Data for: Power spectrum analysis of Jupiter’s South Pole clouds by Juno/JIRAM data

Name: Data for: Power spectrum analysis of Jupiter’s South Pole clouds by Juno/JIRAM data
Creator: Maria Luisa Moriconi
Published: 2019-09-09T12:14:56.056Z
Keywords: Planetary Atmosphere, Fourier Analysis, Atmospheric Turbulence, Polar Regions

Moriconi, Maria Luisa; Migliorini, Alessandra; Altieri, Francesca; Adriani, Alberto; Mura, Alessandro; Orton, Glenn; Lunine, Jonathan; Grassi, Davide; Atreya, Sushil; Ingersoll, Andrew; Dinelli, Bianca; Bolton, Scott; Levin, Steven; Tosi, Federico; Noschese, Raffaella; Plainaki, Christina; Cicchetti, Andrea; Sindoni, Giuseppe; Olivieri, Angelo

doi:10.17632/4f3mrkcxvb.2

Data for: Power spectrum analysis of Jupiter’s South Pole clouds by Juno/JIRAM data

Published: 9 September 2019| Version 2 | DOI: 10.17632/4f3mrkcxvb.2

Contributors:

Maria Luisa Moriconi, Alessandra Migliorini, Francesca Altieri, Alberto Adriani, Alessandro Mura, Glenn Orton, Jonathan Lunine, Davide Grassi, Sushil Atreya, Andrew Ingersoll, Bianca Dinelli, Scott Bolton, Steven Levin, Federico Tosi, Raffaella Noschese, Christina Plainaki, Andrea Cicchetti, Giuseppe Sindoni, Angelo Olivieri

Description

The files equatorward_PSD.txt and poleward_PSD.txt contain power spectral densities (PSD) from JIRAM data acquired at Jupiter's South Pole. The PSDs are computed by means of FFT applied at circular brightness scans outside (file equatorward_PSD.txt) and inside (file poleward_PSD.txt) the circular ring of cyclones. These data refer to the paper "Power spectrum analysis of Jupiter’s South Pole clouds by Juno/JIRAM data" submitted to JGR planets. In the first column the wavenumber bin values are reported, while in the second to seventh columns the PSD from six juno perijove's passes are reported.

Data for: Power spectrum analysis of Jupiter’s South Pole clouds by Juno/JIRAM data

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