12 Oct '16 05:29>1 edit
Originally posted by joe shmoThat is because you are using the rotation vector in the inertial frame for a calculation in the rotating frame. In a local frame at the equator with a vector i pointing eastwards, j pointing north and k pointing straight upwards then at the equator Ω = Ωj. Assuming no upwards movement our velocity vector has components (in the rotating frame) v = v_xi + v_yj. Now the cross product comes to Ωxv = Ωv_xjxi + Ωv_yjxj = -Ωv_xk and the acceleration is directly upwards. So in the rotating frame in the restriction to the two dimensional plane tangent to the Earth's surface the Coriolis force is zero at the equator. In the full three dimensional setting there is a component upwards, but that's irrelevant to meteorology.
There is no way this answer you provided is correct.
"[b]1) Ω=0 ...The Earth is not rotating (relative to an object at the equator)."
The Earth having a rotation is independent of where any body is placed on it.
The Coriolis Force doesn't disapear. It just becomes a radial force at the equator.
Lets align the standard coordinate system so ...[text shortened]... ce goes to zero please elaborate on what I'm donig incorrectly...I honestly can't figure it out?[/b]
What one could do is measure the period of a pendulum on a train going round the equator at high(ish) speed. The Coriolis acceleration upwards is 4πv/T, where v is the speed of the train. There are 86400 seconds in a day which gives us an angular speed of Ω = 2π/T = 7.3e-5 radians per second. A realistic speed for a train is 125 mph or 200 kmh which comes to 55m/s. So the acceleration is 0.008 m/s/s for an effect of a little under 1 part in a thousand. This is a fairly small effect, but I don't see any reason that the experiment wouldn't work. For a long enough railway line at the equator one could just use a 25 cm pendulum which has a period of 1 second and run the experiment for an hour or so. The pendulum should swing around seven more times going west than it will going east. I think this really would demonstrate rotation of the Earth as it seems less vulnerable to local variations in the gravitational field and doesn't require one to work out the difference between downwards and the direction to the centre of the Earth.