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为了解决月基紫外深空观测相机地面定标的难题,研制了一种动态范围大、星等模拟精度高的紫外星模拟器。该模拟器采用5 m离轴光管作为准直光学系统,用双积分球系统作为均匀光源,可模拟3~16等星的弱目标,其星等最小分辨率为0.2等星,星等不确定度为5.48%。通过试验证明,该星模拟器完全满足月基紫外弱光星等深空观测相机地面定标的试验要求,不仅可以在实验室内标定紫外观测相机的探测能力和灵敏度,还可用于测试观测相机的其它参数指标,为发展深空高轨探测相机提供了地面定标基础。 相似文献
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小视场长焦距镜头畸变高精度测量研究 总被引:2,自引:0,他引:2
利用由精密测角仪、显微摄像测量系统、微型双光栅平面干涉仪、平行光管以及星点组成畸变测量系统,对小视场长焦距的镜头进行畸变测量。在计算镜头畸变中,利用中心视场区域内畸变设计无穷小,采用三次多项式拟和的方法,计算镜头理论焦距;在边视场采用像高高次方和视场角正弦高次方加权平均的方法对测量偏差角进行修正,得到各视场的相对和绝对畸变。通过实际测量和计算验证,镜头全视场畸变测量精度可达到0.02%。 相似文献
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在HL-1装置电子密度测量中,进一步改进了密度相移信号的处理方法。在氘放电、氦补充送气条件下得到了HL-1最高电子密度10.8×1013cm-3。总结了密度在各种实验条件下的行为,并对各种实验条件对密度的影响进行了分析。 相似文献
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One-dimensional particle-in-cell simulations are performed to investigate the nonlinear evolution of electromagnetic instabilities excited by the electron temperature anisotropy in homogeneous plasmas with different parameters. The results show that the electron temperature anisotropy can excite the two right-hand electromagnetic instabilities, one has the frequency higher than Ωe, the other is the whistler instability with larger amplitude, and its frequency is below Ωe. Their dispersion relations are consistent with the prediction from the cold plasma theory. In the initial growth stage (prediction from linear theory), the frequency of the dominant mode (the mode whose amplitude is large enough) of the whistler wave almost does not change, but in the saturation stage the situation is different. In the case that the ratio of electron plasma frequency to cyclotron frequency is larger than 1, the frequency of the dominant mode of the whistler wave driRs from high to low continuously. However, for the case of the ratio smaller than 1, besides the original dominant mode of the whistler wave whose frequency is about 2.6ωe, another dominant mode whose frequency is about 1.55ωe also begins to be excited at definite time, and its amplitude increases with time until it exceeds the original dominant mode. 相似文献
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移取小鼠血浆样品100μL于消解罐中,加入5mL硝酸与2mL 30%(质量分数)过氧化氢溶液进行微波密闭消解,冷却后,将样品溶液赶酸至少于0.5mL,用水定容至25mL,以73 Ge为内标,选用标准检测模式(STD)。硒的线性范围为0.2~20μg·L^(-1),检出限(3s)为6.75μg·L^(-1)。加标回收率在93.1%~105%之间,测定值的相对标准偏差(n=6)小于5.0%。利用本方法测定补硒小鼠血浆中的硒含量,可观察到硒含量随给药时间而变化。 相似文献
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Density and impurity profile behaviours in HL-2A tokamak with different gas fuelling methods 下载免费PDF全文
The electron density profile peaking and the impurity accumulation in the HL-2A tokamak plasma are observed when three kinds of fuelling methods are separately used at different fuelling particle locations.The density profile becomes more peaked when the line-averaged electron density approaches the Greenwald density limit n G and,consequently,impurity accumulation is often observed.A linear increase regime in the density range n e < 0.6n G and a saturation regime in n e > 0.6n G are obtained.There is no significant difference in achieved density peaking factor f ne between the supersonic molecular beam injection (SMBI) and gas puffing into the plasma main chamber.However,the achieved f ne is relatively low,in particular,in the case of density below 0.7n G,when the working gas is puffed into the divertor chamber.A discharge with a density as high as 1.2n G,i.e.n e=1.2n G,can be achieved by SMBI just after siliconization as a wall conditioning.The metallic impurities,such as iron and chromium,also increase remarkably when the impurity accumulation happens.The mechanism behind the density peaking and impurity accumulation is studied by investigating both the density peaking factor versus the effective collisionality and the radiation peaking versus density peaking. 相似文献
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