摘要：In order to verify the time variability of free core nutation (FCN) period, global superconducting gravimeter (SG) observations were analyzed based on synthetic test data.The gravity data series were synthesized to check the detectability of resonance variation caused by FCN period change.The tests indicate that the discrepancy between the FCN periods determined by SG and VLBI observations is caused by the high correlation between the FCN parameter and the amplitude factor of the ψ1 wave.The K1 wave is more sensitive to the FCN period change than other diurnal waves.The limit of the standard deviation of the K1 wave is found for more precisely observing the FCN period change.Tidal parameters of diurnal waves estimated from long series of 20 global SG stations were analyzed.A common variation trend is found in the amplitude factor of both K1 and ψ1 waves in all 8 stations above the limit, which indicates the FCN period may be not so stable in time.Furthermore, the variation in the K1 and ψ1 waves constrains the FCN period change to between 2.5 and 4 sidereal days, which also agrees with the possible variation from the current VLBI and SG observations.
