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Table 2 Major observation programs for LIR

From: Absolute calibration of brightness temperature of the Venus disk observed by the Longwave Infrared Camera onboard Akatsuki

Observation name Instruments synchronously observing with LIR m n
Nightside deluxe IR2 (1.73, 2.26, 2.02, 2.32 μm) 32 32
Nightside slim IR2 (2.26 μm) 32 32
Dayside deluxe IR1 (0.9 μm), IR2 (2.02 μm), UVI (283, 365 nm) 32 32
Dayside slim IR1 (0.9 μm), IR2 (2.02 μm) 32 32
Vicinity deluxe UVI (283, 365 nm) 32 01
Vicinity slim UVI (283, 365 nm × 2) 32 01
Vicinity slim UVI (283, 365 nm × 7) 32 01
Nightside vicinity scan IR2 (1.73, 2.26 μm) 32 01
Dayside vicinity scan IR1 (0.9 μm), IR2 (2.02 μm), UVI (365 nm) 32 01
Nightside deluxe IR2 (1.73, 2.26, 2.02, 2.32 μm) with ROI 32 01
Nightside slim IR2 (2.26 μm) with ROI 32 32
Dayside deluxe IR1 (0.9 μm), IR2 (2.02 μm), UVI (283, 365 nm) 32 32
Dayside slim IR1 (0.9 μm), IR2 (2.02 μm), UVI (283, 365 nm) with ROI 32 32
  1. An additional observation with m = 32 and n = 1 was prepared on October 2016
  2. ROI region of interest: a specific area selected from an images of IR1, IR2, and UVI in order to limit data quantity