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.
| Unmantled Central Uplift Feature in Unnamed Crater: PSP_007526_1435 PSP_010875_1435 (Interval in Earth days: 261) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.4 | 178. | 4.32 | -6.88 | 67.4 | 70.7 |
| 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 |
| 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 |
| Possible Chloride Salt Deposit: PSP_007058_1745 ESP_016354_1745 (Interval in Earth days: 724) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.62 | 353. | 4.05 | -22.5 | 42.7 | 49.8 |
| 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 |
| Possible Sulfates in Ius Chasma: PSP_007074_1725 ESP_060136_1725 (Interval in Earth days: 4135) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.31 | 276. | 8.87 | -0.48 | 43.3 | 43.5 |
| 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 |
| Possible Sulfates in Ius Chasma: PSP_007509_1720 ESP_050839_1720 (Interval in Earth days: 3376) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.70 | 279. | -2.3 | 13.43 | 49.3 | 36.5 |
| Flows into the Isidis Basin: PSP_007727_1830 PSP_008808_1830 (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 | 3.147 | 85.9 | -5.8 | 5.575 | 46.5 | 52.1 |
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