How well do we understand the belt/zone circulation of giant planet atmospheres?
The atmospheres of the four giant planets of our Solar System share a common and well-
observed characteristic: they each display patterns of planetary banding, with regions of …
observed characteristic: they each display patterns of planetary banding, with regions of …
Jupiter science enabled by ESA's Jupiter icy moons explorer
Abstract ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …
A high spatial and spectral resolution study of Jupiter's mid-infrared auroral emissions and their response to a solar wind compression
We present mid-infrared spectroscopy of Jupiter's mid-to-high latitudes using the Gemini-
North/Texas Echelon Cross Echelle Spectrograph on 2017 March 17–19. These …
North/Texas Echelon Cross Echelle Spectrograph on 2017 March 17–19. These …
Ice giant circulation patterns: implications for atmospheric probes
LN Fletcher, I de Pater, GS Orton, MD Hofstadter… - Space Science …, 2020 - Springer
Atmospheric circulation patterns derived from multi-spectral remote sensing can serve as a
guide for choosing a suitable entry location for a future in situ probe mission to the Ice …
guide for choosing a suitable entry location for a future in situ probe mission to the Ice …
Enhanced C2H2 Absorption Within Jupiter's Southern Auroral Oval From Juno UVS Observations
Reflected sunlight observations from the Ultraviolet Spectrograph (UVS) on the Juno
spacecraft were used to study the distribution of acetylene (C2H2) at Jupiter's south pole …
spacecraft were used to study the distribution of acetylene (C2H2) at Jupiter's south pole …
Jupiter's equatorial plumes and hot spots: Spectral mapping from Gemini/TEXES and Juno/MWR
We present multiwavelength measurements of the thermal, chemical, and cloud contrasts
associated with the visibly dark formations (also known as 5‐μm hot spots) and intervening …
associated with the visibly dark formations (also known as 5‐μm hot spots) and intervening …
The polar stratosphere of Jupiter
Observations of the Jovian upper atmosphere at high latitudes in the UV, IR and mm/sub-
mm all indicate that the chemical distributions and thermal structure are broadly influenced …
mm all indicate that the chemical distributions and thermal structure are broadly influenced …
Photochemistry, mixing and transport in Jupiter's stratosphere constrained by Cassini
In this work, we aim at constraining the diffusive and advective transport processes in
Jupiter's stratosphere, using Cassini/CIRS observations published by Nixon et al.(2007 …
Jupiter's stratosphere, using Cassini/CIRS observations published by Nixon et al.(2007 …
Radiative-equilibrium model of Jupiter's atmosphere and application to estimating stratospheric circulations
Jupiter's upper troposphere and stratosphere are host to a rich dynamical and chemical
activity. This modulates the thermal structure and distribution of trace species and aerosols …
activity. This modulates the thermal structure and distribution of trace species and aerosols …
Shaping of Silver-Functionalized Metal–Organic Frameworks for Efficient Separation of Ethylene Over Ethane
Z Li, C Wang, T Wang, Y Liu, X Zhao, T Xia… - Industrial & …, 2024 - ACS Publications
Separation of the ethane/ethylene mixture is one of the most important but challenging
processes in the petrochemical industry owing to their closely resembling physical and …
processes in the petrochemical industry owing to their closely resembling physical and …