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1.
Zagidullin  A. A.  Usanin  V. S.  Petrova  N. K.  Nefedyev  Yu. A.  Andreev  A. O.  Gudkova  T. V. 《Astronomy Reports》2020,64(12):1093-1106
Astronomy Reports - The work is devoted to the study of the physical libration of the Moon. Interest in the traditional topic related to the rotation of the Moon is stirred up by the activity of...  相似文献   
2.
Astronomy Reports - The initial form of present-day space optical observations contain considerable geometrical and brightness distortions. This problem can be solved based on geometrical...  相似文献   
3.
Sergienko  M. V.  Sokolova  M. G.  Nefedyev  Yu. A.  Andreev  A. O. 《Astronomy Reports》2020,64(12):1087-1092
Astronomy Reports - This study is focused on the relationships between the κ-Cygnid meteor shower and different groups of asteroids crossing the Earth’s orbit (the so-called near-Earth...  相似文献   
4.
Kronrod  E. V.  Kronrod  V. A.  Kuskov  O. L.  Nefedyev  Yu. A. 《Doklady Earth Sciences》2018,483(1):1475-1479
Doklady Earth Sciences - The bulk composition of the silicate Moon (crust + mantle, BSM) is determined on the basis of inversion of gravitational and seismic data. It is shown that the mantle...  相似文献   
5.
Churkin  K. O.  Nefedyev  Yu. A.  Andreev  A. O.  Demina  N. Yu.  Kronrod  E. V. 《Astronomy Reports》2021,65(7):580-587
Astronomy Reports - One of the priority tasks of modern astronomy is the observation and study of transient celestial processes, which also concerns photoelectric observations of lunar occultations...  相似文献   
6.
Astronomy Reports - This study is focused on the analysis of data of the long-term latitude observations and the Global Navigation Satellite System (GNSS). The latitude observations include...  相似文献   
7.
Usanin  V. S.  Nefedyev  Yu. A.  Sokolova  M. G. 《Astronomy Reports》2019,63(8):666-686

Results of BV R observations of meteors in the Perseid, Taurid, Orionid, Geminid, and Lyrid showers, as well as sporadic meteors, carried out with the Mini-MegaTORTORA system are presented. Two-color diagrams for the brightness maxima are constructed. It is shown that meteors in the Perseid, Taurid, and Geminid showers form clusters in the two-color diagrams. Variations in color with a temporal resolution of 0.1 s are considered for some meteors.

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8.
Petrova  N. K.  Nefedyev  Yu. A.  Zagidullin  A. A.  Andreev  A. O. 《Astronomy Reports》2018,62(12):1021-1025

A brief review of modern observational achievements and the theoretical basis of physical libration of the Moon is presented. Special attention is given to the inferred existence of a lunar core and determination of its parameters. The creation of a theory of physical libration of the Moon, which requires analyses of semi-empirical series of long-term laser observations and the use of the highly accurate DE421 dynamical ephemeris, is related to this. A large role in this area has been played by the analytical theory of physical libration of the Moon constructed by Yu.V. Barkin, which made it possible for the first time to derive parameters of the free nutation of the lunar core from observations. This paper is based on a talk given at the conference “Modern Astrometry 2017,” dedicated to the memory of K.V. Kuimov (Sternberg Astronomical Institute, Moscow State University, October 23–25, 2017).

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9.
Agalakov  B. V.  Ledenev  V. G.  Lubyshev  B. I.  Nefedyev  V. P.  Yazev  S. A.  Zubkova  G. N.  Kerdraon  A.  Urbarz  H. W. 《Solar physics》1997,173(2):305-318
Based on observations from the Siberian solar radio telescope, and invoking data from other observatories, we investigate preflare changes in the sunspot and floccular sources of radio emission and the development of an importance 2N flare in the chromosphere and corona in the active region on August 23, 1988.It has been ascertained that preflare changes became observable six hours prior to the flare onset and manifested themselves in intense flux fluctuations above the sunspot and in an enhancement of the source emission flux above the flocculus.It is shown that the flare onset is associated with a newly emerged magnetic flux in the form of a pore near the filament and with the appearance of radio sources above the filament. The flare was accompanied by type III radio bursts and a noise storm at meter wavelengths. Coronal mass ejection parameters are estimated from type III burst observations.  相似文献   
10.
Nefedyev  Yu. A.  Andreev  A. O.  Petrova  N. K.  Demina  N. Yu.  Zagidullin  A. A. 《Astronomy Reports》2018,62(12):1016-1020

A number of questions about the Moon remain to be answered, including fundamental questions related to the internal structure and origin of the Moon. Studies of the spin–orbital dynamics of the Moon and of selenodesy are required for the practical solution of a number of problems related to navigation on the Moon and in circumlunar space, with the aim of providing coordinate and time support for planned lunar space projects. This paper analyzes existing dynamic selenographic reference grids, considers methods for their development and creation, and describes the modern projects related to navigational support for lunar missions. This paper is based on a presentation made at the conference “Modern Astrometry 2017,” dedicated to the memory of K.V. Kuimov (Sternberg Astronomical Institute, Moscow State University, October 23–25, 2017).

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