Abstract
The purpose TUS space experiment is to study cosmic rays of ultrahigh energies produced by extensive air showers from space. The concentrator is located on satellite, made in the form of the Fresnel mirror towards the earth’s atmosphere, the focus of which is a photodetector. The angle of view of the mirror is ±4.5° that for a given height of the orbit corresponds to the area 80 × 80 km2 on ground. The ground complex consisting of a number of stations, to check the optical system of the experiment is created, (their location and the amount will be determined after the launch of the satellite based on its actual orbit).
Similar content being viewed by others
References
B. Khrenov, “Complementary research ability of ground- and space-based detectors of ultra high energy cosmic rays,” J. Phys. G 29, 881–890 (2003).
N. N. Kalmykov, B. A. Khrenov, and O. P. Shustova, Phys. At. Nucl. 67, 2058 (2004).
B. Khrenov et al., “The TUS space fluorescence detector for study of UHECR and other phenomena of variable fluorescence light in the atmosphere,” Adv. Space Res. 37, 1867 (2006).
P. Colin, A. Chukanov, V. Grebenyuk, D. Naumov, P. Nédélec, Y. Nefedov, A. Onofre, S. Porokhovoi, B. Sabirov, and L. Tkatchev, “Measurement of air and nitrogen fluorescence light yields induced by electron beam for UHECR experiments,” Astropart. Phys. 27, 317–325 (2007).
G. Garipov, A. Gongadze, A. Grinyuk, B. Khrenov, P. Klimov, D. Naumov, A. Puchkov, B. Sabirov, O. Saprykin, L. Tkatchev, and I. Yashin, “R&D of the Fresnel optical system for the TUS space detector,” in Proceedings of the 30th International Cosmic Ray Conference ICRC, Merida, Yucatan, Mexico, July 3–11, 2007, vol. 5, p. 881, ID 0162.
L. Tkachev, G. Garipov, A. Grinyuk, V. Grebenyuk, P. Klimov, B. Khrenov, S. Porokhovoy, A. Puchkov, O. Saprykin, S. Sharakin, A. Skrypnik, M. Slunechka, A. Tkachenko, and I. Yashin, “The TUS Fresnel mirror production and optical parameters measurement,” in Proceedings of the 32nd International Cosmic Ray Conference ICRC, Beijing, China, 2011, vol. 11, ID 272.
A. Tkachenko, A. Ggrinyuk, L. Tkachev, G. Garipov, B. Khrenov, P. Klimov, V. Morozenko, M. Panasyuk, S. Sharakin, A. Shirokov, and I. Yashin, “TUS Fresnel mirror production and optical parameters measurement,” in Proceedings of the 33d International Cosmic Ray Conference ICRC, Rio De Janeiro, Brazil, 2013, ID 0406.
G. Garipov, V. Grebenyuk, A. Grinyuk, B. Khrenov, P. Klimov, S. Porokhovoy, A. Puchkov, B. Sabirov, O. Saprykin, S. Sharakin, A. Skrypnik, M. Slunechka, L. Tkatchev, A. Tkachenko, and I. Yashin, “TUS Fresnel mirror production and optical parameters measurement,” Phys. Part. Nucl. Lett. 10, 49 (2013).
P. A. Klimov, G. K. Garipov, A. A. Grinyuk, B. A. Khrenov, M. I. Panasyuk, V. S. Morozenko, S. A. Sharskin, A. V. Shirokov, L. G. Tkachev, A. V. Tkachenko, and I. V. Yashin, “Ultra high energy cosmic rays detector TUS on-board Lomonosov satellite,” in Proceedings of the 33d International Cosmic Ray Conference ICRC, Rio De Janeiro, Brazil, 2013, ID 0423.
www.ledengin.com/fles/products/LZ4/LZ4-00U600.pdf.
Author information
Authors and Affiliations
Corresponding author
Additional information
The article is published in the original.
Rights and permissions
About this article
Cite this article
Grebenyuk, V., Boreiko, V., Dmitrotsa, A. et al. Ground-based complex for checking the optical system. Phys. Part. Nuclei Lett. 13, 579–582 (2016). https://doi.org/10.1134/S1547477116050265
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1547477116050265