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.
| Wrinkle Ridges in West Meridiani Planum : ESP_050164_1795 ESP_049953_1795 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.25 | 350. | -2.8 | 14.64 | 31.9 | 30.7 |
| Potential Lava Flow in Xanthe Terra : ESP_050152_1785 ESP_050587_1785 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.40 | 318. | -7.9 | 25.14 | 32.2 | 31.3 |
| Alluvial Fans in Northeastern Mojave Crater: ESP_050257_1880 ESP_050890_1880 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.806 | 327. | 26.1 | -7.29 | 31.2 | 35.2 |
| Pitted Cone Crosscut by Wrinkle Ridge in Aurorae Chaos : ESP_050231_1725 ESP_058552_1725 (Interval in Earth days: 648) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.37 | 321. | -6.2 | 6.195 | 32.3 | 29.9 |
| Well-Preserved 4-Kilometer Impact Crater : ESP_050366_1555 ESP_050511_1555 (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 | -24.2 | 237. | -1.2 | 10.47 | 39.1 | 40.4 |
| Fissure Vent Forming Low Shield in Athabasca Valles Region : ESP_050171_1895 ESP_057305_1895 (Interval in Earth days: 556) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.608 | 157. | -0.0 | 28.89 | 34.3 | 49.4 |
| Nili Patera Monitoring : ESP_050438_1890 ESP_051071_1890 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.704 | 67.3 | -0.4 | -29.2 | 33.4 | 38.1 |
| Knob and Flows in Adamas Labyrinthus : ESP_050252_2165 ESP_050542_2165 (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 | 36.05 | 102. | -6.6 | 10.74 | 49.2 | 44.9 |
| Deposit on Crater Floor : ESP_050147_1560 ESP_050358_1560 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.6 | 96.3 | 6.21 | -8.55 | 35.4 | 39.1 |
| Distinctive Lobe of Northern Hargraves Crater Ejecta Blanket : ESP_050187_2025 ESP_050965_2025 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.26 | 76.0 | 29.3 | 10.87 | 38.4 | 35.6 |
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