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1.
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
2.
Joris A. D. L. Blommaert Jan Cami Ryszard Szczerba Michael J. Barlow 《Space Science Reviews》2005,119(1-4):215-243
A large fraction of ISO observing time was used to study the late stages of stellar evolution. Many molecular and solid state
features, including crystalline silicates and the rotational lines of water vapour, were detected for the first time in the
spectra of (post-)Asymptotic Giant Branch (AGB) stars. Their analysis has greatly improved our knowledge of stellar atmospheres
and circumstellar environments. A surprising number of objects, particularly young planetary nebulae with Wolf-Rayet (WR)
central stars, were found to exhibit emission features in their ISO spectra that are characteristic of both oxygen-rich and
carbon-rich dust species, while far-IR observations of the PDR around NGC 7027 led to the first detections of the rotational
line spectra of CH and CH+.
Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries:
France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA. 相似文献
3.
L. B. F. M. Waters 《Space Science Reviews》1992,61(1-2):25-43
In this review the IR emission from circumstellar material is discussed, both of ionized gas and dust grains, and the astrophysical information that can be extracted from such observations. Some emphasis is placed on the possibilities of stellar IR astronomy using a large space-borne telescope, especially with respect to the much better spatial and spectral resolution of such a telescope compared to the current generation of ground-based and space IR telescopes. 相似文献
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文章主要介绍了具有凝视成像功能的红外探测系统的研究和设计。首先简要描述了红外测角系统的组成和工作原理;然后重点论述了红外探测系统的性能指标和光学设计;最后对红外探测系统设计研究作了总结和展望。 相似文献
7.
应用红外遥感寻找地下热水初探 总被引:1,自引:1,他引:1
文章利用陆地卫星TM6波段能反映地物辐射温度差异这一特点,通过HIS彩色变换等处理,对快速寻找地下热水进行了探讨。为研究地下热水开发,发展山西省旅游及医疗事业提供一种具有广泛应用前景的方法。 相似文献
8.
通过对部位安排原则的讨论,结合实例,介绍该类导弹常见的部位安排形式。通过地体制和任务的分析,归纳出该类导弹结构上的特点,列举出反映辽些特点的具体结构实例。 相似文献
9.
用FVM法计算固体火箭羽流的红外特性 总被引:9,自引:2,他引:9
建立了有限体积法(FVM)的理论模型模拟固体火箭羽流的红外特性,研究了燃气组分H2O,CO2,CO,HCL,OH,NO的吸收和发射,以及AL2O3粒子云的吸收、发射和散射,还研究了两相流场中气相和粒子云温度不均匀时对辐射传输方程的修正。计算一单喷管固体火箭的二维轴对称羽流在光谱2~5μm的红外特性,给出羽流辐射的空间分布和光谱分布并与文献计算的结果对比。研究表明:有限体积法能较好地模拟固体火箭羽流的红外特性;粒子辐射占固体火箭羽流红外辐射的主要部分;在光谱2~4μm粒子辐射使羽流辐射增强,而在光谱4~5μm粒子辐射使羽流辐射减弱。 相似文献
10.
红外型空空导弹智能制导律研究 总被引:1,自引:0,他引:1
本文论述了红外型空空导弹应用智能控制的理论基础及结构特点,以多级智能控制的框架和机理设计出以比例导引为主、智能控制为辅的变指令智能制导律,并编制计算机软件以数字仿真的形式验证变指令智能制导规律的有效性和可行性 相似文献