Literature DB >> 17774793

Latitudinal and longitudinal oscillations of cloud features on neptune.

L A Sromovsky.   

Abstract

Voyager observations suggest that three of Neptune's major cloud features oscillate in latitude by 2 degrees to 4 degrees and that two of them simultaneously oscillate in longitude by 7.8 degrees and 98 degrees about their mean drift longitudes. The observations define most convincingly the two orthogonal oscillations of the second dark spot (near 53 degrees south). These oscillations have similar periods near 800 hours and approximately satisfy a simple advective model in which a latitudinal oscillation produces a phase-shifted longitudinal oscillation proportional to the local wind shear. The latitudinal motion of the Great Dark Spot can be fit with an oscillation period of about 2550 hours, whereas its dominant longitudinal motion, if oscillatory at all, has such a long period that it is not well constrained by the Voyager data.

Entities:  

Year:  1991        PMID: 17774793     DOI: 10.1126/science.254.5032.684

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  1 in total

1.  NEPTUNE'S DYNAMIC ATMOSPHERE FROM KEPLER K2 OBSERVATIONS: IMPLICATIONS FOR BROWN DWARF LIGHT CURVE ANALYSES.

Authors:  Amy A Simon; Jason F Rowe; Patrick Gaulme; Heidi B Hammel; Sarah L Casewell; Jonathan J Fortney; John E Gizis; Jack J Lissauer; Raul Morales-Juberias; Glenn S Orton; Michael H Wong; Mark S Marley
Journal:  Astrophys J       Date:  2016-01-28       Impact factor: 5.521

  1 in total

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