Nature 280, 776 - 778 (30 August 1979); doi:10.1038/280776a0

Jovian cloud structure and velocity fields

J. L. Mitchell^*, R. J. Terrile^*, B. A. Smith^†, J.-P. Muller^‡, A. P. Ingersoll^§, G. E. Hunt^‡, S. A. Collins^* & R. F. Beebe

^*Jet Propulsion Laboratory, Pasadena, California 91103
^†Department of Planetary Sciences, University of Arizona, Tucson, Arizona 85721
^‡University College London, London WC1, UK
^§Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125
Department of Astronomy, New Mexico State University, Las Cruces, New Mexico 88003

Regional views of the jovian cloud structures and associated flows demonstrate the asymmetry between the northern and southern hemispheres.

References

1.	Ingersoll, A. P. et al. Nature 280, 773–775 (1979).
2.	Terrile, R. J. & Beebe, R. F. Science 204, 948–951 (1979).
3.	Smith, B. A. et al. Science 204, 951–972 (1979).
4.	Hunt, G. E. & Muller, J.-P. Nature 280, 778–780 (1979).
5.	Beebe, R. F. & Youngblood, L. A. Nature 280, 771–772 (1979).
6.	Peek, B. M. The Planet Jupiter (Faber, London, 1958).
7.	Terrile, R. J. & Westphal, J. A. Icarus 30, 247 (1977).