排序方式: 共有58条查询结果,搜索用时 14 毫秒
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T. Okajima Y. Tawara Y. Ogasaka K. Tamura A. Furuzawa K. Yamashita H. Kunieda 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2682-2687
X-ray telescopes have been providing high sensitivity X-ray observations in numerous missions. For X-ray telescopes in the future, one of the key technologies is to expand the energy band beyond 10 keV. We designed depth-graded multilayer, so-called supermirrors, for a hard X-ray telescope in the energy band up to 40 keV using lightweight thin-foil optics. They were successfully flown in a balloon flight and obtained a hard X-ray image of Cyg X-1 in the 20–40 keV band. Now supermirrors are promising to realize a hard X-ray telescope. We have estimated the performance of a hard X-ray telescope using a platinum–carbon supermirror for future satellite missions, such as NeXT (Japan) and XEUS (Europe). According to calculations, they will have a significant effective area up to 80 keV, and their effective areas will be more than 280 cm2 even at 60 keV. Limiting sensitivity will be down to 1.7 × 10−13 erg cm−2 s−1 in the 10–80 keV band at a 100 ks observation. In this paper, we present the results of the balloon experiment with the first supermirror flown and projected effective areas of hard X-ray telescopes and action items for future missions. 相似文献
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Yu.N. Gnedin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
The theory of polarization effects in radiation from compact X-ray sources is presented. The following four problems are considered: 1) the polarization of X-rays from the magnetized neutron stars; 2) the polarization of X-rays from the accretion disk around a black hole; 3) the optical polarization from X-ray binaries, and 4) the results of X-ray polarimetric observations. 相似文献
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M. Hayashi 《Space Science Reviews》1992,61(1-2):99-102
I describe plans for submillimetre and infrared satellites which are now under discussion among Japanese infrared and millimetre astronomers. We propose a submillimetre and/or infrared mission to be launched around 2000 with a main reflector 1–2 m in diameter and cooled down to 50–150 K. This mission, although a small one, will be able to contribute significantly to the advance in submillimetre and infrared astronomy if its role is specified for suitable purposes like surveys. 相似文献
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建立了一个考虑地球非球形引力摄动的卫星轨道摄动模型并用C++语言编写程序进行轨道计算,其积分器采用Runge-Kutta-Fehlberg7(8)。建模过程中,对岁差、章动等量的计算分别考虑了美国海军天文台1981年和2005年的两种天文标准。通过与STK对比,发现无论采用哪一种标准,轨道传播两天后的位置误差都不会超过分米量级,速度误差不会超过毫米每秒的量级。说明了建模和编程计算的合理性,以及采用新旧两种天文标准计算卫星轨道的差别甚小。 相似文献
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Thérèse Encrenaz 《Space Science Reviews》1992,61(1-2):13-17
The ISO mission is expected to allow significant progress in the study of Solar-System objects, especially concerning planetary and cometary atmospheres. Beyond ISO, future Solar-System studies using infrared space missions will require an extension of the spectral coverage toward longer wavelengths and increased spatial capabilities for imaging spectroscopy. 相似文献
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