基于脉冲星计时的航天器自主定位误差估计方法     

田丰 《天文学进展》2011,29(1):97-104

目前很多学者希望从"X射线脉冲星自主导航"的导航算法研究入手,利用数据分析或仿真进行验证.其中关于航天器自主定位的误差估计方法、误差量级和各种影响因素的讨论,并没有在给定详细初始条件的基础上系统性地说明问题.为了分析上述问题,需从天体测量学的角度出发,对自主定位的各种误差源及其影响因素进行探讨和误差量级的估计.首先,由...  相似文献   

分块DPCM与5/3整数小波变换结合的天文图像无损压缩     

朱贵富  邓辉  王锋  季凯帆 《天文研究与技术》2011,8(1)

针对海量的天文图像数据与有限的存储空间和带宽资源之间矛盾日益突出这一问题,提出一种无损压缩方法,首先将超大天文图像分块,再使用差分脉冲编码调制和5/3整数小波变换,最后使用霍夫曼算法编码。对该方法的原理和具体实现做了详细的分析与介绍,通过实验验证该方法比天文中常用的tar、PKZip、WinZip、WinRar软件在压缩比上分别提高了30%、29%、26%、2%,压缩速度远大于WinZip和WinRar;且该算法实现简单,适合硬件实现和利于并行处理。  相似文献   

基于飞机观测资料的石家庄秋季对流层CH4垂直分布特征     

麦榕  杨洋  范根昌  吕峰  董晓波  梁苗  姚波 《气象与环境学报》2022,38(2):70-77

为研究石家庄秋季对流层内CH₄垂直分布特征,2018年9月使用“空中国王350”飞机搭载Picarro温室气体在线观测仪和气象要素观测设备,对石家庄上空（600—5500 m）CH₄浓度进行探测。探测期间共飞行7架次,取得7条CH₄浓度廓线数据。结果表明: 石家庄上空近地面层（1000 m以下）CH₄平均浓度与同时间段区域背景站上甸子站CH₄浓度呈显著正相关（r=0.81,P < 0.03）。探测到的CH₄浓度最小值为1898×10^-9摩尔分数,最大值为2219×10^-9摩尔分数,平均浓度为1981×10^-9摩尔分数。观测得到的7条廓线均有较好的一致性,2000 m以上,浓度均随高度呈先增大后减小的趋势。利用后向轨迹模式（HYSPLIT）对探测时段内石家庄上空不同高度层主要气流传输路径进行统计分析表明,600 m高度输送路径较短,CH₄浓度受本地排放影响较大; 3000 m受输送作用影响较大,偏西和西南路径可能将较高CH₄浓度气团输送至石家庄上空; 5000 m气团传输对CH₄浓度影响较小,浓度相对较稳定,对传输路径的变化不敏感。  相似文献   

The heating of the solar transition region     

Wen-Bin Song  Xue-Shang Feng  Fang Shen 《中国天文和天体物理学报》2010,10(6)

The temperature curve in the solar chromosphere has puzzled astronomers for a long time.Referring to the structure of supergranular cells,we propose an in ductive heating model.It mainly includes the following three steps.(1) A small-scale dynamo exists in the supergranulation and produces alternating small-scale magnetic fluxes;(2) The supergranular flow distributes these small-scale fluxes according to a regular pattern;(3) A skin effect occurs in the alternating and regularly-distributed magnetic fields.The induced current is concentrated near the transition region and heats it by resistive dissipation.  相似文献   

The “Same Side – Opposite Side Effect” of the Heliospheric Current Sheet in Ionospheric Negative Storms     

Z. Li  F. S. Wei  X. S. Feng  X. H. Zhao 《Solar physics》2010,263(1-2):263-273

Using 141 CME-interplanetary shock (CME-IPS) events and foF2 from eight ionosonde stations from January 2000 to September 2005, from the statistical results we find that there is a “same side?–?opposite side effect” in ionospheric negative storms, i.e., a large portion of ionospheric negative disturbances are induced by the same-side events (referring to the CMEs whose source located on the same side of the heliospheric current sheet (HCS) as the Earth), while only a small portion is associated with the opposite-side events (the CMEs source located on the opposite side of the HCS as the Earth); the ratio is 128 vs. 46, and it reaches 41 vs. 14 for the intense ionospheric negative storms. In addition, the ionospheric negative storms associated with the same-side events are often more intense. A comparison of the same-side event (4 April 2000) and the opposite-side event (2 April 2001) shows that the intensity of the ionospheric negative storm caused by the same-side event is higher than that by the opposite-side event, although their initial conditions are quite similar. Our preliminary results show that the HCS has an “impeding” effect to CME-IPS, which results in a shortage of energy injection in the auroral zone and restraining the development of ionospheric negative perturbations.  相似文献   

AMR Simulations of Magnetohydrodynamic Problems by the CESE Method in Curvilinear Coordinates   总被引：1，自引：0，他引：1  

Chaowei Jiang  Xueshang Feng  Jian Zhang  Dingkun Zhong 《Solar physics》2010,267(2):463-491

