气象无线传感网观测节点的设计与实现     

张亚  罗希昌  陈浩  江春 《气象科技》2015,43(6):1046-1052

针对传统自动气象站对电力和通讯基础设施依赖性强,应用环境受到限制的问题,设计并实现了一种基于无线传感器网络的气象观测节点。气象观测节点的硬件系统以CC2530芯片为核心,使用锂电池供电,通过模拟和数字接口连接气象传感器,射频部分工作在2.4 GHz。软件系统以TinyOS操作系统为基础,开发了基于LEPS协议的多跳路由协议和气象传感器驱动程序。在野外环境中对气象观测节点的功耗、通信距离、传感器及组网性能进行了测试。测试结果表明,气象观测节点在没有电力和通信基础设施的环境中能够形成一个稳定的多跳自组织数据采集与传输网络,适合在高山、海岛、沙漠等艰苦地区进行部署和应用。  相似文献   

Analysis of Boundary-Layer Statistical Properties at Dome C,Antarctica     

Jean-François Rysman  Sébastien Verrier  Alain Lahellec  Christophe Genthon 《Boundary-Layer Meteorology》2015,156(1):145-155

  相似文献   

Effect of snow cover on pan-Arctic permafrost thermal regimes     

Hotaek Park  Alexander N. Fedorov  Mikhail N. Zheleznyak  Pavel Y. Konstantinov  John E. Walsh 《Climate Dynamics》2015,44(9-10):2873-2895

This study quantitatively evaluated how insulation by snow depth (SND) affected the soil thermal regime and permafrost degradation in the pan-Arctic area, and more generally defined the characteristics of soil temperature (T_SOIL) and SND from 1901 to 2009. This was achieved through experiments performed with the land surface model CHANGE to assess sensitivity to winter precipitation as well as air temperature. Simulated T_SOIL, active layer thickness (ALT), SND, and snow density were generally comparable with in situ or satellite observations at large scales and over long periods. Northernmost regions had snow that remained relatively stable and in a thicker state during the past four decades, generating greater increases in T_SOIL. Changes in snow cover have led to changes in the thermal state of the underlying soil, which is strongly dependent on both the magnitude and the timing of changes in snowfall. Simulations of the period 2001–2009 revealed significant differences in the extent of near-surface permafrost, reflecting differences in the model’s treatment of meteorology and the soil bottom boundary. Permafrost loss was greater when SND increased in autumn rather than in winter, due to insulation of the soil resulting from early cooling. Simulations revealed that T_SOIL tended to increase over most of the pan-Arctic from 1901 to 2009, and that this increase was significant in northern regions, especially in northeastern Siberia where SND is responsible for 50 % or more of the changes in T_SOIL at a depth of 3.6 m. In the same region, ALT also increased at a rate of approximately 2.3 cm per decade. The most sensitive response of ALT to changes in SND appeared in the southern boundary regions of permafrost, in contrast to permafrost temperatures within the 60°N–80°N region, which were more sensitive to changes in snow cover. Finally, our model suggests that snow cover contributes to the warming of permafrost in northern regions and could play a more important role under conditions of future Arctic warming.  相似文献   

热带印度洋海温与西北地区东部降水关系研究   总被引：2，自引：0，他引：2  

杨建玲  李艳春  穆建华  王素艳  王敏  田磊 《高原气象》2015,(3):690-699

利用西北地区东部1961 2009年99个气象测站逐月降水量资料,以及Hardley中心逐月海表面温度(SST)资料,采用最大协方差分析(MCA)、相关、回归等统计方法,考虑扣除ENSO(El Ni珘noSouthern Oscillation)影响后,分析了西北地区东部降水量和热带印度洋SST之间年际、年代际变化关系。结果表明:前期冬、春季持续异常的热带印度洋海盆模与西北地区东部5月降水异常主模态存在显著正相关关系,通常超前1~2个季节的暖(冷)海盆模对应5月西北地区东部降水偏多(少),并且这种显著关系存在年代际差异,20世纪70年代中期之前两者关系不显著,之后两者关系加强,通过了0.05显著性水平检验。热带印度洋海盆模对西北地区东部5月降水的影响可能是热带印度洋海盆模"电容器"效应的一种具体体现。  相似文献   

