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Laser induced fluorescence of singly ionized atomic iodine: Measurements in the plasma source of an electric propulsion device

Physical Review E (Plasma physics) - Tue, 09/01/2026 - 10:00

Author(s): Romain Pioch, Marie-Alix Sagnimorte, Benjamin Esteves, and Cyril Drag

A laser induced fluorescence (LIF) scheme is investigated to probe singly ionized iodine ions (I+) in electric propulsion devices. The transition 6sS2o5→6pP35 at 516.261 nm is considered and the theoretical computation of the weights and positions of the hyperfine structure is carried out. First, th…


[Phys. Rev. E 114, 035201] Published Tue Sep 01, 2026

The importance of realistic noise characteristics in neural network inversion of airborne electromagnetic data

Geophysical Journal International - Tue, 09/01/2026 - 00:00
SummaryDeep learning methods such as neural networks offer a rapid alternative to geophysical inversion and are increasingly applied to airborne electromagnetic (AEM) data for a range of earth science problems. Such networks rely on both the network architecture as well as suitable training datasets to produce realistic earth resistivity models. Here we develop a Convolutional Neural Network (CNN) to invert AEM data and pay particular attention to the characteristics of the training dataset. As well as covering a realistic range of subsurface property distributions, the training data must emulate the noise and data gap characteristics of the target survey data. We find neural networks trained on noise free data, while performing very well on validation data, perform poorly on real world data, often inducing geologically unrealistic artifacts in the resistivity model. Conversely, training data conditioned with noise and data gap characteristics appropriate for the survey of interest, fit the validation data less well, but produce fewer artifacts when applied to survey data. Choice of loss function metric and data normalisation method is important and may vary between surveys. Despite strong advances in neural network design, developing training data with broad enough characteristics to be generalised across many surveys and data acquisition platforms remains an important challenge.

An Improved CHAOS-Based Correction Model for Storm-Time External Magnetic Fields

Geophysical Journal International - Tue, 09/01/2026 - 00:00
SummaryAccurate separation of the Earth’s internal and external geomagnetic fields requires robust modeling, especially during the geomagnetic storms. Because the comprehensive CHAOS model is primarily designed to represent the Earth’s magnetic field under geomagnetically quiet periods, residuals of satellite observations relative to the CHAOS model during storms exhibit systematic dependencies on magnetic local time (MLT) and the disturbance levels, highlighting limitations in its representation of external field morphology. To address this limitation, we developed an empirical correction for the CHAOS model that specifically targets the magnetic signatures of the residual ring current at low and mid-latitudes. Using the high-quality scalar magnetic data from Swarm A/B and the Macau Science Satellite-1 (MSS-1) at nighttime hours, between November 2023 and September 2025, we modeled the systematic perturbations remaining after CHAOS background removal. Our separable parameterization explicitly resolves MLT structure while incorporating dependencies on geomagnetic disturbance levels. Event analyses demonstrate that our correction model can successfully capture the pronounced dawn-dusk MLT asymmetries of the external field during storms main and recovery phases. Statistically, the empirical model robustly captures residual ring current signals across all evaluated nighttime sectors, yielding the greatest improvements at dusk. Ultimately, the proposed correction effectively mitigates the activity-dependent biases in the CHAOS model’s external field, yielding a more reliable representation for the accurate interpretation of storm-time magnetic residuals.

An anomalous return of the Odden ice tongue suggests unusual Arctic conditions

Phys.org: Earth science - Mon, 08/31/2026 - 17:30
Data from many sources, including NASA, have shown a significant decrease in Arctic sea ice since 1979. However, the processes driving the melting and freezing of sea ice are complex, and fluctuations occur throughout the year. Short-term variations in temperature, winds, ocean convection and water salinity within a certain region can also affect how much ice can reform or melt.

Earlier volcano warnings could mean more false alarms—but they could also save lives

Phys.org: Earth science - Mon, 08/31/2026 - 17:20
Whakaari/White Island's sudden eruption in December 2019, which killed 22 people and severely injured 25 others, was New Zealand's deadliest volcanic disaster in recent history.

Human-driven fires have shaped the Amazonian forest for over 10,000 years

Phys.org: Earth science - Mon, 08/31/2026 - 14:40
New research is dismantling the longstanding myth of the "pristine" Amazon. A reconstruction of 10,000 years of Amazonian pyrogeography, based on 1,361 radiocarbon (¹⁴C) dates across 303 sites—including soil charcoal and burned archaeological material—shows that fire in the rainforest is almost exclusively a human-driven phenomenon, not a natural one.

