Calculation of the Areas Most Likely to Appear Suitable for Communication Meteor Trails

Abstract

The method of calculation of the areas most likely to appear meteor trails with the electromagnetic waves specular reflection point for the radio links of different lengths is proposed. The linear electron density of the meteor trail, depending on the velocity and mass of the meteoroid, as well as zenith angles, defined by radiants of sporadic meteors and meteor showers are taken into account during calculating.