Earth rotation parameter estimation from LLR

verfasst von
Vishwa Vijay Singh, Liliane Biskupek, Jürgen Müller, Mingyue Zhang
Abstract

LLR measures the distance between observatories on Earth and retro-reflectors on Moon since 1969. In this paper, we estimate the Earth Rotation Parameters (ERP; terrestrial pole offsets, xp and yp, and Earth rotation phase, ΔUT) using LLR data. We estimate the values of ΔUT, and the pole offsets separately. For the pole offsets, we estimate the values of xp and yp together and separately. Overall, the uncertainties of ERP from the new LLR data (after 2000.0) have significantly improved, staying less than 20 μs for ΔUT, less than 2.5 mas for xp, and less than 3 mas for yp for nights selected from subsets of the LLR time series which have 10 and 15 normal points obtained per night. Furthermore, we add the non-tidal loading effect provided by the IMLS, as observation level corrections of the LLR observatories in the analysis. This effect causes deformations of the Earth surface up to the centimetre level. Its addition in the Institute of Geodesy (IfE) LLR model, leads to a marginal improvement in the uncertainties (3-σ values) of about 1% for both, ΔUT and the pole offsets.

Organisationseinheit(en)
Institut für Erdmessung
QuantumFrontiers
Externe Organisation(en)
DLR-Institut für Satellitengeodäsie und Inertialsensorik
Typ
Artikel
Journal
Advances in Space Research
Band
70
Seiten
2383-2398
Anzahl der Seiten
16
ISSN
0273-1177
Publikationsdatum
15.10.2022
Publikationsstatus
Veröffentlicht
Peer-reviewed
Ja
ASJC Scopus Sachgebiete
Luft- und Raumfahrttechnik, Astronomie und Astrophysik, Geophysik, Atmosphärenwissenschaften, Astronomie und Planetologie, Erdkunde und Planetologie (insg.)
Elektronische Version(en)
https://arxiv.org/abs/2110.14274 (Zugang: Offen)
https://doi.org/10.1016/j.asr.2022.07.038 (Zugang: Offen)