Variation of the equatorial moments of inertia associated with a 6-year westward rotary motion in the Earth
Introduction
A 6-year (or 5.9-year to be more precise) westward-propagating rotary wave-2 motion (a wave with azimuthal wavenumber 2) was observed in the Earth's surface deformation field and geomagnetic field (Ding and Chao, 2018). This wave-2 motion consists of a diagonal double-peak pattern making a westward half-round in 6 years around the globe along the equatorial plane, kinematically analogous to a westward-propagating semi-diurnal tide wave except the period is 6 years rather than ∼12 hours. The equatorial double peak is in the form of spatial sectoral spherical harmonic of degree 2 and order 2 (henceforth abbreviated as ). Ding and Chao (2018) proposed a causal connection of this wave-2 motion with the inner-core axial torsional libration (ATL) associated in turn with the 6-year oscillation that is observed in the Earth's length-of-day (Chao, 2017, and references therein). The proposed cause of the ATL is the mantle-inner core gravitational (MICG) restoring torque dictated by the product of the two [2, 2] density multipoles – the interior-type sectoral quadrupole belonging to the mantle and the exterior-type belonging to the inner core (Chao, 2017; see below).
The wave-2 deformation observed in GPS (Global Positioning System) should produce corresponding variations in the gravitational field, and the gravitational signature would reside in the component embodied in the spherical-harmonic Stokes coefficients and of the Earth's external gravitational field. The Stokes coefficients are the (normalized) exterior-type multipoles (Chao and Gross, 1987). In particular, and , or the external-type sectoral quadrupole, are closely related to the two equatorial moments of inertia, A and B (see below). Therefore in this paper we target the and (Δ denoting temporal variation referenced to the mean value) obtained from the satellite laser-ranging (SLR) technique and, to a lesser extent, the GRACE satellite, and focus on their temporal amplitude signatures at the 6-year period. The goal is to be able to detect the signals in and that are expected of the ΔA and ΔB associated with the said deformation in the Earth. Conversely, the quantitative identification of such signals in and would then corroborate the scenario of the 6-year westward wave-2 motion.
Section snippets
Theoretical formulation and predictions
It is customary to express the Earth's external gravitational potential field V in spherical-harmonic expansion referenced to the Earth's mean radius R (Kaula, 1966): at field point r = (radius r, co-latitude θ, East longitude λ) in spherical coordinates, where is the 4π-normalized associated Legendre function; the expansion coefficients and are the th Strokes coefficients of
Observational data and analysis
Low-degree Stokes coefficients of the Earth's external gravity field have been measured by the satellite laser-ranging (SLR) techniques for decades (Pearlman et al., 2002). In particular, the temporal variation of the most prominent coefficient, or the oblateness parameter , has been well observed since the late 1970s (e.g., Cheng and Tapley, 2004). The SLR determination of the variations and (on the order of 10−9) has only become adequately precise since after 1990. In
Discussion and conclusions
Previous study (Ding and Chao, 2018) of a westward-propagating wave-2 displacement field in the mantle predicts a retrograde variation of the sectoral quadrupole or the Earth's gravitational Stokes coefficients and , which in turn signifies a corresponding variation in the Earth's two equatorial principle moments of inertia. In this paper we search such predicted 6-year variations in and monthly data series that have been available from SLR since early 1990s now spanning
Declaration of Competing Interest
The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.
Acknowledgments
The SLR Stokes coefficient data are provided by the Space Research Institute (IWF) of the Austrian Academy of Sciences via website http://geodesy.iwf.oeaw.ac.at/d_slr_monthly.html, based on SLR observations coordinated by ILRS (https://ilrs.cddis.eosdis.nasa.gov/). The GRACE satellite data are available by ftp://podaac-ftp.jpl.nasa.gov/allData/grace/L2/CSR/RL06. We thank Hao Ding for discussion and Yuwen Li for assistance in data preparation. This work is supported by Taiwan Ministry of Science
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