FYFD

Category: Research

  • What Controls an Avalanche?

    What Controls an Avalanche?

    In an avalanche, grains spontaneously flow when a slope reaches a critical angle, and they continue flowing until they settle at a new, lower angle. Scientists have long debated why this angle mismatch occurs, and, in recent years, the general opinion was that the avalanche’s inertia kept it flowing long enough to settle at a lower angle. But a new experiment, using a slowly-rotating drum similar to the one above*, shows that friction, not inertia, is the key player. 

    The researchers used silica beads suspended in water, which allowed them to cleverly control the interparticle friction. In water, silica beads build up negative electrostatic charges, which push the grains apart and eliminate friction. In that frictionless state, the researchers found that the beads tumbled smoothly; their starting and ending angles were always the same. 

    By adding salt to the water, the researchers were able to eliminate some of the electrostatic charge and thereby tune the friction. When they did that, the difference between starting and stopping angles came back and grew more substantial as the friction increased. All in all, the results indicate that friction between particles is what makes an avalanche avalanche. (Image credit: J. Gray and V. Chugunov, source; research credit: H. Perrin et al.; via APS Physics; submitted by Kam-Yung Soh)

    * If you’re curious about the patterns in the image, I explain them in this previous post.

  • Inside the Canopy

    Inside the Canopy

    If you’ve ever gone into the woods on a windy day, you know that conditions there are drastically different than in the open. To blowing wind, trees of different sizes act like enormous roughness that disturbs the flow. Inside the canopy, flows can become incredibly complicated and many of the common techniques used by researchers no longer hold. 

    You can get a sense for this complexity with the second image above, which visualizes data from a wind tunnel experiment. The gray blocks represent roughness elements – the trees of this wind-tunnel-scale forest – and the large, blue arrow shows the direction of the flow. The thin colored lines show the paths taken by particles in the flow. The lines’ colors indicate what height the trajectory began at. 

    Notice how the blue and purple lines are relatively straight and oriented in the direction of the flow. This indicates that the flow here is relatively steady and uncomplicated. At the lower heights, though, especially in the green and yellow regions, the pathlines are far more twisted and complex. The flow here is turbulent, and the particles’ trajectories don’t necessarily correlate at all to the winds higher up. (Image credit: T. Japyassu and R. Shnapp et al.; research credit: R. Shnapp et al.; submitted  by Ron S.)

  • Asymmetric Wakes

    Asymmetric Wakes

    When a ship moves through water, it leaves a distinctive V-shaped wake behind it. In the nineteenth century, Lord Kelvin made some of the earliest theoretical studies of this phenomenon, calculating that the arms of the V should have an angle of about 39 degrees, known as the Kelvin angle. But that theoretical result doesn’t always hold in practice.

    More recently, researchers calculated and experimentally verified an extension to Kelvin’s theory, one which accounts for what’s going on below the water. They found that any shear in the currents below the surface can strongly affect the shape of a boat’s wake, altering angles and creating asymmetry between the two sides. The results have practical consequences, too: they help predict the wave resistance ships will encounter when traversing areas with substantial subsurface shear, like near the mouths of river deltas. (Image credit: M. Adams; research credit: B. Smeltzer et al.; submitted by clogwog)

  • Cavitation Collapse

    Cavitation Collapse

    The collapse of a bubble underwater doesn’t seem like a very important matter, but when it happens near a solid surface, like part of a ship, it can be incredibly destructive. This video, featuring numerical simulations of the bubble’s collapse, shows why. 

    When near a surface, the bubble’s collapse is asymmetric, and this asymmetry creates a powerful jet that pushes through the bubble and impacts the opposite side. That impact generates a shock wave that travels out toward the wall. As the bubble hits its minimum volume, a second shock front is generated. Both shock waves travel toward the wall and reflect off it, generating high pressure all along the surface. (Image and video credit: S. Beig and E. Johnson)

  • Breaking Up

    Breaking Up

    The dripping of a faucet and the break-up of a jet into droplets is universal. That means that the forces – the inertia of the fluid, the capillary forces governed by surface tension, and the viscous dissipation – balance in such a way that the initial conditions of the jet – its size, speed, etc. – don’t matter to the process of break-up. 

