排序方式: 共有23条查询结果,搜索用时 203 毫秒
1.
L.L. Lazutin A.A. Khrushchinsky T.V. Kozelova A.O. Melnikov Ya. Sakharov G. Kremser W.K. Riedler K.M. Torkar K. Glassmeier J.-P. Treilhou A. Pedersen G. Gustafsson R. Pellinen J. Kangas 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(4):171-174
For investigations of the isolated magnetospheric substorm the ground-based and satellite geophysical data are discussed. The active phase of the substorm has two parts: an active-convective phase and a classical active phase. The analysed data show that the breakup of the substorm takes place at closed and not very much stretched magnetic field lines. 相似文献
2.
During strong magnetic storms in July and November of 2004 the fluxes of trapped particles (protons and electrons of MeV energies)
in the Earth’s radiation belts have increased by orders of magnitude and then decreased remaining on an enhanced level for
several months. These enhancements allowed us to study the processes of relaxation of the radiation belts. Measurements of
energetic particles by low-altitude satellites Coronas-F and Servis-1 have shown that predictions of the theory about the rate of pitch-angle diffusion are not always correct, giving both overestimated
and underestimated values for the lifetime of energetic particles. 相似文献
3.
L.P. Block L.L. Lazutin W. Riedler 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(1):121-128
The magnetosphere is explored in situ by satellites, but measurements near the low altitude magnetospheric boundary by rockets, balloons and groundbased instruments play a very significant role. The geomagnetic field provides a frame with anisotropic wave and particle propagation effects, enabling remote sensing of the distant magnetosphere by means of balloon-borne and groundbased instruments. Examples will be given of successful studies, with coordinated satellite and balloon observations, of substorm, pulsation and other phenomena propagating both along and across the geomagnetic field. Continued efforts with sophisticated balloon-borne instrumentations should contribute substantially to our understanding of magnetospheric physics. 相似文献
4.
Deming Ross Schindler John Perlovsky Leonid 《IEEE transactions on aerospace and electronic systems》2009,45(2):593-611
A new approach is described for combining range and Doppler data from multiple radar platforms to perform multi-target detection and tracking. In particular, azimuthal measurements are assumed to be either coarse or unavailable, so that multiple sensors are required to triangulate target tracks using range and Doppler measurements only. Increasing the number of sensors can cause data association by conventional means to become impractical due to combinatorial complexity, i.e., an exponential increase in the number of mappings between signatures and target models. When the azimuthal resolution is coarse, this problem will be exacerbated by the resulting overlap between signatures from multiple targets and clutter. In the new approach, the data association is performed probabilistically, using a variation of expectation-maximization (EM). Combinatorial complexity is avoided by performing an efficient optimization in the space of all target tracks and mappings between tracks and data. The full, multi-sensor, version of the algorithm is tested on simulated data. The results demonstrate that accurate tracks can be estimated by exploiting spatial diversity in the sensor locations. Also, as a proof-of-concept, a simplified, single-sensor range-only version of the algorithm is tested on experimental radar data acquired with a stretch radar receiver. These results are promising, and demonstrate robustness in the presence of nonhomogeneous clutter. 相似文献
5.
6.
J.-P. Treilhou T.V. Kozelova L.L. Lazutin V.G. Petrov I.Z. Zhulin A. Pedersen R. Pellinen W.K. Riedler G. Marklund 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(4):163-169
Measurements of the electric field in the ionosphere and the equatorial plane during the pre-onset and actives phases of a substorm (March 4, 1979) are compared. Correlations and disagrements between the measurements are considered. The preliminary conclusion is reached that the model of electrojet polarisation proposed by CORONITI and KENNEL (1972) could possibly explain part of our observations. 相似文献
7.
Based on a large number of measurements of the magnetic field and energetic particles onboard the CRRES satellite and on ground-based measurements we describe the fine structure of the first several minutes of the expansion activation of a substorm. The main result is that we have found a fast enhancement of the flux of energetic ions immediately before the beginning of substorm dipolization of the magnetic field. This effect was not known earlier, and the enhancement is invisible from the ground during auroras. We suggest that the appearance of an excess flux of energetic ions has a triggering effect on the local expansion activation of a substorm. The model of a current meander is put forward, which explains the generation of an inductance electric field, current wedge, and other effects of the explosive onset of a substorm. 相似文献
8.
Leonid Ksanfomality John Harmon Elena Petrova Nicolas Thomas Igor Veselovsky Johan Warell 《Space Science Reviews》2007,132(2-4):351-397
New planned orbiter missions to Mercury have prompted renewed efforts to investigate the surface of Mercury via ground-based
remote sensing. While the highest resolution instrumentation optical telescopes (e.g., HST) cannot be used at angular distances
close to the Sun, advanced ground-based astronomical techniques and modern analytical and software can be used to obtain the
resolved images of the poorly known or unknown part of Mercury. Our observations of the planet presented here were carried
out in many observatories at morning and evening elongation of the planet. Stacking the acquired images of the hemisphere
of Mercury, which was not observed by the Mariner 10 mission (1974–1975), is presented. Huge features found there change radically
the existing hypothesis that the “continental” character of a surface may be attributed to the whole planet. We present the
observational method, the data analysis approach, the resulting images and obtained properties of the Mercury’s surface. 相似文献
9.
I.N. Myagkova M.I. PanasyukL.L. Lazutin E.A. MuravievaL.I. Starostin T.A. IvanovaN.N. Pavlov I.A. RubinshteinN.N. Vedenkin N.A. Vlasova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The Russian microsatellite “Universitetskiy-Tatiana” was launched on Jan. 20, 2005 and was both a scientific and educational mission. Its two main aims were declared as: (1) monitoring of the energetic particles dynamics in the near-Earth space environment after solar events and during quiet times, (2) educational activities based on experimental data obtained from the spacecraft. In this paper observations acquired during Dec. 5–16, 2006, known as “Solar Extreme Events 2006”, were analyzed. The “Universitetskiy-Tatiana” microsatellite orbit permits one to measure both solar energetic particle dynamics, variations of the boundary of solar particle penetration, as well as relativistic and sub-relativistic electrons of the Earth’s outer radiation belt during and after magnetic storms. Both relativistic electrons of the Earth’s outer radiation and solar energetic particles are an important source of radiation damage in near-Earth space. Therefore, the presented experimental results demonstrate the successful application of a small educational spacecraft both for scientific and educational programs. 相似文献
10.
S.N. Kuznetsov L.L. Lazutin M.I. Panasyuk L.I. Starostin Yu.V. Gotseliuk N. Hasebe K. Sukurai M. Hareyama 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
It is a case study of a chain of three magnetic storms with a special attention to the particle dynamics based on CORONAS-F and SERVIS-1 low altitude satellite measurements. Solar proton penetration inside the polar cap and inner magnetosphere and dynamics at different phases of the magnetic storms was studied. We found, that solar protons were captured to the inner radiation belt at the recovery phase of the first and the second magnetic storms and additionally accelerated during the last one. No evidence of sudden commencement (SC) particle injection was found. Enhanced solar proton belt intensity with small pitch angles decreased slowly during satellite orbits for 30 days until the next magnetic storm. Then in 20–30 h we registered strong precipitation of these protons followed by the trapped proton flux dropout. Intensity decrease was more pronounced at lower altitudes and higher particle energies. 相似文献