main features of our solution can be summarised as follows:

-   it is an exact (i.e., non-perturbative), closed-form and explicit solution;

-   it is expressed as a set of unique formulæ independent of the values of the initial conditions and of the parameters of the system;

-   it is a solution to the full three-dimensional Stark problem (whereas many previous solutions deal only with the restricted case in which the motion is confined to a plane).

The simple form of our solution allows us to examine thoroughly the dynamical features of the Stark problem, and to derive several new results (e.g., regarding questions of (quasi) periodicity and boundness of motion). Our method of solution is in some sense close to the one employed in @lantoine_complete_2011. However, we believe that our solution offers several distinct advantages:

-   by adopting the Weierstrassian formalism (instead of the Jacobian one), we sidestep the issue of categorising the solutions based on the nature of the roots of the polynomials generating the differential equations, and thus our formulæ do not depend on the initial conditions or on the parameters of the system;

-   we provide explicit formulæ for the three-dimensional case;

-   we avoid introducing a 