An approach to the problem of a meteoric complex called the Interaction Meteor Complex (IMG) is applied and discussed, where author^s former idea of the interaction layer (Rajchl 1969) is generalized. The role of an extended interaction of meteoroids is ephasized, both with planet surfaces and/or their satellites and with planet atmospheres, elastic or inelastic in form. The dissipation and related formative aspect are joined in one complex and compared with a topological compact. Examples of all the above mentioned types of interaction are presented. In more detail the
inelastic interaction with the Earth atmosphere of whole "spectrum" from faint meteors detected by TV technique to Fireball Network bolides, is considered. First results in the form of a ψ structure and cross-complementarity are reported. The possibility of the existence of another "enlarged" ψ structure is anticipated from topological
aspects and supported for the outer planets of the Solar Planetary System by results of Levin and Simonenko (1982).