Solar proton events at the growth phase of the 22nd solar activity cycle.

Meteor satellite observations in March, August, September and October 1989 recorded intensive solar proton events which caused a disturbed radiation situation in the near-Earth space. The paper presents the results of analyzing flux and spectral characteristics of the events and their relation to heliogeophysical situation.     

Solid component of interplanetary matter from vehicle observations

This paper contains the data of meteoric particle investigations by means of piezoelectric detectors.The data obtained on the different Soviet vehicles at distances from about 100 km to about 100000000 km from the earth are given.Measurements have demonstrated that apart from fluxes there are individual aggregations of meteoric particles with very unequal spatial density of particles in them. Linear dimensions varied within wide limits.A concept of the mass spectrum of meteoric particles is presented.Very high concentrations of minute dust particles were observed near the earth at altitudes from 100–200 km by means of ground-based methods and rocket measurements.The increased density of interplanetary matter in the vicinity of the moon during April and May 1966 was recorded by means of satellite Luna-10. By means of Luna-12 it could not be discovered whether this aggregation is the moon halo or is the result of the moon passage through some dust particle aggregation, because the investigation on satellite Luna-12 was carried out mostly during meteor showers.     

The Dynamics of Arranging a Spacecraft Tether Group as a Triangular Constellation

Cosmic Research - The method of arranging a tether group of four spacecraft as triangular beam constellation is considered in this paper. The group consists of a central spacecraft, from which the...     

Aerodynamic Characteristics of Thin Cylindrical and Conical Shells in the Incompressible Flow

The paper presents aerodynamic characteristics of thin cylindrical and conical shells in the incompressible flow. Experimental data and results of numerical simulation in the OpenFoam software are compared. It is shown that the aerodynamic characteristics of the thin shells differ from the aerodynamic characteristics of the corresponding solid bodies and depend on the shell geometry parameters.