The objective of this paper is to present new extensions of the space – time conservation element and solution element (CESE) method for simulations of magnetohydrodynamic (MHD) problems in general curvilinear coordinates by using an adaptive mesh refinement (AMR) grid system. By transforming the governing MHD equations from the physical space (x,y,z) to the computational space (ξ,η,ζ) while retaining the form of conservation, the CESE method is established for MHD in the curvilinear coordinates. Utilizing the parallel AMR package PARAMESH, we present the first implementation of applying the AMR CESE method for MHD (AMR-CESE-MHD) in both Cartesian and curvilinear coordinates. To show the validity and capabilities of the AMR-CESE-MHD code, a suite of numerical tests in two and three dimensions including ideal MHD and resistive MHD are carried out, with two of them in both Cartesian and curvilinear coordinates. Numerical tests show that our results are highly consistent with those obtained previously by other authors, and the results under both coordinate systems confirm each other very well.  相似文献   

The Contribution from Radio Quiet Quasars to γ-ray Background     

Feng Min-zi  Wang Jian-min 《Chinese Astronomy and Astrophysics》2010,34(1):30-39

The EGRET observations have confirmed and proposed the new isotropically distributed γ-ray background, but the known objects radiating γ-rays can not supply so much radiation. Meanwhile, EGRET also reveals a population of γ-ray sources with no radio counterparts which are isotropically distributed in the sky, indicating their possible cosmological origins. Wang et al.^[13] proposed a new γ-ray radiation process driven by the radiation feedback of AGNs. The energy of the radiation peaks around 1 GeV—0.1 TeV with the typical luminosity of 10⁴²—10⁴³ ergs · s^?1. This kind of radiation process in the radio quiet quasars make them the potential γ-ray radiation sources as well as the contributors to the γ-ray background. We consider two cases in which the seed photons in the inverse-Compton processes are from the accretion disks of quasars and cosmic microwave background (CMB), respectively. We find that the former contributes 78%—92% of the background radiation around 1 GeV, while the contribution from the latter is negligible. The radio quiet quasars are highly likely to become the objects which contribute the most energy to the γ-ray background around 1 GeV.  相似文献   

海水鱼类寄生虫刺激隐核虫(Cryptocaryon irritans)趋化性研究     

邹峰  苏永全  覃映雪  马英  张艺  韩坤煌  鄢庆枇 《海洋与湖沼》2013,44(4):1003-1007

应用本实验室建立的趋化模型对海水鱼类寄生虫刺激隐核虫(Cryptocaryon irritans)的趋化特性进行研究。结果显示, 刺激隐核虫幼虫在30min时趋化达到饱和, 在温度28℃时趋化率达到最高; 多种硬骨鱼的血清与粘液对刺激隐核虫的幼虫都有着强烈的吸引作用, 刺激隐核虫幼虫对碳水化合物、氨基酸等小分子物质没有趋化作用; 在组织匀浆液中, 刺激隐核虫幼虫对肌肉匀浆液有一定的趋化作用, 对肝、肠、胃的匀浆液都没有趋化作用; 感染后鱼类血清对刺激隐核虫的幼虫有着更加强烈的吸引作用(P<0.01); 18种中草药中的五倍子、大黄、槟榔、苦楝、虎杖、贯众等6种中药草对刺激隐核虫的幼虫有一定的驱虫作用。本文的研究结果有助于深化对刺激隐核虫致病性的认识并对“白点病”的防治有一定的参考价值。  相似文献   

垃圾填埋场渗沥液pH值变化对粘土防渗层压缩性的影响     

黄方媛  魏松  张婉婷  卢昱柏  苏进源  郑海君  吉锋 《地质灾害与环境保护》2022,33(1):102-106

粘土防渗层是垃圾填埋设施中直接接触渗沥液的防渗层,防渗层有效地阻隔了垃圾渗沥液下渗,减少了渗沥液对环境的污染.以成都粘土为研究对象,采用高压固结试验研究粘土防渗层在不同浸润时间、不同pH渗沥液浸润下对粘土层固结参数的影响.结果表明:浸润时间和渗沥液pH对粘土固结参数的影响较大.随着浸润时间的增加,渗沥液pH值对土的压缩...  相似文献   

陕北植被变化遥感监测及对径流的影响   总被引：5，自引：0，他引：5  

孙智辉  罗琳  苏锋  李新亚 《气象科技》2007,35(2):282-285

陕北北部是我国水土流失最为严重的地区,年输入黄河的泥沙量占全河的38%。1999年实施退耕还林草工程后,退耕还林草面积达9617.2 km2。利用1998-2004年NOAA卫星遥感资料,计算陕北北部地区归一化植被指数,发现陕北植被指数增幅在50%-200%之间,其中吴旗县增幅最大。对延安北部及榆林市1998-2004年降水量资料分析,得出植被指数增加是退耕还林草工程初见成效,不是由于降水变化引起的。利用1980-2004年吴旗县气象站观测的降水量和水文站所测径流量进行时间序列相关分析、典型年对比分析,得出该县植被变化对年径流量产生了影响,年径流量和泥沙量减少近一半,对保持水土有积极意义。  相似文献