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The H 3 + ionosphere of Uranus: decades-long cooling and local-time morphology

2019; Royal Society; Volume: 377; Issue: 2154 Linguagem: Inglês

10.1098/rsta.2018.0408

1471-2962

Henrik Melin, Leigh N. Fletcher, Tom Stallard, S. Miller, L. M. Trafton, Luke Moore, J. O’Donoghue, R. J. Vervack, N. Dello Russo, Laurent Lamy, Chihiro Tao, M. N. Chowdhury,

Atmospheric Ozone and Climate

The upper atmosphere of Uranus has been observed to be slowly cooling between 1993 and 2011. New analysis of near-infrared observations of emission from H 3 + obtained between 2012 and 2018 reveals that this cooling trend has continued, showing that the upper atmosphere has cooled for 27 years, longer than the length of a nominal season of 21 years. The new observations have offered greater spatial resolution and higher sensitivity than previous ones, enabling the characterization of the H 3 + intensity as a function of local time. These profiles peak between 13 and 15 h local time, later than models suggest. The NASA Infrared Telescope Facility iSHELL instrument also provides the detection of a bright H 3 + signal on 16 October 2016, rotating into view from the dawn sector. This feature is consistent with an auroral signal, but is the only of its kind present in this comprehensive dataset. This article is part of a discussion meeting issue ‘Advances in hydrogen molecular ions: H 3 + , H 5 + and beyond’.