太阳硬X射线成像望远镜模拟研究   总被引：1，自引：0，他引：1  

滕藤  伍健  常进 《天文学报》2011,52(4):339-351

调制准直器型太阳硬X射线成像望远镜是目前较为通用的太阳观测设备.空间调制望远镜是基于中心轴不旋转的望远镜,适用于3轴稳定的卫星.针对我国可能的太阳观测计划,给出并比较了两组空间调制望远镜的配置方案,然后利用GEANT4高能物理通用软件模拟实际光子的计数情况,使用MATLAB实现图像重建.比较模拟光子计数得到的重建图与几...  相似文献   

CDFS天区中喑蓝星系的测光红移研究     

杜志良 《天文学报》2011,52(1)

从COMBO-17数字巡天数据里,选择了CDFS(Chandra Deep Field South)天区中1231个测光红移在0.1～0.3之间的暗蓝星系作为样本,研究了这些星系分别在只有光学波段和光学加近红外波段数据情况下做测光红移得到的红移分布,以及这些星系在静止参考系下的能谱分布(Spectral Energy Distributions,SEDs)特征.结果表明有183个星系在利用光学加近红外波段数据做测光红移时得到的红移大于1.2,它们的误差为0.046,提高测光的信噪比也有利于区分这类被光学波段误认为低红移的星系.这些暗蓝星系中高红移星系的观测近红外流量相对于光学流量有上升的趋势,而低红移星系的观测近红外流量相对于光学流量有下降的趋势.  相似文献   

非线性相对运动下空间碎片碰撞概率计算的研究     

许晓丽  熊永清 《天文学报》2011,52(1):73-85

空间目标碰撞概率的计算是航天器进行空间碎片预警和规避机动的基础.为了简化计算,目前国内外在计算碰撞概率问题过程中大多基于线性相对运动的条件,将三维碰撞概率计算积分问题简化为位置误差概率密度函数在圆域内的二维积分问题.但是当空间目标相对运动速度较小时,这种线性运动条件不再成立,就需要在真实的非线性相对运动状态下重新考虑碰...  相似文献   

幂律电子谱轫致辐射积分的快速计算     

李友平  甘为群 《天文学报》2011,52(3)

SSW(Solar SoftWare)的能量电子产生X光子的轫致辐射积分计算发展到版本2时,其性能相比初始的版本1提高很多.在版本2的基础上,对这个积分进一步改进.通过对比几种轫致辐射积分方案,结果显示,最终的方案性能上比版本2可以快约2～5倍.在积分的精确性上比版本1及版本2均改进了很多,在缺省的积分控制精度下也不再产生光子谱的尖刺现象.而且,积分耗时不再敏感于积分上限取值.由于积分性能的提高,使得利用精确的轫致辐射截面计算轫致积分成为可能.结果显示,用精确轫致辐射截面比先前的近似截面积分的结果光子流量略小(≤4%),积分时间大约比先前使用近似截面多30%.  相似文献   

Relaxation of protostellar accretion shocks using the smoothed particle hydrodynamics     

M. Nejad‐Asghar 《Astronomische Nachrichten》2011,332(6):631-636

It is believed that protostellar accretion disks are formed from nearly ballistic infall of molecular matter in rotating core collapse. Collisions of this infalling matter leads to formation of strong supersonic shocks, which if they cool rapidly, result in accumulation of that material in a thin structure in the equatorial plane. Here, we investigate the relaxation time of the protostellar accretion post‐shock gas using the smoothed particle hydrodynamics (SPH). For this purpose, a one‐dimensional head‐on collision of two molecular sheets is considered, and the time evolution of the temperature and density of the post‐shock region simulated. The results show that in strong supersonic shocks, the temperature of the post‐shock gas quickly increases proportional to square of the Mach number, and then gradually decreases according to the cooling processes. Using a suitable cooling function shows that in appropriate time‐scale, the center of the collision, which is at the equatorial plane of the core, is converted to a thin dense molecular disk, together with atomic and ionized gases around it. This structure for accretion disks may justify the suitable conditions for grain growth and formation of proto‐planetary entities (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Mining the CFHT Legacy Survey for known Near Earth Asteroids     

O. Vaduvescu  A. Tudorica  M. Birlan  R. Toma  M. Badea  D. Dumitru  C. Opriseanu  D. Vidican 《Astronomische Nachrichten》2011,332(6):580-589

