Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/33253
Title: On the anticorrelation between H-3(+) temperature and density in giant planet ionospheres
Authors: Melin, H.
Stallard, Thomas S.
O'Donoghue, J.
Badman, S. V.
Miller, S.
Blake, J. S. D.
First Published: 21-Dec-2013
Publisher: Oxford University Press (OUP)
Citation: Monthly Notices of the Royal Astronomical Society, 2014, 438 (2), pp. 1611-1617 (7)
Abstract: The intensity of H+3 emission can be driven by both temperature and density, and when fitting a set of infrared H+3 line spectra, an anticorrelation between the fitted temperatures and densities is commonly observed. The ambiguity present in the existing published literature on how to treat this effect puts into question the physical significance of the derived parameters. Here, we examine the nature of this anticorrelation and quantify the inherent uncertainty in the fitted temperature and density that this produces. We find that the uncertainty produced by the H+3 temperature and density anticorrelation is to a very good approximation equal to the uncertainties that are derived from the fitting procedure invoking Cramer's rule. This means that any previously observed correlated variability in the observed H+3 temperature and density outside these errors, in the absence of other error sources, are statistically separated and can be considered physical. These results are compared to recent ground-based infrared Keck Near InfRared echelle SPECtrograph (NIRSPEC) observations of H+3 emission from Saturn's aurora, which show no clear evidence for large-scale radiative cooling, but do show stark hemispheric differences in temperature.
DOI Link: 10.1093/mnras/stt2299
ISSN: 0035-8711
Links: http://mnras.oxfordjournals.org/content/438/2/1611
http://hdl.handle.net/2381/33253
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2013 The Author. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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