Zobrazeno 1 - 10
of 14
pro vyhledávání: '"O. G. Barinov"'
Autor:
E. S. Belenkaya, V. V. Kalegaev, S. W. H. Cowley, G. Provan, M. S. Blokhina, O. G. Barinov, A. A. Kirillov, M. S. Grigoryan
Publikováno v:
Annales Geophysicae, Vol 34, Pp 641-656 (2016)
The paraboloid model of Saturn's magnetosphere describes the magnetic field as being due to the sum of contributions from the internal field of the planet, the ring current, and the tail current, all contained by surface currents inside a magnetop
Externí odkaz:
https://doaj.org/article/1f8833624b21419e8aaadd19c19a6450
Autor:
E. S. Belenkaya, S. W. H. Cowley, C. J. Meredith, J. D. Nichols, V. V. Kalegaev, I. I. Alexeev, O. G. Barinov, W. O. Barinova, M. S. Blokhina
Publikováno v:
Annales Geophysicae, Vol 32, Pp 689-704 (2014)
A unique set of images of Saturn's northern polar UV aurora was obtained by the Hubble Space Telescope in 2011 and 2012 at times when the Cassini spacecraft was located in the solar wind just upstream of Saturn's bow shock. This rare situation pro
Externí odkaz:
https://doaj.org/article/4c4fccf1541844fab9aac1bb107fbd6f
Publikováno v:
Annales Geophysicae, Vol 31, Pp 1447-1458 (2013)
We consider the magnetic interconnection of Saturn's northern and southern polar regions controlled by the interplanetary magnetic field (IMF), studying in particular the more complex and interesting case of southward IMF, when the Kronian magneto
Externí odkaz:
https://doaj.org/article/b6c649ca8836419c861d1cfa24bfb057
Autor:
Irina Myagkova, O. G. Barinov, Yu. S. Shugai, Vladimir Shirokii, R. D. Vladimirov, Sergey Dolenko
Publikováno v:
Russian Meteorology and Hydrology. 46:163-171
The ways are studied to improve the quality of prediction of the time series of hourly mean fluxes and daily total fluxes (fluences) of relativistic electrons in the outer radiation belt of the Earth 1 to 24 hours ahead and 1 to 4 days ahead, respect
Publikováno v:
Russian Meteorology and Hydrology. 46:157-162
The potential is investigated of predicting the time series of the Dst geomagnetic index using various adaptive methods: artificial neural networks (classical multilayer perceptrons), decision trees (random forest), gradient boosting. The prediction
Publikováno v:
Geomagnetism and Aeronomy. 61:138-147
The possible use of artificial neural networks—classical multilayer perceptrons—with coupling functions to forecast time series of the Dst geomagnetic index is studied. The basic forecast is based on parameters of the solar wind and interplanetar
Publikováno v:
Advances in Neural Computation, Machine Learning, and Cognitive Research IV ISBN: 9783030605766
This paper performs comparative analysis of the prediction quality for the time series of hourly average flux of relativistic electrons (E > 2 meV) in the near-Earth space 1 to 24 h ahead by various machine learning methods. As inputs, all the predic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bd1af88344d3a9675ac88227067edca6
https://doi.org/10.1007/978-3-030-60577-3_25
https://doi.org/10.1007/978-3-030-60577-3_25
Autor:
W. O. Barinova, Minh-Duc Nguyen, D. A. Parunakyan, V. E. Eremeev, Vladimir Kalegaev, O. G. Barinov, Irina Myagkova
Publikováno v:
Cosmic Research. 56:32-37
An empirical model of the high-latitude boundary of the outer Earth’s radiation belt (ERB) has been presented, which is based on the measurement data of electron fluxes on the polar low-orbit CORONAS-Photon, Meteor-M1, and Meteor-M2 satellites. The
Autor:
Vladimir Shiroky, Mikhail Panasyuk, O. G. Barinov, Irina Myagkova, Vera Barinova, Minh-Duc Nguyen, Nikolay V. Kusnetsov, Natalia Vlasova, Vladimir Kalegaev, Yuliya S. Shugai, V. E. Eremeev, Sergey Bobrovnikov, A. V. Bogomolov, Sergey Dolenko
Publikováno v:
Proceedings of the International Astronomical Union. 13:232-235
Radiation environment of near-Earth space is one of the most important factors of space weather. Space Monitoring Data Center of Moscow State University provides operational monitor and forecast of radiation conditions both at Geostationary Orbits (G
Autor:
Gabrielle Provan, Alexander Kirillov, Elena Belenkaya, Vladimir Kalegaev, M. S. Blokhina, M. S. Grigoryan, Stanley W. H. Cowley, O. G. Barinov
Publikováno v:
Annales Geophysicae, Vol 34, Pp 641-656 (2016)
The paraboloid model of Saturn's magnetosphere describes the magnetic field as being due to the sum of contributions from the internal field of the planet, the ring current, and the tail current, all contained by surface currents inside a magnetopaus