POSEIDON now includes lab-derived rocky surface albedos, enabling JWST emission spectra to separate thin versus thick atmospheres and potentially identify granite-like versus basaltic surfaces.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2representative citing papers
BCA codes fail to reproduce both sputter yields and angular distributions for He-irradiated minerals, revealing a structural limitation when modeling rough or porous planetary surfaces.
citing papers explorer
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The Rocky Planet Picture Show: Implementation of Surface Reflection and Emission in $\texttt{POSEIDON}$ with Application to and Interpretation of JWST Data
POSEIDON now includes lab-derived rocky surface albedos, enabling JWST emission spectra to separate thin versus thick atmospheres and potentially identify granite-like versus basaltic surfaces.
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Limitations of Using BCA Codes for Modeling the Sputtering Behavior of Planetary Surfaces
BCA codes fail to reproduce both sputter yields and angular distributions for He-irradiated minerals, revealing a structural limitation when modeling rough or porous planetary surfaces.