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1000 results for “fluiddyn”
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“500,000-km Solar Prominence Eruption”
It’s difficult at times to fathom the scale and power of fluid dynamics beyond our day-to-day lives. Here, twists of the Sun‘s magnetic field propel a jet of plasma more than 500,000 kilometers out from its surface in an enormous solar prominence eruption. To give you a sense of scale for this random solar burp, that’s bigger than ten times the distance to satellites in geostationary orbit. (Image credit: P. Chou; via Colossal)
#astrophysics #fluidDynamics #fluidsAsArt #magnetohydrodynamics #physics #science #sun
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Deep Breaths Renew Lung Surfactants + A Special Announcement
Taking a deep breath may actually help you breathe easier, according to a new study. When we inhale, air fills our alveoli–tiny balloon-like compartments within our lungs. To make alveoli easier to open, they’re coated in a surfactant chemical produced by our lungs. Just as soap’s surfactant molecules squeezing between water molecules lowers the interface’s surface tension, our lung surfactants gather at the interface and lower the surface tension, making alveoli easier to inflate.
But things are a little more complicated in our lungs than in our kitchen sink because of our constant cycle of breathing, which stretches and compresses our lungs’ surfaces and surfactant layers. Imagine a flat interface, lined with surfactant molecules; then stretch it. As the interface stretches, gaps open between the surfactant molecules and allowing molecules from the interior of the liquid to push their way to the newly stretched interface, changing the surface tension. If the interface gets compressed, some of the excess molecules will get pushed back into the liquid bulk.
In looking at how lung surfactants respond to these cycles of compression and stretching, the researchers found that the lung liquid develops a microstructure during cycles of shallow breathing that makes the surface tension higher, thus making lungs harder to fill. In contrast, a deep breath like a sigh replenished the saturated lipids at the interface, lowering surface tension and making lungs more compliant. So a deep sigh actually can help you breathe easier. (Image credit: F. Møller; research credit: M.. Novaes-Silva et al.; via Gizmodo)
P.S. — I’ve got a book (chapter)! Several years ago, I joined an amazing group of women to write two books (one for middle grades and one for older audiences) about our journeys as scientists. And they are out now! In fact, today we’re holding a “Book Bomb” where we aim for as many of us as possible to buy the book(s) on the same day. If you’d like to join (and get ahead on your gift shopping), here are (affiliate) links:
- Persevere, Survive, and Thrive (including my story of becoming a science communicator): Amazon, Bookshop.org
- For All the Curious Girls: Amazon, Bookshop.org
#biology #fluidDynamics #lungs #physics #science #surfaceTension #surfactants
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Wobbling Plasma Could Help Planets Grow
To form planets, the dust and gas around a star has to start clumping up. While there are many theories as to how this could happen, it’s a difficult process to observe. A recent study shows that a magnetorotational (MR) instability could do the job.
The team used a Taylor-Couette set-up (where an inner cylinder rotates inside an outer cylinder) filled with a liquid metal alloy. With the cylinders moving relative to one another at over 2,000 rotations per minute, the team measured how the magnetic field changed in the churning fluid. Parts of the liquid metal formed free shear layers, and within these, the MR instability occurred, causing some regions to slow down and others to speed up.
The experiments suggest that triggering a MR instability is easier to achieve than once thought, which supports the possibility that it occurs in protoplanetary disks, helping to drive dust together into planets. (Image credit: ALMA/ESO/NAOJ/NRAO; research credit: Y. Wang et al.; via Eos)
#astrophysics #fluidDynamics #magnetohydrodynamics #magnetorotationalInstability #physics #planetaryCoreFormation #science #taylorCouetteFlow
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Wobbling Plasma Could Help Planets Grow
To form planets, the dust and gas around a star has to start clumping up. While there are many theories as to how this could happen, it’s a difficult process to observe. A recent study shows that a magnetorotational (MR) instability could do the job.
