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Getting to Know Uranus’s “Breathing” Bow Shock

EOS - Fri, 08/07/2026 - 12:02
Source: AGU Advances

Within our solar system, Uranus is a geometric oddball. Its spin axis tilts more than 90° from its orbit, so it essentially rolls on its side through space. In contrast, Earth and other planets tilt only moderately or not at all. What’s more, the ice giant’s magnetic field is strangely offset and tilted another 60°.

These extreme asymmetries mean that the interaction between Uranus’s magnetic field and the solar wind—charged particles constantly streaming out from the Sun in all directions—is also quirky. At Earth and other planets, the boundary where the solar wind slams into the planetary magnetic field and abruptly slows to form a turbulent shock wave, known as the bow shock, is relatively stable. But at Uranus, the bow shock is highly dynamic, changing shape and size throughout each Uranian day, like the expansion and contraction of breathing lungs.

However, the precise extent and underlying drivers of the Uranian bow shock’s “breathing” have so far been unclear. Now, using advanced computer simulations and data from NASA’s Voyager 2 spacecraft, Cao et al. have quantified the specifics of these daily, repeating changes.

The researchers used a three-dimensional multifluid magnetohydrodynamic model, a tool they recently developed to explore how planets’ magnetospheres interact with the solar wind. For these simulations, they incorporated observations made by Voyager 2 in 1986 when it flew by Uranus. They ran the model under the condition of Uranus’s equinox, the part of its 84-Earth-year orbit during which the Sun is directly over the equator and the bow shock’s expansion and contraction are strongest.

The simulations revealed precisely how the bow shock of Uranus evolves in size and shape over the course of one full day. To isolate the role of planetary rotation, the researchers ran some simulations under conditions of steady, unchanging solar wind. The regular, daily pattern persisted, suggesting that rotation-driven daily reconfiguration of the magnetic field geometry, rather than solar wind changes, is primarily responsible for the breathing.

In contrast, at Earth, solar wind changes are the main driver of variability in the bow shock, with only small daily variations arising from the slight angle between Earth’s spin axis and its magnetic field.

These findings could help inform future space missions to Uranus and could aid in understanding the bow shocks of the numerous ice giant exoplanets detected throughout the galaxy. (AGU Advances, https://doi.org/10.1029/2026AV002307, 2026)

—Sarah Stanley, Science Writer

Citation: Stanley, S. (2026), Getting to know Uranus’s “breathing” bow shock, Eos, 107, https://doi.org/10.1029/2026EO260255. Published on 7 August 2026. Text © 2026. AGU. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

A Rare Look at How Life First Colonizes Cooling Lava Tubes

EOS - Fri, 08/07/2026 - 12:00

When the Tajogaite volcano erupted on the Spanish island of La Palma in 2021, it changed the local landscape almost overnight. What started as a small fissure spewing gas and volcanic ash soon grew into a massive volcanic cone. Lava flows destroyed hundreds of homes and basic infrastructure such as roads and water pipes, but they also created a natural laboratory for scientists.

Tajogaite erupted in September 2021. Credit: Eduardo Robaina/Wikimedia Commons, CC BY-SA 3.0

As the lava cooled and slowed on the surface, molten rock continued to flow through channels under the surface. Once the eruption ceased and the lava drained out, the empty tubes remained, forming a tunnel network. Between 12 and 24 months after the eruption, a team of researchers went onto the still cooling lava tubes of La Palma to study how life gets its first foothold and colonizes these newly created environments.

Numerous studies have investigated how life takes hold on new surface lava, and mature microbial communities in lava tubes have also been studied in the past, but this is the first time the colonization process has been studied underground from the very beginning, the researchers said. It could help researchers learn more not just about terrestrial lava tubes but about those on Mars or the Moon.

This photo was taken from the interior of a lava tube formed during the eruption of Tajogaite, including white mineral deposits coating the walls. Credit: Nicasio Jiménez

“This is a unique opportunity; we are studying nature’s blank pages,” said Ana Miller, a geomicrobiologist at the Institute of Natural Resources and Agrobiology of Seville in Spain who led the study published in Environmental Microbiome.

The tubes formed by the Tajogaite eruption were sometimes tall enough for a person to walk upright through them. But the temperatures could be uncomfortably hot, even after toxic gases had dissipated and initial temperatures cooled from upward of 800°C (1472°F). In some sampling sites, air temperatures hovered at a blow-dryer hot 60°C (140°F), while rock surfaces reached 90°C (194°F).

Yet even in such inhospitable conditions, the researchers found adventurous microorganisms already dwelling in the caves and, in some cases, altering the rock.

The Lucky Few

Though these passages are underground, they aren’t entirely sealed from the outside world. In some locations, sections of the tubes collapsed, or bubbling lava created holes in the roofs of the lava flows, known as skylights. Cracks in the rock also allow rainwater to enter the caves.

These openings are entry points for the first colonizers, which are carried by wind and rain or transported by living collaborators, such as birds, rodents, insects, and even worms. The microorganisms are accompanied by a nutrient cache of decaying vegetation, feathers, and guano.

On the basis of previous studies, the researchers thought that only the highly specialized microorganisms that can extract energy from chemical reactions with minerals—known as chemolithotrophs—could survive these early stages. The results at Tajogaite, however, show this isn’t entirely true.

Researchers explore the interior of a lava tube known as “Tubo Rojo,” which formed during the Tajogaite eruption. Credit: Nicasio Jiménez

The team collected scrapings from the cave floors and walls, combining traditional laboratory cultures with advanced genetic sequencing, and found that the microbial communities were not uniform. If light or organic matter was available, opportunistic organisms prevailed, with random luck playing a role in which species made it into the caves—a process called stochastic seeding. However, the harsh interior conditions of the lava tubes decided which microorganisms survived over the long term, favoring highly specialized species adapted to extreme environments. Deep within the caves, where there is no organic input, no light, and very little humidity, only these specialists survived.

