Radioastronomical measurement of ultrahigh-energy cosmic particle fluxes
A.D. Filonenko 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.
PT Journal Article
TI Radioastronomical measurement of ultrahigh-energy cosmic particle fluxes
AU Filonenko A D
FAU Filonenko AD
DP 10 Aug, 2012
TA Phys. Usp.
SO Phys. Usp. 2012 Aug 10;55(8):741-772
Received: 9th, September 2011, revised: 18th, February 2012, accepted: 28th, February 2012