Thermoluminescence, electron paramagnetic resonance and optical absorption in natural and synthetic rhodonite crystals     

J. R. B. Paião  S. Watanabe 《Physics and Chemistry of Minerals》2008,35(9):535-544

Thermoluminescence, electron paramagnetic resonance and optical absorption properties of rhodonite, a natural silicate mineral, have been investigated and compared to those of synthetic crystal, pure and doped. The TL peaks grow linearly for radiation dose up to 4 kGy, and then saturate. In all the synthetic samples, 140 and 340°C TL peaks are observed; the difference occurs in their relative intensities, but only 340°C peak grows strongly for high doses. Al₂O₃ and Al₂O₃ + CaO-doped synthetic samples presented several decades intenser TL compared to that of synthetic samples doped with other impurities. A heating rate of 4°C/s has been used in all the TL readings. The EPR spectrum of natural rhodonite mineral has only one huge signal around g = 2.0 with width extending from 1,000 to 6,000 G. This is due to Mn dipolar interaction, a fact proved by numerical calculation based on Van Vleck dipolar broadening expression. The optical absorption spectrum is rich in absorption bands in near-UV, visible and near-IR intervals. Several bands in the region from 540 to 340 nm are interpreted as being due to Mn³⁺ in distorted octahedral environment. A broad and intense band around 1,040 nm is due to Fe²⁺. It decays under heating up to 900°C. At this temperature it is reduced by 80% of its original intensity. The pink, natural rhodonite, heated in air starts becoming black at approximately 600°C.  相似文献   

利用NOAA卫星资料估算陆地沙尘量的方法   总被引：1，自引：0，他引：1  

郑新江  陈渭民  方翔  罗敬宁 《国土资源遥感》2008,(2):35-39

提出一种利用NOAA卫星可见光通道估算北方干旱陆地上空沙尘含量的方法。该方法考虑到在短时间内某一固定区域的地面反射率变化较小,因此可以利用沙尘暴发生和晴空2个不同时刻卫星测量到的这一像素区的辐射值来消除地面反射率的影响,估算陆地上空沙尘暴的光学厚度。在2002年4月6日左右沙尘暴发生期间,利用该方法计算的沙尘光学厚度与载沙量的结果和同步观测的TSP值与地面气象数据在趋势与分布上是一致的。  相似文献   

Considering combined or separated roughness and vegetation effects in soil moisture retrievals     

《International Journal of Applied Earth Observation and Geoinformation》2017

For more than six years, the Soil Moisture and Ocean Salinity (SMOS) mission has provided multi angular and full-polarization brightness temperature (TB) measurements at L-band. Geophysical products such as soil moisture (SM) and vegetation optical depth at nadir (τ_nad) are retrieved by an operational algorithm using TB observations at different angles of incidence and polarizations. However, the quality of the retrievals depends on several surface effects, such as vegetation, soil roughness and texture, etc. In the microwave forward emission model used in the retrievals (L-band Microwave Emission Model, L-MEB), soil roughness is modelled with a semi-empirical equation using four main parameters (Q_r, H_r, N_rp, with p = H or V polarizations). At present, these parameters are calibrated with data provided by airborne studies and in situ measurements made at a local scale that is not necessarily representative of the large SMOS footprints (43 km on average) at global scale. In this study, we evaluate the impact of the calibrated values of N_rp and H_r on the SM and τ_nad retrievals based on SMOS TB measurements (SMOS Level 3 product) over the Soil Climate Analysis Network (SCAN) network located in North America over five years (2011–2015). In this study, Q_r was set equal to zero and we assumed that N_rH = N_rV. The retrievals were performed by varying N_rp from −1 to 2 by steps of 1 and H_r from 0 to 0.6 by steps of 0.1. At satellite scale, the results show that combining vegetation and roughness effects in a single parameter provides the best results in terms of soil moisture retrievals, as evaluated against the in situ SM data. Even though our retrieval approach was very simplified, as we did not account for pixel heterogeneity, the accuracy we obtained in the SM retrievals was almost systematically better than those of the Level 3 product. Improved results were also obtained in terms of optical depth retrievals. These new results may have key consequences in terms of calibration of roughness effects within the algorithms of the SMOS (ESA) and the SMAP (NASA) space missions.  相似文献   

Forecast of wheat yield throughout the agricultural season using optical and radar satellite images     

《International Journal of Applied Earth Observation and Geoinformation》2017

The aim of this study is to estimate the capabilities of forecasting the yield of wheat using an artificial neural network combined with multi-temporal satellite data acquired at high spatial resolution throughout the agricultural season in the optical and/or microwave domains. Reflectance (acquired by Formosat-2, and Spot 4–5 in the green, red, and near infrared wavelength) and multi-configuration backscattering coefficients (acquired by TerraSAR-X and Radarsat-2 in the X- and C-bands, at co- (abbreviated HH and VV) and cross-polarization states (abbreviated HV and VH)) constitute the input variable of the artificial neural networks, which are trained and validated on the successively acquired images, providing yield forecast in near real-time conditions. The study is based on data collected over 32 fields of wheat distributed over a study area located in southwestern France, near Toulouse. Among the tested sensor configurations, several satellite data appear useful for the yield forecasting throughout the agricultural season (showing coefficient of determination (R²) larger than 0.60 and a root mean square error (RMSE) lower than 9.1 quintals by hectare (q ha⁻¹)): C_VH, C_HV, or the combined used of X_HH and C_HH, C_HH and C_HV, or green reflectance and C_HH. Nevertheless, the best accurate forecast (R² = 0.76 and RMSE = 7.0 q ha⁻¹) is obtained longtime before the harvest (on day 98, during the elongation of stems) using the combination of co- and cross-polarized backscattering coefficients acquired in the C-band (C_VV and C_VH). These results highlight the high interest of using synthetic aperture radar (SAR) data instead of optical ones to early forecast the yield before the harvest of wheat.  相似文献   

