FYFD

Tag: fluid dynamics

  • Avoiding Ice

    Avoiding Ice

    Keeping ice from forming on a surface is a major engineering challenge. Typically, there’s no controlling certain factors – like the size and impact speed of droplets – so engineers try to tame ice by changing the surface. This can be through chemicals – as with deicing fluids used on aircraft – or by tuning the surface itself.

    One way to do this is by making the surface superhydrophobic – or extremely water repellent. These surfaces are rough on a nanoscale level, but they’re delicate, and once ice gets a grip on them, it’s even harder to remove. In a recent study, however, researchers used particles with both hydrophobic and hydrophilic – water-attracting – properties to create a superior ice-resistant surface. The combination of hydrophobic and hydrophilic aspects to the particles made supercooled droplets break up on contact with the surface. This made the drops smaller and decreased their contact time, making it harder for them to stick and freeze. (Image credit: Pixabay; research credit: M. Schwarzer et al.; via Chembites; submitted by Kam-Yung Soh)

  • Simulating Solar Flares

    Simulating Solar Flares

    Few topics in fluid dynamics are more mathematically complicated than magnetohydrodynamics – the marriage between electromagnetism and fluids. That mathematical complexity, along with the vast range of scales necessary to describe physical systems like our sun, means that, until now, researchers had to simplify their assumptions when simulating solar physics. But now, for the first time, a group has built a comprehensive, three-dimensional simulation capable of generating realistic solar flares. This is what you see above.

    Solar flares occur when a tangle of magnetic loops near the sun’s surface break and reconnect, releasing enormous magnetic energy and spewing a fountain of ionized plasma into the corona. They’re a danger particularly to satellites in orbit, so being able to simulate these events realistically is a major advance toward understanding the physics of space weather. (Image and video credit: NCAR & UCAR Science; research credit: M. Cheung et al.; via Bad Astronomy; submitted by Kam-Yung Soh)

  • Liquid Antispiral

    Liquid Antispiral

    Spiral formations are common in nature, from galaxies to chemical reactions. But most examples in nature rotate such that their arms trail the direction of rotation. Viewed side-on, this makes the arms appear to spiral outward from the the center. The opposite – an antispiral, where the arms appear to be drawn in toward the center – also exists, but there are far fewer examples. Which is why it’s notable that physicists have described a new one, seen above.

    You’re watching silicone oil draining through a plate with an array of holes in it. There’s a reservoir of oil on top supplying a constant flow rate. The patterns that form in this system vary widely – they can form between one and six arms – but the results are always antispirals. The driving mechanism seems to be the periodic nature of the discharge from individual holes, which is caused by a Rayleigh-Taylor instability. Hopefully systems like this can shed some light on why spirals are often preferred over antispirals. (Image and research credit: H. Yoshikawa et al.; via APS Physics)

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    Worthington and His Jets

    If you’ve been around fluid mechanics for very long, you’ve probably noticed that we like to name things after people. (Mostly dead, white guys, but that’s another subject.) Whenever someone describes or explains a new phenomenon, it tends to get their name attached to it. Some of the common names in fluid dynamics – Reynolds, Rayleigh, Kelvin, Taylor, von Karman, Prandtl – read like a who’s-who of nineteenth and twentieth century physics. This video gives some historical insight into a couple of those figures – particularly Arthur Worthington, who is known for his contributions to the understanding of splashes. Be sure to check out some of his awesome illustrations and photos. Can you imagine being able to piece together splash physics like that without high-speed video?! (Video credit: Objectivity; submitted by Kam-Yung Soh)

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    The Polar Vortex

    Every year or two, the Northern Hemisphere gets treated to a bout of intensely cold temperatures thanks to the polar vortex. What you may not realize, though, is that it’s not the polar vortex that causes this cold weather – it’s the vortex breaking down. As Simon Clark explains in this video, the polar vortices (one at each pole) are intense and powerful regions of circulation in the stratosphere, or mid-atmosphere. They’re largely responsible for keeping cold air trapped in the Arctic and Antarctic. But occasionally, this region of the atmosphere will suddenly get warmer – to the tune of increasing by 80 degrees Celsius in less than a week! When this happens, a polar vortex will deform and potentially even split into smaller vortices, as seen below. When this happens, the vortex loses its hold on the cold air near the surface, allowing Arctic air to sneak as far south as Texas. After a couple of weeks of affecting our weather, the polar vortex will typically reform and we’ll return to normal. In the meantime, stay warm! (Video and image credit: S. Clark; submitted by Nikhilesh T.)

