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The Mees CCD imaging spectrographThe 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.
Document ID
19920028994
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Penn, Matthew J.
(Hawaii Univ. Honolulu, HI, United States)
Mickey, Donald L.
(Hawaii Univ. Honolulu, HI, United States)
Canfield, Richard C.
(Hawaii Univ. Honolulu, HI, United States)
Labonte, Barry J.
(Hawaii, University Honolulu, United States)
Date Acquired
August 15, 2013
Publication Date
September 1, 1991
Publication Information
Publication: Solar Physics
Volume: 135
ISSN: 0038-0938
Subject Category
Instrumentation And Photography
Report/Patent Number
ISSN: 0038-0938
Accession Number
92A11618
Funding Number(s)
CONTRACT_GRANT: NAGW-1542
Distribution Limits
Public
Copyright
Other

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