内陆水体叶绿素a浓度反演的区域化三波段模型研究

以太湖和石头口门水库为例,建立了一种可直接计算水体叶绿素a浓度的区域化三波段模型。该模型通过对研究水体的光学特性分析,明确三波段组合与叶绿素a浓度间的函数关系参数,不仅可较好指示研究水体叶绿素a浓度水平,而且大大减小了回归算法所带来的模型不确定性。利用高精度、长时间序列的水体光学特性观测数据,建立针对不同研究水体的区域化三波段模型可为实现内陆水体叶绿素a浓度遥感监测业务化运行提供方法借鉴。     

Correction of the ionospheric distortion on the MARSIS surface sounding echoes

Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) on the Mars Express (MEX) spacecraft has made numerous measurements of the Martian surface and subsurface. However, all of these measurements are distorted by the ionosphere and must be compensated before any analysis. We have developed a technique to compensate for the ionospheric distortions. This technique provides a powerful tool to derive the total electron content (TEC) and other higher-order terms of the limited expansion of the plasma dispersion function that are related to overall shape of the electron column profile. The derived parameters are fitted by using a Chapman model to derive ionospheric parameters like n₀, electron density primary peak (maximum for solar zenith angle (SZA) equal 0), and the neutral height scale H.

Our estimated ionospheric parameters are in good agreement with Mars Global Surveyor (MGS) radio-occultation data. However, since MARSIS does not have the observation geometry limitations of the radio occultation measurements, our derived parameters extend over a large range of SZA for each MEX orbit.

The first results from our technique have been discussed by Safaeinili et al. [2007, Estimation of the total electron content of the Martian ionosphere using radar sounder surface echoes. Geophys. Res. Lett. 34, L23204, doi:10.1029/2007GL032154].     

Cosmic dynamics in the era of Extremely Large Telescopes

The redshifts of all cosmologically distant sources are expected to experience a small, systematic drift as a function of time due to the evolution of the Universe's expansion rate. A measurement of this effect would represent a direct and entirely model-independent determination of the expansion history of the Universe over a redshift range that is inaccessible to other methods. Here we investigate the impact of the next generation of Extremely Large Telescopes on the feasibility of detecting and characterizing the cosmological redshift drift. We consider the Lyα forest in the redshift range  2 < z < 5  and other absorption lines in the spectra of high-redshift QSOs as the most suitable targets for a redshift drift experiment. Assuming photon-noise-limited observations and using extensive Monte Carlo simulations we determine the accuracy to which the redshift drift can be measured from the Lyα forest as a function of signal-to-noise ratio and redshift. Based on this relation and using the brightness and redshift distributions of known QSOs we find that a 42-m telescope is capable of unambiguously detecting the redshift drift over a period of ∼20 yr using 4000 h of observing time. Such an experiment would provide independent evidence for the existence of dark energy without assuming spatial flatness, using any other cosmological constraints or making any other astrophysical assumption.     

光纤时间传输及相位补偿

介绍了国外几种利用光纤进行时间频率传递的方法和经验.对无补偿光纤时间频率传递方法、双向时间频率传递方法、光学机械温度补偿方法及电子共轭相位补偿方法作了较详细的描述.光纤时延主要随温度而变化,在200 km以内,时延的日变化为几纳秒,月变化为十几纳秒.在50 km内利用光纤传输100 MHz频率信号时,在不补偿情况下频率稳定度为: 3×10-14/s,1×10-15/d;光学补偿后的频率稳定度可达到1.5×10-14/s,1×10-17/d.电子共轭相位补偿后,温度变化20℃引起的相位变化降低了45倍.光纤传输对短期频率稳定度影响较小,对日及更长期的频率稳定度影响较大.     

Investigation of the linear polarization in infrared absorption bands

We consider the effects of the grain size, shape, structure, and chemical composition as well as the angle between the grain rotation axis and the incident ray on the full widths at half maximum (FWHM) of the polarization bands in the two deepest infrared absorption bands observed in the spectra of protostars, the water-ice band centered at 3.1 μm and the silicate band centered at 9.7 μm, using a core—mantle confocal spheroid model with various axial ratios a/b and relative volumes of the core material. We have found that the observed polarization bands with FWHM_p < 0.3 μm in the water-ice absorption band can be explained only by oblate and prolate particles with r _v ≤ 0.35 μm and the polarization bands with FWHM_p ≈ 0.3 μm can be explained only by particles with r _v ≈ 0.35 μm. Broad silicate absorption bands (FWHM ≈ 3 μm) with broad polarization bands (FWHM_p ≈ 2.7 μm) can be explained by particles with r _v ≈ 0.35 μm. Narrow silicate absorption bands (FWHM ≤ 3 μm) with any FWHM of the polarization bands can be explained by a mixture of particles of two types of olivine. Narrow polarization bands (FWHM_p ≈ 2 μm) with broad absorption bands can be explained only by very small particles, r _v ≤ 0.1 μm. We have found the relationships between the effective polarization and extinction cross sections and estimated the ranges of observed polarizabilities that can be explained by particles of given shape and orientation in each of the bands independently. Independent studies of the observational data for each of the bands are shown to give a wider choice of particle model parameters.     

