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Radioastronomical measurement of ultrahigh-energy cosmic particle fluxes


East-Ukrainian National University, kvartal Molodezhnyi 20-A, Lugansk, 91034, Ukraine

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.

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Fulltext is also available at DOI: 10.3367/UFNe.0182.201208a.0793
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)
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Received: 9th, September 2011, revised: 18th, February 2012, 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

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