Finding the suitable drag-free acceleration noise level for future low-low satellite-to-satellite tracking geodesy missions. Issue 1 (1st January 2019)

• Record Type: Journal Article
• Authors: Hong, Seong Hyeon; Conklin, John W.
• Is Part Of: Advances in space research. Volume 63:Issue 1(2019)
• Page Start: 32
• Page End: 50
• Publication Date: 2019-01-01
• Subjects: Drag-free -- Satellite gradiometry -- GRACE -- GOCE -- LISA Pathfinder -- Acceleration noise; Space sciences -- Periodicals; Astronautics -- Periodicals; Geophysics -- Periodicals; 500.505
• DOI: 10.1016/j.asr.2018.07.022
• Languages: English
• ISSNs: 0273-1177

Abstract

Abstract: This paper evaluates the impact of residual acceleration noise on the estimation of the Earth's time-varying gravity field for future low-low satellite-to-satellite tracking missions. The goal is to determine the maximum level of residual acceleration noise that does not adversely affect the estimation error. The Gravity Recovery And Climate Experiment (GRACE) has provided monthly average gravity field solutions in spherical harmonic coefficients for more than a decade. It provides information about land and ocean mass variations with a spatial resolution of ∼350 km and with an accuracy within 2 cm throughout the entire Earth. GRACE Follow-on was launched in May 2018 to advance the work of GRACE and to test a new laser ranging interferometer, which measures the range between the two satellites with higher precision than the K-Band ranging system used in GRACE. Moreover, there have been simulation studies that show, an additional pair of satellites in an inclined orbit increases the sampling frequency and reduces temporal aliasing errors. Given the fact that future missions will likely continue to use the low-low satellite-to-satellite tracking formation with laser ranging interferometry, it is expected that the residual acceleration noise will become one of the largest error contributor for the time-variable gravity field solution. We evaluate three different levels of residual acceleration noise based on demonstrated drag-free systems to find a suitable drag-free performance target for upcoming geodesy missions. We analyze both a single collinear polar pair and the optimal double collinear pair of drag-free satellites and assume the use of a laser ranging interferometer. A partitioned best linear unbiased estimator that was developed, incorporating several novel features from the ground up is used to compute the solutions in terms of spherical harmonics. It was found that the suitable residual acceleration noise level is around 2 × 10 −12 ms −2 Hz −1/2 . Decreasing the acceleration noise below this level did not result in more accurate gravity field solutions for the chosen mission architecture.