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.
| Extra-Crater Sinuous Ridge: ESP_074972_1030 ESP_074985_1030 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -76.8 | 317. | -8.6 | 6.32 | 58.5 | 57.4 |
| Variety of Spider Terrain: ESP_075003_0995 ESP_074911_0995 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -80.6 | 189. | 8.97 | -8.06 | 59.8 | 61.0 |
| Candidate Lake Deposits Fed by Alluvial Fans: ESP_074827_1655 ESP_073970_1655 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.5 | 298. | 4.36 | -6.62 | 44.2 | 54.0 |
| Fan Apex on Holden Crater Rim: ESP_074892_1525 ESP_075182_1525 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.1 | 326. | -8.3 | 19.73 | 41.8 | 36.5 |
| Channel in Huygens Crater: ESP_074981_1625 ESP_075192_1625 (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 | -17.2 | 53.7 | 6.87 | 0.528 | 41.4 | 39.5 |
| Candidate Recent Impact Site: ESP_074701_1840 ESP_075901_1840 (Interval in Earth days: 93) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.830 | 135. | 21.8 | 7.968 | 52.4 | 40.1 |
| Scarp in Mid-Latitude Mantle: ESP_074821_1245 ESP_074900_1245 (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 | -55.0 | 108. | -0.9 | 20.58 | 47.0 | 44.8 |
| Impact-Related Deposits and Flows Northeast of Ascraeus Mons: ESP_074881_1985 ESP_075382_1985 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.36 | 260. | -3.6 | 24.23 | 61.4 | 54.4 |
| Gullies: ESP_074803_1340 ESP_075225_1340 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.5 | 237. | 5.48 | -8.72 | 43.5 | 41.4 |
| Possible Secondary Craters: ESP_074952_1940 ESP_075875_1940 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.83 | 122. | -5.6 | 19.58 | 57.9 | 45.4 |
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