EOS

Syndicate content Eos
Science News by AGU
Updated: 2 days 9 hours ago

Climate Extremes May Be Reshaping Monkeys’ Social Structures

Thu, 06/18/2026 - 13:18
The Lomas Barbudal Monkey Project takes place in the tropical dry forest of Costa Rica, where Susan Perry and colleagues study 12 different groups of capuchin monkeys. Credit: Keith Hayward

“Even capuchins have their limits. And we need to start paying attention.”

Plants, insects, and larger animals, like the forest’s white-faced capuchin monkeys, are well adapted to these changes. But in 2015, during an abnormally severe drought influenced by the El Niño–Southern Oscillation (ENSO), Perry, an evolutionary anthropologist at the University of California, Los Angeles, observed behaviors that once seemed impossible.

Under normal conditions “The [capuchin] mothers are quite devoted,” she explained. “Now, I was seeing babies crying on the ground piteously. And the mothers just looking down like ‘Too much trouble’ and walking off, abandoning their infants.”

“Even capuchins have their limits,” Perry said. “And we need to start paying attention because all the weather predictions are saying that we’re going to get more unpredictability and more climate extremes.”

Monkeying Around

Odd Jacobson, a behavioral ecologist at the Max Planck Institute of Animal Behavior, was a student at Lomas Barbudal in 2016, a year after this severe drought. His focus was on understanding how the study site’s 12 different capuchin groups were moving through the forest. But now he’s set out to investigate how else climate extremes may affect the behaviors and social structures of these monkeys.

In a paper published in Nature Ecology and Evolution, Jacobson and his coauthors—including Perry—analyzed how climate variability correlated to the 33 years of geolocation data they had on the capuchins.

Their first step was understanding how the size of each group was affecting the relationships between monkeys within the same group. To do this, they observed variables such as daily fruit intake, the size of the group’s home range, and the distance the group traveled each day to find food.

A capuchin monkey holding its baby enjoys some fruit at the Lomas Barbudal site in Costa Rica. Capuchins are omnivores, but they mainly eat fruit. Credit: Keith Hayward

Finally, to understand how monkey groups interacted, they used a “hierarchical social relations model,” which allowed the scientists to predict how two different monkey groups would move through the forest and where their territories would overlap.

The team repeated this process, two monkey groups at a time, until they analyzed the interactions between all 12 monkey groups at Lomas Barbudal. Then, they added the climate-over-time layer to predict how the home range overlap and encounter rates (meaning moments where capuchins from two different groups engaged, often violently) would change with the seasons.

Strength (and Weakness) in Numbers

Generally, large monkey groups have advantages and disadvantages in the forest. One key advantage is the ability to control resource-rich areas, such as land with fruiting trees known as food patches. A key disadvantage is increased intragroup competition for food, meaning the daily fruit intake of individual monkeys was lower.

The researchers found that during climatic extremes, such as extremely wet or dry seasons, this intragroup competition intensifies, making the group less efficient at foraging overall. Behavior between groups changed with the climate as well. For example, in a typical dry season, large groups often overpower smaller ones to take over areas with more available fruit, such as along rivers.

But the new research found that this long-understood idea doesn’t always hold true: During extreme climate events, like a dry season made even drier by the effects of El Niño, capuchins didn’t try to hoard the higher-quality areas.

“We don’t really know exactly why,” Jacobson said. “Maybe there’s not as much heterogeneity in the landscape during these resource poor times, and so there’s not much that larger groups can monopolize.”

Climate extremes, the research suggests, may be upsetting the balance that determines the optimal size of monkey groups. And, as a warming atmosphere makes climate extremes like El Niño or La Niña more intense, it’s growing increasingly important to understand how these changes will affect animal societies.

Filippo Aureli, an ethologist at the Universidad Veracruzana, in Mexico, was not involved with this study, but he has studied the effects of extreme weather events on spider monkeys in Mexico. He also registered the infant mortality rates of capuchin and spider monkeys in the Costa Rican dry tropical forest during that 2015 drought. Capuchin populations experienced high infant mortality during the extreme event, while spider monkey populations tended to stop reproducing.

“With climate change, [climate extremes] are going to be more frequent and intense,” Aureli said. “And we don’t know what’s going to happen. For this period [so far], they’ve held on very well, the spider monkeys, but we don’t know for how much longer.”

Two monkeys from the same group get into a small altercation over a piece of fruit, an example of in-group competition. Credit: Keith Hayward

Perry agreed, noting “the importance of having a baseline when you’re trying to study rare events like El Niño droughts.”

“We know what normal is,” she explained. “If you just try to drop in right now in all the chaos that we’re starting to feel around the planet, then you really can’t study it.”

—Roberto González (@perrobertogg.bsky.social), Science Writer

Citation: González, R. (2026), Climate extremes may be reshaping monkeys’ social structures, Eos, 107, https://doi.org/10.1029/2026EO260198. Published on 18 June 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 Speedy Particles That Could Help Us Learn More About Uranus

Thu, 06/18/2026 - 13:15
Source: Journal of Geophysical Research: Space Physics

Sending a spacecraft to the underexplored planet Uranus is at the top of many planetary scientists’ wish lists. But which spacecraft-mounted instruments would be the most useful for answering questions about the mysterious ice giant?

Several missions to other parts of the solar system have included an instrument that detects energetic neutral atoms (ENAs) zipping through space. An ENA is created when a fast-moving, positively charged ion collides with a neutral particle and “steals” an electron. The now-neutral atom maintains its high energy, and because it is no longer charged, it escapes any influence of a magnetic field and flies onward in a straight line—perhaps right into a spacecraft-mounted ENA detector.

By measuring the numbers, directions, and energies of ENAs produced in a magnetic system, scientists can create three-dimensional images that illuminate the structure and dynamics of that system. ENA imaging previously deepened understanding of the space environments surrounding Earth, Mars, Saturn, and the Sun and highlighted interaction mechanisms occurring at the edge of our solar system.

However, whether ENA imaging would be useful in future exploration of Uranus has been unclear. New simulations by Santos-Costa and André suggest that ENAs are, indeed, likely detectable at Uranus and that studying the ice giant with ENA imaging could return valuable insights into its complex magnetosphere.

The simulations incorporate realistic parameters drawn from what scientists already know about Uranus, such as its strangely offset magnetic field, clouds of neutral particles surrounding its icy moons and the planet itself, and the presence of protons trapped in the planet’s magnetic field. The researchers used the simulations to explore what scientists might have seen if an ENA detector similar to that mounted on the Saturn probe Cassini had been on board the spacecraft Voyager 2 during its brief flyby of Uranus in 1986.

On the left, Uranus is seen by Voyager 2’s analog cameras during the 1986 flyby, when the spacecraft was a few dozen planetary radii from Uranus. The composite image on the right illustrates the hypothetical observation of Uranus’s magnetosphere from an energetic neutral atom perspective based on one of the case scenarios of charged and neutral particle distributions around Uranus discussed by the authors. The Z and M axes indicate the orientation of the planetary and magnetospheric systems, respectively. Credit: Left: NASA/University of Arizona/Erich Karkoschka; right: SwRI/Daniel Santos-Costa

The results point to the strong probability that a “Voyager 2 ENA detector” would have observed ENAs created by collisions between protons and neutral particles that escape the atmosphere and populate a vast region of space—aiding understanding of Uranus’s magnetospheric system. Because the distribution of protons within Uranus’s magnetosphere is poorly understood, the researchers ran the simulations with a few different distribution scenarios. Even in their worst-case scenario, ENAs remained detectable.

ENAs could also result from collisions between protons and neutral particles surrounding Uranus’s moons, rather than the neutral environment originating from the planet itself, but the simulations did not conclusively show whether a Cassini-like detector might capture them.

The researchers conclude that their simulations make a compelling case for including ENA imaging in future exploration of Uranus. (Journal of Geophysical Research: Space Physics, https://doi.org/10.1029/2026JA035080, 2026)

—Sarah Stanley, Science Writer

Citation: Stanley, S. (2026), The speedy particles that could help us learn more about Uranus, Eos, 107, https://doi.org/10.1029/2026EO260196. Published on 18 June 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.

Where Methane is Emitted Matters for Global Burden

Thu, 06/18/2026 - 12:00
Editors’ Highlights are summaries of recent papers by AGU’s journal editors. Source: Journal of Geophysical Research: Atmospheres

Methane is the second largest radiative forcing on climate after carbon dioxide with an atmospheric lifetime of about 9 years. The emissions of methane arise from a variety of sources, including wetlands, fires, agriculture, and industry. Most climate simulations set fixed concentrations of methane that vary by latitude (see top row of figure above), and do not explicitly account for variable emissions.

In contrast, Feng et al. [2026] perform novel simulations that: (1) account for emissions, chemistry, and transport leading to regional differences (bottom row of figure), and (2) track individual source regions to their global contributions. The authors find that emissions from Europe are initially up to 30% more effective at increasing surface concentrations than the global average. In other words, reducing a gram of methane in Europe is more effective at lowering global concentrations than a gram in North America or Asia. This is because Europe is situated at higher latitudes, and whose emissions tend to transport towards polar regions where atmospheric chemistry is slower and methane lives longer. Along with magnitude, the location of emissions also matters for understanding the global burden of methane.

Citation: Feng, C., Xu, Y., Mirrezaei, M. A., Buechler, R., & Gaubert, B. (2026). Distinct efficacy of regional methane emissions in affecting global and regional concentrations: An emission-driven CESM2 modeling study with methane tags. Journal of Geophysical Research: Atmospheres, 131, e2025JD045301. https://doi.org/10.1029/2025JD045301

—Brian McDonald, Associate Editor, Journal of Geophysical Research: Atmospheres

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.

What Tires Leave Behind Can Become Toxic Fish Food

Wed, 06/17/2026 - 13:05

With every work commute or grocery store run, a car’s tires wear down, causing tiny fragments of rubber to break away from the tire surface. That microscopic debris can be washed into streams, waterways, and estuaries when it rains.

“Driving a car or even riding in a bus is a bit like dragging an eraser across the planet, except the crumbs are microplastics. Toxic microplastics.”

“Driving a car or even riding in a bus is a bit like dragging an eraser across the planet, except the crumbs are microplastics. Toxic microplastics,” said Britta Baechler, director of ocean plastics research at the Ocean Conservancy.

Products like packaging materials and microbeads might come to mind long before tires when thinking of microplastics. But rubber hitting the road is actually a major contributor of marine plastic pollution, with some studies showing tire wear particles account for nearly half of the microplastics in terrestrial and aquatic systems. And tire fragments have only recently been classified as nano- and microplastic particles in various environmental studies, meaning the presence of these toxic, tiny particles has likely been underreported.

Tires contain a blend of natural and synthetic rubber as well as other chemicals, additives, and metals. As a tire breaks down and enters the environment, small slivers can make their way into the diets of fish and other marine life. Many studies tend to focus on particles or chemicals from unused tires rather than actual road-worn tire debris.

To better understand how tire particles affect aquatic ecosystems, researchers exposed a pair of estuarine species to a mixture of both weathered and pristine tire particles. By assessing how the study’s fish and shrimp consumed the tire particles and how both particles and the chemicals they release into the water affected the species’ growth and behavior, researchers aimed to capture the ecological risks of tire pollution under more realistic conditions. They published their findings in Environmental Pollution.