The team used a Taylor-Couette set-up (where an inner cylinder rotates inside an outer cylinder) filled with a liquid metal alloy. With the cylinders moving relative to one another at over 2,000 rotations per minute, the team measured how the magnetic field changed in the churning fluid. Parts of the liquid metal formed free shear layers, and within these, the MR instability occurred, causing some regions to slow down and others to speed up.
The experiments suggest that triggering a MR instability is easier to achieve than once thought, which supports the possibility that it occurs in protoplanetary disks, helping to drive dust together into planets. (Image credit: ALMA/ESO/NAOJ/NRAO; research credit: Y. Wang et al.; via Eos)
#astrophysics #fluidDynamics #magnetohydrodynamics #magnetorotationalInstability #physics #planetaryCoreFormation #science #taylorCouetteFlow
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Wobbling Plasma Could Help Planets Grow
To form planets, the dust and gas around a star has to start clumping up. While there are many theories as to how this could happen, it’s a difficult process to observe. A recent study shows that a magnetorotational (MR) instability could do the job.
The team used a Taylor-Couette set-up (where an inner cylinder rotates inside an outer cylinder) filled with a liquid metal alloy. With the cylinders moving relative to one another at over 2,000 rotations per minute, the team measured how the magnetic field changed in the churning fluid. Parts of the liquid metal formed free shear layers, and within these, the MR instability occurred, causing some regions to slow down and others to speed up.
The experiments suggest that triggering a MR instability is easier to achieve than once thought, which supports the possibility that it occurs in protoplanetary disks, helping to drive dust together into planets. (Image credit: ALMA/ESO/NAOJ/NRAO; research credit: Y. Wang et al.; via Eos)
#astrophysics #fluidDynamics #magnetohydrodynamics #magnetorotationalInstability #physics #planetaryCoreFormation #science #taylorCouetteFlow
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Wobbling Plasma Could Help Planets Grow
To form planets, the dust and gas around a star has to start clumping up. While there are many theories as to how this could happen, it’s a difficult process to observe. A recent study shows that a magnetorotational (MR) instability could do the job.
The team used a Taylor-Couette set-up (where an inner cylinder rotates inside an outer cylinder) filled with a liquid metal alloy. With the cylinders moving relative to one another at over 2,000 rotations per minute, the team measured how the magnetic field changed in the churning fluid. Parts of the liquid metal formed free shear layers, and within these, the MR instability occurred, causing some regions to slow down and others to speed up.
The experiments suggest that triggering a MR instability is easier to achieve than once thought, which supports the possibility that it occurs in protoplanetary disks, helping to drive dust together into planets. (Image credit: ALMA/ESO/NAOJ/NRAO; research credit: Y. Wang et al.; via Eos)
#astrophysics #fluidDynamics #magnetohydrodynamics #magnetorotationalInstability #physics #planetaryCoreFormation #science #taylorCouetteFlow
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Wave Energy Through the Meniscus
Even small changes to a meniscus can change how much wave energy passes through it. A new study systemically tests how meniscus size and shape affects the transmission of incoming waves.
As seen above, the meniscus was formed on a suspended barrier. By changing the barrier size and wettability as well as the characteristics of incoming waves, researchers were able to map out how the meniscus affected waves that made it past the barrier.
In particular, they found that drawing the meniscus upward by raising the barrier would, at first, enhance wave transmission but then suppressed wave energy as the barrier moved higher. They attributed the change in behavior to an interplay between water column height and meniscus inclination. (Research and image credit: Z. Wang et al.; via Physics World)
#capillaryWaves #fluidDynamics #meniscus #physics #science #surfaceTension #waves
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Wave Energy Through the Meniscus
Even small changes to a meniscus can change how much wave energy passes through it. A new study systemically tests how meniscus size and shape affects the transmission of incoming waves.
As seen above, the meniscus was formed on a suspended barrier. By changing the barrier size and wettability as well as the characteristics of incoming waves, researchers were able to map out how the meniscus affected waves that made it past the barrier.
