Zobrazeno 1 - 10
of 3 135
pro vyhledávání: '"Kuznetsov O"'
Autor:
Kuznetsov O; Department of Theoretical and Applied Sciences, eCampus University, Via Isimbardi 10, 22060 Novedrate, Italy., Frontoni E; Department of Political Sciences, Communication and International Relations, University of Macerata, Via Crescimbeni, 30/32, 62100 Macerata, Italy., Chernov K; Department of Information and Communication Systems Security, School of Computer Sciences, V. N. Karazin Kharkiv National University, 4 Svobody Sq., 61022 Kharkiv, Ukraine., Kuznetsova K; VRAI-Vision, Robotics and Artificial Intelligence Lab, Via Brecce Bianche 12, 60131 Ancona, Italy., Shevchuk R; Department of Computer Science and Automatics, University of Bielsko-Biala, 43-309 Bielsko-Biala, Poland.; Department of Computer Science, West Ukrainian National University, 46009 Ternopil, Ukraine., Karpinski M; Institute of Security and Computer Science, University of the National Education Commission, 30-084 Krakow, Poland.; Department of Cyber Security, Ternopil Ivan Puluj National Technical University, 46001 Ternopil, Ukraine.
Publikováno v:
Sensors (Basel, Switzerland) [Sensors (Basel)] 2024 Dec 06; Vol. 24 (23). Date of Electronic Publication: 2024 Dec 06.
Autor:
Vasilevich, R. S.1 (AUTHOR) vasilevich.r.s@ib.komisc.ru, Kuznetsov, O. L.2 (AUTHOR), Lodygin, E. D.1 (AUTHOR), Zazovskaya, E. P.3 (AUTHOR), Panyukov, A. N.1 (AUTHOR)
Publikováno v:
Eurasian Soil Science. Jul2022, Vol. 55 Issue 7, p940-956. 17p.
Autor:
Kuznetsov, O. P.1 (AUTHOR) olpkuz@yandex.ru
Publikováno v:
Automation & Remote Control. Jun2022, Vol. 83 Issue 6, p919-934. 16p.
Publikováno v:
Astronomy Reports, vol. 47, Issue 10, p.809-820 (2003)
We analyze heating and cooling processes in accretion disks in binaries. For realistic parameters of the accretion disks in close binaries (with accretion rates from 1e-12 to 1e-7 Msun/year and \alpha from 0.1 to 0.01), the gas temperature in the out
Externí odkaz:
http://arxiv.org/abs/1210.3233
Akademický článek
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Publikováno v:
Astron.Rep. 50 (2006) 537-543
We consider a mechanism for the formation of superhumps in the TV Col system, based on the possible existence of a precessional spiral wave in the accretion disk of the system. This mechanism can act in binaries with arbitrary component-mass ratios,
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606151
Autor:
Mitsumoto, M., Jahanara, B., Matsuda, T., Oka, K., Bisikalo, D. V., Kilpio, E. Yu., Boffin, H. M. J., Boyarchuk, A. A., Kuznetsov, O. A.
Publikováno v:
Astron.Rep.49:884-891,2005
The results of 3D modelling of the flow structure in the classical symbiotic system Z~Andromedae are presented. Outbursts in systems of this type occur when the accretion rate exceeds the upper limit of the steady burning range. Therefore, in order t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0510175
Publikováno v:
Astron.Rep.49:701-708,2005; Astron.Zh.Akad.Nauk SSSR.82:788-796,2005
A thickening at the outer edge of the accretion disk is usually invoked to explain the dips in the light curves of cataclysmic variables with stationary disks at phases ~0.7. The non-collisional interaction between the stream and the disk in the stat
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508353
Autor:
Arapov, Yu. G., Neverov, V. N., Harus, G. I., Shelushinina, N. G., Yakunin, M. V., Kuznetsov, O. A., de Visser, A., Ponomarenko, L.
For a two-dimensional (2D) hole system (confined within Ge layers of a multilayered p-Ge/Ge_{1-x}Si_x heterostructure) described by Luttinger Hamiltonian with the g-factor highly anisotropic for orientations of magnetic field perpendicular and parall
Externí odkaz:
http://arxiv.org/abs/cond-mat/0404355
Publikováno v:
Astron.Rep. 48 (2004) 588-596; Astron.Zh. 81 (2004) 648-657
A new mechanism explaining superoutbursts in binaries of SU UMa type is proposed. In the framework of this mechanism the accretion rate increase leading to the superoutburst is associated with formation of a spiral wave of a new "precessional" type i
Externí odkaz:
http://arxiv.org/abs/astro-ph/0403057