Reflection at large distance from the central engine in Seyferts     

Julien Malzac  Pierre-Olivier Petrucci 《Monthly notices of the Royal Astronomical Society》2002,336(4):1209-1216

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Modelling line profiles in infalling cores     

J.M.C. Rawlings  J.A. Yates 《Monthly notices of the Royal Astronomical Society》2001,326(4):1423-1430

Results are presented from a model of molecular line formation in collapsing star-forming cores. The study includes, for the first time, a self-consistent chemical and dynamical model which is then directly coupled to an appropriate radiative transfer model. The assumptions of chemical uniformity or simple monotonic variations within such cores are shown to be unacceptable. The results show that the abundance variations and the line profiles are highly sensitive to the assumed values of the free parameters in the chemical model. Extreme caution is therefore advised in the quantitative analysis of emission-line profiles from infall sources. The implied degeneracy can be overcome by multiple line-of-sight observations of many species and transitions.  相似文献   

Cosmic reionization by stellar sources: population III stars     

Aaron Sokasian  Naoki Yoshida  Tom Abel  Lars Hernquist  Volker Springel 《Monthly notices of the Royal Astronomical Society》2004,350(1):47-65

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Turbulence in Class 0 and I protostellar envelopes     

D. Ward-Thompson  L. Hartmann  D. J. Nutter 《Monthly notices of the Royal Astronomical Society》2005,357(2):687-690

We estimate the levels of turbulence in the envelopes of class 0 and I protostars using a model based on measurements of the peak separation of double-peaked asymmetric line profiles. We use observations of 20 protostars of both class 0 and I taken in the  HCO⁺(J = 3 → 2)  line that show the classic double-peaked profile. We find that some class 0 sources show high levels of turbulence, whilst others demonstrate much lower levels. In class I protostars, we find predominantly low levels of turbulence. The observations are consistent with a scenario in which class 0 protostars form in a variety of environments and subsequently evolve into class I protostars. The data do not appear to be consistent with a recently proposed scenario in which class 0 protostars can only form in extreme environments.  相似文献   

Bipolar outflow on the asymptotic giant branch – the case of IRC+10011     

Dejan Vinkovi&#;  Thomas Blöcker  Karl-Heinz Hofmann  Moshe Elitzur  Gerd Weigelt 《Monthly notices of the Royal Astronomical Society》2004,352(3):852-862

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ERA-Interim和CMFD气象驱动数据在新疆额尔齐斯河流域的适用性评价     

高黎明  张乐乐  沈永平  张耀南  张伟 《冰川冻土》2022,44(1):179-187

气象驱动数据质量是影响流域水文过程模拟精度的一个重要因素。基于新疆额尔齐斯河流域及周边区域8个气象站记录的数据,对ERA-Interim再分析资料和中国区域地面气象要素驱动数据集（CMFD）在流域的适用性进行了评价,并对比了ERA-Interim和CMFD气象要素年均值在流域的空间分布。结果表明：ERA-Interim和CMFD记录气温、相对湿度、向下短波辐射和向下长波辐射数据与观测数据具有较高的一致性,但降水和风速数据与观测数据的一致性比较差。小时尺度上ERA-Interim记录的气温、相对湿度、降水量、向下短波辐射准确度略高于CMFD数据,而日尺度上CMFD记录的所有气象要素的准确度均高于ERA-Interim数据,结合Noah-MP模型的模拟结果,认为CMFD数据在新疆额尔齐斯河流域的适用性整体优于ERA-Interim数据。从两种驱动数据获取的流域气象要素空间分布来看,ERA-Interim和CMFD获取的年平均气温、风速、相对湿度、降水量、向下长波辐射在流域空间具有高度一致性,但向下短波辐射空间分布差别较大。  相似文献   