The rapidly changing environment in the caves likely also influences the colonization process. “In a newly formed tube, the rock is still cooling down,” said Francesco Sauro, a geologist at the University of Padua in Italy who wasn’t involved with the new study. “You have cracking of the lava linings on the walls, collapses, and a lot of secondary mineralization that is metastable—meaning it exists only at that specific condition of temperature and humidity.”

This close-up shot shows some of the details of the lava formations within Tubo Rojo. Credit: Octavio Fernández

In contrast to mature lava tubes that formed thousands of years ago, which present stable conditions and mature microbial communities that are in equilibrium with the environment, young ones like those in La Palma evolve rapidly. “If you go back to Tajogaite or Iceland after 2, 5, or 10 years,” Sauro said, “the community will have changed for sure.”

Leaving Their Mark

“It isn’t just a case of microbes arriving, depositing on the walls, and surviving. To survive, they must interact with the volcanic substrate.”

Using electron microscopy, the team also found that the organisms are already dissolving and creating new minerals out of the rock.

“The microscopy helps us see if the microorganisms are associated with the mineral structures,” Miller said. “It isn’t just a case of microbes arriving, depositing on the walls, and surviving. To survive, they must interact with the volcanic substrate. That activity confirms we have a community developing.”

The research team poses for a photo with their protective gear before venturing into a lava tube. Credit: Ana Miller

The researchers found that the microbes were already forming biofilms—mat-like structures that help them attach to rock. Biofilms also retain humidity, helping the microbes capture the little moisture available, along with dissolved nutrients. Subtle alterations like biofilm formation represent the very first steps of a process that, over millions of years, will eventually break the rock down to form soil, Miller said.

Mars Underground

Lava tubes like the ones created in La Palma are common features in volcanic environments both on and off Earth. These subsurface structures are considered a possible last redoubt for life on Mars, if it ever existed.

Researchers believe that these features captured by the High Resolution Stereo Camera aboard the European Space Agency’s Mars Express are lava tubes. Credit: ESA/DLR/FU Berlin (G. Neukum), CC BY-SA 3.0 IGO

One of the main controversies surrounding the idea of life in Martian lava tubes, however, is that most of the tubes that exist today formed after the planetary shift that ended habitable surface conditions on Mars roughly 3.8 billion years ago. This timing casts doubt on whether life ever had the chance to colonize them, Sauro said.

However, the larger picture is that lava tubes never stopped forming on Mars, at least throughout the first half of its history. “They were forming 4 billion years ago, and then through up to 2 billion years ago while volcanism was still active,” Sauro said.

In this way, Martian lava tubes could provide temporary “houses” that life could colonize one after the other, Sauro said. The fact that on Earth this colonization is extremely quick—not taking decades, but happening as soon as the temperature drops below a certain threshold—suggests that even young Martian lava tubes could have been rapidly colonized by surviving bacteria, Sauro said. “As soon as the lava tube is below a certain temperature and there is availability of liquid water, then it’s done.”

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

Citation: Barbuzano, J. (2026), A rare look at how life first colonizes cooling lava tubes, Eos, 107, https://doi.org/10.1029/2026EO260253. Published on 7 August 2026. Text © 2026. The authors. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

Efficient computation of stellarator coils with an augmented Lagrangian optimization method

Physical Review E (Plasma physics) - Fri, 08/07/2026 - 10:00

Author(s): Pedro F. Gil, Weiping Li, Julianne Stratton, Alan A. Kaptanoglu, and Eve V. Stenson

Finding feasible coils for stellarator fusion devices is a critical challenge of realizing this concept for future power plants. Current design efforts struggle to navigate the highly nonconvex optimization landscape, spend considerable resources scanning the parameter space, and may produce subopti…


[Phys. Rev. E 114, 025202] Published Fri Aug 07, 2026

Adding an AI tool to Google Earth shook our trust in maps that has been centuries in the making

Phys.org: Earth science - Thu, 08/06/2026 - 20:40
Throughout the 18th and 19th centuries, Europe's cartographers traded on their reputation for accuracy and detail at a time of huge societal change. But as demand grew for increasingly detailed maps of the world to support industrialization at home and colonization overseas, they didn't always get it right.

Earthquake sensors can help forecast how hurricanes intensify

Phys.org: Earth science - Thu, 08/06/2026 - 18:00
Stanford researchers have shown that instruments primarily used to understand earthquakes can capture key details about hurricanes, helping meteorologists better predict how storms will evolve and intensify.

Siberia's growing methane threat could offset 20% of global methane reduction targets by 2050

Phys.org: Earth science - Thu, 08/06/2026 - 18:00
The Arctic is warming at an accelerating pace. As permafrost thaws across vast areas and wildfires become more frequent, large amounts of methane (CH4) are being released. Together, these changes are reshaping the region's greenhouse gas emissions and further intensifying climate change.

Measurements trace European wildfire smoke high into upper troposphere

Phys.org: Earth science - Thu, 08/06/2026 - 16:40
The images of the major forest fires in Spain and France, with fire clouds near Bordeaux, have shocked many people. There have been numerous reports of the formation of a pyrocumulonimbus cloud—a fire-driven thundercloud—and the possible transport of smoke particles to Central Europe.

Giant ice mountains on the other side of Earth once dictated Australia's climate—new study

Phys.org: Earth science - Thu, 08/06/2026 - 15:40
During the most recent ice age, much of North America disappeared beneath ice sheets several kilometers thick. These frozen giants covered most of present-day Canada and parts of the northern United States, while smaller ones spread across northern Europe.

Coupled AI and physics model improves typhoon-wave height forecasting

Phys.org: Earth science - Thu, 08/06/2026 - 13:40
Typhoons pose significant threats, with sudden, dangerous waves that endanger ships, offshore platforms and coastal infrastructure in the northwest Pacific Ocean. Current typhoon forecasting methods sometimes underestimate the largest waves during typhoons, but researchers in China have designed a new model that may offer improvements. Their new study, published in Ocean Engineering, describes how the model combines physics guidance with data-driven learning to improve typhoon forecasting.