A Taste for Tires

In the environment, the tire particles that creatures interact with naturally vary in size. The smallest are often emitted directly into the air right as they’re generated. “You’re going to see higher [tire particle] contamination along roadsides, for example, and not just in waterways,” said Susanne Brander, an ecotoxicologist and courtesy faculty at Oregon State University and one of the study authors.

“These tire particles are small, they’re able to move, some are airborne, some are waterborne, and that’s how they become so pervasive.”

Rain washes those particles off road surfaces and into storm drains, which may lead to freshwater sources. “That’s where the cycle begins. These tire particles are small, they’re able to move, some are airborne, some are waterborne, and that’s how they become so pervasive,” said Baechler, who was not part of the study.

Tires are constructed with complex materials and contain thousands of potential toxins. 6PPD is one such ingredient. It is used to keep rubber from cracking but can be extremely toxic to salmon even in small concentrations.

Researchers used a standard mix of tire types that might be found driving along U.S. roads—14% from light trucks, 41% from passenger cars, and 45% from trucks and buses. They weathered the tire particles by suspending them in water with organic matter and then mechanically processing them with glass beads, shaking, and autoclaving. This broke them down into microparticles between 1 and 20 micrometers in diameter and nanoparticles less than 1 micrometer in diameter. Another portion of the samples was processed even further to isolate the chemical compounds released from the tire particles, representing the leachate.

Researchers exposed inland silverside fish (Menidia beryllina) and mysid shrimp (Americamysis bahia) in their early life stages to a range of tire particles and leachate concentrations to mimic varying levels of environmental contamination.

“We observed significantly higher ingestion rates in both species when they were exposed to weathered tire particles” compared to pristine particles, said lead author Clarissa Raguso, a marine scientist and postdoctoral fellow at Portland State University.

Britta Baechler, director of ocean plastics research at the Ocean Conservancy, collects tire particles from a road in Portland, Ore. Credit: Britta Baechler

Though neither fish nor shrimp experienced significant mortality, weathered tire particles reduced growth in both species, and it took lower amounts of tire particles for shrimp to be affected. The shrimp also ingested more tire particles overall, likely because of their bottom-feeding style.

“I was surprised by the species-specific responses,” Raguso said. “We expected weathered tire particles to consistently have the strongest effects across both species and all end points.”

Tire particles affected the behavior of both species, though the fish were more affected by pristine particles and shrimp were more affected by weathered ones.

“While we did see stronger effects on growth and ingestion in both species, the increase in behavioral alterations associated with weathering was only observed in [mysid shrimp], suggesting that vulnerability to tire pollution varies by species,” said Raguso.

Behavioral effects related to stress altered the animals’ neurological function—some exposures caused hyperactivity and reduced stress responses, whereas others led to decreased activity. In the wild, these behavioral shifts could make the creatures easier targets for predators or disrupt breeding and feeding. This change could lead to a cascade of effects on the food web.

“Mysid shrimp are a really important food item for critical species,” Brander said. “Gray whales, for example, eat millions of those types of organisms per day. The larger fish that we catch as seafood eat mysids. Even though we’re looking at these small larval fish and shrimp that humans don’t eat, they’re a pathway to get to what we do eat.”

Taming Tire Pollution

Though tires are a leading source of microplastic pollution, potential solutions to ensure that fewer particles end up in waterways are in the works. One possibility is to change tires’ chemical composition so they shed fewer harmful microparticles while in use. Other research is being conducted at Portland State University installing traps to catch tire particles in stormwater runoff before they enter marine environments. Another project aims to attach devices to vehicles that capture tire dust before it even hits the road.

“This study is important because it moves microplastics research closer to real-world conditions, the kind of particles that organisms are actually exposed to in nature,” Baechler said. “And understanding how those particles behave after weathering is really critical for assessing ecological risk and informing future prevention and mitigation strategies.”

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

Citation: Owen, R. (2026), What tires leave behind can become toxic fish food, Eos, 107, https://doi.org/10.1029/2026EO260197. Published on 17 June 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.

A Snapshot of Continental Crust in the Making

Wed, 06/17/2026 - 12:00
Editors’ Highlights are summaries of recent papers by AGU’s journal editors. Source: Journal of Geophysical Research: Solid Earth

The formation of continental crust is a major unresolved question in Earth science. Volcanic arcs, such as the Aleutian Islands of Alaska, are thought to be an important source of new continental crust, but modern arc crust is usually more iron- and magnesium-rich than average continental crust. There are few places on Earth where scientists can directly observe the possible transition from mafic arc crust to more silica-rich, continent-like crust while an arc is still active. The Andreanof segment of the Aleutian Arc offers a rare opportunity to study this process because it is an active, relatively intact oceanic arc, without major disruption from back-arc spreading, and it contains several volcanic centers that may record different stages or styles of crustal evolution.

Mark et al. [2026] use seismic waves to image the crust beneath this arc segment. Their results show that this arc crust is still distinct from average continental crust, suggesting that additional chemical or physical changes are needed before arc crust becomes more continent-like. At the same time, localized zones of slower seismic velocity beneath the Atka and Tanaga volcanoes may indicate hotter and/or more silica-rich material in the lower crust. These findings provide an important in-place snapshot of early continental crust formation, while highlighting that the transformation from volcanic arc to continent is complex and still incomplete.

Citation: Mark, H. F., Lizarralde, D., Shillington, D. J., Cortés-Rivas, V., & Behn, M. D. (2026). Along-strike seismic structure of the Andreanof Aleutian Arc segment and implications for the formation of continental crust. Journal of Geophysical Research: Solid Earth, 131, e2025JB033339. https://doi.org/10.1029/2025JB033339

—Lindsay L. Worthington, Associate Editor, JGR: Solid Earth

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.

Soil Biogeochemistry Models Omit Key Processes Due to Geographic Bias

Tue, 06/16/2026 - 17:27
Editors’ Highlights are summaries of recent papers by AGU’s journal editors. Source: Journal of Geophysical Research: Biogeosciences

The landscape takes up carbon (C) from the atmosphere and stores it in soils, mitigating atmospheric greenhouse gas concentrations and the impacts of climate change. Soil biogeochemistry models are the most widely used tools for predicting soil organic carbon (SOC) stocks, particularly in understudied regions that lack comprehensive observations. However, these models were developed based on the dominant processes controlling SOC in North Temperate systems and informed by their data.

von Fromm et al. [2026] test model “transferability” (i.e., the ability to apply the model across sites or regions) to Sub-Saharan Africa, evaluating how three commonly used soil biogeochemistry models predict SOC compare to observations. The authors find that the three models perform poorly even when parameterized with local observations, suggesting that model structure is missing important processes. Upon further evaluation, the authors attribute poor model performance to an overemphasis on net primary productivity and inadequate representation of organo-mineral interactions and exchangeable calcium as controls on SOC.

While this paper’s subject is Sub-Saharan Africa, it begs the question of model transferability to other under-studied regions, either due to lack of observational data or explicit model evaluation such as is presented in this paper. Soil organic carbon sequestration is thought to be one of the largest stocks of stored carbon in the biosphere, so quantifying current soil elemental budgets and predicting future changes requires models to perform well.

Citation: von Fromm, S. F., Rocci, K. S., Anuo, C. O., Asabere, S. B., Kanyiri, J., Kengdo, S. K., et al. (2026). Evaluating soil carbon models for sub-Saharan Africa: Revealing knowledge gaps in subtropical and tropical soil biogeochemistry. Journal of Geophysical Research: Biogeosciences, 131, e2026JG009726. https://doi.org/10.1029/2026JG009726

—Ceara Talbot, Associate Editor, JGR: Biogeosciences

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.

A Hot Jupiter’s Cloudy Mornings and Clear Evenings Provide Clues to Its Chemistry

Tue, 06/16/2026 - 12:47

Clear skies are important for astronomers—not just here on Earth but also on the alien planets they are looking at.

For the past 20 years, scientists studying exoplanets have been literally blinded by fog. Many “hot Jupiters” (massive gas giants orbiting extremely close to their host stars) are constantly wrapped in clouds. This overcast condition acts like a fogged-up window, blocking telescopes from getting a clear reading of the planets’ true composition.

Astronomers using the James Webb Space Telescope (JWST) have now lifted the fog veil by using a novel observation technique published in Science. The technique was used to analyze data from WASP-94A b, an exoplanet nearly 700 light-years away discovered about a decade ago. The scientists were able to detect and account for atmospheric clouds on WASP-94A b by analyzing the planet’s sunrise and sunset zones separately as it crossed in front of its host star.

“It’s almost like we were able to part the clouds and figure out what’s going on three-dimensionally with this planet.”

“It’s almost like we were able to part the clouds and figure out what’s going on three-dimensionally with this planet,” said study coauthor David Sing, a planetary scientist at Johns Hopkins University.

WASP-94A b is so close to the star that it is tidally locked, meaning its rotation has stopped and the same side always faces the star. This creates extreme temperature variations across the planet. While the dayside reaches torrid temperatures well above 1,600 K, the night hemisphere is about 450 K colder. These milder conditions on the dark side allow clouds made of magnesium silicate, a common mineral found in Earth’s rocks, to condense.

This extreme thermal variation drives powerful winds that circulate air throughout the atmosphere, carrying cloud-filled colder air from the nightside over to the dayside. The clouds don’t last long, though. Like morning fog dissipating in the Sun’s warmth, the silicate clouds of WASP-94A b evaporate shortly after they hit the scorching dayside. Because the planet’s weather patterns are locked in place by its synchronized rotation, the morning edge of the planet, where the winds move from nightside to dayside (what we view as the leading edge of the transit from Earth), is permanently overcast, while the evenings (the trailing edge) remain always clear.

Timing Is Everything

The key to this observation was not so much where to look, but when. From our vantage point, WASP-94A b crosses right in front of its star, allowing the researchers to capture the precise moments when the giant planet begins its transit and when it finally moves beyond the edge of the star. As starlight filtered through WASP-94A b’s atmosphere, astronomers separately measured its leading and trailing edges (also known as terminators, or limbs) at the times when the planet began and concluded its transit. By analyzing how the spectral signatures changed between these two phases, they were able to reveal the differences between the morning and evening hemispheres.

These measurements require extreme precision. “As the planet is going in front of the star, you have to measure it in that very short time where only part of the planet is blocking the star,” Sing said. “In only about 10 minutes, you have to get the spectra of a planet, which is really hard because planets are faint and the signals are small. We really needed JWST, the largest telescope in space, to be able to make that measurement that quickly.”

What unfolded was a totally unprecedented view of an exoplanet. “What we found was really surprising,” Sing said. “All of the clouds were basically piled up on the morning terminator, while the evening terminator, which is hotter, was clear.”

The team also realized that the clouds were floating much higher up than anyone anticipated—way above the stratosphere—and were made of surprisingly large particles. This suggests the atmosphere undergoes far more violent, turbulent mixing than previously predicted.

“It’s pretty clear they are magnesium silicate clouds,” Sing said. While scientists expected that this material would form clouds on these planets, “we haven’t really been able to show that before.”

“The study is a great example of how we can measure and understand the multidimensional and complex nature of exoplanet atmospheres,” said Hannah Wakeford, an astrophysicist at the University of Bristol in the United Kingdom who was not involved with the study. “Clouds are the most important part of a planetary atmosphere, and they play a major role in the amount of energy coming into and leaving the planet.”

