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.
| Sinuous Ridge in Aeolis Region: PSP_007395_1775 ESP_016414_1775 (Interval in Earth days: 703) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.46 | 151. | 8.20 | 27.01 | 44.8 | 45.0 |
| 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 |
| Light Outcrop in Aurorae Chaos: PSP_007705_1730 PSP_009498_1730 (Interval in Earth days: 140) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.78 | 327. | -5.9 | 5.161 | 51.2 | 59.1 |
| Well-Preserved 15-Kilometer Diameter Crater Near Nili Fossae: PSP_007912_2030 ESP_018342_2030 (Interval in Earth days: 813) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.63 | 71.3 | 0.11 | 15.86 | 41.5 | 43.9 |
| 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 |
| Diverse Features in Utopia Region: PSP_007951_2220 PSP_008162_2220 (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 | 41.58 | 82.8 | 6.93 | -5.86 | 41.7 | 42.5 |
| Wall Layers of Tooting Crater: PSP_007907_2035 ESP_019115_2035 (Interval in Earth days: 873) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.18 | 208. | -2.3 | 5.434 | 41.6 | 48.0 |
| Light-Toned Layering in Melas Chasma: PSP_007812_1700 PSP_010660_1700 (Interval in Earth days: 222) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.87 | 285. | 5.77 | -12.6 | 53.1 | 60.5 |
| Light-Toned Rock Exposures: PSP_007101_1730 ESP_019311_1730 (Interval in Earth days: 952) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.99 | 260. | -7.9 | 3.361 | 44.7 | 56.7 |
| Well-Peserved Large Crater with Central Peak and Pit: PSP_007366_1360 ESP_024732_1360 (Interval in Earth days: 1353) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.4 | 229. | 2.46 | -27.4 | 70.5 | 67.3 |
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