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1.
V. M. Lipunov E. S. Gorbovskoy V. G. Kornilov V. V. Chazov M. I. Panasyuk S. I. Svertilov I. V. Yashin V. L. Petrov V. V. Kallegaev A. A. Amelushkin D. M. Vlasenko 《Astronomy Reports》2018,62(7):426-435
The results of observations with the MASTER-SHOK robotic wide-field optical cameras onboard the Lomonosov Space Observatory carried out in 2016 are presented. In all, the automated transient detection system transmitted 22 181 images of moving objects with signal-to-noise ratios greater than 5 to the Earth. Approximately 84% of these images are identified with well-known artificial Earth satellites (including repeated images of the same satellite) and fragments of such satellites (space debris), according to databases of known satellites. The remaining 16% of the images are relate to uncatalogued objects. This first experience in optical space-based monitoring of near-Earth space demonstrates the high efficiency and great potential of using large-aperture cameras in space, based on the software and technology of the MASTER robotic optical complexes (the Mobile Astronomical System of TElescope- Robots (MASTER) global network of robotic telescopes of Lomonosov Moscow State University). 相似文献
2.
地球辐射带中有"杀手"电子之称的相对论电子通量增强和损失过程一直是空间物理学和空间天气学研究的热点.本文通过对20002016年间,地球同步轨道相对论电子通量降低至背景通量水平并持续时间长达3天以上这一特殊现象进行了相关统计研究.从事件的时间分布角度,本文研究了约1.5个太阳活动周内共62例事件随太阳活动水平高低的分布情况,结果表明:在太阳活动周下降期有较少的事件发生,而在峰年、谷年这类事件的发生率与太阳活动水平的高低并没有直接联系.随后,我们对这62例事件在开始、持续、结束三个阶段分别做了一些相关参数的统计,探讨相对论电子通量长期倒空事件的客观规律和产生机制.研究结果表明:事件发生前,太阳风动压、密度的显著增加引起磁层顶向内收缩,等离子体层顶一直维持在高L区域,IMF Bz分量南向和磁暴过程使相对论电子通量通过绝热和非绝热等物理损失机制降至背景通量水平.当这些相对论电子达到背景通量水平后,较弱的太阳风条件和地磁活动水平不足以提供充分的可以使相对论电子通量增长的源;虽然有些相对论电子通量长期倒空事件期间存在中、小磁暴过程,但这些强度较弱的磁暴很可能不会显著地影响同步轨道相对论电子损失和增长的动态平衡,因此相对论电子仍然可以维持在背景通量水平.如果有长时间的亚暴活动和高强度的ULF (Ultra-Low Frequency)波活动发生,太阳风速度显著增加,那么这些物理过程能提供足够的种子电子和持续的加速条件,使得相对论电子通量打破倒空状态,进而呈现显著增长趋势. 相似文献
3.
P. A. Klimov G. K. Garipov B. A. Khrenov V. S. Morozenko V. O. Barinova V. V. Bogomolov M. A. Kaznacheeva M. I. Panasyuk K. Yu. Saleev S. I. Svertilov 《Izvestiya Atmospheric and Oceanic Physics》2017,53(9):924-933
In this paper, data obtained by the Vernov satellite are discussed in comparison with the data obtained by Universitetsky–Tatiana-1, 2 satellites. The advanced instrumentation onboard the Vernov satellite improved the capabilities of the data-transmission system, providing an opportunity to acquire more detailed information on transient atmospheric events (TAEs), including a wider range of TAE photon numbers (event brightness) down to lower photon numbers, the opportunity to observe the events in ultraviolet range without the considerable inclusion of red–infrared photons (which indicates the substantial contribution of electric discharges, lightning precursors, at the altitudes of thunderstorm clouds), and the observation of TAE series at a rate of about 10–100 occurrences per second with a period from tens of seconds to several minutes. 相似文献
4.
I. N. Myagkova M. I. Panasyuk Yu. I. Denisov V. V. Kalegayev A. V. Bogomolov V. O. Barinova D. A. Parunakyan L. I. Starostin 《Geomagnetism and Aeronomy》2011,51(7):897-901
The study of variations in the electron flux in the outer Earth radiation belt (ERB) and their correlations with solar processes
is one of the important problems in the experiment with the Electron-M-Peska instrument onboard the CORONAS-Photon solar observatory.
Data on relativistic and subrelativistic electron fluxes obtained by the Electron-M-Peska in 2009 have been used to study
the outer ERB dynamics at the solar minimum. Increases in outer ERB relativistic electron fluxes, observed at an height of
550 km after weak magnetic disturbances induced by high-velocity solar wind arriving to the Earth, have been analyzed. The
geomagnetic disturbances induced by the high-velocity solar wind and that resulted in electron flux variations were insignificant:
there were no considerable storms and substorms during that period; however, several polar ground-based stations observed
an increase in wave activity. An assumption has been made that the wave activity caused the variations in relativistic electron
fluxes. 相似文献
5.