In particular, they found that drawing the meniscus upward by raising the barrier would, at first, enhance wave transmission but then suppressed wave energy as the barrier moved higher. They attributed the change in behavior to an interplay between water column height and meniscus inclination. (Research and image credit: Z. Wang et al.; via Physics World)
#capillaryWaves #fluidDynamics #meniscus #physics #science #surfaceTension #waves
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Wave Energy Through the Meniscus
Even small changes to a meniscus can change how much wave energy passes through it. A new study systemically tests how meniscus size and shape affects the transmission of incoming waves.
As seen above, the meniscus was formed on a suspended barrier. By changing the barrier size and wettability as well as the characteristics of incoming waves, researchers were able to map out how the meniscus affected waves that made it past the barrier.
In particular, they found that drawing the meniscus upward by raising the barrier would, at first, enhance wave transmission but then suppressed wave energy as the barrier moved higher. They attributed the change in behavior to an interplay between water column height and meniscus inclination. (Research and image credit: Z. Wang et al.; via Physics World)
#capillaryWaves #fluidDynamics #meniscus #physics #science #surfaceTension #waves
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Wave Energy Through the Meniscus
Even small changes to a meniscus can change how much wave energy passes through it. A new study systemically tests how meniscus size and shape affects the transmission of incoming waves.
As seen above, the meniscus was formed on a suspended barrier. By changing the barrier size and wettability as well as the characteristics of incoming waves, researchers were able to map out how the meniscus affected waves that made it past the barrier.
In particular, they found that drawing the meniscus upward by raising the barrier would, at first, enhance wave transmission but then suppressed wave energy as the barrier moved higher. They attributed the change in behavior to an interplay between water column height and meniscus inclination. (Research and image credit: Z. Wang et al.; via Physics World)
#capillaryWaves #fluidDynamics #meniscus #physics #science #surfaceTension #waves
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A Gentoo Flotilla
If you’re used to seeing penguins on land, their speed and grace in the water can surprise. Penguins are even capable of extra bursts of speed through supercavitation. They trap air beneath their feathers and then release it underwater when they need to move faster. Their coating of bubbles reduces their drag and gives them the extra speed to help escape predators like leopard seals. (Image credit: R. Barats/OPOTY; via Colossal)
#flowVisualization #fluidDynamics #fluidsAsArt #penguins #physics #science #supercavitation
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▶️ New video!
Watch a Direct Numerical Simulation (DNS) of a pure water Leidenfrost droplet in full detail, simulated with #pyoomph. Footage recorded by Maxim de Wildt (DC#9, #LeidenForce) at @utwente -
Zoom Into the Sun
Fall into our nearest star in this gorgeous high-resolution view of the Sun. Taken by Solar Orbiter, a joint NASA-ESA mission, the image stretches from the fiery photosphere — full of filaments and prominences — to the wispy yet unbelievably hot corona. It’s well worth clicking through to zoom in and around the full size image. (Image credit: ESA & NASA/Solar Orbiter/EUI Team, E. Kraaikamp; via Gizmodo)
#coronalMassEjection #fluidDynamics #magnetohydrodynamics #physics #plasma #science #solarDynamics #sun
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Watch Hagfish Slime Unfurl
The eel-like hagfish has one of the best defenses in the ocean. When threatened, it releases a slime that clogs the gills of its predator but allows the hagfish itself to slough off the slime and escape. The hagfish slime’s secret weapon is long protein threads, which are initially rolled into bundles called skeins. Seen above, these skeins resemble the yarn skeins knitters and crocheters buy, but a hagfish’s skeins are only as big as the width of a human hair.
When water flows by quickly enough, the thread in a skein begins to unwind and stretch out. With enough threads unwound, the slime gets stretchy and viscous. Researchers found that it takes relatively little flow to begin this unwinding because the adhesion between threads and the surrounding fluid is higher than the thread-to-thread sticking power. (Research and image credit: M. Hossain et al., video)
#biology #fluidDynamics #hagfish #physics #rheology #science #viscoelasticity
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Watch Hagfish Slime Unfurl
The eel-like hagfish has one of the best defenses in the ocean. When threatened, it releases a slime that clogs the gills of its predator but allows the hagfish itself to slough off the slime and escape. The hagfish slime’s secret weapon is long protein threads, which are initially rolled into bundles called skeins. Seen above, these skeins resemble the yarn skeins knitters and crocheters buy, but a hagfish’s skeins are only as big as the width of a human hair.
