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11.
Kamide Y. Kihn E.A. Ridley A.J. Cliver E.W. Kadowaki Y. 《Space Science Reviews》2003,107(1-2):307-316
We report the recent progress in our joint program of real-time mapping of ionospheric electric fields and currents and field-aligned
currents through the Geospace Environment Data Analysis System (GEDAS) at the Solar-Terrestrial Environment Laboratory and
similar computer systems in the world. Data from individual ground magnetometers as well as from the solar wind are collected
by these systems and are used as input for the KRM and AMIE magnetogram-inversion algorithms, which calculate the two-dimensional
distribution of the ionospheric parameters. One of the goals of this program is to specify the solar-terrestrial environment
in terms of ionospheric processes, providing the scientific community with more than what geomagnetic activity indices and
statistical models provide.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
12.
13.
Gaurang B. Yodh 《Space Science Reviews》1996,75(1-2):199-212
This paper discusses the properties of using the water Cherenkov technique to detect air showers in the few hundred GeV to 100 TeV energy range. The responses of a 6 m2 2 m deep water Cherenkov counter and that of a 6 m2 10cm thick scintillator-lead sandwich counter to air shower electrons and photons is described. The advantages of water Cherenkov detector is outlined. Its application to do VHE gamma ray astronomy is discussed with particular reference to the MILAGRO telescope currently under construction. Milagro, a water-Cherenkov detector to do gamma ray astronomy above 100 Gev, uses an existing pool 60m × 80m by 8m, located in the Jemez mountains near Los Alamos, NM. The threshold of the MILAGRO detector is comparable to atmospheric Cherenkov detectors, however it has several advantages over these optical detectors. MILAGRO can operate 24 hours a day in all weather conditions and it has an open aperture which allows it to view the entire northern sky every day. These capabilities allow for a systematic all-sky survey to be done for the first time at these energies. MILAGRO will measure the Crab spectrum with high significance over a wide energy range, it will detect and measure the spectra from AGN's such as MRK 421 and it will search for short duration bursts from GRBs and possibly evaporating PBHs. 相似文献
14.
新建他激反激变换器方程及其解析解 总被引:1,自引:1,他引:0
引用文 [1 ]的思路 ,寻找他激反激变换器的运行状态特征参量 (磁通密度增量、剩余磁通密度和占空比 )与构成这一变换器的基本物理参量之间的函数关系。首先阐明由于频率给定 ,他激反激变换器稳态运行时会出现无剩磁工况和有剩磁工况两种。而后确定这两种工况下 ,磁路等效储能空间单位体积每个周期的传输能量 (命名为“磁能传输密度”)。在这基础上 ,分别建立和解出他激反激变换器在不同工况下稳定运行时应满足的方程。最后根据所得的解析解阐明这种变换器的特性。本文和文 [1 ],以磁路分析为基础建立了一种新的反激变换器理论。 相似文献
15.
Y. Futaana S. Barabash A. Grigoriev D. Winningham R. Frahm M. Yamauchi R. Lundin 《Space Science Reviews》2006,126(1-4):315-332
As a part of the global plasma environment study of Mars and its response to the solar wind, we have analyzed a peculiar case
of the subsolar energetic neutral atom (ENA) jet observed on June 7, 2004 by the Neutral Particle Detector (NPD) on board
the Mars Express satellite. The “subsolar ENA jet” is generated by the interaction between the solar wind and the Martian
exosphere, and is one of the most intense sources of ENA flux observed in the vicinity of Mars. On June 7, 2004 (orbit 485
of Mars Express), the NPD observed a very intense subsolar ENA jet, which then abruptly decreased within ∼10 sec followed
by quasi-periodic (∼1 min) flux variations. Simultaneously, the plasma sensors detected a solar wind structure, which was
most likely an interplanetary shock surface. The abrupt decrease of the ENA flux and the quasi-periodic flux variations can
be understood in the framework of the global response of the Martian plasma obstacle to the interplanetary shock. The generation
region of the subsolar ENA jet was pushed towards the planet by the interplanetary shock; and therefore, Mars Express went
out of the ENA jet region. Associated global vibrations of the Martian plasma obstacle may have been the cause of the quasi-periodic
flux variations of the ENA flux at the spacecraft location. 相似文献
16.
17.
有机高分子絮凝剂处理高浊度原水效果和机理研究 总被引:2,自引:0,他引:2
本文研究了有机高分子絮凝剂PAM、CTAB及它们的复配PAM+CTAB处理高浊度原水的最佳实验条件、絮凝性能、效果和机理,为有机高分子絮凝剂的选择和管式絮凝器的研制提供了理论依据。 相似文献
18.
结合介绍国家七·五项目“离心机微机监控设备”的模拟调试,论述了实验室或现场模拟调试的重要性;研究了模拟调试的内容和被物理、电子模拟装置替代的实际系统中的对象的分类;探讨了如何设计与制作一个或若干个既简单又“逼真”的模拟调试辅助装置,建立一个高效率的模拟调试环境。 相似文献
19.
复合材料元件吸能能力的数值模拟 总被引:2,自引:0,他引:2
运用MSC/DYTRAN有限元软件,对碳纤维一环氧树脂“┼”字型、“┬”字型、“┐”字型3种典型复合材料元件的破坏过程、峰值栽荷、平均栽荷和能量吸收能力进行了数值模拟研究。鉴于MSC/DYTRAN有限元软件不能直接用于复合材料的吸能分析,分析时采用了等效的方法。将复合材料结构元件的数值计算结果与准静态轴向压溃试验的结果进行对比,两者较为一致,从而说明运用该有限元软件并采用等效的方法模拟复合材料结构吸能能力的可行性。 相似文献
20.
通过研究柠檬酸钙酸解过程中溶液电导率的变化规律,建立了酸解体系的数学模型,提出了改革酸解工艺路线中的物料添加顺序,并用计算机自动控制物料添加量和添加速率,自动判定酸解终点的方法。 相似文献