Super-Earths May Be Solid Deep Inside Their Mantles

EOS - Thu, 08/06/2026 - 13:26
Source: AGU Advances

Deep inside super-Earths—rocky planets with a mass anywhere between 1 and 10 times that of Earth—high pressure can cause familiar minerals to take forms that are rarely seen on Earth. Understanding more about the temperature and pressure conditions under which these phases are reached could help researchers learn more about how planets evolve.

One such mineral is magnesium orthosilicate, or Mg2SiO4, one of the major building blocks of rocky planets. As pressure increases deep inside a planet, the atoms in this mineral rearrange into different crystal structures. One of these high-pressure forms is called the spinel phase, which is found in Earth’s mantle. At even higher pressures, this phase breaks down into two different minerals: bridgmanite, the most abundant mineral phase in Earth, and ferropericlase, a magnesium-rich oxide. However, under the far more extreme pressures expected inside massive rocky planets known as super-Earths, Mg2SiO4 becomes stable again in an entirely new crystal structure called post-post-spinel. Scientists predict that this ultrahigh-pressure phase of Mg2SiO4 is one of the dominant minerals in the deep mantles of super-Earths, making its melting behavior important for understanding how these planets form and evolve.

Re-creating the high temperatures and extraordinary pressures inside massive rocky planets is challenging in the lab, so Zheng et al. took a computational approach. The team used a technique called thermodynamic integration to study the melting curve of post-post-spinel Mg2SiO4 at up to 1,300 gigapascals of pressure.

They found that post-post-spinel Mg2SiO4 is an exceptionally refractory mineral, meaning it can withstand extremely high temperatures before melting. Depending on the pressure, it melts at between 9,780 K and 14,897 K, significantly hotter than temperatures at which related minerals melt, including bridgmanite and MgSiO3 postperovskite, the high-pressure form of bridgmanite stable near Earth’s core-mantle boundary. Even after moderate amounts of iron were added, something that likely happens to some degree in most exoplanets, the melting point for post-post-spinel Mg2SiO4 remained above the temperatures estimated for the deep mantles of most rocky planets, the authors say.

Their results indicate that many super-Earths likely have solid deep mantles, which has implications for convection deep inside rocky exoplanets, as well as for their magnetic fields, which are created by swirling molten metals in their interiors. (AGU Advances, https://doi.org/10.1029/2026AV002326, 2026)

—Nathaniel Scharping (@nathanielscharp), Science Writer

Citation: Scharping, N. (2026), Super-Earths may be solid deep inside their mantles, Eos, 107, https://doi.org/10.1029/2026EO260256. Published on 7 August 2026. Text © 2026. AGU. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

Molecular dynamics simulations of temperature relaxation in strongly magnetized, non-neutral, equal-density two-component plasmas

Physical Review E (Plasma physics) - Thu, 08/06/2026 - 10:00

Author(s): James C. Welch, III, Louis Jose, Timothy D. Tharp, and Scott D. Baalrud

An important process for antimatter experiments is the cooling of particles in a Penning-Malmberg trap to experimentally useful temperatures. A non-neutral plasma of one species (e.g., antiprotons) can be collisionally cooled on another colder species (e.g., electrons). Modeling temperature relaxati…


[Phys. Rev. E 114, 025201] Published Thu Aug 06, 2026

Fatal landslides in July 2026

EOS - Thu, 08/06/2026 - 06:31

In July 2026 I recorded 48 fatal landslides causing 413 fatalities. This year continues to be atypical in terms of the temporal pattern of fatal landslides.

This is my regular update for the number of fatal global landslides, focusing on July 2026. As usual, this data has been collected in line with the methodology described in Froude and Petley (2018) and in Petley (2012). References are listed below – please cite these articles if you use this analysis. Data presented in these updates should be treated as being provisional at this stage as I will reanalyse them prior to formal publication, and other events will emerge.

Note that this data excludes landslides triggered by earthquakes.

The headline figures are as follows:

July 2026: 100 fatal landslides causing 413 fatalities.

This is the number of landslides by month in 2026 to the end of July:-

The number of global fatal landslides in 2026 by month to the end of July.

We saw a massive uptick in fatal landslide occurrence in July 2026; indeed, this is the first time I have recorded 100 or more landslides in that month, and it is the third highest total in my dataset. This largely reflects an intense start to the South Asian Summer Monsoon.

My preferred way of presenting this data us to use the cumulative total by pentad. This graph is to pentad 42, which captures almost all of the July data (two landslides that occurred on 31 July 2026 are not included):-

The cumulative total number of global fatal landslides in 2026 by pentad to the end of July.

The steepening of the curve that is associated with the Northern Hemisphere rainy season is evident. 2026 continues to run a long way above the long term mean, and very close to the record year of 2024, even though the monthly pattern is markedly different.

It will be interesting to see what August 2026 brings.

References

Froude, M. and Petley, D.N. 2018.  Global fatal landslide occurrence from 2004 to 2016.  Natural Hazards and Earth System Sciences 18, 2161-2181.

Petley, D.N. 2012. Global patterns of loss of life from landslidesGeology 40 (10), 927-930.

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

Climate Change Made This Summer’s Canadian Wildfires Twice as Likely

EOS - Thu, 08/06/2026 - 04:01
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.

Wildfires in the Canadian provinces of Ontario and the Northwest Territories have burned more than 3.9 million hectares this summer, prompted widespread evacuation orders, and created poor air quality for not only Canadians, but more than 120 million people across the midwestern and northeastern United States. The fires spread exceptionally quickly, stressing the resources of local response agencies. About 700 fires are still active across Canada.

 “The impacts of climate change are very real, and we can quantify what those are and the extent to which they have become more serious.”

According to a new analysis, human-induced climate change and its contribution to fire conditions across Canada made these fires twice as likely to occur. The report is from World Weather Attribution, an international climate science partnership. 

