Authors:
BISIKALO DV
BOYARCHUK AA
KUZNETSOV OA
CHECHETKIN VM
Citation: Dv. Bisikalo et al., THE INFLUENCE OF PARAMETERS ON THE FLOW STRUCTURE IN SEMIDETACHED BINARY-SYSTEMS - 3-D NUMERICAL MODELING, Astronomy reports, 42(5), 1998, pp. 621-629
Authors:
BISIKALO DV
BOYARCHUK AA
KUZNETSOV OA
KHRUZINA TS
CHEREPASHCHUK AM
CHECHETKIN VM
Citation: Dv. Bisikalo et al., EVIDENCE FOR THE ABSENCE OF A STREAM-DISK SHOCK INTERACTION SEMI-DETACHED BINARY-SYSTEMS - COMPARISON OF MATHEMATICAL-MODELING RESULTS AND OBSERVATIONS, Astronomy reports, 42(1), 1998, pp. 33-45
Authors:
BISIKALO DV
BOYARCHUK AA
CHECHETKIN VM
KUZNETSOV OA
MOLTENI D
Citation: Dv. Bisikalo et al., 3-DIMENSIONAL NUMERICAL-SIMULATION OF GASEOUS FLOW STRUCTURE IN SEMIDETACHED BINARIES, Monthly Notices of the Royal Astronomical Society, 300(1), 1998, pp. 39-48
Authors:
GERARD JC
BISIKALO DV
SHEMATOVICH VI
DUFF JW
Citation: Jc. Gerard et al., AN UPDATED MODEL OF THE HOT NITROGEN ATOM KINETICS AND THERMOSPHERIC NITRIC-OXIDE, J GEO R-S P, 102(A1), 1997, pp. 285-294
Authors:
BISIKALO DV
SHEMATOVICH VI
GERARD JC
GLADSTONE GR
WAITE JH
Citation: Dv. Bisikalo et al., THE DISTRIBUTION OF HOT HYDROGEN-ATOMS PRODUCED BY ELECTRON AND PROTON PRECIPITATION IN THE JOVIAN AURORA, J GEO R-PLA, 101(E9), 1996, pp. 21157-21168
Authors:
HUBERT B
GERARD JC
SHEMATOVICH VI
BISIKALO DV
Citation: B. Hubert et al., HIGH ROTATIONAL-EXCITATION OF NO INFRARED THERMOSPHERIC AIRGLOW - A SIGNATURE OF SUPERTHERMAL NITROGEN-ATOMS, Geophysical research letters, 23(17), 1996, pp. 2215-2218
Citation: Dv. Bisikalo et al., A KINETIC-MODEL OF THE FORMATION OF THE HOT OXYGEN GEOCORONA .2. INFLUENCE OF O+ ION PRECIPITATION, J GEO R-S P, 100(A3), 1995, pp. 3715-3720
Authors:
GERARD JC
RICHARDS PG
SHEMATOVICH VI
BISIKALO DV
Citation: Jc. Gerard et al., THE IMPORTANCE OF NEW CHEMICAL SOURCES FOR THE HOT OXYGEN GEOCORONA, Geophysical research letters, 22(3), 1995, pp. 279-282
Authors:
BISIKALO DV
BOYARCHUK AA
KUZNETSOV OA
POPOV YP
CHECHETKIN VM
Citation: Dv. Bisikalo et al., STRUCTURE OF THE ACCRETION DISK IN BINARI ES WITH COMPONENTS THAT ARENOT FILLING THEIR ROCHE LOBE, ASTRONOM ZH, 72(2), 1995, pp. 190-202
Citation: Vi. Shematovich et al., A KINETIC-MODEL OF THE FORMATION OF THE HOT OXYGEN GEOCORONA .1. QUIET GEOMAGNETIC CONDITIONS, J GEO R-S P, 99(A12), 1994, pp. 23217-23228
Authors:
BISIKALO DV
BOYARCHUK AA
KUZNETSOV OA
POPOV YP
CHECHETKIN VM
Citation: Dv. Bisikalo et al., INFLUENCE OF BOUNDARY PARAMETERS OF THE S TELLAR WIND ON THE STRUCTURE OF THE FLOW OF MATTER IN BINARIES WITH COMPONENTS THAT ARE NOT FILLING THEIR ROCHE LOBE, ASTRONOM ZH, 71(4), 1994, pp. 560-571