基于模糊自整定PID的直升机飞行控制律设计

在经典PID控制律基础上,引入模糊控制的概念设计模糊自整定PID控制律改进无人直升机姿态回路控制器,实现了PID控制器的参数在线自整定,并改善了控制器性能.通过Matlab对闭环系统进行算法仿真,表明模糊自整定PID控制器能够发挥优于传统PID控制器的控制性能.最后对所设计的控制器进行半物理仿真验证,通过对比典型输入指令下经典PID和模糊自整定PID两种控制器的控制效果,验证了模糊自整定PID对系统性能的优化.     

长江三峡水坝下游河道悬沙恢复和床沙补给机制

流域水库工程的修建,将改变坝下游原有的水沙输移过程,三峡水库蓄水作用对坝下游水沙输移的影响已初步显现。具体表现为：① 三峡水库坝下游洪水持续时间和流量被削减,下泄沙量大幅减少,沿程上输沙量虽得到一定恢复,但总量仍未超过蓄水前多年均值;② 2003-2014年d > 0.125 mm（粗）输沙量得到一定恢复,至监利站恢复程度最大,基本达到蓄水前均值,在恢复后其下游该组分泥沙冲淤特性与蓄水前一致,其中2008-2014年恢复程度弱于2003-2007年;③ 三峡水库蓄水后坝下游d < 0.125 mm（细）输沙量沿程上得到一定程度恢复,但总量仍小于蓄水前均值;④ 三峡水库蓄水后坝下游d > 0.125 mm泥沙输移量因河床补给作用,沿程上得到恢复,但补给量将不超过0.44亿t/y,主要受制于洪水持续时间及流量均值,而上游干流、河段间支流和湖泊分汇作用占次要地位,而d < 0.125 mm悬沙恢复受上游干流、区间支流和湖泊分汇及河床补给控制,因河床粗化使得床沙对细颗粒悬沙的补给作用减弱;⑤ 2003-2007年和2008-2014年两时段间宜昌至枝城、上荆江为粗细均冲,下荆江为淤粗冲细,汉口至大通河段为淤粗冲细,城陵矶至汉口河段2003-2007年为淤粗冲细,2008-2014年为粗细均冲,这一差异受控于螺山站洪水流量持续时间和量值。     

Solar Stokes Spectrum Observation at Yunnan Astronomical Observatory

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The effect of angle-dependent non-coherent electron scattering and partial redistribution on the polarization of resonance lines

The polarized radiative transfer equation is solved when angle-dependent partial redistribution and non-coherent electron scattering are included as line-scattering mechanisms. A static atmosphere with plane parallel symmetry is assumed. Test calculations are used to illustrate the effects of the electron-scattering coefficient, the thermalization parameter and the continuous absorption coefficient on the line polarization. Results of angle-averaged and angle-dependent redistribution functions are compared and it is shown that angle-dependent functions should be used to model the wing polarization of optically thin lines. The lower the continuous absorption compared with the electron scattering, the higher the wing polarization.     

An irradiation effect in Nova DN Gem 1912 and the significance of the period gap for classical novae

Continuous CCD photometry of the classical nova DN Gem during 52 nights in the years 1992–1998 reveals a modulation with a period of 0.127844 d. The semi-amplitude is about 0.03 mag. The stability of the variation suggests that it is the orbital period of the binary system. This interpretation makes DN Gem the fourth nova inside the cataclysmic variable (CV) period gap, as defined by Diaz & Bruch, and it bolsters the idea that there is no period gap for classical novae. However, the number of known nova periods is still too small to establish this idea statistically. We eliminate several possible mechanisms for the variation, and propose that the modulation is driven by an irradiation effect. We find that model light curves of an irradiated secondary star fit the data well. The inclination angle of the system is restricted by this model to 10°≲ i ≲65°. We also refine a previous estimate of the distance to the binary system, and find d =1.6±0.6 kpc.     

陆面面积平均通量的参数化问

目前,气候和大气边界层物理研究中一个十分重要的研究方向就是面积平均通量的参数化问题。本文对这一研究方向中存在的问题、可能的解决方法和目前的研究进展情况进行了阐述,简要介绍了非均匀陆面影响的高度及其尺度划分,阐述了混合高度、参考层高度（观测高度和模式第一层高度）、近地层高度、内边界层高度、平衡层高度、粗糙度副层和边界层高度等之间的关系及其在非均匀尺度划分中的作用,并且阐述了整体输送公式在不同尺度的非均匀陆面中存在的问题及相应的可能解决办法。同时还对中尺度的非均匀陆面驱动的一类非经典中尺度环流的参数化,即中尺度通量的参数化问题进行了评述。最后针对内蒙古草原实验和青藏高原实验等具体问题,提出了边界层观测和非均匀陆面参数化方法的几点问题。     

Correction of atmospheric effect on ADEOS/OCTS ocean color data: Algorithm description and evaluation of its performance

This paper first describes the atmospheric correction algorithm for OCTS visible band data used at NASDA/EOC. Sharing a basic structure with Gordon and Wang’s Sea WiFS algorithm, it uses 10 candidate aerosol models including the “Asian dust model” introduced in consideration of the unique feature of aerosols over the east Asian waters. Based on the observations at 670 and 865 nm bands, the algorithm selects a pair of aerosol models that account best for the observed spectral reflectances, and synthesizes the aerosol reflectance used for the atmospheric correction. Two different schemes for determining the value of the parameter for the aerosol model selection are presented and their anticipated estimation error is analyzed in terms of retrieved water reflectance at 443 nm. The results of our numerical simulation show that the standard deviation of the estimation error of the “weighted average” scheme is mostly within the permissible level of ±0.002, reducing the error by 18% on average compared to the “simple average” scheme. The paper further discusses the expected error under the old CZCS-type atmospheric correction, which assumes constant aerosol optical properties throughout the given image. Although our algorithm has a better performance than the CZCS algorithm, further analysis shows that the error induced by the assumption taken in the algorithm that the water-leaving radiance at 670 nm band is negligibly small may be large in high pigment concentration waters, indicating the necessity for future improvements.