Fig. 5From: An uppermost haze layer above 100 km found over Venus by the SOIR instrument onboard Venus ExpressExample of a vertical profile of extinction coefficients (top panel) and the corresponding normalized extinction coefficients (bottom panel) for orbit 137, order 149 (Sep. 05, 2006, latitude \( 79\,{\text{N}}^\circ \), longitude \( 237^\circ \)). The average errors are almost 26% for the extinction coefficient and 42% for the normalized extinction coefficientBack to article page