The dynamics of astrozole clouds and its interaction with solar wind plasma

Summary form only given, as follows. The problem of dynamics of astrozole clouds which consist of fine-grained diamagnetic radioactive particles was theoretically studied. This problem is the basic part of the new method of irrevocable radioactive waste disposal in the cosmic space. Mechanisms of interactions of astrozole clouds with the solar wind plasma was analysed. The authors considered the ensemble of spherical diamagnetic microparticles under the influence of nongravitational forces such as solar photon radiation pressure, solar corpuscular wind pressure, magnetic forces and electromagnetic forces due to the solar wind plasma. The evaluation of accelerations which astrozole clouds may acquire under the influence of these forces was carried out by means of computer simulation. A very wide range of values was obtained. The highest value of the acceleration can be achieved using charged clouds. In this case the influence of solar wind plasma rises.