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国家自然科学基金(J1210039)

作品数:11 被引量:5H指数:2
相关作者:谢懿刘景昊张羽飞黄勇黄永锋更多>>
相关机构:南京大学中国科学院上海天文台更多>>
发文基金:国家自然科学基金国家教育部博士点基金国家重点基础研究发展计划更多>>
相关领域:天文地球文化科学更多>>

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11 条 记 录,以下是 1-10
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A revised rotation curve of the Milky Way with maser astrometry
2013年
We reconstruct the rotation curve of the Milky Way using the new trigono-metric parallax and proper motion data for masers in 43 high-mass star-forming re-gions obtained by VLBI, as well as the existing data from the literature, based on a new set of galactic constants (R0, -0) = (8.4 kpc, 254 km s^-1) measured by Reid et al. The revised rotation curve of the Milky Way is almost fiat or slightly rising in the region from about 6 to 15 kpc. The rotation velocities within 5 kpc of the Galactic center, as determined by VLBI, differ from those obtained by measurement of the HI-and CO-line tangent velocities. We fitted the revised rotation curve arising from three mass components: the bulge, disk and dark matter halo. The total mass of the Milky Way is found to be 2.3× 10^11 M⊙ (20 kpc). This is about 10% larger than that from Sofue et al, and is comparable with the mass of M31, 3.4× 10^11 M⊙ (35 kpc), given by Carignan et al. The limited accurate observational data, especially the VLBI data, do not permit a fully satisfactory fit to the rotation curve. The extensive par-allax and proper motion data that will be produced by the Bar and Spiral Structure Legacy Survey project in the next few years should lead to considerable progress in understanding the rotation curve and dark matter halo of the Milky Way.
Xiao-Sheng XinXing-Wu Zheng
利用“火星快车”三程多普勒跟踪数据限定局部洛伦兹不变性
2015年
目前航天器的三程多普勒跟踪技术已经在深空探测的控制与导航领域起到了重要作用。利用包含了对局部洛伦兹不变性(LLI)以及局部位置不变性(LPI)原理有破坏的三程多普勒跟踪理论,研究分析了"火星快车"(MEX)三程多普勒跟踪数据的残差。这些多普勒观测于2009年8月7日和8日进行,利用了欧洲航天局(ESA)在澳大利亚新诺舍(New Norcia)的上行站和三个分别在中国上海、昆明以及乌鲁木齐的下行站。我们发现,这些观测结果给出的LLI上限在10-2的量级。但由于各观测站本身对频率测量的精度有限,这些数据并不适合于检验LPI。
张羽飞刘景昊黄勇谢懿
关键词:引力多普勒跟踪
天文自适应光学系统实验教学设计
2022年
把天文科学前沿技术引入本科实验教学,开发设计了用于天文专业本科实验教学的自适应光学系统,包含了可变形镜、波前传感器、激光装置等关键设备。通过设计搭建自适应光学系统平台,将科研成果融入实验教学,帮助学生了解自适应光学系统的原理、架构与功能,在培养学生创新意识和开拓科学视野方面发挥了很好的作用。
彭志欣陈亮
关键词:自适应光学
Relativistic time transfer for a Mars lander: from Areocentric CoordinateTime to Barycentric Coordinate Time
2017年
As the second step of relativistic time transfer for a Mars lander,we investigate the transformation between Areocentric Coordinate Time(TCA)and Barycentric Coordinate Time(TCB)in the framework of IAU Resolutions.TCA is a local time scale for Mars,which is analogous to the Geocentric Coordinate Time(TCG)for Earth.This transformation has two parts:contributions associated with gravitational bodies and those depending on the position of the lander.After setting the instability of an onboard clock to 10;and considering that the uncertainty in time is about 3.2 microseconds after one Earth year,we find that the contributions of the Sun,Mars,Jupiter and Saturn in the leading term associated with these bodies can reach a level exceeding the threshold and must be taken into account.Other terms can be safely ignored in this transformation for a Mars lander.
Wen-Zheng YangDe-Wang XuQing-Shan YuJie LiuYi Xie
南京大学天文与空间科学学院本科人才培养创新举措
2013年
阐述了南京大学天文与空间科学学院在施行"三三制"本科教学改革以来,依托教育部实施的"基础学科拔尖学生培养试验计划",结合学科特色,逐步形成的一套独特的、适合天文与空间科学学科特点的本科人才培养模式.该模式重视学生的个性特征和多元化发展需求,强调通识教育,突出了对国际视野和创新能力的培养.
