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

• Autorzy: Kharchenko H. V.
• Języki publikacji: EN

Abstrakty

EN

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.

Słowa kluczowe

EN

meteor trail; specular reflection; linear electron density; radiant; zenith angle

• Wydawca: Polish Academy of Sciences, Committee of Electronics and Telecommunication
• Czasopismo: International Journal of Electronics and Telecommunications
• Rocznik: 2012
• Tom: Vol. 58, No. 2
• Strony: 105--110
• Opis fizyczny: Bibliogr. 5 poz., wykr.

Twórcy

autor

Kharchenko H. V.

• Institute of Radio Physics and Electronics NAS of Ukraine, Ukraine, 61085, Kharkov, Ac. Proskury str., 12,

Bibliografia

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• [2] O. I. Belkovich, The theory of meteor radio location. Kazan: KSU, 1977.
• [3] A. A. Weiss, “Elevation, height, and electron density of echoing points of meteor trails,” Australian Journal of Physics, vol. 12, pp. 65-76, 1959.
• [4] H. V. Kharchenko, “Estimated formation probability of meteoric trails with mirror reflection,” in Proceedings of 6-th IEEE East-West Design and Test Symposium, St.Peterburg, Russia, Sep. 2010, pp. 289-291.
• [5] I. E. Antipov, J. A. Koval, and V. V. Obelchenko, Development and improvement of the theory of meteor radio communication systems and synchronization. Kharkov: Collegium, 2006.
• [6] H. V. Kharchenko, “Method of estimation interval delay in scattering of the signals reflected from the meteor trails,” Radio Engineering, vol. 160, pp. 56-61, 2010.
• [7] P. S. Aleksandrov, Lectures on analytical geometry. Moscow: Science, 1968.