排序方式: 共有28条查询结果,搜索用时 31 毫秒
21.
M. I. Panasyuk S. I. Svertilov V. V. Bogomolov G. K. Garipov V. O. Barinova A. V. Bogomolov N. N. Veden’kin I. A. Golovanov A. F. Iyudin V. V. Kalegaev P. A. Klimov A. S. Kovtyukh E. A. Kuznetsova V. S. Morozenko O. V. Morozov I. N. Myagkova V. L. Petrov A. V. Prokhorov G. V. Rozhkov E. A. Sigaeva B. A. Khrenov I. V. Yashin S. I. Klimov D. I. Vavilov V. A. Grushin T. V. Grechko V. V. Khartov V. A. Kudryashov S. V. Bortnikov P. V. Mzhel’skiy A. P. Papkov S. V. Krasnopeev V. V. Krug V. E. Korepanov S. Belyaev A. Demidov Ch. Ferenz L. Bodnar P. Szegedi H. Rotkel M. Moravskiy Il Park Jin-A Jeon Ji-In Kim Jik Lee 《Cosmic Research》2016,54(5):343-350
We present the first experimental results on the observation of optical transients, gamma-ray bursts, relativistic electrons, and electromagnetic waves obtained during the experiment with the RELEC complex of scientific equipment on the Vernov satellite. 相似文献
22.
L. M. Zelenyi A. V. Gurevich S. I. Klimov V. N. Angarov O. V. Batanov A. V. Bogomolov V. V. Bogomolov L. Bodnar D. I. Vavilov G. A. Vladimirova G. K. Garipov V. M. Gotlib M. B. Dobriyan M. S. Dolgonosov N. A. Ivlev A. V. Kalyuzhnyi V. N. Karedin S. O. Karpenko V. M. Kozlov I. V. Kozlov V. E. Korepanov A. A. Lizunov A. A. Ledkov V. N. Nazarov M. I. Panasyuk A. P. Papkov V. G. Rodin P. Segedi S. I. Svertilov A. A. Sukhanov Ch. Ferenz N. A. Eysmont I. V. Yashin 《Cosmic Research》2014,52(2):87-98
23.
Myagkova I. N. Bogomolov A. V. Eremeev V. E. Shiryaev A. O. Ginzburg E. A. 《Cosmic Research》2021,59(6):433-445
Cosmic Research - The results of a comparative analysis from Russian satellite data on the radiation environment in the near-Earth space during September–November 2020 are presented. The... 相似文献
24.
A.V. Bogomolov A.V. Dmitriev I.N. Myagkova S.P. Ryumin O.N. Smirnova I.M. Sobolevsky 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1998,21(12):1801-1804
The spectra of neutrons >10 MeV and gamma-rays 1.5–100 MeV under the Earth Radiation Belts, restored from the data, obtained onboard orbital complex “SALUTE-7”-“KOSMOS-1686”, are presented. The spectra shapes are similar to those for albedo neutrons and gamma-rays, but absolute values of their fluxes (0.2 cm−2 s−1 for neutrons, 0.8 cm−2 s−1 for gamma-rays at the equator and 1.2 cm−2 s−1, 1.9 cm−2 s−1, accordingly, at L=1.9) are several times as large. It is possibly explained by the fact that most of the detected particles were produced by the cosmic ray interactions with the orbital complex matter. Neutron and gamma-ray fluxes obtained from “CORONAS-I” data are near those for albedo particles. 相似文献
25.
In this paper, we consider the thermogasodynamic relations describing the working process in the axial-radial gas turbine stage when the working fluid flows inside the rotor blades taking into account the initiation of the Coriolis forces and heating. The expressions for the air turbine efficiency are derived and illustrated by the calculation results. 相似文献
26.
M.I. Kudryavtsev A.V. Bogomolov V.V. Bogomolov Yu.I. Denisov S.I. Svertilov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1998,21(12):1785-1788
The measurements of high-energy neutron (with energies 30–300 MeV) and proton (with energies 1–200 MeV) fluxes are being conducted on-board “Mir-Spectr” orbital complex. Neutrons are detected by the undirected (FOV 4π sr) scintillator spectrometer, consisting of 4 identical CsI(Tl) detector units (the effective area for neutrons 30 cm2). The gamma-quanta, which can be also detected by this instrument, are separated from neutrons by the analysis of the scintillator output pulse shape. To exclude registration of charged particles an anticoincidence plastic scintillator shield is realized in each detector unit. The proton fluxes are measured by the telescope based on 3 semiconductor detectors with small geometry factor (1 cm2×sr). As the first result of the experiment the upper limit of the integral flux of local and albedo neutrons in the equatorial region (L<1.1) was estimated. The results of this measurements can be useful for the radiation security. Also, the neutrons of solar flares can be detected in this experiment. 相似文献
27.
V. A. Sadovnichiy A. M. Amelyushkin V. Angelopoulos V. V. Bengin V. V. Bogomolov G. K. Garipov E. S. Gorbovskoy B. Grossan P. A. Klimov B. A. Khrenov Jeark Lee V. M. Lipunov Gi Wu Na M. I. Panasyuk I. H. Park V. L. Petrov C. T. Russell S. I. Svertilov E. A. Sigaeva G. F. Smoot Yu. Shprits N. N. Veden’kin I. V. Yashin 《Cosmic Research》2014,52(3):250-250
28.
G Rogovski V Bogomolov M Ivanov J Runavot A Debus A Victorov J C Darbord 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1996,18(1-2):323-332
Mars surface in-situ exploration started in 1975 with the American VIKING mission. Two probes landed on the northern hemisphere and provided, for the first time, detailed information on the martian terrain, atmosphere and meteorology. The current goal is to undertake larger surface investigations and many projects are being planned by the major Space Agencies with this objective. Among these projects, the Mars 94/96 mission will make a major contributor toward generating significant information about the martian surface on a large scale. Since the beginning of the Solar System exploration, planets where life could exist have been subject to planetary protection requirements. Those requirements accord with the COSPAR Policy and have two main goals: the protection of the planetary environment from influence or contamination by terrestrial microorganisms, the protection of life science, and particularly of life detection experiments searching extra-terrestrial life, and not life carried by probes and spacecrafts. As the conditions for life and survival for terrestrial microorganisms in the Mars environment became known, COSPAR recommendations were updated. This paper will describe the decontamination requirements which will be applied for the MARS 94/96 mission, the techniques and the procedures which are and will be used to realize and control the decontamination of probes and spacecrafts. 相似文献