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.
| Pasted-on Material on Crater Ejecta : ESP_050957_1835 ESP_052025_1835 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.147 | 297. | -0.6 | 29.33 | 35.6 | 42.4 |
| Candidate ExoMars Landing Site in Oxia Palus : ESP_051272_1985 ESP_071529_1985 (Interval in Earth days: 1578) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.46 | 335. | 6.24 | 27.25 | 35.7 | 47.6 |
| Central Structure of Impact Crater : ESP_051128_1495 ESP_059238_1495 (Interval in Earth days: 632) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.4 | 315. | -20. | 1.812 | 55.8 | 43.2 |
| Layering in Walls in Depression in Nereidum Montes : ESP_050904_1425 ESP_051049_1425 (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 | -37.2 | 309. | 7.87 | 19.67 | 55.5 | 57.1 |
| Knobs in West Candor Chasma : ESP_050918_1750 ESP_051762_1750 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.12 | 283. | 4.71 | -22.3 | 37.1 | 48.3 |
| Hellas Planitia Sand Dune Changes : ESP_051190_1315 ESP_051111_1315 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.1 | 61.0 | 20.5 | -6.00 | 67.7 | 67.8 |
| Exposed Bedrock Ridges with Flow Pitted Material in Hale Crater Ejecta : ESP_050943_1440 ESP_050666_1440 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.7 | 325. | -1.9 | 25.98 | 55.5 | 49.3 |
| Channel and Fan Structure of Ceraunius Tholus : ESP_050945_2050 ESP_051235_2050 (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 | 24.69 | 262. | 2.86 | 27.57 | 37.0 | 34.5 |
| Tilted Layers in Electris Region : ESP_051146_1430 ESP_051001_1430 (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 | -36.5 | 182. | 7.45 | -5.79 | 58.8 | 57.2 |
| Contact in Western Hellas Planitia : ESP_050979_1415 ESP_051124_1415 (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 | -37.9 | 63.2 | -6.8 | 5.638 | 58.0 | 59.6 |
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