2013
DOI: 10.1007/s00190-013-0671-y
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Optimal orbits for temporal gravity recovery regarding temporal aliasing

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Cited by 21 publications
(12 citation statements)
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“…The simulations presented in this study have been conducted on IAPG's closed-loop reducedscale simulation software which is described in detail in Murböck (2015) and Murböck et al (2014). Compared to a real gravity mission processing scheme this tool uses various simplifications as a trade-off for improved computation time.…”
Section: Simulation Environment and Parametersmentioning
confidence: 99%
“…The simulations presented in this study have been conducted on IAPG's closed-loop reducedscale simulation software which is described in detail in Murböck (2015) and Murböck et al (2014). Compared to a real gravity mission processing scheme this tool uses various simplifications as a trade-off for improved computation time.…”
Section: Simulation Environment and Parametersmentioning
confidence: 99%
“…Correspondingly, the science and user needs of NGGMs were defined in [4]. In several previous studies, different mission concepts have been studied in detail, with emphasis on orbit design and resulting spatial-temporal ground track pattern, enhanced processing and parameterization strategies, and improved post-processing/filtering strategies in order to reduce temporal aliasing effects, which are one of the main error sources of current temporal gravity field solutions [5]. The typical GRACE-type concept of two satellites (satellite pair) following each other on the same orbit with an inter-satellite distance of about 200 km observes only the along-track component of the Earth's gravity field, and therefore leads to a very anisotropic error structure and the typical striping patterns in the resulting temporal gravity solutions.…”
Section: Introductionmentioning
confidence: 99%
“…To analyze the effect of deterministic error sources like ocean tide (OT) signal, an OT difference signal is added to the observations, leading to the residual SH degree RMS drawn in the dashed lines. As described in [18], characteristic RMS peaks, induced by incomplete OT de-aliasing affecting specific SH order bands, can be seen in the dashed gray line around SH degrees 46, 61, and 107. As one can conclude from the dashed red line, the OT signal is almost completely removed from the observations and the residuals are almost as small as for the case without deterministic errors.…”
Section: Determination Of a Favorable Filter Designmentioning
confidence: 75%
“…In order to perform the closed-loop simulations, we employ the closed-loop mission simulator described by [18] to simulate GRACE-like observations and to calculate monthly GRACE-like time variable gravity field solutions. Acceleration differences along the line of sight between the two satellites serve as observations.…”
Section: The Closed-loop Simulation Environmentmentioning
confidence: 99%