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Space Grant Consortium - University of Wisconsin - Green Bay

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Reflection and Refraction <strong>of</strong> Vortex Rings ∗<br />

Kerry Kuehn, Matthew Moeller, Michael Schulz and Daniel Sanfelippo<br />

Department <strong>of</strong> Physical Sciences<br />

<strong>Wisconsin</strong> Lutheran College, Milwaukee, WI<br />

Abstract<br />

We have experimentally studied the impact <strong>of</strong> a planar axisymmetric vortex ring,<br />

incident at an oblique angle, upon a sharp gravity-induced interface separating two<br />

fluids <strong>of</strong> differing densities. After impact, the vortex ring was found to exhibit a variety<br />

<strong>of</strong> subsequent trajectories, which we have organized according to both the incidence<br />

angle, and the ratio <strong>of</strong> the Atwood and Froude numbers, A/F . For relatively small<br />

angles <strong>of</strong> incidence, the vortices tended to penetrate the interface. In such cases, the<br />

more slowly moving vortices, having values <strong>of</strong> A/F � 0.004, tended to subsequently<br />

curve back up toward the interface. Quickly moving vortices, on the other hand, tended<br />

to refract downward, similar to a light ray entering a medium having a higher refractive<br />

index. A simplistic application <strong>of</strong> Snell’s law <strong>of</strong> refraction cannot, however, account<br />

for the observed trajectories. For grazing angles <strong>of</strong> incidence, fast moving vortices<br />

tended to penetrate the interface, whereas slower vortices tended to reflect from the<br />

interface. In some cases, the reflected vortices executed damped oscillations before<br />

finally disintegrating.<br />

Introduction<br />

One <strong>of</strong> the early successes <strong>of</strong> the wave theory <strong>of</strong> light was its ability to explain the law <strong>of</strong><br />

refraction by appealing to the variation <strong>of</strong> the speed <strong>of</strong> light when crossing a boundary separating<br />

media <strong>of</strong> different densities [Huygens, 1952]. Early models <strong>of</strong> light which emphasized<br />

its corpuscular nature proved less convincing in explaining refraction, largely because these<br />

models required that light travel more rapidly when entering a denser media, such as water<br />

or glass, an ostensibly counterintuitive postulate which was later rejected on experimental<br />

grounds [Smith, 1987].<br />

With the advent <strong>of</strong> Hamilton-Jacobi theory [Wolf and Born, 1965], and later wave mechanics<br />

[Schrödinger, 1964], the refraction <strong>of</strong> light was eventually reconciled with a corpuscular<br />

nature, albeit only in a statistical sense. Quantum theory, <strong>of</strong> course, makes no predictions<br />

as to the trajectory <strong>of</strong> an individual photon. Nonetheless, recent experiments in high energy<br />

physics and quantum optics have revived a significant amount <strong>of</strong> speculation as to the<br />

nature, and even the structure, <strong>of</strong> the photon [Nisius, 2000, Tiwari, 2002].<br />

tium.<br />

∗ This work was supported by a Research Infrastructure <strong>Grant</strong> from the <strong>Wisconsin</strong> <strong>Space</strong> <strong>Grant</strong> Consor-<br />

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