EFFECTIVE BAROMETRIC ADMITTANCE AND GRAVITY RESIDUALS

In the analysis of surface gravity signals that may originate from the Earth's core, the step of correcting for the atmospheric pressure fluctuations is one that must be done carefully. We apply two techniques for determining the local, or effective, barometric admittance function between simultaneous observations of surface gravity and pressure. The first is a frequency domain fit that computes the admittance on a band-by-band basis. Using data from both the Canadian and French superconducting gravimeters we determined that the magnitude of the local, or background, admittance increases smoothly and monotonically from about 0.2 mu gal mbar(-1) at long periods (>10 days) to about 0.35 mu gal mbar(-1) at frequencies greater than 3 cycles per day (c.p.d.); the phase lap is within a few degrees of 180 degrees. By comparison, the effective admittances of the large-scale harmonics of the solar heating tide (S-1-S-7) are much smaller, between 0.1 and 0.3 mu gal mbar(-1), for most of the harmonics of a day. In the second approach we fit a symmetrical time domain admittance function having lengths between 1 and 19 h using both a standard least-squares fit to a white noise residual and a new, and clearly superior, fit assuming a brown noise residual. Both time and frequency domain approaches give comparable results and contribute to a significant lowering of the residual level in non-tidal bands.