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diskEvolution documentation
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Contents:
Introduction
Background
Geochemical characteristics of the Earth- Moon system:
Model:
Step 1: Setting up a magma disk and evolving it over time:
Step 2: Adding Temperature gradient to the Proto-Lunar disk:
Step 3: Adding atmosphere to the proto-Earth and the proto-Lunar disk:
Step 4: Adding tracer species (for volatile transport as well as Isotopic signatures):
Getting Started
Examples
References
Indices and tables
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