REMOVAL OF TROPOSPHERIC PATH-LENGTH VARIATIONS IN VERY LONG-BASE-LINEINTERFEROMETRY WITH MEASUREMENT OF TROPOSPHERIC EMISSION

We present our first results of the application of the measurement of atmospheric emission to correct for atmospheric phase variations in ve ry long baseline interferometry. This technique corrects for the fluct uations in the phase path length through the atmosphere by measuring t he water vapor content through its emissivity. Two epochs of 3-mm wave length (lambda) observations under different atmospheric conditions sh ow that total power monitoring at Hat Creek and Kitt Peak Observatorie s can be used to reduce the rms interferometer phase when liquid water is not present in the beam. In the best cases, the root-mean-square ( rips) phase is reduced by a factor of 2 to 1 rad. Instability in the r eceiver gain at the level of one part in 10(3) creates the 1-rad limit in the rms phase. The technique is currently most successful at elimi nating variability on timescales greater than 10 s. However, it is not always successful, and we discuss sources for the residual variabilit y in the phase. Sire also derive the expected value of the scale facto r relating delay to brightness temperature at 86 and 230 GHz. As this technique is improved, future experiments will have greater sensitivit y to weak sources, accurate astrometry and geodesy will be possible, a nd imaging at 1-mm lambda may be explored.