Abstract
The results of the simulation of cascade radio emission from ultrahigh-energy cosmic rays in the LORD lunar experiment using circularly polarized antennas are presented. It is shown that based on the characteristics of radio emission caused by cascades from protons and iron nuclei in lunar regolith and escaped into vacuum it is impossible to distinguish these cascades in the primary energy region above 1020 eV.
Similar content being viewed by others
References
V. A. Tsarev, J. Rad. Phys. Chem. 75, 805 (2006).
G. A. Gusev, B. N. Lomonosov, K. M. Pichkhadze, et al., Kosm. Issled. 44, 1 (2006) [Cosmic Research 44, 19 (2006)].
G. A. Gusev, B. N. Lomonosov, K.M. Pichkhadze, et al., Dokl. Akad. Nauk 406, 327 (2006) [Dokl. Phys. 51, 22 (2006)].
K. D. de Vries, J. Scholten, and K. Verner, Astropart. Phys. 45, 23 (2013).
G. A. Gusev, B. N. Lomonosov, K.M. Pichkhadze, et al., Mathematicheskoe Modelirovanie 20(6), 67 (2008).
G. A. Gusev, I. A. Krol, and V. A. Tsarev, Kratkie Soobshcheniya po Fizike FIAN 34(10), 12 (2007) [Bulletin of the Lebedev Physics Institute 34, 277 (2007)].
F. G. Stremler, Introduction to Communication Systems, 3rd ed. (Addison-Wesley, New York, 1991).
V. V. Zheleznyakov, Radio Emission of the Sun and Planets (Nauka, Moscow, 1964) [in Russian].
Author information
Authors and Affiliations
Corresponding author
Additional information
Original Russian Text © G.A. Gusev, Kyaw Maung, 2014, published in Kratkie Soobshcheniya po Fizike, 2014, Vol. 41, No. 4, pp. 37–43.
About this article
Cite this article
Gusev, G.A., Maung, K. Is it possible to determine the chemical composition of cosmic rays in the “LORD” lunar experiment?. Bull. Lebedev Phys. Inst. 41, 110–114 (2014). https://doi.org/10.3103/S1068335614040058
Received:
Published:
Issue Date:
DOI: https://doi.org/10.3103/S1068335614040058