The analysis is an attribution study, which determines the extent to which climate change is responsible for a specific extreme weather event. Current science is best at determining climate change’s role in driving extreme temperatures and precipitation events, but wildfires are more difficult to attribute to climate change due to the many factors that drive their occurrence. Still, scientists’ attribution methods have greatly improved over the past decade, according to a recent report

“The impacts of climate change are very real, and we can quantify what those are and the extent to which they have become more serious,” said Theodore Keeping, a climate scientist at Imperial College London and coauthor of the new report.

Detected fire activity in Canada from 1-18 July, 2026. Study regions for the new World Weather Attribution analysis are represented by the two boxes overlaying the Northwest Territories and Ontario. Credit: World Weather Attribution

To determine the role of climate change in driving this summer’s Canadian wildfires, the research team analyzed the so-called Daily Severity Rating (DSR), a measure of fire weather that reflects how difficult it is to suppress a fire once it ignites. Using climate models, the team tested the likelihood that similar DSRs to those present in Ontario and the Northwest Territories this summer would occur in a hypothetical world without human-caused climate change.

Researchers determined that the sustained, severe DSRs present in Ontario and the Northwest Territories in July were made about twice as likely by climate change. The worst of the fire weather, a particularly high-DSR week in the Northwest Territories, was made about 27 times more likely by climate change, according to the researchers. 

However, such fire weather is “no longer rare in today’s climate,” the authors wrote. In a world without human-caused climate change, similar extreme fire events would have been expected about every 40 years. In our warming world, though, such fires are expected to occur every 2-6 years in the Northwest Territories and every 6-15 years in Ontario. 

Though a doubling of the likelihood of extreme fires may sound small, “a small change makes a huge difference for an ecosystem and a community,” said Frederike Otto, scientific lead of WWA and coauthor of the new report, in a press conference. The Canadian fires, she said, are “incredibly hard to suppress with the available people power and available technology. Even if [things get] just a little bit worse, it would mean that everything is stretched further.” 

Frequent Fires, Vulnerable People

The increasing occurrence of destructive fires means some communities are facing displacement repeatedly, especially as the last three fire seasons in Canada have been “exceptionally severe,” the authors wrote. 

Repeated extreme fire events make it difficult for communities to recover, and Indigenous communities are particularly vulnerable because they’re overrepresented in fire-prone areas. One 2024 study, for example, found that though Indigenous communities are only about 5% of Canada’s population, they made up 42% of its wildfire evacuations between 1980 and 2021. Fires in Ontario this summer have put thirteen First Nations communities under evacuation orders.

 
Related

“Repeated displacement can disrupt cultural practices of Indigenous communities, as well as access to hunting grounds and traditional food,” said Chris Boyer, technical advisor and climate scientist at the Red Cross Red Crescent Climate Centre and coauthor of the new analysis, in a press conference. “Some of these communities are also dealing with the shortened response and recovery times between disasters due to the recent successive wildfires affecting longer-term resilience.”

“If you care about anyone but the super-rich, you have to stop burning fossil fuels,” Otto said. “The most vulnerable are hit hardest.”

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

These updates are made possible through information from the scientific community. Do you have a story about science or scientists? Send us a tip at eos@agu.org. Text © 2026. AGU. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

Damaging coastal storm conditions have become twice as frequent at a New Jersey Beach since 1979

Phys.org: Earth science - Wed, 08/05/2026 - 22:00
Storm conditions capable of causing major coastal erosion at New Jersey's North Beach on Sandy Hook are occurring about twice as often as they did in 1979, according to Rutgers researchers. The finding offers new evidence that storm impacts are becoming more frequent along the Mid-Atlantic coast.

Human activity more than doubles Arctic fire occurrence, satellite analysis suggests

Phys.org: Earth science - Wed, 08/05/2026 - 15:20
Fires in the Arctic are not solely a regional issue, as shown by the hazy skies in Switzerland last summer despite otherwise sunny weather. Smoke from major fires in northern Canada crossed the Atlantic and reached Europe. Until now, large-scale studies of Arctic tundra fires have focused primarily on rising temperatures and drought as the main drivers. The role of human activity has received much less attention, even as industrial development, settlements, roads and other infrastructure expand rapidly in parts of the Arctic, particularly in connection with extractive industries such as oil and gas production and mining.

Avalanche cracks may appear globally supersonic while remaining locally subsonic

Phys.org: Earth science - Wed, 08/05/2026 - 15:00
Can a crack be supersonic? Can the fracture that triggers an avalanche propagate faster than the limiting velocity predicted by classical fracture mechanics? The question remains the subject of debate within the scientific community. While some numerical and experimental studies suggest that avalanche cracks may propagate at supersonic speeds, others offer a different interpretation.

How Bubbles Reshape Air-Sea Gas Exchange

EOS - Wed, 08/05/2026 - 14:00
Editors’ Vox is a blog from AGU’s Publications Department.

Air-sea gas exchange regulates climate and ocean biogeochemistry. A new article in Reviews of Geophysics brings together theories, laboratory experiments, field observations, and models to explain how bubbles contribute to this exchange, why their effects differ among gases, and what scientists still need to learn. Here, we asked the lead author about some of the key concepts and challenges explored in the review article, and future directions for research.

What is air-sea gas exchange, and why is it important?

Air-sea gas exchange is the movement of gases between the atmosphere and the ocean. Carbon dioxide enters and leaves the ocean through this process, and the global ocean takes up a quarter of human-emitted CO2 through this exchange. The same process regulates the air-sea exchange of oxygen and many other climatically and biologically important gases. Gas exchange is therefore central to understanding climate, marine ecosystems, and the global carbon cycle. However, the ocean surface is not a simple, flat boundary. Wind, waves, turbulence, temperature differences, surface films, rain, and bubbles all influence how rapidly gases cross it.

A schematic of air-sea gas exchange, comprising interfacial transfer (orange arrow) and bubble-mediated transfer (yellow arrows, invasion scenario). Various physical processes govern the air-sea gas exchange. Credit: Dong et al. [2026], Figure 1

In simple terms, what is bubble-mediated gas transfer?

