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Published March 12, 2021 | Version v1
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Data accompanying the paper "Early habitability and crustal decarbonation of a stagnant-lid Venus"

Authors/Creators

  • 1. VU Amsterdam
  • 2. TU Berlin, DLR Berlin
  • 3. DLR Berlin
  • 4. NASA New York, GSFC Collaboration, Uppsala University

Description

Produced data from a coupled interior-atmosphere model depicting Venus' early evolution assuming stagnant-lid convection, CO2 degassing, weathering, carbonate burial, and crustal decarbonation. The data accompanies the paper "Early habitability and crustal decarbonation of a stagnant-lid Venus", submitted to JGR: Planets.

Files

data.zip

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