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.
| Faults in Ius Chasma: PSP_008010_1720 PSP_009658_1720 (Interval in Earth days: 129) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.82 | 279. | -4.9 | 7.572 | 54.5 | 59.5 |
| Layered Terrain on Hellas Basin Floor: PSP_007399_1385 ESP_016563_1385 (Interval in Earth days: 715) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.4 | 48.4 | -6.2 | 22.94 | 69.9 | 72.6 |
| Valley Juncture Along Plains West of Ganges Chasma with Light-Toned Deposit: PSP_008009_1715 PSP_009578_1715 (Interval in Earth days: 122) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.51 | 306. | 1.52 | -24.6 | 54.4 | 62.1 |
| Vertical Exposure of Layering in West Candor Chasma: PSP_007021_1740 PSP_007232_1740 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.82 | 283. | 5.28 | -9.86 | 42.3 | 45.8 |
| Cut Crater in Ganges Chasma: PSP_008101_1710 ESP_016263_1710 (Interval in Earth days: 636) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.91 | 314. | -5.3 | 21.95 | 55.9 | 47.3 |
| Well-Preserved 40-Kilometer Diameter Unnamed Crater Near Tartarus Region: PSP_007091_1995 PSP_007447_1995 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.43 | 170. | -0.1 | -9.73 | 39.0 | 40.9 |
| Ridges and Mounds Near Hecates Tholus: PSP_007672_2155 PSP_007883_2155 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.92 | 142. | 6.64 | -7.98 | 40.8 | 42.0 |
| Fresh 10-Kilometer Diameter Unnamed Crater in Terra Sabaea: PSP_007966_1615 ESP_025055_1615 (Interval in Earth days: 1331) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.1 | 41.5 | 5.02 | 25.73 | 59.9 | 51.0 |
| Bright Gully Fans: PSP_007429_2440 PSP_008141_2440 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 63.78 | 292. | 2.14 | -7.16 | 55.0 | 50.5 |
| Central Peak Region of Canso Crater: PSP_007139_2015 ESP_085442_2015 (Interval in Earth days: 6101) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.34 | 299. | -1.5 | -10.2 | 39.3 | 44.2 |
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