When waves break, they trap air beneath the sea surface and create clouds of bubbles. Gas can then move between the air inside each bubble and the surrounding seawater. This creates an additional exchange pathway beyond transfer directly across the ocean surface.

A bubble is not simply a piece of the atmosphere placed underwater. Water pressure and surface tension compress the gas inside it, while the bubble’s size, depth, and lifetime continually change. Some bubbles dissolve completely; others rise and burst at the surface. During this journey, gases can enter or leave the surrounding water. The combined effect of millions of short-lived bubbles can substantially influence gas exchange, particularly during strong winds and energetic wave breaking.

How does bubble-mediated transfer differ from interfacial transfer?

Interfacial transfer occurs directly across the boundary between air and water. It is controlled mainly by wind-driven turbulence close to the surface and by how rapidly a gas moves through the thin layers of air and water on either side.

Bubble-mediated transfer has three distinctive properties. First, it is directly linked with the wave breaking, which has a nonlinear dependence on the wind speed. Second, it depends on gas solubility. A highly soluble gas can approach equilibrium within a bubble quickly, whereas a poorly soluble gas may continue to transfer throughout the bubble’s lifetime. Third, submerged bubbles are compressed, so the gas inside them is slightly over-pressured. This can favor gas entering the ocean over gas leaving it. Consequently, bubbles may change not only the rate of exchange but also the apparent equilibrium between the ocean and atmosphere.

How do scientists study the effects of bubbles?

No single method can fully describe bubble-mediated gas exchange due to its complex properties, so researchers combine several approaches. Laboratory wind-wave tanks allow controlled experiments in which wind, waves, bubble populations, and gas solubilities can be varied. Field techniques include measuring the saturation states of inert gases and directly measuring turbulent gas fluxes above the sea using the eddy covariance technique. Different gases act as complementary tracers because their solubilities and molecular properties differ. Noble gases, oxygen, carbon dioxide, and dimethyl sulfide can therefore reveal different parts of the exchange process. Finally, physical models resolve the bubble dynamics and combine with gas exchange processes, providing independent constraint and a testbed for bubble-mediated gas exchange. To provide the bubble dynamic information, researchers use acoustic and optical instruments to measure bubbles and wave breaking.

Approaches to studying bubble-mediated gas transfer. Left: field observations in the natural ocean, including measurements of multiple gases with different solubilities and upper-ocean bubble dynamics. Right: laboratory experiments conducted under controlled conditions to investigate the underlying mechanisms. Middle: physically based bubble models that connect and inform both field observations and laboratory experiments. Credit: Dong et al. [2026], Figure 9

Why is bubble-mediated transfer difficult to quantify?

First, the underlying processes are highly complex. Accurate simulation requires understanding and representing the full sequence from wave development and breaking to air entrainment, bubble-size distributions, bubble cloud movement, and gas exchange between individual bubbles and seawater. Uncertainty at any stage can propagate into the final transfer estimate.

Second, observations are difficult. Bubble-mediated exchange is more significant under high winds and intense wave breaking, when field measurements are most challenging and remain scarce. Measuring bubbles very close to an active sea surface is especially difficult and such measurements are crucial to validating models. Traditional linear wind-wave tanks also have limited breaking capacity, fetch, and water depth, making it difficult to reproduce open-ocean conditions.

Third, bubble-mediated and interfacial transfer occur simultaneously and their separation is difficult. Interpretation of measurements and the scaling from one gas to another is difficult, complicated by the dependence of the bubble contribution on solubility.

What are the most important remaining research questions?

Three questions are especially important. First, we need to understand what happens to bubbles in the uppermost meter of the real ocean: how much air is injected (bubble volume), how bubble sizes are distributed, and how bubble clouds are influenced by upper ocean water movement.

Second, we need to determine how bubble-mediated transfer changes across gases with different solubilities. This is essential for transferring knowledge from commonly studied gases to climate-relevant gases such as CO2 and O2.

Third, we need to explain why laboratory experiments and field observations often produce different estimates of the bubble contribution. Progress will require coordinated measurements of near-surface bubble properties and the exchange of several gases with contrasting solubilities across laboratory and ocean environments. These observations should ultimately be used to develop physically based parameterizations for ocean biogeochemical and Earth system models.

—Yuanxu Dong (Yuanxu.Dong@lmd.ipsl.fr, 0000-0002-1468-1623), completed this work while affiliated with GEOMAR Helmholtz Centre for Ocean Research Kiel and Heidelberg University. He is now at LMD-IPSL, École Normale Supérieure-PSL, École polytechnique, Institut Polytechnique de Paris, Sorbonne Université, CNRS, Paris France

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

Citation: Dong, Y. (2026), How bubbles reshape air-sea gas exchange, Eos, 107, https://doi.org/10.1029/2026EO265028. Published on 5 August 2026. This article does not represent the opinion of AGU, Eos, or any of its affiliates. It is solely the opinion of the author(s). Text © 2026. The authors. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

A Hybrid Approach for Revealing Headwater Hydrology

EOS - Wed, 08/05/2026 - 13:17

Earth’s rivers, modest and mighty alike, all have humble beginnings in small rain-, snowmelt-, and groundwater-fed headwaters. These streams deliver nutrients and sediment to larger waterways downstream, provide critical habitat for numerous species, and make up more than 70% of total stream length globally. Yet they are among the least known components of river networks.

Gauges used to measure streamflow are disproportionately placed in large, perennial rivers, leaving headwater systems largely unmonitored.

This lack of knowledge stems in part from the fact that stream gauges used to measure streamflow are disproportionately placed in large, perennial rivers, leaving headwater systems largely unmonitored.

Better documenting and understanding these systems’ behavior could improve predictions of downstream effects of changing precipitation patterns and snowmelt timings, which are already subjecting communities to unprecedented risks including historic floods, droughts, and structural failures. It could also increase the accuracy of water availability estimates for agricultural planning, ecological water needs assessments, and downstream water quality management.

