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41.
Marian Karlický 《Space Science Reviews》2006,122(1-4):161-168
An acceleration process in the collapsing magnetic trap, formed in the flare with cusp magnetic field topology, is described.
Computations show that high-energy electrons are accumulated in the central part of the collapsing magnetic trap due to an
increase of their pitch angles. The effect explains in a natural way the formation of X-ray loop-top sources. Then, using
the model with the collapsing trap and considering only the adiabatic heating process, a possible explanation for the motion
of the X-ray loop-top source observed at the beginning of some cusp-type flares is presented. 相似文献
42.
高超声速飞行器流动特征分析 总被引:6,自引:2,他引:4
在非流线型构件或突起物的扰动效应、高马赫数和低雷诺数极限效应、低湍流度环境效应和由激波或摩擦导致的气动加热效应等4个方面的影响下,未来高超声速飞行器涉及的流动主要表现出这样的特点:典型流动结构强度高、尺度大,如强激波和厚边界层;局部流动结构数量多;激波、膨胀波和边界层结构之间相互干扰十分严重;转捩、压力脉动和一些流动结构对细微因素非常敏感;压力、摩擦应力和热流峰值现象普遍;升阻比屏障难以突破;流场同时依赖大量无量纲参数和有量纲参数,导致实验模拟难度大。本文在回顾传统高超声速流动主要流动现象的基础上,对上述7个方面涉及的典型流动现象的基础研究现状、问题本质和因果关系进行综合描述,讨论如何更有效地面对基础研究和工程实际问题。该文既可为解决典型流动现象中尚未解决的基础研究提供帮助,也可为如何合理地利用有限的已知知识解决工程应用问题提供指导。 相似文献
43.
为验证和指导高速飞行器的防隔热设计,准确地模拟气动热产生的热量穿透防隔热材料进而影响舱内温度空间分布和时间变化的过程,研究了一种同时求解机体外流场及气动热、机体结构传热及舱内流场温度场仿真计算方法,其中的传热方式包括热传导、热对流及热辐射。采用两套计算模型、两种求解器、一个数据交换文件的计算结构,构建了一种针对流场-热-结构的多场耦合分析方法,实现了对固体隔绝内外流场温度动态变化问题的仿真分析。最后通过计算实例验证了整套计算方法,得到的飞行器舱内温度变化特性能够用于指导高速飞行器的防隔热设计。 相似文献
44.
45.
M. Kalinkov K. Stavrev I. Kuneva 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
An attempt is made to compare optical properties of Abell clusters with X-ray sources. 相似文献
46.
Guido Chincarini 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
In this lecture I review part of the published and unpublished observational evidence showing that cluster spiral galaxies are hydrogen deficient. Always using observational data, it is argued that the deficiency is due to the interaction between the galaxies and the intergalactic medium. Furthermore it is shown that the stellar population of deficient galaxies has also been affected and a brief discussion is given of the mechanisms at work. 相似文献
47.
A.A. Stepanian 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
A brief review of very high energy gamma-ray astronomy achievements is presented. The results of observations of the Crab nebula, the Cygnus X-3, Vela pulsar, radiogalaxy Centaurus A and 2CG 195+4 show that all these objects are the sources of very high energy gamma-quanta. The most powerfull source is Cygnus X-3. Its gamma-ray luminosity is no less than 3·1037 erg.s−1. The upper limit of quanta energy is no less than 1016eV. All sources are variable in different time scales, from milliseconds up to years. The nature of all these sources is not known yet, but known ones are pulsars. 相似文献
48.
针对高超声速滑翔飞行器再入过程中面对的多约束问题,提出一种基于虚拟多触角探测的路航点规划机动制导策略。该机动制导策略通过飞行器最大转弯轨迹计算速度-剩余地面距离-航向角约束,在分段定点模式中发出多条粗略预测触角,引用触角末端反馈的信息计算优先级以确定临时路航点;同时在机动制导模式中发出精细探测触角,计算触角末端信息优先级,经倾侧角延时滤波器得出控制指令,对飞行器进行机动制导。基于多触角探测的路航点规划机动制导策略,降低了三触角机动制导方法中的计算时间;同时,4种典型禁飞区条件下的仿真结果表明,该策略能够有效稳定地解决机动制导过程中的多约束问题。 相似文献
49.
This paper proposes a novel algorithm for Two-Dimensional (2D) central Direction-of-Arrival (DOA) estimation of incoherently distributed sources. In particular, an orthogonal array structure consisting of two Non-uniform Linear Arrays (NLAs) is considered. Based on first-order Taylor series approximation, the Generalized Array Manifold (GAM) model can first be established to separate the central DOAs from the original array manifold. Then, the Hadamard rotational invariance relationships inside the GAMs of two NLAs are identified. With the aid of such relationships, the central elevation and azimuth DOAs can be estimated through a search-free polynomial rooting method. Additionally, a simple parameter pairing of the estimated 2D angular parameters is also accomplished via the Hadamard rotational invariance relationship inside the GAM of the whole array. A secondary but important result is a derivation of closed-form expressions of the Cramer-Rao lower bound. The simulation results show that the proposed algorithm can achieve a remarkably higher precision at less complexity increment compared with the existing low-complexity methods, which benefits from the larger array aperture of the NLAs. Moreover, it requires no priori information about the angular distributed function. 相似文献
50.
It is well known that the Two-step Weighted Least-Squares(TWLS) is a widely used method for source localization and sensor position refinement. For this reason, we propose a unified framework of the TWLS method for joint estimation of multiple disjoint sources and sensor locations in this paper. Unlike some existing works, the presented method is based on more general measurement model, and therefore it can be applied to many different localization scenarios.Besides, it does not have the initialization and local convergence problem. The closed-form expression for the covariance matrix of the proposed TWLS estimator is also derived by exploiting the first-order perturbation analysis. Moreover, the estimation accuracy of the TWLS method is shown analytically to achieve the Cramér-Rao Bound(CRB) before the threshold effect takes place. The theoretical analysis is also performed in a common mathematical framework, rather than aiming at some specific signal metrics. Finally, two numerical experiments are performed to support the theoretical development in this paper. 相似文献