When water flows by quickly enough, the thread in a skein begins to unwind and stretch out. With enough threads unwound, the slime gets stretchy and viscous. Researchers found that it takes relatively little flow to begin this unwinding because the adhesion between threads and the surrounding fluid is higher than the thread-to-thread sticking power. (Research and image credit: M. Hossain et al., video)
#biology #fluidDynamics #hagfish #physics #rheology #science #viscoelasticity
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Watch Hagfish Slime Unfurl
The eel-like hagfish has one of the best defenses in the ocean. When threatened, it releases a slime that clogs the gills of its predator but allows the hagfish itself to slough off the slime and escape. The hagfish slime’s secret weapon is long protein threads, which are initially rolled into bundles called skeins. Seen above, these skeins resemble the yarn skeins knitters and crocheters buy, but a hagfish’s skeins are only as big as the width of a human hair.
When water flows by quickly enough, the thread in a skein begins to unwind and stretch out. With enough threads unwound, the slime gets stretchy and viscous. Researchers found that it takes relatively little flow to begin this unwinding because the adhesion between threads and the surrounding fluid is higher than the thread-to-thread sticking power. (Research and image credit: M. Hossain et al., video)
#biology #fluidDynamics #hagfish #physics #rheology #science #viscoelasticity
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Watch Hagfish Slime Unfurl
The eel-like hagfish has one of the best defenses in the ocean. When threatened, it releases a slime that clogs the gills of its predator but allows the hagfish itself to slough off the slime and escape. The hagfish slime’s secret weapon is long protein threads, which are initially rolled into bundles called skeins. Seen above, these skeins resemble the yarn skeins knitters and crocheters buy, but a hagfish’s skeins are only as big as the width of a human hair.
When water flows by quickly enough, the thread in a skein begins to unwind and stretch out. With enough threads unwound, the slime gets stretchy and viscous. Researchers found that it takes relatively little flow to begin this unwinding because the adhesion between threads and the surrounding fluid is higher than the thread-to-thread sticking power. (Research and image credit: M. Hossain et al., video)
#biology #fluidDynamics #hagfish #physics #rheology #science #viscoelasticity
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Thawing Permafrost Primes Slumps
As permafrost thaws on Arctic hillsides and shorelines, the land often deforms in a unique fashion, known as a slump. Formally known as mega retrogressive thaw slumps, these areas superficially resemble a landslide. They’re also prone to repeat performances: as many as 90% of Canada’s Arctic slumps recur in the same place as previous slumps. Researchers used ground-penetrating radar and other tools to study the underground structure at slumps and found that several factors contribute to this repetitive cycle.
