Universität zu Köln

Lora, Juan M., Tokano, Tetsuya, d'Ollone, Jan Vatant, Lebonnois, Sebastien and Lorenz, Ralph D. (2019). A model intercomparison of Titan's climate and low-latitude environment. Icarus, 333. S. 113 - 127. SAN DIEGO: ACADEMIC PRESS INC ELSEVIER SCIENCE. ISSN 1090-2643

Full text not available from this repository.

Abstract

Cassini-Huygens provided a wealth of data with which to constrain numerical models of Titan. Such models have been employed over the last decade to investigate various aspects of Titan's atmosphere and climate, and several three-dimensional general circulation models (GCMs) now exist that simulate Titan with a high degree of fidelity. However, substantial uncertainties persist, and at the same time no dedicated intercomparisons have assessed the degree to which these models agree with each other or the observations. To address this gap, and motivated by the proposed Dragonfly Titan lander mission, we directly compare three Titan GCMs to each other and to in situ observations, and also provide multi-model expectations for the low-latitude environment during the early northern winter season. Globally, the models qualitatively agree in their representation of the atmospheric structure and circulation, though one model severely underestimates meridional temperature gradients and zonal winds. We find that, at low latitudes, simulated and observed atmospheric temperatures closely agree in all cases, while the measured winds above the boundary layer are only quantitatively matched by one model. Nevertheless, the models simulate similar near-surface winds, and all indicate these are weak. Likewise, temperatures and methane content at low latitudes are similar between models, with some differences that are largely attributable to modeling assumptions. All models predict environments that closely resemble that encountered by the Huygens probe, including little or no precipitation at low latitudes during northern winter. The most significant differences concern the methane cycle, though the models are least comparable in this area and substantial uncertainties remain. We suggest that, while the overall low-latitude environment on Titan at this season is now fairly well constrained, future in situ measurements and monitoring will transform our understanding of regional and temporal variability, atmosphere-surface coupling, Titan's methane cycle, and modeling thereof.

Item Type:	Journal Article
Creators:	Creators Email ORCID ORCID Put Code Lora, Juan M. UNSPECIFIED UNSPECIFIED UNSPECIFIED Tokano, Tetsuya UNSPECIFIED UNSPECIFIED UNSPECIFIED d'Ollone, Jan Vatant UNSPECIFIED UNSPECIFIED UNSPECIFIED Lebonnois, Sebastien UNSPECIFIED UNSPECIFIED UNSPECIFIED Lorenz, Ralph D. UNSPECIFIED UNSPECIFIED UNSPECIFIED
URN:	urn:nbn:de:hbz:38-127584
DOI:	10.1016/j.icarus.2019.05.031
Journal or Publication Title:	Icarus
Volume:	333
Page Range:	S. 113 - 127
Date:	2019
Publisher:	ACADEMIC PRESS INC ELSEVIER SCIENCE
Place of Publication:	SAN DIEGO
ISSN:	1090-2643
Language:	English
Faculty:	Unspecified
Divisions:	Unspecified
Subjects:	no entry
Uncontrolled Keywords:	Keywords Language HUYGENS PROBE; ATMOSPHERE; CLOUDS; CIRCULATION; DESCENT; WINDS; DISR; PRECIPITATION; TEMPERATURES; SIMULATIONS Multiple languages Astronomy & Astrophysics Multiple languages
Refereed:	Yes
URI:	http://kups.ub.uni-koeln.de/id/eprint/12758