October 2000: practicum proposed to design and build spin tank
January 2001: begin work on ideas, theory, desired demonstrations
February 2001: get donated base and platter from CU
March 2001 - September 2001: work on tank, mechanics, electronics
September 2001: present spin tank to department at seminar
October 2001 - present: use spin tank in classrooms
May 2002: submit paper to BAMS on design and construction of spin tank
August 2002 - December 2002: practicum on rotating convection
April 2003: submit revised final manuscript to BAMS
December 2003: paper published in BAMS (DOWNLOAD PDF)
January 2004 - May 2004: practicum on Hadley/Rossby waves
Power demand through slip rings: 115W [40W (x2) for lights, 35W for camcorder]
Current demand through slip rings: 0.95A [.33A (x2) for lights, .29A for camcorder]
Tank material: 1.3 cm thick acrylic from Regal Plastics
Tank adhesive: IPS Weld-On #16
Tank dimensions: 50.8 cm internal diameter, 53.4 cm external diameter, 61.0 cm height
Base dimensions: 92.0 cm long, 61.0 cm wide, 40 cm tall (55 cm with platter, 177 cm with superstructure)
Maximum tank capacity: 124 kg water
Motor type: Oriental Motor model FBL5120AW-50
Maximum motor horsepower/power: 0.17hp / 120W
Maximum motor angular velocity: 3.0 rad/s
Maximum motor torque: 34.0 N m
Motor drive cord: Polycord UPRB2 (1/8" diam)
Digital Camcorder: Canon ZR-20
Acrylic (tube and sheets): $960
Motor (controller, dial, wheel, drive cord): $740
Hardware, Tools, Misc. supplies: $400
Superstructure (rods, clamps, lights): $215
Shop labor: $200
Wooden platform (with wheels, handle): $175
TOTAL: ~$2690
Ekman pumping works on the principle of frictional geostrophic motion. If the fluid is at solid body rotation and the rotation rate is then increased, the bulk of the fluid (except near the walls) is now in relative motion to the new rotation rate of the inertial reference frame. A frictional, viscous layer is created along the floor (Ekman layer) and the walls (Stewartson layer) of the tank. At this point, the geostrophic balance between Coriolis force and pressure gradient force is destroyed, and the Coriolis force dominates, forcing mass transport to the right of the surface stress, or outward along the floor of the tank and upward along the walls. A secondary circulation is then induced.
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The Taylor-Proudman Theorem states that the motion of a homogeneous fluid will be the same in all planes perpendicular to the axis of rotation, assuming friction is negligible and the Rossby number is small. The water is brought up to solid body rotation and an obstacle (can of cat food) is placed on the bottom of the tank approximately 2/3 out from the center. If the rotation rate is then increased slightly, a relative flow around the obstacle will be introduced, and the flow pattern at low levels will be mirrored at all depths in the fluid, creating a Taylor column.
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While experimenting with spin-up and spin-down, it is easy to produce flow instabilities. For example, near the end of the spin-up process shown in the previous Ekman pumping section, water containing red and green dye has moved radially outward along the bottom, up the side wall, and then radially inward a small distance, stopping its inward radial displacement when spin-up is complete. We end up with a banded pattern near the outer edge of the tank. Now suppose the rotation rate of the tank is abruptly (but within reason) and significantly decreased. The relative flow is now counterclockwise, with a large radial shear of the azimuthal velocity near the edge of the tank (see below). In this region of large shear, barotropic instability begins to set in, as shown by the waviness in the upper right figure below. As this instability extracts increasing amounts of kinetic energy from the primary circulation, the waves continue to amplify, resembling the cresting and breaking of ocean waves, as shown in the bottom row of figures. These eddies can rapidly mix the dye, leaving a featureless colored haze. This process can be repeated over and over until the water is too murky with dye to see these features. If the change in rotation rate is not large enough, the spin-up time will actually be shorter than the time required to set up the barotropic instability, and the aforementioned features will never be seen.
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