UK and Ireland face greatest risk from rare tropical cyclones reaching Europe

Phys.org: Earth science - Mon, 08/31/2026 - 14:00
Europe is no stranger to powerful windstorms, but some storms capable of causing serious damage have an unusual origin. Tropical cyclones can occasionally travel north from lower latitudes and reach Europe, where they can bring damaging winds and heavy rain even after losing some of their tropical characteristics.

Communities Affected by Climate Change Need More Than Data

EOS - Mon, 08/31/2026 - 13:07
Source: Community Science

Resources such as sea level rise viewers, heat maps, and flood prediction services are crucial tools in a changing climate. NASA Earth Observations (NASA EO) datasets provide important information on these and other natural hazards, but many communities who may benefit from these tools face barriers to accessing them.

La Margarita, a community along Puerto Rico’s southern coast, faces hazards including flooding, storm exposure, crumbling infrastructure, and inadequate government investment. Residents of this historically underserved community contend with pollution from nearby power plants and an industrial sterilization facility. Hurricane Fiona exposed many of the region’s vulnerabilities in 2022, after 30 inches of rain destroyed homes in low-lying areas and left residents without basic services.

Raub et al. worked with La Margarita residents to learn about their environmental concerns and preferred solutions and to assess ways NASA EO datasets might be able to address those concerns in a three-phase project over 9 months.

In phase 1, one-on-one bilingual interviews with 16 local leaders and residents helped researchers determine participants’ environmental justice concerns as well as familiarity with EO tools and the possible barriers to using them. In phase 2, a NASA representative showed community members how EO tools could be used, such as to show patterns of power outages and to project rates of sea level rise. For phase 3, researchers created a bilingual English-Spanish report to summarize the study participants’ concerns and the available NASA EO resources. La Margarita community members were invited to provide feedback to ensure that the report accurately reflected their needs and concerns.

Key concerns that study participants identified were flooding (56%), land misuse from illegal development (63%), and air quality and accompanying health conditions (50%). Government inaction was participants’ biggest concern (69%). Participants initially had little awareness of the EO tools but felt that flood mapping and air quality monitoring systems would be useful, especially if they were paired with support for how to use the tools. Barriers to EO tools included spotty internet access, unfamiliarity with the technology, previous experiences with unhelpful authorities, and the language barrier.

Study participants did not want solutions imposed on them by outside experts—they wanted collaboration with researchers and agencies who would listen to their concerns and work toward community-led decisionmaking. The study authors suggest that environmental justice means more than providing data: Building trusting relationships between scientists, communities, and agencies like NASA can ensure that important tools reach and are used by the people who need them most, the authors say. (Community Science, https://doi.org/10.1029/2025CSJ000157, 2026)

—Rebecca Owen (@beccapox.bsky.social), Science Writer

Citation: Owen, R. (2026), Communities affected by climate change need more than data, Eos, 107, https://doi.org/10.1029/2026EO260277. Published on 31 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.

Decoding Rocks to Reveal What the Critical Zone Hides

EOS - Mon, 08/31/2026 - 12:00
Editors’ Vox is a blog from AGU’s Publications Department.

As environmental conditions change, it is increasingly important to understand the structure and properties of the Earth’s critical zone, the layer where rock, soil, water, air, and living organisms meet and interact. While several geophysical methods provide images of the subsurface, they do not directly measure rock properties, such as porosity and water saturation.

A new article in Reviews of Geophysics explores rock physics models, which help bridge the gap between these geophysical methods and rock properties. Here, we asked the lead author to give an overview of the critical zone, the different types of rock physics models, and some of the remaining challenges for researchers.

In simple terms, what is the critical zone?

The critical zone is Earth’s thin outer layer that stretches from the tops of the trees down to the base of weathered bedrock.

The critical zone is Earth’s thin outer layer that stretches from the tops of the trees down to the base of weathered bedrock. Within it, physical, chemical, and biological weathering slowly transforms intact rock into a porous material that stores and transmits the water and nutrients ecosystems depend on. It is called “critical” because these near-surface processes sustain life, regulate water supplies, and shape landscapes over long timescales. Indeed, the critical zone controls how much water is available to plants, how groundwater is recharged, and how landscapes evolve over time.

