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.
| Polar Layered Deposits Unconformity: PSP_010048_2615 PSP_010509_2615 (Interval in Earth days: 36) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.49 | 49.1 | -3.5 | 16.55 | 63.8 | 68.5 |
| Exposure of North Polar Layered Deposits: PSP_009967_2660 PSP_009980_2660 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.86 | 102. | -16. | -13.4 | 66.5 | 66.4 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_010130_2675 PSP_010263_2675 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.47 | 297. | -7.6 | -19.1 | 68.9 | 70.9 |
| Stratigraphy Exposed in Ausonia Cavus: PSP_009889_1480 ESP_079872_1480 (Interval in Earth days: 5452) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.7 | 96.8 | -1.5 | 12.44 | 74.4 | 76.4 |
| Rayed Crater on Southeast Flank of Elysium Mons: PSP_009333_2025 PSP_009834_2025 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.46 | 151. | -21. | -0.87 | 47.7 | 47.8 |
| Fluvial and Alluvial Features on North Wall of Eos Chasma: PSP_009894_1665 PSP_010606_1665 (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 | -13.3 | 317. | 3.44 | 21.18 | 62.6 | 59.5 |
| Sapping Features East of Tooting Crater: PSP_010333_2025 PSP_010689_2025 (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 | 22.14 | 208. | -3.9 | 0.754 | 50.8 | 53.1 |
| Mounds in Ulysses Fossae: PSP_009409_1860 PSP_009554_1860 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.804 | 237. | -7.2 | 8.646 | 53.1 | 52.1 |
| Look for Change Due to Mass Wasting on Scarps of Different Slopes: PSP_009408_2640 PSP_009882_2640 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.00 | 230. | 0.72 | 16.89 | 60.3 | 62.9 |
| Gullies in North Mid-Latitude Crater: PSP_009744_2305 PSP_010245_2305 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.11 | 84.3 | -0.6 | 14.78 | 47.4 | 50.9 |
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