The eastern and western elongations of Venus, 1991-1998

摘要

This Report discusses ten successive morning and evening elongations. Data concerning phase anomaly, bright and dark atmospheric markings, cusp extensions and the Ashen Light are discussed. Systematic visual observations over days and weeks again provided definitive evidence for the'four-day' retrograde 'weather' period, and measurements over a longer, eight-year epoch yielded a reliable average period of 3.99524 ±0.00027 days, closely comparable with the long-term average derived by C. Boyer and others. The phase anomaly was never very large, but 1994 E yielded a significantly higher anomaly than the other elongations. Occasional records were made of the blunting of the S cusp near dichotomy; the less commonly blunted N cusp was well observed at the 1995 W elongation. High resolution data for two elongations suggest that cusp-blunting may simply be due to the presence of high latitude dark bands at such times, or strong polar turbulence. Of the other discrete bright features (recorded mostly at the limb), there was a definite preponderance of the southern over the northern hemisphere. During 1991 to 1998 there were somewhat more records of the true Ashen Light (i.e., when it appeared brighter than the surrounding sky) compared with the equivalent period from 1999 to 2006, with the 1991, 1993 and 1996 evening elongations yielding a significant number of independently confirmed sightings.