Saturn's Seasonal Variability from Four Decades of Ground-Based Mid-Infrared Observations episode artwork

EPISODE · Nov 21, 2022 · 1 MIN

Saturn's Seasonal Variability from Four Decades of Ground-Based Mid-Infrared Observations

from Astro arXiv | all categories · host Corentin Cadiou

Saturn's Seasonal Variability from Four Decades of Ground-Based Mid-Infrared Observations by James S. D. Blake et al. on Monday 21 November A multi-decade record of ground-based mid-infrared (7-25 $\mu$m) images of Saturn is used to explore seasonal and non-seasonal variability in thermal emission over more than a Saturnian year (1984-2022). Thermal emission measured by 3-m and 8-m-class observatories compares favourably with synthetic images based on both Cassini-derived temperature records and the predictions of radiative climate models. 8-m class facilities are capable of resolving thermal contrasts on the scale of Saturn's belts, zones, polar hexagon, and polar cyclones, superimposed onto large-scale seasonal asymmetries. Seasonal changes in brightness temperatures of $\sim30$ K in the stratosphere and $\sim10$ K in the upper troposphere are observed, as the northern and southern polar stratospheric vortices (NPSV and SPSV) form in spring and dissipate in autumn. The timings of the first appearance of the warm polar vortices is successfully reproduced by radiative climate models, confirming them to be radiative phenomena, albeit entrained within sharp boundaries influenced by dynamics. Axisymmetric thermal bands (4-5 per hemisphere) display temperature gradients that are strongly correlated with Saturn's zonal winds, indicating winds that decay in strength with altitude, and implying meridional circulation cells forming the system of cool zones and warm belts. Saturn's thermal structure is largely repeatable from year to year (via comparison of infrared images in 1989 and 2018), with the exception of low-latitudes. Here we find evidence of inter-annual variations because the equatorial banding at 7.9 $\mu$m is inconsistent with a $\sim15$-year period for Saturn's equatorial stratospheric oscillation, i.e., it is not strictly semi-annual. Finally, observations between 2017-2022 extend the legacy of the Cassini mission, revealing the continued warming of the NPSV during northern summer. [Abr.] arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.07486v2

Episode metadata supplied by the publisher feed · Published Nov 21, 2022

Embed this episode

NOW PLAYING

Saturn's Seasonal Variability from Four Decades of Ground-Based Mid-Infrared Observations

0:00 1:00

No transcript for this episode yet

We transcribe on demand. Request one and we'll notify you when it's ready — usually under 10 minutes.

No similar episodes found.

No similar podcasts found.

Frequently Asked Questions

How long is this episode of Astro arXiv | all categories?

This episode is 1 minute long.

When was this Astro arXiv | all categories episode published?

This episode was published on November 21, 2022.

Can I download this Astro arXiv | all categories episode?

Yes. Use the download control on the episode player to save the publisher-provided media file.
URL copied to clipboard!