基于改进NCC算法的东南极极记录冰川流速提取研究          下载免费PDF全文

牛牧野周春霞  刘婷婷 《极地研究》2016,28(2):243-249

南极冰川的流速在南极物质平衡研究中有着重要的作用。将SIFT算子的旋转参数引入传统的基于归一化互相关(NCC)的冰川流速提取方法,使其拥有旋转不变的特性。利用此方法,基于Landsat 8 OLI数据对东南极的极记录冰川流速进行了提取,并通过利用模拟影像和NASA发布的MEa SUREs冰川流速结果对该方法的精度进行了验证。结果表明,改进的NCC算法能够在冰川流速方向改变区域提取更多的流速信息,极记录冰川流速最大可达870m·a~(-1),提取结果与MEa SUREs结果相比,平均偏差为23.9 m·a~(-1)。  相似文献   

地球的时变主惯性矩和变化的自转(英文)   总被引：1，自引：0，他引：1  

SHEN Wenbin CHEN Wei SUN RongSHEN Wenbin  School of Geodesy  Geomatics  Wuhan University  Luoyu Road  Wuhan  China  The Key Laboratory of Geospace Environment  Geodesy  Wuhan University  Luoyu Road  Wuhan  China. 《地球空间信息科学学报》2008,(2)

Based on the gravity field models EGM96 and EIGEN-GL04C, the Earth's time-dependent principal moments of inertia A, B, C are obtained, and the variable rotation of the Earth is determined. Numerical results show that A, B, and C have increasing tendencies; the tilt of the rotation axis increases 2.1×10-8 mas/yr; the third component of the rotational angular velocity, ω 3, has a decrease of 1.0×10-22 rad/s2, which is around 23% of the present observed value. Studies show in detail that both θ and ω 3 experience complex fluctua-tions at various time scales due to the variations of A, B and C.  相似文献   

Planetary and figure-figure effects on the moon's rotational motion     

E. Bois  I. Wytrzyszczakz  A. Journet 《Celestial Mechanics and Dynamical Astronomy》1992,53(2):185-201

An accurate theory of the rotation of the Moon has been constructed by numerical integration. All direct perturbations on the Moon's rotational motion have been analysed. The requirements of the current observational accuracy are such that some improvements had to be added to the theoretical models. First, the gravitational figure of the Moon has been developed up to the fifth degree harmonics. Second, mutual potential effects between the figure of the Moon and the figure of the Earth have been expanded farther up. The direct action of planets must be taken into account, its effects being very small but not always negligible. The physical librations resulting of planetary effects and Earth-Moon figure-figure interactions are presented in this paper.  相似文献   

河西走廊地块古生代地层古地磁初步研究     

贺正轩  郑昭昌  朱鸿 《现代地质》1988,2(2):186

古地磁初步研究结果表明,早古生代阶段,河西走廊过渡带与阿拉善地块古纬度接近,且漂移过程中形影相随,说明其间并无洋盆相隔。志留纪末,河西走廊过渡带与阿拉善地块拼接,但二者磁极位置与古方位均有差异,可能表明走廊过渡带相对于阿拉善地块同时作了顺时针旋转。泥盆纪时,两地块古纬度一致,但古方位不同,可能反映在碰撞拼合后二者间仍有相对的旋转运动。二叠纪时,二块体的空间位置及其配置关系已与现状接近。  相似文献   

一种基于扫描线填充算法的分块影像旋转的实现方法     

潘志超  陈换新 《测绘与空间地理信息》2010,33(1):170-171,176

针对分块影像旋转时的效率问题,提出了一种基于扫描线填充算法的实现方法,详细说明了实现步骤,并举例进行了验证。  相似文献   

Matching the frequency spectrum of pre-main sequence stars by means of standard and rotating models     

M. Di Criscienzo  P. Ventura  F. D'Antona  M. Marconi  A. Ruoppo  V. Ripepi 《Monthly notices of the Royal Astronomical Society》2008,389(1):325-332

We applied the aton evolutionary code to the computation of detailed grids of standard (non-rotating) and rotating pre-main sequence (PMS) models and computed their adiabatic oscillation spectra, with the aim of exploring the seismic properties of young stars. As, until now, only a few frequencies have been determined for ∼40 PMS stars, the way of approaching the interpretation of the oscillations is not unique. We adopt a method similar to the matching mode method by Guenther and Brown making use, when necessary, also of our rotating evolutionary code to compute the models for PMS stars. The method is described by a preliminary application to the frequency spectrum of two PMS stars (85 and 278) in the young open cluster NGC 6530. For the Star 85, we confirm with self-consistent rotating models, previous interpretation of the data, attributing three close frequencies to the mode   n = 4, l = 1  and   m = 0  , +1 and −1. For the Star 278, we find a different fit for the frequencies, corresponding to a model within the original error box of the star, and dispute the possibility that this star has a T _eff much cooler that the red boundary of the radial instability strip.  相似文献   

