes compound extremes to occur.

The new findings are in line with several key facets of earlier work and offer more insights into temporal patterns and drivers. (AGU Advances, https://doi.org/10.1029/2025AV002112, 2026)

—Rebecca Dzombak, Science Writer

Citation: Dzombak, R. (2026), Why marine heat waves and acidification strike together, Eos, 107, https://doi.org/10.1029/2026EO260269. Published on 24 August 2026. Text © 2026. AGU. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

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