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Variations in the color of jupiter

Published online by Cambridge University Press:  14 August 2015

Neil B. Hopkins  and
William M. Irvine
Neil B. Hopkins
Affiliation:
Dept. of Physics and Astronomy, University of Massachusetts, Amherst, Mass. U.S.A.
William M. Irvine
Affiliation:
Dept. of Physics and Astronomy, University of Massachusetts, Amherst, Mass. U.S.A.

Abstract

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Observations of Jupiter by multicolor photoelectric photometry in 10 narrow bands between 3150 Å and 1.06 μ and in UBV showed a brightening for shorter wavelengths in 1965 relative to 1963. An opposite effect occurred for the band at 7300 Å. These results are consistent with observed activity in the Jovian atmosphere. No obvious correlation could be found between brightness fluctuations and longitude of the central meridian, indicating that the activity was uniform in longitude or occurred on time scales short compared to a month.

Type
Part III: Outer Planets
Information
Symposium - International Astronomical Union , Volume 40: Planetary Atmospheres , 1971 , pp. 349 - 352
Copyright
Copyright © Reidel 1971 

References

Aksenov, A. N., Grigor'eva, A. N., Priboeva, N. V., Romanenco, A. G., and Teifel, V. G.: 1967, ‘Atmospheric Activity of Jupiter in 1964–1965 According to Photometric Data’, Solar Systems Res. (U.S.S.R.) 1, 129–133.Google Scholar
Allen, C. W.: 1963, Astrophysical Quantities, Athlone Press, London, 2nd ed., Section 82.Google Scholar
Focas, J. H. and Banos, C. J.: 1964, ‘Photometric Study of the Atmospheric Activity on the Planet Jupiter and Peculiar Activity in Its Equatorial Area’, Ann. Astrophys. 27, 36–45.Google Scholar
Irvine, W. M., Simon, T., Menzel, D. H., Charon, J., Lecomte, G., Griboval, P., and Young, A. T.: 1968a, ‘Multicolor Photo-Electric Photometry of the Brighter Planets. II. Observations from Le Houga Observatory’, Astron. J. 73, 251–264 (Paper II).Google Scholar
Irvine, W. M., Simon, T., Menzel, D. H., Pikoos, C., and Young, A. T.: 1968b, ‘Multicolor Photo-Electric Photometry of the Brighter Planets. III: Observations from Boyden Observatory’, Astron. J. 73, 807–828 (Paper III).Google Scholar
King, I.: 1952, ‘Effective Extinction Values in Wide-Band Photometry’, Astron. J. 67, 253–258.Google Scholar
Low, F. L.: 1969, in Third Arizona Conference on Planetary Atmospheres. Google Scholar
Reese, E. V. and Solberg, H. G. Jr.: 1966, ‘Recent Measures of the Latitude and Longitude of Jupiter's Red Spot’, Icarus 5, 266–273.Google Scholar
Shapiro, R.: 1953, ‘A Planetary-Atmospheric Response to Solar Activity’, J. Meteorol. 10, 350–355.Google Scholar
Wasiutinsky, J.: 1946, ‘Studies in Hydrodynamics and Structure of Stars and Planets’, Astrophys. Norvegica 4, 318–331.Google Scholar
Young, A. T. and Irvine, W. M.: 1967, ‘Multicolor Photo-Electric Photometry of the Brighter Planets. I: Program and Procedure’, Astron. J. 72, 945–950 (Paper I).Google Scholar