Ionospheric bending correction for GNSS radio occultation signals

Abstract

Ionospheric propagation effects on Global Navigation Satellite Systems (GNSS) signals are the most pronounced during radio occultation due to long ionospheric travel paths of the received signal on low Earth orbiting satellites. Inhomogeneous plasma distribution and anisotropy cause higher order nonlinear refraction effects on GNSS signals which cannot be fully removed through a linear combination of dual-frequency observables. In this paper, higher order ionospheric effects due to straight line of sight (LoS) propagation assumption such as the excess path length of the signal in addition to the LoS path and the total electron content difference between the curved path and the LoS path have been investigated for selected GPS-CHAMP occultation events. Based on simulation studies we have derived correction formulas for computing ray path bending effects as functions of signal frequency, tangential height of the ray path, ionospheric parameters such as the maximum ionization and total electron content. If these parameters are known the proposed correction method is able to correct on an average about 65 - 80% bending errors of GNSS occultation signals.