There is a nice description of the geodesics on the upper sheet of the hyperboloid $H^2 \subset \mathbb{R}^3$ in terms of hyperbolic sine and cosine as $$ \lambda(t)= (\cosh(t))x + (\sinh(t))y $$ where $x,y$ are Lorentz othonormal vectors in $\mathbb{R}^3$.
The geodesics in the upper half-plane $U \subset \mathbb{C}$ are Euclidean lines and circles that intersect the real line orthogonally. For example ,the imaginary line $\lambda(t)=it$, for $t \in \mathbb{R}$ is a geodesic in $U$.
I am curious how to describe geodesics in $U$ in terms of hyperbolic functions.
Is there a way of parameterizing $\lambda(t) = it$ in terms of hyperbolic functions?
( I am asking about this because I am reading a paper that is describing geodesics in the upper half-plane in terms of hyperbolic tangent and hyperbolic secant, as $$ \lambda(t) = c_1 \left( \tanh \omega(t+ t_0) + i \operatorname{sech} \omega(t + t_0) \right) $$)
The best parametrization of geodesics of the upper-half plane (in the hyperbolic metric) follows from that $PSL_2(\Bbb{R})$ acts transitively and isometrically on those, so any geodesic is of the form $\{ \gamma (i e^t), t\in (-\infty,\infty)\}$ for some $\gamma \in PSL_2(\Bbb{R})$, which reduces to a quotient of $\sinh,\cosh,\exp$.
(or $PSL_2(\Bbb{R})$ quotiented by the diagonal matrices, leaving the imaginary axis fixed)
where $i e^t,t\in (-\infty,\infty)$ is the parametrization of the imaginary axis such that $hyperbolicDistance(ie^t,ie^u)=|t-u|$.
https://en.wikipedia.org/wiki/Poincar%C3%A9_half-plane_model#Geodesics