Abstract
With the aim of the best approximation to the actual conditions of the LORD experiment on detection of ultrahigh-energy cosmic rays and neutrinos, the experiment modeling algorithm is refined by allowing for the parameters of the directivity diagram, polarization mismatch, and galactic noise.
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Additional information
Original Russian Text © G.A. Gusev, I.A. Krol, V.A. Tsarev, 2007, published in Kratkie Soobshcheniya po Fizike, 2007, Vol. 34, No. 10, pp. 3–11.
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Gusev, G.A., Krol, I.A. & Tsarev, V.A. Modeling of the LORD (Lunar Orbital Radio Detector) experiment with regard to the antenna directivity diagram, radiation polarization, and galactic noise. Bull. Lebedev Phys. Inst. 34, 277–281 (2007). https://doi.org/10.3103/S1068335607100016
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DOI: https://doi.org/10.3103/S1068335607100016