Clouds and Ammonia in the Atmospheres of Jupiter and Saturn Determined From a Band‐Depth Analysis of VLT/MUSE Observations
Journal of Geophysical Research E: Planets American Geophysical Union 130:1 (2025)
A Detailed Study of Jupiter’s Great Red Spot over a 90-day Oscillation Cycle
The Planetary Science Journal IOP Publishing 5:10 (2024) 223
Abstract:
Jupiter’s Great Red Spot (GRS) is known to exhibit oscillations in its westward drift with a 90-day period. The GRS was observed with the Hubble Space Telescope on eight dates over a single oscillation cycle in 2023 December to 2024 March to search for correlations in its physical characteristics over that time. Measured longitudinal positions are consistent with a 90-day oscillation in drift, but no corresponding oscillation is found in latitude. We find that the GRS size and shape also oscillate with a 90-day period, having a larger width and aspect ratio when it is at its slowest absolute drift (minimum date-to-date longitude change). The GRS’s UV and methane gas absorption-band brightness variations over this cycle were small, but the core exhibited a small increase in UV brightness in phase with the width oscillation; it is brightest when the GRS is largest. The high-velocity red collar also exhibited color changes, but out of phase with the other oscillations. Maximum interior velocities over the cycle were about 20 m s−1 larger than minimum velocities, slightly larger than the mean uncertainty of 13 m s−1, but velocity variability did not follow a simple sinusoidal pattern as did other parameters such as longitude width or drift. Relative vorticity values were compared with aspect ratios and show that the GRS does not currently follow the Kida relation.The Thermal Structure and Composition of Jupiter's Great Red Spot From JWST/MIRI
Journal of Geophysical Research Planets American Geophysical Union (AGU) 129:10 (2024)
Data availability and requirements relevant for the Ariel space mission and other exoplanet atmosphere applications
RAS Techniques and Instruments Oxford University Press 3:1 (2024) 636-690
Abstract:
The goal of this white paper is to provide a snapshot of the data availability and data needs primarily for the Ariel space mission, but also for related atmospheric studies of exoplanets and cool stars. It covers the following data-related topics: molecular and atomic line lists, line profiles, computed cross-sections and opacities, collision-induced absorption and other continuum data, optical properties of aerosols and surfaces, atmospheric chemistry, UV photodissociation and photoabsorption cross-sections, and standards in the description and format of such data. These data aspects are discussed by addressing the following questions for each topic, based on the experience of the ‘data-provider’ and ‘data-user’ communities: (1) what are the types and sources of currently available data, (2) what work is currently in progress, and (3) what are the current and anticipated data needs. We present a GitHub platform for Ariel-related data, with the goal to provide a go-to place for both data-users and data-providers, for the users to make requests for their data needs and for the data-providers to link to their available data. Our aim throughout the paper is to provide practical information on existing sources of data whether in data bases, theoretical, or literature sources.NEMESISPY: A Python package for simulating and retrieving exoplanetary spectra
The Journal of Open Source Software The Open Journal 9:101 (2024) 6874-6874