Table 1.

Input Galileo Image Sequences Used for Constructing the High‐Resolution Base Mosaic

Galileo mosaic	Latitude range	Pixel scale (m)	Incidence angle	Emission angle
11ESREGMAP01	20.2°S–9.2°N	219–222	70.8°–85.5°	12.1°–36.6°
15ESREGMAP01	18.4°N–61.3°N	228–235	69.3°–87.6°	19.1°–64.1°
17ESNERTRM01	47.6°S–6.4°N	210–212	76.1°–84.9°	7.8°–41.3°
17ESREGMAP01	70.4°S–20°N	222–228	50.8°–85.6°	0°–68.5°
19ESNORLAT01	49.2°N–84.9°N	202	73.6°–88.6°	53.0°–90°
19ESNORPLN01	57.1°N–76.9°N	166–171	74.4°–85.5°	60.7°–90°
19ESREGMAP01	11.7°N–20.1°N	201–203	73.8°–90°	13.6°–29.7°
Other images in mosaic that are not used in plate reconstructions in this study
C3ESWEDGES01	18.9°S–10.2°S	421	71.8°–81.5°	13.0°–25.9°
14ESWEDGES01	36.7°S–12.5°S	230–238	34.1°–63.5°	24.2°–55.0°
17ESAGENOR01	44.4°S–38.7°S	187–206	50.6°–71.2°	34.2°–51.1°
Background images used in mosaic
G1ESGLOBAL01	50°S–85°N	1,570–1,582	0°–90°	0°–77°
14ESGLOCOL01	82°S–22°N	1,439–1,456	7°–90°	0°–90°

Note. This mosaic has been utilized in the community beyond our plate reconstruction project, and is sometimes referred to in conference abstracts as the “Supermosaic” (Laura & Beyer, 2021).