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.
| Candidate Recent Impact Site : ESP_050129_2055 ESP_050696_2055 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.45 | 222. | -2.3 | -15.1 | 43.1 | 39.6 |
| Wrinkle Ridge in Sacra Sulci Region : ESP_050430_2000 ESP_050720_2000 (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 | 19.63 | 283. | 8.44 | 28.67 | 36.6 | 33.7 |
| Gully Monitoring : ESP_050125_1480 ESP_050046_1480 (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 | -31.4 | 337. | 16.6 | -14.6 | 38.5 | 39.5 |
| Possible Dike Associated with Aromatum Chaos : ESP_050363_1785 ESP_050429_1785 (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 | -1.26 | 316. | -0.5 | -24.5 | 32.2 | 34.6 |
| Dark-Toned Disks in Light-Toned Layer along Samara Valles : ESP_050415_1565 ESP_050626_1565 (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 | -23.4 | 339. | -6.5 | -17.9 | 39.6 | 43.5 |
| Floor of Ius Chasma: ESP_050338_1720 ESP_050483_1720 (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 | -7.81 | 279. | 0.96 | 12.74 | 32.5 | 32.8 |
| Monitor Small Fresh Impact Crater in Meridiani Planum : ESP_050322_1740 ESP_059566_1740 (Interval in Earth days: 720) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.09 | 356. | 4.50 | 19.72 | 31.9 | 34.6 |
| Smaller Deposit of Hargraves Crater Ejecta in Nili Fossae Trough : ESP_050319_2020 ESP_050385_2020 (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 | 21.64 | 74.9 | -1.4 | -23.0 | 39.0 | 40.2 |
| Clays Exposed in Electris Region Deposit : ESP_050236_1445 ESP_050170_1445 (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 | -35.0 | 188. | -1.1 | 20.77 | 43.5 | 41.1 |
| Search for Active Glacial Flow: ESP_050279_1420 ESP_050490_1420 (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 | -37.8 | 95.4 | -8.5 | -19.1 | 46.5 | 50.6 |
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