便携式光电望远镜用于流星暴观测的探讨     

顾光德  余月花 《紫金山天文台台刊》1999,18(1):76-79

本文介绍了便携式人卫光电望远镜的主要性能特点,探讨了将其应用于狮子座流星暴观测的可能性。  相似文献   

Spectral index determination between 408 MHz and 5 GHz in the northern sky     

A.W. Jones  R.J. Davis  A. Wilkinson  G. Giardino  S.J. Melhuish  H. Asareh  R.D. Davies  A.N. Lasenby 《Monthly notices of the Royal Astronomical Society》2001,327(2):545-551

We present the joint analysis of two 5-GHz interferometric surveys of the northern sky, taken with different baselines. The two surveys were carried out on the Jodrell Bank 5-GHz interferometer based at Manchester. The Maximum Entropy Method is used to check the consistency of the two surveys and the final two-dimensional maps are used, together with low-frequency full sky surveys, to put constraints on the Galactic spectral index. It is found that synchrotron emission is the dominant process at high Galactic latitudes below 5 GHz.  相似文献   

A moderate-resolution Nasmyth-focus spectrograph of the 6-m BTA telescope     

D. N. Monin  V. E. Panchuk 《Astronomy Letters》2002,28(12):847-852

We report on the development of a fast crossed-dispersion spectrograph (CRAB) mounted at the Nasmyth focus of the 6-m telescope. The spectrograph is designed for visible and near-infrared (3800–10 500 Å) CCD observations with the spectral resolution R=4000. We give the basic parameters of the optical scheme and the parameters of the echelle frame. We determined the gain involved in putting the spectrograph into observational practice and discuss the possible range of spectroscopic problems for which the instrument is optimal.  相似文献   

Multi-station electro-optical observations of the 1999 Leonid meteor storm     

P. Brown  M.D. CampbellR.L. Hawkes  C. TheijsmeijerJ. Jones 《Planetary and Space Science》2002,50(1):45-55

  相似文献   

差分GPS水下立体定位系统   总被引：15，自引：3，他引：15  

王权  程鹏飞  章传银  王泽民  蔡艳辉  丁剑 《测绘科学》2006,31(5):18-19,21

差分GPS水下立体定位系统包括GPS差分基准站、GPS浮标、水下收发机、船基控制中心四部分。差分基准站提供GPS差分改正,实现浮标内置GPS高精度实时定位。GPS浮标完成水上和水下的集成,检测水下收发机发射的定位信号并测量信号到达的时间,同时将各种数据发送到船基控制中心。船基控制中心接收各个浮标的数据后实时解算水下收发机的位置,同时将结果发送给水下收发机。本文首先对系统的总体构成和各个部分的功能进行了介绍,然后详细推导了系统定位算法,最后结合系统试验情况给出了系统试验精度统计结果。  相似文献   

慢滑移及相关脉动和慢地震研究的历史和现状   总被引：1，自引：2，他引：1  

王阎昭  沈正康 《中国地震》2007,23(1):1-9

观测表明,慢滑移事件通常发生在活动断裂带内,为发震层之下的短暂滑移,能够造成地表的瞬态运动。与慢滑移密切相关的慢地震能够发射出频率在一定范围内的脉动信号,但不造成灾害性事件。慢滑移和慢地震很可能是断裂带上形变能释放的基本方式,其观测有可能为人们更深入地了解断裂带的动力学过程提供基础和依据。本文重点介绍近10年来关于慢地震和慢滑移事件的研究历史和现状。目前对慢滑移引发的地表形变和慢地震发射的脉动信号特征有了深入细致的研究,开展了对慢滑移的数值模拟和慢地震定位的研究;但对慢地震和慢滑移发生的位置、两者的关系以及物理机制等方面还存在很多争论和问题。  相似文献   

Do stratocumulus clouds detrain? FIRE I data revisited     

Stephan R. de Roode  Qing Wang 《Boundary-Layer Meteorology》2007,122(2):479-491

Analyses of aircraft observations of the stratocumulus-topped boundary layer during the First ISCCP (International Satellite Cloud Climatology Project) Regional Experiment (FIRE I) show the frequent presence of clear, but relatively moist, air patches near the stratocumulus cloud-top interface. A conditional sampling of measurements in these clear air patches shows that their thermodynamic properties do more resemble boundary-layer air characteristics than those of free troposphere air. From an aircraft leg through cloud tops it is demonstrated that turbulent mixing across the cloud-top interface can lead to the local dissipation of the cloud top. Analogous to the terminology used for shallow cumulus parameterizations this process can be considered as detrainment, with which we mean that after a mixing event across the cloud-top boundaries, mixed unsaturated parcels become part of the clear environment of the cloud.  相似文献   

基于PPP技术的GPS浮标海啸预警模拟研究     

程世来  张小红 《武汉大学学报(信息科学版)》2007,32(9):764-766

提出了利用精密单点定位（precise point positioning,PPP）技术进行海啸预警的方法,并利用TriP软件对实测浮标数据进行了处理,将得出的海面高数据和海啸波模型叠加进行了模拟分析。仿真结果表明,利用精密单点定位技术进行海啸预警,能够监测判断海啸的发生,并获得海啸波到达海岸的波高和时间,提供一定的预警信息。  相似文献   

The ROSAT Brightest Cluster Sample — I. The compilation of the sample and the cluster log N–log S distribution     

H. Ebeling    A. C. Edge    H. Bo¨hringer    S. W. Allen    C. S. Crawford    A. C. Fabian    W. Voges  & J. P. Huchra 《Monthly notices of the Royal Astronomical Society》1998,301(4):881-914

  相似文献   

Red quasars not so dusty     

C. R.Benn  M.Vigotti  R.Carballo  J. I.Gonzalez-Serrano  S. F.SÃ&#;¡nchez 《Monthly notices of the Royal Astronomical Society》1998,295(2):451-456

Webster et al. claimed that up to 80 per cent of QSOs may be obscured by dust. They inferred the presence of this dust from the remarkably broad range of B − K optical–infrared colours of a sample of flat-spectrum PKS radio QSOs. If such dust is typical of QSOs, it will have rendered invisible most of those which would otherwise have been detected by optical surveys. We used the William Herschel Telescope on La Palma to obtain K infrared images of 54 B3 radio QSOs selected at low frequency (mainly steep-spectrum), and we find that although several have very red optical–infrared colours, most of these can be attributed to an excess of light in K rather than a dust-induced deficit in B. We present evidence that some of the infrared excess comes from the light of stars in the host galaxy (some, as previously suggested, comes from synchrotron radiation associated with flat-spectrum radio sources). The B − K colours of the B3 QSOs provide no evidence for a large reddened population. Either the Webster et al. QSOs are atypical in having such large extinctions, or their reddening is not due to dust; either way, the broad range of their B − K colours does not provide evidence that a large fraction of QSOs has been missed from optical surveys.  相似文献