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NASA's ICON MIGHTI instrument measures horizontal wind speed and direction in the thermosphere using Doppler spectroscopy. The dataset is produced by combining line-of-sight observations from two perpendicular fields of view (A and B) to determine the wind vector, and includes temperature measurements derived from molecular oxygen A-band spectra. The data was last updated on 2026-03 13.
License is listed as 'other-license-specified'; specific terms must be reviewed before use. Primary file formats are BIN and HTML.