There is a desire to observe the sun's poles to further deepen our
understanding of solar activity. However, because of the large speeds needed to
perform out-of-ecliptic plane maneuvers, chemical and electric rocket
propulsion mechanisms have been proven to be costly and impractical, leaving
alternative space technology systems like solar sails to be considered for
these applications. In this paper, we study the possibility of using a solar
sail as a probe observing the sun. We design and optimize the trajectories of
the solar sail probe through the surface constraint approach, with the
assumption that the sail moves on a displaced spherical surface. We first
review the surface constraint approach, focusing on its important assumptions
and limitations. Then, we solve and obtain a family of radial and azimuthal
trajectory equations by choosing the correct constraint equation. We
characterize the trajectories based on the functional dependence of the sail's
orientation with the polar angle. Finally, we determine the trajectories of the
probe that will give us the minimum flight time. Results show that increasing
the number of mission stages decreases the total flight time, with minimal
changes in the sail's radial and polar velocities. Furthermore, changing the
functional dependence of the clock angle resets the azimuthal velocity, making
the sail not reverse its direction and directly approach the sun along the
spherical surface.Comment: 25 pages, 8 figure