A Different Composition

Breaking through the cloud barrier allowed researchers to see the true chemical makeup of this world. Previous observations of exoplanet atmospheres using the Hubble Space Telescope had to rely on an “average spectrum,” blending the composition of both sides of a planet on a single profile, mostly because Hubble can’t get a planet’s spectra as quickly and precisely as JWST does. As a result, researchers were getting wrong readings of essential components, such as the amounts of oxygen, carbon, and other heavy elements.

“That kind of rewrites much of what we’ve been learning with Hubble over the last few decades.”

These average spectrum readings meant that models were predicting that WASP-94A b had a heavy metal abundance up to 100 times greater than our Sun. By separating the limbs, the new observations have revealed that this number is actually closer to 10. “That kind of rewrites much of what we’ve been learning with Hubble over the last few decades,” Sing said.

Sing and his colleagues think the same findings could apply to countless other hot Jupiters. In fact, there’s nothing special about WASP-94A b, except that it has the right geometry. “Not all hot Jupiters will be good candidates to reveal this limb asymmetry,” Sing said. “For instance, if a planet just grazes across the bottom of the star during transit, you won’t be able to cleanly separate the two sides out.”

Getting a better handle on what hot Jupiters are made of is a significant step for planetary science and could also help refine atmospheric circulation models on Earth and beyond, Sing said.

Apart from WASP-94A b, the team applied the same method to eight other hot gas giants, discovering hints of similar cloud cycles in two of them: WASP-39 b and WASP-17 b. The team plans to continue studying similar planets with JWST, including a gas planet in the habitable zone of its host star.

—Javier Barbuzano (@javibar.bsky.social), Science Writer

Citation: Barbuzano, J. (2026), A hot Jupiter’s cloudy mornings and clear evenings provide clues to its chemistry, Eos, 107, https://doi.org/10.1029/2026EO260195. Published on 16 June 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.

冷斑与印度季风之间的惊人关联

Tue, 06/16/2026 - 12:44
Source: AGU Advances

This is an authorized translation of an Eos article. 本文是Eos文章的授权翻译。

过去25年间,印度季风发生了变化。印度西北部地区的降雨量比以往大幅增加,而印度-恒河平原则因降雨不足而面临干旱。

超过10亿人依靠季风维持南亚地区的经济稳定;这一气候系统的进一步变化可能导致大范围的困境。由于常用的气候模型无法捕捉到已经发生的季风变化,科学家们一直难以预测这种气候模式未来的发展趋势。

Mahendra等人指出,现有模型既不能充分反映大西洋温度的变化,也不能充分反映这些温度变化与全球其他地区气候模式之间的联系。因此,耦合模型往往无法预测这种季风转变。

具体而言,目前的气候模型缺乏将有关冷斑(cold blob)的信息纳入其中的能力,冷斑是位于格陵兰岛南部的一片冷水区域。当研究人员将冷斑添加到气候模型结果中时,他们发现,它可以改变急流,使其将水汽输送到印度西北部,同时阻止其他地区风暴系统的形成。这正是季风模式中观测到的那种转变。当一个大尺度风型以这种方式阻止较小尺度天气型的形成时,这种机制被称为正压调控机制(barotropic governor mechanism)。

这种正压调控机制也解释了为什么近年来全球中纬度地区观测到了更多的风暴活动。作者指出,这些结果强调了在构建气候模型时,将全球不同地区的各种过程联系起来的重要性。

—科学撰稿人Saima May Sidik (@saimamay.bsky.social)

This translation was made by Wiley. 本文翻译由Wiley提供。

Read this article on WeChat. 在微信上分享本文。

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.

Trekking Tourism Leaves a Microplastic Footprint in a High Himalayan Lake

Mon, 06/15/2026 - 12:46

From Antarctica’s frozen wilderness to the heights of Mount Everest, microplastics have been found in some of the most remote places on Earth. And their reach continues to expand.

A recent study published in iScience found that one of Nepal’s highest snow-fed lakes, situated at an altitude of 4,917 meters (16,132 feet) in the Himalayas, contains a significant amount of microplastic pollution. Researchers detected an average of 42 microplastic particles per liter of water, highlighting how microscopic plastic contamination has reached even some of the world’s most remote environments.

“It is yet another piece of evidence that our massive consumption of plastic in countries across the Global South is coming back to harm us. We are basically hitting an axe on our own foot.”

“It is yet another piece of evidence that our massive consumption of plastic in countries across the Global South is coming back to harm us,” said Tista Prasai Joshi, a water scientist at the Nepal Academy of Science and Technology in Kathmandu. “We are basically hitting an axe on our own foot.” Joshi, who was not involved in the new research, added that plastic use is so deeply woven into daily life that many people fail to recognize its effect on ecosystems. Rising tourism in countries like Nepal is only accelerating the spread, carrying microplastic pollution to remote corners of the Himalayas.

In 2019, marine scientist Imogen Napper and colleagues at the University of Plymouth reported a significant presence of microplastics in snow and stream water around the Everest Base Camp region, about 5,300 meters (17,388 feet) above sea level. The findings made headlines around the world.

Despite the publicity given the Everest Base Camp research, very few studies have examined microplastic pollution in highland lakes. Such studies are particularly important because water stays in these lakes much longer than in rivers, making them valuable archives of pollution, able to preserve evidence of contamination over years or even decades.

A Trip to Tilicho

To help address this gap in research, Sahil Shrestha, an environmental researcher at Tribhuvan University’s Institute of Engineering, Pulchowk Campus, and a colleague turned a couple of days of Himalayan trekking into a field expedition. Shrestha selected six accessible shoreline locations around Tilicho Lake for sampling. At each location, using his bare hands to prevent microplastic pollution from gloves, he submerged a stainless steel bottle about 20 centimeters below the water surface, opened the cap, filled the bottle, and resealed it before bringing the sample back for analysis.

Shrestha was particularly concerned about environmental contamination, as transporting samples from a remote lake to a laboratory in Kathmandu takes time, and contamination can occur en route. To account for possible contamination scenarios, he implemented several control measures.

“We carried a trip blank for this,” he said. “Essentially, in a rinsed and cleaned steel bottle, I carried distilled water throughout the trip.”

Because he knew the water was uncontaminated at the start of the trip, Shrestha could measure it again upon returning to the lab to see whether it became contaminated during the trip (for example, by being carried in a backpack). If the trip blank showed signs of contamination, the scientists could assume the collected samples were similarly contaminated and could subtract the known level of contamination from their analysis. Trip blanks and field blanks are standard quality assurance practices used in environmental chemistry research.

Shrestha also carried field blanks to account for possible microplastics in the air. At the field site, he poured distilled water from the laboratory into another bottle. The idea was to account for possible airborne microplastics that could later be subtracted to calculate the net microplastics in the water alone.

The sampling experience left a lasting impression on Shrestha, in part because he and his colleague had to carry up to 15 liters of water between sampling sites. “For two individuals, carrying so many liters of water around each site was a challenging yet fun part of the process,” he said.

Plastics Aplenty

Polyester, polyethylene, and polypropylene are commonly used in hiking gear, jackets, tents, plastic bottles, and bags, all of which can shed microplastics while visitors explore the area.

Once in the lab, Shrestha’s team carried out further analyses, including the removal of organic material, filtration, and microscopy to categorize the types of microplastics. They found that microplastic contamination was higher in areas of the lake more easily accessible to tourists. Polyester, polyethylene, and polypropylene were the main types detected. These materials are commonly used in hiking gear, jackets, tents, plastic bottles, and bags, all of which can shed microplastics while visitors explore the area, suggesting tourism was the most likely source of contamination.

Shrestha noted that there is not yet evidence that Tilicho Lake drains into rivers, but many Himalayan lakes do drain into rivers that, in turn, feed communities downstream. The findings hint that microplastic contamination at the water’s source has a far-reaching ripple effect on human health and downstream ecosystems.

Shrestha stressed the need for such research to inform policy and regulatory decisions.

“Tilicho Lake is situated in the Annapurna Conservation Area Project (ACAP) region, and these conservation programs should restrict trekkers from carrying plastic bottles and polyethylene bags,” he said. “Overall, the trekking gear industry is [contributing] significantly to microplastic pollution in remote regions, and this should be addressed through international collaboration.”

—Saugat Bolakhe, Science Writer

Citation: Bolakhe, S. (2026), Trekking tourism leaves a microplastic footprint in a high Himalayan lake, Eos, 107, https://doi.org/10.1029/2026EO260191. Published on 15 June 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.

An update on landslides from the 8 June 2026 M=7.8 earthquake offshore Mindanao in the Philippines

Mon, 06/15/2026 - 07:17

It is now clear that more than half the fatalities from last week’s earthquake in the Philippines were caused by landslides.

In the areas of the Philippines affected by the 8 June 2026 M=7.8 earthquake offshore Mindanao, operations have shifted from rescue to recovery. Inquirer has an interesting report about information provided by an official from the Office of Civil Defense (OCD) today. The death toll has risen to 65, but a further 36 people are missing. There is now no prospect of their having survived. The report notes that:

The people reported to be missing were likewise due to earthquake-induced landslides, he further noted.

Asked whether there were still any signs of life among the locations of the reported missing persons, Alejandro pointed to Jose Abad Santos town in Davao Occidental.

“One of the areas there, I think, the team has already pulled out or called off the search and rescue because it’s immense. It was a mountain that really came down, so it’s very hard,” he explained.

There is now a good Sentinel 2 image, collected on 14 June 2026, showing the area affected by the earthquake. There are some fascinating areas. Thus, for example, this image is centred on [5.63777, 125.45305]:-

Sentinel 2 image dated 14 June 2026 showing landslides triggered by the Mindanao earthquake.

There are at least two, and maybe three, large (>500 m long) landslides in this image, and a host of other failures too. Meanwhile, to the north, centred on [5.75674, 125.55459] we have this:-

Sentinel 2 image dated 14 June 2026 showing landslides triggered by the Mindanao earthquake.

The latest NDRRMC Situation Report indicates that 66 damaging landslides have been recorded.

To date, I have seen reports of 17 confirmed fatalities in landslides, plus the 36 missing, so at least 53 of the 101 fatalities are from landslides. However, it is likely that there are some that I have yet to track down.

Return to The Landslide Blog homepage 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.

How Einstein’s Lost Theory Could Help Us Find Minerals

Fri, 06/12/2026 - 12:00

Albert Einstein postulated in his 1905 theory of special relativity that the speed of light in a vacuum is constant. Ever since, that’s been one of the fundamental assumptions of physics.

Now Enbang Li, a physicist at the University of Wollongong in Australia, has challenged this idea by building a machine he says is capable of detecting changes in the speed of light as it crosses Earth’s surface. The findings suggest that light is, in fact, sped up by gravity, which could have implications for Earth science applications ranging from climate monitoring to mineral resource exploration.

An Old Conundrum

The idea that light is influenced by gravity is not new. Einstein’s ideas, which were further developed with his theory of general relativity in 1915, predicted massive objects in space would bend light with their gravitational grab. This theory was famously proven in 1919 when two independent teams measured starlight passing a solar eclipse at two different points on Earth’s surface and found the results matched Einstein’s predictions.

