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.
| Meander in Channel in Cydonia Mensae : ESP_043623_2160 ESP_051126_2160 (Interval in Earth days: 585) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.86 | 1.35 | 1.88 | -15.6 | 39.4 | 42.2 |
| 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 |
| 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 |
| 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 |
| 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 |
| 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 |
| Western Interior of Tooting Crater : ESP_043721_2035 ESP_043866_2035 (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 | 23.18 | 207. | 2.34 | 18.38 | 40.5 | 39.3 |
| USGS Dune Database Entry Number 0795-196 Changes : ESP_043607_2000 ESP_044385_2000 (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 | 19.67 | 79.5 | 9.89 | 22.91 | 40.5 | 40.5 |
| Columbia Hills Candidate Landing Site for 2020 Mission : ESP_043551_1655 ESP_043696_1655 (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 | -14.4 | 175. | -24. | -7.34 | 60.0 | 59.6 |
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