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    Dripping Down the Rivulet

    If you’ve ever watched water running down the side of the street, you’ve probably noticed that it doesn’t flow smoothly. Instead, you’ll see waves, rivulets, and disturbances that form. That’s because the simple action of flowing down an incline is unstable. Water and other viscous liquids can’t flow downhill smoothly. Any disturbances – an uneven surface, the rumble of passing cars, a pebble in the way – will create a disruption that grows, often until the entire flow is affected. This video shows some of the complex and beautiful patterns you get then. (Video and image credit: G. Lerisson et al.)

  • Enormous Ice Disk

    Enormous Ice Disk

    We’ve seen spinning ice disks before, but this month Westbrook, Maine has developed the largest one I’ve ever seen. A research paper from 2016 indicates that this seemingly alien formation spins due to an oddity of water. Water is at its densest around 4 degrees Celsius, so as the ice of the disk melts in the warmer waters of the river, it sinks. That downward plume sets up a vortex in the water beneath the disk. And as the water spins, it drags the ice with it, causing the disk’s rotation. The warmer the water is, the faster the disk spins. (Image credit: T. Radel/City of Westbrook; research credit: S. Dorbolo et al.; via Gizmodo; submitted by jpshoer)

  • An Inverted Leidenfrost Drop

    An Inverted Leidenfrost Drop

    Leidenfrost drops – liquid drops that levitate on a layer of their own vapor over a hot surface – have been all the rage in recent years. We’ve seen how they can be guided, trapped, and self-propelled. What you see here is a bit different. This is a droplet of room-temperature ethanol deposited on a bath of liquid nitrogen. What levitates the droplet in this case is vaporous nitrogen evaporating from the bath.

    The droplet is quickly cooling down; it freezes after its second or third bounce off the side walls of the beaker. What causes the droplet to self-propel is an asymmetry of the thin vapor layer beneath the droplet. As soon as some instability causes a slight difference in the thickness of the vapor layer, that triggers the propulsion, which the drop maintains even after freezing. (Image and research credit: A. Gauthier et al.)

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    The Boston Molasses Flood

    Today marks the 100th anniversary of the Boston Molasses Flood, and to commemorate this bizarre disaster, I’ve made a video about the key findings from my research with colleagues at Harvard University. Check it out below!

    And, if you’re still hankering to learn more about the Molasses Flood, here are some recent articles and interviews on the subject:

    – Boston.com
    – NBC News
    –  New England News Collective
    – Historium Unearthia podcast

     (Video and image credits: N. Sharp)

  • Lava Bomb

    Lava Bomb

    What you see above is a homemade lava bomb. To systematically study what happens when groundwater meets lava, scientists melted basalt and created their own meter-scale explosion-on-demand. Inside the container, they can inject water and observe the resulting dynamics.

    Beneath the lava, the water forms what scientists call a domain. Thanks to the Leidenfrost effect, it can be protected from direct contact with the lava by a thin vapor layer that boils off it. If the water domain is large enough, buoyancy will pull it upward through the lava. Whether the water maintains a spherical shape or begins to distort and break up into smaller domains depends on the speed of its rise.

    At some point, though, either naturally or through an external trigger (like the sledgehammer you see above), the water and lava can contact, resulting in explosive vaporization of the water and an explosion. What’s visible at the surface depends on the depth at which the explosion takes place. Scientists are eager to characterize these variations, which will help them better predict the explosive danger of eruptions like Kilauea and Eyjafjallajökull. (Image and research credit: I. Sonder et al.; video credit: NYTimes; submitted by Kam-Yung Soh)