3.8-μm photometry during the secondary eclipse of the extrasolar planet HD 209458b     

Drake Deming †  L. Jeremy Richardson  Joseph Harrington 《Monthly notices of the Royal Astronomical Society》2007,378(1):148-152

We report infrared photometry of the extrasolar planet HD 209458b during the time of secondary eclipse (planet passing behind the star). Observations were acquired during two secondary eclipses at the NASA Infrared Telescope Facility (IRTF) in 2003 September. We used a circular variable filter (1.5 per cent bandpass) centred at 3.8 μm to isolate the predicted flux peak of the planet at this wavelength. Residual telluric absorption and instrument variations were removed by offsetting the telescope to nearby bright comparison stars at a high temporal cadence. Our results give a secondary eclipse depth of 0.0013 ± 0.0011, not yet sufficient precision to detect the eclipse, whose expected depth is  ∼0.002 –0.003  . We here elucidate the current observational limitations to this technique, and discuss the approach needed to achieve detections of hot Jupiter secondary eclipses at 3.8 μm from the ground.  相似文献   

多模式智能路灯控制系统     

张秀再  罗歆瑶  韦镇余  沈旭晖 《南京气象学院学报》2014,6(6):510-514

使用AT89S52单片机作为主控芯片,设计了一种多模式智能路灯控制系统,该系统能够根据道路、巷口或定时应用3种情况进行工作模式选择,并根据环境光亮度决定是否启动所设定的工作模式.巷口工作模式时,系统通过红外传感器检测道路上有汽车或行人通过时,将识别信号送入单片机,由单片机控制交通灯开启;道路工作模式时,路灯处于开启状态,以保障行人畅行;定时模式时,通过DS1302定时模块,可以设定路灯的开关时间.此外,该系统还具有自动故障检测功能,功能全面,有较强的实用价值.  相似文献   

华北区域冰雹天气分型及云系特征   总被引：2，自引：0，他引：2       下载免费PDF全文

蓝渝  郑永光  毛冬艳  林隐静  朱文剑  方翀 《应用气象学报》2014,25(5):538-549

基于地面加密观测资料、FY-2E静止气象卫星观测资料和NCEP分析资料,选取2010—2012年华北区域内27次冰雹过程,按大气环流背景、主要影响系统和云系的云型特征等将其分为冷涡云系尾部型、低涡槽前型和偏北气流控制型3种类型。分析结果表明:3种天气型下冰雹对流云系特征存在差异,但90%以上的冰雹过程发生在对流云团的快速发展阶段中,降雹集中出现于准圆形或椭圆形对流云团边缘或带状对流云系的传播前沿区域,对应于云顶亮温梯度的大值区。在掌握背景环境的前提下,综合分析红外图像中对流系统的发展演变、水汽图像暗带和暗区变化等信息,对冰雹的监测和预警有一定的参考价值。定量统计分析表明,大的亮温梯度值 (不低于8 ℃/0.05°) 是辅助判断冰雹能否发生的重要参量,而当冰雹云同时具备低云顶亮温和大亮温梯度的情况下,更有利于大于10 mm大冰雹的发生。  相似文献   

Estimation of the Land Surface Emissivity in the Hinterland of Taklimakan Desert   总被引：3，自引：2，他引：1  

LIU Yong-qiang  Ali MAMTIMIN  HUO Wen  YANG Xing-hua  LIU Xin-chun  MENG Xian-yong  HE Qing 《山地科学学报》2014,(6):1543-1551

An accurate accounting of land surface emissivity(ε) is important both for the retrieval of surface temperatures and the calculation of the longwave surface energy budgets.Since ε is one of the important parameterizations in land surface models(LSMs),accurate accounting also improves the accuracy of surface temperatures and sensible heat fluxes simulated by LSMs.In order to obtain an accurate emissivity,this paper focuses on estimating ε from data collected in the hinterland of Taklimakan Desert by two different methods.In the first method,ε was derived from the surface broadband emissivity in the 8–14 μm thermal infrared atmospheric window,which was determined from spectral radiances observed by field measurements using a portable Fourier transform infrared spectrometer,the mean ε being 0.9051.The second method compared the observed and calculated heat fluxes under nearneutral atmospheric stability and estimated ε indirectly by minimizing the root-mean-square difference between them.The result of the second method found a mean value of 0.9042,which is consistent with the result by the first method.Although the two methods recover ε from different field experiments and data,the difference of meanvalues is 0.0009.The first method is superior to the indirect method,and is also more convenient.  相似文献   

