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21.
Yingtai Chen Yumin Li Hong Zhang Yi Xie Xuezhong Chen Jinyu Ren Xiaowei Zhang Zijiang Zhu Hongliang Liu Yawei Zhang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The aim of this study was to estimate the acute effects of low dose 12C6+ ions or X-ray radiation on human immune function. The human peripheral blood lymphocytes (HPBL) of seven healthy donors were exposed to 0.05 Gy 12C6+ ions or X-ray radiation and cell responses were measured at 24 h after exposure. The cytotoxic activities of HPBL were determined by 3-(4,5-dimethylthiazol-2-yl)-2,5-diphenyl tetrazolium bromide (MTT); the percentages of T and NK cells subsets were detected by flow cytometry; mRNA expression of interleukin (IL)-2, tumor necrosis factor (TNF)-α and interferon (IFN)-γ were examined by real time quantitative RT-PCR (qRT-PCR); and these cytokines protein levels in supernatant of cultured cells were assayed by enzyme-linked immunosorbent assays (ELISA). The results showed that the cytotoxic activity of HPBL, mRNA expression of IL-2, IFN-γ and TNF-α in HPBL and their protein levels in supernatant were significantly increased at 24 h after exposure to 0.05 Gy 12C6+ ions radiation and the effects were stronger than observed for X-ray exposure. However, there was no significant change in the percentage of T and NK cells subsets of HPBL. These results suggested that 0.05 Gy high linear energy transfer (LET) 12C6+ radiation was a more effective approach to host immune enhancement than that of low LET X-ray. We conclude that cytokines production might be used as sensitive indicators of acute response to LDI. 相似文献
22.
S. Narendranath P.S. Athiray P. Sreekumar V. Radhakrishna A. Tyagi B.J. Kellett the CLASS team 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Surface chemistry of airless bodies in the solar system can be derived from remote X-ray spectral measurements from an orbiting spacecraft. X-rays from planetary surfaces are excited primarily by solar X-rays. Several experiments in the past have used this technique of X-ray fluorescence for deriving abundances of the major rock forming elements. The Chandrayaan-2 orbiter carries an X-ray fluorescence experiment named CLASS that is designed based on results from its predecessor C1XS flown on Chandrayaan-1. We discuss the new aspects of lunar science that can be potentially achieved with CLASS. 相似文献
23.
B. Sylwester J. Sylwester K.J.H. Phillips E. Landi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
We present the observations of He-like Ar triplet lines obtained by RESIK spectrometer aboard CORONAS-F. Interpretation of intensity ratios between triplet lines of lower Z elements is known to provide useful diagnostics of plasma conditions within the emitting source. Here, we investigate whether triplet line ratios are useful for interpretation of higher Z element spectra. A high sensitivity, low background and precise absolute calibration of RESIK allow to consider in addition also the continuum contribution. This provides a way to determine the Ar absolute abundance from the observed triplet component ratios. The method is presented and the results are shown for two selected flares. Derived values of Ar absolute abundance for these flares are found to be similar: 2.6 × 10−6 and 2.9 × 10−6. They fall in the range between presently accepted Ar photospheric and coronal abundances. 相似文献
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25.
H.S. Ahluwalia C. Lopate 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Solar modulations of galactic cosmic ray (GCR) intensity contain a wealth of information about their transport in the heliosphere. To extract this information from the data one studies the dependence of the observed modulations on the mean energy of response of detectors providing data for the analyses. There is a great deal of confusion about the detector energy response to GCR spectrum in the literature. We present a preliminary report on the computations of the mean energy of response for the Climax neutron monitor (CL/NM) and IMP 8 cosmic ray nuclear composition instrument to GCR protons for 1973–1998, covering the solar cycles 21 and 22. We find that for penetrating proton channel on IMP 8 the mean energy changes by a factor of over two whereas for the neutron monitor the change is only 21%. However, the corresponding change for the computed modulation function is a factor of about 3.5. 相似文献
26.
本文介绍了X光电子能谱(XPS)分析技术在复合固体推进剂燃烧机理研究中的应用。用XPS分析对一种呈负压力指数燃烧特性的聚氨酯复合固体推进剂(404-5A)的未然表面和在2、2.5、3.0、3.5、4.0MPa压强下快速降压熄火后的燃烧表面作元素组成及其化学价态的分析,得到了不同价态的各元素原子百分含量。从实验结果可以确定CaCO_3在凝相反应中生成了CaCl_2。从燃面上碳原子浓度随燃烧压强的变化说明了燃烧过程中存在着熔化的粘合剂对过氯酸铵表面的流动覆盖,覆盖程度随着燃烧压强的上升而增加。本文还对CaCO_3、粘合剂流动覆盖在燃烧过程中的作用进行了探讨。 相似文献
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28.
对X光安检图像进行去噪处理可以更清楚地显示出危险物。针对传统小波软硬阈值去噪方法的缺陷.给出了一种自适应阈值的去噪方法,在此方法中,首先进行软硬阈值的折中处理,然后分别对大于和小于阈值的两部分进行自适应处理。利用Tennessee大学提供的实际采集的X光安栓图像进行实验,结果表明该方法能有效地去除安检图像中的噪声,图像去噪后的信噪比、峰值信噪比分别是25.2229dB、27.708dB.与含噪图像相比分别增加了7.7253dB和7.739dB。因此该方法表现出较高的去噪性能。 相似文献
29.
A.R. Engel K. Beurle A. Bewick P.K.S. Harper J.J. Quenby N.J.C. Spooner A.G. Fenton K.B. Fenton A.B. Giles J.G. Greenhill D.M. Warren I.M. Martin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
Hard X-ray balloon altitude measurements with a 1600 cm2 phoswich array are described. Data from observations on Sco X-1, GX1+4, GX5−1, Nova Oph. 1977, SMC X-1, SS433, IC 4329A and MR 2251-178 are presented. The role of Comptonisation in X-ray production for Sco X-1 and GX1+4 is discussed. 相似文献
30.
采用2θ-ω对称扫描,对(111)、(333)、(044)不同衍射面进行了ω扫描,得到了InSb不同衍射面之间强度和半峰宽度的规律;对晶片上不同位置进行了同一衍射面的ω扫描,得到半峰宽度的mapping,此外,还对材料进行了倒易空间(RSM)扫描。测试结果表明InSb材料结晶质量完好,均匀性好,符合制造良好光电器件的标准。 相似文献