What is the subsurface critical zone comprised of, and why is it important to study?

Below the soil, the subsurface critical zone grades downward from chemically altered and physically weakened rock (called “saprolite”), to fractured and partially weathered bedrock, and finally to fresh bedrock at the base. These layers are not sharply separated; they blend gradually, and their thicknesses vary with rock type, climate, topography, and tectonic history. This complex architecture governs how water infiltrates, how much is stored, and how it moves toward streams and plant roots. It matters because it controls water availability, groundwater recharge, nutrient cycling, and landscape evolution. Since it is hidden from direct view beneath our feet, we rely on indirect methods to map it across entire hillslopes.

Why is rock physics important for understanding the critical zone?

Rock physics supplies the missing bridge: it is the set of quantitative relationships that translate these geophysical signals into meaningful properties.

Geophysical surveys can image the subsurface over large areas, but they can’t measure the properties that critical zone scientists care about, such as porosity or water content. Instead, they record how signals (e.g., seismic waves, electrical currents, radar, or magnetic responses) move through the ground. Rock physics supplies the missing bridge: it is the set of quantitative relationships that translate these geophysical signals into meaningful properties such as porosity, water saturation, and permeability.

Without rock physics, a seismic velocity map is just a picture of how fast waves travel; however, that same picture becomes an estimate of how much water the subsurface can hold when rock physics is applied. This transforms qualitative images into quantitative characterization, letting us test ideas about weathering, water storage, and how the critical zone responds to climate and environmental change.

What are the most common geophysical methods that scientists use to study the critical zone?

Several complementary methods are used in critical zone studies. Seismic refraction and surface-wave techniques measure how fast elastic waves travel, revealing subsurface layering, weathering profiles, and depth to bedrock. Electrical resistivity tomography (ERT) injects current into the ground to map resistivity, which is sensitive to porosity, water content, and the presence of clay. Ground-penetrating radar (GPR) uses radio-frequency waves to produce detailed images of subsurface contrasts in dielectric permittivity due to boundaries in porosity, composition, and water content. Nuclear magnetic resonance (NMR) directly detects hydrogen in water, providing quantitative water content and pore-size information. Because each method senses a different physical property, combining them yields a fuller and less ambiguous picture of water and structure in the critical zone.

An example modeling workflow for characterizing the critical zone using rock physics. Geophysical measurements are first converted through geophysical inversion into maps of seismic velocity, resistivity, and other geophysical properties. Rock physics models then translate those into estimates of porosity and water saturation. Credit: Grana et al. [2026], Figure 1

Why do scientists use rock physics models?

Geophysical images are inherently non-unique: different combinations of porosity, water, mineralogy, and structure can produce the same measured response. Rock physics models resolve this ambiguity by encoding the physical relationships between what we measure and the underlying rock and fluid properties. Some are empirical, derived from laboratory and field observations, while others are physics-based, built from first principles describing how grains, pores, and fluids behave. Combined with mathematical inversion, these models convert geophysical property fields into quantitative estimates of porosity, saturation, and permeability, as well as into estimates of the uncertainty in those values. This is what allows geophysical data to be integrated into hydrological and geochemical models of the critical zone.

What types of rock physics models are explored in your review article?

We review models grouped by the geophysical property they address. Elastic models link seismic velocities to porosity and saturation, using granular-media theories for loose, weathered material, inclusion models for fractured bedrock, and Gassmann’s equations to account for pore fluids. Electrical and electromagnetic models relate resistivity to porosity and water content. Dielectric mixing models connect GPR measurements to water content. NMR models tie relaxation signals to pore size, water content, and permeability. We also discuss soil physics effects, like matric suction, that become important in the shallow, unsaturated near surface where standard rock physics assumptions begin to break down.

Examples of rock physics models: an elastic model estimates P-wave velocity from porosity and water saturation, while an electrical model estimates resistivity from the same properties using Archie’s equation. Credit: Grana et al. [2026], Figure 2 (left panel) and 3

What are some of the remaining challenges where additional research efforts are needed?

