Feed aggregator

Measurement of turbulent velocity and bounds for thermal diffusivity in laser shock compressed foams by x-ray photon correlation spectroscopy

Physical Review E (Plasma physics) - Wed, 10/29/2025 - 10:00

Author(s): Charles Heaton, Hao Yin, Dimitri Khaghani, Hae Ja Lee, Hannah Poole, Eric Blackman, Nina Boiadjieva, Xiaoqian M. Chen, Celine Crépisson, Gilbert W. Collins, Adrien Descamps, Arianna E. Gleason, Christian Gutt, Alexander N. Petsch, Lisa Randolph, Silke Nelson, Peregrine McGehee, Rajan Plumley, Christopher Spindloe, Thomas Stevens, Charlotte Stuart, Joshua J. Turner, Hussein Aluie, Jessica K. Shang, and Gianluca Gregori

Experimental benchmarking of transport coefficients under extreme conditions is required for validation of differing theoretical models. To date, measurement of transport properties of dynamically compressed samples remains a challenge with only a limited number of studies able to quantify transport…


[Phys. Rev. E 112, 045218] Published Wed Oct 29, 2025

ID-GInSAR: An Improved Methodology for Integrating GNSS to Enhance InSAR-Based Deformation Monitoring

Geophysical Journal International - Wed, 10/29/2025 - 00:00
SummaryThis study presents an enhanced method for integrating Global Navigation Satellite System (GNSS) and Interferometric Synthetic Aperture Radar (InSAR), referred to as Iterative Decomposition-based GNSS-enhanced InSAR (ID-GInSAR), to address both spatially correlated components (SCCs) and topographically correlated components (TCCs) in interferogram errors. While traditional GInSAR (GNSS-enhanced InSAR) is effective in mitigating long-wavelength SCCs, it often overlooks TCCs, which are particularly significant in regions with steep topographic gradients. The proposed ID-GInSAR approach employs an iterative decomposition process to decouple and independently model SCCs and TCCs, utilizing a combination of exponential and statistical models. The method is validated using Sentinel-1 SAR and GNSS data from California’s southern Central Valley. Results demonstrate that ID-GInSAR significantly lowers noise in interferograms, enhances the robustness of displacement time series, and improves the accuracy of co-seismic deformation and velocity field estimates. Specifically, ID-GInSAR reduces the root mean square (RMS) between GNSS and InSAR by up to 55% in individual interferograms and by an average of 30.4% in displacement time series compared to traditional GInSAR methods. Furthermore, ID-GInSAR effectively highlights subtle transient deformation, such as coseismic offsets, and provides more robust velocity fields over shorter time spans (less than three years). Finally, we compare our method with other approaches, including Remove/Filter/Restore (RFR) and GACOS, and discuss their applicability scenarios. Collectively, ID-GInSAR provides an alternative integration method for regions with complex topography where ground-based GNSS observations are available.

Rupture Directivity of Moderate to Large Earthquakes in the Slow Deforming Iranian Plateau

Geophysical Journal International - Wed, 10/29/2025 - 00:00
SummaryRupture directivity significantly increases horizontal peak ground acceleration, elongates aftershock clouds, and enlarges meizoseismal areas beyond the fault end in front of the direction of rupture propagation. In this study, we examine the directivity of 25 moderate to large earthquakes (Mw ≥ 6) from 1968 to 2017 in the Iranian plateau by employing relocated earthquake clusters, mapped surface ruptures, focal mechanisms of earthquakes, slip distribution models, spatial distribution of Peak Ground Acceleration (PGA) amplitudes and macroseismic effects. The methodology overcomes the lack of dense seismic networks required to study directivity using methods based on the azimuthal variation of the spectrum of seismic waves. We show that 16 out of the 25 (i.e., 64%) of the earthquakes investigated have mostly unidirectional rupture. This implies that unidirectional ruptures in a slow deforming continental collision zone such as the Iranian Plateau is only slightly less common than those observed globally. With the understanding that unidirectional rupture increases the probability of ground shaking off the termination of the causative faults, our findings highlight the importance of considering the directivity effect in earthquake hazard assessment in Iran and also in other slow deforming continental regions.

