Zobrazeno 1 - 10
of 11
pro vyhledávání: '"D V, Milanov"'
Autor:
I. I. Shevchenko, A. V. Mel’nikov, V. B. Titov, R. V. Baluev, A. V. Veselova, A. V. Krivov, D. V. Mikryukov, D. V. Milanov, A. A. Mülläri, I. I. Nikiforov, N. P. Pit’ev, E. N. Polyakhova, L. L. Sokolov, V. Sh. Shaidulin
Publikováno v:
Solar System Research. 57:175-189
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e356c55829ce21ec21d6a349a2c9a874
https://doi.org/10.1134/s0038094623020077
https://doi.org/10.1134/s0038094623020077
Autor:
I. I. Shevchenko, A. V. Mel’nikov, V. B. Titov, R. V. Baluev, A. V. Veselova, A. V. Krivov, D. V. Mikryukov, D. V. Milanov, A. A. Mülläri, I. I. Nikiforov, N. P. Pit’ev, E. N. Polyakhova, L. L. Sokolov, V. Sh. Shaidulin
Publikováno v:
Solar System Research. 57:85-102
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::104c5d5c4791e75c98e57436f85b12c6
https://doi.org/10.1134/s0038094623010069
https://doi.org/10.1134/s0038094623010069
Publikováno v:
Vestnik of Saint Petersburg University. Mathematics. Mechanics. Astronomy. 8:359-369
The distance functions on the set of Keplerian orbits play an important role in solving the problems of searching for the parent bodies of meteoroid streams. A special kind of function is the distances in the quotient spaces of orbits. Three metrics
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4d0997e9bb22f7ec0fc8a172dd09d56d
https://doi.org/10.21638/spbu01.2021.215
https://doi.org/10.21638/spbu01.2021.215
Autor:
D. V. Milanov
Publikováno v:
Vestnik St. Petersburg University, Mathematics. 52:317-326
Geometric properties of spaces of Keplerian orbits are of interest for celestial mechanics problems related to the search for groups of celestial bodies with close orbits. Those groups include asteroid families and meteor streams. Studying these grou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0be81da2b94bdae3062de79de91db265
https://doi.org/10.1134/s1063454119030130
https://doi.org/10.1134/s1063454119030130
Publikováno v:
Vestnik St. Petersburg University, Mathematics. 50:406-413
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1e9f9977793c830f807b300051ba7950
https://doi.org/10.3103/s1063454117040112
https://doi.org/10.3103/s1063454117040112
Publikováno v:
Vestnik St. Petersburg University, Mathematics. 50:318-324
The theory of equilibrium figures was actively developed in the 19th century, when it was found that the observed massive celestial bodies (the Sun, planets, and satellites) had an almost ellipsoidal form. The existence of exactly ellipsoidal figures
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2ce593d09c72c7bfbf35c6e5b770421d
https://doi.org/10.3103/s1063454117030098
https://doi.org/10.3103/s1063454117030098
Publikováno v:
Vestnik of Saint Petersburg University. Mathematics. Mechanics. Astronomy. 4:695-703
The theory of figures of equilibrium was extensively studied in the nineteenth century, when the reasons for which observed massive celestial bodies (such as the Sun, planets, and satellites) are almost ellipsoidal were discovered. The existence of e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f247c18198f40cbeacb8c8ad390e6c3e
https://doi.org/10.21638/11701/spbu01.2017.417
https://doi.org/10.21638/11701/spbu01.2017.417
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 131
In this article, we prove the relaxed triangle inequality for Southworth and Hawkins, Drummond and Jopek orbital similarity criteria on the set of non-rectilinear Keplerian orbits with the eccentricity bounded above. We give estimates of the minimal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::abf301da4f09dc2a24713165594c9937
https://doi.org/10.1007/s10569-019-9884-6
https://doi.org/10.1007/s10569-019-9884-6
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 130
The outer gravitational potential V of the level ellipsoid of revolution T is uniquely determined by two quantities: the eccentricity $$\varepsilon $$ of the ellipsoid and Clairaut parameter q, proportional to the angular velocity of rotation squared
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dc150697a34463ea2e17436f2841f6f2
https://doi.org/10.1007/s10569-018-9851-7
https://doi.org/10.1007/s10569-018-9851-7
Autor:
D. V. Milanov
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 130
Quotient spaces of Keplerian orbits are important instruments for the modelling of orbit samples of celestial bodies on a large time span. We suppose that variations of the orbital eccentricities, inclinations and semi-major axes remain sufficiently
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dd3c1a9353c2e795c30dceedcf3c7608
https://doi.org/10.1007/s10569-018-9820-1
https://doi.org/10.1007/s10569-018-9820-1