Seawater soaking into the foot of a hilly shore can destabilize the permafrost, creating a slump. That changes the nearby ground cover, exposing more permafrost to warming; their measurements showed this warming could extend tens of meters underground, priming the area for future slumps. Similarly, the mudslides and narrow ravines that form on an active slump also shift away ground cover and warm the underlying permafrost. Together, these factors suggest that once a slump forms, more slumps will occur as the underlying permafrost warms. (Image credit: M. Krautblatter; research credit: M. Krautblatter et al.; via Eos)
#erosion #fluidDynamics #geophysics #granularMaterial #physics #science #slump
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Thawing Out
Lake Erie, the shallowest of the Great Lakes, can almost completely freeze over in winter. In this satellite image of the lake in March 2025, about a third of the lake remains ice-covered, while sediment — resuspended by wind and currents — and phytoplankton swirl in the ice-free zone. In recent decades, scientists discovered that diatoms, one of the phytoplankton groups found in the lake, can live within and just below Erie’s ice, thanks to a symbiotic relationship with an ice-loving bacteria. This symbiosis allows the diatoms to attach to the underside of the ice and gather the light needed for photosynthesis. Even in the depths of winter, an ice-covered lake can teem with life. (Image credit: M. Garrison; via NASA Earth Observatory)
#biology #fluidDynamics #physics #phytoplankton #satelliteImage #science #sedimentation
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A Variety of Vortices
Winds parted around the Kuril Islands and left behind a string of vortices in this satellite image from April 2025. This pattern of alternating vortices is known as a von Karman vortex street. The varying directions of the vortex streets show that winds across the islands ranged from southeasterly to southerly. Notice also that the size of the island dictates the size of the vortices. Larger islands create larger vortices, and smaller islands have smaller and more frequent vortices. (Image credit: M. Garrison; via NASA Earth Observatory)
#flowVisualization #fluidDynamics #physics #satelliteImage #science #vonKarmanVortexStreet
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Capturing River Waves
Rainfall, ice jams, and dam breaks create surges of high flow that make their way down a river in a wave that stretches tens to thousands of kilometers in length. Traditionally, scientists monitor such flow waves using river gauges, which measure river height at specific locations. But gauges are few and far between on many rivers, so a group of researchers are supplementing that data with the SWOT (Surface Water and Ocean Topography) spacecraft. SWOT bounces microwaves off the water to precisely measure the water’s height, giving researchers a glimpse of the flow wave’s shape along the entire river.
In their paper, the team identify and describe flow waves on three different rivers — the Yellowstone, Colorado, and Ocmulgee rivers — ranging in height up to 9 meters and stretching up to 400 kilometers. (Image credit: CNES; research credit: H. Thurman et al.; via Gizmodo)
#flooding #fluidDynamics #geophysics #physics #rivers #satelliteImage #science
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South Island Sediments
In April and May late autumn storms ripped through Aotearoa New Zealand. This image shows the central portion of South Island, where coastal waters are unusually bright thanks to suspended sediment. We typically think of storm run-off as water, but these flows can carry lots of sediment as well. Here, the large amount of sediment is likely a combination of increased run-off from rivers and coastal sediment stirred up by faster river flows. (Image credit: W. Liang; via NASA Earth Observatory)
#flowVisualization #fluidDynamics #physics #satelliteImage #science #sedimentTransport #sedimentation
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Blooming in Blue
Summers in the Barents Sea — a shallow region off the northern coasts of Norway and Russia — trigger phytoplankton blooms like the one in this satellite image. The blue shade of the bloom suggests the work of coccolithophores, a type of plankton armored in white calcium carbonate. This type of plankton thrives in the warm, stratified waters of the late summer. Earlier in the year, the water tends to be nutrient-rich and well-mixed, conditions which favor diatom plankton species instead. Their blooms appear greener in satellite images. (Image credit: W. Liang; via NASA Earth Observatory)
#flowVisualization #fluidDynamics #mixing #physics #phytoplankton #satelliteImage #science #stratification
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“Dispersion”
In “Dispersion,” particles spread under the influence of an unseen fluid. Like Roman de Giuli’s work, filmmaker Susi Sie creates macro images that look like ice floes, deserts, and river deltas viewed from above. This similarity of patterns at both large and small scales is a specialty of fluid physics. Just as artists use it to mimic larger flows, scientists use it to study planet-scale problems in the lab. (Video and image credit: S. Sie et al.)
#dispersion #fluidDynamics #fluidsAsArt #granularFlow #granularMaterial #particulates #physics #reynoldsSimilarity #science
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If you sell #milkshakes, please include straws with rigidity commensurate with the static pressure conveyed by the thickness of the shake. So so so tired of straws collapsing just trying to drink through them... 😭
I mean, doesn't every ice cream shop owner study #FluidDynamics??? 👀😂
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Rolling Down Soft Surfaces
Place a rigid ball on a hard vertical surface, and it will free fall. Stick a liquid drop there, and it will slide down. But researchers discovered that with a soft sphere and a soft surface, it’s possible to roll down a vertical wall. The effect requires just the right level of squishiness for both the wall and sphere, but when conditions are right, the 1-millimeter radius sphere rolls (with a little slipping) down the wall.
