Table 1.
Basic Information of the global maps of Jupiter and Saturn.
| Planet | Filter (Wavelength) | Number of Maps | Observational Time | Spatial Resolution |
|---|---|---|---|---|
| Jupiter | BL1 (455 nm) | 6 | Dec. 7–16, 2000 | 103–145 km/pixel |
| Jupiter | CB2 (750 nm) | 6 | Dec. 7–16, 2000 | 103–145 km/pixel |
| Jupiter | MT3 (889 nm) | 4 | Dec. 7–16, 2000 | 103–145 km/pixel |
| Jupiter | UV1 (264 nm) | 3 | Dec. 7–14, 2000 | 227–289 km/pixel |
| Saturn | MT2 (728 nm) | 1 | Oct. 23, 2009 | 110–111 km/pixel |
| Saturn | RED (647 nm) | 1 | Aug. 12, 2011 | 161 km/pixel |
| Saturn | GRN (568 nm) | 1 | Aug. 12, 2011 | 161 km/pixel |
| Saturn | BL1 (463 nm) | 1 | Aug. 12, 2011 | 161 km/pixel |
| Saturn | RGB | 2 | Aug. 12, 2011 | 161 km/pixel |
Note: The wavelength corresponding to each filter represents the effective wavelength. The BL1 filter wavelength for Jupiter corresponds to the narrow-angle camera, while the BL1 filter wavelength for Saturn corresponds to the wide-angle camera in the ISS. Each global map of Jupiter and Saturn is constructed using several ISS images taken over 8–11 hours, with varying spatial resolutions. “RGB” refers to color global maps composed of three individual global maps captured using the RED, GRN, and BL1 filters, respectively. The two RGB maps of Saturn represent the original map and the feature-contrast-enhanced map, respectively. More information on these global maps of Jupiter and Saturn is available on the Planetary Atmospheres Node of NASA’s Planetary Data System (PDS) website (https://atmos.nmsu.edu/data_and_services/atmospheres_data/Cassini/sat_global_map.html).