杨艳黄永锋
关键词:本科人才培养
Preliminary limits on deviation from the inverse-square law of gravity in the solar system:a power-law parameterization
2014年
New physics beyond the standard model of particles might cause a deviation from the inverse-square law of gravity. In some theories, it is parameterized by a power-law correction to the Newtonian gravitational force, which might originate from the simultaneous exchange of particles or modified and extended theories of gravity. Using the supplementary advances of the perihelia provided by INPOP 10a (IMCCE, France) and EPM2011 (IAA RAS, Russia) ephemerides, we obtain preliminary limits on this correction. In our estimation, we take the Lense-Thirring effect due to the Sun's angular momentum into account. The parameters of the power-law correction and the uncertainty of the Sun's quadrupole moment are simultaneously estimated with the method of minimizing X2. From INPOP10a, we find N - 0.605 for the exponent of the power-law correction. However, from EPM2011, we find that, although it yields N = 3.001, the estimated uncertainty in the Sun's quadrupole moment is much larger than the value given by current observations. This might be caused by the intrinsic nonlinearity in the power-law correction, which makes the estimation very sensitive to the supplementary advances of the perihelia.
Meng-Yao LiuZe-Hao ZhongYi-Chen HanXiao-Yu WangZong-Shui YangYi Xie
A two-step energy injection explanation for the rebrightenings of the multi-band afterglow of GRB 081029被引量:2
2013年
The afterglow of GRB 081029 showed unusual behavior, with a signifi- cant rebrightening being observed at the optical wavelength at about 3000 s after the burst. One possible explanation is that the rebrightening resulted from an energy in- jection. Here we present a detailed numerical study of the energy injection process and interpret the X-ray and optical afterglow light curves of GRB 081029. In our model, we have assumed two periods of energy injection, each with a constant injec- tion power. One injection starts at 2.8 × 10^3 s and lasts for about 2500 s, with a power of 7.0 × 10^47 erg s-1. This energy injection mainly accounts for the rapid rebrighten- ing at about 3000 s. The other injection starts at 8.0 × 10^3 s and lasts for about 5000 s. The injection power is 3.5 × 10^47 erg s-1. This energy injection can help to explain the slight rebrightening at about 10 000 s. It is shown that the observed optical after- glow, especially the marked rebrightening at about 3000 s, can be reproduced well. In the X-ray band, the predicted amplitude of the rebrightening is much shallower, which is also consistent with the observed X-ray afterglow light curve. It is argued that the two periods of energy injection can be produced by clumpy materials falling onto the central compact object of the burster, which leads to an enhancement of accretion and gives rise to a strong temporary outflow.
Yong-Bo YuYong-Feng Huang
火星任务中星上原时τ与TCG的相对论变换被引量:3
2015年
爱因斯坦的广义相对论已成为当今深空探测任务中一部分,为此将在研究环火星探测器星载钟原时τ与地球质心坐标时(TCG)的变换中应用相对论变换关系,将τ与地球相关联的局部时间尺度联系起来,从而扩展了之前关于τ与太阳系质心坐标时(TCB)相对论变换的工作(TCB是应用于整个太阳系的全局坐标时)。研究发现τ和TCG的差在经历一年的时间后可达到0.2s量级。为了区分相对论变换中各种效应的贡献,用数值方法计算了太阳、八大行星、三个大质量小行星以及探测器的贡献。发现在精确到1μs量级下,相对论变换必须包括太阳、金星、月球、火星、木星、土星的引力影响以及探测器和地球的速度影响。
潘军洋谢懿
关键词:参考系空间探测器
Parametrized post-Newtonian secular transit timing variations for exoplanets
2013年
Ground-based and space-borne observatories used for studying exoplanet transits now and in the future will considerably increase the number of exoplanets known from transit data and the precision of the measured times of transit minima.Variations in the transit times can not only be used to infer the presence of additional planets,but might also provide opportunities to test the general theory of relativity in these systems.To build a framework for these possible tests,we extend previous studies on the observability of the general relativistic precessions of periastron in transiting exoplanets to variations in secular transit timing under parametrized post-Newtonian formalism.We find that if one can measure the difference between observed and predicted variations of general relativistic secular transit timing to 1 s yr-1in a transiting exoplanet system with a Sun-like mass,a period of;day and a relatively small eccentricity of;.1,general relativity will be tested to the level of;%.
Shan-Shan ZhaoYi Xie
Relativistic time transfer for a Mars lander:from proper time to Areocentric Coordinate Time
2016年
As the first step in relativistic time transfer for a Mars lander from its proper time to the time scale at the ground station, we investigate the transformation between proper time and Areocentric Coordinate Time (TCA) in the framework of IAU Resolutions. TCA is a local time scale for Mars, which is analogous to the Geocentric Coordinate Time (TCG) for Earth. This transformation contains two contributions: inter- hal and external. The internal contribution comes from the gravitational potential and the rotation of Mars. The external contribution is due to the gravitational fields of other bodies (except Mars) in the Solar System. When the (in)stability of an onboard clock is assumed to be at the level of 10-13, we find that the internal contribution is dominated by the gravitational potential of spherical Mars with necessary corrections asso- ciated with the height of the lander on the areoid, the dynamic form factor of Mars, the flattening of the areoid and the spin rate of Mars. For the external contribution, we find the gravitational effects from other bodies in the Solar System can be safely neglected in this case after calculating their maximum values.
De-Wang XuQing-Shan YuYi Xie
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