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.
| Crater with Exposed Layered Walls Superposed on Ejecta of Larger Crater: ESP_033067_1580 ESP_059559_1580 (Interval in Earth days: 2064) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.7 | 188. | 6.07 | 22.04 | 43.7 | 41.7 |
| Possible Terraced Crater in Arcadia Planitia: ESP_033066_2230 ESP_033501_2230 (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 | 42.78 | 209. | -7.0 | 19.40 | 50.0 | 44.4 |
| Large Meander in Sinuous Ridge in Aeolis Region: ESP_033187_1780 ESP_034321_1780 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.77 | 150. | -1.5 | 7.93 | 37.7 | 48.4 |
| Light-Toned Deposits along Coprates Chasma Floor: ESP_033142_1655 ESP_029028_1655 (Interval in Earth days: 320) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.1 | 301. | -5.8 | 7.091 | 41.8 | 55.4 |
| Massif in Northwest Hellas Region: ESP_033006_1545 ESP_033296_1545 (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 | -25.0 | 55.1 | 2.01 | 24.62 | 44.9 | 47.9 |
| Possible Terraced Crater in Arcadia Planitia: ESP_033146_2250 ESP_033225_2250 (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 | 44.40 | 183. | -0.1 | 22.61 | 49.8 | 47.4 |
| Monitoring Arabia Terra Dune Field: ESP_032942_1910 ESP_033008_1910 (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 | 10.73 | 358. | -1.7 | -24.6 | 36.0 | 38.1 |
| Complex of Fresh Shallow Valleys: ESP_033134_1385 ESP_068014_1385 (Interval in Earth days: 2718) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.3 | 162. | -0.6 | -21.4 | 57.7 | 56.8 |
| Gullies: ESP_032989_1435 ESP_067209_1435 (Interval in Earth days: 2666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.3 | 161. | -5.2 | 6.212 | 52.1 | 41.1 |
| 2-Kilometer Diameter Crater: ESP_033096_1445 ESP_033386_1445 (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 | -35.2 | 120. | -8.6 | 14.22 | 53.4 | 56.8 |
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