The Airborne Infrared Spectrometer: Development, characterization, and the 2017 August 21 eclipse observation

The instrument successfully observed the five coronal emission lines that it was designed to measure: Si x 1.431 mu m, S xi 1.921 mu m, Fe ix 2.853 mu m, Mg viii 3.028 mu m, and Si ix 3.935 mu m. Characterizing these magnetically sensitive emission lines is an important first step in designing future instruments to monitor the coronal magnetic field, which drives space weather events, as well as coronal heating, structure, and dynamics.

The AIR-Spec instrument includes an image stabilization system, feed telescope, grating spectrometer, and slit-jaw imager. This paper details the instrument design, optical alignment method, image processing, and data calibration approach. The eclipse observations are described and the available data are summarized.