Several challenges remain. Weathered materials are far more heterogeneous than the sedimentary rocks most rock physics models were originally built for, so relationships are often site-specific and don’t transfer easily between locations. Calibrating and validating models requires direct measurements from cores or boreholes but this is expensive, coverage is sparse, and the process can alter the properties of the very material being sampled. Additionally, some properties are difficult to constrain from surface data alone. For example, permeability and fracture connectivity are critical for predicting water flow but are notoriously difficult to measure in the field. Relying instead on data from the lab has its own problems: laboratory samples are centimeters wide, while geophysical surveys average over meters. Promising directions include systematic laboratory measurements of critical zone materials, inversion methods that explicitly quantify uncertainty, physics-guided machine learning, and emerging monitoring technologies such as distributed acoustic sensing that can track subsurface changes continuously over time.

—Dario Grana (dgrana@uwyo.edu; 0000-0003-4220-053X), University of Wyoming, United States; Brady A. Flinchum (brady.flinchum@newcastle.edu.au; 0000-0003-0395-0450), University of Newcastle, Australia; Denys Grombacher (denys.grombacher@geo.au.dk; 0000-0003-2447-0085), University of Aarhus, Denmark; Andrew D. Parsekian (aparseki@uwyo.edu; 0000-0001-5072-9818), University of Wyoming, United States; Clifford S. Riebe (criebe@uwyo.edu; 0000-0002-8744-8208), University of Wyoming, United States; and W. Steven Holbrook (wstevenh@vt.edu, 0000-0003-0065-8841), Virginia Tech, United States

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: Grana, D., B. A. Flinchum, D. Grombacher, A. D. Parsekian, C. S. Riebe, and W. S. Holbrook (2026), Decoding rocks to reveal what the critical zone hides, Eos, 107, https://doi.org/10.1029/2026EO265033. Published on 31 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.

3D cross-gradient joint inversion of gravity, magnetic and MT data using a reweighting strategy: application in the Yanggao geothermal field, China

Geophysical Journal International - Mon, 08/31/2026 - 00:00
SummaryGeophysical joint inversion offers a robust approach for integrating diverse geophysical datasets, leveraging their complementary information to mitigate the nonuniqueness inherent in individual data inversion. This approach thereby enhances model consistency and improves subsurface characterization. In this study, we investigate the effectiveness of three-dimensional (3D) joint inversion of gravity, magnetic and magnetotelluric (MT) data for deep geothermal exploration. We first implemented a reweighting optimization strategy for gravity and magnetic data to increase the vertical resolution of jointly inverted models of potential data. Subsequently, we integrated the optimized gravity and magnetic inversion scheme with MT data using a cross-gradient constraint for comprehensive joint inversion. Synthetic experiments validated the effectiveness of our developed reweighting optimization strategy and joint inversion scheme, demonstrating improved structural resolution and model reliability compared to separate inversions. Finally, we applied the methodology to the Yanggao geothermal field in northern Datong Basin, China, to assess its applicability for deep geothermal exploration. The joint inversion approach, offering an advantage over separate inversions, provides enhanced subsurface characterization by more accurately delineating hydrothermal pathways and potential geothermal reservoirs of the geothermal system within the investigated area.

A Semi-Analytical Solution for Topographic Amplification and Broadband Scattering of SH Waves by Step-like Rock Slopes

Geophysical Journal International - Mon, 08/31/2026 - 00:00
SummaryLocal seismic topographic amplification of rock slopes is a primary cause of earthquake-induced damage in mountainous engineering. To resolve the scattering of plane SH waves by individual rock slopes, this study introduces an analytical model derived from the Uniform Theory of Diffraction. Conventional wave function expansion methods (WFEM) often struggle with non-closed free boundary conditions across varying elevations and tend to suffer from series divergence under high-frequency incidence. This approach precisely partitions the slope into two semi-infinite ideal wedge domains sharing a common face, reconstructing the generalized geometric wave field through rigorous global ray tracing. Second-order coupled diffraction terms with a slope-diffraction correction are introduced to describe the two-way interaction between the slope crest and toe, while the UTD transition functions ensure continuity of the wavefield across shadow boundaries. Systematic numerical evaluations in both frequency and time domains reveal a frequency-selective interference mechanism with distinct spatial variability. Under horizontal grazing incidence, energy is strongly focused on the leeward face, while the back-slope forms a high-frequency seismic shadow zone due to intense destructive interference between direct and secondary diffracted waves. At certain oblique incidence angles, repeated scattering of broadband waves between the slope crest and toe leads to strong local resonance in the slope region. Findings indicate that the location of maximum dynamic response shifts sensitively with the incident wavefront inclination. The results show that the maximum amplification does not always occur at the slope crest, highlighting the importance of incidence angle in seismic microzonation and site planning for mountainous areas.