红外光谱和拉曼光谱在热处理海蓝宝石鉴定中的应用     

杨如增  杨松 《地质科学译丛》2014,(1):46-49

在适当的热处理条件下,黄绿色绿柱石能够转变为理想颜色的海蓝宝石。天然海蓝宝石与热处理海蓝宝石的价格差异较大,因此探索热处理海蓝宝石的诊断性鉴定特征就显得十分必要。对不同温度下热处理海蓝宝石进行傅里叶变换红外光谱和激光拉曼光谱的测试分析,结果发现,当热处理温度超过400℃后,随着加热温度的升高,在红外光谱中由[Fe2（OH）4]2＋伸缩振动gI起的3233cm叫处吸收谱峰明显减弱,直至消失。5268cm叫附近由水伸缩和弯曲振动}I起合频区的吸收带由尖峰变得宽缓;8700,6818cm叫两处水吸收峰的相对强度也随着加热温度升高而减弱。热处理海蓝宝石Si-0-Si伸缩振动产生的在682,3604cm叫处的拉曼光谱谱峰强度随着加热温度升高逐渐减弱,1070cm“处的拉曼峰强度明显降低。经700℃加热后,拉曼光谱基线明显向上方漂移。这些光谱特征变化对热处理海蓝宝石的鉴定有重要意义。  相似文献   

用相关分析法约简MCSs空间数据库     

方兆宝  林珲  吴立新  江吉喜 《地理科学进展》2004,23(3):27-33,i002,i003

长江流域出现致洪大暴雨与青藏高原上中尺度对流系统(MCSs)的东移密切相关。为了寻找MCSs移动和传播的规律,我们将MCSs的移动路径与其中心附近一定范围内的环境物理量场之间建立联系,构造出MCSs东移空间数据挖掘数据库。在这个数据库中,包含由9个环境物理量生成的18个属性项,除此,还包括由MCSs本身的空间特征量构成的5个属性项,即TBB强度、面积、地理位置、形状等,共计23个属性项。利用1998年6月至8月日本地球静止气象卫星(GMS)的青藏高原逐时红外遥感云图计算出的云顶黑体辐射温度(TBB)及青藏高原高分辨率有限区域数值分析预报值系统(HLAFS)环境场物理量数据,构造出上述空间数据挖掘数据库,运用空间相关分析技术对其进行约简,结果表明：在高度(H)、温度（T）、涡度(VOR)、散度(DIV)、水汽通量散度(IFVQ)、垂直速度(W）、假相当位温（θse)、K指数(K)、相对湿度(RH)等9个因素中,高度、涡度、散度、水汽通量散度、垂直速度及k指数6个因素相对独立;而温度(T)、假相当位温(θse)、相对湿度（RH)之间相关性较强,而且与高度等其它6个因素密切相关。根据数据库约简原则,可将温度（T）、假相当位温(θse)、相对湿度(RH)3个因素生成的6个属性项从数据库中删除,以便提高数据挖掘效率。  相似文献   

Noise reduction methods in the analysis of near infrared lunar occultation light curves for high angular resolution measurements     

Tapas Baug  Thyagarajan Chandrasekhar 《天文和天体物理学研究(英文版)》2013,(11):1363-1380

A lunar occultation （LO） technique in the near-infrared （NIR） provides angular resolution down to milliarcseconds for an occulted source, even with ground- based 1 m class telescopes. LO observations are limited to brighter objects because they require a high signal-to-noise ratio （S/N ~40） for proper extraction of angular diameter values. Hence, methods to improve the S/N ratio by reducing noise using Fourier and wavelet transforms have been explored in this study. A sample of 54 NIR LO light curves observed with the IR camera at Mt Abu Observatory has been used. It is seen that both Fourier and wavelet methods have shown an improvement in S/N compared to the original data. However, the application of wavelet transforms causes a slight smoothing of the fringes and results in a higher value for angular diameter. Fourier transforms which reduce discrete noise frequencies do not distort the fringe. The Fourier transform method seems to be effective in improving the S/N, as well as improving the model fit, particularly in the fainter regime of our sample. These methods also provide a better model fit for brighter sources in some cases, though there may not be a significant imorovement in S/N.  相似文献   

WFCAM, Spitzer/IRAC and SCUBA observations of the massive star-forming region DR21/W75 – I. The collimated molecular jets     

C. J. Davis  M. S. N. Kumar  G. Sandell  D. Froebrich  M. D. Smith  M. J. Currie 《Monthly notices of the Royal Astronomical Society》2007,374(1):29-53

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恒星脉泽源的IRAS观测结果和分析     

陈培生  高衡  鲍梦贤 《中国天文和天体物理学报》1991,(3)

本文利用红外天文卫星(IRAS)点源表(PSC)及低分辨率光谱表(LRS)的资料,较为系统地讨论了各种恒星脉泽源在中远红外颜色及光谱的特征,并结合其空间分布,物理性质和演化状态探讨了产生这些特征的原因。  相似文献   

The nature of the molecular gas system in the core of NGC 1275     

R. J. Wilman  A. C. Edge  R. M. Johnstone 《Monthly notices of the Royal Astronomical Society》2005,359(2):755-764

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