ABOUT EXPANSION OF TERRESTRIAL RADIOPHYSICAL METHODS FOR DETECTION OF ULTRA-HIGH-ENERGY COSMIC RAY

Автор(и)

  • V. B. Kozhukhar Observatory URAN-4 of Institute of radioastronomy of NASU Odessa, Ukraine
  • I. O. Lytvynenko Observatory URAN-4 of Institute of radioastronomy of NASU Odessa, Ukraine
  • O. A. Lytvynenko Observatory URAN-4 of Institute of radioastronomy of NASU Odessa, Ukraine

DOI:

https://doi.org/10.18524/1810-4215.2013.26.83841

Ключові слова:

cosmic rays, extensive air showers, HF signal, Moon reflection, radio telescopes

Анотація

Low arrival density of the ultra-high- energy cosmic rays is one of the main obstacles of their experimental research.

Overcoming this problem was based on the increase in the sensitive area of terrestrial facilities. Currently, the area of such installations reached a practical limit. The further development of researches is connected with remote registration of accompanying electromagnetic radiation. The projects of remote sensor installation on space vehicles are known. In this work the opportunity of use of ground-based radio telescopes and Moon, as return reflector, for global remote detection of electromagnetic bursts caused by space ultra-high-energy cosmic rays in an atmosphere of the Earth is considered.

 

Посилання

Filonenko А.: 2002, Uspehi fizicheskih nauk, 172, 439.

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Опубліковано

2013-11-19

Номер

Том 26 № 2 (2013)

Розділ

Статті

Ліцензія

Авторське право (c) 2016 Odessa Astronomical Publications

Creative Commons License

Ця робота ліцензується відповідно до Creative Commons Attribution-NonCommercial 4.0 International License.

Відповідно Закону України про авторське право і суміжні права N 3792-XII від 23 грудня 1993 року