On the extraction of extended structure from Herschel-SPIRE scanning observations in the presence of 1/f noise

We present results from a study of the impact of uncorrelated 1/ f noise on the extraction of spatial structure, on a range of scales, from sky mapping observations made using the Herschel-SPIRE (the spectral and photometric imaging receiver) photometer in the scan-map mode. These studies were carried out using a detailed instrument simulator, and the output reduced using the map-making algorithm to be implemented in the SPIRE data pipeline. The influence of source size scale, telescope-scanning rate and 1/ f noise knee frequency is investigated, and operational bounds to the expected losses are presented, using the case of zero 1/ f (white) noise as a benchmark. Both cross-linked and non-cross-linked observing options are studied. The results presented here represent the best current estimate of the sensitivity of the SPIRE photometer to emission on arbitrary scales. The data presented are general and scalable to any SPIRE observation made using the scanning mode.     

Periastron precession measurements in transiting extrasolar planetary systems at the level of general relativity

Transiting exoplanetary systems are surpassingly important among the planetary systems since they provide the widest spectrum of information for both the planet and the host star. If a transiting planet is on an eccentric orbit, the duration of transits T _D is sensitive to the orientation of the orbital ellipse relative to the line of sight. The precession of the orbit results in a systematic variation in both the duration of individual transit events and the observed period between successive transits,   P _obs  . The periastron of the ellipse slowly precesses due to general relativity and possibly the presence of other planets in the system. This secular precession can be detected through the long-term change in   P _obs  (transit timing variations, TTV) or in T _D (transit duration variations, TDV). We estimate the corresponding precession measurement precision for repeated future observations of the known eccentric transiting exoplanetary systems (XO-3b, HD 147506b, GJ 436b and HD 17156b) using existing or planned space-borne instruments. The TDV measurement improves the precession detection sensitivity by orders of magnitude over the TTV measurement. We find that TDV measurements over a approximately 4 yr period can typically detect the precession rate to a precision well exceeding the level predicted by general relativity.     

Observations of Low-Latitude Coronal Plumes

Using Fe ix/x 17.1 nm observations from the Extreme-Ultraviolet Imaging Telescope (EIT) on the Solar and Heliospheric Observatory (SOHO), we have identified many coronal plumes inside low-latitude coronal holes as they transited the solar limb during the late declining phase of cycle 23. These diffuse, linear features appear to be completely analogous to the familiar polar plumes. By tracking them as they rotate from the limb onto the disk (or vice versa), we confirm that EUV plumes seen against the disk appear as faint, diffuse blobs of emission surrounding a brighter core. When the EIT images are compared with near-simultaneous magnetograms from the SOHO Michelson Doppler Imager (MDI), the low-latitude, on-disk plumes are found to overlie regions of mixed polarity, where small bipoles are in contact with unipolar flux concentrations inside the coronal hole. The birth and decay of the plumes are shown to be closely related to the emergence of ephemeral regions, their dispersal in the supergranular flow field, and the cancellation of the minority-polarity flux against the dominant-polarity network elements. In addition to the faint polar and nonpolar plumes associated with ephemeral regions, we note the existence of two topologically similar coronal structures: the giant plume-like features that occur above active regions inside coronal holes, and the even larger scale “pseudostreamers” that separate coronal holes of the same polarity. In all three cases, the basic structure consists of open field lines of a given polarity overlying a photospheric region of the opposite polarity; ongoing interchange reconnection at the X-point separating the open field domains from the underlying double-arcade system appears to result in the steady evaporation of material from the closed into the open region.     

公路路面热效应对环境气温的影响分析

为定量研究公路对气温观测的影响,本文使用2014年1—5月在陕西省开展的两组公路观测试验的逐分钟温度、风向、风速等气象资料,对比分析了合阳县国道和渭蒲高速公路在不同季节、不同天空状况以及不同背景风速条件下对周围环境气温观测的影响程度和影响距离。试验结果表明:公路对周围的环境温度有一定的增温影响,合阳国道对环境温度的增温影响至75m,增温效应达0.25~0.4℃。高速公路的增温影响至125m,增温效应达0.2~0.4℃。冬季,两条公路白天增温效应较夜间明显,春季,高速公路夜间增温更明显。晴天、多云天气比阴天、降雨天气增温程度大。公路对气温的增温影响存在风速阈值,当风速小于对应阈值时,增温效应明显。公路上来往车流量对气温有一定的叠加增温影响,合阳国道白天车流量150~350辆,叠加增温效应0.05~0.1℃,蒲渭高速白天车流量2000~3500辆,叠加增温效应0.16℃。     

