Peer-reviewedLicence not statedIcarus
Uranus evolution models with simple thermal boundary layers
Related
- Thermal evolution of neo-neutron stars. II. Temperature-dependent crusts
- Dynamical and thermal evolution of localized reconnecting current sheets under varying guide fields in the solar corona
- Ice Giants Revisited: Uranus and Neptune as Magma Ocean Worlds
- Solving the Mystery of the Electron Radiation Belt at Uranus: Leveraging Knowledge of Earth's Radiation Belts in a Re-Examination of Voyager 2 Observations
- The Evolution of Thermal and Non-thermal Emission Components in GRB 250920C
BibTeX
@article{nettelmann2026uranus,
title = {{Uranus evolution models with simple thermal boundary layers}},
author = {N. Nettelmann and K. Wang and J.J. Fortney and S. Hamel and S. Yellamilli and M. Bethkenhagen and R. Redmer},
journal = {Icarus},
year = {2026},
month = oct,
doi = {10.1016/j.icarus.2016.04.008},
eprint = {1605.00171},
archivePrefix = {arXiv},
url = {https://hal.science/hal-05791472v1},
}
RIS
TY - JOUR
TI - Uranus evolution models with simple thermal boundary layers
AU - N. Nettelmann
AU - K. Wang
AU - J.J. Fortney
AU - S. Hamel
AU - S. Yellamilli
AU - M. Bethkenhagen
AU - R. Redmer
PY - 2026
DA - 2026/10/10
JO - Icarus
DO - 10.1016/j.icarus.2016.04.008
UR - https://hal.science/hal-05791472v1
SN - 0019-1035
SN - 1090-2643
ER -