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Table 1 Characteristics of cameras on Akatsuki orbiter

From: Venus looks different from day to night across wavelengths: morphology from Akatsuki multispectral images

Camera Channel name Band center (μm) Bandwidth (micron) Transmittance Pixel size (mm) # Lines # Samples Focal length (mm) Day/night
IR1 090d 0.900 0.00910 0.0027 0.017 1024 1024 84.2 Day
090n 0.898 0.02890 0.74 0.017 1024 1024 84.2 Night
097 0.969 0.03860 0.78 0.017 1024 1024 84.2 Night
101 1.009 0.03910 0.75 0.017 1024 1024 84.2 Night
IR2 174 1.735 0.041 0.85 0.017 1024 1024 85.41 Night
226 2.26 0.052 0.67 0.017 1024 1024 85.44 Night
232 2.32 0.036 0.67 0.017 1024 1024 85.41 Night
202 2.02 0.039 0.06 0.017 1024 1024 85.50 Day
165 1.65 0.283 0.93 0.034 520 520 85.35
UVI 283 0.283 0.014 0.280 0.013 1024 1024 63.3 Day
365 0.365 0.014 0.509 0.013 1024 1024 63.3 Day
LIR   10.00 4.00 0.037 328 248 42.2 Day and night