Cosmological and astrophysical neutrino mass measurements     

K.N. AbazajianE. Calabrese  A. CoorayF. De Bernardis  S. Dodelson  A. FriedlandG.M. Fuller  S. HannestadB.G. Keating  E.V. Linder  C. LunardiniA. Melchiorri  R. Miquel  E. PierpaoliJ. Pritchard  P. SerraM. Takada  Y.Y.Y. Wong 《Astroparticle Physics》2011,35(4):177-184

Cosmological and astrophysical measurements provide powerful constraints on neutrino masses complementary to those from accelerators and reactors. Here we provide a guide to these different probes, for each explaining its physical basis, underlying assumptions, current and future reach.  相似文献   

Elemental abundance analyses with DAO spectrograms. XXVIII. Comparisons with two series of automated elemental abundance analyses     

K. Yüce  S.J. Adelman  A.F. Gulliver 《New Astronomy》2011,16(3):191-193

We compare the results of our series of fine analyses based on Dominion Astrophysical Observatory long camera coudé spectra with those of the same stars from the series of automated elemental abundance analyses by Hill (1995) and by Erspamer and North (2003). We usually find good agreement with the results of the first paper for those elements with well-determined abundances and somewhat poorer agreement with results of the second paper.  相似文献   

Nonradial eruption of a kinking filament observed from STEREO     

Y. Bi  Y.C. Jiang  L.H. Yang  R.S. Zheng 《New Astronomy》2011,16(4):276-283

On 5 April 2008, a filament at the periphery of an active region was observed by the Extreme Ultraviolet Imager telescope aboard the STEREO-A spacecraft, which showed up as a prominence eruption in the field-of-view from STEREO-B. The filament at STEREO-A 304 Å was first lengthened toward a region with weak overlying magnetic field so evolved as a large-scale one consisting of bright and dark threads twisting with each other, and then the portion below the weak field underwent an eruption. Meanwhile, the corresponding STEREO-B 304 Å prominence threads exhibited a kinking structure and tilting motion, with its center deflecting from the radial direction. By using three-dimension (3D) reconstruction technology, we obtain the 3D topology for the kinked prominence when its apex arrived at 1.4 radii, from which a clockwise rotation of about 90° is found in the course of the eruption. By comparing the 3D structure with the magnetic-field configuration computed by using the Potential-Field Source-Surface (PFSS) model, it is suggested that the filament erupted against the rather weaker than stronger overlying magnetic field, which make it appear to tilt toward one side.  相似文献   

Ten CoRoT eclipsing binaries: Photometric solutions     

S.C. Maciel  Y.F.M. Osorio  J.R. De Medeiros 《New Astronomy》2011,16(2):68-71

Ten eclipsing binaries, identified in the scope of the CoRoT Space Mission, were selected for analysis. The photometric light curves were processed and analyzed, resulting in the first study of eclipsing binary candidates with their possible photometric solution, in the context of the above-mentioned Space Mission. The selected targets are detached and overcontact systems, for which we computed 2MASS temperatures, in addition to different physical parameters, including orbital period, orbit inclination angle, and temperatures, radius and luminosity ratios. This study reveals a large diversity of eclipsing binary systems obtained from the CoRoT data.  相似文献   

A class of well behaved charged superdense star models of embedding class one     

Y. K. Gupta  Jitendra Kumar 《Astrophysics and Space Science》2011,336(2):419-426

A class of well behaved charged superdense star models of embedding class one is obtained by taking perfect fluid to be interior matter. In the process we come across the models for white dwarf, quark and neutron stars. Maximum mass of the star of this class is found to be 6.716998M _Θ with its radius is 18.92112 Km. In the absence of charge the models reduce to Schwarzchild’s interior model with constant density.  相似文献   

A class of well behaved charged analogues of Vaidya–Tikekar type super-dense star     

Y. K. Gupta  Jitendra Kumar 《Astrophysics and Space Science》2011,334(2):273-279

In the present article a model of well behaved charged superdense star with surface density 2×10¹⁴ gm/cm³ is constructed by considering a static spherically symmetric metric with t=const hypersurfaces as hyperboloid. So far well behaved model described by such metric could not be obtained. Maximum mass of the star is found to be 0.343457M _⊙ and the corresponding radius is 9.57459 km. The red shift at the centre and on the surface are given as 0.068887 and 0.031726 respectively.  相似文献