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.
| Olympica Fossae: ESP_079985_2060 ESP_079919_2060 (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 | 25.63 | 246. | -9.1 | 8.47 | 47.8 | 46.2 |
| North Polar Residual Cap Topography: ESP_080100_2695 ESP_080075_2695 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 89.45 | 266. | -21. | -22.9 | 66.0 | 65.9 |
| Polar Terrain Sample: ESP_080021_2575 ESP_079968_2575 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.09 | 332. | -8.2 | 7.25 | 57.6 | 56.2 |
| Crater in Arabia Terra: ESP_080007_2175 ESP_079941_2175 (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 | 37.24 | 4.87 | -8.5 | 6.122 | 46.5 | 45.0 |
| North Polar Residual Cap Topography: ESP_079975_2675 ESP_071774_2675 (Interval in Earth days: 639) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.55 | 135. | -18. | -29.7 | 63.9 | 69.6 |
| Dune Interaction with Residual Polar Ice: ESP_080069_2605 ESP_080583_2610 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.66 | 98.6 | -8.3 | 6.294 | 59.7 | 63.1 |
| Vent near Olympica Fossae: ESP_080130_2070 ESP_080407_2070 (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 | 26.88 | 247. | 4.53 | -6.84 | 47.0 | 49.3 |
| Crater Exposing Deposits in Candidate ExoMars Landing Site in Oxia Planum: ESP_080140_1980 ESP_079652_1980 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.61 | 335. | 1.31 | 15.69 | 49.7 | 47.2 |
| North Polar Residual Cap: ESP_080027_2685 ESP_072140_2685 (Interval in Earth days: 615) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.45 | 183. | -27. | -19.8 | 65.4 | 73.7 |
| Valleys along Lower Wallrock Slopes in Juventae Chasma: ESP_079825_1760 ESP_080313_1760 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.19 | 297. | -2.1 | -14.2 | 59.4 | 60.5 |
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