Zobrazeno 1 - 10
of 143
pro vyhledávání: '"Dmitry Bisikalo"'
Publikováno v:
Atmosphere, Vol 14, Iss 7, p 1092 (2023)
Auroral events are the prominent manifestation of solar/stellar forcing on planetary atmospheres because they are closely related to the stellar energy deposition by and evolution of planetary atmospheres. A numerical kinetic Monte Carlo model was de
Externí odkaz:
https://doaj.org/article/60e42c8c88b54912b6d12a7ef73ad5dd
Publikováno v:
Galaxies, Vol 10, Iss 6, p 110 (2022)
A three-dimensional numerical model has been developed to study the flow structure in close binary systems with a magnetic field. The model uses a system of equations of modified magnetic hydrodynamics, which allows describing all the main dynamic ef
Externí odkaz:
https://doaj.org/article/fb1af8583e984292ba86e8b2832b24ae
Publikováno v:
Galaxies, Vol 9, Iss 4, p 110 (2021)
In this paper, the characteristics of hot spots on an accretor surface are investigated for two types of polars: the eclipsing synchronous polar V808 Aur and the non-eclipsing asynchronous polar CD Ind in configuration of an offset and non-offset mag
Externí odkaz:
https://doaj.org/article/0648c46b4c394655a6ae4e9d34ea6500
Publikováno v:
Atmosphere; Volume 14; Issue 7; Pages: 1092
Auroral events are the prominent manifestation of solar/stellar forcing on planetary atmospheres because they are closely related to the stellar energy deposition by and evolution of planetary atmospheres. A numerical kinetic Monte Carlo model was de
Publikováno v:
Proceedings of the International Astronomical Union. 16:228-233
In this paper, the effect of hot spots movement by accretor surface on the appearance of bolometric light curves for two types of polars - synchronous V808 Aur and asynchronous CD Ind is studied. The analysis was carried out under the assumption of a
Publikováno v:
Astronomy Reports. 64:259-271
The orientation parameter effect of a hot Jupiter’s intrinsic dipole magnetic field on the flow structure in an extended gaseous (ionospheric) envelope of the planet is studied with a three-dimensional numerical simulation. For example, the hot Jup
Publikováno v:
Astronomy Reports. 64:159-167
—Currently, hot Jupiters have extended gaseous (ionospheric) envelopes extending far beyond the Roche lobe. The envelopes are loosely bound to the planet and are subject to a strong influence by stellar wind fluctuations. Since hot Jupiters are clo
Autor:
Dmitry Bisikalo, Andrey Zhilkin
Publikováno v:
Anais da Academia Brasileira de Ciências, Vol 93, Iss suppl 1 (2021)
Anais da Academia Brasileira de Ciências, Volume: 93 Supplement 1, Article number: e20200801, Published: 17 MAY 2021
Anais da Academia Brasileira de Ciências v.93 suppl.1 2021
Anais da Academia Brasileira de Ciências
Academia Brasileira de Ciências (ABC)
instacron:ABC
Anais da Academia Brasileira de Ciências, Volume: 93 Supplement 1, Article number: e20200801, Published: 17 MAY 2021
Anais da Academia Brasileira de Ciências v.93 suppl.1 2021
Anais da Academia Brasileira de Ciências
Academia Brasileira de Ciências (ABC)
instacron:ABC
In the paper a scenario of an electromagnetic response formation from the merging of two black holes is considered. In this scenario it’s assumed that the binary black hole is surrounded by an accretion disk. As a result of the black holes merging
Autor:
Dmitry Bisikalo, Andrey Zhilkin
Publikováno v:
Proceedings of the International Astronomical Union. 15:268-279
Hot Jupiters have extended gaseous (ionospheric) envelopes, which extend far beyond the Roche lobe. The envelopes are loosely bound to the planet and, therefore, are strongly influenced by fluctuations of the stellar wind. We show that, since hot Jup
Autor:
Dmitry Bisikalo, V. I. Shematovich, Christian Möstl, Luca Fossati, A. A. Cherenkov, I. F. Shaikhislamov
Publikováno v:
Astronomy Reports. 63:94-106
Results of a study of the influence of solar-type host stars superflares on the gas dynamics of the extended envelopes of giant exoplanets are presented. During flare events, the radiation intensity of the host star in the extreme ultraviolet and sof