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辐射测温仪工作波长的选择方法 总被引:8,自引:3,他引:5
在辐射测温仪工作波长的选择上,以往一直参照维思位移定律。通过理论分析,发现依照该定律选择测温仪工作彼长是不完善的。为了提高仪表灵敏度和测温准确度,推导出了一种新公式,提出了一种新的工作波长的选择方法,并在理论上证明该方法较目前常用的方法更为理想。 相似文献
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根据固体火箭发动机羽焰特征研制了多目标多光谱高温仪,它可同时测量羽焰六个目标点的温度,每个目标点均有八个工作波长。同时提出了求解真温的实用方法,完成了固体火箭发动机羽焰温度及其分布的测量。 相似文献
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P.O. Petrucci J. Ferreira G. Henri L. Sauge G. Pelletier 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2909-2911
We present a unified accretion–ejection picture that explains the different spectral state of Black Hole X-ray binaries (BHXrB) from radio to X/γ-rays. In this view, the central region of BHXrB has a multi-flow configuration which consists in (1) an outer standard accretion disc, (2) an inner magnetized accretion disc driving, (3) a self-collimated electron–proton MHD jet, surrounding and (4) a relativistic electron–positron beam when adequate conditions are met. This picture provides a simple and unified explanation to the various canonical spectral states of BH X-ray binaries, by varying the transition radius rJ between the inner disc driving jets and the outer standard disc. In this framework, large rJ correspond to Quiescent and Hard states while small rJ correspond to Thermal Dominant ones. In between these two extremes, rJ can reach values that switches on the pair cascade process giving birth to a relativistic electron–positron beam. This would correspond to the bright intermediate state. 相似文献