The influence of a stably stratified layer on the hydromagnetic waves in the Earth’s core and their electromagnetic torques

Geophysical Journal International - Wed, 10/29/2025 - 00:00
SummaryEvidence from seismic studies, mineral physics, thermal evolution models and geomagnetic observations is inconclusive about the presence of a stably stratified layer at the top of the Earth’s fluid outer core. Such a convectively stable layer could have a strong influence on the internal fluid waves propagating underneath the core-mantle boundary (CMB) that are used to probe the outermost region of the core through the wave interaction with the geomagnetic field and the rotation of the mantle. Here, we numerically investigate the effect of a top stable layer on the outer core fluid waves by calculating the eigenmodes in a neutrally stratified sphere permeated by a magnetic field with and without a top stable layer. We use a numerical model, assuming a flow with an m-fold azimuthal symmetry, that allows for radial motions across the lower boundary of the stable layer and angular momentum exchanges across the CMB through viscous and electromagnetic coupling. On interannual time-scales, we find torsional Alfvén waves that are only marginally affected by weak to moderate stratification strength in the outer layer. At decadal time-scales similarly weak stable layers promote the appearance of waves that propagate primarily within the stable layer itself and resemble Magneto-Archimedes-Coriolis (MAC) waves, even though they interact with the adiabatic fluid core below. These waves can exert viscous and electromagnetic torques on the mantle that are several orders of magnitude larger than those in the neutrally stratified case.

Time-Lapse Airborne EM for monitoring the evolution of a saltwater aquifer - The Bookpurnong case study

Geophysical Journal International - Wed, 10/29/2025 - 00:00
SummaryA novel time-lapse modelling scheme for Airborne Electromagnetics (AEM) monitoring datasets is presented, using data from multiple surveys applied to study the hydro-related evolution of the Bookpurnong floodplain in South Australia. Additionally, it introduces a new wide-ranging approach for this type of study, incorporating new processing, validation, and interpretation tools.Time-Lapse studies are widespread in the literature but are not commonly applied to model EM data, particularly AEM data. This is linked to the challenges of performing overlapping data acquisition with inductive systems. The key features of the new time-lapse scheme, which address these issues, include the definition of independent forward and model meshes, essential for considering discrepancies in the location of soundings which arise in multitemporal AEM data acquisition, and the incorporation of system flight height in the inversion. This proved crucial for achieving satisfactory data fitting and limiting artifact propagation in the time-lapse models.Additionally, a novel processing workflow for AEM multitemporal datasets is presented. This has proven important for effectively processing the multitemporal datasets, which presents new challenges in identifying noise coupling arising from the use of different systems across vintages of data, possible variations in acquisition settings operated by different field crews, and changes in subsurface resistivity in the survey area. Results generated from the time-lapse modelling are evaluated with an Independent Hydrogeological Validation (IHV), designed to support the geophysical models validation and interpretation by providing a first-step hydrogeological evaluation.At Bookpurnong, along a sector of the Murray River floodplain, multitemporal AEM surveys were collected in 2015, 2022 and 2024, to study natural and engineered changes in the groundwater system over time. The time-lapse models show significantly smaller variations compared to those determined with individually modelled survey data sets, while delineating sharply bounded changes in resistivity across the floodplain. This demonstrates the effectiveness of the new time-lapse scheme in minimizing inversion variations typically encountered with independently modelled results affected by larger equivalence issues.Here, AEM models are first compared with resistivity borehole measurements, revealing a strong match between the two methodologies and spatial variations in resistivity consistent with a meandering river across the floodplain. These variations are further validated and interpreted using the IHV approach, which revealed a direct correlation between the hydrological stress of the Murray River and the response of shallow aquifers. Additionally, time-lapse geophysical models, combined with a hydrostratigraphic analysis, allow for a direct correlation between shallow and deep hydrogeological responses.We believe that the time-lapse methodology described here can be widely applied to multitemporal studies using AEM datasets, enabling the study of a broad range of natural processes with great accuracy and at the basin scale.

Judge Stops Shutdown-Related RIFs Indefinitely

EOS - Tue, 10/28/2025 - 21:51
body {background-color: #D2D1D5;} Research & Developments is a blog for brief updates that provide context for the flurry of news regarding law and policy changes that impact science and scientists today.

