What I never understood is that when viewing a sattelite photo of the earth, people tend to say that the curly movement of the clouds is due to the Coriolis force. The Coriolis force emerges because one goes to a non-inertial frame, so on the Earth one would experience the Coriolis force, while in outer space, one would NOT experience something like a Coriolis force.
Maybe this video helps,
The mathematical easiest way to see the emergence of inertial forces is, I think, the following: consider Newton's law in Cartesian coordinates, which holds in inertial frames:
[tex]
\frac{d^2 x^i}{dt^2} = 0[/tex]
Now one goes (transforms) to a rotating frame. This can be achieved by
[tex]
x^i \rightarrow x^{'i} = R^i_{\ j}(t) x^j \ \ ,[/tex]
where R is an element of SO(3) (which describes rotations), but in which the angles can be arbitrary functions of time t. Plugging this in Newton's law gives
[tex]
\ddot{R}^i_{\ j}(t)x^j + 2 \dot{R}^i_{\ j}(t)\dot{x}^j + R^i_{\ j}(t)\ddot{x}^j = 0[/tex]
Using the orthogonality of the rotation matrices R (which, ofcourse still holds if you make the angles time dependent) you see the centrifugal force (first term) and Coriolis force (second term) arising. If you take an explicit example, like a rotation around the z-axis, you can explicitly calculate the corresponding R and see that it coincides with the expressions you learn in classical mechanics.