Contribution of Starlette, Stella, and AJISAI to the SLR-derived global reference frame

The contribution of Starlette, Stella, and AJI-SAI is currently neglected when defining the International Terrestrial Reference Frame, despite a long time series of precise SLR observations and a huge amount of available data. The inferior accuracy of the orbits of low orbiting geodetic satellites is the main reason for this neglect. The Analysis Centers of the International Laser Ranging Service (ILRS ACs) do, however, consider including low orbiting geodetic satellites for deriving the standard ILRS products based on LAGEOS and Etalon satellites, instead of the sparsely observed, and thus, virtually negligible Etalons. We process ten years of SLR observations to Starlette, Stella, AJISAI, and LAGEOS and we assess the impact of these Low Earth Orbiting (LEO) SLR satellites on the SLR-derived parameters. We study different orbit parameterizations, in particular different arc lengths and the impact of pseudo-stochastic pulses and dynamical orbit parameters on the quality of the solutions. We found that the repeatability of the East and North components of station coordinates, the quality of polar coordinates, and the scale estimates of the reference are improved when combining LAGEOS with low orbiting SLR satellites. In the multi-SLR solutions, the scale and the Z component of geocenter coordinates are less affected by deficiencies in solar radiation pressure modeling than in the LAGEOS-1/2 solutions, due to substantially reduced correlations between the Z geocenter coordinate and empirical orbit parameters. Eventually, we found that the standard values of Center-of-mass corrections (CoM) for geodetic LEO satellites are not valid for the currently operating SLR systems. The variations of station-dependent differential range biases reach 52 and 25 mm for AJISAI and Starlette/Stella, respectively, which is why estimating station dependent range biases or using station-dependent CoM, instead of one value for all SLR stations, is strongly recommended.This clearly indicates that the ILRS effort to produce CoM corrections for each satellite, which are site-specific and depend on the system characteristics at the time of tracking,is very important and needs to be implemented in the SLR data analysis.

Giovanna Stella, Brustbild

Signatur des Originals: S 36/F01907

Helena Forti, Rollenbild, Hüftbild, in: Alfred Kaiser: Stella Maris

Signatur des Originals: S 36/F03743

Stella Hohenfels als Iphigenie, Rollenbild, Brustbild, in: Johann Wolfgang von Goethe: Iphigenie auf Tauris, Burgtheater Wien, 1900

Signatur des Originals: S 36/F04548

Stella Hohenfels, Rollenbild

Signatur des Originals: S 36/F04549

Stella Hohenfels als Nymphas, Rollenbild, in: Adolf von Wilbrandt: Der Meister von Palmyra

Signatur des Originals: S 36/F04550

Eva Plaschke-von der Osten als Stella, Rollenbild, Brustbild

Signatur des Originals: S 36/F05627

Eva Plaschke-von der Osten als Stella, Rollenbild, Brustbild

Signatur des Originals: S 36/F05629

Stella Hohenfels, Rollenbild, in: William Shakespeare: Ein Sommernachtstraum

Signatur des Originals: S 36/F08845

Stella Hohenfels als Fräulein von Seiglière, Rollenbild, in: Jules Sandeau: Das Fräulein von Seiglière

Signatur des Originals: S 36/F08846

Stella Hohenfels als Nymphas, Rollenbild, in: Adolf von Wilbrandt: Der Meister von Palmyra

Signatur des Originals: S 36/F08847

Stella, Hüftbild

Signatur des Originals: S 36/F09966

Stella Hohenfels als Georg, Rollenbild, in: Johann Wolfgang von Goethe: Götz von Berlichingen, Burgtheater Wien 1881

Signatur des Originals: S 36/F10792