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.
| 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 |
| Light-Toned Tilted Layering in Central Peak of Oudemans Crater: PSP_007694_1700 ESP_027882_1700 (Interval in Earth days: 1574) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.92 | 268. | 1.09 | -17.4 | 52.3 | 59.3 |
| Finely-Layered Fan Deposit of Possible Subaqueous Origin: PSP_007087_1700 PSP_007667_1700 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.81 | 283. | -7.7 | 22.30 | 45.8 | 50.5 |
| 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 |
| 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 |
| Contact between Two Different Units in Ganges Mensa: PSP_007666_1725 PSP_008022_1725 (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 | -7.65 | 311. | 6.47 | -5.41 | 50.4 | 54.5 |
| Fresh Crater in Tyrrhena Terra: PSP_007172_1680 PSP_007462_1680 (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 | -11.7 | 122. | -7.6 | 6.154 | 47.7 | 50.4 |
| Light-Toned Rock in Central Peak of Alga Crater: PSP_007573_1555 PSP_007929_1555 (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 | -24.3 | 333. | 8.34 | -3.28 | 59.4 | 64.1 |
| Gullies and Bedrock Exposures in Impact Crater Wall: PSP_008153_1480 PSP_009155_1480 (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 | -31.4 | 337. | 4.51 | -12.3 | 70.8 | 76.3 |
| 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 |
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