Zobrazeno 1 - 10
of 272
pro vyhledávání: '"Shibalova, A. A."'
Autor:
Porokhov, N. V., Anikanov, A. A., Sirotina, A. P., Pershina, E. A., Shibalova, A. A., Shibalov, M. V., Diudbin, G. D., Mumlyakov, A. M., Trofimov, I. V., Vovk, N. A., Tarkhov, M. A.
The present study delves into exploring the impact of a thin protective layer of scandium nitride (ScN) on the superconductive properties of thin films of niobium nitride (NbN) generated through reactive magnetron deposition. This is the first time s
Externí odkaz:
http://arxiv.org/abs/2404.17827
The phenomenon of the Gnevyshev gap was first identified in the solar-corona irradiance data (green line). Later, it was studied in the sunspot, coronal, and heliospheric data. We have investigated the Gnevyshev gap in the magnetic field data and hav
Externí odkaz:
http://arxiv.org/abs/2403.18568
The solar cycle is a complex phenomenon, a comprehensive understanding of which requires the study of various tracers. Here, we consider the solar cycle as manifested in the harmonics of the solar large-scale surface magnetic field, including zonal,
Externí odkaz:
http://arxiv.org/abs/2403.06293
Traditionally, the solar activity cycle is thought as an interplay of the main dipole component of the solar poloidal magnetic field and the toroidal magnetic field. However, the real picture as presented in the extended solar-cycle models is much mo
Externí odkaz:
http://arxiv.org/abs/2305.19427
Autor:
Bulyarskiy, Sergey V., Litvinova, Kristina I., Rudakov, Grigory A., Shibalova, Anastasia A., Gusarov, Georgy G.
Publikováno v:
In Surfaces and Interfaces December 2024 55
According to the scheme of action of the solar dynamo, the poloidal magnetic field can be considered a source of production of the toroidal magnetic field by the solar differential rotation. From the polar magnetic field proxies, it is natural to exp
Externí odkaz:
http://arxiv.org/abs/2108.10527
We compare spectra of the zonal harmonics of the large-scale magnetic field of the Sun using observation results and solar dynamo models. The main solar activity cycle as recorded in these tracers is a much more complicated phenomenon than the eigen
Externí odkaz:
http://arxiv.org/abs/2104.06808
The evolution of the solar activity comprises, apart from the well-known 11-year cycle, various temporal scales ranging from months up to the secondary cycles known as mid-term oscillations. Its nature deserves a physical explanation. In this work, w
Externí odkaz:
http://arxiv.org/abs/2007.14779
We considered variations the dipole and the quadrupole components of the solar large-scale magnetic field. Both the axial and the equatorial dipoles exhibit a systematic decrease in the past four cycles in accordance with the general decrease of sola
Externí odkaz:
http://arxiv.org/abs/2001.05433
Autor:
Evlashin, S.A., Volkova, A.A., Mendagaliev, R.V., Babkin, K.D., Bondareva, J.V., Simonov, A.P., Kuzminova, Yu.O., Dubinin, O.N., Chernodubov, D.A., Shibalova, A.A., Kobykhno, I.A., Klimova-Korsmik, O.G.
Publikováno v:
In Materials Today Communications December 2023 37