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.
| Crater with Gullies Seen in MOC Image E14-02164: PSP_007250_1415 ESP_015979_1415 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.3 | 155. | 5.87 | -13.0 | 64.8 | 64.5 |
| Dark Dune-Like Forms in Southern Melas Chasma: PSP_007522_1685 ESP_025666_1685 (Interval in Earth days: 1414) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.1 | 284. | 0.94 | -27.7 | 51.1 | 56.6 |
| Wrinkle Ridge: PSP_007052_1870 ESP_016361_1870 (Interval in Earth days: 726) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.101 | 156. | -6.0 | 26.66 | 39.8 | 40.6 |
| Reull Vallis: PSP_007819_1390 PSP_009612_1390 (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 | -40.6 | 99.6 | -6.4 | 7.67 | 74.7 | 81.0 |
| Possible Submarine Fan in Eastern Portion of Small Melas Chasma Basin: PSP_007377_1700 PSP_008379_1700 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.82 | 283. | 5.56 | -6.99 | 48.4 | 58.5 |
| Layers and Scallops: PSP_007252_2265 PSP_007687_2265 (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 | 46.28 | 90.9 | -7.8 | 5.11 | 47.3 | 44.0 |
| Eroded Craters on the Medusae Fossae Formation: PSP_008186_1840 PSP_009267_1840 (Interval in Earth days: 84) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.049 | 152. | -4.4 | 16.56 | 49.4 | 52.0 |
| Landforms in Eastern Amazonis Planitia: PSP_008131_1930 PSP_008421_1930 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.68 | 213. | -6.4 | 3.766 | 45.6 | 46.2 |
| Central Peak of Large Crater in Northwest Arabia Terra: PSP_007664_2160 ESP_045443_2160 (Interval in Earth days: 2944) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.80 | 0.55 | 8.68 | -7.28 | 40.8 | 44.8 |
| Layering in East Coprates Chasma Wall: PSP_007864_1655 PSP_007508_1655 (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 | -14.1 | 307. | -8.1 | 4.599 | 57.2 | 52.4 |
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