This bending of light’s path, according to general relativity, is achieved by a warping of the space-time fabric. Under this scenario, the speed of light remains constant—it just has to travel farther as it navigates the warped space-time around celestial bodies, so to a distant observer, it appears to have been slowed.

But what if light doesn’t navigate warped space-time and actually is slowed down or sped up by the gravity of large objects?

Li pointed out that Einstein himself was not always convinced the speed of light was constant. In 1911, he wrote a paper postulating that light speed changed depending on the gravity of objects it passed by. However, “when he published his general theory,” said Li, “he just abandoned this model.”

If the movement of light can be affected by gravity, Li reasoned, it might be possible to detect variations in its speed on a local level—such as an elevator shaft in a building on the campus of the University of Wollongong.

Raising the Big Issues

Gravity on Earth varies locally, depending on altitude, underground density, and topography. Gravity at the top of a tall building, for example, is measurably weaker than it is at the bottom.

With these variations in mind, Li installed an experiment in an elevator. It consisted of a coil of fiber-optic cable that if stretched out in one direction, would be 10 kilometers (6.2 miles) long. Laser beams were fired through the cables and then reflected back, thus traveling 20 kilometers (12.4 miles) before reaching an ultrafast photodetector. An oscilloscope measured the time it took for the beam to travel that distance. The experiment was run at the top of the shaft and at the bottom.

The biggest challenge, Li said, was filtering out all the surrounding environmental “noise,” such as changing temperature and humidity, electromagnetic disturbance, and building vibrations. Li designed a temperature control system, and the experiment was sealed in an enclosure with electromagnetic shielding to isolate air flows. Li ran the experiment and found light moved minutely faster at the bottom of the shaft than at the top.

Gravity Sensing on the Go

Next, Li took his research a step further by building a small, portable machine he claims can detect changes in the speed of light as it nears more gravitationally dense objects.

In this second experiment, Li positioned a moveable 72-kilogram (159-pound) weight near the machine. Light, he found, moved faster when the weight was near the machine than when it was farther away.

The results, which were published in Scientific Reports, are consistent with the variable speed of light model Einstein proposed in 1911, although Li’s preliminary results are much larger than that model predicts.

If proven, the findings would present a fundamental challenge to our understanding of both general and special relativity.

In the world of Earth sciences, they could lead to greatly improved gravity-sensing technologies. Because of their sensitivity to changes in mass, gravity sensors are used to map the seafloor and to locate underground mineral reserves. Gravity sensing can also improve our understanding of Earth’s climate as variations in the gravity field can be linked to factors like changes in ice mass and shifts in groundwater.

Currently, gravimeters are vulnerable to vibrations and movement, whereas Li’s machine, which has no moving parts, could even be used on board a plane or submarine.

“A Striking Claim”

Chris Stevens, a numerical relativist with the University of Canterbury in New Zealand, called the work “intriguing and ambitious.” While Stevens, who was not involved in the research, said that Li’s work is “well founded,” he noted that any observable effects of gravity on light on Earth would be “extraordinarily small” and therefore these results must be treated with caution.

“In my own research on observable gravitational phenomena,” he explained, “I usually require a few black holes colliding somewhere in the universe. Separating genuine gravitational signatures from environmental and instrumental noise will therefore be exceptionally demanding.”

“The work is exciting because it pushes precision photonic measurement techniques into a regime where relativistic effects may become practically useful for geophysics and sensing applications.”

Stevens said the implications of Li’s research, if validated, would be far-reaching. “The work is exciting because it pushes precision photonic measurement techniques into a regime where relativistic effects may become practically useful for geophysics and sensing applications.”

John Norton, an historian of physics at the University of Pittsburgh who was also not involved in the research, called the findings a “striking claim.” He was, however, skeptical of them, saying “if there is a coupling between light and gravity of magnitude greater than general relativity predicts, it is hard to see how the 1919 eclipse test and later studies of gravitational lensing would not have found it.”

Li acknowledged there is a long way to go before his device finds everyday use. Disentangling the intricacies of space and time, he said, is a vast challenge. “In physics, people still say gravity is a mystery. Light is another mystery. So if you put these two mysteries together, that’s going to be a giant mystery.”

—Bill Morris, Science Writer

Citation: Morris, B. (2026), How Einstein’s lost theory could help us find minerals, Eos, 107, https://doi.org/10.1029/2026EO260189. Published on 12 June 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.

6 Ways This Year’s “Super El Niño” Could Affect Climate, Humans, and Marine Creatures

Thu, 06/11/2026 - 22:16
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.

The key word here is could. Experts including Ken Graham, the director of NOAA’s National Weather Service, all emphasize that no two El Niños are alike.

“Each one is unique with its own imprint on our weather,” Graham said in a NOAA press release. However, scientists have learned a few things from watching the ways that this warm phase of a natural climate cycle over the tropical Pacific has affected our weather patterns in the past.

“Advanced monitoring and an improved understanding of El Niño patterns allow the NWS to better predict and better prepare the public and our core partners for what is to come,” Graham said.

 Related

This morning, NOAA released an El Niño Advisory, announcing that the climate phenomenon (the warm phase of the El Niño–Southern Oscillation) has officially arrived in the tropical Pacific. The agency forecasts a 63% chance of a “very strong” El Niño from November 2026 to January 2027 that “would rank among the largest El Niño events in the historical record.”

NOAA defines a “very strong” El Niño as when the Pacific’s surface waters are more than 2°C warmer than average. The agency doesn’t use the phrase “Super El Niño,” but there have only been three such “super” or “very strong” El Niño events since 1980. The last one was in 2015.

What does this mean for climate, for humans, and marine species? Here’s a roundup of some potential forecasted effects—some good, some bad—of the weather pattern that’s been making headlines over the past few months.

1. More rain and snow in the southern U.S.

In a typical year, a warm pool of water in the equatorial Pacific would be transported westward—away from the western coast of the Americas—by trade winds. But during an El Niño event, those trade winds weaken, and the warm pool of water extends east, explained Ariel Cohen, the meteorologist in charge of the National Weather Service’s Los Angeles and Oxnard Office in a press briefing at the Aquarium of the Pacific in Long Beach, Calif.

This warm water “causes jet energy in the atmosphere to bring disturbed weather southward across the southern United States, which can bring wetter than normal conditions to our area with drier conditions farther to the north,” Cohen said.

The southward shift of the storm track could also lead to drier conditions over the northern Rockies and as far east as the Ohio and Tennessee Valleys.

2. More shark and whale sightings off the Southern California coast

In the past, strong El Niños have led to decreased amounts of plankton in the Pacific, particularly the open ocean, forcing species that rely on plankton (and the species that rely on the species that rely on plankton, and so forth) to widen their net when searching for food.

“[Plankton] is important because that’s the base of the food web,” explained Andrew Leising, a research oceanographer at NOAA, at the Aquarium of the Pacific. “Marine mammals and other migratory species end up being closer to shore, because they’re going to where their food is.”

Whales in particular rely on the upwelling of cold water to bring them krill to eat. As they are driven nearer to the coast in search of food, they also grow more likely to become entangled in fishing nets.

3. A milder Atlantic hurricane season

Warm water is a key ingredient in a hurricane, so it might seem, at first thought, that the Pacific’s unusually warm waters might augur a more extreme hurricane season. But another effect of El Niño is that it strengthens vertical wind shear over the Atlantic. When winds are too strong, they can tear a storm apart before it picks up the momentum to become a hurricane.

“Wind shear is good for us, bad for the hurricanes,” Phil Klotzbach, a hurricane forecaster at Colorado State University and lead author of the university’s 2026 Atlantic Hurricane Forecast, told Eos.

NOAA’s 2026 Atlantic Hurricane Forecast suggests that the 2026 season has a 55% chance of being below normal, and will likely include 8 to 14 named storms with winds of at least 39 miles per hour.

4. Fewer squid along the California coast

Past El Niño events have shown that warmer Pacific waters can increase the likelihood of harmful algal blooms. Among other effects, these blooms can lead to a lower abundance, and a northward shift, of market squid. Market squid and Dungeness crab bring the most volume and value to California’s commercial fisheries.

In 2014, a large mass of hot water in the Pacific known as the Blob was followed up by an El Niño event. That year, “we had several closures of crab and shellfish fisheries due to harmful algal blooms,” Leising said.

However, Leising also explained that the warm patch of water in the Pacific this year is much smaller and farther from shore than the Blob was in 2014. So, though we may see effect similar those in 2014, they’re likely to be less extreme.

In addition, the same conditions driving sharks and whales toward the coast could also drive tuna toward the coast, leading to increased opportunities for that fishery.

5. More high-tide flooding on U.S. coasts

With El Niño shifting the Pacific jet stream south of its usual position, sea levels along the U.S. West Coast may rise, exacerbating the existing sea level rise linked to climate change. On the East Coast, the jet stream shift can lead to more storm surges, which combine with higher-than-typical precipitation levels.

“It usually ends up being a double whammy,” said NOAA oceanographer and high tide flooding expert William Sweet, in a NOAA news story. “The first punch is decades of sea level rise, which has waters close to the brim in many coastal communities. And now with this second punch—a strong El Niño—coastal communities face more frequent, deeper and widespread high tide flooding along both the West and East Coasts.”

6. A bad year for sea lions

El Niño events can have harmful effects on sea lions. Algal blooms can lead to severe illness, or even death, for the pinnipeds. Algal blooms can also kill off fish and cephalopod species (such as market squid) that sea lions rely on for food. During past El Niño events, California sea lions have also experienced lower rates of reproduction and produced smaller pups, Leising said.

“California sea lions are indicator species, meaning they will be one of the first species which may show signs of domoic acid toxicity, respond to changes in their ecosystem, and signal to the public how our oceans and ecosystem are doing,” said Brett Long, vice president of animal care at the Aquarium of the Pacific.

—Emily Gardner (@emfurd.bsky.social), Associate Editor

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.

Multi-Scale Fault Roughness Encapsulated in a Friction Law

Thu, 06/11/2026 - 17:33
Editors’ Highlights are summaries of recent papers by AGU’s journal editors. Source: Journal of Geophysical Research: Solid Earth

Earthquakes release energy and result in source properties defined across a wide range of scales that are not represented in conventional frictional laws. Norisugi and Noda [2026] introduce a new rate- and roughness-dependent friction (RRF) law which incorporates both effects from fault slip rate and multi-scale variation in fault topography. By limiting the number of state variables in the RRF formulation, the authors show with efficient earthquake cycle simulation that this multi-scale approach can reproduce a key observed relationship between fracture energy and fault slip.

Although further refinement is needed to better represent roughness evolution, this study marks a major advance in earthquake modeling by demonstrating the necessity and feasibility of incorporating multi-scale fault topography in the characterization of earthquake source process.  

Citation: Norisugi, R., & Noda, H. (2026). Multi-scale rate- and roughness-dependent frictional constitutive law and dynamic earthquake sequence simulation. Journal of Geophysical Research: Solid Earth, 131, e2025JB033580. https://doi.org/10.1029/2025JB033580

—Yajing Liu, Associate Editor, JGR: Solid Earth

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.

