Atmospheric confinement of jet streams on Uranus and Neptune View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2013-05-15

AUTHORS

Yohai Kaspi, Adam P. Showman, William B. Hubbard, Oded Aharonson, Ravit Helled

ABSTRACT

On Uranus and Neptune, the measured fourth-order gravity harmonic, J4, constrains the atmospheric dynamics to the outermost 0.15 per cent and 0.2 per cent, respectively, of the planetary mass, indicating that these dynamics are confined to a thin weather layer no more than 1,000 kilometres deep on both planets.

PAGES

344-347

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/nature12131

DOI

http://dx.doi.org/10.1038/nature12131

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1049438319

PUBMED

https://www.ncbi.nlm.nih.gov/pubmed/23676751


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