    We’d expect that the inverse situation – the breakup of a gas into bubbles in a liquid – would be similarly universal, but it’s not. When unconfined bubbles pinch off, the way they do so is heavily influenced by initial conditions. But that changes, according to a new study, if you confine the gas to a liquid-filled tube before pinch-off. Confinement forces a different balance between viscous and capillary effects, one which effectively erases the initial conditions of the flow and restores universality to the pinch-off process. (Image and research credit: A. Pahlavan et al.; via phys.org)

  • Splashes on Hairy Surfaces

    Splashes on Hairy Surfaces

    The question of whether a droplet will splash is a complicated one, even for smooth surfaces, but researchers are also interested in what happens to hairy surfaces when droplets strike. By varying the droplet viscosity and speed, along with the spacing of the hairs, researchers sketched out the variety of impacts one can get. 

    What happens during impact depends largely on how the kinetic energy of the droplet compares to the dissipation caused by interaction with the hairs. When the two balance, the droplet gets captured, like in the upper right image. If the hairy dissipation wins, you get a drop that stays mostly on the surface of the hairs. And if the kinetic energy outweighs the dissipation, you end up with a star-shaped splash that spreads between the hairs. (Image and research credit: A. Nasto et al.)

  • Hiding From Waves

    Hiding From Waves

    Ocean waves can be dangerous for boats, particularly when operating near off-shore platforms. But a new study, inspired by electromagnetic waveguides, demonstrates a lab-scale water waveguide capable of damping out a range of waves experienced by any ship inside its protected area. The water waveguide sits below the surface, changing the water depth and therefore the propagation of surface waves. 

    When properly positioned, the waveguide nearly eliminates wave motion in a protected channel. You can see this in the right image, where waves are clearly present in the foreground but the toy boat hardly moves. Contrast this with the image on the left, where the boat bobs and rocks under the same wave conditions without the waveguide. The researchers hope their waveguide concept can help protect ships in wharves and harbors soon. (Image and research credit: S. Zou et al.; via APS Physics; submitted by Kam-Yung Soh)

  • Blowing Smoke

    Blowing Smoke

    It’s unusual – but not entirely unheard of – to see volcanoes blowing smoke rings during inactive periods. But given their unpredictability, scientists had not studied this phenomenon in much depth. In a recent presentation, though, a group unveiled results from numerical studies of volcanic vortex rings. They found that the decreasing pressure on rising magma allows dissolved gases to emerge as bubbles. If the magma has the right viscosity, those bubbles can merge into one big pocket that depressurizes explosively in the vent. As the hot gases burst upward, the walls of the vent cause them to curl up into a vortex ring, provided the vent is fairly circular and uniform. That sends the roiling vortex up into the atmosphere, where it cools, condenses, and becomes visible.

    The need for a circular vent matches observations of volcanic vortex rings in nature, like the infrared image shown above. Volcano watchers find that vortex rings only form from some vents, and the more circular the vent, the more likely it can produce vortex rings. (Image credit: B. Simons; research credit: F. Pulvirenti et al.; via Nat Geo; submitted by Kam-Yung Soh)

  • Featured Video Play Icon

    How Ant Stingers Work

    Anyone who’s felt the sting of a fire ant knows it only takes an instant for this species to deliver a painful blow. Scientists are uncovering why that is using some of the first-ever high-speed footage of ant stingers in action. Stingers are actually made up of multiple separate pieces, including a central stylet and a pair of lancets that move up and down along the stylet. This lancet motion pulls the stinger deeper and helps form and deliver droplets of venom. The back-and-forth motion helps ants release up to 13 venom droplets per second, a level of speed that’s key for some of its high-speed, small-scale battles. (Image and video credit: Ant Lab; research credit: A. Smith)

  • Plasma Shock Waves

    Plasma Shock Waves

    Solar flares and coronal mass ejections send out shock waves that reverberate through our solar system. But shock waves through plasma – the ionized, high-energy particles making up the solar wind – do not behave like our typical terrestrial ones. Instead of traveling through collisions between particles, these astrophysical shock waves are driven by interactions between moving, charged particles and magnetic fields. 

    A driving burst of plasma accelerated into ambient plasma creates electromagnetic forces that accelerate ambient ions to supersonic speeds, pushing the shock wave onward even without particles directly colliding. Thus far, piecing together the physics of these interactions has been a challenge because spacecraft are limited in what and where they can measure. But a group here on Earth has now recreated and observed some of this process in the lab. (Image credit: NASA Solar Dynamics Observatory; research credit: D. Schaeffer et al.; via phys.org)