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.
| Athabasca Valles Lava Contact Relation: ESP_051002_1840 ESP_053204_1840 (Interval in Earth days: 172) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.995 | 149. | -1.3 | 7.887 | 35.9 | 49.0 |
| East Ophir Chasma Floor : ESP_051287_1755 ESP_051999_1755 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.24 | 289. | -0.1 | 23.09 | 41.2 | 46.7 |
| Possible Repetitive Bedding in Eastern Medusae Fossae Formation : ESP_050960_1835 ESP_051105_1835 (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 | 3.559 | 216. | -3.8 | 11.32 | 35.8 | 35.8 |
| Meroe Patera Dune Monitoring : ESP_051084_1875 ESP_050939_1875 (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 | 7.174 | 67.7 | 25.4 | 12.24 | 33.7 | 33.9 |
| Layered Light-Toned Deposits on Floor of Orson Welles Crater : ESP_050996_1790 ESP_051919_1790 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.19 | 313. | -4.7 | 10.12 | 37.3 | 45.3 |
| 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 |
| 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 |
| Streamlined Forms in Lava Channel : ESP_051104_1940 ESP_051249_1940 (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 | 14.08 | 242. | 5.71 | 20.15 | 35.0 | 34.4 |
| 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 |
| Channel East of Olympus Mons : ESP_051012_1990 ESP_051856_1990 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.60 | 233. | 7.07 | -16.2 | 35.1 | 39.7 |
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