A judge has announced that the government cannot issue further reduction-in-force (RIF) notices to federal employees because of the government shutdown, nor implement RIFs that had already been issued during the shutdown.

The ruling by U.S. District Judge Susan Illston will mark the latest in a months-long court battle over RIFs at federal agencies.

“I think it’s important that we remember that, although we are here talking about statutes and administrative procedure and the like, we are also talking about human lives, and these human lives are being dramatically affected by the activities that we’re discussing this morning,” Judge Illston said at the top of the hearing, which was held at the headquarters of the Northern District of California in San Francisco.

 
Related

The case, American Federation of Government Employees, AFL-CIO v. United States Office of Personnel Management (OPM) (3:25-cv-01780), was first filed in February. AGU joined as a plaintiff in the case in March. Other plaintiffs include Climate Resilient Communities, the Coalition to Protect America’s National Parks, and the American Public Health Association.

Judge Illston granted a temporary restraining order earlier this month, which prevented the government from executing RIFs during the shutdown until further notice.

However, the Trump administration only paused some RIFs, arguing that most of the thousands of layoffs announced since the shutdown are not covered by the court order.

As part of the temporary restraining order, the court ordered the government to provide an accounting of “all RIFs, actual or imminent,” that it planned to execute during the shutdown. The list included 143 Fish and Wildlife Service employees, 355 USGS employees, 272 National Park Service employees, and 474 Bureau of Land Management employees.

On 22 October, Judge Illston broadened the reach of who was protected by the temporary restraining order by adding several unions representing federal employees as plaintiffs.

In today’s hearing, the plaintiffs argued for a preliminary injunction, a move that essentially preserves the status quo before the final judgement of a trial. Danielle Leonard, an attorney representing the plaintiffs, argued that, in this case, the state of affairs prior to the government shutdown should be considered the “status quo.” In essence, this meant seeking for a halt to RIFs that have occurred since the shutdown, not just future RIFs.

The plaintiffs sought prove that the RIFs were “arbitrary or capricious,” a legal standard that is part of the Administrative Procedure Act, which governs how federal agencies operate.

Michael Velchick, an attorney representing the U.S. government, argued that the government’s actions were not only not arbitrary or capricious, but good policy, and “the right thing to do.”

“Morally it’s the right thing to do, and it’s the democratic thing to do,” he said. “The American people selected someone known above all else for his eloquence in communicating to employees that, ‘You’re fired.’”

This was seemingly a reference to the president’s former reality TV show, The Apprentice.

Leonard argued that Velchick’s statement was offensive to the 1.5 million federal employees represented by her clients. She summed up the defendant’s argument like this:

“There is some general authority, and therefore that blesses the specific actions that are happening here for the reasons that the government has given, regardless of how poor those reasons are. And that’s just not the way the law works.”

Judge Illston seemed to agree, stating that the Office of Personnel Management and Office of Management and Budget were prohibited from issuing more RIF notices or implementing those already issued.

The judge noted that she will likely hold an evidentiary hearing to settle a potential dispute over whether specific RIF notices were issued because of the shutdown, or were “already in the works” and unrelated to the shutdown.

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

These updates are made possible through information from the scientific community. Do you have a story about how changes in law or policy are affecting scientists or research? Send us a tip at eos@agu.org. Text © 2025. 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.

Six-million-year-old ice discovered in Antarctica offers unprecedented window into a warmer Earth

Phys.org: Earth science - Tue, 10/28/2025 - 20:37
A team of U.S. scientists has discovered the oldest directly dated ice and air on the planet in the Allan Hills region of East Antarctica.

