1 citations · 1 across the 4 of their papers we have counts for
4 papers
Cloud and ammonia vertical profiles in the equatorial atmosphere of Jupiter determined from visible to near-IR observations made by VLT/MUSE, Cassini/VIMS, IRTF/SpeX and Juno/JIRAM
Patrick G. J. Irwin, Asier Anguiano-Arteaga, Michelle Colantoni +8
We present a combined cloud/ammonia model for Jupiter's equatorial atmosphere from 0.1 to 10 bar, consistent with observations made at a range of observation geometries from 0.35 t…
Colour changes of Jupiter's Oval BA through microphysical modelling
Asier Anguiano-Arteaga, Santiago Pérez-Hoyos, Agustín Sánchez-Lavega +1
Jupiter's Oval BA undergoes recurrent colour changes whose physical origin remains uncertain. Radiative transfer retrievals indicate that these changes occur in the upper chromopho…
A Processing Workflow for Cassini VIMS Jupiter Cubes
Asier Anguiano-Arteaga, Patrick G. J. Irwin, Santiago Pérez-Hoyos +2
We present a calibrated catalog of Cassini Visible and Infrared Mapping Spectrometer (VIMS) observations of Jupiter, together with the processing workflow used to generate the fina…
Microphysical Model of Jupiter's Great Red Spot Upper Chromophore Haze
Asier Anguiano-Arteaga, Santiago Perez-Hoyos, Agustin Sanchez-Lavega +1
The origin of the red colouration in Jupiter's Great Red Spot (GRS) is a long-standing question in planetary science. While several candidate chromophores have been proposed, no cl…