Vast Space, Sparse Data: An AI Answer to Twin Space Weather Challenges

Thu, 06/11/2026 - 13:29

Solar activity affecting Earth and its planetary neighbors encompasses a wide range of phenomena, from the steady solar wind and the interplanetary magnetic field to extreme events like solar flares, coronal mass ejections (CMEs), and solar energetic particle (SEP) events. These space weather phenomena interact in complex ways with planetary magnetospheres and atmospheres. On Earth, we see the results in the dancing lights of stunning auroras and in less frequent but sometimes severe disruptions to telecommunications, navigation, and energy infrastructure.

Forecasting conditions throughout the heliosphere (the region influenced by the solar wind), understanding the variety of Sun-Earth interactions, and predicting arrivals of space weather events—both benign and potentially hazardous—are a grand challenge.

The Sun-Earth challenge requires tracking and predicting conditions—from routine and quiet to rare and extreme—across tens of millions of kilometers of interplanetary space.

Solar flares emit electromagnetic radiation that spreads in all directions. In contrast, the propagation of CMEs and SEP events depends on their source location on the Sun and on the heliospheric magnetic field, which is carried outward by the solar wind. The impacts these events have on magnetosphere systems further vary depending on particle energies and intensities in SEPs and on particle speeds and the magnetic field orientation in CMEs. The Sun-Earth challenge thus requires tracking and predicting conditions—from routine and quiet to rare and extreme—across tens of millions of kilometers of interplanetary space.

This tracking and prediction is powered by petabyte-scale datasets from solar observatories and spacecraft measurements that provide rich observational archives. Researchers use these data to deduce physically meaningful quantities describing the heliosphere and to identify patterns to distinguish quiet from active conditions. The resulting insights not only answer fundamental science questions but also provide critical prediction time frames needed by space weather forecasters.

Even with all these data, the enormity of space between the Sun and Earth presents a major obstacle to our predictive capabilities. Another obstacle is that the data are obtained by different instruments operating at different locations and times. These factors combine to create a unique data sparsity challenge that complicates large-scale analysis.

These fundamental issues—the massive yet still insufficient supply of data available, the extreme differences in the scales of the processes we must illuminate, and the need for actionable predictions—suggest opportunities for artificial intelligence (AI) and machine learning (ML) to complement traditional physics-based analytical approaches [Camporeale, 2019]. In a series of workshops—insights from which inform the discussion below—scientists explored such opportunities and how they can advance heliophysics research and operational space weather forecasting.

The Need for Space Weather Forecasting

Space weather events can have significant impacts on infrastructure and humans. They can disrupt satellite operations (e.g., by enhancing atmospheric drag on satellites), damage electronics in space, interfere with radio communications and GPS, and even affect power grids (e.g., through geomagnetically induced currents) during the most severe events. They can also pose risks to people, especially astronauts beyond the protection of Earth’s atmosphere and airline crews and passengers on long-distance polar flights, during which exposure to energetic particles is elevated. Forecasting offers a first line of defense in preparing for or preventing damaging and hazardous effects of space weather.

In assessing major CMEs, forecasters consider whether and when events will reach Earth and whether they will trigger geomagnetic storms and substorms. For SEP events, predictions must include arrival times, peak intensities, durations, and energy characteristics.

Predicting extreme space weather phenomena is vital, but equally important is forecasting periods when no significant activity is expected, which is critical information for satellite operators and other stakeholders. Making such predictions requires understanding physics spanning 8 orders of magnitude in space and time, from subsecond processes in Earth’s magnetic environment to multiday solar eruptions propagating across the 150 million kilometers between the Sun and Earth (Figure 1) and long-term interactions at scales associated with the 11-year solar cycle.

Fig 1. Length scales and Sun-to-Earth transit times vary greatly for different types of space weather (SW), including solar flares, solar energetic particle (SEP) events, coronal mass ejections (CMEs), and interplanetary coronal mass ejections (ICMEs). High-speed particles are the first to arrive, usually within minutes of a flare, whereas CMEs arrive in 2–4 days. Credit: Georgoulis et al. [2026], CC BY-NC-ND 4.0

In addition to operational forecasting, these challenges are fundamental in heliophysics research. Such research includes work to reveal how the Sun generates its magnetic field, how solar wind accelerates and evolves, how planetary magnetospheres respond to external forcing, how particles are accelerated, and how energy transfers across multiple scales and regimes.

Unique Challenges in Heliophysics

Modern AI and ML algorithms excel at analyzing well-curated, extensive datasets that include millions of training examples. For example, AI-aided terrestrial weather forecasting relying on continuous, high-resolution coverage from thousands of ground stations, weather balloons, and satellites has advanced dramatically in recent years.

Fewer than a dozen spacecraft monitor Earth’s magnetosphere, a region spanning tens of Earth radii. Solar wind observations are even sparser.

Heliophysics, however, presents a unique and somewhat opposite scenario. Fewer than a dozen spacecraft monitor Earth’s magnetosphere, a region spanning tens of Earth radii (about 6,371 kilometers). Solar wind observations are even sparser, with just a handful of monitors scattered across the space between the Sun and Earth. This fundamental scarcity poses a challenge for data-driven approaches, which typically depend on abundant observations that are well distributed in space and time to produce trustworthy (i.e., generalizable and reproducible) models.

Data sparsity is further compounded by the relative rarity of intense space weather phenomena such as CMEs, major geomagnetic storms, and extreme substorms, which occur only a few times per solar cycle. Most heliophysical observations capture quiet, low-activity conditions when the solar wind is steady and magnetospheres are calm. Standard ML approaches trained on such imbalanced datasets may achieve high statistical accuracy by simply predicting a “nothing-will-happen” outcome but completely fail when extreme events occur.

Although solar eruptions and geomagnetic storms are relatively rare, they exhibit recurring patterns and consistency in their physical drivers. This regularity suggests that historical observations, when properly clustered and analyzed, can be used to enhance prediction capabilities. The challenge therefore lies in extracting meaningful patterns from sparse measurements of rare events while avoiding models that work well for average conditions but fail when they matter most [Chu et al., 2025].

AI Solutions for Data Sparsity

Heliophysics research employs clever approaches to extract maximum information from the limited available observations. One strategy is to mine multidecade observational records from various satellites and to match and group together measurements collected at times with similar solar wind and geomagnetic activity conditions.

This process clusters tens of thousands of data points from similar magnetospheric states. Such clustering enables reconstruction of dynamic features like nightside magnetic field changes during substorms [Stephens et al., 2019] and the presence of near-Earth magnetotail reconnections [Angelopoulos et al., 2020].

Another, more universal approach is to embed fundamental physical laws directly into ML models through physics-informed neural networks [Raissi et al., 2019], ensuring that predictions respect physical reality even when training data are limited. Data assimilation techniques used in weather forecasting similarly blend sparse observations with physics-based simulations and update models as new measurements arrive.

This animated model shows Earth’s magnetosphere during a powerful May 2024 geomagnetic storm that involved strong solar flares and multiple CMEs. The visualization uses the Multiscale Atmosphere-Geospace Environment (MAGE) model from the Johns Hopkins Applied Physics Laboratory to depict wind rushing toward Earth and disturbing its magnetic field (orange and purple lines). The green cloud represents electric field current intensity; the blue squiggles are tracers of solar wind velocities. Credit: NASA Scientific Visualization Studio and NASA DRIVE Science Center for Geospace Storms

These methods converge on a common theme: building gray box models (so named because they’re less opaque than black box models) that are data driven but grounded in physically real constraints. For data-starved applications, hybrid approaches can outperform purely data-driven or purely physics-based methods [Liu et al., 2025].

Satellite instruments are generating increasingly large solar wind datasets. However, the variables obtained (e.g., solar wind speed and pressure) are highly intercorrelated [Borovsky, 2018], making it difficult to identify which ones truly drive magnetospheric responses. New algorithms are helping to distill datasets without losing critical scientific information [e.g., Camporeale, 2025]. Meanwhile, advanced statistical and ML methods can cut through dataset complexity by reducing dimensionality, identifying causal relationships among variables, and providing clues about dominant drivers.

For instance, information theory provides tools to detect dependencies in complex systems, establish causality, and rank variables that most effectively predict space weather outcomes [Wing et al., 2022]. Such techniques can be paired with other “explainable” tools, such as SHAP (SHapley Additive exPlanations) values, a method inspired by game theory, to pinpoint physical variables (e.g., solar wind speed or magnetic orientation) that drive a prediction [Ma et al., 2023].

Distilling datasets and improving model interpretability help make ML more practical and more scientifically trustworthy and its predictions more robust. But fully trusting ML models in operational environments requires rigorous validation and uncertainty quantification. These models must not only make predictions but also indicate their confidence levels for operational decisionmaking.

When a model forecasts a major geomagnetic storm, operators need to know whether that prediction carries 60% or 95% confidence, for example.

When a model forecasts a major geomagnetic storm, operators need to know whether that prediction carries 60% or 95% confidence, for example. Ensemble approaches, in which multiple models provide a range of outcomes, help quantify this uncertainty, while using standardized, well-documented datasets enables fair model intercomparisons.

The research community is developing ML-ready benchmark datasets with consistent formatting and clear metadata to establish such validation procedures [e.g., Angryk et al., 2020]. These resources allow researchers to test new algorithms against common baselines, accelerating progress while ensuring that advances are robust and reproducible rather than artifacts of specific data processing choices.

Notably, one domain in heliophysics that is not affected by severe data sparsity is solar imaging. Decades of continuous, high-resolution observations from the Solar Dynamics Observatory (SDO), which delivers 1.5 terabytes of data every day, have created enormous data archives. Because the Sun drives space weather throughout the heliosphere, these datasets offer an ideal opportunity for use in foundation models, large-scale ML systems trained to learn comprehensive internal representations that can then be easily adapted to specific scientific tasks with minimal additional training.

Surya, a foundation model designed to construct a digital representation of the Sun, represents one such effort. It is still in early development and has yet to be validated, but this approach illustrates how data-rich domains can be leveraged with modern AI techniques to create tools that broadly benefit heliophysics research and space weather forecasting.

Advancing Research and Operational Forecasting Together

In addition to the needs for data and model development and validation, applying AI to address the challenges of heliophysics requires sustained, multidisciplinary collaborations. Fostering those collaborations has been the focus of a series of workshops, with the most recent being 2025’s Machine Learning, Data Mining and Data Assimilation in Geospace (LMAG25) meeting at the Johns Hopkins University Applied Physics Laboratory. The workshops have brought together heliophysicists, machine learning experts, data scientists, and specialists from weather forecasting and applied mathematics to exchange knowledge and establish community standards.

Space weather forecasters need models that are accurate and interpretable and that provide not just statistical metrics but also actionable predictions.

The LMAG forums also serve as gathering spaces for scientists to validate models against diverse datasets, compare physics-based and data-driven approaches, develop performance benchmarks, and discuss how to bridge research and operational requirements. Space weather forecasters need models that are accurate and interpretable and that provide not just statistical metrics but also actionable predictions with known limitations and reliability. Of course, researchers also benefit. These conversations allow them to gain insight into operational constraints that shape how modeling approaches become practical in real-world settings.

LMAG and similar initiatives facilitate direct exchanges among adjacent communities, including by making meeting presentations openly available. These efforts are helping translate cutting-edge AI and ML techniques into practical tools that help protect critical infrastructure and human well-being. They are also deepening our understanding of how the Sun shapes space weather throughout the solar system and its effects—both mundane and major—on Earth.