空隙特征对砂岩水致劣化规律的影响

针对南京秦淮东河开挖后的稳定性问题,选取黄马青组（T2h）砂岩为研究对象,对砂岩在吸水-干燥循环条件下的单轴抗压、抗拉特性进行试验研究。考虑到未来边坡运营过程中水的影响,试验时分别考虑自然吸水和饱和吸水两种情况。根据试验结果对所研究砂岩的空隙特征、水致劣化特征和劣化机制进行了详细分析。随着吸水-干燥循环次数增加,岩石的抗压、抗拉强度和凝聚力均呈劣化趋势,说明循环次数的增加对岩石的损伤有累积作用。岩石自然吸水条件下（小开空隙未进水时）强度和弹性模量下降速度较慢,而饱和吸水条件下（开空隙被水充满时）强度和弹性模量下降速度较快,表明岩石中小开空隙对岩石的劣化效果显著。微观结构分析结果表明,随着吸水-干燥循环次数增加,岩石中空隙率增大。结合抗剪强度特征分析认为,干-湿循环导致岩石的黏结强度不断下降,而摩擦强度变化较小,表明黏结强度劣化是岩石水致劣化的主要原因,干-湿循环导致水-岩反应,岩石颗粒胶结物发生松散,边缘发生开裂,宏观上表现为岩石劣化。该研究成果对于新开挖河道边坡稳定性分析具有较大的参考价值,为河岸边坡的长期稳定性分析提供了依据。     

不同超富集、富集植物-玉米间作模式对玉米中镉吸收、转运的影响研究

为了研究Cd污染条件下,玉米分别与苋菜、黑麦草、龙葵间作对重金属Cd吸收和转运的特点,从而选择适宜与玉米间作的富集植物,同时达到修复重金属Cd污染土壤的目的。该文以镉(Cd)污染的河南棕壤黏土为供试土壤,通过盆栽试验,基于玉米各器官中Cd含量、富集系数、转运系数、土壤有效态Cd含量的变化,研究了间作苋菜、黑麦草、龙葵对玉米各器官Cd的积累特性的影响及其迁移转运机制。结果表明：(1)龙葵、苋菜、黑麦草间作使得玉米地上部Cd含量显著性降低(P<0.05),其中以籽粒中Cd含量的下降最为显著。间作苋菜、黑麦草、龙葵,玉米籽粒中Cd含量分别下降了67.6%、75.7%和79.9%。(2)间作苋菜、黑麦草、龙葵使得玉米的富集系数较单作处理下玉米的富集系数分别下降了49.3%、39.7%和68.5%,且差异达到显著水平。(3)与苋菜、黑麦草间作相比,间作龙葵的玉米转运系数分别下降了27.5%、24.2%,且差异均达到显著水平。通过对人体每天摄入Cd量的安全值计算得出间作后土壤中Cd全量应低于2.26 mg·kg-1,土壤有效态Cd含量低于0.88 mg·kg-1。该污染农田在间作模式下,食用玉米Cd暴露对居民健康不存在风险。间作苋菜、黑麦草、龙葵能够抑制玉米对Cd的吸收,同时阻控玉米地上部Cd向地上部的转移,尤其是向籽粒转移。通过间作苋菜、黑麦草、龙葵,不仅降低了主栽作物玉米的Cd累积量,实现玉米安全、优质种植,同时也达到了修复污染土壤的目的。     

高效优化非分裂PML边界二阶标量波方程数值模拟方法

卷积完全匹配层（convolution perfectly matched layer,CPML）吸收边界是一种高效处理波动方程数值模拟中人工边界反射波的方法。本文基于传统的一阶系统CPML吸收边界条件推广并推导了新的二阶系统CPML边界条件（NCPML）。与常规二阶系统CPML边界条件不同,新边界条件推导的核心思想是在复数-频率域中忽略部分衰减因子空间变化特性,避免其在时间域产生复杂卷积算子,然后反变换至时间域得到基于CPML吸收条件的二阶标量波方程,并应用于二阶标量波方程数值模拟。均匀介质模型测试验证了NCPML吸收条件在内存使用上相对于常规二阶系统CPML与SPML（split PML）吸收条件更少。在对人工边界反射的吸收效果上,NCPML稍逊色于常规二阶系统CPML,但二者均相对于SPML优势明显。最后通过层状模型和Marmousi模型测试验证了NCPML的稳定性及其在效率上的优势。     

捷联惯性导航系统算法简化机制

随着低精度惯性导航系统的广泛使用,算法简化也成了研究热点。本文通过实验来验证简化导航算法对于不同惯导尤其是低精度惯导的可行性,这对实时性应用有很大影响。通过对以上内容的介绍,希望可以为进一步研究捷联算法、低精度惯导的实时应用提供一定的参考。