Image:Coriolis effect15.gif

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Description:
Illustration for Coriolis effect article.
Elliptical orbit in the presence of a centripetal force that is proportional to the distance to the center of rotation.
The parametric equation is as follows:

x = a * cosω
y = b * sinω

This can also be written as follows, showing that the elliptical motion with that particular velocity profile can be seen as a vector addition of two uniform circular motions:

x =(\frac{a+b}{2})\cos\omega + (\frac{a-b}{2})\cos\omega
y =(\frac{a+b}{2})\sin\omega - (\frac{a-b}{2})\sin\omega

To be used in conjunction with the animations Image:Coriolis_effect06.gif and Image:Coriolis_effect.07.gif.

Created: august 16, 2005

Author: Cleon Teunissen


I, the author of this work, hereby publish it under the following licenses:
GNU head Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled "GNU Free Documentation License".

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