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Correlated Variations of Planetary Albedos and Solar-Interplanetary Parameters

Published online by Cambridge University Press:  14 August 2015

G. W. Lockwood ,
S. T. Suess  and
D. T. Thompson
G. W. Lockwood
Affiliation:
Lowell Observatory, Flagstaff, Arizona
S. T. Suess
Affiliation:
NOAA/ERL, Boulder, Colorado
D. T. Thompson
Affiliation:
Lowell Observatory, Flagstaff, Arizona

Extract

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The brightnesses of Titan and Neptune have been monitored photo-electrically at 472 and 551 nm since 1972 at the Lowell Observatory, yielding annual mean magnitudes accurate to 0.3 percent (0.003 mag). Both objects increased steadily in brightness until 1976 and declined thereafter (Lockwood 1977, Lockwood and Thompson 1979). The range of variation was about 0.08 mag for Titan and 0.03 mag for Neptune.

Type
Part II. Coronal and Interplanetary Responses to Long Time Scale Phenomena
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 163 - 166
Copyright
Copyright © Reidel 1980 

References

Hinteregger, H. E.: 1979, J. Geophys. Res. 84, 1933.CrossRefGoogle Scholar
Lockwood, G. W.: 1977, Icarus 32, 413.CrossRefGoogle Scholar
Lockwood, G. W. and Thompson, D. T.: 1979, Nature 280, 43.CrossRefGoogle Scholar
White, O. R., (ed.): 1977, The Solar Output and Its Variations , Colorado Associated University Press, Boulder.Google Scholar