New consideration of atmospheric refraction in laser ranging data

In this paper we reconsider the formulae of tropospheric refraction correction for the Satellite Laser Range technique. From the expansion of the complementary error function, a new continued fraction form of the mapping function at optical frequencies is derived. The correction terms related to the operation frequency of the laser beam are considered in both the zenith delay and the mapping function. The correction for low-elevation satellites is briefly reviewed. The theoretical accuracy of the new mapping function has been analysed via the ray tracing integrals under the standard atmospheric profile. With respect to the radiosonde data, the deviations of the new mapping function are investigated in an elevation range down to near 1°, which is comparable with the results of the Marini–Murray formulae .     

一次黄海爆发性气旋的观测分析和数值模拟研究

本文利用再分析资料和WRFV3.9模式（Weather Research and Forecasting Model）对2020年7月22－24日发生在黄海海域的一次爆发性气旋进行了研究,并对其演变过程和发展机制进行了详细分析。该气旋22日12UTC在山东南部生成,入海后开始爆发性发展,最大加深率达到1.2 Bergeron,23日在黄海中部气压降至最低990 hPa左右,24日在韩国登陆。高空强辐散、低层的暖舌结构、水汽输送和下垫面热通量的变化增强了大气斜压性,使其迅速发展。使用WRF模式对气旋进行模拟,涡度的诊断分析表明,大气低层强斜压性主要通过涡度方程的散度项对气旋的发展起作用,对流项在涡度发展旺盛的时刻也有一定影响。海温的敏感性试验表明,海温变化对气旋移动路径和中心气压影响明显。     

某地下空间承压含水层抽水试验及成果分析

由于地下水突涌风险,地下空间在施工作业中有必要通过抽水试验确定承压含水层的水文地质参数。依据勘察报告的初步评价,基坑开挖15.5m时,场地内第⑦1层承压含水层有可能产生突涌,为确保工程安全施工,需开挖前进行承压含水层抽水试验,取得场地承压含水层水文地质参数及降水引起的沉降特征,为地下空间设计和施工提供可靠依据。本次布设抽水井、观测井、分层沉降标组、孔隙水压力观测孔及地面沉降观测点,依据抽水试验技术要求获取渗透系数、抽水影响半径等相关水文地质参数。最后,针对工程场地内承压水情况及特点进行分析,提出基坑开挖时的承压水降压建议方案。     

Extragalactic research in Europe and the United States in the early 20th century

While the theoretical foundations of modern relativistic cosmology were laid, to a large extent, by European researchers like Einstein, de Sitter, Friedmann, Lemaître, and others, observational cosmology was (and to a large extent, still is) dominated by US astronomers, working at Lick and Mt. Wilson observatories. From today's viewpoint, Hubble appears to dwarf all his – national and international – peers. However, Keeler and Curtis, Fath and Slipher carried put pioneering work in the US, as did Wolf, Wirtz, Lundmark, de Sitter in Europe, both by observation and by statistical analysis of data. European extragalactic research during the early 20th century is outlined and compared with studies in the United States. Reasons for the small impact of European research are a mixture of deliberate and accidental neglect and suppression, as well as the lack of technical and organizational infrastructure, which was especially noticeable after World War I.     

地震资料约束下大地电磁资料反演

应用地震资料约束下大地电磁资料反演古潜山或基底内部结构的新方法. 首先利用地震及井资料,反演得到古潜山或基底之上各层的厚度及电阻率,建立了古潜山或基底以上的地电模型;并利用大地电磁一维反演资料,建立了古潜山或基底及其以下的地电模型. 在初始模型建立的基础上,应用高效快速的二维大地电磁正演算法——模式匹配方法,进行正演计算. 利用共扼梯度迭代方法,进行正反演迭代计算. 通过对胜利油田南北618剖面反演, 基底以下在地震资料没有显示的构造信息,在反演结果中得到了较好地反映.      

浮式油气生产储卸装置风倾力臂解析解及相关线性关系研究

为了建立驳船型浮式生产储卸装置的风倾力臂和船型参数之间的函数关系,构造了与其主尺度及设计工况对应吃水、排水量和正浮状态侧向所受风倾力臂相关的3个无因次量——"相对力臂"、"相对排水量"和"相对吃水",使前二者的乘积与相对吃水呈现出线性变化关系,通过拟合直线得到风倾力臂的解析解,其有效性经6艘我国现役FPSO的设计数据和理论分析验证,结果理想。