Measurements from the Galileo probe suggest that the zonal winds are deep rooted. Jupiter's high rotation rate makes it likely that the whole outer molecular H/He layer is involved in these longlived jet flows. Assuming that the primary flows are geostrophic, and that the banded surface structure st
Baroclinic instabilities in Jupiter's zonal flow
β Scribed by Peter J. Gierasch; Andrew P. Ingersoll; David Pollard
- Publisher
- Elsevier Science
- Year
- 1979
- Tongue
- English
- Weight
- 596 KB
- Volume
- 40
- Category
- Article
- ISSN
- 0019-1035
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## Abstract Extrusion flow experiments of linear and branched syndiotactic poly(propylene)s were carried out. The work was focused on flow instabilities. Ionized radiation was employed to induce long chain branching in linear samples. Sharkskin and melt fracture were postponed in the case of slight