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Thermal Structure and Dynamics of Saturn’s Northern Springtime Disturbance
Author(s) -
Leigh N. Fletcher,
B. E. Hesman,
P. G. J. Irwin,
K. H. Baines,
T. Momary,
A. SánchezLavega,
F. M. Flasar,
P. L. Read,
Glenn S. Orton,
A. A. Simon,
R. Hueso,
G. L. Bjoraker,
A. A. Mamoutkine,
T. del RíoGaztelurrutia,
José María Gómez,
B. J. Buratti,
R. N. Clark,
P. D. Nicholson,
C. Sotin
Publication year - 2011
Publication title -
science
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 12.556
H-Index - 1186
eISSN - 1095-9203
pISSN - 0036-8075
DOI - 10.1126/science.1204774
Subject(s) - anticyclone , disturbance (geology) , saturn , atmospheric sciences , northern hemisphere , stratosphere , storm , environmental science , troposphere , atmospheric circulation , rossby wave , polar vortex , subsidence , geology , climatology , physics , astronomy , oceanography , planet , geomorphology , structural basin
Saturn's slow seasonal evolution was disrupted in 2010-2011 by the eruption of a bright storm in its northern spring hemisphere. Thermal infrared spectroscopy showed that within a month, the resulting planetary-scale disturbance had generated intense perturbations of atmospheric temperatures, winds, and composition between 20° and 50°N over an entire hemisphere (140,000 kilometers). The tropospheric storm cell produced effects that penetrated hundreds of kilometers into Saturn's stratosphere (to the 1-millibar region). Stratospheric subsidence at the edges of the disturbance produced "beacons" of infrared emission and longitudinal temperature contrasts of 16 kelvin. The disturbance substantially altered atmospheric circulation, transporting material vertically over great distances, modifying stratospheric zonal jets, exciting wave activity and turbulence, and generating a new cold anticyclonic oval in the center of the disturbance at 41°N.

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