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Autor:
Jörg P. Rachen, Pim Schellart, Jörg R. Hörandel, Sander ter Veen, Olaf Scholten, Laura Rossetto, Katey Mulrey, Heino Falcke, J. Emilio Enriquez, Antonio Bonardi, Satyendra Thoudam, Gia Trinh, Anna Nelles, Stijn Buitink, Pragati Mitra, Tobias Winchen, Arthur Corstanje, Maaijke Mevius
Publikováno v:
EPJ Web of Conferences, 135, pp. 1-4
EPJ Web of Conferences, 135, 1-4
7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2016), 135
EPJ Web of Conferences, Vol 135, p 04004 (2017)
EPJ Web of Conferences, 135, 1-4
7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2016), 135
EPJ Web of Conferences, Vol 135, p 04004 (2017)
One of the main ways to use radio to detect Ultra High Energy Neutrinos and Cosmic Rays is the Lunar Askaryan technique, that uses the Moon as a target and searches for nanosecond pulses with large radio telescopes. To use low frequency aperture arra