1991年8月季风涡旋个例形成的模拟研究     

李箭  葛旭阳  施东雷 《热带气象学报》2020,36(1):72-84

季风涡旋对台风活动有重要的影响, 因此研究季风涡旋的形成机制有利于提高台风预报的准确性。此研究利用中尺度非静力数值模式WRF-ARW模拟1991年8月季风涡旋的生成过程, 并对其生成机制进行分析。模式结果表明, 此次季风涡旋个例是由一个中纬度气旋性低压发展而来。初期中纬度高层正位势涡度的强迫作用有利于对流层低层气旋性低压的发展和维持, 随后高层动力强迫作用减弱, 但中纬度气旋性低压在南移过程中其东南侧对流带逐渐与低纬地区的对流带合并, 使得对流潜热释放增强, 进而使低压在Gill响应的作用下不断加强并最终形成季风涡旋。同时, 涡旋的对流结构表现出明显的非对称性, 因而使其得以维持较大尺度。敏感性试验的结果表明对流层高层强迫对于初始低层扰动的发展至关重要, 而后期热带地区的潜热释放有利于季风涡旋的增强。   相似文献   

Simulation of the Direct Radiative Effect of Mineral Dust and Sea Salt Aerosols in a Doubled Carbon Dioxide Climate          下载免费PDF全文

YUE Xu  LIAO Hong  TANG Jin-Ping 《大气和海洋科学快报》2013,6(5):343-348

The authors examine the equilibrium climatic response to the direct radiative effect(DRE)of mineral dust and sea salt aerosols in a doubled-CO2climate with two-way coupling of aerosol-climate interactions.In response to the drier and windier conditions,dust emissions increase by 26%in the Sahara Desert and by 18%on the global scale relative to present day.Sea salt emissions increase in high latitudes(60°)but decrease in middle latitudes(30°–60°)of both hemispheres due to the poleward shift of westerlies,leading to a 3%decrease in global emissions.The burdens of dust and sea salt increase by 31%and 7%respectively,because reductions in rainfall over the tropical oceans increase the lifetime of particles in the warmer climate.The higher aerosol loading in the doubled-CO2climate reinforces aerosol DRE by0.2 W m 2,leading to an additional cooling of 0.1°C at the surface compared with the climatic effects of aerosols in present day.The additional cooling from changes in natural aerosols compensates for up to 15%of the regional warming induced by doubled CO2.  相似文献   

中国大气气溶胶辐射特性参数的观测与研究进展   总被引：1，自引：1，他引：0  

范学花  陈洪滨  夏祥鳌 《大气科学》2013,37(2):477-498

长期系统的气溶胶辐射特性观测资料是定量研究气溶胶辐射和气候效应的重要基础.本文综合介绍中国大气气溶胶辐射特性观测与研究现状和成果,重点包括以下内容:地面太阳光度计联网观测气溶胶光学厚度、单次散射反照率、尺度谱;从全波段太阳辐射反演气溶胶光学厚度、单次散射反照率;浊度计和黑碳仪测量地面气溶胶散射系数和吸收系数;地基/星载激光雷达观测气溶胶(后向散射系数)垂直分布;极轨/静止卫星遥感反演气溶胶光学特性.  相似文献   

基于MonoRTM模型的微波辐射计反演方法研究   总被引：3，自引：0，他引：3  

黄兴友  张曦  冷亮  李峰  樊雅文 《气象科学》2013,33(2):138-145

基于辐射传输模型MonoRTM计算天空亮温度,使用多元线性统计回归方法和BP神经网络方法分别对大气温度和水汽密度廓线进行了反演,检验并分析了两种方法的反演精度.结果表明,多元线性回归方法反演的温度偏差总体不大于6K,反演的水汽密度偏差小于4 g/m3;神经网络方法反演的温度偏差小于2K,反演的水汽密度误差总体不大于2 g/m3.与探空数据的对比表明,对于大气温度和水汽密度反演,BP神经网络方法的反演结果都要比多元线性回归方法的反演结果更接近探空资料值.  相似文献