Bifocal frame of reference
One calls bifocal frame of reference compared to two points A1 (0,0, a) and A2 (0,0, - A), a system where the current point P is located by its Azimut, and its distance A1P and A2P.
The practice is to pose:
U = + A2P /2a and v = A1P - A2P /2a.
Application
In mechanics, it is very much used as soon as it potential-of-force is of the type:
In particular problem of the movement of a planet between two fixed stars celebrates it, solved by Euler, uses this type of coordinates.
See too
- Keplerian Movement
- Keplerian Movement, movement of Euler.
- parabolic Frame of reference
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