Cited by 33Ionosphere and magnetosphere dynamicsAstro and Planetary ScienceLightning and Electromagnetic Phenomena

The DOI matches its Crossref record; 18 of the 18 references it cites were found in a registry or an index.

Location of Saturn's northern infrared aurora determined from Cassini VIMS images

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Abstract

[1] The location of Saturn's northern infrared aurora is described in detail using 12 selected images acquired by Cassini VIMS during 2006–2008. Bright main oval arcs and prevalent polar features are displayed, which do not exhibit a preferred local time or spatial extent. The average equatorward limit of the aurora was determined using a best fit circle method. The average circle has a radius of 16.4 ± 0.2° latitude, centred 1.6° anti-sunward of Saturn's pole. The low standard deviation of the fitted circle radii (<1°) indicates the relative stability of the equatorward auroral boundary. For the first time we show that the average location of the infrared oval is similar to that of the ultraviolet oval, suggesting that the auroral emissions at different wavelengths are very likely produced by a common driver despite the distinct emission mechanisms.

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Crossref · 10.1029/2010gl046193

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  • Saturn's main auroral oval occurs at an average latitude of 76.5°N and completely encompasses the area of the NPSV, sitting ~1° south of the hexagon latitude (78°N).

    “Saturn’s main auroral oval, associated with the boundary between open and closed magnetic field lines, occurs at an average latitude of 76.5°N 55 and therefore completely encompasses the area of the NPSV, sitting ~1° south of the hexagon latitude (78°N).”

    From A hexagon in Saturn's northern stratosphere surrounding the emerging summertime polar vortex (2018) · cites this paper as [55]

    The Boundary Determination and Fitting section (§3, paragraph 12) gives the average oval a radius of 16.4° from a centre offset 1.6° from the pole, not an average latitude of 76.5°N. The Introduction associates the main oval with the open–closed field-line boundary, but that does not support the cited latitude. The NPSV and hexagon comparison is the citing authors’ inference, not a finding attributed to this source. (LLM, conf=0.88)

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Metadata

Authors
Badman, S. V., Achilleos, N., Baines, K. H., Brown, R. H., Bunce, E. J., Dougherty, M. K., Melin, H., Nichols, J. D., & Stallard, T.
Affiliations
  • Japan Aerospace Exploration Agency (JP)
  • University College London (GB)
  • University of Wisconsin–Madison (US)
  • University of Arizona (US)
  • University of Leicester (GB)
  • Imperial College London (GB)
Venue
Geophysical Research Letters
Published
2011-02
Volume
38
Issue
3
Pages
n/a-n/a
ISSN
0094-8276 (ISSN-L)
OpenAlex
W1572080249
Cited by
33
References
18
Citations by year
2026: 1 · 2020: 2 · 2019: 4 · 2018: 5 · 2016: 2 · 2015: 5 · 2014: 3 · 2013: 3 · 2012: 4
FWCI
2.38
Type
journal article
Language
en
Open access
Locations
  • Geophysical Research Letters (publishedVersion)
  • Leicester Research Archive (University of Leicester) (submittedVersion)
Funders
Science and Technology Facilities Council (PP/E001076/1, ST/G002223/1, ST/H001972/1, ST/H002480/1)
Topics
  • Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Ionosphere and magnetosphere dynamics
  • Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
  • Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Lightning and Electromagnetic Phenomena
Keywords
Saturn, auroral oval, Cassini VIMS, ultraviolet aurora

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