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References: 《极地研究(英文版)》2007,18(1):54-62
Chinese meteorological satellite FY-1D can obtain global data from four spectral channels which include visible channel(0.58-0.68 μm) and infrared channels(0.84-0.89 μm,10.3-11.3 μm,11.5-12.5 μm).2366 snow and ice samples,2024 cloud samples,1602 land samples and 1648 water samples were selected randomly from Arctic imageries.Land and water can be detected by spectral features.Snow-ice and cloud can be classified by textural features.The classifier is Bayes classifier.By synthesizing five d ays classifying result of Arctic snow and ice cover area,complete Arctic snow and ice cover area can be obtained.The result agrees with NOAA/NESDIS IMS products up to 70%. 相似文献
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Josef Gochermann Walter F. Wargau Claus Tappert Theodor Schmidt-Kaler Robert S. Stobie Fred Marang Greg Roberts Francois G. van Wyk Peter Rucks 《Experimental Astronomy》1999,9(1):1-15
In order to decide whether the seeing conditions at SAAO/Sutherland justify the erection of a 3.5 m telescope and also to compare Sutherland with the Gamsberg/Namibia site, a seeing campaign covering 15 months has been carried out. For direct comparison with the results of the seeing campaign at Gamsberg twenty years before the same QUESTAR telescope was employed. The seeing is determined by the scattering of the star-trail exposed on a film in the focal plane of the telescope. The campaign commenced in February 1992. Up to May 1993, data for 204 nights, that is 47.3% of the total number of nights, were collected. Due to wind speeds above 30 km h-1, 25 out of the 204 nights were not considered in the final reduction. The useful 179 nights are evenly distributed over the campaign period. The median seeing value for the whole period is = 0.52. There are differences during the year: the best season gives = 0.42, the worst = 0.67. Each night was divided into three intervals, although data for each of the three intervals were not always available. Generally, there is an improvement in the seeing during the course of a night. The results are compared to the seeing values of Gamsberg/Namibia and ESO/La Silla. 相似文献
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V. K. Dubrovich 《Astronomy Letters》2003,29(1):6-9
We consider the image formation for an extremely distant source in an optically dense, homogeneous, and isotropic medium. We show that the angular size of the image would presently be θ0 ≈ 10′, irrespective of the initial redshift z. Parameters of the inhomogeneities capable of producing the observed effect were estimated. We note that this effect should be taken into account for the baryon density fluctuations that were damped according to Silk at the prerecombination epoch. The spot radiation spectrum is shown to be a diluted Planckian spectrum with a dilution factor much larger than unity. We also point out the presence of peculiar tangential polarization in the spot, which reaches several tens of percent at the spot edge. All these observational features clearly distinguish the fluctuations under consideration from the standard fluctuations. 相似文献
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【目的】探讨和实践基于多源数据融合的山地实况业务体系建设,以提高山地地区的监测、预警和灾害应对能力。【方法】通过分析山地地区面临的地理环境、气象条件以及自然灾害的特点,以及基于对已有实况业务发展的现状分析,建设全面、精准、实时的山地实况业务体系。【结果】明确贵州省实况产品建设方向并介绍了在山地实况业务体系建设中的技术路线,包括数据采集、传输、处理、展示、全流程监控等关键步骤,以及各环节的技术创新和方法改进。最后分析了面向重大服务、重点行业、重要区域开展有针对性的实况产品服务时仍需重点解决的问题。【结论】该文的研究成果为山地区域的实况业务体系建设提供了思路和方法,对于提升山地区域的灾害管理水平具有实际应用价值。 相似文献
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CR 21气象仪的SC 1串行接口与标准的RS 232接口并不兼容,难以并入滑坡遥测系统。对此特研制CS-1型串行接口转换器。它能使SC 1串行接口电平与标准的RS 232接口电平彼此转换。由此在微型计算机专用软件支持下,CR 21气象仪便能自动而又准确地向滑坡遥测系统传输数据。 相似文献