Haze and cloud structure of Saturn's North Pole and Hexagon Wave from Cassini/ISS imaging
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Tropospheric hazes moved deeper and became optically thinner poleward of the hexagon.
“A recent study of Saturn’s reflectivity by Cassini’s Imaging Science Subsystem47 observed that the tropospheric hazes moved deeper and became optically thinner poleward of the hexagon.”
From A hexagon in Saturn's northern stratosphere surrounding the emerging summertime polar vortex (2018) · cites this paper as [47]
The polar region exhibits an increased optical thickness of stratospheric hazes that is potentially related to aerosol production associated with Saturn's aurora.
“In addition, the polar region exhibits an increased optical thickness of stratospheric hazes47,54 that is potentially related to aerosol production associated with Saturn’s aurora.”
From A hexagon in Saturn's northern stratosphere surrounding the emerging summertime polar vortex (2018) · cites this paper as [47]
The base of the tropospheric haze in Saturn's north polar atmosphere is located at around 600 mbar and descends towards the polar region.
“specific studies of the overall structure of the polar aerosols conclude that the base of the tropospheric haze in Saturn's north polar atmosphere is located at around 600 mbar and descends towards the polar region (Sanz-Requena et al., 2018).”
From Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon (2020) · cites this paper as Sanz-Requena et al., 2018
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A hexagon in Saturn's northern stratosphere surrounding the emerging summertime polar vortex
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The Dynamics of the Atmosphere of Saturn
Sánchez-Lavega, A. (2026) · doi:10.1093/9780197851500.003.0342
Self-citation
- Authors
- Sanz-Requena, J. F., Pérez-Hoyos, S., Sánchez-Lavega, A., Antuñano, A., & Irwin, P. G. J.
- Affiliations
- University of the Basque Country (ES)
- University of Oxford (GB)
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 2018-05
- Volume
- 305
- Pages
- 284-300
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2781006379
- Semantic Scholar
- 50d733a2ae5c8e35fd93895e458fd50f9c2f4e63
- Cited by
- 25
- References
- 52
- Citations by year
- 2026: 3 · 2025: 1 · 2023: 1 · 2021: 6 · 2020: 4 · 2019: 5 · 2018: 5
- FWCI
- 2.09
- Type
- journal article
- Language
- en
- Open access
- green
- ora.ox.ac.uk
- Licence
- cc-by-nc-nd
- www.elsevier.com/tdm/userlicense/1.0/ (tdm)
- Locations
- Icarus (publishedVersion)
- Oxford University Research Archive (ORA) (University of Oxford) (acceptedVersion, cc-by-nc-nd)
- Funders
- Federación Española de Enfermedades Raras (IT-765-13)
- Ministerio de Economía y Competitividad
- Euskal Herriko Unibertsitatea (UFI11/55)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- Saturn, polar atmosphere, stratospheric haze, particle size distribution, refractive index, absolute reflectivity, radiative transfer modeling, Cassini Imaging Science Subsystem, methane absorption bands
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