The ＂CO2-rich gas vents＂ of Mt. Amiata volcano （Tuscany, Central Italy）： Geochemistry,genetic mechanism and hazard evaluation

Mt. Amiata （Southern Tuscany, Central Italy） is an extinct Quaternary volcano located in an area still marked by high heat-flow that is caused by deep seated （6-10 km） hot masses related to Pliocene magmatic activity. The anomalous geothermal gradient gives rise, within the Mesozoic limestone formation （Tuscan series）, to geothermal systems that fed the Ca-SO4 thermal springs characterizing this area. Besides of thermal fluids, several cold, dry CO2-rich gas emissions seep out on the NE flank of the volcano. These gas vents mostly consist of large sub-circular craters at variable depth and diameter （5-15 m and 10-50 m, respectively）, and represent a serious hazard for the local population, as testified by the several asphyxia casualties that have been repeatedly occurred within these morphological depressions. In this work, the chemical and isotopic compositions of the Mt. Amiata ＂CO2-rich gas vents＂ and the estimation of both the CO2 flux from the soil and the CO2 distribution in air of their surroundings, has been carried out in order to： （1） assess the origin of gases, （2） recognize the mechanism of formation for these gas emissions and their relationship with local tectonics, and （3） to evaluate the CO2 hazard in the high flux emanations. The chemical composition of the gases is largely dominated by CO2 （up to 98 % by vol） and shows relatively high concentrations of N2, CH4 and H2S （up to 1.1%, 0.9% and 3.9 % by vol, respectively）. These features, coupled with the carbon and nitrogen isotopic signatures, suggest that the origin of the main gas compounds may be related to the contribution of deep （i.e., thermometamorphic processes on carbonate formations for CO2） and shallow （i.e. thermal decomposition of organic material for CH4, N2 and H2S） sources.     

辽东湾红沿河附近海域2017—2018年冬季气温-水温-冰情关系研究

辽东湾是我国冰情最严重海域,每年冬季都会受到海冰的显著影响,冰情预测评估可为辽东湾涉海活动提供防冰抗冰的技术依据。建立气温-水温-冰情的相关性,结合便于获取的现场高精度连续气象数据和高精度冰情预测模型,可实现局地小尺度的冰情快速预测评估。基于2017—2018年冬季辽东湾东岸红沿河附近海域实测气象-水温-冰情同步观测数据,结合辽东湾大尺度整体冰情（浮冰面积）,推演局地气温、水温与不同尺度冰情评价参数（浮冰范围与冰厚）的相关关系,提出基于不同气温区间的气温变化规律的冰底热通量选取方法,进而建立适用于辽东湾的气温-水温-冰情评估方法。相关性分析结果显示：观测点气温与水温存在明显相关性;浮冰范围与气象数据存在明显相关性,临界温度为 -5 ℃的累计负气温能很好拟合本年度盛冰期浮冰范围。基于HIGHTSI进行数值模拟后发现：水温与块体积法计算冰底热通量时,冰水间的热传递系数取2.2×10^-5是可行的;水温对冰情的影响表现在海冰冰厚最大值与冰期长短。为弥补辽东湾其他海域因缺少实测海水温度观测数据欠缺、冰底热通量选取不准选取导致的冰情模拟预测评估困难的问题,本文依据水温与气温的相关性,将水温随气温变化划分为结冰区（气温小于-10 ℃时水温维持冰点附近）、过渡区（气温为-10~-5 ℃时水温处于-1.4~-0.4 ℃）、融冰区（气温高于-5 ℃时水温随气温的增大逐渐增大）,进而提出适用于辽东湾所有海域的冰底热通量计算方法和冰情评估方法。     

区域煤炭资源流动及其宏观经济效应初探——以内蒙古为例

从流量、流向以及流动通道三方面,探讨了内蒙古煤炭资源流动平衡现状,采用向量自回归模型解析了内蒙古煤炭资源流动与其宏观经济发展的相互作用关系,结果表明:(1)内蒙古已成长为中国最大的能源输出基地,煤炭交流活动主要集中在其周边地区,尤以华北和东北地区为主。(2)内蒙古铁路煤炭运能不足,缺乏独立、完善的运输网络。(3)内蒙古煤炭资源流动与区内经济发展水平的提高、重工业的发展、第三产业发展以及税收增长均存在着长期稳定的均衡关系,且对区内重工业发展和税收增长具有明显的单向推动作用,但对区内人均GDP和第三产业发展的促进作用相对比较微弱。(4)建立独立、完善的煤炭运输网络;重视发展煤炭运输及其相关服务业;转变能源输出战略,提高输出资源附加值,带动区内煤炭工业以及整体经济发展水平提高的政策建议。     