查找表方法确定气溶胶类型   总被引：2，自引：0，他引：2  

贾臣  孙林  陈允芳  吕喆鹏  韦晶  于会泳  田信鹏 《遥感学报》2017,21(3):386-395

针对传统气溶胶类型确定方法的局限性以及当前气溶胶类型确定存在的困难,提出一种使用多波段气溶胶光学厚度数据确定气溶胶类型的方法。基于大气颗粒物的散射与吸收特性分析,通过构建查找表的方法实现气溶胶类型的确定。该方法利用Mie散射理论通过正向模拟不同类型气溶胶粒子数量与多波段光学厚度之间的关系来构建查找表,基于该查找表,使用440 nm、670 nm、870 nm及1020 nm 4个波段的气溶胶光学厚度确定气溶胶类型。使用模拟的多波段气溶胶光学厚度数据开展了气溶胶类型的确定实验,分析了不同波段气溶胶光学厚度误差对气溶胶类型确定结果的影响。结果表明,该方法可根据4个波段的气溶胶光学厚度以较高的精度确定出沙尘性、水溶性和煤烟3种气溶胶粒子的数量,从而确定气溶胶类型。  相似文献   

从空间探测闪电的综述   总被引：10，自引：0，他引：10  

陈洪滨  吕达仁 《气象学报》2001,59(3):377-383

从空间探测闪电 30多年的历史看 ,一些卫星闪电遥感仪器已提供了许多极有价值的资料 ,例如 ,闪电全球范围内发生的频率 ,其随纬度和季节的变化以及日变化 ,超级闪电的发生等等。这些资料在雷电灾害预警预防、强对流天气监测、某些军事目标的识别等业务和科研工作中得到了应用。本文是关于空间探测闪电的一个综述 ,主要介绍过去 35a一些星载闪电光学探测器 ,并给出由这些仪器观测资料分析所得到的一些重要结果。最后 ,对发展中国星载闪电探测器提出几点建议。  相似文献   

贺兰山地区大气气溶胶光学特征研究   总被引：24，自引：9，他引：24  

牛生杰  孙继明 《高原气象》2001,20(3):298-301

利用M－120型太阳光度表的观测资料并结合有关资料，分析了贺兰山地区大气气溶胶的光学特征，并对在各类天气条件下，大气气溶胶光学厚度以及Angstrom浑浊度系数和波长指数的变化规律进行了讨论。利用实测地面大气气溶胶粒子谱资料，探讨了大气气溶胶粒子数浓度与Angstrom浑浊系数β之间的关系以及大气气溶胶粒子几可平均尺度与波长指数α之间的相关关系。  相似文献   

A note on Earth's rotation angular velocity in the general-relativity framework     

V. A. Brumberg  E. Groten 《Journal of Geodesy》2001,75(12):673-676

 The value of the Earth's rotational angular velocity determined from observations is given in the GCRS (geocentric celestial reference system) defined by Resolution B1 of the 2000 IAU General Assembly. The same quantity derived from dynamical theories of the Earth's rotation, such as SMART97, is referred to the␣DGRSC (dynamically non-rotating ecliptical reference system). The relativistic theory of reference systems (RSs) enables unambiguous general-relativity relations between these quantities to be derived. Received: 9 November 2000 / Accepted: 9 July 2001  相似文献   

本世纪初我国大陆7级大震危险性研究     

李海华  沈繁銮  吴德珍  袁锡文  王正尚 《华南地震》2001,21(2):1-8

地震大形势研究结果表明，我国大陆地区（含边境）１９９９年已进入为期１２年的相对平静幕，幕内可能发生３次７级地震，最大震级不超过７．２级。首发７级地震为２０００年６月８日缅甸７级（位于中缅边境）。预计第二个７级地震危险时间在２００５±０．５年。第三个在２００８年前后。分析了我国主要地震区强震概率增益，给出了３个危险地点。未来３年即２００１～２００３年是相对安全时段，我国大陆不会发生７级以上破坏性地震。２０１１～２０２０年可能进入新世纪第一个７级大地震相对活跃幕，预计该幕持续１０年， 可发生１０次７～７.６级大震。  相似文献   

n维广义Radon变换     

李远钦  刘雯林 《地球物理学进展》1997,12(4):59-66

本文提出了一种在任意变换曲线族情况下的广义Ｒａｄｏｎ变换及反投影公式，研究了在何种变换曲线情况下，其反变换能唯一恢复原出数。事实上，并非任意变换曲线簇作广义Ｒａｄｏｎ变换都能由象函数唯一恢复原出数，同时探讨了广义Ｒａｄｏｎ变换比常规Ｒａｄｏｎ变换地震数据处理中具有更广泛的应用。  相似文献