Abstract
A correlation study between solar wind activity and Jupiter's decametric radiation seems to indicate that the solar wind has a suppressive effect on the non Io-related emission. A basic model for the non Io-related emission is presented, to explain this and other characteristics of the non Io-related emission.
Similar content being viewed by others
References
Bass, J.: 1966,Elements of Probability Theory, Academic Press, New York and London.
Bigg, E. K.: 1964,Nature 203, 1088.
Carr, T. D., Smith, A. G., Bollhagen, H., Six, N. F., and Chatterton, N. E.: 1961,Astrophys. J. 134, 105.
Chappel, C. R., Harris, K. K., and Sharp, G. W.: 1970a,J. Geophys. Res. 75, 50.
Chappel, C. R., Harris, K. K., and Sharp, G. W.: 1970b,J. Geophys. Res. 75, 3848.
Chappel, C. R., Harris, K. K., and Sharp, G. W.: 1971,J. Geophys. Res. 76, 7632.
Goertz, C. K.: 1973,Planetary Space Sci. 21, 1431.
Gruber, G. M. and Way-Jones, C.: 1972,Nature Phys. Sci. 237, 137.
Hundhausen, A. J.: 1970,Rev. Geophys. Space Sci. 8, 729.
Intriligator, D. S.: 1974,Astrophys. J. 188, L32.
Smith, E. J., Davis, L., Jones, D. E., Colburn, D. S., Coleman, P. J., Dyal, P., and Sonett, C. P.: 1974,Science 183, 305.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Gruber, G.M. Jupiter's non Io-related decametric radiation. Astrophys Space Sci 37, 169–172 (1975). https://doi.org/10.1007/BF00646070
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00646070