Sub-arcsec 10 μm imaging of β pictoris and other star disk candidates

We have used the ESO 10 m camera, TIMMI, to image with a very high angular resolution (PFoV: 0.3; FWHM:0.9) several main-sequence star disk candidates. Information on the -Pictoris dust disk has been obtained in a region largely inaccessible to previous observations: 0–80 AU, with a resolution of about 5 AU after deconvolution. Another promising target for 10 m imaging, 51 Ophiuchi, appears point-like.based on data collected at the European Southern Observatory (ESO), La Silla, Chile     

Neutron background in large-scale xenon detectors for dark matter searches

Simulations of the neutron background for future large-scale particle dark matter detectors are presented. Neutrons were generated in rock and detector elements via spontaneous fission and (α,n) reactions, and by cosmic-ray muons. The simulation techniques and results are discussed in the context of the expected sensitivity of a generic liquid xenon dark matter detector. Methods of neutron background suppression are investigated. A sensitivity of 10⁻⁹–10⁻¹⁰ pb to WIMP-nucleon interactions can be achieved by a tonne-scale detector.     

台风“麦莎”移动过程中水汽输送特征

利用NCEP1°×1°的再分析资料,用大尺度水汽通量流函数和速度势以及水汽收支对台风“麦莎”在移动过程中水汽输送流函数和速度势进行了分析。结果表明：台风“麦沙”在北上过程中,主要有2支水汽通道,一支是从太平洋开始向西经赤道到达印度洋,在索马里转向,经过孟家加拉湾呈西南气流向西北方向输送;另一支来自副高南侧偏东气流。计算分析还表明,用无辐散风流场来定台风中心要比用总的流场更精确。     

Estimation of the Land Surface Emissivity in the Hinterland of Taklimakan Desert

An accurate accounting of land surface emissivity(ε) is important both for the retrieval of surface temperatures and the calculation of the longwave surface energy budgets.Since ε is one of the important parameterizations in land surface models(LSMs),accurate accounting also improves the accuracy of surface temperatures and sensible heat fluxes simulated by LSMs.In order to obtain an accurate emissivity,this paper focuses on estimating ε from data collected in the hinterland of Taklimakan Desert by two different methods.In the first method,ε was derived from the surface broadband emissivity in the 8–14 μm thermal infrared atmospheric window,which was determined from spectral radiances observed by field measurements using a portable Fourier transform infrared spectrometer,the mean ε being 0.9051.The second method compared the observed and calculated heat fluxes under nearneutral atmospheric stability and estimated ε indirectly by minimizing the root-mean-square difference between them.The result of the second method found a mean value of 0.9042,which is consistent with the result by the first method.Although the two methods recover ε from different field experiments and data,the difference of meanvalues is 0.0009.The first method is superior to the indirect method,and is also more convenient.     

Two Different Dust Storms in Northeast China:the Sources and Influences in East Asia

There are two different dust storms in Northeast China, normal dust and alkali dust, from Kerqin sand land and Songnen saline land. As well as visible damages of the dust storms, there are some invisible influences. The authors provide evidences that the bacteria carried by dusts from remote area should not be ignored, but the damages of the alkali dusts are still not clear.     

Evolution of the dusty rings of Uranus

We present high quality images of the uranian ring system, obtained in August 2002, October 2003, and July 2004 at 2.2 μm with the adaptive optics camera NIRC2 on the Keck II telescope. Using these data, we report the first detection in backscattered light of a ring (which we refer to as the ζ ring) interior to Uranus' known rings. This ring consists of a generally uniform sheet of dust between 37,850 and 41,350 km with an equivalent width (in 2004; or ), and extends inward to 32,600 km at a gradually decreasing brightness. This ring might be related to the Voyager ring R/1986 U 2, although both its location and extent differ. This could be attributed to a difference in observing wavelength and/or solar phase angle, or perhaps to temporal variations in the ring. Through careful modeling of the I/F of the individual rings at each ansa, we reveal the presence of narrow (few 100 km wide) sheets of dust between the δ and ε rings, and between rings 4 and α. We derived a typical anisotropy factor g≈0.7 in the scattering behavior of these particles. The spatial distribution and relative intensity of these dust sheets is different than that seen in Voyager images taken in forward scattered light, due either to a difference in observing wavelength, and/or solar phase angle or to changes over time. We may have detected the λ ring in one scan at , but other scans provided upper limits below this value. A single detection, however, would be consistent with azimuthal asymmetries known to exist in this ring. We further demonstrate the presence of azimuthal asymmetries in all rings. We confirm the eccentricity of ∼0.001 in rings 4, 5, 6, which in 2004 are ∼70 km closer to Uranus in the north (near periapse; lower I/F) than in the south. We find a global optical depth of τ∼0.3 in the main rings, and of τ=0.25±0.05 in the ε ring.     

Magnetosonic waveguide model of solar wind flow tubes

We consider solar wind flow tubes as a magnetosonic wave-guide. Assuming a symmetric expansion in edges of slab-modelled wave-guide, we study the propagation characteristics of magnetosonic wave in the solar wind flow tubes. We present the preliminary results and discuss their implications.