Abstract

Within this work, a new geodetic very long baseline interferometry (VLBI) scheduling approach inspired by evolutionary processes based on selection, crossover and mutation is presented. It mimics the biological concept “surviving of the fittest” to iteratively explore the scheduling parameter space looking for the best solution. Besides providing high-quality results, one main benefit of the proposed approach is that it enables the generation of fully automated and individually optimized schedules. Moreover, it generates schedules based on transparent rules, well-defined scientific goals and by making decisions based on Monte Carlo simulations. The improvements in terms of precision of geodetic parameters are discussed for various observing programs organized by the International VLBI Service for Geodesy and Astrometry (IVS), such as the OHG, R1, and T2 programs. In the case of schedules with a difficult telescope network, an improvement in the precision of the geodetic parameters up to 15% could be identified, as well as an increase in the number of observations of up to 10% compared to classical scheduling approaches. Due to the high quality of the produced schedules and the reduced workload for the schedulers, various IVS observing programs are already making use of the evolutionary parameter selection, such as the AUA, INT2, INT3, INT9, OHG, T2 and VGOS-B program.

Highlights

  • Very long baseline interferometry (VLBI) (Sovers et al 1998; Schuh and Böhm 2013) is, together with the global navigation satellite system (GNSS), satellite laser ranging (SLR), and Doppler orbitography and radiopositioning integrated by satellite (DORIS), one of the geometric space geodetic techniques

  • – n number of generations – m0 number of individuals in the initial population – m j number of individuals for generation j > 0 – nbest number of parents selected based on fitness function – nrand number of parents selected randomly – npar number of parents used during crossover

  • We present a new approach to individually optimize geodetic VLBI schedules using a general approach

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Summary

Introduction

Very long baseline interferometry (VLBI) (Sovers et al 1998; Schuh and Böhm 2013) is, together with the global navigation satellite system (GNSS), satellite laser ranging (SLR), and Doppler orbitography and radiopositioning integrated by satellite (DORIS), one of the geometric space geodetic techniques. Sackenrieder Str. 25, 93444 Bad Kötzting, Germany mines the celestial reference frame in radio frequencies (Fey et al 2015; Charlot et al 2020). It is the only technique capable of determining the full set of earth orientation parameters (EOPs) (Petit and Luzum 2010), which are critical for positioning and navigation in space and on Earth. When multiple telescopes observe the same radio source simultaneously, this is called a scan. Each pair of telescopes forms one baseline and provides one observation. VLBI sessions can be divided into two groups:

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