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.
| Cerberus Fossae Ripple Changes: ESP_065863_1875 ESP_065929_1875 (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 | 7.577 | 167. | 4.24 | -9.95 | 57.1 | 57.5 |
| Active Gully in Matara Crater: ESP_065789_1300 ESP_065934_1300 (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 | -49.4 | 34.8 | 7.58 | 29.10 | 47.6 | 44.3 |
| Low Thermal Inertia Mound in Terra Sabaea Bedrock Plain: ESP_066039_1605 ESP_074968_1605 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.0 | 48.7 | -2.1 | 8.696 | 44.8 | 41.0 |
| Small Shield in Eastern Tharsis Region: ESP_065794_1790 ESP_066757_1790 (Interval in Earth days: 75) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.94 | 252. | 3.39 | -10.0 | 53.4 | 44.7 |
| Graben and Lava Flows East of Arsia Mons: ESP_065834_1685 ESP_065768_1685 (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 | -11.1 | 242. | -8.6 | 7.596 | 49.8 | 49.3 |
| Layers in Depression South of Antoniadi Crater: ESP_065867_1940 ESP_074928_1940 (Interval in Earth days: 706) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.06 | 57.9 | 3.81 | -6.21 | 60.8 | 58.3 |
| Outflow Channel from Morella Crater: ESP_065792_1700 ESP_057880_1700 (Interval in Earth days: 617) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.85 | 309. | -13. | 5.997 | 51.0 | 33.6 |
| Candidate ExoMars Landing Site in Oxia Planum: ESP_065936_1985 ESP_066147_1985 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.19 | 335. | -5.2 | 14.27 | 63.5 | 60.7 |
| Elongated Collapse Pit in Ceraunius Fossae: ESP_066005_2110 ESP_074143_2110 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.54 | 250. | -3.7 | -15.7 | 71.0 | 72.0 |
| Lobate Debris Apron with Superposed Gullies in Nereidum Montes: ESP_066056_1330 ESP_065911_1330 (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 | -46.8 | 308. | -2.7 | -27.2 | 44.9 | 48.3 |
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