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71.
LIU Zhenxing CAO Jinbin 《空间科学学报》2008,(5)
This paper presents the status of two satellites of Double Star Program,and a part of scientific results based on the data of Double Star Program obtained during the period of 2006-2008.Other scientific results in the magnetospheric physics research can be found in "Multi scale physical process in the magnetosphere" of this issue. 相似文献
72.
A.N. Petrov O.R. GrigoryanM.I. Panasyuk 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(8):1269-1273
The results of proton energy (tens keV – several MeV) spectrum measurements near geomagnetic equator (L < 1.15) at low altitudes (<1000 km) are presented. We used data of experiments onboard ACTIVE, SAMPEX, NOAA TIROS-N satellites and SPRUT-VI (MIR station) and cover a time range of about 30 years (including previous measurements). It was found that the kappa-distribution function fits the experimental spectrum with the best correlation coefficient. A comparison of energy spectra of near-equatorial protons and ring-current protons was made. Using the estimation of the life time of near-equatorial protons we explain the difference in spectral indices of radiation belt and near-equatorial proton formation. We conclude that the ring current is the main source of the near-equatorial protons. 相似文献
73.
M.G.G.T. Taylor B. Lavraud C.P. Escoubet S.E. Milan K. Nykyri M.W. Dunlop J.A. Davies R.H.W. Friedel H. Frey Y.V. Bogdanova A. Åsnes H. Laakso P. Trávnı´cek A. Masson H. Opgenoorth C. Vallat A.N. Fazakerley A.D. Lahiff C.J. Owen F. Pitout Z. Pu C. Shen Q.G. Zong H. Rème J. Scudder T.L. Zhang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(10):1619-1629
During conditions of northward interplanetary magnetic field (IMF), the near-tail plasma sheet is known to become denser and cooler, and is described as the cold-dense plasma sheet (CDPS). While its source is likely the solar wind, the prominent penetration mechanisms are less clear. The two main candidates are solar wind direct capture via double high-latitude reconnection on the dayside and Kelvin–Helmholtz/diffusive processes at the flank magnetopause. This paper presents a case study on the formation of the CDPS utilizing a wide variety of space- and ground-based observations, but primarily from the Double Star and Polar spacecraft on December 5th, 2004. The pertinent observations can be summarized as follows: TC-1 observes quasi-periodic (∼2 min period) cold-dense boundary layer (compared to a hot-tenuous plasma sheet) signatures interspersed with magnetosheath plasma at the dusk flank magnetopause near the dawn-dusk terminator. Analysis of this region suggests the boundary to be Kelvin–Helmholtz unstable and that plasma transport is ongoing across the boundary. At the same time, IMAGE spacecraft and ground based SuperDARN measurements provide evidence of high-latitude reconnection in both hemispheres. The Polar spacecraft, located in the southern hemisphere afternoon sector, sunward of TC-1, observes a persistent boundary layer with no obvious signature of boundary waves. The plasma is of a similar appearance to that observed by TC-1 inside the boundary layer further down the dusk flank, and by TC-2 in the near-Earth magnetotail. We present comparisons of electron phase space distributions between the spacecraft. Although the dayside boundary layer at Polar is most likely formed via double high-altitude reconnection, and is somewhat comparable to the flank boundary layer at Double Star, some differences argue in favour of additional transport that augment solar wind plasma entry into the tail regions. 相似文献
74.
Michael A. Raadu 《Space Science Reviews》1994,68(1-4):29-38
A Double layer (DL) in a current carrying plasma sustains a localised net potential difference and acts as an impedance converting electrical energy to directed particle energy determined by the DL potential. DL's accelerate equal numbers of ions and electrons for relativistic energies, otherwise electron energisation predominates. Their time independent structure may be described as a BGK (Bernstein-Greene-Kruskal) state analogous to that for laminar shocks, and certain existence criteria must be satisfied. The generalised Langmuir criterion requires total particle pressure balance over the DL and may imply propagation in the plasma reference frame. The Bohm criteria require sufficiently large current densities and are closely related to the local stability condition at the edges of the DL. The DL potential must be sustained externally, for example by the release of stored magnetic energy. A steady state is also possible where (externally maintained) mass motions drive a dynamo region connected by currents to the DL which acts as an electrical load. 相似文献
75.
Pair creation in relativistic double layers in shown to have consequences for the charge density in the double layer and the current flowing through it. 相似文献
76.
研究了炭黑对低燃温双基平台推进剂燃烧性能的影响。指出随着炭黑含量的增加,推进剂燃速也增加,平台或麦撒燃烧区向高压移动;但当炭黑达到某一含量后,炭黑含量再增加,燃速反而下降,平台燃烧区消失。对此现象作了理论解释,并用二次多项式拟合出炭黑含理与燃速的关系。 相似文献
77.
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79.
分析了碳单元的结构特征,推论出双基和改性双基推进剂的分解温度、表面温度不随压力和初温而改变,以及碳单元顶端温度相对稳定.依此讨论了燃速温度系数及其规律. 相似文献
80.