Tides can be mapped much more locally using a new method based on satellite images

Phys.org: Earth science - Sun, 08/30/2026 - 19:00
When high or low tide occurs, the water does not necessarily rise and fall uniformly along the entire coastline. In fact, the height of the tide in a bay can vary by up to one meter (3 feet) from one location to another just a few kilometers away.

As super El Nino strengthens, study suggests that climate change is intensifying El Ninos

Phys.org: Earth science - Sun, 08/30/2026 - 18:00
A new study suggests that El Ninos—the natural climatic chaos agent that pops up periodically and spikes global temperatures—are getting stronger because of human-caused climate change.

Roman Telescope Begins Quest to Reveal Evolving Universe

EOS - Sun, 08/30/2026 - 11:28
body {background-color: #D2D1D5;} Research & Developments is a blog for brief updates that provide context for the flurry of news that impacts science and scientists today.

A new era of space exploration began today with the launch of the Nancy Grace Roman Space Telescope. Roman is poised to solve one of the fundamental mysteries of the universe: what it’s made of.

“There’s something really fundamental that we don’t understand about the nature of our universe itself, and Roman is purpose-built to address and provide the data that we need to address these questions,” Julie McEnery, Roman’s senior project scientist and an astrophysicist at NASA Goddard Space Flight Center in Greenbelt, Md., said in a 27 August interview on NASA’s Curious Universe podcast.

Roman launched from Kennedy Space Center in Florida at 7:26 a.m. local time on 30 August. The telescope is named after NASA’s first chief of astronomy, Dr. Nancy Grace Roman (1925–2018). Roman was also the first woman to be a NASA executive and is widely considered to be the “Mother of the Hubble Space Telescope” for her work to make that pioneering telescope a reality.

A Universe to Discover

Roman is a NASA mission and received instrumentation and science support from the Centre national d’études spatiales in France, the European Space Agency, Japan Aerospace Exploration Agency, and the Max Planck Institute for Astronomy in Germany. The telescope has a field of view 100 times that of the Hubble Space Telescope and is capable of capturing much more detail in a single glimpse.

Roman is expected to probe deep into the early universe and study more than a billion galaxies. In doing so, scientists hope to create 3D maps of the evolving universe.

Nancy Grace Roman stands next to a scale model of the Hubble Space Telescope outside the Hubble control center. Credit: NASA

“One of the motivations for Roman was the discovery that our universe is not just expanding, but that expansion is accelerating,” McEnery said. “That was crazy. It’s like if you were to throw a ball in the air, and instead of the ball coming back down, it just keeps shooting away.”

Cosmologists theorize that around 75% of the universe is composed of a mysterious substance called dark energy that is pushing space-time itself apart. One way of measuring the impact of dark energy, and thereby narrowing down just what dark energy might be, is to track the expansion history of the universe. This can be done by mapping the locations and distances of supernovae across the universe and measuring how quickly they are receding from us.

“We can best do that with something that has a huge view because when you’re measuring the property of a large chunk of the sky, you can be reasonably confident you’re understanding how the universe itself is behaving, rather than the vagaries of a particular small group of galaxies in one particular spot,” McEnery said.

Roman will also add to our knowledge of dark matter, which makes up about 20% of the universe and is mostly understood through its invisible gravitational effects on light as it passes near galaxies.

Scientists expect Roman to discover as many as 200,000 exoplanets in the Milky Way.

On the opposite end of the astrophysical paradigm are exoplanets. Roman is designed to find “an awful lot of them,” McEnery said.

The telescope is equipped with three ways to detect exoplanets: by monitoring starlight for dips as an orbiting planet passes in front (transit method), by watching for spikes in starlight as a foreground planet wanders past (microlensing), and by blocking a star’s light to see the glow from the planet itself (direct imaging).

Astronomers currently know of more than 14,000 confirmed and candidate exoplanets. Through these three methods, scientists expect Roman to discover as many as 200,000 exoplanets in the Milky Way.

What’s more, each detection method is best at detecting different subsets of exoplanets, so Roman can help provide a more complete picture of exoplanet populations, which can help astronomers understand how exoplanets form.

After Launch

The telescope’s primary mission is 5 years, with an expected lifetime of 10 years.

Roman scientists will spend the next three months ensuring Roman reaches its distant orbit and testing the telescope’s systems. The team expects the first science images to be released in early 2027. Those images will likely offer stunning views of familiar places of the sky to demonstrate Roman’s capabilities.

