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Volume 11 Issue 3, March 2018

Spinning up Saturn‘s cyclonic circulation

Saturn‘s cyclonic atmospheric circulation may be explained by the dynamics of small-scale convection, suggest laboratory analogue experiments. The image shows the surface signature of a heated fluid rising from the base of a rotating fluid layer in a laboratory experiment that simulates a planetary atmosphere.

See Afanasyev & Zhang

Image: Y. D. Afanasyev, Memorial University of Newfoundland. Cover Design: Lauren Heslop.

Editorial

  • Preprint servers afford a platform for sharing research before peer review. We are pleased that two dedicated preprint servers have opened for the Earth sciences and welcome submissions that have been posted there first.

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