Novel monitoring approaches that document when water is present and provide flow estimates are beginning to fill data gaps for headwater streams. Pairing such observations with emerging hybrid modeling approaches, which combine physics‑based model components with data‑driven machine learning, could dramatically improve both understanding of headwater processes and fine-scale predictions of water availability in headwater systems.

Progress, until recently, has been limited mainly by the difficulties of bringing fragmented observations together and connecting observational and modeling research communities. But emerging tools and coordinated efforts are helping to overcome these limitations.

Bridging Gaps Between Data and Models

The contemporary study of headwater hydrology has advanced along two largely parallel tracks. Expanding observational networks, including community science programs and low-cost camera and sensor systems, are documenting when headwater streams flow and, in some cases, their approximate stage (water height) and discharge. At the same time, increasingly sophisticated physics-based models are simulating runoff, snow dynamics, and subsurface storage using the highest-resolution meteorological data available as input.

  • Headwater streams across the United States occur in a variety of landscapes and have diverse characteristics. Whereas some flow all the time (perennial), others flow only seasonally (intermittent) or after storms (ephemeral). Likewise, some streams have relatively fixed paths, while others migrate. Headwaters also differ in their “order,” with hillslopes generating first-order streams that merge to form second-order streams, and so on. Here, an intermittent first-order tributary of Shaker Creek in Warren County, Ohio, runs over Ordovician limestone and shale in a suburban park. It has a drainage area of 1.2 square kilometers. Credit: Jay Christensen
  • Kanarra Creek, a perennial third-order stream, runs through a sandstone canyon in Iron County, Utah, just northwest of Zion National Park and drains a 20.5-square-kilometer catchment. Credit: Jay Christensen
  • An ephemeral first-order tributary of Salado Creek in Bexar County, Texas, drains a 0.1-square-kilometer area of Cretaceous limestone and marine sediment. Credit: Jay Christensen
  • This dry, ephemeral second-order tributary in Little Rock Canyon in Utah County, Utah, drains 5 square kilometers amid the limestone bedrock slopes of the Wasatch Mountains. Credit: Samuel Christensen
  • This perennial second-order tributary of Big Fiery Gizzard Creek in Marion County, Tennessee, drains an area of 2.5 square kilometers and flows through sandstone and shale of the Cumberland Plateau. Credit: Jay Christensen
  • A perennial second-order tributary of Lookout Creek in Lane County, Oregon, drains a 1-square-kilometer area of weathered basalts in the H. J. Andrews Experimental Forest. Credit: Jay Christensen

Headwater modeling is still limited, however, by the spatial resolution of precipitation and snowmelt estimates, because small stream channels respond to spatial variability in weather that is often unresolved in current meteorological datasets. The coarse spatial resolution of soil and geological datasets, which capture landscape characteristics that influence streamflow, are also limiting. Bridging this mismatch of scales would help to increase the accuracy of headwater modeling.

Physics-based models capture basin-scale dynamics and water balances and offer the benefits of transparency and physical grounding in the laws of nature. However, they are often unable to resolve fine-scale intermittency in streamflows and extreme conditions in small basins. They also often rely only on stream gauges and do not incorporate irregular and heterogeneous data types more commonly collected in headwaters.

Artificial intelligence and machine learning (ML) models, which have rapidly improved weather forecasting, offer flexibility and can learn complex relationships directly from data. But most applications for stream hydrology depend heavily on continuous discharge records, which are typically sparse in headwater systems.

We still struggle to answer basic questions about headwaters in many watersheds such as, “Are the streams flowing today?”

Targeted data collection and modeling efforts demonstrate that headwater intermittency can be predicted regionally when the right data are assembled. For example, France’s Observatoire National des Étiages (ONDE) program coordinates systematic monitoring of intermittent tributaries across France, generating large-scale presence-absence datasets that have been used to evaluate climate sensitivity and downscale simulated runoff.

However, to date, the scope of such efforts has been isolated. Physics-based models and watershed-scale simulations covering areas broader than those considered in individual, localized studies rarely integrate flow presence-absence observations or community science records from small streams. Meanwhile, ML models are typically trained on continuous stream gauge datasets while ignoring other informative, grounding constraints.

Despite the availability of unprecedented modeling capabilities and expanding collections of observations, much of the available data about headwater streams remain fragmented and unused. The barrier has been less a matter of cost or technological readiness than of the effort required to integrate heterogeneous datasets and link observational and modeling communities that have historically worked separately. As a result, we still struggle to answer basic questions about headwaters in many watersheds such as, “Are the streams flowing today?”

Learning from Available Information

The most expedient opportunity to better understand headwater hydrology lies not in building entirely new systems to continuously monitor discharge—a standard unlikely to be met across all headwater systems—but in integrating data already collected and treating diverse observation types as complementary information (Figure 1).

Fig. 1. This figure illustrates different types of headwater streamflow observations as well as types of outputs from physics-informed machine learning modeling (left). Also shown are the flow network for an example watershed (middle)—the West River watershed in Vermont—and an overlay of modeling units on this watershed’s flow network, including the National Hydro Geospatial Fabric (right). Diverse observation types combined with limited continuous monitoring data help estimate flow durations for all segments of the network. Click image for larger version. Credit: John Hammond

Continuous stream gauges capture the full temporal dynamics of flow on waterways, including during and after storms, revealing how and when flows rise, peak, and decline. Spot measurements, on the other hand, anchor hydrographs by quantifying flow at key moments.