大气对地球自转季节性变化的贡献   总被引：2，自引：0，他引：2  

虞南华  郑大伟 《天文学报》2000,41(2):148-152

采用１９７９－１９９５年期间新的大气角动量资料,研究了大气在季节性时间尺度上对日长变化和极移的贡献。结果表明,考虑了风和大气压的贡献后,大气在周年和半年时间尺度上对日长变化的贡献分别可达９５％和８８％。同时还给出了大气对极移激发的定量结果,其中,大气的周年尺度上对极移Ｘ分同的贡献为１６％,对Ｙ分量的贡献为４３％;在半年尺度上海洋的贡献,才能进上步解决地球自转激发的问题。  相似文献   

Scaling of motion and governing equations for baroclinic large-scale motions in equatorial ocean     

Fan Zhisong  Pu Shuzhen 《海洋学报(英文版)》2000,19(1):15-24

PROPOSALOFPROBLEMTheequatorialoceanicdynamicsintightconnectionwiththeEINinoeventshasbeenthefocusoftheoceanographer'sattention.Asabasisofequatorialoceanicdynamics,theconventionaltheoryoftheequatoriallytrappedwaves,whichwerefertothetrappedwavetheoryinextensiveliteratureuptodate(Matsuno,1966;Blandford,1966;MunkandMoors,1968;WunschandGill,1976;MoorsandPhilandet,1977;Eriksen,1985;Pedlosky,1987),hasbeenprogressivelydevelopedandemployed.However,thedetailedinvestigationsrevealthattheproper…  相似文献   

Rotation, planets, and the 'second parameter' of the horizontal branch     

Noam Soker  Amos Harpaz 《Monthly notices of the Royal Astronomical Society》2000,317(4):861-866

We analyse the angular momentum evolution from the red giant branch (RGB) to the horizontal branch (HB) and along the HB. Using rotation velocities for stars in the globular cluster M13, we find that the required angular momentum for the fast rotators is up to 1–3 orders of magnitude (depending on some assumptions) larger than that of the Sun. Planets of masses up to 5 times Jupiter's mass and up to an initial orbital separation of ~2 au are sufficient to spin-up the RGB progenitors of most of these fast rotators. Other stars have been spun-up by brown dwarfs or low-mass main-sequence stars. Our results show that the fast rotating HB stars have been probably spun-up by planets, brown dwarfs or low-mass main-sequence stars while they evolved on the RGB. We argue that the angular momentum considerations presented in this paper further support the 'planet second parameter' model. In this model, the 'second parameter' process, which determines the distribution of stars on the HB, is interaction with low-mass companions, in most cases with gas-giant planets, and in a minority of cases with brown dwarfs or low-mass main-sequence stars. The masses and initial orbital separations of the planets (or brown dwarfs or low-mass main-sequence stars) form a rich spectrum of different physical parameters, which manifests itself in the rich varieties of HB morphologies observed in the different globular clusters.  相似文献   

Differential Pulse Polarographic Determination of the Oxime Carbamante Insecticide Alanycarb     

Recai &#x;nam  Esma iek 《洁净——土壤、空气、水》2009,37(1):75-79

As basis for the development of a sensitive analytical method for the determination of the insecticide alanycarb, a study of the differential pulse polarographic (DPP) reduction of alanycarb on a dropping mercury electrode (DME) was performed. The pesticide was found to give a single DP peak over the pH range 1.0 to 6.0 and the pH dependency of the peak potential showed a linear segment with a slope of 65.2 mV (at 20°C). For the analytical DPP method running at pH 6.0 (peak at –503.4 mV), the relationship between the peak current and alanycarb concentration was linear in the range of 1.10 to 9.76 μg mL^–1 with a detection limit of 0.33 μg mL^–1. The proposed method was applied for the determination of alanycarb in spiked dam water and orange juice samples. The recoveries calculated for both types of dam water and orange juice samples spiked with 12.0 μg mL^–1 alanycarb were 96.3 and 99.0% with relative standard deviations of 5.2 and 1.3%, respectively. The sufficiently good recoveries and low relative standard deviations for the data reflect the high accuracy and precision of the proposed differential pulse polarographic method. The effects of diverse metal ions and other commonly used pesticides on the determination of alanycarb were also investigated.  相似文献