%0 Book
%T Thermal evolution models for Uranus and Neptune
%A Scheibe, Ludwig
%D 2021
%C Rostock
%C Universität Rostock
%G English
%F 1795113855
%O vorgelegt von Ludwig Scheibe
%O GutachterInnen: Ronald Redmer (Universität Rostock, Institut für Physik) ; Doris Breuer (Deutsches Zentrum für Luft- und Raumfahrt, Institut für Planetenforschung)
%O Dissertation Universität Rostock 2022
%X Uranus and Neptune (U&N) have highly different intrinsic heat fluxes. Here, the principles behind a new computer code for calculating numerical structure and evolution models of planets are presented, and with this program the thermal evolution of U&N is investigated using up-to-date equation of state data. Particularly, it is shown that the assumption of a thermal boundary layer in the planet's envelope, trapping part of its heat in the deep interior, impacts the planet's cooling drastically and thus allows for an explanation of U&N's heat fluxes within the same framework.<eng>
%L 530
%9 theses
%9 Text
%9 Hochschulschrift
%R 10.18453/rosdok_id00003533
%U http://purl.uni-rostock.de/rosdok/id00003533
%U https://nbn-resolving.org/urn:nbn:de:gbv:28-rosdok_id00003533-9
%U https://d-nb.info/1293536997/34
%U https://doi.org/10.18453/rosdok_id00003533