Monitoring streamflow duration with data loggers and trail cameras provides additional data to models that augment more expensive streamflow data collected with stream gauges. The top photo shows data loggers and pressure transducers (yellow circles) deployed across the dry stream channel of Rossmoyne Creek, a second-order, intermittent stream in Hamilton County, Ohio, on 5 November 2021. A trail camera and barologger (red circle), which records barometric pressure and air temperature, were also installed on a bankside tree. The bottom photo shows a view from the trail camera, which was set to take a photo every 2 hours, on 13 November 2021. Click image for larger version. Credit: Ken Fritz

Community science programs document wet-dry status at many points in space using observations from passersby or low-cost wet-dry sensors. Camera-based systems validate intermittency and, with calibration, provide relative streamflow information. Each dataset is incomplete, with trade-offs in spatial footprint, temporal resolution, and measurement accuracy. Together, however, they describe hydroperiod (the pattern of days each year when water is present), connectivity, and flow dynamics far more completely than any one data type alone.

Beyond direct observational networks, remote sensing data—for example, from the Surface Water and Ocean Topography (SWOT) and NASA-ISRO Synthetic Aperture Radar (NISAR) missions—have potential for monitoring stream surface water indirectly, particularly where it is difficult to access. Headwater streams are often below detection levels for current satellites, but landscape-scale patterns in the water levels of neighboring water bodies may be reflective of headwater streamflow dynamics, providing information on when and where headwater streams are likely to be flowing.

Furthermore, depending on vegetation density and topography, high-resolution imagery and altimetry allow researchers to map surface water presence, estimate surface runoff patterns, characterize riparian vegetation, and detect changes in moisture or temperature patterns that signal hydrologic activity. By analyzing remotely sensed time series, scientists may be able to track how headwater streams respond to climatic variability, land use change, and disturbances such as wildfires.

Rather than replacing physics-based models with machine learning approaches, the two can be combined.

Modern ML architectures facilitate learning from these heterogeneous data types simultaneously, leveraging the different spatial densities of the relatively limited number of high-cost, continuous measurements at select locations and the vastly more abundant spot observations from community science efforts that often represent the only available streamflow information for an area. Rather than replacing physics-based models with ML approaches, however, the two can be combined.

Hybrid approaches can use physics-based outputs that capture watershed-integrated moisture state, snow water storage, and large-scale climate variability, but do not accurately predict headwater flows, especially low flows. Meanwhile, a data-driven component learns the ways that headwater reaches deviate from coarse-resolution estimates to make refined, fine-scale predictions.

Hybrid modeling has shown promise in other hydrologic contexts, and its ability to generate fine-scale predictions about headwaters can be evaluated explicitly. This sort of framework offers a way to integrate heterogeneous observations while remaining grounded in hydrologic reality.

Heading Toward a Hybrid Approach

An initial, achievable implementation of a hybrid headwater modeling approach would prioritize technically feasible and directly actionable metrics, namely, daily wet-dry classifications, seasonal counts of flowing days, and annual flow durations. These hydroperiod metrics underpin ecological processes, watershed connectivity assessments, and water quality management—even when discharge magnitudes remain uncertain.

Many streams experience dry periods because rainfall is minimal or due to increased evapotranspiration. In 2020, this small, unnamed, intermittent tributary of Rossmoyne Creek in Hamilton County, Ohio, flowed in May (left), was dry in July (middle), and then was flowing again in November (right). The stream drains a small urban catchment and is not shown on national stream maps. Credit: Ken Fritz

Multiple hybrid model architectures can support headwater prediction. Physics-informed neural networks can incorporate water balance information while focusing on tracking flow intermittency timing more precisely. Alternatively, tree-based ML approaches offer straightforward interpretability of the relative importance of environmental drivers and can readily incorporate mixed data types.

Both architectures could be configured to produce classification outputs (e.g., presence-absence, flow duration categories) and regression outputs (e.g., discharge magnitude, where reliable data exist).

As data compilation efforts expand and more observations become available, the same hybrid framework could later support increasingly sophisticated discharge predictions. Although the specific architectures that will exist in the future are uncertain, work to compile interoperable headwater datasets now ensures that future model advances can be rapidly applied.

Beyond predictive capabilities, models also create opportunities for discovery. By integrating and analyzing heterogeneous observations across different climatic and geomorphic environments, for example, models may reveal dominant controls on headwater intermittency (e.g., aridity, subsurface storage, or land cover or disturbance) and expose systematic biases in continental-scale water models.

From Idea to Operational Reality

The first step toward implementation of a hybrid headwater modeling framework is assembling multiple existing observational datasets.

Coordinating data compilation, standardizing workflows, and validating models among federal agencies, academic researchers, and regional watershed management organizations could effectively advance a hybrid headwater modeling framework from conceptual idea to operational reality. The first step toward implementation is assembling multiple existing observational datasets.

Initial efforts could focus on regions where flow observations are already available and observation densities are highest. The Pacific Northwest and upper Missouri River basin, where the U.S. Geological Survey’s Probability of Streamflow Permanence project has assembled extensive discrete flow observations, and the Chesapeake Bay watershed, where comparable observations have been compiled, are strong candidate pilot basins before methods are applied more broadly.

A fundamental but often underappreciated challenge at headwater scales is spatial referencing of data. Small stream channels do not typically align cleanly with gridded meteorological datasets used as model inputs, or with modeled watershed units or mapped hydrographic datasets. In some regions, channel heads migrate seasonally, and ephemeral tributaries may not be consistently represented in digital hydrographic maps.

These issues complicate the direct transfer of coarse-resolution model outputs to smaller spatial units. Scale mismatches between observation points, gridded data, and modeled spatial units are therefore a central consideration for any modeling framework operating at headwater scales.

Validation of headwater models could benchmark their predictive capabilities against standardized physics-based wet-dry and hydroperiod estimates, considering both gauged versus ungauged streams as well as predictions of both current and future conditions. And future conditions could be projected by forcing the hybrid models with downscaled climate projections and land use change scenarios, translating anticipated shifts in precipitation, snowmelt, and land cover into changes in the timing and duration of headwater flow.

The primary metrics for an initial implementation would, again, focus on basic understanding and forecasting of streamflow presence versus absence and on predicting seasonal or annual numbers of flow days within reasonable error bounds (e.g., 20%).

Scientists already have the essential ingredients for developing effective headwater models. What is missing is a systematic, interdisciplinary effort to deploy models that translate observations into fine-scale predictions.

