“…Analysis of time-series of images provide parameters of the motion of the observed structure (its translation, velocity and acceleration) only in a plane of the sky (e.g. Rothschild, Pecker and Roberts, 1955;McCabe and Fisher, 1970;Rompolt, 1975;Kim, 1990;Aurass et al, 1991;Vrsnak et al, 1993;Uddin, Gaur and Pande, 1994;Tandberg-Hanssen, 1995;Rudawy and Madjarska, 1998) while 3D trajectories of the plasma (namely separated knots of material) could be evaluated only under certain strong and arbitrary assumptions. To do this Billing and Pecker assumed that the acceleration of the prominence knots is always normal relative to their velocity vector (Billings and Pecker, 1954), Paluš assumed spiral motions of the knots on conical surfaces (Paluš, 1972), Makhmudov and coauthors assumed constant acceleration of the falling knots (Makhmudov, Nikolsky and Zhugzda , 1980), and Ballester and Kleczek introduced their own method based on an extended geometrical analysis of the data (Ballester and Kleczek, 1983).…”