Ionospheric electron density profiling and modeling of COSMIC follow-on simulations: Fid-Bau Portal

Ionospheric electron density profiling and modeling of COSMIC follow-on simulations

Tsai, L.-C. / Su, S.-Y. / Liu, C. H. / Tulasi Ram, S.

Abstract The FormoSat-3/ Constellation Observing System for Meteorology, Ionosphere and Climate (FS3/COSMIC) has been proven a successful mission on profiling ionospheric electron density $$( {N_e })$$ using the radio occultation (RO) technique. A follow-on program (called FS7/COSMIC2) is now in progress. The FS3/COSMIC follow-on mission will have six 24$$^{\circ }$$-inclination and 550-km low Earth orbiting (LEO) satellites and six 72$$^{\circ }$$-inclination and 750-km LEO satellites to receive Tri-G (GPS, GLONASS, and Galileo) satellite signals. FS7/COSMIC2 RO observations were simulated in this study by calculating limb-viewing GNSS-to-LEO TEC values separately through two independent ionospheric models (the TWIM and NeQuick models). We propose a compensatory Abel-inversion scheme to improve vertical $$N_e $$ profiling and three-dimensional (3D) $$N_e $$ modeling in this FS7/COSMIC2 simulation study with future real observations. In this FS7/COSMIC2 feasibility study the number of RO observations will increase of around 10 times compared with FS3/COSMIC, and the windowing day number to collect $$N_e $$ profiles and to derive every half-hour 3D $$N_e $$ model could be decreased from 30 to 3 days. The results show that the root-mean-square (RMS) foF2 and hmF2 difference improvements are 46 % (32 %) and 21 % (4.6 %), respectively, in relative percentage over the standard Abel inversion at the TWIM-background (NeQuick-background) simulation experiment. The RMS modeling errors are about one order less than those from FS3/COSMIC simulations.