Analysis of Joint Channel Coexistence Time at Space-Diversity Radio Reception of Meteor Reflections

This paper examines the possibility of joint reception of radio reflections from the same meteor trails simultaneously at two spaced receivers. A refined simulation of a joint reception area (JRA) of meteor radio reflections on the basis of a diffraction theory of oblique scattering of radio waves off ionized meteor trails is performed for radio links of moderate (500 km) and medium (1000 km) lengths. The obtained results may be particularly useful for territory planning of meteor burst communication (MBC) networks with the spatial division of subscribers (SDMA technology). The simulated JRAs also characterize an interception probability of messages. This knowledge is especially important in designing highly secure MBC, such as meteor key distribution systems, intended for the creation of two identical copies of a shared secret key at both sides of the meteor radio link.

[1]  S. Y. Mui,et al.  Meteor trail footprint statistics , 1990, IEEE Conference on Military Communications.

[2]  Paul S. Cannon,et al.  Spaced antenna diversity in temperate latitude meteor burst systems operating near 40 MHz: Variation of signal cross-correlation coefficients with antenna separation , 1993 .

[3]  O. G. Villard,et al.  Some properties of oblique radio reflections from meteor ionization trails , 1956 .

[4]  J. Oetting An Analysis of Meteor Burst Communications for Military Applications , 1980, IEEE Trans. Commun..

[5]  R. I. Desourdis,et al.  Meteor scatter signal footprint variation with range, power margin and time of day , 1989, IEEE Military Communications Conference, 'Bridging the Gap. Interoperability, Survivability, Security'.

[6]  G. R. Sugar Radio propagation by reflection from meteor trails , 1964 .

[7]  R. Desourdis,et al.  Spatial diversity in meteor scatter radio links , 1995 .

[8]  R. Closs,et al.  I. Theory of radio reflections from meteor trails: I , 1952 .

[9]  A. Nejatince Spatial properties of meteor-burst propagation , 1980 .

[10]  Jay Weitzen,et al.  A study of the ground illumination footprint of meteor scatter communication , 1990, IEEE Trans. Commun..

[11]  V. Eshleman,et al.  Directional Characteristics of Meteor Propagation Derived from Radar Measurements , 1957, Proceedings of the IRE.

[12]  A. Ladd Diversity Reception for Meteoric Communications , 1961 .

[13]  D. Yavuz Meteor burst communications , 1990, IEEE Communications Magazine.

[14]  L. A. Epictetov,et al.  Time&frequency coordination using unsteady, variable-precision measurements on meteor burst synchronization and communication equipment , 2003, IEEE International Frequency Control Symposium and PDA Exhibition Jointly with the 17th European Frequency and Time Forum, 2003. Proceedings of the 2003.

[15]  A. I. Sulimov,et al.  Secure key distribution based on meteor burst communications , 2014, 2014 11th International Conference on Security and Cryptography (SECRYPT).