摘要：IR2, a near-infrared camera in the 2-μm region onboard Akatsuki has been developed to primarily study the middle-to-lower atmospheric dynamics of Venus as probed in the 1.74- and 2.3-μm “windows” of the \(\hbox {CO}_2\) atmosphere on the night side.The spatial and temporal variability of CO below the clouds is also studied by differentiating 2.32-μm CO-band images from simultaneous 2.26-μm images.Images of the night-side disk in these wavelengths will enable us to determine the zonal and meridional winds near the cloud-base altitudes.IR2 also images at 2.02 μm, the center of a \(\hbox {CO}_2\) absorption band.Such images can visualize the variation of the cloud-top altitudes as contrast features due to different absorption path lengths of the reflected sunlight.Tracking of the 2.02-μm features will also enable us to obtain wind information at the cloud-top level.Together with the other cameras and the radio science equipment on Akatsuki, IR2 will contribute to understanding of the production and maintenance mechanism of super-rotation in the Venusian atmosphere.During cruise, IR2 observed zodiacal light with a broad-band H filter (1.65 μm), imaged the Earth–moon remotely from a distance of ~30 million km, and determined Venus’s phase curves at small phase angles.We have just started the early phase operation check of IR2 at Venus, as the orbit insertion in December 2015 was successful.
