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.
| Exposure of North Polar Layered Deposits: ESP_037198_2675 ESP_037197_2675 (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 | 87.39 | 28.1 | -8.0 | -1.68 | 77.3 | 77.5 |
| Crater in Utopia Planitia: ESP_036894_2250 ESP_042182_2250 (Interval in Earth days: 412) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.62 | 98.3 | -1.2 | 28.07 | 52.8 | 46.2 |
| Pits and Troughs in Tempe Terra: ESP_036900_2135 ESP_053805_2140 (Interval in Earth days: 1318) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.25 | 296. | -6.1 | 5.668 | 51.4 | 41.8 |
| Candidate ExoMars Landing Site: ESP_036872_2025 ESP_036582_2025 (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 | 22.17 | 341. | 3.08 | -17.1 | 50.3 | 50.2 |
| Star and Barchan Dune Changes: ESP_037066_1710 ESP_037132_1710 (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 | -8.75 | 89.0 | 3.25 | -20.7 | 58.4 | 60.1 |
| Candidate New Impact Site: ESP_036976_2095 ESP_037398_2095 (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 | 29.18 | 22.1 | -4.1 | -14.6 | 51.7 | 57.0 |
| North Polar Basal Unit Exposure: ESP_036862_2645 ESP_072362_2645 (Interval in Earth days: 2766) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.31 | 222. | 0 | 14.33 | 69.8 | 72.7 |
| Remnant Dissected Surface: ESP_036988_1570 ESP_043186_1570 (Interval in Earth days: 483) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.7 | 61.1 | -4.9 | -20.6 | 65.6 | 62.7 |
| Lava Erupted from Fissure on Jovis Tholus: ESP_037113_1990 ESP_037680_1990 (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 | 18.53 | 242. | -3.6 | 9.25 | 52.7 | 56.2 |
| Crater with Interior Flow Lobe of Material North of Alba Region: ESP_036875_2320 ESP_062932_2320 (Interval in Earth days: 2031) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 51.86 | 255. | -0.8 | 8.59 | 54.5 | 48.7 |
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