collaborators

5 papers

astro-ph.EP2026

Juno Microwave Observations Reveal Jupiter's Deep Alkali-Chlorine Relation

Xi Zhang, Jiheng Hu, Cheng Li +2

The longest-wavelength channel of the Juno Microwave Radiometer (MWR) probes Jupiter's kilobar atmosphere through free electrons produced by sodium and potassium ionization. Under…

astro-ph.EP2026

Implications of a Stable Layer on the Vertical Structure of Jet Streams on Jupiter

Keren Duer-Milner, Louis Siebenaler, Lillian Haley +1

The vertical structure of Jupiter's jet streams remains a critical open question for understanding the planet's atmospheric dynamics and interior. Traditional models often assume a…

astro-ph.EP2026

Mean opacity tables for probing the interior and atmosphere of giant planets

Louis Siebenaler, Yamila Miguel

We present new Rosseland and Planck mean opacity tables relevant to the shallow interiors and atmospheres of giant planets. The tables span metallicities from 0.31 to 50 times sola…

astro-ph.IM2025

pyROX: Rapid Opacity X-sections

Sam de Regt, Siddharth Gandhi, Louis Siebenaler +1

In recent years, significant advances have been made in exoplanet and brown dwarf observations. By using state-of-the-art models, astronomers can determine properties of their atmo…

astro-ph.EP2025

Conditions for radiative zones in the molecular hydrogen envelope of Jupiter and Saturn: The role of alkali metals

Louis Siebenaler, Yamila Miguel, Sam de Regt +1

Interior models of gas giants in the Solar System traditionally assume a fully convective molecular hydrogen envelope. However, recent observations from the Juno mission suggest a…