EVALUATION OF MODELS FOR ESTIMATION OF NET RADIATION FOR ALPINE SLOPING SURFACES          下载免费PDF全文

Huo Zonghui  W. G. Bailey 《Acta Meteorologica Sinica》1992,6(2):189-197

This paper describes and tests two models for estimating net radiation(or the radiation balance)on sloping surfacesof alpine environments.They are an empirical method based on the linear relationship between net radiation and globalsolar radiation and a flux-by-flux method involving the estimation of all the individual components of radiation budgetindependently.The results show that the empirical method is capable of predicting hourly net radiation on sloping sur-faces to within about±53 W m~(-2) under all sky conditions.During clear sky conditions,it could predict net radiation onslopes to within±58 W m~(-2) or 16% of the measured values.The flux-by-flux method,although it did not perform aswell as the empirical method,performed adequately and could give estimates of net radiation on slopes with root meansquare error of less than 74 W m~(-2)(20%)and a mean bias error of 27 W m~(-2)(7%).  相似文献   

关于总辐射与地表净辐射的相关性问题   总被引：1，自引：1，他引：1  

翁笃鸣  高庆先 《南京气象学院学报》1992,15(4):500-507

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火山气溶胶的辐射影响   总被引：2，自引：1，他引：2  

汪宏七  赵高祥 《大气科学》1992,16(6):755-760

本文应用辐射传输计算研究了火山气溶胶,特别是大的火山爆发后短时期及火山周围地区内的火山气溶胶,对到达地面的向下的总的太阳辐射通量、行星反照率及大气加热率的可能影响.  相似文献   

我国日照时数和总辐射的空间分布场     

文传甲 《山地学报》1992,(4)

运用多项式回归分析和双随机样本检验,模拟日照时数和总辐射及其影响因子(可照时间、总云量和天文辐射、日照百分率)年值和1月值、7月值的三度空间分布场,取得了满意结果。这可应用在无测站地区,仅凭经纬度和海拔估算出上述气候要素值,估算的平均相对误差大多在5％以下(最好的达0.3‰)。  相似文献   

辐射传输模式中地表参数对大气长波辐射的影响   总被引：2，自引：0，他引：2       下载免费PDF全文

王可丽  钟强 《大气科学》1995,19(5):606-614

本文利用Liou-Ou一维宽带辐射传输模式，对地表热力参数取值部分作了改进，使用模式大气和青藏高原实测资料对下垫面温度与地表空气温度两者不能合二为一的问题进行了分析，同时还讨论了下垫面温度的日变化对大气长波辐射通量日变化的影响及地表比辐射率的变化对大气长波辐射通量计算结果的修正作用。  相似文献   

中国地－气系统净辐射的气候特征     

翁笃鸣  李炬 《南京气象学院学报》1995,(2)

根据ＥＲＢＥ和ＩＳＣＣＰ资料讨论了总云量等因子对地－气系统净辐射的影响，分析了地－气系统净辐射与其各分量及地表净辐射的相关联系。发现行星反射率和地气短波吸收辐射对地－气净辐射的影响最大，而云和纬度的作用主要通过该两因子变化表现出来，ＯＬＲ的作用则相对较弱。地－气净辐射与地表净辐射的相关性也较明显。文中还就地－气净辐射在全国的地理分布作了分析。各地区地－气净辐射的年变曲线均为简单的夏大冬小型，云等因素的影响主要造成最大值出现月份的推移。  相似文献   

日本地震电磁辐射研究的进展与动向   总被引：3，自引：0，他引：3  

钱书清 《国际地震动态》1993,(6):6-9

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The remote sensing observation in experiments of rock failure and the beginning of remote sensing rock mechanics     

Nai-Guang Geng  Cheng-Yu Cui  Ming-De Deng 《地震学报(英文版)》1993,6(4):971-980

The remote sensing observational study for infrared radiation of rocks was proceeded during the loading on rocks until failure. The major instruments used in experiments were transient spectrum apparatus, intelligent spectrum apparatus, infrared radiation thermometer, infrared spectrum radiometer, and infrared thermal imaging system. The experiments for 26 kinds of rocks were made. The studies show that infrared radiation temperature of rocks increases along with increasing of stress. The amplitude of infrared radiation spectrum of rocks also increases along with increasing of stress. The observational results of infrared thermal imaging of rocks are consistent with infrared radiation temperature. Before formation of major faults for some rocks, the belt-shape thermal imaging of temperature anomaly displaies in position of future major faults. This study has led the new technology of remote sensing into rock mechanics and tend to establish a new field in rock mechanics — remote sensing rock mechanics (or remote sensing rock physics). The application of remote sensing rock mechanics in prediction of earthquake and rock burst, and in measurement of stress field in rock mass is expected. The Chinese version of this paper appeared in the Chinese edition ofActa Seismologica Sinica,14, Supp., 645–652, 1992. Jin-Shen HAO, Ji-Han LI, Xiao-Hong LIU, Yi-Qiao ZHI, Jin-Kai ZHANG, Yong-Hong Lü, Yi LIU, Yun-Shen YU, He ZHANG, Quan-Quan JI, Xiao-Fan ZHU and Ning CHEN took part in this work. This subject is supported by the Chinese Joint Seismological Science Foundation (91006). Work of Institute of Geophysics, SSB (93A0009).  相似文献   

活动星系核与类星体中致密天体的形成与并合：伽玛爆发与引力辐射     

王建民 《紫金山天文台台刊》1999,18(3):271-273

频繁的超新星爆发可用以解释活动星系核与类星体的超高金属丰度。星团中的恒星与吸积盘相互作用导致致密天体中子星和黑洞的形成率很高,这些致密天体与红巨星很容易形成双星系统,而后形成（ＮＳ／ＢＨ,ＮＳ／ＢＨ） 双星由于引力辐射最终导致并合而形成伽玛射线爆发。我们估计了伽玛射线爆的爆发频率,发现与观测相符。  相似文献   

太阳射电三频率高时间分辨率三年同步观测的结果     

谢瑞祥  汪敏  陈国强  汪从云 《中国天文和天体物理学报》1993,(1)

本文总结了1987年2月到1989年12月三波段(1.42GHz、2.84GHz和4.0GHz)高时间分辨率同步观测的资料,介绍了各波段尖峰辐射出现的频次、持续时间以及与射电爆发、光学耀斑和X射线爆的统计关系.  相似文献