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.
| Gullied Slope in Tempe Terra : ESP_043626_2260 ESP_050918_2260 (Interval in Earth days: 569) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.51 | 277. | 2.72 | -7.34 | 40.7 | 48.5 |
| Fractured Ground in Northeast Syrtis Major Region : ESP_043739_1975 ESP_043884_1975 (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 | 17.47 | 77.0 | 0.78 | 18.10 | 42.2 | 41.1 |
| Dunes and Slopes in Crater Southwest of Xainza Crater : ESP_043597_1800 ESP_043742_1800 (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 | -0.18 | 355. | 3.97 | 21.58 | 49.6 | 49.0 |
| Fresh Crater on Northern Plains : ESP_043601_2310 ESP_044313_2310 (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 | 50.71 | 238. | 5.53 | 24.49 | 42.0 | 39.6 |
| Mamers Valles Source : ESP_043583_2210 ESP_043649_2210 (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 | 40.56 | 12.3 | 4.01 | -11.3 | 39.7 | 40.9 |
| Line of Cones Northwest of Arsia Mons : ESP_043773_1770 ESP_043918_1770 (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 | -3.06 | 231. | -0.1 | 19.25 | 52.3 | 51.5 |
| Pit Near Elysium Mons : ESP_043763_2100 ESP_071022_2100 (Interval in Earth days: 2124) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.69 | 139. | 10.5 | -3.75 | 38.7 | 47.6 |
| Relation of Flow Inside and Outside of Impact Crater in Tharsis Region : ESP_043588_2015 ESP_044076_2015 (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 | 21.34 | 239. | -5.6 | -27.5 | 41.3 | 44.0 |
| Potential Lava Flow in Xanthe Terra : ESP_043572_1785 ESP_052209_1785 (Interval in Earth days: 673) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.43 | 318. | 5.53 | -4.69 | 50.1 | 48.8 |
| Gullied Northern Hemisphere Crater in CTX Image: ESP_043704_2230 ESP_061928_2230 (Interval in Earth days: 1420) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.53 | 308. | 3.43 | 24.09 | 39.9 | 38.9 |
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