SUMMARY
The expression for pressure distribution in a rotating tornado can be derived using the hydrostatic equation, which states that the pressure gradient is equal to the product of air density and radial acceleration. Given a tornado with constant angular velocity ##\omega## and uniform temperature T, the pressure gradient can be expressed as ##\frac{dp}{dr} = \rho (\omega^2 r)##. To calculate the central pressure ##p_0##, one must apply the ideal gas law, which relates pressure, density, and temperature. For the conditions specified (T = 300 K, p = 100 kPa at 0.1 km), the density must be determined to find ##p_0##.
PREREQUISITES
- Understanding of hydrostatic equations in fluid dynamics
- Familiarity with the ideal gas law (PV = nRT)
- Knowledge of angular velocity and radial acceleration concepts
- Basic principles of atmospheric pressure and density relationships
NEXT STEPS
- Study the derivation of the hydrostatic equation in rotating systems
- Learn about the application of the ideal gas law in dynamic environments
- Research the effects of angular velocity on pressure distribution in fluids
- Explore numerical methods for modeling tornado dynamics and pressure fields
USEFUL FOR
Students in meteorology, physicists studying fluid dynamics, and engineers involved in atmospheric modeling will benefit from this discussion.