 
Related

But one of the most anticipated early looks will be Roman’s first deep field survey. Like its predecessors from Hubble, Roman’s deep field will reveal millions of distant galaxies hidden within a seemingly blank patch of the sky. Those surveys will look as far back into the early universe as Hubble’s do, but they will be more than 1,500 times larger. McEnery said it would take more than half a million 4K TVs to fully display Roman’s largest survey.

“It’s the equivalent of covering 45 city blocks,” she said. “You can think about Mount Rushmore, but Mount Rushmore is too small. You would need to fully cover El Capitán with 4K TVs to fully display Roman’s largest survey. I don’t think we should do that, but it gives you a sense of how amazing this survey is going to be.”

—Kimberly M. S. Cartier (@astrokimcartier.bsky.social), Staff Writer

These updates are made possible through information from the scientific community. Do you have a story about science or scientists? Send us a tip at eos@agu.org. 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.

Why some earthquakes caused by fracking come with warning signs

Phys.org: Earth science - Fri, 08/28/2026 - 17:10
Fracking, the injection of high-pressure fluid to fracture rock and release oil or gas, can trigger earthquakes. While some sites generate small tremors beforehand that may provide an early warning, others produce few or none.

Nepal's devastating floods reveal the danger of 'cascading hazards' in Himalayas

Phys.org: Earth science - Fri, 08/28/2026 - 14:40
The devastating floods that have swept through the Nepal–Tibet border region are first and foremost a human tragedy. Hundreds of people have died or remain missing. But as scientists begin to reconstruct what happened, the event also exposes something fundamental about the way we understand natural hazards in high mountain regions. Mountains and rivers do not reset after an extreme event.

Engineered bacteria offer a new way to accelerate rock weathering for carbon removal

Phys.org: Earth science - Fri, 08/28/2026 - 14:20
Rock weathering, the breakdown and dissolving of rocks and minerals caused by their exposure to water, air and biological life, is a major regulator of Earth's atmospheric CO2 levels and climate. Throughout Earth's history, rock weathering has been faster during warm periods with increased atmospheric CO2 levels.

Prioritizing Quality Before Synthesis in Paleoenvironmental Hazard Science

EOS - Fri, 08/28/2026 - 12:00

In May 1992, a group of scientists gathered at the edge of Marble Canyon in northern Arizona, where the Colorado River has cut into Permian sandstone to form cliffs that rise hundreds of feet above the water. The occasion was the First International Workshop on Paleoflood Hydrology, organized by Vic Baker of the University of Arizona. For Baker and his colleagues, the canyon walls were not just scenery. They were a kind of archive.

Here, sediment deposits mark the high-water lines of floods that surged through the canyon centuries before any stream gauges were there to measure them. In particular, Baker and his colleagues studied slackwater deposits, fine-grained sediments emplaced by floodwaters in sheltered alcoves and tributary mouths.

Over the course of decades, Baker, together with collaborators and students, developed methods to read the Marble Canyon deposits. Researchers used hydraulic models to back-calculate past flood discharge and used radiocarbon dates to pinpoint when floods occurred. Their analyses revealed floods that were nearly twice the size of those captured by the instrumental record and that recurred far more frequently than engineers had assumed [Greenbaum et al., 2014].

Baker and his collaborators also mapped out statistical frameworks to translate their data into flood frequency estimates that present-day engineers and water managers could use.

The U.S. Bureau of Reclamation put those data to use, incorporating the long flood history written on the canyon walls into formal hazard assessments for dam safety and infrastructure design on the Colorado River. The logic was straightforward: The biggest, most destructive floods are also the rarest, which means they are routinely missing from the short instrumental records engineers rely on, leading to dangerous underestimates of risk.

Expanding the Field in Breadth and Depth

In the decades since Baker helped establish paleoflood hydrology as a discipline, the field has expanded to encompass a much wider range of settings and methods, including boulder berms in mountain rivers, alluvial fills in lowland valleys, tree ring “flood rings” in riparian (riverbank) forests, detrital layers on stalagmites in caves, and historical archives stretching back centuries in regions with long written records, to name just a few.

The study of riverine flooding represents just one of several fields that use geological records to improve hazard assessments.