References

Angelopoulos, V., et al. (2020), Near-Earth magnetotail reconnection powers space storms, Nat. Phys., 16(3), 317–321, https://doi.org/10.1038/s41567-019-0749-4.

Angryk, R. A., et al. (2020), Multivariate time series dataset for space weather data analytics, Sci. Data, 7(1), 227, https://doi.org/10.1038/s41597-020-0548-x.

Borovsky, J. E. (2018), The spatial structure of the oncoming solar wind at Earth and the shortcomings of a solar-wind monitor at L1, J. Atmos. Sol. Terr. Phys., 177, 2–11, https://doi.org/10.1016/j.jastp.2017.03.014.

Camporeale, E. (2019), The challenge of machine learning in space weather: Nowcasting and forecasting, Space Weather, 17(8), 1,166–1,207, https://doi.org/10.1029/2018SW002061.

Camporeale, E. (2025), PARIS: Pruning Algorithm via the Representer theorem for Imbalanced Scenarios, arXiv:2512.06950, https://doi.org/10.48550/arXiv.2512.06950.

Chu, X., et al. (2025), Imbalanced Regression Artificial Neural Network Model for Auroral Electrojet Indices (IRANNA): Can we predict strong events?, Space Weather, 23(5), e2024SW004236, https://doi.org/10.1029/2024SW004236.

Georgoulis, M. K., et al. (2026), Prediction of solar energetic events impacting space weather conditions, Adv. Space Res., in press, https://doi.org/10.1016/j.asr.2024.02.030.

Liu, Y., et al. (2025), Data-driven modeling of electrostatic turbulence by physics-informed Fourier neural operator, Mach. Learn. Sci. Technol., 6(4), 045050, https://doi.org/10.1088/2632-2153/ae19cd.

Ma, D., et al. (2023), Opening the black box of the radiation belt machine learning model, Space Weather, 21(4), e2022SW003339, https://doi.org/10.1029/2022SW003339.

Raissi, M., P. Perdikaris, and G. E. Karniadakis (2019), Physics-informed neural networks: A deep learning framework for solving forward and inverse problems involving nonlinear partial differential equations, J. Comput. Phys., 378, 686–707, https://doi.org/10.1016/j.jcp.2018.10.045.

Stephens, G. K., et al. (2019), Global empirical picture of magnetospheric substorms inferred from multimission magnetometer data, J. Geophys. Res. Space Phys., 124(2), 1,085–1,110, https://doi.org/10.1029/2018JA025843.

Wing, S., et al. (2022), Modeling radiation belt electrons with information theory informed neural networks, Space Weather, 20(8), e2022SW003090, https://doi.org/10.1029/2022SW003090.

Author Information

Savvas Raptis (savvas.raptis@jhuapl.edu), Manolis K. Georgoulis, Mikhail Sitnov, Anthony Sciola, and Simon Wing, Johns Hopkins University Applied Physics Laboratory, Laurel, Md.

Citation: Raptis, S., M. K. Georgoulis, M. Sitnov, A. Sciola, and S. Wing (2026), Vast space, sparse data: An AI answer to twin space weather challenges, Eos, 107, https://doi.org/10.1029/2026EO260188. Published on 11 June 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.

Our new paper: Extreme rainfall further endangers the world’s rarest great ape

Thu, 06/11/2026 - 07:19

In November 2025, Cyclone Senyar generated extreme rainfall in parts of Sumatra, Indonesia, triggering thousands of landslides. Our new paper in the journal Current Biology demonstrates that these landslides might have a devastating impact on a critically endangered population of Tapanuli orangutan.

In November 2025, Cyclone Senyar brought extreme rainfall to large parts of Sumatra in Indonesia. I have written about this on previous occasions – the rainfall triggered vast numbers of landslides.

In my line of work, we often focus on the landslide impacts on the landscape, on human lives and on infrastructure. We rarely consider the impacts on th eanimal population. This is certainly a weakness that the Cyclone Senyar event brings to focus.

Part of the area devastated by the landslides is that slopes around the Batang Toru rover, an area of forest that is home to a rare species of orangutang. These great apes, Pongo tapanuliensis, live in a habitat known as the West Block of Tapanuli. There are only 800 individuals left in the wild, a situation that is highly precarious. The loss of even a small number of adults could tip the species towards extinction.

I was a part of a consortium of scientists that considered the landslide impacts of Cyclone Senyar on the habitat of these orangutangs. The results have just been published in the journal Current Biology (Meijaard et al. 2026) – the paper is open access and published under a creative commons license.

This image, from the paper, shows the landslide impacts of Cyclone Senyar:-

Before and after satellite imagery of the impacts of Cyclone Senyar. From: Meijaard et al. (2026).

In the study area of 71,161 hectares, the mapping indicates that there were 50, 185 individual landslides, covering a surface area of 8,303 hectares. This is about 11% of the forested area. We then estimate the likely loss of the orangutang population, which is likely to be in the range of 18-120 individuals, with a central estimate of 58 individuals. This is likely to have been a devastating loss for this highly endangered population.

This level of habitat loss might also be placing a severe pressure on the remaining population, so further fatalities are very possible through, for example, reduced food availability.

The intensity of the rainfall was almost certainly supercharged by climate change. The impacts of Cyclone Senyar are being replicated widely – and of course we are now in the northern hemisphere tropical cyclone season again.

Our paper makes some policy recommendations for this population of orangutans. First, the government of Indonesia needs to permanently protect this area of forest against mining , palm oil and hydropower developments. Ideally, the protected area should be expanded. Second, Indonesia needs support for biodiversity-recovery, hazard forecasting and ecological restoration planning.

Reference

Meijaard, E. … Petley. D. … et al. 2026, Extreme rainfall further endangers the world’s rarest great ape. Current Biology. https://doi.org/10.1016/j.cub.2026.05.029

Return to The Landslide Blog homepage 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.

As Wildfires Increase in the West, So Does Suppression Spending

Wed, 06/10/2026 - 13:18
Source: Earth’s Future

Hotter, drier conditions in the western United States have led to a rise in wildfire activity that has damaged or destroyed infrastructure, natural ecosystems, and entire towns across the region. As fires grow larger and more destructive, the cost of managing them rises as well.

Fire management agencies in the United States have been feeling the pressure. Between 2014 and 2023, fire management agencies across all levels of government experienced a 131% increase in total area burned and a 268% increase in total fire spending adjusted for inflation compared to the period between 1985 and 1994.

Today, federal agencies like the Department of the Interior (DOI) and the U.S. Department of Agriculture Forest Service (USFS) continue to invest in aiding states and managing hazardous fuel growth on public land, as well as suppressing active fires. Policymakers and federal agencies alike must decide how to manage limited budgets while protecting people, property, and natural resources.

Prestemon et al. built statistical models based on historical data to examine the potential increase in spending by the DOI and the USFS between now and 2100. Their models link wildfire activity to climate variables such as temperature and water vapor deficit and then connect fire activity to suppression costs. To capture a range of possible future conditions on federal lands, the study predicts 10 fire and suppression spending scenarios by applying five different climate models to two different warming pathways (the moderate Representative Concentration Pathways (RCP) 4.5 scenario and the high-emissions RCP 8.5 scenario).

The results varied by region and scenario, but each of the 10 scenarios suggested a rise in area burned as well as inflation-adjusted fire suppression spending, with higher fire activity translating to higher costs. Projected changes in DOI and USFS land burned increased 80% by mid-century and 208% by late century.

By the middle of the century, both agencies are projected to see spending increases: about 0.65% per year for DOI spending and about 0.87% per year for USFS spending from 2020 to 2100. Although uncertainty increased with time and outcomes varied across climate models and warming pathways, the largest increases in both cost and wildfire activity were consistently projected for the northwestern United States. (Earth’s Future, https://doi.org/10.1029/2025EF007985, 2026).

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

Citation: Owen, R. (2026), As wildfires increase in the West, so does suppression spending, Eos, 107, https://doi.org/10.1029/2026EO260187. Published on 10 June 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.

Archetypes Could Accelerate Agricultural Adaptation to Less Snowpack

Tue, 06/09/2026 - 13:22

“Future winters promise less snow, more rain. Nobody’s prepared.” So proclaims the title of a recent article in the Proceedings of the National Academy of Sciences of the United States of America that frames adaptation to snow loss as the “million-dollar question” facing the western United States.

As the largest sectoral consumer of fresh water globally, agriculture is particularly vulnerable to snow loss.

Declining snowfall—and snowmelt—affects ecosystems, urban and rural water supplies, hydropower, recreation, tourism, and agriculture. As the largest sectoral consumer of fresh water globally, agriculture is particularly vulnerable to snow loss.

Much of the U.S. West faces one of the worst snow years on record, and the statistics on future conditions feel dire. Up to 40% of the water demand for agriculture in the region is likely to go unmet as it gets warmer and less snowy. Similar scenarios are shaping up elsewhere around the world, including southern Europe, high-mountain and Central Asia, western Russia, and the southern Andes [Qin et al., 2020].

In response, water managers have developed a range of approaches for adapting to snow loss: infrastructure-based approaches like managed aquifer recharge, nature-based solutions such as forest management and beaver dam analogues, demand-side approaches like multibenefit land repurposing, and polarizing supply-side approaches like reservoir expansion and cloud seeding (Figure 1).

Fig. 1. Potential approaches to reduce negative impacts to agriculture from snow loss include a variety of adaptive strategies that address either water supply or demand. Click image for larger version.

However, efforts to identify which of these strategies to implement for different drainage basins, or watersheds, using the variety of available approaches seem to fall into one of two traps: either searching for unrealistic one-size-fits-all panaceas [Ostrom, 2007] or treating every basin as unique, which is costly and inefficient.

The “trillion-dollar question” isn’t how to adapt but, rather, where existing strategies may make the most—and fastest—difference.

Importantly, continuing along this trajectory means that we’re on track to offset only about a third of global climate-induced crop yield losses by 2100. For the western United States, previous work has estimated cumulative economic losses from declining snowfall of hundreds of billions to trillions of dollars while noting that rational adaptation decisions are hampered by the lack of financial analyses of the importance of snow [Sturm et al., 2017].

We thus suggest that the “trillion-dollar question” isn’t how to adapt but, rather, where existing strategies may make the most—and fastest—difference to offset projected losses. Answering this question requires an approach that matches strategies to the contexts where they are more likely to succeed—one that treats basins as neither uniform nor unique.

A Mismatch in Research and Operational Scales

Physical scientists tend to look at snow loss as a basin-scale problem, in part because this view aligns with hydrologic boundaries. However, as our colleague, applied economist Joey Blumberg, explains, “county lines were not drawn to follow watersheds, and rivers do not conform to political borders, creating a patchwork of mismatched boundaries.”

Scientists have long emphasized that mitigating climate change requires us to “think globally, assess regionally, act locally.” And in 1992, the authors of the Dublin Principles reasoned that moving the needle on “wicked water problems” requires targeting decisionmaking at the “lowest appropriate level,” where stakeholders can collaborate most effectively.

