陇中黄土高原冬季地表辐射和能量平衡特征

利用定西试验基地2003年12月至2004年2月获取的地气相互作用观测资料,分析了陇中黄土高原冬季典型天气（晴天、阴天及雪天）和平均状况下的地表辐射能量平衡和土壤温度等微气象特征的日变化规律。结果表明,在典型天气间微气象特征有较大差异,但冬季的平均特征与晴天比较接近,云和降雪的扰动影响有限。冬季地表能量平衡以感热输送为主,土壤热通量为辅,且普遍存在不平衡现象。冬季初的2／3时段净辐射及土壤热通量日总量基本为负值,之后的1／3时段为正值,冬季地面加热场为热源。冬季土壤温度在地表及20 cm土壤层存在日变化,30 cm及以下土壤温度日变化很小。冬季地表日平均反射率基本在0.20～0.25之间变化,平均值为0.22。     

Interaction of waves,currents and tides,and wave-energy impact on the beach area of Sylt Island

Erosion due to waves is an important and actual problem for most coastal areas of the North Sea. The objective of this study was to estimate the impact of wave action on the coastline of Sylt Island. From a 2-year time series (November 1999 to October 2001) of hydrological and wave parameters generated with a coupled wave–current modelling system, a period comprising storm ‘Anatol’ (3–4 December 1999) is used to investigate the effects of waves on currents and water levels and the input of wave energy into the coastline. The wave-induced stress causes an increase of the current velocity of 1 m/s over sand and an additional drift along the coast of about 20 cm/s. This produces a water level increase of more than 20 cm in parts of the tidal basin. The model system also calculates the wave energy input into the coastline. Scenario runs for December 1999 with a water level increase of 50 cm and wind velocity increased by 10% show that the input of the wave energy into the west coast of Sylt Island increases by 30% compared to present conditions. With regard to the forecasted near-future (Woth et al., Ocean Dyn 56:3–15, 2006) increase of strong storm surges, the scenario results indicate an increased risk of coastal erosion in the surf zone of Sylt Island.     

BOBMEX-98 pilot: Measurement and analysis of incoming shortwave radiation data

Empirical formulae for estimation of hourly incoming shortwave radiation over the Indian Ocean under different cloud amounts have been developed by using the pyranometer measurements of the incoming solar radiation and the cloud observations during BOBMEX Pilot (October–November 1998) cruise.     

Short-wave radiation flux divergence in arctic cirrus: a case study

Radiation and particle measurements have been performed with an aircraft in deep cirrus cloud fields near the island of Svalbard. The data of 12 March 1993, when measurements at 10 different levels could be obtained, are used in a comparative study with radiative transfer calculations. In a first analysis, the cirrus cloud field was assumed to be horizontally homogeneous and invariable during the time of measurements (frozen properties). Calculations of the up and downward radiative flux densities showed root mean square differences of 9 Wm⁻² from the measurements. To estimate the possible effect of changes of the optical properties of cirrus with time, the flux densities in the upper part (6000–8500 m) and the lower part (3000–5500 m) of the cirrus cloud were analyzed separately. In these simulations, the optical thickness in the lower (upper) part was increased (decreased) by 50%. By this treatment, most of all calculated flux densities were within one standard deviation of the natural variability in each leg. Finally, the effect of inhomogeneities in the cloud field on the solar flux density has been simulated using a Monte Carlo method, since the upper part of the cirrus field has indeed been very inhomogeneous. This paper is a result of a collaborative effort between the MRI in Tsukuba, Japan, and the GKSS in Geesthacht, Germany.     

动水压力作用下深水桥墩非线性地震响应分析

为研究动水压力作用对深水桥墩地震响应的影响,本文分别采用Morison方程和辐射波浪理论建立了动水压力计算方法,分析了动水压力作用对桥墩地震响应的影响;同时分析了考虑材料非线性时动水压力作用对桥墩地震响应的影响。研究表明:动水压力作用增大了桥墩的地震响应,其影响随着相对水深的增加而增强;考虑材料非线性时动水压力对桥墩地震响应的影响,相对线性材料而言有所变化。     

Optical spectroscopy study of variously colored gem-quality topazes from Ouro Preto,Minas Gerais,Brazil

