Ice satellites of planets of the Solar System and the on-orbit radio detection of ultrahigh-energy particles

G.A. Gusev, B.N. Lomonosov, V.A. Ryabov, V.A. Chechin
Lebedev Physical Institute, Russian Academy of Sciences, Leninsky prosp. 53, Moscow, 119991, Russian Federation

The problem of detecting nature’s most energetic particles — cosmic rays and neutrinos — is reviewed. Prospects for using orbital radio detectors for these highest-energy particles are examined. Apertures are calculated for space experiments using the Moon and similar-sized ice satellites of planets of the Solar System as targets for the interaction of cosmic-ray particles and neutrinos. A comparative analysis shows that using the Moon as a target is the most promising scenario.

PACS: 95.55.Vj, 95.85.Ry, 96.50.S− (all)
DOI: 10.3367/UFNe.0180.201009c.0957
URL: https://ufn.ru/en/articles/2010/9/c/
Web of Science

000286041500003
Scopus

2-s2.0-78751469087
ADS NASA

2010PhyU...53..915G
Citation: Gusev G A, Lomonosov B N, Ryabov V A, Chechin V A "Ice satellites of planets of the Solar System and the on-orbit radio detection of ultrahigh-energy particles" Phys. Usp. 53 915–921 (2010)

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Оригинал: Гусев Г А, Ломоносов Б Н, Рябов В А, Чечин В А «Ледяные спутники планет Солнечной системы и орбитальные радиодетекторы для регистрации частиц ультравысоких энергий» УФН 180 957–964 (2010); DOI: 10.3367/UFNr.0180.201009c.0957

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