Data for: Power spectrum analysis of Jupiter’s South Pole clouds by Juno/JIRAM data
The files SFT_81d7_PSD_ave&STDA, equatorward_PSD.txt and poleward_PSD.txt refer to Figure 2 and 3 respectively of the paper " Turbulence Power Spectra in Regions Surrounding Jupiter's South Polar Cyclones from Juno/JIRAM " submitted to JGR planets. They contain average power spect...
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| Format: | Dataset |
| Language: | unknown |
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Mendeley
2020
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| Online Access: | https://dx.doi.org/10.17632/4f3mrkcxvb.3 https://data.mendeley.com/datasets/4f3mrkcxvb/3 |
| Summary: | The files SFT_81d7_PSD_ave&STDA, equatorward_PSD.txt and poleward_PSD.txt refer to Figure 2 and 3 respectively of the paper " Turbulence Power Spectra in Regions Surrounding Jupiter's South Polar Cyclones from Juno/JIRAM " submitted to JGR planets. They contain average power spectral densities (PSDs) from JIRAM data acquired at Jupiter's South Pole. The PSDs are computed by means of FFT applied to circular brightness scans extracted from JIRAM images. In the file SFT_81d7_PSD_ave&STDA the wavenumber bin values (column 1), the average PSD (column 2) and the error bars (column 3), related to the equatorward dataset of the Juno’s 4th perijove, are reported. The files equatorward_PSD.txt and poleward_PSD.txt refer to PSDs computed for regions equatorward and poleward the ring of cyclones at Jupiter's South Pole. In both files the first column contains the wavenumber bin values, while in column 2 to column 7 the PSDs from six Juno perijove's passes are reported. Figure 4c.pdf, Figure 4d.png and Figure 4e.png are the single panels of Figure 4 in the paper. They are in sequence: the inverse FFT of the JIR_IMG_RDR_2017033T150327_V01 dataset after high-pass filtering (from the Juno’s 4th perijove), the detail of the region into the black square of Figure 4c and the detail of the region inside the red circle of Figure 4c. |
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