Variously colored gem-quality topazes from Ouro Preto, Minas Gerais, Brazil, were studied by optical absorption spectroscopy and photoluminescence methods. In the near infrared range (750–2500 nm) the absorption spectra display an identical pattern of narrow intense absorption lines caused by overtones and combination vibrations of OH groups, which do not relate to the coloration of the topazes studied. Their colors were found to be caused by combination of three sets of absorption features, (1), (2), and (3) in the visible and near-UV range, which are due to different color center. (1) denotes a pair of broad split bands with maxima 18 000 and 25 000 cm^–1 caused by electronic spin-allowed dd transitions of Cr³⁺ ions. They cause a light rose to deep violet color and characteristic pleochroism of Cr³⁺-containing topazes. Photoluminescence evidences of at least three different types of Cr³⁺ complexes which, most probably, differ by ligand surroundings, O₄F₂, O₄F(OH) and O₄(OH) (2) Corresponds to the intense weakly polarized UV absorption edge. Two different parts, the thermally stable one, caused by ligand-to-metal charge transfer, and the thermally unstable one, caused by some defect center(s), contribute to the edge. (3) denotes a system of two broad unstructured bands with maxima around 19 000 cm^–1 (X>Y Z) and 24 000 cm^–1 (Y Z X). They cause the unique orange color and characteristic pleochroism of Brazilian Imperial topazes. Combinations of (1) and (3) absorption features cause various yellow-rose colors of the samples. Investigations of natural irradiated and thermally treated topazes show that the color centers (1) and (3) transform to each other at annealing and X- or gamma irradiation. The color of natural orange-red Imperial topazes is assumed to be caused by Cr⁴⁺, stabilized by other impurity ions and/or defect irradiation EPR centers. At T=300 °C Cr⁴⁺ reduces to Cr³⁺, the color of Imperial topazes changes to pale rose, caused by spin-allowed bands of Cr³⁺. In artificially irradiated crystals the (3)-center, Cr⁴⁺, may be induced according to the reaction 2Cr³⁺ Cr⁴⁺ + Cr²⁺, which involves chromium pairs in adjacent Al sites of the structure. Such artificially induced color is unstable at room temperature and in daylight. The process of the decay of (3)-centers may be described as a recombination Cr⁴⁺+Cr²⁺ 2Cr³⁺ that results in vanishing of the (3)-bands accompanied by the appearance or increase in Cr³⁺ dd bands, the original orange color turning to a pale rose.     

AN ERROR ANALYSIS ON THE SIMULATED DATA OF TOVS HIRS BY RTTOV5 MODEL*

The sounding data of meteorological satellites provide not only the real time weather information about the distribution of both cloud and rainfall,but also some others about the movement and state of atmosphere.They are important variables and parameters for NWP model used to simulate and predict atmospheric state.In order to introduce remote sensing information from satellites into NWP model,there is an efficient way of establishing an RT model by use of the atmosphere radiation sounding data of meteorological satellites to get the variables and parameters valuable to NWP model.In this paper,we set up profiles of air temperature and water vapor from the surface to upper (0.1 hPa) using the radiosounding data and the surface data from May to August 1998 atmosphere East Asia.A TOVS RT model (RTTOV5) is provided to compute the value of radiation value of HIRS channels in NOAA14.Then the radiation values of 19 HIRS channels are gotten.After matching these data computed by the RT model and the corresponding values coming from satellite sounding in time,the statistic distribution of bias between tile model output and the satellite sounding at each sounding channel can be gotten.At the same time.the distribution of RMS to every TOVS HIRS channel,the standard biases to different scanning angle to each channel are also obtained.     

Radiation stress due to ocean waves and the resulting currents and set-up/set-down

The authors have developed a model to predict the radiation stresses in the coastal zone and to estimate currents and set-up/set-down of mean sea level. The values of radiation stress are calculated from velocity potential, which can be obtained by analytical means or from a finite element model of the elliptic extended mild slope equation depending on the complexity of the situation in question. The values of radiation stress are then input into a hydrodynamic model which gives the resulting set-up/set-down and currents caused by these stresses. The developed model includes convective acceleration and bottom friction. The radiation stress results of the model have been compared with analytical results and published values. Results for set-up/set-down and currents have been compared with published results for seven other similar models. The model has been compared with published results for set-up/set-down and currents created in the vicinity of a detached breakwater and also around a conical island. The results of the authors’ model compare well with the analytical results, and published results for similar models. An erratum to this article can be found at     

Optical alteration of complex organics induced by ion irradiation:: 1. Laboratory experiments suggest unusual space weathering trend

Most ion irradiation experiments relevant to primitive outer Solar System objects have been performed on ice and silicate targets. Here we present the first ion irradiation experiments performed on natural complex hydrocarbons (asphaltite and kerite). These materials are very dark in the visible and have red-sloped spectra in the visible and near-infrared. They may be comparable in composition and structure to refractory organic solids on the surfaces of primitive outer Solar System objects. We irradiated the samples with 15-400 keV H⁺, N⁺, Ar⁺⁺, and He⁺ ions and measured their reflectance spectra in the range of 0.3-2.5 μm before ion implantation and after each irradiation step. The results show that irradiation-induced carbonization gradually neutralizes the spectral slopes of these red organic solids. This implies a similar space weathering trend for the surfaces of airless bodies optically dominated by spectrally red organic components. The reduction of spectral slope was observed in all experiments. Irradiation with 30 keV protons, which transfers energy to the target mostly via electronic (inelastic) collisions, showed lower efficiency than the heavier ions. We found that spectral alteration in our experiments increased with increasing contribution of nuclear versus electronic energy loss. This implies that nuclear (elastic) energy deposition plays an important role in changing the optical properties of irradiated refractory complex hydrocarbon materials. Finally, our results indicated that temperature variations from 40 K to room temperature did not influence the spectral properties of these complex hydrocarbon solids.