The geophysical approach towards the nutation of a rigid Earth

被引:12
作者
Hartmann, T
Soffel, M
Ron, C
机构
[1] Univ Tubingen, D-72076 Tubingen, Germany
[2] Lohrmann Observ, Inst Planetare Geodasie, D-01062 Dresden, Germany
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1999年 / 134卷 / 02期
关键词
celestial mechanics; stellar dynamics; reference system; Earth;
D O I
10.1051/aas:1999139
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper presents the new and complete series named H96NUT for the nutation of a rigid Earth model. In contrast to the traditional computation method, the nutation is calculated here indirectly via the new and highly accurate tidal potential development recently given by Hartmann & Wenzel (1995a,b), (HW95). All contributions up to 0.45 mu as were taken into account leading to 699 nutation terms separated after origin (or 607 terms summed according to the same arguments). These are: the main terms due to the Moon, the Sun and the planets; indirect planetary effects, effects due to the triaxiality of the Earth, effects due to the J(3) and J(4) geopotential, the geodesic nutation and second order terms. Nutation series for the angular momentum axis, the figure axis and the rotation axis are derived. they are in good agreement with those given in Roosbeek & Dehant (1997) with exception of several terms whose cause is discussed. Modern constants (like the precession constant) have been used throughout. The value for the dynamical ellipticity H(dyn), which is compatible with these computations, is H(dyn) = 3.273 792 489 10(-3). In addition, some other values related with precession are also deduced from the tidal potential. One main advantage of this work is that a completely independent analytical computation method has been established which is extensively described here (see also Hartmann (1996) for more details) and which provides - besides a numerical calculation - a useful validation of existing nutation series.
引用
收藏
页码:271 / 286
页数:16
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