Rolling requires torque, something that’s usually lacking on a vertical surface. But the team found that their soft spheres got the torque needed to roll from their asymmetric contact with the surface. More of the sphere contacted above its centerline than below it. The researchers compared the way the sphere contacted the surface to a crack opening (at the back of the sphere) and a crack closing (at the front of the sphere). That asymmetry creates just enough torque to roll the sphere slowly. The team hopes their discovery opens up new possibilities for soft robots to climb and descend vertical surfaces. (Image and research credit: S. Mitra et al.; via Gizmodo)
#adhesion #fluidDynamics #physics #science #slip #softMatter #solidMechanics
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🤓 Oh joy, another thrilling episode of "Let's Pretend We Understand Hilbert and Boltzmann" — because fluid dynamics and kinetic theory are obviously everyone's favorite cocktail party topics. 🍸🔬 Good luck keeping your eyes open through this math-induced coma! 😴💤
https://arxiv.org/abs/2503.01800 #HackerNews #FluidDynamics #KineticTheory #MathHumor #ScienceComedy #HackerNews #ngated -
Thawing Permafrost Primes Slumps
As permafrost thaws on Arctic hillsides and shorelines, the land often deforms in a unique fashion, known as a slump. Formally known as mega retrogressive thaw slumps, these areas superficially resemble a landslide. They’re also prone to repeat performances: as many as 90% of Canada’s Arctic slumps recur in the same place as previous slumps. Researchers used ground-penetrating radar and other tools to study the underground structure at slumps and found that several factors contribute to this repetitive cycle.
Seawater soaking into the foot of a hilly shore can destabilize the permafrost, creating a slump. That changes the nearby ground cover, exposing more permafrost to warming; their measurements showed this warming could extend tens of meters underground, priming the area for future slumps. Similarly, the mudslides and narrow ravines that form on an active slump also shift away ground cover and warm the underlying permafrost. Together, these factors suggest that once a slump forms, more slumps will occur as the underlying permafrost warms. (Image credit: M. Krautblatter; research credit: M. Krautblatter et al.; via Eos)
#erosion #fluidDynamics #geophysics #granularMaterial #physics #science #slump
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Thawing Permafrost Primes Slumps
As permafrost thaws on Arctic hillsides and shorelines, the land often deforms in a unique fashion, known as a slump. Formally known as mega retrogressive thaw slumps, these areas superficially resemble a landslide. They’re also prone to repeat performances: as many as 90% of Canada’s Arctic slumps recur in the same place as previous slumps. Researchers used ground-penetrating radar and other tools to study the underground structure at slumps and found that several factors contribute to this repetitive cycle.
Seawater soaking into the foot of a hilly shore can destabilize the permafrost, creating a slump. That changes the nearby ground cover, exposing more permafrost to warming; their measurements showed this warming could extend tens of meters underground, priming the area for future slumps. Similarly, the mudslides and narrow ravines that form on an active slump also shift away ground cover and warm the underlying permafrost. Together, these factors suggest that once a slump forms, more slumps will occur as the underlying permafrost warms. (Image credit: M. Krautblatter; research credit: M. Krautblatter et al.; via Eos)
#erosion #fluidDynamics #geophysics #granularMaterial #physics #science #slump
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A Sandy Spine
Where sea and sand meet, Gaia’s spine rises. Photographer Satheesh Nair captured this striking image in western Australia, where wind and wave action have dragged a dune into vertebrae-like cusps. Notice how the size and shape of the curves differs between the under- and above-water sections. Those differences reflect the differing forces that shape them — just water for one set, water and air for the other. (Image credit: S. Nair/IAPOTY; via Colossal)
#beachCusps #fluidDynamics #fluidsAsArt #oceanWaves #physics #science #sedimentTransport #sedimentation