New 4D tables of giant planet atmosphere boundary conditions and spectra with consistent metal EOS, showing on-the-fly interpolation changes late-stage evolution and helium depletion.
Evi- dence of hydrogen-helium immiscibility at Jupiter-interior conditions
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The paper reviews the use of the imaginary-time correlation function to extract temperature, normalization, and Rayleigh weight from XRTS spectra without model dependence.
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Next-Generation Atmosphere Models for Giant Planets with Application to Coupled Interior Composition and Spectral Evolution I: Cloudless Models with Equilibrium Chemistry
New 4D tables of giant planet atmosphere boundary conditions and spectra with consistent metal EOS, showing on-the-fly interpolation changes late-stage evolution and helium depletion.