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Solar rotation results at Mount WilsonSolar rotation results from Doppler velocity measurements made at Mount Wilson over a period of more than 14 years are presented based on a single reduction procedure. The observations were made with the wavelength 5250.2 A line of Fe I, and wavelength shifts of the line were simultaneously recorded. Data from 188 rotations are presented. Measurements of scattered light along with its effect on the measured rotation rate are given.
Document ID
19830048770
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1007/BF00148283
Authors
Howard, R. (Mount Wilson Observatory Pasadena, CA, United States)
Adkins, J. M. (Mount Wilson Observatory Pasadena, CA, United States)
Boyden, J. E. (Mount Wilson Observatory Pasadena, CA, United States)
Cragg, T. A. (Mount Wilson Observatory Pasadena, CA, United States)
Gregory, T. S. (Mount Wilson Observatory Pasadena, CA, United States)
Labonte, B. J. (Mount Wilson Observatory Pasadena, CA, United States)
Padilla, S. P. (Mount Wilson Observatory Pasadena, CA, United States)
Webster, L. (Mount Wilson and Las Campanas Observatories Pasadena, CA, United States)
Date Acquired
August 11, 2013
Publication Date
March 1, 1983
Publication Information
Publication: Solar Physics
Volume: 83
ISSN: 0038-0938
Subject Category
Solar Physics
Accession Number
83A29988
Funding Number(s)
CONTRACT_GRANT: N00014-18-C-0065
CONTRACT_GRANT: F19628-72-C-0208
CONTRACT_GRANT: NGR-09-140-015
CONTRACT_GRANT: NSF AST-80-20445
Distribution Limits
Public
Copyright
Other

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