Year: 2011

  • Reader Question: Rotor Ships

    Reader Question: Rotor Ships

    lazenby asks:

    Can you explain how the magnus effect makes rotor ships move?

    When a spinning body is placed in a flow, the body experiences a force perpendicular to the direction of the flow. This is called the Magnus effect and is, for example, why baseballs, soccer balls, and tennis balls veer from the path we expect them to take. To understand why a spinning body experiences this force, take a look at the streamlines around a rotating cylinder.

    In this picture, the flow goes from left to right and the cylinder is spinning in the clockwise direction. The red dots represent the stagnation points of the flow. Air over the top of the cylinder gets accelerated by the spinning, shown here by the narrowing of space between streamlines. On the underside of the cylinder, the surface is moving in the opposite direction of the air, which decelerates the flow. We know from Bernoulli that this means there is low pressure on the top of the cylinder and high pressure on the bottom. As a result, the cylinder experiences a upward force – lift! You can explore the effect of rotation on the streamlines yourself using this neat demo from Wolfram.

    Rotor ships, invented in the 1920s, used this effect for ship’s propulsion. They used a regular motor to begin moving, and, once they had some wind, used motors to spin giant cylinders on the deck. As the rotors spun, the ships were pushed in a direction perpendicular to the wind. They could apparently tack 20-30 degrees into the wind while conventional ships could only manage 45 degrees. Unfortunately, so much energy was required to spin the rotors that the design was pretty inefficient and never caught on.

  • Hello, New Folks!

    Lots of new faces around here at FYFD, so thanks, everyone, for spreading the word! As a reminder, you’re welcome to submit post ideas if you see something neat online and you can also ask any questions you have related to fluid mechanics, and I’ll do my best to answer them or find someone who can! I also respond to comments on Twitter, if you prefer.

  • Hole-Punch Clouds

    Hole-Punch Clouds

    These hole-punch clouds seen over Myrtle Beach, SC were probably caused by three aircraft flying in military formation. When airplanes pass through supercooled water vapor, the acceleration of air over the wing causes a pressure drop that can flash-freeze the water vapor, resulting in a localized snow shower. See National Geographic for more. #

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    How Ferrofluids Work

    Here’s a ferrofluid video with a little more explanation about how ferrofluids work. Surfactants prevent the tiny magnetic particles suspended in the fluid from separating out when exposed to a magnetic field.

  • Marangoni Effect

    Marangoni Effect

    Dyed milk pulls away after a drop of acetone is added. The acetone creates a gradient in the surface tension, which causes mass flow due to the Marangoni effect. See a video of the effect (or try it yourself at home!) here.

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    Geometrical Droplet Splashes

    Sadly, this video shows no droplet impacts on a heart-shaped post, but maybe you can imagine what it would look like after seeing other geometrical shapes. Happy Valentine’s Day, guys!

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    High-Speed Leidenfrost Levitation

    The Leidenfrost effect occurs when a liquid encounters a surface with a temperature much higher than its boiling point. Some of the liquid is instantly vaporized and then a droplet will skate across the surface on that vapor. This video shows the process at 3000 frames per second.

  • Volcanic Turbulence

    Volcanic Turbulence

    One of the characteristics of turbulence is its large range of lengthscales. Consider the ash plume from this Japanese volcano. Some of the eddy structures are tens, if not hundreds, of meters in size, yet there is also coherence down to the scale of centimeters. In turbulence, energy cascades from these very large scales to scales small enough that viscosity can dissipate it. This is one of the great challenges in directly calculating or even simply modeling turbulence because no lengthscale can be ignore without affecting the accuracy of the results. #

  • Reader Question: Froude vs. Reynolds

    @spooferbarnabas asks: I was wondering what the difference is between Froude’s number and Reynold’s number? they seem very similar

    Fluid dynamicists often use nondimensional numbers to characterize different flows because it’s possible to find similarity in their behaviors this way. The Reynolds number is the most common of these dimensionless numbers and is equal to (fluid density)*(mean fluid velocity)*(characteristic length)/(fluid dynamic viscosity). The Reynolds number is considered a ratio of total momentum (or inertial forces) to the molecular momentum (or viscous forces). A small Reynolds number indicates a flow dominated by viscosity; whereas a flow with a large Reynolds number is considered one where viscous forces have little effect.

    The Froude number, in contrast, focuses on resistance to flow caused by gravitational effects, not molecular effects. It is defined as (mean fluid velocity)/(characteristic wave propagation velocity). Initially, it was developed to describe the resistance of a model floating in water when towed at a given speed. As the boat’s hull moves through the water, it creates a wave that travels forward (and backward in the form of the wake), carrying information about the boat–much like pressure waves travel before and behind a subsonic aircraft. The speed of the wave created by the boat depends on gravity (see shallow water waves). The closer the boat’s speed comes to the water wave’s speed, the greater the resistance the boat experiences. In this respect, the Froude number is actually analogous to the Mach number in compressible fluids.

    I hope that helps explain some of the differences!

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    The Pistol Shrimp’s Secret Weapon

    The pistol shrimp (or pistol crab) is a finger-sized crustacean with a fluid dynamical superpower. When it snaps its claw, a jet of water shoots out so quickly (62 mph) that a low-pressure bubble forms in its wake. When the bubble collapses, it emits a bang and a flash of light in a process known as sonoluminescence. The whole event takes less than 300 microseconds. The light emitted suggests that temperatures inside the bubble reach 5,000 degrees Kelvin, around the temperature of the surface of the sun. #