基于LabVIEW的车灯日行灯自动化测试

设计了一种汽车日行灯自动测试系统。该系统主要由工业计算机、高性能数字摄像机硬件平台和LabVIEW软件平台两部分构成。采用摄像机拍摄一张标准日行灯图片作为模板,对待测试的日行灯进行图像采集且与模板比较。由模板定位出测试窗口,然后对各个窗口进行RGB模型分析和HSL模型分析,从而完成对日行灯颜色和明度的检测。此外,系统可同时对多个窗口进行分析,并可实时显示测试画面和测试结果,一次测试时间不超过6 s,且准确度和重复性较好,已在实际中应用。     

云层对近红外白天测星的影响

大气层内白天测星最大的困难是过强的天空背景辐射,白天近红外波段可以探测到足够多的星体用以导航。目前已有研究针对理想情况下的白天恒星探测进行了分析,然而,对于实际情况来说,天空背景很难像理想分析中那样无风无雨无云,尤其是云层自身的热辐射及散射的太阳辐射对近红外白天恒星探测造成极大的影响;根据经验公式,对云层和太阳的红外辐射进行计算,分析了白天云层对恒星探测的影响,并以层云和积云为例,具体分析了恒星辐射透过云层的衰减,对实际工作具有一定的指导意义。     

Daytime observation technology of a lidar using an atomic filter

Based on the dual-wavelength high altitude detecting lidar we developed, daytime observation capability was realized in its sodium fluorescence channel by employing a Na (sodium) atomic filter and other relevant technologies. Because of the very narrow passband and very high out-of-band suppression of the Na atomic filter, the lidar echo at an 80-110 km altitude can be obtained even at noontime when background light from the sun is very strong. The capability for a 24-h continuous observation of the lidar system has been demonstrated by the preliminary observation result. This development makes the constant detection and investigation of high altitude atmosphere over the country possible.     

Loneliness impairs daytime functioning but not sleep duration.

Objective: To assess the prospective association between daily feelings of loneliness and subsequent feelings of daytime dysfunction indicative of poor sleep quality. Design: Three consecutive end-of-day diaries were completed by a population-based sample of 215 adults (mean age = 57.5 years, SD = 4.4). Diary questions probed sleep duration, daytime dysfunction (i.e., fatigue, low energy, sleepiness), loneliness, physical symptoms, and depressed affect experienced that day. Chronic health condition data and body mass index were also obtained. Autoregressive cross-lagged panel models were used to examine the magnitude of reciprocal prospective associations between loneliness and daytime dysfunction. Main Outcome Measures: Unstandardized path coefficients adjusted for race/ethnicity, sleep duration, marital status, household income, chronic health conditions, and health symptom severity. Results: Daily variations in loneliness predicted subsequent feelings of daytime dysfunction (B = 0.16, p     

数字摄像法测量白天能见度算法设计

数字摄像法测量白天大气能见度,常用的方法是双亮度差法,此方法需尽可能保证标准的观测条件,例如两组目标-背景视线方向一致,尽量选择观测反射率低得可以忽略的人工实用黑体目标物等,否则会产生较大的误差。为此设计了一种新的基于数字摄像机的白天能见度算法:拍摄包含合适的目标物和天空背景图像,通过暗原色先验估计透射率,通过调节光圈大小获得散焦图像,把S变换应用到图像处理中,计算视觉距离,可以得出大气消光系数,从而反演出大气能见度值。实验数据表明,该算法在能见度的值在4 000~8 000 m范围内最大误差小于9%,测量结果比双亮度差方法误差减小2.1%~3.4%。     

基于SUSAN算子的白天红外星目标检测

受多种因素的影响,白天获得的红外星图像信噪比低,且背景通常是不均匀的,为红外星目标的提取造成了极大的困难。通过理论计算,实际白天拍摄的近红外星图信噪比极低,使用一般的滤波方法无法提取出恒星目标,目前常用的形态学方法对于星图像的处理也不甚理想。首先分析背景特性,采用多帧叠加的方法削弱随机噪声,增大信噪比;然后设定阈值对叠加后的星图进行背景消除,得到只含有目标及噪声的图像;最后基于图像的特性,使用改进的SUSAN算子对星图进行目标检测,进而分割出目标,实验证明,与传统方法相比,该方法可较好地分离出恒星目标。     

利用视频判读进行白天测星方法的研究

针对测量船光测设备的电视测量系统白天测星能力的不足,提出了一种新型的白天测星方法.该方法将光测设备测星的视频图像实时记录于计算机的硬盘,并根据判读存储于硬盘中星体图像的脱靶量,完成测量船的航向修正和动态标校.应用这种方法,可以提高光测设备白天测星的能力及测量船的总体测量精度,是一种准实时的、切实可行的白天测星方法.     

大气成分对中波红外地基光电系统观测的影响分析

地基光电系统白天在可见光波段对空间目标观测时,因受大气散射等因素的影响,探测能力会急剧下降。红外波段较可见光波段具有较强的大气穿透能力,因此在红外波段观测空间目标可以较好地解决白天探测的问题。利用MODTRAN模型计算了不同大气成分对中波红外透射率的影响并进行了分析,并用中波红外成像系统在地基望远镜上进行了观测。实验结果表明,中波红外探测器在白天能极限探测到7等星,平均信噪比为6.236。本研究对白天红外波段地基的空间探测具有一定参考意义。