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/ 000286041500003 2-s2.0-78751469087 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) BibTexBibNote ® (generic)BibNote ® (RIS)MedlineRefWorks @article{Gusev:2010, author = {G. A. Gusev and B. N. Lomonosov and V. A. Ryabov and V. A. Chechin}, title = {Ice satellites of planets of the Solar System and the on-orbit radio detection of ultrahigh-energy particles}, publisher = {Physics-Uspekhi}, year = {2010}, journal = {Phys. Usp.}, volume = {53}, number = {9}, pages = {915-921}, url = {https://ufn.ru/en/articles/2010/9/c/}, doi = {10.3367/UFNe.0180.201009c.0957} } 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