Applied Physics and Mathematics Annotation << Back GEONEUTRINO AND THE EFFECT OF ANOMALOUS NEUTRINO RADIOISOTOPE (HENRI) ABSORPTION O.B. KHAVROSHKIN, V.V. TSYPLAKOV Analogues of the existing methods and devices used to register astrophysical mostly solar neutrinos are now beginning to be used to search for geoneutrinos. These structures, as a rule, have significant, often cyclopean dimensions, insignificant sensitivity and difficulties in determining the direction to the neutrino source of arrival, foreign and domestic scientists made a significant contribution to the creation of these systems: Ray Davis, G.T. Zatsepin, A.E. Chudakov, G.A. Askorian, and B.A. Dolgoshein and American T. Bowen, Japanese authors of the “Super Kamiokanda” installation. New types of neutrino telescope are described, which are based on the physical effect of anomalous neutrino radioisotope (HENRI) absorption [1,2]. One type has a high sensitivity, small size, low cost, but also how all existing ones determine the direction of neutrino arrival through interaction tracks [1]. The other type of telescope, while maintaining these advantages, points to a neutrino source similarly to an optical one - by not directing the axis of the structure to the neutrino interaction tracks, but to their source [1], a similar circuit as the original one was used in the geoneutrino search device [3]. The results of a successful test of an operating model of a neutrino telescope operating in the geoneutrino registration mode are given. Keywords: Neutrino and geoneutrino, telescope geoneutrino mode, internal structure and heat flows of the Earth. DOI: 10.25791/pfim.02.2019.597 Contacts: E-mail: khavole@ifz.ru Pp. 17-25.