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

Location of Saturn's northern infrared aurora determined from Cassini VIMS images,10.1029/2010GL046193,Geophysical Research Letters,S. V. Badman,N. Ac

Location of Saturn's northern infrared aurora determined from Cassini VIMS images   (Citations: 3)
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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.
Journal: Geophysical Research Letters - GEOPHYS RES LETT , vol. 38, no. 3, 2011
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    • ...Thus, emission poleward of the main auroral oval, located at a statistical average of ∼73°S latitude in both the UV [Badman et al., 2006; Lamy et al., 2009] and the IR [Badman et al., 2011], could be mapped to open field lines such that any excitation or ionisation of the atmosphere is caused by direct sourcing from the field‐aligned component of the solar wind [Clarke et al., 2005]...

    H. Melinet al. Simultaneous Cassini VIMS and UVIS observations of Saturn's southern a...

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