Zobrazeno 1 - 10
of 574
pro vyhledávání: '"Galkin, A I"'
Autor:
Ivanov, V. A., Galkin, V. I., Bonvech, E. A., Roganova, T. M., Chernov, D. V., Podgrudkov, D. A., Ziva, M. D., Latypova, V. S., Azra, C. G., Entina, E. L.
The study of cosmic rays in the energy range from 1 to 1000 PeV is crucial for understanding their origins and propagation paths. As part of this research, a new SPHERE-3 installation is being developed, featuring enhanced light sensitivity and optic
Externí odkaz:
http://arxiv.org/abs/2410.14921
Autor:
Galkin, V. I., Azra, C. G., Bonvech, E. A., Chernov, D. V., Entina, E. L., Ivanov, V. I., Latypova, V. S., Podgrudkov, D. A., Roganova, T. M., Ziva, and M. A.
A new Cherenkov telescope of the SPHERE type is under development. Its main goal is to promote the solution of the problem of the primary cosmic ray mass composition at ultra high energies (1--100 PeV) using a newly developed technique of the primary
Externí odkaz:
http://arxiv.org/abs/2410.13022
Autor:
Entina, E. L., Podgrudkov, D. A., Azra, C. G., Bonvech, E. A., Cherkesova, O. V., Chernov, D. V., Galkin, V. I., Ivanov, V. A., Kolodkin, T. A., Ovcharenko, N. O., Roganova, T. M., Ziva, M. D.
A new SPHERE-3 telescope is being developed for cosmic rays spectrum and mass composition studies in the 5--1000 PeV energy range. Registration of extensive air showers using reflected Cherenkov light method applied in the SPHERE detector series requ
Externí odkaz:
http://arxiv.org/abs/2410.01781
Autor:
Agafonova, N. Y., Alexandrov, A., Anokhina, A. M., Asada, T., Ashikhmin, V. V, Boccia, V., Centanni, D., Chernyavskii, M. M., D'Ambrosio, N., De Lellis, G., Di Crescenzo, A., Dowdy, Y. C., Dmitrievski, S., Enikeev, R. I., Galati, G., Galkin, V. I., Golovatiuk, A., Gorbunov, S. A., Gornushkin, Y., Guler, A. M., Gulyaeva, V. V., Iuliano, A., Khalikov, E. V., Kim, S. H., Konovalova, N. S., Krasilnikova, Y. O., Lauria, A., Lee, K. Y., Loschiavo, V. P., Managadze, A. K., Miloi, A., Montesi, M. C., Naka, T., Okateva, N. M., Park, B. D, Podgrudkov, D. A., Polukhina, N. G., Roganova, T. M., Rosa, G., Samoilov, M. A., Sadykov, Z. T., Saeki, K., Sato, O., Shakiryanova, I. R., Shchedrina, T. V., Shiraishi, T., Sohn, J. Y., Sotnikov, A., Starkov, N. I., Starkova, E. N., Strekalina, D. M., Tioukov, V., Ursov, E. D., Ustyuzhanin, A., Vasina, S., Voronkov, R. A., Yoon, C. S.
We present a study of a directional search for Dark Matter boosted forward when scattered by cosmic-ray nuclei, using a module of the NEWSdm experiment. The boosted Dark Matter flux at the edge of the Earth's atmosphere is expected to be pointing to
Externí odkaz:
http://arxiv.org/abs/2305.00112
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 516, 4, 5379-5388 (2022)
Properties of the extragalactic magnetic field (EGMF) outside of clusters and filaments of the large-scale structure are essentially unknown. The EGMF could be probed with $\gamma$-ray observations of distant (redshift $z > 0.1$) blazars. TeV $\gamma
Externí odkaz:
http://arxiv.org/abs/2204.11110
Autor:
Bonvech, E. A., Chernov, D. V., Finger, M., Finger Jr., M., Galkin, V. I., Podgrudkov, D. A., Roganova, T. M., Vaiman, I. A.
The SPHERE project studies primary cosmic rays by detection of the Cherenkov light of extensive air showers reflected from the snowy surface of the earth. Measurements with the aerial-based detector SPHERE-2 were performed in 2011-2013. The detector
Externí odkaz:
http://arxiv.org/abs/2109.14537
Autor:
Aysin, Rinat R.1 (AUTHOR) aysin@ineos.ac.ru, Galkin, Konstantin I.2,3 (AUTHOR) glkn@ioc.ac.ru
Publikováno v:
Molecules. Apr2024, Vol. 29 Issue 8, p1704. 8p.
Autor:
Antonov, R. A., Bonvech, E. A., Chernov, D. V., Dzhatdoev, T. A., Galkin, V. I., Podgrudkov, D. A., Roganova, T. M.
A compact device lifted over the ground surface might be used to observe optical radiation of extensive air showers (EAS). Here we consider spatial and temporal characteristics of Vavilov-Cherenkov radiation ("Cherenkov light") reflected from the sno
Externí odkaz:
http://arxiv.org/abs/1901.00452
Autor:
Galkin, Konstantin I.
Publikováno v:
In Mendeleev Communications January-February 2023 33(1):1-8
Autor:
Kurt, Victoria G., Yushkov, Boris Yu., Galkin, Vladimir I., Kudela, Karel, Kashapova, Larisa K.
Publikováno v:
2017,New astronomy, 56, 102-112
Appreciable hard X-ray (HXR) and gamma-ray emissions in the 0.04 to 150 MeV energy range associated with the 2003 October 29 solar flare (X10/3B) were observed at 20:38 to 20:58 UT by the SONG instrument onboard the CORONAS-F mission. To restore flar
Externí odkaz:
http://arxiv.org/abs/1808.02627