Vertically Resolved Magma Ocean–Protoatmosphere Evolution: H 2 , H 2 O, CO 2 , CH 4 , CO, O 2 , and N 2 as Primary Absorbers-Reference-Cited by-同舟云学术

Vertically Resolved Magma Ocean–Protoatmosphere Evolution: H 2 , H 2 O, CO 2 , CH 4 , CO, O 2 , and N 2 as Primary Absorbers

Published:2021-02 Issue:2 Volume:126 Page:
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J Geophys Res Planets

Author:

Lichtenberg Tim¹^ORCID,Bower Dan J.²^ORCID,Hammond Mark³^ORCID,Boukrouche Ryan¹^ORCID,Sanan Patrick⁴^ORCID,Tsai Shang‐Min¹^ORCID,Pierrehumbert Raymond T.¹^ORCID

Affiliation:

1. Atmospheric, Oceanic and Planetary Physics, Department of Physics University of Oxford Oxford UK

2. Center for Space and Habitability University of Bern Bern Switzerland

3. Department of the Geophysical Sciences University of Chicago Chicago IL USA

4. Institute of Geophysics, Department of Earth Sciences ETH Zurich Zurich Switzerland

Funder

Simons Foundation

H2020 European Research Council

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020JE006711

Reference189 articles.

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2. Abe Y.(1995).Basic equations for evolution of partially molten mantle and core. InT.Yukutake(Ed.) The Earth’s central part: Its structure and dynamics(pp.215–230).Tokyo:Terra Scientific Publishing Company.

3. Thermal and chemical evolution of the terrestrial magma ocean

4. Early evolution of the Earth: Accretion, atmosphere formation, and thermal history

5. Accuracy tests of radiation schemes used in hot Jupiter global circulation models

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