Zobrazeno 1 - 10
of 35
pro vyhledávání: '"K. A. Bychkov"'
Publikováno v:
Advances in Geochemistry, Analytical Chemistry, and Planetary Sciences ISBN: 9783031098826
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d7dfc14362817d782273a964b116e4a0
https://doi.org/10.1007/978-3-031-09883-3_3
https://doi.org/10.1007/978-3-031-09883-3_3
Autor:
Valerii Kotok, K. L. Bychkov, Kostiantyn Sukhyy, B. A. Ananchenko, François Henn, Volodymyr Verbitskiy, Alexey Sykchin, Vadym Kovalenko, S. Deabate, A. Mehdi, Jean-Louis Bantignies, Andrey A. Burkov, A. V. Chernyad'ev
Publikováno v:
Journal of The Electrochemical Society
Journal of The Electrochemical Society, Electrochemical Society, 2020, 167 (10), pp.100530. ⟨10.1149/1945-7111/ab9a2a⟩
Journal of The Electrochemical Society, Electrochemical Society, 2020, 167 (10), pp.100530. ⟨10.1149/1945-7111/ab9a2a⟩
International audience
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8ea19bb3fdbb811a9a73c0370ec6e0c8
https://hal.archives-ouvertes.fr/hal-02924352
https://hal.archives-ouvertes.fr/hal-02924352
Autor:
O. M. Belova, K. V. Bychkov
Publikováno v:
Astrophysics. 61:224-240
With the hydrogen atom as an example, the effect of photospheric thermal radiation on the upper layers of stellar atmospheres is studied. It is shown that when the radiation temperature exceeds 5000 K, the rates of stimulated processes in free-bound,
Autor:
K. V. Bychkov, O. M. Belova
Publikováno v:
Astrophysics. 61:101-112
The effect of the number K of atomic hydrogen levels taken into account on the cooling of the gas behind a shock front is studied. The calculations are done for the conditions in the atmospheres of long-period Mira Ceti type variables. K ranges from
Publikováno v:
Journal of Petrology. 59:283-298
Autor:
O. M. Belova, K. V. Bychkov
Publikováno v:
Astrophysics. 60:358-364
We study the emission from a gas heated in a shock front in the atmosphere of a giant star and examine the deviation of the populations of the discrete levels of hydrogen from their quasiequilibrium values according to the Saha formula as functions o
Autor:
K. V. Bychkov, O. M. Belova
Publikováno v:
Astrophysics. 60:200-212
It is shown that for the luminescence of hydrogen in shock fronts in the atmospheres of stars in late spectral classes, the level populations of the hydrogen atoms are determined by the entire prehistory of the process, beginning with heating in the
Publikováno v:
Geochemistry International. 55:465-473
This paper presents principles of the method of modeling metal concentrations in sulfide at the occurrence of silicate–sulfide liquid immiscibility during middle and late stages of the crystallization of mafic–ultramafic magmas. The proposed appr
Autor:
O. M. Belova, K. V. Bychkov
Publikováno v:
Astrophysics. 60:111-117
In stellar atmospheres and regions of the interstellar medium with electron densities above 104 cm-3, three-body recombination into high levels of the hydrogen atom with principal quantum numbers k >> 1 can play a more important role than radiative r
Autor:
M. Yu. Puzankov, A. B. Perepelov, O. V. Dirksen, M. Yu. Shur, L. I. Bazanova, N. A. Nekrylov, P. Yu. Plechov, K. A. Bychkov
Publikováno v:
Moscow University Geology Bulletin. 70:233-239
Compositions of melts for the youngest and located hypsometrically below others eruption centers of Sedankinskiy field of areal volcanics were studied by the olivinehosted melt inclusions method. The trace� element content in the melts is reported