A high energy cosmic-ray and gamma-ray observatory at the Moon South Pole: the MoonRay concept

Publication date: Available online 24 October 2025

Source: Advances in Space Research

Author(s): P.S. Marrocchesi

Pre-seismic ionospheric disturbances following the 2025 <math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si15.svg" class="math"><mrow><msub><mrow><mi>M</mi></mrow><mrow><mi>w</mi></mrow></msub></mrow></math> 7.7 Mandalay, Burma (Myanmar) Earth

Publication date: Available online 24 October 2025

Source: Advances in Space Research

Author(s): Husan Eshkuvatov, Shuanggen Jin, Bobomurat Ahmedov, Shukhrat Mardonov, Shahzod Numonjonov

Automated Annotation and Optimization of Multitask Dataset for Spacecraft

Publication date: Available online 23 October 2025

Source: Advances in Space Research

Author(s): Shengyun Zhao, Linyan Cui, Rui Zhong

Direct simulations of very high energy cosmic ray acceleration in 3D MHD model of a compact star cluster

Publication date: Available online 23 October 2025

Source: Advances in Space Research

Author(s): M.E. Kalyashova, A.M. Bykov, D.V. Badmaev

Remote sensing helps confirm Aliso Canyon methane plumes traveled at least 6.2 miles downwind during blowout

Phys.org: Earth science - Tue, 10/28/2025 - 18:44
Using a mix of airborne and satellite images as well as data from ground sensors, a UCLA-led research team has reconstructed how the shape and reach of the methane plumes from the 2015–16 Aliso Canyon gas blowout evolved during the 112-day disaster.

Image: Hurricane Melissa barrels through the Caribbean

Phys.org: Earth science - Tue, 10/28/2025 - 16:30
This image captured by the Copernicus Sentinel-3 mission on 26 October 2025 shows the "brightness temperature" at the top of Hurricane Melissa as it barreled through the Caribbean Sea toward Jamaica, where it is expected to make landfall.

Geoscientist's innovative approach aims to safeguard irrigation canals

Phys.org: Earth science - Tue, 10/28/2025 - 14:04
Irrigation canal maintenance in western Nebraska is taking a giant step forward thanks to an innovative, non-invasive method by Husker geoscientist Mohamed Khalil to check canal integrity. His sophisticated time-lapse analysis pinpoints canal seepage and structural settlement far more accurately and efficiently than traditional approaches—using a technology that can have wide-ranging uses statewide for agriculture, industry and natural resources management.

AI is Changing our Understanding of Earthquakes

EOS - Tue, 10/28/2025 - 13:48

This story was originally published by Knowable Magazine.

When the biggest earthquake in more than a decade rattled Russia’s remote Kamchatka Peninsula in July, seismologists around the world knew within moments. For earthquakes big or small, sensors around the globe detect the tremors and relay that information to researchers, who quickly analyze the observations and issue alerts.

Now artificial intelligence is poised to make almost everything about earthquake research much faster—and to rewrite researchers’ very understanding of how earthquakes happen.

“Machine learning opened a whole new window.”

By using a subfield of AI called machine learning, some scientists are identifying up to millions of tiny, previously unseen earthquakes in data gathered from seismically active places. These new and improved databases are helping researchers to better understand the geological faults along which quakes happen, and can help to illuminate the risks of future quakes. Some scientists are even using machine learning to improve their forecasts of how many aftershocks may rattle a location that has just experienced a large and damaging earthquake.

More broadly, researchers hope that machine learning, with its ability to crunch through huge amounts of information and learn from the patterns within, will reveal fresh insights into some of the biggest mysteries about earthquakes, including how a quake unfolds in its first devastating seconds.

“Machine learning opened a whole new window,” says Mostafa Mousavi, a seismologist at Harvard University.

Shaking Earth, Exploding Data

Earthquakes happen when geological stress builds up in the ground, such as when two plates of Earth’s crust grind alongside one another, as they do at California’s San Andreas Fault. At some point, the stress reaches a critical threshold and the fault ruptures, breaking the rock and causing seismic energy to ripple outward and shake the ground.

The San Andreas fault, seen here as a dramatic slash across the Carrizo Plain in Southern California, is an example of a geologically active area where seismologists are using AI to better understand earthquake patterns. Credit: John Wiley, Wikimedia Commons, CC BY 3.0

That energy is recorded by seismometers and other instruments around the world, which are positioned in great numbers in geologically active areas like California and Japan. The data feed into national and international systems for tracking earthquakes and alerting the world. The amount of data has exploded in recent years as seismologists find new ways to gather information on ground movements—like detecting seismic signals over fiber optic networks, or using the accelerometers built into smartphones to create a phone-based earthquake warning network.