A landmark synthesis by Wilhelm et al. [2019] documented this methodological diversity across flood settings worldwide. Each approach requires its own deep disciplinary expertise and preserves different aspects of flood history. The approaches vary considerably in the precision and accuracy of the estimates they produce, and not all have matured to the point where their outputs can be directly incorporated into formal hazard assessments in the way Baker’s analyses of slackwater deposits were.

Moreover, the study of riverine flooding represents just one of several fields that use geological records to improve hazard assessments. Want to reconstruct the history of tropical cyclones and coastal storms? Paleotempestology uses sediment cores from coastal ponds and sinkholes, and isotopic signatures preserved in tree rings, to do just that. Need to understand how often a fault experiences a major earthquake? Paleoseismology reads fault scarps, liquefaction features, disturbed stratigraphy, and tsunami deposits to find out.

Each of these fields has its own methods, its own archives, its own hard-won expertise—its own Vic Bakers. And each faces the same fundamental challenge: translating qualitative or semiquantitative evidence of past events into the precise, uncertainty-bounded estimates that planners, engineers, and risk managers can use.

A Proposed Center for Paleoenvironmental Records of Extreme Events

A new report from the National Academies of Sciences, Engineering, and Medicine (NASEM) [2026] (“A Synthesis Center for Paleoenvironmental Records of Extreme Events”) represents a welcome and timely recognition that these fields have something important to offer. Despite decades of progress, the report finds, these long-term records of extreme events remain underused by the agencies, industries, and communities that manage risk.

The report proposes a new center with a mandate to “focus on the integration, synthesis, and translation of paleoenvironmental data.” The report envisions this work carried out through mission-oriented working groups spanning academia, government, and industry. This is a laudable structure, given how disconnected these communities’ incentives and timelines often are.

But this framing raises a fundamental question: Is the primary barrier to translation really a lack of synthesis? Or is it that most of these records have not yet reached the standard that made Baker’s analysis of slackwater deposits useful to the Bureau of Reclamation?

The answer, I would argue, is that the quality of the records themselves represents a fundamental barrier to bridging the translational gap. The report recognizes this, at least implicitly, by distinguishing “Tier 1” records (those that provide quantitative, precise estimates of past hazard magnitudes directly comparable to instrumental data) from lower-quality records. It also acknowledges that such records are rare.

Across most settings and hazard types, the majority of existing records of paleoenvironmental hazards fall short of the Tier 1 standard.

Across most settings and hazard types, the majority of existing records of paleoenvironmental hazards fall short of the Tier 1 standard. This matters enormously, as incorporating paleoflood estimates with large errors into flood frequency analysis increases uncertainties rather than reducing them [Reinders and Muñoz, 2021].

Records need to meet a quality threshold—roughly 20% error or less—to help rather than hurt. Synthesizing records that fall below that threshold widens the translational gap instead of closing it.

In addition to quality, these records face a second challenge that resists synthesis: They are, by their very nature, site-specific. What gets recorded at a given site depends on factors that can vary enormously over short distances—the geometry of a canyon, the height and orientation of a beach barrier, the elevation of a tree in a floodplain.

Two nearby sites on the same river can preserve fundamentally different flood histories, not because the floods were different, but because local geomorphic conditions controlled what was recorded and preserved. This site specificity is simply how these archives work.

Site specificity means that such records resist the kind of broad synthesis that works well for more standardized data types. Aggregating them in a database does not produce a clean regional picture of hazard frequency and magnitude. Rather, it produces a collection of site-specific stories that require deep disciplinary expertise to interpret, compare, and contextualize.

A Path Forward: Investing in Methods and People

There are promising methodological pathways to elevate records toward a quality that practitioners can use. My lab, which focuses on hydrologic extremes across a range of settings and timescales, has worked on integrating paleoenvironmental records with physical model simulations. Such simulations enable researchers to move beyond qualitative or semiquantitative evidence and toward precise, uncertainty-bounded estimates of hazard magnitude. Other frontiers exist across geochronology, proxy development, and statistical frameworks.

In paleoflood hydrology, hydraulic models can simulate the water levels, velocities, and depositional conditions associated with floods. This ability links sediment properties directly to flood magnitude and reduces uncertainties in paleoflood estimates [Reinders et al., 2023].

The number of labs actively producing high-quality paleoenvironmental records of extreme events, and advancing the methodologies to improve them, remains small.