Lake Tahoe, pictured here, contains 37 trillion gallons of water, roughly half of which is supplied by snowmelt in the Sierra Nevada Mountains. Credit: Beatrice L. Gordon

The challenge is that “local” isn’t a single, consistent unit. We recently explored the lowest appropriate level concept for agricultural water management in the U.S. West by defining local operational contexts on the basis of intermediaries such as irrigation districts, water conservancies, and mutual water companies that connect individual farmers to their hydrology [Gordon et al., 2024].

Working at this scale, we found one-size-fits-all strategies often don’t hold up, even within the same hydrologic basin [Gordon et al., 2024; Boisramé et al., 2026]. In the Upper Colorado River Basin, for example, expanding reservoir storage could buffer agriculture in northeastern Utah against declining snowpack, but the same strategy may fail miles away in southwestern Wyoming, where a thirstier atmosphere may make it harder to refill existing reservoirs.

However, collecting detailed local-scale information for just 13 of the roughly 2,600 operational contexts nationwide took almost 3 years of searching websites, reading working papers, and calling water managers.

Scaling this approach across the entire western United States is understandably overwhelming. We need a more systematic approach to help managers identify which strategies could work most effectively, and where.

A Diagnostic for Agriculture and Snow Loss

Ostrom [2007] argued that complex systems, such as Western agriculture, “are partially decomposable in their structure.” This insight is woven into archetype analysis, an approach for identifying recurrent patterns across otherwise diverse systems.

Like workplace assessments—which are genuinely useful, albeit imperfect, tools for understanding successful management styles—archetypes draw on qualitative, quantitative, or hybrid approaches to group diverse operational contexts on the basis of shared characteristics [Sietz et al., 2019]. These groupings enable systematic knowledge transfer about, for example, how management strategies that work in one context can also guide adaptation elsewhere.

Three main characteristics interact to define operational contexts in snow-dependent agriculture in the western United States: physical constraints, governance systems, and human behavior.

“Researchers can empirically derive building blocks or components that comprise archetypes to represent key features of a system,” explains Elizabeth Koebele, who studies urban water sustainability [Garcia et al., 2019] and has begun applying archetypes in that context. However, she notes, these building blocks “vary based on the system context, available data, and study goal.”

We propose three main characteristics that interact to define operational contexts in snow-dependent agriculture in the western United States: physical constraints, governance systems, and human behavior. Physical constraints, including biophysical setting, infrastructure, and climate, determine available water supplies. Governance capacity relative to governance complexity shapes how those supplies are allocated across competing uses. Human behaviors influence both water demand and how users respond to supply conditions and governance rules.

Using these characteristics to establish archetypes of water management contexts could define a path forward for operationalizing an approach to accelerate successful adaptations to declining snowpacks in the West.

Constraining How Snowmelt Becomes Water Supply

Physical constraints stem from biophysical processes that influence how, when, and how much snow becomes streamflow; infrastructure that stores and conveys water; and hydrologic and climatic uncertainties about future supplies. These constraints can vary substantially from basin to basin.

Consider the Walker River Basin and California’s San Joaquin Valley, both of which rely on Sierra Nevada snowpack but have different biophysical settings. In some parts of the central Sierra, forest management can reduce wildfire risk and increase streamflow by up to 14% during low-snow years. Elsewhere, however, water made available by forest management may be consumed by remaining vegetation, limiting downstream gains.

These biophysical differences interact with uses of built infrastructure, including irrigation systems, reservoir outlets, and canals, to determine how and when water is stored and released. As temperatures warm and snowmelt declines, officials in both the Walker River and San Joaquin Valley basins must increasingly manage for a wider range of extremes, including “cold-water droughts.” However, the infrastructure to manage these trade-offs through reservoir storage and operations that balance agricultural deliveries with aquatic habitat needs is more developed in the highly managed San Joaquin than in the Walker.

Thankfully, measuring physical constraints on snowmelt at basin scales is becoming more feasible today with newly developed tools.

Layered on top of biophysical and infrastructural constraints are climatic and hydrological uncertainties, such as whether snow loss will lead to more evapotranspiration and less streamflow. These uncertainties complicate management decisions based on cost-benefit modeling of individual strategies: Should districts expand reservoir storage if precipitation is predicted to increase or decrease depending on the model? Frameworks like Decision Making Under Deep Uncertainty emphasize the need to select strategies that are robust across many possible futures.

Thankfully, measuring physical constraints on snowmelt at basin scales—a means, along with improved modeling, to reduce hydroclimatic uncertainties—is becoming more feasible today with newly developed tools. Water managers can turn, for example, to databases like the U.S. Geological Survey’s ResOpsUS [Steyaert et al., 2022], which catalogs historical reservoir operations across the contiguous United States, and to publicly available hydrologic projections such as those from Oak Ridge National Laboratory’s Coupled Models Intercomparison Project phase 6 (CMIP6) ensemble.

Governance Controls Supply Allocations

We frame governance around capacity and complexity. Capacity in this context is the ability of stakeholders “to mobilize resources in order to make equitable and fair decisions around shared challenges,” according to governance scholar Gina Gilson. Complexity refers to the number and intricacy of jurisdictions, authorities, regulations, and stakeholders involved. As governance complexity increases, the effectiveness of adaptation strategies becomes more sensitive to capacity constraints, particularly regarding timescales and funding.

For example, infrastructure in the Walker is controlled locally by a single water district, and jurisdictional coordination involves two states and the Walker River Paiute Tribe. Coordination on water management is never simple, but fewer jurisdictions generally means faster decisionmaking and clearer authority, allowing the single water district to implement strategies like multibenefit land repurposing more readily. Such implementations, in turn, enable reduced agricultural water use, directly supporting restoration of Walker Lake and recovery of endangered species.

Walker Lake in Nevada is part of the Walker River Basin. Credit: Alan Levine/Flickr, CC BY 2.0

The San Joaquin Valley is vastly different in scale and complexity, covering eight California counties, one of which alone has 22 water districts and seven cities. Following the passage of the state’s Sustainable Groundwater Management Act, water users in the basin formed more than 120 groundwater sustainability agencies. Agricultural water management thus involves overlapping federal and state systems that operate under different rules, contracts, and regulatory requirements. While land repurposing programs can be implemented, more substantial capacity, time, and resources are typically needed to do so.

Emerging efforts like the Western States Water Data Access and Analysis Tool (WestDAAT) and the Harmonized Database of Western U.S. Water Rights make it easier to assess governance in a basin by standardizing data about rules, regulations, and water rights across states. Combined with mapping of irrigation service areas and water transfers [Siddik et al., 2023], these resources help stakeholders identify the jurisdictions involved, how authority is distributed, and what coordination mechanisms exist for agricultural water management.

Human Behavior Shapes Demand Responses

Once snowmelt reaches water users, behavioral dynamics—how people respond to crises, policies, and changing conditions—determine how effectively management strategies achieve desired results.

Water demand is influenced by consumption choices and by economic, political, and cultural factors.

Water demand is influenced by consumption choices and by economic, political, and cultural factors. It is also influenced by factors that typical hydrologic models rarely account for, including social structure, social memory, and affluence. More affluent users are less likely to modify their behavior to reduce water use under conditions of scarcity.

The dynamics of water demand in the South Platte River Basin, for example, are especially complex, as they are balanced across cities, agriculture, and ecosystems across parts of Colorado, Nebraska, and Wyoming. Water prices in the basin’s Big Thompson project, a federal water diversion system in northern Colorado, jumped from $1,500 per acre-foot in 1990 to more than $30,000 in 2018, driven by economic factors that resulted in cities owning 70% of water originally intended for agriculture.

Even with reliable projections of future climate and water supply, carefully planned strategies can be overwhelmed by economic and behavioral factors, resulting in transfers and reallocations of water. What’s more, behavioral responses to adaptation strategies can paradoxically increase demand when users perceive that scarcity problems are solved.

The “reservoir effect” occurs when water security perceptions encourage expansion of water-intensive activities [Di Baldassarre et al., 2018]. Similarly, the irrigation efficiency paradox shows how efficiency gains can lead to expanded production and reduced return flows (how much irrigation water returns to streams and aquifers) downstream [Grafton et al., 2018].

Conceptual frameworks, models, and global case studies have all been used as approaches to study the effects of human behavior on hydrology. With sufficient training data, we believe tools like machine learning could be used to further explore how behaviors influence adaptation and to anticipate shifts as snow loss continues.

Archetypes in Practice

By evaluating how physical factors, governance systems, and human behavior shape outcomes across places like the Walker, South Platte, and San Joaquin basins, researchers and practitioners can establish archetypes to help identify patterns in what strategies are most effective in different places and assess how to transfer lessons from one setting to another (Figure 2).

Fig. 2. An archetype-based diagnostic grounded in evaluating the physical constraints, governance, and human behavioral dynamics affecting hydrologic basins could facilitate more rapid transfer of learning about successful adaptation approaches across snowmelt-dependent agriculture in the western United States.

The Walker River Basin exemplifies an archetype common to agriculturally dominated headwaters in the western United States with low governance complexity (few jurisdictions), adequate capacity (resources), low behavioral complexity (more predictable and unified user groups), and substantial physical constraints (significant future snow loss and limited infrastructure for water storage and supplementation).

With this profile, the Walker is an ideal testing ground for evaluating how effectively different strategies offset changes in snowmelt. Does cloud seeding increase snowpack? Could beaver dam analogues—a nature-based solution reminiscent of Idaho Fish and Game’s mid-20th century effort to parachute beavers into the wilderness—meaningfully increase water retention? Could multibenefit land repurposing buffer people and ecosystems against supply volatility while restoring ecosystem functionality?

The value of organizing operational contexts by archetypes is that each context need not be treated as unique.

The value of organizing operational contexts by archetypes is that each context need not be treated as unique. Lessons learned from the Walker could be systematically transferred to other areas with similar characteristics and could be incrementally tested in others.

The South Platte has physical constraints similar to Walker’s but features greater governance complexity because of multiple interstate compacts, as well as greater behavioral complexity. Modeling analyses indicate that demand-side strategies could adapt to more volatile water supply in the South Platte [Gharib et al., 2023]. But implementing them requires balancing perspectives from both agricultural and urban water users—a behavioral dynamic absent in Walker.

Crop switching to cultivate higher-value crops on less acreage could reduce water use. However, options for what crops can be grown where are constrained by factors like elevation and climate. Even where feasible, new crops would require investments in education, new infrastructure, risk management, and agronomic knowledge.

Through iterative expansion and testing, broad archetypes like “high behavioral complexity” could be specified to reflect dynamics like rural-urban competition or concerns around buy-and-dry economics. Archetypes may also point to contexts where governance complexity signals that decisionmaking is occurring above the lowest appropriate level.

Agricultural fields line a canal in California’s San Joaquin Valley. Credit: Don Graham/Flickr, CC BY-SA 2.0

The San Joaquin, with its extremely complex governance involving numerous local, state, and federal agencies managing surface and groundwater, is one potential example. Recognizing this pattern can help identify where substantial resources and long timelines may be required to implement programs (e.g., LandFlex) requiring legislative authorization, multiagency coordination, and stakeholder engagement. It may also signal the need to identify smaller operational contexts within larger settings so implementations proceed more rapidly.

Operationalizing Archetypes from Diagnosis to Action

Developing a systematic approach to match adaptation strategies with areas where they are most likely to succeed in operation is only a first step. Applying diagnostics without mechanisms to implement new strategies is often insufficient to drive timely action.