Just a decade or two ago, much of the analysis of seismic signals was done by hand, with scientists working as quickly as possible to assess recordings coming in from their observing networks. But today, there are just too many data points. “Now the only—almost—way that you can deal with the seismic data is to go to automatic processing,” says Mousavi, who coauthored a 2023 article in the Annual Review of Earth and Planetary Sciences on machine learning in earthquake seismology.

One of the most common uses of machine learning in seismology is measuring the arrival time of seismic waves at a particular location, a process known as phase picking. Earthquakes generate two kinds of seismic waves, known as P and S waves, that affect the ground in different ways and show up as different types of squiggles on a seismogram. In the past, a seismologist would analyze data arriving from seismic sensors and hand-select what they gauged to be the start of P waves or S waves on those seismogram plots. Picking the starts of those waves accurately and precisely is important for understanding factors such as where exactly the earthquake hit. But phase picking is very time consuming.

An earthquake’s energy appears as a squiggly waveform on measurements made by seismometers. The first type of signal to arrive is a ground movement known as a P wave, followed by a type known as an S wave. Picking where the waves first arrive on a seismometer reading is an important part of understanding an earthquake’s impact—this has typically been done by human seismologists but in recent years the process has been made much quicker by incorporating machine-learning algorithms. Credit: Knowable Magazine, adapted from USGS.gov

In the past few years, seismologists have been using machine learning algorithms to pick seismic phases much faster than a human can. There are a number of automated methods that can do phase picking, but machine learning algorithms, which have been trained on huge volumes of data on past quakes, can identify a wide variety of signals from different types of tremors in a way that was not possible before. The practice is now so standard that the term “machine learning” is no longer stated in the titles of research papers, says Mousavi. “By default, everybody knows.”

AI-based phase picking is faster than phase picking by humans and at least as accurate, Mousavi says. Seismologists are now working to expand these tools to other types of seismic analysis.

Expanding Quake Catalogs

One area that has already seen big discoveries is the use of machine learning to expand earthquake catalogs—basically, lists of what earthquakes happened where in a particular region. Earthquake catalogs include all the quakes that seismologists can identify from recorded signals—but AI can find exponentially more tremors than human scientists can.

Essentially, machine learning can trawl through the data to identify small earthquakes that people don’t have the ability or time to flag. “Either you don’t see them by eye, or there’s no time to go and look at all those tiny events,” says Leila Mizrahi, a seismologist with the Swiss Seismological Service at ETH Zürich. Often, these tremors are obscured by background noise in the data.

Tiny earthquakes are important as a window into how larger earthquakes begin.

In a pioneering 2019 study in Science, researchers used an AI algorithm that matched patterns of seismic waves to identify more than 1.5 million tiny earthquakes that happened in Southern California between 2008 and 2017 but had not been spotted before. These are itty-bitty quakes that most people wouldn’t feel even if they were standing on top of them. But knowing they exist is important in helping seismologists understand patterns of behavior along a geological fault.

In particular, Mousavi says, tiny earthquakes are important as a window into how larger earthquakes begin. Large earthquakes may happen along a particular fault once every century or more—far too long a time period for scientists to observe in order to understand the rupture process. Tiny quakes behave much the same as big ones, but they happen much more frequently. So studying the pattern of tiny quakes in the newly expanded earthquake catalogs could help scientists better understand what gets everything going. In this way, the richer catalogs “have potential to help us to understand and to model better the seismic hazard,” Mousavi says.

Expanded earthquake catalogs can also illuminate the structure of geological faults below a region much better than before. It’s like going from a simplistic sketch of how the faults are arranged to a painting with more photorealistic details. In 2022, a team led by seismologist Yongsoo Park, then at Stanford University, used machine learning to build an expanded catalog of quakes in Oklahoma and Kansas between 2010 and 2019, many of them induced by oil and gas companies injecting wastewater into the ground. The work illuminated fault structures that weren’t visible before, allowing the scientists to map the faults more precisely and to better understand seismic risk.

