The exponential form z(θ)=ρeiθz(\theta)=\rho\,e^{i\theta} is already a parametrisation: as θ[0,2π)\theta\in[0,2\pi) varies, z(θ)z(\theta) describes the circle of radius ρ\rho. It is a kinematic point of view: the curve is the image of the motion of a point as a parameter varies. Let us look at three examples.

Circle. Centre (x0,y0)(x_0,y_0), radius rr: {x(t)=x0+rcosty(t)=y0+rsint,t[0,2π).\begin{cases} x(t) = x_0 + r\cos t \\ y(t) = y_0 + r\sin t\end{cases}, \quad t\in[0,2\pi). Check: (xx0)2+(yy0)2=r2(cos2t+sin2t)=r2(x-x_0)^2 + (y-y_0)^2 = r^2(\cos^2 t + \sin^2 t) = r^2. The parametrisation traverses the circle anticlockwise exactly once.

Ellipse. Canonical form x2/a2+y2/b2=1x^2/a^2 + y^2/b^2 = 1: {x(t)=acosty(t)=bsint,t[0,2π).\begin{cases} x(t) = a\cos t \\ y(t) = b\sin t\end{cases}, \quad t\in[0,2\pi). Note: tt is not the geometric angle of the point with respect to the centre (unless a=ba=b). It is an auxiliary angular parameter: in the astronomical formalism of orbits it is called the eccentric anomaly, following the Keplerian terminology taken up by Stillwell.

Lissajous curve. Two perpendicular oscillations of different frequencies: {x(t)=Asin(ω1t)y(t)=Bsin(ω2t+δ).\begin{cases} x(t) = A\sin(\omega_1 t) \\ y(t) = B\sin(\omega_2 t + \delta)\end{cases}. If ω1/ω2\omega_1/\omega_2 is rational, the curve is closed; if irrational, it densely fills the rectangle [A,A]×[B,B][-A,A]\times[-B,B]. The case ω2/ω1=1:1\omega_2/\omega_1 = 1{:}1 with δ=π/2\delta=\pi/2 gives a circle (A=BA=B) or an ellipse with parallel axes; the ratio 1:21{:}2 gives the classic figure of eight.

Topics: Complex numbers
Concepts: Eccentric anomaly · Circle · Lissajous curve · Ellipse · Exponential form · Parametrisation
Skills: Model
People: Johannes Kepler (Keplero) · Lissajous