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.
| Monitoring East Headscarp of Chasma Boreale: PSP_009944_2650 PSP_009943_2650 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.69 | 3.94 | -8.0 | 12.57 | 65.0 | 64.2 |
| Ejecta Flow Around Obstacles in Eastern Elysium Region: PSP_010018_2000 PSP_010519_2000 (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 | 19.94 | 168. | -4.6 | 18.56 | 49.5 | 50.4 |
| 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 |
| Exposure of Light-Toned Layering along Wallrock in Coprates Chasma: PSP_009684_1695 PSP_010396_1695 (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 | -10.2 | 290. | -2.2 | 19.86 | 61.5 | 58.8 |
| Unconformity in Gemini Lingula Layered Deposits: PSP_009482_2605 PSP_009878_2605 (Interval in Earth days: 31) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.31 | 22.5 | -0.8 | -19.1 | 58.4 | 62.7 |
| Clays Exposed in Channels along West Ladon Valles: PSP_010342_1600 ESP_034552_1600 (Interval in Earth days: 1886) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.6 | 327. | 0.85 | -19.2 | 65.0 | 63.0 |
| 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 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_009309_2725 PSP_009589_2675 (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 | 87.52 | 327. | -4.7 | -14.4 | 64.2 | 64.4 |
| Cluster of Craters and Edifices on Top of Mesa: PSP_009642_2215 PSP_010143_2215 (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 | 41.10 | 350. | -1.2 | 16.64 | 45.5 | 47.8 |
| A North Polar Crater: PSP_009689_2645 PSP_010084_2645 (Interval in Earth days: 31) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.33 | 120. | -1.7 | 12.07 | 62.3 | 65.3 |
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