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.
| Fresh Small Impact Crater on Rim of Much Larger Crater : ESP_053737_1720 ESP_060700_1720 (Interval in Earth days: 543) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.15 | -0.3 | -5.2 | 7.347 | 57.1 | 49.8 |
| Flow Lobes in Northern Plains Crater : ESP_053753_2505 ESP_061824_2505 (Interval in Earth days: 629) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 70.32 | 266. | 7.54 | -9.99 | 52.6 | 51.4 |
| Sample Terrain between Candidate Landing Sites for 2020 Mission : ESP_053734_1985 ESP_055145_1985 (Interval in Earth days: 110) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.27 | 77.3 | 5.83 | -7.23 | 43.9 | 52.3 |
| North Polar Residual Cap Topography : ESP_053780_2715 ESP_053491_2715 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.33 | 75.7 | -26. | -19.2 | 68.5 | 66.1 |
| Scalloped Depression : ESP_053694_2240 ESP_053984_2240 (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 | 43.57 | 85.9 | 2.72 | 21.56 | 42.2 | 42.5 |
| Landforms and Dark-Toned Surface at Apparent Distal End of Hrad Vallis : ESP_053653_2235 ESP_053508_2235 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.97 | 125. | 4.87 | -4.79 | 41.7 | 41.9 |
| Chasma Boreale Sand Production : ESP_053711_2625 ESP_053751_2625 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.64 | 315. | 6.93 | -8.10 | 60.1 | 61.2 |
| Candidate Landing Site for 2020 Mission in Northeast Syrtis Major Region : ESP_053945_1985 ESP_053879_1985 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.23 | 77.2 | -1.0 | 19.86 | 45.0 | 43.1 |
| Transition from Cratered Upland to Southwest Chryse Planitia : ESP_053765_1960 ESP_060860_1960 (Interval in Earth days: 553) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.47 | 310. | 19.9 | -5.80 | 43.7 | 41.3 |
| Gypsum Dunes : ESP_053821_2605 ESP_053729_2605 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.41 | 198. | 7.77 | -6.06 | 59.3 | 59.4 |
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