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Published August 11, 2023 | Published
Journal Article Open

Long-lasting, deep effect of Saturn's giant storms

Abstract

Planetary-scale giant storms erupt on Saturn quasiperiodically. There have been at least six recorded occurrences of past eruptions, and the most recent one was in 2010, with its whole life span captured by the Cassini mission. In 2015, we used the Very Large Array to probe the deep response of Saturn's troposphere to the giant storms. In addition to the remnant effect of the storm in 2010, we have found long-lasting signatures of all mid-latitude giant storms, a mixture of equatorial storms up to hundreds of years old, and potentially an unreported older storm at 70°N. We derive an ammonia anomaly map that shows an extended meridional migration of the storm's aftermath and vertical transport of ammonia vapor by storm dynamics. Intriguingly, the last storm in 2010 splits into two distinct components that propagate in opposite meridional directions, leaving a gap at 43°N planetographic latitude.

Copyright and License

© 2023 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC).

Acknowledgement

The National Radio Astronomy Observatory (NRAO) is a facility of NSF operated under cooperative agreement by Associated Universities Inc. VLA data used in this report, associated with project code VLA/14B-401, are available from the NRAO Science Data Archive at https://archive.nrao.edu/archive/advquery.jsp.

Funding

This work is supported by the Heising-Simons Foundation under the 51 Pegasi b fellowship.

Contributions

I.d.P., B.B., R.J.S., and Z.Z. performed observation and data reduction (I.d.P. was the principal investigator on the observing proposal). C.L. performed the analysis, including radiative transfer modeling, deconvolution, and differential spectral inversion. I.d.P. and C.M. performed independent radiative transfer modeling to verify the result. C.L., I.d.P., and C.M. wrote the manuscript. D.d. provided the radiobear software for an independent check.

Data Availability

Raw data are available at https://data.nrao.edu. The computer codes to process the raw data are available at https://casa.nrao.edu, and the Miriad software is available at https://atnf.csiro.au/computing/software/miriad/. The processed images, data, and processing scripts are available at https://github.com/chengcli/2023.SaturnVLA/. The spectral inversion codes are available at https://github.com/david-deboer/radiobear and https://github.com/chengcli/canoe/. A frozen version of the code that performed the inversion is uploaded to the Zenodo archive with DOI:10.5281/zenodo.8117538. The VLA images are uploaded to the Zenodo archive with DOI:10.5281/zenodo.8117555. All data needed to evaluate the conclusions in the paper are present in the paper and/or the Supplementary Materials.

Conflict of Interest

The authors declare that they have no competing interest.

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Additional details

Created:
October 18, 2023
Modified:
October 18, 2023