This dramatic example shows the power of machine learning to enhance scientists’ knowledge of earthquakes. Top is a depiction of an earthquake swarm that occurred near Pawnee, Oklahoma, in September 2016. Each dot represents an earthquake measured by seismometers (with yellow representing quakes that occurred early in the swarm, and red representing quakes that occurred later). Bottom is the same earthquake swarm, but in this case when scientists used machine learning to pinpoint additional, smaller quakes in the observations. The enhanced earthquake catalog shows far more detail of where the quakes occurred, including illuminating the underlying geological faults. Credit: Courtesy of Yongsoo Park

Park and his colleagues showed that 80 percent of the larger earthquakes that happened could have been anticipated based on the smaller earthquakes that occurred before the big ones. “There is always a possibility that the next major earthquake can occur on a fault that is still not mapped,” says Park, who is now at Los Alamos National Laboratory in New Mexico. “Routinely capturing smaller earthquakes might be able to reveal such hidden faults before a major earthquake happens.”

Scientists are applying this approach around the globe. Researchers in Taiwan, for instance, recently used machine learning to produce a more detailed catalog of a magnitude 7.3 tremor in April 2024 that killed at least 18 people on the island and damaged hundreds of buildings. The study, reported at a seismology meeting in April 2025, found the AI-based catalog to be about five times more complete than the one produced by human analysts, and it was made within a day rather than taking months. It revealed new details on the location and orientation of geological faults—information that can help officials better prepare for how the ground might move in future quakes. Such catalogs “will become the standard in every earthquake-prone region in the future,” says team leader and seismologist Hsin-Hua Huang of Academia Sinica in Taiwan.

Forecasting is Still a Problem

So far, AI hasn’t been as successful in tackling another of seismology’s biggest challenges—forecasting the probability of future quakes.

The field of earthquake forecasting deals with general probabilities—such as the chances of a quake of magnitude X happening in region Y over time period Z. Currently, seismologists create quake forecasts using mathematical analyses of past earthquakes, such as a statistical method that relies on observations of how past earthquakes triggered subsequent quakes. This approach works well enough for specific tasks, like understanding how many aftershocks may rattle a region after a Big One. That sort of information can help people in a disaster zone know whether it’s safe to return to their houses or whether more aftershocks might be on the way, threatening to collapse more buildings.

But this kind of analysis can’t always accurately capture the real seismic risk, especially along faults that only rarely yield big quakes and thus aren’t well represented in the seismic record. Seismologists are testing AI-based algorithms for earthquake forecasting to see if they might do better, but so far, the news is tepid. In their best performances, the machine learning analyses are about as good as the standard methods of quake forecasting. “They are not outperforming the traditional ones yet,” says Mousavi, who summarized the state of the field in an August 2025 article in Physics Today.

Overall, though, seismologists see a bright future in using AI to understand earthquakes better.

In one of the more promising experiments, Mizrahi has been trying to use AI to speed up producing aftershock forecasts in the crucial minutes and hours after a large earthquake hits. She and a colleague trained a machine-learning algorithm on the older statistical method of quake forecasting, then unleashed it on its own to see how the AI would do. It did perform much faster than the older, non-AI approach, but there’s still more work to do. “We’re in the process of evaluating how happy we are with it,” says Mizrahi, who published the findings last year in Seismological Research Letters.

In the future, researchers hope to speed up these types of forecasting analyses. Other areas of seismology could eventually benefit, too. Some early research hints that machine learning could be used in earthquake early warning, for instance estimating exactly how much the ground will move in the seconds after an earthquake has started nearby. But the usefulness of this is limited to the few parts of the world that have early warning systems in place, like California and Japan.

Park also cautions about relying too much on machine learning tools. Scientists need to be careful about maintaining quality control so they can be sure they are interpreting the results of any AI analysis correctly, he says.

Overall, though, seismologists see a bright future in using AI to understand earthquakes better. “We’re on the way,” Mizrahi says.

—Alexandra Witze, Knowable Magazine

This article originally appeared in Knowable Magazine, a nonprofit publication dedicated to making scientific knowledge accessible to all. Sign up for Knowable Magazine’s newsletter. Read the original article here.

