Fig. 7From: Science requirements and description of the 1 μm camera onboard the Akatsuki Venus OrbiterContribution functions for the 0.90 (solid line), 0.97 (short dashed line) and 1.01 εm (long dashed line) channels. Most of contributions are from the surface (86, 76 and 89%, respectively). That of 0.97 εm differs from the others due to atmospheric H2O absorption.Back to article page