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Earth’s precession–nutation motion: the error analysis of the theories IAU 2000 and IAU 2006 applying the VLBI data of the years 1984–2006

机译:地球的岁差-运动:利用1984-2006年的VLBI数据对IAU 2000和IAU 2006理论进行的误差分析

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摘要

The long-term systematic errors of the analytical theories IAU 2000 and IAU 2006 of the Earth’s precession–nutational motion are studied making use of the VLBI data of 1984–2007. Several independent methods give indubitable evidence of the significant quadratic error ${dphi = (23 pm 3),{rm mas/cy}^2}$ in the IAU 2000 residuals of the precessional angle ${phi}$ while the adopted value of the secular decrease ${dot e=-7.9times 10^{-9}}$ /cy of the Earth’s ellipticity e (derived from Satellite Laser Ranging data) should manifest itself in the residuals of ${phi}$ as the negative quadratic trend ${dphi_{dot e} approx -8,{rm mas}/{cy}^2}$ . The problem with the precession of the IAU 2006 theory adopted as a new international standard and based on the precession model P03 (Capitaine et al., Astron Astrophys 432:355–367, 2005) appears to be even more serious because the above mentioned quadratic term ${dphi_{dot e}}$ has already been incorporated into the P03 precession. Our analysis of the VLBI data demonstrates that the quadratic trend of the IAU 2006 residuals ${dphi}$ does amount to the expected value (30.0 ± 3) mas/cy2. It means, first, that the theoretical precession rate of IAU 2006 should be augmented by the large secular correction ${dp_s=2 dphi approx(60.0 pm 6) {rm mas/cy}^2}$ and, second, that the available VLBI data have potentiality of estimating the rate ${dot e}$ . And indeed, processing these data by the numerical theory ERA of the Earth’s rotation (Krasinsky, Celest Mech Dyn Astron 96:169–217, 2006, Krasinsky and Vasilyev, Celest Mech Dyn Astron 96:219–237, 2006) yields the estimate ${dot e=-(14 pm 4)times 10^{-9}}$ /cy statistically in accordance with the satellite-based ${dot e}$ . On the other hand, applying IAU 2000/2006 models, the positive value ${dot e=(27 pm 4)times 10^{-9}}$ /cy is found which is incompatible with the SLR estimate and, evidently, has no physical meaning. The large and steadily increasing error of the precession motion of the IAU 2006 theory makes the task of replacing IAU 2006 by a more accurate model be most pressing.
机译:利用1984-2007年的VLBI数据研究了地球进动-运动的分析理论IAU 2000和IAU 2006的长期系统误差。几种独立的方法给出了进动角$ {phi} $的IAU 2000残差中显着二次误差$ {dphi =(23 pm 3),{rm mas / cy} ^ 2} $的不容置疑的证据,而采用的是地球椭圆度e(根据卫星激光测距数据得出)的长期下降$ {dot e = -7.9乘以10 ^ {-9}} $ / cy应显示在$ {phi} $的残差中,作为负二次方趋势$ {dphi_ {dot e}约为-8,{rm mas} / {cy} ^ 2} $。 IAU 2006理论的进动问题被采纳为新的国际标准,并基于进动模型P03(Capitaine等人,Astron Astrophys 432:355-367,2005)而出现的问题似乎更加严重,因为上述二次方术语$ {dphi_ {dot e}} $已被合并到P03进动中。我们对VLBI数据的分析表明,IAU 2006残差$ {dphi} $的二次趋势确实等于mas / cy2 的期望值(30.0±3)。这意味着,首先,应该通过大的长期校正$ {dp_s = 2 dphirox(60.0 pm 6){rm mas / cy} ^ 2} $来增加IAU 2006的理论进动率,其次,可用VLBI数据具有估算速率$ {dot e} $的潜力。实际上,通过地球自转的数值理论ERA处理这些数据(Krasinsky,Celest Mech Dyn Astron 96:169-217、2006,Krasinsky和Vasilyev,Celest Mech Dyn Astron 96:219-237、2006)得出估算值$根据基于卫星的$ {dot e} $,{dot e =-((4 pm pm)4)乘以10 ^ {-9}} $ / cy。另一方面,使用IAU 2000/2006模型,发现正值$ {dot e =(27 pm 4)乘以10 ^ {-9}} $ / cy与SLR估计值不兼容,并且显然具有没有物理意义。 IAU 2006理论进动的巨大且稳定的误差使以更精确的模型代替IAU 2006的任务成为最紧迫的任务。

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