Several research directions could receive further attention in later implementation stages. Improving discharge magnitude predictions at ungauged sites, for example, is critical and will require understanding of how well existing continuous measurements inform ML models and where denser observations might be needed. Developing methods to quantify uncertainty and communicate prediction confidence against specified reliability thresholds, especially when extrapolating beyond training conditions, could help strengthen predictions. Standardizing protocols for compiling diverse data, including procedures for quality control and metadata reporting, could also help.

Leveraging scarce data, modernizing approaches, and accelerating discovery in headwater stream modeling would benefit from a community of hydrologists, groundwater modelers, computer scientists, and social scientists working together across disciplines and organizations. For example, whereas key contributions of groundwater in headwater systems are often poorly understood and underrepresented in models, there is now potential to reveal groundwater behavior at finer scales, which would be supported by including groundwater expertise in modeling efforts. Shared tools, training, and collaborative spaces can help bridge these fields and build stronger communities of practice.

Scientists already have the essential ingredients for developing effective headwater models, including physics-based hydrological models, diverse observational networks, and powerful machine learning methods capable of integrating heterogeneous data.

What is missing is a systematic, interdisciplinary effort to compile existing headwater observations and deploy hybrid models that translate observations into fine-scale predictions. By coordinating this effort, headwater hydrology could become a predictive foundation supporting risk prevention for vulnerable downstream communities as well as needs for agricultural planning, environmental flows, and water management.

Acknowledgments

This work was developed in part from discussions by the Headwater Modeling Research Working Group at the John Wesley Powell Center for Analysis and Synthesis. We especially thank Ken Fritz for his help in providing images showing headwater stream sensor placements and wet-dry comparisons. The views expressed in this article are those of the authors and do not necessarily reflect the views or policies of the U.S. EPA but do represent the views of the U.S. Geological Survey. Any use of trade, firm, or product names is for descriptive purposes only and does not imply endorsement by the U.S. government.

Author Information

John Hammond (jhammond@usgs.gov), Maryland-Delaware-D.C. Water Science Center, U.S. Geological Survey, Catonsville, Md.; Jay Christensen, Office of Water, U.S. EPA, Cincinnati; Kristin Jaeger, Washington Water Science Center, U.S. Geological Survey, Tacoma; Roy Sando, Wyoming-Montana Water Science Center, U.S. Geological Survey, Helena, Mont.; and Jacob Zwart, Integrated Information Dissemination Division, Water Resources Mission Area, U.S. Geological Survey, San Francisco

Citation: Hammond, J., J. Christensen, K. Jaeger, R. Sando, and J. Zwart (2026), A hybrid approach for revealing headwater hydrology, Eos, 107, https://doi.org/10.1029/2026EO260248. Published on 5 August 2026. This article does not represent the opinion of AGU, Eos, or any of its affiliates. It is solely the opinion of the author(s). Text not subject to copyright.
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刚果河每秒向大西洋注入4万立方米淡水。一项新研究追踪了这些淡水的去向。

EOS - Wed, 08/05/2026 - 13:16
Source: Journal of Geophysical Research: Oceans

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

刚果河是世界第二大河流,平均每秒向大西洋注入4万立方米的水量。如此巨大的流量,形成了一股绵延800公里的淡水羽流

在雨季,这股羽流会向西南方向移动,并可能被称为“中尺度涡旋”的大型旋转洋流所捕获,这些涡旋的尺度可达上百公里。这些涡旋可将淡水输送到距离海岸数百公里之外的地方。在图卢兹空间地球物理学和海洋学研究实验室(LEGOS)及其合作实验室开展的一项研究中,Cardot等人结合模型模拟与实测数据,分析了中尺度涡旋的旋转洋流,以深入理解淡水从刚果河流入大西洋的过程。

研究人员使用了一个分辨率为3公里的海洋环流模型——NEMO(欧洲海洋建模核心模型)来模拟刚果河的流量。该研究聚焦于2016年,因为这一年间,热带大西洋预测与研究系泊阵列(PIRATA)的观测数据,以及该区域的盐度和海流卫星记录都极为丰富。研究人员利用eOdyn公司通过船舶自动识别系统(Automatic Identification System, AIS)收集的海面盐度、海面高度和表层洋流数据,对模型输出结果进行了验证。总体而言,该模型能够成功复现刚果河淡水羽流的空间范围、地理位置及其季节变化特征。

2016年期间发生了多次中尺度天气事件。其中一次涡旋在3月和4月将大量淡水输送至海洋。该反气旋涡(在南半球呈逆时针旋转)形成于刚果河羽流附近,持续了49天,半径增长至150公里。该涡旋将羽流中的低盐度水裹挟于其核心,并将其输送至离岸约200公里处,随后逐渐消散。

粒子追踪实验追溯了被涡旋捕获的水体来源,揭示了河水向大西洋输送的具体路径。研究人员通过时间倒推,追踪了超过5000个虚拟粒子,发现这些4月被困于涡旋核心内的粒子,可追溯至3月初刚形成的刚果河羽流南部区域。这一发现表明,2016年类似事件等间歇性过程主导了淡水向海洋的输送,而非刚果河水的持续扩散。这些发现对区域海洋环流,以及依赖此类淡水输入的海洋生态系统和渔业,具有重要意义。(Journal of Geophysical Research: Oceans, https://doi.org/10.1029/2025JC023642, 2026)

—科学撰稿人Rebecca Owen (@beccapox.bsky.social)

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

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Study finds climate-driven greening is reshaping East Asia's air pollution

Phys.org: Earth science - Wed, 08/05/2026 - 13:10
The effects of climate change extend far beyond rising temperatures. As forests and other vegetation respond to a warming world, they also change the amount of biogenic emissions released into the atmosphere, influencing the formation of ozone (O3) and fine particulate pollution. Yet many atmospheric chemistry models still estimate these emissions using vegetation data from 2003, despite major ecological changes across East Asia over the past two decades.

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