In paleotempestology, overwash deposits in coastal ponds record when hurricanes occurred, but not their tracks or magnitudes. Coastal hydrodynamic and morphodynamic models offer a promising path to fill that gap, back-calculating storm surge magnitudes from the sedimentary deposits that storms leave behind. Site-specific factors such as sea level change and barrier morphology present real challenges, but the approach shows promise and warrants sustained investment.

Developing these methods requires a strong professional cohort. Here, the field faces a compounding challenge. The number of labs actively producing high-quality paleoenvironmental records of extreme events, and advancing the methodologies to improve them, remains small. This means there are few graduate students and postdoctoral researchers trained in these approaches, few experienced reviewers for papers and proposals, and a limited capacity to evaluate whether new work is actually meeting the quality threshold that translation of paleoenvironmental data requires.

The NASEM report itself names education and training as a core function of the proposed center, envisioning opportunities for postdoctoral researchers, students, and visiting scholars. Training researchers who understand both the science and the needs of practitioners—those who speak the languages of both sedimentology and flood frequency analysis, for example, or stratigraphy and storm surge modeling—is exactly what government agencies and industry partners need, and exactly what would make a center so valuable.

A Center Worth Building

A center dedicated to paleoenvironmental records of extreme events is an idea worth pursuing. Its design, however, will determine whether it actually closes the translational gap it aims to address.

What such a center could accomplish would differ fundamentally from what any single lab can. One group can advance one method for one hazard type, but a center could convene parallel working groups across hazard types, drawing together expertise currently dispersed across a small number of labs and sustaining training pipelines beyond the durations of individual grants. The National Center for Ecological Analysis and Synthesis and the National Socio-Environmental Synthesis Center are both National Science Foundation–funded synthesis centers built on a convening structure. They offer templates for how such a center might be organized and hosted.

I recommend that such a center explicitly prioritize methods development and workforce training alongside synthesis and translation.

I recommend that such a center explicitly prioritize methods development and workforce training alongside synthesis and translation.

This means funding graduate and postdoctoral fellowships and sabbatical residencies that convene early-career scientists, established researchers, and practitioners. Working together, these groups can develop approaches to elevate records toward more effective translation across disciplines and professions.

It means establishing working groups organized around specific hazard types and methodological approaches, each charged with developing and disseminating best practices and evaluating what it takes to produce records that practitioners can use.

And it means recognizing that these same sectors have a direct stake in this investment. Such partners include the Federal Emergency Management Agency, the U.S. Army Corps of Engineers, and the insurance and catastrophe risk industries. These sectors need researchers trained to speak the languages of both science and industry, and cofunding a center that produces them would serve the interests of both communities.

The scientists who gathered at Marble Canyon in 1992 had spent decades building the foundation that made their work useful. The proposed center offers an opportunity to accelerate that process across a much wider set of hazards and settings, but only if it invests in the foundation first.

References

Greenbaum, N., et al. (2014), A 2000 year natural record of magnitudes and frequencies for the largest Upper Colorado River floods near Moab, Utah, Water Resour. Res., 50(6), 5,249–5,269, https://doi.org/10.1002/2013WR014835.

National Academies of Sciences, Engineering, and Medicine (NASEM) (2026), A Synthesis Center for Paleoenvironmental Records of Extreme Events, 132 pp., Natl. Acad. Press, Washington, D.C., https://doi.org/10.17226/29290.

Reinders, J. B., and S. E. Muñoz (2021), Improvements to flood frequency analysis on alluvial rivers using paleoflood data, Water Resour. Res., 57(4), e2020WR028631, https://doi.org/10.1029/2020WR028631.

Reinders, J. B., et al. (2023), A hydraulic modelling approach to study flood sediment deposition in floodplain lakes, Earth Surf. Processes Landforms, 48(4), 756–769, https://doi.org/10.1002/esp.5515.

Wilhelm, B., et al. (2019), Interpreting historical, botanical, and geological evidence to aid preparations for future floods, WIREs Water, 6(1), e1318, https://doi.org/10.1002/wat2.1318.

Author Information

Samuel E. Muñoz (s.munoz@northeastern.edu), Department of Marine and Environmental Sciences, Northeastern University, Nahant, Mass.; and Department of Civil and Environmental Engineering, Northeastern University, Boston

Citation: Muñoz, S. E. (2026), Prioritizing quality before synthesis in paleoenvironmental hazard science, Eos, 107, https://doi.org/10.1029/2026EO260275. Published on [DAY MONTH] 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
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