Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| Ganges Catena Pit Crater Chain Cut by Wrinkle Ridge: PSP_008326_1775 PSP_008827_1775 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.33 | 289. | 5.91 | -12.9 | 52.9 | 56.5 |
| Landslides in Ganges Chasma: PSP_009037_1715 PSP_009538_1715 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.54 | 315. | -14. | 7.943 | 60.9 | 59.8 |
| Potential Phyllosilicates in Acidalia Region: PSP_009182_2215 PSP_009472_2215 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.28 | 309. | -4.4 | 16.00 | 43.6 | 43.0 |
| Possible Gullies in Dunes: PSP_008751_1795 PSP_009186_1795 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.40 | 204. | -13. | 14.12 | 55.2 | 54.4 |
| Light Toned Materials and Plains in South Meridiani (MSL): PSP_009563_1770 PSP_009708_1770 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.06 | 354. | -15. | 0.701 | 58.4 | 57.3 |
| Central Peak and Floor of Large Crater West of Schiaparelli Crater: PSP_008613_1760 PSP_008969_1760 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.93 | 12.2 | 1.91 | -18.6 | 55.6 | 58.3 |
| Depression at the Base of a Hill in the Hibes Montes: PSP_008884_1845 ESP_020000_1845 (Interval in Earth days: 866) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.255 | 170. | 3.27 | -9.06 | 51.9 | 55.1 |
| Merging Lobate Debris Aprons of Deuteronilus Mensae: PSP_008744_2240 PSP_009535_2240 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.76 | 29.3 | -6.2 | 15.83 | 43.0 | 43.5 |
| Cratered Cones in Isidis Region: PSP_008887_1985 PSP_009177_1985 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.11 | 88.2 | -12. | 9.193 | 47.0 | 46.1 |
| Flows on the Northeastern Flank of Arsia Mons: PSP_008565_1720 PSP_009844_1720 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.68 | 242. | 9.15 | -10.2 | 57.2 | 60.4 |
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