An instructive precedent of success in water quality management comes from the 1970s. By then, pollution controls on factories had improved compared with the early 20th century, yet water quality in surface waters across the country still declined because of pollution in agricultural runoff. The breakthrough came with the EPA’s total maximum daily load (TMDL) program, which created a structured process that set measurable goals for reducing pollution and assigned responsibility for meeting those goals to the sources of the pollution, allowing for local control over adaptation.

Archetypes could play a similar role in facilitating beneficial snow-loss adaptations, and a structure like the TMDL program could start by assessing supply-demand risks across operational areas, setting performance targets such as reservoir reliability and shortage frequency, and then using the diagnostic to identify which strategies fit each archetype. Results and lessons could be shared region-wide, while implementation would remain locally driven.

This suggestion is, emphatically, not a prescription for specific policy mechanisms. But it serves as a reminder that—just as few of us engage with workplace assessments or change behavior on the basis of their results without organizational support—archetypes will need to be paired with implementation structures to translate diagnosis into action.

Beyond Silver Bullets

There is no single answer to our trillion-dollar question, but one path forward for sustaining complex Western ecosystems lies in developing archetypes of different types of basins.

Nearly 20 years ago, Ostrom [2007] warned against seeking panaceas for complex environmental problems. There is no silver bullet for snow loss or single answer to our trillion-dollar question, but one path forward for sustaining complex Western ecosystems lies in developing archetypes of different types of basins.

A small irrigation district, for example, wouldn’t need to independently test every strategy in Figure 1 or develop complex decision support tools when a similar archetype already evaluated which strategies work under comparable governance, behavioral, and physical conditions.

Critically, these archetypes can be developed and refined by managers and scientists to capture more nuanced realities. Physically constrained systems, for example, could include areas facing high future uncertainty or limited reservoir flexibility. Governance and behavioral dimensions could likewise evolve to represent contexts where subsidies lead to incoherent incentives or where cultural norms link water use to local identities and traditions.

Like workplace assessments, the goal isn’t to diminish unique personalities but to work with them more strategically. Archetypes can show where we don’t need to reinvent the wheel to adapt and where the wheel might need to be tweaked. By leveraging collective knowledge and learning across regions facing similar challenges, rather than crafting new solutions basin by basin, we can reduce the time and resources needed to implement equitable and sustainable adaptation solutions.

Acknowledgments

This work is supported by the National Science Foundation (NSF) under grants 1828902 and OIA-2148788. Where We Live is funded by a grant from NSF’s Established Program to Stimulate Competitive Research (EPSCoR) RII Track-2 program and features partnerships across the University of Idaho (award 2316126); the University of Nevada, Reno (award 2316127); and the University of South Carolina (award 2316128). Work was also supported by internal funds from the Division of Hydrologic Resources at the Desert Research Institute.

References

Boisramé, G. F., et al. (2026), Think globally, model locally: Complex responses of agricultural water supplies to different climate projections, J. Am. Water Resour. Assoc., 62(3), e70117, https://doi.org/10.1111/1752-1688.70117.

Di Baldassarre, G., et al. (2018), Water shortages worsened by reservoir effects, Nat. Sustainability, 1(11), 617–622, https://doi.org/10.1038/s41893-018-0159-0.

Garcia, M., et al. (2019), Towards urban water sustainability: Analyzing management transitions in Miami, Las Vegas, and Los Angeles, Global Environ. Change, 58, 101967, https://doi.org/10.1016/j.gloenvcha.2019.101967.

Gharib, A. A., et al. (2023), Assessment of vulnerability to water shortage in semi-arid river basins: The value of demand reduction and storage capacity, Sci. Total Environ., 871, 161964, https://doi.org/10.1016/j.scitotenv.2023.161964.

Gordon, B. L., et al. (2024), The essential role of local context in shaping risk and risk reduction strategies for snowmelt‐dependent irrigated agriculture, Earth’s Future, 12(6), e2024EF004577, https://doi.org/10.1029/2024EF004577.

Grafton, R. Q., et al. (2018), The paradox of irrigation efficiency, Science, 361(6404), 748–750, https://doi.org/10.1126/science.aat9314.

Ostrom, E. (2007), A diagnostic approach for going beyond panaceas, Proc. Natl. Acad. Sci. U. S. A., 104(39), 15,181–15,187, https://doi.org/10.1073/pnas.0702288104.

Qin, Y., et al. (2020), Agricultural risks from changing snowmelt, Nat. Clim. Change, 10, 459–465, https://doi.org/10.1038/s41558-020-0746-8.

Siddik, M. A. B., et al. (2023), Interbasin water transfers in the United States and Canada, Sci. Data, 10, 27, https://doi.org/10.1038/s41597-023-01935-4.

Sietz, D., et al. (2019), Archetype analysis in sustainability research: Methodological portfolio and analytical frontiers, Ecol. Soc., 24(3), 34, www.jstor.org/stable/26796999.

Steyaert, J. C., et al. (2022), ResOpsUS, a dataset of historical reservoir operations in the contiguous United States, Sci. Data, 9, 34, https://doi.org/10.1038/s41597-022-01134-7.

Sturm, M., et al. (2017), Water and life from snow: A trillion dollar science question, Water Resour. Res., 53(5), 3,534–3,544, https://doi.org/10.1002/2017WR020840.

Author Information

Beatrice L. Gordon (beatrice.gordon@dri.edu), Gabrielle F. S. Boisrame, Christine M. Albano, and Rosemary W. H. Carroll, Desert Research Institute, Reno, Nev.; and Adrian A. Harpold, University of Nevada, Reno

Citation: Gordon, B. L., G. F. S. Boisrame, C. M. Albano, R. W. H. Carroll, and A. A. Harpold (2026), Archetypes could accelerate agricultural adaptation to less snowpack, Eos, 107, https://doi.org/10.1029/2026EO260184. Published on 9 June 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.

Reports of landslides triggered by the 8 June 2026 M=7.8 earthquake offshore Mindanao in the Philippines

Tue, 06/09/2026 - 07:31

To date news reports suggest two fatal landslides with a combined toll of 17 people.

There are various news reports trickling in about the landslides triggered by the 8 June 2026 M=7.8 earthquake offshore Mindanao in the Philippines. As usual, the remote locations of many of the landslides means that the information is a bit hit and miss at this point.

To date, the most serious event appears to have occurred at a community called New Aklan, located in Glan, Sarangani. It appears that New Aklan is at: [5.7705 N, 125.3356]. News reports indicate that 13 people were killed, although there are also indications of additional fatalities in this area.

A further four people are missing under a landslide at Sitio Buhangin, Barangay Patuco, Sarangani. Patuco is in the area of [5.4770, 125.4859]. This appears to have been a failure on a coastal cliff:-

A failure in a coastal cliff at Sitio Buhangin, Barangay Patuco, Sarangani following the 8 June 2026 earthquake near Mindanao. Image tweeted by Radyo Pilipinas.

Over the next few days, satellite imagery should become available that will help identify the landslide impacts, but in the meantime Dan Shugar has identified some (using Planet imagery, I’d imagine):-

Return to The Landslide Blog homepage 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.

Rocket Launches and Reentries Harm Earth’s Ozone Layer

Mon, 06/08/2026 - 13:23
Source: Earth’s Future

The space industry is surging. In coming years, nearly 10,000 spacecraft are slated to launch into low-Earth orbit for a variety of purposes, such as global surveillance, space tourism, and satellite “megaconstellations” providing internet service.

Rocket engine exhaust, as well as the burnup of inactive satellites and rocket parts reentering Earth’s atmosphere, releases a suite of pollutants. These chemicals have long been considered to pose little threat to our climate, given the historically small size of the space industry. Now, the sector’s rapid growth will send its emissions skyrocketing—but scientists don’t yet have a clear picture of the environmental ramifications.

An analysis by Vliex et al. of rockets launched in 2022 revealed that spaceflight depletes the ozone layer and contributes to global warming, with a significant portion of this ozone loss attributable to nitrogen oxide emissions released by objects reentering Earth’s atmosphere.

The researchers calculated emissions from all 186 rockets launched in 2022, as well as all 472 objects—with a combined total mass of nearly 5,000 tons—that reentered the atmosphere that year. They conducted computational simulations of each launch’s trajectory and emissions at various altitudes up to 100 kilometers, and they calculated emissions released by object reentry. They also accounted for the effects of chemical reactions that occur in rocket exhaust plumes, which alter emissions’ chemical composition.

Incorporation of the calculated emissions into GEOS-Chem, a computational model of atmospheric chemistry, revealed their ozone-depleting and Earth-warming effects, with reentry emissions identified as playing a key role in ozone depletion. The researchers found that accounting for plume reactions reduced the estimated effects of spaceflight emissions, highlighting the value of considering plume chemistry in future assessments.

The analysis also underscored the varying effects of different rocket fuel types. Solid-state fuels, used recently in rocket boosters for NASA’s Artemis II mission to return astronauts to the Moon, appeared to cause the greatest amount of ozone depletion relative to propellant mass, while rocket-grade kerosene caused the greatest amount of warming.

On the basis of their findings, the researchers call for further research into reentry emissions and rocket plume chemistry as the space industry continues to expand and evolve. (Earth’s Future, https://doi.org/10.1029/2025EF007795, 2026)

—Sarah Stanley, Science Writer

Citation: Stanley, S. (2026), Rocket launches and reentries harm Earth’s ozone layer, Eos, 107, https://doi.org/10.1029/2026EO260183. Published on 8 June 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.

Potential landslides and liquefaction from the 8 June 2026 M=7.8 earthquake offshore Mindanao in the Philippines

Mon, 06/08/2026 - 07:19

Initial analyses suggest that the earthquake this morning has the potential to have triggered significant numbers of landslides and areas of liquefaction.

At the time of writing, the impacts of the M=7.8 earthquake that occurred offshore the south coast of Mindanao in the Philippines remain unclear. Initial reports in the local press suggest 15 fatalities so far, but as always it could be the case that there is no information from those areas most seriously impacted.

The USGS Pager site is the best source of information about potential landslide impacts, bearing in mind there is a high level of uncertainty. This estimates that the area exposed to landslides is at the high end of the “significant” scale and that the population exposed to landslides lies in the 1,000 to 10,000 people range. This is the Pager landslide hazard map:-

Initial Pager map of landslide hazard from the 8 June 2026 earthquake offshore Mindanao in the Philippines. Source: USGS.

The area with the highest level of landslide hazard is remote and rural, so we may not get good information from this area for a while.

The potential for liquefaction may be even more serious, with a broad swathe having a high level of hazard:-

Initial Pager map of liquefaction hazard from the 8 June 2026 earthquake offshore Mindanao in the Philippines. Source: USGS.

Past earthquakes have generated large liquefaction-related landslides on low angle slopes, with devastating effects. Hopefully, there won’t have been an event on this scale in Mindanao.

One final point to note is that the Philippines is just entering the typhoon season. Fortunately, Mindanao is sufficiently far south to be away from the main typhoon zone. However, these storms are so large that they can bring very heavy rainfall – see for example Typhoon Bopha in 2012. A similar event this year could have very significant consequences.

Return to The Landslide Blog homepage 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.

Theme by Danetsoft and Danang Probo Sayekti inspired by Maksimer