The article discusses the progress made in studying space radiation in the heliosphere using SINP MSU instruments on board a spacecraft built by the Lavochkin Association, in predicting flight radiation conditions, and in studying the radiation resistance of spacecraft components. 相似文献
6.
A model of transformational superplasticity in the upper mantle 总被引：1，自引：0，他引：1
7.
M. I. Panasyuk S. N. Kuznetsov Yu. V. Kutuzov B. Yu. Yushkov I. N. Myagkova V. M. Petrov V. V. Bengin 《Solar System Research》2007,41(5):425-432
We present the results of our calculations of the absorbed radiation doses onboard the International Space Station (ISS) based on CORONAS-F data on the spectra of protons in near-Earth space and on the conditions of their penetration into the polar caps. Our estimates are compared with the dosimetry data onboard the ISS and with the results of similar calculations based on GOES-10 (Geostationary Operational Environmental Satellite) data. There is satisfactory agreement between the absorbed doses estimated from CORONAS-F data and the measurements on the ISS. When the data from the high-apogee GOES-10 satellite are used, the agreement between calculations and measurements is considerably poorer. This is probably due to the influence of solar cosmic ray proton penetration into the polar caps. 相似文献
8.
L. L. Lazutin Yu. V. Gotselyuk E. A. Murav’eva I. N. Myagkova M. I. Panasyuk L. I. Starostin B. Yu. Yushkov K. Kudela N. Hasebe K. Sukurai M. Hareyama 《Geomagnetism and Aeronomy》2010,50(2):168-180
The processes of penetration, trapping, and acceleration of solar protons in the Earth’s magneto-sphere during magnetic storms in November 2004 and January 2005 are studied based on the energetic particle measurements on the CORONAS-F and SERVIS-1 satellites. Acceleration of protons by 1–2 orders of magnitude was observed after trapping of solar protons with an energy of 1–15 MeV during the recovery phase of the magnetic storm of November 7–8, 2004. This acceleration was accompanied by an earthward shift of the particle flux maximum for several days, during which the series of magnetic storms continued. The process of relativistic electron acceleration proceeded simultaneously and according to a similar scenario including acceleration of protons. At the end of this period, the intensification was terminated by the process of precipitation, and a new proton belt split with the formation of two maximums at L ～ 2 and 3. In the January 2005 series of moderate storms, solar protons were trapped at L = 3.7 during the storm of January 17–18. However, during the magnetic storm of January 21, these particles fell in the zone of quasi-trapping, or precipitated into the atmosphere, or died in the magnetosheath. At the same time, the belts that were formed in November at L ～ 2 and 3 remained unchanged. Transformations of the proton (and electron) belts during strong magnetic storms change the intensity and structure of belts for a long time. Thus, the consequences of changes during the July 2004 storm did not disappear until November disturbances. 相似文献
9.
A. S. Kovtyukh I. N. Myagkova A. V. Bogomolov V. V. Bogomolov M. I. Panasyuk S. I. Svertilov 《Geomagnetism and Aeronomy》2016,56(6):661-672
The structure and dynamics of electron fluxes of subrelativistic energies in the range 235–300 keV at L < 4 during December 3–8, 2014, are analyzed according to the RELEC instrument onboard the Vernov satellite. Sharp changes in the parameters of the solar wind and the IMF were detected on December 6, but they did not lead to a magnetic storm. However, after the event of December 6, subrelativistic electron fluxes in the inner belt and the slot region were enhanced and structured. The dynamics of electron fluxes in the local transient bursts at L ~ 1.5–1.7 is considered in detail. It is shown that these bursts are associated with the development of the cyclotron instability in the tops of magnetic flux tubes near the inner belt maximum. The electron anisotropic index is estimated in these bursts. It is shown that in the beginning these bursts are anisotropic and that they become isotropic as the decay proceeds. The most likely chain of physical mechanisms that could lead to variations in electron fluxes of the inner belt described in this paper is presented. For the first time, the topological effects in stationary distributions of the electrons of the inner belt observed at low altitudes in the South Atlantic Anomaly region are explained. 相似文献
10.
V. I. Zatsepin A. D. Panov N. V. Sokolskaya J. H. Adams Jr. H. S. Ahn G. L. Bashindzhagyan J. Chang M. Christl A. R. Fazely T. G. Guzik J. B. Isbert K. C. Kim E. N. Kouznetsov M. Panasyuk E. S. Seo J. Watts J. P. Wefel J. Wu 《Astronomy Letters》2009,35(5):338-342
Titanium is a rare, secondary nucleus among Galactic cosmic rays. Using the Silicon matrix in the ATIC experiment, Titanium
has been separated. The energy dependence of the Ti to Fe flux ratio in the energy region from 5 GeV per nucleon to about
500 GeV per nucleon is presented.
The article was translated by the authors. 相似文献