Researchers identify million-year orbital cycles as 'pacemaker' for Earth's ancient oxygenation pulses

Phys.org: Earth science - Tue, 10/28/2025 - 13:40
A research team from the Nanjing Institute of Geology and Paleontology of the Chinese Academy of Sciences (NIGPAS), along with collaborators, has found that long-term orbital variations occurring over million-year timescales may have served as the "pacemaker" for Earth's ancient oxygenation pulses. Their findings were recently published in Geophysical Research Letters.

Martian Dust Devils Reveal Dynamic Surface Winds

EOS - Tue, 10/28/2025 - 13:40

In 2020, the scientists and engineers behind NASA’s InSight lander were optimistic. The mission was performing spectacularly, and it had no end in sight. Then, its power began to fade. Fine Martian dust was relentlessly piling on top of its solar panels, blocking sunlight. Mission operators had anticipated this but hoped that occasional wind gusts or passing dust devils would sweep the panels clean. Such fortuitous cleaning had prolonged the lives of earlier robotic explorers, such as the Spirit and Opportunity rovers. But for InSight, no such wind ever came, and its batteries slowly ran out of juice. InSight fell silent in December 2022.

InSight’s demise illustrates a long-standing gap in Martian science: Researchers still know little about how winds move across the planet’s surface and interact with dust. To help fill this gap, a group of researchers has now reviewed decades of orbital imagery from two European Space Agency (ESA) spacecraft—Mars Express and the ExoMars Trace Gas Orbiter, operational since 2004 and 2016, respectively—looking for dust devils and using them as a proxy for surface winds.

Over the years, these orbiters have captured thousands of high-resolution images of Mars’s surface. Hidden within this vast dataset are countless sightings of dust devils, which drift with the prevailing winds. Because surface winds are otherwise impossible to measure directly from Martian orbit with the available instruments, tracking the motion of these vortices provides a rare window into their direction and velocity.

To measure these parameters, the researchers exploited a technical quirk of the spacecraft cameras, namely, the slight temporal delay between capturing different color layers of an image or between the right and left images in stereoscopic views. By tracking the dust devils’ movement between exposures, the team could track the velocity and directions of the winds carrying them. Their observations revealed some of the fastest surface wind speeds ever detected on Mars, challenging existing atmospheric models.

The Colour and Stereo Surface Imaging System (CaSSIS) on board the European Space Agency’s ExoMars Trace Gas Orbiter captured this dust devil tracking across the Martian surface on 28 February 2019. Credit: ESA/TGO/CaSSIS, CC BY-SA 3.0 IGO

“With dust devils, we now have a tool to measure wind velocities across the planet, across space and time,” said Valentin Bickel, a planetary scientist at the University of Bern and lead author of the study. “We get a measurement of wind speeds in a distributed way around the planet, not just in specific lander locations.”

AI-Assisted Research

Detecting dust devils in orbital images, however, is not easy. For instance, the Colour and Stereo Surface Imaging System (CaSSIS) camera on board the ExoMars Trace Gas Orbiter resolves the surface at about 4 meters per pixel, meaning that dust devils dozens of meters wide appear as tiny smudges. Finding all these dust devils in the images is something that “an army of people could do in a few months or years, but nobody can pay for that,” Bickel said.

To automate the search, Bickel and colleagues trained a convolutional neural network—a type of artificial intelligence (AI) commonly used in image recognition—to identify the dust devils. After training the algorithm with about 50 examples labeled by experts, they let it loose on their full dataset of 50,000 orbital images. “Its only function is to identify dust levels in images; it can’t do anything else. It’s very stupid,” Bickel said. However, it needed only a few hours to scan the entire collection.

“The velocities we measured are totally surprising; I didn’t think we would see so many fast dust devils on Mars.”

The neural network detected more than a thousand dust devils across nearly all Martian latitudes. Each detection offered a new data point on local surface winds. The analysis revealed that Martian surface winds are generally faster than current atmospheric models suggest—and occasionally stronger than any speeds directly recorded by landers or rovers equipped with weather instruments. For instance, the researchers detected wind speeds of up to 44 meters per second, which is substantially faster than the previous 32 meters per second mark recorded by the Perseverance rover. Scientists previously assumed that dust devils might not even have been able to form at such wind speeds, as they could be destroyed by currents, Bickel said.