The Canada‐France‐Hawaii Legacy Survey (CFHTLS) comprising about 25 000 MegaCam images was data mined to search for serendipitous encounters of known Near Earth Asteroids (NEAs) and Potentially Hazardous Asteroids (PHAs). A total of 143 asteroids (109 NEAs and 34 PHAs) were found on 508 candidate images which were field corrected and measured carefully, and their astrometry was reported to Minor Planet Centre. Both recoveries and precoveries (apparitions before discovery) were reported, including data for 27 precovered asteroids (20 NEAs and 7 PHAs) and 116 recovered asteroids (89 NEAs and 27 PHAs). Our data prolonged arcs for 41 orbits at first or last opposition, refined 35 orbits by fitting data taken at one new opposition, recovered 6 NEAs at their second opposition and allowed us to ameliorate most orbits and their Minimal Orbital Intersection Distance (MOID), an important parameter to monitor for potential Earth impact hazard in the future (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Horizon synthesis for archaeo‐astronomical purposes     

F. Patat 《Astronomische Nachrichten》2011,332(7):743-749

In this paper I describe a simple numerical procedure to compute synthetic horizon altitude profiles for any given site. The method makes use of a simplified model of local Earth's curvature, and it is based on the availability of digital elevation models describing the topography of the area surrounding the site under study. Examples constructed using the Shuttle Radar Topographic Mission (SRTM) data (with 90 m horizontal resolution) are illustrated, and compared to direct theodolite measurements. The proposed method appears to be reliable and applicable in all cases when the distance to the local horizon is larger than ∼10 km, yielding a rms accuracy of ∼0.1 degrees (both in azimuth and elevation). Higher accuracies can be achieved with higher resolution digital elevation models, like those produced by many modern national geodetic surveys (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Predation and intertidal zonation of barnacles at Leigh,New Zealand     

Penelope A. Luckens 《新西兰海洋与淡水研究杂志》2013,47(3):355-378

Experiments using cages at four shore levels were carried out to determine the part played by the feeding of the gastropods Neothais scalaris and Lepsiella scobina on the zonation of three species of intertidal barnacles: Chamaesipho brunnea, C. columna, and Epopella plicata. The lower limit of the two larger barnacle species was determined by predation, but C. columna was affected only in the absence of the other two barnacles.  相似文献   

A Novel Approach of Using Selected Unconventional Geodesic Methods of Estimation on VTS Areas     

Krzysztof Czaplewski  Mariusz Wąż  Marek Hubert Zienkiewicz 《Marine Geodesy》2013,36(5):447-468

Abstract

The Vessel Traffic Service (VTS) systems belong to the fundamental tools used in ensuring a high level of safety across sea basins with heavy traffic, where the presence of navigational hazards poses a great risk of collision or a ship running aground. In order to determine the mutual location of ships, VTS systems obtain information from different facilities, such as coastal radar stations, AIS, and vision systems. Fixing a ship’s position is always accompanied by a degree of error, but the degree of error depends on the specific position fixing system used. In order to increase the accuracy of position fixing in VTS systems, the authors propose the use of contemporary geodetic methods. The article presents the theoretical fundamentals of two unconventional geodesic methods of estimation: M estimation and M_split(q)estimation and the authors’ own proposal of their application in VTS systems. The article concludes with a test verifying theoretical assumptions, performed with the use of a computer application allowing position fixing with the use of selected robust adjustment methods. Furthermore, an example is presented of M_split(q)estimation as used for the acquisition of low-signal radar echoes, which in VTS systems are not automatically identified for tracking. The level of the echo signal makes it difficult for a VTS controller to separate these objects from typical radar noise and interference.  相似文献   

土壤碳储量计算中不同插值方法对比研究——以吉林省大安市为例   总被引：1，自引：0，他引：1  

汪媛媛  杨忠芳  余涛  文宇博  夏学齐  白荣杰 《中国岩溶》2011,30(4):479-486

土壤碳储量问题是大气温室效应和全球变化研究的热点问题。本文采用“单位土壤碳量”方法,计算了吉林省大安市表层土壤有机碳总储量和平均土壤有机碳储量,以为全球碳循环研究提供精确的基础数据。分析和比较了反距离加权、全局多项式、局部多项式、径向基函数和普通克里格等不同插值模型对表层单位土壤有机碳储量空间插值结果的影响,结果表明全局多项式插值的均差最小,径向基函数中张力样条法的平均绝对误差最小,普通克里格法的标准差最小。综合分析来看,普通克里格的有理二次方程式模型插值精度最高。   相似文献