TIME-DEPENDENT ANALYSIS OF 8 DAYS OF CN SPATIAL PROFILES IN COMET-P/HALLEY

CN profiles in comet P/Halley were constructed from observations taken at three observatories during an 8 day period in April 1986. These data provide a time series of CN spatial profiles spanning just over one 7.37 day period from 1986 April 7 to April 15 and sample distances from the nucleus from just over 10(3) km to 10(6) km. The effect of the 7.37 day periodic variation on the CN distribution in P/Halley has been examined by using the time-dependent model applied earlier to a subset of the data. Because of the large spatial scale of the data on April 7, 8, and 9 (similar to 10(6) km), and the corresponding transport time in the coma, information present in the spatial profiles regarding the gas production rate actually covers nearly two full periods. These spatially extended profiles clearly show the wavy structures outside 10(5) km. Such structures were predicted in a previous analysis (Combi and Fink 1993) that was based solely on the photometric light curve and on profiles which only extended to distances less than 10(5) km. We are now able to reproduce the highly variable Halley CN profiles using the same model as before, with the same standard scale lengths, phase lag, and amplitude correction for the variation in gas production rate.