The basic principles underlying the radio telescope measurement of ultrahigh-energy particle fluxes are reviewed. Experimental lunar regolith emission data are presented for the 10²⁰ eV energy range. Some conclusions from theoretical work are discussed, as is the influence of a number of factors on the intensity of the radio pulse due to the cascade disk under the Moon’s surface.

PACS: 95.55.Vj, 95.85.Bh, 96.50.S− (all) DOI: 10.3367/UFNe.0182.201208a.0793 URL: https://ufn.ru/en/articles/2012/8/a/ 000310831300001 2-s2.0-84869008767 Citation: Filonenko A D "Radioastronomical measurement of ultrahigh-energy cosmic particle fluxes" Phys. Usp. 55 741–772 (2012) BibTex BibNote ® (generic)BibNote ® (RIS)MedlineRefWorks %0 Journal Article %T Radioastronomical measurement of ultrahigh-energy cosmic particle fluxes %A A. D. Filonenko %I Physics-Uspekhi %D 2012 %J Phys. Usp. %V 55 %N 8 %P 741-772 %U https://ufn.ru/en/articles/2012/8/a/ %U https://doi.org/10.3367/UFNe.0182.201208a.0793 Received: 9th, September 2011, revised: 18th, February 2012, accepted: 28th, February 2012 Оригинал: Филоненко А Д «Радиоастрономический метод измерения потоков космических частиц сверхвысокой энергии» УФН 182 793–827 (2012); DOI: 10.3367/UFNr.0182.201208a.0793