Published in
American Astronomical Society, Astrophysical Journal, (427), p. L111, 1994
DOI: 10.1086/187377
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A method of determining possible brightness variations of the Sun in past centuries from observations of solar-type stars
Journal article published in 1994 by
Q. Zhang 
,
W. H. Soon,
S. L. Baliunas,
G. W. Lockwood,
B. A. Skiff,
R. R. Radick
,
W. H. Soon,
S. L. Baliunas,
G. W. Lockwood,
B. A. Skiff,
R. R. Radick
This paper was not found in any repository, but could be made available legally by the author.
Full text: Unavailable
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