“The velocities we measured are totally surprising; I didn’t think we would see so many fast dust devils on Mars,” Bickel said. “You always picture them as these slowly moving clouds of dust, but it turns out they’re like superfast, highway speed level objects. I think it’s just crazy.”

The second key finding is that fast winds are more widespread across the planet than previously thought. To showcase this, the researchers produced a map with the locations of all 1,039 dust devils detected, including the direction of motion for 373 of them, confirming that dust devils are found all over Mars, even atop the tallest volcanoes. However, dust devils tend to cluster in specific regions, for instance, in Amazonis Planitia (visible at upper left in the map), a vast area known to be covered by an extensive, fine layer of dust and sand.

Researchers created a map showing 1,039 dust devils that occurred on the Martian surface, as seen in 20 years’ worth of images from European Mars orbiters. Credit: ExoMars TGO data: ESA/TGO/CaSSIS; Mars Express data: ESA/DLR/FU Berlin; Background: NASA Viking color mosaic, CC BY-SA 3.0 IGO

“Of course,” Bickel noted, “we have a bias because we need dust devils to see [the winds], so if there’s no dust at ground level, we don’t see the wind.”

The team also observed a clear seasonal pattern: Dust devils and strong winds appear more frequently during each hemisphere’s spring and summer, typically happening around midday, when surface heating is more intense. The researchers published their findings in Science Advances.

Blowing in the Dusty Wind

Deciphering how Martian winds work is key to understanding how dust shapes the planet’s weather and climate. Wind is the main force that lifts and transports the Red Planet’s abundant dust, which in turn regulates how the Martian atmosphere absorbs and radiates heat.

Understanding dust transport is thus critical for future exploration, both robotic and human. A global map of wind patterns might have helped InSight’s engineers choose a landing site less prone to rapid dust accumulation. On a larger scale, planet-encircling dust storms that erupt every decade or so—sometimes blocking sunlight for months—remain a serious hazard for exploration.

“Wind is one of the holy grails for human exploration and to understand the Martian climate.”

“Wind is one of the holy grails for human exploration and to understand the Martian climate,” said Germán Martínez, a researcher at the Center for Astrobiology in Madrid, Spain, who wasn’t involved with the new study. “Surface winds are very important, for Martian climatology, but especially at this time for human exploration safety, and we know very little.” In that sense, Martínez said, this research is important because it provides a map of surface wind speeds and directions that we didn’t have before, even if it’s a bit coarse.

Bickel agreed that more data, and more tools in orbit, will improve understanding of the Martian wind system. In the meantime, he hopes the new map will be used to validate and improve climate and wind models of Mars.

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

Citation: Barbuzano, J. (2025), Martian dust devils reveal dynamic surface winds, Eos, 106, https://doi.org/10.1029/2025EO250404. Published on 28 October 2025. Text © 2025. 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.

Earth's 'boring billion years' created the conditions for complex life, study reveals

Phys.org: Earth science - Tue, 10/28/2025 - 12:59
A study led by researchers from the University of Sydney and the University of Adelaide has revealed how the breakup of an ancient supercontinent 1.5 billion years ago transformed Earth's surface environments, paving the way for the emergence of complex life.

New method can measure ocean acidification using ambient wind noise

Phys.org: Earth science - Tue, 10/28/2025 - 11:30
Since the Industrial Revolution, scientists estimate that the ocean has become around 30% more acidic from the uptake of additional anthropogenic carbon dioxide. Ocean acidification has widespread effects, including loss of coral reefs and a decline in shellfish. Current methods for measuring acidification in the ocean are point-based and labor-intensive, making large-scale, long-term monitoring challenging.

Cul-de-sac effect: Why Mediterranean regions are becoming more prone to extreme floods in a changing climate

Phys.org: Earth science - Tue, 10/28/2025 - 10:00
In May 2023, Italy's Emilia-Romagna region experienced devastating, if not unprecedented, floods that caused widespread damage to infrastructure, homes, businesses, and farmland. Seventeen people lost their lives, and the disaster caused an estimated €8.5 billion in damages. The persistent rainfall and resulting landslides and flooding displaced tens of thousands of residents, leaving a deep mark on the region's economy and communities.

Theme by Danetsoft and Danang Probo Sayekti inspired by Maksimer