NASA NTRS · 19920028994
The Mees CCD imaging spectrograph
Abstract
The Mees CCD (MCCD0 instrument is an imaging spectroscopy device which uses the 25-cm coronagraph telescope and the 3.0-m Coude spectrograph at Mees Solar Observatory on Haleakala, Maui. The instrument works with resolving power up to about 200,000 with significant throughput from 3934 A (Ca II K) to about 10,000 A. A fast guiding active mirror stabilizes the image during observations. A rapidly writing magnetic tape storage system allows observations to be recorded at 256 kbytes/s. Currently, the MCCD is used for imaging spectroscopy of solar flares at 6563 A (H-alpha), and velocity measurements of umbral oscillations; future plans include emission line studies of active region coronae, and photospheric studies of solar oscillations.
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Penn, Matthew J., Mickey, Donald L., Canfield, Richard C., Labonte, Barry J.. 1991-09-01. The Mees CCD imaging spectrograph. https://ntrs.nasa.gov/citations/19920028994
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